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Sample records for submillimeter array sma

  1. A submillimeter VLBI array

    Energy Technology Data Exchange (ETDEWEB)

    Weintroub, Jonathan [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA (United States)], E-mail: jweintroub@cfa.harvard.edu

    2008-10-15

    A VLBI array operating at {lambda} 1.3 mm and 0.8 mm is being designed using existing submillimeter telescopes as ad-hoc stations. Initial three station {lambda} = 1.3 mm observations of SgrA* and other AGN have produced remarkable results, which are reported by Doeleman elsewhere in this proceedings. Future observations are planned with an enhanced array which has longer baselines, more stations, and greater sensitivity. At {lambda} = 0.8 mm and on the long baselines, the array will have about a 20 {mu}as angular resolution which equals the diameter of the event horizon of the massive black hole in SgrA*. Candidate single dish facilities include the Arizona Radio Observatory Submillimeter Telescope (SMT) in Arizona, the Caltech Submillimeter Observatory (CSO) and the James Clerk Maxwell telescope (JCMT) in Hawaii, the Large Millimeter Telescope (LMT) in Mexico, ASTE and APEX in Chile, and the IRAM 30 m in Spain; interferometers include the Submillimeter Array (SMA) in Hawaii, the Combined Array for Research in Millimeter-wave Astronomy (CARMA) in California, IRAM PdB Interferometer in France, and the Atacama Large Millimeter Array (ALMA) in Chile. I will discuss the techniques we have developed for phasing interferometric arrays to act as single VLBI station. A strategy for detection of short (10s) time-scale source variability using VLBI closure phase will be described.

  2. Submillimeter Array reveals molecular complexity of dying stars

    Science.gov (United States)

    Tomasz

    2018-01-01

    The unique capabilities of the Submillimeter Array (SMA) have allowed unprecedented studies of cool evolved stars at submillimeter wavelengths. In particular, the SMA now offers the possibility to image multiple molecular transitions at once, owing to the 32-GHz wide instantaneous bandwidth of SWARM, the SMA’s new correlator. Molecular gas located far and very close to the photosphere of an asymptotic-giant branch (AGB) star, a red supergiant, or a pre-planetary nebula can now be examined in transitions observed simultaneously from a wide range of energy levels. This allows a very detailed quantitative investigation of physical and chemical conditions around these variable objects. Several imaging line surveys have been obtained with the SMA to reveal the beautiful complexity of these evolved systems. The surveys resulted in first submillimeter-wave identifications of molecules of prime astrophysical interest, e.g. of TiO, TiO2, and of rotational transitions at excited vibrational states of CO. An overview of recent SMA observations of cool evolved stars will be given with an emphasize on the interferometric line surveys. We will demonstrate their importance in unraveling the mass-loss phenomena, propagation of shocks in the circumstellar medium, and production of dust at elevated temperatures. The SMA studies of these molecular factories have a direct impact on our understanding of the chemical evolution of the Galaxy and stellar evolution at low and high masses.

  3. SMA Submillimeter Observations of HL Tau: Revealing a Compact Molecular Outflow

    Science.gov (United States)

    Lumbreras, Alba M.; Zapata, Luis A.

    2014-04-01

    We present archival high angular resolution (~2'') 12CO(3-2) line and continuum submillimeter observations of the young stellar object HL Tau made with the Submillimeter Array. The 12CO(3-2) line observations reveal the presence of a compact and wide opening angle bipolar outflow with a northeast to southwest orientation (P.A. = 50°) that is associated with the optical and infrared jet emanating from HL Tau with a similar orientation. On the other hand, the 850 μm continuum emission observations exhibit a strong and compact source in the position of HL Tau that has a spatial size of ~200 × 70 AU with a P.A. = 145° and a dust mass of around 0.1 M ⊙. These physical parameters are in agreement with values obtained recently from millimeter observations. This submillimeter source is therefore related to the disk surrounding HL Tau.

  4. SMA submillimeter observations of HL Tau: revealing a compact molecular outflow

    Energy Technology Data Exchange (ETDEWEB)

    Lumbreras, Alba M.; Zapata, Luis A. [Centro de Radioastronomía y Astrofísica, UNAM, Morelia (Mexico)

    2014-04-01

    We present archival high angular resolution (∼2'') {sup 12}CO(3-2) line and continuum submillimeter observations of the young stellar object HL Tau made with the Submillimeter Array. The {sup 12}CO(3-2) line observations reveal the presence of a compact and wide opening angle bipolar outflow with a northeast to southwest orientation (P.A. = 50°) that is associated with the optical and infrared jet emanating from HL Tau with a similar orientation. On the other hand, the 850 μm continuum emission observations exhibit a strong and compact source in the position of HL Tau that has a spatial size of ∼200 × 70 AU with a P.A. = 145° and a dust mass of around 0.1 M {sub ☉}. These physical parameters are in agreement with values obtained recently from millimeter observations. This submillimeter source is therefore related to the disk surrounding HL Tau.

  5. Deciphering Debris Disk Structure with the Submillimeter Array

    Science.gov (United States)

    MacGregor, Meredith Ann

    2018-01-01

    More than 20% of nearby main sequence stars are surrounded by dusty disks continually replenished via the collisional erosion of planetesimals, larger bodies similar to asteroids and comets in our own Solar System. The material in these ‘debris disks’ is directly linked to the larger bodies such as planets in the system. As a result, the locations, morphologies, and physical properties of dust in these disks provide important probes of the processes of planet formation and subsequent dynamical evolution. Observations at millimeter wavelengths are especially critical to our understanding of these systems, since they are dominated by larger grains that do not travel far from their origin and therefore reliably trace the underlying planetesimal distribution. The Submillimeter Array (SMA) plays a key role in advancing our understanding of debris disks by providing sensitivity at the short baselines required to determine the structure of wide-field disks, such as the HR 8799 debris disk. Many of these wide-field disks are among the closest systems to us, and will serve as cornerstone templates for the interpretation of more distant, less accessible systems.

  6. Arrays of Bolometers for Far-infrared and Submillimeter Astronomy

    Science.gov (United States)

    Chuss, D. T.; Allen, C. A.; Babu, S.; Benford, D. J.; Dotson, J. L.; Dowell, C. D.; Jhabvala, M.; Harper, D. A.; Moseley, S. Harvey; Silverberg, R. F.; Staguhn, J. G.; Voellmer, G.; Wollack, E. J.

    We describe 12 x 32 arrays of semiconducting cryogenic bolometers designed for use in far-infrared and submillimeter cameras. These 12 x 32 arrays are constructed from 1 x 32 monolithic pop-up detectors developed at NASA Goddard Space Flight Center. The pop-up technology allows the construction of large arrays with high filling factors that provide efficient use of space in the focal planes of far-infrared and submillimeter astronomical instruments. This directly leads to a significant decrease in integration time. The prototype array is currently operating in the second generation Submillimeter High Angular Resolution Camera (SHARC II), a facility instrument in use at the Caltech Submillimeter Observatory (CSO). The elements of this array employ a bismuth absorber coating and quarter wave backshort to optimize the bolometer absorption for passbands centered at 350 and 450 microns. A second array is to be installed in the High-resolution Airborne Widebandwidth Camera (HAWC), a far-infrared imaging camera for the Stratospheric Observatory for Infrared Astronomy (SOFIA). This array has been completed and is now awaiting integration into the HAWC test cryostat. HAWC is scheduled for commissioning in 2005. The HAWC array employs titanium-gold absorbers and is optimized for uniform absorption from 40 to 300 microns to accommodate all four of its far-infrared passbands. We describe the details of the HAWC array construction including the mechanical design and electrical characterization of the constituent linear arrays.

  7. Two bolometer arrays for far-infrared and submillimeter astronomy

    Science.gov (United States)

    Silverberg, Robert F.; Allen, Christine A.; Babu, Sachidananda R.; Benford, Dominic J.; Chuss, David T.; Dotson, Jessie L.; Dowell, Charles D.; Harper, Doyle A.; Jhabvala, Murzy D.; Loewenstein, Robert F.; Moseley, S. H., Jr.; Staguhn, Johannes G.; Voellmer, George M.; Wollack, Edward J.

    2004-10-01

    We describe the development, construction, and testing of two 384 element arrays of ion-implanted semiconducting cryogenic bolometers designed for use in far-infrared and submillimeter cameras. These two dimensional arrays are assembled from a number of 32 element linear arrays of monolithic Pop-Up bolometer Detectors (PUD) developed at NASA/Goddard Space Flight Center. PUD technology allows the construction of large, high filling factor, arrays that make efficient use of available focal plane area in far-infrared and submillimeter astronomical instruments. Such arrays can be used to provide a significant increase in mapping speed over smaller arrays. A prototype array has been delivered and integrated into a ground-based camera, the Submillimeter High Angular Resolution Camera (SHARC II), a facility instrument at the Caltech Submillimeter Observatory (CSO). A second array has recently been delivered for integration into the High-resolution Airborne Widebandwidth Camera (HAWC), a far-infrared imaging camera for the Stratospheric Observatory for Infrared Astronomy (SOFIA). HAWC is scheduled for commissioning in 2005.

  8. SUBMILLIMETER ARRAY AND SPITZER OBSERVATIONS OF BOK GLOBULE CB 17: A CANDIDATE FIRST HYDROSTATIC CORE?

    Energy Technology Data Exchange (ETDEWEB)

    Chen Xuepeng; Arce, Hector G.; Dunham, Michael M. [Department of Astronomy, Yale University, Box 208101, New Haven, CT 06520-8101 (United States); Zhang Qizhou; Bourke, Tyler L. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Launhardt, Ralf; Schmalzl, Markus; Henning, Thomas, E-mail: xuepeng.chen@yale.edu [Max Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg (Germany)

    2012-06-01

    We present high angular resolution Submillimeter Array (SMA) and Spitzer observations toward the Bok globule CB 17. SMA 1.3 mm dust continuum images reveal within CB 17 two sources with an angular separation of {approx}21'' ({approx}5250 AU at a distance of {approx}250 pc). The northwestern continuum source, referred to as CB 17 IRS, dominates the infrared emission in the Spitzer images, drives a bipolar outflow extending in the northwest-southeast direction, and is classified as a low-luminosity Class 0/I transition object (L{sub bol} {approx} 0.5 L{sub Sun }). The southeastern continuum source, referred to as CB 17 MMS, has faint dust continuum emission in the SMA 1.3 mm observations ({approx}6{sigma} detection; {approx}3.8 mJy), but is not detected in the deep Spitzer infrared images at wavelengths from 3.6 to 70 {mu}m. Its bolometric luminosity and temperature, estimated from its spectral energy distribution, are {<=}0.04 L{sub Sun} and {<=}16 K, respectively. The SMA CO (2-1) observations suggest that CB 17 MMS may drive a low-velocity molecular outflow ({approx}2.5 km s{sup -1}), extending in the east-west direction. Comparisons with prestellar cores and Class 0 protostars suggest that CB 17 MMS is more evolved than prestellar cores but less evolved than Class 0 protostars. The observed characteristics of CB 17 MMS are consistent with the theoretical predictions from radiative/magnetohydrodynamical simulations of a first hydrostatic core, but there is also the possibility that CB 17 MMS is an extremely low luminosity protostar deeply embedded in an edge-on circumstellar disk. Further observations are needed to study the properties of CB 17 MMS and to address more precisely its evolutionary stage.

  9. Taiwanese antennas for the Sub-Millimeter Array: a progress report

    Science.gov (United States)

    Raffin, Phillippe A.; Liu, Ching-Tang; Cervera, Mathieu; Chang, Chi-Ling; Chen, Ming-Tang; Lee, Cheng-Ching; Lee, Typhoon; Lo, Kwok-Yung; Ma, Rwei-Ping; Martin, Robert N.; Martin-Cocher, Pierre; Ong, Ching-Long; Park, Yong-Sun; Tsai, Rong-Den; Wu, Enboa; Yang, Shun-Cheng; Yang, Tien-Szu

    2000-07-01

    The Academia Sinica, Institute for Astronomy and Astrophysics (ASIAA) is building two antennas to be added to the six antennas of the Sub-Millimeter Array (SMA) of the Smithsonian Astrophysical Observatory (SAO). The antennas have been designed at SAO and are currently under construction at Mauna Kea. ASIAA's two antennas are made in Taiwan from parts manufactured locally and imported from Europe and from the USA. This report will focus on the manufacturing and testing of 2 major components: the alidade and the reflector. We will emphasize the work done on the composite parts used in the 6- meter reflectors, namely the carbon fiber tubes for the backup structure, the carbon fiber legs of the quadrupod and the composite central hub. We will discuss the modal testing and pointing tests of the antennas. Finally this report will show how the Taiwanese industry was able to respond to the high manufacturing standards required to build sub-millimeter antennas. The design and manufacturing capabilities of the Aeronautical Research Laboratories and China Shipbuilding Corporation have made possible the construction of the telescopes in Taiwan.

  10. Velocity-resolved Hot Water Emission Detected toward HL Tau with the Submillimeter Array

    Science.gov (United States)

    Kristensen, Lars E.; Brown, Joanna M.; Wilner, David; Salyk, Colette

    2016-05-01

    Using the Submillimeter Array (SMA) on Mauna Kea, the {{{H}}}216{{O}} {10}{2,9}-9{}{3,6} transition ({E}{{up}} = 1863 K) at 321.2 GHz has been detected toward the embedded low-mass protostar HL Tau. The line centroid is blueshifted by 20 km s-1 with respect to the source velocity, and it has a FWHM of 25 km s-1. The emission is tentatively resolved and extends ˜3″-4″ over the sky (˜2 beams), or ˜500 au at the distance of Taurus. The velocity offset, and to a lesser degree the spatial extent of the emission, show that the line originates in the protostellar jet or wind. This result suggests that at least some water emission observed with Herschel and Spitzer toward embedded sources, and perhaps also disk sources, contains a wind or jet component, which is crucial for interpreting these data. These pathfinder observations done with the SMA open a new window into studying the origin of water emission with e.g., ALMA, thus providing new insights into where water is in protostellar systems.

  11. Superconducting Microwave Resonator Arrays for Submillimeter/Far-Infrared Imaging

    Science.gov (United States)

    Noroozian, Omid

    Superconducting microwave resonators have the potential to revolutionize submillimeter and far-infrared astronomy, and with it our understanding of the universe. The field of low-temperature detector technology has reached a point where extremely sensitive devices like transition-edge sensors are now capable of detecting radiation limited by the background noise of the universe. However, the size of these detector arrays are limited to only a few thousand pixels. This is because of the cost and complexity of fabricating large-scale arrays of these detectors that can reach up to 10 lithographic levels on chip, and the complicated SQUID-based multiplexing circuitry and wiring for readout of each detector. In order to make substantial progress, next-generation ground-based telescopes such as CCAT or future space telescopes require focal planes with large-scale detector arrays of 104--10 6 pixels. Arrays using microwave kinetic inductance detectors (MKID) are a potential solution. These arrays can be easily made with a single layer of superconducting metal film deposited on a silicon substrate and pattered using conventional optical lithography. Furthermore, MKIDs are inherently multiplexable in the frequency domain, allowing ˜ 10 3 detectors to be read out using a single coaxial transmission line and cryogenic amplifier, drastically reducing cost and complexity. An MKID uses the change in the microwave surface impedance of a superconducting thin-film microresonator to detect photons. Absorption of photons in the superconductor breaks Cooper pairs into quasiparticles, changing the complex surface impedance, which results in a perturbation of resonator frequency and quality factor. For excitation and readout, the resonator is weakly coupled to a transmission line. The complex amplitude of a microwave probe signal tuned on-resonance and transmitted on the feedline past the resonator is perturbed as photons are absorbed in the superconductor. The perturbation can be

  12. Gravitational lens models based on submillimeter array imaging of Herschel -selected strongly lensed sub-millimeter galaxies at z > 1.5

    Energy Technology Data Exchange (ETDEWEB)

    Bussmann, R. S.; Gurwell, M. A. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Pérez-Fournon, I. [Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife (Spain); Amber, S. [Department of Physical Sciences, The Open University, Milton Keynes MK7 6AA (United Kingdom); Calanog, J.; De Bernardis, F.; Wardlow, J. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Dannerbauer, H. [Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu-CNRS-Université Paris Diderot, CE-Saclay, pt courrier 131, F-91191 Gif-sur-Yvette (France); Fu, Hai [Department of Physics and Astronomy, The University of Iowa, 203 Van Allen Hall, Iowa City, IA 52242 (United States); Harris, A. I. [Department of Astronomy, University of Maryland, College Park, MD 20742-2421 (United States); Krips, M. [Institut de RadioAstronomie Millimétrique, 300 Rue de la Piscine, Domaine Universitaire, 38406 Saint Martin d' Hères (France); Lapi, A. [Department Fisica, Univ. Tor Vergata, Via Ricerca Scientifica 1, 00133 Rome, Italy and SISSA, Via Bonomea 265, 34136 Trieste (Italy); Maiolino, R. [Cavendish Laboratory, University of Cambridge, 19 J.J. Thomson Ave., Cambridge CB3 OHE (United Kingdom); Omont, A. [Institut d' Astrophysique de Paris, UMR 7095, CNRS, UPMC Univ. Paris 06, 98bis boulevard Arago, F-75014 Paris (France); Riechers, D. [Department of Astronomy, Space Science Building, Cornell University, Ithaca, NY 14853-6801 (United States); Baker, A. J. [Department of Physics and Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Rd, Piscataway, NJ 08854 (United States); Birkinshaw, M. [HH Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol BS8 1TL (United Kingdom); Bock, J. [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); and others

    2013-12-10

    Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution imaging and Gemini-South and Multiple Mirror Telescope optical spectroscopy of strong lens candidates discovered in the two widest extragalactic surveys conducted by the Herschel Space Observatory: the Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) and the Herschel Multi-tiered Extragalactic Survey (HerMES). From a sample of 30 Herschel sources with S {sub 500} > 100 mJy, 21 are strongly lensed (i.e., multiply imaged), 4 are moderately lensed (i.e., singly imaged), and the remainder require additional data to determine their lensing status. We apply a visibility-plane lens modeling technique to the SMA data to recover information about the masses of the lenses as well as the intrinsic (i.e., unlensed) sizes (r {sub half}) and far-infrared luminosities (L {sub FIR}) of the lensed submillimeter galaxies (SMGs). The sample of lenses comprises primarily isolated massive galaxies, but includes some groups and clusters as well. Several of the lenses are located at z {sub lens} > 0.7, a redshift regime that is inaccessible to lens searches based on Sloan Digital Sky Survey spectroscopy. The lensed SMGs are amplified by factors that are significantly below statistical model predictions given the 500 μm flux densities of our sample. We speculate that this may reflect a deficiency in our understanding of the intrinsic sizes and luminosities of the brightest SMGs. The lensed SMGs span nearly one decade in L {sub FIR} (median L {sub FIR} = 7.9 × 10{sup 12} L {sub ☉}) and two decades in FIR luminosity surface density (median Σ{sub FIR} = 6.0 × 10{sup 11} L {sub ☉} kpc{sup –2}). The strong lenses in this sample and others identified via (sub-)mm surveys will provide a wealth of information regarding the astrophysics of galaxy formation and evolution over a wide range in redshift.

  13. Solar Observations with the Atacama Large Millimeter/submillimeter Array

    Science.gov (United States)

    Wedemeyer, Sven

    2015-08-01

    The interferometric Atacama Large Millimeter/submillimeter Array (ALMA) has already demonstrated its impressive capabilities by observing a large variety of targets ranging from protoplanetary disks to galactic nuclei. ALMA is also capable of observing the Sun and has been used for five solar test campaigns so far. The technically challenging solar observing modes are currently under development and regular observations are expected to begin in late 2016.ALMA consists of 66 antennas located in the Chilean Andes at an altitude of 5000 m and is a true leap forward in terms of spatial resolution at millimeter wavelengths. The resolution of reconstructed interferometric images of the Sun is anticipated to be close to what current optical solar telescopes can achieve. In combination with the high temporal and spectral resolution, these new capabilities open up new parameter spaces for solar millimeter observations.The solar radiation at wavelengths observed by ALMA originates from the chromosphere, where the height of the sampled layer increases with selected wavelength. The continuum intensity is linearly correlated to the local gas temperature in the probed layer, which makes ALMA essentially a linear thermometer. During flares, ALMA can detect additional non-thermal emission contributions. Measurements of the polarization state facilitate the valuable determination of the chromospheric magnetic field. In addition, spectrally resolved observations of radio recombination and molecular lines may yield great diagnostic potential, which has yet to be investigated and developed.Many different scientific applications for a large range of targets from quiet Sun to active regions and prominences are possible, ranging from ultra-high cadence wave studies to flare observations. ALMA, in particular in combination with other ground-based and space-borne instruments, will certainly lead to fascinating new findings, which will advance our understanding of the atmosphere of our Sun

  14. A DETAILED GRAVITATIONAL LENS MODEL BASED ON SUBMILLIMETER ARRAY AND KECK ADAPTIVE OPTICS IMAGING OF A HERSCHEL-ATLAS SUBMILLIMETER GALAXY AT z = 4.243 {sup ,} {sup ,}

    Energy Technology Data Exchange (ETDEWEB)

    Bussmann, R. S.; Gurwell, M. A. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Fu Hai; Cooray, A. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Smith, D. J. B.; Bonfield, D.; Dunne, L. [Centre for Astrophysics, Science and Technology Research Institute, University of Hertfordshire, Hatfield, Herts AL10 9AB (United Kingdom); Dye, S.; Eales, S. [School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD (United Kingdom); Auld, R. [Cardiff University, School of Physics and Astronomy, Queens Buildings, The Parade, Cardiff CF24 3AA (United Kingdom); Baes, M.; Fritz, J. [Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent (Belgium); Baker, A. J. [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019 (United States); Cava, A. [Departamento de Astrofisica, Facultad de CC. Fisicas, Universidad Complutense de Madrid, E-28040 Madrid (Spain); Clements, D. L.; Dariush, A. [Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Coppin, K. [Department of Physics, McGill University, Ernest Rutherford Building, 3600 Rue University, Montreal, Quebec, H3A 2T8 (Canada); Dannerbauer, H. [Universitaet Wien, Institut fuer Astronomie, Tuerkenschanzstrasse 17, 1180 Wien, Oesterreich (Austria); De Zotti, G. [Universita di Padova, Dipto di Astronomia, Vicolo dell' Osservatorio 2, IT 35122, Padova (Italy); Hopwood, R., E-mail: rbussmann@cfa.harvard.edu [Department of Physics and Astronomy, Open University, Walton Hall, Milton Keynes, MK7 6AA (United Kingdom); and others

    2012-09-10

    We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 {mu}m and the Keck adaptive optics (AO) system at the K{sub S}-band of a gravitationally lensed submillimeter galaxy (SMG) at z = 4.243 discovered in the Herschel Astrophysical Terahertz Large Area Survey. The SMA data (angular resolution Almost-Equal-To 0.''6) resolve the dust emission into multiple lensed images, while the Keck AO K{sub S}-band data (angular resolution Almost-Equal-To 0.''1) resolve the lens into a pair of galaxies separated by 0.''3. We present an optical spectrum of the foreground lens obtained with the Gemini-South telescope that provides a lens redshift of z{sub lens} = 0.595 {+-} 0.005. We develop and apply a new lens modeling technique in the visibility plane that shows that the SMG is magnified by a factor of {mu} = 4.1 {+-} 0.2 and has an intrinsic infrared (IR) luminosity of L{sub IR} = (2.1 {+-} 0.2) Multiplication-Sign 10{sup 13} L{sub Sun }. We measure a half-light radius of the background source of r{sub s} = 4.4 {+-} 0.5 kpc which implies an IR luminosity surface density of {Sigma}{sub IR} (3.4 {+-} 0.9) Multiplication-Sign 10{sup 11} L{sub Sun} kpc{sup -2}, a value that is typical of z > 2 SMGs but significantly lower than IR luminous galaxies at z {approx} 0. The two lens galaxies are compact (r{sub lens} Almost-Equal-To 0.9 kpc) early-types with Einstein radii of {theta}{sub E1} 0.57 {+-} 0.01 and {theta}{sub E2} = 0.40 {+-} 0.01 that imply masses of M{sub lens1} = (7.4 {+-} 0.5) Multiplication-Sign 10{sup 10} M{sub Sun} and M{sub lens2} = (3.7 {+-} 0.3) Multiplication-Sign 10{sup 10} M{sub Sun }. The two lensing galaxies are likely about to undergo a dissipationless merger, and the mass and size of the resultant system should be similar to other early-type galaxies at z {approx} 0.6. This work highlights the importance of high spatial resolution imaging in developing models of strongly lensed galaxies

  15. The Submillimeter Array – current status and future plans

    Science.gov (United States)

    Blundell, Raymond

    2018-01-01

    The current SMA receiver systems were designed in the mid-1990s and have been operating for more than fifteen years. With regular upgrades to receivers, deployment of the SWARM correlator, expansion of the IF signal transport bandwidth via improvements to the analog IF signal processing hardware, and many other enhancements, the SMA currently greatly outperforms its original specifications in terms of sensitivity, instantaneous bandwidth, and availability of observing modes such as full-Stokes polarization and dual frequency operation.We have recently started to implement a three-year instrument upgrade plan, which we are calling the wSMA. The wSMA will offer even wider bandwidth operation than the current SMA and improved sensitivity. The major subsystems that will form the wSMA include significantly improved, dual polarization receiver cartridges housed in a new cryostat; local oscillator units incorporating modern mm-wave technology; an upgraded signal transmission system; and a further expansion of the SWARM correlator. The cryostat will be cooled by a low-maintenance pulse-tube cryocooler. Two dual-polarization receiver cartridges will cover approximately the same sky frequencies as the current receiver sets; the low-band receiver will be fed by an LO unit covering 210-270 GHz, and the high-band receiver will be fed by an LO covering 280-360 GHz. With a receiver IF band of 4-20 GHz, this will enable continuous sky frequency coverage from 190 GHz to 380 GHz.Details of the upgrade plans will be presented together with a discussion of scientific opportunities afforded by this upgrade, which, once implemented, will enable the SMA to continue to produce the highest quality science throughout the next decade.

  16. A deeply embedded young protoplanetary disk around L1489 IRS observed by the Submillimeter Array

    DEFF Research Database (Denmark)

    Brinch, C.; Crapsi, A.; Jørgensen, J. K.

    2007-01-01

    aim to identify whether an embedded Keplerian protoplanetary disk resides in the L1489 IRS system. Given the amount of envelope material still present, such a disk would respresent a very young example of a protoplanetary disk. Methods. Using the Submillimeter Array we have observed the HCO + J = 3......-2 line with a resolution of about 1". At this resolution a protoplanetary disk with a radius of a few hundred AUs should be detectable, if present. Radiative transfer tools are used to model the emission from both continuum and line data. Results. We find that these data are consistent with theoretical...

  17. The Atacama Large Millimeter/submillimeter Array - from Early Science to Full Operations.

    Science.gov (United States)

    Remijan, Anthony

    2017-06-01

    The Atacama Large Millimeter/Submillimeter Array (ALMA) is now entering its 6th cycle of scientific observations. Starting with Cycle 3, science observations were no longer considered "Early Science" or "best efforts". Cycle 5 is now the third cycle of "steady state" observations and Cycle 7 is advertised to begin ALMA "full science" operations. ALMA Full Science Operations will include all the capabilities that were agreed upon by the international consortium after the ALMA re-baselining effort. In this talk, I will detail the upcoming ALMA Cycle 5 observing capabilities, describe the process of selecting new observing modes for upcoming cycles and provide an update on the status of the ALMA Full Science capabilities.

  18. A sub-millimeter resolution PET detector module using a multi-pixel photon counter array

    Science.gov (United States)

    Song, Tae Yong; Wu, Heyu; Komarov, Sergey; Siegel, Stefan B.; Tai, Yuan-Chuan

    2010-05-01

    A PET block detector module using an array of sub-millimeter lutetium oxyorthosilicate (LSO) crystals read out by an array of surface-mount, semiconductor photosensors has been developed. The detector consists of a LSO array, a custom acrylic light guide, a 3 × 3 multi-pixel photon counter (MPPC) array (S10362-11-050P, Hamamatsu Photonics, Japan) and a readout board with a charge division resistor network. The LSO array consists of 100 crystals, each measuring 0.8 × 0.8 × 3 mm3 and arranged in 0.86 mm pitches. A Monte Carlo simulation was used to aid the design and fabrication of a custom light guide to control distribution of scintillation light over the surface of the MPPC array. The output signals of the nine MPPC are multiplexed by a charge division resistor network to generate four position-encoded analog outputs. Flood image, energy resolution and timing resolution measurements were performed using standard NIM electronics. The linearity of the detector response was investigated using gamma-ray sources of different energies. The 10 × 10 array of 0.8 mm LSO crystals was clearly resolved in the flood image. The average energy resolution and standard deviation were 20.0% full-width at half-maximum (FWHM) and ±5.0%, respectively, at 511 keV. The timing resolution of a single MPPC coupled to a LSO crystal was found to be 857 ps FWHM, and the value for the central region of detector module was 1182 ps FWHM when ±10% energy window was applied. The nonlinear response of a single MPPC when used to read out a single LSO was observed among the corner crystals of the proposed detector module. However, the central region of the detector module exhibits significantly less nonlinearity (6.5% for 511 keV). These results demonstrate that (1) a charge-sharing resistor network can effectively multiplex MPPC signals and reduce the number of output signals without significantly degrading the performance of a PET detector and (2) a custom light guide to permit light sharing

  19. Submillimeter Array 12CO (2-1) Imaging of the NGC 6946 Giant Molecular Clouds

    Science.gov (United States)

    Wu, Ya-Lin; Sakamoto, Kazushi; Pan, Hsi-An

    2017-04-01

    We present a 12CO (2-1) mosaic map of the spiral galaxy NGC 6946 by combining data from the Submillimeter Array and the IRAM 30 m telescope. We identify 390 giant molecular clouds (GMCs) from the nucleus to 4.5 kpc in the disk. GMCs in the inner 1 kpc are generally more luminous and turbulent, some of which have luminosities >106 K km s-1 pc2 and velocity dispersions >10 km s-1. Large-scale bar-driven dynamics likely regulate GMC properties in the nuclear region. Similar to the Milky Way and other disk galaxies, GMC mass function of NGC 6946 has a shallower slope (index > -2) in the inner region, and a steeper slope (index outer region. This difference in mass spectra may be indicative of different cloud formation pathways: gravitational instabilities might play a major role in the nuclear region, while cloud coalescence might be dominant in the outer disk. Finally, the NGC 6946 clouds are similar to those in M33 in terms of statistical properties, but they are generally less luminous and turbulent than the M51 clouds.

  20. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging

    Science.gov (United States)

    Shimojo, M.; Bastian, T. S.; Hales, A. S.; White, S. M.; Iwai, K.; Hills, R. E.; Hirota, A.; Phillips, N. M.; Sawada, T.; Yagoubov, P.; Siringo, G.; Asayama, S.; Sugimoto, M.; Brajša, R.; Skokić, I.; Bárta, M.; Kim, S.; de Gregorio-Monsalvo, I.; Corder, S. A.; Hudson, H. S.; Wedemeyer, S.; Gary, D. E.; De Pontieu, B.; Loukitcheva, M.; Fleishman, G. D.; Chen, B.; Kobelski, A.; Yan, Y.

    2017-07-01

    Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic phenomena such as jets and flares. High-resolution observations of the Sun at millimeter and submillimeter wavelengths are challenging due to the intense, extended, low-contrast, and dynamic nature of emission from the quiet Sun, and the extremely intense and variable nature of emissions associated with energetic phenomena. The Atacama Large Millimeter/submillimeter Array (ALMA) was designed with solar observations in mind. The requirements for solar observations are significantly different from observations of sidereal sources and special measures are necessary to successfully carry out this type of observations. We describe the commissioning efforts that enable the use of two frequency bands, the 3-mm band (Band 3) and the 1.25-mm band (Band 6), for continuum interferometric-imaging observations of the Sun with ALMA. Examples of high-resolution synthesized images obtained using the newly commissioned modes during the solar-commissioning campaign held in December 2015 are presented. Although only 30 of the eventual 66 ALMA antennas were used for the campaign, the solar images synthesized from the ALMA commissioning data reveal new features of the solar atmosphere that demonstrate the potential power of ALMA solar observations. The ongoing expansion of ALMA and solar-commissioning efforts will continue to enable new and unique solar observing capabilities.

  1. The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?

    Science.gov (United States)

    Hsu, Li-Yen; Cowie, Lennox L.; Barger, Amy J.; Wang, Wei-Hao

    2017-12-01

    In this third paper of the Hawaii SCUBA-2 Lensing Cluster Survey series, we present Submillimeter Array (SMA) detections of six intrinsically faint 850 μm sources detected in SCUBA-2 images of the lensing cluster fields, A1689, A2390, A370, MACS J0717.5+3745, and MACS J1423.8+2404. Two of the SCUBA-2 sources split into doublets, yielding a total of eight SMA detections. The intrinsic 870 μm flux densities of these submillimeter galaxies (SMGs) are ∼1 mJy. Five of the eight SMGs are not detected in optical or near-infrared (NIR) images. The NIR-to-submillimeter flux ratios of these faint SMGs suggest that most of them are extremely dusty and/or are at very high redshifts. By combining these SMGs and several other samples from the literature, we find a bimodal distribution for the faint sources in the space of submillimeter flux versus NIR-to-submillimeter flux ratio. While most of the SMA-detected lensed sources are very obscured, the other SMGs with similar flux densities are mostly bright in the NIR. Future Atacama Large Millimeter/submillimeter Array observations of a large sample of SCUBA-2 sources in cluster fields will allow us to decide whether or not the bimodality we observe here really exists.

  2. MEASURING MASS ACCRETION RATE ONTO THE SUPERMASSIVE BLACK HOLE IN M87 USING FARADAY ROTATION MEASURE WITH THE SUBMILLIMETER ARRAY

    Energy Technology Data Exchange (ETDEWEB)

    Kuo, C. Y.; Asada, K.; Rao, R.; Nakamura, M.; Algaba, J. C.; Liu, H. B.; Inoue, M.; Koch, P. M.; Ho, P. T. P.; Matsushita, S.; Pu, H.-Y.; Nishioka, H.; Pradel, N. [Academia Sinica, Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 10617, Taiwan (China); Akiyama, K. [National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 181-8588 (Japan)

    2014-03-10

    We present the first constraint on the Faraday rotation measure (RM) at submillimeter wavelengths for the nucleus of M87. By fitting the polarization position angles (χ) observed with the Submillimeter Array at four independent frequencies around ∼230 GHz and interpreting the change in χ as a result of external Faraday rotation associated with accretion flow, we determine the RM of the M87 core to be between –7.5 × 10{sup 5} and 3.4 × 10{sup 5} rad m{sup –2}. Assuming a density profile of the accretion flow that follows a power-law distribution and a magnetic field that is ordered, radial, and has equipartition strength, the limit on the RM constrains the mass accretion rate M-dot to be below 9.2 × 10{sup –4} M {sub ☉} yr{sup –1} at a distance of 21 Schwarzschild radii from the central black hole. This value is at least two orders of magnitude smaller than the Bondi accretion rate, suggesting significant suppression of the accretion rate in the inner region of the accretion flow. Consequently, our result disfavors the classical advection-dominated accretion flow and prefers the adiabatic inflow-outflow solution or convection-dominated accretion flow for the hot accretion flow in M87.

  3. Cure SMA

    Science.gov (United States)

    ... Research Publications Spinraza Support & Care For Newly Diagnosed Care Packages Information Packets Equipment Pool Living With SMA Medical Issues Palliative Breathing Orthopedics Nutrition Equipment Daily Life At School At Home Adults With SMA Play Travel Grief & Loss Community & ...

  4. Performance evaluation of a sub-millimeter spatial resolution PET detector module using a digital silicon photomultiplier coupled LGSO array

    Science.gov (United States)

    Leem, Hyun Tae; Choi, Yong; Kim, Kyu Bom; Lee, Sangwon; Yamamoto, Seiichi; Yeom, Jung-Yeol

    2017-02-01

    In positron emission tomography (PET) for breast, brain and small animal imaging, the spatial resolution of a PET detector is crucial to obtain high quality PET images. In this study, a PET detector for sub-millimeter spatial resolution imaging purpose was assembled using 4×4 pixels of a digital silicon photomultiplier (dSiPM, DPC-3200-22-44, Philips) coupled with a 15×15 LGSO array with BaSO4 reflector, and a 1 mm thick acrylic light guide for light distribution between the dSiPM pixels. The active area of each dSiPM pixel was 3.2×3.9 mm2 and the size of each LGSO scintillator element was 0.7×0.7×6 mm3. In this paper, we experimentally demonstrated the performance of the PET detector by measuring the energy resolution, 2D flood map, peak to valley (P/V) ratio, and coincidence resolving time (CRT). All measurements were performed at a temperature of 10±1 ℃. The average energy resolution was 15.6% (without correcting for saturation effects) at 511 keV and the best CRT was 242±5 ps. The 2D flood map obtained with an energy window of 400-600 keV demonstrated clear identification of all pixels, and the average P/V ratio of the X- and Y-directions were 7.31 and 7.81, respectively. This study demonstrated that the PET detector could be suitable for application in high resolution PET while achieving good timing resolution.

  5. Performance evaluation of a sub-millimeter spatial resolution PET detector module using a digital silicon photomultiplier coupled LGSO array

    Energy Technology Data Exchange (ETDEWEB)

    Leem, Hyun Tae [Molecular Imaging Research & Education (MiRe) Laboratory, Department of Electronic Engineering, Sogang University, Seoul (Korea, Republic of); Choi, Yong, E-mail: ychoi@sogang.ac.kr [Molecular Imaging Research & Education (MiRe) Laboratory, Department of Electronic Engineering, Sogang University, Seoul (Korea, Republic of); Kim, Kyu Bom; Lee, Sangwon [Molecular Imaging Research & Education (MiRe) Laboratory, Department of Electronic Engineering, Sogang University, Seoul (Korea, Republic of); Yamamoto, Seiichi [Department of Medical Technology, Nagoya University Graduate School of Medicine, Nagoya (Japan); Yeom, Jung-Yeol, E-mail: jungyeol@korea.ac.kr [School of Biomedical Engineering, Korea University, Seoul (Korea, Republic of)

    2017-02-21

    In positron emission tomography (PET) for breast, brain and small animal imaging, the spatial resolution of a PET detector is crucial to obtain high quality PET images. In this study, a PET detector for sub-millimeter spatial resolution imaging purpose was assembled using 4×4 pixels of a digital silicon photomultiplier (dSiPM, DPC-3200-22-44, Philips) coupled with a 15×15 LGSO array with BaSO{sub 4} reflector, and a 1 mm thick acrylic light guide for light distribution between the dSiPM pixels. The active area of each dSiPM pixel was 3.2×3.9 mm{sup 2} and the size of each LGSO scintillator element was 0.7×0.7×6 mm{sup 3}. In this paper, we experimentally demonstrated the performance of the PET detector by measuring the energy resolution, 2D flood map, peak to valley (P/V) ratio, and coincidence resolving time (CRT). All measurements were performed at a temperature of 10±1 ℃. The average energy resolution was 15.6% (without correcting for saturation effects) at 511 keV and the best CRT was 242±5 ps. The 2D flood map obtained with an energy window of 400–600 keV demonstrated clear identification of all pixels, and the average P/V ratio of the X- and Y-directions were 7.31 and 7.81, respectively. This study demonstrated that the PET detector could be suitable for application in high resolution PET while achieving good timing resolution.

  6. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Fast-Scan Single-Dish Mapping

    Science.gov (United States)

    White, S. M.; Iwai, K.; Phillips, N. M.; Hills, R. E.; Hirota, A.; Yagoubov, P.; Siringo, G.; Shimojo, M.; Bastian, T. S.; Hales, A. S.; Sawada, T.; Asayama, S.; Sugimoto, M.; Marson, R. G.; Kawasaki, W.; Muller, E.; Nakazato, T.; Sugimoto, K.; Brajša, R.; Skokić, I.; Bárta, M.; Kim, S.; Remijan, A. J.; de Gregorio, I.; Corder, S. A.; Hudson, H. S.; Loukitcheva, M.; Chen, B.; De Pontieu, B.; Fleishmann, G. D.; Gary, D. E.; Kobelski, A.; Wedemeyer, S.; Yan, Y.

    2017-07-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope has commenced science observations of the Sun starting in late 2016. Since the Sun is much larger than the field of view of individual ALMA dishes, the ALMA interferometer is unable to measure the background level of solar emission when observing the solar disk. The absolute temperature scale is a critical measurement for much of ALMA solar science, including the understanding of energy transfer through the solar atmosphere, the properties of prominences, and the study of shock heating in the chromosphere. In order to provide an absolute temperature scale, ALMA solar observing will take advantage of the remarkable fast-scanning capabilities of the ALMA 12 m dishes to make single-dish maps of the full Sun. This article reports on the results of an extensive commissioning effort to optimize the mapping procedure, and it describes the nature of the resulting data. Amplitude calibration is discussed in detail: a path that uses the two loads in the ALMA calibration system as well as sky measurements is described and applied to commissioning data. Inspection of a large number of single-dish datasets shows significant variation in the resulting temperatures, and based on the temperature distributions, we derive quiet-Sun values at disk center of 7300 K at λ = 3 mm and 5900 K at λ = 1.3 mm. These values have statistical uncertainties of about 100 K, but systematic uncertainties in the temperature scale that may be significantly larger. Example images are presented from two periods with very different levels of solar activity. At a resolution of about 25'', the 1.3 mm wavelength images show temperatures on the disk that vary over about a 2000 K range. Active regions and plages are among the hotter features, while a large sunspot umbra shows up as a depression, and filament channels are relatively cool. Prominences above the solar limb are a common feature of the single-dish images.

  7. DIRECT DETECTION OF PRECURSORS OF GAS GIANTS FORMED BY GRAVITATIONAL INSTABILITY WITH THE ATACAMA LARGE MILLIMETER/SUBMILLIMETER ARRAY

    Energy Technology Data Exchange (ETDEWEB)

    Mayer, Lucio [Center for Theoretical Astrophysics and Cosmology, Institute for Computational Science, University of Zurich, Winterthurerstrasse 190, CH-8057 Zürich (Switzerland); Peters, Thomas [Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching (Germany); Pineda, Jaime E. [Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching (Germany); Wadsley James; Rogers, Patrick, E-mail: p.rogers@marianopolis.edu [Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1 (Canada)

    2016-06-01

    Phases of gravitational instability are expected in the early phases of disk evolution, when the disk mass is still a substantial fraction of the mass of the star. Disk fragmentation into sub-stellar objects could occur in the cold exterior part of the disk. Direct detection of massive gaseous clumps on their way to collapse into gas giant planets would offer an unprecedented test of the disk instability model. Here we use state-of-the-art 3D radiation-hydro simulations of disks undergoing fragmentation into massive gas giants, post-processed with RADMC-3D to produce dust continuum emission maps. These are then fed into the Common Astronomy Software Applications (CASA) ALMA simulator. The synthetic maps show that both overdense spiral arms and actual clumps at different stages of collapse can be detected with the Atacama Large Millimeter/submillimeter Array (ALMA) in the full configuration at the distance of the Ophiuchus star forming region (125 pc). The detection of clumps is particularly effective at shorter wavelengths (690 GHz) combining two resolutions with multi-scale clean. Furthermore, we show that a flux-based estimate of the mass of a protoplanetary clump can be comparable to a factor of three higher than the gravitationally bound clump mass. The estimated mass depends on the assumed opacity, and on the gas temperature, which should be set using the input of radiation-hydro simulations. We conclude that ALMA has the capability to detect “smoking gun” systems that are a signpost of the disk instability model for gas giant planet formation.

  8. A novel gamma-ray detector with submillimeter resolutions using a monolithic MPPC array with pixelized Ce:LYSO and Ce:GGAG crystals

    Energy Technology Data Exchange (ETDEWEB)

    Kato, T., E-mail: katou.frme.8180@asagi.waseda.jp [Research Institute for Science and Engineering, Waseda University, 3-4-1, Ohkubo, Shinjuku, Tokyo (Japan); Kataoka, J.; Nakamori, T.; Miura, T.; Matsuda, H.; Kishimoto, A. [Research Institute for Science and Engineering, Waseda University, 3-4-1, Ohkubo, Shinjuku, Tokyo (Japan); Sato, K.; Ishikawa, Y.; Yamamura, K.; Nakamura, S.; Kawabata, N. [Solid State Division, Hamamatsu Photonics K. K., 1126-1, Ichino-cho, Hamamatsu, Shizuoka (Japan); Ikeda, H. [ISAS/JAXA, 3-1-1, Yoshinodai, Chuo-ku, Sagamihara-shi, Kanagawa (Japan); Yamamoto, S. [Kobe City College of Technology, 8-3, Gakuenhigashimati, Nishi-ku, Kobe-shi, Hyougo 651-2194 (Japan); Kamada, K. [Materials Research Laboratory, Furukawa Co., Ltd., 1-25-13, Kannondai, Tsukuba, Ibaraki 305-0856 (Japan)

    2013-01-21

    We have developed a large-area monolithic Multi-Pixel Photon Counter (MPPC) array consisting of 4×4 channels with a three-side buttable package. Each channel has a photosensitive area of 3×3 mm{sup 2} and 3600 Geiger mode avalanche photodiodes (APDs). For typical operational gain of 7.5×10{sup 5} at +20 °C, gain fluctuation over the entire MPPC device is only ±5.6%, and dark count rates (as measured at the 1 p.e. level) amount to ≤400kcps per channel. We first fabricated a gamma-ray camera consisting of the MPPC array with one-to-one coupling to a Ce-doped (Lu,Y){sub 2}(SiO{sub 4})O (Ce:LYSO) crystal array (4×4 array of 3×3×10 mm{sup 3} crystals). Energy and time resolutions of 11.5±0.5% (FWHM at 662 keV) and 493±22ps were obtained, respectively. When using the charge division resistor network, which compiles signals into four position-encoded analog outputs, the ultimate positional resolution is estimated as 0.19 mm in both X and Y directions, while energy resolution of 10.2±0.4% (FWHM) was obtained. Finally, we fabricated submillimeter Ce:LYSO and Ce-doped Gd{sub 3}Ga{sub 3}Al{sub 2}O{sub 12} (Ce:GGAG) scintillator matrices each consisting of 1.0×1.0, 0.7×0.7 and 0.5×0.5 mm{sup 2} pixels, to further improve the spatial resolution. In all types of Ce:LYSO and Ce:GGAG matrices, each crystal was clearly resolved in the position histograms when irradiated by a {sup 137}Cs source. The energy resolutions for 662 keV gamma-rays for each Ce:LYSO and Ce:GGAG scintillator matrix were ≤14.3%. These results suggest excellent potential for its use as a high spatial medical imaging device, particularly in positron emission tomography (PET). -- Highlights: ► We developed a newly designed large-area monolithic MPPC array. ► We obtained fine gain uniformity, and good energy and time resolutions when coupled to the LYSO scintillator. ► We fabricated gamma-ray camera consisting of the MPPC array and submillimeter pixelized LYSO and GGAG scintillators. ► In

  9. SUBMILLIMETER ARRAY OBSERVATIONS OF MAGNETIC FIELDS IN G240.31+0.07: AN HOURGLASS IN A MASSIVE CLUSTER-FORMING CORE

    Energy Technology Data Exchange (ETDEWEB)

    Qiu, Keping [School of Astronomy and Space Science, Nanjing University, 22 Hankou Road, Nanjing 210093 (China); Zhang, Qizhou [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Menten, Karl M. [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany); Liu, Hauyu B.; Tang, Ya-Wen [Academia Sinica Institute of Astronomy and Astrophysics, P. O. Box 23-141, Taipei 106, Taiwan (China); Girart, Josep M., E-mail: kpqiu@nju.edu.cn [Institut de Ciències de l' Espai (CSIC-IEEC), Campus UAB, Facultat de Ciències, C5p 2, E-08193 Bellaterra, Catalonia (Spain)

    2014-10-10

    We report the first detection of an hourglass magnetic field aligned with a well-defined outflow rotation system in a high-mass, star-forming region. The observations were performed with the Submillimeter Array toward G240.31+0.07, which harbors a massive, flattened, and fragmenting molecular cloud core and a wide-angle bipolar outflow. The polarized dust emission at 0.88 mm reveals a clear hourglass-shaped magnetic field aligned within 20° of the outflow axis. Maps of high-density tracing spectral lines, e.g., H{sup 13}CO{sup +} (4-3), show that the core is rotating about its minor axis, which is also aligned with the magnetic field axis. Therefore, both the magnetic field and kinematic properties observed in this region are surprisingly consistent with the theoretical predictions of the classic paradigm of isolated low-mass star formation. The strength of the magnetic field in the plane of sky is estimated to be ∼1.1 mG, resulting in a mass-to-magnetic flux ratio of 1.4 times the critical value and a turbulent-to-ordered magnetic energy ratio of 0.4. We also find that the specific angular momentum almost linearly decreases from r ∼ 0.6 pc to 0.03 pc scales, which is most likely attributed to magnetic braking.

  10. Detection of Circular Polarization from Sagittarius A* at Submillimeter Wavelengths

    Science.gov (United States)

    Munoz, Diego; Marrone, D.; Moran, J.

    2009-05-01

    We report the detection of circularly polarized (CP) emission from the compact radio source Sagittarius A* at a level of 1.5% at a frequency of 235 GHz (1.4 mm). Sgr A* is associated with the supermassive black hole (SMBH) in the Galactic Center. The observations, taken with the Submillimeter Array (SMA) on 03/31/2007, also show a linearly polarized (LP) component of 7%. The snr of our detection of CP is about 14. Before our measurements, CP had only been detected at frequencies between 1.4 and 15 GHz (21 and 2 cm) at levels Faraday rotation in the stationary screen (constant RM)acts on a time variable background source. A cold, optically thin plasma screen cannot be responsible for both a constant RM and Faraday conversion from LP to CP, therefore the observed amounts of CP are likely to be originated close to the central source. Sgr A* shows a flat-to-inverted radio spectrum and a submillimeter excess referred to as the "submillimeter bump". This excess it thought to come from the closest regions to the SMBH. In such a scenario, millimeter wavelength data is associated with regions in which the material is likely to be relativistic and the magnetic field ordered. We have carried out polarized radiative transfer calculations exploring different combinations of ordered and stochastic magnetic fields looking for a favored scenario that can explain the apparent constant increase of CP with frequency as well as the sudden jump in LP between 40 and 80 GHz.

  11. Filters for Submillimeter Electromagnetic Waves

    Science.gov (United States)

    Berdahl, C. M.

    1986-01-01

    New manufacturing process produces filters strong, yet have small, precise dimensions and smooth surface finish essential for dichroic filtering at submillimeter wavelengths. Many filters, each one essentially wafer containing fine metal grid made at same time. Stacked square wires plated, fused, and etched to form arrays of holes. Grid of nickel and tin held in brass ring. Wall thickness, thickness of filter (hole depth) and lateral hole dimensions all depend upon operating frequency and filter characteristics.

  12. Radio Interferometry with the SMA: Uncovering Hidden Star Formation in Our Extreme Galactic Center

    Science.gov (United States)

    Gutierrez, Elizabeth; Battersby, Cara; MacGregor, Meredith Ann

    2018-01-01

    Radio interferometry provides the best tool to identify embedded star-forming cores in cold, dense, molecular clouds of gas and dust. Observations at long, submillimeter wavelengths can be used to investigate the physical properties in the youngest stages of star formation. Interferometers provide the resolution necessary to resolve small scale structures like dense cores where star formation is expected to occur. CMZoom is the first large area survey of the Central Molecular Zone (CMZ) at high resolution in the submillimeter, allowing us to identify early sites of star formation. The survey uses both the subcompact and compact configurations of the Submillimeter Array (SMA) interferometric radio telescope. The CMZ, or the inner 500 pc of the Milky Way Galaxy, is a high extinction region comprised of hot, dense, and turbulent molecular gas. This region is forming about an order of magnitude fewer stars than predicted based on simple star formation prescriptions. Here, we present new high resolution images of G0.068-0.075, a region from the CMZoom survey, obtained using CASA. We highlight the importance of interferometric observations of different baseline lengths by comparing the spatial information obtained through different configurations. We will use these new images, in conjunction with the rest of the CMZoom survey, to reveal the mechanisms driving star formation at the center of the galaxy.

  13. Design and Fabrication of Two-Dimensional Semiconducting Bolometer Arrays for the High Resolution Airborne Wideband Camera (HAWC) and the Submillimeter High Angular Resolution Camera II (SHARC-II)

    Science.gov (United States)

    Voellmer, George M.; Allen, Christine A.; Amato, Michael J.; Babu, Sachidananda R.; Bartels, Arlin E.; Benford, Dominic J.; Derro, Rebecca J.; Dowell, C. Darren; Harper, D. Al; Jhabvala, Murzy D.

    2002-01-01

    The High resolution Airborne Wideband Camera (HAWC) and the Submillimeter High Angular Resolution Camera II (SHARC II) will use almost identical versions of an ion-implanted silicon bolometer array developed at the National Aeronautics and Space Administration's Goddard Space Flight Center (GSFC). The GSFC 'Pop-up' Detectors (PUD's) use a unique folding technique to enable a 12 x 32-element close-packed array of bolometers with a filling factor greater than 95 percent. A kinematic Kevlar(trademark) suspension system isolates the 200 mK bolometers from the helium bath temperature, and GSFC - developed silicon bridge chips make electrical connection to the bolometers, while maintaining thermal isolation. The JFET preamps operate at 120 K. Providing good thermal heat sinking for these, and keeping their conduction and radiation from reaching the nearby bolometers, is one of the principal design challenges encountered. Another interesting challenge is the preparation of the silicon bolometers. They are manufactured in 32-element, planar rows using Micro Electro Mechanical Systems (MEMS) semiconductor etching techniques, and then cut and folded onto a ceramic bar. Optical alignment using specialized jigs ensures their uniformity and correct placement. The rows are then stacked to create the 12 x 32-element array. Engineering results from the first light run of SHARC II at the Caltech Submillimeter Observatory (CSO) are presented.

  14. Spinal Muscular Atrophy (SMA)

    Science.gov (United States)

    ... encouraging progress. The Muscular Dystrophy Association is the leading sponsor of SMA research. The Association also provides a full program of services for individuals and families coping with SMA, and up-to-date informa- tion ...

  15. Evidence for Dust Clearing Through Resolved Submillimeter Imaging

    Science.gov (United States)

    Brown, J. M.; Blake, G. A.; Qi, C.; Dullemond, C. P.; Wilner, D. J.; Williams, J. P.

    2009-10-01

    Mid-infrared spectrophotometric observations have revealed a small subclass of circumstellar disks with spectral energy distributions (SEDs) suggestive of large inner gaps with low dust content. However, such data provide only an indirect and model-dependent method of finding central holes. Imaging of protoplanetry disks provides an independent check of SED modeling. We present here the direct characterization of three 33-47 AU radii inner gaps, in the disks around LkHα 330, SR 21N, and HD 135344B, via 340 GHz (880 μm) dust continuum aperture synthesis observations obtained with the Submillimeter Array (SMA). The large gaps are fully resolved at ~0farcs3 by the SMA data and mostly empty of dust, with less than (1-7.5) × 10-6 M sun of fine grained solids inside the holes. Gas (as traced by atomic accretion markers and CO 4.7 μm rovibrational emission) is still present in the inner regions of all three disks. For each, the inner hole exhibits a relatively steep rise in dust emission to the outer disk, a feature more likely to originate from the gravitational influence of a companion body than from a process expected to show a more shallow gradient like grain growth. Importantly, the good agreement between the spatially resolved data and spectrophotometry-based models lends confidence to current interpretations of SEDs, wherein the significant dust emission deficits arise from disks with inner gaps or holes. Further SED-based searches can therefore be expected to yield numerous additional candidates that can be examined at high spatial resolution.

  16. Faint Submillimeter Galaxies Behind Lensing Clusters

    Science.gov (United States)

    Hsu, Li-Yen; Lauchlan Cowie, Lennox; Barger, Amy J.; Desai, Vandana; Murphy, Eric J.

    2017-01-01

    Faint submillimeter galaxies are the major contributors to the submillimeter extragalactic background light and hence the dominant star-forming population in the dusty universe. Determining how much these galaxies overlap the optically selected samples is critical to fully account for the cosmic star formation history. Observations of massive cluster fields are the best way to explore this faint submillimeter population, thanks to gravitational lensing effects. We have been undertaking a lensing cluster survey with the SCUBA-2 camera on the James Clerk Maxwell Telescope to map nine galaxy clusters, including the northern five clusters in the HST Frontier Fields program. We have also been using the Submillimeter Array and the Very Large Array to determine the accurate positions of our detected sources. Our observations have discovered high-redshift dusty galaxies with far-infrared luminosities similar to that of the Milky Way or luminous infrared galaxies. Some of these galaxies are still undetected in deep optical and near-infrared images. These results suggest that a substantial amount of star formation in even the faint submillimeter population may be hidden from rest-frame optical surveys.

  17. SMA observations of Class 0 Protostars

    DEFF Research Database (Denmark)

    Chen, Xuepeng; Arce, Héctor G.; Zhang, Qizhou

    2013-01-01

    We present high angular resolution 1.3 mm and 850 μm dust continuum data obtained with the Submillimeter Array toward 33 Class 0 protostars in nearby clouds (distance <500 pc), which represents so far the largest survey toward protostellar binary/multiple systems. The median angular resolution in...

  18. An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South : Source Catalog and Multiplicity

    NARCIS (Netherlands)

    Hodge, J.; Karim, A.; Smail, I.; Swinbank, A.; Walter, F.; Biggs, A.; Ivison, R.; Weiss, A.; Alexander, D.; Bertoldi, F.; Brandt, W.; Chapman, S.; Coppin, K.; Cox, P.; Danielson, A.; Dannerbauer, H.; De, Breuck C.; Decarli, R.; Edge, A.; Greve, T.; Knudsen, K.; Menten, K.; Rix, H.; Schinnerer, E.; Simpson, J.; Wardlow, J.; Werf, van der P.P.

    2013-01-01

    We present an Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 survey of 126 submillimeter sources from the LABOCA ECDFS Submillimeter Survey (LESS). Our 870 {$μ$}m survey with ALMA (ALESS) has produced maps ~{}3{ imes} deeper and with a beam area ~{}200{ imes} smaller than the original

  19. Spinal Muscular Atrophy (SMA)

    Science.gov (United States)

    ... early, it can cause children to miss certain developmental milestones, such as rolling over, sitting up without support, ... has SMA only after the child misses certain developmental milestones, such as being able to support his or ...

  20. Comparative Life Cycle Assessment between Warm SMA and Conventional SMA

    Science.gov (United States)

    2011-09-01

    This report presents the comparative life cycle assessment (LCA) between warm stone mastic asphalt (SMA) and conventional : SMA. Specifically, the study evaluated and compared the life cycle environmental and economic performances of two mixtures: a ...

  1. Submillimeter Continuum Observations of Comets

    Science.gov (United States)

    Jewitt, David

    1998-01-01

    The aim of this proposal was to study the submillimeter continuum emission from comets. The study was based mainly on the exploitation of the world's leading submillimeter telescope, the JCMT (James Clerk Maxwell Telescope) on Mauna Kea. Submillimeter wavelengths provide a unique view of cometary physics for one main reason. The cometary size distribution is such that the scattering cross-section is dominated by small dust grains, while the mass is dominated by the largest particles. Submillimeter continuum radiation samples cometary particles much larger than those sampled by more common observations at shorter (optical and infrared) wavelengths and therefore provides a nearly direct measure of the cometary dust mass.

  2. A Black Hole Mass-Variability Timescale Correlation at Submillimeter Wavelengths

    NARCIS (Netherlands)

    Bower, G.C.; Dexter, J.; Markoff, S.; Gurwell, M.A.; Rao, R.; McHardy, I.

    2015-01-01

    We analyze the light curves of 413 radio sources at submillimeter wavelengths using data from the Submillimeter Array calibrator database. The database includes more than 20,000 observations at 1.3 and 0.8 mm that span 13 years. We model the light curves as a damped random walk and determine a

  3. HERTZ, A Submillimeter Polarimeter

    Science.gov (United States)

    Schleuning, D. A.; Dowell, C. D.; Hildebrand, R. H.; Platt, S. R.; Novak, G.

    1997-03-01

    We describe a 32 pixel polarimeter, Hertz, for use at the Caltech Submillimeter Observatory. We present polarization maps of the Orion molecular cloud (OMC-1) at 350 \\mum (46 detections) and 450 \\mum (19 detections) with 3\\sigma or better statistical significance. The 350 \\mum polarization ranges from 1.4 to 6.8% with a median value of 3.3%. The position angles are fairly uniform across the souce at an angle of \\sim30 degrees (east of north). We describe the design and performance characteristics of the polarimeter and discuss systematic effects due to telescope and instrumental polarization, atmospheric fluctuations, and reference beam flux. (SECTION: Astronomical Instrumentation)

  4. THE IMPORTANCE OF THE MAGNETIC FIELD FROM AN SMA-CSO-COMBINED SAMPLE OF STAR-FORMING REGIONS

    Energy Technology Data Exchange (ETDEWEB)

    Koch, Patrick M.; Tang, Ya-Wen; Ho, Paul T. P.; Chen, Huei-Ru Vivien; Liu, Hau-Yu Baobab; Yen, Hsi-Wei; Lai, Shih-Ping [Academia Sinica, Institute of Astronomy and Astrophysics, Taipei, Taiwan (China); Zhang, Qizhou; Chen, How-Huan; Ching, Tao-Chung [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Girart, Josep M. [Institut de Ciències de l' Espai, CSIC-IEEC, Campus UAB, Facultat de Ciències, C5p 2, 08193 Bellaterra, Catalonia (Spain); Frau, Pau [Observatorio Astronómico Nacional, Alfonso XII, 3 E-28014 Madrid (Spain); Li, Hua-Bai [Department of Physics, The Chinese University of Hong Kong (Hong Kong); Li, Zhi-Yun [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Padovani, Marco [Laboratoire Univers et Particules de Montpellier, UMR 5299 du CNRS, Université de Montpellier II, place E. Bataillon, cc072, F-34095 Montpellier (France); Qiu, Keping [School of Astronomy and Space Science, Nanjing University, 22 Hankou Road, Nanjiing 210093 (China); Rao, Ramprasad, E-mail: pmkoch@asiaa.sinica.edu.tw [Academia Sinica, Institute of Astronomy and Astrophysics, 645 N. Aohoku Place, Hilo, HI 96720 (United States)

    2014-12-20

    Submillimeter dust polarization measurements of a sample of 50 star-forming regions, observed with the Submillimeter Array (SMA) and the Caltech Submillimeter Observatory (CSO) covering parsec-scale clouds to milliparsec-scale cores, are analyzed in order to quantify the magnetic field importance. The magnetic field misalignment δ—the local angle between magnetic field and dust emission gradient—is found to be a prime observable, revealing distinct distributions for sources where the magnetic field is preferentially aligned with or perpendicular to the source minor axis. Source-averaged misalignment angles (|δ|) fall into systematically different ranges, reflecting the different source-magnetic field configurations. Possible bimodal (|δ|) distributions are found for the separate SMA and CSO samples. Combining both samples broadens the distribution with a wide maximum peak at small (|δ|) values. Assuming the 50 sources to be representative, the prevailing source-magnetic field configuration is one that statistically prefers small magnetic field misalignments |δ|. When interpreting |δ| together with a magnetohydrodynamics force equation, as developed in the framework of the polarization-intensity gradient method, a sample-based log-linear scaling fits the magnetic field tension-to-gravity force ratio (Σ {sub B}) versus (|δ|) with (Σ {sub B}) = 0.116 · exp (0.047 · (|δ|)) ± 0.20 (mean error), providing a way to estimate the relative importance of the magnetic field, only based on measurable field misalignments |δ|. The force ratio Σ {sub B} discriminates systems that are collapsible on average ((Σ {sub B}) < 1) from other molecular clouds where the magnetic field still provides enough resistance against gravitational collapse ((Σ {sub B}) > 1). The sample-wide trend shows a transition around (|δ|) ≈ 45°. Defining an effective gravitational force ∼1 – (Σ {sub B}), the average magnetic-field-reduced star formation efficiency is at least a

  5. Photon caliper to achieve submillimeter positioning accuracy

    Science.gov (United States)

    Gallagher, Kyle J.; Wong, Jennifer; Zhang, Junan

    2017-09-01

    The purpose of this study was to demonstrate the feasibility of using a commercial two-dimensional (2D) detector array with an inherent detector spacing of 5 mm to achieve submillimeter accuracy in localizing the radiation isocenter. This was accomplished by delivering the Vernier ‘dose’ caliper to a 2D detector array where the nominal scale was the 2D detector array and the non-nominal Vernier scale was the radiation dose strips produced by the high-definition (HD) multileaf collimators (MLCs) of the linear accelerator. Because the HD MLC sequence was similar to the picket fence test, we called this procedure the Vernier picket fence (VPF) test. We confirmed the accuracy of the VPF test by offsetting the HD MLC bank by known increments and comparing the known offset with the VPF test result. The VPF test was able to determine the known offset within 0.02 mm. We also cross-validated the accuracy of the VPF test in an evaluation of couch hysteresis. This was done by using both the VPF test and the ExacTrac optical tracking system to evaluate the couch position. We showed that the VPF test was in agreement with the ExacTrac optical tracking system within a root-mean-square value of 0.07 mm for both the lateral and longitudinal directions. In conclusion, we demonstrated the VPF test can determine the offset between a 2D detector array and the radiation isocenter with submillimeter accuracy. Until now, no method to locate the radiation isocenter using a 2D detector array has been able to achieve such accuracy.

  6. SMA Spectral Line Survey of the Proto-Planetary Nebula CRL 618

    Science.gov (United States)

    Patel, Nimesh A.; Gottlieb, Carl; Young, Ken; (Tomek) Kaminski, Tomasz; McCarthy, Michael; Menten, Karl; Primiani, Rurik; Lee, Chin-Fei; Gupta, Harshal

    2018-01-01

    Carbon-rich Asymptotic Giant Branch (AGB) stars are major sources of gas and dust in the interstellar medium. AGB stars remain in their evolutionary stage for 1 to 10 Myrs, during which they have very high mass loss rates that increase at the end. During the brief (~1000 yr) period in the evolution from the AGB to the Planetary Nebula (PN) stage there are dramatic changes in the morphology from nearly spherical symmetry, to bipolar, quadrupolar and more complex structures, with the development of both slow and fast (100 km/s) outflows. The molecular composition of these objects' cirumstellar envelopes also evolves from being similar to that of parent AGB star (mainly diatomic and small polyatomic species), to more complex molecules (including ions).We have started an observational study of a sample of Proto-Planetary nebulae (PPN) with the Submillimeter Array to carry out spectral-line surveys of ~60 GHz frequency coverage in the 345 GHz band (similar to our published IRC+10216 line survey of 2011). Here we present preliminary results from the line survey of the carbon-rich PPN CRL 618, covering a frequency range of 281.9 to 359.4 GHz. Observations were carried out in January 2016 and September 2017, with the SMA in compact (3" angular resolution) and very extended (0.5") configurations, respectively.More than 1100 lines were detected in CRL 618. The majority of them can be attributed to HC3N and c-C3H2, and their isotopologues. About 350 lines are as yet unassigned. The continuum emission is unresolved even at 0.5" resolution. Several hydrogen recombination lines are detected from the central HII region. Lines of CO, HCO+, CS show the fast outflow wings, while the majority of molecular emission arises from a compact region of about 1" diameter. We present LTEmodeling and rotation temperature diagram analysis of HC3N, c-C3H2, CH3CN, and their isotopologues. We plan to observe another PPN, CRL 2688 with the SMA in 2018. Together, these imaging line surveys will

  7. Types of SMA (Spinal Muscular Atrophy)

    Science.gov (United States)

    ... Research Publications Spinraza Support & Care For Newly Diagnosed Care Packages Information Packets Equipment Pool Living With SMA Medical Issues Palliative Breathing Orthopedics Nutrition Equipment Daily Life At School At Home Adults With SMA Play Travel Grief & Loss Community & ...

  8. SUBMILLIMETER LIGHTCURVES OF ASTEROIDS V1.0

    Data.gov (United States)

    National Aeronautics and Space Administration — Submillimeter lightcurves of large asteroids Ceres, Davida, Io, Juno, Pallas, Vesta, and Victoria, observed at the Heinrich-Hertz Submillimeter Telescope from...

  9. Molecular Reconnaissance of the β Pictoris Gas Disk with the SMA: A Low HCN/(CO+CO2) Outgassing Ratio and Predictions for Future Surveys

    Science.gov (United States)

    Matrà, L.; Wilner, D. J.; Öberg, K. I.; Andrews, S. M.; Loomis, R. A.; Wyatt, M. C.; Dent, W. R. F.

    2018-02-01

    The exocometary origin of CO gas has been confirmed in several extrasolar Kuiper belts, with CO ice abundances consistent with solar system comets. We here present a molecular survey of the β Pictoris belt with the Submillimeter Array (SMA), reporting upper limits for CN, HCN, HCO+, N2H+, and H2CO, as well as for H2S, CH3OH, SiO, and DCN from archival ALMA data. Nondetections can be attributed to rapid molecular photodissociation due to the A-star’s strong UV flux. CN is the longest lasting and most easily detectable molecule after CO in this environment. We update our nonlocal thermodynamic equilibrium excitation model to include UV fluorescence, finding it plays a key role in CO and CN excitation, and we use it to turn the SMA CN/CO flux ratio constraint into an upper limit of value is consistent with, but at the low end of, the broad range observed in solar system comets. If sublimation dominates outgassing, then this low value may be caused by decreased outgassing for the less volatile molecule HCN compared to CO. If instead UV photodesorption or collisional vaporization of unbound grains dominates outgassing, then this low ratio of rates would imply a low ice abundance ratio, which would in turn indicate a variation in cometary cyanide abundances across planetary systems. To conclude, we make predictions for future molecular surveys and show that CN and HCN should be readily detectable with ALMA around β Pictoris for solar-system-like exocometary compositions.

  10. CLUMPY AND EXTENDED STARBURSTS IN THE BRIGHTEST UNLENSED SUBMILLIMETER GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Iono, Daisuke; Hatsukade, Bunyo; Kawabe, Ryohei; Matsuda, Yuichi; Nakanishi, Kouichiro [National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Yun, Min S.; Wilson, Grant [University of Massachusetts, Department of Astronomy, 710 North Pleasant Street, Amherst, MA 01003 (United States); Aretxaga, Itziar; Hughes, David [Instituto Nacional de Astrofisica, Optica y Electronica (INAOE), Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla (Mexico); Ikarashi, Soh [Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen (Netherlands); Izumi, Takuma; Kohno, Kotaro; Tamura, Yoichi; Umehata, Hideki [Institute of Astronomy, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Lee, Minju; Saito, Toshiki [Department of Astronomy, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 133-0033 (Japan); Ueda, Junko [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Michiyama, Tomonari; Ando, Misaki, E-mail: d.iono@nao.ac.jp [SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

    2016-09-20

    The central structure in three of the brightest unlensed z = 3–4 submillimeter galaxies is investigated through 0.″015–0.″05 (120–360 pc) 860 μ m continuum images obtained using the Atacama Large Millimeter/submillimeter Array (ALMA). The distribution in the central kiloparsec in AzTEC1 and AzTEC8 is extremely complex, and they are composed of multiple ∼200 pc clumps. AzTEC4 consists of two sources that are separated by ∼1.5 kpc, indicating a mid-stage merger. The peak star formation rate densities in the central clumps are ∼300–3000 M {sub ⊙} yr{sup −1} kpc{sup −2}, suggesting regions with extreme star formation near the Eddington limit. By comparing the flux obtained by ALMA and Submillimeter Array, we find that 68%–90% of the emission is extended (≳1 kpc) in AzTEC4 and 8. For AzTEC1, we identify at least 11 additional compact (∼200 pc) clumps in the extended 3–4 kpc region. Overall, the data presented here suggest that the luminosity surface densities observed at ≲150 pc scales are roughly similar to that observed in local ULIRGs, as in the eastern nucleus of Arp 220. Between 10% and 30% of the 860 μ m continuum is concentrated in clumpy structures in the central kiloparsec, while the remaining flux is distributed over ≳1 kpc regions, some of which could also be clumpy. These sources can be explained by a rapid inflow of gas such as a merger of gas-rich galaxies, surrounded by extended and clumpy starbursts. However, the cold mode accretion model is not ruled out.

  11. Active Millimeter and Submillimeter Sensing Applications Project

    Data.gov (United States)

    National Aeronautics and Space Administration — The workshop will have three main objectives. The first will be to inventory the signatures and measurements that are desirable to make using submillimeter active...

  12. Demonstration of Submillimeter Astrophysics Technology at Caltech Submillimeter Observatory Project

    Data.gov (United States)

    National Aeronautics and Space Administration — The following are the objectives of this project:(1) Demonstration of 1600-element Kinetic Inductance Detector (KID) imaging array operating at 350 micron with near...

  13. Dielectric Covered Planar Antennas at Submillimeter Wavelengths for Terahertz Imaging

    Science.gov (United States)

    Chattopadhyay, Goutam; Gill, John J.; Skalare, Anders; Lee, Choonsup; Llombart, Nuria; Siegel, Peter H.

    2011-01-01

    Most optical systems require antennas with directive patterns. This means that the physical area of the antenna will be large in terms of the wavelength. When non-cooled systems are used, the losses of microstrip or coplanar waveguide lines impede the use of standard patch or slot antennas for a large number of elements in a phased array format. Traditionally, this problem has been solved by using silicon lenses. However, if an array of such highly directive antennas is to be used for imaging applications, the fabrication of many closely spaced lenses becomes a problem. Moreover, planar antennas are usually fed by microstrip or coplanar waveguides while the mixer or the detector elements (usually Schottky diodes) are coupled in a waveguide environment. The coupling between the antenna and the detector/ mixer can be a fabrication challenge in an imaging array at submillimeter wavelengths. Antennas excited by a waveguide (TE10) mode makes use of dielectric superlayers to increase the directivity. These antennas create a kind of Fabry- Perot cavity between the ground plane and the first layer of dielectric. In reality, the antenna operates as a leaky wave mode where a leaky wave pole propagates along the cavity while it radiates. Thanks to this pole, the directivity of a small antenna is considerably enhanced. The antenna consists of a waveguide feed, which can be coupled to a mixer or detector such as a Schottky diode via a standard probe design. The waveguide is loaded with a double-slot iris to perform an impedance match and to suppress undesired modes that can propagate on the cavity. On top of the slot there is an air cavity and on top, a small portion of a hemispherical lens. The fractional bandwidth of such antennas is around 10 percent, which is good enough for heterodyne imaging applications.The new geometry makes use of a silicon lens instead of dielectric quarter wavelength substrates. This design presents several advantages when used in the submillimeter

  14. Apparent SMA I unlinked to 5q

    NARCIS (Netherlands)

    Cobben, J. M.; Scheffer, H.; de Visser, M.; Begeer, J. H.; Molenaar, W. M.; van der Steege, G.; Buys, C. H.; van Ommen, G. J.; ten Kate, L. P.

    1994-01-01

    A proband with a clinical picture indistinguishable from SMA type I is described. The parents are second cousins. On DNA analysis it appeared that the proband and his healthy 2 year old sib had inherited the same haplotypes for DNA markers flanking the SMA locus on 5q. This supports non-linkage of

  15. SMA millimeter observations of hot molecular cores

    Energy Technology Data Exchange (ETDEWEB)

    Hernández-Hernández, Vicente; Zapata, Luis; Kurtz, Stan [Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apdo. Postal 3-72 (Xangari), 58090 Morelia, Michoacán (Mexico); Garay, Guido, E-mail: v.hernandez@crya.unam.mx [Departamento de Astronomía, Universidad de Chile, Camino del Observatorio 1515, Las Condes, Santiago (Chile)

    2014-05-01

    We present Submillimeter Array observations in the 1.3 mm continuum and the CH{sub 3}CN (12 {sub K}-11 {sub K}) line of 17 hot molecular cores associated with young high-mass stars. The angular resolution of the observations ranges from 1.''0 to 4.''0. The continuum observations reveal large (>3500 AU) dusty structures with gas masses from 7 to 375 M {sub ☉}, which probably surround multiple young stars. The CH{sub 3}CN line emission is detected toward all the molecular cores at least up to the K = 6 component and is mostly associated with the emission peaks of the dusty objects. We used the multiple K-components of the CH{sub 3}CN and both the rotational diagram method and a simultaneous synthetic local thermodynamic equilibrium model with the XCLASS program to estimate the temperatures and column densities of the cores. For all sources, we obtained reasonable fits from XCLASS by using a model that combines two components: an extended and warm envelope and a compact hot core of molecular gas, suggesting internal heating by recently formed massive stars. The rotational temperatures lie in the range of 40-132 K and 122-485 K for the extended and compact components, respectively. From the continuum and CH{sub 3}CN results, we infer fractional abundances from 10{sup –9} to 10{sup –7} toward the compact inner components, which increase with the rotational temperature. Our results agree with a chemical scenario in which the CH{sub 3}CN molecule is efficiently formed in the gas phase above 100-300 K, and its abundance increases with temperature.

  16. An alma survey of submillimeter galaxies in the extended Chandra deep field-south: The agn fraction and X-ray properties of submillimeter galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Wang, S. X.; Brandt, W. N.; Luo, B. [Department of Astronomy and Astrophysics, 525 Davey Lab, The Pennsylvania State University, University Park, PA 16802 (United States); Smail, I.; Alexander, D. M.; Danielson, A. L. R.; Karim, A.; Simpson, J. M.; Swinbank, A. M. [Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE (United Kingdom); Hodge, J. A.; Walter, F. [Max-Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany); Lehmer, B. D. [The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218 (United States); Wardlow, J. L. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Xue, Y. Q. [Key Laboratory for Research in Galaxies and Cosmology, Center for Astrophysics, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui 230026 (China); Chapman, S. C. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Coppin, K. E. K. [Centre for Astrophysics, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Dannerbauer, H. [Universität Wien, Institute für Astrophysik, Türkenschanzstraße 17, 1180 Wien (Austria); De Breuck, C. [European Southern Observatory, Karl-Schwarzschild Straße 2, D-85748 Garching (Germany); Menten, K. M. [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany); Van der Werf, P., E-mail: xxw131@psu.edu, E-mail: niel@astro.psu.edu [Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden (Netherlands)

    2013-12-01

    The large gas and dust reservoirs of submillimeter galaxies (SMGs) could potentially provide ample fuel to trigger an active galactic nucleus (AGN), but previous studies of the AGN fraction in SMGs have been controversial largely due to the inhomogeneity and limited angular resolution of the available submillimeter surveys. Here we set improved constraints on the AGN fraction and X-ray properties of the SMGs with Atacama Large Millimeter/submillimeter Array (ALMA) and Chandra observations in the Extended Chandra Deep Field-South (E-CDF-S). This study is the first among similar works to have unambiguously identified the X-ray counterparts of SMGs; this is accomplished using the fully submillimeter-identified, statistically reliable SMG catalog with 99 SMGs from the ALMA LABOCA E-CDF-S Submillimeter Survey. We found 10 X-ray sources associated with SMGs (median redshift z = 2.3), of which eight were identified as AGNs using several techniques that enable cross-checking. The other two X-ray detected SMGs have levels of X-ray emission that can be plausibly explained by their star formation activity. Six of the eight SMG-AGNs are moderately/highly absorbed, with N {sub H} > 10{sup 23} cm{sup –2}. An analysis of the AGN fraction, taking into account the spatial variation of X-ray sensitivity, yields an AGN fraction of 17{sub −6}{sup +16}% for AGNs with rest-frame 0.5-8 keV absorption-corrected luminosity ≥7.8 × 10{sup 42} erg s{sup –1}; we provide estimated AGN fractions as a function of X-ray flux and luminosity. ALMA's high angular resolution also enables direct X-ray stacking at the precise positions of SMGs for the first time, and we found four potential SMG-AGNs in our stacking sample.

  17. Superconducting Bolometer Array Architectures

    Science.gov (United States)

    Benford, Dominic J.; Chervenak, James A.; Irwin, Kent D.; Moseley, S. H., Jr.; Shafer, Richard A.; Staguhn, Johannes G.; Wollack, Ed

    2003-02-01

    The next generation of far-infrared and submillimeter instruments require large arrays of detectors containing thousands of elements. These arrays will necessarily be multiplexed, and superconducting bolometer arrays are the most promising present prospect for these detectors. We discuss our current research into superconducting bolometer array technologies, which has recently resulted in the first multiplexed detections of submillimeter light and the first multiplexed astronomical observations. Prototype arrays containing 512 pixels are in production using the Pop-Up Detector (PUD) architecture, which can be extended easily to 1000 pixel arrays. Planar arrays of close-packed bolometers are being developed for the GBT and for future space missions. For certain applications, such as a slewed far-infrared sky survey, feedhorn-coupling of a large sparsely-filled array of bolometers is desirable, and is being developed using photolithographic feedhorn arrays. Individual detectors have achieved a Noise Equivalent Power (NEP) of ~10-17 W/√Hz at 300mK, but several orders of magnitude improvement are required and can be reached with existing technology. The testing of such ultralow-background detectors will prove difficult, as this requires optical loading of below 1fW. Antenna-coupled bolometer designs have advantages for large format array designs at low powers due to their mode selectivity. We also present a design and preliminary results for an enhanced-dynamic-range transition edge sensor suitable for broadband ultralow-background detectors.

  18. High-Sensitivity AGN Polarimetry at Sub-Millimeter Wavelengths

    Directory of Open Access Journals (Sweden)

    Ivan Martí-Vidal

    2017-10-01

    Full Text Available The innermost regions of radio loud Active Galactic Nuclei (AGN jets are heavily affected by synchrotron self-absorption, due to the strong magnetic fields and high particle densities in these extreme zones. The only way to overcome this absorption is to observe at sub-millimeter wavelengths, although polarimetric observations at such frequencies have so far been limited by sensitivity and calibration accuracy. However, new generation instruments such as the Atacama Large mm/sub-mm Array (ALMA overcome these limitations and are starting to deliver revolutionary results in the observational studies of AGN polarimetry. Here we present an overview of our state-of-the-art interferometric mm/sub-mm polarization observations of AGN jets with ALMA (in particular, the gravitationally-lensed sources PKS 1830−211 and B0218+359, which allow us to probe the magneto-ionic conditions at the regions closest to the central black holes.

  19. Design of shape memory alloy (SMA) actuators

    CERN Document Server

    Rao, Ashwin; Reddy, J N

    2015-01-01

    This short monograph presents an analysis and design methodology for shape memory alloy (SMA) components such as wires, beams, and springs for different applications. The solid-solid, diffusionless phase transformations in thermally responsive SMA allows them to demonstrate unique characteristics like superelasticity and shape memory effects. The combined sensing and actuating capabilities of such materials allows them to provide a system level response by combining multiple functions in a single material system. In SMA, the combined mechanical and thermal loading effects influence the functionality of such materials. The aim of this book is to make the analysis of these materials accessible to designers by developing a "strength of materials" approach to the analysis and design of such SMA components inspired from their various applications with a review of various factors influencing the design process for such materials.

  20. The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Bright-end of the Sub-millimeter Number Counts

    NARCIS (Netherlands)

    Simpson, J. M.; Smail, Ian; Swinbank, A. M.; Chapman, S. C.; Geach, J. E.; Ivison, R. J.; Thomson, A. P.; Aretxaga, I.; Blain, A. W.; Cowley, W. I.; Chen, Chian-Chou; Coppin, K. E. K.; Dunlop, J. S.; Edge, A. C.; Farrah, D.; Ibar, E.; Karim, A.; Knudsen, K. K.; Meijerink, R.; Michałowski, M. J.; Scott, D.; Spaans, M.; van der Werf, P. P.

    We present high-resolution 870 μm Atacama Large Millimeter/sub-millimeter Array (ALMA) continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1 degree2 850 μm maps from the SCUBA-2 Cosmology Legacy Survey, and are representative of the

  1. Assessing the Needs of the SMA Population

    Directory of Open Access Journals (Sweden)

    Matthew A. Halanski

    2014-11-01

    Full Text Available To define issues of greatest importance to families and health care professionals (HCP involved in caring for patients with spinal muscular atrophy (SMA, an electronic survey was distributed to patients, families, and HCPs to determine the most important issues facing patients with SMA. Seventy-seven patients/families (30 SMA type I, 36 SMA type II, 11 SMA type III and 89 HCPs (17 pulmonologists; 10 physical, speech, and occupational therapists; 19 orthopedic surgeons, 12 neurologists; 13 nurses; 10 nutritionists; 8 others completed the survey. Breathing issues, impact of diet, impact of disease on the family, spinal deformity, and surgical interventions were the five most frequently identified topics in order of importance to the patients/families. Important topics were similar for the HCP ranking those as follows: breathing issues, impact on family, spinal deformity, impact of diet, and impact of medications. This investigation reports the current most important perceived health care needs of patients with SMA. The perceived needs were similar between patients, families, and HCPs.

  2. Nutcracker and SMA syndromes: What is the normal SMA angle in children?

    Energy Technology Data Exchange (ETDEWEB)

    Arthurs, O.J., E-mail: oja20@owenarthurs.co.uk [Department of Radiology, Box 219, Addenbrooke' s Hospital, Cambridge University Teaching Hospitals NHS Foundation Trust, Hills Road, Cambridge, CB2 0QQ (United Kingdom); Mehta, U. [Department of Radiology, Box 219, Addenbrooke' s Hospital, Cambridge University Teaching Hospitals NHS Foundation Trust, Hills Road, Cambridge, CB2 0QQ (United Kingdom); Set, P.A.K., E-mail: p.set@addenbrookes.nhs.uk [Department of Radiology, Box 219, Addenbrooke' s Hospital, Cambridge University Teaching Hospitals NHS Foundation Trust, Hills Road, Cambridge, CB2 0QQ (United Kingdom)

    2012-08-15

    Objective: The nutcracker and superior mesenteric artery (SMA) syndromes are rare conditions where the left renal vein or duodenum may be compressed by an unusually acute angle between the SMA and aorta, although the normal angle in children is unknown. We measured the SMA angle to define the normal range in children. Methods: We retrospectively measured SMA angles, left renal vein (LRV) distance, and duodenal distance (DD) in 205 consecutive pediatric abdominal CT. Total and visceral intra-abdominal fat at the level of the umbilicus were also assessed. Results: Mean SMA angle was 45.6 {+-} 19.6 Degree-Sign (range 10.6-112.9 Degree-Sign ), mean LRV distance was 8.6 {+-} 3.9 mm (range 2.0-28.6 mm) and mean DD was 11.3 {+-} 4.8 mm (range 3.6-35.3 mm). There was a significant but weak correlation between %visceral fat volume (%VF) and SMA angle (R = 0.30; p < 0.001), LRV distance (R = 0.37, p < 0.001) and DD (R = 0.32; p < 0.001). Conclusion: There is a wide range of SMA angle, LRV and DD in normal children, which correlated weakly with visceral fat volume. Using a definition of SMA angle <25 Degree-Sign would diagnose 9.3% of asymptomatic children with nutcracker syndrome, and using a DD definition of <8 mm would diagnose 20% with SMA compression. Our findings suggest exercising caution when attributing these rare syndromes to an absolute SMA angle.

  3. Submillimeter solar images from the JCMT

    Energy Technology Data Exchange (ETDEWEB)

    Kopp, G.; Lindsey, C.

    1992-01-01

    We present nearly full-disk, diffraction-limited solar images made at 350 and 850 [mu]m and at 1.3 mm from the 15 m James Clerk Maxwell Telescope on Mauna Kea. These wavelengths sample the thermal structure of the solar chromosphere at altitude from 500 to about 1500 km, providing a height-dependent diagnostic of the atmosphere. Filament channels and neutral lines are apparent in the submillimeter images, although filaments themselves are not clearly visible. The submillimeter images show plage approximately 20% brigher than the surrounding quiet Sun, while sunspot intensities are comparable to the quiet Sun. Circumfacules,' dark are similar to those seen in Ca 8542; comparison with Ca H and K may give estimates of the temperature and filing factor of the hot gas present in these probably bifurcated regions.

  4. The millimeter and submillimeter spectrum of CF(+)

    Science.gov (United States)

    Plummer, G. M.; Anderson, T.; Herbst, E.; De Lucia, F. C.

    1986-01-01

    The application of a recently described technique for producing significantly enhanced concentrations of molecular ions for spectroscopic study to the detection and measurement of the millimeter and submillimeter wave spectrum of CF(+) is reported. The experimental procedure is discussed, and the measured absorption frequencies are shown and compared with those calculated from spectral constants. These constants are given together with those from the infrared spectrum by Kawaguchi and Hirota (1985).

  5. Status of MUSIC, the MUltiwavelength Sub/millimeter Inductance Camera

    Science.gov (United States)

    Golwala, Sunil R.; Bockstiegel, Clint; Brugger, Spencer; Czakon, Nicole G.; Day, Peter K.; Downes, Thomas P.; Duan, Ran; Gao, Jiansong; Gill, Amandeep K.; Glenn, Jason; Hollister, Matthew I.; LeDuc, Henry G.; Maloney, Philip R.; Mazin, Benjamin A.; McHugh, Sean G.; Miller, David; Noroozian, Omid; Nguyen, Hien T.; Sayers, Jack; Schlaerth, James A.; Siegel, Seth; Vayonakis, Anastasios K.; Wilson, Philip R.; Zmuidzinas, Jonas

    2012-09-01

    We present the status of MUSIC, the MUltiwavelength Sub/millimeter Inductance Camera, a new instrument for the Caltech Submillimeter Observatory. MUSIC is designed to have a 14', diffraction-limited field-of-view instrumented with 2304 detectors in 576 spatial pixels and four spectral bands at 0.87, 1.04, 1.33, and 1.98 mm. MUSIC will be used to study dusty star-forming galaxies, galaxy clusters via the Sunyaev-Zeldovich effect, and star formation in our own and nearby galaxies. MUSIC uses broadband superconducting phased-array slot-dipole antennas to form beams, lumpedelement on-chip bandpass filters to define spectral bands, and microwave kinetic inductance detectors to sense incoming light. The focal plane is fabricated in 8 tiles consisting of 72 spatial pixels each. It is coupled to the telescope via an ambient-temperature ellipsoidal mirror and a cold reimaging lens. A cold Lyot stop sits at the image of the primary mirror formed by the ellipsoidal mirror. Dielectric and metal-mesh filters are used to block thermal infrared and out-ofband radiation. The instrument uses a pulse tube cooler and 3He/ 3He/4He closed-cycle cooler to cool the focal plane to below 250 mK. A multilayer shield attenuates Earth's magnetic field. Each focal plane tile is read out by a single pair of coaxes and a HEMT amplifier. The readout system consists of 16 copies of custom-designed ADC/DAC and IF boards coupled to the CASPER ROACH platform. We focus on recent updates on the instrument design and results from the commissioning of the full camera in 2012.

  6. The Status of MUSIC: A Multicolor Sub/millimeter MKID Instrument

    Science.gov (United States)

    Schlaerth, J. A.; Czakon, N. G.; Day, P. K.; Downes, T. P.; Duan, R.; Glenn, J.; Golwala, S. R.; Hollister, M. I.; LeDuc, H. G.; Maloney, P. R.; Mazin, B. A.; Nguyen, H. T.; Noroozian, O.; Sayers, J.; Siegel, S.; Zmuidzinas, J.

    2012-05-01

    We report on the recent progress of the Multicolor Submillimeter (kinetic) Inductance Camera, or MUSIC. MUSIC will use antenna-coupled Microwave Kinetic Inductance Detectors to observe in four colors (150 GHz, 230 GHz, 290 GHz and 350 GHz) with 2304 detectors, 576 per band, at the Caltech Submillimeter Observatory. It will deploy in 2012. Here we provide an overview of the instrument, focusing on the array design. We have also used a pathfinder demonstration instrument, DemoCam, to identify problems in advance of the deployment of MUSIC. In particular, we identified two major limiters of our sensitivity: out-of-band light directly coupling to the detectors (i.e. not through the antenna), effectively an excess load, and a large 1/f contribution from our amplifiers and electronics. We discuss the steps taken to mitigate these effects to reach background-limited performance (BLIP) in observation.

  7. GAS KINEMATICS AND THE DRAGGED MAGNETIC FIELD IN THE HIGH-MASS MOLECULAR OUTFLOW SOURCE G192.16-3.84: AN SMA VIEW

    Energy Technology Data Exchange (ETDEWEB)

    Liu Hauyu Baobab; Ho, Paul T. P. [Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 106, Taiwan (China); Qiu Keping [School of Astronomy and Space Science, Nanjing University, Nanjing 210093 (China); Zhang Qizhou [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Girart, Josep M. [Institut de Ciencies de l' Espai, (CSIC-IEEC), Campus UAB, Facultat de Ciencies, C5p 2, E-08193 Bellaterra, Catalonia (Spain)

    2013-07-01

    We report Submillimeter Array (SMA) observations of polarized 0.88 mm thermal dust emission and various molecular line transitions toward the early B-type (L{sub *} {approx} 2 Multiplication-Sign 10{sup 3} L{sub Sun }) star-forming region G192.16-3.84 (IRAS 05553+1631). The peak of the continuum Stokes-I emission coincides with a hot rotating disk/envelope (SO{sub 2} rotational temperature T{sub rot}{sup SO{sub 2}}{approx}84{sup +18}{sub -13} K), with a north-south velocity gradient. Joint analysis of the rotation curve traced by HCO{sup +} 4-3 and SO{sub 2} 19{sub 1,19}-18{sub 0,18} suggests that the dense molecular gas is undergoing a spinning-up rotation, marginally bound by the gravitational force of an enclosed mass M{sub *+gas+dust} {approx} 11.2-25.2 M{sub Sun }. Perpendicular to the rotational plane, a {approx}>100/cos (i) km s{sup -1} (i {approx} 63 Degree-Sign ) high velocity molecular jet and a {approx}15-20 km s{sup -1} expanding biconical cavity were revealed in the CO 3-2 emission. The polarization percentage of the 0.88 mm continuum emission decreases toward the central rotating disk/envelope. The polarization angle in the inner {approx}2'' (0.015 pc) disk/envelope is perpendicular to the plane of the rotation. The magnetic field lines, which are predominantly in the toroidal direction along the disk plane, are likely to be dragged by the gravitationally accelerated rotation.

  8. Characteristics Analysis and Testing of SMA Spring Actuator

    Directory of Open Access Journals (Sweden)

    Jianzuo Ma

    2013-01-01

    Full Text Available The biasing form two-way shape memory alloy (SMA actuator composed of SMA spring and steel spring is analyzed. Based on the force equilibrium equation, the relationship between load capacity of SMA spring and geometric parameters is established. In order to obtain the characteristics of SMA spring actuator, the output force and output displacement of SMA spring under different temperatures are analyzed by the theoretical model and the experimental method. Based on the shape memory effect of SMA, the relationship of the SMA spring actuator's output displacement with the temperature, the stress and strain, the material parameters, and the size parameters is established. The results indicate that the trend of theoretical results is basically consistent with the experimental data. The output displacement of SMA spring actuator is increased with the increasing temperature.

  9. Lightweight Thermally Stable Multi-Meter Aperture Submillimeter Reflectors Project

    Data.gov (United States)

    National Aeronautics and Space Administration — Future astrophysics missions will require lightweight, thermally stable, submillimeter reflectors in sizes of 4m and greater. To date, graphite fiber reinforced...

  10. Pengembangan Animasi Komputer pada Pembelajaran Fisika SMA

    Directory of Open Access Journals (Sweden)

    Suharyanto Suharyanto

    2007-06-01

    Full Text Available Penelitian ini bertujuan untuk: (1 mengembangkan software pembelajaran Fisika SMA; (2 mengungkapkan kelayakan software untuk pembelajaran; dan (3 mengungkapkan kenaikan nilai posttest terhadap nilai pretest setelah pembelajaran dengan software yang dikembangkan. Subjek uji coba adalah tiga orang guru mata pelajaran Fisika, tiga siswa untuk uji coba perorangan, sembilan siswa untuk uji coba kelompok kecil, dan 30 siswa untuk uji coba lapangan. Pengumpulan data menggunakan kuesioner dan tes. Penilaian terhadap kelayakan software dilakukan oleh ahli materi, ahli media, dan guru mata pelajaran Fisika. Tanggapan terhadap penggunaan software dilakukan oleh siswa SMA Negeri 1 Minggir Sleman kelas X. Analisis data menggunakan statistik deskriptif dengan teknik kategorisasi dan persentase. Hasil penelitian menunjukkan bahwa software pada kategori baik menurut penilaian ahli materi dan guru mata pelajaran Fisika, pada kategori sangat baik menurut penilaian ahli media, dan pada kategori baik siswa SMA Negeri 1 Minggir Sleman ditinjau dari aspek pembelajaran, tampilan, dan penggunaan program. Secara umum software dinyatakan layak untuk pembelajaran Fisika SMA. Hasil pretest dan posttest menunjukkan bahwa setelah pembelajaran dengan menggunakan software terjadi kenaikan nilai rata-rata yang cukup besar. Kata kunci: pengembangan animasi^ pembelajaran fisika.

  11. PENDIDIKAN NILAI KEBANGSAAN MELALUI BUDAYA SEKOLAH DI SMA TARUNA NUSANTARA DAN SMA KOLESE DE BRITTO

    Directory of Open Access Journals (Sweden)

    Emmanuel Kus Eddy Sartono

    2016-10-01

    Full Text Available Penelitian ini bertujuan untuk menemukan pola pendidikan nilai kebangsaan hasil sintesis dari pola pendidikan nilai kebangsaan melalui budaya sekolah di SMA Taruna Nusantara dan SMA Kolese De Britto. Jenis penelitian ini adalah penelitian kualitatif-fenomenologi. Subyek penelitian adalah pengurus yayasan, kepala sekolah, wakil kepala sekolah, guru, siswa, karyawan dan orang tua. Data dikumpulkan melalui wawancara mendalam, observasi, dan dokumentasi. Teknik analisis data menggunakan model analisis interaktif, meliputi: reduksi data, penyajian data dan kesimpulan. Hasil penelitian menunjukkan bahwa ada perbedaan dan persamaan pola pendidikan nilai-nilai kebangsaan melalui budaya sekolah antara SMA Taruna Nusantara dengan SMA Kolese De Britto, meskipun demikian penelitian ini menemukan budaya sekolah efektif untuk membentuk karakter kebangsaan siswa. Sintesisnya penggabungan Sistem Among, cara Tutwuri Handayani, budaya kedisiplinan, Paradigma Pedagogi Ignasian, cura personalis dan budaya pendidikan bebas akan meningkatkan penanaman nilai kebangsaan siswa tidak sekedar pada ranah kognitif dan afektif tetapi sampai pada ranah perilaku kebangsaan.

  12. PENDIDIKAN NILAI KEBANGSAAN MELALUI BUDAYA SEKOLAH DI SMA TARUNA NUSANTARA DAN SMA KOLESE DE BRITTO

    OpenAIRE

    Emmanuel Kus Eddy Sartono; Noeng Muhadjir; Sumarno Sumarno

    2016-01-01

    Penelitian ini bertujuan untuk menemukan pola pendidikan nilai kebangsaan hasil sintesis dari pola pendidikan nilai kebangsaan melalui budaya sekolah di SMA Taruna Nusantara dan SMA Kolese De Britto. Jenis penelitian ini adalah penelitian kualitatif-fenomenologi. Subyek penelitian adalah pengurus yayasan, kepala sekolah, wakil kepala sekolah, guru, siswa, karyawan dan orang tua. Data dikumpulkan melalui wawancara mendalam, observasi, dan dokumentasi. Teknik analisis data menggunakan model ana...

  13. Population screening and cascade testing for carriers of SMA

    NARCIS (Netherlands)

    Smith, Melanie; Calabro, Vanessa; Chong, Belinda; Gardiner, Nicole; Cowie, Shannon; du Sart, Desiree

    Spinal muscular atrophy (SMA) is one of the most common autosomal-recessive diseases, caused by absence of both copies of the survival motor neuron 1 (SMN1) gene. Identification of SMA carriers has important implications for individuals with a family history and the general population. SMA carriers

  14. Adaptable radiative transfer innovations for submillimeter telescopes (ARTIST)

    DEFF Research Database (Denmark)

    Padovani, Marco; Jørgensen, Jes Kristian; Bertoldi, Frank

    2011-01-01

    Submillimeter observations are a key for answering many of the big questions in modern-day astrophysics, such as how stars and planets form, how galaxies evolve, and how material cycles through stars and the interstellar medium. With the upcoming large submillimeter facilities ALMA and Herschel...

  15. Probing Galaxy Formation and Submillimeter Surveys

    Science.gov (United States)

    Dwek, Eli; Arendt, Richard G.; Benford, Dominic J.; Moseley, Harvey S.; Shafer, Richard A.; Staguhn, Johannes G.; Fisher, Richard R. (Technical Monitor)

    2002-01-01

    Multiwavelength observations of galaxies have revealed that a significant fraction of the their stellar or accretion luminosity is absorbed and reradiated by dust at far-infrared (FIR) and submillimeter (submm) wavelengths. Submillimeter (850 micron) surveys conducted by the SCUBA instrument on the JCMT have detected a population of high redshift (z approximately equal to 1-4) ultraluminous infrared galaxies, that dominate the luminosity densities at those redshifts. Their cumulative contribution to the cosmic infrared background (CIB) detected by the COBE satellite is comparable to the observations, suggesting that at 850 microns the CIB is resolved into its constituent sources. This suggests that the early universe was much more dust enshrouded than the present one. FIR and submm surveys can therefore address fundamental questions regarding the early processes of galaxy formation and their evolution in number and luminosity over cosmic history. The scientific information that can be obtained from such surveys depend on a number of parameters, the most important of which are the diameter of the telescope and the wavelengths of the survey. We summarize the effect of these parameters on the scientific return from such surveys.

  16. KEBERADAAN DAN KENDALA PEMBELAJARAN ANTROPOLOGI DI SMA

    Directory of Open Access Journals (Sweden)

    Totok Rochana

    2013-04-01

    Full Text Available Mata pelajaran Antropologi di SMA tergabung dalam kelompok IPS (Ilmu Pengetahuan Sosial. Meskipun telah menjadi salah satu bagian mata pelajaran di SMA,  keberadaan mata pelajaran Antropologi tidak pernah berdiri menjadi mata pelajaran sendiri, melainkan menjadi bagian mata pelajaran Sejarah dan Sosiologi. Tujuan artikel ini adalah untuk membahas bagaimanakah keberadaan mata pelajaran antropologi di SMA setelah merger ini dan bagaimana kendala-kendala pembelajaran antropologi di SMA. Metode penelitian yang digunakan adalah pendekatan kualitatif, pengumpulan data dilakukan dengan observasi, wawancara dan dokumentasi. Hasil penelitian menunjukkan bahwa dalam tahun terakhir yang sibuk dengan penyempurnaan kurikulum, mata pelajaran Antropologi justru semakin termarjinalisasi. Antropologi hanya menjadi sub-bahasan  saja dalam mata pelajaran lain. Antropologi juga semakin dianggap kurang penting, padahal antropologi sangat penting dalam konteks masyarakat multikultural seperti Indonesia. Hal tersebut menyebabkan terjadinya kendala-kendala dalam proses pembelajaran di antaranya kendala struktural, kultural, dan keterbatasan sumber daya manusia.Anthropology in high school subjects is incorporated in IPS batch (Social Sciences. Although it has become one of the subjects at the high school, Anthropology is a not an independent subject.  It isonly part of History and Sociology subjects. The objective of this article is to study the existence of anthropological subjects in high school. The research method used is  qualitative approach, data collection was done by observation, interview and documentation. The results show that over the years of curriculum improvement, anthropology subjects are becoming more and more marginalised.  Anthropology is only a sub topics of other school subjects. Many regards anthropology no longer important though in fact anthropology is an important subject in a multicultural society like Indonesia. This

  17. Submillimeter Spectroscopy of the R Coronae Australis Molecular Cloud Region

    Science.gov (United States)

    Dunn, Marina Madeline; Walker, Christopher K.; Pat, Terrance; Sirsi, Siddhartha; Swift, Brandon J.; Peters, William L.

    2018-01-01

    The Interstellar Medium is comprised of large amounts of gas and dust which coalesce to form stars. Observing in the Terahertz regime of the electromagnetic spectrum, approximately 0.3 -300 microns, allows astronomers to study the ISM in unprecedented detail. Using the high spectral resolution imaging system of the SuperCam receiver, a 64-pixel array previously installed on the Submillimeter Telescope on Mt. Graham, AZ, we have begun a 500 square degree survey of the galactic plane. This instrument was designed to do a complete survey of the Milky Way from the ground, with the main focus being to observe two specific transitions of the carbon monoxide molecule, 12CO(3-2) and 13CO(3-2), at 345 GHz. In this work, we present results from these observations for the R Coronae Australis (R Cr A) complex, a region in the southern hemisphere of the sky, using spectroscopic data from a portion of the survey to gain better insight into the life cycle of the ISM. The majority of stars being formed here are similar to the stellar class of the Sun, making it an excellent area of observing interest. Using these results, we attempt to better ascertain the large-scale structure and kinematics inside of the molecular cloud.

  18. Millimeter and submillimeter spectrum of propylene oxide

    Science.gov (United States)

    Mesko, A. J.; Zou, Luyao; Carroll, P. Brandon; Widicus Weaver, Susanna L.

    2017-05-01

    The spectrum of propylene oxide was collected from 70 GHz to 1 THz using direct absorption millimeter and submillimeter spectroscopy. Analysis of the spectrum was performed using the SPFIT/SPCAT programs for the A state. A full internal rotor analysis was performed using the XIAM program. The barrier to internal rotation of the methyl group was determined to be 893 cm-1. The precision of the rotation constants, centrifugal distortion constants, and internal rotor parameters was increased over the results reported by previous low-frequency studies. The results of this laboratory study and the associated analysis, as well as a spectral prediction for the ground vibrational state of propylene oxide, are presented.

  19. Millimeter and Submillimeter Observations of Ceres

    Science.gov (United States)

    Kuan, Yi-Jehng; Chuang, Yo-Ling; Tseng, Wei-Ling; Coulson, Iain M.; Chung, Ming-Chi

    2016-07-01

    1 Ceres is the largest celestial body in the Main Asteroid Belt and is also the sole dwarf planet in the inner solar system. Water vapor from small icy solar-system bodies, including Ceres and Europa, was detected by Herschel infrared space telescope recently. Data taken from Dawn spacecraft suggest that a subsurface layer of briny water ice, together with ammonia-rich clays, may exist on Ceres. We hence observed Ceres using the 15-m James Clerk Maxwell Telescope (JCMT) to search for other atmospheric molecules besides H _{2}O. Submillimeter continuum observations employing SCUBA-2 were also carried out. Here we report the tentative detection of hydrogen cyanide in the atmosphere of Ceres. If confirmed, our finding could imply that Ceres may have a comet-like chemical composition. However, further observational confirmation and more detailed analysis is needed.

  20. Influence of Embedding SMA Fibres and SMA Fibre Surface Modification on the Mechanical Performance of BFRP Composite Laminates.

    Science.gov (United States)

    Liu, Yanfei; Wang, Zhenqing; Li, Hao; Sun, Min; Wang, Fangxin; Chen, Bingjie

    2018-01-04

    In this paper, a new shape memory alloy (SMA) hybrid basalt fibre reinforced polymer (BFRP) composite laminate was fabricated and a new surface modification method with both silane coupling agent KH550 and Al₂O₃ nanoparticles was conducted to enhance the interface performance. The mechanical performance of BFRP composite laminates with and without SMA fibres and the influence of SMA surface modification were studied in this paper. Different SMA fibre surface treatment methods, including etching with both H₂SO₄ and NaOH, modification with the silane coupling agent KH550 and new modification method with both KH550 and Al₂O₃ nanoparticles, were conducted to enhance the bonding between the SMA fibres and polymer matrix. Scanning electron microscopy (SEM) was used to observe the micromorphology of the SMA fibre surfaces exposed to different treatments and the damage morphology of composite laminates. The mechanical performance of the composites was investigated with tensile, three-point bending and low-velocity impact tests to study the influence of embedded SMA fibres and the different surface modifications of the SMA fibres. The results demonstrated that the embedded Ni-Ti SMA fibres can significantly enhance the mechanical performance of BFRP composite laminates. SMA fibres modified with both the silane coupling agent KH550 and Al₂O₃ nanoparticles illustrate the best mechanical performance among all samples.

  1. Modeling and experimentation of a positioning system of SMA wires

    Science.gov (United States)

    Lei, KinFong; Yam, Yeung

    2000-06-01

    This work reports two modeling and control attempts performed on a positioning system comprising of linking SMA wires and an overlooking video system for on-line measurements. The first attempt takes the model by Ikuta and identifies experimentally the parameters of the SMA wire. The identified single wire model is then extended to a system of two SMA wires joining together at their tips, based upon which open loop position control of the linkage is then conducted. The approach, however, becomes too complicated when more SMA wires are involved. The second attempt utilizes a neuro-fuzzy based approach for positioning control of a linkage point joining together four SMA wires. The second approach involves four ANFIS neuro-networks with hybrid learning algorithm trained to model the currents to the SMA wires as functions of present and target positions of the linkage point. Experimentation for both the two-wires and four-wires system yield quite satisfactory performance.

  2. Sistem Informasi SMA Negeri 3 Binjai Berbasis Web

    OpenAIRE

    Pangestu, Dimas

    2017-01-01

    142406075 Pada penulisan tugas akhir ini, penulis membuat website sistem informasi SMA negeri 3 Binjai. Website ini digunakan untuk memberikan informasi yang berkaitan tentang SMA Negeri 3 Binjai. Seiring perkembangan teknologi membuat membuat informasi kepada siswa/i mulai terabaikan, belum lagi jadwal sekolah mereka yang padat menyebabkan tingkat stress juga semakin tinggi. Berdasarkan hal tersebut penulis tertarik untuk membuat website sistem informasi sekolah SMA Negeri 3 Binjai yang d...

  3. A Submillimeter Resolution PET Prototype Evaluated With an 18F Inkjet Printed Phantom

    Science.gov (United States)

    Schneider, Florian R.; Hohberg, Melanie; Mann, Alexander B.; Paul, Stephan; Ziegler, Sibylle I.

    2015-10-01

    This work presents a submillimeter resolution PET (Positron Emission Tomography) scanner prototype based on SiPM/MPPC arrays (Silicon Photomultiplier/Multi Pixel Photon Counter). Onto each active area a 1 ×1 ×20 mm3 LYSO (Lutetium-Yttrium-Oxyorthosilicate) scintillator crystal is coupled one-to-one. Two detector modules facing each other in a distance of 10.0 cm have been set up with in total 64 channels that are digitized by SADCs (Sampling Analog to Digital Converters) with 80 MHz, 10 bit resolution and FPGA (Field Programmable Gate Array) based extraction of energy and time information. Since standard phantoms are not sufficient for testing submillimeter resolution at which positron range is an issue, a 18F inkjet printed phantom has been used to explore the limit in spatial resolution. The phantom could be successfully reconstructed with an iterative MLEM (Maximum Likelihood Expectation Maximization) and an analytically calculated system matrix based on the DRF (Detector Response Function) model. The system yields a coincidence time resolution of 4.8 ns FWHM, an energy resolution of 20%-30% FWHM and a spatial resolution of 0.8 mm.

  4. MKID multicolor array status and results from DemoCam

    Science.gov (United States)

    Schlaerth, James A.; Czakon, Nicole G.; Day, Peter K.; Downes, Thomas P.; Duan, Ran; Gao, Jiansong; Glenn, Jason; Golwala, Sunil R.; Hollister, Matthew I.; LeDuc, Henry G.; Mazin, Benjamin A.; Maloney, Philip R.; Noroozian, Omid; Nguyen, Hien T.; Sayers, Jack; Siegel, Seth; Vaillancourt, John E.; Vayonakis, Anastasios; Wilson, Philip R.; Zmuidzinas, Jonas

    2010-07-01

    We present the results of the latest multicolor Microwave Kinetic Inductance Detector (MKID) focal plane arrays in the submillimeter. The new detectors on the arrays are superconducting resonators which combine a coplanar waveguide section with an interdigitated capacitor, or IDC. To avoid out-of-band pickup by the capacitor, a stepped-impedance filter is used to prevent radiation from reaching the absorptive aluminum section of the resonator. These arrays are tested in the preliminary demonstration instrument, DemoCam, a precursor to the Multicolor Submillimeter Inductance Camera, MUSIC. We present laboratory results of the responsivity to light both in the laboratory and at the Caltech Submillimeter Observatory. We assess the performance of the detectors in filtering out-of-band radiation, and find the level of excess load and its effect on detector performance. We also look at the array design characteristics, and the implications for the optimization of sensitivities expected by MUSIC.

  5. Lightweight Thermally Stable Multi-Meter Aperture Submillimeter Reflectors Project

    Data.gov (United States)

    National Aeronautics and Space Administration — The objective of the Phase II effort will be an affordable demonstrated full-scale design for a thermally stable multi-meter submillimeter reflector. The Phase I...

  6. A Submillimeter HCN Laser in IRC +10216.

    Science.gov (United States)

    Schilke; Mehringer; Menten

    2000-01-01

    We report the detection of a strong submillimeter-wavelength HCN laser line at a frequency near 805 GHz toward the carbon star IRC +10216. This line, the J=9-8 rotational transition within the (0400) vibrationally excited state, is one of a series of HCN laser lines that were first detected in the laboratory in the early days of laser spectroscopy. Since its lower energy level is 4200 K above the ground state, the laser emission must arise from the innermost part of IRC +10216's circumstellar envelope. To better characterize this environment, we observed other, thermally emitting, vibrationally excited HCN lines and found that they, like the laser line, arise in a region of temperature approximately 1000 K that is located within the dust formation radius; this conclusion is supported by the line width of the laser. The (0400), J=9-8 laser might be chemically pumped and may be the only known laser (or maser) that is excited both in the laboratory and in space by a similar mechanism.

  7. Black Holes and Sub-millimeter Dimensions

    CERN Document Server

    Argyres, Philip C; March-Russell, John David; Argyres, Philip C.; Dimopoulos, Savas; March-Russell, John

    1998-01-01

    Recently, a new framework for solving the hierarchy problem was proposed which does not rely on low energy supersymmetry or technicolor. The fundamental Planck mass is at a TeV and the observed weakness of gravity at long distances is due the existence of new sub-millimeter spatial dimensions. In this letter, we study how the properties of black holes are altered in these theories. Small black holes---with Schwarzschild radii smaller than the size of the new spatial dimensions---are quite different. They are bigger, colder, and longer-lived than a usual $(3+1)$-dimensional black hole of the same mass. Furthermore, they primarily decay into harmless bulk graviton modes rather than standard-model degrees of freedom. We discuss the interplay of our scenario with the holographic principle. Our results also have implications for the bounds on the spectrum of primordial black holes (PBHs) derived from the photo-dissociation of primordial nucleosynthesis products, distortion of the diffuse gamma-ray spectrum, overcl...

  8. Infrared/submillimeter optical properties data base

    Science.gov (United States)

    Alley, Phillip W.

    1989-01-01

    The general goal was to build a data base containing optical properties, such as reflectance, transmittance, refractive index, in the far infrared to submillimeter wavelength region. This data base would be limited to selected crystalline materials and temperature between 300 and 2 K. The selected materials were: lithium, lead, and strontium; the bromides of potassium and thallium; the carbides of silicone and tungsten; and the materials of KRS5, KRS6, diamond, and sapphire. Last summer, barium fluoride was selected as prototype material for building the data base. This summer the literature search, preparation of the data for barium fluoride was completed. In addition the literature search for data related to the compounds mentioned was completed. The current status is that barium fluoride is in a form suitable for a NASA internal publication. The papers containing the data on the other materials were xeroxed and they are ready to be reduced. On the reverse side, the top figure is a sample combination of data for the index of refraction at 300 K. The lower figure shows the transmittance vs wavelength at 300 and 80 K. These figures are a sample of many which were developed. Since barium fluoride was studied more than most of the materials listed above, it is clear that additional measurements should be made to fill in the gaps present on both temperature and wavelength data.

  9. Switchable Shape Memory Alloys (SMA) Thermal Materials Project

    Science.gov (United States)

    Falker, John; Zeitlin, Nancy; Williams, Martha; Fesmire, James

    2014-01-01

    Develop 2-way switchable thermal systems for use in systems that function in cold to hot temperature ranges using different alloy designs for SMA system concepts. In this project, KSC will specifically address designs of two proof of concept SMA systems with transition temperatures in the 65-95 C range and investigate cycle fatigue and "memory loss" due to thermal cycling.

  10. APPARENT SMA-I UNLINKED TO 5Q

    NARCIS (Netherlands)

    COBBEN, JM; SCHEFFER, H; DEVISSER, M; BEGEER, JH; MOLENAAR, WM; VANDERSTEEGE, G; BUYS, CHCM; VANOMMEN, GJ; TENKATE, LP

    A proband with a clinical picture indistinguishable from SMA type I is described. The parents are second cousins. On DNA analysis it appeared that the proband and his healthy 2 year old sib had inherited the same haplotypes for DNA markers flanking the SMA locus on 5q. This supports non-linkage of

  11. Influence of SMA reinforcement on the impact resistance of GFRP ...

    Indian Academy of Sciences (India)

    Owing to the addi- tion of SMA fillers, the flexural rigidity of SMA/epoxy com- posites increases; especially, the storage modulus increases remarkably with increasing filler content in the high tem- perature region [3]. This is attributable to transformation to austenitic phase facilitating better dynamic characteristics. In this study ...

  12. SMA actuators: a viable practical technology (Presentation Video)

    Science.gov (United States)

    Browne, Alan L.; Brown, Jeffrey; Hodgson, Darel E.

    2015-04-01

    Diverse products either based solely on or incorporating Shape Memory Alloys (SMA) have and are being made in a wide range of industries, and IP is being captured. Why then compared to SE (superelastic) Nitinol, and especially conventional technology, do so few ideas reach production? This presentation delves deeply into this topic in reaching the final assessment that SMA actuators are indeed now a viable practical technology. The presentation begins with an introduction to and description of the fundamental basis of SMA actuator technology. Examples of multiple commercially available geometric forms of SMA actuators are given and the functionalities that they provide are described. This is followed by examples of multiple commercial products incorporating such SMA actuators. Given that there are literally millions of commercial products incorporating conventional actuator technologies, indications are given as to why there are their less than 1000 that utilize SMA. Experience based challenges to the commercial use of SMA actuators are described. Besides having to compete with existing non-SMA technology which is quite mature additional challenges that are unique to SM actuators are indicated these including a wider than expected set of technical engineering problems and challenges and that a broader scope of dynamics is required.

  13. The effectiveness of styrene-maleic acid (SMA) copolymers for solubilisation of integral membrane proteins from SMA-accessible and SMA-resistant membranes.

    NARCIS (Netherlands)

    Swainsbury, David J K; Scheidelaar, S.|info:eu-repo/dai/nl/413333418; Foster, Nicolas; Van Grondelle, Rienk; Killian, J.A.|info:eu-repo/dai/nl/071792317; Jones, Michael R.

    2017-01-01

    Solubilisation of biological lipid bilayer membranes for analysis of their protein complement has traditionally been carried out using detergents, but there is increasing interest in the use of amphiphilic copolymers such asstyrene maleic acid (SMA) for the solubilisation, purification and

  14. A Submillimeter Perspective on the Goods Fields. II. The High Radio Power Population in the Goods-N

    Science.gov (United States)

    Barger, A. J.; Cowie, L. L.; Owen, F. N.; Hsu, L.-Y.; Wang, W.-H.

    2017-01-01

    We use ultradeep 20 cm data from the Karl G. Jansky Very Large Array and 850 μm data from SCUBA-2 and the Submillimeter Array of an 124 arcmin2 region of the Chandra Deep Field-north to analyze the high radio power ({P}20{cm}> {10}31 erg s-1 Hz-1) population. We find that 20 (42 ± 9%) of the spectroscopically identified z> 0.8 sources have consistent star formation rates (SFRs) inferred from both submillimeter and radio observations, while the remaining sources have lower (mostly undetected) submillimeter fluxes, suggesting that active galactic nucleus (AGN) activity dominates the radio power in these sources. We develop a classification scheme based on the ratio of submillimeter flux to radio power versus radio power and find that it agrees with AGN and star-forming galaxy classifications from Very Long Baseline Interferometry. Our results provide support for an extremely rapid drop in the number of high SFR galaxies above about a thousand solar masses per year (Kroupa initial mass function) and for the locally determined relation between X-ray luminosity and radio power for star-forming galaxies applying at high redshifts and high radio powers. We measure far-infrared (FIR) luminosities and find that some AGNs lie on the FIR-radio correlation, while others scatter below. The AGNs that lie on the correlation appear to do so based on their emission from the AGN torus. We measure a median radio size of 1.″0 ± 0.3 for the star-forming galaxies. The radio sizes of the star-forming galaxies are generally larger than those of the AGNs. The W. M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, and was made possible by the generous financial support of the W. M. Keck Foundation.

  15. EVALUASI STRATEGI BERSAING SMA KRISTEN 1 SALATIGA

    Directory of Open Access Journals (Sweden)

    Eclesia Tehupeiory

    2015-06-01

    Full Text Available This study aims to evaluate the competitive strategies of SMA Kristen 1 Salatiga. The type of this study was a qualitative evaluation, through data collection by means of interviews, questionnaires, observation and documentation study. Data obtained and analyzed by an evaluation component based on Rumelt (2000 were consistency, consonance, advantage and feasibility. The results showed that: (1 Consistency evaluation of competitive strategy applied by SMA Kristen 1 Salatiga has shown consistency with the goals, values and policies of the school. (2 Consonance evaluation of competitive strategy has demonstrated suitability with the needs of society, while for competition with other schools, the school programs such as Peduli Kasih program, Sekolah Lima Hari, moving class, SMUQI Radio and multimedia extracurricular namely cinematography and photography are not appropriate. (3 Advantage evaluation of competitive strategy in the school programs such as Peduli Kasih, moving class, and Sekolah Lima Hari do not excel the resources, skills and superior positions. Other programs such as multimedia Extracurricular namely photography and cinematography is not superior to the superior position. Meanwhile, special programs such as the education expo, parenting day, career day and the Field Trip program through Live In and outdoor study do not excel in superior skills. (4 Feasibility evaluation shows that multimedia extracurricular programs have not showed the feasibility of the physical resources which involves computer supporting facilities and Wi-Fi. Suggestion to school in order to maintain the consistency that was owned, suitability to the needs of society as well as pay attention to competition with other schools also enhance the achievement of advantage and checking of IT facilities.

  16. Fabrication of an absorber-coupled MKID detector and readout for sub-millimeter and far-infrared astronomy

    Science.gov (United States)

    Brown, Ari-David; Hsieh, Wen-Ting; Moseley, S. Harvey; Stevenson, Thomas R.; U-yen, Kongpop; Wollack, Edward J.

    2010-07-01

    We have fabricated absorber-coupled microwave kinetic inductance detector (MKID) arrays for sub-millimeter and farinfrared astronomy. Each detector array is comprised of λ/2 stepped impedance resonators, a 1.5μm thick silicon membrane, and 380μm thick silicon walls. The resonators consist of parallel plate aluminum transmission lines coupled to low impedance Nb microstrip traces of variable length, which set the resonant frequency of each resonator. This allows for multiplexed microwave readout and, consequently, good spatial discrimination between pixels in the array. The Al transmission lines simultaneously act to absorb optical power and are designed to have a surface impedance and filling fraction so as to match the impedance of free space. Our novel fabrication techniques demonstrate high fabrication yield of MKID arrays on large single crystal membranes and sub-micron front-to-back alignment of the microstrip circuit.

  17. Fabrication of an Absorber-Coupled MKID Detector and Readout for Sub-Millimeter and Far-Infrared Astronomy

    Science.gov (United States)

    Brown, Ari-David; Hsieh, Wen-Ting; Moseley, S. Harvey; Stevenson, Thomas R.; U-yen, Kongpop; Wollack, Edward J.

    2010-01-01

    We have fabricated absorber-coupled microwave kinetic inductance detector (MKID) arrays for sub-millimeter and farinfrared astronomy. Each detector array is comprised of lambda/2 stepped impedance resonators, a 1.5µm thick silicon membrane, and 380µm thick silicon walls. The resonators consist of parallel plate aluminum transmission lines coupled to low impedance Nb microstrip traces of variable length, which set the resonant frequency of each resonator. This allows for multiplexed microwave readout and, consequently, good spatial discrimination between pixels in the array. The Al transmission lines simultaneously act to absorb optical power and are designed to have a surface impedance and filling fraction so as to match the impedance of free space. Our novel fabrication techniques demonstrate high fabrication yield of MKID arrays on large single crystal membranes and sub-micron front-to-back alignment of the microstrip circuit.

  18. The SMA Trust: the role of a disease-focused research charity in developing treatments for SMA.

    Science.gov (United States)

    Christie-Brown, V; Mitchell, J; Talbot, K

    2017-09-01

    SMA is a rare hereditary neuromuscular disease that causes weakness and muscle wasting as a result of the loss of spinal motor neurons. In its most severe form, SMA is the commonest genetic cause of death in infants, and children with less severe forms of SMA face the prospect of lifelong disability from progressive muscle wasting, loss of mobility and limb weakness. The initial discovery of the defective gene has been followed by major advances in our understanding of the genetic, cellular and molecular basis of SMA, providing the foundation for a range of approaches to treatment, including gene therapy, antisense oligonucleotide treatments and more traditional drug-based approaches to slow or halt disease progression. The approval by the US Food and Drug Administration (FDA) of Spinraza (nusinersen), the first targeted treatment for spinal muscular atrophy (SMA), is a historic moment. Disease-focused research charities, such as The SMA Trust (UK), continue to have a crucial role in promoting the development of additional treatments for SMA, both by funding translational research and by promoting links between researchers, people living with SMA and other stakeholders, including pharmaceutical companies and healthcare providers.

  19. Alterations in the ankyrin domain of TRPV4 cause congenital distal SMA, scapuloperoneal SMA and HMSN2C

    NARCIS (Netherlands)

    Auer-Grumbach, Michaela; Olschewski, Andrea; Papic, Lea; Kremer, Hannie; McEntagart, Meriel E.; Uhrig, Sabine; Fischer, Carina; Froehlich, Eleonore; Balint, Zoltan; Tang, Bi; Strohmaier, Heimo; Lochmueller, Hanns; Schlotter-Weigel, Beate; Senderek, Jan; Krebs, Angelika; Dick, Katherine J.; Petty, Richard; Longman, Cheryl; Anderson, Neil E.; Padberg, George W.; Schelhaas, Helenius J.; van Ravenswaaij-Arts, Conny M. A.; Pieber, Thomas R.; Crosby, Andrew H.; Guelly, Christian

    Spinal muscular atrophies (SMA, also known as hereditary motor neuropathies) and hereditary motor and sensory neuropathies (HMSN) are clinically and genetically heterogeneous disorders of the peripheral nervous system. Here we report that mutations in the TRPV4 gene cause congenital distal SMA,

  20. The SOFIA/SAFIRE Far-Infrared Spectrometer: Highlighting Submillimeter Astrophysics and Technology

    Science.gov (United States)

    Benford, Dominic J.

    2009-01-01

    The Submillimeter and Far-InfraRed Experiment (SAFIRE) on the SOFIA airborne observatory is an imaging spectrometer for wavelengths between 28 microns and 440 microns. Our design is a dual-band long-slit grating spectrometer, which provides broadband (approx. 4000 km/s) observations in two lines simultaneously over a field of view roughly 10" wide by 320" long. The low backgrounds in spectroscopy require very sensitive detectors with noise equivalent powers of order 10(exp -18) W/square root of Hz. We are developing a kilopixel, filled detector array for SAFIRE in a 32 x 40 format. The detector consists of a transition edge sensor (TES) bolometer array, a per-pixel broadband absorbing backshort array, and a NIST SQUID multiplexer readout array. This general type of array has been used successfully in the GISMO instrument, so we extrapolate to the sensitivity needed for airborne spectroscopy. Much of the cryogenic, electronics, and software infrastructure for SAFIRE have been developed. I provide here an overview of the progress on SAFIRE.

  1. Hypothalamic germinoma masquerading as superior mesenteric artery (SMA) syndrome.

    Science.gov (United States)

    Vethakkan, Shireene R; Venugopal, Yogeswari; Tan, Alexander T B; Paramasivam, Sharmila S; Ratnasingam, Jeyakantha; Razak, Rohaya A; Alias, Azmi; Kassim, Fauziah; Choong, Karen

    2013-01-01

    To report a case of superior mesenteric artery (SMA) syndrome secondary to hypothalamic germinoma. We describe the clinical presentation, diagnostic work-up, management, and clinical course of a patient admitted with SMA syndrome who was subsequently found to have a hypothalamic germinoma. An adolescent boy was admitted to the surgical ward with progressive weight loss over a 2 year period and postprandial vomiting. He was diagnosed with SMA syndrome based on evidence of proximal duodenal dilatation, extrinsic compression of the distal duodenum, and a narrowed aortomesenteric angle (16°). Investigations performed to exclude thyrotoxicosis unexpectedly revealed secondary hypothyroidism and further evaluation demonstrated evidence of pan-hypopituitarism. Psychiatric evaluation excluded anorexia nervosa and bulimia. Magnetic resonance imaging (MRI) of the brain revealed a heterogeneously enhancing hypothalamic lesion, but a normal pituitary gland. Hormone replacement with hydrocortisone, desmopressin, testosterone, and thyroxine resulted in weight gain and resolution of gastrointestinal symptoms. A transventricular endoscopic biopsy subsequently confirmed a hypothalamic germinoma and he was referred to an oncologist. SMA syndrome secondary to severe weight loss is an uncommon cause of upper gastrointestinal obstruction. While there have been reports of poorly controlled diabetes mellitus and thyrotoxicosis manifesting as SMA syndrome, there are no published reports to date of SMA syndrome secondary to hypothalamic/pituitary disease. Management of SMA syndrome is conservative, as symptoms of intestinal obstruction resolve with weight gain following treatment of the underlying cause. Awareness of this uncommon presentation of endocrine cachexia/hypothalamic disease will prevent unnecessary laparotomies and a misdiagnosis of an eating disorder.

  2. Development Of A Multicolor Sub/millimeter Camera Using Microwave Kinetic Inductance Detectors

    Science.gov (United States)

    Schlaerth, James A.; Czakon, N. G.; Day, P. K.; Downes, T. P.; Duan, R.; Glenn, J.; Golwala, S. R.; Hollister, M. I.; LeDuc, H. G.; Maloney, P. R.; Mazin, B. A.; Noroozian, O.; Sayers, J.; Siegel, S.; Vayonakis, A.; Zmuidzinas, J.

    2011-01-01

    Microwave Kinetic Inductance Detectors (MKIDs) are superconducting resonators useful for detecting light from the millimeter-wave to the X-ray. These detectors are easily multiplexed, as the resonances can be tuned to slightly different frequencies, allowing hundreds of detectors to be read out simultaneously using a single feedline. The Multicolor Submillimeter Inductance Camera, MUSIC, will use 2304 antenna-coupled MKIDs in multicolor operation, with bands centered at wavelengths of 0.85, 1.1, 1.3 and 2.0 mm, beginning in 2011. Here we present the results of our demonstration instrument, DemoCam, containing a single 3-color array with 72 detectors and optics similar to MUSIC. We present sensitivities achieved at the telescope, and compare to those expected based upon laboratory tests. We explore the factors that limit the sensitivity, in particular electronics noise, antenna efficiency, and excess loading. We discuss mitigation of these factors, and how we plan to improve sensitivity to the level of background-limited performance for the scientific operation of MUSIC. Finally, we note the expected mapping speed and contributions of MUSIC to astrophysics, and in particular to the study of submillimeter galaxies. This research has been funded by grants from the National Science Foundation, the Gordon and Betty Moore Foundation, and the NASA Graduate Student Researchers Program.

  3. A sub-millimeter resolution detector module for small-animal PET applications

    Science.gov (United States)

    Sacco, I.; Dohle, R.; Fischer, P.; Gola, A.; Piemonte, C.; Ritzert, M.

    2017-01-01

    We present a gamma detection module optimized for very high resolution PET applications, able to resolve arrays of scintillating crystals with sub-millimeter pitch. The detector is composed of a single ceramic substrate (LTCC): it hosts four flip-chip mounted PETA5 ASICs on the bottom side and an array of SiPM sensors on the top surface, fabricated in HD-RGB technology by FBK. Each chip has 36 channels, for a maximum of 144 readout channels on a sensitive area of about 32 mm × 32 mm. The module is MR-compatible. The thermal decoupling of the readout electronics from the photon sensors is obtained with an efficient internal liquid channel, integrated within the ceramic substrate. Two modules have been designed, based on different SiPM topologies: • Light spreader-based: an array of 12 × 12 SiPMs, with an overall pitch of 2.5 mm, is coupled with a scintillators array using a 1 mm thick glass plate. The light from one crystal is spread over a group of SiPMs, which are read out in parallel using PETA5 internal neighbor logic. • Interpolating SiPM-based: ISiPMs are intrinsic position-sensitive sensors. The photon diodes in the array are connected to one of the four available outputs so that the center of gravity of any bunch of detected photons can be reconstructed using a proper weight function of the read out amplitudes. An array of ISiPMs, each 7.5 mm× 5 mm sized, is directly coupled with the scintillating crystals. Both modules can clearly resolve LYSO arrays with a pitch of only 0.833 mm. The detector can be adjusted for clinical PET, where it has already shown ToF resolution of about 230 ps CRT at FWHM. The module designs, their features and results are described.

  4. Seismic Protection of an Ancient Aqueduct Using SMA Devices

    Science.gov (United States)

    Chrysostomou, Christis Z.; Demetriou, Themos; Stassis, Andreas; Hamdaoui, Karim

    2008-07-01

    The effectiveness of the use of Cu-based shape memory alloy (SMA) prestressing devices on an ancient aqueduct is examined in this paper. The dynamic characteristics of the aqueduct were measured within the span of three years and computational models were developed that matched very closely its dynamic behaviour. Using this as a bench mark, SMA prestressing devices were applied on the structure and the effects on its dynamic characteristics were assessed. It was noted that the SMA prestressing devices have a significant effect on the dynamic response of the structure. This is attributed to the stiffening of the structure due to the increase in contact between the masonry units and hence the increase of its stiffness through the increase of the modulus of elasticity of the masonry matrix. It can be concluded that the SMA prestressing devices can provide an inconspicuous means of stiffening masonry structures and increase their resistance to earthquake loads.

  5. Sistem Informasi Akademik pada SMA Hang Tuah Belawan

    OpenAIRE

    Tanjung, Dini Syahroni

    2015-01-01

    Informasi yang disampaikan oleh SMA HANG TUAH BELAWAN selama ini disebarkan melalui brosur dan cara yang seperti itu kurang efektif. Oleh karena itu dibuatlah sistem informasi akademik ini agar penyampaian informasinya lebih efektif dan efisien. 092406181

  6. Scanning strategies for imaging arrays

    Science.gov (United States)

    Kovács, Attila

    2008-07-01

    Large-format (sub)millimeter wavelength imaging arrays are best operated in scanning observing modes rather than traditional position-switched (chopped) modes. The choice of observing mode is critical for isolating source signals from various types of noise interference, especially for ground-based instrumentation operating under a bright atmosphere. Ideal observing strategies can combat 1/f noise, resist instrumental defects, sensitively recover emission on large scales, and provide an even field coverage - all under feasible requirements of telescope movement. This work aims to guide the design of observing patterns that maximize scientific returns. It also compares some of the popular choices of observing modes for (sub)millimeter imaging, such as random, Lissajous, billiard, spiral, On-The-Fly (OTF), DREAM, chopped and stare patterns. Many of the conclusions are also applicable other imaging applications and imaging in one dimension (e.g. spectroscopic observations).

  7. Manajemen Kelas oleh Wali Kelas di SMA Negeri 1 Tempunak

    OpenAIRE

    Riesanthy, Yullia; Djudin, Tomo; Fadillah

    2015-01-01

    Tujuan penelitian adalah untuk mengetahui bagaimana manajemen kelas oleh wali kelas. Dalam penelitian ini peneliti menggunakan metode kualitatif dengan jenis studi kasus. Lokasi penelitian di SMA Negeri 1 Tempunak. Subyek penelitian Kepala Sekolah. Wali Kelas dan siswa. Hasil penelitian, perencanaan manajemen kelas SMA Negeri 1 Tempunak belum terimplementasi dengan baik dan belum jelas, pelaksanaan manajemen kelas oleh wali kelas cukup baik, tetapi belum sesuai dengan ketentuan atau teori man...

  8. Sistem Informasi Akademik pada SMA Swasta Hang Tuah Belawan

    OpenAIRE

    Syarifuddin, Ruisya

    2015-01-01

    Perancangan Sistem Informasi Akademik pada SMA Swasta Hang Tuah Belawan ini bertujuan untuk mempermudah proses pencarian atau searching data dan informasi untuk seluruh Siswa SMA Swasta Hang Tuah Belawan yang mengalami kesulitan dalam memperoleh data mengenai masalah Akademik tersebut. Faasilitas yang terdapat dalam aplikasi ini berupa penyediaan data dan informasi mengenai beritaberita terbaru, profil agenda kegiatan, dan data-data yang berguna untuk kelangsungan belajar si...

  9. Infrared and submillimeter space missions in the coming decade programmes, programmatics, and technology

    CERN Document Server

    Sauvage, Marc; Gallais, Pascal; Vigroux, Laurent

    1996-01-01

    A revolution similar to that brought by CCDs to visible astronomy is still ahead in IR and submillimeter astronomy. There is certainly no wavelength range which has, over the past several years, seen such impressive advances in technology: large-scale detector arrays, new designs for cooling in space, lightweight mirror technologies. Scientific cases for observing the cold universe are outstanding. Observations in the FIR/Submm range will provide answers to such fundamental questions as: What is the spectrum of the primordial fluctuations? How do primeval galaxies look? What are the first stages of star formation? Most of the international space missions that have been triggered by these questions are presented in detail here. Technological issues raised by these missions are reviewed, as are the most recent achievements in cooling and detector technologies.

  10. The ALMA Phasing System: A Beamforming Capability for Ultra-high-resolution Science at (Sub)Millimeter Wavelengths

    Science.gov (United States)

    Matthews, L. D.; Crew, G. B.; Doeleman, S. S.; Lacasse, R.; Saez, A. F.; Alef, W.; Akiyama, K.; Amestica, R.; Anderson, J. M.; Barkats, D. A.; Baudry, A.; Broguière, D.; Escoffier, R.; Fish, V. L.; Greenberg, J.; Hecht, M. H.; Hiriart, R.; Hirota, A.; Honma, M.; Ho, P. T. P.; Impellizzeri, C. M. V.; Inoue, M.; Kohno, Y.; Lopez, B.; Martí-Vidal, I.; Messias, H.; Meyer-Zhao, Z.; Mora-Klein, M.; Nagar, N. M.; Nishioka, H.; Oyama, T.; Pankratius, V.; Perez, J.; Phillips, N.; Pradel, N.; Rottmann, H.; Roy, A. L.; Ruszczyk, C. A.; Shillue, B.; Suzuki, S.; Treacy, R.

    2018-01-01

    The Atacama Millimeter/submillimeter Array (ALMA) Phasing Project (APP) has developed and deployed the hardware and software necessary to coherently sum the signals of individual ALMA antennas and record the aggregate sum in Very Long Baseline Interferometry (VLBI) Data Exchange Format. These beamforming capabilities allow the ALMA array to collectively function as the equivalent of a single large aperture and participate in global VLBI arrays. The inclusion of phased ALMA in current VLBI networks operating at (sub)millimeter wavelengths provides an order of magnitude improvement in sensitivity, as well as enhancements in u–v coverage and north–south angular resolution. The availability of a phased ALMA enables a wide range of new ultra-high angular resolution science applications, including the resolution of supermassive black holes on event horizon scales and studies of the launch and collimation of astrophysical jets. It also provides a high-sensitivity aperture that may be used for investigations such as pulsar searches at high frequencies. This paper provides an overview of the ALMA Phasing System design, implementation, and performance characteristics.

  11. Fabrication and testing of SMA composite beam with shape control

    Science.gov (United States)

    Noolvi, Basavaraj; S, Raja; Nagaraj, Shanmukha; Mudradi, Varada Raj

    2017-07-01

    Smart materials are the advanced materials that have characteristics of sensing and actuation in response to the external stimuli like pressure, heat or electric charge etc. These materials can be integrated in to any structure to make it smart. From the different types of smart materials available, Shape Memory Alloy (SMA) is found to be more useful in designing new applications, which can offer more actuating speed, reduce the overall weight of the structure. The unique property of SMA is the ability to remember and recover from large strains of upto 8% without permanent deformation. Embedding the SMA wire/sheet in fiber-epoxy/flexible resin systems has many potential applications in Aerospace, Automobile, Medical, Robotics and various other fields. In this work the design, fabrication, and testing of smart SMA composite beam has been carried out. Two types of epoxy based resin systems namely LY 5210 resin system and EPOLAM 2063 resin system are used in fabricating the SMA composite specimens. An appropriate mould is designed and fabricated to retain the pre-strain of SMA wire during high temperature post curing of composite specimens. The specimens are fabricated using vacuum bag technique.

  12. Submillimeter Wave Antenna With Slow Wave Feed Line

    DEFF Research Database (Denmark)

    Zhurbenko, Vitaliy; Krozer, Viktor; Kotiranta, Mikko

    2009-01-01

    Submillimeter wave radiation, which is also referred to as terahertz radiation, has not been extensively explored until recently due to a lack of reliable components and devices in this frequency range. Current advances in technology have made it possible to explore this portion of the electromag...

  13. The effectiveness of styrene-maleic acid (SMA) copolymers for solubilisation of integral membrane proteins from SMA-accessible and SMA-resistant membranes.

    Science.gov (United States)

    Swainsbury, David J K; Scheidelaar, Stefan; Foster, Nicholas; van Grondelle, Rienk; Killian, J Antoinette; Jones, Michael R

    2017-10-01

    Solubilisation of biological lipid bilayer membranes for analysis of their protein complement has traditionally been carried out using detergents, but there is increasing interest in the use of amphiphilic copolymers such as styrene maleic acid (SMA) for the solubilisation, purification and characterisation of integral membrane proteins in the form of protein/lipid nanodiscs. Here we survey the effectiveness of various commercially-available formulations of the SMA copolymer in solubilising Rhodobacter sphaeroides reaction centres (RCs) from photosynthetic membranes. We find that formulations of SMA with a 2:1 or 3:1 ratio of styrene to maleic acid are almost as effective as detergent in solubilising RCs, with the best solubilisation by short chain variants (membranes was uniformly low, but could be increased through a variety of treatments to increase the lipid:protein ratio. However, proteins isolated from such membranes comprised clusters of complexes in small membrane patches rather than individual proteins. We conclude that short-chain 2:1 and 3:1 formulations of SMA are the most effective in solubilising integral membrane proteins, but that solubilisation efficiencies are strongly influenced by the size of the target protein and the density of packing of proteins in the membrane. Copyright © 2017 The Authors. Published by Elsevier B.V. All rights reserved.

  14. The effectiveness of styrene-maleic acid (SMA) copolymers for solubilisation of integral membrane proteins from SMA-accessible and SMA-resistant membranes

    NARCIS (Netherlands)

    Swainsbury, David J. K.; Scheidelaar, Stefan; Foster, Nicholas; van Grondelle, Rienk; Killian, J. Antoinette; Jones, Michael R.

    2017-01-01

    Solubilisation of biological lipid bilayer membranes for analysis of their protein complement has traditionally been carried out using detergents, but there is increasing interest in the use of amphiphilic copolymers such as styrene maleic acid (SMA) for the solubilisation, purification and

  15. SMA-MAP: a plasma protein panel for spinal muscular atrophy.

    Directory of Open Access Journals (Sweden)

    Dione T Kobayashi

    Full Text Available OBJECTIVES: Spinal Muscular Atrophy (SMA presents challenges in (i monitoring disease activity and predicting progression, (ii designing trials that allow rapid assessment of candidate therapies, and (iii understanding molecular causes and consequences of the disease. Validated biomarkers of SMA motor and non-motor function would offer utility in addressing these challenges. Our objectives were (i to discover additional markers from the Biomarkers for SMA (BforSMA study using an immunoassay platform, and (ii to validate the putative biomarkers in an independent cohort of SMA patients collected from a multi-site natural history study (NHS. METHODS: BforSMA study plasma samples (N = 129 were analyzed by immunoassay to identify new analytes correlating to SMA motor function. These immunoassays included the strongest candidate biomarkers identified previously by chromatography. We selected 35 biomarkers to validate in an independent cohort SMA type 1, 2, and 3 samples (N = 158 from an SMA NHS. The putative biomarkers were tested for association to multiple motor scales and to pulmonary function, neurophysiology, strength, and quality of life measures. We implemented a Tobit model to predict SMA motor function scores. RESULTS: 12 of the 35 putative SMA biomarkers were significantly associated (p<0.05 with motor function, with a 13(th analyte being nearly significant. Several other analytes associated with non-motor SMA outcome measures. From these 35 biomarkers, 27 analytes were selected for inclusion in a commercial panel (SMA-MAP for association with motor and other functional measures. CONCLUSIONS: Discovery and validation using independent cohorts yielded a set of SMA biomarkers significantly associated with motor function and other measures of SMA disease activity. A commercial SMA-MAP biomarker panel was generated for further testing in other SMA collections and interventional trials. Future work includes evaluating the panel in other

  16. Resilience Post-Disaster of Students SMA Negeri in Padang

    Directory of Open Access Journals (Sweden)

    Ifdil Ifdil

    2012-03-01

    Full Text Available Penelitian ini bertujuan untuk mengungkapkan tingkat resiliensi siswa, dan perbedaan tingkat resiliensi siswa SMA Negeri Pasca bencana di Kota Padang berdasarkan jenis kelamin, dan lokasi sekolah. Pemilihan sampel dilakukan secara Cluster Random Sampling sampling yang dibagi menjadi 3 (tiga kelompok yaitu sekolah di wilayah bagian Pusat Kota, Tengah Kota dan Pinggiran Kota Padang. Dari hasil penelitian diperoleh tingkat resiliensi siswa SMA Negeri pasca bencana di Kota Padang pada kategori sangat rendah 7,74%, rendah 34,19%, sedang 32,25%, tinggi 20% dan sangat tinggi 5,80%. Kemudian tidak terdapat perbedaan yang signifikan antara resiliensi siswa SMA Negeri pasca bencana di Kota Padang berdasarkan jenis kelamin, lokasi sekolah. Temuan penilitian ini selanjutnya dijadikan dasar penting  perlunya layanan bimbingan dan konseling yang terfokus pada resiliensi siswa pasca bencana di Kota Padang.

  17. Graphical design for thin-film SMA microactuators

    Science.gov (United States)

    Ishida, A.; Sato, M.; Yoshikawa, W.; Tabata, O.

    2007-10-01

    Simple graphical designs for bridge- and diaphragm-type actuators using shape-memory alloy (SMA) thin films are proposed. The performance (force and displacement) of these actuators is predicted on the basis of the stress-strain curves of an SMA film by introducing the material parameter K that represents the mechanical properties of both the austenite and martensite films. The methods of designing actuators are presented along with numerical examples and their validity is discussed, referring to some actual devices such as a microvalve and a micropump. A comparison of theory and actual device performance shows that the proposed design gives a useful approximation for practical applications. The advantage of the proposed design method is that, once the value of K is obtained for a given SMA film, one can design various actuators with various dimensions without detailed information about its mechanical properties.

  18. A New Bistable SmA Display Mode

    Science.gov (United States)

    Chen, Hui-Yu; Shao, Renfan; Korblova, Eva; Walba, David; Lee, Wei; Clark, Noel A.

    2007-03-01

    In the traditional SmA display, crossed polarizers are absent and one can switch a light transparent state to an opaque light scattering state by using laser addressing or electric addressing. Such displays are bright, but of only moderate contrast ratio. Here, we present a new operation mode for a SmA display using two sets of electrodes, with one to induce homeotropic orientation and the other having an in-plane structure to induce planar orientation. This switching with crossed polarizer and analyzer enables a high contrast, bistable electro-optical effect. This SmA display mode exhibits a high contrast ratio (2500:1) for non-striped ITO pattern cells, prefect bistability, and reasonably fast switching (a few ms). These characteristics may enable potential applications on e-paper.

  19. Adaptive and energy efficient SMA-based handling systems

    Science.gov (United States)

    Motzki, P.; Kunze, J.; Holz, B.; York, A.; Seelecke, S.

    2015-04-01

    Shape Memory Alloys (SMA's) are known as actuators with very high energy density. This fact allows for the construction of very light weight and energy-efficient systems. In the field of material handling and automated assembly process, the avoidance of big moments of inertia in robots and kinematic units is essential. High inertial forces require bigger and stronger robot actuators and thus higher energy consumption and costs. For material handling in assembly processes, many different individual grippers for various work piece geometries are used. If one robot has to handle different work pieces, the gripper has to be exchanged and the assembly process is interrupted, which results in higher costs. In this paper, the advantages of using high energy density Shape Memory Alloy actuators in applications of material-handling and gripping-technology are explored. In particular, light-weight SMA actuated prototypes of an adaptive end-effector and a vacuum-gripper are constructed via rapid-prototyping and evaluated. The adaptive end-effector can change its configuration according to the work piece geometry and allows the handling of multiple different shaped objects without exchanging gripper tooling. SMA wires are used to move four independent arms, each arm adds one degree of freedom to the kinematic unit. At the tips of these end-effector arms, SMA-activated suction cups can be installed. The suction cup prototypes are developed separately. The flexible membranes of these suction cups are pulled up by SMA wires and thus a vacuum is created between the membrane and the work piece surface. The self-sensing ability of the SMA wires are used in both prototypes for monitoring their actuation.

  20. Linewidth of submillimeter wave flux-flow oscillators

    DEFF Research Database (Denmark)

    Koshelets, V.P.; Shitov, S.V.; Shchukin, A.V.

    1996-01-01

    A reliable technique for wide band measurements of the spectral linewidth of superconducting oscillators integrated on-chip with superconductor-insulator-superconductor (SIS) detectors has been, developed, The spectral linewidth of flux-flow oscillators (FFO) based on the unidirectional and visco...... reference source has been demonstrated. The proposed technique may improve the sensitivity, frequency resolution, and stability of the fully superconducting integrated submillimeter wave receiver. (C) 1996 American Institute of Physics....

  1. Passive magnetic shielding for the submillimeter and far infrared experiment

    Energy Technology Data Exchange (ETDEWEB)

    Kamiya, Koji; Warner, B.A.; Di Pirro, M.J.; Numazawa, Takenori

    2003-05-01

    Goddard Space Flight Center is developing the submillimeter and far infrared experiment (SAFIRE). SAFIRE will use SQUIDs as amplifiers for detectors, which must be shielded from the magnet cooling system, an adiabatic demagnetization refrigerator (ADR). The magnetic field at the detector package must remain at or below the 10{sup -7} tesla level while the detectors are operating. We discuss laboratory tests of the passive shielding and simulations.

  2. Laying the foundation stone of CERN Building SMA18

    CERN Multimedia

    Patrice Loiez

    1999-01-01

    Photo 10 : Le Directeur general du CERN, Luciano Maiani inaugure avec le President du Conseil general de l'Ain, M. Jean Pepin, la 1ere pierre du futur batiment SMA 18 a Prevessin-Moens. Photo 14 : Discours du President du Conseil general de l'Ain, M. Jean Pepin lors de la pose de la 1ere pierre au futur batiment SMA 18. Photo 15 : CERN director-general L. Maiani speaks at the official ceremony to lay the foundation stone of a new CERN building.

  3. Mezclas SMA (Stone Mastic Asphalt) con alto contenido de ligante

    OpenAIRE

    Costa, Andrés; Cervantes, Rocío; Loma, Javier; Hidalgo, María Elena; Hergueta, José Antonio; Sánchez, Fernando; Lanchas, Santiago; Núñez, Ruy; Rubio, Baltasar; Jiménez, Rafael; Pérez Jiménez, Félix Edmundo; Botella Nieto, Ramón; Expósito, Santiago; Fernández, Victoriano; Potti, Juan José

    2013-01-01

    Las denominadas mezclas bituminosas en caliente SMA (Stone Mastic Asphalt) están recogidas en la normativa UNE EN 13108-5 y aunque en España apenas se han utilizado, su uso esta extendido por todo el mundo. Un grupo de empresas y algunos centros de investigación españoles, estamos desarrollando un proyecto de investigación denominado: Mezclas SMA de la familia de la norma UNE EN 13108-5 que sean Sostenibles y Medioambientalmente Amigables. Financiado por el Centro Tecnológico para el Desarrol...

  4. Analysis of the Sub-Millimeter Rotational Spectrum of Urea

    Science.gov (United States)

    Thomas, Jessica R.; Fosnight, Alyssa M.; Medvedev, Ivan R.

    2013-06-01

    Urea, ((NH_{2})_{2}CO), has broad presence in biological species. As a byproduct of human metabolism, this molecule is commonly tested for in blood to diagnose different pathologies. Furthermore, urea is seen in interstellar medium and its detection could yield valuable insight into the mechanisms governing star formation. Despite the prevalence of urea, an absence exists in recorded frequencies of this molecule. The new generation of the sub-millimeter telescopes, such as ALMA, HERSCHEL, and SOFIA, allows detection of interstellar molecular spectra at unprecedented spatial and spectral resolutions. The knowledge of the precise frequencies of spectra transitions present in interstellar molecular clouds would alleviate the problem of spectral congestion and aid in molecular identification. This paper reports the most recent investigation of the submillimeter/terahertz gas phase spectrum of urea. Up until now, only the microwave laboratory spectrum of urea's vibrational ground state has been available. This paper reports the high-resolution spectra of urea in the sub-millimeter range, and extends the spectroscopic assignment of the rotational transitions in the vibrational ground state. Additionally, the assignment of the first vibrational state and tentative assignments of two additional vibrational states have been made.

  5. A SUBMILLIMETER CONTINUUM SURVEY OF LOCAL DUST-OBSCURED GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Lee, Jong Chul [Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055 (Korea, Republic of); Hwang, Ho Seong [School of Physics, Korea Institute for Advanced Study, 85 Hoegiro, Dongdaemun-gu, Seoul 02455 (Korea, Republic of); Lee, Gwang-Ho, E-mail: jclee@kasi.re.kr [Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742 (Korea, Republic of)

    2016-12-20

    We conduct a 350 μ m dust continuum emission survey of 17 dust-obscured galaxies (DOGs) at z = 0.05–0.08 with the Caltech Submillimeter Observatory (CSO). We detect 14 DOGs with S{sub 350μm} = 114–650 mJy and signal-to-noise > 3. By including two additional DOGs with submillimeter data in the literature, we are able to study dust content for a sample of 16 local DOGs, which consist of 12 bump and four power-law types. We determine their physical parameters with a two-component modified blackbody function model. The derived dust temperatures are in the range 57–122 K and 22–35 K for the warm and cold dust components, respectively. The total dust mass and the mass fraction of the warm dust component are 3–34 × 10{sup 7} M {sub ⊙} and 0.03%–2.52%, respectively. We compare these results with those of other submillimeter-detected infrared luminous galaxies. The bump DOGs, the majority of the DOG sample, show similar distributions of dust temperatures and total dust mass to the comparison sample. The power-law DOGs show a hint of smaller dust masses than other samples, but need to be tested with a larger sample. These findings support that the reason DOGs show heavy dust obscuration is not an overall amount of dust content, but probably the spatial distribution of dust therein.

  6. Achieving dynamic switchable filter based on a transmutable metasurface using SMA

    Science.gov (United States)

    Chen, Xin; Gao, Jinsong; Kang, Bonan

    2017-09-01

    We propose a switchable filter composed of transmutable array using shape memory alloys (SMA). It could exhibit a temperature induced morphology change spontaneously like the biological excitability, acting as a shutter that allows the incident energy to be selectively transmitted or reflected with in excess of 12dB isolation at the certain frequencies for both polarizations. Equivalent circuit models describe the operational principle qualitatively and the switching effect is underpinned by the full-wave analysis. A further physical mechanism is shown by contrasting the distributions of electric field and surface current on the surface at the same frequency for the two working modes. The experimental results consist with the theoretical simulations, indicating that the metasurface could serve as one innovative solution for manipulating the electromagnetic waves and enlighten the next generation of advanced electromagnetic materials with more freedom in the processes of design and manufacturing.

  7. Pemanfaatan Informasi Olahraga di Media Massa Cetak oleh Guru Pendidikan Jasmani dan Kesehatan dalam Pembelajaran Pendidikan Jasmani dan Kesehatan di SMA 5, SMA 6, SMA 11 Semarang

    Directory of Open Access Journals (Sweden)

    Muhaimin Muhaimin

    2011-01-01

    Full Text Available Utilization of information in mass media print by master of physical education and health in physical education and health in SMA 5, SMA 6, SMA 11 Semarang. The presence of print media is now a community needs. That's because, the print media presents a variety of information including information of actual politics, culture, economy, crime, entertainment, and sports. Basically, sports information in the print media have educational value and can add insight to a reading of new knowledge. The study produced these findings: (1 third physical education and health teacher at school who becomes the object research have made use of sports information in the print media to support the success of teaching and learning process, (2 the type of information they use to support the success of learning teaching is a form of news, articles about health, (3 form of utilization is appropriate to set clipping and through direct delivery of the material in the field while providing practice in the field. This method is considered more effective because all students can immediately practice, (4 sports information in the print media meets the needs of teachers and physical health education in supporting the learning process.

  8. Research Status and Action of Sub-millimeter Debris Impact Damage on Spacecraft Structure

    OpenAIRE

    Higashide, Masumi; Kurosaki, Hirohisa; Hasegawa, Sunao; 東出, 真澄; 黒崎, 裕久; 長谷川, 直

    2015-01-01

    To assess debris impact risk for the satellite, submillimeter debris impact damage has not been investigated enough to conduct satellite protective designing. JAXA is researching vulnerability of satellite structure materials against submillimeter debris impact, and proposing shielding methods. This report shows summary of submillimeter impact damages of honeycomb sandwich panels. The damage of the panel was investigated by hypervelocity impact experiments with the two-stage light gas gun in ...

  9. Aplikasi Sistem Pembayaran Administrasi Kesiswaan Di SMA Ya BAKII Kesugihan

    Directory of Open Access Journals (Sweden)

    Novi Ika Atikah

    2011-11-01

    Full Text Available Sekolah sebagai salah satu bentuk organisasi memerlukan pengolahan administrasi yang efektif dan efisien, yaitu berorientasi pada tujuan penggunaan semua sumber daya serta mekanisme pengelolaan sekolah. Salah satu fungsi administrasi sekolah adalah pengelolaan data pembayaran administrasi kesiswaan. Yang terjadi di SMA Ya BAKII Kesugihan yang masih menggunakan sistem manual dalam pengelolaan data pembayaran. Dengan memanfaatkan software komputer kita dapat mengelola data-data pembayaran administrasi kesiswaan dengan lebih mudah.  Dalam kegiatan ini mencakup bagaimana perancangan program basis data tentang pengelolaan data pembayaran sekolah di SMA Ya BAKII Kesugihan dengan menggunakan software Visual Basic 6.0 dan MySQL Server 5.1. Hasil dari perancangan dan pembuatan Aplikasi Sistem Pembayaran Administrasi Kesiswaan di SMA Ya BAKII Kesugihan adalah untuk mengoptimalisasikan pengolahan data pembayaran administrasi kesiswaan. Aplikasi ini dapat menghasilkan laporan-laporan yang dapat digunakan oleh bagian Tata Usaha lain yang berkaitan dengan administrasi kesiswaan. Berdasarkan hasil kegiatan di atas, pihak Sekolah disarankan dapat meningkatkan kualitas dan pengelolaan sekolah terutama bagian pembayaran administrasi kesiswaan di SMA Ya BAKII Kesugihan.

  10. Transfer bonding technology for batch fabrication of SMA microactuators

    Science.gov (United States)

    Grund, T.; Guerre, R.; Despont, M.; Kohl, M.

    2008-05-01

    Currently, the broad market introduction of shape memory alloy (SMA) microactuators and sensors is hampered by technological barriers, since batch fabrication methods common to electronics industry are not available. The present study intends to overcome these barriers by introducing a wafer scale transfer process that allows the selective transfer of heat-treated and micromachined shape memory alloy (SMA) film or foil microactuators to randomly selected receiving sites on a target substrate. The technology relies on a temporary adhesive bonding layer between SMA film/foil and an auxiliary substrate, which can be removed by laser ablation. The transfer technology was tested for microactuators of a cold-rolled NiTi foil of 20 μm thickness, which were heat-treated in free-standing condition, then micromachined on an auxiliary substrate of glass, and finally selectively transferred to different target substrates of a polymer. For demonstration, the new technology was used for batch-fabrication of SMA-actuated polymer microvalves.

  11. Influence of SMA reinforcement on the impact resistance of GFRP ...

    Indian Academy of Sciences (India)

    Home; Journals; Bulletin of Materials Science; Volume 39; Issue 3. Influence of SMA reinforcement on the impact resistance of GFRP composite laminates under different temperatures. K PAZHANIVEL G B BHASKAR A ELAYAPERUMAL P ANANDAN S ARUNACHALAM. Volume 39 Issue 3 June 2016 pp 889-899 ...

  12. Advanced Amplifier Based Receiver Front Ends for Submillimeter-Wave-Sounders Project

    Data.gov (United States)

    National Aeronautics and Space Administration — Develop high electron mobility transistor (HEMT) amplifier based heterodyne radiometers to provide high sensitivity at millimeter and submillimeter wavelengths with...

  13. KONSTRUKSI SOSIAL TERHADAP PENDIDIKAN MUSIK SMA PONDOK MODERN SELAMAT KENDAL

    Directory of Open Access Journals (Sweden)

    Nurmila Sari Djau

    2015-08-01

    Full Text Available Tujuan dari penelitian ini adalah untuk mengkaji konstruksi sosial terhadap pendidikan musik oleh lembaga pendidikan Islam dan peran sekolah dala membangun orientasi musik yang bersifat sekuler pada siswa. Adanya kesenjangan antara konsep pendidikan seni menurut pandangan Islam dengan paham pendidikan musik yang dilaksanakan pada SMA Pondok Modern Selamat selaku lembaga pendidikan berbasis Islam. Melalui bentuk pengajaran musik yang bersifat bebas baik sekuler maupun religi secara tidak langsung dapat membangun orientasi musik yang berbeda di setiap siswa. Pendekatan penelitian ini adalah sosiologi dengan menggunakan metode penelitian kualitatif. Lokasi penelitian adalah SMA Pondok Modern Selamat yang berada di Kendal. Hasil Penelitian ini menunjukkan bahwa Konstruksi sosial oleh SMA Pondok Modern Selamat tentang pendidikan musik adalah pendidikan musik dianggap sebagai wadah untuk mengekspresikan diri dan wadah untuk mewariskan budaya bangsa yang tercermin dalam penerapan pembelajaran musik yang bersifat sekuler maupun islami sehingga secara tidak langsung mempengaruhi atau membangun musik pada siswa terhadap suatu jenis musik. The purpose of this study was to examine the social construction of the educational music by Islamic educational institutions and the role of schools dala building orientation secular music to students. The gap between the concept of art education in the view of Islam to understand the music education conducted at SMA Pondok Modern Selamat as the Islamic-based educational institutions. Through teaching form of music that is free both secular and religious can indirectly establish the orientation of different music in each student. This study is sociological approach using qualitative research methods. Location of the study is the high school Pondok Modern Selamat located in Kendal. The results of this study indicate that the social construction by SMA Pondok Modern Selamat on music education music education is

  14. Confirmation of clinical diagnosis in requests for prenatal prediction of SMA type I

    NARCIS (Netherlands)

    Cobben, J. M.; de Visser, M.; Scheffer, H.; Osinga, J.; van der Steege, G.; Buys, C. H.; van Ommen, G. J.; ten Kate, L. P.

    1993-01-01

    The recent discovery of a major SMA-locus in the chromosomal region 5q makes it possible to carry out prenatal DNA studies in families in which a child with SMA type I has been born. Since direct mutation analysis is not yet possible, the reliability of prenatal prediction of SMA type I usually

  15. CONFIRMATION OF CLINICAL-DIAGNOSIS IN REQUESTS FOR PRENATAL PREDICTION OF SMA TYPE-I

    NARCIS (Netherlands)

    COBBEN, JM; DEVISSER, M; SCHEFFER, H; OSINGA, J; VANDERSTEEGE, G; BUYS, CHCM; VANOMMEN, GJ; TENKATE, LP

    The recent discovery of a major SMA-locus in the chromosomal region 5q makes it possible to carry out prenatal DNA studies in families in which a child with SMA type I has been born. Since direct mutation analysis is not yet possible, the reliability of prenatal prediction of SMA type I usually

  16. Superconductor Semiconductor Research for NASA's Submillimeter Wavelength Missions

    Science.gov (United States)

    Crowe, Thomas W.

    1997-01-01

    Wideband, coherent submillimeter wavelength detectors of the highest sensitivity are essential for the success of NASA's future radio astronomical and atmospheric space missions. The critical receiver components which need to be developed are ultra- wideband mixers and suitable local oscillator sources. This research is focused on two topics, (1) the development of reliable varactor diodes that will generate the required output power for NASA missions in the frequency range from 300 GHZ through 2.5 THz, and (2) the development of wideband superconductive mixer elements for the same frequency range.

  17. Solar Science with the Atacama Large Millimeter/Submillimeter Array—A New View of Our Sun

    Science.gov (United States)

    Wedemeyer, S.; Bastian, T.; Brajša, R.; Hudson, H.; Fleishman, G.; Loukitcheva, M.; Fleck, B.; Kontar, E. P.; De Pontieu, B.; Yagoubov, P.; Tiwari, S. K.; Soler, R.; Black, J. H.; Antolin, P.; Scullion, E.; Gunár, S.; Labrosse, N.; Ludwig, H.-G.; Benz, A. O.; White, S. M.; Hauschildt, P.; Doyle, J. G.; Nakariakov, V. M.; Ayres, T.; Heinzel, P.; Karlicky, M.; Van Doorsselaere, T.; Gary, D.; Alissandrakis, C. E.; Nindos, A.; Solanki, S. K.; Rouppe van der Voort, L.; Shimojo, M.; Kato, Y.; Zaqarashvili, T.; Perez, E.; Selhorst, C. L.; Barta, M.

    2016-04-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can address a broad range of fundamental scientific questions in solar physics. The radiation observed by ALMA originates mostly from the chromosphere—a complex and dynamic region between the photosphere and corona, which plays a crucial role in the transport of energy and matter and, ultimately, the heating of the outer layers of the solar atmosphere. Based on first solar test observations, strategies for regular solar campaigns are currently being developed. State-of-the-art numerical simulations of the solar atmosphere and modeling of instrumental effects can help constrain and optimize future observing modes for ALMA. Here we present a short technical description of ALMA and an overview of past efforts and future possibilities for solar observations at submillimeter and millimeter wavelengths. In addition, selected numerical simulations and observations at other wavelengths demonstrate ALMA's scientific potential for studying the Sun for a large range of science cases.

  18. Fatigue crack behavior on a Cu-Zn-Al SMA

    Directory of Open Access Journals (Sweden)

    V. Di Cocco

    2014-10-01

    Full Text Available In recent years, mechanical property of many SMA has improved in order to introduce these alloys in specific field of industry. Main examples of these alloys are the NiTi, Cu-Zn-Al and Cu-Al-Ni which are used in many fields of engineering such as aerospace or mechanical systems. Cu-Zn-Al alloys are characterized by good shape memory properties due to a bcc disordered structure stable at high temperature called β-phase, which is able to change by means of a reversible transition to a B2 structure after appropriate cooling, and reversible transition from B2 secondary to DO3 order, under other types of cooling. In β-Cu-Zn-Al shape memory alloys, the martensitic transformation is not in equilibrium at room temperature. It is therefore often necessary to obtain the martensitic structure, using a thermal treatment at high temperature followed by quenching. The martensitic phases can be either thermally-induced spontaneous transformation, or stressinduced, or cooling, or stressing the β- phase. Direct quenching from high temperatures to the martensite phase is the most effective because of the non-diffusive character of the transformation. The martensite inherits the atomic order from the β-phase. Precipitation of many kinds of intermetallic phases is the main problem of treatment on cu-based shape memory alloy. For instance, a precipitation of α-phase occurs in many low aluminum copper based SMA alloy and presence of α-phase implies a strong degradation of shape recovery. However, Cu-Zn-Al SMA alloys characterized by aluminum contents less than 5% cover a good cold machining and cost is lower than traditional NiTi SMA alloys. In order to improve the SMA performance, it is always necessary to identify the microstructural changing in mechanical and thermal conditions, using X-Ray analyses. In this work a Cu-Zn-Al SMA alloy obtained in laboratory has been microstructurally and metallographically characterized by means of X-Ray diffraction and Light

  19. Thousand-Element Multiplexed Superconducting Bolometer Arrays

    Science.gov (United States)

    Benford, Dominic; Chervenak, Jay; Voellmer, George; Staguhn, Johannes; Shafer, Rick; Stacey, Gordon; Irwin, Kent

    Large format, two-dimensional arrays of close-packed bolometers will enable submillimeter cameras and spectrometers to obtain images and spectra orders of magnitude faster than present instruments. The South Pole Imaging Fabry-Perot Interferometer (SPIFI) for the AST/RO observatory and the Submillimeter and Far-InfraRed Experiment (SAFIRE) on the SOFIA airborne observatory will employ a large-format, two-dimensional, close-packed bolometer arrays. Both these instruments are imaging Fabry-Perot spectrometers operating at wavelengths between 100μm and 700μm. The array format is 16x32 pixels, using a 32-element multiplexer developed in part for this purpose. The low backgrounds achieved in spectroscopy require very sensitive detectors with NEPs of order 5x10-18 W/Hz1/2. Superconducting detectors can be close-packed using the Pop-Up Detector (PUD) format, and SQUID multiplexers operating at the detector bas temperature can be intimately coupled to them. We are fabricating an engineering model array with this technology which features a very compact, modular approach for large format arrays.

  20. Properties of Submillimeter Galaxies in the CANDELS GOODS-South Field

    NARCIS (Netherlands)

    Wiklind, Tommy; Conselice, Christopher J.; Dahlen, Tomas; Dickinson, Mark E.; Ferguson, Henry C.; Grogin, Norman A.; Guo, Yicheng; Koekemoer, Anton M.; Mobasher, Bahram; Mortlock, Alice; Fontana, Adriano; Davé, Romeel; Yan, Haojing; Acquaviva, Viviana; Ashby, Matthew L. N.; Barro, Guillermo; Caputi, Karina I.; Castellano, Marco; Dekel, Avishai; Donley, Jennifer L.; Fazio, Giovanni G.; Giavalisco, Mauro; Grazian, Andrea; Hathi, Nimish P.; Kurczynski, Peter; Lu, Yu; McGrath, Elizabeth J.; de Mello, Duilia F.; Peth, Michael; Safarzadeh, Mohammad; Stefanon, Mauro; Targett, Thomas

    We derive physical properties of 10 submillimeter galaxies located in the CANDELS coverage of the GOODS-S field. The galaxies were first identified as submillimeter sources with the LABOCA bolometer and subsequently targeted for 870 μm continuum observation with ALMA. The high angular resolution of

  1. InP HEMT Integrated Circuits for Submillimeter Wave Radiometers in Earth Remote Sensing

    Science.gov (United States)

    Deal, William R.; Chattopadhyay, Goutam

    2012-01-01

    The operating frequency of InP integrated circuits has pushed well into the Submillimeter Wave frequency band, with amplification reported as high as 670 GHz. This paper provides an overview of current performance and potential application of InP HEMT to Submillimeter Wave radiometers for earth remote sensing.

  2. Pelaksanaan Pendidikan Agama di SMA Katolik Soverdi Kabupaten Badung Bali

    Directory of Open Access Journals (Sweden)

    Mulyani Mudis Taruna

    2010-12-01

    Full Text Available This research was conducted at SMA Catholic Soverdi under umbrella ofCatholic foundation in Badung district Bali Province. Focuses of this study are,implementation of religious education was seen from the aspects of curriculumimplementation, influencing factors of curriculum implementation. Thisis a qualitative research. Finding of the research depicts that developmentof the religious education’s curriculum uses curriculum set by ministry ofeducation. This affects in developing of atmosphere of religious life at school.Substantially, implementation of curriculum on religious education areable to provide services for students, namely giving religious education fitwith students’ religion, and the teacher’s religion is the same as student’s religion.DI SMA KATOLIK SOVERDI KABUPATEN BADUNG BALIKeywords : Relegius education, curiculum

  3. Josephson frequency meter for millimeter and submillimeter wavelengths

    Energy Technology Data Exchange (ETDEWEB)

    Anischenko, S.E.; Larkin, S.Y.; Chaikovsky, V.I. [State Research Center, Kiev (Ukraine)] [and others

    1994-12-31

    Frequency measurements of electromagnetic oscillations of millimeter and submillimeter wavebands with frequency growth due to a number of reasons become more and more difficult. First, these frequencies are considered to be cutoff for semiconductor converting devices and one has to use optical measurement methods instead of traditional ones with frequency transfer. Second, resonance measurement methods are characterized by using relatively narrow bands and optical ones are limited in frequency and time resolution due to the limited range and velocity of movement of their mechanical elements as well as the efficiency of these optical techniques decreases with the increase of wavelength due to diffraction losses. That requires the apriori information on the radiation frequency band of the source involved. Method of measuring frequency of harmonic microwave signals in millimeter and submillimeter wavebands based on the ac Josephson effect in superconducting contacts is devoid of all the above drawbacks. This approach offers a number of major advantages over the more traditional measurement methods, that is the one based on frequency conversion, resonance and interferrometric techniques. It can be characterized by high potential accuracy, wide range of frequencies measured, prompt measurement and the opportunity to obtain panoramic display of the results as well as full automation of the measuring process.

  4. A Sub-millimeter, Inductively Powered Neural Stimulator

    Directory of Open Access Journals (Sweden)

    Daniel K. Freeman

    2017-11-01

    Full Text Available Wireless neural stimulators are being developed to address problems associated with traditional lead-based implants. However, designing wireless stimulators on the sub-millimeter scale (<1 mm3 is challenging. As device size shrinks, it becomes difficult to deliver sufficient wireless power to operate the device. Here, we present a sub-millimeter, inductively powered neural stimulator consisting only of a coil to receive power, a capacitor to tune the resonant frequency of the receiver, and a diode to rectify the radio-frequency signal to produce neural excitation. By replacing any complex receiver circuitry with a simple rectifier, we have reduced the required voltage levels that are needed to operate the device from 0.5 to 1 V (e.g., for CMOS to ~0.25–0.5 V. This reduced voltage allows the use of smaller receive antennas for power, resulting in a device volume of 0.3–0.5 mm3. The device was encapsulated in epoxy, and successfully passed accelerated lifetime tests in 80°C saline for 2 weeks. We demonstrate a basic proof-of-concept using stimulation with tens of microamps of current delivered to the sciatic nerve in rat to produce a motor response.

  5. Structured Antireflective Coating for Silicon at Submillimeter Frequencies

    Science.gov (United States)

    Padilla, Estefania

    2018-01-01

    Observations at millimeter and submillimeter wavelengths are useful for many astronomical studies, such as the polarization of the cosmic microwave background or the formation and evolution of galaxy clusters. In order to allow observations over a broad spectral bandwidth (approximatively from 70 to 420 GHz), innovative broadband anti-reflective (AR) optics must be utilized in submillimeter telescopes. Due to its low loss and high refractive index, silicon is a fine optical material at these frequencies, but an AR coating with multiple layers is required to maximize its transmission over a wide bandwidth. Structured multilayer AR coatings for silicon are currently being developed at Caltech and JPL. The development process includes the design of the structured layers with commercial electromagnetic simulation software, the fabrication by using deep reactive ion etching, and the test of the transmission and reflection of the patterned wafers. Geometrical 3D patterns have successfully been etched at the surface of the silicon wafers creating up to 2 layers with different effective refractive indices. The transmission and reflection of single AR layer wafers, measured between 75 and 330 GHz, are close to the simulation predictions. These results allow the development of new designs with 5 or 6 AR layers in order to improve the bandwidth and transmission of the silicon AR coatings.

  6. Pelaksanaan Pendidikan Agama di SMA Katolik Soverdi Kabupaten Badung Bali

    OpenAIRE

    Taruna, Mulyani Mudis

    2010-01-01

    This research was conducted at SMA Catholic Soverdi under umbrella ofCatholic foundation in Badung district Bali Province. Focuses of this study are,implementation of religious education was seen from the aspects of curriculumimplementation, influencing factors of curriculum implementation. Thisis a qualitative research. Finding of the research depicts that developmentof the religious education’s curriculum uses curriculum set by ministry ofeducation. This affects in developing of atmosphere ...

  7. IDENTIFICATION OF KEY RECOMBINANTS IN MULTIPLEX SMA FAMILIES

    NARCIS (Netherlands)

    VANDERSTEEGE, G; COBBEN, JM; BRAHE, C; OSINGA, J; ZAPPATA, S; SCHEFFER, H; NERI, G; VANOMMEN, GJB; BUYS, CHCM; TENKATE, LP

    1994-01-01

    Recent reports have provided evidence that a major gene for autosomal recessive proximal spinal muscular atrophy (SMA) resides in a small genetic interval in bands q12-q13 of chromosome 5, a 4-cM region proximally flanked by D5S125 (EF(TG/AG)n) and distally by MAP1B/D5S112 or a 0.7-cM interval

  8. FAKTOR-FAKTOR PENENTU KOMITMEN ORGANISASI GURU SMA

    Directory of Open Access Journals (Sweden)

    Tiur Asi Siburian

    2013-05-01

    Full Text Available Abstract: Factors Determining Organization Commitment of Senior High School Teachers. This survey aims to examine the effects of interpersonal communication, organization culture, job satisfaction, and achievement motivation on the organization commitment of senior high school teachers. Utilizing questionnaires distributed to 150 respondents, this study found that teachers’ organization commitment was directly as well as indirectly affected by the variables of interpersonal communication, organization culture, job satisfaction, and achievement motivation. Abstrak: Faktor-faktor Penentu Komitmen Organisasi Guru SMA. Tujuan penelitian adalah untuk menguji pengaruh komunikasi interpersonal, budaya organisasi, kepuasan kerja, dan motivasi berprestasi terhadap komitmen organisasi guru SMA Negeri di Kabupaten Humbang Hasundutan. Penelitian memggunakan desain eksplanatif, dan pengambilan data dilakukan melalui survey pada 150 responden yang diambil dengan sampling random proporsional. Hasil penelitian menunjukkan bahwa komitmen or­ganisasi guru SMA dipengaruhi secara langsung dan tidak langsung oleh empat variabel, yaitu komunikasi interpersonal, budaya organisasi, kepuasan kerja, dan motivasi berprestasi. Temuan penelitian menunjuk­kan bahwa keempat variabel tersebut masih perlu ditingkatkan lebih lanjut.

  9. KEEFEKTIFAN TEKNIK RELAKSASI UNTUK MENURUNKAN STRES AKADEMIK SISWA SMA

    Directory of Open Access Journals (Sweden)

    Suyono Suyono

    2016-08-01

    Full Text Available Abstract: This study aims at examining the effectiveness of relaxation techniques to release students’stress and tension regarding academic within Senior High School Assádah in Gresik City. This study employed quasi-experiment design using one group pretest-posttest model. The data of this study were obtained through academic stress inventory to attain a depiction of stress level encountered by the subject. The subjects of this study were seven students of Tenth Graders in SMA Assaadah Bungah Gresik who experienced low to average stress regarding exam preparation. The data were, then, analyzed by using Wilcoxon Statistic Analysis. The result of the study indicated that relaxation technique could lower and release the level of students stress in exam preparation. Key Words: relaxation technique, student academic stress   Abstrak: Penelitian ini bertujuan untuk  menguji keefektifan teknik relaksasi untuk menurunkan stres akademik siswa SMA Ass’adah di Kota Gresik dengan menggunakan rancangan kuasi eksperimen dengan model “one group pretest posttest design. Pengumpulan data dengan menggunakan inventori stres akademik tujuannya untuk memperoleh gambaran tingkat stres akademik pada subjek penelitian. Subjek penelitian adalah siswa yang mengalami stres akademik sedang dan rendah  dalam menghadapi ujian berjumlah 7 orang siswa pada kelas X SMA Assaadah Bungah Gresik. Teknik analisis data dengan menggunakanan analisis statistic Wilcoxon. Hasil penelitian menunjukkan adanya penurunan tingkat stres akademik menjelang ujian sesudah subjek mendapatkan layanan dengan teknik  relaksasi. Kata kunci: Teknik relaksasi, stres akademik siswa

  10. Pengembangan Program Macromedia Flash 8 untuk Pembelajaran Fisika di SMA

    Directory of Open Access Journals (Sweden)

    Wiji Susilowati

    2007-12-01

    Full Text Available Tujuan penelitian adalah membuat dan mengevaluasi media pembelajaran fisika SMA menggunakan program Macromedia Flash 8. Subjek coba pada penelitian ini berjumlah 40 orang yang terdiri dari 10 siswa untuk uji coba instrumen penelitian, 10 siswa untuk ujicoba kelompok kecdl, dan 20 siswa untuk uji coba lapangan. Pengumpulan data dilakukan dengan mengguna­kan kuesioner dan tes fisika (pre-test dan post-test. Evaluasi terhadap program ditinjau dari aspek pembelajaran dan aspek media. Kritik dan saran digunakan untuk memperbaiki program. Hasil penelitian menunjukkan bahwa program Macromedia Flash 8 untuk pembelajaran fisika di SMA: (1 dirancang sesuai dengan prinsip-prinsip desain pembelajaran, (2 terbukti mampu menaikkan skor rerata tes fisika siswa sebesar 55,42%, (3 memiliki efisiensi waktu yang tinggi, (4 ditinjau dari aspek media Hinilai cukup bagus/menarik (dinilai/dikategorikan sedang oleh siswa, (5 ditinjau dari aspek pembelajaran secara keseluruhan program ini dinilai tinggi/jelas dimengerti oleh siswa, (6 ditinjau dari aspek media dinilai menarik (bagus/kategori tinggi oleh guru fisika, dan (7 ditinjau dari aspek pembelajaran juga dinilai menarik (bagus/kategori tinggi oleh guru fisika. Kata kunci: media pembelajaran fisika diSMA.

  11. ASPIRASI KARIER SISWA SMA BERDASARKAN STATUS SOSIAL EKONOMI DAN GENDER

    Directory of Open Access Journals (Sweden)

    Nunik Widiastuti

    2017-07-01

    Full Text Available Career Aspirations of SMA Students Based Socio-Economic Status and Gender. This research is a descriptive study about career aspirations aimed to describe the career aspirations of students by socio-economic status and gender in SMA Negeri 1 Batujajar. The method used the quantitative descriptive method. Respondents in this study are students of class X SMA Negeri 1 Batujajar that are at the stage of self-orientation. At this stage people start selecting, establishing and looking for alternatives on the planning himself and his work. Selection of the sample using purposive sampling techniques so that the respondents in this study were 234 students. In general, the career aspirations of students 10.3% were in the low category, which is the category of being as much as 63.2%, and 26.5 % At the high category. Based on the socio-economic status of education last seen parents are in the moderate category. Based on parent income in middle category. Meanwhile, based on the gender ratio of the career aspirations of learners battery and men do not have a difference, with a probability value of 0.53.

  12. Implementation of vortex wake control using SMA-actuated devices

    Science.gov (United States)

    Quackenbush, Todd R.; Bilanin, Alan J.; Batcho, P. F.; McKillip, Robert M., Jr.; Carpenter, Bernie F.

    1997-05-01

    Mitigation of the undesirable effects of trailing vortex wakes has been a long-standing priority for both reduction of submarine wake signature and alleviation of aircraft vortex wake hazard. A recent study established the feasibility of using relatively weak, secondary vortices with carefully selected unsteady amplitude and phasing to accelerate the breakup of the primary vortex system of a lifting surface, a technique denoted `vortex leveraging'. This paper will summarize progress on the development of SMA-actuated devices for implementing vortex leveraging for hydrodynamic applications. The methods being applied to the hydrodynamic design of these deformable Smart Vortex Leveraging Tabs (SVLTs) will be described, and the results of a preliminary assessment of SVLT performance in achieving wake breakup will be presented. Also, previous work on the design and testing of deformable control surfaces actuated via embedded SMA agonist wires will be reviewed and the design process being employed in the present applications will be discussed. Finally, the plans for near-term computational and experimental work to validate the use of SMA-driven devices for the wake mitigation task will be briefly outlined.

  13. Low power consumption mini rotary actuator with SMA wires

    Science.gov (United States)

    Manfredi, Luigi; Huan, Yu; Cuschieri, Alfred

    2017-11-01

    Shape memory alloys (SMAs) are smart materials widely used as actuators for their high power to weight ratio despite their well-known low energy efficiency and limited mechanical bandwidth. For robotic applications, SMAs exhibit limitations due to high power consumption and limited stroke, varying from 4% to 7% of the total length. Hysteresis, during the contraction and extension cycle, requires a complex control algorithm. On the positive side, the small size and low weight are eminently suited for the design of mini actuators for robotic platforms. This paper describes the design and construction of a light weight and low power consuming mini rotary actuator with on-board contact-less position and force sensors. The design is specifically intended to reduce (i) energy consumption, (ii) dimensions of the sensory system, and (iii) provide a simple control without any need for SMA characterisation. The torque produced is controlled by on-board force sensors. Experiments were performed to investigate the energy consumption and performance (step and sinusoidal angle profiles with a frequency varying from 0.5 to 10 Hz and maximal amplitude of {15}\\circ ). We describe a transient capacitor effect related to the SMA wires during the sinusoidal profile when the active SMA wire is powered and the antagonist one switched-off, resulting in a transient current time varying from 300 to 400 ms.

  14. Modiolus-Hugging Intracochlear Electrode Array with Shape Memory Alloy

    Directory of Open Access Journals (Sweden)

    Kyou Sik Min

    2013-01-01

    Full Text Available In the cochlear implant system, the distance between spiral ganglia and the electrodes within the volume of the scala tympani cavity significantly affects the efficiency of the electrical stimulation in terms of the threshold current level and spatial selectivity. Because the spiral ganglia are situated inside the modiolus, the central axis of the cochlea, it is desirable that the electrode array hugs the modiolus to minimize the distance between the electrodes and the ganglia. In the present study, we propose a shape-memory-alloy-(SMA- embedded intracochlear electrode which gives a straight electrode a curved modiolus-hugging shape using the restoration force of the SMA as triggered by resistive heating after insertion into the cochlea. An eight-channel ball-type electrode array is fabricated with an embedded titanium-nickel SMA backbone wire. It is demonstrated that the electrode array changes its shape in a transparent plastic human cochlear model. To verify the safe insertion of the electrode array into the human cochlea, the contact pressures during insertion at the electrode tip and the contact pressures over the electrode length after insertion were calculated using a 3D finite element analysis. The results indicate that the SMA-embedded electrode is functionally and mechanically feasible for clinical applications.

  15. Compact Receiver Front Ends for Submillimeter-Wave Applications

    Science.gov (United States)

    Mehdi, Imran; Chattopadhyay, Goutam; Schlecht, Erich T.; Lin, Robert H.; Sin, Seth; Peralta, Alejandro; Lee, Choonsup; Gill, John J.; Gulkis, Samuel; Thomas, Bertrand C.

    2012-01-01

    The current generation of submillimeter-wave instruments is relatively mass and power-hungry. The receiver front ends (RFEs) of a submillimeter instrument form the heart of the instrument, and any mass reduction achieved in this subsystem is propagated through the instrument. In the current implementation, the RFE consists of different blocks for the mixer and LO circuits. The motivation for this work is to reduce the mass of the RFE by integrating the mixer and LO circuits in one waveguide block. The mixer and its associated LO chips will all be packaged in a single waveguide package. This will reduce the mass of the RFE and also provide a number of other advantages. By bringing the mixer and LO circuits close together, losses in the waveguide will be reduced. Moreover, the compact nature of the block will allow for better thermal control of the block, which is important in order to reduce gain fluctuations. A single waveguide block with a 600- GHz RFE functionality (based on a subharmonically pumped Schottky diode pair) has been demonstrated. The block is about 3x3x3 cubic centimeters. The block combines the mixer and multiplier chip in a single package. 3D electromagnetic simulations were carried out to design the waveguide circuit around the mixer and multiplier chip. The circuit is optimized to provide maximum output power and maximum bandwidth. An integrated submillimeter front end featuring a 520-600-GHz sub-harmonic mixer and a 260-300-GHz frequency tripler in a single cavity was tested. Both devices used GaAs MMIC membrane planar Schottky diode technology. The sub-harmonic mixer/tripler circuit has been tested using conventional metal-machined blocks. Measurement results on the metal block give best DSB (double sideband) mixer noise temperature of 2,360 K and conversion losses of 7.7 dB at 520 GHz. The LO input power required to pump the integrated tripler/sub-harmonic mixer is between 30 and 50 mW.

  16. Micro-Spec: an Integrated, Direct-Detection Spectrometer for Far-Infrared and Submillimeter Astronomy

    Science.gov (United States)

    Cataldo, Giuseppe

    2014-01-01

    The far-infrared and submillimeter portions of the electromagnetic spectrum provide a unique view of the astrophysical processes present in the early universe. Our ability to fully explore this rich spectral region has been limited, however, by the size and cost of the cryogenic spectrometers required to carry out such measurements. Micro-Spec (u-Spec) is a high-sensitivity, direct-detection spectrometer concept working in the 450-1000 micromillimeter wavelength range which will enable a wide range of flight missions that would otherwise be challenging due to the large size of current instruments with the required spectral resolution and sensitivity. The spectrometer design utilizes two internal antenna arrays, one for transmitting and one for receiving, superconducting microstrip transmission lines for power division and phase delay, and an array of microwave kinetic inductance detectors (MKIDs) to achieve these goals. The instrument will be integrated on a approximately 10 square cm silicon chip and can therefore become an important capability under the low background conditions accessible via space and high-altitude borne platforms. In this paper, an optical design methodology for Micro-Spec is presented, with particular attention given to its twodimensional diffractive region, where the light of different wavelengths is focused on the different detectors. The method is based on the maximization of the instrument resolving power and minimization of the RMS phase error on the instrument focal plane. This two-step optimization can generate geometrical configurations given specific requirements on spectrometer size, operating spectral range and performance. A point design with resolving power of 257, an RMS phase error less than 0.1 radians and four stigmatic points was developed for initial demonstration and will be the basis of future instruments with resolving power up to about 1200.

  17. Transition-Edge Hot-Electron Microbolometers for Millimeter and Submillimeter Astrophysics

    Science.gov (United States)

    Hsieh, Wen-Ting; Stevenson, Thomas; U-yen, Kongpop; Wollack, Edward; Barrentine, Emily

    2014-01-01

    The millimeter and the submillimeter wavelengths of the electromagnetic spectrum hold a wealth of information about the evolution of the universe. In particular, cosmic microwave background (CMB) radiation and its polarization carry the oldest information in the universe, and provide the best test of the inflationary paradigm available to astronomy today. Detecting gravity waves through their imprint on the CMB polarization would have extraordinary repercussions for cosmology and physics. A transition-edge hot-electron micro - bolometer (THM) consists of a superconducting bilayer transition-edge sensor (TES) with a thin-film absorber. Unlike traditional monolithic bolometers that make use of micromachined structures, the THM em ploys the decoupling between electrons and phonons at millikelvin temperatures to provide thermal isolation. The devices are fabricated photolithographically and are easily integrated with antennas via microstrip transmission lines, and with SQUID (superconducting quantum interference device) readouts. The small volume of the absorber and TES produces a short thermal time constant that facilitates rapid sky scanning. The THM consists of a thin-film metal absorber overlapping a superconducting TES. The absorber forms the termination of a superconducting microstripline that carries RF power from an antenna. The purpose of forming a separate absorber and TES is to allow flexibility in the optimization of the two components. In particular, the absorbing film's impedance can be chosen to match the antenna, while the TES impedance can be chosen to match to the readout SQUID amplifier. This scheme combines the advantages of the TES with the advantages of planar millimeter-wave transmission line circuits. Antenna-coupling to the detectors via planar transmission lines allows the detector dimensions to be much smaller than a wavelength, so the technique can be extended across the entire microwave, millimeter, and submillimeter wavelength ranges. The

  18. Multipass millimeter/submillimeter spectrometer to probe dissociative reaction dynamics.

    Science.gov (United States)

    Laas, Jacob C; Hays, Brian M; Widicus Weaver, Susanna L

    2013-10-03

    We present here the instrument design and first experimental results from a multipass millimeter/submillimeter spectrometer designed to probe dissociative reaction dynamics. This work focuses on benchmarking the instrument performance through detection of the CH3O and H2CO products from methanol dissociation induced by a high-voltage plasma discharge. Multiple rotational lines from CH3O and H2CO were observed when this plasma discharge was applied to a sample of methanol vapor seeded in an argon supersonic expansion. The rotational temperature of the dissociation products and their abundance with respect to methanol were determined using a Boltzmann analysis. The minimum detectable absorption coefficient for this instrument was determined to be αmin ≤ 5 × 10(-9) cm(-1). We discuss these results in the context of future applications of this instrument to the study of photodissociation branching ratios for small organic molecules that are important in complex interstellar chemistry.

  19. The role of THz and submillimeter wave technology in DHS

    Science.gov (United States)

    Coty, Thomas; Fuller-Tedeschi, Anna

    2011-06-01

    THz and submillimeter wave technology is of great interest to DHS S&T due to the non-ionizing and clothing penetrating properties of the spectral region. Imaging in the region allows for standoff imaging of concealed threats such as Improvised Explosive Devices (IED) at operationally relevant distances. DHS S&T is investing in this area with the development of components such as detectors and sources for active imaging as well as full sensor systems in the future. The fundamental characterization of the region is also being explored with DHS funding by imaging well-characterized rough surface scattering targets. Analysis of these images will yield data to be used in evaluating assumptions currently made in current performance models. This along with the relevant field applications will be addressed.

  20. SUBMILLIMETER FOLLOW-UP OF WISE-SELECTED HYPERLUMINOUS GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Wu Jingwen; Eisenhardt, Peter R. M.; Stern, Daniel; Assef, Roberto [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Tsai, Chao-Wei; Cutri, Roc; Griffith, Roger; Jarrett, Thomas [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Sayers, Jack; Bridge, Carrie [Division of Physics, Math and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States); Benford, Dominic [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Blain, Andrew [Department of Physics and Astronomy, University of Leicester, LE1 7RH Leicester (United Kingdom); Petty, Sara; Lake, Sean [Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, CA 90095 (United States); Bussmann, Shane [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS78, Cambridge, MA 02138 (United States); Comerford, Julia M.; Evans, Neal J. II [Department of Astronomy, University of Texas, Austin, TX 78731 (United States); Lonsdale, Carol [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Rho, Jeonghee [SETI Institute, 189 BERNARDO Avenue, Mountain View, CA 94043 (United States); Stanford, S. Adam, E-mail: jingwen.wu@jpl.nasa.gov [Department of Physics, University of California Davis, One Shields Avenue, Davis, CA 95616 (United States); and others

    2012-09-01

    We have used the Caltech Submillimeter Observatory (CSO) to follow-up a sample of Wide-field Infrared Survey Explorer (WISE) selected, hyperluminous galaxies, the so-called W1W2-dropout galaxies. This is a rare ({approx}1000 all-sky) population of galaxies at high redshift (peaks at z = 2-3), which are faint or undetected by WISE at 3.4 and 4.6 {mu}m, yet are clearly detected at 12 and 22 {mu}m. The optical spectra of most of these galaxies show significant active galactic nucleus activity. We observed 14 high-redshift (z > 1.7) W1W2-dropout galaxies with SHARC-II at 350-850 {mu}m, with nine detections, and observed 18 with Bolocam at 1.1 mm, with five detections. Warm Spitzer follow-up of 25 targets at 3.6 and 4.5 {mu}m, as well as optical spectra of 12 targets, are also presented in the paper. Combining WISE data with observations from warm Spitzer and CSO, we constructed their mid-IR to millimeter spectral energy distributions (SEDs). These SEDs have a consistent shape, showing significantly higher mid-IR to submillimeter ratios than other galaxy templates, suggesting a hotter dust temperature. We estimate their dust temperatures to be 60-120 K using a single-temperature model. Their infrared luminosities are well over 10{sup 13} L{sub Sun }. These SEDs are not well fitted with existing galaxy templates, suggesting they are a new population with very high luminosity and hot dust. They are likely among the most luminous galaxies in the universe. We argue that they are extreme cases of luminous, hot dust-obscured galaxies (DOGs), possibly representing a short evolutionary phase during galaxy merging and evolution. A better understanding of their long-wavelength properties needs ALMA as well as Herschel data.

  1. Submillimeter observations of the sun from the James Clerk Maxwell Telescope

    Energy Technology Data Exchange (ETDEWEB)

    Lindsey, C.A.; Yee, S.; Roellig, T.L.; Hills, R.; Brock, D. (Hawaii Univ., Honolulu (USA) NASA, Ames Research Center, Moffett Field, CA (USA) Mullard Radio Astronomy Observatory, Cambridge (England) Joint Astronomy Centre, Hilo, HI (USA))

    1990-04-01

    The first submillimeter solar observations from the 15 m James Clerk Maxwell Telescope (JCMT) on Mauna Kea are reported. The JCMT submillimeter heterodyne receiver is used to observe the sun in 850 micron radiation. These are the first submillimeter observations of features on the size scale of the chromospheric supergranular network and of sunspots. A comparison is made between 850 micron images and calcium K line images of the chromospheric supergranular network in the quiet sun and in plage. Images of sunspots are given, noting that their 850 micron brightness is comparable to, or somewhat greater than, that of the quiet sun. 7 refs.

  2. Submillimeter observations of the sun from the James Clerk Maxwell Telescope

    Science.gov (United States)

    Lindsey, Charles A.; Yee, Selwyn; Roellig, Thomas L.; Hills, Richard; Brock, David

    1990-01-01

    The first submillimeter solar observations from the 15 m James Clerk Maxwell Telescope (JCMT) on Mauna Kea are reported. The JCMT submillimeter heterodyne receiver is used to observe the sun in 850 micron radiation. These are the first submillimeter observations of features on the size scale of the chromospheric supergranular network and of sunspots. A comparison is made between 850 micron images and calcium K line images of the chromospheric supergranular network in the quiet sun and in plage. Images of sunspots are given, noting that their 850 micron brightness is comparable to, or somewhat greater than, that of the quiet sun.

  3. PENDEKATAN PENDIDIKAN MULTIKULTURAL PADA MATA PELAJARAN SOSIOLOGI SMA KELAS XI

    Directory of Open Access Journals (Sweden)

    Akbar Wahyu Riyadi

    2013-04-01

    Full Text Available Tujuan penelitian ini adalah untuk menggambarkan penggunaan pendekatan pendidikan multikultural pada pelajaran Sosiologi SMA kelas XI. Penelitian ini merupakan penelitian kualitatif yang dilakukan di SMAN 4 Purworejo. Data dikumpulkan melalui metode pengamatan dan wawancara dengan guru Sosiologi SMAN 4 Purworejo. Hasil penelitian menunjukkan bahwa karakteristik Pendekatan Pendidikan multikultural yang dilakukan oleh guru sosiologi SMA menekankan pada tiga bentuk: optimalisasi peran rasionalitas bagi siswa, praktek dan pembiasaan perbedaan pendapat. Pendekatan ini tepat dilakukan dalam kegiatan pembelajaran pada materi kelompok sosial dalam masyarakat multikultural. Kendala dalam pelaksanaan pendekatan multikultural di SMA adalah, alokasi waktu pertemuan, konsentrasi siswa dalam menerima materi pelajaran yang berhubungan dengan multikultural, keterbatasan media pembelajaran yang digunakan saat pembelajaran serta minat siswa dalam belajar. Hal ini membuat guru bekerja ekstra untuk membuat variasi dalam pembelajaran agar kegiatan belajar mengajar dapat berhasil dengan baik.The objective of this article is to describe the use of multicultural education approach to the study of sociology for senior high school student class XI. This study is a qualitative study conducted in SMAN 4 Purworejo. Data were collected through a method of observation and interviews with teachers of Sociology. The results show that the characteristics of a multicultural approach to education implemented by high school sociology include three forms: teacher’s emphasis on the optimization of students’ rationality, practice and dissent habituation. This approach is appropriate for the learning activities on material of social groups in multicultural societies. Constraints in the implementation of a multicultural approach in high school include time allocation, student’s concentration, the limitations of instructional media used during the learning process

  4. PENGARUH MODEL EXPERIENTIAL LEARNING TERHADAP KEMAMPUAN BERPIKIR SISWA SMA

    Directory of Open Access Journals (Sweden)

    Mar’atus Sholihah

    2016-11-01

    Full Text Available The purpose of this study was to determine the effect of Experiential Learning models developed by Kolb's theory of the critical thinking skills of high school students. This study uses a quasi experiment conducted in SMA Assa'adah Gresik. The population of students of class X IS second semester of academic year 2015/2016. Samples are 2 classes that are homogeneous. Methods of data collection using test questions and the ability to think critically using observation sheet. Data were analyzed by comparing the average acquisition value of critical thinking skills with experimental class control class. Average value of the critical thinking skills using model Experiential Learning higher at 80.9 while the control class is 71.2. Based on the average it can be concluded that the learning model of Experiential Learning can improve students' critical thinking skills. This study is expected to provide information on the application and benefits of the model Experiential Learning in teaching geography and make it more meaningful for students. Tujuan dari penelitian ini adalah mengetahui pengaruh model Experiential Learning yang dikembangkan oleh teori Kolb terhadap kemampuan berpikir kritis siswa SMA. Penelitian ini menggunakan metode quasi experimen yang dilakukan di SMA Assa’adah Gresik. Populasi siswa kelas X IS semester genap tahun pelajaran 2015/2016. Sampel yang digunakan sebanyak 2 kelas yang bersifat homogen. Metode pengumpulan data menggunakan soal tes kemampuan berpikir kritis serta menggunakan lembar observasi. Data yang diperoleh kemudian dianalisis dengan membandingkan rata-rata perolehan nilai kemampuan berpikir kritis kelas kontrol dengan kelas eksperimen. Nilai rata rata kemampuan berpikir kritis yang menggunakan model pembelajaran Experiential Learning lebih tinggi, yaitu sebesar 80,9, sedangkan kelas kontrol sebesar 71,2. Berdasarkan nilai rata-rata tersebut dapat disimpulkan bahwa model pembelajaran Experiential Learning dapat

  5. Effect of SMA bars on cyclic behaviour of low-rise shear walls

    Science.gov (United States)

    Liao, W. I.; Effendy, E.; Song, G.; Mo, Y. L.; Hsu, T. T. C.; Loh, C. H.

    2006-03-01

    Past RC panel tests performed at the University of Houston show that reinforced concrete membrane elements under reversed cyclic loading have much greater ductility when steel bars are provided in the direction of principal tensile stress. In order to improve the ductility of low-rise shear walls under earthquake loading, high seismic performance shear walls have been proposed to have steel bars in the same direction as the tensile principal direction of applied stresses in the critical region of shear walls. This paper presents the results of reversed cyclic tests on three low-rise shear walls with SMA bars. The height, width, and thickness of the designed shear walls are 1.0 m, 2.0 m, and 0.12 m, respectively. SMA bars are provided in the directions of 27 degrees to the horizontal that are in the diagonal direction. The reinforcing bars of the shear walls are in vertical and horizontal directions. The ratios of both SMA and reinforcing bars are 0.24%. The main parameter used in the study is the type of SMA bar, namely Superelastic and Martensite SMA bars. The test results from the walls with SMA bars are also compared to a conventional wall without SMA bars. Test results also show that the maximum shear strengths of the tested walls are affected by the SMA bars. It was found that the shear wall with Martensite SMA bars has greater residual displacement. In contrast, the shear wall with superelastic SMA bars has less residual displacement. At the ultimate state, one of the four superelastic SMA bars buckled, resulting in less energy dissipation capacity than the expected value. Preventing buckling of SMA bars is the research focus in the near future.

  6. TANGGAPAN GENERASI MUDA TERHADAP VLOG PRESIDEN JOKOWI (STUDI KHALAYAK SISWA SMA DI KOTA MAKASSAR)

    OpenAIRE

    -

    2017-01-01

    ABSTRAK MUFLISHA SETYAFAJRINI, E31113320. Tanggapan Generasi Muda Terhadap Vlog Presiden Jokowi (Studi Khalayak Siswa SMA di Kota Makassar). (Dibimbing oleh Muh Nadjib and Tuti Bahfiarti) Skripsi : Program S-1 Universitas Hasanuddin. Skripsi ini bertujuan : (1) Untuk mengethaui tanggapan siswa SMA di Kota Makassar terhadap vlog Presiden Jokowi. (2) Untuk mengetahui citra yang terbentuk dari vlog Presiden Jokowi terhadap siswa SMA di Kota Makassar. Penelitian ini dilakukan selama kura...

  7. PEMANFAATAN INTERNET SEBAGAI SUMBER BELAJAR OLEH GURU DI SMA HANG TUAH 1 JAKARTA

    OpenAIRE

    Jaslim, Dania Karima

    2013-01-01

    Tujuan penelitian ini adalah untuk mendeskripsikan bagaimana pemanfaatan internet sebagai sumber belajar oleh gurudi SMA Hang Tuah 1 Jakarta. Penelitian ini adalah penelitian deskriptif menggunakan metode survai yang bertujuan untuk memperoleh gambaran dan data  empirik mengenai  pemanfaatan internet sebagai sumber belajar oleh Guru di SMA Hang Tuah 1 Jakarta. Penelitian dilaksanakan di SMA Hang Tuah 1 Jakarta pada bulan Januari 2012. Pengumpulan data dilakukan dengan kuisioner atau...

  8. KONTRIBUSI KONSELOR DALAM MEMBENTUK KARAKTER PESERTA DIDIK SMA

    Directory of Open Access Journals (Sweden)

    Agung Slamet Kusmanto

    2015-11-01

    Full Text Available Pengembangan model Pendidikan Holistik Berbasis Karakter, yang memfokuskan pada pembentukan seluruh aspek dimensi manusia, sehingga dapat menjadi manusia yang berkarakter. Kurikulum Holistik Berbasis Karakter ini disusun berdasarkan Kurikulum Berbasis Kompetensi (KBK dan diterapkan dengan menggunakan pendekatan Student Active Learning, Integrated Learning, Developmentally Appropriate Practices, Contextual Learning, Collaborative Learning, dan Multiple Intelligences yang semuanya dapat menciptakan suasana belajar yang efektif dan menyenangkan, serta dapat mengembangkan seluruh aspek dimensi manusia secara holistik. Maka diperlukan peran yang sangat besar dari guru pembimbing (konselor SMA dalam mengembangkan potensi peserta didiknya dalam mengembangkan potensinya dan membentuk karakter individu itu sendiri dan memberikan warna positif dalam suasana pembelajaran.

  9. NASA Keynote at the 2015 Trilateral SMA Conference, Frascati, Italy

    Science.gov (United States)

    Groen, Frank

    2015-01-01

    The purpose of this presentation is to illustrate some new directions within NASA's safety and mission function in response to changes in missions, technology, and practices. The presentation lists last year's highlights from NASA's human and robotic spaceflight missions, and discusses anticipated highlights for the coming year taken from existing Agency presentations. It will highlight changes to NASA's mission and the way NASA does business, as described in the 2014 strategic plan. It will then discuss how these changes pose challenges to trusted SMA practices, and provide some examples of initiatives NASA is taking action to address these challenges.

  10. KEEFEKTIFAN TEKNIK RELAKSASI UNTUK MENURUNKAN STRES AKADEMIK SISWA SMA

    OpenAIRE

    Suyono Suyono; Triyono Triyono; Dany M. Handarini

    2016-01-01

    Abstract: This study aims at examining the effectiveness of relaxation techniques to release students’stress and tension regarding academic within Senior High School Assádah in Gresik City. This study employed quasi-experiment design using one group pretest-posttest model. The data of this study were obtained through academic stress inventory to attain a depiction of stress level encountered by the subject. The subjects of this study were seven students of Tenth Graders in SMA Assaadah Bungah...

  11. MODEL PENGEMBANGAN PERANGKAT PEMBELAJARAN SEJARAH BERORIENTASI METAKOGNITIF JENJANG SMA

    Directory of Open Access Journals (Sweden)

    Cahyo Budi Utomo

    2015-01-01

    Full Text Available The importance of metacognitive based history learning in the high school level as requested in the “curriculum 2013” is the main background of this research. The research is focused to find the model of development of metacognitive based learning through research and development (R&D type research. The results showed an essential component in achieving successful management of metacognitive based history learning in high school education which the curriculum as a core competency analysis and basic competencies, lesson plan development, and the development of assessment tools. Development model of metacognitive based learning at high school education have main characteristic of the inclusion of explicit metacognitive learning goals and assignments and devices equipped with a rubric and assessment questionnaire. Metacognitive based history learning instructional tools that are developed in senior high school level has been carried out as optimally as possible by involving history teachers in the process of development and testing through focus group discussions and questionnaire.Keywords: Model, Instructional tool, Metacognitive, senior high school levelPentingnya orientasi metakognitif dalam perangkat pembelajaran sejarah jenjang SMA sebagaimana yang dikehendaki dalam implementasi kurikulum 2013 merupakan latar belakang utama penelitian ini. Penelitian difokuskan untuk menemukan model pengembangan perangkat pembelajaran berorientasi metakognitif melalui penelitian berjenis riset dan pengembangan (R&D. Metode penelitian R&D dilaksanakan melalui tiga tahap utama yaitu: tahap studi pendahuluan, tahap pengembangan, dan tahap uji publik. Hasil penelitian menunjukkan komponen esensial dalam mewujudkan keberhasilan penge-lolaan pembelajaran sejarah berorientasi metakognitif pada jenjang pendidikan SMA adalah kurikulum sebagai bahan analisis kompetensi inti dan kompetensi dasar, pengembangan RPP, dan pengembangan perangkat assesmen. Model

  12. STRATEGI KOMUNIKASI GURU SMA ISLAM TERPADU DALAM MENGHASILKAN SISWA YANG UNGGUL

    Directory of Open Access Journals (Sweden)

    Chatia Hastasari

    2016-12-01

    Full Text Available The study aims to explain how the concept of integrated Islamic and the strategy of the teacher in SMA IT Abu Bakar Yogyakarta and SMA Muhammadiyah 1 Yogyakarta produce the superior students. It refers to the development of SMA IT which always puts ethics, religion and the quality of the students. However, the main key to produce the superior students is the role of professional teacher who encourages the strong characteristic of students. The method of this research is qualitative and takes place in SMA IT Abu Bakar and SMA Muhammadiyah 1 Yogyakarta. Furthermore, the samples of this research consist of twenty teachers. The result is that (1 SMA IT Abu Bakar and SMA Muhammadiyah 1 Yogyakarta combine three elements such as the cooperation among the shool, societies, and family; the structured and programmed curriculum from kindergarten to university; tsaqafah Islam and science oriented. These are done to produce a superior student who masters science and technology and also has a good characteristic. (2 The communication strategy of the teachers in SMA IT Abu Bakar and SMA Muhammadiyah 1 Yogyakarta is effective. It can be seen from the fulfillment of communication elements on communication strategy which is used by the teacher to produce a superior student.

  13. Superior mesenteric artery (SMA) syndrome: an unusual cause of intestinal obstruction in palliative care.

    Science.gov (United States)

    So, Chun-Yan; Chan, Kwok-Ying; Au, Ho-Yan; Chan, Man-Lui; Lai, Theresa

    2017-01-01

    Superior mesenteric artery (SMA) syndrome is an uncommon cause of intestinal obstruction and seldom been mentioned in palliative care. Hereby, we reported a case of SMA syndrome who presented with symptoms of upper intestinal obstruction in a 68-year-old patient; subsequent CT findings were classical of SMA syndrome. The patient's history of poliomyelitis and recent significant weight loss were the predisposing factors for SMA syndrome. It also highlights the importance of monitoring signs and symptoms of intestinal obstruction in such patients before considering switching to oral feeding.

  14. Fast Fourier transform spectrometer readout for large arrays of microwave kinetic inductance detectors

    NARCIS (Netherlands)

    Yates, S. J. C.; Baryshev, A. M.; Baselmans, J. J. A.; Klein, B.; Guesten, R.

    2009-01-01

    Microwave kinetic inductance detectors have great potential for large, very sensitive detector arrays for use in, for example, submillimeter imaging. Being intrinsically readout in the frequency domain, they are particularly suited for frequency domain multiplexing allowing similar to 1000 s of

  15. Membrane wrinkling patterns and control with SMA and SMPC actuators

    Science.gov (United States)

    Lu, Mingyu; Li, Yunliang; Tan, Huifeng; Zhou, Limin

    2009-07-01

    Wrinkling is a main factor affecting the performance of the membrane structures and is always considered to be a failure as it can cause dramatic decrease of shape accuracy. The study of membrane wrinkling control has the analytical and experimental meanings. In this paper, a feasible membrane shape control method is presented. An expression of wrinkle wavelength using stress extremum principle is established based on the tension field theory and the Von Karman large deflection formula which verifies the generation and evolution reason of membrane wrinkles. The control mechanism for membrane wrinkles is developed using shape memory alloy (SMA) and shape memory polymer composite (SMPC) actuators which are attached to the boundaries of the membrane for producing contraction/expansion forces to adjust the shape of the membrane. The whole control process is monitored by photogrammetric technique. Numerical simulations are also conducted using ANSYS finite element software with the nonlinear post-buckling analytical method. Both the experimental and numerical results show that the amplitudes of wrinkles are effectively controlled by SMA and SMPC actuators. The method introduced in this paper provides the foundation for shape control of the membrane wrinkling and is important to the future work on vibration control of space membrane structures.

  16. Shape Memory Alloy (SMA)-Based Launch Lock

    Science.gov (United States)

    Badescu, Mircea; Bao, Xiaoqi; Bar-Cohen, Yoseph

    2014-01-01

    Most NASA missions require the use of a launch lock for securing moving components during the launch or securing the payload before release. A launch lock is a device used to prevent unwanted motion and secure the controlled components. The current launch locks are based on pyrotechnic, electro mechanically or NiTi driven pin pullers and they are mostly one time use mechanisms that are usually bulky and involve a relatively high mass. Generally, the use of piezoelectric actuation provides high precession nanometer accuracy but it relies on friction to generate displacement. During launch, the generated vibrations can release the normal force between the actuator components allowing shaft's free motion which could result in damage to the actuated structures or instruments. This problem is common to other linear actuators that consist of a ball screw mechanism. The authors are exploring the development of a novel launch lock mechanism that is activated by a shape memory alloy (SMA) material ring, a rigid element and an SMA ring holding flexure. The proposed design and analytical model will be described and discussed in this paper.

  17. KESANTUNAN TUTURAN DIREKTIF DALAM INTERAKSI PEMBELAJARAN DI SMA

    Directory of Open Access Journals (Sweden)

    Mardiyah Putri Astuti

    2017-03-01

    Full Text Available Politeness speech in learning interactions in the classroom tend to be effected through a directive speech. Assessment of form directive speech made by using a guide to the theory and analysis based on speech act theory directive Bach and Harnish. This study aims to determine the form of politeness directive in an interaction study in SMA 1 Batu. Forms directive speech in learning interactions are marked with (1 directive requests, (2 directive question, (3 directive command, (4 The prohibition directive, (5 directive licensing, and (6 the directive advice. The results of the analysis of the forms of speech directive shows that teachers do politeness predominantly through commands, prohibitions, permissions, and advice, while the shape of the directive utterances made by teachers and students to consider cultural aspects. Kesantunan tuturan dalam interaksi pembelajaran di dalam kelas cenderung dilakukan melalui bentuk tuturan direktif. Pengkajian terhadap bentuk tuturan direktif dilakukan dengan mengggunakan teori dan panduan analisis berdasarkan teori tindak tutur direktif Bach dan Harnish. Penelitian ini bertujuan untuk mengetahui bentuk kesantunan direktif dalam interaksi pembelajaran di SMA 1 Batu. Bentuk tuturan direktif dalam interaksi pembelajaran ditandai dengan (1 direktif permintaan, (2 direktif pertanyaan, (3 direktif perintah, (4 direktif larangan, (5 direktif pemberian izin, dan (6 direktif nasihat. Hasil analisis mengenai bentuk tuturan direktif menunjukkan bahwa guru melakukan kesantunan secara dominan melalui perintah, larangan, izin, dan nasihat, sedangkan bentuk tuturan direktif dilakukan oleh guru dan siswa dengan mempertimbangkan aspek budaya.

  18. Superconducting Resonator Spectrometer for Millimeter- and Submillimeter-Wave Astrophysics Project

    Data.gov (United States)

    National Aeronautics and Space Administration — "We propose to develop a novel ultra-compact spectrograph-on-a-chip for the submillimeter and millimeter waveband. SuperSpec uses planar lithographed superconducting...

  19. THE SCUBA-2 COSMOLOGY LEGACY SURVEY: MULTIWAVELENGTH COUNTERPARTS TO 10{sup 3} SUBMILLIMETER GALAXIES IN THE UKIDSS-UDS FIELD

    Energy Technology Data Exchange (ETDEWEB)

    Chen, Chian-Chou; Smail, Ian; Ma, Cheng-Jiun; Simpson, James M.; Swinbank, A. Mark [Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Ivison, Rob J.; Arumugam, Vinodiran; Mortlock, Alice; Dunlop, James S.; Michałowski, Michał J. [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Almaini, Omar; Conselice, Christopher J.; Hartley, Will G. [University of Nottingham, School of Physics and Astronomy, Nottingham, NG7 2RD (United Kingdom); Geach, James E. [Center for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Simpson, Chris [Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF (United Kingdom); Aretxaga, Itziar [Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE), Luis Enrique Erro 1, Sta. Ma. Tonantzintla, Puebla (Mexico); Blain, Andrew [Physics and Astronomy, University of Leicester, Leicester, LE1 7RH (United Kingdom); Chapman, Scott C. [Department of Physics and Atmospheric Science, Dalhousie University, 6310 Coburg Road, Halifax, NS B3H 4R2 (Canada); Farrah, Duncan [Department of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); Halpern, Mark [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); and others

    2016-04-01

    We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama Large Millimeter Array (ALMA) pilot study on a subset of our bright SCUBA-2 sample as a training set, along with the deep optical–near-infrared (OIR) data available in this field, we develop a novel technique, Optical–IR Triple Color (OIRTC), using z − K, K − [3.6], [3.6] − [4.5] colors to select the candidate submillimeter galaxy (SMG) counterparts. By combining radio identification and the OIRTC technique, we find counterpart candidates for 80% of the Class = 1 ≥ 4σ SCUBA-2 sample, defined as those that are covered by both radio and OIR imaging and the base sample for our scientific analyses. Based on the ALMA training set, we expect the accuracy of these identifications to be 82% ± 20%, with a completeness of 69% ± 16%, essentially as accurate as the traditional p-value technique but with higher completeness. We find that the fraction of SCUBA-2 sources having candidate counterparts is lower for fainter 850 μm sources, and we argue that for follow-up observations sensitive to SMGs with S{sub 850} ≳ 1 mJy across the whole ALMA beam, the fraction with multiple counterparts is likely to be >40% for SCUBA-2 sources at S{sub 850} ≳ 4 mJy. We find that the photometric redshift distribution for the SMGs is well fit by a lognormal distribution, with a median redshift of z = 2.3 ± 0.1. After accounting for the sources without any radio and/or OIRTC counterpart, we estimate the median redshift to be z = 2.6 ± 0.1 for SMGs with S{sub 850} > 1 mJy. We also use this new large sample to study the clustering of SMGs and the far-infrared properties of the unidentified submillimeter sources by stacking their Herschel SPIRE far-infrared emission.

  20. EVIDENCE FOR ENVIRONMENTAL CHANGES IN THE SUBMILLIMETER DUST OPACITY

    Energy Technology Data Exchange (ETDEWEB)

    Martin, Peter G.; Roy, Arabindo; Miville-Deschenes, Marc-Antoine [Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8 (Canada); Bontemps, Sylvain [Observatoire de Bordeaux, BP 89, F-33270 Floirac (France); Ade, Peter A. R.; Griffin, Matthew; Hargrave, Peter C.; Mauskopf, Philip [Department of Physics and Astronomy, Cardiff University, 5 The Parade, Cardiff, CF24 3AA (United Kingdom); Bock, James J. [Jet Propulsion Laboratory, Pasadena, CA 91109-8099 (United States); Chapin, Edward L.; Halpern, Mark; Marsden, Gaelen [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); Devlin, Mark J.; Dicker, Simon R.; Klein, Jeff [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Gundersen, Joshua O. [Department of Physics, University of Miami, 1320 Campo Sano Drive, Carol Gables, FL 33146 (United States); Hughes, David H. [Instituto Nacional de Astrofisica Optica y Electronica (INAOE), Aptdo. Postal 51 y 72000 Puebla (Mexico); Netterfield, Calvin B. [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Olmi, Luca [INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 (Italy); Patanchon, Guillaume [Laboratoire APC, 10, rue Alice Domon et Leonie Duquet F-75205 Paris (France); and others

    2012-05-20

    The submillimeter opacity of dust in the diffuse interstellar medium (ISM) in the Galactic plane has been quantified using a pixel-by-pixel correlation of images of continuum emission with a proxy for column density. We used multi-wavelength continuum data: three Balloon-borne Large Aperture Submillimeter Telescope bands at 250, 350, and 500 {mu}m and one IRAS band at 100 {mu}m. The proxy is the near-infrared color excess, E(J - K{sub s}), obtained from the Two Micron All Sky Survey. Based on observations of stars, we show how well this color excess is correlated with the total hydrogen column density for regions of moderate extinction. The ratio of emission to column density, the emissivity, is then known from the correlations, as a function of frequency. The spectral distribution of this emissivity can be fit by a modified blackbody, whence the characteristic dust temperature T and the desired opacity {sigma}{sub e}(1200) at 1200 GHz or 250 {mu}m can be obtained. We have analyzed 14 regions near the Galactic plane toward the Vela molecular cloud, mostly selected to avoid regions of high column density (N{sub H} > 10{sup 22} cm{sup -2}) and small enough to ensure a uniform dust temperature. We find {sigma}{sub e}(1200) is typically (2-4) Multiplication-Sign 10{sup -25} cm{sup 2} H{sup -1} and thus about 2-4 times larger than the average value in the local high Galactic latitude diffuse atomic ISM. This is strong evidence for grain evolution. There is a range in total power per H nucleon absorbed (and re-radiated) by the dust, reflecting changes in the strength of the interstellar radiation field and/or the dust absorption opacity. These changes in emission opacity and power affect the equilibrium T, which is typically 15 K, colder than at high latitudes. Our analysis extends, to higher opacity and lower temperature, the trend of increasing {sigma}{sub e}(1200) with decreasing T that was found at high latitudes. The recognition of changes in the emission opacity

  1. Detection of Submillimeter-wave [C i] Emission in Gaseous Debris Disks of 49 Ceti and β Pictoris

    Energy Technology Data Exchange (ETDEWEB)

    Higuchi, Aya E.; Sakai, Nami [The Institute of Physical and Chemical Research (RIKEN), 2-1, Hirosawa, Wako-shi, Saitama 351-0198 (Japan); Sato, Aki; Tsukagoshi, Takashi; Momose, Munetake [College of Science, Ibaraki University, Bunkyo 2-1-1, Mito 310-8512 (Japan); Iwasaki, Kazunari [Department of Environmental Systems Science, Doshisha University, Tatara Miyakodani 1-3, Kyotanabe City, Kyoto 610-0394 (Japan); Kobayashi, Hiroshi; Ishihara, Daisuke; Watanabe, Sakae; Kaneda, Hidehiro [Department of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602 (Japan); Yamamoto, Satoshi, E-mail: aya.higuchi@riken.jp [Department of Physics, The University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)

    2017-04-10

    We have detected [C i] {sup 3} P {sub 1}–{sup 3} P {sub 0} emissions in the gaseous debris disks of 49 Ceti and β Pictoris with the 10 m telescope of the Atacama Submillimeter Telescope Experiment, which is the first detection of such emissions. The line profiles of [C i] are found to resemble those of CO( J = 3–2) observed with the same telescope and the Atacama Large Millimeter/submillimeter Array. This result suggests that atomic carbon (C) coexists with CO in the debris disks and is likely formed by the photodissociation of CO. Assuming an optically thin [C i] emission with the excitation temperature ranging from 30 to 100 K, the column density of C is evaluated to be (2.2 ± 0.2) × 10{sup 17} and (2.5 ± 0.7) × 10{sup 16} cm{sup −2} for 49 Ceti and β Pictoris, respectively. The C/CO column density ratio is thus derived to be 54 ± 19 and 69 ± 42 for 49 Ceti and β Pictoris, respectively. These ratios are higher than those of molecular clouds and diffuse clouds by an order of magnitude. The unusually high ratios of C to CO are likely attributed to a lack of H{sub 2} molecules needed to reproduce CO molecules efficiently from C. This result implies a small number of H{sub 2} molecules in the gas disk, i.e., there is an appreciable contribution of secondary gas from dust grains.

  2. SMA chemical modification for application as diesel oil additive; Modificacao quimica do SMA visando aplicacao como aditivo para oleo diesel

    Energy Technology Data Exchange (ETDEWEB)

    Soldi, Rafael A.; Oliveira, Angelo R.S.; Zawadzki, Sonia F.; Cesar-Oliveira, Maria Aparecida F. [Parana Univ., Curitiba, PR (Brazil). Dept. de Quimica. Lab. de Polimeros Sinteticos]. E-mails: rafaelsoldi@hotmail.com, mafco@quimica.ufpr.br

    2003-07-01

    The deposition of paraffinic material during the crude oil and their derivatives production and transportation is one of the principal problems in the petroleum industry. Polymer derivatives obtained from styrene-maleic anhydride copolymers (SMA), containing long pendant hydrocarbon segments in the polymeric backbone, are known as efficient polymeric additives to prevent the wax deposition and to reduce the oil pour point. Nevertheless, this application for this class of polymer is not much evaluated in Brazil. In this work, a new procedure was developed for SMA synthesis and chemical modification using stearyl alcohol. The performance of these polymeric materials as pour point depressants were evaluated using a Brazilian diesel oil from REPAR/PETROBRAS. The best results were obtained for the polymeric additives with small amounts of octadecyl ester groups. When it was used only 25 ppm of one of these additives, the oil presented a pour point value of -17 deg C and the diesel oil containing 100 ppm of this same additive presented a pour point value of -30 deg C. This last result indicates a 24 deg C pour point decreasing. (author)

  3. SHARC II: A Caltech Submillimeter Observatory Facility Camera with 384 Pixels

    Science.gov (United States)

    Dowell, C. Darren; Allen, Christine A.; Babu, Sachidananda; Freund, Minoru; Gardner, Matthew B.; Groseth, Jeffrey; Jhabvala, Murzy; Kovacs, Attila; Lis, Dariusz C.; Moseley, S. Harvey, Jr.

    2002-01-01

    SHARC II is a background-limited 350 micron and 450 micron facility camera for the Caltech Submillimeter Observatory undergoing commissioning in 2002. The key component of SHARC II is a 12 x 32 array of doped silicon 'pop-up' bolometers developed at NASA/Goddard. Each 1 mm x 1 mm pixel is coated with a 400 Omega/square bismuth film and located lambda/4 above a reflective backshort to achieve greater than 75% absorption efficiency. The pixels cover the focal plane with greater than 90% filling factor. At 350 microns, the SHARC II pixels are separated by 0.65 lambda/D. In contrast to the silicon bolometers in the predecessor of SHARC II, each doped thermistor occupies nearly the full area of the pixel, which lowers the 1/f knee of tile detector noise to less than 0.03 Hz, under load, at tile bath temperature of 0.36 K. The bolometers are AC-biased and read in 'total power' mode to take advantage of the improved stability. Each bolometer is biased through a custom approx. 130 MOmega CrSi load resistor at 7 K and read with a commercial JFET at 120 K. The JFETs and load resistors are integrated with the detectors into a single assembly to minimize microphonic noise. Electrical connection across the 0.36 K to 4 K and 4 K to 120 K temperature interfaces is accomplished with lithographed metal wires on dielectric substrates. In the best 25% of winter nights on Mauna Kea, SHARC II is expected to have an NEFD at 350 micron of 1 Jy Hz(sup -1/2) or better. The new camera should be at least 4 times faster at detecting known point sources and 30 times faster at mapping large areas compared to the prior instrument.

  4. The rest-frame submillimeter spectrum of high-redshift, dusty, star-forming galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Spilker, J. S.; Marrone, D. P. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Aguirre, J. E. [University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Aravena, M. [European Southern Observatory, Alonso de Cordova 3107, Casilla 19001 Vitacura Santiago (Chile); Ashby, M. L. N. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Béthermin, M. [Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu-CNRS-Université Paris Diderot, CEA-Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette (France); Bradford, C. M. [Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Bothwell, M. S. [Cavendish Laboratory, University of Cambridge, JJ Thompson Ave, Cambridge CB3 0HA (United Kingdom); Brodwin, M. [Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States); Carlstrom, J. E.; Crawford, T. M. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Chapman, S. C. [Dalhousie University, Halifax, Nova Scotia (Canada); De Breuck, C.; Gullberg, B. [European Southern Observatory, Karl Schwarzschild Straße 2, D-85748 Garching (Germany); Fassnacht, C. D. [Department of Physics, University of California, One Shields Avenue, Davis, CA 95616 (United States); Gonzalez, A. H. [Department of Astronomy, University of Florida, Gainesville, FL 32611 (United States); Greve, T. R. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Hezaveh, Y. [Department of Physics, McGill University, 3600 Rue University, Montreal, Quebec H3A 2T8 (Canada); Holzapfel, W. L., E-mail: jspilker@as.arizona.edu [Department of Physics, University of California, Berkeley, CA 94720 (United States); and others

    2014-04-20

    We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250 to 770 GHz. This spectrum was constructed by stacking Atacama Large Millimeter/submillimeter Array (ALMA) 3 mm spectra of 22 such sources discovered by the South Pole Telescope and spanning z = 2.0-5.7. In addition to multiple bright spectral features of {sup 12}CO, [C I], and H{sub 2}O, we also detect several faint transitions of {sup 13}CO, HCN, HNC, HCO{sup +}, and CN, and use the observed line strengths to characterize the typical properties of the interstellar medium of these high-redshift starburst galaxies. We find that the {sup 13}CO brightness in these objects is comparable to that of the only other z > 2 star-forming galaxy in which {sup 13}CO has been observed. We show that the emission from the high-critical density molecules HCN, HNC, HCO{sup +}, and CN is consistent with a warm, dense medium with T {sub kin} ∼ 55 K and n{sub H{sub 2}}≳10{sup 5.5} cm{sup –3}. High molecular hydrogen densities are required to reproduce the observed line ratios, and we demonstrate that alternatives to purely collisional excitation are unlikely to be significant for the bulk of these systems. We quantify the average emission from several species with no individually detected transitions, and find emission from the hydride CH and the linear molecule CCH for the first time at high redshift, indicating that these molecules may be powerful probes of interstellar chemistry in high-redshift systems. These observations represent the first constraints on many molecular species with rest-frame transitions from 0.4 to 1.2 mm in star-forming systems at high redshift, and will be invaluable in making effective use of ALMA in full science operations.

  5. High-resolution submillimeter and near-infrared studies of the transition disk around Sz 91

    Energy Technology Data Exchange (ETDEWEB)

    Tsukagoshi, Takashi; Momose, Munetake [College of Science, Ibaraki University, Bunkyo 2-1-1, Mito 310-8512 (Japan); Hashimoto, Jun [Department of Physics and Astronomy, The University of Oklahoma, 440 West Brooks Street, Norman, OK 73019 (United States); Kudo, Tomoyuki; Saito, Masao; Ohashi, Nagayoshi; Kawabe, Ryohei; Akiyama, Eiji [National Astronomical Observatory Japan (NAOJ), Osawa 2-21-1, Mitaka, Tokyo 181-8588 (Japan); Andrews, Sean; Wilner, David [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kitamura, Yoshimi [Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Yoshinodai 3-1-1, Sagamihara, Kanagawa 229-8510 (Japan); Abe, Lyu [Lboratoire Lagrange (UMR 7293), Université de Nice-Sophia Antipolis, CNRS, Observatoire de la Côte d' Azur, 28 avenue Valrose, F-06108 Nice Cedex 2 (France); Brandner, Wolfgang [Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany); Brandt, Timothy D. [Department of Astrophysical Sciences, Princeton University, Peyton Hall, Ivy Lane, Princeton, NJ 08544 (United States); Carson, Joseph [Department of Physics and Astronomy, College of Charleston, 58 Coming Street, Charleston, SC 29424 (United States); Currie, Thayne [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street M5S 3H4, Toronto, Ontario (Canada); Egner, Sebastian E.; Guyon, Olivier [Subaru Telescope, 650 North A' ohoku Place, Hilo, HI 96720 (United States); Goto, Miwa [Universitäts-Sternwarte München, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 München (Germany); Grady, Carol, E-mail: ttsuka@mx.ibaraki.ac.jp [Exoplanets and Stellar Astrophysics Laboratory, Code 667, Goddard Space Flight Center, Greenbelt, MD 20771 (United States); and others

    2014-03-10

    To reveal the structures of a transition disk around a young stellar object in Lupus, Sz 91 , we have performed aperture synthesis 345 GHz continuum and CO(3-2) observations with the Submillimeter Array (∼1''-3'' resolution) and high-resolution imaging of polarized intensity at the K{sub s} -band using the HiCIAO instrument on the Subaru Telescope (0.''25 resolution). Our observations successfully resolved the inner and outer radii of the dust disk to be 65 and 170 AU, respectively, which indicates that Sz 91 is a transition disk source with one of the largest known inner holes. The model fitting analysis of the spectral energy distribution reveals an H{sub 2} mass of 2.4 × 10{sup –3} M {sub ☉} in the cold (T < 30 K) outer part at 65 AU 3 × 10{sup –9} M {sub ☉}) of hot (T ∼ 180 K) dust possibly remains inside the inner hole of the disk. The structure of the hot component could be interpreted as either an unresolved self-luminous companion body (not directly detected in our observations) or a narrow ring inside the inner hole. Significant CO(3-2) emission with a velocity gradient along the major axis of the dust disk is concentrated on the Sz 91 position, suggesting a rotating gas disk with a radius of 420 AU. The Sz 91 disk is possibly a rare disk in an evolutionary stage immediately after the formation of protoplanets because of the large inner hole and the lower disk mass than other transition disks studied thus far.

  6. The role of the supplementary motor area (SMA) in word production.

    Science.gov (United States)

    Alario, F-Xavier; Chainay, Hanna; Lehericy, Stéphane; Cohen, Laurent

    2006-03-03

    The supplementary motor area (SMA) is a key structure for behavioral planning and execution. Recent research on motor control conducted with monkeys and humans has put to light an anatomical and functional distinction between pre-SMA and SMA-proper. According to this view, the pre-SMA would be involved in higher level processes while the SMA-proper would be more closely tied to motor output. We extended this general framework to the verbal domain, in order to investigate the role of the SMA in speech production. We conducted two speech production experiments with fMRI where we manipulated parameters such as familiarity, complexity or constraints on word selection. The results reveal a parcellation of the SMA into three distinct regions, according to their involvement in different aspects of word production. More specifically, following a rostrocaudal gradient, we observed differential activations related to lexical selection, linear sequence encoding and control of motor output. A parallel organization was observed in the dorsolateral frontal cortex. By refining its anatomical and functional parcellation, these results clarify the roles of the SMA in speech production.

  7. Natural History of Denervation in SMA: Relation to Age, SMN2 Copy Number, and Function

    Science.gov (United States)

    Swoboda, Kathryn J.; Prior, Thomas W.; Scott, Charles B.; McNaught, Teresa P.; Wride, Mark C.; Reyna, Sandra P.; Bromberg, Mark B.

    2014-01-01

    Denervation was assessed in 89 spinal muscular atrophy (SMA) 1, 2, and 3 subjects via motor unit number estimation (MUNE) and maximum compound motor action potential amplitude (CMAP) studies, and results correlated with SMN2 copy, age, and function. MUNE and maximum CMAP values were distinct among SMA subtypes (p < 0.05). Changes in MUNE and maximum CMAP values over time were dependent on age, SMA type, and SMN2 copy number. SMN2 copy number less than 3 correlated with lower MUNE and maximum CMAP values (p < 0.0001) and worse functional outcomes. As SMN2 copy number increases, so does functional status (p < 0.0001). Change in MUNE longitudinally over the time intervals examined in this study was not statistically significant for any SMA cohort. However, a decline in maximum CMAP over time was apparent in SMA2 subjects (p = 0.049). Age-dependent decline in MUNE and maximum CMAP was apparent in both SMA 1 (p < 0.0001) and SMA 2 (p < 0.0001) subjects, with age as an independent factor regardless of type. Maximum CMAP at the time of the initial assessment was most predictive of functional outcome (p < 0.0001). Prospective longitudinal studies in four prenatally diagnosed infants demonstrated significant progressive denervation in association with symptomatic onset or functional decline. These data highlight the potential value of such measures in increasing our understanding of pathophysiological factors involved in denervation in SMA. PMID:15852397

  8. Pengembangan multimedia pembelajaran geografi berbasis memory sport pada materi litosfer untuk peserta didik SMA

    OpenAIRE

    Yoga Prismanata; Christina Ismaniati

    2017-01-01

    Penelitian ini bertujuan: (1) mendeskripsikan pengembangan produk multimedia pembelajaran geografi berbasis memory sport yang layak pada peserta didik SMA, dan (2) mendeskripsikan efektivitas produk multimedia pembelajaran geografi berbasis memory sport terhadap hasil belajar peserta didik SMA. Penelitian pengembangan ini menggunakan model pengembangan jenis prosedural yang diformulasikan oleh Alessi & Trollip. Desain pengembangan dengan menggunakan model tersebut terdiri dari tiga fase, yait...

  9. Modeling and Dynamical Behavior of Rotating Composite Shafts with SMA Wires

    Directory of Open Access Journals (Sweden)

    Yongsheng Ren

    2014-01-01

    Full Text Available A dynamical model is developed for the rotating composite shaft with shape-memory alloy (SMA wires embedded in. The rotating shaft is represented as a thin-walled composite of circular cross-section with SMA wires embedded parallel to shaft’s longitudinal axis. A thermomechanical constitutive equation of SMA proposed by Brinson is employed and the recovery stress of the constrained SMA wires is derived. The equations of motion are derived based on the variational-asymptotical method (VAM and Hamilton’s principle. The partial differential equations of motion are reduced to the ordinary differential equations of motion by using the Galerkin method. The model incorporates the transverse shear, rotary inertia, and anisotropy of composite material. Numerical results of natural frequencies and critical speeds are obtained. It is shown that the natural frequencies of the nonrotating shaft and the critical rotating speed increase as SMA wire fraction and initial strain increase and the increase in natural frequencies becomes more significant as SMA wire fraction increases. The initial strain of SMA wires appears to have marginal effect on dynamical behaviors of the shaft. The actuation performance of SMA wires is found to be closely related to the ply-angle.

  10. Submillimeter Imaging of Dust Around Main Sequence Stars

    Science.gov (United States)

    Jewitt, David

    1998-01-01

    This grant was to image circumstellar dust disks surrounding main-sequence stars. The delivery of the SCUBA detector we had planned to use for this work was delayed repeatedly, leading us to undertake a majority of the observations with the UKT14 submillimeter detector at the JCMT (James Clerk Maxwell Telescope) and optical imagers and a coronagraph at the University of Hawaii 2.2-m telescope. Major findings under this grant include: (1) We discovered 5 asymmetries in the beta Pictoris regenerated dust disk. The discovery of these asymmetries was a surprise, since smearing due to Keplerian shear should eliminate most such features on timescales of a few thousand years. One exception is the "wing tilt" asymmetry, which we interpret as due to the scattering phase function of dust disk particles. From the wing tilt and a model of the phase function, we find a disk plane inclination to the line of sight of JCMT). It is possible, for instance, that the main 850 micro-m blob is merely a galaxy or other high-z source projected onto the beta Pic mid-plane.

  11. Extending the Millimeter-Submillimeter Spectrum of Protonated Formaldehyde

    Science.gov (United States)

    Roenitz, Kevin; Zou, Luyao; Widicus Weaver, Susanna L.

    2017-06-01

    Protonated formaldehyde has been detected in the interstellar medium, where it participates in the formation and destruction of methanol. The rotational spectrum for protonated formaldehyde has been previously recorded by Amano and coworkers from 120-385 GHz using a hollow cathode discharge source for ion production. Additionally, protonated formaldehyde was produced in a supersonic expansion discharge source by Duncan and coworkers, but it was detected using time-of-flight mass spectrometry. Higher frequency spectra would help to guide additional observational studies of protonated formaldehyde using instruments such as the ALMA and SOFIA observatories. As such, we have used a supersonic expansion discharge source to produce protonated formaldehyde, and recorded its spectrum using millimeter-submillimeter direct absorption spectroscopy. The rotational spectrum was recorded from 350-1000 GHz. Here we will present the experimental design, specifically focusing on the optimization of the source for production of organic ions. We will also present the spectroscopic results for protonated formaldehyde and a spectral analysis with associated prediction that can be extended to frequencies above 1 THz.

  12. Faint submillimeter galaxies revealed by multifield deep ALMA observations: number counts, spatial clustering, and a dark submillimeter line emitter

    Energy Technology Data Exchange (ETDEWEB)

    Ono, Yoshiaki; Ouchi, Masami; Momose, Rieko [Institute for Cosmic Ray Research, The University of Tokyo, Kashiwa, Chiba 277-8582 (Japan); Kurono, Yasutaka, E-mail: ono@icrr.u-tokyo.ac.jp [Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago 763-0355 (Chile)

    2014-11-01

    We present the statistics of faint submillimeter/millimeter galaxies (SMGs) and serendipitous detections of a submillimeter/millimeter line emitter (SLE) with no multi-wavelength continuum counterpart revealed by the deep ALMA observations. We identify faint SMGs with flux densities of 0.1-1.0 mJy in the deep Band-6 and Band-7 maps of 10 independent fields that reduce cosmic variance effects. The differential number counts at 1.2 mm are found to increase with decreasing flux density down to 0.1 mJy. Our number counts indicate that the faint (0.1-1.0 mJy, or SFR{sub IR} ∼ 30-300 M {sub ☉} yr{sup –1}) SMGs contribute nearly a half of the extragalactic background light (EBL), while the remaining half of the EBL is mostly contributed by very faint sources with flux densities of <0.1 mJy (SFR{sub IR} ≲ 30 M {sub ☉} yr{sup –1}). We conduct counts-in-cells analysis with multifield ALMA data for the faint SMGs, and obtain a coarse estimate of galaxy bias, b {sub g} < 4. The galaxy bias suggests that the dark halo masses of the faint SMGs are ≲ 7 × 10{sup 12} M {sub ☉}, which is smaller than those of bright (>1 mJy) SMGs, but consistent with abundant high-z star-forming populations, such as sBzKs, LBGs, and LAEs. Finally, we report the serendipitous detection of SLE-1, which has no continuum counterparts in our 1.2 mm-band or multi-wavelength images, including ultra deep HST/WFC3 and Spitzer data. The SLE has a significant line at 249.9 GHz with a signal-to-noise ratio of 7.1. If the SLE is not a spurious source made by the unknown systematic noise of ALMA, the strong upper limits of our multi-wavelength data suggest that the SLE would be a faint galaxy at z ≳ 6.

  13. Artificial heart for humanoid robot using coiled SMA actuators

    Science.gov (United States)

    Potnuru, Akshay; Tadesse, Yonas

    2015-03-01

    Previously, we have presented the design and characterization of artificial heart using cylindrical shape memory alloy (SMA) actuators for humanoids [1]. The robotic heart was primarily designed to pump a blood-like fluid to parts of the robot such as the face to simulate blushing or anger by the use of elastomeric substrates for the transport of fluids. It can also be used for other applications. In this paper, we present an improved design by using high strain coiled SMAs and a novel pumping mechanism that uses sequential actuation to create peristalsis-like motions, and hence pump the fluid. Various placements of actuators will be investigated with respect to the silicone elastomeric body. This new approach provides a better performance in terms of the fluid volume pumped.

  14. KONSUMSI SUPLEMEN ATLET REMAJA DI SMA RAGUNAN JAKARTA

    Directory of Open Access Journals (Sweden)

    Muhammad Q Aliyyan Wijaya

    2015-05-01

    Full Text Available ABSTRACTThe objective of this study was to investigate consumption of supplement among Ragunan High School Jakarta athletes. The cross sectional study was done with total subjects were 79 students of Ragunan high school who were willing to join the study and they were at school when the study was conducted. There was 92.4% athletes consumed supplement in last one year. All athletes from light and heavy sport category were found consumed supplement. The most popular supplement were vitamin, mineral, and phytonutrition in tablet form. There was 89.0% athletes consumed supplement everyday. Moreover, the main reason for supplementation was to meet a nutrition requirement. The source of information about food supplement was mostly from coach advisor. More than half of athletes got supplement for free from any sources. There was a significant correlation between category of sport and number of supplement used (p<0.05.Keywords: adolescent, athlete, high school, supplementABSTRAKTujuan penelitian adalah menggambarkan konsumsi suplemen pada atlet remaja di SMA Ragunan Jakarta. Desain penelitian ini menggunakan cross sectional dengan total subjek sebanyak 79 siswa SMA Ragunan yang bersedia mengikuti penelitian dan berada di sekolah saat penelitian dilakukan. Sebanyak 92,4% atlet mengaku mengonsumsi suplemen dalam satu tahun terakhir. Atlet dari kategori olahraga ringan dan berat sekali semuanya mengonsumsi suplemen. Suplemen vitamin, mineral, dan fitonutrisi dalam bentuk tablet merupakan jenis dan bentuk suplemen yang paling banyak dikonsumsi. Sebanyak 89,0% dari atlet mengonsumsi suplemen setiap hari. Alasan utama atlet mengonsumsi suplemen adalah untuk memenuhi kebutuhan gizi. Pelatih merupakan sumber infomasi tentang suplemen yang paling banyak dipilih oleh atlet. Lebih dari 50,0% atlet mendapatkan suplemen dengan cara diberi. Kategori olahraga dan jumlah suplemen yang dikonsumsi menunjukkan hubungan positif signifikan (p<0,05.Kata kunci: atlet, remaja

  15. Formation of Combined Surface Features of Protrusion Array and Wrinkles atop Shape-Memory Polymer

    Science.gov (United States)

    Sun, L.; Zhao, Y.; Huang, W. M.; Tong, T. H.

    We demonstrate a simple and cost-effective approach to realize two combined surface features of different scales together, namely submillimeter-sized protrusion array and microwrinkles, atop a polystyrene shape-memory polymer. Two different types of protrusions, namely flat-top protrusion and crown-shaped protrusion, were studied. The array of protrusions was produced by the Indentation-Polishing-Heating (IPH) process. Compactly packed steel balls were used for making array of indents. A thin gold layer was sputter deposited atop the polymer surface right after polishing. After heating for shape recovery, array of protrusions with wrinkles on the top due to the buckling of gold layer was produced.

  16. An SMA Continuum Survey of Circumstellar Disks in the Serpens Star-forming Region

    Science.gov (United States)

    Law, Charles J.; Ricci, Luca; Andrews, Sean M.; Wilner, David J.; Qi, Chunhua

    2017-12-01

    We present observations with the Submillimeter Array of the continuum emission at λ =1.3 {mm} from 62 young stars surrounded by a protoplanetary disk in the Serpens star-forming region. The typical angular resolution for the survey in terms of beam size is 3\\buildrel{\\prime\\prime}\\over{.} 5× 2\\buildrel{\\prime\\prime}\\over{.} 5 with a median rms noise level of 1.6 mJy beam‑1. These data are used to infer the dust content in disks around low-mass stars (0.1{--}2.5 {M}ȯ ) at a median stellar age of 1–3 Myr. Thirteen sources were detected in the 1.3 mm dust continuum with inferred dust masses of ≈ 10{--}260 {M}\\oplus and an upper limit to the median dust mass of {5.1}-4.3+6.1 {M}\\oplus , derived using survival analysis. Comparing the protoplanetary disk population in Serpens to those of other nearby star-forming regions, we find that the populations of dust disks in Serpens and Taurus, which have a similar age, are statistically indistinguishable. This is potentially surprising as Serpens has a stellar surface density two orders of magnitude in excess of Taurus. Hence, we find no evidence that dust disks in Serpens have been dispersed as a result of more frequent and/or stronger tidal interactions due to its elevated stellar density. We also report that the fraction of Serpens disks with {M}{dust}≥slant 10 {M}\\oplus is less than 20%, which supports the notion that the formation of giant planets is likely inherently rare or has substantially progressed by a few Myr.

  17. Diamond Heat-Spreader for Submillimeter-Wave Frequency Multipliers

    Science.gov (United States)

    Lin, Robert H.; Schlecht, Erich T.; Chattopadhyay, Goutam; Gill, John J.; Mehdi, Imran; Siegel, Peter H.; Ward, John S.; Lee, Choonsup; Thomas, Bertrand C.; Maestrini, Alain

    2010-01-01

    The planar GaAs Shottky diode frequency multiplier is a critical technology for the local oscillator (LO) for submillimeter- wave heterodyne receivers due to low mass, tenability, long lifetime, and room-temperature operation. The use of a W-band (75-100 GHz) power amplifier followed by a frequency multiplier is the most common for submillimeter-wave sources. Its greatest challenge is to provide enough input power to the LO for instruments onboard future planetary missions. Recently, JPL produced 800 mW at 92.5 GHz by combining four MMICs in parallel in a balanced configuration. As more power at W-band is available to the multipliers, their power-handling capability be comes more important. High operating temperatures can lead to degradation of conversion efficiency or catastrophic failure. The goal of this innovation is to reduce the thermal resistance by attaching diamond film as a heat-spreader on the backside of multipliers to improve their power-handling capability. Polycrystalline diamond is deposited by hot-filament chemical vapor deposition (CVD). This diamond film acts as a heat-spreader to both the existing 250- and 300-GHz triplers, and has a high thermal conductivity (1,000-1,200 W/mK). It is approximately 2.5 times greater than copper (401 W/mK) and 20 times greater than GaAs (46 W/mK). It is an electrical insulator (resistivity approx. equals 10(exp 15) Ohms-cm), and has a low relative dielectric constant of 5.7. Diamond heat-spreaders reduce by at least 200 C at 250 mW of input power, compared to the tripler without diamond, according to thermal simulation. This superior thermal management provides a 100-percent increase in power-handling capability. For example, with this innovation, 40-mW output power has been achieved from a 250-GHz tripler at 350-mW input power, while the previous triplers, without diamond, suffered catastrophic failures. This breakthrough provides a stepping-stone for frequency multipliers-based LO up to 3 THz. The future work

  18. Submillimeter Galaxies as Progenitors of Compact Quiescent Galaxies

    Science.gov (United States)

    Toft, S.; Smolcic, V.; Magnelli, B.; Karim, A.; Zirm, A.; Michalowski, M.; Capak, P.; Sheth, K.; Schawinski, K.; Krogager, J.-K.; hide

    2014-01-01

    Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were already old, quiescent systems with little to no residual star formation and extremely compact with stellar mass densities at least an order of magnitude larger than in low-redshift ellipticals, their descendants. Little is known about how they formed, but their evolved, dense stellar populations suggest formation within intense, compact starbursts 1-2 Gyr earlier (at 3 < z < 6). Simulations show that gas-rich major mergers can give rise to such starbursts, which produce dense remnants. Submillimeter-selected galaxies (SMGs) are prime examples of intense, gas-rich starbursts.With a new, representative spectroscopic sample of compact, quiescent galaxies at z = 2 and a statistically well-understood sample of SMGs, we show that z = 3-6 SMGs are consistent with being the progenitors of z = 2 quiescent galaxies, matching their formation redshifts and their distributions of sizes, stellar masses, and internal velocities. Assuming an evolutionary connection, their space densities also match if the mean duty cycle of SMG starbursts is 42(sup+40) -29 Myr (consistent with independent estimates), which indicates that the bulk of stars in these massive galaxies were formed in a major, early surge of star formation. These results suggest a coherent picture of the formation history of the most massive galaxies in the universe, from their initial burst of violent star formation through their appearance as high stellar-density galaxy cores and to their ultimate fate as giant ellipticals.

  19. Submillimeter galaxies as progenitors of compact quiescent galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Toft, S.; Zirm, A.; Krogager, J.-K.; Man, A. W. S. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Mariesvej 30, DK-2100 Copenhagen (Denmark); Smolčić, V.; Krpan, J. [Physics Department, University of Zagreb, Bijenička cesta 32, 10002 Zagreb (Croatia); Magnelli, B.; Karim, A. [Argelander Institute for Astronomy, Auf dem Hügel 71, Bonn, D-53121 (Germany); Michalowski, M. [Scottish Universities Physics Alliance, Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ (United Kingdom); Capak, P. [Spitzer Science Center, 314-6 Caltech, 1201 East California Boulevard, Pasadena, CA 91125 (United States); Sheth, K. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Schawinski, K. [ETH Zurich, Institute for Astronomy, Department of Physics, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich (Switzerland); Wuyts, S.; Lutz, D.; Staguhn, J.; Berta, S. [MPE, Postfach 1312, D-85741 Garching (Germany); Sanders, D. [Institute for Astronomy, 2680 Woodlawn Drive, University of Hawaii, Honolulu, HI 96822 (United States); Mccracken, H. [Institut dAstrophysique de Paris, UMR7095 CNRS, Universite Pierre et Marie Curie, 98 bis Boulevard Arago, F-75014 Paris (France); Riechers, D., E-mail: sune@dark-cosmology.dk [Department of Astronomy, Cornell University, 220 Space Sciences Building, Ithaca, NY 14853 (United States)

    2014-02-20

    Three billion years after the big bang (at redshift z = 2), half of the most massive galaxies were already old, quiescent systems with little to no residual star formation and extremely compact with stellar mass densities at least an order of magnitude larger than in low-redshift ellipticals, their descendants. Little is known about how they formed, but their evolved, dense stellar populations suggest formation within intense, compact starbursts 1-2 Gyr earlier (at 3 < z < 6). Simulations show that gas-rich major mergers can give rise to such starbursts, which produce dense remnants. Submillimeter-selected galaxies (SMGs) are prime examples of intense, gas-rich starbursts. With a new, representative spectroscopic sample of compact, quiescent galaxies at z = 2 and a statistically well-understood sample of SMGs, we show that z = 3-6 SMGs are consistent with being the progenitors of z = 2 quiescent galaxies, matching their formation redshifts and their distributions of sizes, stellar masses, and internal velocities. Assuming an evolutionary connection, their space densities also match if the mean duty cycle of SMG starbursts is 42{sub −29}{sup +40} Myr (consistent with independent estimates), which indicates that the bulk of stars in these massive galaxies were formed in a major, early surge of star formation. These results suggest a coherent picture of the formation history of the most massive galaxies in the universe, from their initial burst of violent star formation through their appearance as high stellar-density galaxy cores and to their ultimate fate as giant ellipticals.

  20. Analysis and Evaluation of the Dynamic Performance of SMA Actuators for Prosthetic Hand Design

    Science.gov (United States)

    O'Toole, Kevin T.; McGrath, Mark M.; Coyle, Eugene

    2009-08-01

    It is widely acknowledged within the biomedical engineering community that shape memory alloys (SMAs) exhibit great potential for application in the actuation of upper limb prosthesis designs. These lightweight actuators are particularly suitable for prosthetic hand solutions. A four-fingered, 12 degree-of-freedom prosthetic hand has been developed featuring SMA bundle actuators embedded within the palmar structure. Joule heating of the SMA bundle actuators generates sufficient torque at the fingers to allow a wide range of everyday tasks to be carried out. Transient characterization of SMA bundles has shown that performance/response during heating and cooling differs substantially. Natural convection is insufficient to provide for adequate cooling during elongation of the actuators. An experimental test-bed has been developed to facilitate analysis of the heat transfer characteristics of the appropriately sized SMA bundle actuators for use within the prosthetic hand design. Various modes of heat sinking are evaluated so that the most effective wire-cooling solution can be ascertained. SMA bundles of varying size will be used so that a generalized model of the SMA displacement performance under natural and forced cooling conditions can be obtained. The optimum cooling solution will be implemented onto the mechanical hand framework in future work. These results, coupled with phenomenological models of SMA behavior, will be used in the development of an effective control strategy for this application in future work.

  1. Cervical Spinal Cord Atrophy Profile in Adult SMN1-Linked SMA.

    Directory of Open Access Journals (Sweden)

    Mohamed-Mounir El Mendili

    Full Text Available The mechanisms underlying the topography of motor deficits in spinal muscular atrophy (SMA remain unknown. We investigated the profile of spinal cord atrophy (SCA in SMN1-linked SMA, and its correlation with the topography of muscle weakness.Eighteen SMN1-linked SMA patients type III/V and 18 age/gender-matched healthy volunteers were included. Patients were scored on manual muscle testing and functional scales. Spinal cord was imaged using 3T MRI system. Radial distance (RD and cord cross-sectional area (CSA measurements in SMA patients were compared to those in controls and correlated with strength and disability scores.CSA measurements revealed a significant cord atrophy gradient mainly located between C3 and C6 vertebral levels with a SCA rate ranging from 5.4% to 23% in SMA patients compared to controls. RD was significantly lower in SMA patients compared to controls in the anterior-posterior direction with a maximum along C4 and C5 vertebral levels (p-values < 10-5. There were no correlations between atrophy measurements, strength and disability scores.Spinal cord atrophy in adult SMN1-linked SMA predominates in the segments innervating the proximal muscles. Additional factors such as neuromuscular junction or intrinsic skeletal muscle defects may play a role in more complex mechanisms underlying weakness in these patients.

  2. Pelaksanaan Manajemen Personalia Sekolah di SMA Darul Ulum 2 BPPT Jombang

    Directory of Open Access Journals (Sweden)

    Muhamad Zaki

    2016-12-01

    Full Text Available Artikel ini membahas pelaksanaan manajemen personalia sekolah di salah satu sekolah menengah atas terkemuka di Jombang, yaitu SMA Darul Ulum 2 BPPT Jombang yang berada di lingkungan Pondok Pesantren Darul Ulum. SMA Darul Ulum 2 Unggulan BPPT Jombang adalah salah satu sekolah yang relevan dengan persoalan manajemen personalia. Dengan latar belakang pesantren, maka kurikulum yang diterapkan di SMA Darul Ulum 2 Unggulan BPPT tentu tidak lepas dari warna-warni dunia pesantren. Ini bisa dianggap sebagai pengembangan kurikulum nasional khususnya pada mata pelajaran Pendidikan Agama Islam. Dua warna yang berbeda namun bisa disejajarkan bersama inilah yang menjadi ciri khas yang unik dan bisa dibilang tidak terdapat pada sekolah lain. Dari latar belakang tersebut peneliti bermaksud untuk melakukan sebuah kajian dan penelitian yang terkait dengan bagaimana manajemen personalia yang ada di SMA Darul Ulum 2 Unggulan BPPT di Pondok Pesantren Darul Ulum Jombang Jawa Timur Indonesia. || This article discusses implementation of school personnel management in one of the best high schools in Jombang, namely SMA Darul Ulum 2 BTTP Jombang located inside the Pondok Pesantren Darul Ulum Jombang. SMA Darul Ulum 2 BTTP Jombang is one of the schools that are relevant to the issue of personnel management. Because of it’s pesantren (Islamic boarding school background, the curriculum applied in SMA Darul Ulum 2 BPPT Jombang is not separated from the pesantren world. This can be considered as a national curriculum development, especially on the subjects of Islamic education. Two different colors can be lumped together. It is the characteristic of the SMA Darul Ulum 2 BTTP Jombang that may not be found in other reguler schools. Thus, the researcher intend to conduct research related to how is the implementation of personnel management at SMA Darul Ulum 2 BPPT Jombang located inside Pondok Pesantren Darul Ulum Jombang, East Java, Indonesia.

  3. National education ideology as the orientation of the school culture development policy at SMA N 1 and SMA N 3 Yogyakarta

    Directory of Open Access Journals (Sweden)

    Lusila Andriani Purwastuti

    2017-09-01

    Full Text Available This study aimed at describing the national education ideology as the orientation of the school culture development policy at SMA N 1 and SMAN 3 Yogyakarta. This research employed the qualitative approach through ethnography method. The subjects of the research were the school community. The object was the implementation of Pancasila on the development of the school culture. The data were collected through interviews, observations, and documentation. The data were analyzed using ethnography analysis as suggested by Spradley and they were validated by data triangulation and member checks. The results show that the national education ideology as the orientation of the school culture development is understood: (1 as an open ideology; (2 implemented on the basis value; instrumental values; the value of practices in the school culture; (3 The school culture in SMA N 1 and SMA N 3 is the implementation and contextualization of the values of Pancasila, along with the uniqueness of SMA N 1 with its “Teladan” icon which represents the religious morality and intellectual, as well as at SMA N 3 with its “Padmanaba” icon representing noble behavior. (4  Both schools have developed the school culture, namely: religious morality, social-culture, intellectual, and environment/management/leadership.

  4. Probabilistic fiber tracking of the language and motor white matter pathways of the supplementary motor area (SMA) in patients with brain tumors.

    Science.gov (United States)

    Jenabi, Mehrnaz; Peck, Kyung K; Young, Robert J; Brennan, Nicole; Holodny, Andrei I

    2014-12-01

    Accurate localization of anatomically and functionally separate SMA tracts is important to improve planning prior to neurosurgery. Using fMRI and probabilistic DTI techniques, we assessed the connectivity between the frontal language area (Broca's area) and the rostral pre-SMA (language SMA) and caudal SMA proper (motor SMA). Twenty brain tumor patients completed motor and language fMRI paradigms and DTI. Peaks of functional activity in the language SMA, motor SMA and Broca's area were used to define seed regions for probabilistic tractography. fMRI and probabilistic tractography identified separate and unique pathways connecting the SMA to Broca's area - the language SMA pathway and the motor SMA pathway. For all subjects, the language SMA pathway had a larger number of voxels (Planguage and motor SMA pathways than in background pathways (Planguage SMA pathway (degree of connectivity: Planguage SMA and motor SMA to Broca's area. The language SMA is more significantly connected to Broca's area than is the motor subdivision of the SMA proper. Copyright © 2013 Elsevier Masson SAS. All rights reserved.

  5. Mu-Spec: A High Performance Compact Spectrometer for Submillimeter Astronomy

    Science.gov (United States)

    Hsieh, Wen-Ting; Moseley, Harvey; Stevenson, Thomas; Brown, Ari; Patel, Amil; U-yen, Kongpop; Ehsan, Negar; Cataldo, Giuseppe; Wollack, Ed

    2012-01-01

    We describe the Mu-Spec, an extremely compact high performance spectrometer for the submillimeter and millimeter spectral ranges. We have designed a fully integrated submillimeter spectrometer based on superconducting microstrip technology and fabricated its critical elements. Using low loss transmission lines, we can produce a fully integrated high resolution submillimeter spectrometer on a single four inch Si wafer. A resolution of 500 can readily be achieved with standard fabrication tolerance, higher with phase trimming. All functions of the spectrometer are integrated - light is coupled to the microstrip circuit with a planar antenna, the spectra discrimination is achieved using a synthetic grating, orders are separated using a built-in planar filter, and the light is detected using photon counting Microwave Kinetic Inductance Detectors (MKID). We will discus the design principle of the instrument, describe its technical advantages, and report the progress on the development of the instrument.

  6. Micro-Spec: A High Performance Compact Spectrometer for Submillimeter Astronomy

    Science.gov (United States)

    Hsieh, Wen-Ting; Moseley, Harvey; Stevenson, Thomas; Brown, Ari; Patel, Amil; U-Yen, Kongpop; Ehsan, Negar; Caltado, Giuseppe; Wollock, Edward

    2012-01-01

    We describe the micro-Spec, an extremely compact high performance spectrometer for the submillimeter and millimeter spectral ranges. We have designed a fully integrated submillimeter spectrometer based on superconducting microstrip technology and fabricated its critical elements. Using low loss transmission lines, we can produce a fully integrated high resolution submillimeter spectrometer on a single four inch Si wafer. A resolution of 500 can readily be achieved with standard fabrication tolerance, higher with phase trimming. All functions of the spectrometer are integrated - light is coupled to the micro strip circuit with a planar antenna, the spectra discrimination is achieved using a synthetic grating, orders are separated using a built-in planar filter, and the light is detected using photon counting Microwave Kinetic Inductance Detectors (MKID). We will discus the design principle of the instrument, describe its technical advantages, and report the progress on the development of the instrument.

  7. Ionoacoustic characterization of the proton Bragg peak with submillimeter accuracy

    Energy Technology Data Exchange (ETDEWEB)

    Assmann, W., E-mail: walter.assmann@lmu.de; Reinhardt, S.; Lehrack, S.; Edlich, A.; Thirolf, P. G.; Parodi, K. [Department for Medical Physics, Ludwig-Maximilians-Universität München, Am Coulombwall 1, Garching 85748 (Germany); Kellnberger, S.; Omar, M.; Ntziachristos, V. [Institute for Biological and Medical Imaging, Technische Universität München and Helmholtz Zentrum München, Ingolstädter Landstrasse 1, Neuherberg 85764 (Germany); Moser, M.; Dollinger, G. [Institute for Applied Physics and Measurement Technology, Universität der Bundeswehr, Werner-Heisenberg-Weg 39, Neubiberg 85577 (Germany)

    2015-02-15

    Purpose: Range verification in ion beam therapy relies to date on nuclear imaging techniques which require complex and costly detector systems. A different approach is the detection of thermoacoustic signals that are generated due to localized energy loss of ion beams in tissue (ionoacoustics). Aim of this work was to study experimentally the achievable position resolution of ionoacoustics under idealized conditions using high frequency ultrasonic transducers and a specifically selected probing beam. Methods: A water phantom was irradiated by a pulsed 20 MeV proton beam with varying pulse intensity and length. The acoustic signal of single proton pulses was measured by different PZT-based ultrasound detectors (3.5 and 10 MHz central frequencies). The proton dose distribution in water was calculated by Geant4 and used as input for simulation of the generated acoustic wave by the matlab toolbox k-WAVE. Results: In measurements from this study, a clear signal of the Bragg peak was observed for an energy deposition as low as 10{sup 12} eV. The signal amplitude showed a linear increase with particle number per pulse and thus, dose. Bragg peak position measurements were reproducible within ±30 μm and agreed with Geant4 simulations to better than 100 μm. The ionoacoustic signal pattern allowed for a detailed analysis of the Bragg peak and could be well reproduced by k-WAVE simulations. Conclusions: The authors have studied the ionoacoustic signal of the Bragg peak in experiments using a 20 MeV proton beam with its correspondingly localized energy deposition, demonstrating submillimeter position resolution and providing a deep insight in the correlation between the acoustic signal and Bragg peak shape. These results, together with earlier experiments and new simulations (including the results in this study) at higher energies, suggest ionoacoustics as a technique for range verification in particle therapy at locations, where the tumor can be localized by ultrasound

  8. Next Generation Solar Array Technologies for Small Satellites

    OpenAIRE

    Fosness, E.; Guerrero, J.; Mayberry, C; Carpenter, B; Goldstein, D.

    2002-01-01

    Recent advances in Shape Memory Alloy (SMA), Elastic Memory Composites (EMC), and ultra- light composites along with thin-film Copper-Indium- Diselinide (CIS) photovoltaics have offered the potential to provide solar array systems for small satellites that are significantly lighter than the current state of the practice. The Air Force Research Laboratory (AFRL), National Aeronautics and Space Administration (NASA) Langley, Defense Advanced Research Projects Agency (DARPA), and Lockheed Martin...

  9. Kondisi Stres Akademik Siswa SMA Negeri di Kota Padang

    Directory of Open Access Journals (Sweden)

    Taufik Taufik

    2014-01-01

    Full Text Available This research conduct base from increasing the National Examination standards from recent years, and overload student’s learning activity in Senior High School (SMA. These conditions as triggers stress students, from a long time, its influence on their learning. Based that, the research is to identify level of student academic stress, and differences base gender, and school location. This research use Cluster Random Sampling. Samples are grouped into 3 (three, that’s school is located in downtown, midtown and the Suburbs. Research findings show that there are 15% of student’s stress academic at low levels of, 71,8% experiencing stress academic at medium level, and 13.2% of students experiencing stress academic at high level. There was no significant difference between the academic stress Student SMAN in Padang by location and gender. These research findings can then be an important basic need for guidance and counseling services in order to decrease the level of stress of academic students in Padang city, so that they can learn by making every effort that is optimal.

  10. ALTERNATIF STRATEGI PENINGKATAN DAYA SAING SMA KRISTEN 2 SALATIGA

    Directory of Open Access Journals (Sweden)

    Innes Septa Nindiarini

    2015-06-01

    Full Text Available This research and development aims to formulate strategic plan to enhancing competitiveness in SMA Kristen 2 Salatiga. Data were gathered by means of Focus Group Discussion (FGD, interview, questionnaire, and documentation study. Fishbone analysis is used to identify the root causes of low school competitiveness. The analysis was categorized based on five factors i.e. reputation, school resources, information and technology, human resource, and partnership. Based on the analysis, the strategies are formulated with educational reengineering approach as follows: 1 reconstructing school image by improving academic and non academic achievement, 2 developing innovative curriculum based on outdoor experience and IT, 3 increasing student discipline, 4optimizing IT usage on promotion and marketing, 5 improving the quality of school programs, 6 developing entrepreneurship programs, 7 improving the quantity and quality school infrastructures, 8 improving teachers’ skill and competence of IT, 9 enhancing the role of school board, 10 maximizing the role of parents, alumnae, and other institution to develop the school programs, and 11 establishing a vocational high school. It is recommended for the school to have cooperation with the stakeholder and the school board to implement the strategic plan so that the competitiveness will enhance in the future.

  11. Klasifikasi dan Klastering Penjurusan Siswa SMA Negeri 3 Boyolali

    Directory of Open Access Journals (Sweden)

    Yusuf Sulistyo Nugroho

    2015-12-01

    Full Text Available SMA N 3 Boyolali merupakan salah satu sekolah menengah di kota Boyolali yang saat ini telah memiliki 2 jurusan yaitu IPA dan IPS. Penjurusan siswa ini dapat mengarahkan peserta didik agar lebih fokus dalam mengembangkan kemampuan diri dan minat yang dimiliki. Pemilihan jurusan yang tidak tepat bisa sangat merugikan siswa terhadap minat dan karir mereka di masa mendatang. Dengan penjurusan tersebut diharapkan dapat memaksimalkan potensi, bakat atau talenta individu, sehingga dapat memaksimalkan nilai akademisnya. Berdasarkan latar belakang tersebut, maka dengan menerapkan teknik data mining diharapkan dapat membantu siswa untuk menentukan jurusan yang tepat sesuai dengan kriteria yang ditetapkan. Adapaun teknik data mining yang digunakan dalam penentuan jurusan ini menggunakan 3 buah metode yaitu Algoritma C4.5, Naive Bayes dan Algoritma K-Means. Sedangkan atribut yang digunakan terdiri dari Gender, Minat, Rata-rata nilai IPA, Rata-rata nilai IPS, nilai Psikotest IPA, nilai Psikotest IPS, Asal Sekolah dan Jurusan. Analisis dilakukan dengan bantuan aplikasi RapidMiner 5 untuk mengetahui nilai-nilai perbandingan terhadap metode yang digunakan. Hasil penelitian menggunakan perbandingan 3 metode menunjukkan bahwa berdasarkan nilai precision, metode naive bayes lebih baik dibandingkan dengan metode yang lain dengan nilai 77,51%. Sedangkan berdasarkan nilai recall dan accuracy, decision tree lebih baik dibandingkan dengan metode yang lain dengan nilai recall sebesar 90,80% dan nilai accuracy sebesar 79,14%. Variabel yang paling berpengaruh dalam menentukan penjurusan yaitu rata-rata nilai IPA sehingga perlu dijadikan pertimbangan bagi pihak sekolah untuk menentukan jurusan siswa.

  12. The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS

    NARCIS (Netherlands)

    Simpson, J. M.; Smail, Ian; Swinbank, A. M.; Ivison, R. J.; Dunlop, J. S.; Geach, J. E.; Almaini, O.; Arumugam, V.; Bremer, M. N.; Chen, Chian-Chou; Conselice, C.; Coppin, K. E. K.; Farrah, D.; Ibar, E.; Hartley, W. G.; Ma, C. J.; Michałowski, M. J.; Scott, D.; Spaans, M.; Thomson, A. P.; van der Werf, P. P.

    2017-01-01

    We present a multi-wavelength analysis of 52 submillimeter galaxies (SMGs), identified using ALMA 870 μm continuum imaging in a pilot program to precisely locate bright SCUBA-2-selected submillimeter sources in the UKIDSS Ultra Deep Survey (UDS) field. Using the available deep (especially

  13. Internal rupture and rapid bouncing of impacting drops induced by submillimeter-scale textures

    Science.gov (United States)

    Zhang, Rui; Zhang, Xiwen; Hao, Pengfei; He, Feng

    2017-06-01

    We demonstrate an internal breakup mechanism for high Weber number drop impact on superhydrophobic surfaces uniformly patterned with submillimeter-scale textures, in which the liquid film ruptures from both interior and rim. The employment of submillimeter-scale posts could help decrease the critical Weber number of internal rupture, due to the small solid fraction and the large dimension ratio between primary structures and droplets. The internal rupture is found to promote more rapid drop bouncing than conventional rebound and rim breakup on superhydrophobic surfaces with small roughness, with a 10%-50% reduction of contact time. The internal rupture results from the film instability inside and the jet instability outside.

  14. Internal rupture and rapid bouncing of impacting drops induced by submillimeter-scale textures.

    Science.gov (United States)

    Zhang, Rui; Zhang, Xiwen; Hao, Pengfei; He, Feng

    2017-06-01

    We demonstrate an internal breakup mechanism for high Weber number drop impact on superhydrophobic surfaces uniformly patterned with submillimeter-scale textures, in which the liquid film ruptures from both interior and rim. The employment of submillimeter-scale posts could help decrease the critical Weber number of internal rupture, due to the small solid fraction and the large dimension ratio between primary structures and droplets. The internal rupture is found to promote more rapid drop bouncing than conventional rebound and rim breakup on superhydrophobic surfaces with small roughness, with a 10%-50% reduction of contact time. The internal rupture results from the film instability inside and the jet instability outside.

  15. Persepsi Siswa Terhadap Pembelajaran Guru Pendidikan Jasmani Di SMA Muhammadiyah Kediri

    Directory of Open Access Journals (Sweden)

    Hendra Mashuri

    2017-05-01

    Full Text Available Tujuan yang ingin dicapai dalam penelitian ini adalah untuk memperoleh informasi tentang persepsi siswa terhadap pembelajaran guru pendidikan jasmani di SMA Muhammadiyah Kediri. Rumusan masalah dalam penelitian ini adalah bagaimana persepsi siswa terhadap pembelajaran guru pendidikan jasmani di SMA Muhammadiyah Kediri? Jenis penelitian ini adalah penelitian survei. Populasi yang digunakan adalah seluruh siswa SMA Muhammadiyah Kediri, sampel yang diambil berjumlah 60 siswa yang terdiri dari 20 siswa dari masing-masing kelas. Instrumen yang digunakan adalah angket dan dokumentasi. Teknik analisis data menggunakan persentase. Hasil penelitian menunjukkan bahwa persepsi siswa terhadap proses pembelajaran SMA Muhammadiyah Kediri mendapatkan skor 3115 atau rata-rata jawaban siswa 51,917 dengan persentase sebesar 74% dan masuk dalam kategori “Baik”. Dengan demikian dapat dikatakan bahwa persepsi siswa terhadap pembelajaran guru pendidikan jasmani adalah baik.

  16. Application of martensitic SMA alloys as passive dampers of GFRP laminated composites

    Directory of Open Access Journals (Sweden)

    M. Bocciolone

    2013-01-01

    Full Text Available This paper describes the application of SMA (Shape Memory Alloy materials to enhance the passive damping of GFRP (Glass Fiber Reinforced Plastic laminated composite. The SMA has been embedded as reinforcement in the GFRP laminated composite and a SMA/GFRP hybrid composite has been obtained. Two SMA alloys have been studied as reinforcement and characterized by thermo-mechanical tests. The architecture of the hybrid composite has been numerically optimized in order to enhance the structural damping of the host GFRP laminated, without significant changes of the specific weight and of the flexural stiffness. The design and the resultant high damping material are interesting and will be useful in general for applications related to passive damping. The application to a new designed lateral horn of railway collector of the Italian high speed trains is discussed.

  17. Optimal design of damping layers in SMA/GFRP laminated hybrid composites

    Science.gov (United States)

    Haghdoust, P.; Cinquemani, S.; Lo Conte, A.; Lecis, N.

    2017-10-01

    This work describes the optimization of the shape profiles for shape memory alloys (SMA) sheets in hybrid layered composite structures, i.e. slender beams or thinner plates, designed for the passive attenuation of flexural vibrations. The paper starts with the description of the material and architecture of the investigated hybrid layered composite. An analytical method, for evaluating the energy dissipation inside a vibrating cantilever beam is developed. The analytical solution is then followed by a shape profile optimization of the inserts, using a genetic algorithm to minimize the SMA material layer usage, while maintaining target level of structural damping. Delamination problem at SMA/glass fiber reinforced polymer interface is discussed. At the end, the proposed methodology has been applied to study the hybridization of a wind turbine layered structure blade with SMA material, in order to increase its passive damping.

  18. Evaluation of Fatigue Life of CRM-Reinforced SMA and Its Relationship to Dynamic Stiffness

    National Research Council Canada - National Science Library

    Mashaan, Nuha Salim; Karim, Mohamed Rehan; Abdel Aziz, Mahrez; Ibrahim, Mohd Rasdan; Katman, Herda Yati; Koting, Suhana

    2014-01-01

    .... The aim of this study is to evaluate the effect of crumb rubber modifier (CRM) on stiffness and fatigue properties of SMA mixtures at optimum binder content, using four different modification levels, namely, 6%, 8%, 10%, and 12...

  19. Pengaruh Motivasi Belajar terhadap Hasil Belajar Mata Pelajaran Sosiologi Kelas X Iis SMA Negeri 4 Pontianak

    OpenAIRE

    Putri, Yessi Pratiwi

    2017-01-01

    The title of this thesis “The Influence of Student Motivation on Sociology Learning Outcome Class X IIS SMA Negeri 4 Pontianak”. The common problem studies “How the influence of students' motivation on learning outcome of sociology class X IIS SMA Negeri 4 Pontianak?”. The method used is descriptive method and form of study correlation. Total population is 120 respondents and sample is 93 respondents. Data collection technique used indirect communication technique and documentation techniques...

  20. Feasibility of Using Foamed Styrene Maleic Anhydride (SMA) Co-polymer in Wood Based Composites

    OpenAIRE

    Mustafa Zor; Nurgul Tankut; Alper Kiziltas; Douglas Gardner; Hikmet Yazici

    2017-01-01

    Wood plastic composites (WPCs) have often been used in consumer applications, automotive industry and exterior construction. WPCs consist mostly of wood and thermoplastic polymer. WPCs can have superior outdoor durability and much lower maintenance costs than regular wood. WPCs can be used instead of wood. Styrene maleic anhydride (SMA) is used in plastic composites for the automotive industry and also in engineering applications. SMA wood composites, as one of the WPCs using wood fibers as r...

  1. Pengembangan Media Pembelajaran Spesimen Moluska Pada Materi Animalia Kelas X Di SMA Negeri 1 Rambah Samo

    OpenAIRE

    Rofiza Yolanda., Yuni Artasari Rena Lestari

    2017-01-01

    . This research aims to determine the feasibility of using instructional media with material molluscs specimens Animalia class X SMA. This research was conducted from April to June 2016. This type of research is the development of research (Research and Development) developed by Borg and Gall have been modified. The data collection is done by using a questionnaire and the data were analyzed descriptively. The results showed that the use of instructional media molluscs specimens in class X SMA...

  2. Sistem Informasi Berbasis Web Untuk Mendata Semua SMA Di Kabupaten Langkat

    OpenAIRE

    Pratiwi, Erwina

    2011-01-01

    Kajian ini bertujuan untuk membangun website yang dinamis. Sistem informasi berbasis web untuk mendata semua SMA di Kabupaten Langkat, ini dikembangkan dengan menggunakan sistem operasi Windows XP dan software Dreamweaver Marcomedia 8, web browser Mozilla Firefox 4.0 Beta 1 dan Xampp-Win32-1.6.4 yang merupakan gabungan dari Apache web server, PHP, dan MySQL. Tujuan website ini untuk menyajikan dan menyebarkan informasi umum mengenai semua SMA di Kabupaten Langkat secara onli...

  3. An alma survey of sub-millimeter galaxies in the extended Chandra deep field south: Sub-millimeter properties of color-selected galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Decarli, R.; Walter, F.; Hodge, J. A.; Rix, H.-W.; Schinnerer, E. [Max-Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); Smail, I.; Swinbank, A. M.; Karim, A.; Simpson, J. M. [Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE (United Kingdom); Chapman, S. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Coppin, K. E. K. [Centre for Astrophysics, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Cox, P. [IRAM, 300 rue de la piscine, F-38406 Saint-Martin d' Hères (France); Dannerbauer, H. [Universität Wien, Institut für Astrophysik, Türenschanzstrasse 17, A-1180 Wien (Austria); Greve, T. R. [University College London, Department of Physics and Astronomy, Gower Street, London WC1E 6BT (United Kingdom); Ivison, R. [Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Knudsen, K. K.; Lindroos, L. [Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, Onsala SE-439 92 (Sweden); Van der Werf, P. [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Weiß, A., E-mail: decarli@mpia.de [Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany)

    2014-01-10

    We study the sub-millimeter properties of color-selected galaxies via a stacking analysis applied for the first time to interferometric data at sub-millimeter wavelengths. We base our study on 344 GHz ALMA continuum observations of ∼20''-wide fields centered on 86 sub-millimeter sources detected in the LABOCA Extended Chandra Deep Field South (ECDFS) Sub-millimeter Survey. We select various classes of galaxies (K-selected, star-forming sBzK galaxies, extremely red objects, and distant red galaxies) according to their optical/near-infrared fluxes. We find clear, >10σ detections in the stacked images of all these galaxy classes. We include in our stacking analysis Herschel/SPIRE data to constrain the dust spectral energy distribution of these galaxies. We find that their dust emission is well described by a modified blackbody with T {sub dust} ≈ 30 K and β = 1.6 and infrared luminosities of (5-11) × 10{sup 11} L {sub ☉} or implied star formation rates of 75-140 M {sub ☉} yr{sup –1}. We compare our results with those of previous studies based on single-dish observations at 870 μm and find that our flux densities are a factor 2-3 higher than previous estimates. The discrepancy is observed also after removing sources individually detected in ALESS maps. We report a similar discrepancy by repeating our analysis on 1.4 GHz observations of the whole ECDFS. Hence, we find tentative evidence that galaxies that are associated in projected and redshift space with sub-mm bright sources are brighter than the average population. Finally, we put our findings in the context of the cosmic star formation rate density as a function of redshift.

  4. Mapping the thermal structure and minor species of Venus mesosphere with ALMA submillimeter observations

    Science.gov (United States)

    Piccialli, A.; Moreno, R.; Encrenaz, T.; Fouchet, T.; Lellouch, E.; Widemann, T.

    2017-10-01

    Context. Water vapor and sulfur compounds are key species in the photochemistry of Venus mesosphere. These species, together with mesospheric temperatures, exhibit drastic temporal variations, both on short timescales (diurnal and day-to-day) as well on long timescales, far from being understood. Aims: We targeted CO, SO, HDO and SO2 transitions in the submillimeter range using the Atacama Large Millimeter Array (ALMA) to study their spatial and temporal variations. Methods: Four sets of observations were acquired on different dates in November 2011 during the first ALMA Early Science observation Cycle 0. Venus angular diameter was about 11'' with an illumination factor of 92%, so that mostly the day side of the planet was mapped. Assuming a nominal CO abundance profile, we retrieved vertical temperature profiles over the entire disk as a function of latitude and local time. Temperature profiles were later used to retrieve SO, SO2, and H2O. We used HDO as a tracer for water assuming a D/H enrichment of 200 times the terrestrial value. Results: We derived 3D maps of mesospheric temperatures in the altitude range 70-105 km. SO, SO2, and H2O are characterized by a negligible abundance below 85 km followed by an increase with altitude in the upper mesosphere. Disk-averaged SO abundances present a maximum mixing ratio of 15.0 ± 3.1 ppb on November 26 followed the next day by a minimum value of 9.9 ± 1.2 ppb. Due to a very low S/N, SO2 could only be derived from the disk-averaged spectrum on the first day of observation revealing an abundance of 16.5 ± 4.6 ppb. We found a SO2/SO ratio of 1.5 ± 0.4. Global maps of SO reveal strong variations both with latitude and local time and from day to day with abundance ranging from < 1 to 15 ppb. H2O disk-averages retrievals reveal a steady decrease from November 14 to 27, with the abundance varying from 3.6 ± 0.6 ppm on the first day to 2.9 ± 0.7 ppm on the last day. H2O maps reveal a slightly higher abundance on the evening

  5. Experimental and numerical study on hysteretic performance of SMA spring-friction bearings

    Science.gov (United States)

    Zhuang, Peng; Xue, Suduo; Nie, Pan; Wang, Wenting

    2016-12-01

    This paper presents an experimental and numerical study to investigate the hysteretic performance of a new type of isolator consisting of shape memory alloy springs and friction bearing called an SMA spring-friction bearing (SFB). The SFB is a sliding-type isolator with SMA devices used for the seismic protection of engineering structures. The principle of operation of the isolation bearing is introduced. In order to explore the possibility of applying SMA elements in passive seismic control devices, large diameter superelastic tension/compression NiTi SMA helical springs used in the SFB isolator were developed. Mechanical experiments of the SMA helical spring were carried out to understand its superelastic characteristics. After that, a series of quasi-static tests on a single SFB isolator prototype were conducted to measure its force-displacement relationships for different loading conditions and study the corresponding variation law of its mechanical performance. The experimental results demonstrate that the SFB exhibits full hysteretic curves, excellent energy dissipation capacity, and moderate recentering ability. Finally, a theoretical model capable of emulating the hysteretic behavior of the SMA-based isolator was then established and implemented in MATLAB software. The comparison of the numerical results with the experimental results shows the efficacy of the proposed model for simulating the response of the SFB.

  6. Behavior of NiTiNb SMA wires under recovery stress or prestressing.

    Science.gov (United States)

    Choi, Eunsoo; Nam, Tae-Hyun; Chung, Young-Soo; Kim, Yeon-Wook; Lee, Seung-Yong

    2012-01-05

    The recovery stress of martensitic shape-memory alloy [SMA] wires can be used to confine concrete, and the confining effectiveness of the SMA wires was previously proved through experimental tests. However, the behavior of SMA wires under recovery stress has not been seriously investigated. Thus, this study conducted a series of tests of NiTiNb martensitic SMA wires under recovery stress with varying degrees of prestrain on the wires and compared the behavior under recovery stress with that under prestressing of the wires. The remaining stress was reduced by the procedure of additional strain loading and unloading. More additional strains reduced more remaining stresses. When the SMA wires were heated up to the transformation temperature under prestress, the stress on the wires increased due to the state transformation. Furthermore, the stress decreased with a decreasing temperature of the wires down to room temperature. The stress of the NiTiNb wires was higher than the prestress, and the developed stress seemed to depend on the composition of the SMAs. When an additional strain was subsequently loaded and unloaded on the prestressed SMA wires, the remaining stress decreased. Finally, the remaining stress becomes zero when loading and unloading a specific large strain.

  7. Energy-dissipating and self-repairing SMA-ECC composite material system

    Science.gov (United States)

    Li, Xiaopeng; Li, Mo; Song, Gangbing

    2015-02-01

    Structural component ductility and energy dissipation capacity are crucial factors for achieving reinforced concrete structures more resistant to dynamic loading such as earthquakes. Furthermore, limiting post-event residual damage and deformation allows for immediate re-operation or minimal repairs. These desirable characteristics for structural ‘resilience’, however, present significant challenges due to the brittle nature of concrete, its deformation incompatibility with ductile steel, and the plastic yielding of steel reinforcement. Here, we developed a new composite material system that integrates the unique ductile feature of engineered cementitious composites (ECC) with superelastic shape memory alloy (SMA). In contrast to steel reinforced concrete (RC) and SMA reinforced concrete (SMA-RC), the SMA-ECC beams studied in this research exhibited extraordinary energy dissipation capacity, minimal residual deformation, and full self-recovery of damage under cyclic flexural loading. We found that the tensile strain capacity of ECC, tailored up to 5.5% in this study, allows it to work compatibly with superelastic SMA. Furthermore, the distributed microcracking damage mechanism in ECC is critical for sufficient and reliable recovery of damage upon unloading. This research demonstrates the potential of SMA-ECC for improving resilience of concrete structures under extreme hazard events.

  8. Stiffness and Confinement Ratios of SMA Wire Jackets for Confining Concrete

    Science.gov (United States)

    Choi, Eunsoo; Kim, Dong Joo; Youn, Heejung

    2014-07-01

    This article discusses the effects of the stiffness and confinement ratios of shape memory alloy (SMA) wire jackets on the behavior of confined concrete. SMA wire jackets are an effective confining material to improve concrete behavior; for example, by increasing peak strength and failure strain. The stiffness and confinement ratios of fiber-reinforced polymer jackets have been extensively discussed and their effects are well known. However, assessment of the stiffness and confinement ratios of SMA wire jackets has not previously been conducted. In this study, we investigate the effects of the stiffness and confinement ratios of steel jackets, and then compare the results with those of SMA wire jackets. In general, the stiffness ratios of SMA wire jackets are relatively smaller than those of steel jackets, and most of them have lower stiffness ratios because the Young's moduli of the SMAs are relatively small. The active confining pressure of the SMA wires does not improve the lower stiffness-ratio effect since the amount of active confining pressure is not sufficiently large.

  9. Mandibular dysfunction as a reflection of bulbar involvement in SMA type 2 and 3.

    Science.gov (United States)

    van Bruggen, H Willemijn; Wadman, Renske I; Bronkhorst, Ewald M; Leeuw, Maureen; Creugers, Nico; Kalaykova, Stanimira I; van der Pol, W Ludo; Steenks, Michel H

    2016-02-09

    In a cross-sectional study, we aimed to determine (1) the effect of spinal muscular atrophy (SMA) type 2 and 3 on mandibular function reflected as masticatory performance, mandibular range of motion, and bite force and (2) the predictors of mandibular dysfunction. Sixty patients with SMA type 2 and 3 (mean age 32.3 years, SD 17.4 years) and 60 age-matched controls filled out questionnaires about impairments of mandibular function. All participants underwent detailed clinical examination to document the mandibular range of motion including maximal mouth opening, bite force, and masticatory function. All mandibular movements, including mouth opening, lateral range of motion, and protrusion of the mandible, were reduced in patients with SMA type 2 and 3 compared to healthy controls (p mandibular range of motion (R(2) = 0.82) and weakness of neck muscles for bite force (R(2) = 0.47). Reduced mandibular mobility and bite force are common complications in SMA. SMA type and neck muscle strength are important correlates of these complications. We provide further evidence for clinically relevant bulbar involvement in patients with SMA. © 2016 American Academy of Neurology.

  10. New technologies for the detection of millimeter and submillimeter waves

    Energy Technology Data Exchange (ETDEWEB)

    Richards, P.L.; Clarke, J.; Gildemeister, J.M.; Lanting, T.; Lee, A.T.; Myers, M.J.; Schwan, D.; Skidmore, J.T.; Spieler, H.G.; Yoon, Jongsoo

    2001-09-20

    Voltage-biased superconducting bolometers have many operational advantages over conventional bolometer technology including sensitivity, linearity, speed, and immunity from environmental disturbance. A review is given of the Berkeley program for developing this new technology. Developments include fully lithographed individual bolometers in the spiderweb configuration, arrays of 1024 close-packed absorber-coupled bolometers, antenna-coupled bolometers, and a frequency-domain SQUID readout multiplexer.

  11. Profil Antisipasi Siswa SMA Dalam Memecahkan Masalah Integral

    Directory of Open Access Journals (Sweden)

    Erfan Yudianto

    2015-06-01

    Full Text Available Penelitian ini dilatarbelakangi oleh sulitnya siswa dalam menyelesaikan masalah integral khusunya luas daerah. Banyak siswa hanya menyelesaikan masalah integral hanya berdasarkan rumus yang sudah disediakan. Siswa jarang mengaitkan konsep-konsep yang saling terkait, dalam hal ini konsep integral subpokokbahasan luas daerah.Tujuan penelitian ini untuk mendeskripsikan Profil antisipasi siswa SMA dalam memecahkan masalah integral. Hasil penelitian ini dapat dimanfaatkan oleh guru untuk membantu siswa mengaitkan konsep-konsep yang belum terkait.  Penelitian ini menggunakan metode tes dan wawancara. Tes berupa  tes kemampuan matematika yang diberikan kepada siswa, sehingga diperoleh siswa berkemampuan tinggi dan wawancara diberikan kepada siswa yang bersangkutan untuk menggali dan melihat jaringan konsep yang dimiliki siswa dalam menyelesaikan masalah integral. Subjek dalam penelitian ini termasuk dalam antisipasi terinternasilsasi dikarenakan siswa secara spontan menerapkan rumus integral tanpa menganalisis soal yang diberikan.This research is motivated by the difficulty of students in solving integral problems especially the area. Many students just completed the integral problems just based on a formula that has been provided. Students rarely associate the concepts are interrelated, in this case the integral concept of the area. The purpose of this study was to describe the profile anticipation of high school students in problem solving integrals. The results could be used by teachers to help students link the concepts are not related. This study uses tests and interviews. The tests such as math skills test given to students, in order to obtain a high ability students and interviews given to the student to explore and see the network concept of the students in problem solving integrals. Subjects in this study are included in anticipation terinternasilsasi because students spontaneously apply the integral formula without analyzing the questions

  12. Skeletal muscle DNA damage precedes spinal motor neuron DNA damage in a mouse model of Spinal Muscular Atrophy (SMA.

    Directory of Open Access Journals (Sweden)

    Saniya Fayzullina

    Full Text Available Spinal Muscular Atrophy (SMA is a hereditary childhood disease that causes paralysis by progressive degeneration of skeletal muscles and spinal motor neurons. SMA is associated with reduced levels of full-length Survival of Motor Neuron (SMN protein, due to mutations in the Survival of Motor Neuron 1 gene. The mechanisms by which lack of SMN causes SMA pathology are not known, making it very difficult to develop effective therapies. We investigated whether DNA damage is a perinatal pathological event in SMA, and whether DNA damage and cell death first occur in skeletal muscle or spinal cord of SMA mice. We used a mouse model of severe SMA to ascertain the extent of cell death and DNA damage throughout the body of prenatal and newborn mice. SMA mice at birth (postnatal day 0 exhibited internucleosomal fragmentation in genomic DNA from hindlimb skeletal muscle, but not in genomic DNA from spinal cord. SMA mice at postnatal day 5, compared with littermate controls, exhibited increased apoptotic cell death profiles in skeletal muscle, by hematoxylin and eosin, terminal deoxynucleotidyl transferase dUTP nick end labeling, and electron microscopy. SMA mice had no increased cell death, no loss of choline acetyl transferase (ChAT-positive motor neurons, and no overt pathology in the ventral horn of the spinal cord. At embryonic days 13 and 15.5, SMA mice did not exhibit statistically significant increases in cell death profiles in spinal cord or skeletal muscle. Motor neuron numbers in the ventral horn, as identified by ChAT immunoreactivity, were comparable in SMA mice and control littermates at embryonic day 15.5 and postnatal day 5. These observations demonstrate that in SMA, disease in skeletal muscle emerges before pathology in spinal cord, including loss of motor neurons. Overall, this work identifies DNA damage and cell death in skeletal muscle as therapeutic targets for SMA.

  13. COMPACT STARBURSTS IN z similar to 3-6 SUBMILLIMETER GALAXIES REVEALED BY ALMA

    NARCIS (Netherlands)

    Ikarashi, Soh; Ivison, R. J.; Caputi, Karina I.; Aretxaga, Itziar; Dunlop, James S.; Hatsukade, Bunyo; Hughes, David H.; Iono, Daisuke; Izumi, Takuma; Kawabe, Ryohei; Kohno, Kotaro; Lagos, Claudia D. P.; Motohara, Kentaro; Nakanishi, Kouichiro; Ohta, Kouji; Tamura, Yoichi; Umehata, Hideki; Wilson, Grant W.; Yabe, Kiyoto; Yun, Min S.

    2015-01-01

    We report the source size distribution, as measured by ALMA millimetric continuum imaging, of a sample of 13 AzTEC-selected submillimeter galaxies (SMGs) at z(phot) similar to 3-6. Their infrared luminosities and star formation rates (SFRs) are L-IR similar to, 2-6 x 10(12) L-circle dot and similar

  14. VizieR Online Data Catalog: Sub-millimeter spectra of 2-hydroxyacetonitrile (Margules+, 2017)

    Science.gov (United States)

    Margules, L.; McGuire, B. A.; Senent, M. L.; Motiyenko, R. A.; Remijan, A.; Guillemin, J. C.

    2017-02-01

    Measured frequencies and residuals from the global fit of the submillimeter-wave data for 2-hydroxyacetonitrile and files used for SPFIT. Detailled explanations on SPFIT could be found at https://www.astro.uni-koeln.de/cdms/pickett (4 data files).

  15. AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: NEAR-INFRARED MORPHOLOGIES AND STELLAR SIZES

    Energy Technology Data Exchange (ETDEWEB)

    Chen, Chian-Chou; Smail, Ian; Swinbank, A. M.; Simpson, J. M.; Ma, Cheng-Jiun; Alexander, D. M.; Danielson, A. L. R.; Edge, A. C. [Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE (United Kingdom); Biggs, A. D.; Ivison, R. J. [European Southern Observatory, Karl Schwarzschild Strasse 2, D-85748 Garching (Germany); Brandt, W. N. [Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802 (United States); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 (Canada); Coppin, K. E. K. [Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Dannerbauer, H. [Institut für Astrophysik, Universität Wien, Türkenschanzstraße 17, A-1180 Wien (Austria); Greve, T. R. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Karim, A. [Argelander-Institute for Astronomy, Bonn University, Auf dem Hügel 71, D-53121 Bonn (Germany); Menten, Karl M. [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany); Schinnerer, E.; Walter, F. [Max-Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany); Wardlow, J. L. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen (Denmark); and others

    2015-02-01

    We analyze Hubble Space Telescope WFC3/H {sub 160}-band observations of a sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South field, to study their stellar morphologies and sizes. We detect 79% ± 17% of the SMGs in the H {sub 160}-band imaging with a median sensitivity of 27.8 mag, and most (80%) of the nondetections are SMGs with 870 μm fluxes of S {sub 870} < 3 mJy. With a surface brightness limit of μ {sub H} ∼ 26 mag arcsec{sup –2}, we find that 82% ± 9% of the H {sub 160}-band-detected SMGs at z = 1-3 appear to have disturbed morphologies, meaning they are visually classified as either irregulars or interacting systems, or both. By determining a Sérsic fit to the H {sub 160} surface brightness profiles, we derive a median Sérsic index of n = 1.2 ± 0.3 and a median half-light radius of r{sub e} = 4.4{sub −0.5}{sup +1.1} kpc for our SMGs at z = 1-3. We also find significant displacements between the positions of the H {sub 160} component and 870 μm emission in these systems, suggesting that the dusty starburst regions and less-obscured stellar distribution are not colocated. We find significant differences in the sizes and the Sérsic index between our z = 2-3 SMGs and z ∼ 2 quiescent galaxies, suggesting that a major transformation of the stellar light profile is needed in the quenching processes if SMGs are progenitors of the red-and-dead z ∼ 2 galaxies. Given the short-lived nature of SMGs, we postulate that the majority of the z = 2-3 SMGs with S {sub 870} ≳ 2 mJy are early/mid-stage major mergers.

  16. Technology Needs for Far-Infrared, Submillimeter, and Millimeter Missions

    Science.gov (United States)

    Moseley, S. Harvey

    2004-01-01

    SAFIR will: Study the important and relatively unexplored region of the spectrum between 30 and 300 m; Enable the study of galaxy formation and the earliest stage of star formation by revealing regions too enshrouded by dust to be studied by NGST; Be more than 100 times as sensitive as SIRTF or the European [Herschel] mission.SAFIR is projected to cost around $600M total. The decadal review committee recommends that $100M be allocated in this decade to start the SAFIR project, and that additional technology developments be funded separately: Far-Infrared Array Development ($10M ) Refrigerators ($50M ) Large, Lightweight Optics ($80M ). Current developments are also described.

  17. Plastin 3 Expression Does Not Modify Spinal Muscular Atrophy Severity in the ∆7 SMA Mouse.

    Directory of Open Access Journals (Sweden)

    Vicki L McGovern

    Full Text Available Spinal muscular atrophy is caused by loss of the SMN1 gene and retention of SMN2. The SMN2 copy number inversely correlates with phenotypic severity and is a modifier of disease outcome. The SMN2 gene essentially differs from SMN1 by a single nucleotide in exon 7 that modulates the incorporation of exon 7 into the final SMN transcript. The majority of the SMN2 transcripts lack exon 7 and this leads to a SMN protein that does not effectively oligomerize and is rapidly degraded. However the SMN2 gene does produce some full-length SMN and the SMN2 copy number along with how much full-length SMN the SMN2 gene makes correlates with severity of the SMA phenotype. However there are a number of discordant SMA siblings that have identical haplotypes and SMN2 copy number yet one has a milder form of SMA. It has been suggested that Plastin3 (PLS3 acts as a sex specific phenotypic modifier where increased expression of PLS3 modifies the SMA phenotype in females. To test the effect of PLS3 overexpression we have over expressed full-length PLS3 in SMA mice. To ensure no disruption of functionality or post-translational processing of PLS3 we did not place a tag on the protein. PLS3 protein was expressed under the Prion promoter as we have shown previously that SMN expression under this promoter can rescue SMA mice. High levels of PLS3 mRNA were expressed in motor neurons along with an increased level of PLS3 protein in total spinal cord, yet there was no significant beneficial effect on the phenotype of SMA mice. Specifically, neither survival nor the fundamental electrophysiological aspects of the neuromuscular junction were improved upon overexpression of PLS3 in neurons.

  18. The design, hysteresis modeling and control of a novel SMA-fishing-line actuator

    Science.gov (United States)

    Xiang, Chaoqun; Yang, Hui; Sun, Zhiyong; Xue, Bangcan; Hao, Lina; Asadur Rahoman, M. D.; Davis, Steve

    2017-03-01

    Fishing line can be combined with shape memory alloy (SMA) to form novel artificial muscle actuators which have low cost, are lightweight and soft. They can be applied in bionic, wearable and rehabilitation robots, and can reduce system weight and cost, increase power-to-weight ratio and offer safer physical human-robot interaction. However, these actuators possess several disadvantages, for example fishing line based actuators possess low strength and are complex to drive, and SMA possesses a low percentage contraction and has high hysteresis. This paper presents a novel artificial actuator (known as an SMA-fishing-line) made of fishing line and SMA twisted then coiled together, which can be driven directly by an electrical voltage. Its output force can reach 2.65 N at 7.4 V drive voltage, and the percentage contraction at 4 V driven voltage with a 3 N load is 7.53%. An antagonistic bionic joint driven by the novel SMA-fishing-line actuators is presented, and based on an extended unparallel Prandtl-Ishlinskii (EUPI) model, its hysteresis behavior is established, and the error ratio of the EUPI model is determined to be 6.3%. A Joule heat model of the SMA-fishing-line is also presented, and the maximum error of the established model is 0.510 mm. Based on this accurate hysteresis model, a composite PID controller consisting of PID and an integral inverse (I-I) compensator is proposed and its performance is compared with a traditional PID controller through simulations and experimentation. These results show that the composite PID controller possesses higher control precision than basic PID, and is feasible for implementation in an SMA-fishing-line driven antagonistic bionic joint.

  19. SMA OBSERVATIONS OF CLASS 0 PROTOSTARS: A HIGH ANGULAR RESOLUTION SURVEY OF PROTOSTELLAR BINARY SYSTEMS

    Energy Technology Data Exchange (ETDEWEB)

    Chen Xuepeng [Purple Mountain Observatory, Chinese Academy of Sciences, 2 West Beijing Road, Nanjing 210008 (China); Arce, Hector G.; Dunham, Michael M. [Department of Astronomy, Yale University, Box 208101, New Haven, CT 06520-8101 (United States); Zhang Qizhou; Bourke, Tyler L. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Launhardt, Ralf; Henning, Thomas [Max Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg (Germany); Jorgensen, Jes K. [Niels Bohr Institute and Centre for Star and Planet Formation, Copenhagen University, Juliane Maries Vej 30, DK-2100 Copenhagen O (Denmark); Lee, Chin-Fei [Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 106, Taiwan (China); Foster, Jonathan B. [Institute for Astrophysical Research, Boston University, Boston, MA 02215 (United States); Pineda, Jaime E., E-mail: xpchen@pmo.ac.cn, E-mail: xuepeng.chen@yale.edu [ESO, Karl Schwarzschild Str. 2, D-85748 Garching bei Munchen (Germany)

    2013-05-10

    We present high angular resolution 1.3 mm and 850 {mu}m dust continuum data obtained with the Submillimeter Array toward 33 Class 0 protostars in nearby clouds (distance < 500 pc), which represents so far the largest survey toward protostellar binary/multiple systems. The median angular resolution in the survey is 2.''5, while the median linear resolution is approximately 600 AU. Compact dust continuum emission is observed from all sources in the sample. Twenty-one sources in the sample show signatures of binarity/multiplicity, with separations ranging from 50 AU to 5000 AU. The numbers of singles, binaries, triples, and quadruples in the sample are 12, 14, 5, and 2, respectively. The derived multiplicity frequency (MF) and companion star fraction (CSF) for Class 0 protostars are 0.64 {+-} 0.08 and 0.91 {+-} 0.05, respectively, with no correction for completeness. The derived MF and CSF in this survey are approximately two times higher than the values found in the binary surveys toward Class I young stellar objects, and approximately three (for MF) and four (for CSF) times larger than the values found among main-sequence stars, with a similar range of separations. Furthermore, the observed fraction of high-order multiple systems to binary systems in Class 0 protostars (0.50 {+-} 0.09) is also larger than the fractions found in Class I young stellar objects (0.31 {+-} 0.07) and main-sequence stars ({<=}0.2). These results suggest that binary properties evolve as protostars evolve, as predicted by numerical simulations. The distribution of separations for Class 0 protostellar binary/multiple systems shows a general trend in which CSF increases with decreasing companion separation. We find that 67% {+-} 8% of the protobinary systems have circumstellar mass ratios below 0.5, implying that unequal-mass systems are preferred in the process of binary star formation. We suggest an empirical sequential fragmentation picture for binary star formation, based on this

  20. EVALUASI PEMBELAJARAN SEJARAH PADA SMA NEGERI DI DKI JAKARTA

    Directory of Open Access Journals (Sweden)

    Umasih Umasih

    2012-07-01

    Full Text Available This article discusses the evaluation done by history teachers in high school in Jakarta, especially on the understanding of teachers about the evaluation of learning and the types and models of evaluation they perform. The instrument used to get the data s in the form of questionnaire given to 38 teachers from 152 people as the population using survey techniques. The results showed that most respondents (94.73% understand the principles of competency-oriented evaluation. Evaluation after the implementation of KTSP (the curriculum at the level of education units is different in quantity, form and manner about assessment. 23.69% of the respondents differ in quantity (frequency, the methods of evaluation and weighted score. Assessment given not only to answer the questions either multiple choice or essay, but students are also working on a quiz question, analyzing sources, practicing skills in developing mind mapping as well as a portfolio. While the types and models of assessment that are suitable for assessing history learning outcomes is the judgment that can measure cognitive and affective discourse up to the levels of analysis. Keywords: principles of evaluation, competence, and model evaluation Artikel ini membahas tentang evaluasi yang dilaksanakan guru-guru sejarah SMA Negeri  di DKI Jakarta, khususnya tentang pemahaman guru mengenai pelaksanaan evaluasi pembelajaran serta jenis dan model evaluasi apa yang dilaksanakannya. Instrumen yang digunakan untuk menjaring data berupa angket yang diberikan kepada 38 orang guru dari 152 orang sebagai populasi dengan menggunakan teknik survei. Hasil penelitian menunjukkan bahwa sebagian besar responden (94,73 % memahami prinsip evaluasi yang berorientasi pada kompetensi. Pelaksanaan evaluasi sesudah pemberlakuan KTSP berbeda  dalam kuantitas, bentuk soal dan cara penilaian. 23,69 % responden menyatakan berbeda dalam kuantitas (frekuensi, cara penilaian dan bobot skornya. Penilaian yang diberikan

  1. Histochemical and Immunohistochemical Study of α-SMA, Collagen, and PCNA in Epithelial Ovarian Neoplasm

    Science.gov (United States)

    Anggorowati, Nungki; Ratna Kurniasari, Chatarina; Damayanti, Karina; Cahyanti, Titik; Widodo, Irianiwati; Ghozali, Ahmad; Romi, Muhammad Mansyur; Sari, Dwi Cahyani Ratna; Arfian, Nur

    2017-03-01

    Background: Alpha-smooth muscle actin (α-SMA) is an isoform of actin, positive in myofibroblasts and is an epithelial to mesenchymal transition (EMT) marker. EMT is a process by which tumor cells develop to be more hostile and able to metastasize. Progression of tumor cells is always followed by cell composition and extracellular matrix component alteration. Increased α-SMA expression and collagen alteration may predict the progressivity of ovarian neoplasms. Objective: The aim of this research was to analyse the characteristic of α-SMA and collagen in tumor cells and stroma of ovarian neoplasms. In this study, PCNA (proliferating cell nuclear antigen) expression was also investigated. Methods: Thirty samples were collected including serous, mucinous, endometrioid, and clear cell subtypes. The expression of α-SMA and PCNA were calculated in cells and stroma of ovarian tumors. Collagen was detected using Sirius Red staining and presented as area fraction. Results: The overexpressions of α-SMA in tumor cells were only detected in serous and clear cell ovarian carcinoma. The histoscore of α-SMA was higher in malignant than in benign or borderline ovarian epithelial neoplasms (105.3±129.9 vs. 17.3±17.1, P=0.011; mean±SD). Oppositely, stromal α-SMA and collagen area fractions were higher in benign than in malignant tumors (27.2±6.6 vs 20.5±8.4, P=0.028; 31.0±5.6 vs. 23.7±6.4, P=0.04). The percentages of epithelial and stromal PCNA expressions were not significantly different between benign and malignant tumors. Conclusion: Tumor cells of serous and clear cell ovarian carcinoma exhibit mesenchymal characteristic as shown by α-SMA positive expression. This expression might indicate that these subtypes were more aggressive. This research showed that collagen and α-SMA area fractions in stroma were higher in benign than in malignant neoplasms. 10.22034/APJCP.2017.18.3.667

  2. Prestressing effect of cold-drawn short NiTi SMA fibres in steel reinforced mortar beams

    Science.gov (United States)

    Choi, Eunsoo; Kim, Dong Joo; Hwang, Jin-Ha; Kim, Woo Jin

    2016-08-01

    This study investigated the prestressing effect of cold-drawn short NiTi shape memory alloy (SMA) fibres in steel reinforced mortar beams. The SMA fibres were mixed with 1.5% volume content in a mortar matrix with the compressive strength of 50 MPa. The SMA fibres had an average length of 34 mm, and they were manufactured with a dog-bone shape: the diameters of the end- and middle-parts were 1.024 and 1.0 mm, respectively. Twenty mortar beams with the dimensions of 40 mm × 40 mm × 160 mm (B × H × L) were prepared. Two types of tests were conducted. One was to investigate the prestressing effect of the SMA fibres, and the beams with the SMA fibres were heated at the bottom. The other was to assess the bending behaviour of the beams prestressed by the SMA fibres. The SMA fibres induced upward deflection and cracking at the top surface by heating at the bottom; thus, they achieved an obvious prestressing effect. The beams that were prestressed by the SMA fibres did not show a significant difference in bending behaviour from that of the SMA fibre reinforced beams that were not subjected to heating. Stress analysis of the beams indicated that the prestressing effect decreased in relation to the cooling temperature.

  3. PENINGKATAN KEAKTIFAN SISWA DALAM PEMBELAJARAN SEJARAH KELAS XI IA SMA IBU KARTINI SEMARANG DENGAN METODE COOPERATIVE LEARNING

    Directory of Open Access Journals (Sweden)

    - Ba'in

    2010-04-01

    Full Text Available Pada penelitian ini masalah yang dibahas adalah (1 apakah dengan metode cooperative learning model STAD dalam pembelajaran sejarah dapat meningkatkan minat dan keaktifan siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010; (2 bagaimana respon siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010 terhadap pembelajaran sejarah dengan menggunakan metode cooperative learning model STAD? Penelitian ini bertujuan untuk mengetahui dapat tidaknya metode cooperative learning model STAD meningkatkan minat dan keaktifan siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010 dalam pembelajaran sejarah, dan respon siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010 terhadap pembelajaran sejarah. Subyek penelitian adalah siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010, guru mata pelajaran sejarah SMA Ibu Kartini, dan tim peneliti sebagai konsultas. Penelitian dilakukan dalam 2 (dua siklus, dan proses pembelajaran yang diteliti pada setiap silus meliputi perencaan, pelaksanaan dan refleksi. Hasil penelitian menunjukkan bahwa minat dan keaktifan siswa kelas XI IA 1 SMA Ibu Kartini Semarang tahun 2009/2010 dalam pembelajaran sejarah dengan menggunakan metode cooperative learning model STAD mengalami peningkatan, dari 22,50% pada pra siklus menjadi 69,91% pada sikulus 1 dan 80,00% pada siklus 2. Demikian pula untuk respon siswa, pembelajaran Sejarah di kelas XI IA 1 SMA Ibu Kartini Semarang dengan metode Cooperative Learning direspon positif oleh sebagian besar siswa.Kata Kunci: pembelajaran sejarah, metode Cooperative Learning, SMA Ibu Kartini

  4. Active Cooling and Strain-Ratios to Increase the Actuation Frequency of SMA Wires

    Science.gov (United States)

    Lara-Quintanilla, A.; Bersee, H. E. N.

    2015-10-01

    The maximum actuation frequency of an SMA wire does not only depend on the heating and cooling rates but also on the amplitude of strains at which it works. Smaller working amplitudes mean faster working frequencies. SMA-based actuators rarely work throughout their full strain range but they usually work at small amplitudes, which are amplified by means of mechanisms or by the optimised positioning of the wires within the actuator. Furthermore, the nonlinear relationship between the temperature and the strain on SMAs can be used in our favour to increase the actuation frequency of SMA wires by finding the optimum range of temperatures within which the wires must work for a specific strain amplitude. This work presents a method to find the maximum attainable actuation frequency of an SMA wire that is Joule heated and actively cooled while performing at different strain-ratios. The experimental results show that the actuation frequency of an SMA wire can be increased up to three and a half-fold (from 0.8 to 3 Hz) just by making it work within the most appropriate range of temperatures, under similar heating and cooling rate, wire's diameter and applied stress.

  5. Simulated and Experimental Damping Properties of a SMA/Fiber Glass Laminated Composite

    Science.gov (United States)

    Arnaboldi, S.; Bassani, P.; Biffi, C. A.; Tuissi, A.; Carnevale, M.; Lecis, N.; Loconte, A.; Previtali, B.

    2011-07-01

    In this article, an advanced laminated composite is developed, combining the high damping properties of shape memory alloy (SMA) with mechanical properties and light weight of a glass-fiber reinforced polymer. The composite is formed by stacking a glass-fiber reinforced epoxy core between two thin patterned strips of SMA alloy, and two further layers of fiber-glass reinforced epoxy. The bars of the laminated composite were assembled and cured in autoclave. The patterning was designed to enhance the interface adhesion between matrix and SMA inserts and optimally exploit the damping capacity of the SMA thin ribbons. The patterned ribbons of the SMA alloy were cut by means of a pulsed fiber laser source. Damping properties at different amplitudes on full scale samples were investigated at room temperature with a universal testing machine through dynamic tension tests, while temperature dependence was investigated by dynamic mechanical analyses (DMA) on smaller samples. Experimental results were used in conjunction with FEM analysis to optimize the geometry of the inserts. Experimental decay tests on the laminated composite have been carried out to identify the adimensional damping value related to their first flexural mode.

  6. Pengembangan dan Pelaksanaan Kurikulum Pendidikan Agama Pada SMA di Bawah Yayasan Keagamaan

    Directory of Open Access Journals (Sweden)

    Wahab Wahab

    2011-06-01

    Full Text Available The purpose of this study is to investigate the development and the implementationof  religious education curriculum developed by senior high schools  (SMA under religious foundations. This is a case study of SMA Muhammadiyah I Palangkaraya. Research design applied in this study is Stufflebeam’s  CIPP (Context, Input, Process, Product. The results how:1 SMA Muhammadiyah I Palangkaraya develops not only curriculum designed by Ministry  of National Education but also local religious education one (curriculum developed by the foundation of Muhammadiyah; the way the school develops  the curriculum can also be considered as especial because it provides its nonmuslims  students facilities for learning their religious teachings, 2 some supporting factors are the participation of the foundation, the principal, and the school committee in the curriculum implementation, and 3 the obstacle of the curriculum implementation is the absence of a particular place such as laboratory for religious education.

  7. PENGEMBANGAN MEDIA PEMBELAJARAN PENDIDIKAN JASMANI OLAHRAGA DAN KESEHATAN BERBASIS KOMPUTER UNTUK SMA

    Directory of Open Access Journals (Sweden)

    Suci Cahyati

    2014-04-01

    Full Text Available Penelitian ini bertujuan untuk menghasilkan produk berupa CD pembelajaran pendidikan jasmani olahraga dan kesehatan berbasis komputer untuk SMA yang valid dan efektif. Penelitian ini menggunakan metode Research and Development (R&D. Media yang dikembangkan memuat materi tentang HIV/AIDS. Pengembangan media pembelajaran ini menggunakan software Adobe Flash Cs3 Professional. Media yang telah dikembangkan melalui dua tahap penelitiannya itu validasi ahli dan uji coba lapangan. Berdasarkan validasi ahli dan uji coba lapangan hasil penelitian menunjukkan produk termasuk kriteria “Sangat baik” dengan rerata skor 4,25. Hasil tes siswa mengalami peningkatan dari rerata skor pretest 5,53 dan rerata skor posttest 7,56. Berdasarkan hasil tes tersebut dapat disimpulkan bahwa media pembelajaran pendidikan jasmani olahraga dan kesehatan efektif digunakan dalam pembelajaran di SMA. Kata kunci: Pengembangan media, penjasorkes, SMA

  8. Natural Heat-Sinking Control Method for High-Speed Actuation of the SMA

    Directory of Open Access Journals (Sweden)

    Tamio Arai

    2008-11-01

    Full Text Available This paper describes two methodologies for increasing the actuation speed of the shape memory alloy (SMA actuator in ambient environment. The first method involves the implementation of a simple, light-weight heat sink, which consists only of a combination of an outer metal tube with the silicone grease, but able to cool the heated alloy effectively. The second method describes a high current pulse actuation that actuates the alloy fastly using pulses in the milliseconds order. We hypothesize that a fast actuation of the SMA results in small increase in temperature, due to energy transformation from heat energy to the kinetic energy in the SMA. This new heating method revolutionizes the actuation of the alloy for a significantly faster response.

  9. Pemodelan Enterprise Architecture Sistem Informasi Akademik SMA PL Don Bosko Semarang Dengan Framework Zachman

    Directory of Open Access Journals (Sweden)

    Maria Alfonsa Chintia Dea Prananingrum

    2017-05-01

    Full Text Available Abstrak SMA PL Don Bosko Semarang belum dapat memanfaatkan teknologi komputer secara optimal karena masih menggunakan cara manual dalam pengelolaan berbagai macam data akademik sehingga memberikan masalah seperti lambatnya dalam pembuatan laporan yang menyulitkan kepala sekolah dalam pengambilan keputusan. Oleh sebab itu, SMA PL Don Bosko Semarang membutuhkan Sistem Informasi Akademik untuk memberikan kemudahan dalam mengelola berbagai macam data akademik secara terintegrasi serta memberikan layanan yang lebih baik kepada siswanya. Sebuah model architecture enterprise Sistem Informasi Akademik dibutuhkan agar meminimalisir kegagalan ketika menerapkan sistem tersebut sekaligus dapat berjalan sesuai kebutuhan di SMA PL Don Bosko Semarang. Metode analisis dalam penelitian ini menggunakan Framework Zachman yang memberikan pondasi dalam membantu menyediakan struktur dasar organisasi sehingga dapat mendukung perancangan dan pengembangan sistem informasi suatu organisasi. Hasil dari penelitian ini berupa blueprint (cetak biru pemodelan Sistem Informasi Akademik. Kata kunci— sistem informasi akademik, architecture enterprise, framework zachman, bluprint

  10. UPAYA PENINGKATAN KARAKTER SISWA SMA DALAM PERMAINAN BOLA BASKET MELALUI MODEL TPSR

    Directory of Open Access Journals (Sweden)

    Titis Nurina

    2014-04-01

    Full Text Available Pembelajaran pendidikan jasmani dalam model TPSR lebih menekankan pada kondisi siswa dan pendekatannya juga berorientasi kepada aktualisasi diri dan rekonstruksi sosial siswa di dalam pembelajaran permainan bola basket. Penelitian ini bertujuan untuk meningkatkan karakter tanggung jawab, kerja sama, dan percaya diri siswa putri kelas XI IPS 2 SMA Muhammadiyah 3 Yogyakarta dengan model TPSR dalam pembelajaran permainan bola basket. Penelitian ini menggunakan metode penelitian tindakan kelas yang dilaksanakan dalam dua siklus. Subjek dalam penelitian adalah seluruh siswa putri kelas XI IPS 2 SMA Muhammadiyah 3 yang berjumlah sembilan siswa. Analisis data menggunakan analisis diskriptif, kualitatif, dan kuantitatif. Hasil penelitian menunjukkan bahwa model pembelajaran TPSR dapat meningkatkan karakter tanggung jawab dan kerja sama dalam pembel-ajaran permainan bola basket yang berdampak pada kepercayaan diri siswa putri kelas XI IPS 2 SMA Muhammadiyah 3 Yogyakarta yang dapat dilihat dari peningkatan nilai keterampilan psikomotor, kognitif, dan afektif siswa. Kata Kunci: TPSR, karakter, permainan bola basket

  11. Perancangan dan Implementasi Presensi Digital Guru dan Karyawan SMA Negeri 9 Semarang

    Directory of Open Access Journals (Sweden)

    Th. Didot Septiawan

    2016-04-01

    Full Text Available Berdasarkan surat edaran dari Kepala Dinas Pendidikan Kota Semarang, terhitung mulai Januari 2015 tiap sekolah dihimbau untuk beralih dari sistem presensi manual menjadi digital. Hingga awal Maret ini, presensi guru dan karyawan di SMA Negeri 9 Semarang masih dilakukan secara manual. Maka diperlukan sebuah penelitian untuk merancang dan menerapkan sistem presensi digital bagi SMA Negeri 9 Semarang. Tahapan penelitian meliputi perencanaan, analisis, perancangan, implementasi, pengujian, dan pemeliharaan. Perangkat lunak dibangun dengan framework PHP Phalcon, basis data MySQL, dan aplikasi webserver Nginx pada sistem operasi Ubuntu 14.04. Mesin presensi dengan metode pengenalan wajah dipilih untuk mendapatkan data kehadiran yang bersifat autentik. Pengujian dilakukan dengan metode kotak hitam dan kotak putih. Semua kebutuhan fungsional telah diimplementasikan pada aplikasi web dan kebutuhan non-fungsional pun telah terpenuhi. Sistem presensi digital ini menjadi solusi bagi SMA Negeri 9 Semarang dalam usaha uji coba penggunaan presensi digital.

  12. Nonlinear Dynamic Characteristics and Optimal Control of SMA Composite Wings Subjected to Stochastic Excitation

    Directory of Open Access Journals (Sweden)

    Zhi-Wen Zhu

    2015-01-01

    Full Text Available A kind of high-aspect-ratio shape memory alloy (SMA composite wing is proposed to reduce the wing’s fluttering. The nonlinear dynamic characteristics and optimal control of the SMA composite wings subjected to in-plane stochastic excitation are investigated where the great bending under the flight loads is considered. The stochastic stability of the system is analyzed, and the system’s response is obtained. The conditions of stochastic Hopf bifurcation are determined, and the probability density of the first-passage time is obtained. Finally, the optimal control strategy is proposed. Numerical simulation shows that the stability of the system varies with bifurcation parameters, and stochastic Hopf bifurcation appears in the process; the reliability of the system is improved through optimal control, and the first-passage time is delayed. Finally, the effects of the control strategy are proved by experiments. The results of this paper are helpful for engineering applications of SMA.

  13. Deployment shock attenuation of a solar array tape hinge by means of the Martensite detwinning of NiTi Shape Memory Alloy.

    Science.gov (United States)

    Lee, Chang-Ho; Jeong, Ju-Won; Kim, Young-Jin; Lee, Jung-Ju

    2016-03-01

    This paper presents a new tape hinge for attenuating the deployment shock of a satellite solar array. This hinge uses the Martensite detwinning of Shape Memory Alloy (SMA). To attenuate the deployment shock, a NiTi SMA strip is assembled between two curved steel strips. The attenuation performance of the hinge is analyzed using a SMA detwinning constitutive equation. A prototype of the hinge is manufactured and its characteristics are measured in a bending test and in a deployment test. Finally, the deployment performance of the prototype hinge is investigated on a satellite model. It is shown that the new SMA damped tape hinge can effectively minimize the deployment shock and dynamic perturbation while also maintaining suitable deployment performance.

  14. PENGEMBANGAN CD PEMBELAJARAN INTERAKTIF KIMIA SMA BERBASIS INTERTEKSTUALITAS SEBAGAI ALTERNATIF MODEL PEMBELAJARAN

    Directory of Open Access Journals (Sweden)

    Mr Sjaeful Anwar

    2011-10-01

    Full Text Available Studi aplikasi model pembelajaran intertekstual menggunakan CD pembelajaran telah dilakukan di 3 SMA, yaitu SMA A, SMA B dan SMA C selama bulan Mei 2010. Pemilihan tiga sekolah ini diharapkan dapat mewakili sekolah dengan kualitas rendah sampai kualitas tinggi. Selama proses ujicoba pembelajaran berlangsung, siswa dapat mengikuti secara aktif dengan memberikan respon yang baik. Dari tampilan-tampilan yang diberikan, siswa bisa memahami konsep-konsep pada materi hidrolisis garam dengan baik meskipun terkadang tampilan tersebut harus diberikan secara bolak-balik untuk dapat mempertautkan ketiga level representasi. Secara umum, siswa merespon dengan baik terhadap implementasi strategi pembelajaran intertekstual ini karena merasa tertarik dengan proses pembelajaran yang dilakukan dan memudahkan untuk memahami konsep-konsep yang diberikan secara sistematis dan selalu menghubungkan dengan konsep-konsep yang sudah dipelajari. Tanggapan guru terhadap implementasi strategi pembelajaran intertekstual ini memberikan pandangan yang positif, hal tersebut dikarenakan dengan proses pembelajaran yang dilakukan dapat memudahkan guru untuk menyampaikan materi hidrolisis garam yang disusun secara sistematis melalui pertautan ketiga level representasi dan dikemas dalam bentuk multimedia sehingga konsep-konsep yang disampaikan dapat diterima oleh siswa dengan utuh dan mudah. Aplikasi model pembelajaran intertekstual pada materi hidrolisis garam ternyata mampu meningkatkan penguasaan konsep-konsep pada materi tersebut. Peningkatan penguasaan konsep siswa terhadap materi hidrolisis garam diperoleh berdasarkan perhitungan nilai N-gain, secara keseluruhan diperoleh nilai N-gain sebesar 0,67 yang berarti implementasi strategi pembelajaran intertekstual pada materi hidrolisis garam ini dapat meningkatkan penguasaan konsep dengan kriteria tinggi. Hal ini didukung juga data model mental siswa untuk proses pelarutan berbagai garam. Model ini ternyata juga dapat meningkatkan

  15. Direct measurement of additional Ar-H2O vibration-rotation-tunneling bands in the millimeter-submillimeter range

    Science.gov (United States)

    Zou, Luyao; Widicus Weaver, Susanna L.

    2016-06-01

    Three new weak bands of the Ar-H2O vibration-rotation-tunneling spectrum have been measured in the millimeter wavelength range. These bands were predicted from combination differences based on previously measured bands in the submillimeter region. Two previously reported submillimeter bands were also remeasured with higher frequency resolution. These new measurements allow us to obtain accurate information on the Coriolis interaction between the 101 and 110 states. Here we report these results and the associated improved molecular constants.

  16. SMN transcript levels in leukocytes of SMA patients determined by absolute real-time PCR

    OpenAIRE

    Tiziano, Francesco Danilo; Pinto, Anna Maria; Fiori, Stefania; Lomastro, Rosa; Messina, Sonia; Bruno, Claudio; Pini, Antonella; Pane, Marika; D'Amico, Adele; Ghezzo, Alessandro; Bertini, Enrico; Mercuri, Eugenio; Neri, Giovanni; Brahe, Christina

    2009-01-01

    Spinal muscular atrophy (SMA) is an autosomal recessive neuromuscular disorder caused by homozygous mutations of the SMN1 gene. Three forms of SMA are recognized (type I–III) on the basis of clinical severity. All patients have at least one or more (usually 2–4) copies of a highly homologous gene (SMN2), which produces insufficient levels of functional SMN protein, because of alternative splicing of exon 7. Recently, evidence has been provided that SMN2 expression can be enhanced by pharmacol...

  17. The effect of aggregate density on pavement performance of SMA-13 asphalt mixture

    Directory of Open Access Journals (Sweden)

    Qiao Yinping

    2016-05-01

    Full Text Available This paper chooses the top layer SMA-13 asphalt mixture material as the research object. Basalt was selected as pavement material, and modified SBS asphalt was used as a cementing material. Two basalt aggregates with different densities were used to carry out standard Marshall test in the laboratory.Aimed at the volume parameters of the asphalt mixture carry on anaiysis,and obtian the effect of aggregate density on pavement performance of SMA-13 asphalt mixture, which is that the density of aggregate has a significant effect on the void ratio, saturation, and the gap rate of the aggregate, thus affecting the pavement performance of the asphalt mixture

  18. Columbia SMA Project: A Randomized, Control Trial of the Effects of Exercise on Motor Function and Strength in Patients with Spinal Muscular Atrophy (SMA)

    Science.gov (United States)

    2012-06-01

    deconditioning resulting from limited engagement in physical activity secondary to physical function limitations associated with SMA. This is supported by data...characteristics as well as clinical measures are included in Table 1 below. All clinical assessments were performed by our blinded physical therapist...perceived fatigue (Fatigue Severity Scale and Pediatric Multidimensional Fatigue Scale) at all clinic visits. Habitual physical activity levels using the

  19. THE SCUBA-2 COSMOLOGY LEGACY SURVEY: ALMA RESOLVES THE REST-FRAME FAR-INFRARED EMISSION OF SUB-MILLIMETER GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Simpson, J. M.; Smail, Ian; Swinbank, A. M.; Chen, Chian-Chou; Danielson, A. L. R.; Edge, A. C.; Ma, C.-J. [Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Almaini, O.; Conselice, C.; Hartley, W. G.; Lani, C. [School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD (United Kingdom); Blain, A. W. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Bremer, M. N.; Coppin, K. E. K. [School of Physics, HH Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL (United Kingdom); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 (Canada); Dunlop, J. S.; Ivison, R. J. [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford HIll, Edinburgh EH9 3HJ (United Kingdom); Farrah, D. [Department of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); Geach, J. E. [Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Karim, A., E-mail: j.m.simpson@dur.ac.uk [Argelander-Institute for Astronomy, Bonn University, Auf dem Hügel 71, D-53121 Bonn (Germany); and others

    2015-01-20

    We present high-resolution (0.''3) Atacama Large Millimeter Array 870 μm imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey field to investigate the size and morphology of the sub-millimeter (sub-mm) emission on 2-10 kpc scales. We derive a median intrinsic angular size of FWHM = 0.''30 ± 0.''04 for the 23 SMGs in the sample detected at a signal-to-noise ratio (S/N) >10. Using the photometric redshifts of the SMGs we show that this corresponds to a median physical half-light diameter of 2.4 ± 0.2 kpc. A stacking analysis of the SMGs detected at S/N <10 shows they have sizes consistent with the 870 μm bright SMGs in the sample. We compare our results to the sizes of SMGs derived from other multi-wavelength studies, and show that the rest-frame ∼250 μm sizes of SMGs are consistent with studies of resolved {sup 12}CO (J = 3-2 to 7-6) emission lines, but that sizes derived from 1.4 GHz imaging appear to be approximately two times larger on average, which we attribute to cosmic ray diffusion. The rest-frame optical sizes of SMGs are around four times larger than the sub-millimeter sizes, indicating that the star formation in these galaxies is compact relative to the pre-existing stellar distribution. The size of the starburst region in SMGs is consistent with the majority of the star formation occurring in a central region, a few kiloparsecs in extent, with a median star formation rate surface density of 90 ± 30 M {sub ☉} yr{sup –1} kpc{sup –2}, which may suggest that we are witnessing an intense period of bulge growth in these galaxies.

  20. Ground-Based Submillimeter Spectroscopic Cosmological Surveys and Synergies with Space FIR Surveys

    Science.gov (United States)

    Spinoglio, Luigi

    2018-01-01

    To study the dust obscured processes of both star formation and black hole accretion during galaxy evolution and establish their role, as well as their mutual feedback processes, rest frame IR to submillimeter spectroscopy is needed. At these frequencies dust extinction is at its minimum and a variety of atomic and molecular transitions, tracing most astrophysical domains, occur. A large ground based submillimeter telescope with a large field of view and high sensitivity in the TeraHertz domain will pave the way of future FIR space telescope missions, such as SPICA in the late 2020's and the Origins Telescope later. I will present predictions demonstrating the synergies of such instruments to fully understand galaxy evolution, during its obscured phase, which has built most of the stellar populations in galaxies.

  1. Mu-Spec - A High Performance Ultra-Compact Photon Counting spectrometer for Space Submillimeter Astronomy

    Science.gov (United States)

    Moseley, H.; Hsieh, W.-T.; Stevenson, T.; Wollack, E.; Brown, A.; Benford, D.; Sadleir; U-Yen, I.; Ehsan, N.; Zmuidzinas, J.; hide

    2011-01-01

    We have designed and are testing elements of a fully integrated submillimeter spectrometer based on superconducting microstrip technology. The instrument can offer resolving power R approximately 1500, and its high frequency cutoff is set by the gap of available high performance superconductors. All functions of the spectrometer are integrated - light is coupled to the microstrip circuit with a planar antenna, the spectra discrimination is achieved using a synthetic grating, orders are separated using planar filter, and detected using photon counting MKID detector. This spectrometer promises to revolutionize submillimeter spectroscopy from space. It replaces instruments with the scale of 1m with a spectrometer on a 10 cm Si wafer. The reduction in mass and volume promises a much higher performance system within available resource in a space mission. We will describe the system and the performance of the components that have been fabricated and tested.

  2. Human brain diffusion tensor imaging at submillimeter isotropic resolution on a 3Tesla clinical MRI scanner.

    Science.gov (United States)

    Chang, Hing-Chiu; Sundman, Mark; Petit, Laurent; Guhaniyogi, Shayan; Chu, Mei-Lan; Petty, Christopher; Song, Allen W; Chen, Nan-kuei

    2015-09-01

    The advantages of high-resolution diffusion tensor imaging (DTI) have been demonstrated in a recent post-mortem human brain study (Miller et al., NeuroImage 2011;57(1):167-181), showing that white matter fiber tracts can be much more accurately detected in data at a submillimeter isotropic resolution. To our knowledge, in vivo human brain DTI at a submillimeter isotropic resolution has not been routinely achieved yet because of the difficulty in simultaneously achieving high resolution and high signal-to-noise ratio (SNR) in DTI scans. Here we report a 3D multi-slab interleaved EPI acquisition integrated with multiplexed sensitivity encoded (MUSE) reconstruction, to achieve high-quality, high-SNR and submillimeter isotropic resolution (0.85×0.85×0.85mm(3)) in vivo human brain DTI on a 3Tesla clinical MRI scanner. In agreement with the previously reported post-mortem human brain DTI study, our in vivo data show that the structural connectivity networks of human brains can be mapped more accurately and completely with high-resolution DTI as compared with conventional DTI (e.g., 2×2×2mm(3)). Copyright © 2015 Elsevier Inc. All rights reserved.

  3. ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance

    Science.gov (United States)

    Oteo, I.; Zwaan, M. A.; Ivison, R. J.; Smail, I.; Biggs, A. D.

    2016-05-01

    We have exploited ALMA calibration observations to carry out a novel, wide, and deep submillimeter (submm) survey, almacal. These calibration data comprise a large number of observations of calibrator fields in a variety of frequency bands and array configurations. By gathering together data acquired during multiple visits to many ALMA calibrators, it is possible to reach noise levels which allow the detection of faint, dusty, star-forming galaxies (DSFGs) over a significant area. In this paper, we outline our survey strategy and report the first results. We have analyzed data for 69 calibrators, reaching depths of ˜25 μJy beam-1 at sub-arcsec resolution. Adopting a conservative approach based on ≥5σ detections, we have found 8 and 11 DSFGs in ALMA bands 6 and 7, respectively, with flux densities S 1.2 mm ≥ 0.2 mJy. The faintest galaxies would have been missed by even the deepest Herschel surveys. Our cumulative number counts have been determined independently at 870 μm and 1.2 mm from a sparse sampling of the astronomical sky, and are thus relatively free of cosmic variance. The counts are lower than reported previously by a factor of at least 2×. Future analyses will yield large, secure samples of DSFGs with redshifts determined via the detection of submm spectral lines. Uniquely, our strategy then allows for morphological studies of very faint DSFGs—representative of more normal star-forming galaxies than conventional submm galaxies—in fields where self-calibration is feasible, yielding milliarcsecond spatial resolution.

  4. Design and Fabrication of a Two-Dimensional Superconducting Pop-up Bolometer Array

    Science.gov (United States)

    Benford, Dominic J.; Staguhn, Johannes G.; Chervenak, James A.; Allen, Christine A.; Moseley, S. Harvey; Irwin, Kent D.; Stacey, Gordon J.; Page, Lyman A.

    2004-01-01

    We have been developing an architecture for producing large format, two dimensional arrays of close-packed bolometers, which will enable submillimeter cameras and spectrometers to obtain images and spectra orders of magnitude faster than present instruments. The low backgrounds achieved in these instruments require very sensitive detectors with NEPs of order 5 x 10(exp -18) W/square root of Hz. Superconducting transition edge sensor bolometers can be close-packed using the Pop-up Detector (PUD) format, and SQUID multiplexers operating at the detector base temperature can be intimately coupled to them. The array unit cell is 8 x 32 pixels, using 32- element detector and multiplexer components. We have fabricated an engineering model array with this technology which features a very compact, modular approach for large format arrays. We report on the production of the 32-element components for the arrays. Planned instruments using this array architecture include the Submillimeter and Far-InfraRed Experiment (SAFIRE) on the SOFIA airborne observatory, the South Pole Imaging Fabry-Perot Interferometer (SPIFI) for the AST/RO observatory, the Millimeter Bolometer Camera for the Atacama Cosmology Telescope (MBC/ACT), and the Redshift (Z) Early Universe Spectrometer (ZEUS j.

  5. Stress Relaxation Effects in TiNi SMA During Superelastic Deformation: Experiment and Constitutive Model

    Science.gov (United States)

    Pieczyska, Elżbieta A.; Kowalewski, Zbigniew L.; Dunić, Vladimir Lj.

    2017-12-01

    This paper presents an investigation of thermomechanical effects related to the phenomena of stress relaxation occurring in TiNi SMA subjected to modified program of displacement-controlled tension. The deformation data were taken from testing machine, whereas the temperature changes accompanying the exothermic/endothermic martensite forward/reverse transformation were measured by infrared camera. At the advanced stages of the transformations, the strain was kept constant for a few minutes and the SMA load and temperature were recorded continuously. As a consequence, the stress and temperature changed significantly during the loading stops. A large stress drop, caused by the transformation, was observed during the relaxation stage in both courses of the SMA loading and unloading. Moreover, the non-uniform temperature distribution, reflecting macroscopically inhomogeneous transformation, lapsed while the strain was kept constant, yet restarted at the end of the relaxation stop and developed at the reloading stage. Along with the experimental results, the mechanical and thermal responses induced by the transformation were obtained by 3D coupled thermomechanical numerical analysis, realized in partitioned approach. Latent heat production was correlated with an amount of the martensitic volume fraction. The stress and temperature drops recorded during the experiment were satisfactorily reproduced by the model proposed for the SMA thermomechanical coupling.

  6. PELAKSANAAN PROGRAM BOARDING SCHOOL DALAM PEMBINAAN MORAL SISWA DI SMA TARUNA INDONESIA PALEMBANG

    Directory of Open Access Journals (Sweden)

    Hendriyenti H

    2014-12-01

    Full Text Available AbstractIndonesia nowadays faces some moral issues in teenagers scope or adult scope such as the use of drugs, violence, rascality, abortion, persecution, gambling, prostitution, and so on. Those problems are very danger for the country. Therefore, moral education is very important in this situation. The study was done at SMA Taruna Indonesia Palembang by the tittle: “the Implementation of boarding School Program for Students Moral education at SMA Taruna Indonesia Palembang”.Based on the result of the stuy, it was found that the implementation of boarding school program to educate students’moral at SMA Taruna Indonesia Palembang was applied throug dicipline implementation program and religion education program. Those two programs were applied by preventive and currative treatment. Moreover, there were some factors which support students’ moral education at SMA Taruna Indonesia Palembang such as students motivation, advisors dedication, 24 hours education and guidance, good coordination between advisors, teachers, securities, and other staff, and far location of boarding school from city center. As long as the teenager is an unstable period, there weremany difficulties in educate them. Finally,it is hoped that school stakeholders could improve the school management so that those difficulties could be solved and moral education could be applied.  Keywords: boarding school, morality building

  7. Disrupting SMA activity modulates explicit and implicit emotional responses: an rTMS study.

    Science.gov (United States)

    Rodigari, Alessia; Oliveri, Massimiliano

    2014-09-05

    Supplementary Motor Area (SMA) has been considered as an interface between the emotional/motivational system and motor effector system. Here, we investigated whether it is possible to modulate emotional responses using non-invasive brain stimulation of the SMA. 1Hz repetitive transcranial magnetic stimulation (rTMS) trains were applied over the SMA of healthy subjects performing a task requiring to judge the valence and arousal of emotional stimuli. rTMS trains over the SMA increased the perceived valence of emotionally negative visual stimuli, while decreasing the perceived valence of emotionally positive ones. The modulatory effect on emotional valence was specific for stimuli with emotional content, since it was not observed for neutral visual stimuli. The effect was also specific for the site of stimulation, since rTMS of the visual cortex failed to modulate either perceived valence or arousal. These findings provide the first example of neuromodulation of emotional responses based on non-invasive brain stimulation. Copyright © 2014. Published by Elsevier Ireland Ltd.

  8. 'The crab', a new cryo magnet transport vehicle, in action in building SMA18

    CERN Multimedia

    2006-01-01

    The crab is used to transport LHC cryo-magnets and their components in the assembly and preparation building, SMA18, and test building, SM18. It has many capabilities that allow CERN staff and contractors transport magnets between the two buildings and to locate them in the right position on the test beds.

  9. A PROVISIONAL TRANSCRIPT MAP OF THE SPINAL MUSCULAR-ATROPHY (SMA) CRITICAL REGION

    NARCIS (Netherlands)

    VANDERSTEEGE, G; DRAAIJERS, TG; GROOTSCHOLTEN, PM; OSINGA, J; ANZEVINO, R; VELONA, [No Value; DENDUNNEN, JT; SCHEFFER, H; BRAHE, C; VANOMMEN, GJB; BUYS, CHCM

    1995-01-01

    YACs from the region containing the spinal muscular atrophy (SMA) locus at 5q12 have been used as probes in a direct screening of cDNA libraries to isolate 8 cDNAs, mapped to different YAC fragments. Three clones showed complete identity to the genes for cyclin B1 (CCNB1), the p44 subunit of the

  10. Bulbar muscle MRI changes in patients with SMA with reduced mouth opening and dysphagia.

    NARCIS (Netherlands)

    Wadman, R.I.; Bruggen, H.W. van; Witkamp, T.D.; Kalaykova, S.I.; Stam, M.; Berg, L.H. van den; Steenks, M.H.; Pol, W.L. van der

    2014-01-01

    OBJECTIVE: We performed a study in patients with proximal spinal muscular atrophy (SMA) to determine the prevalence of reduced maximal mouth opening (MMO) and its association with dysphagia as a reflection of bulbar dysfunction and visualized the underlying mechanisms using MRI. METHODS: We

  11. Metal muscles and nerves—a self-sensing SMA-actuated hand concept

    Science.gov (United States)

    Simone, F.; Rizzello, G.; Seelecke, S.

    2017-09-01

    Bio-inspired hand-like grippers actuated by Shape Memory Alloy (SMA) wires represent an emerging new technology with potential applications in many different fields, ranging from industrial assembly processes to biomedical systems. The inherently high energy density makes SMAs a natural choice for compact, lightweight, and silent actuator systems capable of producing a high amount of work, such as hand prostheses or robotic systems in industrial human/machine environments. In this work, a concept for a compact and versatile gripping system is developed, in which SMA wires are implemented as antagonistic muscles actuating an artificial hand with three fingers. In order to combine high gripping force with sufficient actuation speed, the muscle implementation pursues a multi-wire concept with several 0.1 mm diameter NiTi wires connected in parallel, in order to increase the surface-to-volume ratio for accelerated cooling. The paper starts with an illustration of the design concept of an individual 3-phalanx-finger, along with kinematic considerations for optimal placement of SMA wires. Three identical fingers are subsequently fabricated via 3D printing and assembled into a hand-like gripper. The maximum displacement of each finger phalanx is measured, and an average phalanxes dynamic responsiveness is evaluated. SMA self-sensing is documented by experiments relating the wires change in resistance to the finger motion. Several finger force measurements are also performed. The versatility of the gripper is finally documented by displaying a variety of achievable grasping configurations.

  12. Mandibular dysfunction as a reflection of bulbar involvement in SMA type 2 and 3.

    NARCIS (Netherlands)

    Bruggen, H.W. van; Wadman, R.I.; Bronkhorst, E.M.; Leeuw, M. de; Creugers, N.H.; Kalaykova, S.I.; Pol, W.L. van der; Steenks, M.H.

    2016-01-01

    OBJECTIVE: In a cross-sectional study, we aimed to determine (1) the effect of spinal muscular atrophy (SMA) type 2 and 3 on mandibular function reflected as masticatory performance, mandibular range of motion, and bite force and (2) the predictors of mandibular dysfunction. METHODS: Sixty patients

  13. Design and fabrication of a three-finger prosthetic hand using SMA muscle wires

    Science.gov (United States)

    Simone, Filomena; York, Alexander; Seelecke, Stefan

    2015-03-01

    Bio-inspired hand-like gripper systems based on shape memory alloy (SMA) wire actuation have the potential to enable a number of useful applications in, e.g., the biomedical field or industrial assembly systems. The inherent high energy density makes SMA solutions a natural choice for systems with lightweight, low noise and high force requirements, such as hand prostheses or robotic systems in a human/machine environment. The focus of this research is the development, design and realization of a SMA-actuated prosthetic hand prototype with three fingers. The use of thin wires (100 μm diameter) allows for high cooling rates and therefore fast movement of each finger. Grouping several small wires mechanically in parallel allows for high force actuation. To save space and to allow for a direct transmission of the motion to each finger, the SMA wires are attached directly within each finger, across each phalanx. In this way, the contraction of the wires will allow the movement of the fingers without the use of any additional gears. Within each finger, two different bundles of wires are mounted: protagonist ones that create bending movement and the antagonist ones that enable stretching of each phalanx. The resistance change in the SMA wires is measured during actuation, which allows for monitoring of the wire stroke and potentially the gripping force without the use of additional sensors. The hand is built with modern 3D-printing technologies and its performance while grasping objects of different size and shape is experimentally investigated illustrating the usefulness of the actuator concept.

  14. Increased SMA-M1 coherence in Parkinson's disease - Pathophysiology or compensation?

    Science.gov (United States)

    Pollok, Bettina; Kamp, Daniel; Butz, Markus; Wojtecki, Lars; Timmermann, Lars; Südmeyer, Martin; Krause, Vanessa; Schnitzler, Alfons

    2013-09-01

    Parkinson's disease (PD) is a common neurodegenerative disorder owing to loss of dopaminergic cells. Akinesia - one of the core symptoms of PD - is associated with exaggerated oscillations at beta frequency (13-30 Hz) within the subthalamic nucleus (STN). Thus, enhanced oscillations below 30 Hz are assumed to represent a pathophysiological marker of PD. However, recent data suggest that OFF medication exaggerated beta oscillations within basal ganglia (BG) cortical networks may serve for the compensation of BG dysfunctions. The STN is functionally connected to mesial prefrontal areas like the supplementary motor area (SMA). But, it is still not fully understood how enhanced beta oscillations within the BG exert dominance over the primary motor cortex (M1) thereby yielding motor impairment. The present study, therefore, investigates the effect of dopaminergic state on SMA-M1 functional connectivity using Magnetoencephalography (MEG). MEG data were recorded in 7 patients suffering from PD with preponderance of akinesia during isometric contraction of the right forearm and during rest. Coherence as a measure of functional connectivity between M1 and SMA was calculated OFF and ON medication and correlated with the motor part of the Unified Parkinson's Disease Rating Scale (UPDRS III) and with disease duration. During rest a significant positive correlation between disease duration and SMA-M1 coherence was found ON but not OFF medication. Conversely, during isometric contraction SMA-M1 coherence and UPDRS III were inversely correlated OFF but not ON medication explaining more than 80% of variance. The results favor the hypothesis that OFF medication exaggerated cortical coherence at beta frequency represents a compensatory mechanism rather than a pathophysiological marker per se. Copyright © 2013 Elsevier Inc. All rights reserved.

  15. Band-1 receiver front-end cartridges for Atacama Large Millimeter/submillimeter Array (ALMA): design and development toward production

    Science.gov (United States)

    Hwang, Yuh-Jing; Chiong, Chau-Ching; Huang, Yau-De; Huang, Chi-Den; Liu, Ching-Tang; Kuo, Yue-Fang; Weng, Shou-Hsien; Ho, Chin-Ting; Chiang, Po-Han; Wu, Hsiao-Ling; Chang, Chih-Cheng; Jian, Shou-Ting; Lee, Chien-Feng; Lee, Yi-Wei; Pospieszalski, Marian; Henke, Doug; Finger, Ricardo; Tapia, Valeria; Gonzalez, Alvaro

    2016-07-01

    The ALMA Band-1 receiver front-end prototype cold and warm cartridge assemblies, including the system and key components for ALMA Band-1 receivers have been developed and two sets of prototype cartridge were fully tested. The measured aperture efficiency for the cold receiver is above the 80% specification except for a few frequency points. Based on the cryogenically cooled broadband low-noise amplifiers provided by NRAO, the receiver noise temperature can be as low as 15 - 32K for pol-0 and 17 - 30K for pol-1. Other key testing items are also measured. The receiver beam pattern is measured, the results is well fit to the simulation and design. The pointing error extracted from the measured beam pattern indicates the error is 0.1 degree along azimuth and 0.15 degree along elevation, which is well fit to the specification (smaller than 0.4 degree). The equivalent hot load temperature for 5% gain compression is 492 - 4583K, which well fit to the specification of 5% with 373K input thermal load. The image band suppression is higher than 30 dB typically and the worst case is higher than 20 dB for 34GHz RF signal and 38GHz LO signal, which is all higher than 7 dB required specification. The cross talk between orthogonal polarization is smaller than -85 dB based on present prototype LO. The amplitude stability is below 2.0 x 10-7 , which is fit to the specification of 4.0 x 10-7 for timescales in the range of 0.05 s ≤ T ≤ 100 s. The signal path phase stability measured is smaller than 5 fs, which is smaller than 22 fs for Long term (delay drift) 20 s ≤ T power level is -28 to -30.5 dBm with 300K input load. The measured IF output power flatness is less than 5.6 dB for 2GHz window, and 1.3dB for 31MHz window. The first batch of prototype cartridges will be installed on site for further commissioning on July of 2017.

  16. The Spitzer survey of interstellar clouds in the Gould Belt. III. A multi-wavelength view of Corona Australis

    DEFF Research Database (Denmark)

    Peterson, Dawn E.; Caratti o Garatti, Alessio; Bourke, Tyler L.

    2011-01-01

    with the Submillimeter Array (SMA) covering R CrA, IRS 5, IRS 7, and IRAS 18595-3712 (IRAS 32). We also present multi-epoch H2 maps and detect jets and outflows, study their proper motions, and identify exciting sources. The Spitzer and ISAAC/VLT observations of IRAS 32 show a bipolar precessing jet, which drives a CO(2......-1) outflow detected in the SMA observations. There is also clear evidence for a parsec-scale precessing outflow, which is east-west oriented and originates in the SMA 2 region and likely driven by SMA 2 or IRS 7A....

  17. Evaluation of SMN Protein, Transcript, and Copy Number in the Biomarkers for Spinal Muscular Atrophy (BforSMA) Clinical Study

    Science.gov (United States)

    Crawford, Thomas O.; Paushkin, Sergey V.; Kobayashi, Dione T.; Forrest, Suzanne J.; Joyce, Cynthia L.; Finkel, Richard S.; Kaufmann, Petra; Swoboda, Kathryn J.; Tiziano, Danilo; Lomastro, Rosa; Li, Rebecca H.; Trachtenberg, Felicia L.; Plasterer, Thomas; Chen, Karen S.

    2012-01-01

    Background The universal presence of a gene (SMN2) nearly identical to the mutated SMN1 gene responsible for Spinal Muscular Atrophy (SMA) has proved an enticing incentive to therapeutics development. Early disappointments from putative SMN-enhancing agent clinical trials have increased interest in improving the assessment of SMN expression in blood as an early “biomarker” of treatment effect. Methods A cross-sectional, single visit, multi-center design assessed SMN transcript and protein in 108 SMA and 22 age and gender-matched healthy control subjects, while motor function was assessed by the Modified Hammersmith Functional Motor Scale (MHFMS). Enrollment selectively targeted a broad range of SMA subjects that would permit maximum power to distinguish the relative influence of SMN2 copy number, SMA type, present motor function, and age. Results SMN2 copy number and levels of full-length SMN2 transcripts correlated with SMA type, and like SMN protein levels, were lower in SMA subjects compared to controls. No measure of SMN expression correlated strongly with MHFMS. A key finding is that SMN2 copy number, levels of transcript and protein showed no correlation with each other. Conclusion This is a prospective study that uses the most advanced techniques of SMN transcript and protein measurement in a large selectively-recruited cohort of individuals with SMA. There is a relationship between measures of SMN expression in blood and SMA type, but not a strong correlation to motor function as measured by the MHFMS. Low SMN transcript and protein levels in the SMA subjects relative to controls suggest that these measures of SMN in accessible tissues may be amenable to an “early look” for target engagement in clinical trials of putative SMN-enhancing agents. Full length SMN transcript abundance may provide insight into the molecular mechanism of phenotypic variation as a function of SMN2 copy number. Trial Registry Clinicaltrials.gov NCT00756821 PMID:22558076

  18. Evaluation of SMN protein, transcript, and copy number in the biomarkers for spinal muscular atrophy (BforSMA clinical study.

    Directory of Open Access Journals (Sweden)

    Thomas O Crawford

    Full Text Available BACKGROUND: The universal presence of a gene (SMN2 nearly identical to the mutated SMN1 gene responsible for Spinal Muscular Atrophy (SMA has proved an enticing incentive to therapeutics development. Early disappointments from putative SMN-enhancing agent clinical trials have increased interest in improving the assessment of SMN expression in blood as an early "biomarker" of treatment effect. METHODS: A cross-sectional, single visit, multi-center design assessed SMN transcript and protein in 108 SMA and 22 age and gender-matched healthy control subjects, while motor function was assessed by the Modified Hammersmith Functional Motor Scale (MHFMS. Enrollment selectively targeted a broad range of SMA subjects that would permit maximum power to distinguish the relative influence of SMN2 copy number, SMA type, present motor function, and age. RESULTS: SMN2 copy number and levels of full-length SMN2 transcripts correlated with SMA type, and like SMN protein levels, were lower in SMA subjects compared to controls. No measure of SMN expression correlated strongly with MHFMS. A key finding is that SMN2 copy number, levels of transcript and protein showed no correlation with each other. CONCLUSION: This is a prospective study that uses the most advanced techniques of SMN transcript and protein measurement in a large selectively-recruited cohort of individuals with SMA. There is a relationship between measures of SMN expression in blood and SMA type, but not a strong correlation to motor function as measured by the MHFMS. Low SMN transcript and protein levels in the SMA subjects relative to controls suggest that these measures of SMN in accessible tissues may be amenable to an "early look" for target engagement in clinical trials of putative SMN-enhancing agents. Full length SMN transcript abundance may provide insight into the molecular mechanism of phenotypic variation as a function of SMN2 copy number. TRIAL REGISTRY: Clinicaltrials.gov NCT00756821.

  19. Design and fabrication of two-dimensional superconducting bolometer arrays

    Science.gov (United States)

    Benford, Dominic J.; Staguhn, Johannes G.; Stacey, Gordon J.; Page, Lyman; Moseley, S. H., Jr.; Irwin, Kent D.; Chervenak, James A.; Allen, Christine A.

    2004-10-01

    We have been developing an architecture for producing large format, two-dimensional arrays of close-packed bolometers, which will enable far-infrared to millimeter wavelength (lambda=100µm-2mm) cameras and spectrometers to obtain images and spectra orders of magnitude faster than present instruments. The low backgrounds achieved in these instruments require very sensitive detectors with NEPs ranging from 10-17 to 10-19 W/(Hz-1/2). Superconducting transition edge sensor bolometers can be close-packed using the Pop-Up Detector (PUD) format, and SQUID multiplexers operating at the detector base temperature can be intimately coupled to them. The array unit cell is 8x32 pixels, using 32-element detector and multiplexer components. We have fabricated an engineering model array with this technology featuring a very compact, modular approach for large format arrays. We report on the production of the 32-element components for the arrays. Planned instruments using this array architecture include the Submillimeter and Far-InfraRed Experiment (SAFIRE) on the SOFIA airborne observatory, the South Pole Imaging Fabry-Perot Interferometer (SPIFI) for the AST/RO observatory, the Millimeter Bolometer Camera for the Atacama Cosmology Telescope (MBC/ACT), and the Redshift "Z" Early Universe Spectrometer (ZEUS).

  20. Design of SMA - 13 asphalt mixture ratio on Z3and Z18 of the capital airport

    Science.gov (United States)

    Tian, Shuaituan; Ye, Song; Kong, Fandong

    2017-12-01

    According to the demand of T2 terminal airlines to operate A380 models, to meet the smooth running of the A380 airliner at the west end of the Capital Airport, So Z3 and Z18 taxiway area of the transformation is imperative. According to the design, the upper layer of this project adopts SMA - 13 modified asphalt mastic macadam mixture. We design the SMA-13 modified asphalt mixture on Z3 and Z18 of the capital airport from any respects, including coarse and fine aggregate, filler, asphalt, fiber and anti-rutting agent, and we hope we can find the best SMA-13 modified asphalt mixture.

  1. Note: A SMA wire actuated extremely long-lifetime release actuator using two ball-lock mechanisms

    Science.gov (United States)

    Huang, Dawei; Yan, Xiaojun; Zhang, Xiaoyong; Bai, Haibo; Wang, Xian; Liu, Ying

    2017-05-01

    A shape memory alloy (SMA)-wire actuated release actuator with an extremely long lifetime was designed and validated. To ensure the ability of repeated actuation, two stages of ball-lock mechanisms were adopted to reduce the load in the SMA wire. In addition, a length-increasing design of the SMA wire was employed. Validation tests, including function tests, vibration tests, shock tests, and thermal vacuum tests were conducted on prototypes. According to the test results, the actuator can release a maximum preload of 15 kN and has a lifetime of more than 693 cycles. Furthermore, the actuator can function well, even under severe thermal and vibration environments.

  2. PENGEMBANGAN MODEL KKBB SEBAGAI UPAYA PENINGKATAN KUALITAS PEMBELAJARAN SEJARAH SMA DI SOLO RAYA

    Directory of Open Access Journals (Sweden)

    Leo Agung S.

    2014-01-01

    Full Text Available This paper was aimed providing training assistance KKBB models to history teachers in high schools; Doing trials, extensive testing and the effective test of KKBB models; promoting a model of KKBB Solo Raya. The subjects of those research are teachers and high school students in Solo Raya. Data collection use some techniques, namely  observation, interview, and test. The method of data analysis uses quantitative analysis by t test. It can be concluded that: (1 the team has successfully conducted training assistance to high school history teachers Solo Raya KKBB model, (2 Trial in High School 1 Ngemplak with Classroom Action Research, extensive testing in 2 High school Boyolali and 3 High School Kartasura, effective trials in 2 Karangnyar  High School, 8 High School  Surakarta, and  2 High School  Sukoharjo  KKBB is able to improve the quality of learning noted by the development of competence and strengthen of character values among students in the various school groups. In the other words, KBBImodel is more effective than the KKBB Varied-Lecture model. Keywords: teaching history, KKBB models, character education Penelitian ini bertujuan memberikan pelatihan pendampingan model KKBB kepada guru-guru Sejarah SMA, melakukan uji coba, uji luas dan uji efektivitas model  KKBB, dan  mensosialisasikan model KKBB se Solo Raya. Subjek penelitian guru-guru dan siswa SMA Solo Raya. Teknik pengumpulan data menggunakan observasi, wawancara, dan test. Adapun metode analisis data menggunakan analisis kuantitatif dengan uji t. Hasil penelitian dapat disimpulkan bahwa tim telah berhasil melakukan pelatihan pendam-pingan kepada guru-guru Sejarah SMA Solo Raya dengan model KKBB. Uji coba di SMA 1 Ngemplak dengan PTK, uji luas di   SMA  2 Boyolali  dan SMA  1 Kartasura,  uji efektivitas di SMA  2 Karangnyar, SMA  8 Surakarta, dan SMA 2 Sukoharjo terbukti pembelajaran model  KKBB mampu meningkatkan kualitas pembela-jaran yang ditandai dengan

  3. PEMANFAATAN MUSEUM BLAMBANGAN SEBAGAI SUMBER BELAJAR SEJARAH DI KELAS X SMA NEGERI KABUPATEN BANYUWANGI

    Directory of Open Access Journals (Sweden)

    Agus Mursidi

    2011-10-01

    Full Text Available The purpose of this study is to determine: (1 Type of Blambangan Museum collection that can be utilized as a resource for high school students learning history, (2 How to utilize Blambangan Museum collection as a source for high school students learning history, (3 Appreciation of high school students to the Museum Blambangan as a source of high school students learning history, and (4 The constraints faced by students and teachers in utilizing the Museum Blambangan as a source of learning history. Types of collections that can be used as a source to learn the history in SMA is keramologika (jar, filologika (sword, historika (clothing regent, etnografika (ax square, arkeologika (papyrus manuscript, teknologika (phonograph and the fine arts (brick berelief and miniature art infatuated, (2 In accordance with the standards of competence and basic competence as a source of how to utilize the museum to learn history, the learning process can be done is through the method of study tours and home work by teachers to students.   Key words: Blambangan Museum, Learning Resources, Learning History, high school   Tujuan penelitian ini adalah untuk mengetahui: (1 Jenis koleksi Museum Blambangan yang dapat dimanfaatkan sebagai sumber daya untuk siswa SMA belajar sejarah, (2 Bagaimana memanfaatkan koleksi Museum Blambangan sebagai sumber untuk siswa SMA belajar sejarah, (3 Apresiasi siswa sekolah tinggi ke Museum Blambangan sebagai sumber siswa SMA belajar sejarah, dan (4 kendala yang dihadapi oleh siswa dan guru dalam memanfaatkan Blambangan Museum sebagai sumber belajar sejarah. Jenis koleksi yang dapat digunakan sebagai sumber untuk belajar sejarah SMA keramologika (jar, filologika (pedang, historika (pakaian, etnografika (kapak persegi, arkeologika (naskah papirus, teknologika (phonograph dan denda seni (batu bata berelief dan seni miniatur tergila-gila, (2 Sesuai dengan Standar Kompetensi dan Kompetensi Dasar sebagai sumber bagaimana

  4. Observational Approach to Molecular Cloud Evolutation with the Submillimeter-Wave CI Lines

    Science.gov (United States)

    Oka, T.; Yamamoto, S.

    Neutral carbon atoms (CI) play important roles both in chemistry and cooling processes of interstellar molecular clouds. It is thus crucial to explore its large area distribution to obtain information on formation processes and thermal balance of molecular clouds. However, observations of the submillimeter-wave CI lines have been limited to small areas around some representative objects. We have constructed a 1.2 m submillimeter-wave telescope at the summit of Mt.Fuji. The telescope was designed for the exclusive use of surveying molecular clouds in two submillimeter-wave CI lines, 3 P1 -3 P0 (492GHz) and 3 P2 -3 P1 (809 GHz), of atomic carbon. A superconductor-insulator-superconductor (SIS) mixer receiver was equipped on the Nasmyth focus of the telescope. The receiver noise temperatures [Trx(DSB)] are 300 K and 1000 K for the 492 GHz and the 809 GHz mixers, respectively. The intermediate frequency is centered at 2 GHz, having a 700 MHz bandwidth. An acousto-optical spectrometer (AOS) with 1024 channel outputs is used as a receiver backend. The telescope was installed at Nishi-yasugawara (alt. 3725 m), which is 200 m north of the highest peak, Kengamine (3776 m), in July 1998. It has b en operatede successfully during 4 observing seasons in a remote way from the Hongo campus of the University of Tokyo. We have already observed more than 40 square degrees of the sky with the CI 492 GHz line. The distribution of CI emission is found to be different from those of the 13 CO or C1 8 O emission in some clouds. These differences are discussed in relation to formation processes of molecular clouds.

  5. Sensitivity Study of Ice Crystal Optical Properties in the 874 GHz Submillimeter Band

    Science.gov (United States)

    Tang, Guanglin; Yang, Ping; Wu, Dong L.

    2015-01-01

    Testing of an 874 GHz submillimeter radiometer on meteorological satellites is being planned to improve ice water content retrievals. In this paper we study the optical properties of ice cloud particles in the 874 GHz band. The results show that the bulk scattering and absorption coefficients of an ensemble of ice cloud particles are sensitive to the particle shape and effective diameter, whereas the latter is also sensitive to temperature. The co-polar back scattering cross-section is not sensitive to particle shape, temperature, and the effective diameter in the range of 50200 m.

  6. cluster-in-a-box: Statistical model of sub-millimeter emission from embedded protostellar clusters

    Science.gov (United States)

    Kristensen, Lars E.; Bergin, Edwin A.

    2016-10-01

    Cluster-in-a-box provides a statistical model of sub-millimeter emission from embedded protostellar clusters and consists of three modules grouped in two scripts. The first (cluster_distribution) generates the cluster based on the number of stars, input initial mass function, spatial distribution and age distribution. The second (cluster_emission) takes an input file of observations, determines the mass-intensity correlation and generates outflow emission for all low-mass Class 0 and I sources. The output is stored as a FITS image where the flux density is determined by the desired resolution, pixel scale and cluster distance.

  7. Solar Flash Sub-Millimeter Wave Range Spectrum Part Radiation Modeling

    Directory of Open Access Journals (Sweden)

    V. Yu. Shustikov

    2015-01-01

    Full Text Available Currently, solar flares are under observation on the RT-7.5 radio telescope of BMSTU. This telescope operates in a little-studied range of the spectrum, at wavelengths of 3.2 and 2.2 mm (93 and 140 GHz, thereby providing unique information about parameters of the chromosphere plasma and zone of the temperature minimum. Observations on various instruments provided relatively small amount of data on the radio emission flare at frequencies close to 93 GHz, and at frequency of 140 GHz such observations were not carried out. For these reasons, data collected from the RT-7.5 radio telescope are of high value (Shustikov et al., 2012.This work describes modeling and gives interpretation of the reason for raising flux density spectrum of sub-millimeter radio frequency emission using as an example the GOES flare of class M 5.3 occurred on 04.07.2012 in the active region 11515. This flare was observed on the RT-7.5 radio telescope of BMSTU and was described by Shustikov et al. (2012 and by Smirnova et al. (2013, where it has been suggested that the reason for raising radio frequency emission is a bremsstrahlung of the thermal electrons in the hot plasma of the solar chromosphere. Rough estimates of the plasma temperature at the flare source were obtained.This paper proposes model calculations of the flux density spectrum of the sub-millimeter radio emission based on the gyrosynchrotron Fleischman-Kuznetsov code (Fleishman & Kuznetsov, 2010. Section 1 briefly describes observational data, tools and processing methods used in the work. Section 2 shows results of modeling the flare radio emission. Section 3 discusses results and conclusions.Numerical modeling the sub-millimeter part of the spectrum of the radio flux density for the GOES flare of class M5.3 has been carried out. This flare occurred in the active region 11515 on 04.07.2012. Modeling was based on the observations on the BMSTU’s RT-7.5 radio telescope.The paper draws conclusion based on the

  8. Wavefront Sensing and Control Technology for Submillimeter and Far-Infrared Space Telescopes

    Science.gov (United States)

    Redding, Dave

    2004-01-01

    The NGST wavefront sensing and control system will be developed to TRL6 over the next few years, including testing in a cryogenic vacuum environment with traceable hardware. Doing this in the far-infrared and submillimeter is probably easier, as some aspects of the problem scale with wavelength, and the telescope is likely to have a more stable environment; however, detectors may present small complications. Since this is a new system approach, it warrants a new look. For instance, a large space telescope based on the DART membrane mirror design requires a new actuation approach. Other mirror and actuation technologies may prove useful as well.

  9. Submillimeter-resolution radiography of shielded structures with laser-accelerated electron beams

    Directory of Open Access Journals (Sweden)

    Vidya Ramanathan

    2010-10-01

    Full Text Available We investigate the use of energetic electron beams for high-resolution radiography of flaws embedded in thick solid objects. A bright, monoenergetic electron beam (with energy >100  MeV was generated by the process of laser-wakefield acceleration through the interaction of 50-TW, 30-fs laser pulses with a supersonic helium jet. The high energy, low divergence, and small source size of these beams make them ideal for high-resolution radiographic studies of cracks or voids embedded in dense materials that are placed at a large distance from the source. We report radiographic imaging of steel with submillimeter resolution.

  10. Submillimeter-Resolution Radiography of Shielded Structures with Laser-Accelerated Electron Beams

    Energy Technology Data Exchange (ETDEWEB)

    Ramanathan, Vidya [University of Nebraska, Lincoln; Banerjee, Sudeep [University of Nebraska, Lincoln; Powell, Nathan [University of Nebraska, Lincoln; Cummingham, N. J. [University of Nebraska, Lincoln; Chandler-Smith, Nate [University of Nebraska, Lincoln; Zhao, Kun [University of Nebraska, Lincoln; Brown, Kevin [University of Nebraska, Lincoln; Umstadter, Donald [University of Nebraska, Lincoln; Clarke, Shaun [University of Michigan; Pozzi, Sara [University of Michigan; Beene, James R [ORNL; Vane, C Randy [ORNL; Schultz, David Robert [ORNL

    2010-10-01

    We investigate the use of energetic electron beams for high-resolution radiography of flaws embedded in thick solid objects. A bright, monoenergetic electron beam (with energy >100 MeV) was generated by the process of laser-wakefield acceleration through the interaction of 50-TW, 30-fs laser pulses with a supersonic helium jet. The high energy, low divergence, and small source size of these beams make them ideal for high-resolution radiographic studies of cracks or voids embedded in dense materials that are placed at a large distance from the source. We report radiographic imaging of steel with submillimeter resolution.

  11. Study of optical output couplers for submillimeter wavelength backward-wave oscillators (BWO's)

    Science.gov (United States)

    Cook, Jerry D.; Stankiewicz, Norbert; Podany, Mark

    1989-01-01

    Several scaled experiments of optical output couplers for submillimeter backward-wave oscillators (BWOs). Various designs of planar antennas (Vivaldi horns) lens-feed systems (hyperhemispherical lens) were constructed and tested between 20 and 100 GHz using a spectrum analyzer. The lens system was also tested at 337 GHz using a CO2 pumped FIR laser. It is found that Vivaldi horns have unsatisfactory resonances, perhaps because the horns studied were relatively short. Several techniques to maximize and flatten the frequency response of these horns are presented. The results suggest that alternate coupling schemes are superior to Vivaldi horns.

  12. Seismic Performance and Ice-Induced Vibration Control of Offshore Platform Structures Based on the ISO-PFD-SMA Brace System

    Directory of Open Access Journals (Sweden)

    Jigang Zhang

    2017-01-01

    Full Text Available Pall-typed frictional damper (PFD has higher capacity of energy dissipation, whereas shape memory alloy (SMA has excellent superelastic performance. Therefore, combining PFD and SMA together as a brace system has a great prospect in vibration control of structures. This paper investigates the performance of offshore platform with three structural configurations including the SMA brace system, the ISO-SMA (where ISO stands for isolation brace system, and the ISO-PFD-SMA brace system, which are subjected to seismic and ice-induced excitations. In this study, PFD-SMA brace system is installed on the isolation layer of jacket platform, which is under earthquake excitations and ice loading. Then, the reduction of vibration is evaluated by using ANSYS program. The results show that the PFD-SMA brace system is useful in reducing the seismic response and ice-induced response of offshore platform structures; meanwhile, it also demonstrates excellent energy dissipation and hysteretic behavior.

  13. Experimental and numerical analysis of penetration/removal response of endodontic instrument made of single crystal Cu-based SMA: comparison with NiTi SMA instruments

    Science.gov (United States)

    Vincent, M.; Xolin, P.; Gevrey, A.-M.; Thiebaud, F.; Engels-Deutsch, M.; Ben Zineb, T.

    2017-04-01

    This paper presents an experimental and numerical study showing that single crystal shape memory alloy (SMA) Cu-based endodontic instruments can lead to equivalent mechanical performances compared to NiTi-based instruments besides their interesting biological properties. Following a previous finite element analysis (FEA) of single crystal CuAlBe endodontic instruments (Vincent et al 2015 J. Mater. Eng. Perform. 24 4128-39), prototypes with the determined geometrical parameters were machined and experimentally characterized in continuous rotation during a penetration/removal (P/R) protocol in artificial canals. The obtained mechanical responses were compared to responses of NiTi endodontic files in the same conditions. In addition, FEA was conducted and compared with the experimental results to validate the adopted modeling and to evaluate the local quantities inside the instrument as the stress state and the distribution of volume fraction of martensite. The obtained results highlight that single crystal CuAlBe SMA prototypes show equivalent mechanical responses to its NiTi homologous prototypes in the same P/R experimental conditions.

  14. CT muscle scanning in the evaluation of patients with spinal muscular atrophy (SMA)

    Energy Technology Data Exchange (ETDEWEB)

    Sambrook, P.; Rickards, D.; Cumming, W.J.K.

    1988-12-01

    One hundred with spinal muscular atrophy (SMA) were assessed by CT scanning using a standardised technique. The spectrum of CT abnormality occurring in SMA was observed and by overall analysis the patients were divided into 4 groups. While the CT appearances of these groups correlated well with clinical assessment of severity of disease, the disease process was usually much more widespread than clinical examination suggested. CT abnormality was first observed in the leg and gluteal muscles, progressing to the posterior spinal, thigh, shoulder girdle and sternomastoid muscles. Hypertrophy of sartorius and gracilis was observed in a significant number of patients. Fascial planes were preserved in involved muscles in over half of the patients, even in late-stage disease. Asymmetrical muscle involvement was seen with increasing frequency as the disease process increased in extent as evaluated by CT scanning. There was no discernible difference in the CT appearances in those patients who clinically had limb-girdle, facioscapulohumeral or scapuloperoneal distribution of weakness.

  15. TINGKAT PENGETAHUAN TENTANG SEKS BEBAS PADA REMAJA KELAS XI DI SMA NEGERI 11 YOGYAKARTA TAHUN 2014

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    Suherni

    2018-01-01

    Full Text Available Background: Free sex has become more familiar to teenagers in today's life. This phenomenon occurs within many teenagers in junior and senior high schools, in big cities as well as in remote villages. Free sex may result in unwanted pregnancy, sexually transmitted infections, and social disruption in the society. Objective: This study aimed to determine the level of knowledge about free sex in adolescents. Methods: This research was conducted in April 2014, at SMA 11 Yogyakarta. The subjects were all students of class XI, consisted of 270 students. This study used a questionnaire as a measuring tool. Data analysis was performed with a univariate analysis. Results: Results showed that most respondents had adequate level of knowledge (81%, 17% had moderate level of knowledge and 2% have low level of knowledge about free sex. Conclusion: The level of knowledge about free sex in SMA Negeri 11 Yogyakarta students was majority adequate.

  16. PEMBINAAN KEBERAGAMAAN SISWA MELALUI PENGEMBANGAN BUDAYA AGAMA DI SMA NEGERI 16 PALEMBANG

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    Ermis Suryana

    2013-11-01

    Full Text Available AbstractThe purpose of the study was to describe the religious development student trought the development of religious culture at SMA Negeri 16 Palembang. The result of the study showed that the implementation of coaching student’s religious through the development of religious culture at SMA 16 Palembang has been going well and programmed, both conducted by the school as an educational institution that is intact with the wisdom which relate to the development of the religious culture in school and community activities undertaken by Rohis (The Spiritual of Islam as a kind of special school extracurricular activities shade other religious activities. This success can be achieved due to the efforts of the principal and the support of the entire school community by showing commitment each of which takes place together and support each other.Keywords: Religious development, Religious culture.

  17. Pengembangan Modul Pembelajaran dengan Pendekatan Inkuiri Terbimbing pada Materi Koloid di SMA

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    Lita Novilia

    2017-03-01

    Abstrak: Materi koloid bersifat kontekstual, tetapi dalam pelaksanaannya materi koloid cenderung dihafal sehingga dapat menimbulkan beberapa miskonsepsi. Penelitian ini bertujuan untuk menguji kelayakan modul yang dikembangkan dengan pendekatan inkuiri terbimbing di SMA. Desain pengembangan mengacu pada Pedoman Penulisan Modul oleh Direktorat Tenaga Kependidikan Departemen Pendidikan Nasional (2008. Kelayakan modul ditinjau dari kriteria isi, penyajian, kebahasaan, dan kegrafikaan, serta respon siswa. Hasil penelitian menunjukkan bahwa modul pembelajaran yang telah dikembangkan layak digunakan. Kata kunci: pengembangan modul, materi koloid, inkuiri terbimbing, kelayakan modul

  18. Hubungan Pola Asuh Keluarga dengan Perilaku Remaja di SMA Negeri 14 Medan

    OpenAIRE

    Tarigan, Yuli Anita

    2015-01-01

    Teenagers are vulnerable to performing negative behavior because adolescence is a changing period, and a teenager will undergo physical, psychological, and social changes. Parents’ role in providing raising pattern is very important to forestall the incidence of adolescence negative behavior. The research was a quantitative study with descriptive correlation approach which was aimed to identify the correlation between family caring pattern and teenagers’ behavior at SMA Negeri 14, Medan. The ...

  19. Hubungan Facebook Addiction Disorder (Fad) dengan Perilaku Asertif Remaja di SMA Kristen 1 Tomohon

    OpenAIRE

    Polii, Gloria Gratia; Bidjuni, Hendro; Wowiling, Ferdinand

    2014-01-01

    : Facebook addiction berarti menghabiskan jumlah waktu yang berlebihan di facebook. Facebook merupakan situs jejaring sosial yang mudah digunakan, dan yang paling penting adalah mempunyai efek mencandu. Secara psikologis, dampak negatif kecanduan facebook dapat dibagi atas: Pribadi yang anti sosial dan Dualisme kepribadian. Tujuan penelitian ini untuk mengetahui hubungan Facebook Addiction Disorder (FAD) dengan Perilaku Asertif Remaja di SMA Kristen 1 Tomohon. Desain penelitian ini dilaksanak...

  20. Hubungan Penggunaan Media Sosial Dengan Kemampuan Interaksi Sosial Remaja di SMA Negeri 1 Kota Medan

    OpenAIRE

    Nugraheni, Auliya Tunnisaa

    2016-01-01

    Social media today is considered as an important daily need. The intensity of using it by adolescents is influenced by their need for information, either academic or non-academic information. The inclination of using it as a communication facility can directly effects one of the social interactions aspect among individual. The objective of this research was to find out the correlation of using social media with the capacity of social interaction in adolescents at SMA Negeri 1, Medan, using co...

  1. Pengaruh Metode Pembelajaran dan Berpikir Kritis terhadap Hasil Belajar Sejarah Siswa SMA Kesatuan Bogor

    OpenAIRE

    Iryance, Iin

    2014-01-01

    Absrtact The aim of the study is to reveal the empirical data about the effect of instructional methodology and student's critical thinking capability level on the outcome of history learning on the students of SMA Kesatuan Bogor. The methodology used is the experimental method with a 2x2 factorial design. Research instrumentation will include a test that will be used to measure student's learning outcome, and a questionnaire that will be used to measure student's critical thinking capabil...

  2. Pengaruh Strategi Pembelajaran dan Kemampuan Berpikir Kritis Terhadap Hasil Belajar Sejarah Siswa SMA Negeri 72 Jakarta

    OpenAIRE

    Horohiung, Veronika

    2017-01-01

    The aim of this research is to find The influence of Instructional Strategy and Critical Thinking to History Learning Outcomes in SMA Negeri 72 Jakarta. The type of this research is used experiment design treatment method. The Instrument that used to know the learning outcomes is Multiple Choice, and the instrument that used to know the result of Critical Thinking is Quisioner. The result of this research refer to: (1) to history learning outcomes that was giving PBL Instructional Strategy is...

  3. Tingkat Pengetahuan Siswa-Siswi SMA Methodist Pematang Siantar Terhadap Konjungtivitis

    OpenAIRE

    Erwin

    2012-01-01

    Conjunctivitis is a disease that occurs worldwide and can be suffered by the entire community regardless of age. Conjunctivitis must be quickly addressed because it can cause complications that vary depending on the type of cause. Common complication of conjunctivitis is a decrease in vision that will greatly affect the patient in doing daily activities. This study aims to determine the knowledge of high school students in SMA Methodist Siantar against conjunctivitis. Research carried out is ...

  4. Kajian Fisis Energi Terbarukan Panel Surya Melalui Eksperimen Sederhana untuk Siswa SMA

    OpenAIRE

    Sunaryo, Sunaryo; Retno Budi, Ajeng; Ruliana, Ruliana; Kholimah, Siti

    2015-01-01

    Abstract Has conducted research on the effects of light intensity on the output voltage, current, and power. Research conducted generate data in the form of quantitative and graphs that show a link between the intensity of light, the output voltage, current, and power. The data obtained were used as sources of learning in senior high school (SMA). The implication is capable of enhancing creativity, motivation and learning outcomes of Physics subject of high school students in future studies. ...

  5. INFORMATION MANAGEMENT SPECIAL EVENT HUTTEL 62 By SMA NEGERI 3 JAKARTA

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    Syahidatia Chairunissa Aulia

    2017-07-01

    Full Text Available The purpose of this research is to know how to process information management special event conducted by organizers HUTTEL 62 ranging from research, design, planning, coordination, and evaluation in accordance with the concept special event belongs to Joe Goldblatt. Research methods a descriptive, qualitative data with the paradigm of positivism. The results of this study suggested that the management of the special event HUTTEL 62 categorized in five stages, namely research, design, planning, coordination, and evaluation. Research carried out in the form of informal research with secondary data searches ways be monitoring news coverage about SMA Negeri 3 Jakarta. Hasl research shows the overview of the situation of informing host HUTTEL 62 is the assumption that the community name of the example contained in the SMA Negeri 3 Jakarta not sesuaid with what happened at that school. The design of the color purple and blue created the Customize the theme carried HUTTEL 62 ‘ Return Teladanku ‘. Motion design elements and sounds indicated by performers in closing. 62 HUTTEL planning begins with setting goals to be achieved, namely restoring the image of ‘ exemplary ‘ to SMA Negeri 3 Jakarta Post acts of bullying incidents. Coordination is done by the Organizer HUTTEL 62 include coordination with internal and external parties the Committee involved in organizing HUTTEL 62. The communication is done by informal meetings and mandatory meetings and communications with online messenger. The evaluation was conducted to measure the achievement of HUTTEL 62, the evaluation is conducted in the Division and the Division of any series of events have been implemented and later serve as a report on liability. Hasl acquired evaluation of barriers in the internal Committee namely the barriers of communication and information in the internal Committee. A summary of this research menenujukan that special event management HUTTEL 62 made by SMA Negeri 3 Jakarta

  6. Force-Deformation Response of a SMA-Based Actuator Considering the Electric Current Intensity as Step-Input

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    Ion-Cornel Mituletu

    2015-06-01

    Full Text Available The goal of the paper is to accomplish the response regarding the force-displacement characteristic evolution, of a Shape Memory Alloy (SMA actuator element. This reveals the first research stage in controlling the SMA behavior, providing important information about the heating-cooling time intervals. Step excitation of the SMA is performed by few values of electric current intensity, which produces the heating of SMA element up to 90-95 oC. To meet the testing requirements, an adequate test stand has been set up, consisting of sensors for force, displacement and temperature. The analog values provided by sensors were acquired and afterwards analyzed. The values of temperature, displacement and force were achieved, and their characteristic evolution has been performed. Thus, the time intervals are resulted and some other important aspects have been observed, regarding the delay between parameters and the temperature overshoot

  7. Analysis on Factors Affecting the Self-Repair Capability of SMA Wire Concrete Beam

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    Li Sun

    2013-01-01

    Full Text Available Crack expansion of concrete is the initial damage stage of structures, which may cause greater damage to structures subject to long-term loads or under extreme conditions. In recent years, the application of intelligent materials to crack self-repair has become a hotspot among researchers. In order to study the influence of factors on the self-repair capability of shape memory alloy (SMA wire concrete beam, both theoretical and experimental methods were employed for analysis. For the convenience of experiment, composite materials (epoxy cement mortar and silicone polymer clay instead of concrete were used. The SMA wires were externally installed on and internally embedded in epoxy resin cement mortar beams and silicone polymer clay beams. Comparison of crack repair situation between two installation methods turns out that both methods possess their own advantages and disadvantages and should be employed according to the actual situation. The influence of unbonded length on the self-repair capability of embedded type SMA wire beams and the necessary minimum unbonded length to achieve self-repair function were studied. The results state clearly that the longer the unbonded length is, the better the crack repair situation is.

  8. English Standar Kompetensi, Kompetensi Dasar, & Ujian Nasional of SMA in Revised Bloom`s Taxonomy

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    Putri Kamalia Hakim

    2017-10-01

    Full Text Available Abstract: This study was conducted to investigate the coverage of Revised Bloom’s taxonomy in the English Standar Kompetensi (SK, Kompetensi Dasar (KD and the English test items of Ujian Nasional for SMA. Content analysis method was chosen as the research design for this study. The writer analyzed the data by categorizing the verbs and the nouns of the data in relation to the categories and dimension of Revised Bloom’s Taxonomy. The results of this study revealed that 53% of SKs and KDs cover Understand category and the rest cover Analyze category. All of the SKs and KDs cover conceptual knowledge and other knowledge dimensions are not covered. Moreover, the coverage of Revised Bloom’s Taxonomy in English test items of Ujian Nasional for SMA is not aligned with the coverage of Revised Bloom’s Taxonomy in English SK and KD. The SKs and KDs only cover Remember, Understand, Apply and Analyze categories while the test items were associated with Remember, Understand, Apply, Analyze, and Evaluate categories. More than 90% of English test items of Ujian Nasional for SMA only covered low order of cognitive categories (Remember, Understand, and Apply. Most of the test items covered factual knowledge and the rest of them covered conceptual knowledge and none of them covered procedural and metacognitive knowledge.

  9. Simulación basada en SMA de sistemas originalmente representados con EDO

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    Ekaitz Zulueta Guerrero

    2011-10-01

    Full Text Available Resumen: En el presente trabajo se expone una metodología para modelar mediante un Sistema Multi-Agente (SMA sistemas biológicos y fisiológicos dinámicos con variables cuantificadas discretas, como el crecimiento y decrecimiento de poblaciones o el modelado epidemiológico de enfermedades. Se muestra un procedimiento para transformar un sistema de Ecuaciones Diferenciales Ordinarias (EDO (que modela un entorno de forma correcta en un SMA equivalente mediante un esquema basado en el método de Monte Carlo. Se utiliza un caso práctico fundamentado en un modelo matemático de Leucemia Mieloide Crónica (LMC para comparar la metodología basada en agentes con el modelado tradicional basado en un sistema de EDO. Se realiza una simulación con cada modelo (SMA y EDO y se compara los resultados obtenidos con ambas metodologías. Palabras clave: Ecuaciones diferenciales, modelo basado en agentes, Monte Carlo

  10. Peningkatan Mutu Pendidikan SMA Muhammadiyah 2 Sidoarjo sebagai Sekolah Berkategori The Outstanding School of Muhammadiyah

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    Hidayatulloh Hidayatulloh

    2016-09-01

    Full Text Available This article examines about improving the education quality of SMA Muhammadiyah 2 Sidoarjo as the Outstanding School of Muhammadiyah. This article reveals that the quality improvement of SMA Muhammadiyah 2 Sidoarjo was conducted through: the arrangement of school program and self evaluation, the reinforcement of vision, mission and education objective, the reinforcement of leadership and teamwork, the improvement of teachers and educators competence, the improvement learners quality input, the development of curriculum and learning, the development of school culture, the development of facilities and infrastructure, the development of community service, the cooperation of education and student exchange, the mobilization of education funding resources, the develop-ment of SIM, monitoring and evaluation, and education quality system. The management quality of SMA Muhammadiyah 2 Sidoarjo was run through input-process-output formula. The process of quality containes the process of quality planning, main process, supporting process, dan quality improvement process. Factors supporting the quality improvement are: Muhammadiyah’s popular name, the doctrine of education quality improvement, the leadership of TORSIE paradigm, the school academicians’ spirit of gaining achievement, the synergy of school academicians, the appropriate facilities, and the supports of all stakeholders.

  11. Budaya Sekolah Islami (BUSI: Studi Kasus di SMA Islam Sultan Agung 1 Semarang

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    Mustopa Mustopa

    2017-10-01

    Full Text Available The value crisis has affected the Indonesian people in all areas of life including education. These conditions lead to the importance of intensive value education in schools. This paper aims to find out the concept of Islamic School Culture (Busi and its implementation pattern in SMA Islam Sultan Agung 1 Semarang. The type of this research is descriptive qualitative. The result of the research shows that Busi in Sultan Agung 1 Semarang Islamic High School includes iqra 'culture, congregational prayer culture, thaharah culture, social interaction culture, and exemplary culture. The implementation pattern has been using top down with three step: socialization, habituation and monitoring. This pattern has succeeded in applying these Islamic values to unite in other school cultural activities in accordance with the vision, mission and objectives of the institution.   Abstrak Krisis nilai telah menimpa bangsa Indonesia pada semua bidang kehidupan  termasuk dunia pendidikan. Kondisi seperti ini menyebabkan pentingnya pendidikan nilai secara intensif di sekolah-sekolah. Tulisan ini bertujuan untuk mengetahui konsep Budaya Sekolah Islami (Busi dan pola pelaksanaannya di SMA Islam Sultan Agung 1 Semarang. Jenis penelitian ini adalah deskriptif kualitatif. Hasil penelitian menunjukkan bahwa Busi di SMA Islam Sultan Agung 1 Semarang meliputi budaya iqra, budaya shalat berjamaah, budaya thaharah, budaya pergaulan islami, dan budaya keteladanan.  Pola Pelaksanaan Busi dilaksanakan secara top down dengan tahapan sosialisasi, pembiasaan dan monitoring. Pola ini telah berhasil menerapkan nilai-nilai Islam tersebut menyatu dalam aktifitas budaya sekolah yang lain sesuai dengan visi, misi dan tujuan lembaga

  12. ANALISIS FAKTOR-FAKTOR YANG MEMPENGARUHI HASIL BELAJAR KELAS XI IPS DI SMA NEGERI 2 SEMARANG

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    Desi Setiani

    2014-11-01

    Full Text Available Penelitian ini bertujuan untuk mengetahui faktor-faktor dan faktor paling dominan yang mempengaruhi hasil belajar Ekonomi siswa kelas XI IPS di SMA Negeri 2 Semarang. Seluruh populasi yaitu kelas XI IPS di SMA Negeri 2 Semarang dijadikan responden sejumlah 85 siswa. Variabel dalam penelitian ini adalah faktor-faktor yang mempengaruhi hasil belajar Ekonomi siswa sejumlah 32 faktor. Metode pengumpulan data yang digunakan adalah metode observasi dan angket/kuesioner. Analisis data yang digunakan adalah analisis deskriptif persentase dan analisis faktor. Berdasarkan hasil pengujian analisis faktor terdapat 6 kelompok faktor yang terbentuk yaitu: Kondisi Psikologis, Lingkungan Belajar di Sekolah, Gangguan Belajar, Lingkungan Keluarga, Lingkungan Masyarakat dan Kondisi Fisiologis. Saran untuk penelitian ini hendaknya siswa memaksimalkan faktor-faktor yang berpotensi mempengaruhi peningkatan hasil belajar ekonomi siswa. This research aims to know factors and dominant factor which influenced economics learning outcomes grade XI social at SMA Negeri 2 Semarang. All students of population is being respondent which are student grade XI social are 85 students. Variabel of this research are factors who influenced student’s economic learning outcomes is 32 factors. Data accumulation methode are observation and questionnaire. Data analysis which used are presentation descriptive analysis and factor analysis. Based on result of testing factors analysis, there are 6 groups of factor that are: Psychology, School Environment, Learning Disturbance, Family Environment, Society Environment; and Physiology. The suggestion is should all students improve factors which influenced increasing economics learning outcomes

  13. Evaluation of Fatigue Life of CRM-Reinforced SMA and Its Relationship to Dynamic Stiffness

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    Nuha Salim Mashaan

    2014-01-01

    Full Text Available Fatigue cracking is an essential problem of asphalt concrete that contributes to pavement damage. Although stone matrix asphalt (SMA has significantly provided resistance to rutting failure, its resistance to fatigue failure is yet to be fully addressed. The aim of this study is to evaluate the effect of crumb rubber modifier (CRM on stiffness and fatigue properties of SMA mixtures at optimum binder content, using four different modification levels, namely, 6%, 8%, 10%, and 12% CRM by weight of the bitumen. The testing undertaken on the asphalt mix comprises the dynamic stiffness (indirect tensile test, dynamic creep (repeated load creep, and fatigue test (indirect tensile fatigue test at temperature of 25°C. The indirect tensile fatigue test was conducted at three different stress levels (200, 300, and 400 kPa. Experimental results indicate that CRM-reinforced SMA mixtures exhibit significantly higher fatigue life compared to the mixtures without CRM. Further, higher correlation coefficient was obtained between the fatigue life and resilient modulus as compared to permanent strain; thus resilient modulus might be a more reliable indicator in evaluating the fatigue life of asphalt mixture.

  14. Evaluation of fatigue life of CRM-reinforced SMA and its relationship to dynamic stiffness.

    Science.gov (United States)

    Mashaan, Nuha Salim; Karim, Mohamed Rehan; Abdel Aziz, Mahrez; Ibrahim, Mohd Rasdan; Katman, Herda Yati; Koting, Suhana

    2014-01-01

    Fatigue cracking is an essential problem of asphalt concrete that contributes to pavement damage. Although stone matrix asphalt (SMA) has significantly provided resistance to rutting failure, its resistance to fatigue failure is yet to be fully addressed. The aim of this study is to evaluate the effect of crumb rubber modifier (CRM) on stiffness and fatigue properties of SMA mixtures at optimum binder content, using four different modification levels, namely, 6%, 8%, 10%, and 12% CRM by weight of the bitumen. The testing undertaken on the asphalt mix comprises the dynamic stiffness (indirect tensile test), dynamic creep (repeated load creep), and fatigue test (indirect tensile fatigue test) at temperature of 25°C. The indirect tensile fatigue test was conducted at three different stress levels (200, 300, and 400 kPa). Experimental results indicate that CRM-reinforced SMA mixtures exhibit significantly higher fatigue life compared to the mixtures without CRM. Further, higher correlation coefficient was obtained between the fatigue life and resilient modulus as compared to permanent strain; thus resilient modulus might be a more reliable indicator in evaluating the fatigue life of asphalt mixture.

  15. PROFIL KESULITAN BELAJAR FISIKA POKOK BAHASAN KELISTRIKAN SISWA SMA DI KOTA SEMARANG

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    Ani Rusilowati

    2012-01-01

    Full Text Available Tujuan penelitian ini adalah menentukan profil kesulitan belajar Fisika, khususnya pokok bahasan Kelistrikan yang dialami oleh siswa SMA di kota Semarang. Sampel penelitian adalah siswa SMA kelas X di kota Semarang, diambil secara cluster, dari SMA negeri dan swasta peringkat I, II, dan III, sebanyak 214 siswa. Kesulitan belajar didiagnosis dengan lima pendekatan, yaitu tujuan pembelajaran, pengetahuan prasyarat, profil materi, miskonsepsi, dan pengetahuan terstruktur. Kesulitan belajar Kelistrikan antara lain disebabkan oleh rendahnya penguasaan konsep, lemahnya kemampuan matematis, dan kekurangmampuan mengkonversi satuan. Penyebab kesulitan belajar dalam pengetahuan terstruktur adalah rendahnya kemampuan: verbal, menggunakan skema, membuat strategi pemecahan masalah, dan membuat algoritma. Hasil penelitian menunjukkan bahwa kesulitan belajar Kelistrikan rata-rata terjadi pada sub pokok bahasan: Kuat Arus Listrik, Hukum Ohm, Hambatan Penghantar, Hukum Kirchof II, Energi & Daya Listrik, dan Transformator. Sebagian siswa masih mengalami miskonsepsi terhadap konsep Hukum Ohm dan Hambatan Penghantar. Bagi siswa  sekolah peringkat III mengalami kesulitan belajar di semua aspek dan materi Kelistrikan Kata kunci : profil, kesulitan belajar, kelistrikan

  16. Analysis of SMA Hybrid Composite Structures in MSC.Nastran and ABAQUS

    Science.gov (United States)

    Turner, Travis L.; Patel, Hemant D.

    2005-01-01

    A thermoelastic constitutive model for shape memory alloy (SMA) actuators and SMA hybrid composite (SMAHC) structures was recently implemented in the commercial finite element codes MSC.Nastran and ABAQUS. The model may be easily implemented in any code that has the capability for analysis of laminated composite structures with temperature dependent material properties. The model is also relatively easy to use and requires input of only fundamental engineering properties. A brief description of the model is presented, followed by discussion of implementation and usage in the commercial codes. Results are presented from static and dynamic analysis of SMAHC beams of two types; a beam clamped at each end and a cantilever beam. Nonlinear static (post-buckling) and random response analyses are demonstrated for the first specimen. Static deflection (shape) control is demonstrated for the cantilever beam. Approaches for modeling SMAHC material systems with embedded SMA in ribbon and small round wire product forms are demonstrated and compared. The results from the commercial codes are compared to those from a research code as validation of the commercial implementations; excellent correlation is achieved in all cases.

  17. FUS-SMN Protein Interactions Link the Motor Neuron Diseases ALS and SMA

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    Tomohiro Yamazaki

    2012-10-01

    Full Text Available Mutations in the RNA binding protein FUS cause amyotrophic lateral sclerosis (ALS, a fatal adult motor neuron disease. Decreased expression of SMN causes the fatal childhood motor neuron disorder spinal muscular atrophy (SMA. The SMN complex localizes in both the cytoplasm and nuclear Gems, and loss of Gems is a cellular hallmark of fibroblasts in patients with SMA. Here, we report that FUS associates with the SMN complex, mediated by U1 snRNP and by direct interactions between FUS and SMN. Functionally, we show that FUS is required for Gem formation in HeLa cells, and expression of FUS containing a severe ALS-causing mutation (R495X also results in Gem loss. Strikingly, a reduction in Gems is observed in ALS patient fibroblasts expressing either mutant FUS or TDP-43, another ALS-causing protein that interacts with FUS. The physical and functional interactions among SMN, FUS, TDP-43, and Gems indicate that ALS and SMA share a biochemical pathway, providing strong support for the view that these motor neuron diseases are related.

  18. Subcutaneous administration of TC007 reduces disease severity in an animal model of SMA

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    Chang Cheng-Wei

    2009-11-01

    Full Text Available Abstract Background Spinal Muscular Atrophy (SMA is the leading genetic cause of infantile death. It is caused by the loss of functional Survival Motor Neuron 1 (SMN1. There is a nearly identical copy gene, SMN2, but it is unable to rescue from disease due to an alternative splicing event that excises a necessary exon (exon 7 from the majority of SMN2-derived transcripts. While SMNΔ7 protein has severely reduced functionality, the exon 7 sequences may not be specifically required for all activities. Therefore, aminoglycoside antibiotics previously shown to suppress stop codon recognition and promote translation read-through have been examined to increase the length of the SMNΔ7 C-terminus. Results Here we demonstrate that subcutaneous-administration of a read-through inducing compound (TC007 to an intermediate SMA model (Smn-/-; SMN2+/+; SMNΔ7 had beneficial effects on muscle fiber size and gross motor function. Conclusion Delivery of the read-through inducing compound TC007 reduces the disease-associated phenotype in SMA mice, however, does not significantly extend survival.

  19. SMA-Based System for Environmental Sensors Released from an Unmanned Aerial Vehicle

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    Lorenzo Pellone

    2017-01-01

    Full Text Available In the work at hand, a shape memory alloy (SMA-based system is presented. The system, conceived for releasing environmental sensors from ground or small unmanned aerial vehicles, UAV (often named UAS, unmanned aerial system, is made of a door, integrated into the bottom of the fuselage, a device distributor, operated by a couple of antagonistic SMA springs, and a kinematic chain, to synchronize the deployment operation with the system movement. On the basis of the specifications (weight, available space, energy supply, sensors size, etc., the system design was addressed. After having identified the main system characteristics, a representative mock-up was manufactured, featuring the bottom part of the reference fuselage. Functionality tests were performed to prove the system capability to release the sensors; a detailed characterization was finally carried out, mainly finalized at correlating the kinematic chain displacement with the SMA spring temperature and the supplied electrical power. A comparison between theoretical predictions and experimental outcomes showed good agreement.

  20. Kajian Fisis Energi Terbarukan Panel Surya Melalui Eksperimen Sederhana untuk Siswa SMA

    Directory of Open Access Journals (Sweden)

    Sunaryo Sunaryo

    2015-12-01

    Full Text Available Abstract Has conducted research on the effects of light intensity on the output voltage, current, and power. Research conducted generate data in the form of quantitative and graphs that show a link between the intensity of light, the output voltage, current, and power. The data obtained were used as sources of learning in senior high school (SMA. The implication is capable of enhancing creativity, motivation and learning outcomes of Physics subject of high school students in future studies. Keywords: light intensity, current, voltage, solar panel Abstrak Telah dilakukan penelitian tentang pengaruh intensitas cahaya terhadap tegangan output, arus, dan daya listrik. Penelitian yang dilakukan menghasilkan data dalam bentuk kuantitatif dan grafik yang menunjukkan adanya kaitan antara intensitas cahaya, tegangan output, arus, dan daya listrik. Data yang diperoleh dijadikan sebagai sumber informasi dalam pembelajaran di Sekolah Menengah Atas (SMA. Implikasinya adalah mampu meningkatkan kreativitas, motivasi, dan hasil belajar Fisika siswa SMA pada penelitian selanjutnya. Kata-kata kunci: intensitas cahaya, arus, tegangan, panel surya

  1. Minimizing the Moisture Damage and Drain down of Iraqi SMA Mixtures Using Waste Additives

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    Ali Al-Hadidy

    2013-04-01

    Full Text Available This research deals with the viability of using polyester fiber (PF, crumb rubber tire (CRT and cellulose fiber (CF as stabilizing waste additives in producing Iraqi SMA mixtures that sustain drain down phenomenon and moisture damage sensitivity. Different ratios of these additives (0.1, 0.2, and 0.3% by weight of aggregate and filler were mixed with 40/50 paving asphalt by means of dry process. Unmodified and modified SMA mixtures were subjected to drain down, Marshall, static indirect tensile strength, tensile stiffness modulus, static compressive strength, tensile strength ratio and index of retained strength tests. A set of regression equations between these tests were established. In addition, an optimization table based on these tests, which can be used to select the type or amount of additive for any field applications has been determined and reported. The results indicated that the inclusion of these additives in SMA mixtures can satisfy the performance requirement of high temperature and much rain zone.

  2. A starfish robot based on soft and smart modular structure (SMS) actuated by SMA wires.

    Science.gov (United States)

    Jin, Hu; Dong, Erbao; Alici, Gursel; Mao, Shixin; Min, Xu; Liu, Chunshan; Low, K H; Yang, Jie

    2016-09-09

    This paper describes the design, fabrication and locomotion of a starfish robot whose locomotion principle is derived from a starfish. The starfish robot has a number of tentacles or arms extending from its central body in the form of a disk, like the topology of a real starfish. The arm, which is a soft and composite structure (which we call the smart modular structure (SMS)) generating a planar reciprocal motion with a high speed of response upon the actuation provided by the shape memory alloy (SMA) wires, is fabricated from soft and smart materials. Based on the variation in the resistance of the SMA wires during their heating, an adaptive regulation (AR) heating strategy is proposed to (i) avoid overheating of the SMA wires, (ii) provide bending range control and (iii) achieve a high speed of response favorable to successfully propelling the starfish robot. Using a finite-segment method, a thermal dynamic model of the SMS is established to describe its thermal behavior under the AR and a constant heating strategy. A starfish robot with five SMS tentacles was tested with different control parameters to optimize its locomotion speed. As demonstrated in the accompanying video file, the robot successfully propelled in semi-submerged and underwater environments show its locomotion ability in the multi-media, like a real starfish. The propulsion speed of the starfish robot is at least an order of magnitude higher than that of those reported in the literature-thanks to the SMS controlled with the AR strategy.

  3. Implementasi Sistem Informasi Akademik Menggunakan Aplikasi Jibas pada SMA Negeri 9 Padang

    Directory of Open Access Journals (Sweden)

    Ricky Akbar

    2015-10-01

    Full Text Available SMA Negeri 9 Padang is one of the institutions engaged in the field of education, which requires the design of software to manage and run all school activities, one of which is the Academic Information System (SIA. SIA currently in SMA 9 Padang yet well integrated, so it still has many shortcomings in meeting the needs of the school or institution, in particular to deal with academic problems. Therefore, it needs to be implemented Academic Information System that can overcome the various shortcomings earlier. Implementation of this application starts with a preliminary study. Activities, the introduction of the school as a whole with interviews and observations, identify business processes academically at school is running and then make the proposed system as terkomputerisasinya, which is described by using the tools of Business Process Model Notation (BPMN, as well as the depiction of a working model of the system to be applied using use case diagram. The next stage is to study the literature of various books and journals to find the theoretical basis and related research. Then selecting software for SIA School, after the configuration and customization of the software modules, and the latter carry out the implementation and testing. These results indicate that the software SIA Schools that have been selected and applied that JIBAS applications, which can solve the problems on SMA Negeri 9 Padang

  4. Studying Star and Planet Formation with the Submillimeter Probe of the Evolution of Cosmic Structure

    Science.gov (United States)

    Rinehart, Stephen A.

    2005-01-01

    The Submillimeter Probe of the Evolution of Cosmic Structure (SPECS) is a far- infrared/submillimeter (40-640 micrometers) spaceborne interferometry concept, studied through the NASA Vision Missions program. SPECS is envisioned as a 1-km baseline Michelson interferometer with two 4- meter collecting mirrors. To maximize science return, SPECS will have three operational modes: a photometric imaging mode, an intermediate spectral resolution mode (R approximately equal to 1000-3000), and a high spectral resolution mode (R approximately equal to 3 x 10(exp 5)). The first two of these modes will provide information on all sources within a 1 arcminute field-of-view (FOV), while the the third will include sources in a small (approximately equal to 5 arcsec) FOV. With this design, SPECS will have angular resolution comparable to the Hubble Space Telescope (50 mas) and sensitivity more than two orders of magnitude better than Spitzer (5sigma in 10ks of approximately equal to 3 x 10(exp 7) Jy Hz). We present here some of the results of the recently-completed Vision Mission Study for SPECS, and discuss the application of this mission to future studies of star and planet formation.

  5. Extending the LHC reach for new physics with sub-millimeter displaced vertices

    Science.gov (United States)

    Ito, Hayato; Jinnouchi, Osamu; Moroi, Takeo; Nagata, Natsumi; Otono, Hidetoshi

    2017-08-01

    Particles with a sub-millimeter decay length appear in many models of physics beyond the Standard Model. However, their longevity has been often ignored in their LHC searches and they have been regarded as promptly-decaying particles. In this letter, we show that, by requiring displaced vertices on top of the event selection criteria used in the ordinary search strategies for promptly-decaying particles, we can considerably extend the LHC reach for particles with a decay length of ≳ 100 μm. We discuss a way of reconstructing sub-millimeter displaced vertices by exploiting the same technique used for the primary vertex reconstruction on the assumption that the metastable particles are always pair-produced and their decay products contain high-pT jets. We show that, by applying a cut based on displaced vertices on top of standard kinematical cuts for the search of new particles, the LHC reach can be significantly extended if the decay length is ≳ 100 μm. In addition, we may measure the lifetime of the target particle through the reconstruction of displaced vertices, which plays an important role in understanding the new physics behind the metastable particles.

  6. The status of MUSIC: the multiwavelength sub-millimeter inductance camera

    Science.gov (United States)

    Sayers, Jack; Bockstiegel, Clint; Brugger, Spencer; Czakon, Nicole G.; Day, Peter K.; Downes, Thomas P.; Duan, Ran P.; Gao, Jiansong; Gill, Amandeep K.; Glenn, Jason; Golwala, Sunil R.; Hollister, Matthew I.; Lam, Albert; LeDuc, Henry G.; Maloney, Philip R.; Mazin, Benjamin A.; McHugh, Sean G.; Miller, David A.; Mroczkowski, Anthony K.; Noroozian, Omid; Nguyen, Hien Trong; Schlaerth, James A.; Siegel, Seth R.; Vayonakis, Anastasios; Wilson, Philip R.; Zmuidzinas, Jonas

    2014-08-01

    The Multiwavelength Sub/millimeter Inductance Camera (MUSIC) is a four-band photometric imaging camera operating from the Caltech Submillimeter Observatory (CSO). MUSIC is designed to utilize 2304 microwave kinetic inductance detectors (MKIDs), with 576 MKIDs for each observing band centered on 150, 230, 290, and 350 GHz. MUSIC's field of view (FOV) is 14' square, and the point-spread functions (PSFs) in the four observing bands have 45'', 31'', 25'', and 22'' full-widths at half maximum (FWHM). The camera was installed in April 2012 with 25% of its nominal detector count in each band, and has subsequently completed three short sets of engineering observations and one longer duration set of early science observations. Recent results from on-sky characterization of the instrument during these observing runs are presented, including achieved map- based sensitivities from deep integrations, along with results from lab-based measurements made during the same period. In addition, recent upgrades to MUSIC, which are expected to significantly improve the sensitivity of the camera, are described.

  7. Stratospheric isotopic water profiles from a single submillimeter limb scan by TELIS

    Directory of Open Access Journals (Sweden)

    A. de Lange

    2009-08-01

    Full Text Available Around 490 GHz relatively strong HDO and H218O emission lines can be found in the submillimeter thermal-emission spectrum of the Earth's atmosphere, along with lines of the principal isotopologue of water vapour. These can be used for remote sensing of the rare/principal isotope ratio in the stratosphere. A sensitivity study has been performed for retrieval simulations of water isotopologues from balloon-borne measurements by the limb sounder TELIS (TErahertz and submillimeter LImb Sounder. The study demonstrates the capability of TELIS to determine, from a single limb scan, the profiles for H218O and HDO between 20 km and 37 km with a retrieval error of ≈3 and a spatial resolution of 1.5 km, as determined by the width of the averaging kernel. In addition HDO can be retrieved in the range of 10–20 km, albeit with a strongly deteriorated retrieval error. Expected uncertainties in instrumental parameters have only limited impact on the retrieval results.

  8. A Multiwavelength Study of the Intracluster Medium and the Characterization of the Multiwavelength Sub/millimeter Inductance Camera

    Science.gov (United States)

    Siegel, Seth Robert

    The first part of this thesis combines Bolocam observations of the thermal Sunyaev-Zel'dovich (SZ) effect at 140 GHz with X-ray observations from Chandra, strong lensing data from the Hubble Space Telescope (HST), and weak lensing data from HST and Subaru to constrain parametric models for the distribution of dark and baryonic matter in a sample of six massive, dynamically relaxed galaxy clusters. For five of the six clusters, the full multiwavelength dataset is well described by a relatively simple model that assumes spherical symmetry, hydrostatic equilibrium, and entirely thermal pressure support. The multiwavelength analysis yields considerably better constraints on the total mass and concentration compared to analysis of any one dataset individually. The subsample of five galaxy clusters is used to place an upper limit on the fraction of pressure support in the intracluster medium (ICM) due to nonthermal processes, such as turbulent and bulk flow of the gas. We constrain the nonthermal pressure fraction at r500c to be less than 0.11 at 95% confidence, where r500c refers to radius at which the average enclosed density is 500 times the critical density of the Universe. This is in tension with state-of-the-art hydrodynamical simulations, which predict a nonthermal pressure fraction of approximately 0.25 at r500c for the clusters in this sample. The second part of this thesis focuses on the characterization of the Multiwavelength Sub/millimeter Inductance Camera (MUSIC), a photometric imaging camera that was commissioned at the Caltech Submillimeter Observatory (CSO) in 2012. MUSIC is designed to have a 14 arcminute, diffraction-limited field of view populated with 576 spatial pixels that are simultaneously sensitive to four bands at 150, 220, 290, and 350 GHz. It is well-suited for studies of dusty star forming galaxies, galaxy clusters via the SZ Effect, and galactic star formation. MUSIC employs a number of novel detector technologies: broadband phased-arrays

  9. Guaranteed behaviour of shape memory alloys: after quench and long time effects in CuZnAl SMA

    Energy Technology Data Exchange (ETDEWEB)

    Isalgue, A.; Torra, V. [CIRG, Barcelona (Spain). Dept. Fisica Aplicada UPC

    2001-11-01

    The use of shape memory alloys (SMA) in critical ''high tech'' applications such as robotics and in continuous actuators needs an increased reliability and a guaranteed behaviour lasting several years. High resolution measurements enabled to quantify the time effects of aging near room temperature on the properties of CuZnAl SMA and to modelize the macroscopic behaviour. Some structural measurements showed small changes on the material structure. (orig.)

  10. Faktor-faktor yang Mempengaruhi Motivasi Belajar Siswa Jurusan IPS Mata Pelajaran Ekonomi Kelas XI SMA N 6 Sijunjung

    OpenAIRE

    Areva, Desi; Akhirmen, Akhirmen; Wahyuni, Tri

    2013-01-01

    AbstrackThe purpose of this study is (1) Determine the influence of students perceptions about the variety of teaching styles to students learning motivation of economic subjects majoring in social studies class XI SMA 6 Sijunjung. (2) Determine the influence of instructional media on the students motivation of economic subjects majoring in social studies class XI SMA 6 Sijunjung. (3) Determine the influence of discipline on students motivation to learn social studies department of economic s...

  11. Dissociable roles of preSMA in motor sequence chunking and hand switching-a TMS study.

    Science.gov (United States)

    Muessgens, Diana; Thirugnanasambandam, Nivethida; Shitara, Hitoshi; Popa, Traian; Hallett, Mark

    2016-12-01

    Motor chunking, the grouping of individual movements into larger units, is crucial for sequential motor performance. The presupplementary motor area (preSMA) is involved in chunking and other related processes such as task switching, response selection, and response inhibition that are crucial for organizing sequential movements. However, previous studies have not systematically differentiated the role of preSMA in motor chunking and hand switching, thus leaving its relative contribution to each of these processes unclear. The aim of this study is to demonstrate the differential role of preSMA in motor chunking and hand switching. We designed motor sequences in which different kinds of hand switches (switching toward the right or left hand or continuing with the right hand) were counterbalanced across between- and within-chunk sequence points. Eighteen healthy, right-handed participants practiced four short subsequences (chunks) of key presses. In a subsequent task, these chunks had to be concatenated into one long sequence. We applied double-pulse transcranial magnetic stimulation (TMS) over left preSMA or left M1 areas at sequence initiation, between chunks, or within chunks. TMS over the left preSMA significantly slowed the next response when stimulation was given between chunks, but only if a hand switch toward the contralateral (right) hand was required. PreSMA stimulation within chunks did not interfere with responses. TMS over the left M1 area delayed responses with the contralateral hand, both within and between chunks. Both preSMA and M1 stimulation decreased response times at sequence initiation. These results suggest that left preSMA is not necessary for chunking per se, but rather for organizing complex movements that require chunking and hand switching simultaneously.

  12. Dissociable roles of preSMA in motor sequence chunking and hand switching—a TMS study

    Science.gov (United States)

    Thirugnanasambandam, Nivethida; Shitara, Hitoshi; Popa, Traian; Hallett, Mark

    2016-01-01

    Motor chunking, the grouping of individual movements into larger units, is crucial for sequential motor performance. The presupplementary motor area (preSMA) is involved in chunking and other related processes such as task switching, response selection, and response inhibition that are crucial for organizing sequential movements. However, previous studies have not systematically differentiated the role of preSMA in motor chunking and hand switching, thus leaving its relative contribution to each of these processes unclear. The aim of this study is to demonstrate the differential role of preSMA in motor chunking and hand switching. We designed motor sequences in which different kinds of hand switches (switching toward the right or left hand or continuing with the right hand) were counterbalanced across between- and within-chunk sequence points. Eighteen healthy, right-handed participants practiced four short subsequences (chunks) of key presses. In a subsequent task, these chunks had to be concatenated into one long sequence. We applied double-pulse transcranial magnetic stimulation (TMS) over left preSMA or left M1 areas at sequence initiation, between chunks, or within chunks. TMS over the left preSMA significantly slowed the next response when stimulation was given between chunks, but only if a hand switch toward the contralateral (right) hand was required. PreSMA stimulation within chunks did not interfere with responses. TMS over the left M1 area delayed responses with the contralateral hand, both within and between chunks. Both preSMA and M1 stimulation decreased response times at sequence initiation. These results suggest that left preSMA is not necessary for chunking per se, but rather for organizing complex movements that require chunking and hand switching simultaneously. PMID:27655967

  13. SMA spring-based artificial muscle actuated by hot and cool water using faucet-like valve

    Science.gov (United States)

    Park, Cheol Hoon; Son, Young Su

    2017-04-01

    An artificial muscle for a human arm-like manipulator with high strain and high power density are under development, and an SMA(Shape memory alloy) spring is a good actuator for this application. In this study, an artificial muscle composed of a silicon tube and a bundle of SMA(Shape memory alloy) springs is evaluated. A bundle of SMA springs consists of five SMA springs which are fabricated by using SMA wires with a diameter of 0.5 mm, and hot and cool water actuates it by heating and cooling SMA springs. A faucet-like valve was also developed to mix hot water and cool water and control the water temperature. The mass of silicon tube and a bundle of SMA springs is only 3.3 g and 2.25 g, respectively, and the total mass of artificial muscle is 5.55 g. It showed good actuating performance for a load with a mass of 2.3 kg and the power density was more than 800 W/kg for continuous valve switching with a cycle of 0.6 s. The faucet-like valve can switch a water output from hot water to cold water within 0.3s, and the artificial muscle is actuated well in response to the valve position and speed. It is also presented that the temperature of the mixed water can be controlled depending on the valve position, and the displacement of the artificial muscle can be controlled well by the mixed water. Based on these results, SMA spring-based artificial muscle actuated by hot and cool water could be applicable to the human arm-like robot manipulators.

  14. SCUBA-2 arrays to system interfaces

    Energy Technology Data Exchange (ETDEWEB)

    Duncan, W. E-mail: william.duncan@roe.ac.uk; Audley, D.; Holland, W.; Atkinson, D.; Baillie, T.; Cliffe, M.; Ellis, M.; Gao, X.; Gostick, D.; Hodson, T.; Kelly, D.; MacIntosh, M.; McGregor, H.; Peacocke, T.; Smith, I.; Robson, I.; Walton, A.; Parkes, W.; Dunare, C.; Smith, S.; Terry, J.; Stevenson, T.; Gundlach, A.; Ruthven, A.; Ade, P.; Tucker, C.; Gannaway, F.; Walker, I.; Sudiwala, R.; Woodcraft, A.; Griffin, M.; Bintley, D.; Schulte, E.; Fich, M.; Kycia, J.; Halpern, M.; Molnar, J.; Burger, B.; Naylor, D.; Bastien, P.; Mitchell, G.; Irwin, K.; Hilton, G.; Ullom, J.; Reintsema, C.; Vale, L.; Ferreira, L.; Doriese, W

    2004-03-11

    Submillimeter common user bolometer array (SCUBA)-2 is a wide field sub-mm bolometer camera designed to replace the existing SCUBA instrument on the JCMT in Hawaii. It will be many hundreds of times faster in large area mapping than SCUBA and will also go deeper in a single frame. It will enable the many discoveries of SCUBA to be followed up with deep systematic surveys and help act as a pathfinder for the ALMA interferometer. The key technologies for making the arrays have been demonstrated and will be put together to fabricate the first prototype later this year (2003). The wide field nature of the SCUBA-2 bolometer camera, combined with the diffraction limit at sub-mm wavelengths, leads to physically large focal planes where the issues of stray light control, magnetic shielding, and electrical, thermal and mechanical connection must be carefully addressed in order to realise a successful instrument. We describe the solutions we have adopted for these problem areas.

  15. Experimental techniques for characterizing the thermo-electro-mechanical shakedown response of SMA wires and tubes

    Science.gov (United States)

    Churchill, Christopher B.

    Shape Memory Alloys (SMAs) are a unique and valuable group of active materials. NiTi, the most popular SMA, has a power density orders of magnitude greater than any other known material, making it valuable in the medical and transportation industries where weight and space are at a premium. In the nearly half-century since its discovery, the adoption of NiTi has been slowed primarily by the engineering difficulties associated with its use: strong thermal coupling, material level instabilities, and rapid shakedown of material properties during cycling. Material properties change drastically with minute changes in alloy composition, so it is common to require a variety of experiments to fully characterize a new SMA material, all of which must be performed and interpreted with specialized techniques. This thesis collects many of these techniques into a series of characterization experiments, documenting several new phenomena in the process. First, three different alloys of NiTi wire are characterized through differential scanning calorimetry, isothermal tension, and constant load thermal cycling experiments. New techniques are presented for ER measurement and temperature control of SMA wires and temperature measurement of SMA tubes. It is shown that the shakedown of material properties with thermal cycling is not only dependent on the applied load and number of cycles, but has a large association with the direction of phase transformation. Several of these techniques are then applied to a systematic characterization of NiTi tubes in tension, compression, and bending. Particular attention is given to the nucleation and propagation of transformation fronts in tensile specimens. Compression experiments show dramatic asymmetry in the uniaxial response, with compression characterized by a lower transformation strain, higher transformation stress, and uniform transformations (no fronts). A very simple SMA actuator model is introduced. After identifying the relevant non

  16. MEDIA FOTO UNTUK MENINGKATKAN KETERAMPILAN MENULIS DESKRIPSI SISWA SMA NEGERI 2 KEBUMEN

    Directory of Open Access Journals (Sweden)

    Rina Tri Indrianingrum

    2015-05-01

    Full Text Available Penelitian ini bertujuan untuk menjelaskan meningkatnya keterampilan menulis deskripsi berbahasa Jawa siswa kelas X SMA N 2 Kebumen dengan menggunakan pendekatan proses dan media foto. Penelitian ini merupakan penelitian tindakan kelas atau classroom action research. Desain yang digunakan dalam penelitian ini adalah desain penelitian tindakan Kemmis dan Taggart. Penelitian ini dilaksanakan dua siklus. Subjek penelitian ini adalah siswa kelas X2 SMA Negeri 2 Kebumen tahun pelajaran 2011/2012 yang berjumlah 32 siswa. Pengumpulan data dilakukan dengan menggunakan observasi, catatan lapangan dan tes. Validitas yang digunakan adalah validitas demo-krasi, validitas proses dan validitas dialogis. Teknik yang digunakan untuk menganalisis data dalam penelitian tindakan ini adalah deskriptif. Hasil penelitian menunjukkan (1 siswa dapat menemukan ide lebih cepat, (2 siswa dapat membuat kerangka karangan, (3 siswa dapat mengembangkan kerang-ka karangan, (4 siswa dapat berpikir sistematis, (5 siswa semakin antusiasnya dalam mengikuti pembelajaran menulis karangan, (6 siswa paham melakukan proses mengarang. _________________________________________________________________________________________________________________________________________________________________________________________________________________________________________________________________________________ PHOTOGRAPH MEDIA TO IMPROVE THE DESCRIPTION WRITING SKILL OF THE STUDENTS AT SMA NEGERI 2 KEBUMEN   Abstract This research is aimed to describe and to explain the improvement in the description writing skill of the tenth grade students at SMA N 2 Kebumen by using  approach process and photography media. This research is classroom action research or classroom action research. The design used in this research was action research design by Kemmis and Taggart. The subject of the research was X2 class students at SMA Negeri 2 Kebumen in the academic year of 2011/2012, consisted of 32

  17. S&MA Internship to Support Orion and the European Service Module

    Science.gov (United States)

    Hutcheson, Connor

    2016-01-01

    As a University Space Research Association (USRA) intern for NASA Johnson Space Center (JSC) during the summer 2016 work term, I worked on three main projects for the Space Exploration Division (NC) of the Safety and Mission Assurance (S&MA) Directorate. I worked on all three projects concurrently. One of the projects involved facilitating the status and closure of technical actions that were created during European Service Module (ESM) safety reviews by the MPCV Safety & Engineering Review Panel (MSERP). The two main duties included accurately collecting and summarizing qualitative data, and communicating that information to the European Space Agency (ESA) and Airbus (ESA's prime contractor) in a clear, succinct and precise manner. This project also required that I create a report on the challenges and opportunities of international S&MA. With its heavy emphasis on soft skills, this project taught me how to communicate better, by showing me how to present and share information in an easy-to-read and understandable format, and by showing me how to cooperate with and culturally respect international partners on a technical project. The second project involved working with the Orion Thermal Protection System (TPS) Process Failure Modes and Effects Analysis (PFMEA) Working Group to create the first full version of the Orion TPS PFMEA. The Orion TPS PFMEA Working Group met twice a week to analyze the Avcoat block installation process for failure modes, the failure modes effects, and how such failure modes could be controlled. I was in charge of implementing changes that were discussed in meeting, but were not implemented real time. Another major task included creating a significant portion of the content alongside another team member outside the two weekly meetings. This project caused me to become knowledgeable about TPS, heatshields, space-rated manufacturing, and non-destructive evaluation (NDE). The project also helped me to become better at working with a small

  18. Phased arrays '85

    Science.gov (United States)

    Stiglitz, M. R.

    1985-11-01

    The conference Phased Arrays '85 was held in Bedford, MA, on October 15-18, 1985. It is pointed out that the 15 years between the 1970 and 1985 conferences dedicated to phased array antennas have seen many technological advances. Attention is given to the principle of operation, monolithic phased arrays, active arrays of monopole elements, scan compensated active element patterns, microstrip arrays, time delay technologies for phased array systems, ferrite materials for mm-wave phase shifters, phase-only optimization of phased array excitation by B-quadratic programming, a nearly frequency-independent sidelobe suppression technique for phased arrays, and active impedance effects in low sidelobe and ultrawideband phased arrays.

  19. The JCMT Transient Survey: Detection of Submillimeter Variability in a Class I Protostar EC 53 in Serpens Main

    Science.gov (United States)

    Yoo, Hyunju; Lee, Jeong-Eun; Mairs, Steve; Johnstone, Doug; Herczeg, Gregory J.; Kang, Sung-ju; Kang, Miju; Cho, Jungyeon; The JCMT Transient Team

    2017-11-01

    During the protostellar phase of stellar evolution, accretion onto the star is expected to be variable, but this suspected variability has been difficult to detect because protostars are deeply embedded. In this paper, we describe a submillimeter luminosity burst of the Class I protostar EC 53 in Serpens Main, the first variable found during our dedicated JCMT/SCUBA-2 monitoring program of eight nearby star-forming regions. EC 53 remained quiescent for the first six months of our survey, from 2016 February to August. The submillimeter emission began to brighten in 2016 September, reached a peak brightness of 1.5 times the faint state, and has been decaying slowly since 2017 February. The change in submillimeter brightness is interpreted as dust heating in the envelope, generated by a luminosity increase of the protostar of a factor of ≥4. The 850 μm light curve resembles the historical K-band light curve, which varies by a factor of ˜6 with a 543 period and is interpreted as accretion variability excited by interactions between the accretion disk and a close binary system. The predictable detections of accretion variability observed at both near-infrared and submillimeter wavelengths make the system a unique test-bed, enabling us to capture the moment of the accretion burst and to study the consequences of the outburst on the protostellar disk and envelope.

  20. Observing ice clouds in the submillimeter spectral range: the CloudIce mission proposal for ESA's Earth Explorer 8

    Directory of Open Access Journals (Sweden)

    S. A. Buehler

    2012-07-01

    Full Text Available Passive submillimeter-wave sensors are a way to obtain urgently needed global data on ice clouds, particularly on the so far poorly characterized "essential climate variable" ice water path (IWP and on ice particle size. CloudIce was a mission proposal to the European Space Agency ESA in response to the call for Earth Explorer 8 (EE8, which ran in 2009/2010. It proposed a passive submillimeter-wave sensor with channels ranging from 183 GHz to 664 GHz. The article describes the CloudIce mission proposal, with particular emphasis on describing the algorithms for the data-analysis of submillimeter-wave cloud ice data (retrieval algorithms and demonstrating their maturity. It is shown that we have a robust understanding of the radiative properties of cloud ice in the millimeter/submillimeter spectral range, and that we have a proven toolbox of retrieval algorithms to work with these data. Although the mission was not selected for EE8, the concept will be useful as a reference for other future mission proposals.

  1. TU-F-CAMPUS-T-02: Vernier Picket Fence Test: A Non-Imaging Method to Localize the Radiation Isocenter with Submillimeter Accuracy

    Energy Technology Data Exchange (ETDEWEB)

    Wong, J; Gallagher, K [Oregon Health & Science University, Portland, OR (United States); Oregon State University, Corvallis, OR (United States); Zhang, J [Oregon Health & Science University, Portland, OR (United States)

    2015-06-15

    Purpose: The purpose of this study is to propose a new non-imaging method to localize the radiation isocenter with submillimeter accuracy. Methods: The Vernier picket fence (VPF) is a multileaf collimator (MLC) picket fence sequence in which the fence spacing is 1/N smaller than the detector spacing of the QA phantom, where N is the magnification factor, typically set to 10 or 20. Similar to reading a Vernier caliper, the user can easily achieve the resolution of 1/N of the detector spacing by visually inspecting the maximum signal. To achieve higher accuracy, a Gaussian model was used to interpolate the peak position, which can fall between adjacent detectors. In two separate tests, precise MLC offsets and imprecise couch offsets were applied to a 2D detector array (MapCheck, Sun Nuclear Corp., Melbourne, Florida) to introduce setup errors. Two vertical VPF fields were delivered with collimator angles at 0° and 90° to detect the lateral and longitudinal setup errors, respectively. For a rotational QA phantom, an additional lateral VPF field is needed to detect the vertical setup error for three-dimensional capabilities. Results: With N set to 20 and a detector spacing of 5 mm for MapCheck, the resolution of the VPF’s visual analysis is 0.25 mm. With the Gaussian interpretation, the VPF can achieve an accuracy of 0.02 mm, as shown by the MLC offset test. The couch offset test measured the couch hysteresis and demonstrated that the setup error detected by the VPF differed from the ExacTrac™ (Brainlab AG, Feldkirchen, Germany) optical tracking by 0.055 mm in the lateral direction and 0.041 mm in the longitudinal direction on average. The VPF was also shown to be feasible in the vertical direction as well. Conclusion: This study verified the VPF as a non-imaging method to localize the radiation isocenter with submillimeter accuracy. Funding is in part by the Portland Chapter of the Achievement Rewards for College Scientists. The content is solely the

  2. Candidate proteins, metabolites and transcripts in the Biomarkers for Spinal Muscular Atrophy (BforSMA clinical study.

    Directory of Open Access Journals (Sweden)

    Richard S Finkel

    Full Text Available Spinal Muscular Atrophy (SMA is a neurodegenerative motor neuron disorder resulting from a homozygous mutation of the survival of motor neuron 1 (SMN1 gene. The gene product, SMN protein, functions in RNA biosynthesis in all tissues. In humans, a nearly identical gene, SMN2, rescues an otherwise lethal phenotype by producing a small amount of full-length SMN protein. SMN2 copy number inversely correlates with disease severity. Identifying other novel biomarkers could inform clinical trial design and identify novel therapeutic targets.To identify novel candidate biomarkers associated with disease severity in SMA using unbiased proteomic, metabolomic and transcriptomic approaches.A cross-sectional single evaluation was performed in 108 children with genetically confirmed SMA, aged 2-12 years, manifesting a broad range of disease severity and selected to distinguish factors associated with SMA type and present functional ability independent of age. Blood and urine specimens from these and 22 age-matched healthy controls were interrogated using proteomic, metabolomic and transcriptomic discovery platforms. Analyte associations were evaluated against a primary measure of disease severity, the Modified Hammersmith Functional Motor Scale (MHFMS and to a number of secondary clinical measures.A total of 200 candidate biomarkers correlate with MHFMS scores: 97 plasma proteins, 59 plasma metabolites (9 amino acids, 10 free fatty acids, 12 lipids and 28 GC/MS metabolites and 44 urine metabolites. No transcripts correlated with MHFMS.In this cross-sectional study, "BforSMA" (Biomarkers for SMA, candidate protein and metabolite markers were identified. No transcript biomarker candidates were identified. Additional mining of this rich dataset may yield important insights into relevant SMA-related pathophysiology and biological network associations. Additional prospective studies are needed to confirm these findings, demonstrate sensitivity to change with

  3. A Compact 600 GHz Electronically Tunable Vector Measurement System for Submillimeter Wave Imaging

    Science.gov (United States)

    Dengler, Robert; Maiwald, Frank; Siegel, Peter H.

    2006-01-01

    The design of a complete vector measurement system being tested over 560-635 GHz is presented. The topics include: 1) Current State-of-the-Art in Vector Measurements; 2) Submillimeter Active Imaging Requirements; 3) 600 GHz Vector Measurement System; 4) 450 MHz IF Signal; 5) 450 MHz IF signal @ 1 kHz Res. BW; 6) 450 MHz IF Signal Mixed with Shifted 450 MHz Reference Signal; 7) Reference Signal Offset Generator; 8) Cavity Bandpass Filter; 9) Miniature Multistage Helical Filter; 10) X36 450 MHz Multiplier; 11) 600 GHz Test Setup; 12) 600 GHz Transmit Module; 13) 600 GHz Receive Module; 14) Performance Tests: Amplitude Stability & Dynamic Range; 15) Performance Tests: Phase Stability; 16) Stability at Imaging Bandwidths; 17) Phase Measurement Verification; and 18) The Next Step: Imaging.

  4. Estimation of physiological sub-millimeter displacement with CW Doppler radar.

    Science.gov (United States)

    Jia Xu; Xiaomeng Gao; Padasdao, Bryson E; Boric-Lubecke, Olga

    2015-01-01

    Doppler radar physiological sensing has been studied for non-contact detection of vital signs including respiratory and heartbeat rates. This paper presents the first micrometer resolution Wi-Fi band Doppler radar for sub-millimeter physiological displacement measurement. A continuous-wave Doppler radar working at 2.4GHz is used for the measurement. It is intended for estimating small displacements on the body surface resulting from physiological activity. A mechanical mover was used as target, and programmed to conduct sinusoidal motions to simulate pulse motions. Measured displacements were compared with a reference system, which indicates a superior performance in accuracy for having absolute errors less than 10μm, and relative errors below 4%. It indicates the feasibility of highly accurate non-contact monitoring of physiological movements using Doppler radar.

  5. Metal-mesh achromatic half-wave plate for use at submillimeter wavelengths.

    Science.gov (United States)

    Pisano, Giampaolo; Savini, Giorgio; Ade, Peter A R; Haynes, Vic

    2008-11-20

    A metal-mesh achromatic half-wave plate (HWP) has been designed, manufactured, and tested for potential use in millimeter and submillimeter astronomical instruments. The prototype device presented here is based on a 12-grid Shatrow [IEEE Trans. Antennas Propag. 43, 109 (1995)] recipe to operate over the frequency range of 120-180 GHz. Transmission line modeling and finite-element analysis [Ansoft HFSS website: http://www.ansoft.com/hfss/] were used to optimize the design geometrical parameters in terms of the device transmission, reflection, absorption, phase-shift, and cross-polarization as a function of frequency. The resulting prototype device was constructed and characterized using incoherent radiation from a polarizing Fourier transform spectrometer to explore its frequency and polarization behavior. These measurements are shown to be in excellent agreement with the models. Lists of the achieved HWP performance characteristics are reported.

  6. EPR and AFMR of Bi2CuO4 in Submillimeter Wave Region

    Science.gov (United States)

    Ohta, Hitoshi; Yoshida, Kazuhiro; Matsuya, Takashi; Nanba, Takao; Motokawa, Mitsuhiro; Yamada, Kazuyoshi; Endoh, Yasuo; Hosoya, Shoichi

    1992-08-01

    Paramagnetic and antiferromagnetic resonance have been observed in single crystals of Bi2CuO4 in submillimeter wave region using pulsed magnetic fields at temperatures from 4.2 K to 265 K. At the paramagnetic state, g-values have been determined to be g//{=}2.26± 0.01 and g\\bot{=}2.04± 0.01. The angular independent line-widths are 0.37± 0.03 T which is quantitatively explained by the dipole interaction and anisotropic exchange interaction. An antiferromagnetic resonance mode of planer type antiferromagnet has been observed below the Néel temperature and explained by the conventional antiferromagnetic theory.

  7. Submillimeter ionoacoustic range determination for protons in water at a clinical synchrocyclotron

    Science.gov (United States)

    Lehrack, Sebastian; Assmann, Walter; Bertrand, Damien; Henrotin, Sebastien; Herault, Joel; Heymans, Vincent; Vander Stappen, Francois; Thirolf, Peter G.; Vidal, Marie; Van de Walle, Jarno; Parodi, Katia

    2017-09-01

    Proton ranges in water between 145 MeV to 227 MeV initial energy have been measured at a clinical superconducting synchrocyclotron using the acoustic signal induced by the ion dose deposition (ionoacoustic effect). Detection of ultrasound waves was performed by a very sensitive hydrophone and signals were stored in a digital oscilloscope triggered by secondary prompt gammas. The ionoacoustic range measurements were compared to existing range data from a calibrated range detector setup on-site and agreement of better than 1 mm was found at a Bragg peak dose of about 10 Gy for 220 MeV initial proton energy, compatible with the experimental errors. Ionoacoustics has thus the potential to measure the Bragg peak position with submillimeter accuracy during proton therapy, possibly correlated with ultrasound tissue imaging.

  8. A low-cost fabrication method for sub-millimeter wave GaAs Schottky diode

    Science.gov (United States)

    Jenabi, Sarvenaz; Deslandes, Dominic; Boone, Francois; Charlebois, Serge A.

    2017-10-01

    In this paper, a submillimeter-wave Schottky diode is designed and simulated. Effect of Schottky layer thickness on cut-off frequency is studied. A novel microfabrication process is proposed and implemented. The presented microfabrication process avoids electron-beam (e-beam) lithography which reduces the cost. Also, this process provides more flexibility in selection of design parameters and allows significant reduction in the device parasitic capacitance. A key feature of the process is that the Schottky contact, the air-bridges, and the transmission lines, are fabricated in a single lift-off step. This process relies on a planarization method that is suitable for trenches of 1-10 μm deep and is tolerant to end-point variations. The fabricated diode is measured and results are compared with simulations. A very good agreement between simulation and measurement results are observed.

  9. Pengembangan Set Praktikum Fluida Dinamis untuk Sekolah Menengah Atas (SMA Kelas XI

    Directory of Open Access Journals (Sweden)

    Sifa Alfiyah

    2016-12-01

    Full Text Available Abstract This research aims to develop and produce a practicum set of dynamic fluid as a media lab practicum teaching high school physics class XI. The research was conducted in 81 Senior High School Jakarta, 89 Senior High School Jakarta and 115 Senor High School Jakarta. The method used, methods of Research and Development which refers to the process of development research Dick and Carey. This research was conducted through several phases, namely (1 assess the demands of curriculum standards in 2013, (2 designing media and manufacturing, (3 the development, test legibility or small scale test, test experts, tested against a teacher in physics and high school students in class XI. The instrument uses a Likert scale ratings. The result of the development of fluid dynamic lab set to produce a tool that consists of a large tank of small holes (TBLK of the inner diameter of 0.8 cm and 1.6 cm in five holes with a height variation, TBLK diameter of the inner circumference of 0.8 cm with a variation of the angle 20,5o and 30o five holes with a height variation, venturimeter with manometer fluid containing oil, venturimeter without manometer, large fluid capacity tubs, manual book and the Student Activity Sheet (LKS. The test results set against the dynamic fluid lab experts and students gain excellent assessment level is in the range of interpretation score of 81-100%. Keywords: Practicum Set of Dynamic Fluid, Development Research, and XI Grade of High School Abstrak Penelitian ini bertujuan untuk mengembangkan dan menghasilkan set praktikum fluida dinamis sebagai media praktikum pembelajaran fisika SMA kelas XI. Penelitian dilakukan di SMA N 81 Jakarta, SMA N 89 Jakarta, dan SMA N 115 Jakarta. Metode penelitian yang digunakan, metode penelitian dan pengembangan (Research and Development yang mengacu pada proses penelitian pengembangan Dick dan Carey. Penelitian ini dilakukan melalui beberapa tahapan, yaitu (1 mengkaji tuntutan standar kurikulum 2013

  10. The first steps of planet formation : studying grain growth with millimetre interferometers

    NARCIS (Netherlands)

    Lommen, Dave Jacobus Petronella

    2009-01-01

    We present Submillimeter-Array (SMA) observations of two embedded young stellar objects, Elias 29 and IRS 63. The masses of the central stars, the discs, and the envelopes are determined for such young objects for the first time. A survey of bright T-Tauri stars in the southern constellations Lupus

  11. Coupling in reflector arrays

    DEFF Research Database (Denmark)

    Appel-Hansen, Jørgen

    1968-01-01

    In order to reduce the space occupied by a reflector array, it is desirable to arrange the array antennas as close to each other as possible; however, in this case coupling between the array antennas will reduce the reflecting properties of the reflector array. The purpose of the present communic......In order to reduce the space occupied by a reflector array, it is desirable to arrange the array antennas as close to each other as possible; however, in this case coupling between the array antennas will reduce the reflecting properties of the reflector array. The purpose of the present...

  12. Observational Approach to Molecular Cloud Evolution with the Submillimeter CI Lines

    Science.gov (United States)

    Oka, T.; Yamamoto, S.; Mt. Fuji Submillimeter-Wave Telescope Group

    Neutral carbon atoms (CI) play important role both in chemistry and cooling processes of interstellar molecular clouds. It is thus crucial to explore its large area distribution to investigate formation processes and thermal balance of molecular clouds. We have constructed a 1.2 m submillimeter-wave telescope at the summit of Mt.Fuji. The telescope was designed for the exclusive use of surveying molecular clouds in two submillimeter CI lines, 3P1--3P0 (492 GHz) and 3P2--3P1 (809 GHz), of atomic carbon. It has been operated successfully during 4 observing seasons since July 1998 in a remote way from the Hongo campus of the University of Tokyo. We have already revealed large-scale CI 492 GHz distributions of many giant molecular clouds, including Orion MC, Taurus MC, DR15, DR21, NGC2264, M17, W3, W44, W51, Rosette MC, covering more than 40 square degrees of the sky. The distribution of CI 492 GHz emission is found to be different from those of the 13CO or C18O emission in some clouds. We found the spatial order of C+/CO/C from UV sources. This is the general property of the cloud illuminated by intense UV radiation, whereas it is apparently inconsistent with the standard photodissociation region (PDR) picture. We also found CI-rich areas (C/CO˜1) in several dark clouds without strong UV sources. These results are discussed in relation to formation processes of molecular clouds and dense cloud cores.

  13. CORRELATIONS IN THE (SUB)MILLIMETER BACKGROUND FROM ACT Multiplication-Sign BLAST

    Energy Technology Data Exchange (ETDEWEB)

    Hajian, Amir; Battaglia, Nick; Bond, J. Richard [Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, ON M5S 3H8 (Canada); Viero, Marco P.; Bock, James J. [California Institute of Technology, Pasadena, CA 91125 (United States); Addison, Graeme [Department of Astrophysics, Oxford University, Oxford, OX1 3RH (United Kingdom); Aguirre, Paula [Departamento de Astronomia y Astrofisica, Facultad de Fisica, Pontificia Universidad Catolica, Casilla 306, Santiago 22 (Chile); Appel, John William; Duenner, Rolando; Essinger-Hileman, Thomas; Fowler, Joseph W.; Hincks, Adam D. [Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University, Princeton, NJ 08544 (United States); Das, Sudeep; Dunkley, Joanna [Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States); Devlin, Mark J.; Dicker, Simon R. [Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104 (United States); Hughes, John P. [Department of Physics and Astronomy, Rutgers, State University of New Jersey, Piscataway, NJ 08854-8019 (United States); Halpern, Mark [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z4 (Canada); Hasselfield, Matthew [Laboratoire APC, Universite Paris Diderot, 75205 Paris (France); Hilton, Matt [Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Durban 4041 (South Africa); and others

    2012-01-01

    We present measurements of the auto- and cross-frequency correlation power spectra of the cosmic (sub)millimeter background at 250, 350, and 500 {mu}m (1200, 860, and 600 GHz) from observations made with the Balloon-borne Large Aperture Submillimeter Telescope (BLAST); and at 1380 and 2030 {mu}m (218 and 148 GHz) from observations made with the Atacama Cosmology Telescope (ACT). The overlapping observations cover 8.6 deg{sup 2} in an area relatively free of Galactic dust near the south ecliptic pole. The ACT bands are sensitive to radiation from the cosmic microwave background, to the Sunyaev-Zel'dovich effect from galaxy clusters, and to emission by radio and dusty star-forming galaxies (DSFGs), while the dominant contribution to the BLAST bands is from DSFGs. We confirm and extend the BLAST analysis of clustering with an independent pipeline and also detect correlations between the ACT and BLAST maps at over 25{sigma} significance, which we interpret as a detection of the DSFGs in the ACT maps. In addition to a Poisson component in the cross-frequency power spectra, we detect a clustered signal at 4{sigma}, and using a model for the DSFG evolution and number counts, we successfully fit all of our spectra with a linear clustering model and a bias that depends only on redshift and not on scale. Finally, the data are compared to, and generally agree with, phenomenological models for the DSFG population. This study demonstrates the constraining power of the cross-frequency correlation technique to constrain models for the DSFGs. Similar analyses with more data will impose tight constraints on future models.

  14. Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2

    Energy Technology Data Exchange (ETDEWEB)

    Robson, E. I.; Holland, W. S. [United Kingdom Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Ivison, R. J. [European Space Observatory, Karl Schwarzschild Strasse 2, D-85748 Garching (Germany); Smail, Ian [Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE (United Kingdom); Geach, J. E. [Centre for Astrophysics Research, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Gibb, A. G. [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); Riechers, D. [Astronomy Department, Cornell University, Ithaca, NY 14853 (United States); Ade, P. A. R. [Astronomy and Instrumentation Group, Cardiff University, Cardiff, Wales CF10 3XQ (United Kingdom); Bintley, D. [Joint Astronomy Centre, 660 North Ahoku Place, University Park, Hilo, HI 96720 (United States); Bock, J. [Jet Propulsion Laboratory, National Aeronautics and Space Administration, Pasadena, CA 91109 (United States); Chapin, E. L. [XMM-Newton Science Operations Centre, European Space Astronomy Centre, Apartado 79, E-28691 Villaneueva de la Canada, Madrid (Spain); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Coburg Road, Halifax B3H 1A6 (Canada); Clements, D. L. [Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Conley, A. [Center for Astrophysics and Space Astronomy, 389 UCB, University of Colorado, Boulder, CO 80309 (United States); Cooray, A. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Dunlop, J. S. [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Farrah, D., E-mail: rob.ivison@gmail.com [Department of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); and others

    2014-09-20

    We describe a search for submillimeter emission in the vicinity of one of the most distant, luminous galaxies known, HerMES FLS3, at z = 6.34, exploiting it as a signpost to a potentially biased region of the early universe, as might be expected in hierarchical structure formation models. Imaging to the confusion limit with the innovative, wide-field submillimeter bolometer camera, SCUBA-2, we are sensitive to colder and/or less luminous galaxies in the surroundings of HFLS3. We use the Millennium Simulation to illustrate that HFLS3 may be expected to have companions if it is as massive as claimed, but find no significant evidence from the surface density of SCUBA-2 galaxies in its vicinity, or their colors, that HFLS3 marks an overdensity of dusty, star-forming galaxies. We cannot rule out the presence of dusty neighbors with confidence, but deeper 450 μm imaging has the potential to more tightly constrain the redshifts of nearby galaxies, at least one of which likely lies at z ≳ 5. If associations with HFLS3 can be ruled out, this could be taken as evidence that HFLS3 is less biased than a simple extrapolation of the Millennium Simulation may imply. This could suggest either that it represents a rare short-lived, but highly luminous, phase in the evolution of an otherwise typical galaxy, or that this system has suffered amplification due to a foreground gravitational lens and so is not as intrinsically luminous as claimed.

  15. Diffusion in and around alginate and chitosan films with embedded sub-millimeter voids

    Energy Technology Data Exchange (ETDEWEB)

    Patra, Subhajit; Bal, Dharmendra Kumar; Ganguly, Somenath, E-mail: snganguly@che.iitkgp.ernet.in

    2016-02-01

    Hydrogel scaffolds from biopolymers have potential use in the controlled release of drugs, and as 3-D structure for the formation of tissue matrix. This article describes the solute release behavior of alginate and chitosan films with embedded voids of sub-millimeter dimensions. Nitrogen gas was bubbled in a fluidic arrangement to generate bubbles, prior to the crosslinking. The crosslinked gel was dried in a vacuum oven, and subsequently, soaked in Vitamin B-12 solution. The dimensions of the voids immediately after the cross-linking of gel, and also after complete drying were obtained using a digital microscope and scanning electron microscope respectively. The porosity of the gel was measured gravimetrically. The release of Vitamin B-12 in PBS buffer on a shaker was studied. The release experiments were repeated at an elevated temperature of 37 °C in the presence of lysozyme. The diffusion coefficient within the gel layer and the mass transfer coefficient at the interface with the bulk-liquid were estimated using a mathematical model. For comparison, the experiment was repeated with a film that does not have any embedded void. The enhancement in diffusion coefficient due to the presence of voids is discussed in this article. - Highlights: • Formation of sub-millimeter voids in biopolymer films using fluidic arrangement • The retention of self-assembled bubbles in films after crosslinking, and drying • The enhancement observed in release of model drug with introduction of voids • The diffusion coefficients in and around biopolymer films from model regression • Use of classical model in explaining release profiles from dual porosity media.

  16. KEMAMPUAN PROFESIONAL GURU BIOLOGI DALAM MEMAHAMI DAN MERANCANG MODEL PEMBELAJARAN KONSERVASI BIODIVERSITAS DI SMA

    Directory of Open Access Journals (Sweden)

    Suroso Mukti Leksono

    2013-11-01

    Full Text Available Abstrak: Tujuan penelitian ini adalah untuk mengetahui penguasaan konsep konservasi biodiversitas guru biologi dan cara mengajarkannya. Penelitian ini menggunakan metode deskriptif dengan menggunakan angket pada 31 guru SMA/MA di Kota/Kab Serang. Hasil penelitian menunjukkan bahwa 52% guru telah memahami konsep biodiversitas, namun hanya 3% yang memahami konsep konservasi. Model yang digunakan guru dalam mengajarkan konservasi biodiversitas, 58% menggunakan observasi, 45% diskusi, 23% ceramah dan 16% tanya jawab. Untuk tingkat kesukaran, 87% guru beranggapan mudah memahami materi konservasi biodiversitas dan 81% beranggapan mudah mengajarkannya dibandingkan dengan materi IPA lainnya. Guru-guru selama ini hanya 6% saja yang memperoleh pengetahuan tentang konservasi biodiversitas pada saat pelatihan. Oleh sebab itu diperlukan pelatihan-pelatihan melalui Continuing Professional Development (CPD. Kata Kunci: guru profesional, konservasi biodiversitas, continuing professional development (CPD BIOLOGY TEACHERS’ PROFESSIONAL ABILITY IN UNDERSTANDING AND DESIGNING INSTRUCTION ON BIODIVERSITY CONSERVATION IN SMA Abstract: The purpose of this study was to gain the knowledge about biology teachers’ concept mastery on biodiversity conservation as well as how to teach it. This study used descriptive methods with the questionnaires to 31 respondents of SMA/MA in Kota/KabSerang. The research result showed that 52% respondents had mastered the biodiversity concept. However, only 3% of respondents had fully mastered biodiversity conservation. In addition, for the teaching methods 58% respondents used observation, 45% respondents used discussion, 23% respondents used lecturing and 16% respondents used an interactive method. Moreover, for the difficulty level, 87% of respondents argued that it was easy to master the biodiversity conservation materials and 81% said that it was easier to teach the concept than other concepts. Only 6% of the teachers had gained

  17. Profil Problem Emosi/ Perilaku Pada Remaja Pelajar SMP-SMA Di Kota Semarang

    Directory of Open Access Journals (Sweden)

    Annastasia Ediati

    2015-10-01

    Full Text Available The aims of this study is to identify the profile of emotional/behavioral problems on adolescents students of junior and senior high school (SMP-SMA in Semarang, Central Java. The subjects comprised 568 students (grade VII and X; males and females, aged between 13-17 years. Data were collected using the Indonesian translation of the Youth Self Report (YSR. The results of data analysis showed that adolescents in the junior high school/SMP reported emotional/behavioral problems more frequently than the adolescents in the senior high school/SMA (t (566 = 2.08, p = .038, especially in terms of social relations (t (566 = 2.92, p = .004, thought problems (t (566 = 2.47, p = .014, somatic complaints (t(566 = 2.98, p = .002, rule-breaking behavior (t (566 = 6.63, p < .001, and externalizing problems (t(566 = 3,37; p = .001. Gender differences was found in the adolescents’ emotional/behavioral problems. In group of junior high school students (SMP, girls reported more emotional problems than boys (t(335 = -3.55; p < .001, particularly in anxiety/depression (t(335 = -6.51; p < .001; withdrawal (t(335 = -4.26; p < .001, somatic complaints (t(335 = -2.86; p = .004; social problems (t(335 = -3.30; p = .001, attention problems (t(335 = -2.39; p = .017; and internalizing problem (t(335 = -5.76; p < .001. In group of senior high school students (SMA, boys reported more externalizing problems (t(229 = 2.10; p = .037 and rule-breaking behavior (t(229 = 4.44; p < .001 than girls. In contrasts, girls reported more somatic complaints than boys (t(229 = -3.09; p = .001. Adolescents’ emotional/behavioral problems should gained more attention. Preventive as well as curative intervention is needed, particularly intervention that sensitive to gender and age, which also involve significant figures for adolescents (parents, school teachers, and peers.

  18. PEMBELAJARAN FISIKA DI SMA MELALUI PERTANYAAN (LEARNING BY QUESTIONING DAN KETERAMPILAN BERPIKIR

    Directory of Open Access Journals (Sweden)

    Nadi Suprapto

    2013-11-01

    Full Text Available ABSTRAK   Paradigma pembelajaran saat ini adalah Student Center Learning (SCL, yang dapat dicapai apabila pembelajaran khususnya pembelajaran fisika di SMA dirancang sedemikian rupa hingga dapat membelajarkan siswa. Salah satu desain pembelajaran (learning design yang dapat digunakan untuk membelajarkan siswa adalah pembelajaran melalui pertanyaan –Learning by Questioning- (LBQ. LBQ berpotensi lebih memberdayakan keterampilan berpikir dan dapat mengkonstruk pengetahuan. Untuk itu sangat perlu dihasilkan contoh perangkat pembelajaran melalui bertanya (LBQ dan selanjutnya diuji secara empiris. Artikel ini akan mendeskripsikan hasil-hasil pengujian empiris tersebut, sehingga rumusan masalah yang dikemukakan adalah bagaimanakah hasil implementasi perangkat pembelajaran melalui bertanya (LBQ di kelas? Setelah dihasilkan contoh perangkat pembelajaran melalui pertanyaan (Learning by Questioning yang terdiri dari dua topik fisika SMA: fluida statis yang sesuai dengan Kurikulum Tingkat satuan Pendidikan (KTSP, dan Hukum-hukum Newton sesuai dengan Kurikulum 2013. Perangkat pembelajaran tersebut terdiri atas silabus, RPP, LKS dan panduannya, buku siswa, Lembar penilaian LBQ dan kuncinya. Selanjutnya terkait hasil uji empiris atau hasil implementasi perangkat pembelajaran di kelas, diperoleh temuan-temuan: (a Penerapan pembelajaran bertanya (LBQ dapat meningkatkan keterampilan berpikir siswa dengan perolehan gain peningkatan untuk 10 atribut keterampilan berpikir berada pada rentang 0,27 sampai 0,73 dengan rata-rata 0,48 (sedang, (b Ditemukan delapan atribut keterampilan berpikir (80% dari sepuluh yang diteliti yang konsisten dan dapat ditingkatkan dengan pembelajaran melalui pertanyaan (LBQ. Kedelapan atribut tersebut adalah menganalisis dan mensintesis (analizing and synthesizing, meningkatkan kualitas pertanyaan (raises questions, menggali informasi (information searching, menggunakan konsep (utilizes concept, membuat inferensi (makes inferences

  19. PEMBERIAN METODE QUIZ TEAM PADA PEMBELAJARAN MATEMATIKA SISWA KELAS X SMA PGRI 1 PADANG

    Directory of Open Access Journals (Sweden)

    Rudi Chandra

    2016-05-01

    Full Text Available This research is motivated by the high school students' mathematics learning results are still not satisfactory. The low learning outcomes as a result of saturation of the students towards mathematics teaching methods as well as less active students in participating in learning. The purpose of this study is to determine whether the findings of a review study mathematics of Students group were given a quiz teams Better From the findings of Students learn math following the conventional learning in class X SMA PGRI 1 Padang. This type of research is experimental research is research by giving treatment to the experimental group and the control group did not. The treatment given in this research was the method quiz team. The study population was all class X SMA PGRI 1 Padang sample is class X 7 as an experimental class and the class X 6 as the control class. The data analysis technique used is the t test of the party at = 0.05 with the help of Minitab software. The average score of the experimental class achievement test is 73.18 with a standard deviation of 11.60 and an average score of control classroom achievement test is 57.40 with a standard deviation of 12.90. Based on the analysis of mathematics achievement test scores of students using the t test with Minitab software obtained P-value = 0.001 less than = 0.05. The research results obtained are the result of students' mathematics learning with quiz team giving better mathematics learning outcomes of students who take conventional learning in class X SMA PGRI 1 Padang on the real level of 95%.

  20. Kinerja Campuran Split Mastic Asphalt (SMA) Yang Menggunakan Serat Selulosa Alami Dedak Padi

    OpenAIRE

    Tahir, Anas

    2011-01-01

    Split Mastic Asphalt (SMA) is one of the hot mix asphalt concretes use with open graded and it has high coarse agregate content (70% - 80%) and a high asphalt content. Since the content of the high asphalt needs requires additional material such as cellulosa fiber to stabilize the asphalt. Through with this study, the another try to use rice bran as the additional material. In addition, rice bran is a natural cellulose fiber which cames from the rice milling proces. It was relatifevely cheape...

  1. PENGARUH PROJECT BASED LEARNING TERHADAP KETERAMPILAN PROSES SAINS SISWA KELAS X SMA NEGERI SIDOARJO

    Directory of Open Access Journals (Sweden)

    Nuril Maghfiroh

    2016-08-01

    Tujuan penelitian ini adalah untuk mengetahui pengaruh pembelajaran Project Based Learning terhadap keterampilan proses sains siswa kelas X SMA Negeri 4 Sidoarjo. Penelitian ini menggunakan metode Quasi Eksperimen dengan rancangan pretest postest non-equivalent control group design. Penentuan sampel mempertimbangkan kemampuan kognitif yang setara antara dua kelas yang menjadi kelompok kontrol dan kelompok eksperimen. Keterampilan proses sains diukur melalui tes tulis yang kemudian dianalisis dengan rubrik penilaian yang sudah disesuaikan untuk setiap aspek keterampilan proses sains. Hasil penelitian menunjukkan bahwa ada pengaruh pembelajaran Project Based Learning terhadap keterampilan proses sains siswa.

  2. Pengaruh Metode Pembelajaran dan Berpikir Kritis Terhadap Hasil Belajar Sejarah Siswa SMA Kesatuan Bogor

    OpenAIRE

    Iryance, Iin

    2017-01-01

    Absrtact The aim of the study is to reveal the empirical data about the effect of instructional methodology and student’s critical thinking capability level on the outcome of history learning on the students of SMA Kesatuan Bogor. The methodology used is the experimental method with a 2x2 factorial design. Research instrumentation will include a test that will be used to measure student’s learning outcome, and a questionnaire that will be used to measure student’s critical thinking capabil...

  3. Analisis Kemampuan Berpikir Matematis Siswa SMA kota Sorong terhadap Butir Soal dengan Graded Response Model

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    Muhammad Syahrul Kahar

    2017-06-01

    Full Text Available This research aims to know the level of mathematical thinking ability of students by using scored model Graded Response Model (GRM. The subject here is the students of Class XI IPA 1 SMA Negeri 3 Sorong the 2016/2017 academic year, which amounted to 38 students with 22 students are male and 16 female students. This research is a descriptive research experiment. The results of this study indicate that the scored model GRM is effective in analyzing the ability of mathematical thinking of students. The effectiveness is shown an increase in student learning outcomes grade XI IPA 1 SMA Negeri 3 Kota Sorong, where the average grade results visible increase of 56.7 until 78, and the value of the completeness students improved significantly, and student learning outcomes were shown in graded contents relevance criteria students with score 4 there are 18 students (47.37%, while the relevance of the contents with a score of 1 there are 4 students (10.53%. From the criteria of completeness students who achieve complete answers by a score of 4, there are 1 students (2.64%, and the answers are far from finished with a score of 1 there were 7 students (19.52%. Then to organizing criteria, students are working on a very systematic, there are 8 students (21.05%, and organizing with not systematically there are 10 students (26.32%. Penelitian ini bertujuan untuk mengetahui tingkat kemampuan berpikir matematis siswa dengan menggunakan model penyekoran Graded Response Model (GRM. Subjek penelitian disini adalah siswa kelas XI IPA 1 SMA Negeri 3 Kota Sorong tahun ajaran 2016/2017, yang berjumlah 38 siswa dengan 22 siswa laki-laki dan 16 siswa perempuan. Penelitian ini adalah penelitian eksperimen yang bersifat Deskriptif. Hasil penelitian ini menunjukkan bahwa model penyekoran GRM ini efektif dalam menganalisis kemampuan berpikir matematis siswa. Keefektifan tersebut terlihat adanya peningkatan hasil belajar siswa kelas XI IPA 1 SMA Negeri 3 Kota Sorong, dimana

  4. Code Switching Types Used by the English Teacher in English Classroom at SMA 1 Malili

    OpenAIRE

    Rahmawati Upa

    2014-01-01

    This research aimed at finding out: (1) the types of code switching used by the English teacher (2) the dominant types of code switching used by the teacher and (3) the teacher’s perceptions toward the use of teachers’ code switching in English classroom at SMA I Malili. This research took one of the English teachers as the subject of the research and the data were gathered through observation, interview, and recorded by using video recorder and field notes. The data were then analyzed using ...

  5. An ALMA survey of submillimeter galaxies in the extended Chandra deep field south: The redshift distribution and evolution of submillimeter galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Simpson, J. M.; Swinbank, A. M.; Smail, Ian; Alexander, D. M.; Danielson, A. L. R.; Thomson, A. P. [Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Brandt, W. N. [Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802 (United States); Bertoldi, F.; Karim, A. [Argelander-Institute for Astronomy, Bonn University, Auf dem Hügel 71, D-53121 Bonn (Germany); De Breuck, C. [European Southern Observatory, Karl-Schwarzschild Straße, D-85748 Garching bei München (Germany); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 (Canada); Coppin, K. E. K. [Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Da Cunha, E.; Hodge, J. A.; Schinnerer, E. [Max-Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany); Dannerbauer, H. [Universität Wien, Institut für Astrophysik, Türkenschanzstraße 17, A-1180 Wien (Austria); Greve, T. R. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Ivison, R. J. [Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Knudsen, K. K. [Department of Earth and Space Science, Onsala Space Observatory, Chalmers University of Technology, SE-43992 Onsala (Sweden); Poggianti, B. M., E-mail: j.m.simpson@dur.ac.uk [INAF-Astronomical Observatory of Padova, I-35122 Padova (Italy); and others

    2014-06-20

    We present the first photometric redshift distribution for a large sample of 870 μm submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA. In our analysis we consider 96 SMGs in the Extended Chandra Deep Field South, 77 of which have 4-19 band photometry. We model the SEDs for these 77 SMGs, deriving a median photometric redshift of z {sub phot} = 2.3 ± 0.1. The remaining 19 SMGs have insufficient photometry to derive photometric redshifts, but a stacking analysis of Herschel observations confirms they are not spurious. Assuming that these SMGs have an absolute H-band magnitude distribution comparable to that of a complete sample of z ∼ 1-2 SMGs, we demonstrate that they lie at slightly higher redshifts, raising the median redshift for SMGs to z {sub phot} = 2.5 ± 0.2. Critically we show that the proportion of galaxies undergoing an SMG-like phase at z ≥ 3 is at most 35% ± 5% of the total population. We derive a median stellar mass of M {sub *} = (8 ± 1) × 10{sup 10} M {sub ☉}, although there are systematic uncertainties of up to 5 × for individual sources. Assuming that the star formation activity in SMGs has a timescale of ∼100 Myr, we show that their descendants at z ∼ 0 would have a space density and M{sub H} distribution that are in good agreement with those of local ellipticals. In addition, the inferred mass-weighted ages of the local ellipticals broadly agree with the look-back times of the SMG events. Taken together, these results are consistent with a simple model that identifies SMGs as events that form most of the stars seen in the majority of luminous elliptical galaxies at the present day.

  6. The Next-Generation Very Large Array: Technical Overview

    Science.gov (United States)

    McKinnon, Mark; Selina, Rob

    2018-01-01

    As part of its mandate as a national observatory, the NRAO is looking toward the long range future of radio astronomy and fostering the long term growth of the US astronomical community. NRAO has sponsored a series of science and technical community meetings to consider the science mission and design of a next-generation Very Large Array (ngVLA), building on the legacies of the Atacama Large Millimeter/submillimeter Array (ALMA) and the Very Large Array (VLA).The basic ngVLA design emerging from these discussions is an interferometric array with approximately ten times the sensitivity and ten times higher spatial resolution than the VLA and ALMA radio telescopes, optimized for operation in the wavelength range 0.3cm to 3cm. The ngVLA would open a new window on the Universe through ultra-sensitive imaging of thermal line and continuum emission down to milli-arcsecond resolution, as well as unprecedented broadband continuum polarimetric imaging of non-thermal processes. The specifications and concepts for major ngVLA system elements are rapidly converging.We will provide an overview of the current system design of the ngVLA. The concepts for major system elements such as the antenna, receiving electronics, and central signal processing will be presented. We will also describe the major development activities that are presently underway to advance the design.

  7. Recent developments on SMA actuators: predicting the actuation fatigue life for variable loading schemes

    Science.gov (United States)

    Wheeler, Robert W.; Lagoudas, Dimitris C.

    2017-04-01

    Shape memory alloys (SMAs), due to their ability to repeatably recover substantial deformations under applied mechanical loading, have the potential to impact the aerospace, automotive, biomedical, and energy industries as weight and volume saving replacements for conventional actuators. While numerous applications of SMA actuators have been flight tested and can be found in industrial applications, these actuators are generally limited to non-critical components, are not widely implemented and frequently one-off designs, and are generally overdesigned due to a lack of understanding of the effect of the loading path on the fatigue life and the lack of an accurate method for predicting actuator lifetimes. In recent years, multiple research efforts have increased our understanding of the actuation fatigue process of SMAs. These advances can be utilized to predict the fatigue lives and failure loads in SMA actuators. Additionally, these prediction methods can be implemented in order to intelligently design actuators in accordance with their fatigue and failure limits. In the following paper, both simple and complex thermomechanical loading paths have been considered. Experimental data was utilized from two material systems: equiatomic Nickel-Titanium and Nickelrich Nickel-Titanium.

  8. Biomechanics of smart wings in a bat robot: morphing wings using SMA actuators.

    Science.gov (United States)

    Colorado, J; Barrientos, A; Rossi, C; Bahlman, J W; Breuer, K S

    2012-09-01

    This paper presents the design of a bat-like micro aerial vehicle with actuated morphing wings. NiTi shape memory alloys (SMAs) acting as artificial biceps and triceps muscles are used for mimicking the morphing wing mechanism of the bat flight apparatus. Our objective is twofold. Firstly, we have implemented a control architecture that allows an accurate and fast SMA actuation. This control makes use of the electrical resistance measurements of SMAs to adjust morphing wing motions. Secondly, the feasibility of using SMA actuation technology is evaluated for the application at hand. To this purpose, experiments are conducted to analyze the control performance in terms of nominal and overloaded operation modes of the SMAs. This analysis includes: (i) inertial forces regarding the stretchable wing membrane and aerodynamic loads, and (ii) uncertainties due to impact of airflow conditions over the resistance-motion relationship of SMAs. With the proposed control, morphing actuation speed can be increased up to 2.5 Hz, being sufficient to generate lift forces at a cruising speed of 5 m s(-1).

  9. PANDATARA DAN JARLATSUH: MODEL PENDIDIKAN MULTIKULTURAL DI SMA TARUNA NUSANTARA MAGELANG

    Directory of Open Access Journals (Sweden)

    Laila Octaviani

    2013-04-01

    Full Text Available Penelitian ini bertujuan untuk membahas model pendidikan multikultural di SMA Taruna Nusantara (TN Magelang Jawa Tengah. Metode penelitian yang digunakan adalah metode penelitian kualitatif dengan pendekatan fenomenologi. Implementasi pendidikan multicultural tercermin dalam beberapa aspek: (1 aspek visi dan misi, (2 kehidupan keseharian peserta didik; (3 kegiatan seni yang dikenal dengan nama pandatara, (4 nilai-nilai yang dikembangkan di SMA TN berkaitan dengan wawasan kebangsaan, kejuangan, dan kebudayaan; serta (5 proses pendidikan melalui tahap-tahap pembentukan kepribadian dan karakter melalui jarlatsuh (pengajaran, pengasuhan, dan pelatihan. The objective of this study is to discuss the implementation and a model of multicultural education in Taruna Nusantara (TN high school, Magelang, Central Java. The research method used in this study is phenomenological approach. The study shows that the implementation of multicultural education is reflected in several aspects: (1, vision and mission; (2 daily life activities of the learners; (3 activities related to culture and arts, which are called pandatara; (4 the values associated with the concept of nationalism, effort, and culture; and (5 the implementation of developmental stages of the personality and character of the students through jarlatsuh which include teaching activities, care, training.

  10. PENYUSUNAN MEDIA PEMBELAJARAN BERBANTUAN KOMPUTER UNTUK PBL DAN KEEFEKTIFANNYA TERHADAP CTS PESERTA DIDIK SMA

    Directory of Open Access Journals (Sweden)

    Atik Kurniawati

    2015-04-01

    Full Text Available This study aims to investigate: (1 the feasibility of computer-assisted learning media based problem based learning (PBL on Environmental Pollution materials for high school students of class X, and (2 the effectiveness of instructional media for improving of critical thinking skill (CTS learners class X SMA Negeri 5 Magelang. This research was adapted from the ADDIE model of development that includes analyze, design, develop, implement, and evaluate. Products validated by subject matter experts, media experts, educators of Biology, and peer reviewer. Subject of this study is tenth grade students of SMA Negeri 5 Magelang. Collecting data was using questionnaires, observation sheets, and test critical thinking skills. The media according to the validator and the students is classified to the category of good. Instructional media was improved to learners' critical thinking skills effectively, which demonstrated by the significant value of 0:00. This results showed that media computer-assisted learning based PBL is effective for improving of the critical thinking skills of learners.

  11. SMA foil-based elastocaloric cooling: from material behavior to device engineering

    Science.gov (United States)

    Bruederlin, F.; Ossmer, H.; Wendler, F.; Miyazaki, S.; Kohl, M.

    2017-10-01

    The elastocaloric effect associated with the stress-induced first order phase transformation in pseudoelastic shape memory alloy (SMA) films and foils is of special interest for cooling applications on a miniature scale enabling fast heat transfer and high cycling frequencies as well as tunable transformation temperatures. The focus is on TiNi-based materials having the potential to meet the various challenges associated with elastocaloric cooling including large adiabatic temperature change and ultra-low fatigue. The evolution of strain and temperature bands during tensile load cycling is investigated with respect to strain and strain-rate by in situ digital image correlation and infrared thermography with a spatial resolution in the order of 25 µm. Major design issues and challenges in fabrication of SMA film-based elastocaloric cooling devices are discussed including the efficiency of heat transfer as well as force recovery to enhance the coefficient of performance (COP) on the system level. Advanced demonstrators show a temperature span of 13 °C after 30 s, while the COP of the overall device reaches almost 10% of Carnot efficiency.

  12. MENGEMBANGKAN KEMAMPUAN BERPIKIR KREATIF DAN KEMANDIRIAN BELAJAR SISWA SMA MELALUI PEMBELAJARAN BERBASIS MASALAH

    Directory of Open Access Journals (Sweden)

    Budiyanto A.M

    2014-10-01

    Full Text Available Penelitian ini merupakan penelitian kuasi eksperimen dengan desain pretest-posttest kelompok kontrol eksperimental yang dilakukan pada tahun 2014 dengan menggunakan pendekatan Problem Based Learning (PBL untuk menginvestigasi kemampuan berpikir kreatif matematis dan kemandirian belajar siswa SMA. Subjek penelitian ini adalah 93  orang siswa kelas 11 pada sebuah SMA di Karawang. Instrumen penelitian yang digunakan adalah  tes berpikir kreatif matematis, skala dan sikap tentang kemandirian belajar. Hasil penelitian  menunjukkan bahwa kemampuan berpikir kreatif matematis siswa yang mendapat pendekatan PBL (berada pada level baik  lebih baik daripada siswa yang mendapat pembelajaran  konvensional (berada pada level sedang. Tidak terdapat  perbedaan kemandirian belajar  siswa pada kedua kelompok pembelajaran, dan  keduanya berada pada level cukup baik. Selain itu terdapat asosiasi yang cukup antara kemampuan berpikir kreatif matematik dan kemandirian belajar siswa dimana siswa juga menunjukkan persepsi yang positif terhadap pembelajaran berbasis masalah. Kata Kunci : Berpikir kreatif, kemandirian belajar, PBL.

  13. PENGEMBANGAN E-LEARNING MATA PELAJARAN TEKNOLOGI INFORMASI DAN KOMUNIKASI (TIK DI SMA NEGERI 3 KUPANG

    Directory of Open Access Journals (Sweden)

    Ariyanto S. Helianak

    2014-04-01

    Full Text Available Pengembangan E-learning Mata Pelajaran Teknologi Informasi dan Komunikasi (TIK di SMA Negeri 3 Kupang. Penelitian ini bertujuan untuk: (1 menghasilkan produk e-learning mata pelajaran Teknologi Informasi dan Komunikasi (TIK yang layak digunakan sebagai media pembelajaran bagi siswa SMA Negeri 3 Kupang; (2 mengetahui peningkatan hasil belajar siswa setelah menggunakan produk e-learning TIK. Jenis penelitian adalah penelitian dan pengembangan (R&D. Hasil penelitian menunjukkan: (1 e-learning TIK yang dihasilkan adalah sebuah sistem manajemen pembelajaran (LMS online yang dibuat dengan software aplikasi Moodle 1.9.12. E-learning TIK menyajikan materi pembelajaran TIK, khususnya kelas X, SK ke-5, KD ke-5.1 beserta modul, video, latihan, tugas dan tesnya. E-learning layak sebagai media pembelajaran TIK berdasarkan validasi ahli media, materi dan siswa, kelayakannya mencapai rerata skor 4.16 (kategori “Baik”; (2 peningkatan hasil belajar TIK siswa menggunakan e-learning lebih baik dari pada power point berdasarkan pencapaian hasil belajar. Untuk pencapaian KKM kelompok e-learning yang berjumlah 32 orang siswa, dinyatakan tuntas 30 orang siswa (94% dan 2 orang siswa (6% dinyatakan belum tuntas   sedangkan kelompok Power Point yang berjumlah 32 orang siswa, 24 orang siswa (75% dinyatakan tuntas dan 8 orang siswa  (25% dinyatakan belum tuntas. Kata kunci: e-learning, TIK

  14. KONTRIBUSI MEDIA PEMBELAJARAN INTERAKTIF UNTUK MEMBANTU MENINGKATKAN PEMAHAMAN KONSEP PEMBIASAN CAHAYA PADA SISWA KELAS X SMA

    Directory of Open Access Journals (Sweden)

    E. Bambang Saputro, A. Sopyan, B. Subali

    2016-02-01

    Full Text Available Dalam mengajarkan pokok bahasan pembiasan cahaya, terdapat kendala yang mendasar di SMA Negeri 1 Mijen Demak, yaitu visualisasi tentang jalannya sinar pada peristiwa pembiasan. Oleh karena itu untuk meningkatkan pemahaman konsep fisika perlu dilakukan terobosan baru dalam menyajikan pokok bahasan ini, salah satunya adalah dengan menggunakan media pembelajaran interaktif. Tujuan dari penelitian ini adalah untuk mengetahui kontribusi media pembelajaran interaktif dengan macromedia flash profesional 8 terhadap peningkatkan pemahaman konsep pembiasan cahaya. Subyek dalam PTK ini adalah siswa kelas X-1 SMA Negeri 1 Mijen Demak Tahun 2008/2009. Hasil penelitian menunjukkan bahwa media pembelajaran interaktif program macromedia flash professional 8 dapat meningkatkan pemahaman konsep pembiasan cahaya. Pada siklus I nilai rata-rata adalah 63,07 dan ketuntasan klasikal 64,10 %. Setelah siklus II nilai rata-rata meningkat  menjadi 74,10 dan ketuntasan klasikal  menjadi 92,31 %.. Dari hasil uji t diperoleh nilai thitung sebesar 4,66 dan ttabel sebesar 1,68. Nilai thitung >ttabel, berarti terjadi peningkatan yang signifikan untuk pemahaman siswa dari siklus I ke siklus II. Simpulan dari penelitian adalah media pembelajaran interaktif berkontribusi positif dalam meningkatkan pemahaman siswa.

  15. PENERAPAN PEER ASSESSMENT DAN SELF ASSESSMENT PADA TES FORMATIF HIDROKARBON UNTUK FEEDBACK SISWA SMA KELAS X

    Directory of Open Access Journals (Sweden)

    Wiwi Siswaningsih

    2013-04-01

    Full Text Available Penelitian dengan judul “Penerapan Peer Assessment dan Self Assessment Pada Tes Formatif Hidrokarbon Untuk Feedback Siswa SMA Kelas X” ini bertujuan memberikan feedback kepada siswa untuk meningkatkan pengetahuannya serta mendapatkan metode penilaian yang inovatif. Metode yang digunakan dalam penelitian ini adalah metode deskriptif. Penerapan peer assessment dan self assessment dilaksanakan melalui enam tahapan. Rincian keterlaksanaan setiap tahapan yaitu tahap pemotivasian siswa (75,44%, tahap pelatihan peer assessment dan self assessment (71,05%, tahap pelaksanaan tes formatif dan pemberian feedback (59,65%, tahap pelaksanaan peer assessment, self assessment dan pemberian feedback (90,35%, tahap keterlaksanaan pengkomunikasian hasil (100%, serta tahap pemanfaatan hasil (78,95%. Subjek penelitian penelitian ini adalah siswa SMA kelas X sebanyak 19 orang. Dalam pelaksanaan peer assessment, sebanyak 47,37% siswa berkategori sangat baik, 31,58% siswa berkategori baik, 15,79% siswa berkategori cukup, dan 5,26% siswa berkategori kurang. Dalam pelaksanaan self assessment, sebanyak 57,89% siswa berkategori sangat baik, 15,79%, berkategori baik, dan 26,32% siswa berkategori cukup. Sebanyak 63,16% siswa merasa puas dengan feedback yang diberikan dengan menggunakan rubrik peer assessment dan self assessment pada tes formatif hidrokarbon. Sebanyak 63,16% siswa merasa memperoleh manfaat berupa feedback dari rubrik peer assessment dan self assessment. Tahap pemotivasian dan pelatihan yang kurang maksimal menyebabkan pelaksanaan peer assessment dan self assessment kurang optimal. Kata Kunci: feedback, hidrokarbon, peer assessment, self assessment

  16. THE INFLUENCE OF STUDENTS’ SELF EFFICACY TOWARD THEIR READING ACHIEVEMENT AT SMA SRIJAYA NEGARA PALEMBANG

    Directory of Open Access Journals (Sweden)

    Sri Yuliani

    2016-09-01

    Full Text Available The formulation of the problem was “Is there any significant influence of students’self efficacy toward their English reading achievement?”. Therefore, the objective ofthis study was to find out whether or not : there is a significant influence of students’sself efficacy toward their English reading achievement. To conduct this studydescriptive quantitative was used. The population of the study consisted of 242students of SMA Srijaya Negara Palembang in the academic year of 2014/2015. Thewriter chose 2 classes of tenth grade students which consisted of 68 students. Thesample was selected by using convinience sampling. The data were collected by usingquestionnaire and test. The data were analyzed by using correlational (spearman rhoand regression analysis. The result showed that there was weak correlation betweenstudents’ self efficacy toward their English reading achievement (r=.399. Theinfluence of students’ self efficacy was 0.219 or 21.9 % to the students’ Englishreading achievement. From the F-test, it can be seen that the F-obtained was 18.472with the significant level p < 0.05 was higher than the value of F-table (F-table = 3.98. Since the F-obtained was higher than F-table, the alternative hypothesis (Ha wasaccepted and the null hypothesis (H o was rejected. So it could be concluded that therewas a significant influence of students’ self efficacy toward their English readingachievement at SMA Srijaya Negara Palembang.Keywords : Influence, Self Efficacy, and English Reading Achievement

  17. PENGEMBANGAN MODUL PEMBELAJARAN MEMPRODUKSI TEKS CERPEN BERSUMBER DARI MAJALAH REMAJA UNTUK SISWA SMA/SMK

    Directory of Open Access Journals (Sweden)

    Lilis Sumaryanti

    2016-04-01

    Full Text Available The purpose of this study, the learning module generates a text producing stories for SMA/SMK. The specific objectives of this study are (1 to develop products in the form of text materials producing short stories, short story text example, training, evaluation, and reflection and (2 describe the results of the test result validity and effectiveness of the product. This type of research is the development of research development model modified Borg & Gall. Modules developed in three parts. The first section contains text comprehension of short stories, the second part contains the steps to write short stories, and three short stories edited text. Tujuan penelitian ini, yaitu menghasilkan modul pembelajaran memproduksi teks cerpen untuk siswa SMA/SMK. Tujuan khusus penelitian ini, yaitu (1 mengembangkan produk berupa materi memproduksi teks cerpen, contoh teks cerpen, latihan,evaluasi, dan refleksi dan (2 mendeskripsikan hasil validitas dan hasil uji keefektifan produk. Jenis penelitian ini adalah penelitian pengembangan dengan model pengembangan modifikasi Borg & Gall. Modul yang dikembangkan terdiri atas tiga bagian. Bagian pertama berisi tentang pemahaman teks cerpen, bagian kedua berisi langkah-langkah menulis cerpen, dan ketiga menyunting teks cerpen.

  18. Natural history of SMA IIIb: muscle strength decreases in a predictable sequence and magnitude.

    Science.gov (United States)

    Deymeer, Feza; Serdaroglu, Piraye; Parman, Yesim; Poda, Mehves

    2008-08-26

    To assess the natural progression of muscle weakness in spinal muscular atrophy (SMA) IIIb. Ten patients with SMA IIIb were followed for at least 10 years. Age at disease onset varied between 9 and 18 years. Patients were initially seen 2 to 10 years after disease onset. They were evaluated at approximately 2, 5, 10, 15, and 20 years of disease duration depending on the timing of their initial visit after onset. Medical Research Council (MRC) scale was used with particular attention to proximal muscles. The MRC grade declined with years in all of the muscles. The decline was usually not more than by one MRC grade for each 5-year period. There were 5-10 year periods when some muscles appeared to remain stationary. The succession of weakness was first triceps, then biceps and deltoid for upper extremity muscles and first thigh adductors, then iliopsoas, then quadriceps femoris, then hamstrings, thigh abductors, and gluteus maximus for lower extremity muscles. There was a remarkable uniformity between patients in the MRC grade for each muscle at each stage: in the first 5 years of the disease, triceps, iliopsoas, thigh adductors, and quadriceps femoris were the muscles which had noticeable weakness. These findings show that strength in spinal muscular atrophy IIIb decreases over time, explaining the progressive functional loss. The sequence of weakness in the lower extremities suggests that the disease starts segmentally involving the upper lumbar segments of the medulla spinalis initially. The slowness of the deterioration may have implications for clinical trials.

  19. PENGARUH INTELEGENSI, TASK COMMITMENT DAN SELF EFFICACY TERHADAP HASIL BELAJAR MATEMATIKA SISWA SMA

    Directory of Open Access Journals (Sweden)

    Nur Qalbi Tayibu

    2016-12-01

    Full Text Available This study aims to determine the effect of intelligence, task commitment and self efficacy towards learning outcomes math class X SMA country Bulukumba District of Bulukumba. This type of research is ex-post facto nature of causality. The population in the study were students of Class X SMAN in District Bulukmpa Bulukumba 2014/2015 school year as many as 420 students and 201 students sample, taken by using proportional random sampling. The instrument used consisted of intelligence tests (tests of verbal linguistic intelligence, logical mathematical intelligence and visual-spatial, self-efficacy scale and the scale of task commitment and math achievement test. Data were analyzed using descriptive statistics and inferential statistics that path analysis (path anlysis. The research concludes that: (i Most students of class X SMA in Bulukumba, have intelligence with the category average, task commitment in learning mathematics with high category, self-efficacy in mathematics with high category and yield learning mathematics are the very low category. (Ii a variable that significantly that intelligence directly influence the outcome of learning mathematics, self-efficacy directly influence learning outcomes and task commitment directly influence the results of students' mathematics learning, intelligence indirect effect on the result of learning mathematics through task commitment and self-efficacy influential indirectly of mathematics learning outcomes through task commitment.

  20. High shape recovery Ni–Ti SMA wire produced from electron beam melted ingot

    Energy Technology Data Exchange (ETDEWEB)

    Antunes, A.S. [Instituto Tecnologico de Aeronautica – ITA, 12.228-900, S. J. Campos, SP (Brazil); Instituto Federal de Mato Grosso do Sul – IFMS, 79.331-040, Corumba, MS (Brazil); Tosetti, J.P.V. [Instituto Tecnologico de Aeronautica – ITA, 12.228-900, S. J. Campos, SP (Brazil); Otubo, J., E-mail: jotubo@ita.br [Instituto Tecnologico de Aeronautica – ITA, 12.228-900, S. J. Campos, SP (Brazil)

    2013-11-15

    Highlights: ► It was obtained a remarkable complete shape recovery up to 9% pre-strain. ► Shape recovery higher than 9% was obtained for a pre-strain up to 15%. ► These good results are attributed to a high purity NiTi SMA wire produced from EBM ingot. -- Abstract: Shape recovery of a 2 mm in diameter shape memory alloy (SMA) wire produced from EB melted NiTi ingot is presented. The results indicate complete shape recovery as high as 9% and a shape recovery higher than 9% for a pre-strain between 10 and 15%. These excellent results are attributed to the high purity of starting ingot with carbon content of 0.016 wt%. It was observed no change in reverse martensitic transformation temperature for pre-strain up to 9% and for higher pre-strain there was a 50 °C increase in reverse martensitic transformation peak temperatures indicating some work hardening of the material.

  1. Biomarker for Spinal Muscular Atrophy: Expression of SMN in Peripheral Blood of SMA Patients and Healthy Controls.

    Directory of Open Access Journals (Sweden)

    Christian Czech

    Full Text Available Spinal muscular atrophy is caused by a functional deletion of SMN1 on Chromosome 5, which leads to a progressive loss of motor function in affected patients. SMA patients have at least one copy of a similar gene, SMN2, which produces functional SMN protein, although in reduced quantities. The severity of SMA is variable, partially due to differences in SMN2 copy numbers. Here, we report the results of a biomarker study characterizing SMA patients of varying disease severity. SMN copy number, mRNA and Protein levels in whole blood of patients were measured and compared against a cohort of healthy controls. The results show differential regulation of expression of SMN2 in peripheral blood between patients and healthy subjects.

  2. MODEL PERMAINAN AKTIVITAS LUAR KELAS UNTUK MENGEMBANGKAN RANAH KOGNITIF, AFEKTIF, DAN PSIKOMOTORIK SISWA SMA

    Directory of Open Access Journals (Sweden)

    Hendra Setyawan

    2015-10-01

    Full Text Available Penelitian ini bertujuan menghasilkan model-model permainan Aktivitas Luar kelas (ALK yang layak digunakan sebagai materi pembelajaran penjas, serta efektif untuk mengembangkan ranah kognitif, afektif, dan psikomotorik siswa SMA. Penelitian ini dilakukan dengan langkah-langkah sebagai berikut: (1 pengumpulan informasi di lapangan, (2 menganalisis informasi yang telah dikumpulkan, (3 mengembangkan produk awal, (4 validasi ahli dan revisi, (5 uji coba skala kecil dan  revisi, (6 uji coba skala besar dan revisi, dan (7 pembuatan produk final. Uji coba skala kecil dilakukan terhadap siswa kelas X-D dan XI-IPA 4 dari SMA N I Prambanan berjumlah 66 orang. Uji coba skala besar dilakukan terhadap siswa kelas X-G, X-H, XI-IPS 3, dan XI-BHS dari SMA N I Prambanan berjumlah 132 orang. Instrumen pengumpulan data yang digunakan yaitu; (1 pedoman wawancara, (2 skala nilai, (3 pedoman observasi permainan, (4 pedoman observasi keefektifan permainan, (5 pedoman observasi terhadap guru pelaku uji coba, dan (6 rubrik penilaian siswa. Teknik analisis data dengan analisis deskriptif kuantitatif dan kualitatif. Hasil penelitian berupa tujuh model permainan yang layak dan efektif digunakan dalam pembelajaran penjas, hal ini dibuktikan dengan perolehan persentase sebesar 100% dari data hasil kuesioner skala nilai, observasi model permainan, observasi keefektifan permainan, dan observasi guru pelaku uji coba. Model permainan juga efektif untuk mengembangkan ranah kognitif, afektif, dan psikomotorik, yang dibuktikan dengan terjadinya peningkatan persentase nilai rata-rata siswa sebesar 21%. Kata kunci: model, permainan, aktivitas luar kelas, kognitif, afektif, psikomotorik THE OUTDOOR ACTIVITY GAME MODEL TO DEVELOP THE ASPECT OF COGNITIVE, AFFECTIVE, AND PSYCHOMOTOR OF THE SENIOR HIGH SCHOOL STUDENTS Abstract This study aims at producing outdoor activity game models which are proper to be used for physicall education learning and developing cognitive, affective, and

  3. Pengembangan Instrumen Ranah Kognitif pada Pokok Bahasan Fluida Statis SMA/MA

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    Mukarramah Mustari

    2016-04-01

    Full Text Available This study aims to: 1 Develop Instrument Domains Cognitive at Static Fluid material in SMA / MA, 2 determine the validity of the instrument of cognitive tests on the static fluid material, 3 determine the reliability of cognitive principal static fluid discussion, 4 determine the level of difficulty of the cognitive tests on the static fluid material, 5 determine distinguishing cognitive test on static fluid material. The result products include cognitive aspects such instruments multiple choice tests and essay tests. Instrument developed on cognitive aspects in the form of multiple choice tests and a description to the extent of competence Bloom C1 to C6 on the material of Static Fluid. The Design of this study is used the development procedure Reasearch and Depelopment (R & D from Borg and Gall adopted by Sugiono ie; up to the stage seven form consisting of: the potential and problems, data collection, product design, design validation, design revisions, product trials, product revision. The data collecting is obtained from the results of expert validation instrument, the response of teachers, and product trials, and then analyzed by quantitative descriptive. The results of the analysis of the development of the instrument can be concluded that the cognitive instruments on the material of static fluid SMA / MA is excellent to be used by teachers in the assessment of competence of learners. Penelitian Pengembangan Instrumen Ranah Kognitif pada Pokok Bahasan Fluida Statis SMA/MA Ini dilakukan bertujuan;1 mengembangkan Instrumen Ranah Kognitif pada Pokok Bahasan Fluida Statis SMA/MA, 2 mengetahui validitas instrumen tes kognitif pokok bahasan fluida statis, 3 mengetahui reliabilitas kognitif pokok bahasan fluida statis, 4 mengetahui tingkat kesukaran tes kognitif pokok bahasan fluida statis, 5 mengetahui daya pembeda tes kognitif pada pokok bahasan fluida statis. Produk yang dihasilkan meliputi instrumen aspek kognitif berupa

  4. Implementasi Lembar Kerja Berbasis Pertanyaan Produktif untuk Meningkatkan Kemampuan Berinkuiri Siswa SMA

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    Herman Anis

    2016-12-01

    Full Text Available Abstract Tulisan ini merupakan hasil penelitian R & D (Research and Development yang bertujuan untuk memperoleh gambaran/profil kemampuan berinkuiri siswa. Model pengembangan perangkat mengikuti model pengembangan 4-D dari Thiagarajan dkk, yang terdiri dari define, design, develop, dan disseminate. Pada tahun 2015 telah dihasilkan perangkat pembelajaran berupa lembar kerja peserta didik yang memenuhi kriteria valid baik oleh pakar maupun oleh praktisi. Model/kerangka lembar kerja yang dihasilkan terdiri dari judul, pertanyaan penyelidikan, pertanyaan analisis, dan pertanyaan penyimpulan. Model/kerangka ini meminimalkan pernyataan tuntunan seperti dalam bentuk penuntun praktikum (yang mirip ”resep kue. Ujicoba terbatas dalam penelitian ini berada pada tahap develop, metode pendekatan yang digunakan adalah metode deskriptif analitis. Subjek penelitian adalah  siswa kelas X1 yang berjumlah 30 orang,  di SMA N 1 Makassar  pada tahun akademik 2016/2017 semester genap pada tema suhu dan kalor. Hasil penelitian menunjukkan bahwa kemampuan berinkuiri rata–rata siswa SMA N 1 Makassar  berada pada kategori cukup terampil. Proses pembelajaran dengan menggunakan LKPD berbasis pertanyaan produktif dapat melatihkan kemampuan berinkuiri siswa oleh karena LKPD memuat kegiatan ilmiah yang berbasis pada keterampilan proses sains. Siswa SMA yang dijadikan subjek penelitian belum terbiasa untuk belajar mandiri, oleh karena itu penggunaan LKPD yang sejenis pada tema/topik materi yang lain perlu dilatihkan ke siswa sehingga dengan kebiasaan menggunakan LKPD seperti ini, kemampuan berinkuiri siswa akan semakin baik dan siswa akan terbiasa bekerja secara ilmiah, sehingga sikap-sikap ilmiah akan mulai terbentuk dan diharapkan akan menjadi karakter. Kata-kata kunci: lembar kerja peserta didik, pertanyaan produktif, inkuiri Abstrak This article was result of research and development (R & D which aims to obtain profile of inquiry ability of students. Model of the

  5. Integrated infrared array technology

    Science.gov (United States)

    Goebel, J. H.; Mccreight, C. R.

    1987-01-01

    An overview of integrated infrared (IR) array technology is presented. Although the array pixel formats are smaller, and the readout noise of IR arrays is larger than the corresponding values achieved with optical charge-coupled-device silicon technology, substantial progress is being made in IR technology. Both existing IR arrays and those being developed are described. Examples of astronomical images are given which illustrate the potential of integrated IR arrays for scientific investigations.

  6. Pengembangan Modul Fisika Pokok Bahasan Hukum Newton bagi Anak Berkebutuhan Khusus (Tunanetra Di Kelas Inklusi SMA/MA Kelas X

    Directory of Open Access Journals (Sweden)

    Fitriany Yudistia R

    2014-04-01

    Full Text Available Siswa tunanetra SMA Muhammadiyah 4 Yogyakarta, MAN Maguwoharjo dan SMAN 1 Sewon belum memiliki sumber belajar mandiri berupa modul Braille khususnya pada materi Hukum Newton. Berdasarkan kenyataan ini maka dibutuhkan sebuah sumber belajar yang didesain khusus bagi siswa tunanetra di kelas Inklusi yakni modul Braille pada pokok bahasan Hukum Newton.Telah dilakukan penelitian yang bertujuan untuk: (1 mengembangkan modul fisika pokok bahasan Hukum Newton untuk siswa tunanetra SMA/MA kelas X sebagai sumber belajar mandiri, (2 mengetahui kualitas modul fisika Braille materi Hukum Newton untuk siswa tunanetra SMA/MA kelas X, (3 mengetahui respon siswa terhadap modul fisika Braille yang telah dikembangkan.Penelitian ini merupakan penelitian R & D dengan model prosedural yang mengadaptasi dari pengembangan perangkat model 4-D, yakni Define, Design, Develop, and Disseminate. Instrumen penelitian berupa angket kualitas modul yaitu menggunakan skala Likert yang dibuat dalam bentuk checklist. Instrumen untuk siswa berupa angket respon siswa yaitu menggunakan skala Guttman yang dibuat dalam bentuk checklist. Modul dinilai kualitasnya oleh 3 ahli materi, 1 ahli media, dan 2 guru fisika SMA/MA. Kelayakan modul berdasarkan respon siswa pada uji coba terbatas sebanyak 2 siswa dan uji coba luas sebanyak 8 siswa.Hasil penelitian berdasarkan penilaian dari ahli materi, ahli media dan guru fisika SMA/MA modul memiliki kategori sangat baik (SB. Persentase keidealan menurut ahli materi adalah 87,88%; persentase keidealan menurut ahli media adalah 90,00% dan persentase keidealan menurut guru Fisika SMA/MA adalah 75,00%. Respon siswa terhadap modul fisika Braille pada uji coba terbatas diperoleh persentase 97,22%; sedangkan pada uji coba luas diperoleh persentase 89,58%. Hasil penelitian ini menunjukkan bahwa modul layak dijadikan sebagai salah satu sumber belajar mandiri bagi siswa tunanetra.

  7. Expression of Muscle-Specific MiRNA 206 in the Progression of Disease in a Murine SMA Model.

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    Valeria Valsecchi

    Full Text Available Spinal muscular atrophy (SMA is a severe neuromuscular disease, the most common in infancy, and the third one among young people under 18 years. The major pathological landmark of SMA is a selective degeneration of lower motor neurons, resulting in progressive skeletal muscle denervation, atrophy, and paralysis. Recently, it has been shown that specific or general changes in the activity of ribonucleoprotein containing micro RNAs (miRNAs play a role in the development of SMA. Additionally miRNA-206 has been shown to be required for efficient regeneration of neuromuscular synapses after acute nerve injury in an ALS mouse model. Therefore, we correlated the morphology and the architecture of the neuromuscular junctions (NMJs of quadriceps, a muscle affected in the early stage of the disease, with the expression levels of miRNA-206 in a mouse model of intermediate SMA (SMAII, one of the most frequently used experimental model. Our results showed a decrease in the percentage of type II fibers, an increase in atrophic muscle fibers and a remarkable accumulation of neurofilament (NF in the pre-synaptic terminal of the NMJs in the quadriceps of SMAII mice. Furthermore, molecular investigation showed a direct link between miRNA-206-HDAC4-FGFBP1, and in particular, a strong up-regulation of this pathway in the late phase of the disease. We propose that miRNA-206 is activated as survival endogenous mechanism, although not sufficient to rescue the integrity of motor neurons. We speculate that early modulation of miRNA-206 expression might delay SMA neurodegenerative pathway and that miRNA-206 could be an innovative, still relatively unexplored, therapeutic target for SMA.

  8. PKCδ as a regulator for TGFβ1-induced α-SMA production in a murine nonalcoholic steatohepatitis model.

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    Su Jin Lee

    Full Text Available The precise mechanism of TGFβ1 signaling in the progression of non-alcoholic steatohepatitis (NASH has remained unclear. In particular, a potential regulatory mechanism by which PKCδ affects profibrogenic gene expression had never been explored. In this study, therefore, the role of PKCδ in TGFβ1 mediated α-SMA expression was investigated using NASH model mice. In preparation of the NASH model, male C57BL6/J mice were fed a methionine-choline-deficient (MCD diet for 3 weeks, after which time they were intraperitoneally injected with lipopolysaccharide (LPS. In addition, Tlr4(Lps-d (CH3/HeJ mice were used to demonstrate the TGFβ1 signaling's dependency on TLR4 induction. Liver histology and hepatic hepatitis markers were investigated, and hepatic gene expression levels were determined by real-time PCR. Acute liver injury by LPS injection specifically elevated not only α-SMA expression but also phospho-PKCδ in this model. In contrast, Tlr4(Lps-d (CH3/HeJ and blockade of TGFβ1 receptor by SB431542 resulted in a significant reduction of PKCδ activation and α-SMA expression. Moreover, the TGFβ1-induced α-SMA production was significantly reduced by a specific PKCδ inhibitor. These findings suggested that PKCδ plays a critical role in TGFβ1-induced α-SMA production in a NASH model. Thus, this was the first demonstration of the involvement of PKCδ in the regulation of α-SMA expression in NASH liver tissues, and the impaired induction of PKCδ phosphorylation by LPS in a steatohepatitis condition. Interestingly, treatment by PKCδ inhibitor caused dramatic reduction of myofibroblast activation, indicating that PKCδ represents a promising target for treating NASH.

  9. Carrier screening for spinal muscular atrophy (SMA in 107,611 pregnant women during the period 2005-2009: a prospective population-based cohort study.

    Directory of Open Access Journals (Sweden)

    Yi-Ning Su

    Full Text Available BACKGROUND: Spinal muscular atrophy (SMA is the most common neuromuscular autosomal recessive disorder. The American College of Medical Genetics has recently recommended routine carrier screening for SMA because of the high carrier frequency (1 in 25-50 as well as the severity of that genetic disease. Large studies are needed to determine the feasibility, benefits, and costs of such a program. METHODS AND FINDINGS: This is a prospective population-based cohort study of 107,611 pregnant women from 25 counties in Taiwan conducted during the period January 2005 to June 2009. A three-stage screening program was used: (1 pregnant women were tested for SMA heterozygosity; (2 if the mother was determined to be heterozygous for SMA (carrier status, the paternal partner was then tested; (3 if both partners were SMA carriers, prenatal diagnostic testing was performed. During the study period, a total of 2,262 SMA carriers with one copy of the SMN1 gene were identified among the 107,611 pregnant women that were screened. The carrier rate was approximately 1 in 48 (2.10%. The negative predictive value of DHPLC coupled with MLPA was 99.87%. The combined method could detect approximately 94% of carriers because most of the cases resulted from a common single deletion event. In addition, 2,038 spouses were determined to be SMA carriers. Among those individuals, 47 couples were determined to be at high risk for having offspring with SMA. Prenatal diagnostic testing was performed in 43 pregnant women (91.49% and SMA was diagnosed in 12 (27.91% fetuses. The prevalence of SMA in our population was 1 in 8,968. CONCLUSION: The main benefit of SMA carrier screening is to reduce the burden associated with giving birth to an affected child. In this study, we determined the carrier frequency and genetic risk and provided carrier couples with genetic services, knowledge, and genetic counseling.

  10. Design framework for spherical microphone and loudspeaker arrays in a multiple-input multiple-output system.

    Science.gov (United States)

    Morgenstern, Hai; Rafaely, Boaz; Noisternig, Markus

    2017-03-01

    Spherical microphone arrays (SMAs) and spherical loudspeaker arrays (SLAs) facilitate the study of room acoustics due to the three-dimensional analysis they provide. More recently, systems that combine both arrays, referred to as multiple-input multiple-output (MIMO) systems, have been proposed due to the added spatial diversity they facilitate. The literature provides frameworks for designing SMAs and SLAs separately, including error analysis from which the operating frequency range (OFR) of an array is defined. However, such a framework does not exist for the joint design of a SMA and a SLA that comprise a MIMO system. This paper develops a design framework for MIMO systems based on a model that addresses errors and highlights the importance of a matched design. Expanding on a free-field assumption, errors are incorporated separately for each array and error bounds are defined, facilitating error analysis for the system. The dependency of the error bounds on the SLA and SMA parameters is studied and it is recommended that parameters should be chosen to assure matched OFRs of the arrays in MIMO system design. A design example is provided, demonstrating the superiority of a matched system over an unmatched system in the synthesis of directional room impulse responses.

  11. The ArTéMiS wide-field sub-millimeter camera: preliminary on-sky performance at 350 microns

    Science.gov (United States)

    Revéret, Vincent; André, Philippe; Le Pennec, Jean; Talvard, Michel; Agnèse, Patrick; Arnaud, Agnès.; Clerc, Laurent; de Breuck, Carlos; Cigna, Jean-Charles; Delisle, Cyrille; Doumayrou, Eric; Duband, Lionel; Dubreuil, Didier; Dumaye, Luc; Ercolani, Eric; Gallais, Pascal; Groult, Elodie; Jourdan, Thierry; Leriche, Bernadette; Maffei, Bruno; Lortholary, Michel; Martignac, Jérôme; Rabaud, Wilfried; Relland, Johan; Rodriguez, Louis; Vandeneynde, Aurélie; Visticot, François

    2014-07-01

    ArTeMiS is a wide-field submillimeter camera operating at three wavelengths simultaneously (200, 350 and 450 μm). A preliminary version of the instrument equipped with the 350 μm focal plane, has been successfully installed and tested on APEX telescope in Chile during the 2013 and 2014 austral winters. This instrument is developed by CEA (Saclay and Grenoble, France), IAS (France) and University of Manchester (UK) in collaboration with ESO. We introduce the mechanical and optical design, as well as the cryogenics and electronics of the ArTéMiS camera. ArTeMiS detectors consist in Si:P:B bolometers arranged in 16×18 sub-arrays operating at 300 mK. These detectors are similar to the ones developed for the Herschel PACS photometer but they are adapted to the high optical load encountered at APEX site. Ultimately, ArTeMiS will contain 4 sub-arrays at 200 μm and 2×8 sub-arrays at 350 and 450 μm. We show preliminary lab measurements like the responsivity of the instrument to hot and cold loads illumination and NEP calculation. Details on the on-sky commissioning runs made in 2013 and 2014 at APEX are shown. We used planets (Mars, Saturn, Uranus) to determine the flat-field and to get the flux calibration. A pointing model was established in the first days of the runs. The average relative pointing accuracy is 3 arcsec. The beam at 350 μm has been estimated to be 8.5 arcsec, which is in good agreement with the beam of the 12 m APEX dish. Several observing modes have been tested, like "On- The-Fly" for beam-maps or large maps, spirals or raster of spirals for compact sources. With this preliminary version of ArTeMiS, we concluded that the mapping speed is already more than 5 times better than the previous 350 μm instrument at APEX. The median NEFD at 350 μm is 600 mJy.s1/2, with best values at 300 mJy.s1/2. The complete instrument with 5760 pixels and optimized settings will be installed during the first half of 2015.

  12. Far-Infrared and Submillimeter Emission from Galactic and Extragalactic Photodissociation Regions

    Science.gov (United States)

    Kaufman, Michael J.; Wolfire, Mark G.; Hollenbach, David J.; Luhman, Michael L.

    1999-12-01

    Photodissociation region (PDR) models are computed over a wide range of physical conditions, from those appropriate to giant molecular clouds illuminated by the interstellar radiation field to the conditions experienced by circumstellar disks very close to hot massive stars. These models use the most up-to-date values of atomic and molecular data, the most current chemical rate coefficients, and the newest grain photoelectric heating rates, which include treatments of small grains and large molecules. In addition, we examine the effects of metallicity and cloud extinction on the predicted line intensities. Results are presented for PDR models with densities over the range n=101-107 cm-3 and for incident far-ultraviolet radiation fields over the range G0=10-0.5-106.5 (where G0 is the far-ultravioliet [FUV] flux in units of the local interstellar value), for metallicities Z=1 and 0.1 times the local Galactic value, and for a range of PDR cloud sizes. We present line strength and/or line ratio plots for a variety of useful PDR diagnostics: [C II] 158 μm, [O I] 63 μm and 145 μm, [C I] 370 μm and 609 μm, CO J=1-0, J=2-1, J=3-2, J=6-5, and J=15-14, as well as the strength of the far-infrared continuum. These plots will be useful for the interpretation of Galactic and extragalactic far-infrared and submillimeter spectra observable with the Infrared Space Observatory (ISO), the Stratospheric Observatory for Infrared Astronomy, the Submillimeter Wave Astronomy Satellite, the Far Infrared and Submillimeter Telescope, and other orbital and suborbital platforms. As examples, we apply our results to ISO and ground-based observations of M82, NGC 278, and the Large Magellanic Cloud. Our comparison of the conditions in M82 and NGC 278 show that both the gas density and FUV flux are enhanced in the starburst nucleus of M82 compared with those in the normal spiral NGC 278. We model the high [C II]/CO ratio observed in the 30 Doradus region of the LMC and find that it can be

  13. Submillimeter residual losses in high-Tc superconductors

    Energy Technology Data Exchange (ETDEWEB)

    Miller, David [Univ. of California, Berkeley, CA (United States)

    1993-09-01

    Bolometry was used obtain accurate submillimeter residual loss data for epitaxial films of YBa2Cu3O7 (YBCO), Tl2Ca2Ba2Cu3O10, Tl2CaBa2Cu2O8 (TCBCO), and Ba0.6K0.4BiO3 (BKBO). We were able to fit the absorptivity measured for Nb films to an Eliashberg strong coupling calculation; excellent agreement resulted between parameters from best fits and measured Residual Resistivity Ratio. Microwave surface resistance measurements made on the same YBCO and TCBCO films are in excellent agreement with submillimeter measurements. Absorptivities for all YBCO films studied are qualitatively similar, increasing smoothly with frequency, with no gap-like features below the well known absorption edge at 450 cm-1. Losses in YBCO films were fit to a weakly coupled grain model for the a-b plane conductivity. Strong phonon structure was observed in TCBCO films between 60 and 700 cm-1 (2 THz and 23 THz); these losses could not be fitted to the simple weakly coupled grain model, in contrast to the case for other high-Tc superconductors where phonon structure observed in ceramics are is absent in epitaxial oriented films and crystals because of electronic screening due to high conductivity of a-b planes. Absorptivity data for the BKBO films all show a strong absorption onset near the BCS tunneling gap of 3.5 kBTc. Comparison with strong coupling Eliashberg predictions and of a Kramers-Kronig analysis indicate that the absorption onset is consistent with a superconducting energy gap. Effects of magnetic field on residual losses in YBCO films show a resonant absorption feature in vicinity of predicted

  14. Comparing Submillimeter Polarized Emission with Near-infrared Polarization of Background Stars for the Vela C Molecular Cloud

    Science.gov (United States)

    Santos, Fabio P.; Ade, Peter A. R.; Angilè, Francesco E.; Ashton, Peter; Benton, Steven J.; Devlin, Mark J.; Dober, Bradley; Fissel, Laura M.; Fukui, Yasuo; Galitzki, Nicholas; Gandilo, Natalie N.; Klein, Jeffrey; Korotkov, Andrei L.; Li, Zhi-Yun; Martin, Peter G.; Matthews, Tristan G.; Moncelsi, Lorenzo; Nakamura, Fumitaka; Netterfield, Calvin B.; Novak, Giles; Pascale, Enzo; Poidevin, Frédérick; Savini, Giorgio; Scott, Douglas; Shariff, Jamil A.; Diego Soler, Juan; Thomas, Nicholas E.; Tucker, Carole E.; Tucker, Gregory S.; Ward-Thompson, Derek

    2017-03-01

    We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight with polarized emission data at submillimeter wavelengths for the Vela C molecular cloud. The near-IR data consist of more than 6700 detections probing a range of visual extinctions between 2 and 20 {mag} in and around the cloud. The submillimeter data were collected in Antarctica by the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry. This is the first direct combination of near-IR and submillimeter polarization data for a molecular cloud aimed at measuring the “polarization efficiency ratio” ({R}{eff}), a quantity that is expected to depend only on grain-intrinsic physical properties. It is defined as {p}500/({p}I/{τ }V), where p 500 and p I are polarization fractions at 500 μ {{m}} and the I band, respectively, and {τ }V is the optical depth. To ensure that the same column density of material is producing both polarization from emission and from extinction, we conducted a careful selection of near-background stars using 2MASS, Herschel, and Planck data. This selection excludes objects contaminated by the Galactic diffuse background material as well as objects located in the foreground. Accounting for statistical and systematic uncertainties, we estimate an average {R}{eff} value of 2.4 ± 0.8, which can be used to test the predictions of dust grain models designed for molecular clouds when such predictions become available. The ratio {R}{eff} appears to be relatively flat as a function of the cloud depth for the range of visual extinctions probed.

  15. A SUBLOCUS OF THE MULTICOPY MICROSATELLITE MARKER CMS1 MAPS PROXIMAL TO SPINAL MUSCULAR-ATROPHY (SMA) AS SHOWN BY RECOMBINANT ANALYSIS

    NARCIS (Netherlands)

    VANDERSTEEGE, G; COBBEN, JM; OSINGA, J; SCHEFFER, H; VANOMMEN, GJB; BUYS, CHCM

    1995-01-01

    The critical region containing the spinal muscular atrophy (SMA) gene is flanked by the 5q11-q13 markers, D5S435 and D5S557, as determined by linkage analysis. Here we present the results of an analysis of a Dutch SMA family with the multicopy microsatellite marker CMS1. A crossover is revealed in

  16. PENGEMBANGAN BUDAYA SEKOLAH BERPRESTASI: STUDI TENTANG PENANAMAN NILAI DAN ETOS BERPRESTASI DI SMA KARANGTURI

    Directory of Open Access Journals (Sweden)

    Agus Yuliono

    2013-04-01

    Full Text Available Tujuan penelitian ini adalah untuk mendeskripsikan bentuk budaya sekolah berprestasi, proses penanaman nilai dan etos berprestasi kepada peserta didik dan mengetahui implikasi dari pengembangan budaya sekolah berprestasi di SMA Karangturi. Penelitian ini menggunakan pendekatan deskriptif kualitatif. Pengumpulan data menggunakan teknik observasi, wawancara dan dokumentasi. Hasil penelitian menunjukkan bahwa bentuk budaya sekolah berprestasi di SMA Karangturi mencakup empat poin yaitu: keseimbangan antara pembinaan akademik dan nonakademik, penanaman karakter melalui pelajaran, budaya mencintai almamater dan pentingnya nilai kerokhanian. Penanaman nilai dan etos berprestasi pada peserta didik dilakukan melalui kegiatan orientasi sekolah, proses pembelajaran, evaluasi belajar, ekstrakurikuler, penghargaan prestasi, kecintaan terhadap almamater, keteladanan guru, kerjasama dengan orangtua peserta didik dan seragam patriot sebagai media penanaman budaya berprestasi. Implikasi penanaman pengembangan budaya sekolah berprestasi di SMA Karangturi terdapat dalam input (penerimaan siswa baru dan pencarian siswa berpotensi, proses (pengembangan program sekolah serta pengembangan kerjasama dan output (prestasi akademik dan nonakademik serta jumlah alumni yang melanjutkan ke perguruan tinggi. The objective of this study is to describe a model of school achievement culture, the cultivation of values ​​and ethos of achievement to students and know the implications of the development of school culture on students’ achievement in Karangturi high school. This study used a qualitative descriptive approach. Techniques of collecting data were observation, interviews and documentation. This study uses sources and methods triangulation for data validation. The results show that the  school achievement culture in Karangturi high school contains four pillars, namely: a balance between academic and non-academic achievement, building character

  17. PENGEMBANGAN PERANGKAT PEMBELAJARAN BERBASIS PROBLEM BASED LEARNING UNTUK MENINGKATKAN KINERJA DALAM MENYUSUN LAPORAN SISWA SMA

    Directory of Open Access Journals (Sweden)

    Ratna Ningsih

    2016-11-01

    Full Text Available This study aims to analyze the validity, practicality and effectifity of the development of  learning tools through the test of control class, test of treatment class  and the effectivity test in order to produce biology learning tools based PBL (problem based learning that valid, practical and effective to improve performance in prepared a report to 11th grade of high school students. The development of the learning tools refers to a Borg and Gall development model. Data was collected using observation sheets, validation sheet, questionnaire, and test. Methods of data analysis done by quantitative descriptive analysis of the needs analysis, the validity and practicality of the learning tools. The effectifity of the learning is done by pretest posttest. Effectifity of learning tools analyzed by paired t-test. Results showed that the learning tools otherwise (1 very valid with a percentage of 98.91%, (2 practical with a percentage of 84,68%, and (3 effective with Tvalue amounting to 3,51 (Tvalue> Ttable at significance level of 5%. Based on the results of this study concluded that the PBL Based Learning has met the criteria perfectly valid, prractical, and effective way to improve performance in preparing the reports of students through learning biology in high school, so it can be used in a broader scope. Penelitian ini bertujuan untuk menganalisis kebutuhan guru, kelayakan, kepraktisan dan keefektifan dalam pengembangan perangkat pembelajaran berbasis Problem Based Learning untuk meningkatkan kinerja dalam menyusun laporan siswa SMA kelas XI Tahun Pembelajaran 2016/2017. Pengembangan perangkat pembelajaran mengacu pada model pengembangan Borg and Gall. Data dikumpulkan dengan menggunakan lembar observasi, lembar validasi, angket, dan tes. Metode analisis data dilakukan dengan analisis deskriptif kuantitatif terhadap analisis kebutuhan, validitas dan kelayakan perangkat pembelajaran. Efektivitas perangkat pembelajaran dilakukan dengan pretest

  18. The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields

    Science.gov (United States)

    Hsu, Li-Yen; Desai, Vandana; Murphy, Eric J.; Cowie, Lennox L.; Heywood, Ian; Momjian, Emmanuel; Barger, Amy J.; Smail, Ian

    2017-05-01

    In this second paper of the Hawaii SCUBA-2 Lensing Cluster Survey series, we cross-match SCUBA-2 maps with 3 and 6 GHz images from the Janksy-VLA Frontier Fields Legacy Survey for three cluster fields, MACS J0416.1-2403, MACS J0717.5+3745, and MACS J1149.5+2223. Within the HST coverage, 14 out of 44 850 μm sources have 3 GHz counterparts, five of which are also detected at 6 GHz. The 850 μm flux densities of these detected sources span from 0.7 to 4.4 mJy after correcting for lensing amplification. The median redshift of the sample is z={1.28}-0.09+0.07, much lower than the typical redshifts (z = 2-3) of brighter submillimeter galaxies (SMGs) in the literature. In addition, we find that our sources have lower dust temperatures than those of the brighter SMGs. This is also confirmed by an analysis of the ratio between infrared star-formation rate and 850 μm flux density. However, these 14 sources may not represent the general submillimeter population at the same flux range, given that the SCUBA-2 sources without radio counterparts are likely at higher redshifts. Detection of these sources would require deeper radio images or submillimeter interferometry.

  19. Protostellar accretion traced with chemistry

    DEFF Research Database (Denmark)

    Frimann, Søren; Jørgensen, Jes Kristian; Dunham, Michael M.

    2017-01-01

    . Our aim is to characterise protostellar accretion histories towards individual sources by utilising sublimation and freeze-out chemistry of CO. Methods. A sample of 24 embedded protostars are observed with the Submillimeter Array (SMA) in context of the large program "Mass Assembly of Stellar Systems...... and their Evolution with the SMA" (MASSES). The size of the C18O-emitting region, where CO has sublimated into the gas-phase, is measured towards each source and compared to the expected size of the region given the current luminosity. The SMA observations also include 1.3 mm continuum data, which are used...

  20. Submillimeter Detection of the van der Waals Stretching Vibration of the Ar-CO Complex

    Science.gov (United States)

    Gendriesch, R.; Pak, I.; Lewen, F.; Surin, L.; Roth, D. A.; Winnewisser, G.

    1999-07-01

    With the Cologne submillimeter-wave supersonic jet spectrometer, we extended molecular jet spectroscopy with backward wave oscillators up to frequencies of about 600 GHz. For the first time, the van der Waals stretching vibration of the Ar-CO molecular complex was detected in direct absorption. We measured 13 ro-vibrational transitions (Kvstretch = 1 ← 0, Ka = 0 ← 0) in the frequency range from 528 to 600 GHz and additionally the two R(3) K doublet (Ka = 4 ← 3) pure rotational transitions at 447 GHz with an accuracy of about 200 kHz. The ro-vibrational transitions were assigned and fitted within experimental accuracy to a simple Hamiltonian taking into account the Coriolis interaction between the stretching and bending states, i.e., between vstretch = 1, Ka = 0, and vbend = 1, Ka = 1. The intensity of the transitions in the van der Waals stretching mode was estimated to be a factor of 5-10 less than that in the bending mode of Ar-CO.

  1. Micro-Spec: An Ultracompact, High-sensitivity Spectrometer for Far-Infrared and Submillimeter Astronomy

    Science.gov (United States)

    Cataldo, Giuseppe; Hsieh, Wen-Ting; Huang, Wei-Chung; Moseley, S. Harvey; Stevenson, Thomas R.; Wollack, Edward J.

    2014-01-01

    High-performance, integrated spectrometers operating in the far-infrared and submillimeter ranges promise to be powerful tools for the exploration of the epochs of reionization and initial galaxy formation. These devices, using high-efficiency superconducting transmission lines, can achieve the performance of a meter-scale grating spectrometer in an instrument implemented on a 4 inch silicon wafer. Such a device, when combined with a cryogenic telescope in space, provides an enabling capability for studies of the early universe. Here, the optical design process for Micro-Spec (micron-Spec) is presented, with particular attention given to its two-dimensional diffractive region, where the light of different wavelengths is focused on the different detectors. The method is based on the stigmatization and minimization of the light path function in this bounded region, which results in an optimized geometrical configuration. A point design with an efficiency of (is) approximately 90% has been developed for initial demonstration and can serve as the basis for future instruments. Design variations on this implementation are also discussed, which can lead to lower efficiencies due to diffractive losses in the multimode region.

  2. T-shaped emitter metal heterojunction bipolar transistors for submillimeter wave applications

    Science.gov (United States)

    Fung, Andy; Samoska, Lorene; Velebir, Jim; Siege, Peter; Rodwell, Mark; Paidi, Vamsi; Griffth, Zach; Urteaga, Miguel; Malik, Roger

    2004-01-01

    We report on the development of submillimeter wave transistors at JPL. The goal of the effort is to produce advance-reliable high frequency and high power amplifiers, voltage controlled oscillators, active multipliers, and high-speed mixed-signal circuits for space borne applications. The technology in development to achieve this is based on the Indium Phosphide (InP) Heterojunction Bipolar Transistor (HBT). The HBT is well suited for high speed, high power and uniform (across wafer) performance, due to the ability to tailor the material structure that electrons traverse through by well-controlled epitaxial growth methods. InP with its compatible lattice matched alloys such as indium gallium arsenide (InGaAs) and indium aluminium arsenide (InAlAs) provides for high electron velocities and high voltage breakdown capabilities. The epitaxial methods for this material system are fairly mature, however the implementation of high performance and reliable transistors are still under development by many laboratories. Our most recently fabricated, second generation mesa HBTs at JPL have extrapolated current gain cutoff frequency (FJ of 142GHz and power gain cutoff frequency (Fm,) of approximately 160GHz. This represents a 13% and 33% improvement of Ft and F, respectively, compared to the first generation mesa HBTs [l]. Analysis based on the University of California, Santa Barbara (UCSB) device model, RF device characteristics can be significantly improved by reducing base contact resistance and base metal contact width. We will describe our effort towards increasing transistor performance and yield.

  3. Controlled production of sub-millimeter liquid core hydrogel capsules for parallelized 3D cell culture.

    Science.gov (United States)

    Doméjean, Hugo; de la Motte Saint Pierre, Mathieu; Funfak, Anette; Atrux-Tallau, Nicolas; Alessandri, Kevin; Nassoy, Pierre; Bibette, Jérôme; Bremond, Nicolas

    2016-12-20

    Liquid core capsules having a hydrogel membrane are becoming a versatile tool for three-dimensional culture of micro-organisms and mammalian cells. Making sub-millimeter capsules at a high rate, via the breakup of a compound jet in air, opens the way to high-throughput screening applications. However, control of the capsule size monodispersity, especially required for quantitative bioassays, was still lacking. Here, we report how the understanding of the underlying hydrodynamic instabilities that occur during the process can lead to calibrated core-shell bioreactors. The requirements are: i) damping the shear layer instability that develops inside the injector arising from the co-annular flow configuration of liquid phases having contrasting viscoelastic properties; ii) controlling the capillary instability of the compound jet by superposing a harmonic perturbation onto the shell flow; iii) avoiding coalescence of drops during jet fragmentation as well as during drop flight towards the gelling bath; iv) ensuring proper engulfment of the compound drops into the gelling bath for building a closed hydrogel shell. We end up with the creation of numerous identical compartments in which cells are able to form multicellular aggregates, namely spheroids. In addition, we implement an intermediate composite hydrogel layer, composed of alginate and collagen, allowing cell adhesion and thus the formation of epithelia or monolayers of cells.

  4. Simultaneous retrievals of temperature and volume mixing ratio constituents from nonoxygen odin submillimeter radiometer bands.

    Science.gov (United States)

    Baron, P; Merino, F; Murtagh, D

    2001-11-20

    We present the retrieval of temperature and O(3) volume mixing ratio profiles in the middle atmosphere from a single strong O(3) line. We performed the study using simulated limb-sounding measurements in the frame of the submillimeter radiometer (SMR) instrument that will be carried by the Odin satellite that is due to be launched in early 2001. This study is interesting for the Odin SMR data analysis because we first provide additional temperature measurements, and second reduce significantly the O(3) retrieval error that is due to the temperature and pressure uncertainties. Nonlinear retrievals are performed to retrieve the O(3), CO, H(2)O, and temperature profiles simultaneously from the spectral band 576.27-576.67 GHz. The pressure profile is deduced from the hydrostatic equilibrium equation after each iteration. Temperature and O(3) can be retrieved throughout the stratosphere from 15-50 and 20-50 km, respectively, with a vertical resolution of 3 km. The altitude domain corresponds to the parts of the atmosphere where the signal intensity saturates in some spectrometer channels. A total error of 4-6 K has been found in the temperature profile, mainly because of the instrumental thermal noise and to a lesser extent the calibration. The total error in the O(3) profile is 5-10% and is dominated by the O(3) line-broadening parameter. The total error on the retrieved pressure profile is 2-10% because of the errors in calibration and reference pressure.

  5. Laboratory and observational studies of transient molecules at microwave and millimeter/submillimeter wavelengths

    Science.gov (United States)

    Zack, Lindsay Nicole

    In this dissertation, techniques of high-resolution rotational spectroscopy have been used to measure the spectra of molecules in both laboratory and astronomical settings. In the laboratory, small metal-bearing molecules containing zinc, iron, nickel, titanium, yttrium, and scandium have been studied at microwave and millimeter/submillimeter wavelengths in order to determine their rotational, fine, and hyperfine constants. These molecules were synthesized in situ in direct-absorption and Fourier-transform microwave spectrometers using Broida-type ovens and laser ablation methods. From the spectroscopic parameters, information about fundamental physical properties and electronic character could be obtained. Radio telescopes were used to measure the spectra of molecules in different interstellar environments. A new molecule, FeCN, was detected toward the circumstellar envelope of the carbon-rich asymtotic giant branch star, IRC+10216, marking the first iron-bearing molecule detected in the interstellar medium. The telescopes were also used to conduct a study of the evolved planetary nebula, NGC 7293, or the Helix Nebula. In the Helix, CO, HCO+, and H2CO were observed at several positions offset from the central star to obtain densities and kinetic temperatures throughout the Helix. A map of the HCO+ J = 1→ 0 transition was also constructed, showing that HCO+ is widespread throughout the Helix, instead of being photodissociated and destroyed, as theoretical models of planetary nebulae predict.

  6. Submillimeter Measurements of Photolysis Products in Interstellar Ice Analogs: A New Experimental Technique

    Science.gov (United States)

    Milam, Stefanie N.; Weaver, Susanna Widicus

    2012-01-01

    Over 150 molecular species have been confirmed in space, primarily by their rotational spectra at millimeter/submillimeter wavelengths, which yield an unambiguous identification. Many of the known interstellar organic molecules cannot be explained by gas-phase chemistry. It is now presumed that they are produced by surface reactions of the simple ices and/or grains observed and released into the gas phase by sublimation, sputtering, etc. Additionally, the chemical complexity found in meteorites and samples returned from comets far surpasses that of the remote detections for the interstellar medium (ISM), comets, and planetary atmospheres. Laboratory simulations of interstellar/cometary ices have found, from the analysis of the remnant residue of the warmed laboratory sample, that such molecules are readily formed; however, it has yet to be determined if they are formed during the warm phase or within the ice during processing. Most analysis of the ice during processing reveals molecular changes, though the exact quantities and species formed are highly uncertain with current techniques due to overwhelming features of simple ices. Remote sensing with high resolution spectroscopy is currently the only method to detect trace species in the ISM and the primary method for comets and icy bodies in the Solar System due to limitations of sample return. We have recently designed an experiment to simulate interstellar/cometary/planetary ices and detect trace species employing the same techniques used for remote observations. Preliminary results will be presented.

  7. Probing Galaxy Formation and Evolution with Space Born Sub-Millimeter Telescopes

    Science.gov (United States)

    Dwek, Eli; Arendt, Richard G.; Moseley, Harvey; Benford, Dominic; Shafer, Richard; Mather, John; Oegerle, William (Technical Monitor)

    2002-01-01

    A major unresolved question in cosmology is how the complex system of galaxies we see in the present universe evolved from an almost perfectly smooth beginning. Multiwavelength observations of galaxies have revealed that a significant fraction of their UV-visible starlight is absorbed and reradiated by dust at infrared JR) and submillimeter wavelengths. The cumulative IR-submm. emission from galaxies since the epoch of recombination, the cosmic IR background, has recently been recorded by the COBE satellite. The COBE observations in combination with recent submm surveys conducted with the SCUBA on the 15 m JCMT have shown that most of the radiation from star formation that has taken place in the early stages of galaxy evolution is reradiated by dust at submm wavelengths. Therefore, submm telescopes offer a unique probe of the early stages of galaxy formation and evolution. This talk will: (1) consider the impact of telescope diameter on the depth of the survey (what redshift can be probed) at different wavelengths; (2) discuss the relative scientific merits of high-resolution narrow-field surveys versus lower resolution deep surveys; and (3) show how both strategies offer complementary information crucial to our understanding of the structure and evolution of galaxies in the universe.

  8. Optical fiber sensors-based temperature distribution measurement in ex vivo radiofrequency ablation with submillimeter resolution

    Science.gov (United States)

    Macchi, Edoardo Gino; Tosi, Daniele; Braschi, Giovanni; Gallati, Mario; Cigada, Alfredo; Busca, Giorgio; Lewis, Elfed

    2014-11-01

    Radiofrequency thermal ablation (RFTA) induces a high-temperature field in a biological tissue having steep spatial (up to 6°C/mm) and temporal (up to 1°C/s) gradients. Applied in cancer care, RFTA produces a localized heating, cytotoxic for tumor cells, and is able to treat tumors with sizes up to 3 to 5 cm in diameter. The online measurement of temperature distribution at the RFTA point of care has been previously carried out with miniature thermocouples and optical fiber sensors, which exhibit problems of size, alteration of RFTA pattern, hysteresis, and sensor density worse than 1 sensor/cm. In this work, we apply a distributed temperature sensor (DTS) with a submillimeter spatial resolution for the monitoring of RFTA in porcine liver tissue. The DTS demodulates the chaotic Rayleigh backscattering pattern with an interferometric setup to obtain the real-time temperature distribution. A measurement chamber has been set up with the fiber crossing the tissue along different diameters. Several experiments have been carried out measuring the space-time evolution of temperature during RFTA. The present work showcases the temperature monitoring in RFTA with an unprecedented spatial resolution and is exportable to in vivo measurement; the acquired data can be particularly useful for the validation of RFTA computational models.

  9. A New Era of Submillimeter GRB Afterglow Follow-Ups with the Greenland Telescope

    Directory of Open Access Journals (Sweden)

    Yuji Urata

    2015-01-01

    Full Text Available Planned rapid submillimeter (submm gamma-ray-bursts (GRBs follow-up observations conducted using the Greenland Telescope (GLT are presented. The GLT is a 12-m submm telescope to be located at the top of the Greenland ice sheet, where the high altitude and dry weather porvide excellent conditions for observations at submm wavelengths. With its combination of wavelength window and rapid responding system, the GLT will explore new insights on GRBs. Summarizing the current achievements of submm GRB follow-ups, we identify the following three scientific goals regarding GRBs: (1 systematic detection of bright submm emissions originating from reverse shock (RS in the early afterglow phase, (2 characterization of forward shock and RS emissions by capturing their peak flux and frequencies and performing continuous monitoring, and (3 detections of GRBs at a high redshift as a result of the explosion of first generation stars through systematic rapid follow-ups. The light curves and spectra calculated by available theoretical models clearly show that the GLT could play a crucial role in these studies.

  10. Demonstration of a phase-lockable microwave to submillimeter wave sweeper

    Science.gov (United States)

    Waltman, Steve B.; Hollberg, Leo W.; McIntosh, Alexander K.; Brown, Elliott R.

    1996-12-01

    The development of low-temperature-grown GaAs photomixers enables the construction of a microwave to submillimeter- wave source capable of large frequency sweeps. By utilizing semiconductor diode lasers to drive the photomixer, this source is all solid-state and compact, and has small power consumption. Frequency stabilization of the semiconductor diode lasers allows this source to be phase-locked to an external microwave reference. Two 805 nm extended-cavity- diode lasers are mixed in a low-temperature-grown GaAs photoconductive photomixer. The difference-frequency mixing product is radiated by a planar spiral antenna and collimated by a Si lens. This output is phase-locked to a microwave reference by downconverting it in a whisker- contacted Schottky-barrier diode harmonic mixer and using the output to offset-phase-lock one laser to the other. The photomixer output power is 300 nW at 200 GHz and 10 nW at 1.6 THz, as measured by a 4 K InSb bolometer calibrated with a methanol laser and a power meter at 526 and 812 GHz.

  11. Rapid Asymmetric Inflation and Early Cosmology in Theories with Sub-Millimeter Dimensions

    CERN Document Server

    Arkani-Hamed, N; Kaloper, Nemanja; March-Russell, John David; Arkani-Hamed, Nima; Dimopoulos, Savas; Kaloper, Nemanja; March-Russell, John

    2000-01-01

    It was recently pointed out that the fundamental Planck mass could be close to the TeV scale with the observed weakness of gravity at long distances being due the existence of new sub-millimeter spatial dimensions. In this picture the standard model fields are localized to a $(3+1)$-dimensional wall or ``3-brane''. We show that in such theories there exist attractive models of inflation that occur while the size of the new dimensions are still small. We show that it is easy to produce the required number of efoldings, and further that the density perturbations $\\delta\\rho/\\rho$ as measured by COBE can be easily reproduced, both in overall magnitude and in their approximately scale-invariant spectrum. In the minimal approach, the inflaton field is just the moduli describing the size of the internal dimensions, the role of the inflationary potential being played by the stabilizing potential of the internal space. We show that under quite general conditions, the inflationary era is followed by an epoch of contra...

  12. DETECTION OF AN ULTRA-BRIGHT SUBMILLIMETER GALAXY BEHIND THE SMALL MAGELLANIC CLOUD

    Energy Technology Data Exchange (ETDEWEB)

    Takekoshi, Tatsuya; Minamidani, Tetsuhiro; Sorai, Kazuo; Habe, Asao [Department of Cosmosciences, Graduate School of Science, Hokkaido University, Sapporo 060-0810 (Japan); Tamura, Yoichi; Kohno, Kotaro [Institute of Astronomy, University of Tokyo, Osawa, Mitaka, Tokyo 181-0015 (Japan); Oogi, Taira [Department of Physics, Faculty of Science, Hokkaido University, Sapporo 060-0810 (Japan); Ezawa, Hajime; Komugi, Shinya; Mizuno, Norikazu; Muller, Erik; Kawamura, Akiko [Chile Observatory, National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan); Oshima, Tai [Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano 384-1305 (Japan); Scott, Kimberly S. [North American ALMA Science Center, National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Austermann, Jason E. [Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309 (United States); Tosaki, Tomoka [Joetsu University of Education, Joetsu, Niigata 943-8512 (Japan); Onishi, Toshikazu [Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, 599-8531 Osaka (Japan); Fukui, Yasuo [Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Matsuo, Hiroshi [Advanced Technology Center, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Aretxaga, Itziar [Instituto Nacional de Astrofisica, Optica y Electronica (INAOE), 72000 Puebla (Mexico); and others

    2013-09-10

    We report the discovery of a new ultra-bright submillimeter galaxy (SMG) behind the Small Magellanic Cloud (SMC). This SMG is detected as a 43.3 {+-} 8.4 mJy point source (MM J01071-7302, hereafter MMJ0107) in the 1.1 mm continuum survey of the SMC by AzTEC on the ASTE telescope. MMJ0107 is also detected in the radio (843 MHz), Herschel/SPIRE, Spitzer MIPS 24 {mu}m, all IRAC bands, Wide-field Infrared Survey Explorer, and near-infrared (J, H, K{sub S} ). We find an optical (U, B, V) source, which might be the lensing object, at a distance of 1.''4 from near-infrared and IRAC sources. Photometric redshift estimates for the SMG using representative spectral energy distribution templates show the redshifts of 1.4-3.9. We estimate total far-infrared luminosity of (0.3-2.2) Multiplication-Sign 10{sup 14} {mu}{sup -1} L{sub Sun} and a star formation rate of 5600-39, 000 {mu}{sup -1} M{sub Sun} yr{sup -1}, where {mu} is the gravitational magnification factor. This apparent extreme star formation activity is likely explained by a highly magnified gravitational lens system.

  13. Effect of Rubberized Bitumen Blending Methods on Permanent Deformation of SMA Rubberized Asphalt Mixtures

    Directory of Open Access Journals (Sweden)

    Herda Yati Katman

    2016-01-01

    Full Text Available This study aims at comparing the permanent deformation of Stone Mastic Asphalt (SMA rubberized asphalt mixtures produced by the wet process. In this study, rubberized binders were prepared using two different blending methods, namely, continuous blend and terminal blend. To study the creep behaviour of control and rubberized asphalt mixtures, the dynamic creep test was performed using Universal Materials Testing Apparatus (UMATTA at different temperatures and stress levels. Zhou three-stage creep model was utilized to evaluate the deformation characteristics of the mixtures. In all test conditions, the highest resistance to permanent deformation is showed by the rubberized mixtures produced with continuous blend binders. This study also reveals that the permanent deformation of rubberized mixtures cannot be predicted based on the characteristics of the rubberized binders.

  14. Code Switching Types Used by the English Teacher in English Classroom at SMA 1 Malili

    Directory of Open Access Journals (Sweden)

    Rahmawati Upa

    2014-08-01

    Full Text Available This research aimed at finding out: (1 the types of code switching used by the English teacher (2 the dominant types of code switching used by the teacher and (3 the teacher’s perceptions toward the use of teachers’ code switching in English classroom at SMA I Malili. This research took one of the English teachers as the subject of the research and the data were gathered through observation, interview, and recorded by using video recorder and field notes. The data were then analyzed using discourse analysis. The result of analysis showed that (1 the teacher used three types of code switching, namely: intrasentential code switching, inter-sentential code switching, and tag switching; (2 the dominant types of code switching used was intrasentential code switching followed by inter sentential code switching and tag switching (3 the interviewed teacher responded positively toward the use of code switching by the English teacher in English classroom.

  15. Test results for an SMA-actuated vortex wake control system

    Science.gov (United States)

    Quackenbush, Todd R.; Bilanin, Alan J.; Carpenter, Bernie F.

    1999-07-01

    This paper describes recent test result obtained on a prototype SMA-actuated foil that serves as a key element in a vortex wake control scheme for lifting surfaces. Previous papers have described the theoretical basis and feasibility studies for this scheme - which is based on a novel wake control known as vortex leveraging - as well as prior work on device design, test planning, and fabrication. The critical item in the realization of this scheme is a Smart Vortex Leveraging Tab (SVLT), a device designed to provide perturbations in the vortex system downstream of lifting surfaces at frequencies and amplitudes carefully selected to accelerate overall wake breakup. The paper summarizes the background of the effort, but focuses on the detail design and fabrication techniques used in the construction of a prototype SVLT and the results of water tunnel tests of a near full-scale prototype device.

  16. Design, fabrication, and test planning for an SMA-actuated vortex wake control system

    Science.gov (United States)

    Quackenbush, Todd R.; Batcho, P. F.; Bilanin, Alan J.; Carpenter, Bernie F.

    1998-06-01

    This paper describes ongoing design and fabrication work on a vortex wake control system for submarines that employs SMA-actuated devices. Previous work has described the theoretical basis and feasibility studies for this system, which is based on a novel wake control scheme known as vortex leveraging. The critical item in the realization of this system is a Smart Vortex Leveraging Tab (SVLT), whose design and fabrication is the principal focus of this work. This paper outlines the background of the effort and the design principles involved, but will chiefly deal with three closely interrelated topics; the hydrodynamic design requirements and control surface layout for the vortex leveraging system; the detail design and fabrication techniques being used in the construction of a prototype SVLT; and the test planning and experiment design process currently underway for test of both the overall vortex leveraging concept and SVLT device itself.

  17. Surface grain refinement mechanism of SMA490BW steel cross joints by ultrasonic impact treatment

    Science.gov (United States)

    He, Bo-lin; Xiong, Lei; Jiang, Ming-ming; Yu, Ying-xia; Li, Li

    2017-04-01

    Ultrasonic impact treatment (UIT) is a postweld technique for improving the fatigue strength of welded joints. This technique makes use of ultrasonic vibration to impact and plastically deform a weld toe and can achieve surface grain refinement of the weld toe, which is considered as the main reason for the improvement of fatigue strength. In this paper, the microstructure of the surface of a treated weld toe was observed by metallographic microscopy and transmission electron microscopy (TEM). The results show that UIT could produce severe plastic deformation on the surface layer of the weld toe and the maximum depth of plastic deformation extended to approximately 260 μm beneath the treated surface. Repeated processing could exacerbate the plastic deformation on the surface layer, resulting in finer grains. We can conclude that the surface grain refinement mechanism of SMA490BW welded joints is related to the high density of dislocation tangles and dislocation walls.

  18. Acquisition through horizontal gene transfer of plasmid pSMA198 by Streptococcus macedonicus ACA-DC 198 points towards the dairy origin of the species.

    Science.gov (United States)

    Papadimitriou, Konstantinos; Anastasiou, Rania; Maistrou, Eleni; Plakas, Thomas; Papandreou, Nikos C; Hamodrakas, Stavros J; Ferreira, Stéphanie; Supply, Philip; Renault, Pierre; Pot, Bruno; Tsakalidou, Effie

    2015-01-01

    Streptococcus macedonicus is an intriguing streptococcal species whose most frequent source of isolation is fermented foods similarly to Streptococcus thermophilus. However, S. macedonicus is closely related to commensal opportunistic pathogens of the Streptococcus bovis/Streptococcus equinus complex. We analyzed the pSMA198 plasmid isolated from the dairy strain Streptococcus macedonicus ACA-DC 198 in order to provide novel clues about the main ecological niche of this bacterium. pSMA198 belongs to the narrow host range pCI305/pWV02 family found primarily in lactococci and to the best of our knowledge it is the first such plasmid to be reported in streptococci. Comparative analysis of the pSMA198 sequence revealed a high degree of similarity with plasmids isolated from Lactococcus lactis strains deriving from milk or its products. Phylogenetic analysis of the pSMA198 Rep showed that the vast majority of closely related proteins derive from lactococcal dairy isolates. Additionally, cloning of the pSMA198 ori in L. lactis revealed a 100% stability of replication over 100 generations. Both pSMA198 and the chromosome of S. macedonicus exhibit a high percentage of potential pseudogenes, indicating that they have co-evolved under the same gene decay processes. We identified chromosomal regions in S. macedonicus that may have originated from pSMA198, also supporting a long co-existence of the two replicons. pSMA198 was also found in divergent biotypes of S. macedonicus and in strains isolated from dispersed geographic locations (e.g. Greece and Switzerland) showing that pSMA198's acquisition is not a recent event. Here we propose that S. macedonicus acquired plasmid pSMA198 from L. lactis via an ancestral genetic exchange event that took place most probably in milk or dairy products. We provide important evidence that point towards the dairy origin of this species.

  19. Acquisition through horizontal gene transfer of plasmid pSMA198 by Streptococcus macedonicus ACA-DC 198 points towards the dairy origin of the species.

    Directory of Open Access Journals (Sweden)

    Konstantinos Papadimitriou

    Full Text Available Streptococcus macedonicus is an intriguing streptococcal species whose most frequent source of isolation is fermented foods similarly to Streptococcus thermophilus. However, S. macedonicus is closely related to commensal opportunistic pathogens of the Streptococcus bovis/Streptococcus equinus complex.We analyzed the pSMA198 plasmid isolated from the dairy strain Streptococcus macedonicus ACA-DC 198 in order to provide novel clues about the main ecological niche of this bacterium. pSMA198 belongs to the narrow host range pCI305/pWV02 family found primarily in lactococci and to the best of our knowledge it is the first such plasmid to be reported in streptococci. Comparative analysis of the pSMA198 sequence revealed a high degree of similarity with plasmids isolated from Lactococcus lactis strains deriving from milk or its products. Phylogenetic analysis of the pSMA198 Rep showed that the vast majority of closely related proteins derive from lactococcal dairy isolates. Additionally, cloning of the pSMA198 ori in L. lactis revealed a 100% stability of replication over 100 generations. Both pSMA198 and the chromosome of S. macedonicus exhibit a high percentage of potential pseudogenes, indicating that they have co-evolved under the same gene decay processes. We identified chromosomal regions in S. macedonicus that may have originated from pSMA198, also supporting a long co-existence of the two replicons. pSMA198 was also found in divergent biotypes of S. macedonicus and in strains isolated from dispersed geographic locations (e.g. Greece and Switzerland showing that pSMA198's acquisition is not a recent event.Here we propose that S. macedonicus acquired plasmid pSMA198 from L. lactis via an ancestral genetic exchange event that took place most probably in milk or dairy products. We provide important evidence that point towards the dairy origin of this species.

  20. Linking simulations and experiments for the multiscale tracking of thermally induced martensitic phase transformation in NiTi SMA

    Science.gov (United States)

    Gur, Sourav; Frantziskonis, George N.

    2016-10-01

    Martensitic phase transformation in NiTi shape memory alloys (SMA) occurs over a hierarchy of spatial scales, as evidenced from observed multiscale patterns of the martensitic phase fraction, which depend on the material microstructure and on the size of the SMA specimen. This paper presents a methodology for the multiscale tracking of the thermally induced martensitic phase transformation process in NiTi SMA. Fine scale stochastic phase field simulations are coupled to macroscale experimental measurements through the compound wavelet matrix method (CWM). A novel process for obtaining CWM fine scale wavelet coefficients is used that enhances the effectiveness of the method in transferring uncertainties from fine to coarse scales, and also ensures the preservation of spatial correlations in the phase fraction pattern. Size effects, well-documented in the literature, play an important role in designing the multiscale tracking methodology. Molecular dynamics (MD) simulations are employed to verify the phase field simulations in terms of different statistical measures and to demonstrate size effects at the nanometer scale. The effects of thermally induced martensite phase fraction uncertainties on the constitutive response of NiTi SMA is demonstrated.

  1. The Analysis of the Students' English Learning Strategies at the Third Grade of SMA Negeri 3 Gunungsitoli

    OpenAIRE

    Laoli, Adieli

    2010-01-01

    . English Learning Strategies merupakan alat yang digunakan oleh siswa untuk menolongnya dalam memiliki keterampilan berbahasa Inggris. English Learning Strategies terdiri dari cognitive strategy, metacognitive strategy and social strategy. Penelitian ini dilakukan untuk mengetahui apa saja English Learning Strategis yang dilakukan oleh siswa kelas III SMA Negeri 3 Gunungsitoli tahun 2009/2010.

  2. Increased facilitatory connectivity from the pre-SMA to the left dorsal premotor cortex during pseudoword repetition

    DEFF Research Database (Denmark)

    Hartwigsen, Gesa; Saur, Dorothee; Price, Cathy J

    2013-01-01

    that the pre-SMA plays a supervisory role in the generation and subsequent sequencing of motor plans. Diffusion tensor imaging-based fiber tracking in another group of healthy volunteers showed that the functional connection between both regions is underpinned by a direct cortico-cortical anatomical connection....

  3. α-SMA and Ki-67 Immunohistochemistry as Indicators for the Fibrotic Remodeling Process in the Liver of Dogs

    Directory of Open Access Journals (Sweden)

    S. Neumann

    2012-01-01

    Full Text Available Liver cirrhosis is a fatal end-stage of various chronic liver diseases. It develops from persistent liver cell necrosis with resulting fibrosis. Because liver cirrhosis is an irreversible process it is important to recognize the reversible fibrotic stages of the disease. Different markers and staining are currently used to detect fibrosis. Besides plasma markers, some tissue markers are currently being used for this purpose. In this study, we investigated the expression of two immunohistochemical markers (Ki-67, α-SMA in liver diseases with and without fibrosis in dogs and compared their expression with the degree of tissue fibrosis, assessed by Masson trichrome staining. In all the stages of fibrosis, Ki-67 and α-SMA was expressed in the liver tissue. There was no significant difference between Masson trichrome staining which is “gold standard” and expression of Ki-67 or α-smooth muscle actin (SMA. We concluded that Ki-67 and α-SMA can be potentially used as markers for the fibrotic remodeling of the liver.

  4. Sense of agency is related to gamma band coupling in an inferior parietal-preSMA circuitry

    DEFF Research Database (Denmark)

    Ritterband-Rosenbaum, Anina; Nielsen, Jens Bo; Christensen, Mark Schram

    2014-01-01

    In the present study we tested whether sense of agency (SoA) is reflected by changes in coupling between right medio-frontal/supplementary motor area (SMA) and inferior parietal cortex (IPC). Twelve healthy adult volunteers participated in the study. They performed a variation of a line-drawing t......In the present study we tested whether sense of agency (SoA) is reflected by changes in coupling between right medio-frontal/supplementary motor area (SMA) and inferior parietal cortex (IPC). Twelve healthy adult volunteers participated in the study. They performed a variation of a line...... as to the agent of the movement and they reported SoA in approximately 50% of trials when the movement was computer-generated. We tested whether IPC-preSMA coupling was associated with SoA, using dynamic causal modeling (DCM) for induced responses (Chen et al., 2008; Herz et al., 2012). Nine different DCMs were...... constructed for the early and late phases of the task, respectively. All models included two regions: a superior medial gyrus (preSMA) region and a right supramarginal gyrus (IPC) region. Bayesian models selection (Stephan et al., 2009) favored a model with input to IPC and modulation of the forward...

  5. Pre-SMA graymatter density predicts individual differences in action selection in the face of conscious and unconscious response conflict.

    Science.gov (United States)

    van Gaal, Simon; Scholte, H Steven; Lamme, Victor A F; Fahrenfort, Johannes J; Ridderinkhof, K Richard

    2011-02-01

    The presupplementary motor area (pre-SMA) is considered key in contributing to voluntary action selection during response conflict. Here we test whether individual differences in the ability to select appropriate actions in the face of strong (conscious) and weak (virtually unconscious) distracting alternatives are related to individual variability in pre-SMA anatomy. To this end, we scanned 58 participants, who performed a masked priming task in which conflicting response tendencies were elicited either consciously (through primes that were weakly masked) or virtually unconsciously (strongly masked primes), with structural magnetic resonance imaging. Voxel-based morphometry revealed that individual differences in pre-SMA gray-matter density are related to subjects' ability to voluntary select the correct action in the face of conflict, irrespective of the awareness level of conflict-inducing stimuli. These results link structural anatomy to individual differences in cognitive control ability, and provide support for the role of the pre-SMA in the selection of appropriate actions in situations of response conflict. Furthermore, these results suggest that flexible and voluntary behavior requires efficiently dealing with competing response tendencies, even those that are activated automatically and unconsciously.

  6. Analysis-Driven Design Optimization of a SMA-Based Slat-Cove Filler for Aeroacoustic Noise Reduction

    Science.gov (United States)

    Scholten, William; Hartl, Darren; Turner, Travis

    2013-01-01

    Airframe noise is a significant component of environmental noise in the vicinity of airports. The noise associated with the leading-edge slat of typical transport aircraft is a prominent source of airframe noise. Previous work suggests that a slat-cove filler (SCF) may be an effective noise treatment. Hence, development and optimization of a practical slat-cove-filler structure is a priority. The objectives of this work are to optimize the design of a functioning SCF which incorporates superelastic shape memory alloy (SMA) materials as flexures that permit the deformations involved in the configuration change. The goal of the optimization is to minimize the actuation force needed to retract the slat-SCF assembly while satisfying constraints on the maximum SMA stress and on the SCF deflection under static aerodynamic pressure loads, while also satisfying the condition that the SCF self-deploy during slat extension. A finite element analysis model based on a physical bench-top model is created in Abaqus such that automated iterative analysis of the design could be performed. In order to achieve an optimized design, several design variables associated with the current SCF configuration are considered, such as the thicknesses of SMA flexures and the dimensions of various components, SMA and conventional. Designs of experiment (DOE) are performed to investigate structural response to an aerodynamic pressure load and to slat retraction and deployment. DOE results are then used to inform the optimization process, which determines a design minimizing actuator forces while satisfying the required constraints.

  7. PENGARUH PERHATIAN DAN TINGKAT PENDAPATAN ORANG TUA TERHADAP HASIL BELAJAR EKONOMI SISWA KELAS XI DI SMA NEGERI 12 SIJUNJUNG

    Directory of Open Access Journals (Sweden)

    Asli Darnis

    2013-10-01

    Full Text Available Tujuan penelitian ini adalah untuk melihat pengaruh perhatian orang tua dan tingkat pendapatan orang tua terhadap hasil belajar ekonomi siswa kelas XI di SMA Negeri 12 Sijunjung tahun pelajaran 2012/2013. Jenis penelitian yang digunakan adalah kuantitatif. Populasi pada penelitian ini adalah seluruh siswa kelas XI di SMA Negeri 12 Sijunjung sebanyak 49 orang. Instrumen yang digunakan dalam penelitian ini adalah berupa angket. Analisis data digunakan dengan dua cara yaitu: 1 analisis deskriptif, dan 2 analisis induktif. Hasil penelitian menunjukan bahwa: pertama perhatian orang tua terhadap hasil belajar ekonomi siswa kelas XI di SMA Negeri 12 Sijunjung berpengaruh signifikan dengan nilai yaitu 2,819 > 2,021, dan sig 0,072 2,021, dan sig 0,000 yaitu 39,276 > 3,23 dan sig 0,000 < 0,05 maka Ho ditolak dan Ha diterima. Sumbangan yang diberikan oleh perhatian dan pendapatan orang tua terhadap hasil belajar ekonomi siswa kelas XI di SMA Negeri 12 Sijunjung adalah 0,631 atau 63,1%. Perhatian orang tua dan tingkat pendapatan orang tua merupakan faktor penting yang dapat mempengaruhi hasil belajar siswa dalam mata pelajaran ekonomi. Kontribusi dari penelitian ini adalah agar orang tua siswa lebih memperhatikan anaknya mengenai masalah kependidikannya, agar hasil belajar siswa dapat meningkat.

  8. SMN transcript levels in leukocytes of SMA patients determined by absolute real-time PCR

    Science.gov (United States)

    Tiziano, Francesco Danilo; Pinto, Anna Maria; Fiori, Stefania; Lomastro, Rosa; Messina, Sonia; Bruno, Claudio; Pini, Antonella; Pane, Marika; D'Amico, Adele; Ghezzo, Alessandro; Bertini, Enrico; Mercuri, Eugenio; Neri, Giovanni; Brahe, Christina

    2010-01-01

    Spinal muscular atrophy (SMA) is an autosomal recessive neuromuscular disorder caused by homozygous mutations of the SMN1 gene. Three forms of SMA are recognized (type I–III) on the basis of clinical severity. All patients have at least one or more (usually 2–4) copies of a highly homologous gene (SMN2), which produces insufficient levels of functional SMN protein, because of alternative splicing of exon 7. Recently, evidence has been provided that SMN2 expression can be enhanced by pharmacological treatment. However, no reliable biomarkers are available to test the molecular efficacy of the treatments. At present, the only potential biomarker is the dosage of SMN products in peripheral blood. However, the demonstration that SMN full-length (SMN-fl) transcript levels are reduced in leukocytes of patients compared with controls remains elusive (except for type I). We have developed a novel assay based on absolute real-time PCR, which allows the quantification of SMN1-fl/SMN2-fl transcripts. For the first time, we have shown that SMN-fl levels are reduced in leukocytes of type II–III patients compared with controls. We also found that transcript levels are related to clinical severity as in type III patients SMN2-fl levels are significantly higher compared with type II and directly correlated with functional ability in type II patients and with age of onset in type III patients. Moreover, in haploidentical siblings with discordant phenotype, the less severely affected individuals showed significantly higher transcript levels. Our study shows that SMN2-fl dosage in leukocytes can be considered a reliable biomarker and can provide the rationale for SMN dosage in clinical trials. PMID:19603064

  9. HUBUNGAN KETERPAPARAN MEDIA MASSA, PERAN TEMAN SEBAYA TERHADAP TINDAKAN SEKSUAL DI SMA AN-NAAS

    Directory of Open Access Journals (Sweden)

    rika istawati

    2017-06-01

    Full Text Available Masa remaja merupakan masa peralihan antara tahap anak dan dewasa dimana pada masa ini mereka sangat rentan terpapar informasi dari media massa dan teman sebaya terutama seks bebas. Data SKRRI mempunyai teman yang pernah berhubungan seksual pada usia 14-19 tahun dengan persentasi perempuan 37,7% dan laki-laki 30,9% dan Kementerian Komunikasi dan Informasi menyebut 62,1% siswa mengaku penah melakukan hubungan seks. Observasi yang di lakukan oleh peneliti di SMA AN-NAAS Pekanbaru diketahui adanya 2 siswa  yang tertangkap menyimpan dan menonton video porno di handphone dan melalui wawancara peneliti dengan 8 siswi mereka mengatakan adanya 1 siswi yang hamil diluar nikah dan 2 siswi diantaranya mengaku sering datang ketempat yang berisiko terhadap tindakan seksual. Tujuan Penelitian ini untuk mengetahui hubungan keterpaparan media massa dan peran teman sebaya terhadap tindakan seksual. Desain penelitian yang digunakan adalah cross sectional, populasi penelitian adalah seluruh siswa kelas SMA AN-NAAS Pekanbaru yaitu 123 responden. Sampel penelitian 94 orang dengan teknik stratified random sampling. Alat ukur yang digunakan adalah angket, data diolah menggunakan komputer. Analisa data secara univariat dan bivariat dengan uji chi square dengan ketentuan α (0,5. Hasil penelitian didapatkan uji statistik menunjukkan adanya hubungan keterpaparan media massa dengan tindakan seksual dimana nilai p value 0,000 < 0,05, terdapat hubungan yang bermakna antara peran teman sebaya dengan tindakan seksual, dimana p value  0,001 < 0,05. Bagi pihak sekolah diharapkan untuk meningkatkan kegiatan di sekolah seperti ekstrakurikuler dan guru membimbing serta memberi pengawasan yang ketat terhadap siswanya.   

  10. PENGARUH KOMPETENSI MANAJERIAL KEPALA SEKOLAH, LINGKUNGAN, MOTIVASI GURU, TERHADAP PRESTASI SISWA SMA MUHAMMADIYAH KOTA YOGYAKARTA

    Directory of Open Access Journals (Sweden)

    Arif Jamali

    2013-04-01

    Full Text Available Penelitian ini bertujuan untuk mengungkapkan: (1 pengaruh langsung dan tidak langsung kompetensi manajerial kepala sekolah dengan prestasi belajar siswa kompetensi manajerial kepala sekolah dengan prestasi belajar siswa melalui motivasi berprestasi guru; (2 pengaruh langsung dan tidak langsung antara lingkungan sekolah dengan prestasi belajar siswa melalui motivasi berprestasi guru; (3 pengaruh langsung antara motivasi berprestasi guru dengan prestasi belajar siswa. Penelitian ini merupakan penelitian ex-post facto, dengan populasi 318 guru SMA Muhammadiyah Kota Yogyakarta dan sampel 200 orang yang dipilih dengan teknik proportional sampling. Instrumen pengumpulan data berupa kuesioner. Analisis data menggunakan teknik analisis jalur untuk menguji hipotesis penelitian. Hasil penelitian menunjukkan bahwa: (1 terdapat pengaruh langsung dan tak langsung kompetensi manajerial kepala sekolah dengan prestasi belajar siswa, dengan sumbangan efektif 5,52% dengan prestasi belajar siswa melalui motivasi berprestasi guru, (sumbangan efektif sebesar 32,09%; (2 tidak terdapat pengaruh langsung antara lingkungan sekolah dengan prestasi belajar siswa; (3 terdapat pengaruh tidak langsung antara lingkungan sekolah dengan prestasi belajar siswa melalui motivasi berprestasi guru, (sumbangan efektif sebesar 1,04%; (4 terdapat pengaruh langsung antara motivasi berprestasi guru dengan prestasi belajar siswa, (sumbangan efektif sebesar 47,06%. Jadi secara keseluruhan sumbangan yang diberikan oleh kompetensi manajerial kepala sekolah, lingkungan sekolah, motivasi berprestasi guru baik secara langsung maupun tidak terhadap prestasi belajar siswa sebesar 85,71%. Hal ini berarti jika kompetensi manajerial kepala sekolah, lingkungan sekolah dan motivasi berprestasi guru ditingkatkan kualitasnya maka akan berkontribusi positif terhadap peningkatan prestasi belajar siswa SMA Muhammadiyah Kota Yogyakarta. Kata Kunci: kompetensi manajerial kepala sekolah, lingkungan sekolah

  11. PENGGUNAAN BAHAN AJAR DENGAN PENDEKATAN ANDRAGOGI SEBAGAI UPAYA MENINGKATKAN KREATIVITAS DAN HASIL BELAJAR SISWA SMA RSBI

    Directory of Open Access Journals (Sweden)

    M. Umriyah

    2012-01-01

    Full Text Available Andragogi merupakan teori pembelajaran orang dewasa. Konsep pembelajaran orang dewasa merupakan pembelajaran yang berpola non otoriter. Berdasarkan ciri-ciri biologis maupun psikologis sebagian besar siswa SMA telah memasuki usia dewasa, sehingga pendekatan andragogi agaknya lebih sesuai. Penelitian ini merupakan penelitian pengembangan yaitu mengembangkan bahan ajar dengan pendekatan andragogi, bertujuan untuk memperoleh bahan ajar yang dapat meningkatkan kreativitas dan hasil belajar siswa. Subyek penelitian adalah siswa  kelas X-2 SMA Islam Sudirman Ambarawa tahun pelajaran 2010/2011. Pengambilan data dilakukan dengan metode dokumentasi, observasi dan  test hasil belajar.  Hasil penelitian menunjukkan bahwa dengan digunakannya bahan ajar dengan pendekatan andragogi, skor kreativitas  dan hasil test kognitif siswa rata-rata meningkat.Andragogy is adult learning theory. Adult learning concept is learning activity that gets to pattern non authoritarian. Based on biological characteristics and also psychological a large part Senior High School students  have entered adult age, so pedagogy approach (education for children was not suitable anymore for them, it seems that andragogy (education for adult is more suitable. This research is development research which develop learning material in andragogy approach, has an aim to get a learning material that can develop creativity and studying result. The research is executed in X2 class at Sudirman Islamic Senior High School of Ambarawa, academic year 2010 / 2011 which is chosen bases random sampling. Data taking is done by documentation method, observation and learning result test.  Data analysis  indicate   an  improving  of average  value  in creativity and learning result.

  12. INTEGRASI BERPIKIR KRITIS DAN PEDULI LINGKUNGAN MELALUI PEMBELAJARAN GEOGRAFI DALAM MEMBENTUK KARAKTER PESERTA DIDIK SMA

    Directory of Open Access Journals (Sweden)

    Eka Puspitasari

    2016-02-01

    Full Text Available The moral students to induced currents of globalization can be seen from behavior lacking discipline, less responsibility, patriotism and attitude caring environment remain low. This could minimized by character education consistent with the objectives of the curriculum 2013 which includes smart, critical, creative, responsibility, believe, confident, and caring environment. The reality in the field show still had not consistent with the objectives of the curriculum, especially the ability to critical thinking and caring environment. My own concern about the need to begin that students respect and keep the creation. Through geography on matter protect the environment and sustainable development in XI IPS SMA is expected to become a bridge for learners in integrating the ability to critical thinking with the character caring environment. This study attempts to integrate value critical thinking with the character caring environment. Descriptive research was held to technique observation. Critical thinking can build sensibility students in maintaining and protect the environment that can be used sustainably. Penurunan moral peserta didik akibat arus globalisasi dapat dilihat dari perilaku kurang disiplin, kurang tanggung jawab, rasa cinta tanah air dan sikap peduli lingkungan yang masih rendah. Hal ini dapat diminimalisir dengan pembangunan karakter sesuai dengan tujuan Kurikulum 2013 yang meliputi cerdas, kritis, kreatif, tanggung jawab, beriman, percaya diri, dan peduli terhadap lingkungan. Kenyataan di lapangan menunjukkan masih banyak yang belum sesuai dengan tujuan kurikulum, khususnya kemampuan berpikir kritis dan peduli lingkungan. Sikap peduli lingkungan perlu ditanamkan agar peserta didik lebih menghargai dan menjaga ciptaan Tuhan. Melalui Geografi pada materi Pelestarian Lingkungan Hidup dan Pembangunan Berkelanjutan di Kelas XI IPS SMA diharapkan mampu menjadi jembatan bagi peserta didik dalam mengintegrasikan kemampuan berpikir kritis

  13. PEMBELAJARAN MENULIS TEKS PIDATO DAN BERPIDATO KELAS X DI SMA NEGERI 3 SUKOHARJO

    Directory of Open Access Journals (Sweden)

    Jaka Santosa

    2016-02-01

    Full Text Available This study has four aims, (1 the procedure of learning to write text to speech and speech in the classroom, (2 learning strategies and what the media writes text to speech and speech in the classroom, (3 student activity in learning to write text to speech and speech in the classroom, and (4 learning outcomes writing text to speech and speech. This includes descriptive qualitative research which took place in SMA Negeri 3 Sukoharjo. Data in the form of words and actions. Sources of data obtained from sources, events, and documents. Informant is Indonesian teachers and students. Events are learning activities Indonesian X1 class 2nd semester of academic year 2012/2013. The document in question is a document relating to the teaching of writing. Data collection techniques were interviews, observation, and documentary. Research findings in the field, among others, (1 the learning procedure by submitting a text to speech material on speech. Then compose the theme is developed into a framework and final drafting speeches, (2 application of learning strategies to write text to speech and speech with the approach that has been programmed patterns , the approach of process skills and communicative approach, (3 students activate in learning writing text to speech and speech have been carried out by providing learning facilities and trust management using effective learning infrastructure, (4 learning to write text to speech and speech by using the approach of process skills and communicative approaches undertaken by teachers Indonesian subjects in SMA Negeri 3 Sukoharjo obtain following result, students who earn good grades for writing text to speech 80 % and 88 % speech practice, then students who received grades enough to write the speech 20 % and 3 % speech practice, and students who obtain less value to the writing of the speech is not there, to practice speech while there were 9 % .

  14. Pengembangan Naskah Drama Fisika sebagai Media Pembelajaran Fisika SMA berbasis Joyful Learning

    Directory of Open Access Journals (Sweden)

    Neli Fori Karliana

    2015-12-01

    Full Text Available Abstract This research aims to develop a drama script with physics thematic content for senior high school physics- fun based learning and meaningful learning or joyful learning. Joyful learning requires fun learning conditional in the delivery of learning materials. The drama script as a collection of dialog is one form of media that can be used to deliver learning with fun and still has meaningfulness. This development can be used as the basis for research-based instructional media with joyful learning to another subjects. The development research is 4D Thiagarajan Model, and the stage consists of defining, designing, development, and disseminate. This study will describe the process of development of each of its stages. The output of this research is a physics plays eligible to be used as a medium of learning physics in high school. Keywords: a physics drama script, physics learning media, joyful learning Abstrak Penelitian ini bertujuan untuk mengembangkan naskah drama fisika untuk pembelajaran fisika SMA berbasis pembelajaran yang menyenangkan dan bermakna atau joyful learning. Joyfull learning menyaratkan pembelajaran yang menyenangkan dalam penyampaian materi pembelajaran. Naskah drama sebagai kumpulan dialog merupakan salah satu bentuk media yang dapat dimanfaatkan untuk menyampaikan pembelajaran dengan menyenangkan dan tetap memiliki kebermaknaan. Pengembangan naskah drama fisika ini menjadi penelitian yang dapat dijadikan dasar bagi penelitian media pembelajaran berbasis joyfull learning untuk mata pelajaran lainnya. Penelitian pengembangan ini menggunakan model pengembangan 4D Thiagarajan, yang tahapannya terdiri dari pendefinisian, perancangan, pengembangan, dan penyebaran. Penelitian ini akan memaparkan proses pengembangan dari tiap tahapannya. Keluaran dari penelitian ini berupa naskah drama fisika yang layak untuk digunakan sebagai media pembelajaran fisika SMA. Kata-kata kunci: naskah drama fisika, media pembelajaran fisika

  15. Sense of agency is related to gamma band coupling in an inferior parietal-preSMA circuitry

    Directory of Open Access Journals (Sweden)

    Anina eRitterband-Rosenbaum

    2014-07-01

    Full Text Available In the present study we tested whether sense of agency (SoA is reflected by changes in coupling between right medio-frontal/supplementary motor area (SMA and inferior parietal cortex (IPC. Twelve healthy adult volunteers participated in the study. They performed a variation of a line-drawing task (Nielsen, 1963;Fourneret and Jeannerod, 1998, in which they moved a cursor on a digital tablet with their right hand without seeing the hand. Visual feedback displayed on a computer monitor was either in correspondence with or deviated from the actual movement. This made participants uncertain as to the agent of the movement and they reported SoA in approximately 50% of trials when the movement was computer-generated. We tested whether IPC-preSMA coupling was associated with SoA, using dynamic causal modelling (DCM for induced responses (Chen et al., 2008;Herz et al., 2012. Nine different DCMs were constructed for the early and late phases of the task, respectively. All models included two regions: a superior medial gyrus (preSMA region and a right supramarginal gyrus (IPC region. Bayesian models selection (Stephan et al., 2009 favoured a model with input to IPC and modulation of the forward connection to SMA in the late task phase, and a model with input to preSMA and modulation of the backward connection was favoured for the early task phase. The analysis shows that IPC source activity in the 50-60Hz range modulated preSMA source activity in the 40-70 Hz range in the presence of SoA compared with no SoA in the late task phase, but the test of the early task phase did not reveal any differences between presence and absence of SoA. We show that SoA is associated with a directionally specific between frequencies coupling from IPC to preSMA in the higher gamma (ɣ band in the late task phase. This suggests that SoA is a retrospective perception, which is highly dependent on interpretation of the outcome of the performed action.

  16. Axiom turkey genotyping array

    Science.gov (United States)

    The Axiom®Turkey Genotyping Array interrogates 643,845 probesets on the array, covering 643,845 SNPs. The array development was led by Dr. Julie Long of the USDA-ARS Beltsville Agricultural Research Center under a public-private partnership with Hendrix Genetics, Aviagen, and Affymetrix. The Turk...

  17. Clocked combustor can array

    Energy Technology Data Exchange (ETDEWEB)

    Kim, Won-Wook; McMahan, Kevin Weston; Srinivasan, Shiva Kumar

    2017-01-17

    The present application provides a clocked combustor can array for coherence reduction in a gas turbine engine. The clocked combustor can array may include a number of combustor cans positioned in a circumferential array. A first set of the combustor cans may have a first orientation and a second set of the combustor cans may have a second orientation.

  18. SMA actuator material model with self-sensing and sliding-mode control; experiment and multibody dynamics model

    Science.gov (United States)

    Lambert, Tyler Ross; Gurley, Austin; Beale, David

    2017-03-01

    Shape memory alloys (SMA) can be used to create actuators that are simple, high strength, and inexpensive. These benefits come at the cost of low electrical efficiency, moderate lifetime, and complex mechanical behavior that makes them difficult to design into new applications and products. To improve the integration of SMA actuators—in particular thin SMA wires heated by passing electric current through them—into modern mechanical applications, we have created tools for modeling SMA mechanical and thermal behavior in dynamic systems and under feedback controls. Thermo-electro-mechanical constitutive models are implemented in a multibody dynamics software where they are easily applied to an actuator emplaced in a multibody dynamic system. Mechanical behavior is modeled with 1D constitutive equations. The material state determines the electrical resistivity of the material which drives ohmic heating, while thermal cooling is based on a heat transfer analysis of thin cylinders. These models contain states which are very difficult to measure experimentally (such as crystal phase fraction) and thus provide insight into the material behavior and design that experimental results cannot offer. This thermomechanical model is used in conjunction with sliding mode control—historically difficult to simulate in numerically integrated models—to develop a working ball-on-a-beam setup in which the ball position is controlled via current passed through an SMA wire and with application of an original self-sensing method. The constitutive model is developed in the multibody dynamics software MSC ADAMS and validated through the simulation of the same system.

  19. Variable stromal periductular expression of CD34 and smooth muscle actin (SMA in intraductal carcinoma of the breast.

    Directory of Open Access Journals (Sweden)

    Xavier Catteau

    Full Text Available In breast carcinoma, the stromal loss of CD34 expression and acquisition of SMA myofibroblastic features may constitute a prerequisite for tumor invasiveness. However, this hypothesis remains controversial, with some authors describing the loss of CD34 fibrocytes in the absence of SMA myofibroblastic-like cells in the stroma of invasive carcinoma. Others have also described the disappearance of CD34 fibrocytes from in situ carcinoma. To clarify this issue, we compared the distribution of CD34 fibrocytes and SMA reactive myofibroblasts between stromal areas of tumor-free mammary tissue, ductal carcinoma in situ (DCIS and invasive ductal carcinoma (IDC. In addition to 28 IDC, 300 normal duct-lobular units and 600 ducts with DCIS (158 low-grade, 266 intermediate, and 176 high-grade were scored. The relationships between staining patterns and different histological features (grade of DCIS and presence or absence of necrosis were compared. Loss of CD34 expression and acquisition of SMA expression were more frequent in high-grade in situ lesions than in intermediate and low-grade lesions (p<0.001. When necrosis was found in association with grade 2 or 3 DCIS, the decrease in CD34 expression was higher than in lesions without necrosis and that independently of the grade of DCIS (p<0.05. Necrosis did not appear to play a significant role in the expression of SMA (p = 0.35. In all cases, the stroma of invasive carcinomas showed a complete loss of CD34 fibrocytes. Future research on both CD34 fibrocytes and mechanisms stromal changes are essential in the future and may potentially lead to new treatment approaches.

  20. Social/economic costs and health-related quality of life in patients with spinal muscular atrophy (SMA) in Spain.

    Science.gov (United States)

    López-Bastida, Julio; Peña-Longobardo, Luz María; Aranda-Reneo, Isaac; Tizzano, Eduardo; Sefton, Mark; Oliva-Moreno, Juan

    2017-08-18

    The aim of this study was to determine the economic burden and health-related quality of life (HRQOL) of patients with Spinal Muscular Atrophy (SMA) and their caregivers in Spain. This was a cross-sectional and retrospective study of patients diagnosed with SMA in Spain. We adopted a bottom up, prevalence approach design to study patients with SMA. The patient's caregivers completed an anonymous questionnaire regarding their socio-demographic characteristics, use of healthcare services and non-healthcare services. Costs were estimated from a societal perspective (including healthcare costs and non-healthcare costs), and health-related quality of life (HRQOL) was assessed using the EQ-5D questionnaire. The main caregivers also answered a questionnaire on their characteristics and on their HRQOL. A total of 81 caregivers of patients with different subtypes of SMA completed the questionnaire. Based on the reference unitary prices for 2014, the average annual costs per patient were € 33,721. Direct healthcare costs were € 10,882 (representing around 32.3% of the total cost) and the direct non-healthcare costs were € 22,839 (67.7% of the total cost). The mean EQ-5D social tariff score for patients was 0.16, and the mean score of the EQ-5D visual analogue scale was 54. The mean EQ-5D social tariff score for caregivers was 0.49 and their mean score on the EQ-5D visual analogue scale was 69. The results highlight the burden that SMA has in terms of costs and decreased HRQOL, not only for patients but also for their caregivers. In particular, the substantial social/economic burden is mostly attributable to the high direct non-healthcare costs.

  1. Thermophotovoltaic Array Optimization

    Energy Technology Data Exchange (ETDEWEB)

    SBurger; E Brown; K Rahner; L Danielson; J Openlander; J Vell; D Siganporia

    2004-07-29

    A systematic approach to thermophotovoltaic (TPV) array design and fabrication was used to optimize the performance of a 192-cell TPV array. The systematic approach began with cell selection criteria that ranked cells and then matched cell characteristics to maximize power output. Following cell selection, optimization continued with an array packaging design and fabrication techniques that introduced negligible electrical interconnect resistance and minimal parasitic losses while maintaining original cell electrical performance. This paper describes the cell selection and packaging aspects of array optimization as applied to fabrication of a 192-cell array.

  2. Efeito da sequência de mistura nas propriedades de blendas PA6/ABS compatibilizadas com o copolímero SMA Effect from the blending sequence on the properties of PA6/ABS blends compatibilized with SMA copolymer

    Directory of Open Access Journals (Sweden)

    Amanda D. de Oliveira

    2011-01-01

    Full Text Available Blendas de poliamida 6 (PA6 com acrilonitrila-butadieno-estireno (ABS foram preparadas em uma extrusora de rosca dupla, utilizando-se o copolímero estireno-anidrido maleico (SMA, com 7% de anidrido maleico, como compatibilizante. O efeito de três sequências de mistura na microestrutura e propriedades das blendas foi estudado. A morfologia e as propriedades mecânicas dos materiais foram caracterizadas por microscopia eletrônica de transmissão (MET e testes de resistência ao impacto e módulo de elasticidade, respectivamente. Os resultados mostraram que a morfologia e propriedades mecânicas das blendas ternárias foram bastante diferentes e dependem da sequência de mistura. A blenda preparada pela mistura simultânea de todos os componentes, em uma única extrusão, apresentou melhor tenacidade. Por outro lado, quando o ABS e o SMA foram misturados juntos em uma primeira extrusão, antes da incorporação da PA6 em uma segunda extrusão, o valor da resistência ao impacto encontrado foi menor que o da matriz PA6 e da blenda sem compatibilizante PA6/ABS. Evidências de reações químicas entre o compatibilizante SMA e a matriz PA6 também foram investigadas através de reometria de torque.Blends of polyamide 6 (PA6 with acrylonitrile-butadiene-estyrene (ABS were prepared in a twin-screw extruder, using the styrene-maleic anhydride (SMA copolymer containing 7% of maleic anhydride as compatibilizer. The effects from three blending sequences on the microstructure and properties of the blends were investigated. The morphology and mechanical properties of the materials were characterized by transmission electron microscopy and tensile and impact tests. The results showed that the morphology and mechanical properties of ternary blends depend on the sequence of blend preparation. The blend prepared using the mixture of all components in a single-pass extrusion showed the more significant improvement in the material toughness. However, when the

  3. An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts

    Science.gov (United States)

    Danielson, A. L. R.; Swinbank, A. M.; Smail, Ian; Simpson, J. M.; Casey, C. M.; Chapman, S. C.; da Cunha, E.; Hodge, J. A.; Walter, F.; Wardlow, J. L.; Alexander, D. M.; Brandt, W. N.; de Breuck, C.; Coppin, K. E. K.; Dannerbauer, H.; Dickinson, M.; Edge, A. C.; Gawiser, E.; Ivison, R. J.; Karim, A.; Kovacs, A.; Lutz, D.; Menten, K.; Schinnerer, E.; Weiß, A.; van der Werf, P.

    2017-05-01

    We present spectroscopic redshifts of {\\text{}}{S}870μ {{m}} ≳ 2 mJy submillimeter galaxies (SMGs), which have been identified from the ALMA follow-up observations of 870 μm detected sources in the Extended Chandra Deep Field South (the ALMA-LESS survey). We derive spectroscopic redshifts for 52 SMGs, with a median of z = 2.4 ± 0.1. However, the distribution features a high-redshift tail, with ˜23% of the SMGs at z≥slant 3. Spectral diagnostics suggest that the SMGs are young starbursts, and the velocity offsets between the nebular emission and UV ISM absorption lines suggest that many are driving winds, with velocity offsets of up to 2000 km s-1. Using the spectroscopic redshifts and the extensive UV-to-radio photometry in this field, we produce optimized spectral energy distributions (SEDs) using Magphys, and use the SEDs to infer a median stellar mass of {M}\\star = (6 ± 1)× 1010 M {}⊙ for our SMGs with spectroscopic redshift. By combining these stellar masses with the star formation rates (measured from the far-infrared SEDs), we show that SMGs (on average) lie a factor of ˜5 above the so-called “main sequence” at z˜ 2. We provide this library of 52 template fits with robust and uniquely well-sampled SEDs as a resource for future studies of SMGs, and also release the spectroscopic catalog of ˜2000 (mostly infrared-selected) galaxies targeted as part of the spectroscopic campaign.

  4. A retrieval algorithm of hydrometer profile for submillimeter-wave radiometer

    Science.gov (United States)

    Liu, Yuli; Buehler, Stefan; Liu, Heguang

    2017-04-01

    Vertical profiles of particle microphysics perform vital functions for the estimation of climatic feedback. This paper proposes a new algorithm to retrieve the profile of the parameters of the hydrometeor(i.e., ice, snow, rain, liquid cloud, graupel) based on passive submillimeter-wave measurements. These parameters include water content and particle size. The first part of the algorithm builds the database and retrieves the integrated quantities. Database is built up by Atmospheric Radiative Transfer Simulator(ARTS), which uses atmosphere data to simulate the corresponding brightness temperature. Neural network, trained by the precalculated database, is developed to retrieve the water path for each type of particles. The second part of the algorithm analyses the statistical relationship between water path and vertical parameters profiles. Based on the strong dependence existing between vertical layers in the profiles, Principal Component Analysis(PCA) technique is applied. The third part of the algorithm uses the forward model explicitly to retrieve the hydrometeor profiles. Cost function is calculated in each iteration, and Differential Evolution(DE) algorithm is used to adjust the parameter values during the evolutionary process. The performance of this algorithm is planning to be verified for both simulation database and measurement data, by retrieving profiles in comparison with the initial one. Results show that this algorithm has the ability to retrieve the hydrometeor profiles efficiently. The combination of ARTS and optimization algorithm can get much better results than the commonly used database approach. Meanwhile, the concept that ARTS can be used explicitly in the retrieval process shows great potential in providing solution to other retrieval problems.

  5. A submillimeter galaxy illuminating its circumgalactic medium: Lyα scattering in a cold, clumpy outflow

    Energy Technology Data Exchange (ETDEWEB)

    Geach, J. E.; Coppin, K. E. K.; Smith, D. J. B. [Center for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Bower, R. G.; Alexander, D. M.; Swinbank, A. M. [Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Blain, A. W. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Bremer, M. N. [School of Physics, HH Wills Physics Laboratory, Tyndall Avenue, Bristol BS8 1TL (United Kingdom); Chapin, E. L. [XMM SOC, ESAC, Apartado 78, E-28691 Villanueva de la Canada, Madrid (Spain); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University Halifax, NS B3H 3J5 (Canada); Clements, D. L. [Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Dunlop, J. S.; Koprowski, M. P.; Michałowski, M. J. [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Farrah, D. [Virginia Polytechnic Institute and State University Department of Physics, MC 0435, 910 Drillfield Drive, Blacksburg, VA 24061 (United States); Jenness, T. [Joint Astronomy Centre, 660 North A' ohoku Place University Park, Hilo, HI 96720 (United States); Robson, E. I. [UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Scott, D. [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); Spaans, M. [Kapteyn Institute, University of Groningen, PO Box 800, 9700 AV Groningen (Netherlands); Van der Werf, P., E-mail: j.geach@herts.ac.uk [Leiden Observatory, Leiden University, PO box 9513, 2300 RA Leiden (Netherlands)

    2014-09-20

    We report the detection at 850 μm of the central source in SSA22-LAB1, the archetypal 'Lyman-α Blob' (LAB), a 100 kpc scale radio-quiet emission-line nebula at z = 3.1. The flux density of the source, S {sub 850} = 4.6 ± 1.1 mJy, implies the presence of a galaxy or group of galaxies with a total luminosity of L {sub IR} ≈ 10{sup 12} L {sub ☉}. The position of an active source at the center of a ∼50 kpc radius ring of linearly polarized Lyα emission detected by Hayes et al. suggests that the central source is leaking Lyα photons preferentially in the plane of the sky, which undergo scattering in H I clouds at a large galactocentric radius. The Lyα morphology around the submillimeter detection is reminiscent of a biconical outflow, and the average Lyα line profiles of the two 'lobes' are dominated by a red peak, which is expected for a resonant line emerging from a medium with a bulk velocity gradient that is outflowing relative to the line center. Taken together, these observations provide compelling evidence that the central active galaxy (or galaxies) is responsible for a large fraction of the extended Lyα emission and morphology. Less clear is the history of the cold gas in the circumgalactic medium being traced by Lyα: is it mainly pristine material accreting into the halo that has not yet been processed through an interstellar medium (ISM), now being blown back as it encounters an outflow, or does it mainly comprise gas that has been swept-up within the ISM and expelled from the galaxy?.

  6. Improved wedge method for the measurement of sub-millimeter slice thicknesses in magnetic resonance imaging.

    Science.gov (United States)

    Kanazawa, Tsutomu; Ohkubo, Masaki; Kondo, Tatsuya; Miyazawa, Takayuki; Inagawa, Shoichi

    2017-12-01

    The standard method for measuring the slice thickness of magnetic resonance images uses the inclined surface of a wedge (wedge method); it is sensitive to small increases in noise because of the differentiation of the edge response function (ERF) required. The purpose of this study was to improve the wedge method by fitting a curve to the ERF. The curve-fit function was obtained by convolving an ideal ERF (a ramp function) with a Gaussian function to represent ERF blurring. Measurements of 5- and 3-mm slice thicknesses were performed on a 3T scanner using the conventional wedge method, the improved wedge method, and another standard method using an inclined slab (slab method). Subsequently, 0.5- and 0.25-mm slice thicknesses from multiple slices acquired using a three-dimensional sequence were measured using the improved wedge method. When measuring 5-mm slices, the differences in measurements obtained using the improved wedge method and the conventional slab and wedge methods were very small: <0.6% of the 5-mm slice thickness. The difference was ≤1.7% for 3-mm slices. For 0.5- and 0.25-mm slices, the mean values obtained using the improved wedge method were 0.543 ± 0.007 mm and 0.247 ± 0.015 mm, with a 1.2 and 5.9% coefficient of variation across slices, respectively. The improved wedge method is valid and potentially applicable to the measurement of sub-millimeter slice thicknesses.

  7. Metrology Arrangement for Measuring the Positions of Mirrors of a Submillimeter Telescope

    Science.gov (United States)

    Abramovici, Alex; Bartman, Randall K.

    2011-01-01

    The position of the secondary mirror of a submillimeter telescope with respect to the primary mirror needs to be known .0.03 mm in three dimensions. At the time of this reporting, no convenient, reasonably priced arrangement that offers this capability exists. The solution proposed here relies on measurement devices developed and deployed for the GeoSAR mission, and later adapted for the ISAT (Innovative Space Based Radar Antenna Technology) demonstration. The measurement arrangement consists of four metrology heads, located on an optical bench, attached to the secondary mirror. Each metrology head has a dedicated target located at the edge of the primary mirror. One laser beam, launched from the head and returned by the target, is used to measure distance. Another beam, launched from a beacon on the target, is monitored by the metrology head and generates a measurement of the target position in the plane perpendicular to the laser beam. A 100-MHz modulation is carried by a collimated laser beam. The relevant wavelength is the RF one, 3 m, divided by two, because the light carries it to the target and back. The phase change due to travel to the target and back is measured by timing the zero-crossing of the RF modulation, using a 100-MHz clock. In order to obtain good resolution, the 100-MHz modulation signal is down-converted to 1 kHz. Then, the phase change corresponding to the round-trip to the target is carried by a 1-kHz signal. Since the 100-MHz clock beats 100,000 times during one period of the 1-kHz signal, the least-significant-bit (LSB) resolution is LSB = 0.015 mm.

  8. High expression level of Tra2-β1 is responsible for increased SMN2 exon 7 inclusion in the testis of SMA mice.

    Directory of Open Access Journals (Sweden)

    Yu-Chia Chen

    Full Text Available Spinal muscular atrophy (SMA is an inherited neuromuscular disease caused by deletion or mutation of SMN1 gene. All SMA patients carry a nearly identical SMN2 gene, which produces low level of SMN protein due to mRNA exon 7 exclusion. Previously, we found that the testis of SMA mice (smn-/- SMN2 expresses high level of SMN2 full-length mRNA, indicating a testis-specific mechanism for SMN2 exon 7 inclusion. To elucidate the underlying mechanism, we established primary cultures of testis cells from SMA mice and analyzed them for SMN2 exon 7 splicing. We found that primary testis cells after a 2-hour culture still expressed high level of SMN2 full-length mRNA, but the level decreased after longer cultures. We then compared the protein levels of relevant splicing factors, and found that the level of Tra2-β1 also decreased during testis cell culture, correlated with SMN2 full-length mRNA downregulation. In addition, the testis of SMA mice expressed the highest level of Tra2-β1 among the many tissues examined. Furthermore, overexpression of Tra2-β1, but not ASF/SF2, increased SMN2 minigene exon 7 inclusion in primary testis cells and spinal cord neurons, whereas knockdown of Tra2-β1 decreased SMN2 exon 7 inclusion in primary testis cells of SMA mice. Therefore, our results indicate that high expression level of Tra2-β1 is responsible for increased SMN2 exon 7 inclusion in the testis of SMA mice. This study also suggests that the expression level of Tra2-β1 may be a modifying factor of SMA disease and a potential target for SMA treatment.

  9. Gambaran Perilaku Remaja Terhadap Penggunaan Earphone Pada Siswa SMA Negeri Kota Padang

    Directory of Open Access Journals (Sweden)

    Tiara Rahma Zain

    2016-09-01

    Full Text Available AbstrakEarphone adalah alat yang digunakan untukmendengarkan musik dari telepon genggam dan perangkat audio lainnya.Sebuah survey yang dilakukan oleh American Speech Languageand Hearing Association (2006 menemukan bahwa remaja lebih banyak menggunakan perangkat dengar pribadidengan volume keras dan dalam waktu yang lama. Penelitian ini bertujuan untuk mengetahui gambaran perilaku remaja terhadap pengunaan earphone pada siswa SMA Negeri Kota PadangPenelitian ini dilakukan dengan metode deskriptif pada siswa SMAN Negeri Kota Padang yang berjumlah 13.105 orang.Didapatkan sampel berjumlah 427 orang, pengambilan sampel dilakukan dengan teknik Cluster Sampling.Data diambil dengan menggunakan kuesioner.Analisis data menggunakan analisis univarat dengan menggunakan program SPSS (Statistical Product and Service Solution 21.00 for Windows.                Hasil didapatkan proporsi pengguna earphone pada siswa SMA Negeri Kota Padangberjumlah 83,6%. Perilaku siswa dibagi menjadi 3 kategori yaitu pengetahuan, sikap dan tindakan. Hasilnya didapatkan siswa tersebut memiliki pengetahuan dan sikap yang baik terhadap penggunaan earphone dengan persentase 93,4% dan 80,9%. Tindakan siswa ketika menggunakan earphone cukup baik dengan persentasi 66,3%.                Kesimpulan penelitian ini adalah sebagian besar siswa SMA Negeri Kota Padang menggunakan earphone.Siswa tersebut memiliki pengetahuan yang baik mengenai dampak penggunaan earphone dan cara pencegahannya. Siswa juga memiliki sikap yang baik terhadap penggunaan earphone dan bertindak cukup baik ketika menggunakan earphone.Kata Kunci :Earphone, remaja, perilaku AbstractEarphone is a device that used for listening music from their mobile phone and other devices. A survey conducted by American Speech Languageand Hearing Association (2006 found that many teenagers use their personal audio device with maximum volume within a long time. This research aims to describe the teenager

  10. POLA INTERAKSI SOSIAL SISWA PENGGUNA GADGET DI SMA N 1 SEMARANG

    Directory of Open Access Journals (Sweden)

    Doni Harfiyanto

    2015-08-01

    Full Text Available Penelitian ini dilakukan guna melihat pola dan bentuk interaksi sosial antar siswa serta dampak dari penggunaan gadget. Metode penelitian yang digunakan metode kualitatif yang menggambarkan secara objektif pola interaksi sosial yang terjadi pada siswa pengguna gadget. Lokasi penelitian di SMA N 1 Semarang. Pengumpulan data dilakukan dengan cara observasi, wawancara, dan dokumen.  Hasil penelitian adalah didapatkannya gambaran pola interaksi sosial, siswa lebih memilih menggunakan gadget dan jika tidak ditanggapi baru siswa bertemu dengan orang yang dimaksud, bentuk-bentuk interaksi yang terjadi melalui interaksi menggunakan gadget dapat menjadi dua, proses asosiatif  dan proses disasosiatif. Proses asosiatif bentuk-bentuk interaksi sosial yang terjadi menggunakan gadget, siswa banyak melakukan kerjasama mengerjakan tugas, pekerjaan rumah, bertukar informasi, sedangkan proses disasosiatif yaitu konflik, tidak pernah ada konflik yang serius, yang terjadi hanya sebatas perbedaan pendapat serta salah paham yang dapat diselesaikan langsung oleh siswa. Dampak negatif dari penggunaan gadget adalah siswa menjadi lupa waktu. This study was conducted to see the patterns and forms of social interaction between students and the impact caused in connection using gadget. This study used the qualitative approach in order to find out of social interaction pattern in gadget user. The study took place in SMA N 1 Semarang. The data were collected through observation, interview and document review. The study results show that there is social interaction pattern of gadget user students. Students prefer to use gadgets, if there isn’t respon student will go to come to meet the other student. The interaction happened through gadget can be divided in two processes. First, in assossiative process there are cooperation and accomodation, such us many students do assignment, homework, exchange information. Second, in dissossiative, conflict exists. There has never been

  11. ANALISIS KESULITAN SISWA SMA DALAM PEMECAHAN MASALAH MATEMATIKA KELAS XII IPA DI KOTA YOGYAKARTA

    Directory of Open Access Journals (Sweden)

    Ayu Aji Wedaring Tias

    2015-05-01

    Full Text Available Penelitian ini bertujuan untuk mendeskripsikan letak kesulitan siswa yang dominan dan faktor-faktor kesulitan yang dialami siswa SMA dalam memecahkan masalah matematika. Penelitian ini termasuk penelitian deskriptif dengan pendekatan kuantitatif dan kualitatif. Subjek penelitian ini adalah 94 siswa SMA Negeri di Kota Yogyakarta yang berasal dari tiga sekolah dengan kategori tinggi, sedang, dan rendah. Pemilihan subjek penelitian dilakukan dengan stratified proportional random sampling. Pengumpulan data dilakukan dengan menggunakan dokumen, tes, dan wawancara. Analisis data dilakukan dengan metode analisis deskriptif kualitatif dengan pendekatan kuantitatif dan kualitatif yang memberikan gambaran mengenai letak dan faktor kesulitan siswa. Hasil penelitian menunjukkan bahwa kesulitan matematika siswa terletak pada kesulitan mengingat fakta 1,77%, kesulitan memahami fakta 3,54%, kesulitan menerapkan fakta 3,54%, kesulitan menganalisis fakta 10,18%, kesulitan mengingat konsep 1,33%, kesulitan memahami konsep 13,27%, kesulitan menerap-kan konsep 11,95%, kesulitan menganalisis konsep 4,42%, kesulitan memahami prosedur 7,52%, kesulitan menerapkan prosedur 15,49%, kesulitan menganalisis prosedur 16,37%, kesulitan mengingat konsep visual-spasial 1,33%, kesulitan memahami visual-spasial 3,54%, kesulitan menerapakan visual-spasial 3,10%, dan kesulitan menganalisis visual-spasial 2,65%. Faktor-faktor kesulitan yang dialami siswa SMA dalam memecahkan masalah matematika kelas XII program IPA yakni: siswa kurang teliti, tergesa-gesa dalam mengerjakan soal, lupa, kurang waktu untuk mengerjakan soal, cepat menyerah, terkecoh, dan cemas. Kata Kunci: analisis kesulitan, pemecahan masalah matematika, kemampuan pemecahan masalah   AN ANALYSIS OF SENIOR HIGH SCHOOL STUDENTS’ DIFFICULTIES IN MATHEMATICS PROBLEM SOLVING BASED AT GRADE XII OF SCIENCE PROGRAM IN YOGYAKARTA CITY Abstract This research aims to describe the locations of the difficulties and the factors

  12. Electronic Switch Arrays for Managing Microbattery Arrays

    Science.gov (United States)

    Mojarradi, Mohammad; Alahmad, Mahmoud; Sukumar, Vinesh; Zghoul, Fadi; Buck, Kevin; Hess, Herbert; Li, Harry; Cox, David

    2008-01-01

    Integrated circuits have been invented for managing the charging and discharging of such advanced miniature energy-storage devices as planar arrays of microscopic energy-storage elements [typically, microscopic electrochemical cells (microbatteries) or microcapacitors]. The architecture of these circuits enables implementation of the following energy-management options: dynamic configuration of the elements of an array into a series or parallel combination of banks (subarrarys), each array comprising a series of parallel combination of elements; direct addressing of individual banks for charging/or discharging; and, disconnection of defective elements and corresponding reconfiguration of the rest of the array to utilize the remaining functional elements to obtain the desited voltage and current performance. An integrated circuit according to the invention consists partly of a planar array of field-effect transistors that function as switches for routing electric power among the energy-storage elements, the power source, and the load. To connect the energy-storage elements to the power source for charging, a specific subset of switches is closed; to connect the energy-storage elements to the load for discharging, a different specific set of switches is closed. Also included in the integrated circuit is circuitry for monitoring and controlling charging and discharging. The control and monitoring circuitry, the switching transistors, and interconnecting metal lines are laid out on the integrated-circuit chip in a pattern that registers with the array of energy-storage elements. There is a design option to either (1) fabricate the energy-storage elements in the corresponding locations on, and as an integral part of, this integrated circuit; or (2) following a flip-chip approach, fabricate the array of energy-storage elements on a separate integrated-circuit chip and then align and bond the two chips together.

  13. Pengembangan Media e-Learning Mata Pelajaran Teknologi Informasi dan Komunikasi untuk Kelas XI SMA

    Directory of Open Access Journals (Sweden)

    Eril Syahmaidi

    2017-02-01

    Full Text Available Penelitian ini bertujuan untuk menghasilkan media pembelajaran berupa media e-learning Berbasis Video yang valid untuk pelajaran Teknologi Informasi dan Komunikasi. Jenis penelitian ini adalah penelitian pengembangan dengan menggunakan model IDI (Instructional Development Institute. Untuk melihat apakah Media E-Learning Berbasis Video ini valid, dilakukan uji pakar. Desain ini divalidasi oleh 2 orang pakar, pakar perancangan Media E-learning Berbasis Video dan pakar Media E-Learning Berbasis Video. Hasil penelitian menunjukkan bahwa Media E-learning Berbasis Video pada aspek Akses E-Learning (93%, Aspek materi sangat valid (93%, aspek penyajian sangat valid (93%, aspek Media E-learning Berbasis Video sangat  valid (93% serta aspek video Media E-learning sudah sangat valid (94%. Berdasarkan data di atas dapat disimpulkan bahwa Media E-learning Berbasis Video telah valid. Kata kunci: media; e-learning; video; teknologi informasiThis research is aimed to produce E-learning media based on valid, practical, and effective video for Communication and information technology subject. The background of the research is based on the writer observation in SMA N 2 Sungai Penuh. Media development is aimed to help the students to understand the topic about internet by providing online videos which can be accessed anywhere and anytime. This research is a research development which used IDI (Instructional Development Institute model. To prove the validity, practicability, and the effectiveness of this Video-based E-learning media, the writer conducts expert test, one to one evaluation, small group evaluation, and filed test by observing the learning process and learning result of the student. This design is validated by two experts; Video-based E-learning media design expert and Video-based E-learning media development expert. The Video-based E-learning media is tested to 31 students of XI class semester 1 at SMA N 2 Sungai Penuh to figure out the practicability

  14. Kurikulum Tersembunyi Lingkungan di dalam Materi Energi Terbarukan untuk Fisika SMA

    Directory of Open Access Journals (Sweden)

    Desnita Desnita

    2015-12-01

    Full Text Available Abstract Renewable energy resources education, in essence, is the treatment of various topics and issues related to enewable energy resources and technologies as an environmental hidden curriculum in physics education at Senior High School. Based on the statement, environmental Hidden Curriculum in teaching physics concept, especially renewable energy resource was developed. Used research and development method, with step: need assessment, development theoretic models, validation, trial, and revision. The development result is a curriculum with contain: concept of green energy renewal resource and waste cooking oil as a kind of the resources, producing process, and learning strategies to implementation the curriculum. Implementation as trial this curriculum was conducted at a senior high school in South of Jakarta. Didactic exploration improves the learning process, link or integration in physics concept, when worksheets were used in the physics lab and multimedia system. The worksheet content are picture, video, and text or article about green renewable energy resources. Used project based learning and cooperative learning, using the worksheet was improve not only cognitive aspect of the student, but also their skill and attitude to save environmental. Kata-kata Kunci: environmental hidden curricullum, green renewable energy resources, learning strategies. Abstrak Inti dari pendidikan tentang sumber energi terbarukan adalah ujicoba terhadap sejumlah topik dan isu yang terkait dengan sumber energi terbarukan ramah lingkungan dan teknologinya sebagai sebuah kurikulum tersembunyi dalam pendidikan fisika pada tingkat SMA. Berdasarkan alasan tersebut, telah dikembangkan kurikulum lingkungan yang tersembunyi di dalam mengajar konsep fisika, khususnya sumber energi ramah lingkungan. Hasil pengembangan adalah kurikulum yang berisi konsep sumber energi terbarukan ramah lingkungan dan minyak jelanta sebagai salah satu jenisnya, proses produksi, dan

  15. The cryomechanical design of MUSIC: a novel imaging instrument for millimeter-wave astrophysics at the Caltech Submillimeter Observatory

    Science.gov (United States)

    Hollister, Matthew I.; Czakon, Nicole G.; Day, Peter K.; Downes, Thomas P.; Duan, Ran; Gao, Jiansong; Glenn, Jason; Golwala, Sunil R.; LeDuc, Henry G.; Maloney, Philip R.; Mazin, Benjamin A.; Nguyen, Hien Trong; Noroozian, Omid; Sayers, Jack; Schlaerth, James; Siegel, Seth; Vaillancourt, John E.; Vayonakis, Anastasios; Wilson, Philip; Zmuidzinas, Jonas

    2010-07-01

    MUSIC (Multicolor Submillimeter kinetic Inductance Camera) is a new facility instrument for the Caltech Submillimeter Observatory (Mauna Kea, Hawaii) developed as a collaborative effect of Caltech, JPL, the University of Colorado at Boulder and UC Santa Barbara, and is due for initial commissioning in early 2011. MUSIC utilizes a new class of superconducting photon detectors known as microwave kinetic inductance detectors (MKIDs), an emergent technology that offers considerable advantages over current types of detectors for submillimeter and millimeter direct detection. MUSIC will operate a focal plane of 576 spatial pixels, where each pixel is a slot line antenna coupled to multiple detectors through on-chip, lumped-element filters, allowing simultaneously imaging in four bands at 0.86, 1.02, 1.33 and 2.00 mm. The MUSIC instrument is designed for closed-cycle operation, combining a pulse tube cooler with a two-stage Helium-3 adsorption refrigerator, providing a focal plane temperature of 0.25 K with intermediate temperature stages at approximately 50, 4 and 0.4 K for buffering heat loads and heat sinking of optical filters. Detector readout is achieved using semi-rigid coaxial cables from room temperature to the focal plane, with cryogenic HEMT amplifiers operating at 4 K. Several hundred detectors may be multiplexed in frequency space through one signal line and amplifier. This paper discusses the design of the instrument cryogenic hardware, including a number of features unique to the implementation of superconducting detectors. Predicted performance data for the instrument system will also be presented and discussed.

  16. Dust in External Galaxies

    OpenAIRE

    Calzetti, Daniela

    2009-01-01

    Existing (Spitzer Space Telescope) and upcoming (Herschel Space Telescope) facilities are deepening our understanding of the role of dust in tracing the energy budget and chemical evolution of galaxies. The tools we are developing while exploring the local Universe will in turn become pivotal in the interpretation of the high redshift Universe when near--future facilities (the Atacama Large Millimeter Array [ALMA], the Sub--Millimeter Array [SMA], the Large Millimeter Telescope [LMT], the Jam...

  17. Signal to Noise Ratio Maximization in Quiet Zone Acquisitions for Range Assessment at Sub-millimeter Wavelengths

    Directory of Open Access Journals (Sweden)

    A. Muñoz-Acevedo

    2012-06-01

    Full Text Available This paper proposes a quiet zone probing approach which deals with low dynamic range quiet zone acquisitions. Lack of dynamic range is a feature of millimeter and sub-millimeter wavelength technologies. It is consequence of the gradually smaller power generated by the instrumentation, that follows a f^α law with frequency, being α≥1 variable depending on the signal source’s technology. The proposed approach is based on an optimal data reduction scenario which redounds in a maximum signal to noise ratio increase for the signal pattern, with minimum information losses. After theoretical formulation, practical applications of the technique are proposed.

  18. Fast computation of the Narcissus reflection coefficient for the Herschel far-infrared/submillimeter-wave Cassegrain telescope

    Science.gov (United States)

    Lucke, Robert L.; Fischer, Jacqueline; Polegre, Arturo M.; Beintema, Douwe A.

    2005-10-01

    Placement of a scatter cone at the center of the secondary of a Cassegrain telescope greatly reduces Narcissus reflection. To calculate the remaining Narcissus reflection, a time-consuming physical optics code such as GRASP8 is often used to model the effects of reflection and diffraction. Fortunately, the Cassegrain geometry is sufficiently simple that a combination of theoretical analysis and Fourier propagation can yield rapid, accurate results at submillimeter wavelengths. We compare these results with those from GRASP8 for the heterodyne instrument for the far-infrared on the Herschel Space Observatory and confirm the effectiveness of the chosen scatter cone design.

  19. Carbon nanotube nanoelectrode arrays

    Science.gov (United States)

    Ren, Zhifeng; Lin, Yuehe; Yantasee, Wassana; Liu, Guodong; Lu, Fang; Tu, Yi

    2008-11-18

    The present invention relates to microelectode arrays (MEAs), and more particularly to carbon nanotube nanoelectrode arrays (CNT-NEAs) for chemical and biological sensing, and methods of use. A nanoelectrode array includes a carbon nanotube material comprising an array of substantially linear carbon nanotubes each having a proximal end and a distal end, the proximal end of the carbon nanotubes are attached to a catalyst substrate material so as to form the array with a pre-determined site density, wherein the carbon nanotubes are aligned with respect to one another within the array; an electrically insulating layer on the surface of the carbon nanotube material, whereby the distal end of the carbon nanotubes extend beyond the electrically insulating layer; a second adhesive electrically insulating layer on the surface of the electrically insulating layer, whereby the distal end of the carbon nanotubes extend beyond the second adhesive electrically insulating layer; and a metal wire attached to the catalyst substrate material.

  20. Dynamically Reconfigurable Microphone Arrays

    Science.gov (United States)

    2011-05-01

    Static + 2 Wireless Using only a standard computer sound card, a robot is limited to binaural inputs. Even when using wireless microphones, the audio...Abstract—Robotic sound localization has traditionally been restricted to either on-robot microphone arrays or embedded microphones in aware...a microphone array has a significant impact on the mathematics of sound source localization. Arrays, for instance, are commonly designed to

  1. PENGEMBANGAN E-MODULE BERBASIS PROBLEM BASED LEARNING MATA PELAJARAN KIMIA UNTUK SISWA KELAS X SMA NEGERI 8 MALANG

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    Arvi Sekar Farenta

    2016-06-01

    Full Text Available Developing an E-Module of Problem Based Learning, Chemistry for The 11th Grader of SMA Negeri 8 Malang. This development aims to produce a media by validation proccess which is used effectively on learning. Method used by Lee & Owens(2004 is assessment/ analysis; design; development; implementation; and evaluation. The result of  research shows that the media of learning is valid and it is used effectively on learning. Pengembangan E-Module berbasis Problem Based Learning Mata Pelajaran Kimia untuk Siswa Kelas X SMA Negeri 8 Malang. Pengembangan ini bertujuan untuk menghasilkan media pembelajaran yang valid, sehingga dapat mengefektifkan pembelajaran. Metode yang digunakan model Lee & Owens(2004 yaitu: assessment/ analysis; design; development; implementation; dan evaluation. Hasil penelitian menunjukkan bahwa media pembelajaran valid dan efektif digunakan dalam proses pembelajaran.

  2. SISTEM PENDUKUNG KEPUTUSAN PENERIMAAN CALON SISWA BARU DI SMA NEGERI 1 NEGERI KATON MENGGUNAKAN METODE SIMPLE ADDITIVE WEIGHTING (SAW

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    Noca Yolanda Sari

    2017-05-01

    Full Text Available SMA Negeri 1 Negeri  Katon  merupakan salah satu sekolah unggulan di daerah Pesawaran. Setiap tahun ajaran baru, sekolah mengadakan penerimaan dan penyeleksian calon siswa, untuk menentukan proses penyeleksian siswa di  SMA Negeri 1 Negeri  Katon . Dalam proses penyeleksian ini sering timbul permasalahan seperti terbatasnya panitia seleksi yang menyebabkan kesalahan menganalisis calon siswa yang diterima atau ditolak , serta lamanya hasil seleksi siswa. Pada penelitian ini akan diangkat suatu kasus yaitu mencari alternative terbaik bedasarkan kriteria-kriteria yang telah ditentukan dengan menggunakan metode Simple Additive Weighting (SAW. Penelitian dilakukan dengan mencari nilai bobot untuk setiap atribut, kemudian dilakukan proses perankingan yang akan menentukan alternatif yang optimal, yaitu siswa terbaik.

  3. Self-Biased-SMA Drive PU Microgripper with Force Sensing in Visual Servo

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    Ren-Jung Chang

    2013-06-01

    Full Text Available An innovative design of a polyurethane microgripper system with force sensor is developed for the measurement of gripping force in vision-based control. A microgripper mechanism integrated with a force sensing arm is fabricated by an excimer laser. The microgripper is actuated by a self-biased-SMA (Shape Memory Alloy actuator. A computer-vision method through the ERES (Extended Regional Edge Statistics algorithm is employed to track the motion of gripper. The position information of the gripping point together with the deflection of the force sensing arm is utilized for sensing force. A fuzzy expert with a PI controller in a visual servo is employed to test the performance of sensing the gripping force in grasping of 38μm diameter metal rod. In the performance test, the microgripper system provides a maximum gripping size of 40μm, a maximum force resolution of 1μN and a maximum gripping force of 58μN.

  4. PENGEMBANGAN PERANGKAT PEMBELAJARAN BIOLOGI BERORIENTASI PENGEMBANGAN KECERDASAN MAJEMUK SISWA PADA KONSEP SEL KELAS XI SMA

    Directory of Open Access Journals (Sweden)

    Vidya Chaerunnisa

    2017-01-01

    Full Text Available This study aimed to determine the feasibility of the development of student’s multiple intelligence-oriented learning instrument on the cells concept in grade XI senior high school. Research and Development (R & D method was conducted in this research. This research was developed four components in the cell concept learning instrument that included syllabus, lesson plan, student’s worksheet, and assessment instrument. From the four components were obtained an average score of 93.76% with a decent category. The time limited test was conducted in July-August 2016, at SMAN 4 Kota Serang and SMA Prisma Sanjaya Kota Serang. Based on students' responses as a user, it was obtained the value of 79.78% with a fair category. Based on the results of expert test and limited test scale, the learning instrument development of multiple intelligences learning-oriented can be applied for the learning process in the cell concept for grade XI in senior high school.

  5. ANALISIS SOAL JENJANG KOGNITIF TAKSONOMI BLOOM REVISI PADA BUKU SEKOLAH ELEKTRONIK (BSE BIOLOGI SMA

    Directory of Open Access Journals (Sweden)

    Aa Juhanda

    2016-11-01

    Penelitian ini bertujuan untuk menganalisis kemunculan soal jenjang kognitif Bloom Revisi pada Buku Sekolah Elektronik (BSE Biologi SMA. Subjek penelitian adalah 1.650 soal yang terdapat pada BSE Edisi 2009. Instrumen yang digunakan adalah lembar analisis dokumen yang di dalamnya memuat informasi seperti kode soal, soal, dan jenis tingkatan kognitif taksonomi Bloom Revisi. Analisis data dilakukan secara kuantitatif dan kualitatif. Hasil penelitian menunjukkan bahwa rerata persentase kemunculan cukup tinggi diperoleh pada soal yang mengembangkan keterampilan berpikir tingkat rendah (Lower-Order Thinking Skills yaitu soal C1 (mengingat sebesar 46,60% dan C2 (memahami sebesar 47,99%, meskipun untuk C3 (menerapkan persentasenya masih rendah (0,28%. Rerata persentase kemunculan soal yang mengembangkan keterampilan tingkat tinggi (Higher-Order Thinking Skills mulai dari soal C4 (menganalisis sampai dengan C6 (mencipta memiliki rerata persentase yang rendah. Oleh karena itu, kemunculan soal jenjang kognitif Bloom Revisi pada BSE khususnya yang mengembangkan Higher-Order Thinking Skills masih perlu untuk ditingkatkan.

  6. A thermomechanical constitutive model for superelastic SMA wire with strain-rate dependence

    Science.gov (United States)

    Zhu, Songye; Zhang, Yunfeng

    2007-10-01

    The recent increased use of shape memory alloys (SMAs) for civil engineering applications manifests the need for a high-fidelity constitutive model which considers the material's strong dependence on the loading rate. This paper presents an improved thermomechanical constitutive model with strain-rate dependence for predicting the uniaxial superelastic behavior of shape memory alloys. The proposed constitutive model, which is formulated within a thermomechanical framework, is comprised of three principal parts: a mechanical law, an energy balance equation, and a transformation kinetics rule. The analytical derivation of the model and experimental test results for superelastic NiTi wires are described in this paper. The prediction made by this phenomenological model shows good agreement with experimental data for superelastic NiTi wires at various loading rates. Through a comparison with experimental results, the proposed constitutive model was evaluated for several key characteristics of superelastic behavior such as reduction of hysteresis area, increase of transformation plateau, and temperature change with strain rate. The proposed constitutive model offers a useful tool for the design and simulation of superelastic SMA-based devices in civil engineering applications.

  7. Rancang Bangun Sistem Informasi Akademik Berbasis Web ( studi kasus: SMA Swasta Harapan I Medan

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    Haida Dafitri, Marina Elsera

    2017-10-01

    Full Text Available Submission of academic information to students, parents / guardians conducted at private high school SMA Harapan I Medan are still very ineffective and efficient both in terms of delivery time and in terms of finance. This is because the academic delivery is still manual in oral, written or via phone or SMS one by one. The impact of the process is the slow process of delivering academic information and the amount of expenditure in the delivery of information. To overcome these problems, then the academic community wants to improve the delivery of academic information systems using computerized technology. The purpose of the change is by building a School of Academic Information System (SISFO Web-based SCRUM model. The system is built to produce academic information such as value and achievement of students in web-based schools that can be utilized by the academic staff to make it easier in conveying academic information to students, parents / guardians. This system includes and through several aspects of functionality, reliability, efficiency, and usability. And the scrum model used in the design of this system has a framework for building, developing and managing an ever-changing product. Keywords: Information , Academic, Scrum Model, Web

  8. ANALISIS CEDERA OLAHRAGA DALAM AKTIVITAS PENDIDIKAN JASMANI PADA SISWA SMA NEGERI 1 NALUMSARI

    Directory of Open Access Journals (Sweden)

    Hery Supriyadi

    2017-02-01

    Full Text Available The purpose of this study is: To determine the body that are often exposed to injury and the cause of injury to the physical education sports activities in SMAN 1 Jepara regency Nalumsari academic year 2015/2016. The method used is quantitative descriptive. The technique of collecting data using questionnaires, interviews, observation, and documentation. The results of the 84 number of students who suffered an ankle injury (38 students, the fingers (34 students, toe (28 students of the head, neck and wrist (26 students, calves (22 students, chest (18 students , shoulders, elbows, back (16 students and thighs (10 students. The cause of the injury is the movement of the body mistakenly (44 students, physical condition declined (38 students, bumping bodies with friends (34 students, lack of warm (32 students, the movement of excess body (30 students body condition unfit (26 students , the length of the body that are not the same (24 students and trauma due to injury never happened (20 students .Simpulan of students of SMA Negeri 1 Nalumsari Jepara students are exposed parts of the body most injured an ankle injury that caused excessive body movement

  9. KESALAHAN BERBAHASA TATARAN SINTAKSIS PADA PENULISAN PENGALAMAN PRIBADI SISWA KELAS X SMA

    Directory of Open Access Journals (Sweden)

    Yustina Sako

    2017-11-01

    Full Text Available This research aims to describe the level of syntax errors that include aspects of phrases and sentences on writing personal experience grade X SENIOR HIGH SCHOOL Stella Gratia Atambua. This research uses qualitative research designs with the kind of descriptive research. The results of this study indicate that many students make a mistake on a sentence structure that covers ten aspects. These findings prove that students pay attention to the use of grammar in writing, lack of vocabulary which belonged to the students, the influence of the use of local languages, and teachers less use of grammar in writing. Penelitian ini bertujuan mendeskripsikan kesalahan tataran sintaksis yang meliputi aspek frase dan kalimat pada penulisan pengalaman pribadi siswa kelas X SMA Stella Gratia Atambua. Penelitian ini menggunakan rancangan penelitian kualitatif dengan jenis penelitian deskriptif. Hasil penelitian ini menunjukkan bahwa siswa banyak melakukan kesalahan pada struktur kalimat yang meliputi sepuluh aspek. Temuan tersebut membuktikan bahwa siswa kurang memerhatikan penggunaan tata bahasa dalam menulis, minimnya kosakata yang dimiliki siswa, pengaruh penggunaan bahasa daerah, dan guru kurang memerhatikan penggunaan tata bahasa dalam menulis.

  10. PENGEMBANGAN MEDIA PEMBELAJARAN BERBASIS MULTIMEDIA INTERAKTIF UNTUK MENINGKATKAN PEMAHAMAN MATERI BIOTEKNOLOGI MODERN SISWA KELAS XII SMA

    Directory of Open Access Journals (Sweden)

    Sri Riani

    2015-03-01

    Full Text Available Pesatnya perkembangan ilmu dan teknologi menjadikan bioteknologi sebagai salah satu bidang ilmu dalam biologi yang harus dikuasai sejak dini oleh siswa. Berbagai permasalahan yang muncul dalam pembelajaran bioteknologi di sekolah, salah satunya adalah penggunaan media yang kurang tepat sehingga menyebabkan materi tersebut sulit dipahami oleh siswa. Masalah lain adalah adanya keterbatasan waktu, sementara materi yang disampaikam lebih banyak bersifat aplikatif dan abstrak terutama pada bioteknologi modern yang membutuhkan waktu relatif panjang. Tujuan dari penelitian pengembangan ini adalah mengembangkan media pembelajaran berbasis multimedia interaktif untuk meningkatkan pemahaman materi bioteknologi modern pada siswa kelas XII SMA. Model penembangan yang digunakan mengacu pada langkah-langkah pengembangan Borg & Gall (1983 yang dimodifikasi dari Sukmadinata (2009 yang meliputi tiga kegiatan besar, yaitu: studi pendahuluan, pengembangan dan validasi. Penelitian ini dilakukan pada tanggal 19 Januari sampai 28 Maret 2013 di MAN Malang 2 Batu. Hasil penelitian pengembangan ini menghasilkan produk multimedia interaktif yang telah melalui proses uji coba dan telah dilakukan beberapa kali revisi berdasarkan saran ahli materi dan ahli media serta komentar dari siswa sasaran uji coba. Multimedia interaktif yang dihasilkan memiliki kualifikasi sangat baik dan hasil eksperiment juga menunjukkan bahwa terdapat perbedaan tingkat pengetahuan materi bioteknologi modern antara sebelum dan setelah menggunakan multimedia interaktif, yaitu dari nilai rata-rata sebelum menggunakan media (pretest (54,03 meningkat menjadi (92,36 setelah menggunakan media (postest.

  11. Pengaruh Intensitas Kesertaan dalam Program Pendidikan Nonformal terhadap Prestasi Belajar Siswa SMA di Kota Malang

    Directory of Open Access Journals (Sweden)

    Rifa’Atul Machmudah

    2014-04-01

    Full Text Available Penelitian ini bertujuan untuk menganalisis pengaruh intensitas kesertaan dalam program pendidikan nonformal seperti bimbingan belajar (bimbel, les privat, kursus, belajar mandiri, dan bel-ajar dengan teman sebaya terhadap prestasi belajar siswa SMA Kota Malang. Penelitian ini mengguna-kan rancangan kuantitatif dengan desain korelasional yang dilanjutkan dengan regresi lima variabel. Teknik pengambilan sampel menggunakan teknik stratified proportional random sampling. Teknik analisa yang digunakan dalam penelitian adalah deskriptif, regresi sederhana, dan regresi ganda. Ha-sil penelitian jurusan IPA sumbangan efektif (determinasi intensitas mengikuti bimbel sebesar 17,1%, les privat 12,5%, kursus 4,8%, dan belajar mandiri 1,2%, jurusan IPS sumbangan efektif (deter-minasi intensitas mengikuti bimbel sebesar 32,6%, les privat 6,2%, kursus 2,4%, belajar mandiri 10,2%, dan belajar kelompok 0,1%, jurusan Bahasa sumbangan efektif (determinasi intensitas mengi-kuti bimbel sebesar 0,4%, les privat 0,8%, kursus 0,3%, belajar mandiri 9,3%, dan belajar kelompok 1,3%. Jika diregresi secara ganda maka sumbangan efektif program pendidikan nonformal informal jurusan IPA sebesar 32,2%, pada jurusan IPS sebesar 13,3%, dan pada jurusan Bahasa sebesar 88,7%, posisi relatif prestasi akademik, tingkat kelulusan, dan status sosial ekonomi pada kategori menengah, rencana tindak lanjut pasca pendidikan formal adalah melanjutkan pendidikan di perguruan tinggi.  Kata kunci: pendidikan nonformal, bimbingan belajar, pendidikan luar sekolah

  12. PENGEMBANGAN MODUL KAWASAN RUMAH PANGAN LESTARI (KRPL BERBASIS PROYEK UNTUK SISWA SMA

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    Hamim Thohari Mahfudhillah

    2017-03-01

    Full Text Available Ministry of Agriculture formed Sustainable Food House Regional Program (SFHRP program with the aim to meet the needs of the household vegetables to realize food self-sufficiency. In many areas, the implementation of the SFHRP program implementation has not run well and has not made a great contribution to society. One effort that SFHRP program can run well is by introducing SFHRP program through formal education, it is necessary for such learning a resource module which contains materials about the SFHRP program. Research was conducted adapting development stages of ADDIE model. This research resulted projects-based SFHRP program module for senior high schools that have been feasible to be used or implemented in the field. Kementerian Pertanian membentuk program KRPL dengan tujuan untuk memenuhi kebutuhan sayur tingkat rumah tangga sehingga terwujud kemandirian pangan. Di berbagai daerah, pelaksanaan program KRPL belum berjalan dengan baik dan belum memberikan kontribusi yang besar bagi masyarakat. Salah satu upaya agar program KRPL dapat berjalan dengan baik, yaitu dengan mengenalkan program KRPL melalui pendidikan formal, untuk itu diperlukan suatu sumber belajar seperti modul yang memuat materi tentang program KRPL. Penelitian pengembangan yang dilakukan mengadaptasi tahapan model pengembangan ADDIE. Hasil penelitian pengembangan ini yaitu dihasilkannya modul program KRPL berbasis proyek untuk SMA yang telah layak untuk digunakan atau diimplementasikan di lapangan.

  13. SIKAP DAN PEMERTAHANAN BAHASA INDONESIA SISWA KELAS X SMA INTERNASIONAL BUDI MULIA DUA YOGYAKARTA

    Directory of Open Access Journals (Sweden)

    Rizki Amalia Sholihah

    2015-10-01

    Full Text Available Penelitian ini bertujuan untuk mengetahui sikap dan pemertahanan terhadap bahasa Indonesia pada siswa kelas X kelas internasional dan non-internasional di SMA Budi Mulia Dua. Sikap dan pemertahanan bahasa tersebut ditinjau dari tes menulis siswa. Penelitian ini merupakan penelitian deskriptif dengan pendekatan gabungan antata pendekatan kualitatif dan kuantitatif. Hasil penelitian berdasarkan kuesioner menunjukkan bahwa di kelas X GAC terdapat 9 siswa yang memiliki pemerta-hanan bahasa negatif dan kelas X Asia terdapat 2 siswa yang memiliki pemertahanan yang negatif. Berdasarkan hasil menulis, pada kelas GAC hanya terdapat 1 siswa yang memiliki pemertahanan negatif dan di kelas X Asia terdapat 2 siswa. Kata kunci: bahasa Indonesia, sikap bahasa, pemertahanan bahasa   LANGUAGE ATTITUDE AND MAINTENANCE ON INDONESIAN LANGUAGE CLASS X STUDENTS BUDI MULIA DUA INTERNATIONAL SENIOR HIGH SCHOOL YOGYAKARTA Abstract This study is aimed at understanding language attitude and language maintenance on Indone-sian language to Class X students of international class and non-international class at Budi Mulia Dua Senior High School. The language attitude and language maintenance were viewed from students’s writing test. The result of this research from questionnaire, X Asia there are 2 students who have negative language maintenance, and in Class X GAC, there are 9 students who have negative language maintenance. From writing performance in class X Asia there are 2 students who have negative language maintenance and in Class X GAC, there are 1 students. Key words: Indonesian language, language attitude, language maintenance

  14. Pengembangan Laboratorium Virtual Rangkaian RLC Seri berbasis LabVIEW untuk Pembelajaran Fisika SMA

    Directory of Open Access Journals (Sweden)

    Kurnia Risca Maulinda

    2017-10-01

    Full Text Available Rangkaian RLC seri merupakan salah satu topik penting pada materi pelajaran listrik arus bolak-balik. Dalam topik ini terdapat fenomena resonansi rangkaian RLC, yang secara  eksperimental memerlukan perangkat eksperimen cukup kompleks, sehingga tidak mudah untuk divisualisasikan fenomenanya dalam proses pembelajaran. Pada penelitian ini telah dikembangkan laboratorium virtual rangkaian RLC seri berbasis LabVIEW yang dapat digunakan untuk kegiatan eksperimen simulasi dalam mempelajari fenomena resonanasi rangkaian listrik. Menggunakan prosedur penelitian dan pengembangan, laboratorium virtual rangkaian RLC seri telah diujicobakan dan divalidasi. Hasil validasi masuk dalam kategori sangkat baik, sehingga laboratorium virtual RLC seri layak untuk digunakan dalam pembelajaran fisika SMA.Series RLC circuit is one of the important topics on the subject of the AC electric current. In this topic, there is a resonance phenomenon of RLC circuit, which experimentally requires a fairly complex experimental device, so it is not easy to visualize the phenomenon in the learning process. In this research has been developed a virtual laboratory series RLC circuit based on LabVIEW which can be used for simulation experiment in studying the phenomenon of resonance of electrical circuit. Using research and development procedures, the virtual laboratory series RLC circuit has been tested and validated. The validation results fall into very good categories, so the RLC virtual laboratory is feasible for use in high school physics learning.

  15. PENGARUH PENGGUNAAN PEMBELAJARAN KOOPERATIF TIPE STAD BERBANTUAN WINGEOM TERHADAP KEMAMPUAN PEMECAHAN MASALAH GEOMETRI SISWA SMA

    Directory of Open Access Journals (Sweden)

    Ikhsanudin Ikhsanudin

    2014-06-01

    Full Text Available This research is a quasi-experimental with pre-test and post-test non-equivalent group design. The population in this research is all of the students on class X in SMA Negeri 1 Marga Tiga and the sampling technique is total sampling. Data are collected by documentation and test. Data are analyzed with descriptive statistics to compare the mean scores of N-Gain  obtained by each student.  The results of the analysis shows that (1 the student’s geometry problem solving ability with cooperative learning STAD is higher than the conventional learning, (2 the student’s geometry problem solving ability with wingeom software in cooperative learning STAD is higher than the conventional learning, (3 the student’s geometry problem solving ability with wingeom software in cooperative learning STAD is higher than without using wingeom software. This research shows that the cooperative learning STAD by using the wingeom software has a significant effect on the high school students’ geometry problem-solving ability. The finding of this research shows that the students are still having difficulties in solving the problems, especially when the students have to look back whether the finishing is right or not.

  16. Pemanfaatan Teknologi Informasi untuk Sistem Informasi Manajemen Sekolah: Studi Kasus pada SMA 78 Jakarta

    Directory of Open Access Journals (Sweden)

    Ayuliana Ayuliana

    2011-12-01

    Full Text Available Databases to manage data related to student and school are required to support the implemented information technology applications. This study aims to analyze and design a database system that supports the school management information systems, especially for SMA 78 Jakarta as a case study. Included in the system are the students and teachers data management, the management of school tuition, and the management of learning materials and assignments for students. This research uses data collection methods, with a literature study, questionnaires, interviews, observation, and studying the data obtained from the school. Analyses were performed on the results of questionnaires, interviews and observations to identify user needs. The design used conceptual and logical database system design. The result achieved is the application for school management information system that can be used by students, teachers and school officials in supporting learning process and school administration. The developed application is expected to be a medium for students and teachers to share information in teaching and learning activities and administrative processes. 

  17. PENDIDIKAN KARAKTER POLA MUHAMMADIYAH (Studi Kasus SMA Muhammadiyah 1 dan MA Muallimin Yogyakarta

    Directory of Open Access Journals (Sweden)

    Kuswono Kuswono

    2013-09-01

    Full Text Available This research aims to find out the sources of character education at Islamic schools, character- building values application and actualization. This research was conducted in SMA Mubammadiyah I Yogyakarta and MA Muallimin Muhammadiyah Yogyakarta.The result of research showed that teacher's perception on character education relied on Islamic precepts to create akhakul karimah-human beings. The sources of character education included Quran and as=Sunnah/Hadist as well as Ijtihad. The character value implantation was carried out through learning in the classroom, precedents from figures, teachers and peers, well-behaving familiarization in the presence of rule and order, personality report, and extracurricular activities in knowledge, skill, sport, art, and organization fields. The form of character-building values actualization emphasized more on the Islamic activities such as collectively shalat, reading and reciting Quran, social service, participating actively in IPM, hizbul wathan, and tapak suci organizational activities. In addition, there were kader inti/an, mubalig jumat, mubalig hijarah, fasting, Friday sermon, becoming the orator in pengajian, and flag ceremony. Such these activities reflected on religious, cooperative, leadership, loving-to-homeland, social care, environmental care, and creative values.Keywords: Education, Character, Muhammadiyah.

  18. Penggunaan Media Sosial Sesuai Nilai Luhur Budaya di Kalangan Siswa SMA

    Directory of Open Access Journals (Sweden)

    Roswita Oktavianti

    2017-12-01

    Full Text Available The youth as a generation of social media users holds great control over the dissemination of information in groups and families. Social media like Facebook, Twitter, Instagram, Path, becomes a medium of expression and self-existence, and the spread of news and information. In this case, social media becomes a means of spreading the noble values of the culture that is acculturated in one's self and their surrounding environment. However, the younger generation is less aware of the role of social media as a means of spreading the noble values of culture. Information and news in social media are accepted immediately without verifying the truth. Social media is more dominantly used as a means of self-expression, without a positive contribution to other social media users, or, in this case, followers. Therefore, the younger generation needs to be briefed on the use of social media as well as the importance of using social media as a medium that communicates the noble values of culture. The briefing was conducted at SMA Santo Kristoforus 1, West Jakarta. By using survey method to know the effectiveness of the briefing, the younger generation' understanding of the use of social media before and after the briefing. The outcome of this activity, all students are able to show which information that should or should not be disseminated, able to recognize or identify false news (hoaxes, false news information, and the steps taken when receiving the false news.

  19. Upaya Guru Bimbingan dan Konseling dalam Mencegah Perilaku Bullying di SMA Negeri Se Kota Padang

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    Riri Yunika

    2013-09-01

    Full Text Available Bullying is a behavior consciously done by someone to abuse and hurt others. Ideally, the guidance and counseling teachers (BK teachersare demanded to give attentions in preventing bullying behavior. However, in fact, the BK teachers have not plan special programs yet to prevent the bullying behavior among students in school. This research aims to describe the understanding of BK teachers about the concept of bullying behavior. Then, it aims to describe the treatment of the BK given by the teachers to the students. Finally, it aims to describe the cooperation among the BK teachers within the school. This research is kind of descriptive research. The population of this research is all of the BK teachers of SMA Negeri (State school for secondary education in Padang. Sample is taken by using area sampling and simple random sampling techniques. Generally, the result implicates that the BK teachers have done preventing efforts toward bullying behavior among students in the school. Thus, the teachers should increase the understanding in reference to bullying behavior among students to prevent the behavior in school.

  20. Rectenna array measurement results

    Science.gov (United States)

    Dickinson, R. M.

    1980-01-01

    The measured performance characteristics of a rectenna array are reviewed and compared to the performance of a single element. It is shown that the performance may be extrapolated from the individual element to that of the collection of elements. Techniques for current and voltage combining were demonstrated. The array performance as a function of various operating parameters is characterized and techniques for overvoltage protection and automatic fault clearing in the array demonstrated. A method for detecting failed elements also exists. Instrumentation for deriving performance effectiveness is described. Measured harmonic radiation patterns and fundamental frequency scattered patterns for a low level illumination rectenna array are presented.

  1. Integrated Avalanche Photodiode arrays

    Energy Technology Data Exchange (ETDEWEB)

    Harmon, Eric S.

    2017-04-18

    The present disclosure includes devices for detecting photons, including avalanche photon detectors, arrays of such detectors, and circuits including such arrays. In some aspects, the detectors and arrays include a virtual beveled edge mesa structure surrounded by resistive material damaged by ion implantation and having side wall profiles that taper inwardly towards the top of the mesa structures, or towards the direction from which the ion implantation occurred. Other aspects are directed to masking and multiple implantation and/or annealing steps. Furthermore, methods for fabricating and using such devices, circuits and arrays are disclosed.

  2. Integrated avalanche photodiode arrays

    Science.gov (United States)

    Harmon, Eric S.

    2015-07-07

    The present disclosure includes devices for detecting photons, including avalanche photon detectors, arrays of such detectors, and circuits including such arrays. In some aspects, the detectors and arrays include a virtual beveled edge mesa structure surrounded by resistive material damaged by ion implantation and having side wall profiles that taper inwardly towards the top of the mesa structures, or towards the direction from which the ion implantation occurred. Other aspects are directed to masking and multiple implantation and/or annealing steps. Furthermore, methods for fabricating and using such devices, circuits and arrays are disclosed.

  3. Pengaruh Kemampuan Membaca Pemahaman Dan Penguasaan Kosakata Terhadap Keterampilan Menulis Argumentasi Pada Peserta Didik SMA Di Depok

    OpenAIRE

    Irwansyah, Nur; Ikhwati, Azhari

    2016-01-01

    This study generally aims to determine student's reading comprehension, vocabulary mastery of the students, and the ability to write arguments class XI High School in Depok, particularly SMA Tugu Ibu 1 Depok, while specifically to get a picture of whether there is influence between reading comprehension student's ability to write arguments, obtain information whether there is influence between students' vocabulary mastery of the ability to write arguments, get a picture there is influence rea...

  4. PENGARUH BENTUK TES FORMATIF ASSOSIASI PILIHAN GANDA DENGAN REWARD DAN PUNISHMENT SCORE PADA PEMBELAJARAN MATEMATIKA SISWA SMA

    Directory of Open Access Journals (Sweden)

    Slamet Slamet

    2014-02-01

    Full Text Available ABSTRAK                                          Penelitian ini mengkaji dan menemukan bentuk tes formatif yang efektif yaitu dengan penggunaan bentuk tes formatif assosiasi  pilahan ganda dengan reaward dan punishment score pada pembelajaran matematika siswa SMA. Adapun objek penelitian yang akan dilakukan pada penelitian ini adalah SMA Provinsi DKI Jakarta. Sampel yang diambil adalah SMA N 16 Jakarta Barat dan SMA N 46 Jakarta Timur. Tes formatif adalah tes yang diberikan secara periodik dalam proses pembelajaran yang bertujuan untuk memantau perkembangan siswa. Selain itu, sebagai bentuk evaluasi pembelajaran tes formatif diberikan untuk mengetahui bagaimana umpan balik siswa dalam proses pembelajaran untuk perbaikan konteks pembelajaran di dalam kelas. Dari hasiil pengujian diperoleh p-value (Asymp Sig kelas eksperimen adalah 0,355 > 0,05 = a, dan p-value (Asymp Sig kelas kontrol adalah 0,031 0.05 = α, and the p-value (Sig Asymp control class is 0.031 < 0.05 = α, then H0 is rejected. This shows the effect of giving formative test multiple choice form of association with reward math scores on learning outcomes of students on the subject of the derivative function. Thus, multiple-choice tests formative associations with reward and punishment score that matches the effective teaching high school mathematics implemented in the learning process, especially in the evaluation of learning. Keywords      :  association Formative Test double increments, reaward and punishment scores, Learning Outcomes

  5. Pose de la première pierre du bâtiment SMA18 du Cern

    CERN Multimedia

    CERN Press Office. Geneva

    1999-01-01

    On 30 April 1999, Jean Pépin, Sénateur for the Department of the Ain and President of the Conseil Général, and Professor Luciano Maiani the Director-General of CERN will lay the foundation stone of Building SMA18, financed by the Department of the Ain in the framework of France's special contribution to CERN's Large Hadron Collider (LHC) project.

  6. PENGEMBANGAN E-MODULE BERBASIS PROBLEM BASED LEARNING MATA PELAJARAN KIMIA UNTUK SISWA KELAS X SMA NEGERI 8 MALANG

    OpenAIRE

    Arvi Sekar Farenta; Sulton Sulton; Punaji Setyosari

    2016-01-01

    Developing an E-Module of Problem Based Learning, Chemistry for The 11th Grader of SMA Negeri 8 Malang. This development aims to produce a media by validation proccess which is used effectively on learning. Method used by Lee & Owens(2004) is assessment/ analysis; design; development; implementation; and evaluation. The result of  research shows that the media of learning is valid and it is used effectively on learning. Pengembangan E-Module berbasis Problem Based Learning Mata Pelajaran ...

  7. An Analysis of Code Switching by the English Teachers in the Classroom at SMA Darma Yudha Pekanbaru

    OpenAIRE

    Prabowo, Prakas; ', Jismulatif; ', Dahnilsyah

    2017-01-01

    This descriptive qualitative research was aimed to know the frequency of types and functions of code switching by the English teachers in the classroom at SMA Darma Yudha Pekanbaru. The sample of the research was consisted of three English teachers. In order to gather the data, the writer used observation, recorder and students' questionnaire to support the data. The types of code switching appearing in the classroom were observed based on the theory proposed by Poplack, while the functions o...

  8. High spatial resolution brain functional MRI using submillimeter balanced steady-state free precession acquisition

    Energy Technology Data Exchange (ETDEWEB)

    Wu, Pei-Hsin; Chung, Hsiao-Wen [Department of Electrical Engineering, National Taiwan University, Taipei 10617, Taiwan (China); Tsai, Ping-Huei [Imaging Research Center, Taipei Medical University, Taipei 11031, Taiwan and Department of Medical Imaging, Taipei Medical University Hospital, Taipei Medical University, Taipei 11031, Taiwan (China); Wu, Ming-Long, E-mail: minglong.wu@csie.ncku.edu.tw [Institute of Medical Informatics, National Cheng-Kung University, Tainan 70101, Taiwan and Department of Computer Science and Information Engineering, National Cheng-Kung University, Tainan 70101, Taiwan (China); Chuang, Tzu-Chao [Department of Electrical Engineering, National Sun Yat-Sen University, Kaohsiung 80424, Taiwan (China); Shih, Yi-Yu [Siemens Limited Healthcare Sector, Taipei 11503, Taiwan (China); Huang, Teng-Yi [Department of Electrical Engineering, National Taiwan University of Science and Technology, Taipei 10607, Taiwan (China)

    2013-12-15

    Purpose: One of the technical advantages of functional magnetic resonance imaging (fMRI) is its precise localization of changes from neuronal activities. While current practice of fMRI acquisition at voxel size around 3 × 3 × 3 mm{sup 3} achieves satisfactory results in studies of basic brain functions, higher spatial resolution is required in order to resolve finer cortical structures. This study investigated spatial resolution effects on brain fMRI experiments using balanced steady-state free precession (bSSFP) imaging with 0.37 mm{sup 3} voxel volume at 3.0 T. Methods: In fMRI experiments, full and unilateral visual field 5 Hz flashing checkerboard stimulations were given to healthy subjects. The bSSFP imaging experiments were performed at three different frequency offsets to widen the coverage, with functional activations in the primary visual cortex analyzed using the general linear model. Variations of the spatial resolution were achieved by removing outerk-space data components. Results: Results show that a reduction in voxel volume from 3.44 × 3.44 × 2 mm{sup 3} to 0.43 × 0.43 × 2 mm{sup 3} has resulted in an increase of the functional activation signals from (7.7 ± 1.7)% to (20.9 ± 2.0)% at 3.0 T, despite of the threefold SNR decreases in the original images, leading to nearly invariant functional contrast-to-noise ratios (fCNR) even at high spatial resolution. Activation signals aligning nicely with gray matter sulci at high spatial resolution would, on the other hand, have possibly been mistaken as noise at low spatial resolution. Conclusions: It is concluded that the bSSFP sequence is a plausible technique for fMRI investigations at submillimeter voxel widths without compromising fCNR. The reduction of partial volume averaging with nonactivated brain tissues to retain fCNR is uniquely suitable for high spatial resolution applications such as the resolving of columnar organization in the brain.

  9. Kilovoltage beam Monte Carlo dose calculations in submillimeter voxels for small animal radiotherapy.

    Science.gov (United States)

    Bazalova, Magdalena; Zhou, Hu; Keall, Paul J; Graves, Edward E

    2009-11-01

    Small animal conformal radiotherapy (RT) is essential for preclinical cancer research studies and therefore various microRT systems have been recently designed. The aim of this paper is to efficiently calculate the dose delivered using our microRT system based on a microCT scanner with the Monte Carlo (MC) method and to compare the MC calculations to film measurements. Doses from 2-30 mm diameter 120 kVp photon beams deposited in a solid water phantom with 0.2 x 0.2 x 0.2 mm3 voxels are calculated using the latest versions of the EGSnrc codes BEAMNRC and DOSXYZNRC. Two dose calculation approaches are studied: a two-step approach using phase-space files and direct dose calculation with BEAMNRC simulation sources. Due to the small beam size and submillimeter voxel size resulting in long calculation times, variance reduction techniques are studied. The optimum bremsstrahlung splitting number (NBRSPL in BEAMNRC) and the optimum DOSXYZNRC photon splitting (Nsplit) number are examined for both calculation approaches and various beam sizes. The dose calculation efficiencies and the required number of histories to achieve 1% statistical uncertainty--with no particle recycling--are evaluated for 2-30 mm beams. As a final step, film dose measurements are compared to MC calculated dose distributions. The optimum NBRSPL is approximately 1 x 10(6) for both dose calculation approaches. For the dose calculations with phase-space files, Nsplit varies only slightly for 2-30 mm beams and is established to be 300. Nsplit for the DOSXYZNRC calculation with the BEAMNRC source ranges from 300 for the 30 mm beam to 4000 for the 2 mm beam. The calculation time significantly inc