WorldWideScience

Sample records for bowing

  1. Fuel rod bowing

    International Nuclear Information System (INIS)

    The purpose of this investigation was to quantify the extent of fuel rod bowing in Westinghouse pressurized water reactors and to assess the effects of fuel rod bowing on plant safety and reliability. An empirical bow correlation was developed based on data from irradiated assemblies. Analyses conducted with these conservative empirical predictions show that: (1) generically identified DNBR margins are adequate to offset DNBR reductions due to rod bow, (2) the present design practice of increasing the highest calculated core peaking factor is sufficient to account for all deviations, including the effects of rod bow, and (3) fretting and corrosion of bowed rods are negligible. These conclusions indicate that fuel rod bowing results in no impact on plant safety or reliability

  2. Bow Crushing Forces

    DEFF Research Database (Denmark)

    Pedersen, Preben Terndrup

    1996-01-01

    The purpose of these notes is to present a basis for the estimation of the internal collision forces between conventinal merchant vessels and large volume offshore structures in the form of gravity-supported offshore installations and bridges crossing international shipping routes.The main emphas...... is on the presentation of impact loads on fixed offshore structures due to bow collisions. The crushing forces are determined as functions of vessels size, vessels speed, bow profile, collision angles and eccentric impacts....

  3. Fuel pin bowing in CAGR

    International Nuclear Information System (INIS)

    Some of the more important mechanisms by which pin bowing can occur in Advanced Gas Cooled Reactors are examined. These include creep relaxation of the stresses which occur when thermal bowing is restrained and asymmetric axial clad creep. The clad temperature changes which accompany such bowing are also investigated and the theoretical results briefly compared with the empirical behaviour. (author)

  4. Bow shock: Power aspects

    Science.gov (United States)

    Sedykh, P. A.

    2014-07-01

    It is clear that the primary energy source for magnetospheric processes is the solar wind, but the process of energy transfer from the solar wind into the magnetosphere, or rather, to convecting magnetospheric plasma, appears to be rather complicated. Bow shock is a powerful transformer of the solar wind kinetic energy into the gas dynamic and electromagnetic energy. A jump of the magnetic field tangential component at front crossing means that the front carries an electric current. The solar wind kinetic energy partly transforms to gas kinetic and electromagnetic energy during its passage through the bow shock front. The transition layer (magnetosheath) can use part of this energy for accelerating of plasma, but can conversely spend part its kinetic energy on the electric power generation, which afterwards may be used by the magnetosphere. Thereby, transition layer can be both consumer (sink) and generator (source) of electric power depending upon special conditions. The direction of the current behind the bow shock front depends on the sign of the IMF Bz-component. It is this electric current which sets convection of plasma in motion.

  5. Atelier Bow-Wow DELIGHTS

    DEFF Research Database (Denmark)

    Kajita, Masashi

    2011-01-01

    Atelier Bow-Wow bruger det engelske ord 'delights' til at beskrive en arkitektonisk kvalitet, der dækker over fornøjelse, nydelse og glæde. Interviewet med Yoshiharu Tskukamoto, der sammen med Momoyo Kaijima leder Atelier Bow-Wow, udforsker baggrunden for begrebet 'delights', hvordan det spiller...

  6. Articulated coordination of the right arm underlies control of bow parameters and quick bow reversals in skilled cello bowing

    OpenAIRE

    JuliusVerrel; MarjorieHinesWoollacott

    2014-01-01

    Stringed instrument bowing is a complex coordinative motor skill acquired though years of intense practice. We apply a novel “freezing” analysis to investigate how movement at different joints contributes to bow transport (movement amplitude), stabilization of bow parameters (angle, velocity) during bow movements, and quick reversals of bow direction (acceleration amplitude). Participants were ten advanced or professional cellists (19–32 years, at least 10 years of practice) and ten age-match...

  7. Statistical modeling of violin bowing parameter contours

    OpenAIRE

    Maestre G??mez, Esteban

    2009-01-01

    We present a framework for modeling right-hand gestures in bowed-string instrument playing, applied to violin. Nearly non-intrusive sensing techniques allow for accurate acquisition of relevant timbre-related bowing gesture parameter cues. We model the temporal contour of bow transversal velocity, bow pressing force, and bow-bridge distance as sequences of short segments, in particular B??ezier cubic curve segments. Considering different articulations, dynamics, and contexts, a number of n...

  8. Earth's bow shock: Power aspects.

    Science.gov (United States)

    Sedykh, Pavel

    2012-07-01

    The process of energy transfer from the solar wind into the magnetosphere, or rather, to convecting magnetospheric plasma, appears to be rather complicated. The bow shock front is the main converter of solar wind kinetic energy into electromagnetic energy [Ponomarev, Sedykh, J. of Atm. Solar-Terr. Phys. V. 68. 2006; Ponomarev, Sedykh et al., Geomagn. and Aeron., 2009]. Solar wind undergoes significant changes in its parameters during its passing through the bow shock front. Indeed, at the bow point, when crossing the front, the magnetic field tangential component and magnetic energy density increase by factors of almost 4 and approximately 15, respectively. In describing the bow shock, we followed [Whang, 1987; Ponomarev et al., 2006]. A jump of the magnetic field tangential component when crossing the bow shock front means that the front carries an electric current. It is possible to show that electric current is diverging in this layer, that is the front is the generator of the current. Since plasma with magnetic field passes through the bow shock front, electric field arises in the front reference system. Thus, the bow shock front is a source of electric power. The direction of electric current behind the bow shock front depends on the sign of the IMF Bz-component. It is this current which sets convection in motion. Energetically, this external current is necessary for maintaining convection of plasma in the inhomogeneous system (geomagnetosphere). The generator at the bow shock front can be a sufficient source of power for supplying energy to substorm processes [Sedykh, Sun and Geosphere, 2011]. The sign of power does not depend on the IMF sign, and energy flux is always directed into the magnetosphere. The magnitude of the power is different and is realized in different regions of the magnetosphere depending on the IMF direction. When the Bz-component is negative, the electric convection field is larger, with the anticonvection field being smaller, than for

  9. Articulated coordination of the right arm underlies control of bow parameters and quick bow reversals in skilled cello bowing

    Directory of Open Access Journals (Sweden)

    JuliusVerrel

    2014-08-01

    Full Text Available Stringed instrument bowing is a complex coordinative motor skill acquired though years of intense practice. We apply a novel “freezing” analysis to investigate how movement at different joints contributes to bow transport (movement amplitude, stabilization of bow parameters (angle, velocity during bow movements, and quick reversals of bow direction (acceleration amplitude. Participants were ten advanced or professional cellists (19-32 years, at least 10 years of practice and ten age-matched novice players. Arm and bow movements were recorded using 3D motion capture. To assess how performance depends on articulated use of the right arm, actual data were compared to surrogate data, generated by artificially removing movement at (“freezing” individual joints in measured arm movements. This analysis showed that both elbow and shoulder significantly contribute to bow transport in experts, while only the shoulder contributed to bow transport in novices. Moreover, experts showed more strongly increased variability of bow parameters and reduced acceleration amplitudes at bow reversals for surrogate compared to actual movement data. This indicates that movement across joints was organized to reduce bow variability and achieve quick bow reversals. Corresponding effects were less pronounced or absent in the novices, in particular for the wrist and elbow. Our results demonstrate the importance of articulated use of the right arm and clarify the contribution of different joints in experts’ bowing performance. Moreover, they support theories of motor control and learning that propose exploitation of biomechanical degrees of freedom, in particular of distal joints, as a critical component in skilled motor performance.

  10. Dielectric Bow-tie Nanocavity

    CERN Document Server

    Lu, Qijing; Zou, Chang-Ling

    2013-01-01

    We propose a novel dielectric bow-tie nanocavity consisting of two tip-to-tip opposite triangle semiconductor nanowires, whose end faces are coated by silver nanofilms. Based on the advantages of the dielectric slot and tip structures, and the high reflectivity from the silver mirror, light can be confined in this nanocavity with low loss. We demonstrate that the mode excited in this nanocavity has a deep subwavelength mode volume of 2.8*10^-4 um3 and a high quality factor of 4.9*10^4 (401.3), consequently an ultrahigh Purcell factor of 1.6*10^7 (1.36*10^5), at 4.5 K (300 K) around the resonance wavelength of 1550 nm. This dielectric bow-tie nanocavity may find applications for integrated nanophotonic circuits, such as high-efficiency single photon source, thresholdless nanolaser, and cavity QED strong coupling experiments.

  11. Dielectric Bow-tie Nanocavity

    OpenAIRE

    Lu, Qijing; Shu, Fang-Jie; Zou, Chang-Ling

    2013-01-01

    We propose a novel dielectric bow-tie nanocavity consisting of two tip-to-tip opposite triangle semiconductor nanowires, whose end faces are coated by silver nanofilms. Based on the advantages of the dielectric slot and tip structures, and the high reflectivity from the silver mirror, light can be confined in this nanocavity with low loss. We demonstrate that the mode excited in this nanocavity has a deep subwavelength mode volume of 2.8*10^-4 um3 and a high quality factor of 4.9*10^4 (401.3)...

  12. 75 FR 40820 - City of Broken Bow, Oklahoma; Project No. 12470-001-Oklahoma Broken Bow Re-Regulation Dam...

    Science.gov (United States)

    2010-07-14

    ... Energy Regulatory Commission City of Broken Bow, Oklahoma; Project No. 12470-001--Oklahoma Broken Bow Re... included in, or eligible for inclusion in, the National Register of Historic Places at the Broken Bow Re..., 2010, for the Broken Bow Re-Regulation Dam Hydroelectric Project No. 12470 is revised to add...

  13. 75 FR 33802 - City of Broken Bow, OK; Broken Bow Re-Regulation Dam; Hydropower Project; Notice of Proposed...

    Science.gov (United States)

    2010-06-15

    ... Energy Regulatory Commission City of Broken Bow, OK; Broken Bow Re-Regulation Dam; Hydropower Project... eligible for inclusion in, the National Register of Historic Places at the Broken Bow Re-Regulation Dam... the Broken Bow Re-Regulation Dam Hydropower Project would be fulfilled through the...

  14. Dielectric bow-tie nanocavity.

    Science.gov (United States)

    Lu, Qijing; Shu, Fang-Jie; Zou, Chang-Ling

    2013-12-15

    We propose a novel dielectric bow-tie (DBT) nanocavity consisting of two opposing tip-to-tip triangle semiconductor nanowires, whose end faces are coated by silver nanofilms. Based on the advantages of the dielectric slot and tip structures, and the high reflectivity of the silver mirror, light can be confined in this nanocavity with low loss. We demonstrate that at 4.5 K (300 K) around the resonance wavelength of 1550 nm, the mode excited in this nanocavity has a deep subwavelength mode volume of 2.8×10(-4) μm³ and a high quality factor of 4.9×10(4) (401.3), corresponding to an ultrahigh Purcell factor of 1.6×10(7) (1.36×10(5)). This DBT nanocavity may find applications for integrated nanophotonic circuits, such as high-efficiency single photon sources, thresholdless nanolasers, and strong coupling in cavity quantum electrodynamics experiments. PMID:24322245

  15. Modelling the bending/bowing of composite beams such as nuclear fuel: The BOW code

    Energy Technology Data Exchange (ETDEWEB)

    Tayal, M. (Atomic Energy of Canada Ltd., Sheridan Park, Ontario. CANDU Operations)

    1989-09-01

    Arrays of tubes are used in many engineered structures, such as in nuclear fuel bundles and in steam generators. The tubes are bend (bow) due to in-service temperatures and loads. Assessments of bowing of nuclear fuel elements can help demonstrate the integrity of fuel and of surrounding components, as a function of operating conditions such as channel power. The BOW code calculates the bending of composite beams such as fuel elements, due to gradients of temperature and due to hydraulic forces. The deflections and rotations are calculated in both lateral directions, for given conditions of temperatures. Wet and dry operation of the sheath can be simulated. BOW accounts for the following physical phenomena: circumferential and axial variations in the temperatures of the sheath and of the pellet; cracking of pellets; grip and slip between the pellets and the sheath; hydraulic drag; restraints from endplates, from neighbouring elements, and from the pressure-tube; gravity; concentric or eccentric welds between endcaps and endplate; neutron flux gradients; and variations of material properties with temperature. The code is based on fundamental principles of mechanics. The governing equations are solved numerically using the finite element method. Several comparisons with closed-form equations show that the solutions of BOW are accurate. BOW's predictions for initial in-reactor bow are also consistent with two post-irradiation measurements. (orig.).

  16. D3BIER, a program for calculating bowing reactivities

    International Nuclear Information System (INIS)

    The report gives a description of the code D3BIER, which calculates the reactivity effects due to subassembly bowing in three-dimensional hexagonal geometry, based on pre-calculated bowing coefficients and subassembly bowing lines. The input and check of data and the data transfer correspond to the standard of the INTERATOM nuclear code system IANUS. The data blocks have variable dimensioning

  17. The Statics of the Traditional Hungarian Composite Reflex Bow

    Directory of Open Access Journals (Sweden)

    Sándor Horváth

    2006-04-01

    Full Text Available The operation of the Hungarian bow raises several fascinating mechanicalquestions. To answer these questions a good number of experiments and calculations needto be made, moreover the mechanical model of the bow is needed to be prepared whichappropriately confirm the results of experiments. Teachers in the Bánki Donát MechanicalEngineering College of Budapest Polytechnic set up a small laboratory in 1997 in order tostudy and measure the physical characteristics of traditional bows. The mechanicalanalysis of bows is based on the experiments gained in the laboratory and the results ofmeasurements. The knowledge acquired about the mechanical model of bows facilitates notonly the analysis of the traditional Hungarian bow, but also provides a good foundation forthe comparison from the technical point of view of various composite reflex bows belongingto different historic ethnic groups.

  18. Suprathermal electrons at Saturn's bow shock

    CERN Document Server

    Masters, A; Sergis, N; Stawarz, L; Fujimoto, M; Coates, A J; Dougherty, M K

    2016-01-01

    The leading explanation for the origin of galactic cosmic rays is particle acceleration at the shocks surrounding young supernova remnants (SNRs), although crucial aspects of the acceleration process are unclear. The similar collisionless plasma shocks frequently encountered by spacecraft in the solar wind are generally far weaker (lower Mach number) than these SNR shocks. However, the Cassini spacecraft has shown that the shock standing in the solar wind sunward of Saturn (Saturn's bow shock) can occasionally reach this high-Mach number astrophysical regime. In this regime Cassini has provided the first in situ evidence for electron acceleration under quasi-parallel upstream magnetic conditions. Here we present the full picture of suprathermal electrons at Saturn's bow shock revealed by Cassini. The downstream thermal electron distribution is resolved in all data taken by the low-energy electron detector (CAPS-ELS, 18 keV) measured a suprathermal electron signature at 31 of 508 crossings, where typically onl...

  19. Bow shock formation in a complex plasma.

    Science.gov (United States)

    Saitou, Y; Nakamura, Y; Kamimura, T; Ishihara, O

    2012-02-10

    A bow shock is observed in a two-dimensional supersonic flow of charged microparticles in a complex plasma. A thin conducting needle is used to make a potential barrier as an obstacle for the particle flow in the complex plasma. The flow is generated and the flow velocity is controlled by changing a tilt angle of the device under the gravitational force. A void, microparticle-free region, is formed around the potential barrier surrounding the obstacle. The flow is bent around the leading edge of the void and forms an arcuate structure when the flow is supersonic. The structure is characterized by the bow shock as confirmed by a polytropic hydrodynamic theory as well as numerical simulation. PMID:22401079

  20. Bowing and interaction of fast reactor subassemblies

    International Nuclear Information System (INIS)

    Deformations of the subassembly structural components, in particular the bowing of the hexagonal wrapper which encloses the pin bundles, due to stainless steel swelling as a result of fast neutron irradiation give rise to operational and safety problems especially in large breeder reactors where the neutron flux is much larger than in smaller reactors. The restraint on bowing induces heavy restraint loads and high stresses in the wrapper, which tend to limit the target burn-up of the fast reactor fuels. Therefore, a realistic analysis has to include the phenomenon of creep to determine the extent to which the stresses in the wrapper would be relaxed due to both thermally induced and irradiation induced creep. Apart from this, determination of deformations of the subassemblies in the core due to the interaction among them is also necessary. (author)

  1. A survey for Hα pulsar bow shocks

    International Nuclear Information System (INIS)

    We report on a survey for Hα bow shock emission around nearby γ-detected energetic pulsars. This survey adds three Balmer-dominated neutron star bow shocks to the six previously confirmed examples. In addition to the shock around Fermi pulsar PSR J1741–2054, we now report Hα structures around two additional γ-ray pulsars, PSR J2030+4415 and PSR J1509–5850. These are the first known examples of Hα nebulae with pre-ionization halos. With new measurements, we show that a simple analytic model can account for the angular size and flux of the bow shocks' apices. The latter, in particular, provides a new pulsar probe and indicates large moments of inertia and smaller distances than previously assumed in several cases. In particular, we show that the re-measured PSR J0437–4715 shock flux implies I = (1.7 ± 0.2) × 1045/(f HIsin i) g cm2. We also derive a distance d ≈ 0.72 kpc for the γ-ray only pulsar PSR J2030+4415 and revised distances for PSRs J1959+2048 (1.4 kpc) and J2555+6535 (∼1 kpc), smaller than the conventional DM-estimated values. Finally, we report upper limits for 94 additional LAT pulsars. An estimate of the survey sensitivity indicates that for a warm neutral medium filling factor φWNM ∼ 0.3 there should be a total of approximately nine Hα bow shocks in our LAT-targeted survey; given that seven such objects are now known, a much larger φWNM seems problematic.

  2. The sacred weapon: bow and arrow combat in Iran

    Directory of Open Access Journals (Sweden)

    Manouchehr Moshtagh Khorasani

    2012-07-01

    Full Text Available The following article presents the development of the bow and arrow, and its important role in the history of Iran. The bow always played an important role not only on the battlefield, but also in hunting. It was also considered as a sacred weapon and additionally a royal symbol. Bow and arrow were considered as a superior weapon in comparison with other types of weapons because one could fight with them at a safer distance as one offered by swords, maces and axes. The first part of the article presents a short history of the bow in Iran. Based on historical Persian manuscripts, the next part explains the structure of the composite bow and the materials used for making it. The third part describes some types of bows based on the material, place of production, the usage, and bow type based on the length of the bow and the arrows. The following part talks about different types of arrows based on morphology of arrowheads, the type of plume/feather, the material of the shaft, the material of the arrowhead, the length of arrows, the target of arrows, the place of production of arrowheads and terms for describing its different features of an arrowhead. Then, the article talks about different types of thumb rings, bowstrings, quivers and bow cases and arrow guides for shooting short arrows. The next part discusses different principles of archery as explained in Persian manuscripts. Finally the article describes different archery targets.

  3. Discovery of a bow shock around Vela X-1

    CERN Document Server

    Kaper, L; Augusteijn, T; Goudfrooij, P; Patat, N; Zijlstra, A A; Waters, R; Kaper, Lex; Loon, Jacco van; Augusteijn, Thomas; Goudfrooij, Paul; Patat, Nando; Zijlstra, Albert; Waters, Rens

    1996-01-01

    We report the discovery of a symmetric bow shock around the well-known high-mass X-ray binary (HMXB) Vela X-1. Wind bow shocks are a ubiquitous phenomenon around OB-runaway stars, but now such a structure is found around a HMXB. The presence of a bow shock indicates that the system has a high (supersonic) velocity with respect to the interstellar medium. From the symmetry of the bow shock, the direction of motion and, moreover, the origin and age of the system can be derived. Our observation supports Blaauw's scenario for the formation of an OB-runaway star by the supernova explosion of the binary companion.

  4. Effects of pin bowing in the CAGR fuel element

    International Nuclear Information System (INIS)

    A theoretical and experimental investigation of the effects of bowing on pin temperatures in CAGR fuel elements is described. A subchannel code, SCANDAL, has been developed to calculate the effects of bow in arbitrary rod clusters with single phase coolant. The fundamental assumptions of the code and the extra components needed to handle pin bowing are presented. In order to validate SCANDAL a heat transfer experiment has been performed, in which selected pins in a 36 pin CAGR fuel element have been mechanically bowed and detailed temperature effects measured. Results from this experiment are presented and compared with SCANDAL predictions. (author)

  5. Size effects in band gap bowing in nitride semiconducting alloys

    DEFF Research Database (Denmark)

    Gorczyca, I.; Suski, T.; Christensen, Niels Egede;

    2011-01-01

    Chemical and size contributions to the band gap bowing of nitride semiconducting alloys (InxGa1-xN, InxAl1-xN, and AlxGa1-xN) are analyzed. It is shown that the band gap deformation potentials of the binary constituents determine the gap bowing in the ternary alloys. The particularly large gap...

  6. 46 CFR 45.69 - Correction for bow height.

    Science.gov (United States)

    2010-10-01

    ... 46 Shipping 2 2010-10-01 2010-10-01 false Correction for bow height. 45.69 Section 45.69 Shipping COAST GUARD, DEPARTMENT OF HOMELAND SECURITY (CONTINUED) LOAD LINES GREAT LAKES LOAD LINES Freeboards § 45.69 Correction for bow height. (a) The minimum summer freeboard of all manned vessels must...

  7. Evolution of bow-tie architectures in biology.

    Directory of Open Access Journals (Sweden)

    Tamar Friedlander

    2015-03-01

    Full Text Available Bow-tie or hourglass structure is a common architectural feature found in many biological systems. A bow-tie in a multi-layered structure occurs when intermediate layers have much fewer components than the input and output layers. Examples include metabolism where a handful of building blocks mediate between multiple input nutrients and multiple output biomass components, and signaling networks where information from numerous receptor types passes through a small set of signaling pathways to regulate multiple output genes. Little is known, however, about how bow-tie architectures evolve. Here, we address the evolution of bow-tie architectures using simulations of multi-layered systems evolving to fulfill a given input-output goal. We find that bow-ties spontaneously evolve when the information in the evolutionary goal can be compressed. Mathematically speaking, bow-ties evolve when the rank of the input-output matrix describing the evolutionary goal is deficient. The maximal compression possible (the rank of the goal determines the size of the narrowest part of the network-that is the bow-tie. A further requirement is that a process is active to reduce the number of links in the network, such as product-rule mutations, otherwise a non-bow-tie solution is found in the evolutionary simulations. This offers a mechanism to understand a common architectural principle of biological systems, and a way to quantitate the effective rank of the goals under which they evolved.

  8. Evolution of bow-tie architectures in biology.

    Science.gov (United States)

    Friedlander, Tamar; Mayo, Avraham E; Tlusty, Tsvi; Alon, Uri

    2015-03-01

    Bow-tie or hourglass structure is a common architectural feature found in many biological systems. A bow-tie in a multi-layered structure occurs when intermediate layers have much fewer components than the input and output layers. Examples include metabolism where a handful of building blocks mediate between multiple input nutrients and multiple output biomass components, and signaling networks where information from numerous receptor types passes through a small set of signaling pathways to regulate multiple output genes. Little is known, however, about how bow-tie architectures evolve. Here, we address the evolution of bow-tie architectures using simulations of multi-layered systems evolving to fulfill a given input-output goal. We find that bow-ties spontaneously evolve when the information in the evolutionary goal can be compressed. Mathematically speaking, bow-ties evolve when the rank of the input-output matrix describing the evolutionary goal is deficient. The maximal compression possible (the rank of the goal) determines the size of the narrowest part of the network-that is the bow-tie. A further requirement is that a process is active to reduce the number of links in the network, such as product-rule mutations, otherwise a non-bow-tie solution is found in the evolutionary simulations. This offers a mechanism to understand a common architectural principle of biological systems, and a way to quantitate the effective rank of the goals under which they evolved. PMID:25798588

  9. Bowing test of HTGR graphite sleeve

    International Nuclear Information System (INIS)

    Bowing characteristics were examined for IG-11 and H451 graphite sleeve specimens to which temperature gradients were given in the circumferential direction using a specially prepared rig. Measurements were also carried out on load or bending moment which was caused in the sleeve specimens under constraint as a result of temperature gradients. Experimental data were well analyzed on the basis of the elastic theory on the deflection of beams. Bending tests of the sleeve specimens indicated that the bending moment generated in the sleeve specimens under constraint was less than one-third of that at fracture even when the maximum temperature difference along the circumferential direction was more than 2000C. (author)

  10. The sacred weapon: bow and arrow combat in Iran

    OpenAIRE

    Manouchehr Moshtagh Khorasani

    2012-01-01

    The following article presents the development of the bow and arrow, and its important role in the history of Iran. The bow always played an important role not only on the battlefield, but also in hunting. It was also considered as a sacred weapon and additionally a royal symbol. Bow and arrow were considered as a superior weapon in comparison with other types of weapons because one could fight with them at a safer distance as one offered by swords, maces and axes. The first part of the artic...

  11. An approach to predicting bowing control parameter contours in violin performance

    OpenAIRE

    Maestre E.; Ramirez R.

    2010-01-01

    We present a machine learning approach to modeling bowing control parameter contours in violin performance. Using accurate sensing techniques we obtain relevant timbre-related bowing control parameters such as bow transversal velocity, bow pressing force, and bow-bridge distance of each performed note. Each performed note is represented by a curve parameter vector and a number of note classes are defined. The principal components of the data represented by the set of curve p...

  12. On the Earth's bow shock motion and speed

    International Nuclear Information System (INIS)

    The Earth's bow shock has often been shown to have rather high speed (50-150 km s-1) on the basis of different methods of investigation (Formisano et al., 1971; Greenstadt et al., 1972; Formisano et al., 1973; Guha et al., 1972). Voelk and Auer (1973) have recently considered the interaction of Tangential Discontinuities (TD) and Alfven waves with the bow shock in order to explain the shock motion and speed. The conclusion of these authors was that Alfven waves can cause very slow shock motions (up to 10 km s-1) while a TD hitting the bow shock can generate much higher speeds if the density ratio across the TD is high enough. It is the intention, here, to verify experimentally with the HEOS-1 plasma data the importance of TD for the bow shock motion and speed. (Auth.)

  13. Evolution of bow-tie architectures in biology

    OpenAIRE

    Friedlander, Tamar; Mayo, Avraham E.; Tlusty, Tsvi; Alon, Uri

    2014-01-01

    Bow-tie or hourglass structure is a common architectural feature found in biological and technological networks. A bow-tie in a multi-layered structure occurs when intermediate layers have much fewer components than the input and output layers. Examples include metabolism where a handful of building blocks mediate between multiple input nutrients and multiple output biomass components, and signaling networks where information from numerous receptor types passes through a small set of signalin...

  14. Congenital anterolateral tibial bowing and polydactyly: a case report

    Directory of Open Access Journals (Sweden)

    Lemire Edmond G

    2007-07-01

    Full Text Available Abstract Congenital anterolateral bowing of the tibia is a rare deformity that may lead to pseudarthrosis and risk of fracture. This is commonly associated with neurofibromatosis type 1. In this report, we describe a 15-month old male with congenital anterolateral bowing of the right tibia and associated hallux duplication. This is a distinct entity with a generally favourable prognosis that should not be confused with other conditions such as neurofibromatosis type 1. Previously published cases are reviewed.

  15. Anatomy of wood for bows of string instruments

    OpenAIRE

    Čufar, Katarina; Demšar, Blaž; Zupančič, Martin; Koch, Gerald; Oven, Primož

    2007-01-01

    Four specimens of wood originating from string instrument bows or from the material intended to be used for the repair of bows were obtained from the string instrument workshop "Atelje Demšar". Foreign wood traders supplied the specimens under their commercial names: (1) pernambouc, (2) horse flesh, (3) brasil, and (4) snakewood. Macroscopic and microscopic wood anatomical investigations were carried out in order to verify the nomenclature of the traded specimens. The microscopic identificati...

  16. Dual-Frequency Operation of Bow-Tie Microstrip Antenna

    Institute of Scientific and Technical Information of China (English)

    钟顺时; 张需溥

    2005-01-01

    Characteristics of a single-feed dual-frequency bow-tie microstrip antenna are studied. By using the variation method, simple formulas for resonant frequencies of the bow-tie microstrip antenna are derived. It is shown that the dual-frequency ratio can be controlled easily by choosing the parameters of the antenna. This design gives compact antenna size and simple antenna structure. Experimental results are presented, verifying the validity of the design.

  17. Evolution of bow-tie architectures in biology.

    OpenAIRE

    Tamar Friedlander; Mayo, Avraham E.; Tsvi Tlusty; Uri Alon

    2015-01-01

    Bow-tie or hourglass structure is a common architectural feature found in biological and technological networks. A bow-tie in a multi-layered structure occurs when intermediate layers have much fewer components than the input and output layers. Examples include metabolism where a handful of building blocks mediate between multiple input nutrients and multiple output biomass components, and signaling networks where information from numerous receptor types passes through a small set of signalin...

  18. Bowing behavior of subassemblies in experimental fast reactor ''JOYO''

    International Nuclear Information System (INIS)

    In JOYO, the measured power coefficients in the beginning of the operation cycle of MK-I and MK-II cores showed power dependence, while the calculation without taking account of bowing predicted little power dependence. The bowing analysis was performed in order to investigate the power dependence observed in the measured power coefficients and the following conclusions were obtained. (1) The evaluated power coefficients taking account of bowing effect agree better with measured ones than the calculated ones without taking account of bowing effect in MK-I core. (2) In MK-II core, although the analytical results show not so good agreement quantitatively with the measured power coefficients, it is suggested that they agree better depending on the uncertain parameters such as the heat generation in the reflector region, the threshold moment for leaning and the stiffness of the inner reflector. (3) It becomes clear from these results that the power dependence observed in the measured power coefficients in JOYO is due to the bowing effect. (author)

  19. BowTieBuilder: modeling signal transduction pathways

    Directory of Open Access Journals (Sweden)

    Schröder Adrian

    2009-06-01

    Full Text Available Abstract Background Sensory proteins react to changing environmental conditions by transducing signals into the cell. These signals are integrated into core proteins that activate downstream target proteins such as transcription factors (TFs. This structure is referred to as a bow tie, and allows cells to respond appropriately to complex environmental conditions. Understanding this cellular processing of information, from sensory proteins (e.g., cell-surface proteins to target proteins (e.g., TFs is important, yet for many processes the signaling pathways remain unknown. Results Here, we present BowTieBuilder for inferring signal transduction pathways from multiple source and target proteins. Given protein-protein interaction (PPI data signaling pathways are assembled without knowledge of the intermediate signaling proteins while maximizing the overall probability of the pathway. To assess the inference quality, BowTieBuilder and three alternative heuristics are applied to several pathways, and the resulting pathways are compared to reference pathways taken from KEGG. In addition, BowTieBuilder is used to infer a signaling pathway of the innate immune response in humans and a signaling pathway that potentially regulates an underlying gene regulatory network. Conclusion We show that BowTieBuilder, given multiple source and/or target proteins, infers pathways with satisfactory recall and precision rates and detects the core proteins of each pathway.

  20. Foreshock ions observed behind the Martian bow shock

    Science.gov (United States)

    Frahm, R. A.; Yamauchi, M.; Winningham, J. D.; Lundin, R.; Sharber, J. R.; Nilsson, H.; Coates, A. J.

    2016-08-01

    The Mars Express Analyzer of Space Plasmas and Energetic Atoms experiment contains ion and electron instruments for conducting plasma measurements. On January 23, 2012, during in-bound travel of Mars Express in the southern hemisphere of Mars from its dawn side toward periapsis at dusk, the plasma instruments measured foreshock-like ion beams extending from outside the bow shock and into the magnetosphere, continuing to a distance of about a proton gyroradius from the bow shock. These ion beams were mostly protons, were observed to have energies greater than solar wind protons, and were not gyrating, in agreement with reflections of the solar wind proton beam. Furthermore, in the foreshock region the ion energy gradually decreased toward the magnetosheath, in agreement with an acceleration by outward-directed electric field in the bowshock. The observations also suggest that this electric field exists even inside the magnetosheath within the distance of a proton gyroradius from the bow shock.

  1. Planetary Embryo Bow Shocks as a Mechanism for Chondrule Formation

    CERN Document Server

    Mann, Christopher R; Morris, Melissa M

    2016-01-01

    We use radiation hydrodynamics with direct particle integration to explore the feasibility of chondrule formation in planetary embryo bow shocks. The calculations presented here are used to explore the consequences of a Mars-size planetary embryo traveling on a moderately excited orbit through the dusty, early environment of the solar system. The embryo's eccentric orbit produces a range of supersonic relative velocities between the embryo and the circularly orbiting gas and dust, prompting the formation of bow shocks. Temporary atmospheres around these embryos, which can be created via volatile outgassing and gas capture from the surrounding nebula, can non-trivially affect thermal profiles of solids entering the shock. We explore the thermal environment of solids that traverse the bow shock at different impact radii, the effects that planetoid atmospheres have on shock morphologies, and the stripping efficiency of planetoidal atmospheres in the presence of high relative winds. Simulations are run using adia...

  2. Bow and stern waves triggered by the Moon's shadow boat

    Science.gov (United States)

    Liu, J. Y.; Sun, Y. Y.; Kakinami, Y.; Chen, C. H.; Lin, C. H.; Tsai, H. F.

    2011-09-01

    It has been predicted that the Moon's shadow, the cooling region, sweeping over the Earth's atmosphere with a supersonic speed could trigger bow waves since 1970. The longest total solar eclipse within next hundred years occurring on 22 July 2009 sweeps over the Eastern Asia region during the noontime period. An analysis of the Hilbert-Huang transform (HHT) is applied to study ionospheric TEC (total electron content) derived from ground-based GPS receivers in Taiwan and Japan. We not only find the feature of the predicted bow wave but also the stern wave on the equator side of the eclipse path, as well as the stern wake right behind the Moon's shadow boat. The bow and stern waves are formed by acoustic gravity waves of periods about 3 and/or 5 minutes traveling equatorward with a phase speed of about 100 m/s in the ionosphere.

  3. [Forensic medical characteristics of the injuries inflicted by modern sport bow].

    Science.gov (United States)

    Babakhanian, R V; Isakov, V D; Gusev, N Iu; Lebedev, V N

    2006-01-01

    Modern bows are classified as representatives of darts. Construction characteristics of bows and arrows, damage to experimental cotton targets from shooting distance of 1-15 m are described. PMID:16826840

  4. Crushing of ship bows in head-on collision

    DEFF Research Database (Denmark)

    Ocakli, H.; Zhang, S.; Pedersen, Preben Terndrup

    2004-01-01

    Semi-analytical methods for analysis of plate crushing and ship bow damage in head-on collisions are developed in this paper. Existing experimental and theoretical studies for crushing analysis of plated structures are summarized and compared. Simple formulae for determining the crushing force...... approach developed can be used easily to determine the crushing resistance and damage extent of the ship bow when ship length and collision speed are known. The method can be used in probabilistic analysis of damage extents in ship collisions where a large number of calculations are generally required....

  5. A Study on Self Centering of Face Bows

    OpenAIRE

    Veerareddy, Chandrika; Srividya, S.; Chandrasekharan Nair, K.; Shetty, Jayakar; Vishwanath, G.

    2010-01-01

    Hanau spring bow has been in use since 1986. Hanau spring bow is claimed to maintain self centering property when it is positioned in the patient as well as in the articulator. However there is no documented evidence to prove that feature. Mainly it was due to the absence of a testing device. Exclusively for the present study, the testing device consisting of a platform, stops and distance measuring system was designed by the third author. This study proved that Hanau has the capability of se...

  6. A Multichannel THz Detector Using Integrated Bow-Tie Antennas

    OpenAIRE

    Hairui Liu; Junsheng Yu; Peter Huggard; Byron Alderman

    2013-01-01

    This paper presents a kind of a multichannel THz detector using lens-based bow-tie array. A hyperhemispherical silicon lens is employed to provide a focal plane; 8 bow-tie elements are arranged on the focal plane with careful design to show a performance of broadband, high gain, well compact, and easy assembling. These characteristics of the detector are preferred for detecting weak THz signal. Measured far field shows that the radiation pattern of each element is shifted angularly, by ≈9°, w...

  7. Understanding CANDU fuel bowing in dryout: an industry approach

    International Nuclear Information System (INIS)

    Fuel element bow induced by dryout could potentially perturb the coolant flow distribution and heat transfer from the fuel element to the coolant. Some accident scenarios leading to dryout of the fuel element are: loss of power regulation pump trip, pump seizure, small and large break loss of coolant accidents. In these accidents, it is desirable to show with confidence that the fuel remains sufficiently cooled to maintain its geometry, even if it is in dryout. This can be demonstrated if fuel elements are separated from each other and from the pressure tube, with a sufficient (and stable) gap. Therefore, the prediction of the amount of bow, and its effect on heat transfer conditions is required for the assessments. The utilities have joined force in launching an experimental investigation at Stern Laboratories to characterize the bowing phenomena. This program will investigate the amount of deflection, transient and permanent, that results from accident conditions which cause a dry patch on one side of the sheath. This is expected to bound the consequences of fuel bowing due to dryout. Since the accident transients begin at full power and high coolant pressure (about 10 MPa) they generate sharp thermal gradients (dry patch) and it is necessary to develop a simulation with representative dry fuel sheath conditions initiated from a normal full power and coolant state. The amount of bow is driven by thermal gradients in both the fuel pellets and the sheath, therefore, the thermal gradients should be representative. This program is structured in a series of tests progressing from simple representation to complex simulation. It is divided into 3 experimental phases: Phase 1 - Thermalhydraulic simulation of fuel element bow by a heated tube; Phase 2 - Thermal and mechanical bow with a simulator which accounts for pellet / fuel sheath interaction with internal pellet temperature distributions; and Phase 3 - Fuel element bow with a simulator using Zircaloy-4 fuel sheath

  8. Smashing the Guitar: An Evolving Neutron Star Bow Shock

    OpenAIRE

    S Chatterjee; Cordes, J. M.

    2003-01-01

    The Guitar nebula is a spectacular example of an H-alpha bow shock nebula produced by the interaction of a neutron star with its environment. The radio pulsar B2224+65 is traveling at ~800--1600 km/s (for a distance of 1--2 kpc), placing it on the high-velocity tail of the pulsar velocity distribution. Here we report time evolution in the shape of the Guitar nebula, the first such observations for a bow shock nebula, as seen in H-alpha imaging with the Hubble Space Telescope. The morphology o...

  9. 77 FR 19661 - City of Broken Bow, OK; Notice of Technical Conference

    Science.gov (United States)

    2012-04-02

    ... Energy Regulatory Commission City of Broken Bow, OK; Notice of Technical Conference March 21, 2012. Take.... Forest Service on November 16, 2007 for the Broken Bow Re-Regulation Dam Hydroelectric Project No. 12470.... Forest Service's Hochatown Office, Route 4, Broken Bow, OK 74728. All local, state, and federal...

  10. Search for systemic mass loss in Algols with bow shocks

    Science.gov (United States)

    Mayer, A.; Deschamps, R.; Jorissen, A.

    2016-03-01

    Aims: Various studies indicate that interacting binary stars of Algol type evolve non-conservatively. However, direct detections of systemic mass loss in Algols have been scarce so far. We study the systemic mass loss in Algols by looking for the presence of infrared excesses originating from the thermal emission of dust grains, which is linked to the presence of a stellar wind. Methods: In contrast to previous studies, we make use of the fact that stellar and interstellar material is piled up at the edge of the astrosphere where the stellar wind interacts with the interstellar medium. We analyse WISE W3 12 μm and WISE W4 22 μm data of Algol-type binary Be and B[e] stars and the properties of their bow shocks. From the stand-off distance of the bow shock we are able to determine the mass-loss rate of the binary system. Results: Although the velocities of the stars with respect to the interstellar medium are quite low, we find bow shocks present in two systems, namely π Aqr, and ϕ Per; a third system, CX Dra, shows a more irregular circumstellar environment morphology which might somehow be related to systemic mass loss. The properties of the two bow shocks point to mass-loss rates and wind velocities typical of single B stars, which do not support an enhanced systemic mass loss.

  11. THE JET-DRIVEN BOW SHOCK IN OUTFLOWS

    Institute of Scientific and Technical Information of China (English)

    ZhangQing; ZhengXingwu

    1999-01-01

    Recent high resolution observations show the high collimated bipolar molecular outflows from young stellar objects, such as NGC 2 264G and NGC 2 024. Existing models can not yet give complete interpretations of the structure and properties of the observed flow. Here, we propose a jet-driven bow

  12. Multi-Spacecraft Investigation of Terrestrial Bow Shock: Cluster Observations

    Czech Academy of Sciences Publication Activity Database

    Krupařová, Oksana; Krupař, Vratislav; Santolík, Ondřej; Souček, Jan; Šafránková, J.; Němeček, Z.; Němec, F.; Maksimovic, M.

    San Francisco: American Geophysical Union, 2015. SM13C-2516. [AGU Fall Meeting 2015. 14.12.2015-18.12.2015, San Francisco] Institutional support: RVO:68378289 Keywords : magnetosphere * bow shock * Cluster Subject RIV: BL - Plasma and Gas Discharge Physics https://agu.confex.com/agu/fm15/meetingapp.cgi/Paper/81554

  13. Accurate methodology for channel bow impact on CPR

    International Nuclear Information System (INIS)

    An overview is given of existing CPR design criteria and the methods used in BWR reload analysis to evaluate the impact of channel bow on CPR margins. Potential weaknesses in today's methodologies are discussed. Westinghouse in collaboration with KKL and Axpo - operator and owner of the Leibstadt NPP - has developed an enhanced CPR methodology based on a new criterion to protect against dryout during normal operation and with a more rigorous treatment of channel bow. The new steady-state criterion is expressed in terms of an upper limit of 0.01 for the dryout failure probability per year. This is considered a meaningful and appropriate criterion that can be directly related to the probabilistic criteria set-up for the analyses of Anticipated Operation Occurrences (AOOs) and accidents. In the Monte Carlo approach a statistical modeling of channel bow and an accurate evaluation of CPR response functions allow the associated CPR penalties to be included directly in the plant SLMCPR and OLMCPR in a best-estimate manner. In this way, the treatment of channel bow is equivalent to all other uncertainties affecting CPR. The enhanced CPR methodology has been implemented in the Westinghouse Monte Carlo code, McSLAP. The methodology improves the quality of dryout safety assessments by supplying more valuable information and better control of conservatisms in establishing operational limits for CPR. The methodology is demonstrated with application examples from the introduction at KKL. (orig.)

  14. Modeling non-thermal emission from stellar bow shocks

    CERN Document Server

    Pereira, V; Miceli, M; Bonito, R; de Castro, E

    2016-01-01

    Runaway O- and early B-type stars passing throughout the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical models predict the production of high energy photons by non-thermal radiative processes, but their efficiency is still debated. We aim to test and explain the possibility of emission from the bow shocks formed by runaway stars traveling through the interstellar medium by using previous theoretical models. We apply our model to AE Aurigae, the first reported star with an X-ray detected bow shock, to BD+43 3654, in which the observations failed in detecting high energy emission, and to the transition phase of a supergiant star in the late stages of its life.From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high energy fl...

  15. Application of Bow-tie methodology to improve patient safety.

    Science.gov (United States)

    Abdi, Zhaleh; Ravaghi, Hamid; Abbasi, Mohsen; Delgoshaei, Bahram; Esfandiari, Somayeh

    2016-05-01

    Purpose - The purpose of this paper is to apply Bow-tie methodology, a proactive risk assessment technique based on systemic approach, for prospective analysis of the risks threatening patient safety in intensive care unit (ICU). Design/methodology/approach - Bow-tie methodology was used to manage clinical risks threatening patient safety by a multidisciplinary team in the ICU. The Bow-tie analysis was conducted on incidents related to high-alert medications, ventilator associated pneumonia, catheter-related blood stream infection, urinary tract infection, and unwanted extubation. Findings - In total, 48 potential adverse events were analysed. The causal factors were identified and classified into relevant categories. The number and effectiveness of existing preventive and protective barriers were examined for each potential adverse event. The adverse events were evaluated according to the risk criteria and a set of interventions were proposed with the aim of improving the existing barriers or implementing new barriers. A number of recommendations were implemented in the ICU, while considering their feasibility. Originality/value - The application of Bow-tie methodology led to practical recommendations to eliminate or control the hazards identified. It also contributed to better understanding of hazard prevention and protection required for safe operations in clinical settings. PMID:27142951

  16. Hierarchical modularity of nested bow-ties in metabolic networks

    Directory of Open Access Journals (Sweden)

    Luo Jian-Hua

    2006-08-01

    Full Text Available Abstract Background The exploration of the structural topology and the organizing principles of genome-based large-scale metabolic networks is essential for studying possible relations between structure and functionality of metabolic networks. Topological analysis of graph models has often been applied to study the structural characteristics of complex metabolic networks. Results In this work, metabolic networks of 75 organisms were investigated from a topological point of view. Network decomposition of three microbes (Escherichia coli, Aeropyrum pernix and Saccharomyces cerevisiae shows that almost all of the sub-networks exhibit a highly modularized bow-tie topological pattern similar to that of the global metabolic networks. Moreover, these small bow-ties are hierarchically nested into larger ones and collectively integrated into a large metabolic network, and important features of this modularity are not observed in the random shuffled network. In addition, such a bow-tie pattern appears to be present in certain chemically isolated functional modules and spatially separated modules including carbohydrate metabolism, cytosol and mitochondrion respectively. Conclusion The highly modularized bow-tie pattern is present at different levels and scales, and in different chemical and spatial modules of metabolic networks, which is likely the result of the evolutionary process rather than a random accident. Identification and analysis of such a pattern is helpful for understanding the design principles and facilitate the modelling of metabolic networks.

  17. Double tibial osteotomy for bow leg patients: A case series

    Directory of Open Access Journals (Sweden)

    Khalilollah Nazem

    2013-01-01

    Full Text Available Background: High tibia osteotomy (HTO is a common surgical operation for correction of genu varum deformity. In some patients, there are concurrent tibia vara and genu varum (bow leg. This study aimed to consider the possibility of better correction of bow leg deformity after double level tibial osteotomy (DLTO. Materials and Methods: A case series of 10 patients of genu varum in addition to tibia vara (bow leg deformity who were referred to orthopedic ward of an academic hospital of Isfahan- Iran during 2009-2011 were included in the study. The mean age was 17.3 ± 3.1 years and all of them underwent DLTO. The results of treatment have been assessed based on clinical and radiological parameters before and after surgery. Results: The mean pre- and post operative values for Tibia-Femoral Angle, Medial Proximal of Tibia Angle (MPTA, and Lateral Distal of Tibia Angle (LDTA were 18.13 ± 3.05° vs. 3.93 ± 0.66°, 79.13 ± 3.4° vs. 89.7 ± 1.8° and 96.40 ± 1.8° vs. 88.73 ± 3.0° respectively (P < 0.05. Improvement of all radiological parameters was meaningful. Seventy three percent of patients had normal mechanical axis of limb after surgery. The remaining cases had varus deformity in distal femur that was corrected by valgus supracondylar osteotomy in an additional operation. Limited range of motion (ROM near knee and ankle was not observed. Conclusion : DLTO correct bow leg deformity in the point of alignment of limb and paralleling of knee and ankle joint more effectively. This method can be used in metabolic and congenital bow leg which deformities are present in throughout of the lower limb. We described this technique for the first time.

  18. Arctic Bowyery – the Use of Compression Wood in Bows in the Subarctic and Arctic Regions of Eurasia and America

    Directory of Open Access Journals (Sweden)

    Marcus Lepola

    2015-06-01

    Full Text Available This paper is a study of the traditional use of a special kind of wood in bow construction in Eurasia and North America. This special kind of wood, called compression wood and coming from coniferous trees, has unique qualities that makes it suitable for bow construction. Bows made using this special wood have been referred to as Finno-Ugric bows, Sámi bows, Two-Wood bows and Eurasia laminated bows. These bows appear to have developed from archaic forms of compression wood self bows that were made from a single piece of wood. Recently features similar to the Eurasian compression wood bows have been discovered in bows originating from Alaska, and the use of compression wood for bow manufacture has been known to some Canadian Inuit groups. This paper addresses the origin and possible diffusion pattern of this innovation in bow technology in Eurasia and suggests a timeframe and a possible source for the transfer of this knowledge to North America. This paper also discusses the role of the Asiatic composite bow in the development of bows in Eurasia.

  19. Cluster Close Separation at the Bow Shock Campaign: Initial Results.

    Science.gov (United States)

    Balikhin, M. A.; Sagdeev, R.; Walker, S. N.; Malkov, M.; Krasnoselskikh, V.; Khotyaintsev, Y. V.; Fazakerley, A. N.; Doss, N.

    2015-12-01

    The Cluster close separation at the terrestrial bow shock campaign was aimed at probing the terrestrial bow shock front using multi-scale spacecraft separations. The closest separation (structure of the magnetic ramp. It is shown that the magnetic field perturbations observed within the ramp along the shock normal possess spatial scales a few times shorter than the ramp region itself, and are accompanied by variations in the electric field with magnitudes of a few tens mV/m. Using dual spacecraft measurements enables us to show that in the plane of the shock front the characteristic width of these structures corresponds to electron scales. Comparison of the magnetic field profile obtained from Cluster 3 and 4 indicates possibility that the initial stage of the front reformation is observed. However alternative explanations ( kinetic instabilities, corrugation instability) are also discussed.

  20. Energy band bowing parameter in MgZnO alloys

    International Nuclear Information System (INIS)

    We report on bandgap bowing parameters for wurtzite and cubic MgZnO alloys from a study of high quality and single phase films in all Mg content range. The Mg contents in the MgZnO films were accurately determined using the energy dispersive spectrometer and X-ray photoelectron spectroscopy (XPS). The measurement of bandgap energies by examining the onset of inelastic energy loss in core-level atomic spectra from XPS is proved to be valid for determining the bandgap of MgZnO films. The dependence of the energy bandgap on Mg content is found to deviate downwards from linearity. Fitting of the bandgap data resulted in two bowing parameters of 2.01 ± 0.04 eV and 1.48 ± 0.11 eV corresponding to wurtzite and cubic MgZnO films, respectively

  1. Mass-loading of bow shock pulsar wind nebulae

    CERN Document Server

    Morlino, G; Vorster, M

    2016-01-01

    We investigate the dynamics of bow shock nebulae created by pulsars moving supersonically through a partially ionized interstellar medium. A fraction of interstellar neutral hydrogen atoms penetrating into the tail region of a pulsar wind will undergo photo-ionization due to the UV light emitted by the nebula, with the resulting mass loading dramatically changing the flow dynamics of the light leptonic pulsar wind. Using a quasi 1-D hydrodynamic model of relativistic flow we find that if a relatively small density of neutral hydrogen, as low as $10^{-4}$ cm$^{-3}$, penetrate inside the pulsar wind, this is sufficient to strongly affect the tail flow. Mass loading leads to the fast expansion of the pulsar wind tail, making the tail flow intrinsically non-stationary. The shapes predicted for the bow shock nebulae compare well with observations, both in H$\\alpha$ and X-rays.

  2. A Multichannel THz Detector Using Integrated Bow-Tie Antennas

    Directory of Open Access Journals (Sweden)

    Hairui Liu

    2013-01-01

    Full Text Available This paper presents a kind of a multichannel THz detector using lens-based bow-tie array. A hyperhemispherical silicon lens is employed to provide a focal plane; 8 bow-tie elements are arranged on the focal plane with careful design to show a performance of broadband, high gain, well compact, and easy assembling. These characteristics of the detector are preferred for detecting weak THz signal. Measured far field shows that the radiation pattern of each element is shifted angularly, by ≈9°, which can be used for THz imaging. Tested responsivity of the detector shows a good spectral performance from 260 to 400 GHz: respective values were ≥220 V/W, and the best NEP is achieved at about 60 pW/. Besides that, the proposed antenna has advantages of simple structure, easy fabrication, and low cost.

  3. Organizing learning processes on risks by using the bow-tie representation

    International Nuclear Information System (INIS)

    The Aramis method proposes a complete and efficient way to manage risk analysis by using the bow-tie representation. This paper shows how the bow-tie representation can also be appropriate for experience learning. It describes how a pharmaceutical production plant uses bow-ties for incident and accident analysis. Two levels of bow-ties are constructed: standard bow-ties concern generic risks of the plant whereas local bow-ties represent accident scenarios specific to each workplace. When incidents or accidents are analyzed, knowledge that is gained is added to existing local bow-ties. Regularly, local bow-ties that have been updated are compared to standard bow-ties in order to revise them. Knowledge on safety at the global and at local levels is hence as accurate as possible and memorized in a real time framework. As it relies on the communication between safety experts and local operators, this use of the bow-ties contributes therefore to organizational learning for safety

  4. Organizing learning processes on risks by using the bow-tie representation.

    Science.gov (United States)

    Chevreau, F R; Wybo, J L; Cauchois, D

    2006-03-31

    The Aramis method proposes a complete and efficient way to manage risk analysis by using the bow-tie representation. This paper shows how the bow-tie representation can also be appropriate for experience learning. It describes how a pharmaceutical production plant uses bow-ties for incident and accident analysis. Two levels of bow-ties are constructed: standard bow-ties concern generic risks of the plant whereas local bow-ties represent accident scenarios specific to each workplace. When incidents or accidents are analyzed, knowledge that is gained is added to existing local bow-ties. Regularly, local bow-ties that have been updated are compared to standard bow-ties in order to revise them. Knowledge on safety at the global and at local levels is hence as accurate as possible and memorized in a real time framework. As it relies on the communication between safety experts and local operators, this use of the bow-ties contributes therefore to organizational learning for safety. PMID:16125315

  5. Statistical modeling of bowing control applied to violin sound synthesis

    OpenAIRE

    Maestre E.; Blaauw M.; Bonada J.; Guaus E.; Perez A.

    2010-01-01

    Excitation-continuous music instrument control patterns are often not explicitly represented in current sound synthesis techniques when applied to automatic performance. Both physical model-based and sample-based synthesis paradigms would benefit from a flexible and accurate instrument control model, enabling the improvement of naturalness and realism. We present a framework for modeling bowing control parameters in violin performance. Nearly non-intrusive sensing techniques allow fo...

  6. Planetary Embryo Bow Shocks as a Mechanism for Chondrule Formation

    OpenAIRE

    Mann, Christopher R.; Boley, Aaron C.; Morris, Melissa M.

    2016-01-01

    We use radiation hydrodynamics with direct particle integration to explore the feasibility of chondrule formation in planetary embryo bow shocks. The calculations presented here are used to explore the consequences of a Mars-size planetary embryo traveling on a moderately excited orbit through the dusty, early environment of the solar system. The embryo's eccentric orbit produces a range of supersonic relative velocities between the embryo and the circularly orbiting gas and dust, prompting t...

  7. BowTieBuilder: modeling signal transduction pathways

    OpenAIRE

    Schröder Adrian; Dräger Andreas; Planatscher Hannes; Spangenberg Lucía; Supper Jochen; Zell Andreas

    2009-01-01

    Abstract Background Sensory proteins react to changing environmental conditions by transducing signals into the cell. These signals are integrated into core proteins that activate downstream target proteins such as transcription factors (TFs). This structure is referred to as a bow tie, and allows cells to respond appropriately to complex environmental conditions. Understanding this cellular processing of information, from sensory proteins (e.g., cell-surface proteins) to target proteins (e.g...

  8. Performance Characterization of Radial Stub Microstrip Bow-Tie Antenna

    OpenAIRE

    B.T.P.Madhav; S.S. Mohan Reddy; Neha Sharma; J. Ravindranath Chowdary; Bala Rama Pavithra; K.N.V.S. Kishore; G Sriram; B. Sachin Kumar

    2013-01-01

    In this paper a novel radial stub feeding microstrip bow-tie antenna is designed to operate between C and X band and its performance characterization is presented. This antenna is having simple structure and topology over other stub loaded antennas. In addition the proposed antenna adjusts to the desired frequency easily. Antenna output parameters like radiation pattern, axial ratio, directive gain andquality factor are simulated and presented in this current work.

  9. Performance Characterization of Radial Stub Microstrip Bow-Tie Antenna

    Directory of Open Access Journals (Sweden)

    B.T.P.Madhav

    2013-04-01

    Full Text Available In this paper a novel radial stub feeding microstrip bow-tie antenna is designed to operate between C and X band and its performance characterization is presented. This antenna is having simple structure and topology over other stub loaded antennas. In addition the proposed antenna adjusts to the desired frequency easily. Antenna output parameters like radiation pattern, axial ratio, directive gain andquality factor are simulated and presented in this current work.

  10. Broadband bow-tie antenna with tapered balun

    OpenAIRE

    Jaafar, Hussein Mohammed

    2014-01-01

    ABSTRACT: In microwave applications spectrum Industrial, Scientific and Medical (ISM) band, especially in wireless communication systems applications such as GSM, 3G, Wi-Fi and Wi-MAX applications, high antenna characteristics such as high gain and wide bandwidth are required. In this thesis, a broadband Bow Tie Antenna (BTA) with high performance characteristics has been designed, to cover the wireless application requirements. One of the fundamental problems of the transmission line in the ...

  11. Planetary Embryo Bow Shocks as a Mechanism for Chondrule Formation

    Science.gov (United States)

    Mann, Christopher R.; Boley, Aaron C.; Morris, Melissa A.

    2016-02-01

    We use radiation hydrodynamics with direct particle integration to explore the feasibility of chondrule formation in planetary embryo bow shocks. The calculations presented here are used to explore the consequences of a Mars-size planetary embryo traveling on a moderately excited orbit through the dusty, early environment of the solar system. The embryo’s eccentric orbit produces a range of supersonic relative velocities between the embryo and the circularly orbiting gas and dust, prompting the formation of bow shocks. Temporary atmospheres around these embryos, which can be created via volatile outgassing and gas capture from the surrounding nebula, can non-trivially affect thermal profiles of solids entering the shock. We explore the thermal environment of solids that traverse the bow shock at different impact radii, the effects that planetoid atmospheres have on shock morphologies, and the stripping efficiency of planetoidal atmospheres in the presence of high relative winds. Simulations are run using adiabatic and radiative conditions, with multiple treatments for the local opacities. Shock speeds of 5, 6, and 7 km s-1 are explored. We find that a high-mass atmosphere and inefficient radiative conditions can produce peak temperatures and cooling rates that are consistent with the constraints set by chondrule furnace studies. For most conditions, the derived cooling rates are potentially too high to be consistent with chondrule formation.

  12. Spacer grid for reducing bowing in a nuclear fuel assembly

    International Nuclear Information System (INIS)

    A bi-metallic spacer grid having a zircaloy perimeter strip consisting of oppositely facing, thin walled metal plates for closely surrounding the array of fuel rods. A rigid, stainless steel cross member extends between internal surfaces of the oppositely facing perimeter plates. In the preferred embodiment, the perimeter plates have cantilevered portions extending above and below the main body of the perimeter strip. The cross members interact with the enlarged portion by urging them outward relative to the perimeter strip as the fuel assembly heats up during operation. The outwardly projecting interface surfaces of each assembly mechanically interact with the interface surfaces of adjacent assemblies providing a mechanical restraint which limits bowing of the assembly. The effectiveness of the spacer grids in limiting bowing is therefore not dependent upon controlling the mechanisms responsible for causing bow. When the reactor is in a cold condition such as during refueling , the exterior dimensions of the spacer grids are the same as those of the other zircaloy grids, which assures adequate clearance for insertion and withdrawal of individual fuel assemblies

  13. A Survey for H$\\alpha$ Pulsar Bow Shocks

    CERN Document Server

    Brownsberger, Sasha

    2014-01-01

    We report on a survey for H$\\alpha$ bow shock emission around nearby $\\gamma$-detected energetic pulsars. This survey adds three Balmer-dominated neutron star bow shocks to the six previously confirmed examples. In addition to the shock around {\\it Fermi} pulsar PSR J1741$-$2054, we now report H$\\alpha$ structures around two additional $\\gamma$-ray pulsars, PSR J2030+4415 and PSR J1509$-$5850. These are the first known examples of H$\\alpha$ nebulae with pre-ionization halos. With new measurements, we show that a simple analytic model can account for the angular size and flux of the bow shocks' apices. The latter, in particular, provides a new pulsar probe and indicates large moments of inertia and smaller distances than previously assumed, in several cases. In particular we show that the re-measured PSR J0437$-$4715 shock flux implies $I = (1.7\\pm 0.2) \\times 10^{45}/(f_{HI} {\\rm sin}i) {\\rm g\\,cm^2}$. We also derive a distance $d\\approx 0.72$kpc for the $\\gamma$-ray only pulsar PSR J2030+4415 and revised dis...

  14. Polarization of circumstellar bow shocks due to electron scattering

    Science.gov (United States)

    Shrestha, Manisha; Hoffman, J. L.; Neilson, H.; Ignace, R.

    2014-01-01

    Circumstellar material (CSM) provides a link between interacting supernovae and their massive progenitor stars. This CSM arises from stellar winds, outflows, or eruptions from a massive star before it explodes and can be detected around stars or supernovae with polarimetric observations. We use a Monte Carlo based radiative transfer code (SLIP) to investigate the polarization created by different models for the CSM surrounding a central source such as supernovae or massive stars. We vary parameters such as the shape, optical depth, temperature, and brightness of the CSM and compare the simulated flux and polarization behavior with observational data. We present results from new simulations that assume a bow shock shape for the CSM. Bow shocks are commonly observed around massive stars; this shape forms when a star moving more quickly than the speed of sound in the local interstellar medium emits a stellar wind that drives a shock wave into the ISM. Since a bow shock projects an aspherical shape onto the sky, light from the central source that scatters in the shock region becomes polarized. We present electron-scattering polarization maps for this geometry and discuss the behavior of observed polarization with viewing angle in the unresolved case.

  15. Sinogram bow-tie filtering in FBP PET reconstruction.

    Science.gov (United States)

    Abella, M; Vaquero, J J; Soto-Montenegro, M L; Lage, E; Desco, M

    2009-05-01

    Low-pass filtering of sinograms in the radial direction is the most common practice to limit noise amplification in filtered back projection (FBP) reconstruction of positron emission tomography studies. Other filtering strategies have been proposed to prevent the loss in resolution due to low-pass radial filters, although results have been diverse. Using the well-known properties of the Fourier transform of a sinogram, the authors defined a binary mask that matches the expected shape of the support region in the Fourier domain of the sinogram ("bow tie"). This mask was smoothed by a convolution with a ten-point Gaussian kernel which not only avoids ringing but also introduces a pre-emphasis at low frequencies. A new filtering scheme for FBP is proposed, comprising this smoothed bow-tie filter combined with a standard radial filter and an axial filter. The authors compared the performance of the bow-tie filtering scheme with that of other previously reported methods: Standard radial filtering, angular filtering, and stackgram-domain filtering. All the quantitative data in the comparisons refer to a baseline reconstruction using a ramp filter only. When using the smallest size of the Gaussian kernel in the stackgram domain, the authors achieved a noise reduction of 33% at the cost of degrading radial and tangential resolutions (14.5% and 16%, respectively, for cubic interpolation). To reduce the noise by 30%, the angular filter produced a larger degradation of contrast (3%) and tangential resolution (46% at 10 mm from the center of the field of view) and showed noticeable artifacts in the form of circular blurring dependent on the distance to the center of the field of view. For a similar noise reduction (33%), the proposed bow-tie filtering scheme yielded optimum results in resolution (gain in radial resolution of 10%) and contrast (1% increase) when compared with any of the other filters alone. Experiments with rodent images showed noticeable image quality

  16. Dependence of sound characteristics on the bowing position in a violin

    Science.gov (United States)

    Roh, YuJi; Kim, Young H.

    2014-12-01

    A quantitative analysis of violin sounds produced for different bowing positions over the full length of a violin string has been carried out. An automated bowing machine was employed in order to keep the bowing parameters constant. A 3-dimensional profile of the frequency spectrum was introduced in order to characterize the violin's sound. We found that the fundamental frequency did not change for different bowing positions, whereas the frequencies of the higher harmonics were different. Bowing the string at 30 mm from the bridge produced musical sounds. The middle of the string was confirmed to be a dead zone, as reported in previous works. In addition, the quarter position was also found to be a dead zone. Bowing the string 90 mm from the bridge dominantly produces a fundamental frequency of 864 Hz and its harmonics.

  17. Quantification of factors affecting thermally-induced bow in a CANDU fuel element simulator

    International Nuclear Information System (INIS)

    Thermally induced bow, caused by a circumferential temperature distribution around a fuel element, was investigated in this study using a fuel element simulator. The objective was to identify the factors affecting CANDU fuel element bow induced by dryout as a result of some predicted reactor transients in which the maximum fuel temperature reaches 600 deg C. The results showed that circumferential temperature distribution, pellet-to-sheath mechanical interaction and creep were the major factors affecting bow. Transient bow increased with increasing diametral sheath temperature difference and with mechanical interaction between the pellet and the sheath. Permanent bow of the fuel element was observed in some tests which was the result of creep. Mechanical interaction between the sheath and pellet produced the stresses necessary for creep deformation. A simplified ABAQUS model was developed to explain the experimental findings and could be used to predict the bow behaviour of fuel elements during reactor transients, where the dry patches are of different sizes. (author)

  18. Asymmetries in the location of the Venus and Mars bow shock

    International Nuclear Information System (INIS)

    An examination of observations of the position of the terminator bow shock at Venus and Mars shows that the terminator bow shock varies with the angle between the local bow shock normal and the upstream magnetic field, θBN. The part of the shock on the quasi-parallel side is closer to the planet than the part on the quasi-perpendicular side, a result which had been sggested by an earlier computer simulation by Thomas and Winske [1990]. This bow shock asymmetry is observed to be larger at Mars than at Venus

  19. Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances

    DEFF Research Database (Denmark)

    Tatrallyay, M.; Erdos, G.; Nemeth, Z.;

    2012-01-01

    the cusp observed by the Cluster spacecraft were best predicted by the 3-D model of Lin et al. (2010). The applied empirical bow shock models and the 3-D semi-empiric bow shock model combined with magnetohydrodynamic (MHD) solution proved to be insufficient for predicting the observed unusual bow...... shock locations during large interplanetary disturbances. The results of a global 3-D MHD model were in good agreement with the Cluster observations on 17 January 2005, but they did not predict the bow shock crossings on 31 October 2003....

  20. Trends and correlation analysis in diagnosing turbine rotor bow

    Directory of Open Access Journals (Sweden)

    Tomasz GAŁKA

    2009-01-01

    Full Text Available Permanent rotor bow in a steam turbine is a serious failure which usually demands a time-consuming and costly repair. Its vibration-related symptoms are not specific and qualitative diagnosis typically has to employ results obtained during transients.In a 230 MW power steam turbine, gradual dynamic behavior deterioration was observed, immediately after commissioning. Increase of the fundamental component of rear intermediate-pressure turbine bearing vertical vibration was detected, with the time constant of the order of months. Permanent rotor bow, exceeding 200 m, turned out to be the cause. Rotor repair resulted in a dramatic improvement of dynamic behavior, which, however, soon began to deteriorate again. Vibration spectra had been detected in the off-line mode since commissioning, which allowed to determine vibration time histories.Vibration trends analysis does not provide sufficient information to determine root cause, but allows for eliminating a number of possible malfunctions that give similar symptoms. In particular, the possibility of a sudden random-type damage due to human error is eliminated, which in fact is the most common cause of a permanent bow.Analysis of vibration amplitude correlation between vertical and axial directions reveals very strong correlation between fundamental components in the turbine under consideration, as well in the other one, in which similar failure has been observed. Third unit of the same type, apart from qualitatively different vibration trends, is characterized by correlation factors lower by a few times.This particular case is indicative of the importance of evolutionary symptoms (vibration amplitude time dependence and increase rate, as well as correlation factors in qualitative diagnosis. Such symptoms can be very useful in distinguishing between possible failures which result in similar changes of machine vibration behavior.

  1. Tibial bowing in children - what is normal? A radiographic study

    International Nuclear Information System (INIS)

    To define osseous landmarks on tibia radiographs in order to establish age-related normal values characterizing physiological tibial bowing in children. Five hundred and twenty-six patients aged 0-17 years with normal radiographs of the lower legs were identified and retrospectively reviewed by two blinded radiologists. In anteroposterior (ap)/lateral (lat)-views, 3 lines defined tibial length and angulation. Line-A connecting proximal to distal corner of tibial metaphysic, lines B and C corresponding to corners of tibial metaphysis. Angle A/B defines proximal, A/C distal tibial-angulation. Tibial curvature is defined by distance of line-D parallel to A and tangential to tibial cortex. Normal values were calculated with linear-regression. Intra-/Interreader agreement were tested with a Bland-Altman-plot. Intrareader-agreement: Reader 1 showed a bias of -0.1, standard-deviation of bias was 1.9 and 95 %-limits-of-agreement -3.9- 3.7. Reader 2: -0.01, 2.4 and -4.7- 4.7. Interreader: 0.2, 1.6 and -2.9- 3.3. Angle-A/B ap was 80-100 , increasing with age (86.5-88); angle-AC ap was 82-107 (96.8-90.5), angle-AB lat was 81-107 (93.0-98.0); angle-AC lat was 76-102 (89.5-86.5); depth of curve ap was 0-11 % (8-3.5) and lat 2-13 %, (8.5-3.5). Age dependent tibial bowing can be assessed with this new measurement system and age-related normal-values characterizing physiological tibial bowing in children is established. (orig.)

  2. Tibial bowing in children - what is normal? A radiographic study

    Energy Technology Data Exchange (ETDEWEB)

    Zbinden, Isabella [University of Basel, Department of Radiology, Basel (Switzerland); Rutz, Erich [University Children' s Hospital, Department of Orthopedic Surgery, Basel (Switzerland); Jacobson, Jon A. [University of Michigan, Department of Radiology, Ann Arbor, MI (United States); Magerkurth, Olaf [University Children' s Hospital, Department of Radiology, Basel (Switzerland); Kantonsspital Baden, Department of Radiology, Baden (Switzerland)

    2015-12-15

    To define osseous landmarks on tibia radiographs in order to establish age-related normal values characterizing physiological tibial bowing in children. Five hundred and twenty-six patients aged 0-17 years with normal radiographs of the lower legs were identified and retrospectively reviewed by two blinded radiologists. In anteroposterior (ap)/lateral (lat)-views, 3 lines defined tibial length and angulation. Line-A connecting proximal to distal corner of tibial metaphysic, lines B and C corresponding to corners of tibial metaphysis. Angle A/B defines proximal, A/C distal tibial-angulation. Tibial curvature is defined by distance of line-D parallel to A and tangential to tibial cortex. Normal values were calculated with linear-regression. Intra-/Interreader agreement were tested with a Bland-Altman-plot. Intrareader-agreement: Reader 1 showed a bias of -0.1, standard-deviation of bias was 1.9 and 95 %-limits-of-agreement -3.9- 3.7. Reader 2: -0.01, 2.4 and -4.7- 4.7. Interreader: 0.2, 1.6 and -2.9- 3.3. Angle-A/B ap was 80-100 , increasing with age (86.5-88); angle-AC ap was 82-107 (96.8-90.5), angle-AB lat was 81-107 (93.0-98.0); angle-AC lat was 76-102 (89.5-86.5); depth of curve ap was 0-11 % (8-3.5) and lat 2-13 %, (8.5-3.5). Age dependent tibial bowing can be assessed with this new measurement system and age-related normal-values characterizing physiological tibial bowing in children is established. (orig.)

  3. Relative locations of the bow shocks of the terrestrial planets

    International Nuclear Information System (INIS)

    The observed bow shock encounters at Mercury, Venus and Mars are least square fit using the same technique so that their sizes and shapes can be intercompared. The shock front of Mercury most resembles the terrestrial shock in shape, and the shock stand off distance is consistent with the observed moment. The shapes of the Venus and Mars shock fronts more resemble each other than the earth's and the stand off distances are consistent with direct interaction of the solar wind with the ionosphere on the dayside. The Venus shock is closer to the planet than the Mars shock suggesting more absorption of the solar wind at Venus

  4. Effect of Buffer Bow Structure in Ship-Ship Collision

    DEFF Research Database (Denmark)

    Yamada, Yasuhira; Endo, Hisayoshi; Pedersen, Preben Terndrup

    2008-01-01

    structure in ship-ship collisions as compared with that of standard bulbous bows. This is demonstrated by conducting a series of large-scale finite element analyses. The finite element analyses are conducted with the general-purpose nonlinear structural code “LS-DYNA”. The applied scenario is one where a...... very large crude oil carrier (VLCC) in ballast condition collides with the midship region of a D/H VLCC in a laden condition. Fracture of fillet welds, elastic-plastic material properties and strain rate effects, are taken into account in the simulations. The effect of the equivalent failure strain (FS...

  5. Power aspects of processes in the bow shock region

    Science.gov (United States)

    Sedykh, Pavel

    Bow shock is a powerful transformer of the solar wind kinetic energy into the gas dynamic and electromagnetic energy. The solar wind energy also feeds the ion acceleration process, the generation of waves in the region of bow shock, and the energy necessary to build up the foreshock. A jump of the magnetic field tangential component at front crossing means that the front carries an electric current. The solar wind kinetic energy partly transforms to gas kinetic and electromagnetic energy during its passage through the bow shock front. The transition layer (magnetosheath) can use part of this energy for accelerating of plasma, but can conversely spend part its kinetic energy on the electric power generation, which afterwards may be used by the magnetosphere. Thereby, transition layer can be both consumer (sink) and generator (source) of electric power depending upon special conditions. The direction of the current behind the bow shock front depends on the sign of the IMF B _{z}-component. It is this electric current which sets convection of plasma in motion. The process of current penetration into the magnetosphere is two-step. First, a polarization field is formed that penetrates layer-by-layer into the magnetosphere. More exactly, a pulse corresponding to this field penetrates into the plasma. Then, if the system is inhomogeneous, the flow may redistribute the pressure so that gradients appearing in the plasma induce an electric current. In power terms, this electric current is required to maintain convection in the inhomogeneous system. Any change in the external current through the magnetosphere causes a convection restructuring within a time on the order of travel time of the magnetosonic wave from the magnetopause to the center of the system, because the restructuring wave comes from both flanks. Using the expressions obtained in this paper for normal components of the electric current, the flow of matter brought into the magnetosphere can be estimated. A

  6. Effect of Buffer Bow Structure in Ship-Ship Collision

    DEFF Research Database (Denmark)

    Yamada, Yasuhira; Endo, Hisayoshi; Pedersen, Preben Terndrup

    2008-01-01

    structure in ship-ship collisions as compared with that of standard bulbous bows. This is demonstrated by conducting a series of large-scale finite element analyses. The finite element analyses are conducted with the general-purpose nonlinear structural code “LS-DYNA”. The applied scenario is one where...... a very large crude oil carrier (VLCC) in ballast condition collides with the midship region of a D/H VLCC in a laden condition. Fracture of fillet welds, elastic-plastic material properties and strain rate effects, are taken into account in the simulations. The effect of the equivalent failure strain (FS...

  7. Design of Compact Trapezoidal Bow-Tie Chipless RFID Tag

    OpenAIRE

    Lei Xu; Kama Huang

    2015-01-01

    This paper presents a novel compact design of a low cost fully printable slot-loaded bowtie chipless RFID tag. The tag consists of two trapezoidal metallic patches loaded with multiple slot resonators. Slots with similar size or adjacent frequencies are loaded alternately on two bow-tie patches to double the number of data bits within the UWB frequency band without increasing the mutual coupling between slots. A coding capacity of 12 bits is obtained with 12 slots within a reasonable size of ...

  8. 75 FR 59706 - Medicine Bow Hydro, LLC; Notice of Preliminary Permit Application Accepted for Filing and...

    Science.gov (United States)

    2010-09-28

    ... Bow Pumped Storage Project (Medicine Bow Project) to be located in Carbon County, Idaho. The sole...-foot-high earth and rockfill or concrete-face rockfill dam; creating an 121-acre lower reservoir with a...-long concrete-lined low pressure tunnel; (4) a 19-foot-diameter, 5,060-foot-long high pressure...

  9. Far-UV bow shock nebula around PSR J0437-4715

    CERN Document Server

    Rangelov, Blagoy; Kargaltsev, Oleg; Durant, Martin; Bykov, Andrei M; Krassilchtchikov, Alexandre

    2016-01-01

    Pulsars traveling at supersonic speeds are often accompanied by cometary bow shocks seen in Halpha. We report on the first detection of a pulsar bow shock in the far-ultraviolet (FUV). We detected it in FUV images of the nearest millisecond pulsar J0437-4715 obtained with the Hubble Space Telescope. The images reveal a bow-like structure positionally coincident with part of the previously detected Halpha bow shock, with an apex at 10'' ahead of the moving pulsar. Its FUV luminosity, L(1250-2000 A) ~ 5x10^28 erg/s, exceeds the Halpha luminosity from the same area by a factor of 10. The FUV emission could be produced by the shocked ISM matter or, less likely, by relativistic pulsar wind electrons confined by strong magnetic field fluctuations in the bow shock. In addition, in the FUV images we found a puzzling extended (~3'' in size) structure overlapping with the limb of the bow shock. If related to the bow shock, it could be produced by an inhomogeneity in the ambient medium or an instability in the bow shock...

  10. Rare Etiology of Bow Hunter’s Syndrome and Systematic Review of Literature

    Science.gov (United States)

    Rastogi, Vaibhav; Rawls, Ashley; Moore, Omar; Victorica, Benjamin; Khan, Sheema; Saravanapavan, Pradeepan; Midivelli, Sunitha; Raviraj, Prathap; Khanna, Anna; Bidari, Sharathchandra; Hedna, Vishnumurthy S

    2015-01-01

    BACKGROUND Bow Hunter’s Syndrome is a mechanical occlusion of the vertebral artery which leads to a reduction in blood flow in posterior cerebral circulation resulting in transient reversible symptomatic vertebrobasilar insufficiency. CASE DESCRIPTION We present a case of Bow Hunter’s syndrome in a 53-year-old male that occurred after the patient underwent surgical correction of a proximal left subclavian artery aneurysm. Shortly after the surgery, the patient began to complain of transient visual changes, presyncopal spells, and dizziness upon turning his head to the left. A transcranial doppler ultrasound confirmed the diagnosis of Bow Hunter’s syndrome. SYSTEMIC REVIEW We analyzed the data on 153 patients with Bow Hunter’s syndrome from the literature. An osteophyte was the most common cause of vertebral artery occlusion, and left vertebral artery was more commonly involved in patients with Bow Hunter’s syndrome. Dynamic angiography was the definitive imaging modality to confirm the diagnosis, and surgery was most successful in alleviating symptoms. CONCLUSION We believe that this is the first case of iatrogenic Bow Hunter’s syndrome after surgical intervention for an aneurysm repair, and the largest review of literature of Bow Hunter’s syndrome. Dynamic angiography is the gold standard for the diagnosis of Bow Hunter’s syndrome. Surgery should be considered as the primary treatment approach in these patients, especially those who have bony compression as the etiology. PMID:26301025

  11. 76 FR 65717 - City of Broken Bow, OK; Notice of Availability of Final Environmental Assessment

    Science.gov (United States)

    2011-10-24

    ... Commission's (Commission or FERC) regulations, 18 CFR part 380 (Order No. 486, 52 FR 47897), the Office of Energy Projects has reviewed the application for an Original Major License for the Broken Bow Re... Energy Regulatory Commission City of Broken Bow, OK; Notice of Availability of Final...

  12. 75 FR 33290 - City of Broken Bow, OK; Notice of Availability of Environmental Assessment

    Science.gov (United States)

    2010-06-11

    ... Regulatory Commission's (Commission) regulations, 18 CFR part 380 (Order No. 486, 52 FR 47897), the Office of Energy Projects has reviewed the application for an Original Major License for the Broken Bow Re... Energy Regulatory Commission City of Broken Bow, OK; Notice of Availability of Environmental...

  13. Smashing the Guitar: An Evolving Neutron Star Bow Shock

    CERN Document Server

    Chatterjee, S

    2003-01-01

    The Guitar nebula is a spectacular example of an H-alpha bow shock nebula produced by the interaction of a neutron star with its environment. The radio pulsar B2224+65 is traveling at ~800--1600 km/s (for a distance of 1--2 kpc), placing it on the high-velocity tail of the pulsar velocity distribution. Here we report time evolution in the shape of the Guitar nebula, the first such observations for a bow shock nebula, as seen in H-alpha imaging with the Hubble Space Telescope. The morphology of the nebula provides no evidence for anisotropy in the pulsar wind, nor for fluctuations in the pulsar wind luminosity. The nebula shows morphological changes over two epochs spaced by seven years that imply the existence of significant gradients and inhomogeneities in the ambient interstellar medium. These observations offer astrophysically unique, in situ probes of length scales between 5E-4 pc and 0.012 pc. Model fitting suggests that the nebula axis -- and thus the three-dimensional velocity vector -- lies within 20 ...

  14. Quasilinear simulations of interplanetary shocks and Earth's bow shock

    Science.gov (United States)

    Afanasiev, Alexandr; Battarbee, Markus; Ganse, Urs; Vainio, Rami; Palmroth, Minna; Pfau-Kempf, Yann; Hoilijoki, Sanni; von Alfthan, Sebastian

    2016-04-01

    We have developed a new self-consistent Monte Carlo simulation model for particle acceleration in shocks. The model includes a prescribed large-scale magnetic field and plasma density, temperature and velocity profiles and a self-consistently computed incompressible ULF foreshock under the quasilinear approximation. Unlike previous analytical treatments, our model is time dependent and takes full account of the anisotropic particle distributions and scattering in the wave-particle interaction process. We apply the model to the problem of particle acceleration at traveling interplanetary (IP) shocks and Earth's bow shock and compare the results with hybrid-Vlasov simulations and spacecraft observations. A qualitative agreement in terms of spectral shape of the magnetic fluctuations and the polarization of the unstable mode is found between the models and the observations. We will quantify the differences of the models and explore the region of validity of the quasilinear approach in terms of shock parameters. We will also compare the modeled IP shocks and the bow shock, identifying the similarities and differences in the spectrum of accelerated particles and waves in these scenarios. The work has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 637324 (HESPERIA). The Academy of Finland is thanked for financial support. We acknowledge the computational resources provided by CSC - IT Centre for Science Ltd., Espoo.

  15. Design and Analysis of the First BOWS Contest

    Directory of Open Access Journals (Sweden)

    Barni M

    2007-01-01

    Full Text Available The break our watermarking system (BOWS contest was launched in the framework of the activities carried out by the European Network of Excellence for Cryptology ECRYPT. The aim of the contest was to investigate how and when an image watermarking system can be broken while preserving the highest possible quality of the content, in the case the watermarking system is subject to a massive worldwide attack. The great number of participants and the echo that the contest has had in the watermarking community contributed to make BOWS a great success. From a scientific point of view, many insights into the problems attackers have to face with when operating in a practical scenario have been obtained, confirming the threat posed by the sensitivity attack, which turned out to be the most successful attack. At the same time, several interesting modifications of such an attack have been proposed to make it work in a real scenario under limited communication and time resources. This paper describes how the contest has been designed and analyzes the general progress of the attacks during the contest.

  16. Lunar Surface Potential Increases during Terrestrial Bow Shock Traversals

    Science.gov (United States)

    Collier, Michael R.; Stubbs, Timothy J.; Hills, H. Kent; Halekas, Jasper; Farrell, William M.; Delory, Greg T.; Espley, Jared; Freeman, John W.; Vondrak, Richard R.; Kasper, Justin

    2009-01-01

    Since the Apollo era the electric potential of the Moon has been a subject of interest and debate. Deployed by three Apollo missions, Apollo 12, Apollo 14 and Apollo 15, the Suprathermal Ion Detector Experiment (SIDE) determined the sunlit lunar surface potential to be about +10 Volts using the energy spectra of lunar ionospheric thermal ions accelerated toward the Moon. We present an analysis of Apollo 14 SIDE "resonance" events that indicate the lunar surface potential increases when the Moon traverses the dawn bow shock. By analyzing Wind spacecraft crossings of the terrestrial bow shock at approximately this location and employing current balancing models of the lunar surface, we suggest causes for the increasing potential. Determining the origin of this phenomenon will improve our ability to predict the lunar surface potential in support of human exploration as well as provide models for the behavior of other airless bodies when they traverse similar features such as interplanetary shocks, both of which are goals of the NASA Lunar Science Institute's Dynamic Response of the Environment At the Moon (DREAM) team.

  17. Bow Shock Leads the Way for a Speeding Hot Jupiter

    Science.gov (United States)

    Kohler, Susanna

    2015-09-01

    As hot Jupiters whip around their host stars, their speeds can exceed the speed of sound in the surrounding material, theoretically causing a shock to form ahead of them. Now, a study has reported the detection of such a shock ahead of transiting exoplanet HD 189733b, providing a potential indicator of the remarkably strong magnetic field of the planet.Rushing PlanetsDue to their proximity to their hosts, hot Jupiters move very quickly through the stellar wind and corona surrounding the star. When this motion is supersonic, the material ahead of the planet can be compressed by a bow shock and for a transiting hot Jupiter, this shock will cross the face of the host star in advance of the planets transit.In a recent study, a team of researchers by Wilson Cauley of Wesleyan University report evidence of just such a pre-transit. The teams target is exoplanet HD 189733b, one of the closest hot Jupiters to our solar system. When the authors examined high-resolution transmission spectra of this system, they found that prior to the optical transit of the planet, there was a large dip in the transmission of the first three hydrogen Balmer lines. This could well be the absorption of an optically-thick bow shock as it moves past the face of the star.Tremendous MagnetismOperating under this assumption, the authors create a model of the absorption expected from a hot Jupiter transiting with a bow shock ahead of it. Using this model, they show that a shock leading the planet at a distance of 12.75 times the planets radius reproduces the key features of the transmission spectrum.This stand-off distance is surprisingly large. Assuming that the location of the bow shock is set by the point where the planets magnetospheric pressure balances the pressure of the stellar wind or corona that it passes through, the planetary magnetic field would have to be at least 28 Gauss. This is seven times the strength of Jupiters magnetic field!Understanding the magnetic fields of exoplanets is

  18. Method of straightening a bowed nuclear fuel assembly

    International Nuclear Information System (INIS)

    A method of removing bow in a nuclear fuel assembly is disclosed. The fuel assembly has top and bottom ends fittings and a plurality of longitudinally extending thimble tube members interconnecting top and bottom end fittings. At least two transverse fuel rod support grids are axially spaced along the thimble tube members. A plurality of fuel rods are transversely spaced and supported by the fuel rod support grids. In one embodiment, a weight of known magnitude is secured on the bottom end fitting and the fuel assembly is raised with the weight secured thereon so that the weight exerts a downward force on the fuel assembly for straightening the fuel assembly and eliminating compressive stresses within the fuel assembly. In another embodiment, the bottom end fitting is secured onto the upender used for transporting fuel assemblies into and out of the containment building and the fuel assembly is pulled for straightening the fuel assembly and eliminating compressive stresses within the fuel assembly. (Author)

  19. Method of straightening a bowed nuclear fuel assembly

    International Nuclear Information System (INIS)

    This patent describes a method of removing the bow in a nuclear fuel assembly, the fuel assembly having top and bottom end fittings, a plurality of longitudinally extending thimble tube members interconnecting top and bottom end fittings, at least two transverse fuel rod support grids axially spaced along the thimble tube members, and a plurality of fuel rods transversely spaced and supported by the fuel rod support grids, the method comprising the steps of securing the bottom end fitting to a predetermined location under water within the containment building of a nuclear fuel reactor and pulling vertically upward along the longitudinal axis of the nuclear fuel assembly with a force on the top end fitting so that a force of between three thousand and four thousand pounds is exerted on the nuclear fuel assembly for substantially straightening the fuel assembly and eliminating most of the compressive stresses within the fuel assembly

  20. On the peculiar shapes of some pulsar bow-shock nebulae

    Science.gov (United States)

    Bandiera, Rino

    Pulsar bow-shock nebulae are pulsar-wind nebulae formed by the direct interaction of pulsar relativistic winds with the interstellar medium. The bow-shock morphology, well outlined in Hα for some objects, is an effect of the supersonic pulsar motion with respect to the ambient medium. However, in a considerable fraction of cases (e.g. the nebulae associated to PSR B2224+65, PSR B0740-28, PSR J2124-3358) clear deviations from the classical bow shock shape are observed. Such deviations are usually interpreted as due to ambient density gradients and/or to pulsar-wind anisotropies. Here I present a different interpretation, aiming at explaining deviations from the standard morphology as signs of the peculiar physical conditions present in these objects. Using dimensional arguments, I show that, unlike normal pulsar-wind nebulae, in pulsar bow-shock nebulae the mean free path of the highest-energy particles may be comparable with the bow-shock head. I then investigate whether this may affect the shape of the bow-shock; for instance, whether a conical bow shock (like that observed in the "Guitar", the nebula associated to PSR B2224+65) does really imply an ambient density gradient. Finally, I discuss some other possible signatures of these high-energy, long mean-free-path particles.

  1. Using numerical models of bow shocks to investigate the circumstellar medium of massive stars

    International Nuclear Information System (INIS)

    Many massive stars travel through the interstellar medium at supersonic speeds. As a result they form bow shocks at the interface between the stellar wind. We use numerical hydrodynamics to reproduce such bow shocks numerically, creating models that can be compared to observations. In this paper we discuss the influence of two physical phenomena, interstellar magnetic fields and the presence of interstellar dust grains on the observable shape of the bow shocks of massive stars. We find that the interstellar magnetic field, though too weak to restrict the general shape of the bow shock, reduces the size of the instabilities that would otherwise be observed in the bow shock of a red supergiant. The interstellar dust grains, due to their inertia can penetrate deep into the bow shock structure of a main sequence O-supergiant, crossing over from the ISM into the stellar wind. Therefore, the dust distribution may not always reflect the morphology of the gas. This is an important consideration for infrared observations, which are dominated by dust emission. Our models clearly show, that the bow shocks of massive stars are useful diagnostic tools that can used to investigate the properties of both the stellar wind as well as the interstellar medium

  2. BOW. A computer code to predict lateral deflections of composite beams

    International Nuclear Information System (INIS)

    Arrays of tubes are used in many engineered structures, such as in nuclear fuel bundles and in steam generators. The tubes can bend (bow) due to in-service temperatures and loads. Assessments of bowing of nuclear fuel elements can help demonstrate the integrity of fuel and of surrounding components, as a function of operating conditions such as channel power. The BOW code calculates the bending of composite beams such as fuel elements, due to gradients of temperature and due to hydraulic forces. The deflections and rotations are calculated in both lateral directions, for given conditions of temperatures. Wet and dry operation of the sheath can be simulated. Bow accounts for the following physical phenomena: circumferential and axial variations in the temperatures of the sheath and of the pellet; cracking of pellets; grip and slip between the pellets and the sheath; hydraulic drag; restraints from endplates, from neighbouring elements, and from the pressure-tube; gravity; concentric or eccentric welds between endcap and endplate; neutron flux gradients; and variations of material properties with temperature. The code is based on fundamental principles of mechanics. The governing equations are solved numerically using the finite element method. Several comparisons with closed-form equations show that the solutions of BOW are accurate. BOW's predictions for initial in-reactor bow are also consistent with two post-irradiation measurements

  3. On the shape and motion of the Earth's bow shock

    Science.gov (United States)

    Meziane, K.; Alrefay, T. Y.; Hamza, A. M.

    2014-04-01

    Multipoint-measurements by the magnetic field Cluster-FGM (Flux Gate Magnetometer) are used to determine the local shock normal, and in turn allow the study of shock location shape and the velocity of the Earth's bow shock. The shock crossings cover orbits in which the spacecraft separation is of the order of ~600 km or less. A data selection of 133 bow shock crossings, ranging from quasi-steady perpendicular to moderately noisy oblique geometries, have been analyzed using a standard timing analysis. Prior to applying the timing technique, the magnetic field fluctuations, when present, are suppressed using low band-pass filtering. The present study contributes to similar studies conducted in the past and available in the literature through the inclusion of a larger data set. The shock standoff distance is determined conjointly with a paraboloid model and the results from a timing analysis. A statistical study reveals a standoff distance well in agreement with the standard gas dynamics model prediction for high Mach number MA. We have also found that for about half the crossings, the timing shock normals agree, within 11°, with a conic-based shock model. Our results strongly indicate that the motion of the shock is predominantly along the Sun-Earth direction; a departure from this direction is not related to the shock-crossing location. Shock velocities below ~80 km/s satisfactorily follow a nearly Gaussian distribution with zero mean and a standard deviation of ~42 km/s. Finally, we show that high speed motions are correlated with sharp increases in the solar wind upstream ram pressure, and are consistent with gas dynamics model predictions.

  4. Hybrid simulation of comet Shoemaker-Levy 9 interaction with Jovian bow shock

    Science.gov (United States)

    Lipatov, A. S.; Sharma, A. S.

    1994-01-01

    The interaction of the solar wind with comet Shoemaker-Levy 9 leading to the formation of the cometary magnetosphere and its interaction with the Jovian bow shock is simulated using a one dimensional hybrid code. The mass loading of the solar wind by the cometary ions leads to the formation of a bow shock behind which the plasma density is 2-3/cu cm and the electron temperature is 4 eV. The interaction of this system with the Jovian bow shock yields local enhancements of the magnetic field and the plasma density by factors of 4-5 and the electron temperature by 2-3.

  5. Bow shock fragmentation driven by a thermal instability in laboratory-astrophysics experiments

    OpenAIRE

    Suzuki-Vidal, F.; Lebedev, S. V.; Ciardi, A.; Pickworth, L. A.; Rodriguez, R.; Gil, J. M.; Espinosa, G. (Gaudencio); Hartigan, P.; Swadling, G. F.; Skidmore, J.; Hall, G. N.; Bennett, M; Bland, S. N.; Burdiak, G.; de Grouchy, P.

    2015-01-01

    The role of radiative cooling during the evolution of a bow shock was studied in laboratory-astrophysics experiments that are scalable to bow shocks present in jets from young stellar objects. The laboratory bow shock is formed during the collision of two counter-streaming, supersonic plasma jets produced by an opposing pair of radial foil Z-pinches driven by the current pulse from the MAGPIE pulsed-power generator. The jets have different flow velocities in the laboratory frame and the exper...

  6. Calculation of the reactivity feedback due to core assembly bowing in LMFBRs

    International Nuclear Information System (INIS)

    A computational model to calculate the reactivity feedback due to material displacements induced by assembly bowing effects has been developed and embodied in a new code called BOWPERT. While previous bowing feedback models were based on an R-Z representation of the core with user defined worth tables, the BOWPERT model is Hex-Z and requires only unambiguously defined quantities such as cross sections and fluxes. The nonuniformity of the temperature distribution in an LMFBR leads to differential thermal expansion of the walls of the assembly hexcans. These thermal expansion differentials cause the hexcan to distort or bow. Consequentially, the assembly experiences a spatial displacement, thereby resulting in a change in reactivity for the core. Although bowing effects are not expected to be sizable in large heterogeneous LMFBRs, it is important to quantify these effects

  7. Effect of Ship Bow Overhang on Water Shipping for Ship Advancing in Regular Head Waves

    Institute of Scientific and Technical Information of China (English)

    Abdeljalil Benmansour; Benameur Hamoudi; Lahouari Adjlout

    2016-01-01

    This paper presents the results of an experimental investigation dealing with the effect of bow overhang extensions on the quantity of shipping water over the foredeck in case of ships advancing in regular head waves. To perform this investigation, a series of free-running tests was conducted in regular waves using an experimental model of a multipurpose cargo ship to quantify the amount of shipping water. The tests were performed on five bow overhang variants with several combinations of wavelength and ship speed conditions. It was observed that the quantity of shipping water was affected by some parameters such as wavelength, ship speed, and bow shape in terms of an overhang extension. The results show the significant influence of an overhang extension, which is associated with the bow flare shape, on the occurrence of water shipping. These results involve the combined incoming regular waves and model speed.

  8. Bow-tie topological features of metabolic networks and the functional significance

    Institute of Scientific and Technical Information of China (English)

    ZHAO Jing; TAO Lin; YU Hong; LUO JianHua; GAO ZhiWei; LI YiXue

    2007-01-01

    Exploring the structural topology of genome-based large-scale metabolic network is essential for in vestigating possible relations between structure and functionality. Visualization would be helpful for obtaining immediate information about structural organization. In this work, metabolic networks of 75 organisms were investigated from a topological point of view. A spread bow-tie model was proposed to give a clear visualization of the bow-tie structure for metabolic networks. The revealed topological pattern helps to design more efficient algorithm specifically for metabolic networks. This coarsegrained graph also visualizes the vulnerable connections in the network, and thus could have important implication for disease studies and drug target identifications. In addition, analysis on the reciprocal links and main cores in the GSC part of bow-tie also reveals that the bow-tie structure of metabolic networks has its own intrinsic and significant features which are significantly different from those of random networks.

  9. Development of the Joyo MK-II core bowing reactivity calculation code

    International Nuclear Information System (INIS)

    The study on the passive safety test by using the Experimental Fast Reactor Joyo has been performed to demonstrate the inherent safety of fast breeder reactors. In this study, emphasis was placed on the improvement on the accuracy of the feedback reactivity analysis. As a bowing reactivity might play a significant roll in ATWS analysis because of its effectively short time constant and relatively large magnitude, an emphasis was placed upon the evaluation of the analysis precision of bowing reactivity. Taking into account of the refueling and irradiation history of the individual core component, the core bowing behavior in Joyo has been analyzed by using the MK-II core management code system MAGI, the interface code TETRAS which interpolate neutron flux and coolant temperature at the position of wrapper tube, and the core bowing calculation code BEACON. Calculation accuracy of above mentioned system was evaluated through the comparison of calculated and measured permanent distortion of subassemblies. In 1996, core bowing reactivity was calculated by AURORA code using the above calculated bowing behavior of individual core component as input. But because an approximate two dimensional material reactivity worth map was utilized in AURORA, it was made clear that some amount of error caused by extrapolation could not be neglected. Therefore calculation code ARCHCOM (Analysis of Reactivity Change due to Core Mechanics) which utilize three dimensional material reactivity worth map as input was developed for the Joyo MK-II core bowing reactivity calculation. This code reduces above mentioned extrapolation error that used to be occurred at isolated core component, such as control rod or irradiation rig and at the interface region between fuel and reflector which had sharp bowing reactivity worth gradient. (author)

  10. Numerical and experimantal analysis of a shaft bow influence on a rotor to stator contact dynamics:

    OpenAIRE

    Braut, Sanjin; Butković, Mirko; Žigulić, Roberto

    2008-01-01

    The shaft bow problem presents a real situation especially in case of slender rotors. This paper investigates the shaft bow influence on the rotor-stator contact dynamics. For this purpose the rotor is described as a simple Jeffcott model and the stator as an elastically suspended rigid ring. To test the numerical model, except a usual run down analysis, an emergency shut down after the sudden rotor unbalance increase is also analyzed. Numerical integration is carried out by the fourth-order ...

  11. Accuracy of two face-bow/semi-adjustable articulator systems in transferring the maxillary occlusal cant

    OpenAIRE

    Nazia Nazir; M Sujesh; Ravi Kumar; P Sreenivas

    2012-01-01

    Context: The precision of an arbitrary face-bow in accurately transferring the orientation of the maxillary cast to the articulator has been questioned because the maxillary cast is mounted in relation to arbitrary measurements and anatomic landmarks that vary among individuals. Aim: This study was intended to evaluate the sagittal inclination of mounted maxillary casts on two semi-adjustable articulator/face-bow systems in comparison to the occlusal cant on lateral cephalograms. Mat...

  12. Highly modular bow-tie gene circuits with programmable dynamic behavior

    OpenAIRE

    Prochazka, Laura; Angelici, Bartolomeo; Haefliger, Benjamin; Benenson, Yaakov

    2014-01-01

    Synthetic gene circuits often require extensive mutual optimization of their components for successful operation, while modular and programmable design platforms are rare. A possible solution lies in the “bow-tie” architecture, which stipulates a focal component - a “knot” - uncoupling circuits’ inputs and outputs, simplifying component swapping, and introducing additional layer of control. Here we construct, in cultured human cells, synthetic bow-tie circuits that transduce microRNA inputs i...

  13. Bow-tie topological features of metabolic networks and the functional significance

    OpenAIRE

    Jing, Zhao; Lin, Tao; Hong, Yu; Jian-Hua, Luo; Cao, Z W; Yixue, Li

    2006-01-01

    Exploring the structural topology of genome-based large-scale metabolic network is essential for investigating possible relations between structure and functionality. Visualization would be helpful for obtaining immediate information about structural organization. In this work, metabolic networks of 75 organisms were investigated from a topological point of view. A spread bow-tie model was proposed to give a clear visualization of the bow-tie structure for metabolic networks. The revealed top...

  14. On the observability of bow shocks of Galactic runaway OB stars

    CERN Document Server

    Meyer, D M -A; Kuiper, R; Kley, W

    2016-01-01

    Massive stars that have been ejected from their parent cluster and supersonically sailing away through the interstellar medium (ISM) are classified as exiled. They generate circumstellar bow shock nebulae that can be observed. We present two-dimensional, axisymmetric hydrodynamical simulations of a representative sample of stellar wind bow shocks from Galactic OB stars in an ambient medium of densities ranging from n_ISM=0.01 up to 10.0/cm3. Independently of their location in the Galaxy, we confirm that the infrared is the most appropriated waveband to search for bow shocks from massive stars. Their spectral energy distribution is the convenient tool to analyze them since their emission does not depend on the temporary effects which could affect unstable, thin-shelled bow shocks. Our numerical models of Galactic bow shocks generated by high-mass (~40 Mo) runaway stars yield H$\\alpha$ fluxes which could be observed by facilities such as the SuperCOSMOS H-Alpha Survey. The brightest bow shock nebulae are produc...

  15. Multi-Spacecraft Investigation of Terrestrial Bow Shock: Cluster Observations

    Science.gov (United States)

    Kruparova, O.; Krupar, V.; Santolik, O.; Soucek, J.; Safrankova, J.; Nemecek, Z.; Nemec, F.; Maksimovic, M.

    2015-12-01

    Due to the interaction of the solar wind with the Earth's magnetosphere, a permanent collisionless bow shock (BS) is formed in front of the nose of the magnetopause. We investigate a large number of BS crossings observed by the Cluster spacecraft between years 2001 and 2015. The FGM instruments provide us with magnetic field measurements sampled at 22 Hz, which is sufficient for a precise identification of BS crossings. We compare observed BS locations with distances predicted by gas dynamical models based on upstream plasma parameters in the solar wind. We achieve a very good agreement in a case of a paraboloid with the Earth fixed in a focus point. We use a simple timing method for the estimation of a BS normal and velocity along this normal. We found that the deviations of calculated BS normals from the paraboloid shape are within 20 degrees. We compare calculated BS velocities with several upstream parameters. We also investigate BS ramp thickness which is comparable to the Larmor radius in the case of quasi-perpendicular BS crossings.

  16. Motion Prediction of Catamaran with a Semisubmersible Bow in Wave

    Directory of Open Access Journals (Sweden)

    Sun Hanbing

    2016-01-01

    Full Text Available Compared with standard vessels, a slender catamaran with a semi-submerged bow (SSB demonstrates superior seakeeping performance. To predict the motion of an SSB catamaran, computational fluid dynamics methods are adopted in this study and results are validated through small-scale model tests. The pitch, heave, and vertical acceleration are calculated at various wavelengths and speeds. Based on the overset grid and motion region methods, this study obtains the motion responses of an SSB catamaran in regular head waves. The results of the numerical studies are validated with the experimental data and show that the overset grid method is more accurate in predicting the motion of an SSB catamaran; the errors can be controlled within 20%. The movement data in regular waves shows that at a constant speed, the motion response initially increases and then decreases with increasing wavelength. This motion response peak is due to the encountering frequency being close to the natural frequency. Under identical sea conditions, the motion response increases with the increasing Froude number. The motion prediction results, that derive from a short-term irregular sea state, show that there is an optimal speed range that can effectively reduce the amplitude of motion.

  17. Design of Compact Trapezoidal Bow-Tie Chipless RFID Tag

    Directory of Open Access Journals (Sweden)

    Lei Xu

    2015-01-01

    Full Text Available This paper presents a novel compact design of a low cost fully printable slot-loaded bowtie chipless RFID tag. The tag consists of two trapezoidal metallic patches loaded with multiple slot resonators. Slots with similar size or adjacent frequencies are loaded alternately on two bow-tie patches to double the number of data bits within the UWB frequency band without increasing the mutual coupling between slots. A coding capacity of 12 bits is obtained with 12 slots within a reasonable size of 35 mm × 33 mm. RCS of the tag has been given by simulation. Measurements have been done using a bistatic radar configuration in the frequency domain and transmission coefficient is measured. The agreement between the simulation and measurement validates this new concept of design. This tag has high data capacity and low cost and can be directly printed on product such as personal ID, credit cards, paper, and textile because it needs only one conductive layer.

  18. Comparison of accelerated ion populations observed upstream of the bow shocks at Venus and Mars

    Directory of Open Access Journals (Sweden)

    M. Yamauchi

    2011-03-01

    Full Text Available Foreshock ions are compared between Venus and Mars at energies of 0.6~20 keV using the same ion instrument, the Ion Mass Analyser, on board both Venus Express and Mars Express. Venus Express often observes accelerated protons (2~6 times the solar wind energy that travel away from the Venus bow shock when the spacecraft location is magnetically connected to the bow shock. The observed ions have a large field-aligned velocity compared to the perpendicular velocity in the solar wind frame, and are similar to the field-aligned beams and intermediate gyrating component of the foreshock ions in the terrestrial upstream region. Mars Express does not observe similar foreshock ions as does Venus Express, indicating that the Martian foreshock does not possess the intermediate gyrating component in the upstream region on the dayside of the planet. Instead, two types of gyrating protons in the solar wind frame are observed very close to the Martian quasi-perpendicular bow shock within a proton gyroradius distance. The first type is observed only within the region which is about 400 km from the bow shock and flows tailward nearly along the bow shock with a similar velocity as the solar wind. The second type is observed up to about 700 km from the bow shock and has a bundled structure in the energy domain. A traversal on 12 July 2005, in which the energy-bunching came from bundling in the magnetic field direction, is further examined. The observed velocities of the latter population are consistent with multiple specular reflections of the solar wind at the bow shock, and the ions after the second reflection have a field-aligned velocity larger than that of the de Hoffman-Teller velocity frame, i.e., their guiding center has moved toward interplanetary space out from the bow shock. To account for the observed peculiarity of the Martian upstream region, finite gyroradius effects of the solar wind protons compared to the radius of the bow shock curvature and

  19. Ship Bow Force-Deformation Curves for Ship-Impact Demand of Bridges considering Effect of Pile-Cap Depth

    OpenAIRE

    Wei Fan; Wancheng Yuan

    2014-01-01

    Since static analysis procedures in the vessel impact-resistant design codes neglect dynamic amplification effects related to bridge mass, ship-impact responses of bridges may be potentially underestimated. For this reason, several dynamic vessel-impact analysis techniques had been recently proposed, where a force-deformation curve was employed to model the vessel bow stiffness. Most of the recent works mainly focused on the force-deformation curves of the barge bows rather than the ship bows...

  20. Scattering of field-aligned beam ions upstream of Earth's bow shock

    Directory of Open Access Journals (Sweden)

    A. Kis

    2007-03-01

    Full Text Available Field-aligned beams are known to originate from the quasi-perpendicular side of the Earth's bow shock, while the diffuse ion population consists of accelerated ions at the quasi-parallel side of the bow shock. The two distinct ion populations show typical characteristics in their velocity space distributions. By using particle and magnetic field measurements from one Cluster spacecraft we present a case study when the two ion populations are observed simultaneously in the foreshock region during a high Mach number, high solar wind velocity event. We present the spatial-temporal evolution of the field-aligned beam ion distribution in front of the Earth's bow shock, focusing on the processes in the deep foreshock region, i.e. on the quasi-parallel side. Our analysis demonstrates that the scattering of field-aligned beam (FAB ions combined with convection by the solar wind results in the presence of lower-energy, toroidal gyrating ions at positions deeper in the foreshock region which are magnetically connected to the quasi-parallel bow shock. The gyrating ions are superposed onto a higher energy diffuse ion population. It is suggested that the toroidal gyrating ion population observed deep in the foreshock region has its origins in the FAB and that its characteristics are correlated with its distance from the FAB, but is independent on distance to the bow shock along the magnetic field.

  1. Global explicit particle-in-cell simulations of the nonstationary bow shock and magnetosphere

    CERN Document Server

    Yang, Zhongwei; Liu, Ying D; Parks, George K; Wang, Rui; Lu, Quanming; Hu, Huidong

    2016-01-01

    We carry out two-dimensional global particle-in-cell simulations of the interaction between the solar wind and a dipole field to study the formation of the bow shock and magnetosphere. A self-reforming bow shock ahead of a dipole field is presented by using relatively high temporal-spatial resolutions. We find that (1) the bow shock and the magnetosphere are formed and reach a quasi-stable state after several ion cyclotron periods, and (2) under the Bz southward solar wind condition the bow shock undergoes a self-reformation for low \\b{eta}i and high MA. Simultaneously, a magnetic reconnection in the magnetotail is found. For high \\b{eta}i and low MA, the shock becomes quasi-stationary, and the magnetotail reconnection disappears. In addition, (3) the magnetopause deflects the magnetosheath plasmas. The sheath particles injected at the quasi-perpendicular region of the bow shock can be convected to downstream of an oblique shock region. A fraction of these sheath particles can leak out from the magnetosheath ...

  2. Flow separation control by using bowed blade in highly loaded turbine cascades

    Institute of Scientific and Technical Information of China (English)

    YAMAMOTO; Atsumasa

    2009-01-01

    Due to the serious flow separations and centralized vortices,there are high secondary losses in highly loaded turbines.It is imperative to find measures to control the flow separation and vortices hence improve the turbine performance.This paper reports our recent progress on flow separation and vor-tices control in highly loaded turbine cascades by using bowed blades.Two sets of highly loaded tur-bine cascades with the turning angles of 113° and 160°,and each with 7 bowed blade angles 0°(straight),±10°,±20° and ±30° were experimentally investigated.Both internal flow field measurement and flow visualization on the blade surfaces were conducted,and the effects of blade bowing on the flow topology,distribution of vorticity and the flow energy loss were discussed.The results show that,for the cascade with the turning angle of 113°,the appropriately positive bow angle could reduce the flow energy loss;whereas for the cascade with the turning angle of 160°,the well selected negative bow angle can give the better aerodynamic performance.

  3. Flow separation control by using bowed blade in highly loaded turbine cascades

    Institute of Scientific and Technical Information of China (English)

    TAN ChunQing; ZHANG HuaLiang; CHEN HaiSheng; DONG XueZhi; ZHAO HongLei; YAMAMOTO Atsumasa

    2009-01-01

    Due to the serious flow separations and centralized vortices, there are high secondary losses in highly loaded turbines. It is imperative to find measures to control the flow separation and vortices hence improve the turbine performance. This paper reports our recent progress on flow separation and vor-tices control in highly loaded turbine cascades by using bowed blades. Two sets of highly loaded tur-bine cascades with the turning angles of 113°and 160°, and each with 7 bowed blade angles 0°(straight),±10°, ±20° and ±30° were experimentally investigated. Both internal flow field measurement and flow visualization on the blade surfaces were conducted, and the effects of blade bowing on the flow topology, distribution of vorticity and the flow energy loss were discussed. The results show that, for the cascade with the turning angle of 113°, the appropriately positive bow angle could reduce the flow energy loss; whereas for the cascade with the turning angle of 160°, the well selected negative bow angle can give the better aerodynamic performance.

  4. Application of high-turning bowed compressor stator to redesign of highly loaded fan stage

    Institute of Scientific and Technical Information of China (English)

    Shaobin LI; Jiexian SU; Zhongqi WANG

    2008-01-01

    A redesign of a highly loaded fan stage by using high-turning bowed compressor stator was conducted. The original tandem stator was replaced by the highly loaded bowed stator which was applicable to highly sub-sonic flow conditions. 3D contouring technique and local modification of blade were applied to the design of the bowed blade in order to improve the aerodynamic per-formance and the matching of the rotor and stator blade rows. Performance curves at different rotating speeds and performances at different operating points for both the original fan stage and redesigned fan stage were obtained by numerical simulations. The results show that the highly loaded bowed stator can be used not only to improve the structure and the aerodynamic performances at various operating points of the compressor stage but also to pro-vide high performances at off-design conditions. It is believed that the highly loaded bowed stator can advance the design of high-performance compressor.

  5. Bow Shocks from Neutron Stars Scaling Laws and HST Observations of the Guitar Nebula

    CERN Document Server

    Chatterjee, S

    2002-01-01

    The interaction of high-velocity neutron stars with the interstellar medium produces bow shock nebulae, where the relativistic neutron star wind is confined by ram pressure. We present multi-wavelength observations of the Guitar Nebula, including narrow-band H-alpha imaging with HST/WFPC2, which resolves the head of the bow shock. The HST observations are used to fit for the inclination of the pulsar velocity vector to the line of sight, and to determine the combination of spindown energy loss, velocity, and ambient density that sets the scale of the bow shock. We find that the velocity vector is most likely in the plane of the sky. We use the Guitar Nebula and other observed neutron star bow shocks to test scaling laws for their size and H-alpha emission, discuss their prevalence, and present criteria for their detectability in targeted searches. The set of H-alpha bow shocks shows remarkable consistency, in spite of the expected variation in ambient densities and orientations. Together, they support the ass...

  6. On the role of the bow shock in power of magnetospheric disturbances

    Science.gov (United States)

    Sedykh, P. A.

    2011-11-01

    Bow shock is a powerful transformer of the solar wind kinetic energy into the gas dynamic and electromagnetic energy. Indeed, the magnetic field tangential component and magnetic energy density increase by factors of almost 4 and approximately 15, respectively, at the bow point when the front is crossed. A jump of the magnetic field tangential component at front crossing means that the front carries an electric current. The solar wind kinetic energy partly transforms to gas kinetic and electromagnetic energy when passage through the bow shock front. The transition layer (magnetosheath) can use the part of this energy for accelerating of plasma, but can conversely spend the part its kinetic energy on the electric power generation, which afterwards may be used by the magnetosphere. Thereby, transition layer can be both consumer and generator of electric power depending upon special conditions. The direction of current behind the bow shock front depends on the sign of the IMF Bz-component. It is this current which sets plasma convection in motion. Energetically, this external current is necessary for maintaining convection of plasma in the inhomogeneous system (magnetosphere). The generator at the bow shock front can be a sufficient source of power for supplying energy to substorm processes in the geomagnetosphere.

  7. Bow shock fragmentation driven by a thermal instability in laboratory-astrophysics experiments

    CERN Document Server

    Suzuki-Vidal, F; Ciardi, A; Pickworth, L A; Rodriguez, R; Gil, J M; Espinosa, G; Hartigan, P; Swadling, G F; Skidmore, J; Hall, G N; Bennett, M; Bland, S N; Burdiak, G; de Grouchy, P; Music, J; Suttle, L; Hansen, E; Frank, A

    2015-01-01

    The role of radiative cooling during the evolution of a bow shock was studied in laboratory-astrophysics experiments that are scalable to bow shocks present in jets from young stellar objects. The laboratory bow shock is formed during the collision of two counter-streaming, supersonic plasma jets produced by an opposing pair of radial foil Z-pinches driven by the current pulse from the MAGPIE pulsed-power generator. The jets have different flow velocities in the laboratory frame and the experiments are driven over many times the characteristic cooling time-scale. The initially smooth bow shock rapidly develops small-scale non-uniformities over temporal and spatial scales that are consistent with a thermal instability triggered by strong radiative cooling in the shock. The growth of these perturbations eventually results in a global fragmentation of the bow shock front. The formation of a thermal instability is supported by analysis of the plasma cooling function calculated for the experimental conditions with...

  8. Bow-tie antennas on a dielectric half-space - Theory and experiment

    Science.gov (United States)

    Compton, Richard C.; Mcphedran, Ross C.; Popovic, Zorana; Rebeiz, Gabriel M.; Tong, Peter P.

    1987-01-01

    A new formulation is discussed for the rigous calculation of the radiation pattern of a bow-tie antenna of finite length and infinitesimal thickness, placed on a lossless dielectric substrate. The analysis is based on a representation of the current density on the metal surface of the antenna as a sum of an imposed (quasistatic) term and a set of current modes with unknown amplitudes. Free-space fields that are expressed in terms of continuous spectra of symmetrized plane waves are matched to the current modes using the method of moments. The resulting set of equations are solved for the unknown current amplitudes. The calculations show that for increasing bow length the antenna impedance spirals rapidly to a value predicted by transmission line theory. The theory also shows that the E-plane pattern of a two-wavelength, 60-deg bow-tie antenna is dominated by low-loss current modes propagating at the dielectric wavenumber. As the bow tie narrows, the loss of the modes increases, and the dominant wavenumber tends to the quasi-static value. Pattern measurements made at 94 GHz are shown to agree well with theoretical predictions. Measurements for a long-wire antenna, a linear array of bow-tie elements, and a log-periodic antenna are also presented.

  9. Unilateral Outer Bow Expanded Cervical Headgear Force System: 3D Analysis Using Finite Element Method

    Directory of Open Access Journals (Sweden)

    Allahyar Geramy

    2015-10-01

    Full Text Available Objectives: Headgears are among the effective orthodontic appliances to achieve treatment goals. Unilateral molar distal movement is sometimes needed during an orthodontic treat- ment, which can be achieved by an asymmetric headgear. Different unilateral headgears have been introduced. The main goal of this study was to analyze the force system of uni- lateral expanded outer bow asymmetric headgears by the finite element method (FEM.Materials and Methods: Six 3D finite element models of a mesiodistal slice of the maxilla containing upper first molars, their periodontal ligaments (PDLs, cancellous bone, cortical bone, and a cervical headgear with expanded outer bow attached to maxillary first molars were designed in SolidWorks 2010 and meshed in ANSYS Workbench ver. 12.1. The mod- els were the same except for the degree of outer bow expansion. The outer bow ends were loaded with 2-Newton force. The distal driving force and the net moment were evaluated.Results: A decrease in the distalizing force in the normal side molar from 1.69 N to 1.37 N was shown by increasing the degree of unilateral expansion. At the same time, the force increased from 2.19 N to 2.49 N in the expanded side molar. A net moment increasing from 2.26 N.mm to 4.64 N.mm was also shown.Conclusion: Unilateral outer bow expansion can produce different distalizing forces in mo- lars, which increase by increasing the expansion.

  10. Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances

    DEFF Research Database (Denmark)

    Tatrallyay, M.; Erdos, G.; Nemeth, Z.; Verigin, M. I.; Vennerstrøm, Susanne

    2012-01-01

    by the interplanetary magnetic field (IMF) component transverse to the solar wind flow. The observed magnetopause crossings could be predicted with a reasonable accuracy (0.1-0.2 RE) by one of the presented models at least. For geosynchronous magnetopause crossings observed by the GOES satellites, (1......) the new model provided the best predictions when the IMF was extremely large having a large negative Bz component, and (2) the predictions of the model of Shue et al. (1998) agreed best with the observations when the solar wind dynamic pressure was extremely large. The magnetopause crossings close to...... the cusp observed by the Cluster spacecraft were best predicted by the 3-D model of Lin et al. (2010). The applied empirical bow shock models and the 3-D semi-empiric bow shock model combined with magnetohydrodynamic (MHD) solution proved to be insufficient for predicting the observed unusual bow...

  11. Transport of Solar Wind H+ and He++ Ions across Earth’s Bow Shock

    Science.gov (United States)

    Parks, G. K.; Lee, E.; Fu, S. Y.; Kim, H. E.; Ma, Y. Q.; Yang, Z. W.; Liu, Y.; Lin, N.; Hong, J.; Canu, P.; Dandouras, I.; Rème, H.; Goldstein, M. L.

    2016-07-01

    We have investigated the dependence of mass, energy, and charge of solar wind (SW) transport across Earth’s bow shock. An examination of 111 crossings during quiet SW in both quasi-perpendicular and quasi-parallel shock regions shows that 64 crossings had various degrees of heating and thermalization of SW. We found 22 crossings where the SW speed was flat top distribution is ∼50 Volts. We find that the temperatures of H+ and He++ beams that penetrate the shock can sometimes be nearly the same in the upstream and downstream regions, indicating little or no heating had occurred crossing the bow shock. None of the models predict that the SW can cross the bow shock without heating. Our observations are important constraints for new models of collisionless shocks.

  12. A matched Bow-tie antenna at 433MHz for use in underwater wireless sensor networks

    International Nuclear Information System (INIS)

    Electromagnetic (EM) wave propagation underwater is been disregarded because of attenuation at high frequencies, however the theory predicts that propagation is possible at some useful distance in the lower Industrial, Scientific and Medical (ISM) band. Common transceivers rely on narrowband antennas and matching circuit. The aim of this paper is to design a broadband 433MHz bow-tie antenna and experiment it in air and water without a matching circuit. This antenna could be attached to wireless transceivers and form a Wireless Sensor Network for deployment in various underwater applications. The bow-tie antennas were designed, simulated and constructed in laboratory. Experiments were setup carefully by using a completely isolated transmitter from electronics to avoid airborne transmission. The 433MHz. bow-tie proved its suitability for use in Underwater.

  13. Prenatal diagnosis of metatropic dysplasia: beware of the pseudo-bowing sign

    Energy Technology Data Exchange (ETDEWEB)

    Garel, Catherine [Trousseau Hospital, University Hospitals of the East of Paris, Department of Radiology, Paris (France); Hopital d' Enfants Armand-Trousseau, Department of Radiology, Paris (France); Dhouib, Amira; Sileo, Chiara; Ducou le Pointe, Hubert [Trousseau Hospital, University Hospitals of the East of Paris, Department of Radiology, Paris (France); Cormier-Daire, Valerie [Paris Descartes University, Sorbonne Paris Cite, Necker-Enfants-Malades Hospital, Department of Genetics, Paris (France)

    2014-03-15

    Metatropic dysplasia is a very rare form of osteochondrodysplasia with only one case of prenatal diagnosis described in the literature. It is characterized by marked shortening of the long bones with severe platyspondyly and dumbbell-shape metaphyses. We report a case of metatropic dysplasia that was diagnosed prenatally and describe the findings on US and CT. The pregnancy was terminated and the post-mortem radiographs are shown. The woman had been referred for short and bowed long bones. Severe metaphyseal enlargement was a misleading finding because it had been misinterpreted as limb bowing. Thus when abnormal curvature of the long bones is observed at prenatal US, attention should be drawn not only to the diaphyses but also to the metaphyses because severe metaphyseal enlargement might be responsible for pseudo-bowing. (orig.)

  14. An Investigation of the Flow Structure Upstream of Slowly Moving Blunt Bows.

    Science.gov (United States)

    Strayer, T. Darton

    The structure of two dimensional bow waves generated by blunt bows is investigated experimentally, analytically, and numerically. In tow tank experiments, bow wave profiles ahead of cylindrical and box shaped bow models, having drafts of 0.136m and 0.11m respectively, are measured using a capacitance type probe for flows in the 0.21 to 0.74 Froude number range. Far upstream several waves are observed, and using linear wave theory they are shown to be transient in nature, generated during the initial acceleration of the bow models. Measured profiles closer to the towed model show a non-breaking bow wave characterized by a sharp monotonic free surface rise to a relatively flat elevated plateau region located adjacent of the bow. In addition small scale waves are shed from the bow and at moderate Froude numbers these waves completely dissipate inside the plateau region, while at lower Froude numbers they propagate further upstream. Using regular perturbation methods first and second order asymptotic solutions are derived for small draft Froude numbers and their subsequent comparison with experimental results shows that both the double body (leading order) and higher order flow solutions poorly approximate the actual flow near the bow. It is found, however, that if the bow geometry is modified to include a triangular shaped separation region the leading order solution mimics measured wave profiles. This non-negligible region located beneath the plateau region is found to extend upstream to the plateau's leading edge. Moreover, results indicate that the location of the so-called separation point, the point at which the flow separates from the free surface and passes beneath the recirculating flow, coincides with the plateau's leading edge and that the sharp free surface rise is an inviscid flow phenomenon. The generation of a free surface shear layer and the flow separation phenomenon are examined as well as a possible cause and effect relationship between them

  15. Transport of Solar Wind H+ and He++ Ions across Earth’s Bow Shock

    Science.gov (United States)

    Parks, G. K.; Lee, E.; Fu, S. Y.; Kim, H. E.; Ma, Y. Q.; Yang, Z. W.; Liu, Y.; Lin, N.; Hong, J.; Canu, P.; Dandouras, I.; Rème, H.; Goldstein, M. L.

    2016-07-01

    We have investigated the dependence of mass, energy, and charge of solar wind (SW) transport across Earth’s bow shock. An examination of 111 crossings during quiet SW in both quasi-perpendicular and quasi-parallel shock regions shows that 64 crossings had various degrees of heating and thermalization of SW. We found 22 crossings where the SW speed was flat top distribution is ˜50 Volts. We find that the temperatures of H+ and He++ beams that penetrate the shock can sometimes be nearly the same in the upstream and downstream regions, indicating little or no heating had occurred crossing the bow shock. None of the models predict that the SW can cross the bow shock without heating. Our observations are important constraints for new models of collisionless shocks.

  16. The bow shock structure of IRS 7 - Wind-wind collision near the Galactic center

    Science.gov (United States)

    Yusef-Zadeh, Farhad; Melia, Fulvio

    1992-01-01

    New structural details of ionized gas associated with IRS 7, a mass-losing supergiant near the Galactic center, are reported, and radio continuum and theoretical maps are compared. High-resolution multiconfiguration VLA observations of IRS 7 reveal ionized gas with a bow shock structure at a wavelength of 2 cm. The apex of the bow shock is facing more toward the cluster of blue stellar objects, known as IRS 16, than Sgr A*, the compact nonthermal source near the Galaxy's dynamical center. It is inferred that the shape of the mass-losing envelope of IRS 7 is influenced by Galactic winds from IRS 16. It is concluded from a comparison of the morphology of the ionized envelope of IRS 7 with simple theoretical modeling of the bow shock structure that the shape of the shock results from the collision between the Galactic center and stellar winds rather than from the motion of IRS 7 through the interstellar medium.

  17. Active current sheets and hot flow anomalies in Mercury's bow shock

    CERN Document Server

    Uritsky, V M; Boardsen, S A; Sundberg, T; Raines, J M; Gershman, D J; Collinson, G; Sibeck, D; Khazanov, G V; Anderson, B J; Korth, H

    2013-01-01

    Hot flow anomalies (HFAs) represent a subset of solar wind discontinuities interacting with collisionless bow shocks. They are typically formed when the normal component of motional (convective) electric field points toward the embedded current sheet on at least one of its sides. The core region of an HFA contains hot and highly deflected ion flows and rather low and turbulent magnetic field. In this paper, we report first observations of HFA-like events at Mercury identified over a course of two planetary years. Using data from the orbital phase of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission, we identify a representative ensemble of active current sheets magnetically connected to Mercury's bow shock. We show that some of these events exhibit unambiguous magnetic and particle signatures of HFAs similar to those observed earlier at other planets, and present their key physical characteristics. Our analysis suggests that Mercury's bow shock does not only mediate the flo...

  18. Effects of the bow on social organization in Western North America.

    Science.gov (United States)

    Bettinger, Robert L

    2013-01-01

    The bow more than doubled, likely tripled, the success of individuals bent on killing animal or human targets (Box ). The advent of this revolutionary technology generated different responses in western North America depending on subsistence and sociopolitical organization at the time of its arrival, roughly 2300 - 1300 B.P. Its effect was substantial in California and the Great Basin, particularly on group size, which in many places diminished as a consequence of the bow's reliability. The counter-intuitive result was to increase within group-relatedness enough to encourage intensification of plant resources, previously considered too costly. The bow rose to greatest direct economic importance with the arrival of the horse, and was put to most effective use by former Great Basin groups who maintained the family band system that had developed around intensive Great Basin plant procurement, adapting the same organization to a lifestyle centered on the equestrian pursuit of buffalo and warfare. PMID:23776048

  19. A numerical study on bow shocks around the lightning return stroke channel

    International Nuclear Information System (INIS)

    Bow shock structures are important to various hydrodynamics and magnetohydrodynamics (MHD) phenomena in geophysics and astrophysics. The formation and propagation of bow shocks around the lightning return stroke channel are investigated based on the self-similar motion theory and simulated with a two-dimensional Eulerian finite volume resistive radiation MHD code. In this framework, as verification of theoretical models, the evolving structures of many quantities, such as the plasma density, temperature, pressure, shock velocity, and magnetic field, can be obtained, which present all the characteristics of bow shocks in the lightning return stroke processes. The evolution characteristics and the configuration of the curved return stroke channels, e.g., the non-ideal effects and the scaling laws, are discussed in detail. The results may have applications for some observed features of the return stroke channels and other phenomena in the lightning discharge plasmas

  20. A numerical study on bow shocks around the lightning return stroke channel

    Energy Technology Data Exchange (ETDEWEB)

    Chen, Qiang, E-mail: cq0405@126.com; Chen, Bin, E-mail: emcchen@163.com; Yi, Yun [National Key Laboratory of Electromagnetic Environment and Electro-Optical Engineering, PLA University of Science and Technology, Nanjing 210007 (China); Chen, P. F., E-mail: chenpf@nju.edu.cn [School of Astronomy and Space Science, Nanjing University, Nanjing 210023 (China); Mao, Yunfei [The China Satellite Maritime Tracking and Control Department, Yuan Wang III, Jiangyin 214400 (China); Xiong, Run [Engineer Academy of PLA, Xuzhou 221004 (China)

    2015-03-15

    Bow shock structures are important to various hydrodynamics and magnetohydrodynamics (MHD) phenomena in geophysics and astrophysics. The formation and propagation of bow shocks around the lightning return stroke channel are investigated based on the self-similar motion theory and simulated with a two-dimensional Eulerian finite volume resistive radiation MHD code. In this framework, as verification of theoretical models, the evolving structures of many quantities, such as the plasma density, temperature, pressure, shock velocity, and magnetic field, can be obtained, which present all the characteristics of bow shocks in the lightning return stroke processes. The evolution characteristics and the configuration of the curved return stroke channels, e.g., the non-ideal effects and the scaling laws, are discussed in detail. The results may have applications for some observed features of the return stroke channels and other phenomena in the lightning discharge plasmas.

  1. Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances

    Directory of Open Access Journals (Sweden)

    M. Tátrallyay

    2012-12-01

    Full Text Available Three events are discussed from the declining phase of the last solar cycle when the magnetopause and/or the bow shock were observed unusually close to the Earth due to major interplanetary disturbances. The observed extreme locations of the discontinuities are compared with the predictions of three magnetopause and four bow shock models which describe them in considerably different ways using statistical methods based on observations. A new 2-D magnetopause model is introduced (based on Verigin et al., 2009 which takes into account the pressure of the compressed magnetosheath field raised by the interplanetary magnetic field (IMF component transverse to the solar wind flow. The observed magnetopause crossings could be predicted with a reasonable accuracy (0.1–0.2 RE by one of the presented models at least. For geosynchronous magnetopause crossings observed by the GOES satellites, (1 the new model provided the best predictions when the IMF was extremely large having a large negative Bz component, and (2 the predictions of the model of Shue et al. (1998 agreed best with the observations when the solar wind dynamic pressure was extremely large. The magnetopause crossings close to the cusp observed by the Cluster spacecraft were best predicted by the 3-D model of Lin et al. (2010. The applied empirical bow shock models and the 3-D semi-empiric bow shock model combined with magnetohydrodynamic (MHD solution proved to be insufficient for predicting the observed unusual bow shock locations during large interplanetary disturbances. The results of a global 3-D MHD model were in good agreement with the Cluster observations on 17 January 2005, but they did not predict the bow shock crossings on 31 October 2003.

  2. Accuracy of two face-bow/semi-adjustable articulator systems in transferring the maxillary occlusal cant

    Directory of Open Access Journals (Sweden)

    Nazia Nazir

    2012-01-01

    Full Text Available Context: The precision of an arbitrary face-bow in accurately transferring the orientation of the maxillary cast to the articulator has been questioned because the maxillary cast is mounted in relation to arbitrary measurements and anatomic landmarks that vary among individuals. Aim: This study was intended to evaluate the sagittal inclination of mounted maxillary casts on two semi-adjustable articulator/face-bow systems in comparison to the occlusal cant on lateral cephalograms. Materials and Methods: Maxillary casts were mounted on the Hanau and Girrbach semi-adjustable articulators following face-bow transfer with their respective face-bows. The sagittal inclination of these casts was measured in relation to the fixed horizontal reference plane using physical measurements. Occlusal cant was measured on lateral cephalograms. SPSS software (version 11.0, Chicago, IL, USA was used for statistical analysis. Repeated measures analysis of variance and Tukey′s tests were used to evaluate the results (P < 0.05. Results: Comparison of the occlusal cant on the articulators and cephalogram revealed statistically significant differences. Occlusal plane was steeper on Girrbach Artex articulator in comparison to the Hanau articulator. Conclusion: Within the limitations of this study, it was found that the sagittal inclination of the mounted maxillary cast achieved with Hanau articulator was closer to the cephalometric occlusal cant as compared to that of the Girrbach articulator. Among the two articulators and face-bow systems, the steepness of sagittal inclination was greater on Girrbach semi-adjustable articulator. Different face-bow/articulator systems could result in different orientation of the maxillary cast, resulting in variation in stability, cuspal inclines and cuspal heights.

  3. Intervention of laser periphery iridectomy to posterior iris bowing in high myopic eyes

    Institute of Scientific and Technical Information of China (English)

    WANG Hong-tao; WANG Ning-li; LI Shu-ning

    2012-01-01

    Background For some high myopic patients with posterior iris bowing,laser periphery iridectomy should be performed pre-operation to prevent pupil block glaucoma if these patients would have phakic intraocular lens implantation to correct high myopia.So we had the opportunity to analysis the influence of laser iridectomy on posterior iris bowing.Methods Eighteen high myopic patients with posterior iris bowing (11 males and 7 females) were involved in the study in Beijing Tongren Eye Center from March 2008 to July 2008.Phakic intraocular lens were implanted to correct their ametropia.The mean age was (32±6) years (range,25-40 years).The center anterior chamber depth,the pupil diameter,the posterior iris bowing depth and the anterior chamber angle were measured with anterior segment coherence tomography (AS-OCT) under the normal condition,myosis condition induced by 2% pilocarpine,laser periphery iridectomy after myosis,and 2% pilocarpine eluting condition respectively.Results There was no significant difference of center anterior chamber depth under the four conditions (P=0.512).The pupil constricted after pilocarpine (P=0.001).After laser iridectomy performed and pilocarpine eluted,posterior iris bowing depth reduced more than that in normal condition (P=0.003).The anterior chamber angle reduced significantly after laser periphery iridectomy and pilocarpine eluted (P=0.012).Conclusion Laser periphery iridectomy can reduce the posterior iris bowing,which might be due to the change in aqueous circulate pathway.

  4. Asymmetric Outer Bow Length and Cervical Headgear Force System: 3D Analysis Using Finite Element Method

    Directory of Open Access Journals (Sweden)

    Allahyar Geramy

    2015-10-01

    Full Text Available Objectives: This study sought to assess distal and lateral forces and moments of asymmetric headgears by variable outer bow lengths.Materials and Methods: Four 3D finite element method (FEM models of a cer- vical headgear attached to the maxillary first molars were designed in SolidWorks2010 software and transferred to ANSYS Workbench ver. 11 software. Modelscontained the first molars, their periodontal ligament (PDL, cancellous and cor- tical bones, a mesiodistal slice of the maxillae and the headgear. Models were the same except for the outer bow length in headgears. The headgear was symmetric in model 1. In models 2 to 4, the headgears were asymmetric in length with dif- ferences of 5mm, 10mm and 15mm, respectively. A 2.5 N force in horizontal plane was applied and the loading manner of each side of the outer bow was cal- culated trigonometrically using data from a volunteer.Results: The 15mm difference in outer bow length caused the greatest difference in lateral (=0.21 N and distal (= 1.008 N forces and also generated moments (5.044 N.mm.Conclusion: As the difference in outer bow length became greater, asymmetric effects increased. Greater distal force in the longer arm side was associated with greater lateral force towards the shorter arm side and more net yawing moment. Clinical Relevance:A difference range of 1mm to 15 mm of length in cervical headgear can be consi-dered as a safe length of outer bow shortening in clinical use.

  5. 77 FR 16028 - Broken Bow Wind, LLC; Supplemental Notice That Initial Market-Based Rate Filing Includes Request...

    Science.gov (United States)

    2012-03-19

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF ENERGY Federal Energy Regulatory Commission Broken Bow Wind, LLC; Supplemental Notice That Initial Market- Based Rate...-referenced proceeding of Broken Bow Wind, LLC's application for market-based rate authority, with...

  6. Comparison of accelerated ion populations observed upstream of the bow shocks at Venus and Mars

    OpenAIRE

    Yamauchi, M.; Y. Futaana; Fedorov, A.; Frahm, R. A.; Winningham, J. D.; Dubinin, E.; R. Lundin; Barabash, S.; Holmström, M.; Mazelle, C.; Sauvaud, J.-A.; T. L. Zhang; W. Baumjohann; A. J. Coates; Fraenz, M.

    2011-01-01

    Foreshock ions are compared between Venus and Mars at energies of 0.6 similar to 20 keV using the same ion instrument, the Ion Mass Analyser, on board both Venus Express and Mars Express. Venus Express often observes accelerated protons (2 similar to 6 times the solar wind energy) that travel away from the Venus bow shock when the spacecraft location is magnetically connected to the bow shock. The observed ions have a large field-aligned velocity compared to the perpendicular velocity in the ...

  7. Towards a real-time system for teaching novices good violin bowing technique

    OpenAIRE

    van der Linden, Janet; Schoonderwaldt, Erwin; Bird, Jon

    2009-01-01

    We describe the ongoing development of a system to support the teaching of good posture and bowing technique to novice violin players. Using an inertial motion capture system we can track in real-time: i) a player’s bowing action (and measure how it deviates from a target trajectory); ii) whether the player is holding their violin correctly. We detail some initial experiments that show that vibrotactile feedback can guide arm movements in one and two dimensions. We then present some prelimina...

  8. A benchmark study of procedures for analysis of axial crushing of bulbous bows

    DEFF Research Database (Denmark)

    Yamada, Yasuhira; Pedersen, Preben Terndrup

    2008-01-01

    Simplified methods to estimate mean axial crushing forces of plated structures are reviewed and applied to a series of experimental results for axial crushing of large-scale bulbous bow models. Methods based on intersection unit elements such as L-, T- and X-type elements as well as methods based...... on plate unit elements are employed in the analyses. The crushing forces and the total absorbed energy obtained by the simplified analyses are compared with those obtained from large-scale bulbous bow experiments. The accuracy and the applicability of these methods are discussed in detail....

  9. FAILURES AND DEFECTS IN THE BUILDING PROCESS – APPLYING THE BOW-TIE APPROACH

    DEFF Research Database (Denmark)

    Jørgensen, Kirsten

    2009-01-01

    site was observed from the very start to the very end and all failures and defects of a certain size were recorded and analysed. The methodological approach used in this analysis was the bow-tie model from the area of safety research. It combines critical-event analysis for both causes and effects with...... event-tree analysis. The paper describes this analytical approach as an introduction to a new concept for understanding failures and defects in construction. Analysing the many critical events in the building process with the bow-tie model visualises the complexity of causes. This visualisation offers...

  10. Corporate-Feed Multilayer Bow-Tie Antenna Array Design Using a Simple Transmission Line Model

    OpenAIRE

    Didouh, S.; Abri, M.; F. T. Bendimerad

    2012-01-01

    A transmission line model is used to design corporate-fed multilayered bow-tie antennas arrays; the simulated antennas arrays are designed to resonate at the frequencies 2.4 GHz, 5 GHz, and 8 GHz corresponding to RFID, WIFI, and radars applications. The contribution of this paper consists of modeling multilayer bow-tie antenna array fed through an aperture using transmission line model. The transmission line model is simple and precise and allows taking into account the whole geometrical, ele...

  11. Method for evaluating bow tie filter angle-dependent attenuation in CT: Theory and simulation results

    OpenAIRE

    Boone, John M.

    2009-01-01

    Purpose: Dosimetry in computed tomography (CT) is increasingly based on Monte Carlo studies that define the dose in the patient (in mGy) as a function of air kerma (free in air) at isocenter (mGy). The accuracy of Monte Carlo studies depends in part on the accuracy of the characterization of the bow tie filter for a given CT scanner model. A simple method for characterizing the bow tie filter attenuation profile in CT scanners would therefore be very useful. The theory behind such a method is...

  12. Ground-state magnetic phase diagram of bow-tie graphene nanoflakes in external magnetic field

    OpenAIRE

    Szałowski, Karol

    2013-01-01

    The magnetic phase diagram of a ground state is studied theoretically for graphene nanoflakes of bow-tie shape and various size in external in-plane magnetic field. The tight-binding Hamiltonian supplemented with Hubbard term is used to model the electronic structure of the systems in question. The existence of the antiferromagnetic phase with magnetic moments localized at the sides of the bow-tie is found for low field and a field-induced spin-flip transition to ferromagnetic state is predic...

  13. Analysis of Silver Ink Bow-Tie RFID Tag Antennas Printed on Paper Substrates

    OpenAIRE

    Sari Merilampi; Leena Ukkonen; Lauri Sydänheimo; Pekka Ruuskanen; Markku Kivikoski

    2007-01-01

    In this study, polymeric silver inks, paper substrates, and screen printing were used to produce prototype Bow-Tie tags. Because of increasing interest in applying passive UHF-RFID systems in paper industry, the Bow-Tie antenna used in this study was designed to work through paper. The maximum reliable read ranges of the tags were measured thorough stacked paper and also in air. The analysis and functioning of the antenna design are also discussed. All inks and paper substrates were suitable ...

  14. The distant bow shock and magnetotail of Venus - Magnetic field and plasma wave observations

    Science.gov (United States)

    Russell, C. T.; Luhmann, J. G.; Elphic, R. C.; Scarf, F. L.

    1981-01-01

    An examination of the magnetic field and plasma wave data obtained by the Pioneer Venus orbiter in the wake region behind Venus discloses a well developed bow shock whose location is similar to that observed on previous missions in contrast to the dayside bow shock. Venus also has a well developed magnetotail in which the field strenght is enhanced over magnetosheath values and in which the magnetic field is aligned approximately with the solar wind direction. The boundary between magnetosheath and magnetotail is also marked by a change in the plasma wave spectrum.

  15. Application of the Bow Tie method for evaluation of safety in the procedure of logging wells

    International Nuclear Information System (INIS)

    This work consists of an assessment of security in the practice of logging of oil wells, using the method of Bow Tie for being a simple method of evaluation of the risk, which makes it possible in a structured way to set priorities to manage risk

  16. X-ray Emission Line Profiles from Wind Clump Bow Shocks in Massive Stars

    CERN Document Server

    Ignace, R; Cassinelli, J P

    2012-01-01

    The consequences of structured flows continue to be a pressing topic in relating spectral data to physical processes occurring in massive star winds. In a preceding paper, our group reported on hydrodynamic simulations of hypersonic flow past a rigid spherical clump to explore the structure of bow shocks that can form around wind clumps. Here we report on profiles of emission lines that arise from such bow shock morphologies. To compute emission line profiles, we adopt a two component flow structure of wind and clumps using two "beta" velocity laws. While individual bow shocks tend to generate double horned emission line profiles, a group of bow shocks can lead to line profiles with a range of shapes with blueshifted peak emission that depends on the degree of X-ray photoabsorption by the interclump wind medium, the number of clump structures in the flow, and the radial distribution of the clumps. Using the two beta law prescription, the theoretical emission measure and temperature distribution throughout the...

  17. Fuzzy Bayesian Network-Bow-Tie Analysis of Gas Leakage during Biomass Gasification

    Science.gov (United States)

    Yan, Fang; Xu, Kaili; Yao, Xiwen; Li, Yang

    2016-01-01

    Biomass gasification technology has been rapidly developed recently. But fire and poisoning accidents caused by gas leakage restrict the development and promotion of biomass gasification. Therefore, probabilistic safety assessment (PSA) is necessary for biomass gasification system. Subsequently, Bayesian network-bow-tie (BN-bow-tie) analysis was proposed by mapping bow-tie analysis into Bayesian network (BN). Causes of gas leakage and the accidents triggered by gas leakage can be obtained by bow-tie analysis, and BN was used to confirm the critical nodes of accidents by introducing corresponding three importance measures. Meanwhile, certain occurrence probability of failure was needed in PSA. In view of the insufficient failure data of biomass gasification, the occurrence probability of failure which cannot be obtained from standard reliability data sources was confirmed by fuzzy methods based on expert judgment. An improved approach considered expert weighting to aggregate fuzzy numbers included triangular and trapezoidal numbers was proposed, and the occurrence probability of failure was obtained. Finally, safety measures were indicated based on the obtained critical nodes. The theoretical occurrence probabilities in one year of gas leakage and the accidents caused by it were reduced to 1/10.3 of the original values by these safety measures. PMID:27463975

  18. Beacon: A three-dimensional structural analysis code for bowing history of fast breeder reactor cores

    International Nuclear Information System (INIS)

    The core elements of an LMFBR are bowed due to radial gradients of both temperature and neutron flux in the core. Since all hexagonal elements are multiply supported by adjacent elements or the restraint system, restraint forces and bending stresses are induced. In turn, these forces and stresses are relaxed by irradiation enhanced creep of the material. The analysis of the core bowing behavior requires a three-dimensional consideration of the mechanical interactions among the core elements, because the core consists of different kinds of elements and of fuel assemblies with various burnup histories. A new computational code BEACON has been developed for analyzing the bowing behavior of an LMFBR's core in three dimensions. To evaluate mechanical interactions among core elements, the code uses the analytical method of the earlier SHADOW code. BEACON analyzes the mechanical interactions in three directions, which form angles of 600 with one another. BEACON is applied to the 600 sector of a typical LMFBR's core for analyzing the bowing history during one equilibrium cycle. 120 core elements are treated, assuming the boundary condition of rotational symmetry. The application confirms that the code can be an effective tool for parametric studies as well as for detailed structural analysis of LMFBR's core. (orig.)

  19. Non-stationarity of the quasi-perpendicular bow shock: comparison between Cluster observations and simulations

    Czech Academy of Sciences Publication Activity Database

    Comisel, H.; Scholer, M.; Souček, Jan; Matsukiyo, S.

    2011-01-01

    Roč. 29, č. 2 (2011), s. 263-274. ISSN 0992-7689 Institutional research plan: CEZ:AV0Z30420517 Keywords : bow shock * Cluster * plasma waves * shock waves Subject RIV: BL - Plasma and Gas Discharge Physics Impact factor: 1.842, year: 2011 http://www.ann-geophys.net/29/263/2011/angeo-29-263-2011.pdf

  20. "Heaven Starts at Your Parents' Feet": Adolescent Bowing to Parents and Associated Spiritual Attitudes

    Science.gov (United States)

    Thanissaro, Phra Nicholas

    2010-01-01

    In a quantitative survey of religious attitudes and practices in a multi-religious sample of 369 school pupils aged between 13 and 15 in London, the practice of bowing to parents was found widespread in 22% of adolescents spanning several religious affiliations and ethnicities--especially Buddhists, Hindus and those of Indian, African and "Other…

  1. 26 CFR 48.4161(b)-1 - Imposition and rates of tax; bows and arrows.

    Science.gov (United States)

    2010-04-01

    ... 26 Internal Revenue 16 2010-04-01 2010-04-01 true Imposition and rates of tax; bows and arrows. 48.4161(b)-1 Section 48.4161(b)-1 Internal Revenue INTERNAL REVENUE SERVICE, DEPARTMENT OF THE TREASURY (CONTINUED) MISCELLANEOUS EXCISE TAXES MANUFACTURERS AND RETAILERS EXCISE TAXES Sporting Goods §...

  2. Beam-Steerable Microstrip-Fed Bow-Tie Antenna Array for Fifth Generation Cellular Communications

    DEFF Research Database (Denmark)

    Ojaroudiparchin, Naser; Shen, Ming; Pedersen, Gert Frølund

    2016-01-01

    bow-tie antennas have been used at the top-edge region of mobile phone PCB. The antenna elements fed by microstrip lines are designed to operate at 17 GHz. The simulated results give good performances in terms of different antenna parameters. In addition, an investigation on the distance between...

  3. Fuzzy Bayesian Network-Bow-Tie Analysis of Gas Leakage during Biomass Gasification.

    Science.gov (United States)

    Yan, Fang; Xu, Kaili; Yao, Xiwen; Li, Yang

    2016-01-01

    Biomass gasification technology has been rapidly developed recently. But fire and poisoning accidents caused by gas leakage restrict the development and promotion of biomass gasification. Therefore, probabilistic safety assessment (PSA) is necessary for biomass gasification system. Subsequently, Bayesian network-bow-tie (BN-bow-tie) analysis was proposed by mapping bow-tie analysis into Bayesian network (BN). Causes of gas leakage and the accidents triggered by gas leakage can be obtained by bow-tie analysis, and BN was used to confirm the critical nodes of accidents by introducing corresponding three importance measures. Meanwhile, certain occurrence probability of failure was needed in PSA. In view of the insufficient failure data of biomass gasification, the occurrence probability of failure which cannot be obtained from standard reliability data sources was confirmed by fuzzy methods based on expert judgment. An improved approach considered expert weighting to aggregate fuzzy numbers included triangular and trapezoidal numbers was proposed, and the occurrence probability of failure was obtained. Finally, safety measures were indicated based on the obtained critical nodes. The theoretical occurrence probabilities in one year of gas leakage and the accidents caused by it were reduced to 1/10.3 of the original values by these safety measures. PMID:27463975

  4. Turbulence at quasi-parallel and quasi-perpendicular bow shocks

    Science.gov (United States)

    Pitna, Alexander; Zastenker, Georgy; Nemecek, Zdenek; Safrankova, Jana

    2016-07-01

    A solar wind is a highly turbulent medium carrying various modes of magnetohydrodynamic and kinetic instabilities. During its supersonic expansion, it meets obstacles like planetary magnetospheres and bow shocks are formed. Depending on the orientation of the ambient magnetic field with respect to the local shock normal, either quasi-parallel or quasi-perpendicular shocks can be formed. Particles reflected at the ramp of the quasi-parallel shock are streaming far upstream along the magnetic field lines, giving rise to all sorts of instabilities like SLAMS and ULF waves. In the case of the quasi-perpendicular bow shock, the reflected particles influence only a narrow upstream region of the order of the proton gyroradius but the downstream plasma becomes highly turbulent regardless of the shock type. We analyze the high cadence (31 ms) data from the BMSW instrument onboard the Spektr-R spacecraft and compare the frequency spectra of observed turbulence in MHD and kinetic ranges in upstream and downstream regions of the supercritical quasi-parallel and quasi-perpendicular bow shocks. We found that the change in the fluctuation level (from upstream to downstream) as well as the spectral indices differ substantially in the MHD and kinetic ranges for both types of bow shock.

  5. Extended Red Objects and Stellar Wind Bow Shocks in the Carina Nebula

    CERN Document Server

    Sexton, Remington O; Smith, Nathan; Babler, Brian L; Meade, Marilyn R; Rudolph, Alexander L

    2014-01-01

    We report the results of infrared photometry on 39 extended red objects (EROs) in the Carina Nebula, observed with the Spitzer Space Telescope. Most EROs are identified by bright, extended 8.0 um emission, which ranges from 10'' to 40'' in size, but our sample also includes 4 EROs identified by extended 24 um emission. Of particular interest are nine EROs associated with late O or early B-type stars and characterized by arc-shaped morphology, suggesting dusty, stellar-wind bow shocks. These objects are preferentially oriented towards the central regions of the Carina Nebula, suggesting that these bow shocks are generally produced by the interactions of OB winds with the bulk expansion of the H II region rather than high proper motion. We identify preferred regions of mid-infrared color space occupied by our bow shock candidates, which also contain bow shock candidates in M17 and RCW 49 but are well-separated from polycyclic aromatic hydrocarbon emission or circumstellar discs. Color cuts identify an additiona...

  6. Further evidence for a dynamically generated secondary bow in $^{13}$C+$^{12}$C rainbow scattering

    CERN Document Server

    Ohkubo, S; Ogloblin, A A

    2015-01-01

    The existence of a secondary bow is confirmed for 13C+12C nuclear rainbow scattering in addition to the 16O+12C system. This is found by studying the experimental angular distribution of 13C+12C scattering at the incident 13C energy $E_L$=250 MeV with an extended double folding (EDF) model that describes all the diagonal and off-diagonal coupling potentials derived from the microscopic wave functions for 12C using a density-dependent nucleon-nucleon force. The Airy minimum at \\theta$ $\\approx$70$^\\circ$, which is not reproduced by a conventional folding potential, is revealed to be a secondary bow generated dynamically by a coupling to the excited state 2+ (4.44 MeV) of 12C. The essential importance of the quadruple {\\it Y2} term (reorientation term) of potential of the excited state 2+ of 12C for the emergence of a secondary bow is found. The mechanism of the secondary bow is intuitively explained by showing how the trajectories are refracted dynamically into the classically forbidden angular region beyond t...

  7. Double-sided printed bow-tie antenna with notch filter for UWB applications

    OpenAIRE

    Hirata, Akimasa; ヒラタ, アキマサ; 平田, 晃正

    2009-01-01

    This letter proposes a double-sided printed bow-tie antenna with a notch band. The notch filter is based on a grounded patch inserted into the feeding microstrip line. The advantage of the structure is its tunability of the notch band.

  8. Fuzzy Bayesian Network-Bow-Tie Analysis of Gas Leakage during Biomass Gasification.

    Directory of Open Access Journals (Sweden)

    Fang Yan

    Full Text Available Biomass gasification technology has been rapidly developed recently. But fire and poisoning accidents caused by gas leakage restrict the development and promotion of biomass gasification. Therefore, probabilistic safety assessment (PSA is necessary for biomass gasification system. Subsequently, Bayesian network-bow-tie (BN-bow-tie analysis was proposed by mapping bow-tie analysis into Bayesian network (BN. Causes of gas leakage and the accidents triggered by gas leakage can be obtained by bow-tie analysis, and BN was used to confirm the critical nodes of accidents by introducing corresponding three importance measures. Meanwhile, certain occurrence probability of failure was needed in PSA. In view of the insufficient failure data of biomass gasification, the occurrence probability of failure which cannot be obtained from standard reliability data sources was confirmed by fuzzy methods based on expert judgment. An improved approach considered expert weighting to aggregate fuzzy numbers included triangular and trapezoidal numbers was proposed, and the occurrence probability of failure was obtained. Finally, safety measures were indicated based on the obtained critical nodes. The theoretical occurrence probabilities in one year of gas leakage and the accidents caused by it were reduced to 1/10.3 of the original values by these safety measures.

  9. Double bow shocks around young, runaway red supergiants: application to Betelgeuse

    CERN Document Server

    Mackey, Jonathan; Neilson, Hilding R; Langer, Norbert; Meyer, Dominique M -A

    2012-01-01

    A significant fraction of massive stars are moving supersonically through the interstellar medium (ISM), either due to disruption of a binary system or ejection from their parent star cluster. The interaction of their wind with the ISM produces a bow shock. In late evolutionary stages these stars may undergo rapid transitions from red to blue and vice versa on the Hertzsprung-Russell diagram, with accompanying rapid changes to their stellar winds and bow shocks. Recent 3D simulations of the bow shock produced by the nearby runaway red supergiant (RSG) Betelgeuse, under the assumption of a constant wind, indicate that the bow shock is very young (<30000 years old), hence Betelgeuse may have only recently become a RSG. To test this possibility, we have calculated stellar evolution models for single stars which match the observed properties of Betelgeuse in the RSG phase. The resulting evolving stellar wind is incorporated into 2D hydrodynamic simulations in which we model a runaway blue supergiant (BSG) as i...

  10. A ballistic bow shock model for jet-driven protostellar outflow shells

    CERN Document Server

    Ostriker, E C; Stone, J M; Mundy, L G; Ostriker, Eve C.; Lee, Chin-Fei; Stone, James M.; Mundy, Lee G.

    2001-01-01

    We analyze the dynamics of the shell produced when a bow shock from a collimated jet propagates into the surrounding medium. Under interstellar conditions, the shock is radiative, and a ballistic approximation for the shell flow is appropriate beyond the working surface where the jet impacts its surroundings. The solution is then determined by the ambient and jet densities and velocities and by the momentum impulse applied in the working surface. Using estimates for these impulses (confirmed by separate numerical simulations), we obtain solutions for the shell structure, and for the range of velocities in the shell at any point. We provide predictions for the position-velocity and mass-velocity relations expected for plane-of-sky bow-shock shells, and for the bulk shell properties. In a companion paper, we show that these analytic solutions are in excellent agreement with the results of direct numerical simulations. We argue that classical molecular (CO) outflows cannot be purely jet-driven, because the bow-s...

  11. Joyo MK-II core bowing analysis based on thermal-hydraulic analysis

    International Nuclear Information System (INIS)

    A study on the inherent safety test at the Experimental Fast Reactor Joyo has been performed to demonstrate the inherent safety of fast breeder reactors. In this study, emphasis was placed on the improvement on the feedback reactivity calculation accuracy. The investigation work for core bowing calculation has been continued because it is expected to cause negative feedback reactivity that would improve the passive safety of a fast breeder reactor. The core bowing behavior in JOYO has been analyzed by the system which consists of the MK-II core management code system MAGI, the interface code TETRAS and the core bowing calculation code BEACON. As it was supposed that the coolant flow inside of the reactor vessel might effects on wrapper tube temperature, detailed coolant flow was calculated by single phase multidimensional thermal-hydraulic analysis code AQUA. (1) As a result of the AQUA calculation, it was made clear that the coolant flow effect on the coolant temperature was negligible in fuel region. (2) The coolant temperature at the outlet of reflectors adjacent to a fuel subassembly are affected by the coolant flow that comes from the outlet of reflectors in the 6th and the 7th row. It decreases the outlet temperature of the reflectors in the 5th row in AQUA calculation. (3) High temperature coolant flow exists in neighbor of the outlet of reflectors in the 8-10th row. As a result, coolant temperature calculated by AQUA are higher in 30-40degC than that calculated by TETRAS. It was made clear that the coolant flow inside of the reactor vessel had no effect on driver fuel bowing, which was the dominant factor of the core bowing reactivity. On the other hand, in reflectors region, it affects the wrapper tube temperature, which determine the irreversible swelling and creep. Essentially, in order to verify the feedback reactivity effect caused by the core bowing, it is desired to measure the mechanical behavior of the subassemblies under power operation, but it is

  12. Method for evaluating bow tie filter angle-dependent attenuation in CT: Theory and simulation results

    International Nuclear Information System (INIS)

    Purpose: Dosimetry in computed tomography (CT) is increasingly based on Monte Carlo studies that define the dose in the patient (in mGy) as a function of air kerma (free in air) at isocenter (mGy). The accuracy of Monte Carlo studies depends in part on the accuracy of the characterization of the bow tie filter for a given CT scanner model. A simple method for characterizing the bow tie filter attenuation profile in CT scanners would therefore be very useful. The theory behind such a method is proposed. Methods: A measurement protocol is discussed mathematically and demonstrated using computer simulation. The proposed method requires the placement of a radiation monitor at the periphery of the CT field, and the time domain signal (kerma rate versus time) is measured with good temporal resolution (∼200 Hz or better) and with all other objects (e.g., patient couch) retracted from the field of view. Knowledge of the source to isocenter distance (or alternately, the isocenter to probe distance) is required. The stationary detector records the kerma rate versus time signal as the gantry rotates through several revolutions. From this temporal data, signal processing techniques are used to extract in-phase peaks, as well as out-of-phase kerma rate levels. From these data, the distance from isocenter to the probe can be determined (or, alternatively, the source to isocenter distance), and the angle-dependent bow tie filter attenuation can be computed. By measuring the angle-dependent bow tie filter attenuation at several kVp settings, the bow tie composition versus fan angle can be computed using basis decomposition techniques. Results: The simulations illustrated that with 2% added noise in the kerma rate versus time signal, the attenuation properties of a hypothetical two component (aluminum and polymethyl methacrylate) bow tie filter could be determined (r2>0.99). Although the computed basis material thicknesses were not exactly equal to the actual thicknesses, their

  13. Mach 5 bow shock control by a nanosecond pulse surface dielectric barrier discharge

    International Nuclear Information System (INIS)

    Bow shock perturbations in a Mach 5 air flow, produced by low-temperature, nanosecond pulse, and surface dielectric barrier discharge (DBD), are detected by phase-locked schlieren imaging. A diffuse nanosecond pulse discharge is generated in a DBD plasma actuator on a surface of a cylinder model placed in air flow in a small scale blow-down supersonic wind tunnel. Discharge energy coupled to the actuator is 7.3-7.8 mJ/pulse. Plasma temperature inferred from nitrogen emission spectra is a few tens of degrees higher than flow stagnation temperature, T = 340 ± 30 K. Phase-locked Schlieren images are used to detect compression waves generated by individual nanosecond discharge pulses near the actuator surface. The compression wave propagates upstream toward the baseline bow shock standing in front of the cylinder model. Interaction of the compression wave and the bow shock causes its displacement in the upstream direction, increasing shock stand-off distance by up to 25%. The compression wave speed behind the bow shock and the perturbed bow shock velocity are inferred from the Schlieren images. The effect of compression waves generated by nanosecond discharge pulses on shock stand-off distance is demonstrated in a single-pulse regime (at pulse repetition rates of a few hundred Hz) and in a quasi-continuous mode (using a two-pulse sequence at a pulse repetition rate of 100 kHz). The results demonstrate feasibility of hypersonic flow control by low-temperature, repetitive nanosecond pulse discharges.

  14. CPR methodology with new steady-state criterion and more accurate statistical treatment of channel bow

    International Nuclear Information System (INIS)

    An overview is given of existing CPR design criteria and the methods used in BWR reload analysis to evaluate the impact of channel bow on CPR margins. Potential weaknesses in today's methodologies are discussed. Westinghouse in collaboration with KKL and Axpo - operator and owner of the Leibstadt NPP - has developed an optimized CPR methodology based on a new criterion to protect against dryout during normal operation and with a more rigorous treatment of channel bow. The new steady-state criterion is expressed in terms of an upper limit of 0.01 for the dryout failure probability per year. This is considered a meaningful and appropriate criterion that can be directly related to the probabilistic criteria set-up for the analyses of Anticipated Operation Occurrences (AOOs) and accidents. In the Monte Carlo approach a statistical modeling of channel bow and an accurate evaluation of CPR response functions allow the associated CPR penalties to be included directly in the plant SLMCPR and OLMCPR in a best-estimate manner. In this way, the treatment of channel bow is equivalent to all other uncertainties affecting CPR. Emphasis is put on quantifying the statistical distribution of channel bow throughout the core using measurement data. The optimized CPR methodology has been implemented in the Westinghouse Monte Carlo code, McSLAP. The methodology improves the quality of dryout safety assessments by supplying more valuable information and better control of conservatisms in establishing operational limits for CPR. The methodology is demonstrated with application examples from the introduction at KKL. (authors)

  15. Experimental Investigation of the Effect of Bow Profiles on Resistance of an Underwater Vehicle in Free Surface Motion

    Institute of Scientific and Technical Information of China (English)

    Mehran Javadi; Mojtaba Dehghan Manshadi; Saeid Kheradmand; Mohammad Moonesun

    2015-01-01

    In this paper, towing tank experiments are conducted to study the behavior of flow on a model of the underwater vehicle with various shapes of bows, i.e. tango and standard bows in free surface motion tests. The total resistances for different Froude numbers are considered experimentally. The towing tank is equipped with a trolley that can operate in through 0.05–6 m/s speed with ±0.02 m/s accuracy. Furthermore, the study is done on hydrodynamic coefficients i.e. total, residual and friction resistance coefficients, and the results are compared. Finally, the study on flow of wave fields around bows is done and wave filed around two bows are compared. The Froude number interval is between 0.099 and 0.349. Blockage fraction for the model is fixed to 0.005 3. The results showed that the residual resistance of the standard bow in 0.19 to 0.3 Froude number is more than the tango bow in surface motion which causes more total resistance for the submarine. Finally, details of wave generated by the bow are depicted and the effects of flow pattern on resistance drag are discussed.

  16. A comparative analysis of 3D flow fields between straight and bowed blades in a steam turbine

    Institute of Scientific and Technical Information of China (English)

    M.HASSANVAND; WANG Zhong-qi 王仲奇; WANG Song-tao 王松涛

    2004-01-01

    A commercial Navier-Stokes flow solver has been employed tor simulating steady subsonic flow characteristics and analyzing the comparative features of flow fields between straight and bowed blades applied to the stator of a high pressure steam turbine. For comparison, we have studied the effects of bowed blades on the wakes of stator trailing edge and horse shoe vortex in the rotor. It was found that the position of wakes for bowed blades is shifted toward the blade suction side. Also, we have discussed and compared the entropy generation and energy loss caused by dissipation mechanism within the boundary layers on the hub and shroud; and temperature gradient in meridional plane.

  17. THE ROLE OF PICKUP IONS ON THE STRUCTURE OF THE VENUSIAN BOW SHOCK AND ITS IMPLICATIONS FOR THE TERMINATION SHOCK

    Energy Technology Data Exchange (ETDEWEB)

    Lu Quanming; Shan Lican; Zhang Tielong; Wu Mingyu; Wang Shui [CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei 230026 (China); Zank, Gary P. [Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville, AL 35899 (United States); Yang Zhongwei [SOA Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai (China); Du Aimin, E-mail: qmlu@ustc.edu.cn [Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029 (China)

    2013-08-20

    The recent crossing of the termination shock by Voyager 2 has demonstrated the important role of pickup ions (PUIs) in the physics of collisionless shocks. The Venus Express (VEX) spacecraft orbits Venus in a 24 hr elliptical orbit that crosses the bow shock twice a day. VEX provides a unique opportunity to investigate the role of PUIs on the structure of collisionless shocks more generally. Using VEX observations, we find that the strength of the Venusian bow shock is weaker when solar activity is strong. We demonstrate that this surprising anti-correlation is due to PUIs mediating the Venusian bow shock.

  18. Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study

    OpenAIRE

    K. Meziane; Mazelle, C.; Wilber, M.; Lequéau, D.; J. P. Eastwood; H. Rème; Dandouras, I.; J. A. Sauvaud; Bosqued, J. M.; Parks, G. K.; Kistler, L. M.; McCarthy, M.; Klecker, B.; Korth, A.; M.-B. Bavassano-Cattaneo

    2004-01-01

    An energetic ion (E≤40) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at ~0.5 Re from the shock and the averaged bow shock θ

  19. Comparison of plasma wave measurements in the bow shocks at Earth, Jupiter, Saturn, Uranus and Neptune

    International Nuclear Information System (INIS)

    The authors present plasma wave measurements from the Voyager 2 crossing of Neptune's bow shock and compare them with measurements from the bow shocks of Earth, Jupiter, Saturn and Uranus. The wave amplitudes above 0.01fp, when normalized to the solar wind ion thermal energy density at each planet, are significantly higher at the outer planets than at Earth. Despite the differences in amplitude the shock spectra of all the planets can be fitted to curves of similar form in this frequency range. The total normalized electric field energy densities exhibit an exponential dependence on ion thermal Mach number. Magnetosheath wave energies are comparable at all of the planets when normalized to the downstream plasma pressure

  20. A Study of Near-Field Radiation Pattern of Bow-Tie Dipole on Ground

    Institute of Scientific and Technical Information of China (English)

    ZHAN Yi; LIANG Changhong; FANG Guangyou; YUAN Hongwei

    2001-01-01

    The study of bow-tie antenna forpulse'radiation in a ground penetrating radar systemis complicated due to the existence of reflections fromthe feed,the far end of the antenna,the air-groundinterface and their interactions.The FDTD methodsare applied in this paper by incorporating a trans-parent source,a bow-tie antenna above the ground,and a lossy soil to investigate the issues.Numeri-cal verifications are conducted to check the accuracyof the method.The radiation properties are demon-strated by near-field radiation patterns and time do-main waveforms at different positions.The influencesdue to different antenna heights and soil parametersare also discussed in detail.

  1. Characterization of Saturn's bow shock: Magnetic field observations of quasi-perpendicular shocks

    CERN Document Server

    Sulaiman, A H; Dougherty, M K

    2016-01-01

    Collisionless shocks vary drastically from terrestrial to astrophysical regimes resulting in radically different characteristics. This poses two complexities. Firstly, separating the influences of these parameters on physical mechanisms such as energy dissipation. Secondly, correlating observations of shock waves over a wide range of each parameter, enough to span across different regimes. Investigating the latter has been restricted since the majority of studies on shocks at exotic regimes (such as supernova remnants) have been achieved either remotely or via simulations, but rarely by means of in-situ observations. Here we present the parameter space of MA bow shock crossings from 2004-2014 as observed by the Cassini spacecraft. We find that Saturn's bow shock exhibits characteristics akin to both terrestrial and astrophysical regimes (MA of order 100), which is principally controlled by the upstream magnetic field strength. Moreover, we determined the {\\theta}Bn of each crossing to show that Saturn's (days...

  2. Diagnosis of the Thermal Bow of a Shaft in a Three Stage Centrifugal Compressor

    Institute of Scientific and Technical Information of China (English)

    2003-01-01

    In practice many turbo-machines driven by motors are started up to operational speed within a very short time, i.e. in less than 20 seconds. For this type of machines the compatibility of thermal deformation of the rotor structure must be taken into account in the machine design, or the thermal deformation will be constrained and a huge resultant force can cause the shaft bending and consequently resulting in violent vibrations. In this paper, detection of thermal bow of a shaft in a three stage centrifugal compressor in a petrochemical plant is presented. The diagnostic results show that the thermal bow was induced by the incompatibility of axial thermal deformation of the rotor structure. A remedial action allowing free axial thermal expansion of the outer parts of the rotor is suggested.

  3. UWB Bi-directional Bow-tie antenna loaded by rings

    Science.gov (United States)

    Peng, Lin; Sun, Kai; Xie, Ji-yang; Qiu, Yu-jie; Jiang, Xing

    2016-07-01

    Performances of bow-tie antennae can be improved by loading a ring. Specially, the distorted radiation patterns of the reference bow-tie antenna (RBA) at high frequencies become less distorted when a ring is added. That is due to the disciplined current flows trained by the ring. Furthermore, when more rings are loaded, which act as reflectors, higher directivities are obtained and, patterns become bi-directional. Antennae with no ring (RBA), one ring, two rings (three cases), three rings, and four rings are investigated. Research find that loading more rings means better directivity. The directivity of the RBA varies from 2.29 dB to 3.66 dB for the frequency band from 2.5 to 7.5 GHz while the directivity for the four-ring-loaded case varies from 4.27 dB to 7.61 dB in that frequency band.

  4. Intensity and energy spectrum of electrons accelerated in the earth's bow shock

    Science.gov (United States)

    Anderson, K. A.

    1974-01-01

    Shock waves accelerate charged particles in the solar atmosphere, in interplanetary space and around the earth's magnetosphere. Acceleration of both electrons and protons occurs in the earth's bow-shock. The acceleration of protons up to 100 keV appears to be a steady state process and may even occur upstream from the bow shock due to waves generated by reflected solar wind protons. The electrons, on the other hand, are known to be accelerated in or near the shock. The intensity of these electrons ranges from about 100 to 2,000 per sr-sq cm-sec-keV at 14 keV. The energy spectrum is not a simple power low and is highly variable. If segments of the spectra are fitted to a power low, slopes ranging from -2 to -4.5 result over the energy range 0.5 to 100 keV.

  5. Analysis of Silver Ink Bow-Tie RFID Tag Antennas Printed on Paper Substrates

    Directory of Open Access Journals (Sweden)

    Sari Merilampi

    2007-01-01

    Full Text Available In this study, polymeric silver inks, paper substrates, and screen printing were used to produce prototype Bow-Tie tags. Because of increasing interest in applying passive UHF-RFID systems in paper industry, the Bow-Tie antenna used in this study was designed to work through paper. The maximum reliable read ranges of the tags were measured thorough stacked paper and also in air. The analysis and functioning of the antenna design are also discussed. All inks and paper substrates were suitable as antenna material and the prototype tag antennas had good reading performance. The maximum reliable read ranges were quite the same as for copper and aluminum tags studied elsewhere. This means that printed UHF tags are competitive solutions for the identification of simple mass products.

  6. Highly modular bow-tie gene circuits with programmable dynamic behaviour.

    Science.gov (United States)

    Prochazka, Laura; Angelici, Bartolomeo; Haefliger, Benjamin; Benenson, Yaakov

    2014-01-01

    Synthetic gene circuits often require extensive mutual optimization of their components for successful operation, while modular and programmable design platforms are rare. A possible solution lies in the 'bow-tie' architecture, which stipulates a focal component-a 'knot'-uncoupling circuits' inputs and outputs, simplifying component swapping, and introducing additional layer of control. Here we construct, in cultured human cells, synthetic bow-tie circuits that transduce microRNA inputs into protein outputs with independently programmable logical and dynamic behaviour. The latter is adjusted via two different knot configurations: a transcriptional activator causing the outputs to track input changes reversibly, and a recombinase-based cascade, converting transient inputs into permanent actuation. We characterize the circuits in HEK293 cells, confirming their modularity and scalability, and validate them using endogenous microRNA inputs in additional cell lines. This platform can be used for biotechnological and biomedical applications in vitro, in vivo and potentially in human therapy. PMID:25311543

  7. Mapping the Structure of Directed Networks: Beyond the "Bow-tie" Diagram

    OpenAIRE

    Timár, G.; Goltsev, A. V.; Dorogovtsev, S. N.; Mendes, J. F. F.

    2016-01-01

    We reveal a hierarchical organization of finite directed components---tendrils---around the giant components represented by the celebrated "bow-tie" diagram for directed networks. We develop an efficient algorithm to find tendril layers. It is used together with the message passing technique, generalized to directed graphs, to find the structure and attack tolerance of complex networks, such as the World Wide Web, the neural network of Caenorhabditis elegans, and others. We introduce a genera...

  8. 3D hybrid simulations of the interaction of a magnetic cloud with a bow shock

    Science.gov (United States)

    Turc, L.; Fontaine, D.; Savoini, P.; Modolo, R.

    2015-08-01

    In this paper, we investigate the interaction of a magnetic cloud (MC) with a planetary bow shock using hybrid simulations. It is the first time to our knowledge that this interaction is studied using kinetic simulations which include self-consistently both the ion foreshock and the shock wave dynamics. We show that when the shock is in a quasi-perpendicular configuration, the MC's magnetic structure in the magnetosheath remains similar to that in the solar wind, whereas it is strongly altered downstream of a quasi-parallel shock. The latter can result in a reversal of the magnetic field north-south component in some parts of the magnetosheath. We also investigate how the MC affects in turn the outer parts of the planetary environment, i.e., from the foreshock to the magnetopause. We find the following: (i) The decrease of the Alfvén Mach number at the MC's arrival causes an attenuation of the foreshock region because of the weakening of the bow shock. (ii) The foreshock moves along the bow shock's surface, following the rotation of the MC's magnetic field. (iii) Owing to the low plasma beta, asymmetric flows arise inside the magnetosheath, due to the magnetic tension force which accelerates the particles in some parts of the magnetosheath and slows them down in others. (iv) The quasi-parallel region forms a depression in the shock's surface. Other deformations of the magnetopause and the bow shock are also highlighted. All these effects can contribute to significantly modify the solar wind/magnetosphere coupling during MC events.

  9. Serendipitous discovery of an infrared bow shock near PSR J1549–4848 with Spitzer

    Energy Technology Data Exchange (ETDEWEB)

    Wang, Zhongxiang [Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030 (China); Kaplan, David L. [Physics Department, University of Wisconsin-Milwaukee, Milwaukee, WI 53211 (United States); Slane, Patrick [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Morrell, Nidia [Las Campanas Observatory, Observatories of the Carnegie Institution of Washington, La Serena (Chile); Kaspi, Victoria M. [Department of Physics, McGill University, 3600 University Street, Montreal, QC H3A 2T8 (Canada)

    2013-06-01

    We report on the discovery of an infrared cometary nebula around PSR J1549–4848 in our Spitzer survey of a few middle-aged radio pulsars. Following the discovery, multi-wavelength imaging and spectroscopic observations of the nebula were carried out. We detected the nebula in Spitzer Infrared Array Camera 8.0, Multiband Imaging Photometer for Spitzer 24 and 70 μm imaging, and in Spitzer IRS 7.5-14.4 μm spectroscopic observations, and also in the Wide-field Infrared Survey Explorer all-sky survey at 12 and 22 μm. These data were analyzed in detail, and we find that the nebula can be described with a standard bow shock shape, and that its spectrum contains polycyclic aromatic hydrocarbon and H{sub 2} emission features. However, it is not certain which object drives the nebula. We analyze the field stars and conclude that none of them can be the associated object because stars with a strong wind or mass ejection that usually produce bow shocks are much brighter than the field stars. The pulsar is approximately 15'' away from the region in which the associated object is expected to be located. In order to resolve the discrepancy, we suggest that a highly collimated wind could be emitted from the pulsar and produce the bow shock. X-ray imaging to detect the interaction of the wind with the ambient medium- and high-spatial resolution radio imaging to determine the proper motion of the pulsar should be carried out, which will help verify the association of the pulsar with the bow shock nebula.

  10. Low-energy particles at the bow shock, magnetopause, and outer magnetosphere of Saturn

    International Nuclear Information System (INIS)

    Low-energy electron (>22 keV) and protons (> or approx. =30 keV) measured by the Low-Energy Charged Particle Experiment (LECP) during the encounters of the two Voyager spacecraft with Saturn are described. The characteristics of the dayside bow shock, magnetopause, and outer magnetosphere are emphasized. Only one crossing of the Saturian bow shock was observed inbound during the Voyager 1 encounter, whereas five crossings of the bow shock were identified during the Voyager 2 approach to the planet. During several of these bow shock crossings, low energy protons were observed to be streaming from the direction of the dawnside of the magnetosphere. In the magnetosheath the protons were observed to be oriented primarily with pitch angles of approx.900. Prior to the inbound magnetopause crossings (as defined by the magnetometer experiment on Voyager), the low-energy protons and electrons were observed to increase in intensity. Further, during Voyager 2 encounter, an increase in the proton and electron fluxes accompanied a change in orientation of the magnetosheath magnetioc field from one with a vertical component opposite to the planetary field to one with a vertical component in the direction of the planetary field. Examination of the flux distributions of the protons suggests that the magnetopuase was moving inward with a lower limit speed of approx.10 km/s during the Voyager 2 approach to the planet. The observed average subsolar magnetopause position at the time of Voyager 2 encounter was 18.5 R/sub S/, whereas during the Voyager 1 encounter it was considerably more extended, at 23.5 R/sub S/

  11. Potts critical frontiers of inhomogeneous and asymmetric bow-tie lattices

    OpenAIRE

    Scullard, Christian R.; Jacobsen, Jesper Lykke

    2012-01-01

    We study the critical frontiers of the Potts model on two-dimensional bow-tie lattices with fully inhomogeneous coupling constants. Generally, for the Potts critical frontier to be found exactly, the underlying lattice must be a 3-uniform hypergraph. A more general class of lattices are the 4-uniform ones, with unit cells contained within four boundary vertices. We demonstrate that in some cases, such lattices can be decomposed into triangular cells, and solved using a modification of standar...

  12. Bow-tie nano-antenna assisted generation of extreme ultraviolet radiation

    OpenAIRE

    Pfullmann, N.; Waltermann, C.; Noack, M.; Rausch, S.; Nagy, T.; Reinhardt, C.; Kovacev, M.; Knittel, V.; Bratschitsch, R.; Akemeier, D.; Huetten, A.; Leitenstorfer, A.; Morgner, Uwe

    2013-01-01

    We report on the generation of extreme ultraviolet radiation utilizing the plasmonic field enhancement in arrays of bow-tie gold optical antennae. Furthermore, their suitability to support high-order harmonic generation is examined by means of finite-difference time-domain calculations and experiments. Particular emphasis is paid to the thermal properties, which become significant at the employed peak intensities. A damage threshold depending on the antenna length is predict...

  13. Self-assembled silver nanoparticles in a bow-tie antenna configuration.

    Science.gov (United States)

    Eskelinen, Antti-Pekka; Moerland, Robert J; Kostiainen, Mauri A; Törmä, Päivi

    2014-03-26

    The self-assembly of silver nanoparticles into a bow-tie antenna configuration is achieved with the DNA origami method. Instead of complicated particle geometries, spherical silver nanoparticles are used. Formation of the structures in high yields is verified with transmission electron microscopy and agarose gel electrophoresis. According to finite-difference time-domain simulations, the antenna configuration could be used as a DNA sensor. PMID:24659271

  14. Bow-tie wobble artifact: Effect of source assembly motion on cone-beam CT

    OpenAIRE

    Zheng, Dandan; John C. Ford; Lu, Jun; Lazos, Dimitrios; Hugo, Geoffrey D.; Pokhrel, Damodar; Zhang, Lisha; Williamson, Jeffrey F.

    2011-01-01

    Purpose: To investigate the cause of a bow-tie wobble artifact (BWA) discovered on Varian OBI CBCT images and to develop practical correction strategies.Method and Materials: The dependence of the BWA on phantom geometry, phantom position, specific system, and reconstruction algorithm was investigated. Simulations were conducted to study the dependence of the BWA on scatter and beam hardening corrections. Geometric calibration was performed to rule out other gantry-angle dependent mechanical ...

  15. Note: auto-relock system for a bow-tie cavity for second harmonic generation.

    Science.gov (United States)

    Haze, Shinsuke; Hata, Sousuke; Fujinaga, Munekazu; Mukaiyama, Takashi

    2013-02-01

    This Note reports on the implementation of an automatic relocking system for a bow-tie cavity for second harmonic generation to produce an ultra-violet laser source. The system is based on a sample-and-hold technique for controlling the cavity length using simple servo electronics. Long-term stabilization of the cavity output power is successfully achieved, which makes this system suitable for designing stable atomic physics experiments. PMID:23464273

  16. The critical manifolds of inhomogeneous bond percolation on bow-tie and checkerboard lattices

    OpenAIRE

    Ziff, Robert M.; Scullard, Christian R.; Wierman, John C.; Sedlock, Matthew R. A.

    2012-01-01

    We give a conditional derivation of the inhomogeneous critical percolation manifold of the bow-tie lattice with five different probabilities, a problem that does not appear at first to fall into any known solvable class. Although our argument is mathematically rigorous only on a region of the manifold, we conjecture that the formula is correct over its entire domain, and we provide a non-rigorous argument for this that employs the negative probability regime of the triangular lattice critical...

  17. Failures and Defects in the Building Process:Applying the Bow-Tie Approach

    OpenAIRE

    Jørgensen, Kirsten

    2009-01-01

    Function failures, defects, mistakes and poor communication are major problems for the construction sector. A Danish research project focusing on failures and defects in building processes has been carried out over the last 2 years. As the empirical element in the research, a large construction site was observed from the very start to the very end and all failures and defects of a certain size were recorded and analysed. The methodological approach used in this analysis was the bow-tie model ...

  18. Phenomenology of the earth's bow shock system - A summary description of experimental results

    Science.gov (United States)

    Greenstadt, E. W.

    1976-01-01

    Observational data on the earth's bow shock system are classified and characterized. Foreshock components, midshock components, and aftershock components are discussed separately. Schematic representations of the field and plasma particle parameters are elaborated, with attention given to quasi-perpendicular geometry and quasi-parallel geometry. Magnetic pulsation structure is delineated. Schematic profiles of field, particle, and wave behavior through a representative quasi-perpendicular shock crossing are displayed.

  19. Ship Bow Force-Deformation Curves for Ship-Impact Demand of Bridges considering Effect of Pile-Cap Depth

    Directory of Open Access Journals (Sweden)

    Wei Fan

    2014-01-01

    Full Text Available Since static analysis procedures in the vessel impact-resistant design codes neglect dynamic amplification effects related to bridge mass, ship-impact responses of bridges may be potentially underestimated. For this reason, several dynamic vessel-impact analysis techniques had been recently proposed, where a force-deformation curve was employed to model the vessel bow stiffness. Most of the recent works mainly focused on the force-deformation curves of the barge bows rather than the ship bows. In this paper, a high-resolution finite element model is developed to obtain the ship bow force-deformation curves. The global and local characteristics of the ship bow force-deformation curves are discussed based on the finite element crush analyses between the ship bows and the rigid walls. Effect of pile-cap depth on the force-deformation curves (rather than only impact forces is studied in detail, and the corresponding empirical equations are developed using an energy ratio method. Finally, a practical example of ship-bridge collision is investigated to validate the force-deformation curves considering the effect of pile-cap depth. It is found from the case study that the effect of pile-cap depth plays an important role in quantifying structural demand under impact loads. The case study also indicates that the developed equations are reasonable in practical applications.

  20. The procedure for determination of special margin factors to account for a bow of the WWER-1000 fuel assemblies

    International Nuclear Information System (INIS)

    Starting from 1980s, the problem of bow of the WWER-1000 reactor fuel assemblies and the effect of that on the operational safety is being discussed. At the initial period of time, the extension of time for dropping control rods of the control and protection system associated with this bow posed the highest threat. Later on, new more rigid structures were developed for fuel assemblies that eliminated the problems of control rods. However, bow of the WWER-1000 reactor fuel assemblies is observed up to now. The scale of this bow reduced significantly but it still effects safety. Even a minor bow available may lead to the noticeable increase of power of individual fuel pins associated with the local variation of the coolant amount. This effect must be taken into account on designing fuel loadings to eliminate the exceeding of set limitations. The introduction of additional special margins is the standard method for taking this effect into account. The present paper describes the conservative technique for the assessment of additional margins for bow of fuel assemblies of state-of-the-art designs. This technique is employed in the WWER-1000 reactor designing. The chosen conservatism degree is discussed as well as the method for its assurance and acceptable ways for its slackening. The example of the margin evaluation for the up-to-date fuel loading is given. (authors)

  1. The Procedure for Determination of Special Margin Factors to Account for a Bow of the VVER-1000 Fuel Assemblies

    International Nuclear Information System (INIS)

    Starting from 1980's, the problem of bow of the VVER-1000 reactor FAs and the effect of that on the operational safety is being discussed. At the initial period of time, the extension of time for dropping control rods of the control and protection system associated with this bow posed the highest threat. Later on, new more rigid structures were developed for FAs that eliminated the problems of control rods. However, bow of the VVER-1000 reactor FAs is observed up to now. The scale of this bow reduced significantly but it still effects safety. Even a minor bow available may lead to the noticeable increase of power of individual fuel pins associated with the local variation of the coolant amount. This effect must be taken into account on designing fuel loadings to eliminate the exceeding of set limitations. The introduction of additional special margins is the standard method for taking this effect into account. The present paper describes the conservative technique for the assessment of additional margins for bow of FAs of state-of-the-art designs. This technique is employed in the VVER-1000 reactor designing. The chosen conservatism degree is discussed as well as the method for its assurance and acceptable ways for its slackening. The example of the margin evaluation for the up-to-date fuel loading is given. (authors)

  2. The Procedure for Determination of Special Margin Factors to Account for a Bow of the VVER-1000 Fuel Assemblies

    Energy Technology Data Exchange (ETDEWEB)

    Tsyganov, Sergey V.; Marin, Stanislav V.; Shishkov, Lev K. [Russian Research Center ' Kurchatov Institute' , 1., Kurchatov sq., 123182 Moscow (Russian Federation)

    2008-07-01

    Starting from 1980's, the problem of bow of the VVER-1000 reactor FAs and the effect of that on the operational safety is being discussed. At the initial period of time, the extension of time for dropping control rods of the control and protection system associated with this bow posed the highest threat. Later on, new more rigid structures were developed for FAs that eliminated the problems of control rods. However, bow of the VVER-1000 reactor FAs is observed up to now. The scale of this bow reduced significantly but it still effects safety. Even a minor bow available may lead to the noticeable increase of power of individual fuel pins associated with the local variation of the coolant amount. This effect must be taken into account on designing fuel loadings to eliminate the exceeding of set limitations. The introduction of additional special margins is the standard method for taking this effect into account. The present paper describes the conservative technique for the assessment of additional margins for bow of FAs of state-of-the-art designs. This technique is employed in the VVER-1000 reactor designing. The chosen conservatism degree is discussed as well as the method for its assurance and acceptable ways for its slackening. The example of the margin evaluation for the up-to-date fuel loading is given. (authors)

  3. The procedure for determination of special margin factors to account for a bow of the VVER-1000 fuel assemblies

    International Nuclear Information System (INIS)

    Starting from 1980's, the problem of bow of the VVER-1000 reactor FAs and the effect of that on the operational safety is being discussed. At the initial period of time, the extension of time for dropping control rods of the control and protection system associated with this bow posed the highest threat. Later on, new more rigid structures were developed for FAs that eliminated the problems of control rods. However, bow of the VVER-1000 reactor FAs is observed up to now. The scale of this bow reduced significantly but it still effects safety. Even a minor bow available may lead to the noticeable increase of power of individual fuel pins associated with the local variation of the coolant amount. This effect must be taken into account on designing fuel loadings to eliminate the exceeding of set limitations. The introduction of additional special margins is the standard method for taking this effect into account. The present paper describes the conservative technique for the assessment of additional margins for bow of FAs of state-of-the-art designs. This technique is employed in the VVER-1000 reactor designing. The chosen conservatism degree is discussed as well as the method for its assurance and acceptable ways for its slackening. The example of the margin evaluation for the up-to-date fuel loading is given. (authors)

  4. The procedure for determination of special margin factors to account for a bow of the VVER-1000 fuel assemblies

    Energy Technology Data Exchange (ETDEWEB)

    Tsyganov, S.V.; Marin, S.V.; Shishkov, L.K. [Russian Research Center ' Kurchatov Institute' , Moscow (Russian Federation)

    2008-07-01

    Starting from 1980's, the problem of bow of the VVER-1000 reactor FAs and the effect of that on the operational safety is being discussed. At the initial period of time, the extension of time for dropping control rods of the control and protection system associated with this bow posed the highest threat. Later on, new more rigid structures were developed for FAs that eliminated the problems of control rods. However, bow of the VVER-1000 reactor FAs is observed up to now. The scale of this bow reduced significantly but it still effects safety. Even a minor bow available may lead to the noticeable increase of power of individual fuel pins associated with the local variation of the coolant amount. This effect must be taken into account on designing fuel loadings to eliminate the exceeding of set limitations. The introduction of additional special margins is the standard method for taking this effect into account. The present paper describes the conservative technique for the assessment of additional margins for bow of FAs of state-of-the-art designs. This technique is employed in the VVER-1000 reactor designing. The chosen conservatism degree is discussed as well as the method for its assurance and acceptable ways for its slackening. The example of the margin evaluation for the up-to-date fuel loading is given. (authors)

  5. Corporate-Feed Multilayer Bow-Tie Antenna Array Design Using a Simple Transmission Line Model

    Directory of Open Access Journals (Sweden)

    S. Didouh

    2012-01-01

    Full Text Available A transmission line model is used to design corporate-fed multilayered bow-tie antennas arrays; the simulated antennas arrays are designed to resonate at the frequencies 2.4 GHz, 5 GHz, and 8 GHz corresponding to RFID, WIFI, and radars applications. The contribution of this paper consists of modeling multilayer bow-tie antenna array fed through an aperture using transmission line model. The transmission line model is simple and precise and allows taking into account the whole geometrical, electrical, and technological characteristics of the antennas arrays. The proposed transmission line model showed its interest in the design of different multilayered bow-tie antennas and predicted the correct resonance frequency for different applications in telecommunications. To validate the proposed transmission line model, the simulation results obtained are compared with those obtained by the method of moments. The results of simulations are presented and discussed. Using this transmission line approach, the resonant frequency, input impedance, and return loss can be determined simultaneously. The paper reports several simulation results that confirm the validity of the developed model. The obtained results are then presented and discussed.

  6. Interaction of single-pulse laser energy with bow shock in hypersonic flow

    Directory of Open Access Journals (Sweden)

    Hong Yanji

    2014-04-01

    Full Text Available Pressure sensing and schlieren imaging with high resolution and sensitivity are applied to the study of the interaction of single-pulse laser energy with bow shock at Mach 5. An Nd:YAG laser operated at 1.06 μm, 100 mJ pulse energy is used to break down the hypersonic flow in a shock tunnel. Three-dimensional Navier–Stokes equations are solved with an upwind scheme to simulate the interaction. The pressure at the stagnation point on the blunt body is measured and calculated to examine the pressure variation during the interaction. Schlieren imaging is used in conjunction with the calculated density gradients to examine the process of the interaction. The results show that the experimental pressure at the stagnation point on the blunt body and schlieren imaging fit well with the simulation. The pressure at the stagnation point on the blunt body will increase when the transmission shock approaches the blunt body and decrease with the formation of the rarefied wave. Bow shock is deformed during the interaction. Quasi-stationary waves are formed by high rate laser energy deposition to control the bow shock. The pressure and temperature at the stagnation point on the blunt body and the wave drag are reduced to 50%, 75% and 81% respectively according to the simulation. Schlieren imaging has provided important information for the investigation of the mechanism of the interaction.

  7. Bow-shock instability induced by Helmholtz resonator-like feedback in slipstream

    Science.gov (United States)

    Ohnishi, Naofumi; Sato, Yosuke; Kikuchi, Yuta; Ohtani, Kiyonobu; Yasue, Kanako

    2015-06-01

    Bow-shock instability has been experimentally observed in a low-γ flow. To clarify its mechanism, a parametric study was conducted with three-dimensional numerical simulations for specific heat ratio γ and Mach number M. A critical boundary of the instability was found in the γ-M parametric space. The bow shock tends to be unstable with low γ and high M, and the experimental demonstration was designed based on this result. The experiments were conducted with the ballistic range of the single-stage powder gun mode using HFC-134a of γ = 1.12 at Mach 9.6. Because the deformation of the shock front was observed in a shadowgraph image, the numerical prediction was validated to some extent. The theoretical estimation of vortex formation in a curved shock wave indicates that the generated vorticity is proportional to the density ratio across the shock front and that the critical density ratio can be predicted as ˜10. A strong slipstream from the surface edge generates noticeable acoustic waves because it can be deviated by the upstream flow. The acoustic waves emitted by synchronizing the vortex formation can propagate upstream and may trigger bow-shock instability. This effect should be emphasized in terms of unstable shock formation around an edged flat body.

  8. A search for systemic mass loss in Algols with bow shocks

    CERN Document Server

    Mayer, Andreas; Jorissen, Alain

    2016-01-01

    Aims. Various studies indicate that interacting binary stars of Algol type evolve non-conservatively. However, direct detection of systemic mass loss in Algols has been scarce so far. We aim at studying the systemic mass loss in Algols by looking for the presence of infrared excesses originating from the thermal emission of dust grains, which is linked to the presence of a stellar wind. Methods. In contrast to previous studies, we make use of the fact that stellar and interstellar material is piled up at the edge of the asterosphere where the stellar wind interacts with the interstellar medium. We analyse WISE W3 $12\\,\\mu$m and WISE W4 $22\\,\\mu$m data of Algol-type binary Be and B[e] stars and the properties of their bow shocks. From the stand-off distance of the bow shock we are able to determine the mass loss rate of the binary system. Results. Although the velocities of the stars with respect to the interstellar medium are quite low, we find bow shocks to be present in two systems, namely $\\pi$ Aqr, and $\\...

  9. Study and comparison of the parameters of five hot flow anomalies at a bow shock front

    Science.gov (United States)

    Shestakov, A. Yu.; Vaisberg, O. L.

    2016-03-01

    Five hot flow anomalies ( HFA) recorded by the Tail Probe of the INTERBALL satellite in 1996 are analyzed in present work. For the five chosen events the authors determined the characteristics of current sheets whose interaction with the bow shock front led to formation of an HFA, as well as the directions of external electric fields and the directions of motion of these HFAs over a shock front. The analysis of plasma convection in an HFA body is carried out; the average velocities of plasma motion in the HFA are determined in a coordinate system linked with the normal to a current layer and with the normal to the bow shock. According to the character of plasma convection in an HFA body, these five events may be divided into two types, which also differ in the direction of the motion over the front of the bow shock. In the first-type HFAs, the convection of plasma has a component directed from the intermediate region confirming its identification as a source of energy for the formation of an HFA. In the second-type HFAs, plasma motion from the intermediate region in leading and trailing parts is less expressed. This fact, as well as the great variation of peculiar velocities in the body of anomalies, allowed the assumption that second-type anomalies are nonstationary. Evidence is presented that the anomalies considered in the paper are bordered with shocks formed in solar wind passing a large-scale, decelerated body of heated plasma.

  10. Congenital posteromedial bowing of the tibia and fibula: treatment option by multilevel osteotomy.

    Science.gov (United States)

    Napiontek, Marek; Shadi, Milud

    2014-03-01

    Few papers have described patients treated surgically with single osteotomy for congenital posteromedial bowing of the tibia and fibula. Only one paper has described two-level osteotomy for deformity correction: the first for deformity correction and the second for bone lengthening. There are no publications describing the surgical correction of deformation only by the method of multilevel tibial and fibular osteotomy. Research material included four children aged between 3.1 and 5.1 years (average age: 3.7 years) who were operated upon for bowing of the tibia and fibula exceeding 35° in the coronal plane. In all cases, tibial osteotomy was carried out at three or two levels accompanied by fibular osteotomy, and with intramedullary stabilization using K-wires (three patients) or Rush pin (one patient). Follow-up ranged from 3 to 7.7 years. In all cases, axis correction and bone healing were achieved. In large congenital posteromedial bowing of the tibia and fibula, a multilevel tibial and fibular osteotomy may be a better solution than an orthosis or a long time waiting for a spontaneous correction of the deformation. Large circumferential periosteal release that accompanied the surgery influenced the stimulation of bone growth. It may induce the process of lower limbs' equalization not to require the application of intensive surgical procedures. PMID:24390537

  11. Energetic protons and magnetic field fluctuations upstream of the Earth's bow shock

    International Nuclear Information System (INIS)

    The variety of temporal profiles, energy spectra and anisotropy of ions (assuming all being protons) with energies above 10 keV as measured in the dusk-afternoon sector upstream of the Earth's bow shock infers the nature of the flux formation. Several typical events were discussed. The coupled behaviour of waves and particles mutually interacting is stressed and the rough estimation of energy density of the two constituents agrees with the scenario of formation of upstream proton fluxes due to these interactions. The long-duration events exhibit a prolonged inverse velocity dispersion, a sign of regular (or first-order Fermi) acceleration. The rate of energy increase in the course of such a process is satisfactorily explained by the nonstationary regular acceleration at the shock. In several short upstream events inverse velocity dispersion was not observed. The spatial dispersion due to solar wind convection of magnetic field lines controlling the proton motion in the upstream region may significantly distort the pitch angle and energy distribution created near the bow shock if measured at larger distances near the field line tangential to the bow shock surface. Strong anisotropic events not accompanied by wave activity occur in such situations in quasiperpendicular shock geometry. There is some evidence that particle leakage from the magnetosphere contributes substantially to the observed population in one particular case, on May 2, 1985. (author). 6 figs., 18 refs

  12. Reconstructing the Guitar: Blowing Bubbles with a Pulsar Bow Shock Backflow

    Science.gov (United States)

    van Kerkwijk, Marten H.; Ingle, Ashleigh

    2008-08-01

    The Guitar Nebula is an Hα nebula produced by the interaction of the relativistic wind of a very fast pulsar, PSR B2224+65, with the interstellar medium. It consists of a ram-pressure confined bow shock near its head and a series of semicircular bubbles further behind, the two largest of which form the body of the Guitar. We present a scenario in which this peculiar morphology is due to instabilities in the backflow from the pulsar bow shock. From simulations, these backflows appear similar to jets and their kinetic energy is a large fraction of the total energy in the pulsar's relativistic wind. We suggest that, like jets, these flows become unstable some distance downstream, leading to rapid dissipation of the kinetic energy into heat, and the formation of an expanding bubble. We show that in this scenario the sizes, velocities, and surface brightnesses of the bubbles depend mostly on observables, and that they match roughly what is seen for the Guitar. Similar instabilities may account for features seen in other bow shocks.

  13. Comparative Study of Electromagnetic Waves at the Bow Shocks of Venus and Earth

    Science.gov (United States)

    Wei, Hanying; Russell, Christopher T.; Strangeway, Robert J.; Schwartz, Steven J.; Zhang, Tielong

    2016-04-01

    Although the solar interactions with Venus and Earth are quite different in many ways, they both have bow shocks formed upstream of the planet where the solar wind decelerates from a super- to sub- magnetosonic flow. In the upstream foreshock region, there is abundant wave activity generated by the shock or by the back-streaming ions and electrons from the shock. In the downstream magnetosheath region, there is also abundant wave activity either locally generated by the heated electrons or ions from the shock or transported from the shock or foreshock regions by the solar wind. The magnetometers of Venus Express and Magnetospheric Multiscale missions both occasionally record 128 Hz data during their shock crossing, which allow us the search for and analyze waves at such high frequencies. We have found short-duration wave bursts around both Venus and Earth bow shocks, with certain similarities. These waves are mostly quasi-perpendicular propagating and have amplitude and occurrence rate decreasing with distance from the bow shock. In this paper we perform statistical and comparative studies on wave properties to understand their generation mechanisms and their effects to the shock or magnetosheath plasmas.

  14. The propagation and growth of whistler mode waves generated by electron beams in earth's bow shock

    Science.gov (United States)

    Tokar, R. L.; Gurnett, D. A.

    1985-01-01

    In this study, the propagation and growth of whistler mode waves generated by electron beams within earth's bow shock is investigated using a planar model for the bow shock and a model electron distribution function. Within the shock, the model electron distribution function possesses a field-aligned T greater than T beam that is directed toward the magnetosheath. Waves with frequencies between about 1 and 100 Hz with a wide range of wave normal angles are generated by the beam via Landau and anomalous cyclotron resonances. However, because the growth rate is small and because the wave packets traverse the shock quickly, these waves do not attain large amplitudes. Waves with frequencies between about 30 and 150 Hz with a wide range of wave normal angles are generated by the beam via the normal cyclotron resonance. The ray paths for most of these waves are directed toward the solar wind although some wave packets, due to plasma convection travel transverse to the shock normal. These wave packets grow to large amplitudes because they spend a long time in the growth region. The results suggest that whistler mode noise within the shock should increase in amplitude with increasing upstream theta sub Bn. The study provides an explanation for the origin of much of the whistler mode turbulence observed at the bow shock.

  15. Origins of bandgap bowing in compound-semiconductor common-cation ternary alloys

    Energy Technology Data Exchange (ETDEWEB)

    Tit, Nacir; Obaidat, Ihab M [Department of Physics, UAE University, PO Box 17551, Al-Ain (United Arab Emirates); Alawadhi, Hussain [Department of Applied Physics, University of Sharjah, PO Box 27272, Sharjah (United Arab Emirates)], E-mail: ntit@uaeu.ac.ae

    2009-02-18

    We present an investigation into the existence and origins of bandgap bowing in compound-semiconductor common-cation ternary alloys. As examples, we consider CdSe{sub x}Te{sub 1-x} and ZnSe{sub 1-x}Te{sub x} alloys. A calculation, based on the sp{sup 3}s* tight-binding method including spin-orbit coupling within the framework of the virtual crystal approximation, is employed to determine the bandgap energy, local density of states and atomic charge states versus composition and valence-band offset. The results show that (i) in the valence band, the top states are mainly contributed by Te atoms. The degree of ionicity of all atoms is found to vary linearly with mole fraction x. (ii) There is a strong competition between the anions (Se and Te) in trapping/losing charges and this competition is the main reason for the bandgap bowing character. (iii) There is a reasonable agreement between the calculated results and the available photoluminescence data. (iv) The bowing parameter is found to increase with increasing valence-band offset and increasing lattice mismatch.

  16. Measurement of bow tie profiles in CT scanners using a real-time dosimeter

    Energy Technology Data Exchange (ETDEWEB)

    Whiting, Bruce R., E-mail: whitingbrucer@gmail.com [Department of Radiology, University of Pittsburgh, Pittsburgh, Pennsylvania 15213 (United States); Evans, Joshua D.; Williamson, Jeffrey F. [Department of Radiation Oncology, Virginia Commonwealth University, Richmond, Virginia 23298 (United States); Dohatcu, Andreea C. [University of Pittsburgh Medical Center, Pittsburgh, Pennsylvania 15213 (United States); Politte, David G. [Mallinckrodt Institute of Radiology, Washington University, St. Louis, Missouri 63110 (United States)

    2014-10-15

    Purpose: Several areas of computed tomography (CT) research require knowledge about the intensity profile of the x-ray fan beam that is introduced by a bow tie filter. This information is considered proprietary by CT manufacturers, so noninvasive measurement methods are required. One method using real-time dosimeters has been proposed in the literature. A commercially available dosimeter was used to apply that method, and analysis techniques were developed to extract fan beam profiles from measurements. Methods: A real-time ion chamber was placed near the periphery of an empty CT gantry and the dose rate versus time waveform was recorded as the x-ray source rotated about the isocenter. In contrast to previously proposed analysis methods that assumed a pointlike detector, the finite-size ion chamber received varying amounts of coverage by the collimated x-ray beam during rotation, precluding a simple relationship between the source intensity as a function of fan beam angle and measured intensity. A two-parameter model for measurement intensity was developed that included both effective collimation width and source-to-detector distance, which then was iteratively solved to minimize the error between duplicate measurements at corresponding fan beam angles, allowing determination of the fan beam profile from measured dose-rate waveforms. Measurements were performed on five different scanner systems while varying parameters such as collimation, kVp, and bow tie filters. On one system, direct measurements of the bow tie profile were collected for comparison with the real-time dosimeter technique. Results: The data analysis method for a finite-size detector was found to produce a fan beam profile estimate with a relative error between duplicate measurement intensities of <5%. It was robust over a wide range of collimation widths (e.g., 1–40 mm), producing fan beam profiles that agreed with a relative error of 1%–5%. Comparison with a direct measurement technique on

  17. Effect of an isotropic outflow from the Galactic Centre on the bow-shock evolution along the orbit

    Science.gov (United States)

    Zajaček, M.; Eckart, A.; Karas, V.; Kunneriath, D.; Shahzamanian, B.; Sabha, N.; Mužić, K.; Valencia-S., M.

    2016-01-01

    Motivated by the observations of several infrared-excess bow-shock sources and proplyd-like objects near the Galactic Centre, we analyse the effect of a potential outflow from the centre on bow-shock properties. We show that due to the non-negligible isotropic central outflow the bow-shock evolution along the orbit becomes asymmetric between the pre-peribothron and post-peribothron phases. This is demonstrated by the calculation of the bow-shock size evolution, the velocity along the shocked layer, the surface density of the bow shock, and by emission-measure maps close to the peribothron passage. Within the ambient velocity range of ≲2000 km s-1 the asymmetry is profound and the changes are considerable for different outflow velocities. As a case study we perform model calculations for the Dusty S-cluster Object (DSO/G2) as a potential young stellar object that is currently being monitored and has passed the pericentre at ˜2000 Schwarzschild radii from the supermassive black hole (Sgr A*) in 2014. We show that the velocity field of the shocked layer can contribute to the observed increasing line width of the DSO source up to the peribothron. Subsequently, supposing that the line emission originates in the bow shock, a decrease of the line width is expected. Furthermore, the decline of the bow-shock emission measure in the post-peribothron phase could help to reveal the emission of the putative star. The dominant contribution of circumstellar matter (either inflow or outflow) is consistent with the observed stable luminosity and compactness of the DSO/G2 source during its pericentre passage.

  18. Effect of bow-type initial imperfection on the buckling load and mass of graphite-epoxy blade-stiffened panels

    Science.gov (United States)

    Stroud, W. J.; Anderson, M. S.; Hennessy, K. W.

    1977-01-01

    A structural synthesis computer code which accounts for first order effects of an initial bow and which can be used for sizing stiffened composite panels having an arbitrary cross section is used to study graphite blade-stiffened panels. The effect of a small initial bow on both the load carrying ability of panels and on the mass of panels designed to carry a specified load is examined. Large reductions in the buckling load caused by a small initial bow emphasize the need for considering a bow when a panel is designed.

  19. Effect of an isotropic outflow from the Galactic centre on the bow-shock evolution along the orbit

    CERN Document Server

    Zajacek, Michal; Karas, Vladimir; Kunneriath, Devaky; Shahzamanian, Banafsheh; Sabha, Nadeen; Muzic, Koraljka; Valencia-Schneider, Monica

    2015-01-01

    Motivated by the observations of several infrared-excess bow-shock sources and proplyd-like objects near the Galactic centre, we analyse the effect of a potential outflow from the centre on bow shock properties. We show that due to the non-negligible isotropic central outflow the bow-shock evolution along the orbit becomes asymmetric between the pre-peribothron and post-peribothron phases. This is demonstrated by the calculation of the bow-shock size evolution, the velocity along the shocked layer, the surface density of the bow-shock, and by emission-measure maps close to the peribothron passage. Within the ambient velocity range of $\\lesssim 2000\\,{\\rm km\\, s^{-1}}$ the asymmetry is profound and the changes are considerable for different outflow velocities. As a case study we perform model calculations for the Dusty S-cluster Object (DSO/G2) as a potential young stellar object that is currently being monitored and has passed the pericentre at $\\sim 2000$ Schwarzschild radii from the supermassive black hole ...

  20. GYROSURFING ACCELERATION OF IONS IN FRONT OF EARTH's QUASI-PARALLEL BOW SHOCK

    Energy Technology Data Exchange (ETDEWEB)

    Kis, Arpad; Lemperger, Istvan; Wesztergom, Viktor [Research Centre for Astronomy and Earth Sciences, Geodetic and Geophysical Institute, Sopron (Hungary); Agapitov, Oleksiy; Krasnoselskikh, Vladimir [LPC2E/CNRS, F-45071 Orleans (France); Khotyaintsev, Yuri V. [Swedish Institute of Space Physics, SE- 751 21 Uppsala (Sweden); Dandouras, Iannis, E-mail: akis@ggki.hu, E-mail: Kis.Arpad@csfk.mta.hu [CESR, F-31028 Toulouse (France)

    2013-07-01

    It is well known that shocks in space plasmas can accelerate particles to high energies. However, many details of the shock acceleration mechanism are still unknown. A critical element of shock acceleration is the injection problem; i.e., the presence of the so called seed particle population that is needed for the acceleration to work efficiently. In our case study, we present for the first time observational evidence of gyroresonant surfing acceleration in front of Earth's quasi-parallel bow shock resulting in the appearance of the long-suspected seed particle population. For our analysis, we use simultaneous multi-spacecraft measurements provided by the Cluster spacecraft ion (CIS), magnetic (FGM), and electric field and wave instrument (EFW) during a time period of large inter-spacecraft separation distance. The spacecraft were moving toward the bow shock and were situated in the foreshock region. The results show that the gyroresonance surfing acceleration takes place as a consequence of interaction between circularly polarized monochromatic (or quasi-monochromatic) transversal electromagnetic plasma waves and short large amplitude magnetic structures (SLAMSs). The magnetic mirror force of the SLAMS provides the resonant conditions for the ions trapped by the waves and results in the acceleration of ions. Since wave packets with circular polarization and different kinds of magnetic structures are very commonly observed in front of Earth's quasi-parallel bow shock, the gyroresonant surfing acceleration proves to be an important particle injection mechanism. We also show that seed ions are accelerated directly from the solar wind ion population.

  1. Statistical analysis of diffuse ion events upstream of the Earth's bow shock

    Science.gov (United States)

    Trattner, K. J.; Mobius, E.; Scholer, M.; Klecker, B.; Hilchenbach, M.; Luehr, H.

    1994-01-01

    A statistical study of diffuse energetic ion events and their related waves upstream of the Earth's bow shock was performed using data from the Active Magnetospheric Particle Tracer Explorers/Ion Release Module (AMPTE/IRM) satellite over two 5-month periods in 1984 and 1985. The data set was used to test the assumption in the self-consistent model of the upstream wave and particle populations by Lee (1982) that the particle acceleration through hydromagnetic waves and the wave generation are directly coupled. The comparison between the observed wave power and the wave power predicted on the observed energetic particle energy density and solar wind parameters results in a high correlation coefficient of about 0.89. The intensity of diffuse ions falls off approximately exponentially with the distance upstream from the bow shock parallel to the magnetic field with e-folding distances which vary from approximately 3.3 R(sub E) to approximately 11.7 R(sub E) over the energy range from 10 keV/e to 67.3 keV/e for both protons and alpha particles. After normalizing the upstream particle densities to zero bow shock distance by using these exponential variations, a good correlation (0.7) of the density of the diffuse ions with the solar wind density was found. This supports the suggestion that the solar wind is the source of the diffuse ions. Furthermore, the spectral slope of the diffuse ions correlates well with the solar wind velocity component in the direction of the interplanetary magnetic field (0.68 and 0.66 for protons and alpha particles) which concurs with the notion that the solar wind plays an important role in the acceleration of the upstream particles.

  2. Study of the Combination of FTA, ETA and Bow-tie Evaluation Methods and Its Application%基于FTA、ETA、Bow-tie三种评价方法的结合及其应用研究

    Institute of Scientific and Technical Information of China (English)

    李婷婷; 赵姚峰

    2013-01-01

    在FTA与ETA分析方法结合的基础上引入蝴蝶结分析法(Bow-tie法)能很好的克服FTA和ETA的局限性。本文将ETA、FTA及Bow-tie法进行结合并将其应用到燃气管道泄漏的安全评价及分析中。%Introducing Bow-tie analytical method into the combination of FTA and ETA can well overcome the limitation of FTA and ETA. This article combines ETA, FTA and Bon-tie method and apply it into the safety evaluation and analysis of gas pipeline leakage.

  3. Free-hanging bow measurements of LWBR fuel rods (LWBR Development Program)

    International Nuclear Information System (INIS)

    Special inspection equipment was developed to ensure that the fuel rods for the Light Water Breeder Reactor met the required straightness criteria. The fuel rods were hung in a vertical position and the free-hanging shape was measured. These data were then used analytically to predict both the forces required to constrain the rods in a grid array and the resultant restrained shape. The development of a computerized system which was used for measuring the free-hanging bow of fuel rods used in the LWBR core is described in this paper

  4. Determination of main rational biomechanical characteristics in shooting from a bow

    OpenAIRE

    Adashevskiy V.M.; Iermakov S.S.; Shabashov V.A.

    2012-01-01

    The aim is to build rational parameters of technical actions of sportsman in shooting from a bow. It is worked out and decided mathematical model and the task of dynamics. Influence on having a special purpose exactness of corners of flight of arrow with an account and without the account of force of resistance of air environment is certain. It is distinguished the basic technical run-time errors of sportsman exercises. It is set that for successful realization of descriptions of target exact...

  5. Planetary Evaporation and the Dynamics of Planet Wind/Stellar Wind Bow Shocks

    CERN Document Server

    Frank, A; Carroll-Nellenback, J; Quillen, A C; Kasting, J F; Dobbs-Dixon, I; Blackman, E G

    2015-01-01

    We present initial results of a new campaign of simulations focusing on the interaction of planetary winds with stellar environments using Adaptive Mesh Refinement methods. We have confirmed the results of Stone & Proga 2009 that an azimuthal flow structure is created in the planetary wind due to day/night temperatures differences. We show that a backflow towards the planet will occur with a strength that depends on the escape parameter. When a stellar outflow is included, we see unstable bow waves forming through the outflow's interaction with the planetary wind.

  6. Numerical Study on the Effect of Buffer Bow Structure in Ship-to-ship Collisions

    DEFF Research Database (Denmark)

    Yamada, Yasuhira; Endo, Hisayoshi; Pedersen, Preben Terndrup

    structure in ship-ship collisions as compared with that of standard bulbous bows. This is demonstrated by conducting a series of large-scale finite element analyses. The finite element analyses are conducted with the general-purpose nonlinear structural code “LS-DYNA”. The applied scenario is one where a...... very large crude oil carrier (VLCC) in ballast condition collides with the midship region of a D/H VLCC in a laden condition. Fracture of fillet welds, elastic-plastic material properties and strain rate effects, are taken into account in the simulations. The effect of the equivalent failure strain (FS...

  7. A benchmark study of procedures for analysis of axial crushing of bulbous bows

    OpenAIRE

    Yamada, Yasuhira; Pedersen, Preben Terndrup

    2008-01-01

    Simplified methods to estimate mean axial crushing forces of plated structures are reviewed and applied to a series of experimental results for axial crushing of large-scale bulbous bow models. Methods based on intersection unit elements such as L-, T- and X-type elements as well as methods based on plate unit elements are employed in the analyses. The crushing forces and the total absorbed energy obtained by the simplified analyses are compared with those obtained from large-scale bulbous bo...

  8. Asymptotic Steady State Solution to a Bow Shock with an Infinite Mach Number

    CERN Document Server

    Yalinewich, Almog

    2015-01-01

    The problem of a cold gas flowing past a stationary object is considered. It is shown that at large distances from the obstacle the shock front forms a parabolic solid of revolution. The interior of the shock front is obtained by solution of the hydrodynamic equations in parabolic coordinates. The results are verified with a hydrodynamic simulation. The drag force and expected spectra are calculated for such shock, both in case of an optically thin and thick media. Finally, relations to astrophysical bow shocks and other analytic works on oblique shocks are discussed.

  9. Mapping the Structure of Directed Networks: Beyond the "Bow-tie" Diagram

    CERN Document Server

    Timár, G; Dorogovtsev, S N; Mendes, J F F

    2016-01-01

    We reveal a hierarchical organization of finite directed components---tendrils---around the giant components represented by the celebrated "bow-tie" diagram for directed networks. We develop an efficient algorithm to find tendril layers. It is used together with the message passing technique, generalized to directed graphs, to find the structure and attack tolerance of complex networks, such as the World Wide Web, the neural network of Caenorhabditis elegans, and others. We introduce a generalized susceptibility characterizing the response of directed networks to damage.

  10. Analytic MHD Theory for Earth's Bow Shock at Low Mach Numbers

    Science.gov (United States)

    Grabbe, Crockett L.; Cairns, Iver H.

    1995-01-01

    A previous MHD theory for the density jump at the Earth's bow shock, which assumed the Alfven M(A) and sonic M(s) Mach numbers are both much greater than 1, is reanalyzed and generalized. It is shown that the MHD jump equation can be analytically solved much more directly using perturbation theory, with the ordering determined by M(A) and M(s), and that the first-order perturbation solution is identical to the solution found in the earlier theory. The second-order perturbation solution is calculated, whereas the earlier approach cannot be used to obtain it. The second-order terms generally are important over most of the range of M(A) and M(s) in the solar wind when the angle theta between the normal to the bow shock and magnetic field is not close to 0 deg or 180 deg (the solutions are symmetric about 90 deg). This new perturbation solution is generally accurate under most solar wind conditions at 1 AU, with the exception of low Mach numbers when theta is close to 90 deg. In this exceptional case the new solution does not improve on the first-order solutions obtained earlier, and the predicted density ratio can vary by 10-20% from the exact numerical MHD solutions. For theta approx. = 90 deg another perturbation solution is derived that predicts the density ratio much more accurately. This second solution is typically accurate for quasi-perpendicular conditions. Taken together, these two analytical solutions are generally accurate for the Earth's bow shock, except in the rare circumstance that M(A) is less than or = 2. MHD and gasdynamic simulations have produced empirical models in which the shock's standoff distance a(s) is linearly related to the density jump ratio X at the subsolar point. Using an empirical relationship between a(s) and X obtained from MHD simulations, a(s) values predicted using the MHD solutions for X are compared with the predictions of phenomenological models commonly used for modeling observational data, and with the predictions of a

  11. Bowing effect in elastic constants of dilute Ga(As,N) alloys

    Science.gov (United States)

    Berggren, Jonas; Hanke, Michael; Trampert, Achim

    2016-05-01

    We study the elastic properties of dilute Ga(As,N) thin films grown on GaAs(001) by means of nano-indentation and complementary dynamic finite element calculations. The experimental results of indentation modulus are compared with simulations in order to extract the cubic elastic constants cij as a function of nitrogen content of the Ga(As,N) alloys. Both, indentation modulus and elastic constants decrease with increasing nitrogen content, which proves a strong negative bowing effect in this system in contrast to Vegard's law.

  12. Numerical Study on the Effect of Buffer Bow Structure in Ship-to-ship Collisions

    DEFF Research Database (Denmark)

    Yamada, Yasuhira; Endo, Hisayoshi; Pedersen, Preben Terndrup

    2005-01-01

    structure in ship-ship collisions as compared with that of standard bulbous bows. This is demonstrated by conducting a series of large-scale finite element analyses. The finite element analyses are conducted with the general-purpose nonlinear structural code “LS-DYNA”. The applied scenario is one where...... a very large crude oil carrier (VLCC) in ballast condition collides with the midship region of a D/H VLCC in a laden condition. Fracture of fillet welds, elastic-plastic material properties and strain rate effects, are taken into account in the simulations. The effect of the equivalent failure strain (FS...

  13. Broadband millimeter-wave GaAs transmitters and receivers using planar bow-tie antennas

    Science.gov (United States)

    Konishi, Y.; Kamegawa, M.; Case, M.; Yu, R.; Rodwell, M. J. W.; York, R. A.; Rutledge, D. B.

    1992-01-01

    We report broadband monolithic transmitters and receivers IC's for mm-wave electromagnetic measurements. The IC's use nonlinear transmission lines (NLTL) and sampling circuits as picosecond pulse generators and detectors. The pulses are radiated and received by planar monolithic bow-tie antennas, collimated with silicon substrate lenses and off-axis parabolic reflectors. Through Fourier transformation of the received pulse, 30-250 GHz free space gain-frequency measurements are demonstrated with an accuracy approximately = 0.17 dB, RMS.

  14. Bi-Band Bow-Tie Antennas Array Design Using a Simple Equivalent Transmission Line Model

    Directory of Open Access Journals (Sweden)

    M. Abri

    2012-08-01

    Full Text Available In this paper we propose a simple equivalent and accurate transmission line model for bi-band bow-tie antennas array design over a band of frequencies for satellite communications. This model uses the resistance of a square element that appears at the edges of the antenna (radiating slots. To test this model, two antennas array were simulated and results were compared with those obtained by a rigorous method (moment’s method of the simulator ADS/Momentum. Using this transmission line approach the resonant frequency, return loss, VSWR, reflected phase, input impedance can be determined simultaneously. The results confirm the validity of the proposed model.

  15. Near-field enhanced ultraviolet resonance Raman spectroscopy using aluminum bow-tie nano-antenna.

    Science.gov (United States)

    Li, Ling; Fang Lim, Shuang; Puretzky, Alexander A; Riehn, Robert; Hallen, H D

    2012-09-10

    An aluminum bow-tie nano-antenna is combined with the resonance Raman effect in the deep ultraviolet to dramatically increase the sensitivity of Raman spectra to a small volume of material, such as benzene used here. We further demonstrate gradient-field Raman peaks for several strong infrared modes. We achieve a gain of [Formula: see text] in signal intensity from the near field enhancement due to the surface plasmon resonance in the aluminum nanostructure. The on-line resonance enhancement contributes another factor of several thousands, limited by the laser line width. Thus, an overall gain of hundreds of million is achieved. PMID:23066168

  16. Bi-Band Bow-Tie Antennas Array Design Using a Simple Equivalent Transmission Line Model

    OpenAIRE

    Abri, M.; H. Abri Badaoui; Dib, H; A.S.E. Gharnaout

    2012-01-01

    In this paper we propose a simple equivalent and accurate transmission line model for bi-band bow-tie antennas array design over a band of frequencies for satellite communications. This model uses the resistance of a square element that appears at the edges of the antenna (radiating slots). To test this model, two antennas array were simulated and results were compared with those obtained by a rigorous method (moment’s method) of the simulator ADS/Momentum. Using this transmission line appro...

  17. Near-field enhanced ultraviolet resonance Raman spectroscopy using aluminum bow-tie nano-antenna

    OpenAIRE

    Li, Ling; Fang Lim, Shuang; Puretzky, Alexander A.; Riehn, Robert; Hallen, H. D.

    2012-01-01

    An aluminum bow-tie nano-antenna is combined with the resonance Raman effect in the deep ultraviolet to dramatically increase the sensitivity of Raman spectra to a small volume of material, such as benzene used here. We further demonstrate gradient-field Raman peaks for several strong infrared modes. We achieve a gain of ∼105 in signal intensity from the near field enhancement due to the surface plasmon resonance in the aluminum nanostructure. The on-line resonance enhancement contributes ano...

  18. Liquid Crystal Bow-Tie Microstrip antenna for Wireless Communication Applications

    Directory of Open Access Journals (Sweden)

    B.T.P.Madhav

    2014-06-01

    Full Text Available In this paper we presented the design and analysis of Bow-Tie antenna on liquid crystal substrate, which is suitable for the Bluetooth/WLAN-2.4/WiBree/ZigBee applications. The Omni-directional radiation patterns along with moderate gain make the proposed antenna suitable for above mentioned applications. Details of the antenna design and simulated results Return loss, Input impedance, Radiation Patterns, E-Field, H-Field and Current Distributions, VSWR are presented and discussed. The proposed antenna is simulated at 2.4 GHz using Ansoft HFSS-11.

  19. Liquid Crystal Bow-Tie Microstrip antenna for Wireless Communication Applications

    OpenAIRE

    B.T.P.Madhav; VGKM Pisipati; Habibulla Khan; V.G.N.S Prasad; K. Praveen Kumar; KVL Bhavani; M. Ravi Kumar

    2014-01-01

    In this paper we presented the design and analysis of Bow-Tie antenna on liquid crystal substrate, which is suitable for the Bluetooth/WLAN-2.4/WiBree/ZigBee applications. The Omni-directional radiation patterns along with moderate gain make the proposed antenna suitable for above mentioned applications. Details of the antenna design and simulated results Return loss, Input impedance, Radiation Patterns, E-Field, H-Field and Current Distributions, VSWR are presented and discussed. The propose...

  20. Bow-tie optical antenna probes for single-emitter scanning near-field optical microscopy

    OpenAIRE

    Farahani, Javad N.; Eisler, Hans-Jürgen; Pohl, Dieter W; Pavius, Michaël; Flückiger, Philippe; Gasser, Philippe; Hecht, Bert

    2007-01-01

    A method for the fabrication of bow-tie optical antennas at the apex of pyramidal Si3N4 atomic force microscopy tips is described. We demonstrate that these novel optical probes are capable of sub-wavelength imaging of single quantum dots at room temperature. The enhanced and confined optical near-field at the antenna feed gap leads to locally enhanced photoluminescence (PL) of single quantum dots. Photoluminescence quenching due to the proximity of metal is found to be insignificant. The met...

  1. Millimeter-wave near-field imaging with bow-tie antennas.

    Science.gov (United States)

    Omarouayache, Rachid; Payet, Pierre; Raoult, Jérémy; Chusseau, Laurent

    2015-05-01

    A near-field reflectometry experiment operating at 60 GHz is built in view of material and circuit inspection. Experiments are always obtained in constant height mode of operation. The bow-tie near-field probe acts mostly as a linearly-polarized electric dipole and allows strongly subwavelength resolution of ≈ λ/130. Its interaction with sample is shown polarization dependent and sensitive to both the local topography and the local dielectric constant or metal conductivity. Resonant and non-resonant probes are both evaluated. PMID:25969302

  2. Printed Modified Bow-Tie Dipole Antenna for DVB/WLAN Applications

    Directory of Open Access Journals (Sweden)

    Ching-Chih Hung

    2013-01-01

    Full Text Available A printed modified bow-tie dipole antenna which consists of asymmetric-feed and inserted slots is presented to apply to the DVB and WLAN systems. This antenna combines omnidirectional radiation pattern, broad bandwidth, and band rejection in an easy way to fabricate. Experimental results of the constructed prototype indicate that the VSWR 2.5 : 1 bandwidths achieve 166.7%, 28.57%, and 23.63% at 660 MHz, 2450 MHz, and 5500 MHz, respectively.

  3. Printed Modified Bow-Tie Dipole Antenna for DVB/WLAN Applications

    OpenAIRE

    Ching-Chih Hung; Chia-Mei Peng; I-Fong Chen

    2013-01-01

    A printed modified bow-tie dipole antenna which consists of asymmetric-feed and inserted slots is presented to apply to the DVB and WLAN systems. This antenna combines omnidirectional radiation pattern, broad bandwidth, and band rejection in an easy way to fabricate. Experimental results of the constructed prototype indicate that the VSWR 2.5 : 1 bandwidths achieve 166.7%, 28.57%, and 23.63% at 660 MHz, 2450 MHz, and 5500 MHz, respectively.

  4. Beam-Steerable Microstrip-Fed Bow-Tie Antenna Array for Fifth Generation Cellular Communications

    OpenAIRE

    Ojaroudiparchin, Naser; Shen, Ming; Gert F. Pedersen

    2016-01-01

    The design and performance of mm-wave phased array antenna for 5G mobile broadband communication systems has been provided in this manuscript. The antenna is designed on a N9000 PTFE substrate with 0.787 mm thickness and 2.2 dielectric constant and 65×130 mm2 overall dimension. Eight elements of bow-tie antennas have been used at the top-edge region of mobile phone PCB. The antenna elements fed by microstrip lines are designed to operate at 17 GHz. The simulated results give good performances...

  5. Short term memory bowing effect is consistent with presentation rate dependent decay

    OpenAIRE

    Tarnow, Eugen

    2010-01-01

    I reanalyze the free recall data of Murdock, J Exp Psychol 64(5):482–488 (1962) and Murdock and Okada, J Verbal Learn and Verbal Behav 86:263–267 (1970) which show the famous bowing effect in which initial and recent items are recalled better than intermediate items (primacy and recency effects). Recent item recall probabilities follow a logarithmic decay with time of recall consistent with the tagging/retagging theory. The slope of the decay increases with increasing presentation rate. The i...

  6. A new technique to characterize CT scanner bow-tie filter attenuation and applications in human cadaver dosimetry simulations

    International Nuclear Information System (INIS)

    Purpose: To present a noninvasive technique for directly measuring the CT bow-tie filter attenuation with a linear array x-ray detector. Methods: A scintillator based x-ray detector of 384 pixels, 307 mm active length, and fast data acquisition (model X-Scan 0.8c4-307, Detection Technology, FI-91100 Ii, Finland) was used to simultaneously detect radiation levels across a scan field-of-view. The sampling time was as short as 0.24 ms. To measure the body bow-tie attenuation on a GE Lightspeed Pro 16 CT scanner, the x-ray tube was parked at the 12 o’clock position, and the detector was centered in the scan field at the isocenter height. Two radiation exposures were made with and without the bow-tie in the beam path. Each readout signal was corrected for the detector background offset and signal-level related nonlinear gain, and the ratio of the two exposures gave the bow-tie attenuation. The results were used in the GEANT4 based simulations of the point doses measured using six thimble chambers placed in a human cadaver with abdomen/pelvis CT scans at 100 or 120 kV, helical pitch at 1.375, constant or variable tube current, and distinct x-ray tube starting angles. Results: Absolute attenuation was measured with the body bow-tie scanned at 80–140 kV. For 24 doses measured in six organs of the cadaver, the median or maximum difference between the simulation results and the measurements on the CT scanner was 8.9% or 25.9%, respectively. Conclusions: The described method allows fast and accurate bow-tie filter characterization

  7. A new technique to characterize CT scanner bow-tie filter attenuation and applications in human cadaver dosimetry simulations

    Energy Technology Data Exchange (ETDEWEB)

    Li, Xinhua; Shi, Jim Q.; Zhang, Da; Singh, Sarabjeet; Padole, Atul; Otrakji, Alexi; Kalra, Mannudeep K.; Liu, Bob, E-mail: bliu7@mgh.harvard.edu [Department of Radiology, Massachusetts General Hospital, Boston, Massachusetts 02114 (United States); Xu, X. George [Nuclear Engineering Program, Rensselaer Polytechnic Institute, Troy, New York 12180 (United States)

    2015-11-15

    Purpose: To present a noninvasive technique for directly measuring the CT bow-tie filter attenuation with a linear array x-ray detector. Methods: A scintillator based x-ray detector of 384 pixels, 307 mm active length, and fast data acquisition (model X-Scan 0.8c4-307, Detection Technology, FI-91100 Ii, Finland) was used to simultaneously detect radiation levels across a scan field-of-view. The sampling time was as short as 0.24 ms. To measure the body bow-tie attenuation on a GE Lightspeed Pro 16 CT scanner, the x-ray tube was parked at the 12 o’clock position, and the detector was centered in the scan field at the isocenter height. Two radiation exposures were made with and without the bow-tie in the beam path. Each readout signal was corrected for the detector background offset and signal-level related nonlinear gain, and the ratio of the two exposures gave the bow-tie attenuation. The results were used in the GEANT4 based simulations of the point doses measured using six thimble chambers placed in a human cadaver with abdomen/pelvis CT scans at 100 or 120 kV, helical pitch at 1.375, constant or variable tube current, and distinct x-ray tube starting angles. Results: Absolute attenuation was measured with the body bow-tie scanned at 80–140 kV. For 24 doses measured in six organs of the cadaver, the median or maximum difference between the simulation results and the measurements on the CT scanner was 8.9% or 25.9%, respectively. Conclusions: The described method allows fast and accurate bow-tie filter characterization.

  8. The spin-1/2 Ising model on the bow-tie lattice as an exactly soluble free-fermion model

    OpenAIRE

    Strecka, Jozef; Canova, Lucia

    2007-01-01

    The spin-1/2 Ising model on the bow-tie lattice is exactly solved by establishing a precise mapping relationship with its corresponding free-fermion eight-vertex model. Ground-state and finite-temperature phase diagrams are obtained for the anisotropic bow-tie lattice with three different exchange interactions along three different spatial directions.

  9. Hydroelastic Response of Surface-Effect Ship Bow Seals: Large-Scale Experiments and Post-Buckling Analysis

    Science.gov (United States)

    Wiggins, Andrew D.

    Bow seals are critical components on advanced marine vehicles that rely on aerostatic support to reduce drag. They consist of a series of open-ended fabric cylinders ("fingers") that contact the free surface and, when inflated, form a compliant pressure barrier. Bow seals are unique in that, unlike a majority of structures in civil and mechanical engineering, bow seals operate in a buckled state. The response characteristics of these structures are of practical interest due to unacceptable wear rates on seal components and difficulties in predicting seal performance. Despite this, the hydroelastic response of the seal system, particularly basic information on seal vibration modes and the mechanisms responsible for seal wear, remains largely unknown. Similarly, estimates of the hydrodynamic loads on the seal system are inaccurate and based on heuristic scaling of data from small-scale experiments, where similitude is challenging to maintain. Thus, a large-scale test system is necessary to obtain accurate estimates of bow seal response. The work is comprised of three parts. Part one presents detailed observations of bow seal response acquired using a large-scale test platform developed as part of the present study. These high-resolution observations, the first of their kind, show bow seal response to be characterized by complex post-buckling behavior. Part two proposes an analytical framework for interpreting the wide range of behavior observed at large scale. Using this framework, key parameters driving seal conformation and stability are identified. It is found that, due to their buckled state, bow seals are highly susceptible to a mode switching instability, which may be a potential mechanism responsible for the damaging vibrations. In part three, a benchtop experiment is used to demonstrate that the scalings identified in this study hold across a wide range of bending rigidities. This work has implications for improving drag and wear characteristics in future bow

  10. Offset semi-parabolic nanoantenna made of a photonic crystal parabolic mirror and a plasmonic bow-tie antenna.

    Science.gov (United States)

    Hattori, Haroldo T

    2014-10-10

    In a parabolic mirror, light coming parallel to the antenna passes through its focal point. In this work, a waveguide feeds a semi-parabolic photonic crystal mirror and the emerging beam feeds a bow-tie antenna placed at the mirror's focal point-it is shown that the antenna system can not only feed a bow-tie antenna (producing a localized moderately high electric field) but also produces a directional radiation beam. The semi-parabolic mirror is also modified to reduce reflection back to the feeding waveguide. PMID:25322381

  11. Pattern Switchable Antenna System Using Inkjet-Printed Directional Bow-Tie for Bi-Direction Sensing Applications

    OpenAIRE

    Seung-Hyun Eom; Yunsik Seo; Sungjoon Lim

    2015-01-01

    In this paper, we propose a paper-based pattern switchable antenna system using inkjet-printing technology for bi-direction sensor applications. The proposed antenna system is composed of two directional bow-tie antennas and a switching network. The switching network consists of a single-pole-double-throw (SPDT) switch and a balun element. A double-sided parallel-strip line (DSPSL) is employed to convert the unbalanced microstrip mode to the balanced strip mode. Two directional bow-tie antenn...

  12. Experimental validation of a method characterizing bow tie filters in CT scanners using a real-time dose probe

    OpenAIRE

    McKenney, Sarah E.; Nosratieh, Anita; Gelskey, Dale; Yang, Kai; Huang, Shin-ying; Chen, Lin; Boone, John M.

    2011-01-01

    Purpose: Beam-shaping or “bow tie” (BT) filters are used to spatially modulate the x-ray beam in a CT scanner, but the conventional method of step-and-shoot measurement to characterize a beam’s profile is tedious and time-consuming. The theory for characterization of bow tie relative attenuation (COBRA) method, which relies on a real-time dosimeter to address the issues of conventional measurement techniques, was previously demonstrated using computer simulations. In this study, the feasibili...

  13. Diversity of sponges (Porifera) from cryptic habitats on the Belize barrier reef near Carrie Bow Cay.

    Science.gov (United States)

    Rützler, Klaus; Piantoni, Carla; Van Soest, Rob W M; Díaz, M Cristina

    2014-01-01

    The Caribbean barrier reef near Carrie Bow Cay, Belize, has been a focus of Smithsonian Institution (Washington) reef and mangrove investigations since the early 1970s. Systematics and biology of sponges (Porifera) were addressed by several researchers but none of the studies dealt with cryptic habitats, such as the shaded undersides of coral rubble, reef crevices, and caves, although a high species diversity was recognized and samples were taken for future reference and study. This paper is the result of processing samples taken between 1972 and 2012. In all, 122 species were identified, 14 of them new (including one new genus). The new species are Tetralophophora (new genus) mesoamericana, Geodia cribrata, Placospongia caribica, Prosuberites carriebowensis, Timea diplasterina, Timea oxyasterina, Rhaphidhistia belizensis, Wigginsia curlewensis, Phorbas aurantiacus, Myrmekioderma laminatum, Niphates arenata, Siphonodictyon occultum, Xestospongia purpurea, and Aplysina sciophila. We determined that about 75 of the 122 cryptic sponge species studied (61%) are exclusive members of the sciophilic community, 47 (39 %) occur in both, light-exposed and shaded or dark habitats. Since we estimate the previously known sponge population of Carrie Bow reefs and mangroves at about 200 species, the cryptic fauna makes up 38 % of total diversity. PMID:24871152

  14. O+ ion beams reflected below the Martian bow shock: MAVEN observations

    Science.gov (United States)

    Masunaga, K.; Seki, K.; Brain, D. A.; Fang, X.; Dong, Y.; Jakosky, B. M.; McFadden, J. P.; Halekas, J. S.; Connerney, J. E. P.

    2016-04-01

    We investigate a generation mechanism of O+ ion beams observed above the Martian bow shock by analyzing ion velocity distribution functions (VDFs) measured by the Suprathermal and Thermal Ion Composition instrument on the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft. In the solar wind near Mars, MAVEN often observes energetic O+ ion beams (~10 keV or higher). Accompanied with the O+ ion beam events, we sometimes observe characteristic ion VDFs in the magnetosheath: a partial ring distribution. The partial ring distribution corresponds to pickup ions with a finite initial velocity (i.e., not newborn pickup ions), and its phase space density is much smaller than that of local pickup O+ ions of the magnetosheath. Thus, the partial ring distribution is most likely produced by the reflection of pickup O+ ions precipitating from the upstream solar wind below the bow shock. After being injected into the magnetosheath from the solar wind, the precipitating O+ ions are subject to the significantly enhanced magnetic field in this region and start to gyrate around the guiding center of the plasma frame in the magnetosheath. Consequently, a part of precipitating O+ ions are reflected back to the solar wind, generating O+ beams in the solar wind. The beams direct quasi-sunward near the subsolar region but have large angle with respect to the sunward direction at high solar zenith angles (>50°). The reflected O+ beams are accelerated by the convection electric field of the solar wind and may escape Mars.

  15. Reconstructing the Guitar: Blowing Bubbles with a Pulsar Bow Shock Back Flow

    CERN Document Server

    van Kerkwijk, Marten H

    2008-01-01

    The Guitar Nebula is an H-alpha nebula produced by the interaction of the relativistic wind of a very fast pulsar, PSR B2224+65, with the interstellar medium. It consists of a ram-pressure confined bow shock near its head and a series of semi-circular bubbles further behind, the two largest of which form the body of the Guitar. We present a scenario in which this peculiar morphology is due to instabilities in the back flow from the pulsar bow shock. From simulations, these back flows appear similar to jets and their kinetic energy is a large fraction of the total energy in the pulsar's relativistic wind. We suggest that, like jets, these flows become unstable some distance down-stream, leading to rapid dissipation of the kinetic energy into heat, and the formation of an expanding bubble. We show that in this scenario the sizes, velocities, and surface brightnesses of the bubbles depend mostly on observables, and that they match roughly what is seen for the Guitar. Similar instabilities may account for feature...

  16. Compound semiconductor alloys: From atomic-scale structure to bandgap bowing

    International Nuclear Information System (INIS)

    Compound semiconductor alloys such as InxGa1−xAs, GaAsxP1−x, or CuInxGa1−xSe2 are increasingly employed in numerous electronic, optoelectronic, and photonic devices due to the possibility of tuning their properties over a wide parameter range simply by adjusting the alloy composition. Interestingly, the material properties are also determined by the atomic-scale structure of the alloys on the subnanometer scale. These local atomic arrangements exhibit a striking deviation from the average crystallographic structure featuring different element-specific bond lengths, pronounced bond angle relaxation and severe atomic displacements. The latter, in particular, have a strong influence on the bandgap energy and give rise to a significant contribution to the experimentally observed bandgap bowing. This article therefore reviews experimental and theoretical studies of the atomic-scale structure of III-V and II-VI zincblende alloys and I-III-VI2 chalcopyrite alloys and explains the characteristic findings in terms of bond length and bond angle relaxation. Different approaches to describe and predict the bandgap bowing are presented and the correlation with local structural parameters is discussed in detail. The article further highlights both similarities and differences between the cubic zincblende alloys and the more complex chalcopyrite alloys and demonstrates that similar effects can also be expected for other tetrahedrally coordinated semiconductors of the adamantine structural family

  17. Technical Note: Measurement of bow tie profiles in CT scanners using radiochromic film

    Energy Technology Data Exchange (ETDEWEB)

    Whiting, Bruce R., E-mail: whitingbrucer@gmail.com [Department of Radiology, University of Pittsburgh, Pittsburgh, Pennsylvania 15213 (United States); Dohatcu, Andreea C. [University of Pittsburgh Medical Center, Pittsburgh, Pennsylvania 15213 (United States); Evans, Joshua D.; Williamson, Jeffrey F. [Department of Radiation Oncology, Virginia Commonwealth University, Richmond, Virginia 23298 (United States); Politte, David G. [Mallinckrodt Institute of Radiology, Washington University, St. Louis, Missouri 63110 (United States)

    2015-06-15

    Purpose: To provide a noninvasive technique to measure the intensity profile of the fan beam in a computed tomography (CT) scanner that is cost effective and easily implemented without the need to access proprietary scanner information or service modes. Methods: The fabrication of an inexpensive aperture is described, which is used to expose radiochromic film in a rotating CT gantry. A series of exposures is made, each of which is digitized on a personal computer document scanner, and the resulting data set is analyzed to produce a self-consistent calibration of relative radiation exposure. The bow tie profiles were analyzed to determine the precision of the process and were compared to two other measurement techniques, direct measurements from CT gantry detectors and a dynamic dosimeter. Results: The radiochromic film method presented here can measure radiation exposures with a precision of ∼6% root-mean-square relative error. The intensity profiles have a maximum 25% root-mean-square relative error compared with existing techniques. Conclusions: The proposed radiochromic film method for measuring bow tie profiles is an inexpensive (∼$100 USD + film costs), noninvasive method to measure the fan beam intensity profile in CT scanners.

  18. Investigation of radiative bow-shocks in magnetically accelerated plasma flows

    Energy Technology Data Exchange (ETDEWEB)

    Bott-Suzuki, S. C., E-mail: sbottsuzuki@ucsd.edu; Caballero Bendixsen, L. S.; Cordaro, S. W. [University of California San Diego, La Jolla, California 92093 (United States); Blesener, I. C.; Hoyt, C. L.; Cahill, A. D.; Kusse, B. R.; Hammer, D. A.; Gourdain, P. A.; Seyler, C. E.; Greenly, J. B. [Cornell University, Ithaca, New York 14850 (United States); Chittenden, J. P.; Niasse, N.; Lebedev, S. V. [Imperial College London, South Kensington, London SW7 2BW (United Kingdom); Ampleford, D. J. [Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States)

    2015-05-15

    We present a study of the formation of bow shocks in radiatively cooled plasma flows. This work uses an inverse wire array to provide a quasi-uniform, large scale hydrodynamic flow accelerated by Lorentz forces to supersonic velocities. This flow impacts a stationary object placed in its path, forming a well-defined Mach cone. Interferogram data are used to determine a Mach number of ∼6, which may increase with radial position suggesting a strongly cooling flow. Self-emission imaging shows the formation of a thin (<60 μm) strongly emitting shock region, where T{sub e} ∼ 40–50 eV, and rapid cooling behind the shock. Emission is observed upstream of the shock position which appears consistent with a radiation driven phenomenon. Data are compared to 2-dimensional simulations using the Gorgon MHD code, which show good agreement with the experiments. The simulations are also used to investigate the effect of magnetic field in the target, demonstrating that the bow-shocks have a high plasma β, and the influence of B-field at the shock is small. This consistent with experimental measurement with micro bdot probes.

  19. Optical hydrogen absorption consistent with a thin bow shock leading the hot Jupiter HD 189733b

    CERN Document Server

    Cauley, P Wilson; Jensen, Adam G; Barman, Travis; Endl, Michael; Cochran, William D

    2015-01-01

    Bow shocks are ubiquitous astrophysical phenomena resulting from the supersonic passage of an object through a gas. Recently, pre-transit absorption in UV metal transitions of the hot Jupiter exoplanets HD 189733b and WASP12-b have been interpreted as being caused by material compressed in a planetary bow shock. Here we present a robust detection of a time-resolved pre-transit, as well as in-transit, absorption signature around the hot Jupiter exoplanet HD 189733b using high spectral resolution observations of several hydrogen Balmer lines. The line shape of the pre-transit feature and the shape of the time series absorption provide the strongest constraints on the morphology and physical characteristics of extended structures around an exoplanet. The in-transit measurements confirm the previous exospheric H-alpha detection although the absorption depth measured here is ~50% lower. The pre-transit absorption feature occurs 125 minutes before the predicted optical transit, a projected linear distance from the ...

  20. Ground-state magnetic phase diagram of bow-tie graphene nanoflakes in external magnetic field

    Energy Technology Data Exchange (ETDEWEB)

    Szałowski, Karol, E-mail: kszalowski@uni.lodz.pl, E-mail: kszalowski@wp.pl [Department of Solid State Physics, Faculty of Physics and Applied Informatics, University of Łódź, ul. Pomorska 149/153, 90-236 Łódź (Poland)

    2013-12-28

    The magnetic phase diagram of a ground state is studied theoretically for graphene nanoflakes of bow-tie shape and various sizes in external in-plane magnetic field. The tight-binding Hamiltonian supplemented with Hubbard term is used to model the electronic structure of the systems in question. The existence of the antiferromagnetic phase with magnetic moments localized at the sides of the bow-tie is found for low field and a field-induced spin-flip transition to ferromagnetic state is predicted to occur in charge-undoped structures. For small nanoflake doped with a single charge carrier, the low-field phase is ferrimagnetic and a metamagnetic transition to ferromagnetic ordering can be forced by the field. The critical field is found to decrease with increasing size of the nanoflake. The influence of diagonal and off-diagonal disorder on the mentioned magnetic properties is studied. The effect of off-diagonal disorder is found to be more important than that of diagonal disorder, leading to significantly widened distribution of critical fields for disordered population of nanoflakes.

  1. The properties of bow-shock sources at the Galactic Center

    CERN Document Server

    Sanchez-Bermudez, J; Alberdi, A; Muzic, K; Hummel, C A; Pott, J -U

    2014-01-01

    There are an enigmatic population of massive stars around the Galactic Center (GC) that were formed some Ma ago. A fraction of these stars has been found to orbit the supermassive black hole, SgrA*, in a projected clockwise disk, which suggests that they were formed in a formerly existing dense disk around SgrA*. We focus on the extended, near-infrared (NIR) sources IRS1W, IRS5, IRS10W, and IRS21 that have been suggested to be young, massive stars that form bow-shocks through their interaction with the ISM. Their nature has impeded accurate determination of their orbital parameters. We aim at establishing their nature and kinematics to test whether they form part of the clockwise disk. We performed NIR multi-wavelength imaging using adaptive optics (AO) and sparse aperture masking (SAM). We introduce a new method for self-calibration of the SAM PSF in dense stellar fields. The emission mechanism, morphology and kinematics of the targets were examined via 3D bow-shock models. We confirm previous findings that ...

  2. Technical Note: Measurement of bow tie profiles in CT scanners using radiochromic film

    International Nuclear Information System (INIS)

    Purpose: To provide a noninvasive technique to measure the intensity profile of the fan beam in a computed tomography (CT) scanner that is cost effective and easily implemented without the need to access proprietary scanner information or service modes. Methods: The fabrication of an inexpensive aperture is described, which is used to expose radiochromic film in a rotating CT gantry. A series of exposures is made, each of which is digitized on a personal computer document scanner, and the resulting data set is analyzed to produce a self-consistent calibration of relative radiation exposure. The bow tie profiles were analyzed to determine the precision of the process and were compared to two other measurement techniques, direct measurements from CT gantry detectors and a dynamic dosimeter. Results: The radiochromic film method presented here can measure radiation exposures with a precision of ∼6% root-mean-square relative error. The intensity profiles have a maximum 25% root-mean-square relative error compared with existing techniques. Conclusions: The proposed radiochromic film method for measuring bow tie profiles is an inexpensive (∼$100 USD + film costs), noninvasive method to measure the fan beam intensity profile in CT scanners

  3. Absence of the bowing character in the common-anion II-VI ternary alloys

    Energy Technology Data Exchange (ETDEWEB)

    Tit, Nacir [Department of Physics, UAE University, P.O. Box 17551, Al-Ain (United Arab Emirates)], E-mail: ntit@uaeu.ac.ae; Obaidat, Ihab M. [Department of Physics, UAE University, P.O. Box 17551, Al-Ain (United Arab Emirates); Alawadhi, Hussain [Department of Applied Physics, University of Sharjah, P.O. Box 27272, Sharjah (United Arab Emirates)

    2009-07-29

    The absence of bandgap bowing in the common-anion II-VI semiconductor ternary alloys is investigated. As examples, we consider the Cd{sub 1-x}Zn{sub x}Te and Cd{sub 1-x}Zn{sub x}Se alloys. The sp{sup 3}s* tight-binding method with the inclusion of spin-orbit interactions is employed to calculate the alloy's band structure and its corresponding constituents' charge states (ionicities) as a function of composition. The variation is found to be nearly linear. The vanishingly small valence-band offset (VBO{approx_equal}0) in common-anion compounds would yield a linear scaling of bandgap energy with composition, especially as the conduction-band edge state being a singlet state with spherical symmetry. Furthermore, the two cation atoms (Cd and Zn) are found not to compete in changing their charge states as the composition is varied. The absence of such competition is believed to be the main reason for the absence of bowing. The theoretical results are compared to the available experimental data and found to be in good agreement.

  4. Methods for core safety assessment of VVER-1000 reactors with bowed fuel assemblies

    International Nuclear Information System (INIS)

    An increased drop time of control rods exceeding the design limit of four seconds has been observed in most of the operating VVER-1000 reactors in Russia and Ukraine. At the end of second fuel cycle of Kozloduy NPP unit 6 seven control rods had the drop time higher than the design limit of four seconds. The main designer of VVER-1000 had stressed that the reason of increased drop time is the fuel assemblies (FA) bow. The previous solution of the problem contents the measurements of guide tubes' deviations, core geometry determination, calculation of new peaking factors for fuel rods located on FA periphery and set of new limitation for FA volume peaking factors. Thus the reactor power was limited to prevent the core from extending heat-up. The increased coolant flow in FA gap and change of thermal-hydraulic parameters were not taken into account. The analysis of FA bowing and its consequences as well as the preliminary thermal-hydraulic research of INRNE pointed out that the safety assessment of reactor core has to consider the mechanical, neutron-physics and thermal-hydraulic aspects of the phenomenon. The methods for the measurement of guide tubes deviations, FA and core geometry determination and prediction of their evolution during the fuel cycle, the calculation and estimation of neutron-physics and thermal-hydraulic parameters were proposed. The main features of the methods and their application for the previous fourth fuel cycle of Kozloduy NPP unit 6 are presented. (author)

  5. Woods with physical, mechanical and acoustic properties similar to those of Caesalpinia echinata have high potential as alternative woods for bow makers

    Directory of Open Access Journals (Sweden)

    Eduardo Luiz Longui

    2014-09-01

    Full Text Available For nearly two hundred years, Caesalpinia echinata wood has been the standard for modern bows. However, the threat of extinction and the enforcement of trade bans have required bow makers to seek alternative woods. The hypothesis tested was that woods with physical, mechanical and acoustic properties similar to those of C. echinata would have high potential as alternative woods for bows. Accordingly, were investigated Handroanthus spp., Mezilaurus itauba, Hymenaea spp., Dipteryx spp., Diplotropis spp. and Astronium lecointei. Handroanthus and Diplotropis have the greatest number of similarities with C. echinata, but only Handroanthus spp. showed significant results in actual bow manufacture, suggesting the importance of such key properties as specific gravity, speed of sound propagation and modulus of elasticity. In practice, Handroanthus and Dipteryx produced bows of quality similar to that of C. echinata.

  6. Application of the Bow Tie method for evaluation of safety in the procedure of logging wells; Aplicacion del metodo de Bow Tie para la evaluacion de seguridad en la practica de perfilaje de pozos

    Energy Technology Data Exchange (ETDEWEB)

    Alfonso Pallares, C; Perez Reyes, Y.; Sarabia Molina, I.I. [Centro Nacional de Seguridad Nuclear (CNSN), La Habana (Cuba)

    2013-07-01

    This work consists of an assessment of security in the practice of logging of oil wells, using the method of Bow Tie for being a simple method of evaluation of the risk, which makes it possible in a structured way to set priorities to manage risk.

  7. Analysis of Biomass Gasification Poisoning Accident Based on BN-bow-tie%基于BN-bow-tie的生物质气化中毒事故分析

    Institute of Scientific and Technical Information of China (English)

    闫放; 许开立; 姚锡文; 王延瞳

    2015-01-01

    通过将故障树转化为贝叶斯网络,计算生物质气化中毒事故发生的概率为1.202 98×10-4/d,利用贝叶斯网络双向推导与诊断的功能计算基本事件的后验概率及重要度,从而分析出系统中导致事故发生的薄弱环节.结合bow-tie法同时分析导致薄弱环节失效的因素及失效后可能会出现的后果,基于此得出防止薄弱环节失效的预防措施以及失效后采取的控制措施,进而降低事故发生的概率;对薄弱环节阀门泄漏采取措施后,可使得中毒事故发生概率降低20.92%,最终达到降低事故发生概率的目的.

  8. Implications of MODIS bow-tie distortion on aerosol optical depth retrievals, and techniques for mitigation

    Science.gov (United States)

    Sayer, A. M.; Hsu, N. C.; Bettenhausen, C.

    2015-12-01

    The scan geometry of the Moderate Resolution Imaging Spectroradiometer (MODIS) sensors, combined with the Earth's curvature, results in a pixel shape distortion known as the "bow-tie effect". Specifically, sensor pixels near the edge of the swath are elongated along-track and across-track compared to pixels near the centre of the swath, resulting in an increase of pixel area by up to a factor of ∼ 9 and, additionally, the overlap of pixels acquired from consecutive scans. The Deep Blue and Dark Target aerosol optical depth (AOD) retrieval algorithms aggregate sensor pixels and provide level 2 (L2) AOD at a nominal horizontal pixel size of 10 km, but the bow-tie distortion means that they also suffer from this size increase and overlap. This means that the spatial characteristics of the data vary as a function of satellite viewing zenith angle (VZA) and, for VZA > 30°, corresponding to approximately 50 % of the data, are areally enlarged by a factor of 50 % or more compared to this nominal pixel area and are not spatially independent of each other. This has implications for retrieval uncertainty and aggregated statistics, causing a narrowing of AOD distributions near the edge of the swath, as well as for data comparability from the application of similar algorithms to sensors without this level of bow-tie distortion. Additionally, the pixel overlap is not obvious to users of the L2 aerosol products because only pixel centres, not boundaries, are provided within the L2 products. A two-step procedure is proposed to mitigate the effects of this distortion on the MODIS aerosol products. The first (simple) step involves changing the order in which pixels are aggregated in L2 processing to reflect geographical location rather than scan order, which removes the bulk of the overlap between L2 pixels and slows the rate of growth of L2 pixel size vs. VZA. This can be achieved without significant changes to existing MODIS processing algorithms. The second step involves

  9. Hybrid functional calculations on the band gap bowing parameters of In x Ga1‑x N

    Science.gov (United States)

    Mei, Lin; Yixu, Xu; Jianhua, Zhang; Shunqing, Wu; Zizhong, Zhu

    2016-04-01

    The electronic band structures and band gap bowing parameters of In x Ga1‑x N are studied by the first-principles method based on the density functional theory. Calculations by employing both the Heyd-Scuseria-Ernzerh of hybrid functional (HSE06) and the Perdew-Burke-Ernzerhof (PBE) one are performed. We found that the theoretical band gap bowing parameter is dependent significantly on the calculation method, especially on the exchange-correlation functional employed in the DFT calculations. The band gap of In x Ga1‑x N alloy decreases considerably when the In constituent x increases. It is the interactions of s–s and p–p orbitals between anions and cations that play significant roles in formatting the band gaps bowing. In general, the HSE06 hybrid functional could provide a good alternative to the PBE functional in calculating the band gap bowing parameters. Project supported by the National Natural Science Foundation of China (Nos. 11204257, 21233004) and the China Postdoctoral Science Foundation (No. 2012M511447).

  10. Can the magnetic field in the Orion arm inhibit the growth of instabilities in the bow shock of Betelgeuse?

    CERN Document Server

    van Marle, Allard Jan; Meliani, Zakaria

    2013-01-01

    Many evolved stars travel through space at supersonic velocities, which leads to the formation of bow shocks ahead of the star where the stellar wind collides with the interstellar medium (ISM). Herschel observations of the bow shock of $\\alpha$-Orionis show that the shock is almost free of instabilities, despite being, at least in theory, subject to both Kelvin-Helmholtz and Rayleigh-Taylor instabilities. A possible explanation for the lack of instabilities lies in the presence of an interstellar magnetic field. We wish to investigate whether the magnetic field of the interstellar medium (ISM) in the Orion arm can inhibit the growth of instabilities in the bow shock of $\\alpha$-Orionis. We used the code MPI-AMRVAC to make magneto-hydrodynamic simulations of a circumstellar bow shock, using the wind parameters derived for $\\alpha$-Orionis and interstellar magnetic field strengths of $B\\,=\\,1.4,\\, 3.0$, and $5.0\\, \\mu$G, which fall within the boundaries of the observed magnetic field strength in the Orion arm ...

  11. Numerical Analysis of Interaction Between Single-Pulse Laser-Induced Plasma and Bow Shock in a Supersonic Flow

    Institute of Scientific and Technical Information of China (English)

    FANG Juan; HONG Yanji; LI Qian

    2012-01-01

    The interaction of laser-induced plasma and bow shock over a blunt body is inves- tigated numerically in an M∞ =6.5 supersonic flow. A ray-tracing method is used for simulating the process of laser focusing. The gas located at the focused zone is ionized and broken down and transformed into plasma. In a supersonic flow the plasma moves downstream and begins to interact with the bow shock when it approaches the surface of the blunt body. The parameters of flowfield and blunt body surface are changed due to the interaction. By analyzing phenomena occurring in the complex unsteady flowfield during the interaction in detail, we can better under- stand the change of pressure on the blunt body surface and the mechanism of drag reduction by laser energy deposition. The results show that the bow shock is changed into an oblique shock due to the interaction of the laser-induced low-density zone with the bow shock, so the wave drag of the blunt body is reduced.

  12. Spatial and spectral properties of plasma waves observed upstream of Saturn’s bow shock by the Cassini spacecraft

    Czech Academy of Sciences Publication Activity Database

    Píša, David; Santolík, Ondřej; Souček, Jan; Hospodarsky, G. B.; Kurth, W. S.; Gurnett, D. A.

    Göttingen: European Geosciences Union, 2016. EGU2016-8107. ISSN 1607-7962. [EGU General Assembly 2016. 17.04.2016-22.04.2016, Vienna] Institutional support: RVO:68378289 Keywords : plasma waves * bow shock * magnetosphere * Cassini * Saturn Subject RIV: BL - Plasma and Gas Discharge Physics http://meetingorganizer.copernicus.org/EGU2016/EGU2016-8107.pdf

  13. The effect of mass loading outside cometary bow shock for the plasma and wave measurements in the coming cometary missions

    International Nuclear Information System (INIS)

    The neutral gas emitted by comets are partly photoionized along their path. The interaction of the ions with the solar wind leads to observable particle and wave events, in the ambient plasma before the bow shock. These questions are discussed in the paper. (author)

  14. Atelier Bow-Wow on the Representation of Behaviorology: Yosiharu Tsukamoto in conversation with Anne Elisabeth Toft and Christina Capetillo

    DEFF Research Database (Denmark)

    Toft, Anne Elisabeth; Capetillo, Christina

    Yoshiharu Tsukamoto discussing the representational practices of Atelier Bow-Wow and its work on “Behaviorology”: How do you represent the seemingly un-representable? How do you depict and illustrate what is not tangible? How do you represent social practices, time-based processes, situations...

  15. Bow-tie risk assessment combining causes and effects applied to gasoil storage in an abandoned salt cavern,

    NARCIS (Netherlands)

    Visser, K; Hendriks, D.; Wildenborg, T.; Duijne, H.

    2014-01-01

    A semi-quantitative risk assessment is presented for the storage of gas oil in depleted salt caverns in the Twente region, the Netherlands. It is based on a bow-tie model, in which an incident, leakage of gas oil from the storage system (cavern and wells), is evaluated by assessing its possible caus

  16. From Bows to Sound-Chests: Tracing the Ancestry of the Violin

    Directory of Open Access Journals (Sweden)

    Janelle R. Finley

    2016-04-01

    Full Text Available The ancestry of the violin is a subject that has been studied, researched, debated, and written about in great detail. However, despite all of the research and study, the ancestry of the violin is still not certain. This paper presents two schools of thought that propose different theories as to how the ancestry of the violin should be determined and what instruments should be included in the ancestry of the violin. The first school of thought proposes that the violin’s ancestry should be traced through the bow. The second theory proposes that the violin’s ancestry should be traced through the sound-chest of the violin. This paper also presents the different arguments for and against each theory, the importance of this topic, and the paper’s position on this topic. Research for this paper was accomplished through the use of scholarly books on the subject of the history of the violin.

  17. Method for measuring violin sound radiation based on bowed glissandi and its application to sound synthesis.

    Science.gov (United States)

    Perez Carrillo, Alfonso; Bonada, Jordi; Patynen, Jukka; Valimaki, Vesa

    2011-08-01

    This work presents a method for measuring and computing violin-body directional frequency responses, which are used for violin sound synthesis. The approach is based on a frame-weighted deconvolution of excitation and response signals. The excitation, consisting of bowed glissandi, is measured with piezoelectric transducers built into the bridge. Radiation responses are recorded in an anechoic chamber with multiple microphones placed at different angles around the violin. The proposed deconvolution algorithm computes impulse responses that, when convolved with any source signal (captured with the same transducer), produce a highly realistic violin sound very similar to that of a microphone recording. The use of motion sensors allows for tracking violin movements. Combining this information with the directional responses and using a dynamic convolution algorithm, helps to improve the listening experience by incorporating the violinist motion effect in stereo. PMID:21877814

  18. Quantitative spectroscopy on individual wire, slot, bow-tie, rectangular, and square-shaped optical antennas.

    Science.gov (United States)

    Husnik, Martin; Niegemann, Jens; Busch, Kurt; Wegener, Martin

    2013-11-15

    By using a recently introduced approach combining a focus-modulation technique with a common-path interferometer, we measure quantitatively the extinction, scattering, and absorption cross-section spectra of individual optical antennas. The experimental results on thin-wire antennas, slot antennas, bow-tie antennas, rectangular antennas, and square-shaped antennas resonating at around 1.4 μm wavelength are discussed. We find increased resonant scattering cross sections for the latter four antennas compared to the thin-wire antenna, both in absolute terms and relative to the absorption cross section. The square-shaped antenna's resonant extinction cross section approaches the limit of a coherent point dipole. However, the ratio of the resonant extinction cross section to the geometrical cross section of 38 is largest for the simple thin-wire antenna. PMID:24322083

  19. Oxidation of graphene 'bow tie' nanofuses for permanent, write-once-read-many data storage devices.

    Science.gov (United States)

    Pearson, A C; Jamieson, S; Linford, M R; Lunt, B M; Davis, R C

    2013-04-01

    We have fabricated nanoscale fuses from CVD graphene sheets with a 'bow tie' geometry for write-once-read-many data storage applications. The fuses are programmed using thermal oxidation driven by Joule heating. Fuses that were 250 nm wide with 2.5 μm between contact pads were programmed with average voltages and powers of 4.9 V and 2.1 mW, respectively. The required voltages and powers decrease with decreasing fuse sizes. Graphene shows extreme chemical and electronic stability; fuses require temperatures of about 400 °C for oxidation, indicating that they are excellent candidates for permanent data storage. To further demonstrate this stability, fuses were subjected to applied biases in excess of typical read voltages; stable currents were observed when a voltage of 10 V was applied to the devices in the off state and 1 V in the on state for 90 h each. PMID:23478811

  20. Determination of main rational biomechanical characteristics in shooting from a bow

    Directory of Open Access Journals (Sweden)

    Adashevskiy V.M.

    2012-03-01

    Full Text Available The aim is to build rational parameters of technical actions of sportsman in shooting from a bow. It is worked out and decided mathematical model and the task of dynamics. Influence on having a special purpose exactness of corners of flight of arrow with an account and without the account of force of resistance of air environment is certain. It is distinguished the basic technical run-time errors of sportsman exercises. It is set that for successful realization of descriptions of target exactness and minimum values of deviations from an aim on different distances of shooting, sportsman must provide: maintenance of scene and rational pose, implementation of rational technical actions. It is shown directions of choice of necessary biomechanics descriptions that a sportsman can realize for providing target exactness and minimum values of deviations from aim on different distances of shooting.

  1. On the origin of hot diamagnetic cavities near the earth's bow shock

    Science.gov (United States)

    Thomsen, M. F.; Gosling, J. T.; Bame, S. J.; Quest, K. B.; Russell, C. T.

    1988-01-01

    The origin of hot diamagnetic cavities (HDCs) observed occasionally upstream from the earth's bow shock is investigated by examining the results of November 16, 1977, observation, when four of these events occurred on a single day, as well as plasma and field data from that day. The results suggest that HDCs may form as a result of an unusually strong interaction between shock-reflected ions and the incoming solar wind. It is proposed that this interaction stems from a temporary and localized reflection of a larger-than-normal fraction of the incident ions, which is stimulated by sudden changes in the upstream field orientation; the consequences of such a temporary overreflection are found to be consistent with many of the observed features of HDCs, including the strong slowing, deflection, and heating of the flow, as well as the localization, internal recoveries, and occasional formation upstream from the shock itself.

  2. Observational evidence on the origin of ions upstream of the earth's bow shock

    Science.gov (United States)

    Thomsen, M. F.; Gosling, J. T.; Schwartz, S. J.

    1983-01-01

    The kinematic formalism described by Schwartz et al. (1983) is used to quantitatively compare the zeroth order predicted energies for four different source hypotheses for ions detected upstream of the earth's bow shock with previously published observations of upstream field-aligned beams and gyrating ion events. Specular reflection of a fraction of the incident solar wind is found to be the most credible explanation of gyrating ion events observed upstream of shocks ranging from quasi-parallel to nearly perpendicular. The recent hypothesis that field-aligned beams are the result of leakage from the magnetosheath of ions which were originally specularly reflected at quasi-perpendicular portions of the shock provides good agreement with observed energies of many field-aligned beams. Only magnetic moment conserving reflection of solar wind ions is capable of accounting for two very energetic beam events.

  3. Monitoring of turbulence upstream and downstream of the bow shock using the Cluster observations

    International Nuclear Information System (INIS)

    Complete text of publication follows. The paper concerns with the study of plasma turbulence, upstream and downstream of the quasi-parallel bow shock (BS), using the FGM magnetic records of the Cluster mission. The turbulence and its intermittent nature have already been evidenced by several studies, in these regions. We argue that the level of intermittency can be monitored in terms of space and time by intermittency or multifractal model parameters obtained from turbulent (mostly nonlinear) analyses (e.g. probability density function, structure function, or multifractal spectrum analyses) of the continuous spacecraft records. In the analyses, the multi-spacecraft observations have a key role, since with them the intermittency in the plasma fluctuations can be revealed not only in temporal but also in spatial scales. We intend to find relationship between the intermittency level upstream the bow shock and the varying solar wind (SW) parameters, such as the velocity, plasma density, Mach number, etc. Furthermore, the connection between the turbulent properties of the upstream region and the Pc3-Pc4 magnetic pulsation activities observed in Earth magnetic observatories is also intended to be studied. The reason is that part of the surface observations of the Pc3-Pc4 pulsation phenomena origins from the upstream region as a result of enhanced wave activities caused by ion-cyclotron resonance of SW protons backstreaming from the BS boundary. The UWs are carried by the SW towards the magnetosheath and the magnetopause, and finally enter the magnetosphere generating clear pulsation signals in Earth magnetic records. In the comparative studies, the pulsation records of the MM100 meridional magnetometer array are used.

  4. The CHESS survey of the L1157-B1 bow-shock: Dissecting the water content

    Science.gov (United States)

    Busquet, Gemma; Lefloch, Bertrand; Benedettini, Milena; Ceccarelli, Cecilia; Codella, Claudio; Cabrit, Sylvie; Nisini, Brunella; Viti, Serena; Gómez-Ruiz, Arturo; Gusdorf, Antoine; Di Giorgio, Anna Maria; Wiesenfeld, Laurent

    2013-07-01

    Molecular outflows powered by young protostars strongly affect the kinematics and chemistry of the natal molecular cloud through strong shocks, resulting in an increase of the abundance of several species. In particular, water is a powerful tracer of shocked material due to its sensitivity to both physical conditions and chemical processes. The observations of the "Chemical Herschel Survey of Star forming regions" (CHESS) key program towards the shock region L1157-B1 offered a unique and comprehensive view of the water emission in a typical protostellar bow shock across the submillimeter and far-infrared window. A grand total of 13 water lines have been detected with the PACS and HIFI instruments, probing a wide range of excitation conditions and providing us with a detailed picture on both the kinematics and the spatial distribution of water emission. Several gas components have been identified coexisting in the L1157-B1 shock region. Large Velocity Gradient (LVG) analysis reveals that these components have different excitation conditions: i) a warm (T~250 K) and dense (n(H2)~10^6 cm-3) gas component seen also with the CO lines and associated with the partly dissociative shock produced by the impact of the protostellar jet against the bow shock; ii) a compact (size~5''), hot (T~700 K), and less dense (n(H2)~10^4 cm-3) gas component, and iii) an extended component associated with the B1 outflow cavity. These three components present clear differences in terms of water enrichment. Finally, we confront the physical and chemical properties of the H2O emission to the predictions of current shock models.

  5. Using Collaborative Modeling to Inform Policy Decisions in the Bow River Basin

    Science.gov (United States)

    Sheer, A. S.; Sheer, D. P.; Hill, D.

    2011-12-01

    The Bow River in Alberta, Canada serves a wide range of municipal, agricultural, recreational, and industrial purposes in the province. In 2006, the basin was deemed over-allocation and closed to new licenses. The Calgary region, however, continues to expand. In the next 60 to 70 years, population levels are expected to reach 2.8 million (more than double the current 1.2 million) with 800,000 new jobs. This increasing pressure led several stakeholders to work together in the development of a new management model to improve the management of the system as an integrated watershed. The major previous model of the system allowed only limited flexibility in management, focusing instead on strict license based operations. Over a 6 month period, with numerous multi-party meetings, the group developed the Bow River Operations Model (BROM). Based in OASIS software, this model integrated input from the major water users in the region to emulate the real-life decisions that are actually made on a daily bases, even when technically in violation of the strict license agreements (e.x. junior licensees receiving water despite senior priority due to exceedingly low volume requirements). Using historical records as forecasts, and performance measures developed with the best available science through expert opinion, participants jointly developed a new reservoir operation strategy. Even with such a short timeframe, the BROM exercise showed that there was substantial room for improvement. Utilizing a "Water Bank" of purchased storage, downstream flows could be significantly improved without affecting quality. Additional benefits included fishery improvement, new recreation opportunities, dissolved oxygen improvement during critical periods, and the ability to accommodate long-term demand forecasts for surrounding municipalities. This strategy has been presented to, and favorably received by, the Alberta Minister of Environment for guidance during negotiations with the local

  6. On nonstationarity and rippling of the quasiperpendicular zone of the Earth bow shock: Cluster observations

    Directory of Open Access Journals (Sweden)

    V. V. Lobzin

    2008-09-01

    Full Text Available A new method for remote sensing of the quasiperpendicular part of the bow shock surface is presented. The method is based on analysis of high frequency electric field fluctuations corresponding to Langmuir, upshifted, and downshifted oscillations in the electron foreshock. Langmuir waves usually have maximum intensity at the upstream boundary of this region. All these waves are generated by energetic electrons accelerated by quasiperpendicular zone of the shock front. Nonstationary behavior of the shock, in particular due to rippling, should result in modulation of energetic electron fluxes, thereby giving rise to variations of Langmuir waves intensity. For upshifted and downshifted oscillations, the variations of both intensity and central frequency can be observed. For the present study, WHISPER measurements of electric field spectra obtained aboard Cluster spacecraft are used to choose 48 crossings of the electron foreshock boundary with dominating Langmuir waves and to perform for the first time a statistical analysis of nonstationary behavior of quasiperpendicular zone of the Earth's bow shock. Analysis of hidden periodicities in plasma wave energy reveals shock front nonstationarity in the frequency range 0.33 fBiBi, where fBi is the proton gyrofrequency upstream of the shock, and shows that the probability to observe such a nonstationarity increases with Mach number. The profiles observed aboard different spacecraft and the dominating frequencies of the periodicities are usually different. Hence nonstationarity and/or rippling seem to be rather irregular both in space and time rather than resembling a quasiregular wave propagating on the shock surface.

  7. Ion Acceleration at the Quasi-parallel Bow Shock: Decoding the Signature of Injection

    Science.gov (United States)

    Sundberg, Torbjörn; Haynes, Christopher T.; Burgess, D.; Mazelle, Christian X.

    2016-03-01

    Collisionless shocks are efficient particle accelerators. At Earth, ions with energies exceeding 100 keV are seen upstream of the bow shock when the magnetic geometry is quasi-parallel, and large-scale supernova remnant shocks can accelerate ions into cosmic-ray energies. This energization is attributed to diffusive shock acceleration however, for this process to become active, the ions must first be sufficiently energized. How and where this initial acceleration takes place has been one of the key unresolved issues in shock acceleration theory. Using Cluster spacecraft observations, we study the signatures of ion reflection events in the turbulent transition layer upstream of the terrestrial bow shock, and with the support of a hybrid simulation of the shock, we show that these reflection signatures are characteristic of the first step in the ion injection process. These reflection events develop in particular in the region where the trailing edge of large-amplitude upstream waves intercept the local shock ramp and the upstream magnetic field changes from quasi-perpendicular to quasi-parallel. The dispersed ion velocity signature observed can be attributed to a rapid succession of ion reflections at this wave boundary. After the ions’ initial interaction with the shock, they flow upstream along the quasi-parallel magnetic field. Each subsequent wavefront in the upstream region will sweep the ions back toward the shock, where they gain energy with each transition between the upstream and the shock wave frames. Within three to five gyroperiods, some ions have gained enough parallel velocity to escape upstream, thus completing the injection process.

  8. Diffusive Shock Acceleration Simulations: Comparison with Particle Methods and Bow Shock Measurements

    Science.gov (United States)

    Kang, Hyesung; Jones, T. W.

    1995-07-01

    Direct comparisons of diffusive particle acceleration numerical simulations have been made against Monte Carlo and hybrid plasma simulations by Ellison et al. (1993) and against observations at the Earth's bow shock presented by Ellison et al. (1990). Toward this end we have introduced a new numerical scheme for injection of cosmic-ray particles out of the thermal plasma, modeled by way of the diffusive scattering process itself; that is, the diffusion and acceleration across the shock front of particles out of the suprathermal tail of the Maxwellian distribution. Our simulations take two forms. First, we have solved numerically the timedependent diffusion-advection equation for the high-energy (cosmic-ray) protons in one-dimensional quasiparallel shocks. Dynamical feedback between the particles and thermal plasma is included. The proton fluxes on both sides of the shock derived from our method are consistent with those calculated by Ellison et al. (1993). A similar test has compared our methods to published measurements at the Earth's bow shock when the interplanetary magnetic field was almost parallel to the solar wind velocity (Ellison et al. 1990). Again our results are in good agreement. Second, the same shock conditions have been simulated with the two-fluid version of diffusive shock acceleration theory by adopting injection rates and the closure parameters inferred from the diffusion-advection equation calculations. The acceleration efficiency and the shock structure calculated with the two-fluid method are in good agreement with those computed with the diffusion-advection method. Thus, we find that all of these computational methods (diffusion-advection, two-fluid, Monte Carlo, and hybrid) are in substantial agreement on the issues they can simultaneously address, so that the essential physics of diffusive particle acceleration is adequately contained within each. This is despite the fact that each makes what appear to be very different assumptions or

  9. Post-irradiation examination of a bowed PWR fuel rod with contact

    International Nuclear Information System (INIS)

    During reactor operation in the Ringhals 2 PWR a fuel rod bowed and as a result came in contact with an adjacent rod. The rod contact in one of the lower grid spans was observed during visual inspection at the end of life. The visual appearance suggested that there was possibly increased cladding corrosion on both the contacting rods at and close to the position of contact. One of the contacting rods was sent to Studsvik’s Hot Cell Laboratory for investigation where fission gas analysis, gamma scanning, EC oxide thickness, metallography (optical microscopy) and cladding microhardness measurements were performed in order to verify the impact of the bow and the contact on the fuel rod performance, with particular focus on the local cladding corrosion. The influence of the reduction of moderator in the region of the contact point was seen in the Cs-137 axial gamma scanning and in the Ce-144 rotational gamma scanning, which show a local reduction of both the pellet-average power, in the contact region, and specifically on the side with the contact. Visual inspection revealed increased corrosion in the rod-rod contact position. Metallographic examination of a cross-section at the elevation with the contact showed that increased corrosion and loss of material had occurred at the contact position. Outside of the immediate vicinity of the contact region the corrosion was not affected. The cladding microhardness was measured at different radial positions both at the contact position and at other positions around the cladding circumference. Based on the relationship between the microhardness and local temperature during operation on fully wetted cladding, it was possible to estimate the cladding surface temperature at the contact point to approximately 360°C. This local overheating and conditions arising from the local overheating can explain the higher local oxidation of the cladding observed in the visual inspection and metallography. (author)

  10. Based on Bow-Tie Model of the Hanger Failure Analysis of Light-liner Cementing%基于Bow-Tie模型的轻尾管固井中悬挂器失效分析

    Institute of Scientific and Technical Information of China (English)

    孙泽秋; 金磊; 马锦明; 李强

    2015-01-01

    Light-liner Cementing is a dynamic systems with clearly technological process and com-plex construction.For failure research of light-liner hanger cementing process,the hanger failure of Bow-Tie model is constructed,which combine FTA with ETA analysis method.By using fault-tree analytic method,the failure reasons of hanger are induced in this paper,the failure cause of the accident after the whole process is studied,through event-tree analysis,which can understand light liner hanger cementing failure intuitively in the whole development process.Combined with certain oilfield accident analysis of Y well,Bow-Tie model is viable for the hanger failure issue based on the analysis of light-liner cementing.Studies show that Bow-Tie model is of great signifi-cance to prevent the hanger failure,and has a guiding significance for light-liner on-site cementing operation.%轻尾管固井是一个工艺流程清晰、施工较复杂的动态系统。针对轻尾管固井中的悬挂器失效问题,采用事故树和事件树相结合的分析方法,构建了悬挂器失效的Bow-Tie 模型。利用事故树分析法得到了诱发悬挂器失效的原因,通过事件树分析法研究了悬挂器失效后引起事故的全过程,直观地了解轻尾管固井中悬挂器失效的整个发展过程。结合某油田 Y 井的事故分析,验证了Bow-Tie模型在分析轻尾管固井中悬挂器失效方面是可行的。研究得出的悬挂器失效Bow-Tie模型对于防止悬挂器失效的发生具有重要意义,对于轻尾管固井的现场施工具有指导作用。

  11. 基于模糊Bow-tie模型的深水海底管道定量风险评价研究%Quantitative Risk Assessment of Deepwater Submarine Pipeline Based on Fuzzy Bow-tie Model

    Institute of Scientific and Technical Information of China (English)

    胡显伟; 段梦兰; 官耀华

    2012-01-01

    In order to effectively assess risk of deepwater submarine pipeline, a new quantitative risk assessment method based on fuzzy bow - tie model, was therefore proposed. Firstly, leakage possibility of oil/gas was quantitatively analyzed using Bow-tie model, Fuzzy Sets and Delphi method. Moreover, leakage consequence was analyzed by analytic hierarchy process, and weighting coefficients of consequence-influencing factors were obtained. Accordingly, quantitative risk assessment was completed by risk matrix. In the end, the above-mentioned assessment method was applied to a certain submarine pipeline. Leakage possibility level of target submarine pipeline belongs to A and leakage consequence level, Ⅲ, and risk level , high, agreeing well with the reality.%为有效评价深水海底管道风险,提出一种新的模糊Bow-tie模型定量风险评价方法.综合运用Bow-tie图、模糊集以及德尔菲法,定量分析油气泄漏概率.进一步利用层次分析法(AHP)研究油气泄漏后果的严重程度,给出泄漏后果因素的权重系数选择方案.同时,结合风险矩阵,实现对高风险深水海底管道的定量风险评价.将上述方法用到具体海底管道工程中,得出目标海底管道泄漏概率属于A级,泄漏后果属于Ⅲ级,泄漏风险为高风险,这一结果与实际情况较为符合.

  12. O+ pickup ions outside of Venus' bow shock: Venus Express observations

    Science.gov (United States)

    Wei, Yong; Fraenz, Markus; Dubinin, Eduard; Zhang, Tielong; Jarvinen, Riku; Wan, Weixing; Kallio, Esa; Collinson, Glyn; Barabash, Stars; Norbert, Krupp; Woch, Joachim; Lundin, Rickard; delva, Magda

    2013-04-01

    Pickup ions are ions of planetary origin that become assimilated into the solar wind flow through their interaction with the solar wind magnetic and electric field. The speed of pickup ions varies between zero and twice the underlying plasma flow component perpendicular to magnetic field vector. For the unmagnetized planet Venus and Mars, oxygen (O+) pickup ions are known to be important because they can modify the global configuration of planetary plasma environment and significantly contribute to the atmospheric O+ loss [1]. Since the kinetic energy of an O+ pickup ion can reach 64 times that of a co-moving proton, an instrument must be able to measure O+ ions with energy of at least tens of keV to investigate the O+ pickup ion distribution from planetary ionosphere to solar wind. The in-situ observations and simulations at Mars have shown that the energy of O+ pickup ions can be 55-72 keV outside of the bow shock [2]. For Venus case, the plasma analyzer (OPA) onboard Pioneer Venus Orbiter (PVO), which was designed for solar wind monitoring, has an 8 keV energy limit for O+ detection and the limited sampling and data rate [3]. Therefore, OPA can only measure the O+ pickup ions in the sheath flow or inside the induced magnetosphere where the speed of ambient plasma flow is significantly lower than that of the unshocked solar wind outside of the bow shock. In addition, Galileo also did not capture O+ outside bowshock during its 1-hour Venus flyby though its plasma instrument had ability to cover the energy band of O+ pickup ions [4]. The Ion Mass Analyzer (IMA), included in the Analyzer of Space Plasma and Energetic Atoms (ASPERA-4) package on board Venus Express (VEX), determines the composition, energy, and angular distribution of ions in the energy range ~10 eV/q to 30 keV/q. Note that an O+ ion moving at the typical solar wind speed 400 km/s has kinetic energy 13.4 keV. Therefore, IMA has ability to measure the O+ pickup ions outside of Venus' bow shock. We

  13. Protection layer analysis based on bow-tie applying in risk analysis%基于bow-tie的保护层分析法在风险分析中的应用研究

    Institute of Scientific and Technical Information of China (English)

    王旭; 张可旺

    2015-01-01

    充分考虑石化装置的复杂工艺特点,建立了基于领结分析(bow-tie)的保护层(LOPA)风险分析法,能够在相互关联的工艺装置体系中,明确“关系”并客观的进行量化分析.首先运用HAZOP辨识工艺过程中的危险,并对识别出的危险所导致的事故后果进行定性评估,找出事故后果等级较高的危险;然后运用bow-tie-LOPA集成分析对该风险的关键事件进行全面分析,确定事故可能发生的概率,以及保护措施是否将风险降低到可接受水平;若剩余风险等级超过容许标准,则需进行bow-tie分析辨识出使保护层持续有效的关键活动,进而控制后果严重事故的发生.

  14. Application of Bow-tie Technology in the Risk Management of Urban Gas Pipeline%Bow-tie技术在城镇燃气管道风险管理中的应用

    Institute of Scientific and Technical Information of China (English)

    贾朋美; 於孝春; 宋前甫

    2014-01-01

    为完善燃气管道安全评价体系,首次将Bow-tie技术引入到城镇燃气管道的风险管理中,通过Bow-tie图将故障树与事件树结合起来,定性分析了导致燃气管道泄漏的原因和后果,针对性地提出预防减缓措施.Bow-tie技术将风险辨识、风险分析、风险评估、风险控制和风险管理在图形中完整地展现出来,具有广泛的适用性,既可用于事前预防,又能指导事后响应,最大程度杜绝管道事故的发生,为燃气管道完整性管理提供实用的技术支撑.

  15. Dual-Frequency Operation of Bow-Tie Microstrip Antenna%蝶形微带天线的双频工作

    Institute of Scientific and Technical Information of China (English)

    钟顺时; 张需溥

    2005-01-01

    Characteristics of a single-feed dual-frequency bow-tie microstrip antenna are studied. By using the variation method, simple formulas for resonant frequencies of the bow-tie microstrip antenna are derived. It is shown that the dual-frequency ratio can be controlled easily by choosing the parameters of the antenna. This design gives compact antenna size and simple antenna structure. Experimental results are presented, verifying the validity of the design.

  16. Enhanced diffusive ion scattering in front of the Earth's quasi-parallel bow shock: a case study

    Science.gov (United States)

    Kis, Arpad; Scholer, Manfred; Klecker, Berndt; Lucek, Elisabeth; Dandouras, Iannis; Lemperger, István; Wesztergom, Viktor; Novák, Attila; Szalai, Sándor

    2014-05-01

    In our study we report on observations of energetic ions upstream of the Earth's quasi-parallel bow shock by Cluster at times of large inter-spacecraft separation distance. For the analysis we use the ion data provided by the CIS-HIA in the 10-32 keV energy range and the magnetic data recorded by the FGM instrument. We determine the spatial gradient of partial energetic ion densities at various distances from the bow shock. The gradient in all energy channels decreases exponentially with distance and the e-folding distance of the gradients depends approximately linearly on energy but there is a significant difference in their values obtained at the observed three upstream ion events. We demonstrate for the first time that under specific interplanetary conditions the mechanism of the diffuse ion scattering can change significantly and results in an anomalous diffusive process charactized by an unusually small e-folding distance.

  17. Band gap bowings and anomalous pressure effects in III–V nitride alloys: Role of In-segregation

    DEFF Research Database (Denmark)

    Gorczyca, I.; Suski, T.; Christensen, Niels Egede;

    2011-01-01

    Using ab initio calculations a comparison between InxGa1-xN, InxAl1-xN and GaxAl1-xN is performed to examine the role of indium in nitride alloys. The band gap, Eg, as well as its pressure coefficient, dEg/dp, are studied as functions of chemical composition, x. Following theoretical and...... experimental suggestions about the crucial role of In-segregation in InxGa1-xN and InxAl1-xN, different arrangements of In atoms, uniform and clustered are considered. The presence of In and its clustering introduces a significant reduction of both Eg and dEg/dp, as well as strong bowings. These effects are...... responsible for the enhancements of bowings in the case of clustered distribution of indium atoms....

  18. Periodic oscillations of the quasi-parallel bow shock as observed with the AMPTE/CCE spacecraft

    Science.gov (United States)

    Strangeway, R. J.; Zanetti, L. J.

    1991-01-01

    The AMPTE/CCE spacecraft has, on occasion, encountered the earth's bow shock near apogee (about 9 earth radii). During one encounter, on November 1, 1984, the bow shock was observed to pass back and forth over the spacecraft several times in a periodic fashion. The period of the oscillation was about 20 seconds, and an upstream wave with a similar period was observed in the solar wind just prior to the multiple shock crossings. Minimum variance analysis of the shock crossings shows that the magnetic field carried out a single rotation through 360 deg for each pair of shock crossings. This implies that the shock was responding to the rotation of the field in the upstream wave, and it is shown how the plasma displacement associated with the upstream wave can produce the observed oscillations. These data may provide support for the wavelike structure of quasi-parallel shocks predicted in simulations.

  19. X-ray Observations of Bow Shocks around Runaway O Stars. The case of $\\zeta$ Oph and BD+433654

    CERN Document Server

    Toalá, J A; González-Gaán, A; Guerrero, M A; Ignace, R; Pohl, M

    2016-01-01

    Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretical works. We present X-ray observations towards the runaway stars $\\zeta$ Oph (Chandra and Suzaku) and BD+433654 (XMM-Newton) to search for the presence of non-thermal X-ray emission. We found no evidence of non-thermal emission spatially coincident with the bow shocks, nonetheless, diffuse emission is detected in the vicinity of $\\zeta$ Oph. After a careful analysis of its spectral characteristics we conclude that this emission has a thermal nature with a plasma temperature of $T \\approx 2 \\times10^{6}$ K. The cometary shape of this emission seems to be in line with recent predictions of radiation-hydrodynamic models of runaway stars. The case of BD+433654 is puzzling as non-thermal emission has been reported in a previous work for this source.

  20. Study on the effect of the CANFLEX-NU fuel element bowing on the critical heat flux

    International Nuclear Information System (INIS)

    The effect of the CANFLEX-NU fuel element bowing on the critical heat flux is reviewed and analyzed, which is requested by KINS as the Government design licensing condition for the use of the fuel bundles in CANDU power reactors. The effect of the gap between two adjacent fuel elements on the critical heat flux and onset-of-dryout power is studied. The reduction of the width of a single inter-rod gap from its nominal size to the minimum manufacture allowance of 1 mm has a negligible effects on the thermal-hydraulic performance of the bundle for the given set of boundary conditions applied to the CANFLEX-43 element bundle in an uncrept channel. As expected, the in-reactor irradiation test results show that there are no evidence of the element bow problems on the bundle performance

  1. Study on the effect of the CANFLEX-NU fuel element bowing on the critical heat flux

    Energy Technology Data Exchange (ETDEWEB)

    Suk, Ho Chun; Cho, Moon Sung; Jeon, Ji Su

    2001-01-01

    The effect of the CANFLEX-NU fuel element bowing on the critical heat flux is reviewed and analyzed, which is requested by KINS as the Government design licensing condition for the use of the fuel bundles in CANDU power reactors. The effect of the gap between two adjacent fuel elements on the critical heat flux and onset-of-dryout power is studied. The reduction of the width of a single inter-rod gap from its nominal size to the minimum manufacture allowance of 1 mm has a negligible effects on the thermal-hydraulic performance of the bundle for the given set of boundary conditions applied to the CANFLEX-43 element bundle in an uncrept channel. As expected, the in-reactor irradiation test results show that there are no evidence of the element bow problems on the bundle performance.

  2. Band gap energy and bowing parameter of In-rich InAlN films grown by magnetron sputtering

    International Nuclear Information System (INIS)

    The crystal structure, band gap energy and bowing parameter of In-rich InxAl1-xN (0.7 xAl1-xN films were obtained from absorption spectra. Band gap tailing due to compositional fluctuation in the films was observed. The band gap of the as-grown InN measured by optical absorption method is 1.34 eV, which is larger than the reported 0.7 eV for pure InN prepared by molecular beam epitaxy (MBE) method. This could be explained by the Burstein-Moss effect under carrier concentration of 1020 cm-3 of our sputtered films. The bowing parameter of 3.68 eV is obtained for our InxAl1-xN film which is consistent with the previous experimental reports and theoretical calculations.

  3. Pattern Switchable Antenna System Using Inkjet-Printed Directional Bow-Tie for Bi-Direction Sensing Applications.

    Science.gov (United States)

    Eom, Seung-Hyun; Seo, Yunsik; Lim, Sungjoon

    2015-01-01

    In this paper, we propose a paper-based pattern switchable antenna system using inkjet-printing technology for bi-direction sensor applications. The proposed antenna system is composed of two directional bow-tie antennas and a switching network. The switching network consists of a single-pole-double-throw (SPDT) switch and a balun element. A double-sided parallel-strip line (DSPSL) is employed to convert the unbalanced microstrip mode to the balanced strip mode. Two directional bow-tie antennas have different radiation patterns because of the different orientation of the reflectors and antennas. It is demonstrated from electromagnetic (EM) simulation and measurement that the radiation patterns of the proposed antenna are successfully switched by the SPDT switch. PMID:26690443

  4. Pattern Switchable Antenna System Using Inkjet-Printed Directional Bow-Tie for Bi-Direction Sensing Applications

    Directory of Open Access Journals (Sweden)

    Seung-Hyun Eom

    2015-12-01

    Full Text Available In this paper, we propose a paper-based pattern switchable antenna system using inkjet-printing technology for bi-direction sensor applications. The proposed antenna system is composed of two directional bow-tie antennas and a switching network. The switching network consists of a single-pole-double-throw (SPDT switch and a balun element. A double-sided parallel-strip line (DSPSL is employed to convert the unbalanced microstrip mode to the balanced strip mode. Two directional bow-tie antennas have different radiation patterns because of the different orientation of the reflectors and antennas. It is demonstrated from electromagnetic (EM simulation and measurement that the radiation patterns of the proposed antenna are successfully switched by the SPDT switch.

  5. Dispersion of low frequency plasma waves upstream of the quasi-perpendicular terrestrial bow shock

    Directory of Open Access Journals (Sweden)

    A. P. Dimmock

    2013-08-01

    Full Text Available Low frequency waves in the foot of a supercritical quasi-perpendicular shock front have been observed since the very early in situ observations of the terrestrial bow shock (Guha et al., 1972. The great attention that has been devoted to these type of waves since the first observations is explained by the key role attributed to them in the processes of energy redistribution in the shock front by various theoretical models. In some models, these waves play the role of the intermediator between the ions and electrons. It is assumed that they are generated by plasma instability that exist due to the counter-streaming flows of incident and reflected ions. In the second type of models, these waves result from the evolution of the shock front itself in the quasi-periodic process of steepening and overturning of the magnetic ramp. However, the range of the observed frequencies in the spacecraft frame are not enough to distinguish the origin of the observed waves. It also requires the determination of the wave vectors and the plasma frame frequencies. Multipoint measurements within the wave coherence length are needed for an ambiguous determination of the wave vectors. In the main multi-point missions such as ISEE, AMPTE, Cluster and THEMIS, the spacecraft separation is too large for such a wave vector determination and therefore only very few case studies are published (mainly for AMPTE UKS AMPTE IRM pair. Here we present the observations of upstream low frequency waves by the Cluster spacecraft which took place on 19 February 2002. The spacecraft separation during the crossing of the bow shock was small enough to determine the wave vectors and allowed the identification of the plasma wave dispersion relation for the observed waves. Presented results are compared with whistler wave dispersion and it is shown that contrary to previous studies based on the AMPTE data, the phase velocity in the shock frame is directed downstream. The consequences of this

  6. Quantified Energy Dissipation Rates in the Terrestrial Bow Shock. 2; Waves and Dissipation

    Science.gov (United States)

    Wilson, L. B., III; Sibeck, D. G.; Breneman, A. W.; Le Contel, O.; Cully, C.; Turner, D. L.; Angelopoulos, V.; Malaspina, D. M.

    2014-01-01

    We present the first quantified measure of the energy dissipation rates, due to wave-particle interactions, in the transition region of the Earth's collision-less bow shock using data from the Time History of Events and Macro-Scale Interactions during Sub-Storms spacecraft. Our results show that wave-particle interactions can regulate the global structure and dominate the energy dissipation of collision-less shocks. In every bow shock crossing examined, we observed both low-frequency (less than 10 hertz) and high-frequency (approximately or greater than10 hertz) electromagnetic waves throughout the entire transition region and into the magnetosheath. The low-frequency waves were consistent with magnetosonic-whistler waves. The high-frequency waves were combinations of ion-acoustic waves, electron cyclotron drift instability driven waves, electrostatic solitary waves, and whistler mode waves. The high-frequency waves had the following: (1) peak amplitudes exceeding delta B approximately equal to 10 nanoteslas and delta E approximately equal to 300 millivolts per meter, though more typical values were delta B approximately equal to 0.1-1.0 nanoteslas and delta E approximately equal to 10-50 millivolts per meter (2) Poynting fluxes in excess of 2000 microWm(sup -2) (micro-waves per square meter) (typical values were approximately 1-10 microWm(sup -2) (micro-waves per square meter); (3) resistivities greater than 9000 omega meters; and (4) associated energy dissipation rates greater than 10 microWm(sup -3) (micro-waves per cubic meter). The dissipation rates due to wave-particle interactions exceeded rates necessary to explain the increase in entropy across the shock ramps for approximately 90 percent of the wave burst durations. For approximately 22 percent of these times, the wave-particle interactions needed to only be less than or equal to 0.1 percent efficient to balance the nonlinear wave steepening that produced the shock waves. These results show that wave

  7. First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground

    Directory of Open Access Journals (Sweden)

    L. B. N. Clausen

    2009-01-01

    Full Text Available On 5 September 2002 the Geotail satellite observed the cone angle of the Interplanetary Magnetic Field (IMF change to values below 30° during a 56 min interval between 18:14 and 19:10 UT. This triggered the generation of upstream waves at the bow shock, 13 RE downstream of the position of Geotail. Upstream generated waves were subsequently observed by Geotail between 18:30 and 18:48 UT, during times the IMF cone angle dropped below values of 10°. At 18:24 UT all four Cluster satellites simultaneously observed a sudden increase in wave power in all three magnetic field components, independent of their position in the dayside magnetosphere. We show that the 10 min delay between the change in IMF direction as observed by Geotail and the increase in wave power observed by Cluster is consistent with the propagation of the IMF change from the Geotail position to the bow shock and the propagation of the generated waves through the bow shock, magnetosheath and magnetosphere towards the position of the Cluster satellites. We go on to show that the wave power recorded by the Cluster satellites in the component containing the poloidal and compressional pulsations was broadband and unstructured; the power in the component containing toroidal oscillations was structured and shows the existence of multi-harmonic Alfvénic continuum waves on field lines. Model predictions of these frequencies fit well with the observations. An increase in wave power associated with the change in IMF direction was also registered by ground based magnetometers which were magnetically conjunct with the Cluster satellites during the event. To the best of our knowledge we present the first simultaneous observations of waves created by backstreaming ions at the bow shock in the solar wind, the dayside magnetosphere and on the ground.

  8. Bow shock studies at Mercury, Venus, Earth, and Mars with applications to the solar-planetary interaction problem

    International Nuclear Information System (INIS)

    A series of bow shock studies conducted for the purpose of investigating the interaction between the solar wind and the terrestrial planets is presented. Toward this end appropriate modeling techniques have been developed and applied to the bow wave observations at Venus, Earth, and Mars. For Mercury the measurements are so few in number that no accurate determination of shock shape was deemed possible. Flow solutions generated using the observed bow wave surface as a boundary condition in a single fluid variable obstacle shape gasdynamic model produced excellent fits to the measured width and shape of the earth's magnetosheath. This result and the observed ordering of shock shape and position by upstream sonic Mach number provide strong support for the validity of the gasdynamic approximation. At Mercury the application of earth type models to the individual Mariner 10 boundry crossings has led to the determination of an effective planetary magnetic moment of 6+-2 x 1022 G-cm3. Consistent with the presence of a small terrestrial style magnetosphere, southward interplanetary magnetic fields were found to significantly reduce the solar wind stand-off distance most probably through the effects of dayside magnetic reconnection. For Venus the low altitude solar wind flow field derived from gasdynamic modeling of bow shock location and shape indicates that a fraction of the incident streamlines are absorbed by the neutral atmosphere near the ionopause; approximately 1% and 8%, respectively, in the solar maximum Pioneer Venus and solar minimum Venera measurements. Accordingly, it appears that cometary processes must be included in model calculations of the solar wind flow about Venus. At Mars the moderate height of the gasdynamic solar wind-obstacle interface and the weakness of the Martian ionosphere/atmosphere are found to be incompatible with a Venus type interaction

  9. Bond order wave (BOW) phase of the extended Hubbard model: Electronic solitons, paramagnetism, coupling to Peierls and Holstein phonons

    OpenAIRE

    Kumar, Manoranjan; Soos, Zolt'an G.

    2011-01-01

    The bond order wave (BOW) phase of the extended Hubbard model (EHM) in one dimension (1D) is characterized at intermediate correlation $U = 4t$ by exact treatment of $N$-site systems. Linear coupling to lattice (Peierls) phonons and molecular (Holstein) vibrations are treated in the adiabatic approximation. The molar magnetic susceptibility $\\chi_M(T)$ is obtained directly up to $N = 10$. The goal is to find the consequences of a doubly degenerate ground state (gs) and finite magnetic gap $E_...

  10. Investigation on Ring/Split-Ring Loaded Bow-Tie Antenna for Compactness and Notched-Band

    Science.gov (United States)

    Peng, Lin; Xie, Ji-yang; Jiang, Xing; Li, Si-min

    2016-03-01

    In this paper, a Bow-tie antenna with size reduction, impedance matching and radiation pattern improvement characteristics is designed with an encircling ring. Moreover, further size reduction is achieved by utilizing two symmetric split rings with more frequency tuning flexibility. Research found the ring loaded Bow-tie antenna (RLBA) shows better performance than the referenced Bow-tie antenna (RBA), and the mechanisms of performance improvements are also investigated and found to be the loading ring acts as two symmetric dipoles in the direction of the antenna's polarization. Then, using two symmetric split rings on the opposite side of the substrate as replacement of the encircling ring will prolong the length of the dipoles, and achieves further size reduction. The antenna is denoted as dual split ring loaded Bow-tie antenna (DSRBA). The low cutoff frequencies of RBA, RLBA and DSRBA with identical antenna size are 2.65 GHz, 2.27 GHz and 2.06 GHz, respectively. Then, the corresponding diameters of the antennas are 0.353 λc, 0.303 λc, and 0.275 λc, where λc are their corresponding wavelength of the lower cutoff frequencies. Furthermore, a notched-band is generated as a byproduct of the split rings, and it is owing to the new resonance of the overlap areas of the split rings. The notch can be used to alleviate interference of WiMAX band by carefully choosing the split rings' size. Radiation patterns of RLBA and DSRBA are also improved as current distributions of the high frequencies are trained in order by the ring/split-rings. Measurements are performed to verify the designs.

  11. Quasiparticle self-consistent GW theory of III-V nitride semiconductors: Bands, gap bowing, and effective masses

    DEFF Research Database (Denmark)

    Svane, Axel; Christensen, Niels Egede; Gorczyca, I.; van Schilfgaarde, M.; Chantis, A. N.; Kotani, T.

    2010-01-01

    the basis of the local approximation to density functional theory, although generally overestimated by 0.2–0.3 eV in comparison with experimental gap values. Details of the electronic energies and the effective masses including their pressure dependence are compared with available experimental...... information. The band gap of InGaN2 is considerably smaller than what would be expected by linear interpolation implying a significant band gap bowing in InGaN alloys....

  12. Multicentre randomised double bind crossover trial on contamination of conventional ties and bow ties in routine obstetric and gynaecological practice.

    OpenAIRE

    Biljan, M M; Hart, C. A.; Sunderland, D; Manasse, P R; Kingsland, C R

    1993-01-01

    OBJECTIVE--To assess level of contamination of neckwear worn by gynaecologists and obstetricians during routine working week. DESIGN--Multicentre randomised double blind crossover trial. Participants wore the same conventional ties for three days in one week and bow ties for the same period in second week. SETTING--Two teaching and three district general hospitals in the midlands, Wales, and north England. SUBJECTS--15 registrars and senior registrars. INTERVENTIONS--A swab soaked in sterile ...

  13. In situ bow monitoring: towards uniform blue and green InGaN/GaN quantum well structures grown on 100 mm sapphire substrates by MOVPE

    International Nuclear Information System (INIS)

    In this work, a home-made curvature measurement tool is used to monitor the wafer bow evolution during epitaxy of blue-green quantum well structures grown on 100 mm sapphire substrates. A single position detector is installed to real-time record both the surface reflectance and the wafer bowing simultaneously. Due to the low thermal conductivity of sapphire, a very large wafer bow was observed during high temperature thermal annealing before growth. The large wafer bow may lead to non-uniformity of both GaN buffer layers and InGaN/GaN multiple quantum wells (MQW). Careful temperature profile tuning and control of wafer bowing are critical to improve the layer uniformity. With the assistance of this in-situ bow monitoring tool, uniform and high efficiency blue/green InGaN/GaN quantum well structures have been demonstrated on 100 mm sapphire substrates by metal organic vapour phase epitaxy (MOVPE). The internal quantum efficiency (IQE) of the blue MQW structure is as high as 76%. This is deduced from temperature dependent (4 K-300 K) and power dependent photoluminescence (PL) measurements. (copyright 2010 WILEY-VCH Verlag GmbH and Co. KGaA, Weinheim) (orig.)

  14. IR-excesses around nearby Lambda Boo stars are caused by debris disks rather than ISM bow waves

    CERN Document Server

    Draper, Zachary H; Kennedy, Grant M; Wyatt, Mark C; Venn, Kim A; Sibthorpe, Bruce

    2015-01-01

    Lambda Boo stars are predominately A-type stars with solar abundant C, N, O, and S, but up to 2 dex underabundances of refractory elements. The stars' unusual surface abundances could be due to a selective accretion of volatile gas over dust. It has been proposed that there is a correlation between the Lambda Boo phenomenon and IR-excesses which are the result of a debris disk or interstellar medium (ISM) interaction providing the accreting material. We observe 70 or 100 and 160 $\\mu$m excess emission around 9 confirmed Lambda Boo stars with the Herschel Space Observatory, to differentiate whether the dust emission is from a debris disk or an ISM bow wave. We find that 3/9 stars observed host well resolved debris disks. While the remaining 6/9 are not resolved, they are inconsistent with an ISM bow wave based on the dust emission being more compact for its temperature and predicted bow wave models produce hotter emission than what is observed. We find the incidence of bright IR-excesses around Lambda Boo star...

  15. Energy time dispersion of a new class of magnetospheric ion events observed near the Earth's bow shock

    Directory of Open Access Journals (Sweden)

    G. C. Anagnostopoulos

    Full Text Available We have analyzed high time resolution (geq6 s data during the onset and the decay phase of several energetic (geq35 keV ion events observed near the Earth's bow shock by the CCE/AMPTE and IMP-7/8 spacecraft, during times of intense substorm/geomagnetic activity. We found that forward energy dispersion at the onset of events (earlier increase of middle energy ions and/or a delayed fall of the middle energy ion fluxes at the end of events are often evident in high time resolution data. The energy spectra at the onset and the decay of this kind of events show a characteristic hump at middle (50-120 keV energies and the angular distributions display either anisotropic or broad forms. The time scale of energy dispersion in the ion events examined was found to range from several seconds to sim1 h depending on the ion energies compared and on the rate of variation of the Interplanetary Magnetic Field (IMF direction. Several canditate processes are discussed to explain the observations and it is suggested that a rigidity dependent transport process of magnetospheric particles within the magnetosheath is most probably responsible for the detection of this new type of near bow shock magnetospheric ion events. The new class of ion events was observed within both the magnetosheath and the upstream region.

    Key words. Interplanetary physics (energetic particles; planetary bow shocks

  16. Deceleration of the solar wind upstream from the earth's bow shock and the origin of diffuse upstream ions

    Science.gov (United States)

    Bame, S. J.; Asbridge, J. R.; Feldman, W. C.; Gosling, J. T.; Paschmann, G.; Skopke, N.

    1980-01-01

    Observations with the Los Alamos Scientific Laboratory/Max-Planck-Institut crossed-fan solar wind ion experiment on ISEE I reveal that the solar wind is decelerated and deflected away from the direction of the earth's bow shock as it enters that portion of the upstream region populated by diffuse bow shock ions and long-period (10-60 s) waves. Typically, the average directed velocity vector changes by 7-10 km/s as it enters the wave region. At times, average speed changes as large as 25-40 km/s are observed. Superposed upon these changes in average flow speed are large amplitude (+ or - 15) fluctuations in flow speed associated with the waves themselves. The observations suggest that the solar wind deceleration is the result of momentum transfer from reflected bow shock ions to the wind via the long-period waves as the reflected ion beams go unstable. The broad angular distributions of the diffuse ions thus appear to be produced as a consequence of the disruption of reflected ion beams.

  17. Particle injection and acceleration at earth's bow shock - Comparison of upstream and downstream events

    Science.gov (United States)

    Ellison, Donald C.; Moebius, Eberhard; Paschmann, Goetz

    1990-01-01

    The injection and acceleration of thermal solar wind ions at the quasi-parallel earth's bow shock during radial interplanetary magnetic field conditions is investigated. Active Magnetospheric Particle Tracer Explorers/Ion Release Module satellite observations of complete proton spectra, and of heavy ion spectra above 10 keV/Q, made on September 12, 1984 near the nose of the shock, are presented and compared to the predictions of a Monte Carlo shock simulation which includes diffusive shock acceleration. It is found that the spectral observations are in good agreement with the predictions of the simulation when it is assumed that all accelerated ions originate in the solar wind and are injected into the acceleration mechanism by thermal leakage from the downstream plasma. The efficiency, which is determined directly from the downstream observations, is high, with at least 15 percent of the solar wind energy flux going into accelerated particles. The comparisons allow constraints to be placed on the rigidity dependence of the scattering mean free path and suggest that the upstream solar wind must be slowed substantially by backstreaming accelerated ions prior to undergoing a sharp transition in the viscous subshock.

  18. Prey fish escape by sensing the bow wave of a predator.

    Science.gov (United States)

    Stewart, William J; Nair, Arjun; Jiang, Houshuo; McHenry, Matthew J

    2014-12-15

    Prey fish possess a remarkable ability to sense and evade an attack from a larger fish. Despite the importance of these events to the biology of fishes, it remains unclear how sensory cues stimulate an effective evasive maneuver. Here, we show that larval zebrafish (Danio rerio) evade predators using an escape response that is stimulated by the water flow generated by an approaching predator. Measurements of the high-speed responses of larvae in the dark to a robotic predator suggest that larvae respond to the subtle flows in front of the predator using the lateral line system. This flow, known as the bow wave, was visualized and modeled with computational fluid dynamics. According to the predictions of the model, larvae direct their escape away from the side of their body exposed to more rapid flow. This suggests that prey fish use a flow reflex that enables predator evasion by generating a directed maneuver at high speed. These findings demonstrate a sensory-motor mechanism that underlies a behavior that is crucial to the ecology and evolution of fishes. PMID:25520384

  19. Experimental demonstration of bow-shock instability and its numerical analysis

    Science.gov (United States)

    Kikuchi, Y.; Ohnishi, N.; Ohtani, K.

    2016-07-01

    An experimental demonstration was carried out in a ballistic range at high Mach numbers with the low specific heat ratio gas hydrofluorocarbon HFC-134a to observe the unstable bow-shock wave generated in front of supersonic blunt objects. The shadowgraph images obtained from the experiments showed instability characteristics, in which the disturbances grow and flow downstream and the wake flow appears wavy because of the shock oscillation. Moreover, the influence of the body shape and specific heat ratio on the instability was investigated for various experimental conditions. Furthermore, the observed features, such as wave structure and disturbance amplitude, were captured by numerical simulations, and it was demonstrated that computational fluid dynamics could effectively simulate the physical instability. In addition, it was deduced that the shock instability is induced by sound emissions from the edge of the object. This inference supports the dependence of the instability on the specific heat ratio and Mach number because the shock stand-off distance is affected by these parameters and limits the sound wave propagation.

  20. A Novel Design of Circular Edge Bow-Tie Nano Antenna for Energy Harvesting

    Science.gov (United States)

    Haque, Ahasanul; Reza, Ahmed Wasif; Kumar, Narendra

    2015-11-01

    In this study, a novel nano antenna is designed in order to convert the high frequency solar energy, thermal energy or earth re-emitted sun's energy into electricity. The proposed antenna is gold printed on a SiO2 layer, designed as a circular edge bow-tie with a ground plane at the bottom of the substrate. The Lorentz-Drude model is used to analyze the behavior of gold at the infrared band of frequencies. The proposed antenna is designed by 3D-electromagnetic solver, and analyzed for optimization of metal thickness, gap size, and antenna's geometrical length. Simulations are conducted in order to investigate the behavior of the antenna illuminated by the circularly polarized plane wave. The numerical simulations are studied for improving the harvesting E-field of the antenna within 5 THz-40 THz frequency range. The proposed antenna offers multiple resonance frequency and better return loss within the frequency bands of 23.2 THz to 27 THz (bandwidth 3.8 THz) and 31 THz to 35.9 THz (bandwidth 4.9 THz). An output electric field of 0.656 V/µm is simulated at 25.3 THz. The best fitted gap size at the feed point is achieved as 50 nm with the substrate thickness of 1.2 µm.

  1. ANALISA PENGARUH BENTUK LAMBUNG AXE BOW PADA KAPAL HIGH SPEED CRAFT TERHADAP HAMBATAN TOTAL

    Directory of Open Access Journals (Sweden)

    Romadhoni Oni

    2015-06-01

    Full Text Available Hambatan merupakan salah satu faktor utama yang mempengaruhi proses perancangan sebuah kapal. Kapal dengan bentuk lambung yang baik akan menghasilkan hambatan yang efisiensi sehingga operasional kapal dan pergerakan kapal lebih baik. Pada ini penelitian dilakukan dengan memodelkan kapal high speed craft tipe Crew boat panjang 38 meter, lebar 7.6 meter, tinggi 3.65 meter dan draft 1.89 meter. Selanjutnya diselidiki model lambung kapal yang menghasilkan hambatan total paling kecil menggunakan pendekatan studi numerik software (maxsuft hullspeed metode savitsky dan holtrop dan software Computational Fluid Dynamics (CFD. Hasil penelitian berdasarkan analisa numerik (Maxsuft –Hullspeed dan CFD menujukkan pada kecepatan sevice bentuk lambung model AXE Bow memiliki nilai hambatan yang lebih kecil dibandingkan model kapal planing hull chine (HPC dan rounded hull (RH. Hasil perhitungan numerik dan CFD memiliki nilai yang hampir sama pada setiap variasi model. Hasil komparisi yang dilakukan didapatkan selisih total hambatan pada kecepatan 25 knot yaitu  model HPC 1.8 kN, model HPCAB 5.2 kN, model RH 4.8 kN dan model 5.1 kN. Dari perbandingan kedua metode tersebut memiliki selisih cukup kecil yaitu  kurang dari 5%. Selain mendapatkan nilai hambatan Software CFD akan menghasilkan nilai  perbandingan gaya angkat (lift force, dan total pressure yang terdistribusi  pada permukaan model setiap variasi kecepatan.

  2. Rayleigh Laser Guide Star Systems UnISIS Bow Tie Shutter and CCD39 Wavefront Camera

    CERN Document Server

    Thompson, L A; Crawford, S L; Leach, R W; Thompson, Laird A.; Teare, Scott W.; Crawford, Samuel L.; Leach, Robert W.

    2002-01-01

    Laser guide star systems based on Rayleigh scattering require some means to deal with the flash of low altitude laser light that follows immediately after each laser pulse. These systems also need a fast shutter to isolate the high altitude portion of the focused laser beam to make it appear star-like to the wavefront sensor. We describe how these tasks are accomplished with UnISIS, the Rayleigh laser guided adaptive optics system at the Mt. Wilson Observatory 2.5-m telescope. We use several methods: a 10,000 RPM rotating disk, dichroics, a fast sweep and clear mode of the CCD readout electronics on a 10 $\\mu$s timescale, and a Pockel's cell shutter system. The Pockel's cell shutter would be conventional in design if the laser light were naturally polarized, but the UnISIS 351 nm laser is unpolarized. So we have designed and put into operation a dual Pockel's cell shutter in a unique bow tie arrangement.

  3. Quantified Energy Dissipation Rates: Electromagnetic Wave Observations in the Terrestrial Bow Shock

    CERN Document Server

    Wilson, L B; Breneman, A W; Contel, O Le; Cully, C; Turner, D L; Angelopoulos, V

    2013-01-01

    We present the first quantified measure of the rate of energy dissipated per unit volume by high frequency electromagnetic waves in the transition region of the Earth's collisionless bow shock using data from the THEMIS spacecraft. Every THEMIS shock crossing examined with available wave burst data showed both low frequency ( 10 Hz) electromagnetic and electrostatic waves throughout the entire transition region and into the magnetosheath. The waves in both frequency ranges had large amplitudes, but the higher frequency waves, which are the focus of this study, showed larger contributions to both the Poynting flux and the energy dissipation rates. The higher frequency waves were identified as combinations of ion-acoustic waves, electron cyclotron drift instability driven waves, electrostatic solitary waves, and whistler mode waves. These waves were found to have: (1) amplitudes capable of exceeding dB ~ 10 nT and dE ~ 300 mV/m, though more typical values were dB ~ 0.1-1.0 nT and dE ~ 10-50 mV/m; (2) energy flu...

  4. Structure interaction due to thermal bowing of shrouds in steam generator of gas-cooled reactor

    International Nuclear Information System (INIS)

    The design of the gas-cooled reactor steam generators includes a tube bundle support plate system which restrains and supports the helical tubes in the steam generator. The support system consists of an array of radially oriented, perforated plates through which the helical tube coils are wound. These support plates have tabs on their edges which fit into vertical slots in the inner and outer shrouds. When the helical tube bundle and support plates are installed in the steam generator, they most likely cannot fit evenly between the inner and outer shrouds. This imperfection leads to different gaps between two extreme sides of the tube bundle and the shrouds. With different gaps through the tube bundle height, the helium flow experiences different cooling effects from the tube bundle. Hence, the temperature distribution in the shrouds will be non-uniform circumferentially since their surrounding helium flow temperatures are varied. These non-uniform temperatures in the shrouds result in the phenomenon of thermal bowing of shrouds

  5. In-situ wafer bowing measurements of GaN grown on Si (111) substrate by reflectivity mapping in metal organic chemical vapor deposition system

    Science.gov (United States)

    Yang, Yi-Bin; Liu, Ming-Gang; Chen, Wei-Jie; Han, Xiao-Biao; Chen, Jie; Lin, Xiu-Qi; Lin, Jia-Li; Luo, Hui; Liao, Qiang; Zang, Wen-Jie; Chen, Yin-Song; Qiu, Yun-Ling; Wu, Zhi-Sheng; Liu, Yang; Zhang, Bai-Jun

    2015-09-01

    In this work, the wafer bowing during growth can be in-situ measured by a reflectivity mapping method in the 3×2″ Thomas Swan close coupled showerhead metal organic chemical vapor deposition (MOCVD) system. The reflectivity mapping method is usually used to measure the film thickness and growth rate. The wafer bowing caused by stresses (tensile and compressive) during the epitaxial growth leads to a temperature variation at different positions on the wafer, and the lower growth temperature leads to a faster growth rate and vice versa. Therefore, the wafer bowing can be measured by analyzing the discrepancy of growth rates at different positions on the wafer. Furthermore, the wafer bowings were confirmed by the ex-situ wafer bowing measurement. High-resistivity and low-resistivity Si substrates were used for epitaxial growth. In comparison with low-resistivity Si substrate, GaN grown on high-resistivity substrate shows a larger wafer bowing caused by the highly compressive stress introduced by compositionally graded AlGaN buffer layer. This transition of wafer bowing can be clearly in-situ measured by using the reflectivity mapping method. Project supported by the National Natural Science Foundation of China (Grant Nos. 61274039 and 51177175), the National Basic Research Program of China (Grant No. 2011CB301903), the Ph.D. Programs Foundation of Ministry of Education of China (Grant No. 20110171110021), the International Science and Technology Collaboration Program of China (Grant No. 2012DFG52260), the International Science and Technology Collaboration Program of Guangdong Province, China (Grant No. 2013B051000041), the Science and Technology Plan of Guangdong Province, China (Grant No. 2013B010401013), the National High Technology Research and Development Program of China (Grant No. 2014AA032606), and the Opened Fund of the State Key Laboratory on Integrated Optoelectronics, China (Grant No. IOSKL2014KF17).

  6. Application of the improved Bow-tie risk analysis technology in civil airport safety%基于Bow-Tie技术的民用机场安全风险分析应用研究

    Institute of Scientific and Technical Information of China (English)

    孙殿阁; 孙佳; 王淼; 秦康

    2010-01-01

    民用运输机场具有运行环境复杂、事故成因复杂、驻场单位众多等特点,其事故成因更具有动态性、隐蔽性、综合性和因果连带性.因此,机场的日常运行安全风险分析一般需要借助多种工具才能完成.本文系统的介绍了一种实用的风险分析方法-Bow-tie风险技术,Bow-tie是一种风险分析和风险管理的工具,通过识别和评估风险、分析风险因素、设置风险屏障、采取风险控制和(减缓)恢复措施,有效预防事故发生.该方法可以对危害事件发生的原因、后果、屏障建立是否充足提供一个可视化的评估.本文就Bow-tie技术在民用机场安全风险中的具体实施步骤进行了描述,最后给出了其在民用机场风险分析中应用的一个实例,并就其可行性和实际应用进行了系统的研究.Bow-tie风险技术是集故障树、事件树和圆葱图理论相结合的系统风险分析及量化技术,对组织缺陷以及人为失误占主导因素的民用机场运行安全风险分析,具有较高的应用价值.

  7. 基于 Bow-tie模型的城镇输油管道风险评价方法研究%Study on risk assessment method of urban oil pipeline based on Bow-tie model

    Institute of Scientific and Technical Information of China (English)

    陈玉超; 蒋宏业; 吴瑶晗; 姚安林; 韩晓瑜

    2016-01-01

    According to the leakage and explosion accidents of urban oil pipeline frequently occurred in recent years, it was proposed to introduce Bow-tie model into risk evaluation.Through the combination of Bow-tie model with the improved ana-lytic hierarchy process method, the weights of each influence factor were obtained and sorted.Then the risk evaluation was conducted on pipeline so as to put forward reasonable safety management schemes and reduce the occurrence of accidents. The calculation results showed that the third party factor dominates in the influence factors of pipeline failure, while in the a-nalysis of accident consequence, the safety consequence and environment consequence factors have the largest influence, which basically accord with the actual situation of accident.It has certain guiding significance and practical value for the risk analysis of urban oil pipeline.%根据近年来不断发生的城镇输油管道泄漏爆炸事故,提出将Bow-tie模型引入到风险评价中,将Bow-tie模型和改进的层次分析法相结合得出各影响因素的权重并排序,对管道进行风险评价,便于提出合理的安全管理方案,减少事故的发生。通过计算得到第三方因素在管道失效影响因素中占主导,而在事故后果分析中安全后果和环境后果因素影响较大,基本符合事故实际状况,说明该方法对于城镇输油管道风险分析有一定的指导意义和实用价值。

  8. Bow-Tie分析技术在FPSO建造项目中的应用研究%Application research on Bow-Tie analysis technology in FPSO fabrication project

    Institute of Scientific and Technical Information of China (English)

    杨轶; 孙美芳; 窦林华

    2012-01-01

    @@%系统分析了海洋石油115 FPSO建造项目应用Bow-Tie分析技术,构建“蝴蝶结模型”,对建造施工作业有关的危险因素、控制措施及日常管理工作之间的联系进行研究,对各种顶上事件的起因和后果进行系统分析,此方法用于FPSO建造项目的现场安全管理非常有效.

  9. IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves

    Science.gov (United States)

    Draper, Z. H.; Matthews, B. C.; Kennedy, G. M.; Wyatt, M. C.; Venn, K. A.; Sibthorpe, B.

    2016-02-01

    Lambda Boo stars are predominately A-type stars with solar abundant C, N, O, and S, but up to 2 dex underabundances of refractory elements. The stars' unusual surface abundances could be due to a selective accretion of volatile gas over dust. It has been proposed that there is a correlation between the Lambda Boo phenomenon and IR excesses which are the result of a debris disc or interstellar medium (ISM) interaction providing the accreting material. We observe 70 or 100 and 160-μm excess emission around nine confirmed Lambda Boo stars with the Herschel Space Observatory, to differentiate whether the dust emission is from a debris disc or an ISM bow wave. We find that 3/9 stars observed host well-resolved debris discs. While the remaining 6/9 are not resolved; they are inconsistent with an ISM bow wave based on the dust emission being more compact for its temperature and predicted bow-wave models produce hotter emission than what is observed. We find the incidence of bright IR excesses around Lambda Boo stars is higher than normal A-stars. To explain this, given our observations, we explore Poynting-Robertson drag as a mechanism of accretion from a debris disc but find it insufficient. As an alternative, we propose the correlation is due to higher dynamical activity in the discs currently underway. Large impacts of planetesimals or a higher influx of comets could provide enough volatile gas for accretion. Further study on the transport of circumstellar material in relation to the abundance anomalies are required to explain the phenomenon through external accretion.

  10. Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study

    Directory of Open Access Journals (Sweden)

    K. Meziane

    2004-07-01

    Full Text Available An energetic ion (E≤40 event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at ~0.5 Re from the shock and the averaged bow shock θBn0 is about ~30°. The analysis of the three-dimensional angular distribution indicates that ions propagating roughly along the magnetic field direction are observed at the onset of the event. Later on, the angular distribution is gyrophase-bunched and the pitch-angle distribution is peaked at α0Bn0, consistent with the specular reflection production mechanism. The analysis of the waves shows that they are left-handed in the spacecraft frame of reference (right-handed in the solar wind frame and propagate roughly along the ambient magnetic field; we have found that they are in cyclotron-resonance with the field-aligned beam observed just upstream. Using properties of the waves and particles, we explain the observed particle flux-modulation in the context of θBn changes at the shock caused by the convected ULF waves. We have found that the high count rates coincide with particles leaving the shock when θBn angles are less than ~40°, consistent with the specular reflection hypothesis as the production mechanism of ions.

  11. Acceleration of solar wind ions to 1 MeV by electromagnetic structures upstream of the Earth's bow shock

    OpenAIRE

    Stasiewicz, K.; Markidis, S.; Eliasson, B.; Strumik, M.; M. Yamauchi

    2013-01-01

    We present measurements from the ESA/NASA Cluster mission that show in situ acceleration of ions to energies of 1 MeV outside the bow shock. The observed heating can be associated with the presence of electromagnetic structures with strong spatial gradients of the electric field that lead to ion gyro-phase breaking and to the onset of chaos in ion trajectories. It results in rapid, stochastic acceleration of ions in the direction perpendicular to the ambient magnetic field. The electric poten...

  12. Localized radiative energy transfer from a plasmonic bow-tie nano-antenna to a magnetic thin film stack

    OpenAIRE

    Sendur, K.; Kosar, A.; Mengüç, M. Pınar

    2011-01-01

    Localized radiative energy transfer from a near-field emitter to a magnetic thin film structure is investigated. A magnetic thin film stack is placed in the near-field of the plasmonic nano-antenna to utilize the evanescent mode coupling between the nano-antenna and magnetic thin film stack. A bow-tie nano-optical antenna is excited with a tightly focused beam of light to improve near-field radiative energy transfer from the antenna to the magnetic thin film structure. A tightly focused incid...

  13. Localized radiative energy transfer from a plasmonic bow-tie nanoantenna to a magnetic thin film stack

    OpenAIRE

    Şendur, Kürşat; Sendur, Kursat; Koşar, Ali; Kosar, Ali; Mengüç, Pınar; Menguc, Pinar

    2010-01-01

    Localized radiative energy transfer from a near-field emitter to a magnetic thin film structure is investigated. A magnetic thin film stack is placed in the near-field of the plasmonic nanoantenna to utilize the evanescent mode coupling between the nanoantenna and magnetic thin film stack. A bow-tie nano-optical antenna is excited with a tightly focused beam of light to improve near-field radiative energy transfer from the antenna to the magnetic thin film structure. A tightly focused inci...

  14. Multilayered BOW-TIE Antennas Design for RFID and Radar Applications Using a Simple Equivalent Transmission Line Model

    OpenAIRE

    Didouh, S.; Abri, M.; F. T. Bendimerad

    2012-01-01

    In this paper we propose the design of bow-tie antenna based on a simple modified transmission line model. The developed model is simple, accurate and takes into account all the antenna characteristics.The simulated antennas are designed to resonate at the frequencies 2.4 GHz and 8 GHz corresponding to RFID and Radars applications. To validate this last the obtained simulation results are compared to those obtained by the moment’s method (Agilent Momentum software). Using this transmission li...

  15. Significance of the 'bow and lean test' for the diagnosis of benign horizontal semicircular canal paroxysmal positional vertigo

    Directory of Open Access Journals (Sweden)

    Ying CHEN

    2012-10-01

    Full Text Available Objective To observe and assess the positive rate and accuracy of 'bow and lean test' in the horizontal semicircular canal benign paroxysmal positional vertigo (HSC-BPPV. Methods Ninety-two HSC-BPPV patients who were diagnosed by head roll test (HRT were enrolled, and then further tested with 'bow and lean test' (BLT between Oct 1, 2010 and Sep 30, 2011. They were treated by Barbecue maneuver or Brandt-Daroff exercise on the basis of HRT and BLT tests. The positive rate of BLT test was analyzed, and its accuracy for diagnosis and success rate for treatment of HSC-BPPV were compared between HRT and BLT. Results Among the 92 patients, 83(90.2% of them showed BLT nystagmus. Fifty-seven of 83 (68.7% patients showed both bowing nystagmus and leaning nystagmus, and 18(21.7% and 8(9.6% respectively showed bowing nystagmus alone or leaning nystagmus alone. Among 92 patients, 74(80.4% of them the affected side could be determined by HRT with 69 BLT positive and 5 BLT negative. Among the 69 BLT-positive patients, 60 patients showed the same result of HRT, and successful result was achieved by manipulation. 9 patients showed different result between BLT and HRT, in whom manipulation failed according to the result of HRT, but succeeded when manipulation was performed according to BLT. In 18 patients(19.6% it was not able to determine the affected side by HRT, but in 14 patients manipulation was successful when BLT result was applied. In 4 patients BLT failed to evoke nystagmus, but after practicing Brandt-Daroff exercise, vertigo and HRT nystagmus disappeared 3 days later. Among the 92 patients, 65(70.7% were cured according to HRT, while 83(90.2% got successful result according to BLT(P < 0.05. Conclusion The positive rate and accuracy for HSC-BPPV by BLT are high. It is a useful method for determining the affected side in HSC-BPPV, and to provide the basis for selecting effective manipulation treatment.

  16. Compositional bowing of band energies and their deformation potentials in strained InGaAs ternary alloys: A first-principles study

    International Nuclear Information System (INIS)

    Using first-principles calculations, we show that the conduction and valence band energies and their deformation potentials exhibit a non-negligible compositional bowing in strained ternary semiconductor alloys such as InGaAs. The electronic structure of these compounds has been calculated within the framework of local density approximation and hybrid functional approach for large cubic supercells and special quasi-random structures, which represent two kinds of model structures for random alloys. We find that the predicted bowing effect for the band energy deformation potentials is rather insensitive to the choice of the functional and alloy structural model. The direction of bowing is determined by In cations that give a stronger contribution to the formation of the InxGa1−xAs valence band states with x ≳ 0.5, compared to Ga cations

  17. Compositional bowing of band energies and their deformation potentials in strained InGaAs ternary alloys: A first-principles study

    Energy Technology Data Exchange (ETDEWEB)

    Khomyakov, Petr A.; Luisier, Mathieu; Schenk, Andreas [Integrated Systems Laboratory, Department of Information Technology and Electrical Engineering, ETH Zurich, Gloriastrasse 35, 8092 Zurich (Switzerland)

    2015-08-10

    Using first-principles calculations, we show that the conduction and valence band energies and their deformation potentials exhibit a non-negligible compositional bowing in strained ternary semiconductor alloys such as InGaAs. The electronic structure of these compounds has been calculated within the framework of local density approximation and hybrid functional approach for large cubic supercells and special quasi-random structures, which represent two kinds of model structures for random alloys. We find that the predicted bowing effect for the band energy deformation potentials is rather insensitive to the choice of the functional and alloy structural model. The direction of bowing is determined by In cations that give a stronger contribution to the formation of the In{sub x}Ga{sub 1−x}As valence band states with x ≳ 0.5, compared to Ga cations.

  18. Three-dimensional position and shape of the bow shock and their variation with Alfvenic, sonic and magnetosonic Mach numbers and interplanetary magnetic field orientation

    Science.gov (United States)

    Peredo, M.; Slavin, J. A.; Mazur, E.; Curtis, S. A.

    1995-01-01

    A large set of bow shock crossings (i.e., 1392) observed by 17 spacecraft has been used to explore the three-dimensional shape and location of the Earth's bow shock and its dependence on solar wind and interplanetary magnetic field (IMF) conditions. This study investigates deviations from gas dynamic flow models associated with the magnetic terms in the magnetohydrodynamic (MHD) equations. Empirical models predicting the statistical position and shape of the bow shock for arbitrary values of the solar wind pressure, IMF, and Alfvenic Mach number (M(sub A)) have been derived. The resulting data set has been used to fit three-dimensional bow shock surfaces and to explore the variations in these surfaces with sonic (M(sub S)), Alfvenic (M(sub A)) and magnetosonic (M(sub MS)) Mach numbers. Analysis reveals that among the three Mach numbers, M(sub A) provides the best ordering of the least square bow shock curves. The subsolar shock is observed to move Earthward while the flanks flare outward in response to decreasing M(sub A); the net change represents a 6-10% effect. Variations due to changes in the IMF orientation were investigated by rotating the crossings into geocentric interplanetary medium coordinates. Past studies have suggested that the north-south extent of the bow shock surface exceeds the east-west dimension due to asymmetries in the fast mode Mach cone. This study confirms such a north-south versus east-west asymmetry and quantifies its variation with M(sub S), M(sub A), M(sub MS), and IMF orientation. A 2-7% effect is measured, with the asymmetry being more pronounced at low Mach numbers. Combining the bow shock models with the magnetopause model of Roelof and Sibeck (1993), variations in the magnetosheath thickness at different local times are explored. The ratio of the bow shock size to the magnetopause size at the subpolar point is found to be 1.46; at dawn and dusk, the ratios are found to be 1.89 and 1.93, respectively. The subsolar magnetosheath

  19. Occurrence of high-beta superthermal plasma events in the close environment of Jupiter's bow shock as observed by Ulysses

    International Nuclear Information System (INIS)

    The ratio of the plasma pressure to the magnetic field pressure (or of their energy densities) which is known as the plasma parameter 'beta'(β) has important implications to the propagation of energetic particles and the interaction of the solar wind with planetary magnetospheres. Although in the scientific literature the contribution of the superthermal particles to the plasma pressure is generally assumed negligible, we deduced, by analyzing energetic particles and magnetic field measurements recorded by the Ulysses spacecraft, that in a series of events, the energy density contained in the superthermal tail of the particle distribution is comparable to or even higher than the energy density of the magnetic field, creating conditions of high-beta plasma. More explicitly, in this paper we analyze Ulysses/HI-SCALE measurements of the energy density ratio (parameter βep) of the energetic ions'(20 keV to ∼5 MeV) to the magnetic field's in order to find occurrences of high-beta (βep>1) superthermal plasma conditions in the environment of the Jovian magnetosphere, which is an interesting plasma laboratory and an important source of emissions in our solar system. In particular, we examine high-beta ion events close to Jupiter's bow shock, which are produced by two processes: (a) bow shock ion acceleration and (b) ion leakage from the magnetosphere.

  20. Large Scale Earth's Bow Shock with Northern IMF as simulated by PIC code in parallel with MHD model

    CERN Document Server

    Baraka, Suleiman M

    2016-01-01

    In this paper, we propose a 3D kinetic model (Particle-in-Cell PIC ) for the description of the large scale Earth's bow shock. The proposed version is stable and does not require huge or extensive computer resources. Because PIC simulations work with scaled plasma and field parameters, we also propose to validate our code by comparing its results with the available MHD simulations under same scaled Solar wind ( SW ) and ( IMF ) conditions. We report new results from the two models. In both codes the Earth's bow shock position is found to be ~14.8 RE along the Sun-Earth line, and ~ 29 RE on the dusk side. Those findings are consistent with past in situ observations. Both simulations reproduce the theoretical jump conditions at the shock. However, the PIC code density and temperature distributions are inflated and slightly shifted sunward when compared to the MHD results. Kinetic electron motions and reflected ions upstream may cause this sunward shift. Species distributions in the foreshock region are depicted...

  1. Network, degeneracy and bow tie integrating paradigms and architectures to grasp the complexity of the immune system

    Directory of Open Access Journals (Sweden)

    Tieri Paolo

    2010-08-01

    Full Text Available Abstract Recently, the network paradigm, an application of graph theory to biology, has proven to be a powerful approach to gaining insights into biological complexity, and has catalyzed the advancement of systems biology. In this perspective and focusing on the immune system, we propose here a more comprehensive view to go beyond the concept of network. We start from the concept of degeneracy, one of the most prominent characteristic of biological complexity, defined as the ability of structurally different elements to perform the same function, and we show that degeneracy is highly intertwined with another recently-proposed organizational principle, i.e. 'bow tie architecture'. The simultaneous consideration of concepts such as degeneracy, bow tie architecture and network results in a powerful new interpretative tool that takes into account the constructive role of noise (stochastic fluctuations and is able to grasp the major characteristics of biological complexity, i.e. the capacity to turn an apparently chaotic and highly dynamic set of signals into functional information.

  2. Flux-based classification of reactions reveals a functional bow-tie organization of complex metabolic networks.

    Science.gov (United States)

    Singh, Shalini; Samal, Areejit; Giri, Varun; Krishna, Sandeep; Raghuram, Nandula; Jain, Sanjay

    2013-05-01

    Unraveling the structure of complex biological networks and relating it to their functional role is an important task in systems biology. Here we attempt to characterize the functional organization of the large-scale metabolic networks of three microorganisms. We apply flux balance analysis to study the optimal growth states of these organisms in different environments. By investigating the differential usage of reactions across flux patterns for different environments, we observe a striking bimodal distribution in the activity of reactions. Motivated by this, we propose a simple algorithm to decompose the metabolic network into three subnetworks. It turns out that our reaction classifier, which is blind to the biochemical role of pathways, leads to three functionally relevant subnetworks that correspond to input, output, and intermediate parts of the metabolic network with distinct structural characteristics. Our decomposition method unveils a functional bow-tie organization of metabolic networks that is different from the bow-tie structure determined by graph-theoretic methods that do not incorporate functionality. PMID:23767567

  3. [Comparative analysis of edentulous patients treated traditionally and with the use of a face-bow and Quick Master articulator].

    Science.gov (United States)

    Kubrak, J

    1998-01-01

    Correct determination of the occlusal plane is one of the most difficult stages of treatment. After determining the correct occlusal plane its reproduction is possible thanks to the use of articulators. These instruments simulate movements of the jaw in three planes. One of the most optimal articulators is a semi-adjustable type. These instruments are not complicated and give good treatment results. A modern semiadjustable type of articulator is Quick Master. The face-bow which comes together with this instrument is used for recording and transferring the occlusal relation to the articulator. This allows to mount models in an adequate three dimensional position in relation to the temporo-mandibular joint. The use of these instruments leads to many questions and doubts due to difficulties in their use. Therefore the aim of my study was to elaborate a simple method of occlusal recording. I have also compared the treatment results of edentulous patients treated with the use of an articulator and the use of a traditional method. Prosthetic restorations were prepared among 60 patients. The study material was divided into two groups of 30 patients each. In the control group for preparing complete dentures the Gysi method was employed as the most common. In the study group a face-bow and articulator were used. After preparing complete dentures detailed clinical control examinations were carried out and were repeated 24-48 hours after fitting the dentures and also after 3 and 6 months of their use. Working with the face-bow I have employed my own modification of recording the occlusion. The upper wax rim was placed on a slightly warmed bite fork and drawing pins were placed in the recording block to act as a type of key. The lower rim was warmed and brought to occlusal contact a couple of times. Next the face-bow was inserted. The recorded occlusion was transferred and mounted in the articulator. Teeth in both cases were set up similarly to the Gysi method. Lower teeth

  4. The jumps of physical quantities at fast shocks under pressure anisotropy: theory versus observations at the bow shock

    International Nuclear Information System (INIS)

    The interaction of the solar wind with magnetized planets leads to the formation of the so-called magnetosphere, a cavity generated by the geomagnetic field. The supersonic, superalfvenic, and magnetized solar wind flow interacting with blunt bodies produces a detached bow shock, separating the solar wind from the magnetosheath, the region between the shock wave and the magnetopause. On approach to a planetary obstacle, the solar wind becomes subsonic at the bow shock and then flows past the planet in the magnetosheath. At the bow shock, the plasma parameters and the magnetic field strength change from upstream to downstream, i.e., an increase of plasma density, temperature, pressure, and magnetic field strength, and a decrease of the velocity across the shock. In this PhD thesis we mainly concentrate on the variations of all physical quantities across the bow shock taking into account pressure anisotropy, which is an important feature in space plasma physics and observed by various spacecraft missions in the solar wind as well as in the magnetosheath. Dealing with anisotropic plasma conditions, one has to introduce the so-called pressure tensor, characterized by two scalar pressures, the pressure perpendicular (Pperp) and the pressure parallel (Pparallel) with respect to the magnetic field and in general one speaks of anisotropic conditions for Pperp is not Pparallel. Many spacecraft observations of the solar wind show Pparallel > Pperp, whereas observations of the magnetosheath show the opposite case, Pparallel perp. Therefore, dissipation of kinetic energy into thermal energy plays an important role in studying the variations of the relevant physical quantities across the shock. It has to be mentioned that planetary bow shocks are good examples for fast MHD shock waves. Therefore, the basic equations for describing the changes across the shock can be obtained by integrating the MHD equations in conservative form. We note that these equations, the so

  5. 基于Bow-Tie模型的航空事故分析及适航条款生成方法%Analysing Aviation Accident and Generating Airworthiness Provisions using Bow-Tie Model

    Institute of Scientific and Technical Information of China (English)

    崔利杰; 任恒; 李泽

    2015-01-01

    随着航空器需求量的不断增加,人们对航空器安全性水平提出了更高的要求.适航法规作为保证航空器安全性水平的重要依据,其主要来源于航空飞行事故.通过运用Bow-Tie方法模型对民用航空事故进行深入细致分析,找出事故危险源以及相关影响因素,基于分析结果,运用风险管理的理念,提出一种适航条款生成的思路.

  6. 屏蔽罩高度对bow-tie天线性能影响的分析%Numerical and Experimental Analysis of Bow-tie Antennas With Changing of Shield's Height

    Institute of Scientific and Technical Information of China (English)

    周凯; 张文吉; 张晓娟

    2008-01-01

    本文研究了一种终端加载的bow-tie天线,计算所加载的电阻值,并改变其屏蔽罩高度,对其辐射特性和驻波比(VSWR),用软件进行了仿真分析,同时进行了实际测试,并将仿真和实验结果进行了对比.结果表明,仿真和实验的结果基本吻合,为今后进一步的研究工作打下了一定的基础.

  7. AE AURIGAE: FIRST DETECTION OF NON-THERMAL X-RAY EMISSION FROM A BOW SHOCK PRODUCED BY A RUNAWAY STAR

    Energy Technology Data Exchange (ETDEWEB)

    Lopez-Santiago, J.; Pereira, V.; De Castro, E. [Dpto. de Astrofisica y CC. de la Atmosfera, Universidad Complutense de Madrid, E-28040 Madrid (Spain); Miceli, M.; Bonito, R. [Dipartimento di Fisica, Universita di Palermo, Piazza del Parlamento 1, I-90134 Palermo (Italy); Del Valle, M. V.; Romero, G. E. [Instituto Argentino de Radioastronomia (IAR), CCT La Plata (CONICET), C.C.5, 1894 Villa Elisa, Buenos Aires (Argentina); Albacete-Colombo, J. F. [Centro Universitario Regional Zona Atlantica (CURZA), Universidad Nacional del COMAHUE, Monsenor Esandi y Ayacucho, 8500 Viedma, Rio Negro (Argentina); Damiani, F. [INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, I-90134 Palermo (Italy)

    2012-09-20

    Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the production of high-energy photons by non-thermal radiative processes in a number sufficiently large to be detected in X-rays. To date, no stellar bow shock has been detected at such energies. We present the first detection of X-ray emission from a bow shock produced by a runaway star. The star is AE Aur, which was likely expelled from its birthplace due to the encounter of two massive binary systems and now is passing through the dense nebula IC 405. The X-ray emission from the bow shock is detected at 30'' northeast of the star, coinciding with an enhancement in the density of the nebula. From the analysis of the observed X-ray spectrum of the source and our theoretical emission model, we confirm that the X-ray emission is produced mainly by inverse Compton upscattering of infrared photons from dust in the shock front.

  8. Laser resonators with several mirrors and lenses with the bow-tie laser resonator with compensation for astigmatism and thermal lens enects as an example

    DEFF Research Database (Denmark)

    Abitan, Haim; Skettrup, Torben

    2005-01-01

    Laser resonators with several mirrors (lenses) have been investigated in a systematic fashion. They have been grouped into classes according to their number n of mirrors/lenses. Stability polynomials, beam waist radii and locations have been obtained for each group up to n = 4. The bow-tie laser...

  9. 斧艏船加附体改善耐波性的研究%Research on Sea Keeping Performance of an AXE Bow Ship with Appendages

    Institute of Scientific and Technical Information of China (English)

    施军; 曾青; 武庆威; 高霄鹏; 董祖舜

    2015-01-01

    斧艏船型是一种适用于高速排水船的性能优良船型。无论与高速圆舭型船还是常规深 V 型船相比,它在阻力和耐波性能上均有其优势。研究发现,斧艏船在阻力及耐波性方面仍有进一步改善的余地。为此作者对斧艏船进行了加附体的试验研究。通过加防溅条、尾分水踵、尾压浪板、球鼻艏及首部水翼等手段,使斧艏船的阻力和耐波性有了进一步的改善。研究表明,对于不同的航速范围,可以采用不同的附体组合,以达到较理想的效果。%The hull form with AXE bow has good performance for high speed displacement ships. Both performances of resistance and sea keeping are superior to the round bilge or deep-V hull. A series of model tests of a hull with AXE bow, with various appendages added including spray strip, transom plate, skeg, bow-bulb, bow-bulb with fin and hydrofoil, has been carried out. It is indicated that the appendages can improve the performance of the ship with AXE bow, and different composition of appendages should be adopted for various speed ranges.

  10. Composition and energy spectra of low energy ions observed upstream of the earth's bow shock on ISEE-1

    Science.gov (United States)

    Ipavich, F. M.; Galvin, A. B.; Gloeckler, G.; Hovestadt, D.; Klecker, B.; Scholer, M.; Fan, C. Y.; Fisk, L. A.; Ogallagher, J. J.

    1980-01-01

    The characteristics of eleven locally accelerated particle events in the energy range from 30 to 125 keV/Q observed upstream of the earth's bow shock have been determined, including composition, energy spectra, and intensity versus time profiles. The measurements were made with the Ultra Low Energy Charge Analyzer sensor on ISEE-1. The composition in these events is similar to that of the solar wind, with a He to proton ratio of 8% and a CNO to He ratio of 6%. The composition is reasonably constant only when evaluated at equal energy per charge. The energy spectra cannot be adequately fit by a single power law in energy; an exponential or Maxwellian in energy per charge gives a satisfactory representation of the spectra. The time-intensity profiles of these upstream events show an inverse velocity dispersion, which may provide clues to the responsible acceleration mechanism.

  11. Evidence for a dynamically refracted primary bow in weakly bound $^9$Be rainbow scattering from $^{16}$O

    CERN Document Server

    Ohkubo, S

    2016-01-01

    We present for the first time evidence for the existence of a dynamically refracted primary bow for $^{9}$Be+$^{16}$O scattering. This is demonstrated through the use of coupled channel calculations with an extended double folding potential derived from the density-dependent effective two-body force and precise microscopic cluster wave functions for $^{9}$Be. The calculations reproduce the experimental Airy structure in $^{9}$Be+$^{16}$O scattering well.It is found that coupling of a weakly bound $^{9}$Be nucleus to excited states plays the role of a booster lens, dynamically enhancing the refraction over the {\\it static} refraction due to the Luneburg lens mean field potential between the ground states of $^{9}$Be and $^{16}$O.

  12. Feasibility evaluation of x-ray imaging for measurement of fuel rod bowing in CFTL test bundles

    International Nuclear Information System (INIS)

    The Core Flow Test Loop (CFTL) is a high temperature, high pressure, out-of-reactor helium-circulating system. It is designed for detailed study of the thermomechanical performance, at prototypic steady-state and transient operating conditions, of electrically heated rods that simulate segments of core assemblies in the Gas-Cooled Fast Breeder reactor demonstration plant. Results are presented of a feasibility evaluation of x-ray imaging for making measurements of the displacement (bowing) of fuel rods in CFTL test bundles containing electrically heated rods. A mock-up of a representative CFTL test section consisting of a test bundle and associated piping was fabricated to assist in this evaluation

  13. Oxidation of graphene ‘bow tie’ nanofuses for permanent, write-once-read-many data storage devices

    International Nuclear Information System (INIS)

    We have fabricated nanoscale fuses from CVD graphene sheets with a ‘bow tie’ geometry for write-once-read-many data storage applications. The fuses are programmed using thermal oxidation driven by Joule heating. Fuses that were 250 nm wide with 2.5 μm between contact pads were programmed with average voltages and powers of 4.9 V and 2.1 mW, respectively. The required voltages and powers decrease with decreasing fuse sizes. Graphene shows extreme chemical and electronic stability; fuses require temperatures of about 400 °C for oxidation, indicating that they are excellent candidates for permanent data storage. To further demonstrate this stability, fuses were subjected to applied biases in excess of typical read voltages; stable currents were observed when a voltage of 10 V was applied to the devices in the off state and 1 V in the on state for 90 h each. (paper)

  14. Multilayered BOW-TIE Antennas Design for RFID and Radar Applications Using a Simple Equivalent Transmission Line Model

    Directory of Open Access Journals (Sweden)

    S. Didouh

    2012-06-01

    Full Text Available In this paper we propose the design of bow-tie antenna based on a simple modified transmission line model. The developed model is simple, accurate and takes into account all the antenna characteristics.The simulated antennas are designed to resonate at the frequencies 2.4 GHz and 8 GHz corresponding to RFID and Radars applications. To validate this last the obtained simulation results are compared to those obtained by the moment’s method (Agilent Momentum software. Using this transmission line approach the resonant frequency, input impedance, return loss can be determined simultaneously. The paper reports several simulation results that confirm the validity of the developed model. The obtained results are then presented and discussed.

  15. THE CHESS SURVEY OF THE L1157-B1 SHOCK REGION: CO SPECTRAL SIGNATURES OF JET-DRIVEN BOW SHOCKS

    International Nuclear Information System (INIS)

    The unprecedented sensitivity of Herschel coupled with the high resolution of the HIFI spectrometer permits studies of the intensity-velocity relationship I(v) in molecular outflows, over a higher excitation range than possible up to now. Over the course of the CHESS Key Program, we have observed toward the bright bow shock region L1157-B1, the CO rotational transitions between J = 5-4 and J = 16-15 with HIFI, and the J = 1-0, 2-1, and 3-2 with the IRAM 30 m and the Caltech Submillimeter Observatory telescopes. We find that all the line profiles ICO(v) are well fit by a linear combination of three exponential laws ∝exp (– |v/v0|) with v0 = 12.5, 4.4, and 2.5 km s–1. The first component dominates the CO emission at J ≥ 13, as well as the high-excitation lines of SiO and H2O. The second component dominates for 3 ≤ Jup ≤ 10 and the third one for Jup ≤ 2. We show that these exponentials are the signature of quasi-isothermal shocked gas components: the impact of the jet against the L1157-B1 bow shock (Tk ≅ 210 K), the walls of the outflow cavity associated with B1 (Tk ≅ 64 K), and the older cavity L1157-B2 (Tk ≅ 23 K), respectively. Analysis of the CO line flux in the large-velocity gradient approximation further shows that the emission arises from dense gas (n(H2) ≥ 105-106 cm–3) close to LTE up to J = 20. We find that the CO J = 2-1 intensity-velocity relation observed in various other molecular outflows is satisfactorily fit by similar exponential laws, which may hold an important clue to their entrainment process.

  16. Large Scale Earth’s Bow Shock with Northern IMF as Simulated by PIC Code in Parallel with MHD Model

    Indian Academy of Sciences (India)

    Suleiman Baraka

    2016-06-01

    In this paper, we propose a 3D kinetic model (particle-in-cell,PIC) for the description of the large scale Earth’s bow shock. Theproposed version is stable and does not require huge or extensive computerresources. Because PIC simulations work with scaled plasma andfield parameters, we also propose to validate our code by comparing itsresults with the available MHD simulations under same scaled solar wind(SW) and (IMF) conditions. We report new results from the two models.In both codes the Earth’s bow shock position is found to be $\\approx 14.8 R_{E} $along the Sun–Earth line, and $\\approx 29 R_{E} $ on the dusk side. Those findingsare consistent with past in \\textit{situ} observations. Both simulations reproducethe theoretical jump conditions at the shock. However, the PIC codedensity and temperature distributions are inflated and slightly shifted sunwardwhen compared to the MHD results. Kinetic electron motions andreflected ions upstream may cause this sunward shift. Species distributionsin the foreshock region are depicted within the transition of theshock (measured $ \\approx $ 2 $ c/\\omega_{pi} $ for $ \\Theta_{Bn}=90^{o}$ and $M_{MS}=4.7 $) and in thedownstream. The size of the foot jump in the magnetic field at the shock ismeasured to be ($1.7 c/ \\omega_{pi} $). In the foreshocked region, the thermal velocityis found equal to 213 km s^{−1} at 15R_{E} and is equal to 63 km s^{-1} at12 R_{E} (magnetosheath region). Despite the large cell size of the currentversion of the PIC code, it is powerful to retain macrostructure of planetsmagnetospheres in very short time, thus it can be used for pedagogicaltest purposes. It is also likely complementary with MHD to deepen ourunderstanding of the large scale magnetosphere.

  17. Large Scale Earth's Bow Shock with Northern IMF as Simulated by PIC Code in Parallel with MHD Model

    Science.gov (United States)

    Baraka, Suleiman

    2016-06-01

    In this paper, we propose a 3D kinetic model (particle-in-cell, PIC) for the description of the large scale Earth's bow shock. The proposed version is stable and does not require huge or extensive computer resources. Because PIC simulations work with scaled plasma and field parameters, we also propose to validate our code by comparing its results with the available MHD simulations under same scaled solar wind (SW) and (IMF) conditions. We report new results from the two models. In both codes the Earth's bow shock position is found to be ≈14.8 R E along the Sun-Earth line, and ≈29 R E on the dusk side. Those findings are consistent with past in situ observations. Both simulations reproduce the theoretical jump conditions at the shock. However, the PIC code density and temperature distributions are inflated and slightly shifted sunward when compared to the MHD results. Kinetic electron motions and reflected ions upstream may cause this sunward shift. Species distributions in the foreshock region are depicted within the transition of the shock (measured ≈2 c/ ω pi for Θ Bn = 90° and M MS = 4.7) and in the downstream. The size of the foot jump in the magnetic field at the shock is measured to be (1.7 c/ ω pi ). In the foreshocked region, the thermal velocity is found equal to 213 km s-1 at 15 R E and is equal to 63 km s -1 at 12 R E (magnetosheath region). Despite the large cell size of the current version of the PIC code, it is powerful to retain macrostructure of planets magnetospheres in very short time, thus it can be used for pedagogical test purposes. It is also likely complementary with MHD to deepen our understanding of the large scale magnetosphere.

  18. Venusian ion populations and bow shock as seen by the ASPERA-4 ion instrument on Venus Express

    Science.gov (United States)

    Grande, M.; Whittaker, I.; Guymer, G.; Barabash, S.

    2008-09-01

    Introduction We examine ion populations at Venus. Previous models use magnetic crossing points to derive the bow shock position. The current work uses data from the ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) [1] instrument to measure ion populations and derive a bow shock position at Venus. Instrumentation The ASPERA-4 instrument flies onboard Venus Express (VEX) and is comprised of five different detectors (Barabash et al 2006 [1]). A neutral particle detector and analyser, an electron spectrometer and the Ion Mass Analyser (IMA) (ref). This paper uses the IMA instrument for all its data and an explanation of the specifications is required. The instrument is a top hat electrostatic analyser; it runs through voltages to scan look angles and also acceptance energies. In one look direction it scans through 96 different energy values before changing to the next. A full scan of all look directions and energies takes 192 seconds. Data Collection All data is weighed dependant upon its probability of the spacecraft measuring at a particular point and when fitted produces a value of 1.24 RV, somewhat closer distance for the sub solar point than previous authors - see figure 1. We separate the data according to slow or fast solar wind and not the similarities and differences in the results derived. The inbound and outbound bow shock crossings were taken by inspection of 106 orbits between November 2006 and February 2007. Any orbits where the crossing point was not clear or with data missing were ignored. The occupational probability is found from orbital mechanics. By setting up a grid and deriving the amount of time it takes to cross each square the probability as a whole can then be determined. Ion distribution plots Two dimensional maps of the ions are produced and the bow shock model overplotted to verify its accuracy, as shown in figure 3. The test of the bow shock is to place it upon real data and examine the fit. To do this ion distribution plots are

  19. Estimation of the Effect of Green Water and Bow Flare Slamming on the Wave-Induced Vertical Bending Moment Using Closed-Form Ex-pressions

    DEFF Research Database (Denmark)

    Jensen, Jørgen Juncher; Mansour, A. E.

    2003-01-01

    rate. These loads can be due to bow flare slamming, bottom slamming or green water loads as they all can be characterised by a short duration relative to the wave cycle. The magnitude of the bow flare slamming loads is estimated using accurate results from wedge-shaped sections, Zhao and Faltinsen...... (1993) and for green water loads the results from Buchner (1995) and Wang et al .(1998) are applied. The phase lag relative to the wave-induced peak and the decay rate are derived mainly from published experimental results, Sikora, (1998). The results are given in closed-form expressions and the......ABSTRACT: The effect of impulsive loads like slamming and green water on deck on the wave-induced bending mo-ment is estimated by a semi-analytical approach. The impulse loads leading to transient vibrations are described in terms of magnitude, phase lag relative to the wave-induced peak and decay...

  20. Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary

    Directory of Open Access Journals (Sweden)

    R. Modolo

    2006-12-01

    Full Text Available The solar wind plasma interaction with the Martian exosphere is investigated by means of 3-D multi-species hybrid simulations. The influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary is examined by comparing two simulations describing the two extreme states of the solar cycle. The hybrid formalism allows a kinetic description of each ions species and a fluid description of electrons. The ionization processes (photoionization, electron impact and charge exchange are included self-consistently in the model where the production rate is computed locally, separately for each ionization act and for each neutral species. The results of simulations are in a reasonable agreement with the observations made by Phobos 2 and Mars Global Surveyor spacecraft. The position of the bow shock and the magnetic pile-up boundary is weakly dependent of the solar EUV flux. The motional electric field creates strong asymmetries for the two plasma boundaries.

  1. First measurements with a new 6m long violin-bow marine heat probe off Costa Rica

    Science.gov (United States)

    Gennerich, H.-H.; Grevemeyer, I.; Heesemann, B.; Heesemann, M.; Kaul, N.; Müller, M.; Villinger, H.

    2003-04-01

    The design of a new 6m long violin-bow marine heat probe, first successful tests and data collected off Costa Rica during cruise M54-2 on RV METEOR in August 2002 are presented. The mechanically robust heat probe is designed for the operation in a pogo-style mode with a wide application range from 6000m deep sea trenches with mostly soft sediments to the upper continental slope where sediments are often sandy and difficult to penetrate. Due to the 6m length of its temperature sensor string undisturbed temperature gradients can be determined in shallow water with seasonal bottom water temperature variations. The heat probe is constructed in the classical "violin bow" design, with 22 thermistors equidistantly distributed inside an oil filled hydraulic tube attached to the strength member. The sensor tube also contains a heater wire for the generation of a calibrated heat pulse for in situ thermal conductivity measurements. The signal of the temperature sensors is measured with a resolution of 20-bits at a sample rate of 1 sec, resulting in a final temperature resolution of less than 1 mK at ambient sea floor temperatures. A carefully calibrated seawater sensor on top of the weight stand allows to measure the absolute bottom water temperature. Inclination and acceleration of the probe is measured also with a 1 sec sample rate to monitor the penetration process into the sediments and potential disturbances during the measurement period while the probe sits in the sediment. Data from a pressure sensor in conjunction with an acoustic altimeter allow the exact absolute measurement of the final penetration depth of the probe. The complete data set is stored in the probe but also transmitted via coax cable on board in real time which allows operational decisions during long term deployments of the probe. In addition the heat probe can be operated in a completely autonomous mode with internal storage and automated heat pulses. The battery capacity allows for 3 days

  2. Possible Impact of climate change on future extreme precipitation of the Oldman, Bow and Red Deer River Basins of Alberta

    Science.gov (United States)

    Yew Gan, Thian; Gizaw, Mesgana

    2016-04-01

    The impact of climate change on extreme precipitation events in the Oldman (ORB), Bow, (BRB) and Red Deer (RRB) River Basins of southern Alberta, Canada, was assessed using six extreme climate indices for the rainy period of May-August (MJJA), and 9-km resolution Special Report on Emission Scenarios (SRES) A2 and A1B climate scenarios of four Coupled Model Intercomparison Project Phase 3 (CMIP3) Global Climate Models (GCMs) dynamically downscaled by a regional climate model, MM5. R95p of the three study sites showed an increase of 4% for the 2050s (2041-2070) and 10% for the 2080s (2071-2100) period, whereas R99p increased by 39% (2050s) and 42% (2080s) which suggest a projected increase in the volume of precipitation expected in future very wet and particularly extremely wet days. Similarly, R20mm, P30yr, RX1day and RX5day are also projected to increase by about 15% by the mid- and late 21st century in the three study sites. However, compared to BRB and RRB, ORB located in the southernmost part of the study site is projected to undergo a relatively higher increase in both temperature and precipitation intensity, which is assessed in terms of indices such as P30yr, RX1day and RX5day. On the other hand, RRB and BRB are projected to experience higher increase in R20mm, which suggest a relatively higher increase in the number of very heavy precipitation days projected for these two basins. Overall, these results suggest that in the 2050s and 2080s, southern Alberta will be expected to experience more frequent and severe intensive storm events in the MJJA season that could potentially increase the risk of future flooding in this region. Ref: Gizaw, M., and Gan, T. Y., 2015, Possible Impact of climate change on future extreme precipitation of the Oldman, Bow and Red Deer River Basins of Alberta, Int. Journal Climatology, DOI:10.1002/joc.4338

  3. THE CHESS SURVEY OF THE L1157-B1 SHOCK REGION: CO SPECTRAL SIGNATURES OF JET-DRIVEN BOW SHOCKS

    Energy Technology Data Exchange (ETDEWEB)

    Lefloch, B.; Codella, C.; Ceccarelli, C. [UJF-Grenoble 1/CNRS-INSU, Institut de Planetologie et dAstrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041 (France); Cabrit, S. [Observatoire de Paris, LERMA, UMR 8112 du CNRS, ENS, UPMC, UCP, 61 Av. de l' Observatoire, F-75014 Paris (France); Busquet, G.; Benedettini, M. [INAF, Istituto di Astrofisica e Planetologia Spaziali, Via Fosso del Cavaliere 100, I-00133 Roma (Italy); Cernicharo, J.; Pardo, J. R. [Centro de Astrobiologia, INTA, Ctra de Torrejon a Ajalvir, km 4, E-28850 Torrejon de Ardoz, E-28850 Madrid (Spain); Lis, D. C. [California Institute of Technology, Cahill Center for Astronomy and Astrophysics 301-17, Pasadena, CA 91125 (United States); Nisini, B., E-mail: lefloch@obs.ujf-grenoble.fr [INAF, Osservatorio Astronomico di Roma, Via di Frascati 33, I-00040 Monte, Porzio Catone (Italy)

    2012-10-01

    The unprecedented sensitivity of Herschel coupled with the high resolution of the HIFI spectrometer permits studies of the intensity-velocity relationship I(v) in molecular outflows, over a higher excitation range than possible up to now. Over the course of the CHESS Key Program, we have observed toward the bright bow shock region L1157-B1, the CO rotational transitions between J = 5-4 and J = 16-15 with HIFI, and the J = 1-0, 2-1, and 3-2 with the IRAM 30 m and the Caltech Submillimeter Observatory telescopes. We find that all the line profiles I{sub CO}(v) are well fit by a linear combination of three exponential laws {proportional_to}exp (- |v/v{sub 0}|) with v{sub 0} = 12.5, 4.4, and 2.5 km s{sup -1}. The first component dominates the CO emission at J {>=} 13, as well as the high-excitation lines of SiO and H{sub 2}O. The second component dominates for 3 {<=} J{sub up} {<=} 10 and the third one for J{sub up} {<=} 2. We show that these exponentials are the signature of quasi-isothermal shocked gas components: the impact of the jet against the L1157-B1 bow shock (T{sub k} {approx_equal} 210 K), the walls of the outflow cavity associated with B1 (T{sub k} {approx_equal} 64 K), and the older cavity L1157-B2 (T{sub k} {approx_equal} 23 K), respectively. Analysis of the CO line flux in the large-velocity gradient approximation further shows that the emission arises from dense gas (n(H{sub 2}) {>=} 10{sup 5}-10{sup 6} cm{sup -3}) close to LTE up to J = 20. We find that the CO J = 2-1 intensity-velocity relation observed in various other molecular outflows is satisfactorily fit by similar exponential laws, which may hold an important clue to their entrainment process.

  4. Experimental validation of a method characterizing bow tie filters in CT scanners using a real-time dose probe

    International Nuclear Information System (INIS)

    Purpose: Beam-shaping or ''bow tie'' (BT) filters are used to spatially modulate the x-ray beam in a CT scanner, but the conventional method of step-and-shoot measurement to characterize a beam's profile is tedious and time-consuming. The theory for characterization of bow tie relative attenuation (COBRA) method, which relies on a real-time dosimeter to address the issues of conventional measurement techniques, was previously demonstrated using computer simulations. In this study, the feasibility of the COBRA theory is further validated experimentally through the employment of a prototype real-time radiation meter and a known BT filter. Methods: The COBRA method consisted of four basic steps: (1) The probe was placed at the edge of a scanner's field of view; (2) a real-time signal train was collected as the scanner's gantry rotated with the x-ray beam on; (3) the signal train, without a BT filter, was modeled using peak values measured in the signal train of step 2; and (4) the relative attenuation of the BT filter was estimated from filtered and unfiltered data sets. The prototype probe was first verified to have an isotropic and linear response to incident x-rays. The COBRA method was then tested on a dedicated breast CT scanner with a custom-designed BT filter and compared to the conventional step-and-shoot characterization of the BT filter. Using basis decomposition of dual energy signal data, the thickness of the filter was estimated and compared to the BT filter's manufacturing specifications. The COBRA method was also demonstrated with a clinical whole body CT scanner using the body BT filter. The relative attenuation was calculated at four discrete x-ray tube potentials and used to estimate the thickness of the BT filter. Results: The prototype probe was found to have a linear and isotropic response to x-rays. The relative attenuation produced from the COBRA method fell within the error of the relative attenuation measured with the step-and-shoot method

  5. Experimental validation of a method characterizing bow tie filters in CT scanners using a real-time dose probe

    Energy Technology Data Exchange (ETDEWEB)

    McKenney, Sarah E.; Nosratieh, Anita; Gelskey, Dale; Yang Kai; Huang Shinying; Chen Lin; Boone, John M. [Department of Radiology, University of California, Davis Medical Center, Rm. 0505, ACC Ellison Bldg., 4860 Y St., Sacramento, California 95817 (United States) and Department of Biomedical Engineering, University of California, Davis, Rm. 2303, GBSF, 451 E. Health Science Dr., Davis, California 95616 (United States); Diagnostic Imaging Specialists Corporation (DISC), 163 St. Malo Street, St. Malo, Manitoba R0A 1T0 (Canada); Department of Radiology, University of California, Davis Medical Center, Rm. 0505, ACC Ellison Bldg., 4860 Y St., Sacramento, California 95817 (United States); Department of Radiology, University of California, Davis Medical Center, Rm. 0505, ACC Ellison Bldg., 4860 Y St., Sacramento, California 95817 (United States) and Department of Biomedical Engineering, University of California, Davis, Rm. 2303, GBSF, 451 E. Health Science Dr., Davis, California 95616 (United States)

    2011-03-15

    Purpose: Beam-shaping or ''bow tie'' (BT) filters are used to spatially modulate the x-ray beam in a CT scanner, but the conventional method of step-and-shoot measurement to characterize a beam's profile is tedious and time-consuming. The theory for characterization of bow tie relative attenuation (COBRA) method, which relies on a real-time dosimeter to address the issues of conventional measurement techniques, was previously demonstrated using computer simulations. In this study, the feasibility of the COBRA theory is further validated experimentally through the employment of a prototype real-time radiation meter and a known BT filter. Methods: The COBRA method consisted of four basic steps: (1) The probe was placed at the edge of a scanner's field of view; (2) a real-time signal train was collected as the scanner's gantry rotated with the x-ray beam on; (3) the signal train, without a BT filter, was modeled using peak values measured in the signal train of step 2; and (4) the relative attenuation of the BT filter was estimated from filtered and unfiltered data sets. The prototype probe was first verified to have an isotropic and linear response to incident x-rays. The COBRA method was then tested on a dedicated breast CT scanner with a custom-designed BT filter and compared to the conventional step-and-shoot characterization of the BT filter. Using basis decomposition of dual energy signal data, the thickness of the filter was estimated and compared to the BT filter's manufacturing specifications. The COBRA method was also demonstrated with a clinical whole body CT scanner using the body BT filter. The relative attenuation was calculated at four discrete x-ray tube potentials and used to estimate the thickness of the BT filter. Results: The prototype probe was found to have a linear and isotropic response to x-rays. The relative attenuation produced from the COBRA method fell within the error of the relative attenuation

  6. 用于超宽带通信的镜像Bow-ti微带电路天线设计%Printed Mirror Bow-tie Antenna for UWB Applications

    Institute of Scientific and Technical Information of China (English)

    李少甫

    2008-01-01

    介绍了一种用于超宽带通信的平面型的小型天线.该天线采用相对介电常数为2.65的微带电路制作,天线尺寸为3.8 cm×2.8 cm.天线输入阻抗50 Ω,在3~10 GHz之间的驻波系数小于2.首先介绍了各种用于超宽带通信的平面型天线,讨论了镜像Bow-ti微带电路天线设计过程.最后用数字仿真软件对该天线进行了优化设计,并分析了天线的频域和时域特性,结果表明该天线能够满足超宽带通信的要求.

  7. FEASIBILITY OF WIND TO SERVE UPPER SKAGIT'S BOW HILL TRIBAL LANDS AND FEASIBILITY UPDATE FOR RESIDENTIAL RENEWABLE ENERGY.

    Energy Technology Data Exchange (ETDEWEB)

    RICH, LAUREN

    2013-09-30

    A two year wind resource assessment was conducted to determine the feasibility of developing a community scale wind generation system for the Upper Skagit Indian Tribe's Bow Hill land base, and the project researched residential wind resource technologies to determine the feasibility of contributing renewable wind resource to the mix of energy options for our single and multi-family residential units.

  8. Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary

    OpenAIRE

    Modolo, R.; Chanteur, G. M.; E. Dubinin; A. P. Matthews

    2006-01-01

    The solar wind plasma interaction with the Martian exosphere is investigated by means of 3-D multi-species hybrid simulations. The influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary is examined by comparing two simulations describing the two extreme states of the solar cycle. The hybrid formalism allows a kinetic description of each ions species and a fluid description of electrons. The ionization processes (photoionization, electron impact and charge exchange)...

  9. The effect of an outer-element bow on dryout power and post-dryout heat transfer of a 37-element bundle string

    International Nuclear Information System (INIS)

    Dryout and post-dryout tests were performed with a modified 37-element simulated CANDU fuel string, with one outer element of the last bundle gradually bowed toward the flow tube wall. The element had 8% higher heat flux than the remaining outer ring elements and had the narrowest gap between it and the flow-tube wall. The initial dryout occurred on the bowed element for all element-to-wall gap sizes. The dryout power decreased moderately (4% average) as the gap size was reduced to 13.5% of the nominal (unbowed) gap. For smaller than 13.5% gaps, however, the dryout power increased slightly (1.2%) at the low (10.5 kg/s) flow rate and decreased by 5% at the high (16.0 kg/s) flow rate, compared to the nominal gap dryout power. Surface temperatures of the bowed element were recorded for different gap sizes and up to 20% overpower (maximum). The temperature increased by 26% at the maximum overpower as the element was moved from nominal to zero gap position. (author)

  10. Radio Polarization Observations of G319.9-0.7: A Bow-shock Nebula with an Azimuthal Magnetic Field Powered by Pulsar J1509-5850

    CERN Document Server

    Ng, C -Y; Chatterjee, S; Johnston, S

    2010-01-01

    We report radio polarization observations of G319.9-0.7 (MSC 319.9-0.7) at 3 and 6 cm obtained with the Australia Telescope Compact Array. The source shows a highly elongated morphology with the energetic pulsar J1509-5850 located at the tip. We found a flat radio spectrum of index \\alpha=-0.26 +/- 0.04 and a high degree of linear polarization. These results confirm G319.9-0.7 as a bow-shock pulsar wind nebula. The polarization maps suggest a helical magnetic field trailing the pulsar, with the symmetry axis parallel to the system's inferred direction of motion. This is the first time such a field geometry has been seen in a bow-shock nebula, and it may be the result of an alignment between the pulsar spin axis and its space velocity. Compared to other bow-shock examples, G319.9-0.7 exhibits very different properties in the field structure and surface brightness distribution, illustrating the large diversity of the population.

  11. 风险分析工具Bow-Tie在西气东输交叉作业中的成功应用

    Institute of Scientific and Technical Information of China (English)

    曾庆军; 兰明光; 吴玉郎; 崔文彩

    2014-01-01

    两个分属于不同作业者的天然气接收站同时在香港屯门一个约3万m2的区域建设和运营,是典型的交叉作业。针对这项复杂的交叉作业,相关三方采用荷兰CGE公司开发的Bow-tie风险分析软件,对这项交叉作业全面系统地进行风险分析,全方位地辨识风险并提出具有针对性的控制措施。描述了Bow-tie工具的简单可视化操作特点,同时以这项交叉作业为例,介绍了Bow-tie应用步骤和过程以及得到的结果。

  12. The CHESS Survey of the L1157-B1 Shock Region: CO Spectral Signatures of Jet-driven Bow Shocks

    Science.gov (United States)

    Lefloch, B.; Cabrit, S.; Busquet, G.; Codella, C.; Ceccarelli, C.; Cernicharo, J.; Pardo, J. R.; Benedettini, M.; Lis, D. C.; Nisini, B.

    2012-10-01

    The unprecedented sensitivity of Herschel coupled with the high resolution of the HIFI spectrometer permits studies of the intensity-velocity relationship I(v) in molecular outflows, over a higher excitation range than possible up to now. Over the course of the CHESS Key Program, we have observed toward the bright bow shock region L1157-B1, the CO rotational transitions between J = 5-4 and J = 16-15 with HIFI, and the J = 1-0, 2-1, and 3-2 with the IRAM 30 m and the Caltech Submillimeter Observatory telescopes. We find that all the line profiles I CO(v) are well fit by a linear combination of three exponential laws vpropexp (- |v/v 0|) with v 0 = 12.5, 4.4, and 2.5 km s-1. The first component dominates the CO emission at J >= 13, as well as the high-excitation lines of SiO and H2O. The second component dominates for 3 = 105-106 cm-3) close to LTE up to J = 20. We find that the CO J = 2-1 intensity-velocity relation observed in various other molecular outflows is satisfactorily fit by similar exponential laws, which may hold an important clue to their entrainment process.

  13. Plasma waves in the range of the lower hybrid frequency: ISEE 1 and 2 Observations at the Earth's bow shock

    International Nuclear Information System (INIS)

    This report presents a characterization of plasma wave noise in the range of the lower hybrid frequency associated with 65 crossings of Earth's bow shock observed by the ISEE 1 and 2 satellites. Wave growth generally becomes detectable at the upstream edge of the shock foot, increases at the upstream edge of the shock ramp, peaks within the ramp, and then quickly decays to steady downstream values. The upstream extent of the noise is on the same order as that of specularly reflected gyrating ions. Similar profiles were observed in subcritical and supercritical shocks, and no special behavior was associated with the first critical Mach number. Spectra in the foot and ramp were similar in shape, although the noise was 1 to 2 orders of magnitude more intense in the shock ramps than in the feet. Low frequency electric field spectra are rather flat, with spectral indices ∼-2 to -1. Magnetic spectra are steeper, with spectral indices ∼-4. Electric field intensities are positively correlated with solar wind speed and inversely related to electron beta and Mach number. Magnetic components are positively correlated with Mach number and beta. These results are generally consistent with suggestions that the noise consists of lower hybrid waves driven by reflected gyrating ions in the foot, and by additional instabilities, such as the cross-field current, in the shock ramp. copyright American Geophysical Union 1988

  14. Application of Bow-Tie Analysis in Hemp%BTA技术分析在HEMP中的应用

    Institute of Scientific and Technical Information of China (English)

    石天雄

    2010-01-01

    近年来,领结图分析(Bow-Tie Analysis,缩写BTA)技术日益广泛被应用于石油化工建设项目的HSE管理和安全设计中.作为技术核心,BTA对危害及后果管理程序(Hazards and Effects Management Process,缩写HEMP)的成败起到了至关重要的作用.在陈述BTA起源背景、理论方法的基础上,着重细化并解决了在石化项目HSE管理中与领结图中顶事件、威胁预防措施、应急削减措施和升级因素等关键要素相关联的事件和活动任务,给出了BTA在HEMP中的实施程序和应用举例,说明BTA是解决石化项目HSE管理和HEMP的工具.

  15. A bow-tie genetic architecture for morphogenesis suggested by a genome-wide RNAi screen in Caenorhabditis elegans.

    Directory of Open Access Journals (Sweden)

    Matthew D Nelson

    2011-03-01

    Full Text Available During animal development, cellular morphogenesis plays a fundamental role in determining the shape and function of tissues and organs. Identifying the components that regulate and drive morphogenesis is thus a major goal of developmental biology. The four-celled tip of the Caenorhabditis elegans male tail is a simple but powerful model for studying the mechanism of morphogenesis and its spatiotemporal regulation. Here, through a genome-wide post-embryonic RNAi-feeding screen, we identified 212 components that regulate or participate in male tail tip morphogenesis. We constructed a working hypothesis for a gene regulatory network of tail tip morphogenesis. We found regulatory roles for the posterior Hox genes nob-1 and php-3, the TGF-β pathway, nuclear hormone receptors (e.g. nhr-25, the heterochronic gene blmp-1, and the GATA transcription factors egl-18 and elt-6. The majority of the pathways converge at dmd-3 and mab-3. In addition, nhr-25 and dmd-3/mab-3 regulate each others' expression, thus placing these three genes at the center of a complex regulatory network. We also show that dmd-3 and mab-3 negatively regulate other signaling pathways and affect downstream cellular processes such as vesicular trafficking (e.g. arl-1, rme-8 and rearrangement of the cytoskeleton (e.g. cdc-42, nmy-1, and nmy-2. Based on these data, we suggest that male tail tip morphogenesis is governed by a gene regulatory network with a bow-tie architecture.

  16. The effect of copper vacancies on the optical bowing of chalcopyrite Cu(In,Ga)Se2 alloys

    International Nuclear Information System (INIS)

    This paper reports that the optical bowling behavior of polycrystalline thin film CuIn1-yGaySe2 alloys is dependent upon the Cu stoichiometry. The variation in optical band gap, Eg, for alloys in which Cu is near stoichiometric (25 at. %) is parabolic and follows the relationship: Eg(y) = 1.011 + 0.421 y + 0.244 y2 (eV), where y is the alloy parameter, [at.% Ga]/[at.%Ga + at.%In]. Contrary to this, films with Cu-poor stoichiometries (∼19 at.% Cu) exhibit little alloy bowing: Eg(y) = 1.01 + 0.733 y - 0.046 y2 (eV). The increase in Eg with Cu deficiency appears to be the result of both a structural effect associated with tetragonal lattice shrinkage, ΔV = Vstoichiometric - VCu-poor (resulting from the presence of Cu vacancies) and a chemical effect, possibly associated with a counterbalance between p-d repulsion and anion displacement effects

  17. Civil Aircraft Landing Overrun Risk Analysis Based on Bow-tie Model%基于 Bow -tie 模型的民机着陆冲出跑道风险分析

    Institute of Scientific and Technical Information of China (English)

    陆正; 崔振新; 汪磊

    2015-01-01

    To better systematically analyze the civil aircraft landing overrun incident ,a Bow-tie model is applied to con-duct researches .In terms of landing overrun causes identification ,combined with the SHEL model and a Reason model ,a detailed analysis of these causes of the accidents is made and the formation mechanism of landing runway is got .The landing overrun influence factors are concluded as crew technical fault , violation of procedures or standards , loss of situational awareness ,CRM failure ,aircraft mechanical failure ,adverse weather conditions ,wet or contaminated runway and runway design defects .According to the analysis results preventive and controlling measures are put forward .The Bow-tie pattern-ing is used to concisely describe the causes and results of landing overrun and the relevant preventive and control measures . This study provides a systemic risk management method for civil aircraft landing overrun .%为了更加系统全面地分析民机着陆冲出跑道风险,采用Bow-tie模型进行研究。在着陆冲出跑道原因辨识方面,结合SHEL模型和Reason模型对这些事故的原因进行了具体分析,得到了着陆冲出跑道的形成机理,最终将着陆冲出跑道影响因素归纳为机组技能失误、机组违反程序或标准、机组丧失情景意识、机组资源管理失效、航空器机械故障、不利天气条件影响、跑道湿滑或污染、跑道设计缺陷等,并基于上述分析结果绘制航空器着陆冲出跑道Bow-tie图,对着陆冲出跑道的原因和后果以及相应的预防和控制措施进行了描述。最后对着陆冲出跑道历史数据进行统计,结果表明,机组因素和环境因素是导致着陆冲出跑道最主要的两个原因,提出着陆冲出跑道防范的重点,从系统角度提出了民机着陆冲出跑道的风险管理办法。

  18. Quantitative risk assessment of urban gas pipelines based on the fuzzy Bow-tie model%基于模糊Bow-tie模型的城镇燃气管道泄漏定量风险评价

    Institute of Scientific and Technical Information of China (English)

    於孝春; 贾朋美; 张兴

    2013-01-01

    燃气管道事故一旦发生后果大多比较严重.为全面分析燃气管道风险的前因后果,确定重点维护和监控的管段区域,引入了Bow-tie模型,将管道泄漏的故障树与事件树统一到一起对燃气管道进行定量风险评价.采用模糊集相关理论与专家评价相结合的方法得出管道泄漏的模糊可能值;然后基于模糊层次分析法确定管道泄漏后果因素的权重系数;再通过矩阵乘法求得泄漏后果值.以某段燃气管线为案例,全面识别出各风险因素,量化得到管道各泄漏后果事件的风险值.实际应用结果表明:①该方法可快速合理地评判出管道系统的相对风险大小;②三角模糊数与层次分析法的应用减少了传统评价中主观及模糊因素产生的评价偏差,使得评价结果更接近客观实际;③依据评价结果制订有针对性的预防维护措施,能够实现有限维护资源的合理配置,保障燃气管道的安全可靠运行.

  19. 基于Bow-Tie模型的美军航母舰载航飞行安全风险分析%Flight safety risk analysis of U.S.carrier-based aircraft based on Bow-Tie model

    Institute of Scientific and Technical Information of China (English)

    郑卫东; 万辉; 张孝强; 姚永杰; 刘秋红; 王伟

    2014-01-01

    目的 通过分析美军航母舰载机飞行事故发生的规律和成因,为舰载机飞行事故的有效防范提供科学依据.方法 对美军1950-2011年发生的161起舰载机飞行事故进行统计,并采用Bow-Tie模型进行风险分析,提出防范措施和对策.结果 从上世纪50年代到现在,美军航母舰载机飞行事故的危害性处于相对稳定的水平,但着舰阶段的事故发生率和危害性最高;航母舰载机飞行的风险因素主要包括人因素、航母甲板因素、舰载机因素和海上环境因素.结论 应从严格保障人员身心健康、规范化舰载机起降作业、保证装备的良好工作状态、不断研制和充分利用先进技术等方面采取措施和对策保障舰载飞行职业安全.

  20. A comparison of bow shock models with Cluster observations during low Alfvén Mach number magnetic clouds

    Directory of Open Access Journals (Sweden)

    L. Turc

    2013-06-01

    Full Text Available Magnetic clouds (MCs are very geoeffective solar wind structures. Their properties in the interplanetary medium have been extensively studied, yet little is known about their characteristics in the Earth's magnetosheath. The Cluster spacecraft offer the opportunity to observe MCs in the magnetosheath, but before MCs reach the magnetosphere, their structure is altered when they interact with the terrestrial bow shock (BS. The physics taking place at the BS strongly depends on ΘBn, the angle between the shock normal and the interplanetary magnetic field. However, in situ observations of the BS during an MC's crossing are seldom available. In order to relate magnetosheath observations to solar wind conditions, we need to rely on a model to determine the shock's position and normal direction. Yet during MCs, the models tend to be less accurate, because the Alfvén Mach number (MA is often significantly lower than in regular solar wind. On the contrary, the models are generally optimised for high MA conditions. In this study, we compare the predictions of four widely used models available in the literature (Wu et al., 2000; Chapman and Cairns, 2003; Jeřáb et al., 2005; Měrka et al., 2005b to Cluster's dayside BS crossings observed during five MC events. Our analysis shows that the ΘBn angle is well predicted by all four models. On the other hand, the Jeřáb et al. (2005 model yields the best estimates of the BS position during low MA MCs. The other models locate the BS either too far from or too close to Earth. The results of this paper can be directly used to estimate the BS parameters in all studies of MC interaction with Earth's magnetosphere.

  1. Stratigraphic evidence for multiple small Quaternary displacements on the Bow Ridge fault at northeast Yucca Mountain, Nye County, Nevada

    International Nuclear Information System (INIS)

    A detailed study of Trench 14D on the Bow Ridge fault, a north-trending, steeply dipping (75 degree W) normal fault that bounds the northeast edge of Yucca Mountain, indicates that 5--6 small displacements with long recurrence intervals took place during the middle to late Quaternary. Five to six individual surface-rupture events are recognized at discrete stratigraphic intervals in the sequence based on (a) incremental up-section decreases in offset marker horizons, (b) the position of small fault-displacement colluvial wedges deposited adjacent to the fault above downthrown marker horizons, and (c) development of buried degraded fault scarps. Vertical displacements on individual events vary between 5 and 20 cm (ave. 10 cm), which collectively sum to 45 cm of cumulative vertical offset across the lowermost units. Many left-oblique striation sets (65 degree--20 degree plunges) are observed on carbonate fault laminae, which, if tectonic, suggest cumulative and average-event net slip amounts of 76--132 cm and 11--28 cm, respectively. The four oldest events occurred during the middle Pleistocene, based on correlations of faulted units with a dated chronosequence; the fifth and a possible sixth event are bracketed within a late Pleistocene unit. Generally long recurrence intervals (104--105yrs) and very low slip rates (∼ 0.001 mm/yr) are indicated by the small cumulative offsets and stratigraphic separation of events between nontectonic colluvium containing buried paleosols and (or) degraded fault scarps. Other ongoing studies suggest that generally similar behavior characterizes many normal faults in the Yucca Mountain area

  2. Neural network prediction of carbonate lithofacies from well logs, Big Bow and Sand Arroyo Creek fields, Southwest Kansas

    Science.gov (United States)

    Qi, L.; Carr, T.R.

    2006-01-01

    In the Hugoton Embayment of southwestern Kansas, St. Louis Limestone reservoirs have relatively low recovery efficiencies, attributed to the heterogeneous nature of the oolitic deposits. This study establishes quantitative relationships between digital well logs and core description data, and applies these relationships in a probabilistic sense to predict lithofacies in 90 uncored wells across the Big Bow and Sand Arroyo Creek fields. In 10 wells, a single hidden-layer neural network based on digital well logs and core described lithofacies of the limestone depositional texture was used to train and establish a non-linear relationship between lithofacies assignments from detailed core descriptions and selected log curves. Neural network models were optimized by selecting six predictor variables and automated cross-validation with neural network parameters and then used to predict lithofacies on the whole data set of the 2023 half-foot intervals from the 10 cored wells with the selected network size of 35 and a damping parameter of 0.01. Predicted lithofacies results compared to actual lithofacies displays absolute accuracies of 70.37-90.82%. Incorporating adjoining lithofacies, within-one lithofacies improves accuracy slightly (93.72%). Digital logs from uncored wells were batch processed to predict lithofacies and probabilities related to each lithofacies at half-foot resolution corresponding to log units. The results were used to construct interpolated cross-sections and useful depositional patterns of St. Louis lithofacies were illustrated, e.g., the concentration of oolitic deposits (including lithofacies 5 and 6) along local highs and the relative dominance of quartz-rich carbonate grainstone (lithofacies 1) in the zones A and B of the St. Louis Limestone. Neural network techniques are applicable to other complex reservoirs, in which facies geometry and distribution are the key factors controlling heterogeneity and distribution of rock properties. Future work

  3. Simulation Study on Flare Impact of Bow%船舶艏部外飘砰击压力的仿真研究

    Institute of Scientific and Technical Information of China (English)

    赵留平

    2015-01-01

    The slamming problem of 3D ship bow was studied by means of the finite volume method based on the numerical simulation method. A three-dimension coupling finite element model including air,water and hull was built up. The fluid-structure interaction was simulated using general coupling algorithm and the fluid was treated on a fix mess by using an Euler formulation and the structure on a deformable mesh by using a Lagrangian formulation. The space distribution of flare impact pressure on the side region was ana-lyzed. The results show that numerical simulation method could calculate the flare impacting problem of ship bow reliably. The result of this paper could provide the reference base for the design and optimization of the bow.%基于有限体积法的数值仿真方法对三维船舶艏部的砰击问题进行了研究,建立包含空气、水和船舶艏部的完全耦合三维有限元模型,流体域用 Euler 单元模拟,结构部分用 Lagrange 单元模拟,采用一般耦合算法,分析了船舶艏部外飘砰击压力在船舷侧位置的分布情况;结果表明:数值仿真计算方法可以合理计算船舶艏部的外飘砰击问题,为船舶艏部线型的设计优化提供参考基础。

  4. Evidence of the correlation between a strong 4d-As/2p-N orbitals coupling and the bowing effect in GaAsN

    International Nuclear Information System (INIS)

    By means of a simple physical argumentation, we found that the giant bowing observed in GaAsN is correlated to the interaction between 4d-As and 2p-N orbitals. The calculations were carried out within the first principles full potential linear muffin-tin orbitals (FPLMTO) method in its plane wave approximation (PLW) which enables an accurate treatment of the interstitial regions. The choice of this method ensures our work to be free from adjustable parameters and enabled us to perform a microscopic study

  5. Evidence of the correlation between a strong 4d-As/2p-N orbitals coupling and the bowing effect in GaAsN

    Energy Technology Data Exchange (ETDEWEB)

    Mehnane, Noureddine; Badi, Fouzia [Applied Materials Laboratory, Universite de Sidi Bel Abbes, 22000 Sidi Bel Abbes (Algeria); Aced, Mohammed Reda [Laboratoire de Transmission et Traitement Numerique du Signal (LTTNS), Centre de Recherches (ex-CFTE), Universite de Sidi Bel Abbes, 22000 Sidi Bel Abbes (Algeria); Abid, Hamza [Applied Materials Laboratory, Universite de Sidi Bel Abbes, 22000 Sidi Bel Abbes (Algeria); Sekkal, Nadir [Departement de Physique-Chimie, Ecole Normale Superieure de l' Enseignement Technique, BP 1523, El M' Naouer, 31000 Oran (Algeria); Condensed Matter Section, The Abdus Salam International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34014 Trieste (Italy); Physia-Laboratory, BP 47 (RP), 22000 Sidi Bel Abbes (Algeria)], E-mail: nsekkal@yahoo.fr

    2008-12-15

    By means of a simple physical argumentation, we found that the giant bowing observed in GaAsN is correlated to the interaction between 4d-As and 2p-N orbitals. The calculations were carried out within the first principles full potential linear muffin-tin orbitals (FPLMTO) method in its plane wave approximation (PLW) which enables an accurate treatment of the interstitial regions. The choice of this method ensures our work to be free from adjustable parameters and enabled us to perform a microscopic study.

  6. Evidence of the correlation between a strong 4d-As/2p-N orbitals coupling and the bowing effect in GaAsN

    International Nuclear Information System (INIS)

    By means of a simple physical argumentation, we give the proof that the giant bowing observed in GaAsN is correlated to a strong interaction between 4d-As and 2p-N orbitals. The calculations were carried out within the first principles full potential linear muffin-tin orbitals method (FPLMTO) method in its plane wave approximation (PLW) which enables an accurate treatment of the interstitial regions. The choice of this method ensures our work to be free from adjustable parameters and enables us to perform a microscopic study. (author)

  7. Study on effect of bow shape on icebreaking resistance. 2nd Report. Relationship between hull motion and icebreaking resistance in high speed range; Saihyo teiko ni oyobosu senshu keijo no eikyo ni kansuru kenkyu. 2. Kosokuji no sentai undo to saihyo teiko no kakawari

    Energy Technology Data Exchange (ETDEWEB)

    Suzuki, Y.; Uemura, O.; Kato, H.; Yamaguchi, H. [The University of Tokyo, Tokyo (Japan); Izumiyama, K. [Ship Research Inst., Tokyo (Japan)

    1997-06-01

    The effect of ship speed on icebreaking resistance is investigated. The video photographs show that vertical motion of the bow is more noted as ship speed increases. It is expected that there is a correlation between average upward movement of the bow and amplitude of its vertical motion, and the effect of vertical motion of the bow on icebreaking resistance is investigated. It is found that increasing ship speed increases both vertical movement of the bow and amplitude of its vertical motions, and increases icebreaking resistance; the pressure component generated by rotation of broken ice pieces is one of the reasons for increased icebreaking resistance; ice piece rotation speed is determined by hull inclination angle at the hull/ice contact point, and ice piece size by bow waterline angle and curvature; and spoon bow increases in icebreaking resistance more slowly as ship speed increases than the other bow shapes, because of its larger bow waterline angle and more gentle waterline curvature to give wider but shorter ice pieces, and hence a smaller hull inclination angle at the hull/ice contact point. 4 refs., 13 figs.

  8. A theoretical-experimental comparison of the synchronous response of a bowed rotor in five different sets of fluid film bearings

    Science.gov (United States)

    Flack, R. D.; Rooke, J. H.

    1980-12-01

    A comparison of theoretical and experimental synchronous unbalance responses of a bowed Jeffcott rotor in fluid film bearings has been completed. A transfer matrix method was used to predict theoretically the response of a 25·4 mm shaft in fluid film bearings and results were compared to data from a previous experimental study. Four bearing types were used: two axial groove, pressure dam, tilting pad and four-lobe. Very good agreement was found for all bearing types at the rotor critical speed (3000 rpm). Differences less than 15% in peak response were found and the theoretical and experimental peaks were found to occur within 200 rpm. Worst agreement was found for the preloaded four-lobe bearings and this disagreement was found for speeds other than the critical speed. Also, for equal bow and unbalance the tilting pad and four-lobe bearings were found to produce the least and most damping at the critical speed, respectively. Previous to this time a comparison of theoretical and experimental synchronous responses of a rotor system representing industrial turbomachines has not been published, nor has a comparative study of the different bearing types.

  9. The Mouse That Soared: High Resolution X-ray Imaging of the Pulsar-Powered Bow Shock G359.23-0.82

    CERN Document Server

    Gaensler, B M; Camilo, F; Kaspi, V M; Baganoff, F K; Yusef-Zadeh, F; Manchester, R N

    2003-01-01

    We present an observation with the Chandra X-ray Observatory of the unusual radio source G359.23-0.82 ("the Mouse"), along with updated radio timing data from the Parkes radio telescope on the coincident young pulsar J1747-2958. We find that G359.23-0.82 is a very luminous X-ray source (L_X [0.5-8.0 keV] = 5e34 ergs/s for a distance of 5 kpc), whose morphology consists of a bright head coincident with PSR J1747-2958, plus a 45''-long narrow tail whose power-law spectrum steepens with distance from the pulsar. We thus confirm that G359.23-0.82 is a bow-shock pulsar wind nebula powered by PSR J1747-2958; the nebular stand-off distance implies that the pulsar is moving with a space velocity ~600 km/s through gas of density ~0.3 cm^-3. We combine the theory of ion-dominated pulsar winds with hydrodynamic simulations of pulsar bow shocks to show that a bright elongated X-ray and radio feature extending 10'' behind the pulsar represents the surface of the wind termination shock. The X-ray and radio "trails" seen in...

  10. Band gap bowing parameter in pseudomorphic Al{sub x}Ga{sub 1−x}N/GaN high electron mobility transistor structures

    Energy Technology Data Exchange (ETDEWEB)

    Goyal, Anshu; Kapoor, Ashok K.; Raman, R.; Dalal, Sandeep; Mohan, Premila; Muralidharan, R. [Solid State Physics Laboratory, Lucknow Road, Delhi 110054 (India)

    2015-06-14

    A method for evaluation of aluminium composition in pseudomorphic Al{sub x}Ga{sub 1−x}N layer from the measured photoluminescence (PL) peak energy is presented here. The layers were grown by metalorganic chemical vapor deposition and characterized by high resolution X-ray diffraction (HRXRD), PL, cathodoluminescence, and atomic force microscopy. We estimated the value of biaxial stress in pseudomorphic Al{sub x}Ga{sub 1−x}N layers grown on sapphire and silicon carbide substrates using HRXRD scans. The effect of biaxial stress on the room temperature band edge luminescence in pseudomorphic Al{sub x}Ga{sub 1−x}N/GaN layers for various aluminium compositions in the range of 0.2 < x < 0.3 was determined. The value of pressure coefficient of band gap was also estimated. The stress corrected bowing parameter in Al{sub x}Ga{sub 1−x}N was determined as 0.50 ± 0.06 eV. Our values match well with the theoretically obtained value of bowing parameter from the density functional theory.

  11. A bow-tie photoconductive antenna using a low-temperature-grown GaAs thin-film on a silicon substrate for terahertz wave generation and detection

    International Nuclear Information System (INIS)

    This paper presents heterogeneously integrated bow-tie emitter–detector photoconductive antennas (PCAs) based on low-temperature grown-gallium arsenide (LTG-GaAs) thin-film devices on silicon-dioxide/silicon (SiO2/Si) host substrates for integrated terahertz (THz) systems. The LTG-GaAs thin-film devices are fabricated with standard photolithography and thermal evaporation of metal-contact layers of chromium (Cr), nickel (Ni) and gold (Au). They are etched selectively and separated from their growth GaAs substrate. The LTG-GaAs thin-film devices are then heterogeneously integrated on bow-tie antenna electrodes patterned on the surface of a SiO2/Si host substrate for THz emitters and THz detectors. Cost-effective and selective integration of LTG-GaAs thin-film devices on a Si platform is demonstrated. THz radiation from the fabricated THz PCAs is successfully measured using a pump–probe THz time-domain configuration. The THz temporal duration was measured at full width half maximum of 0.36 ps. Its frequency spectrum exhibits a broadband response with a peak resonant frequency of about 0.31 THz. The demonstration illustrates the feasibility of creating heterogeneously integrated THz systems using separately optimized LTG-GaAs devices and Si based electronics. (paper)

  12. Application of Bowtie risk management method in mud logging operation%Bow-tie风险管理法在录井作业中的应用

    Institute of Scientific and Technical Information of China (English)

    郑应钊; 曾祥红; 卢永强

    2008-01-01

    石油勘探开发是高风险、高投入性的项目,如何在工程项目的实施中有效控制安全风险,已成为人们关注的重点之一.Bow-tie风险管理法是壳牌公司的一种管理方法,结合国外Bow-tie风险管理的成果,通过对录井作业中存在的主要安全风险进行分析、识别,找出了这些风险可能引发的顶级事件以及顶级事件可能产生的后果;针对顶级事件的产生原因找出防止危害发生和屏障失效的控制措施;最终提出了控制这些录井作业风险的31个关键活动和57个关键任务.严格执行这些"关键活动和关键任务",可以确保现场录井作业安全有序进行.

  13. Multi-dimensional dynamics of stimulated Brillouin scattering in a laser speckle: Ion acoustic wave bowing, breakup, and laser-seeded two-ion-wave decay

    Science.gov (United States)

    Albright, B. J.; Yin, L.; Bowers, K. J.; Bergen, B.

    2016-03-01

    Two- and three-dimensional particle-in-cell simulations of stimulated Brillouin scattering (SBS) in laser speckle geometry have been analyzed to evaluate the relative importance of competing nonlinear processes in the evolution and saturation of SBS. It is found that ion-trapping-induced wavefront bowing and breakup of ion acoustic waves (IAW) and the associated side-loss of trapped ions dominate electron-trapping-induced IAW wavefront bowing and breakup, as well as the two-ion-wave decay instability over a range of Z Te/Ti conditions and incident laser intensities. In the simulations, the latter instability does not govern the nonlinear saturation of SBS; however, evidence of two-ion-wave decay is seen, appearing as a modulation of the ion acoustic wavefronts. This modulation is periodic in the laser polarization plane, anti-symmetric across the speckle axis, and of a wavenumber matching that of the incident laser pulse. A simple analytic model is provided for how spatial "imprinting" from a high frequency inhomogeneity (in this case, the density modulation from the laser) in an unstable system with continuum eigenmodes can selectively amplify modes with wavenumbers that match that of the inhomogeneity.

  14. DESY: ARGUS bows out

    International Nuclear Information System (INIS)

    Last year the ARGUS experiment at DESY's DORIS electron-positron storage ring stopped taking data after ten years of fruitful physics. Analysis and new results will continue for some time, but members of the group are already looking to new physics horizons. The ARGUS collaboration was formed in 1978 by groups from DESY, Dortmund, Heidelberg (IHEP), Lund, Moscow (ITEP), and South Carolina under the leadership of Walter Schmidt-Parzefall. Later groups joined from IPP Canada, Kansas, Ljubljana, Karlsruhe, Erlangen/Nurnberg, Heidelberg (MPI) and Dresden. The detector was conceived to investigate the physics of the beauty and charm quarks and the tau lepton at the upgraded DORIS II electronpositron storage ring. With a similar programme started by the CLEO collaboration at Cornell's CESR electron-positron collider, the resulting competition ensured good physics. ARGUS rolled into the beam in October 1982 and took data until October 1992. In May 1993 the decision was taken to stop further ARGUS running. During those ten years a broad spectrum of physics has been covered, including weak decays of beauty and charm quarks and tau leptons, hadron spectroscopy, quark/gluon mechanisms, photon-photon interactions and particle searches. In particular, ARGUS has made valuable contributions to determination of many fundamental constants of the Standard Model. These comprise measurements of quark transitions (CKM matrix elements) in the decays of B mesons (containing the beauty quark), the determination of the properties of the tau lepton and its neutrino, as well as a measurement of the quark coupling constant. The charm study has resulted in first observations of many charmed hadrons and decay modes. The study of quark and gluon mechanisms (fragmentation) has yielded valuable input for future experiments, while the first observations of new final states in photon-photon interactions have created much interest. A total luminosity of 520 inverse picobarns has been collected at collision energies around 10 GeV

  15. The CHESS survey of the L1157-B1 bow-shock: high and low excitation water vapor

    Science.gov (United States)

    Busquet, G.; Lefloch, B.; Benedettini, M.; Ceccarelli, C.; Codella, C.; Cabrit, S.; Nisini, B.; Viti, S.; Gómez-Ruiz, A. I.; Gusdorf, A.; di Giorgio, A. M.; Wiesenfeld, L.

    2014-01-01

    Context. Molecular outflows powered by young protostars strongly affect the kinematics and chemistry of the natal molecular cloud through strong shocks. This results in substantial modifications of the abundance of several species. In particular, water is a powerful tracer of shocked material because of its sensitivity to both physical conditions and chemical processes. Aims: As part of the Chemical HErschel Surveys of Star-forming regions (CHESS) guaranteed time key program, we aim at investigating the physical and chemical conditions of H2O in the brightest shock region B1 of the L1157 molecular outflow. Methods: We observed several ortho- and para-H2O transitions using the HIFI and PACS instruments on board Herschel toward L1157-B1, providing a detailed picture of the kinematics and spatial distribution of the gas. We performed a large velocity gradient (LVG) analysis to derive the physical conditions of H2O shocked material, and ultimately obtain its abundance. Results: We detected 13 H2O lines with both instruments probing a wide range of excitation conditions. This is the largest data set of water lines observed in a protostellar shock and it provides both the kinematics and the spatial information of the emitting gas. The PACS maps reveal that H2O traces weak and extended emission associated with the outflow identified also with HIFI in the o-H2O line at 556.9 GHz, and a compact (~10'') bright, higher excitation region. The LVG analysis of H2O lines in the bow-shock show the presence of two gas components with different excitation conditions: a warm (Tkin ≃ 200-300 K) and dense (n(H2) ≃ (1-3) × 106 cm-3) component with an assumed extent of 10'', and a compact (~2''-5'') and hot, tenuous (Tkin ≃ 900-1400 K, n(H2) ≃ 103-4 cm-3) gas component that is needed to account for the line fluxes of high Eu transitions. The fractional abundance of the warm and hot H2O gas components is estimated to be (0.7-2) × 10-6 and (1-3) × 10-4, respectively. Finally, we

  16. Comparisons of CME/ICME stand-off distance ratios from observations with those from semi-empirical relationships based on a bow shock theory

    Science.gov (United States)

    Lee, Jae-Ok; Moon, Yong-Jae; Lee, Jin-Yi; Jang, Soojeong; Lee, Harim

    2016-05-01

    It is generally believed that fast coronal mass ejections (CMEs) and their associated interplanetary CMEs (ICMEs) can generate CME/ICME-driven shocks, which are characterized by faint structures ahead of CMEs in white-light coronagraph images and sheath structures in solar wind data. In this study, we examine whether the observational stand-off distance ratios, which are defined as stand-off distances divided by curvature radiuses, of CMEs and their associated ICMEs are explained by a bow-shock theory or not. For this, we select 16 CME-ICME pairs from September 2009 to October 2012 with the following conditions: (1) limb CMEs by SOHO and their associated ICMEs by twin STEREO spacecraft when both spacecraft were roughly in quadrature, and vice versa; (2) the faint structures ahead of limb CMEs are well identified; and (3) their associated ICMEs have corresponding sheath structures. We determine the observational stand-off distance ratios of the CMEs by using brightness profiles from LASCO-C2 (or SECCHI-COR2) observations. The stand-off distance ratios of the ICMEs are determined by using solar wind data (plasma speed, shock starting time, and ICME starting time) from STEREO-IMPACT/PLASTIC (OMNI database) observations. We compare our estimations with the theoretical stand-off distance ratios of the CME-ICME pairs using semi-empirical relationships based on the bow shock theory. We also examine the changes of observational stand-off distance ratios during CME propagations. We find the following results. (1) 60 % of fast CMEs (6/10), whose Mach number are greater than 1, are explained by the conventional theory in the acceptable ranges of adiabatic gamma and CME geometry. (2) 50 % of fast ICMEs (6/12) are explained by the conventional theory. (3) About 70 % of fast CME-ICME pairs (6/9), observational stand-off distance ratios decrease during CME propagations due to the deceleration of CMEs by the solar wind drag. Our results demonstrate that the observed signatures of

  17. Remote sensing of local structure of the quasi-perpendicular Earth's bow shock by using field-aligned beams

    Directory of Open Access Journals (Sweden)

    B. Miao

    2009-03-01

    Full Text Available Field-aligned ion beams (FABs originate at the quasi-perpendicular Earth's bow shock and constitute an important ion population in the foreshock region. The bulk velocity of these FABs depends significantly on the shock normal angle, which is the angle between shock normal and upstream interplanetary magnetic field (IMF. This dependency may therefore be taken as an indicator of the local structure of the shock. Applying the direct reflection model to Cluster measurements, we have developed a method that uses proton FABs in the foreshock region for remote sensing of the local shock structure. The comparison of the model results with the multi-spacecraft observations of FAB events shows very good agreement in terms of wave amplitude and frequency of surface waves at the shock front.

  18. Evidence of a Mira-like tail and bow shock about the semi-regular variable V CVn from four decades of polarization measurements

    CERN Document Server

    Neilson, Hilding R; Smith, Beverly J; Henson, Gary; Adams, Alyssa M

    2014-01-01

    Polarization is a powerful tool for understanding stellar atmospheres and circumstellar environments. Mira and semi-regular variable stars have been observed for decades and some are known to be polarimetrically variable, however, the semi-regular variable V Canes Venatici displays an unusually large, unexplained amount of polarization. We present ten years of optical polarization observations obtained with the HPOL instrument, supplemented by published observations spanning a total interval of about forty years for V CVn. We find that V CVn shows large polarization variations ranging from 1 - 6%. We also find that for the past forty years the position angle measured for V CVn has been virtually constant suggesting a long-term, stable, asymmetric structure about the star. We suggest that this asymmetry is caused by the presence of a stellar wind bow shock and tail, consistent with the star's large space velocity.

  19. Pick-up ions at Comet P/Halley's bow shock - Observations with the IIS spectrometer on Giotto. [Implanted In Spectrometer

    Science.gov (United States)

    Wilken, B.; Johnstone, A.; Coates, A.; Amata, E.; Borg, H.

    1987-01-01

    Gaseous material expanding from the nucleus of Comet Halley into space forms the neutral coma around the comet. Ionization in the solar UV radiation removes particles from the coma and injects them into the solar wind plasma. These freshly created ions are accelerated by the interplanetary electric field on cycloidal trajectories with gyrocenters moving with the speed of the magnetic field lines. In the solar wind frame of reference these particles move along the magnetic field lines with a fixed pitch angle. Pitch-angle scattering and energy diffusion reduce quickly the initial energy anisotropy which is associated with the narrow pick-up structures. First observations of heavy cometary pick-up ions (water group ions) at the bow shock are presented. The evolution of the distribution function in the vicinity of the shock and radial density profiles are discussed.

  20. On the impact of isoelectric impurities on band bowing and disorder of compound semiconductors; Ueber den Einfluss von isoelektronischen Stoerstellen auf Bandbiegung und Unordnung in Verbindungshalbleitern

    Energy Technology Data Exchange (ETDEWEB)

    Karcher, Christian

    2012-03-16

    Isolectronic impurities and their impact on the properties of compound semiconductors is discussed in two systems: Nitrogen in Ga(As,P) quantum wells on the one hand and Sulfur and Selenium in bulk ZnTe. The properties are reduced to two experimentally observable aspects: Band Bowing, i.e. the non-linearity of the band gap of the compound semiconductor and disorder, i.e. in particular the formation of a strongly localized density of states beneath the fundamental band gap. Apart of the pure experimental studies an insight into the theoretical model of disorder-induced temperature dependent luminescence properties of the compound semiconductors by means of Monte Carlo Simulations is given.

  1. Análise e avaliação de risco de incêndio através de diagramas “Bow-Tie”

    OpenAIRE

    Sequeira, Daniel Guilherme Rodrigues

    2010-01-01

    Dissertação apresentada na Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa para obtenção do grau de Mestre em Engenharia e Gestão Industrial Esta dissertação descreve uma análise e avaliação do risco de incêndio numa instalação industrial. Para tal foi aplicado o modelo “Bow-Tie” em conjunto com matrizes de risco, tendo-se utilizado como ponto de partida o relatório de um incêndio ocorrido na central eléctrica da refinaria de Sines da Galp Energia, em Janeiro de 2009. A a...

  2. Multi‐instrument observations from Svalbard of a traveling convection vortex, electromagnetic ion cyclotron wave burst, and proton precipitation associated with a bow shock instability

    DEFF Research Database (Denmark)

    Engebretson, M. J.; Yeoman, T. K.; Oksavik, K.;

    2013-01-01

    An isolated burst of 0.35 Hz electromagnetic ion cyclotron (EMIC) waves was observed at four sites on Svalbard from 0947 to 0954 UT 2 January 2011, roughly 1 h after local noon. This burst was associated with one of a series of ~50 nT magnetic impulses observed at the northernmost stations of the...... IMAGE magnetometer array. Hankasalmi SuperDARN radar data showed a west-to-east (antisunward) propagating vortical ionospheric flow in a region of high spectral width ~ 1–2° north of Svalbard, confirming that this magnetic impulse was the signature of a traveling convection vortex. Ground...... of Earth observed a steady solar wind and predominantly radial interplanetary magnetic field orientation before and during this event, data from Geotail (near the morning bow shock) showed large reorientations of the interplanetary magnetic field and substantial decreases in ion density several...

  3. East-west crustal structure and "down-bowing" Moho under the northern Tibet revealed by wide-angle seismic profile

    Institute of Scientific and Technical Information of China (English)

    2002-01-01

    We recognized 6 sets of reflecting P- and S-wave events from Moho and other interfaces within the crust, respectively, with the wide-angle seismic data acquired from 510 km-long Selincuo-Ya'anduo profile in the northern Tibet, fitted the observed events with forward modeling, and interpreted crustal structure of P- and S-wave velocities and Poisson's ratio under the profile. The results demonstrate that the crustal structure between Yarlungzangbo and Bangong-Nujiang sutures changes abruptly, and the crust is the thickest at the middle part of the profile with thickness of 80 km or more. The "down-bowing" Moho is the striking feature for the crustal variation along the west-east direction. The Moho uplifts with steps, and the uplifting rate westward is greater than that eastward. The heterogeneity of P- and S-wave velocities exists both vertically and horizontally, and one lower velocity layer (LVL) exists with the depth range of 27-34 km and the thickness range of 5-7 km. For the upper crust, Poisson's ratio is the lowest at the middle part of the profile; for the lower crust, the Poisson's ratio at the east segment is lower than that at west segment, which means that the crustal rigidity for the upper crust is different from the lower crust, and the lower crust under the east segment of the profile is more ductile. We infer that the substance in the lower crust endured eastward flow along with the collision between Eurasian and Indian plates, and the "down-bowing" Moho is attributable to the multi-phase E-W tectonic processes.

  4. Full-Wave Analysis of Compact Bow-Tie Microstrip Antennas%小型化蝶形微带天线的全波分析

    Institute of Scientific and Technical Information of China (English)

    张需溥; 钟顺时

    2001-01-01

    The bow-tie microstrip antenna is analyzed by using the moment method. This analysis can accurately predict the resonant frequency, input impedance, and radiation patterns. For this particular shape of patch, a new hybrid basis function is adopted, which is a combination of a full domain basic function and an impulse basic function. The asymptotic extraction technique is involved in calculating the Sommerfeld-type integral. This formulation allows the infinite double integral of impedance matrix to be transformed into a finite one-dimensional integral, significantly reducing the computation time. The calculated results of this program agree well with experimental ones. It is shown that bow-tie microstrip antenna is a type of new compact antennas with smaller size than that of commonly used rectangular patch antennas.%采用矩量法分析了蝶形微带贴片天线,可用来比较准确地预测这类微带贴片天线的输入阻抗、谐振频率和方向图.根据该天线的特定形状,采用全域基和脉冲基相结合的基函数,同时采用渐进抽取方法处理求解过程中遇到的奇异函数积分,将两维无限积分化为一维有限积分,从而大大缩短了计算时间.通过本程序得到的计算结果和实验结果比较一致.数值结果也表明,这种蝶形天线是比普通矩形微带贴片天线面积小很多的一种小型化设计.

  5. Drill-hole data, drill-site geology, and geochemical data from the study of Precambrian uraniferous conglomerates of the Medicine Bow Mountains and Sierra Madre of southeastern Wyoming

    International Nuclear Information System (INIS)

    This volume is presented as a companion to Volume 1: The Geology and Uranium Potential of Precambrian Conglomerates in the Medicine Bow Mountains and Sierra Madre of Southeastern Wyoming; and to Volume 3: Uranium Assessment for Precambrian Pebble Conglomerates in Southeastern Wyoming. Volume 1 summarized the geologic setting and geologic and geochemical characteristics of uranium-bearing conglomerates in Precambrian metasedimentary rocks of southeastern Wyoming. Volume 3 is a geostatistical resource estimate of U and Th in quartz-pebble conglomerates. This volume contains supporting geochemical data, lithologic logs from 48 drill holes in Precambrian rocks of the Medicine Bow Mountains and Sierra Madre, and drill site geologic maps and cross-sections from most of the holes

  6. Fuel pin bowing and related investigation of the gadolinium fuel pin influence on power release inside of neighbouring fuel pins in a WWER-440 type core

    International Nuclear Information System (INIS)

    As known both the WWER-440 and WWER-1000 reactors are systematically modernized to enhance their safety and economical parameters of operation. For this purpose new fuel assemblies (FAs) were designed with improved technical parameters, e.g., containing fuel pins (FPs) in which Gd2O3 burnable absorber is integrated into fuel. Presence of such FPs in reactor core results in a strong depression of thermal neutrons in their positions and corresponding high gradients in neighbouring FPs. Consequently, similar situation in neighbouring FPs can be expected as for both the power release and temperature gradients. The purpose of this work consists in investigation of the gadolinium FP influence on space power distribution, especially from viewpoint of the values and gradient occurrence inside of the neighbouring FPs that could result in static loads with some consequences, e.g., a contribution to FP/FA bowing. Since detailed power distributions cannot be obtained in the NPPs, needed information is provided by means of experiments on research reactors. As for the power release measurement inside of FPs, some special (e.g. track) detectors placed between fuel pellets are usually used. Since such works are relatively complicated and time consuming, an evaluation method based on mathematical modelling and numerical approximation was proposed by means of that, and using measured (integral) power release in selected FPs, needed power release values inside of investigated FPs, can be estimated. For this purpose, experimental results from light water, zero-power research reactor LR-0 obtained by measurements in a WWER-440 type core with 19 FAs at zero boron concentration and containing some FPs with gadolinium (Gd FPs) were utilized. Application of the proposed evaluation method is demonstrated on investigated FPs neighbouring a Gd FP by means of the: relative azimuthal power distribution estimation inside of investigated FPs on their fuel pellet surface in horizontal plane, and

  7. 蝶形天线阵列电磁辐射特性的CBFM分析%Electromagnetic Radiation Characteristics Analysis of Bow-tie Antenna Array Using CBFM

    Institute of Scientific and Technical Information of China (English)

    王国华; 陈治平; 李刚; 段连飞

    2013-01-01

    针对传统矩量法分析天线阵列效率低的问题,给出了一种分析蝶形天线阵列电磁辐射特性的有效数值方法,该方法基于特征基函数法(CBFM )和等效偶极矩法(EDM ),不仅可以加速阻抗矩阵的产生,还可根据特征基函数(CBFs)的阶数和子域的数目调节系数矩阵的维数,从而可以采用直接法求解缩减矩阵方程,与传统矩量法(MoM)相比,显著地减小了运算量。数值结果验证了蝶形天线阵列的方向图并证实了该方法的精确性和有效性。%In view of the problem of low efficiency in analyzing the antenna arrays using the traditional method of moments (MOM),an efficient numerical approach for the electromagnetic radiation characteristics analysis of bow-tie antenna array is presented based on the combination of the characteristic basis function method(CBFM)and the equivalent dipole moment(EDM)method,which can not only accelerate the production of impedance matrix,but also can adjust the size of the coefficient matrix according to the order of CBFs and the number of sub-blocks,thus it is possible to handle the reduced matrix equation by using a direct solution. The computa-tional cost is reduced significantly compared with the traditional MoM. Numerical results validate the radiation pattern of bow-tie antenna array,as well as the efficiency and accuracy of the approach.

  8. Wind-Snow Interactions and Treeline Advance in the Medicine Bow Mountains, Wyoming: A Coupled Examination Using Dendroecology and Remote Sensing

    Science.gov (United States)

    Elliott, G.; Crawford, C. J.

    2014-12-01

    Research suggests that broad-scale increases in temperature facilitated an abrupt initiation of upper treeline advance beginning in the 1950s at climatic treelines throughout a large portion of the southern and central Rocky Mountains. Despite this regional trend, patterns of finer scale variability often imply the likely influence of both wind-snow interactions and temperature on driving regeneration dynamics in these climatically-sensitive ecotones. This is particularly true for mountain ranges subject to consistently strong winds, such as the Medicine Bow Mountains of southeast Wyoming. A rich history of treeline work exists for this area, yet questions remain regarding how influential wind and snowpack variability are in governing climate-vegetation interactions within upper treeline ecotones and whether this varies according to the level of wind exposure. Here we present a coupled examination using dendroecology and remote sensing to test the hypothesis that sufficient snow cover is required in order for the ecological manifestation of increasing temperatures to appear at upper treeline; namely treeline advance. We used dendroecological methods to reconstruct the history of colonization on the two highest peaks in the range (Medicine Bow Peak Massif and Kannaday Peak). We sampled a total of six sites by placing nested-belt transects on two south-facing and one north-facing site for each peak. To gauge the influence of wind-snow interactions at each site, we analyzed remotely-sensed images. We selected three sets of LANDSAT images for each mountain peak based on years with maximum, minimum, and mean snowfall conditions to capture the entire range of variability. Results demonstrate that snow cover can be a critical modifier of treeline advance, especially on wind-exposed slopes and on mountain peaks with a relatively dry hydroclimatology, where a protective snow layer is only evident during high snow years. Overall, this research suggests that the role of wind

  9. 弯曲母线离心叶轮设计方案比较、分析%NUMERICAL INVESTIGATION OF FLOW THROUGH CENTRIFUGAL IMPELLER WITH BOWED BLADES BY THE USING OF THREE-DIMENSIONAL VISCOUS CODE

    Institute of Scientific and Technical Information of China (English)

    赵晓路

    2001-01-01

    A novel geometry generation method for the centrifugal impeller has been developed to design the bowed blade in order to reducethe secondary flow losses within the blade channel[1]. A number of centrifugal impeller has been drafted with the same meridian form and blade loading but different bowing elements of blades.Numerical simulations have been performed to investigate the flow field and performance of these impellers. The numerical experiments shows that the bowing of blades in the first half of channel plays avery important role in reducing secondary flow losses.%为了探讨叶型弯曲不同分布对叶轮效率的影响,本文使用三元粘性数值模拟方法,对几个具有弯曲母线的离心叶轮进行了分析比较,在减损机理、特别是设计准则方面进行了摸索和探讨。

  10. An analysis of a typical bow echo%一次下击暴流显著弓形回波特征

    Institute of Scientific and Technical Information of China (English)

    李胜山; 张殿江; 胡玲; 吴强; 于莉莉

    2012-01-01

    利用天气图、卫星云图和天津新一代天气雷达资料对2007年7月31日凌晨发生在蓟县的强风过程进行分析。结果表明:此次过程是弓形回波与超级单体在合并过程中产生的下击暴流过程而并非龙卷过程。2007年7月30日夜间至31日凌晨,一条自西南向东北方向移动的弓形回波,先后影响天津地区的6个区县产生雷阵雨短时暴雨天气,最大雨强为37.6 mm.h-1,但6个气象站均未出现飑、冰雹和地面大风。对连续观测的雷达资料分析发现,反射率因子图上,显示一条维持了5 h多的弓形回波在移动过程中与一个预先存在低质心的超级单体在蓟县山区合并,产生了下击暴流;反射率因子图上弱回波缺口出现;同时弓形回波形态发生改变,2.4°仰角以上产生断裂;最大雷达反射率因子为53 dBz。在相对径向速度图上,早期呈现为明显的后侧入流急流,后期有中气旋生成并伴有中低层辐散;高层出现强反气旋特征。风暴发展高度较高,回波顶高超过15 km,随着下击暴流的发生,反射率因子核有一个3 km的急降。%Based on the weather charts,satellite cloud images and the new generation weather radar data,a strong wind process on July 31,2007 was analyzed.The results indicate that the process is downburst but not tornadoes,and it is produced by the merger process of the bow echo and supercell.A bow echo moves from southwest to northeast during the night on July 30 to wee hours on July 31,2007,and it makes six districts and counties of Tianjin generating thunder shower and short-time rainstorm.The maximum precipitation intensity reaches 37.6 mm · h-1,while squall,hail and ground gale do not occur in six weather stations.By analyzing the radar data,it shows that the moving bow echo maintaining more than 5 hours merges with a pre-existing supercell in mountain area of Jixian and produces downburst.The weak echo region gap appears in the reflectivity

  11. Also on the Typology of the Bow-shaped Objects and Relevant Issues%也谈弓形器的形制及相关问题

    Institute of Scientific and Technical Information of China (English)

    滕铭予

    2011-01-01

    The "bow-shaped objects" emerged in the Shang and Zhou Dynasties of China,which were used as "rein holders" for the charioteers or riders to free their hands,could be classified into two types: the narrow-backed ones and the wide-backed ones.Observed from%本文讨论的弓形器,是指出现于殷墟时期、一直到西周前期都存在的一种中部有弓背形弧、两端有弧形臂的青铜器。尽管对于这种器物的功能和使用方法还存在诸多不同意见,但因其形状似弓,所以原始报告在描述这种器物时多使用“弓形器”一名,许多学者在讨论这种器物时也多延用“弓形器”

  12. Effects of Bulbous Bow on Cross-Flow Vortex Structures Around a Streamlined Submersible Body at Intermediate Pitch Maneuver:A Numerical Investigation

    Institute of Scientific and Technical Information of China (English)

    Saeed Abedi; Ali Akbar Dehghan; Ali Saeidinezhad; Mojtaba Dehghan Manshadi

    2016-01-01

    A flow field around a streamlined body at an intermediate angle of incidence is dominated by cross-flow separation and vortical flow fields. The separated flow leads to a pair of vortices on the leeside of the body; therefore, it is essential to accurately determine this pair and estimate its size and location. This study utilizes the element-based finite volume method based on RANS equations to compute a 3D axisymmetric flow around a SUBOFF bare submarined hull. Cross-flow vortex structures are then numerically simulated and compared for a submarine with SUBOFF and DRDC STR bows. Computed results of pressure and shear stress distribution on the hull surface and the strength and locations of the vortex structures are presented at an intermediate incidence angle of 20°. A wind tunnel experiment is also conducted to experimentally visualize the vortex structures and measure their core locations. These experimental results are compared with the numerical data, and a good agreement is found.

  13. Phytophilous Chironomidae (Diptera and other macroinvertebrates in the ox-bow Infernão Lake (Jataí Ecological Station, Luiz Antônio, SP, Brazil

    Directory of Open Access Journals (Sweden)

    TRIVINHO-STRIXINO S.

    2000-01-01

    Full Text Available Infernão Lake, located within the Jataí Ecological Station in Luiz Antônio Municipal district (São Paulo State, Brazil, is one of the most typical ox-bow lake of the Mogi-Guaçu River, and it presents, as the main feature, its great quantity of aquatic macrophytes, whose intensive development, in the last years practically covered the whole mirror of water. With the purpose to point out the composition and to establish the relative participation of the phytophilic zoocoenosis that inhabits the different macrophytes of that lake, a collection program of the main vegetation stands was established. The collections, were carried out randomly, during dry season (1994, in stands of Salvinia auriculata, Utricularia sp., Cabomba piauhyensis, Eichhornia azurea and Scirpus cubensis being used specific methodology for each vegetable type. The analysis of the different macrophytes showed the presence of 4,130 macroinvertebrates of 28 families, in which Chironomidae (Diptera and Naididae (Oligochaeta were the most representative, contributing on the average with 51% and 25% of the total fauna. Asheum, Beardius, Chironomus, Goeldichironomus, Parachironomus and Polypedilum were the most abundant Chironomidae genera. Species of the genus Dero (Dero and D. (Aulophorus represented the most typical Naididae of the phytofauna. With clear faunistic gradient from the shore to the center of the lake, the taxocoenosis indicated low similarity (PSc 60% among the associated communities on different vegetables, when grouped into feeding guilds, with expressive participation, in most of the macrophytes, of the collector-gatherers category, except on S. auriculata, whose predators (> 50% and collector-filterers (> 20% dominance turned that zoocoenosis distinct from the others.

  14. Logs and paleoseismic interpretations from trenches 14C and 14D on the Bow Ridge fault, northeastern Yucca Mountain, Nye County, Nevada

    Energy Technology Data Exchange (ETDEWEB)

    Menges, C.M.; Taylor, E.M.; Vadurro, G.; Oswald, J.A.; Cress, R.; Murray, M.; Lundstrom, S.C.; Paces, J.B.; Mahan, S.A.

    1997-12-31

    Detailed studies of trenches 14D and 14C on the Bow Ridge fault indicate two to three displacements and long recurrence intervals during the middle to late Quaternary. The main trace of the fault is marked by a thick (20--40 centimeters wide) subvertical shear zone coated with multiple carbonate-silica laminae and several generations of fine-grained fissure-fill debris. Exposed in the trenches is a vertically stacked sequence of thin (0.3--1.5 meters thick) fine-grained colluvial, alluvial, and eolian deposits that commonly contain smaller wedge-shaped units or several weakly to strongly developed buried paleosols, or both. The two to three surface-rupture events are recognized at discrete stratigraphic intervals in the sequence based on (1) incremental up-section decreases in offset of marker horizons, (b) upward terminations of shear zones, fissure fills, and fractures, and (c) the position of small scarp-derived colluvial wedges deposited adjacent to the fault above downfaulted marker horizons. Preferred estimates of the vertical displacement per event are 12 and 40 centimeters. Left-oblique striations are observed on carbonate fault laminae, which, if tectonic in origin, increase the vertical displacement by factors of 1.1 to 1.7, yielding preferred net slip displacements per event of 13 to 70 centimeters. Thermoluminescence ages of 48 {+-} 20 and 132 {+-} 23 thousand years bracket the ages of the events, which probably occurred near the bounding ages of the time interval. These age constraints suggest long, average recurrence intervals between the three events of 75 to 210 ky; the preferred values range between 100 to 140 ky. The small net cumulative displacement of two dated reference horizons yield very low fault slip rates of 0.002 to 0.007 millimeters per year; the preferred value is 0.003 millimeters per year.

  15. Logs and paleoseismic interpretations from trenches 14C and 14D on the Bow Ridge fault, northeastern Yucca Mountain, Nye County, Nevada

    International Nuclear Information System (INIS)

    Detailed studies of trenches 14D and 14C on the Bow Ridge fault indicate two to three displacements and long recurrence intervals during the middle to late Quaternary. The main trace of the fault is marked by a thick (20--40 centimeters wide) subvertical shear zone coated with multiple carbonate-silica laminae and several generations of fine-grained fissure-fill debris. Exposed in the trenches is a vertically stacked sequence of thin (0.3--1.5 meters thick) fine-grained colluvial, alluvial, and eolian deposits that commonly contain smaller wedge-shaped units or several weakly to strongly developed buried paleosols, or both. The two to three surface-rupture events are recognized at discrete stratigraphic intervals in the sequence based on (1) incremental up-section decreases in offset of marker horizons, (b) upward terminations of shear zones, fissure fills, and fractures, and (c) the position of small scarp-derived colluvial wedges deposited adjacent to the fault above downfaulted marker horizons. Preferred estimates of the vertical displacement per event are 12 and 40 centimeters. Left-oblique striations are observed on carbonate fault laminae, which, if tectonic in origin, increase the vertical displacement by factors of 1.1 to 1.7, yielding preferred net slip displacements per event of 13 to 70 centimeters. Thermoluminescence ages of 48 ± 20 and 132 ± 23 thousand years bracket the ages of the events, which probably occurred near the bounding ages of the time interval. These age constraints suggest long, average recurrence intervals between the three events of 75 to 210 ky; the preferred values range between 100 to 140 ky. The small net cumulative displacement of two dated reference horizons yield very low fault slip rates of 0.002 to 0.007 millimeters per year; the preferred value is 0.003 millimeters per year

  16. Use of safety case to accomplish with Brazilian regulations for drilling units; Uso de caso de seguranca para cumprir com as normas brasileiras para unidades de perfuracao: metodologia Bow Tie

    Energy Technology Data Exchange (ETDEWEB)

    Bardy, Mariana; Silveira, Paula Dias; Oliveira, Katia [Det Norske Veritas (DNV), Rio de Janeiro, RJ (Brazil). Risk Advisory

    2012-07-01

    The last accidents on the industry, mainly after BP accident in Texas City and Macondo blowout, showed and increased the importance of safety barriers on prevention of such events. The safety barriers can be identified in risk analysis studies such as Preliminary Hazard Analysis or HAZOP. But, the identification of safety barriers is not enough, it is necessary to maintain their integrity to guarantee that when demanded they work properly as expected. The methodology presented in this document aim to evaluate the integrity condition of safety barriers and their compliance with the project original characteristics using the Bow Tie and an audit process, and searching for actions that can guarantee the barriers integrity when demanded in a proactive way. The Bow Tie diagrams provide a graphic picture of accidental scenarios, join a relational perspective between event, cause, consequence and barriers, and additionally provide a clear view of possible threats and consequences related with events with high damage potential. The application of methodology described in this document is presented based on a case study related to an accidental release of flammable liquid due to dropped objects on the topside of an offshore unit. Among the benefits identified using this proposed methodology it can be highlighted the possibility to form an integrated overview of management system and of factors that can reduce losses. The Bow Tie diagram provides an overview of process accidents, in several different organization levels, and the integration between different areas responsible for management of different barriers groups. Complementing those diagrams with an audit process it can be determined the real image of company management system related to process safety, which make possible the identification of main points for improvement. (author)

  17. Синтез ультраширокополосной планарной дипольной bow-tie антенны нейронно-генетическим методом

    OpenAIRE

    F. F. Dubrovka; D. O. Vasylenko

    2008-01-01

    Results of a synthesis of the ultrawideband (3.1–10.6 GHz) planar dipole bow-tie antenna are presented. The optimal design is achieved by properly modifying the linear contour profile of the conventional bow-tie antenna. Theoretical results were verified by measurements.

  18. SURVEY, SILVER BOW COUNTY, MT

    Data.gov (United States)

    Federal Emergency Management Agency, Department of Homeland Security — Survey data includes spatial datasets and data tables necessary to digitally represent data collected in the survey phase of the study. (Source: FEMA Guidelines and...

  19. HYDRAULICS, SILVER BOW COUNTY, MONTANA

    Data.gov (United States)

    Federal Emergency Management Agency, Department of Homeland Security — Recent developments in digital terrain and geospatial database management technology make it possible to protect this investment for existing and future projects to...

  20. BASEMAP, SILVER BOW COUNTY, MONTANA

    Data.gov (United States)

    Federal Emergency Management Agency, Department of Homeland Security — FEMA Framework Basemap datasets comprise six of the seven FGDC themes of geospatial data that are used by most GIS applications (Note: the seventh framework theme,...

  1. Peking Opera Takes a Bow

    Institute of Scientific and Technical Information of China (English)

    2011-01-01

    The admission of this art form to the UNESCO Heritage List will boost protection of this national treasure PEKING Opera was recently inscribed on UNESCO’s Representative List of the Intangible Cultural Heritage of Humanity.The decision was made during the fifth session of UNESCO’s Inter-governmental Committee for the Safeguarding of the Intangible Cultural Heritage held at the end of last year in Nairobi,Kenya. At the session,the committee examined 47 nominations from 29

  2. Another string.... but no bow.

    LENUS (Irish Health Repository)

    Green, Connor

    2011-04-01

    Based on a positive personal experience, the authors advocate the use of a wound protector\\/retractor such as the Alexis system in total hip arthroplasty, to avoid intra-operative bacterial contamination from the skin, while avoiding damage to the skin and other soft tissues.

  3. Bow-tie model for offshore drilling blowout accident%海上钻井井喷事故的蝴蝶结模型

    Institute of Scientific and Technical Information of China (English)

    薛鲁宁; 樊建春; 张来斌

    2013-01-01

    海上钻井是一个复杂的动态系统,同时又与一般的过程工业一样,可以划分为清晰的操作步骤和流程,因此安全屏障理论的过程模型非常适合分析海上钻井作业的安全.井喷是海上钻井作业的重要威胁,井喷事故模型对于指导海上钻井安全有重要意义.以安全屏障为基础,利用事故树和事件树分析方法,建立了海上钻井井喷事故的蝴蝶结模型.利用事故树方法分析了井喷事件的原因,通过事件树方法分析了井喷发生后火灾爆炸事故的发展过程.通过将事件原因及事故后果综合为一个模型,操作者可以很直观地了解井喷事故的发生发展过程,进而为其寻找相应的预防及控制措施提供指导.最后将“深水地平线”事故应用于该模型,验证了该模型分析海上钻井井喷事故的有效性.%Offshore drilling is a complex and dynamic system. Meanwhile, like any other process industry, it can also be divided into several independent operating steps and procedures. Therefore, the process model of safety barrier is very suitable to analyze safety of offshore drilling operations. Blowout was an important threat to offshore drilling. A blowout accident model is very meaningful to instruct offshore drilling safety. Based on safety barrier theory, a bow-tie model for offshore drilling blowout was established by utilizing fault tree and event tree methods. Causes of an offshore drilling blowout event were analyzed by fault tree, while development processes of fire & explosion accident after a blowout event were analyzed by event tree. Causes of an offshore drilling blowout event and consequences of fire & explosion accident after the blowout were combined into a single model. This model is very convenient for operators to understand the whole generating and developing process of an offshore drilling blowout accident. Therefore, it can be used as a guide for offshore drilling operators to find relevant

  4. Madeiras utilizadas na fabricação de arcos para instrumentos de corda: aspectos anatômicos Anatomical features of woods used in the manufacture of bows for stringed instruments

    Directory of Open Access Journals (Sweden)

    Veronica Angyalossy

    2005-12-01

    Full Text Available A madeira de pau-brasil (Caesalpinia echinata Lam. é mundialmente empregada na confecção de arcos para instrumentos de corda, uma vez que apresenta características únicas de ressonância, densidade, durabilidade, beleza, entre outras qualidades, que a tornam ideal para tal uso. Diferentes amostras de pau-brasil, contudo, fornecem arcos com qualidades distintas. No comércio nacional outras madeiras estão sendo empregadas na produção de arcos. Realizou-se, neste estudo, uma análise qualitativa e quantitativa de diferentes amostras de pau-brasil com o objetivo de apontar diferenças na estrutura da madeira que possam contribuir para o entendimento das causas da variação na qualidade do arco, além da análise de outras espécies objetivando determinar, do ponto de vista estrutural, semelhanças ou diferenças com o pau-brasil. Conclui-se que variações no diâmetro dos vasos, distribuição e quantidade de parênquima axial e orientação dos elementos axiais e radiais são parâmetros que devem ser considerados quando se busca determinar as causas das diferenças na qualidade dos arcos de pau-brasil. Constatou-se que arcos de boa qualidade apresentam grã linheira e textura fina. Esta última característica decorre da menor proporção de vasos cujo diâmetro é reduzido, raios homogêneos e fibras com paredes espessas e/ou muito espessas. Assim, a relação entre a estrutura e a qualidade do arco está diretamente relacionada com as dimensões, a distribuição e a proporção das células do lenho.Pernambuco wood (Caesalpinia echinata Lam. has special characteristics like resonance, density, durability, and beauty; for this reason, it is considered the best material for stringed instruments bows. Besides pernambuco wood has been used around the world, some samples, and consequently some bows, are better than others. In Brazil, others woody species have been used in the manufacture of bows. In this paper some wood samples of

  5. Quasi-static locomotion planning for rolling mechanism of close chain five-bow-shaped-bar linkage%闭链弓形五连杆机构的准静态翻滚运动规划

    Institute of Scientific and Technical Information of China (English)

    余联庆; 刘晓军; 王玉金; 吴昌林

    2014-01-01

    A rolling mechanism of close chain five-bow-shaped-bar linkage was presented in this paper . By adjusting the shape of the mechanism ,the centroid of the mechanism was offset from the center of the virtual rolling circle corresponding with the bow-shaped-bar which was touching the ground ,and thus the rolling mechanism was self-propelled by the gravitational moment generated from the centroid offset .Firstly ,the structure of close chain five-bow-shaped-bar linkage was designed based on the symmetrical principle so that the centroid of the mechanism coincided with its geometrical centre when the outer contour of the mechanism was round .Secondly ,the quasi-static rolling kinematics of the mechanism was analyzed by close-loop vector method .The relationship between the centroid vector of the mechanism and the joint angles of the two actuators was obtained both in the process of a bar con-tacting the ground and in the moment of a joint contacting the ground .Then ,the trajectory of the centroid vector which could meet the requirement of stable rolling was figured out when the joint con-tacted the ground .Using the strategy of constant centroid offset ,trajectory planning of quasi-static rolling was carried out by least square method .Finally ,a prototype was manufactured ,and the experi-ment results show the feasibility of stable rolling of the close chain five-bow-shaped-bar linkage .%提出一种闭链弓形五连杆机构,当杆件触地时,通过改变自身的形状,使其质心相对于触地杆对应的虚拟滚动圆心发生偏置,产生重力偏置力矩来驱动机构翻滚。首先,利用对称原理进行闭链弓形五连杆结构设计,当其外轮廓为圆形时,机构的质心与形心重合;其次,利用封闭矢量法对机构准静态翻滚过程进行了运动学分析,得到杆件触地过程和关节触地瞬时机构质心矢量与两个驱动关节角的关系;然后,求解关节触地瞬时机构能够实现平稳过

  6. Lithology, fault displacement, and origin of secondary calcium carbonate and opaline silica at Trenches 14 and 14D on the Bow Ridge Fault at Exile Hill, Nye County, Nevada

    International Nuclear Information System (INIS)

    Yucca Mountain, a proposed site for a high-level nuclear-waste repository, is located in southern Nevada, 20 km east of Beatty, and adjacent to the southwest comer of the Nevada Test Site (NTS) (fig. 1). Yucca Mountain is located within the Basin and Range province of the western United States. The climate is semiarid, and the flora is transitional between that of the Mojave Desert to the south and the Great Basin Desert to the north. As part of the evaluation, hydrologic conditions, especially water levels, of Yucca Mountain and vicinity during the Quaternary, and especially the past 20,000 years, are being characterized. In 1982, the US Geological Survey, in cooperation with the US Department of Energy (under interagency agreement DE-A104-78ET44802), excavated twenty-six bulldozer and backhoe trenches in the Yucca Mountain region to evaluate the nature and frequency of Quaternary faulting (Swadley and others, 1984). The trenches were oriented perpendicular to traces of suspected Quaternary faults and across projections of known bedrock faults into Quaternary deposits. Trench 14 exposes the Bow Ridge Fault on the west side of Exile Hill. Although the original purpose of the excavation of trench 14 was to evaluate the nature and frequency of Quaternary faulting on the Bow Ridge Fault, concern arose as to whether or not the nearly vertical calcium carbonate (the term ''carbonate'' in this study refers to calcium carbonate) and opaline silica veins in the fault zone were deposited by ascending waters (ground water). These veins resemble in gross morphology veins commonly formed by hydrothermal processes

  7. Simultaneous measurements of energetic ion (≥50 keV) and electron (≥220 keV) activity upstream of earth's bow shock and inside the plasma sheet: Magnetospheric source for the November 3 and December 3, 1977 upstream events

    International Nuclear Information System (INIS)

    Simultaneous observations of energetic ions (approx-gt 50 keV) and electrons (approx-gt 220 keV) by the IMP 7 and 8 spacecraft, carrying identical instruments and located within the distant (∼37 RE) magnetotail and upstream from the bow shock, have been employed to separate temporal variations from spatial variations during the upstream ion events observed on December 3, 1977 and November 2-3, 1977, in order to determine the source of these particles. The IMP data, when compared with those from ISEE 1 and 2, have also made possible the determination of field-aligned and flux-tube intensity gradients in the upstream region, thus enabling the test of specific predictions of the Fermi acceleration model for such events. The analysis of these three-spacecraft observations and comparison with theory have revealed the following: (1) For each of the observed upstream enhancements, energetic ions and electrons were simultaneously present inside the plasma sheet - successive increases were in excellent time coincidence with substorm injection events seen on ground-based magnetograms; (2) The low-energy (approx-gt 50 keV) ion intensity profile inside the plasma sheet was relatively flat, while at higher (approx-gt 300 keV) energies there was considerable variability, with one case exhibiting an inverse velocity dispersion profile; (3) Relativistic electron bursts were seen inside the plasma sheet and also upstream of the shock but at substantially reduced intensities; (4) The ion energy spectrum for the December 3 event, extended to energies ∼2 MeV, was identical in form within the plasma sheet and upstream of the shock and can be described well by dj/dE ∝ E-5.5; (5) Ion anisotropies exhibited typically large dawn-dusk or dusk-dawn gradients, depending on spacecraft location, and showed large (up to 20:1) field-aligned streaming away from the bow shock

  8. The Design of a Compact Bow-tie UWB Antenna with Band-notch Filter%便携设备中带陷蝶形UWB天线的设计

    Institute of Scientific and Technical Information of China (English)

    蔡文新; 李少甫; 潘建

    2011-01-01

    This paper presents a bow-tie UWB printed antenna with band-notch function.The antenna uses bow-tie patch as the radiating element and is matched with 50 Ω feeder line by the gradient line. Moreover, by cutting the C-shaped slot at the radiating element, the antenna achievs the band-notch function. At last, the results of the simulation and measure are put forward. The antenna with a bandwidth covering the 3.1 ~ 10. 6 GHz can escap the bandwidth of WLAN at 5. 15~5. 825 GHz, and fits for the application of the UWB communication system.%提出了一种应用于便携设备中具有带陷特性的平面蝶形UWB天线.该天线采用蝶形贴片作为辐射单元,并由渐变线作为阻抗变换器与50 Ω馈线进行匹配.通过在辐射面上挖C形槽实现带陷功能,并给出仿真和实测结果.该天线的工作频带覆盖3.1~10.6 GHz,并有效避免了5.15~5.825 GHz的无线局域网(WLAN)频段,适于便携式超宽带无线通信系统的应用.

  9. 成人前臂创伤性骨弯曲的治疗%Treatment of one case of adult forearm traumatic bowing via an evidence-based medicine approach

    Institute of Scientific and Technical Information of China (English)

    相大勇; 余斌; 金丹; 魏宽海; 金明新; 王钢

    2010-01-01

    目的 寻找治疗成人前臂创伤性骨弯曲的最佳方案.方法 收治1例左前臂创伤性骨弯曲患者,男性,21岁;前臂旋后65°,旋前受限.按照循证实践证据检索原则,以获取当前能获得的最佳临床证据.计算机检索Cochrane图书馆(2007年第4期)、MEDLINE(1976年至2009年10月)、ACP Joumal Club(1991年1月至2009年10月)和中国生物医学文献数据库(1979年至2009年1月),查找相关的系统评价、随机对照试验(RCT)和临床回顾性研究、综述、病例报告等,并对所获证据进行质量评价.从而指导本例患者的治疗.结果 未检索到关于手法复位与切开复位比较的系统评价和大样本RCT,因此选择了与临床问题密切相关的5篇回顾性临床研究和1篇病例报告.证据显示对于成人前臂创伤性骨弯曲早期适合手法复位,而晚期及复位困难患者宜行切开复位"楔形"截骨内固定.对本例患者选择切开复位"楔形"截骨内固定治疗,术后7个月随访,左前臂无明显畸形,功能恢复旋前约85°,旋后约75°.结论 本病例的成功治疗得益于循证医学的方法,但尚需大样本、高质量RCT支持.%Objective To find the best therapy plan for an adult patient with forearm traumatic bowing who sought medical help in our department. Methods We searched Cochrane Library(Issue 4,2007),MEDLINE(1976 to October 2009),ACP Journal Club(1991 to October 2008),and CBMDisc (1979 to January 2009)for meta analyses,systematic reviews,randomized controlled trials (RCTs),casecontrol studies.reviews and case reports concerning adult forearm traumatic bowing.The quality of the included studies was assessed. Results We did not find any systematic reviews or large-scale RCTs involving a comparison between manipulative reduction and open reduction and internal fixation in the treatment of traumatic bowing.Five clinical retrospective studies and one case report closely related to our clinical questions were found and assessed

  10. 共面波导馈电的蝶形缝隙天线及其散射特性研究%Study on Bow-Tie Slot Antenna Fed by CPW and Its Scattering Properties

    Institute of Scientific and Technical Information of China (English)

    闫丽云; 张骥; 张文梅

    2013-01-01

    The bow-tie slot antenna fed by coplanar (CPW) is designed.CST 2011 is used to simulate the effect of antenna parameters (such as the length and width of the bow-tie slot and the thickness of the substrate) on the antenna's performance.The optimized antenna has an impedance bandwidth of 770 MHz,gain of 1.2 dB,and good radiation pattern characteristics.Moreover,the scattering property of the proposed antenna was simulated by CST 2011.The peak RCS of 10.67 dBsm appeares at the resonant frequency 2.56 GHz.Besides,RCS of the designed antenna loaded with resistance was calculated and analyzed.The results indicate that RCS of antenna can be reduced by loading an appropriate resistor.%设计了一种共面波导馈电的蝶形缝隙天线.采用CST电磁仿真软件详细分析了天线结构参数(蝶形缝隙的长度L、宽度W和介质基片的厚度h)对天线性能的影响.优化后的天线阻抗带宽为770 MHz(S11<-10 dB),增益为1.2 dB,并具有良好的辐射方向.另外,采用CST计算了天线的雷达散射截面(RCS),结果表明:天线RCS的最大值出现在谐振频率上,为10.67 dBsm,且主极化平面上的RCS值远大于交叉极化平面上的值.最后计算并分析了加载电阻条件下该天线的雷达散射截面,结果表明:适当加载电阻可以缩减天线的RCS.

  11. First-principles study of spontaneous polarization and band gap bowing in ScxAlyGa1−x−yN alloys lattice-matched to GaN

    International Nuclear Information System (INIS)

    First-principles calculations are carried out to estimate the spontaneous polarization and the band gap bowing in the ScxAlyGa1−x−yN alloys lattice-matched to GaN based on the density functional theory together with a pseudopotential plane-wave method. The results indicate nonlinear behavior of the spontaneous polarization and the band gap energies in the ScxAlyGa1−x−yN alloys similar to that in YxAlyGa1−x−yN (Shimada et al 2011 J. Appl. Phys. 110 074114). The band gap energies and the magnitude of the spontaneous polarization of ScxAlyGa1−x−yN is larger than that of YxAlyGa1−x−yN in a wide range of the mole fraction of Ga. We find that the atomic configuration of Sc affects the magnitude of the polarization in ScxAlyGa1−x−yN. Another finding is the apparent deviation from Vegard's law of the lattice constants of the ScxAlyGa1−x−yN alloys lattice-matched to GaN. (paper)

  12. 基于贝叶斯网络的生物质气化中毒事故定量bow-tie分析%Quantitative Bow-Tie Analyses for Biomass Gasification Poisoning Accidents Based on Bayesian Network

    Institute of Scientific and Technical Information of China (English)

    闫放; 许开立; 姚锡文; 王文菁

    2015-01-01

    Fussell-Vesely worth of each event is calculated by Bayesian network .Prevention measures are adopted to the reason event with higher worth .The event tree analysis is conducted to determine control measures and calculate the probability of biomass gasification poisoning accidents before and after measures are taken .Finally the biomass gasification poisoning acci-dents after using bow-tie analysis based on Bayesian network are evaluated by risk assessment matrix .As the result ,this method can reduce probability and risk of accidents by adopting safety measures to parts of the whole points of the system .%本文通过贝叶斯网络计算各原因事件的弗塞-维思利重要度,选取重要度较高的原因事件采取预防措施;并通过事件树分析确定控制措施,计算采取措施前后生物质气化中毒事故发生的概率,最后通过危险性评价矩阵对采取基于贝叶斯网络的bow-tie分析后的生物质气化中毒事故风险进行评价。结果表明,采用该方法只需对系统中部分节点采取安全措施即可有效降低事故发生概率,从而降低事故风险。

  13. 船-冰碰撞载荷下球鼻艏结构动态响应研究%Research on structure dynamic response of bulbous bow in ship-ice collision load

    Institute of Scientific and Technical Information of China (English)

    张健; 万正权; 陈聪

    2014-01-01

    A ship-ice collision numerical simulation is performed by using nonlinear finite element method. Structural dynamic response is carried out by researching the collisions between bulbous bow and ice with the same weight but different shapes, the same shape but different weights and different collision veloci-ties. The regularity of the damage deformation of the ship, the collision force and the energy absorption un-der different working conditions are revealed. The impact mechanism of the shape of ice, the weight of ice and the collision velocity on ship-ice collision is obtained, which provides reference for anti-ice load struc-tural design of ships.%文章利用非线性有限元法对船-冰碰撞进行了数值仿真,分别研究了船舶球鼻艏与同质量不同形状、同形状不同质量冰体发生碰撞以及不同碰撞速度下的动态结构响应特性,揭示了不同工况下船舶的损伤变形、碰撞力和能量吸收的规律,得到了冰体形状、冰体质量、碰撞速度等因素对船-冰碰撞的影响机理,为提高船舶抗冰载荷设计提供参考。

  14. Impact of different tapered function on filter of electromagnetic band gap structure with bow-tie cells%渐变规律对蝶形单元电磁带隙结构滤波器性能的影响

    Institute of Scientific and Technical Information of China (English)

    陈鹏; 田雨波; 彭涛; 沙莎; 彭智慧; 毛云龙

    2011-01-01

    EBG( Electromagnetic Band Gap) structure is widely used in microwave and millimeter-wave fields. Based on the theory of microwave two-port network, the EBG structure filter with bow-tie cells is given in this study, and impact of bow-tie cell with different tapered functions on the filter is discussed. The tapered functions include Bartlett, Welch, Connes, Exponent, Gaussian, Sine, and Hanning. The simulation results show that the EBG structure filter is with maximum attenuation in stop band (35. 77 dB) and maximum relative band-width (55% ) when tapered function of bow-tie cells is Hanning; whereas the EBG structure filter is with minimum and basically symmetrical ripples in pass band (2. 11 dB at lowpass, and 2. 51 dB at highpass).%电磁带隙结构在微波、毫米波波段具有广泛应用.文中给出了一种具有蝶形单元的电磁带隙结构滤波器,采用微波二端口理论讨论了蝶形单元不同渐变规律对滤波器性能的影响,这些渐变规律包括Bartlett,Welch,Connes,Exponent,Gaussian,Sine,Hanning等形式.从仿真计算结果可以看出,当渐变规律为Hanning时,该滤波器具有最大的阻带衰减(35.77 dB)和最大的相对带宽(55%);当渐变规律为Sine时,该滤波器的通带波纹最小且基本对称(低通部分为2.11 dB,高通部分为2.51 dB).

  15. 利用拖尾能量提高蝶形天线辐射效率%Improve the radiation efficiency of bow-tie antenna by exploiting the energy in end reflections

    Institute of Scientific and Technical Information of China (English)

    王建; 黄春琳; 陆珉; 李禹; 粟毅

    2013-01-01

    蝶形天线在探地雷达中已有广泛的运用,但其辐射效率不高的问题一直存在.究其原因,主要是将近70%的辐射能量是以有碍目标探测的拖尾的形式存在.为了保证探测性能,传统上可观的拖尾能量往往以阻抗加载的方式被吸收掉.本文研究发现,当选择双极性单周波作为激励脉冲时,通过优化天线长度可以实现拖尾能量的有效利用,从而显著地提高蝶形天线的辐射效率.仿真实验结果表明,在较远的探测距离上本文方法可以将辐射效率提高近100%.通过实测实验进一步验证了本文方法的有效性.此外,本文所提的方法易于工程实现,工程应用价值十分明显.%The bow-tie antenna,which is widely used in impulse ground penetrating radar (GPR),has very low radiating efficiency.It is because that nearly 70% of the radiated energy exists as the form of end reflection,which is obstructive to probing objects.In order to keep the probing ability,the remarkable energy in end reflections is usually dissipated by resistive loading.Through the current research,it was found that,if the exciting pulse is bipolar and monocycle,the radiation efficiency can be significantly improved by utilizing the energy in end reflection,and the improvement can be implemented by optimizing the antenna length.The simulated results show that the radiation efficiency can be increased by nearly 100%.The measured results validate the proposed method again.Additionally,the proposed method is easy to be carried out in applications and of great use.

  16. Leaders bow heads for synagogue tragedy

    Index Scriptorium Estoniae

    2005-01-01

    4. juulil 1941 põletasid natsid Riias maha sünagoogi, mille käigus võis hukkuda kuni 2000 juuti. 4. juuli mälestustseremoonial osales hulk tipp-poliitikuid ja väliskülalisi, kellele Iisraeli suursaadik Gary Koren pani südamele propageerida antisemitismi null-tolerantsi Lätis

  17. 对GB/T 13096.2-91中弓形试样截面惯性矩计算公式的讨论%DISCUSS THE CALCULATING FORMULA OF MOMENT OF INERTIA FOR BOW-SHAPED TEST PIECE IN GB/T 13096. 2-91

    Institute of Scientific and Technical Information of China (English)

    周祝林; 易洪雷

    2001-01-01

    本文认为GB/T 13096.2-91中计算弓形试样截面惯性矩的公式有误,同时指出在某些手册中有关计算公式也有误。为此作者给出正确的计算公式,并与美国ASTM D4476-85 中的近似公式进行了比较。结果表明大多数情况下,两个公式的计算结果差异在1%以内,由此证明了本文推荐计算公式的合理性。%This paper believes that the calculating formu la of moment of inertia for bow-shaped test piece in GB/T 13096. 2-91 is wrong b ecause of printing error. Correspondingly, the same error appeared in some handb ooks are also pointed out. Furthermore, a right calculating formula is given . The calculating results are compared with the approximate formula in ASTM D4476-85. It shows that the difference between the two formula is less than 1%, thus, the usability of the formula recommended by this paper is proved.

  18. Синтез ультраширокополосной планарной дипольной bow-tie антенны нейронно-генетическим методом

    Directory of Open Access Journals (Sweden)

    F. F. Dubrovka

    2008-05-01

    Full Text Available Представлены результаты синтеза ультраширокополосной (3.1–10.6 ГГц плоской дипольной антенны типа “bow-tie”. Оптимальный дизайн достигается соответствующей модификацией линейного профиля обычной “bow-tie” антенны. Теоретические результаты подтверждены экспериментом.

  19. CERN Takes a Bow at the Montreux Jazz Festival

    CERN Multimedia

    CERN Bulletin

    2013-01-01

    A year after CERN announced the discovery of a Higgs boson on the world stage, several of the participating scientists found themselves in a new and unfamiliar arena – the renowned Montreux Jazz Festival.   The Canettes Blues Band of the CERN Music Club performing live on the Music In The Park stage at the Montreux Jazz Festival, on 18 July. CERN and the Montreux Jazz Foundation teamed up this summer to host a series of seminars and performances titled “The Physics of Music and the Music of Physics”.  The seminars took place in the historic Petit Palais and included a variety of presentations on the interplay between science and sound. Sound artist Bill Fontana kicked off the series by presenting the concepts and methods behind the creation of  “sound sculptures”.  As the current Collide@CERN artist-in-residence, Fontana has been placing microphones and sensors on accelerators, detectors and other objects at CERN t...

  20. The existence and nature of the interstellar bow shock

    CERN Document Server

    Ben-Jaffel, L; Ratkiewicz, R; Grygorczuk, J

    2013-01-01

    We report a new diagnostic between two different states of the local interstellar medium (LISM) near our solar system using a sensitivity study constrained by several distinct and complementary observations of the LISM, solar wind, and inner heliosphere. Assuming the Interstellar Boundary Explorer (IBEX) He flow parameters for the LISM, we obtain a strength of $\\sim 2.7\\pm0.2$ $\\mu$G and a direction pointing away from galactic coordinates $(28, 52)\\pm 3^\\circ$ for the interstellar magnetic field as resulting from fitting Voyager 1 & 2 in situ plasma measurements and IBEX energetic neutral atoms ribbon}. When using Ulysses parameters for the LISM He flow, we recently reported the same direction but a strength of $2.2\\pm0.1$ $\\mu$G. First, we notice that with Ulysses He flow, our solution is in the expected hydrogen deflection plane (HDP). In contrast, for the IBEX He flow, the solution is $\\sim 20^{\\circ}$ away from the corresponding HDP plane. Second, the long-term monitoring of the interplanetary H I flo...

  1. School Management: Norwegian Legacies Bowing to New Public Management

    Directory of Open Access Journals (Sweden)

    Arild Tjeldvoll

    2008-06-01

    Full Text Available The purpose of the study was to investigate the relevance of school management training programmes to current Norwegian education policies and strategies. A specific question was asked: How relevant is the teaching professors’ understanding of school management competence? The findings indicate a split understanding of policy relevant understanding of school management. A majority of respondents had an understanding of school management coherent with the national policies and strategies. A minority did not. They saw the headmaster primarily as a communicative facilitator for teachers’ work, and an ‘administrative caretaker’. In an international perspective the findings represent a Norwegian particularity. There is a collision between Norwegian anti-management legacies of running schools and the Government’s need for effective and accountable management. This may imply a slower speed of implementing educational reforms in Norway.

  2. Multi-spacecraft analysis of terrestrial bow shock

    Czech Academy of Sciences Publication Activity Database

    Krupařová, Oksana; Krupař, Vratislav; Santolík, Ondřej; Souček, Jan; Šafránková, J.; Němeček, Z.; Němec, F.; Maksimovic, M.

    Venice: CAA - ESA, 2015. s. 58. [ Cluster Workshop /25./. 12.10.2015–16.10.2015, Venice] Institutional support: RVO:68378289 Keywords : bowshock * multiple spacecraft * Cluster Subject RIV: BL - Plasma and Gas Discharge Physics http://caa.estec.esa.int/images/ cluster _workshops/25/ Cluster 25_abstract_book4.pdf

  3. Plasmonic eigenmodes in individual and bow-tie graphene nanotriangles

    DEFF Research Database (Denmark)

    Wang, Weihua; Christensen, Thomas; Jauho, Antti-Pekka;

    2015-01-01

    In classical electrodynamics, nanostructured graphene is commonly modeled by the computationally demanding problem of a three-dimensional conducting film of atomic-scale thickness. Here, we propose an efficient alternative two-dimensional electrostatic approach where all calculation procedures ar...

  4. Band gap bowing in quaternary nitride semiconducting alloys

    DEFF Research Database (Denmark)

    Gorczyka, Isabela; Suski, T.; Christensen, Niels Egede;

    2011-01-01

    Structural properties of InxGayAl1−x−yN alloys are derived from total-energy minimization within the local-density approximation (LDA). The electronic properties are studied by band structure calculations including a semiempirical correction for the “LDA gap error.” The effects of varying the...

  5. Current sensors using highly-birefringent bow-tie fibres

    OpenAIRE

    Qian, J.R.; Li, L.

    1986-01-01

    Faraday-effect optical-fibre current sensors have a number of well-known advantages for use in high-voltage transmission systems and other hostile environments. However, these applications have been restricted by the presence of linear birefringence in the fibre which adversely interacts with the Faraday polarisation rotation produced by magnetic fields. Linear birefringence results from (a) intrinsic effects within the fibre (ellipticity, inbuilt thermal-stress) and (b) packaging and co...

  6. Hierarchical modularity of nested bow-ties in metabolic networks

    OpenAIRE

    Luo Jian-Hua; Yu Hong; Zhao Jing; Cao Zhi-Wei; Li Yi-Xue

    2006-01-01

    Abstract Background The exploration of the structural topology and the organizing principles of genome-based large-scale metabolic networks is essential for studying possible relations between structure and functionality of metabolic networks. Topological analysis of graph models has often been applied to study the structural characteristics of complex metabolic networks. Results In this work, metabolic networks of 75 organisms were investigated from a topological point of view. Network decom...

  7. Plasmonic eigenmodes in individual and bow-tie graphene nanotriangles.

    Science.gov (United States)

    Wang, Weihua; Christensen, Thomas; Jauho, Antti-Pekka; Thygesen, Kristian S; Wubs, Martijn; Mortensen, N Asger

    2015-01-01

    In classical electrodynamics, nanostructured graphene is commonly modeled by the computationally demanding problem of a three-dimensional conducting film of atomic-scale thickness. Here, we propose an efficient alternative two-dimensional electrostatic approach where all calculation procedures are restricted to the graphene sheet. Furthermore, to explore possible quantum effects, we perform tight-binding calculations, adopting a random-phase approximation. We investigate multiple plasmon modes in 20 nm equilateral triangles of graphene, treating the optical response classically as well as quantum mechanically. Compared to the classical plasmonic spectrum which is "blind" to the edge termination, we find that the quantum plasmon frequencies exhibit blueshifts in the case of armchair edge termination of the underlying atomic lattice, while redshifts are found for zigzag edges. Furthermore, we find spectral features in the zigzag case which are associated with electronic edge states not present for armchair termination. Merging pairs of triangles into dimers, plasmon hybridization leads to energy splitting that appears strongest in classical calculations while splitting is lower for armchair edges and even more reduced for zigzag edges. Our various results illustrate a surprising phenomenon: Even 20 nm large graphene structures clearly exhibit quantum plasmonic features due to atomic-scale details in the edge termination. PMID:25856506

  8. Sinogram bow-tie filtering in FBP PET reconstruction

    OpenAIRE

    Abella, Mónica; Vaquero, Juan José; Soto-Montenegro, M. L.; Lage, E.; Desco, Manuel

    2009-01-01

    Low-pass filtering of sinograms in the radial direction is the most common practice to limit noise amplification in filtered back projection FBP reconstruction of positron emission tomography studies. Other filtering strategies have been proposed to prevent the loss in resolution due to low-pass radial filters, although results have been diverse. Using the well-known properties of the Fourier transform of a sinogram, the authors defined a binary mask that matches the expected shape of the sup...

  9. Plasmonic eigenmodes in individual and bow-tie graphene nanotriangles

    OpenAIRE

    Weihua Wang; Thomas Christensen; Antti-Pekka Jauho; Thygesen, Kristian S.; Martijn Wubs; N. Asger Mortensen

    2015-01-01

    Serving as a new two-dimensional plasmonic material, graphene has stimulated an intensive study of its optical properties which benefit from the unique electronic band structure of the underlying honeycomb lattice of carbon atoms. In classical electrodynamics, nanostructured graphene is commonly modeled by the computationally demanding problem of a three-dimensional conducting film of atomic-scale thickness. Here, we propose an efficient alternative two-dimensional electrostatic approach wher...

  10. X-ray line emission produced in clump bow shocks

    OpenAIRE

    Cassinelli, Joe P.; Ignace, R.; Waldron, W.; Cho, J.; Murphy, N; Lazarian, A.

    2008-01-01

    We summarize Chandra observations of the emission line profiles from 17 OB stars. The lines tend to be broad and unshifted. The forbidden/intercombination line ratios arising from Helium-like ions provide radial distance information for the X-ray emission sources, while the H-like to He-like line ratios provide X-ray temperatures, and thus also source temperature versus radius distributions. OB stars usually show power law differential emission measure distributions versus temperature. In mod...

  11. Messenger Observations of Mercury's Bow Shock and Magnetopause

    Science.gov (United States)

    Slavin J. A.; Acuna, M. H.; Anderson, B. J.; Benna, M.; Gloeckler, G.; Krimigis, S. M.; Raines, M.; Schriver, D.; Travnicek, P.; Zurbuchen, T. H.

    2008-01-01

    The MESSENGER spacecraft made the first of three flybys of Mercury on January 14.2008 (1). New observations of solar wind interaction with Mercury were made with MESSENGER'S Magnetometer (MAG) (2.3) and Energetic Particle and Plasma Spectrometer (EPPS) - composed of the Energetic Particle Spectrometer (EPS) and Fast Imaging Plasma Spectrometer (FIPS) (3,4). These MESSENGER observations show that Mercury's magnetosphere has a large-scale structure that is distinctly Earth-like, but it is immersed in a comet-like cloud of planetary ions [5]. Fig. 1 provides a schematic view of the coupled solar wind - magnetosphere - neutral atmosphere - solid planet system at Mercury.

  12. Cluster observations of structures at quasi-parallel bow shocks

    Directory of Open Access Journals (Sweden)

    E. A. Lucek

    2004-07-01

    Full Text Available Collisionless quasi-parallel shocks are thought to be composed of a patchwork of short, large-amplitude magnetic structures (SLAMS which act to thermalise the plasma, giving rise to a spatially extended and time varying shock transition. With the launch of Cluster, new observations of the three-dimensional shape and size of shock structures are available. In this paper we present SLAMS observations made when the Cluster tetrahedron scale size was ~100km. The SLAMS magnetic field enhancement is typically well correlated between spacecraft on this scale, although small differences are observed. The statistical characteristics of these differences contain information on the typical gradients of magnetic field changes within the SLAM structure which, in the case studied here, occur on scales of 100-150km, comparable with the upstream ion inertial length.

  13. Bow-tie分析在水煤浆气化工艺中的应用%Application of Bow-tie analysis in coal Slurry Gasification Unit

    Institute of Scientific and Technical Information of China (English)

    刘昌华; 万古军; 李奇; 张广文; 白永忠

    2010-01-01

    @@ 水煤浆气化工艺开发到现在已经有30多年的历史.由于该工艺是在高温高压操作条件下,在炉内发生激烈的氧化还原反应,生成的水煤气属于易燃、易爆的气体,具有极高的危险性.

  14. Ion reflection and downstream thermalization at the quasi-parallel bow shock

    Science.gov (United States)

    Gosling, J. T.; Thomsen, M. F.; Bame, S. J.; Russell, C. T.

    1989-01-01

    Using the results of ISEE 2 plasma and magnetic field measurements, two features related to the ion thermalization process at high-Mach-number (M above 2) quasi-parallel collisionless shocks are discussed. These are the presence of a coherent secondary beam of ions within the shock layer which is considered to be produced by reflection, and downstream ion distributions which contain both a relatively cold core of directly transmitted ions and a hotter 'shell' of ions, which appear to result from the disruption and scattering of ions initially reflected at the shock. Evidence is presented that coherent ion reflection is an important element of the ion energy dissipation process at high-Mach-number quasi-parallel shocks.

  15. Theoretical research program to study chemical reactions in AOTV bow shock tubes

    Science.gov (United States)

    Taylor, Peter R.

    1993-01-01

    The main focus was the development, implementation, and calibration of methods for performing molecular electronic structure calculations to high accuracy. These various methods were then applied to a number of chemical reactions and species of interest to NASA, notably in the area of combustion chemistry. Among the development work undertaken was a collaborative effort to develop a program to efficiently predict molecular structures and vibrational frequencies using energy derivatives. Another major development effort involved the design of new atomic basis sets for use in chemical studies: these sets were considerably more accurate than those previously in use. Much effort was also devoted to calibrating methods for computing accurate molecular wave functions, including the first reliable calibrations for realistic molecules using full CI results. A wide variety of application calculations were undertaken. One area of interest was the spectroscopy and thermochemistry of small molecules, including establishing small molecule binding energies to an accuracy rivaling, or even on occasion surpassing, the experiment. Such binding energies are essential input to modeling chemical reaction processes, such as combustion. Studies of large molecules and processes important in both hydrogen and hydrocarbon combustion chemistry were also carried out. Finally, some effort was devoted to the structure and spectroscopy of small metal clusters, with applications to materials science problems.

  16. 阿基米德螺旋渐开线圆规%Archimedes Corkscrew Bow Compass

    Institute of Scientific and Technical Information of China (English)

    王元荪

    2005-01-01

    设计作图经常会遇到画阿基米德螺旋线的问题,但是作图者却苦于没有画阿基米德螺旋渐开线的专用工具,均是徒手画出,很不标准,很不圆滑,即使用电脑作图,一般的画图软件里也没有阿基米德螺旋渐开线的图形。所以说到目前为止还没有很简单,很实用的阿基米德螺旋渐开线圆规出现,也还没有很好的解决办法。

  17. A comparison of Themis observed bow shock positions with model predictions

    Czech Academy of Sciences Publication Activity Database

    Šimůnek, Jiří; Šafránková, J.; Němeček, Z.

    Prague: International Union of Geodesy and Geophysics, 2015. A33p-005. [ Earth and Environmental Sciences for Future Generations. General Assembly of International Union of Geodesy and Geophysics /26./. 22.06.2015-02.07.2015, Prague] Institutional support: RVO:68378289 Keywords : magnetospheric physics Subject RIV: DG - Athmosphere Sciences, Meteorology http://www.iugg2015prague.com/abstractcd/data/HtmlApp/main.html#

  18. Optical properties of InAlGaAs quantum wells: Influence of segregation and band bowing

    DEFF Research Database (Denmark)

    Jensen, Jacob Riis; Hvam, Jørn Märcher; Langbein, Wolfgang

    1999-01-01

    Knowledge of the quaternary InAlGaAs material system is very limited for the composition range relevant for growth on GaAs substrates. We report on the characterization and modeling of InAlGaAs quantum wells with AlGaAs barriers, grown pseudomorphically on a GaAs substrate with molecular beam...

  19. On the bowing parameter in Cd1-xZnxTe

    International Nuclear Information System (INIS)

    Cd1-xZnxTe thin films were prepared on 7059 Corning glass substrates using an rf magnetron sputtering system and CdTe(1-y)+ZnTe(y) targets. The concentration (x) of Zn in the films did not coincide with the relative weight (y) of the ZnTe powder in the compressed targets. Values of x were in the range 0-0.30 as determined from x-ray diffraction patterns. The band gap energy (Eg) of the Cd1-xZnxTe samples was calculated from the photoreflectance spectra measured on the films. The position of the experimental points in the Eg versus x plot show a deviation from the phenomenological quadratic relation Eg=Eg0+ax+bx2 calculated within the virtual crystal approximation (VCA). The depart of the Eg values for higher Zn concentrations from the expected VCA model is probably due to a larger clustering of Zn atoms and/or a percolation phenomena. We obtain fitted values for the parameters a and b within the VCA approach. Comparison with data reported by other authors is made

  20. F00585: NOS Hydrographic Survey , Bow Mariner Investigation, 2009-11-10

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The National Oceanic and Atmospheric Administration (NOAA) has the statutory mandate to collect hydrographic data in support of nautical chart compilation for safe...

  1. Buffer Bulbous Bows: A Measure to Reduce Oil Spill in Collisions

    DEFF Research Database (Denmark)

    Yamada, Yasuhira

    2007-01-01

    Formålet med denne afhandling at undersøge, hvor meget man ville kunne reducere olieudslip forårsaget af skibskollisioner ved at indføre mindre stærke bulbstævne på verdens skibe. Analysen omfatter såvel deterministiske som probabilistiske metoder. Afhandlingen består af et sammendrag og fem publ...

  2. Numerical Simulation of the Fluid-Structure Interaction of a Surface Effect Ship Bow Seal

    OpenAIRE

    Bloxom, Andrew Lawrence

    2014-01-01

    Numerical simulations of fluid-structure interaction (FSI) problems were performed in an effort to verify and validate a commercially available FSI tool. This tool uses an iterative partitioned coupling scheme between CD-adapco's STAR-CCM+ finite volume fluid solver and Simulia's Abaqus finite element structural solver to simulate the FSI response of a system. Preliminary verification and validation work (VandV) was carried out to understand the numerical behavior of the codes individually an...

  3. Consequences of mis-loading and the power distribution in bowed fuel assemblies

    Energy Technology Data Exchange (ETDEWEB)

    Andersson, Magnus

    2002-04-01

    The thesis is divided in two parts. The first part will investigate consequences of a mis-loaded fuel assembly in Ringhals 3, which is a pressurised water reactor (PWR). The aim of this work is to show that there are no or very small benefits from making an additional flux map at 30 % power in order to detect anomalies. Out of the 17 simulations, there exists only one type of mis-loading, which leads to problems. The case, which leads to problems, is when a Gd fitted assembly changes place with a non Gd. This leads to a too high power peaking factor and increased quadrant power tilt. The gain of a flux map at 30% power is small.

  4. Consequences of mis-loading and the power distribution in bowed fuel assemblies

    International Nuclear Information System (INIS)

    The thesis is divided in two parts. The first part will investigate consequences of a mis-loaded fuel assembly in Ringhals 3, which is a pressurised water reactor (PWR). The aim of this work is to show that there are no or very small benefits from making an additional flux map at 30 % power in order to detect anomalies. Out of the 17 simulations, there exists only one type of mis-loading, which leads to problems. The case, which leads to problems, is when a Gd fitted assembly changes place with a non Gd. This leads to a too high power peaking factor and increased quadrant power tilt. The gain of a flux map at 30% power is small

  5. How the solar wind controls motion and shape of terrestrial bow shock

    Czech Academy of Sciences Publication Activity Database

    Krupařová, Oksana; Krupař, Vratislav; Santolík, Ondřej; Souček, Jan; Šafránková, J.; Němeček, Z.; Němec, F.; Maksimovic, M.

    Weihai: Shandong University, 2015. s. 76. [Solar Wind 14. 22.06.2015-26.06.2015, Weihai] Institutional support: RVO:68378289 Keywords : magnetosphere * solar wind Subject RIV: BL - Plasma and Gas Discharge Physics http://sw14.csp.escience.cn/dct/page/65580

  6. WARM BREEZE FROM THE STARBOARD BOW: A NEW POPULATION OF NEUTRAL HELIUM IN THE HELIOSPHERE

    Energy Technology Data Exchange (ETDEWEB)

    Kubiak, M. A.; Bzowski, M.; Sokół, J. M.; Swaczyna, P.; Grzedzielski, S. [Space Research Centre of the Polish Academy of Sciences, Warsaw (Poland); Alexashov, D. B.; Izmodenov, V. V. [Space Research Institute (IKI) of the Russian Academy of Sciences, Moscow (Russian Federation); Möbius, E.; Leonard, T. [Space Research Center and Department of Physics, University of New Hampshire, Durham, NH (United States); Fuselier, S. A.; McComas, D. J. [Southwest Research Institute, San Antonio, TX (United States); Wurz, P. [Physics Institute, University of Bern, Bern (Switzerland)

    2014-08-01

    We investigate the signals from neutral helium atoms observed in situ from Earth orbit in 2010 by the Interstellar Boundary Explorer (IBEX). The full helium signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral helium that we call the Warm Breeze. The Warm Breeze is approximately 2 times slower and 2.5 times warmer than the primary interstellar He population, and its density in front of the heliosphere is ∼7% that of the neutral interstellar helium. The inflow direction of the Warm Breeze differs by ∼19° from the inflow direction of interstellar gas. The Warm Breeze seems to be a long-term, perhaps permanent feature of the heliospheric environment. It has not been detected earlier because it is strongly ionized inside the heliosphere. This effect brings it below the threshold of detection via pickup ion and heliospheric backscatter glow observations, as well as by the direct sampling of GAS/Ulysses. We discuss possible sources for the Warm Breeze, including (1) the secondary population of interstellar helium, created via charge exchange and perhaps elastic scattering of neutral interstellar He atoms on interstellar He{sup +} ions in the outer heliosheath, or (2) a gust of interstellar He originating from a hypothetic wave train in the Local Interstellar Cloud. A secondary population is expected from models, but the characteristics of the Warm Breeze do not fully conform to modeling results. If, nevertheless, this is the explanation, IBEX-Lo observations of the Warm Breeze provide key insights into the physical state of plasma in the outer heliosheath. If the second hypothesis is true, the source is likely to be located within a few thousand AU from the Sun, which is the propagation range of possible gusts of interstellar neutral helium with the Warm Breeze characteristics against dissipation via elastic scattering in the Local Cloud. Whatever the nature of the Warm Breeze, its discovery exposes a critical new feature of our heliospheric environment.

  7. WARM BREEZE FROM THE STARBOARD BOW: A NEW POPULATION OF NEUTRAL HELIUM IN THE HELIOSPHERE

    International Nuclear Information System (INIS)

    We investigate the signals from neutral helium atoms observed in situ from Earth orbit in 2010 by the Interstellar Boundary Explorer (IBEX). The full helium signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral helium that we call the Warm Breeze. The Warm Breeze is approximately 2 times slower and 2.5 times warmer than the primary interstellar He population, and its density in front of the heliosphere is ∼7% that of the neutral interstellar helium. The inflow direction of the Warm Breeze differs by ∼19° from the inflow direction of interstellar gas. The Warm Breeze seems to be a long-term, perhaps permanent feature of the heliospheric environment. It has not been detected earlier because it is strongly ionized inside the heliosphere. This effect brings it below the threshold of detection via pickup ion and heliospheric backscatter glow observations, as well as by the direct sampling of GAS/Ulysses. We discuss possible sources for the Warm Breeze, including (1) the secondary population of interstellar helium, created via charge exchange and perhaps elastic scattering of neutral interstellar He atoms on interstellar He+ ions in the outer heliosheath, or (2) a gust of interstellar He originating from a hypothetic wave train in the Local Interstellar Cloud. A secondary population is expected from models, but the characteristics of the Warm Breeze do not fully conform to modeling results. If, nevertheless, this is the explanation, IBEX-Lo observations of the Warm Breeze provide key insights into the physical state of plasma in the outer heliosheath. If the second hypothesis is true, the source is likely to be located within a few thousand AU from the Sun, which is the propagation range of possible gusts of interstellar neutral helium with the Warm Breeze characteristics against dissipation via elastic scattering in the Local Cloud. Whatever the nature of the Warm Breeze, its discovery exposes a critical new feature of our heliospheric environment

  8. -To Bow Heads or Shake Hands - : A Study of Direct and Indirect Communication in Chinese Management

    OpenAIRE

    Bellini, Edith

    2007-01-01

    The world-wide globalisation that has taken place during the past decades has led to more Multinational Enterprises (MNEs) choosing to relocate some parts of their organisation to other countries. China, which is in command of the world’s lowest-cost manufacturing plants, is the first destination for MNEs. Although China presents a great opportunity for MNEs, this investment does not come without its difficulties, MNEs wishing to invest in China are confronted with certain challenges. MNEs ar...

  9. "Not Tied Up Neatly with a Bow": Professionals' Challenging Cases in Informed Consent for Genomic Sequencing.

    Science.gov (United States)

    Tomlinson, Ashley N; Skinner, Debra; Perry, Denise L; Scollon, Sarah R; Roche, Myra I; Bernhardt, Barbara A

    2016-02-01

    As the use of genomic technology has expanded in research and clinical settings, issues surrounding informed consent for genome and exome sequencing have surfaced. Despite the importance of informed consent, little is known about the specific challenges that professionals encounter when consenting patients or research participants for genomic sequencing. We interviewed 29 genetic counselors and research coordinators with considerable experience obtaining informed consent for genomic sequencing to understand their experiences and perspectives. As part of this interview, 24 interviewees discussed an informed consent case they found particularly memorable or challenging. We analyzed these case examples to determine the primary issue or challenge represented by each case. Challenges fell into two domains: participant understanding, and facilitating decisions about testing or research participation. Challenges related to participant understanding included varying levels of general and genomic literacy, difficulty managing participant expectations, and contextual factors that impeded participant understanding. Challenges related to facilitating decision-making included complicated family dynamics such as disagreement or coercion, situations in which it was unclear whether sequencing research would be a good use of participant time or resources, and situations in which the professional experienced disagreement or discomfort with participant decisions. The issues highlighted in these case examples are instructive in preparing genetics professionals to obtain informed consent for genomic sequencing. PMID:25911622

  10. Structure of the quasi-parallel bow shock: Results of numerical simulations

    International Nuclear Information System (INIS)

    Quasi-parallel bowshock structures are simulated by using a one-dimensional nonperiodic hybrid code in which the ion dynamics are treated exactly while the electron dynamics are omitted by neglecting the electron inertia (m/sub e/ = 0) and pressure. The simulations are initialized with the upstream condition specified by theta1 = 100, β1 = 0.5, and M/sub A/1 = 2 to 4 with 0.5 increment while the downstream condition is obtained from the Rankine-Hugoniot relations, where theta1 is the angle between the shock normal and the magnetic field, β1 is the ratio of kinetic to magnetic pressures, and M/sub A/1 is the Alfven Mach number. The main results of our simulations follow: (1) For M/sub A/13, the magnetic field profile of the shock is turbulent. The upstream waves are again right-hand polarized whistlers with wavelengths varying from lambdaapprox.310 km upstream to lambda> or approx. =1250 km downstream. The downstream waves are predominantly the right-hand polarized fast magnetosonic waves (ω< or approx. =Ω/sub i/)

  11. Rayleigh Laser Guide Star Systems: UnISIS Bow Tie Shutter and CCD39 Wavefront Camera

    OpenAIRE

    Thompson, Laird A.; Teare, Scott W.; Crawford, Samuel L.; Leach, Robert W.

    2002-01-01

    Laser guide star systems based on Rayleigh scattering require some means to deal with the flash of low altitude laser light that follows immediately after each laser pulse. These systems also need a fast shutter to isolate the high altitude portion of the focused laser beam to make it appear star-like to the wavefront sensor. We describe how these tasks are accomplished with UnISIS, the Rayleigh laser guided adaptive optics system at the Mt. Wilson Observatory 2.5-m telescope. We use several ...

  12. Design of a Bow-Tie Shaped 50 GeV Muon Storage Ring

    CERN Document Server

    Keil, Eberhard

    2000-01-01

    The design of a muon storage ring for a neutrino factory is described. It operates at 50 GeV and has a bowtie shape. It sends neutrino beams from two long straight sections with a small muon beam divergence to two distant detectors at 1000 and 3000 km distance. It is designed for a normalised emittance of about 1.67 mm and an rms momentum spread of 0.5 %. The procedure for arriving at the parameters of the optical modules and of the whole storage ring and their values are given. The verification of the optical design includes tracking many thousands of muons for their lifetime, and demonstrates that the dynamic aperture is larger than the physical one. The parameters of the RF system and of the fast injection kickers are also considered.

  13. Progetto rete di adattamento di un'antenna in microstriscia di tipo Bow-Tie

    OpenAIRE

    Piras, Marcella

    2007-01-01

    Si cerca di ricostruire il profilo di permittivit? di un oggetto, sulla base della misura del campo da esso scatterato, quando viene investito da una radiazione incidente nota (problema dello scattering inverso). L'ispezione dell'oggetto ? non invasiva, in quanto gli esami e i rilievi devono essere condotti impiegando metodi che non alterano il materiale e non richiedono la distruzione o l'asportazione di campioni della struttura in esame. Tra i sensori che vengono utilizzati per questi scopi...

  14. Warm Breeze from the starboard bow: a new population of neutral helium in the heliosphere

    CERN Document Server

    Kubiak, M A; Sokół, J M; Swaczyna, P; Grzedzielski, S; Alexashov, D B; Izmodenov, V V; Moebius, E; Leonard, T; Fuselier, S A; Wurz, P; McComas, D J

    2014-01-01

    We investigate the signals from neutral He atoms observed from Earth orbit in 2010 by IBEX. The full He signal observed during the 2010 observation season can be explained as a superposition of pristine neutral interstellar He gas and an additional population of neutral He that we call the Warm Breeze. The Warm Breeze is approximately two-fold slower and 2.5 times warmer than the primary interstellar He population, and its density in front of the heliosphere is ~7% that of the neutral interstellar helium. The inflow direction of the Warm Breeze differs by ~19deg from the inflow direction of interstellar gas. The Warm Breeze seems a long-term feature of the heliospheric environment. It has not been detected earlier because it is strongly ionized inside the heliosphere, which brings it below the threshold of detection via pickup ion and heliospheric backscatter glow observations, as well as by the direct sampling of GAS/Ulysses. Possible sources for the Warm Breeze include (1) the secondary population of inters...

  15. Language Development and Social Integration in Bromley-by-Bow Nursery.

    Science.gov (United States)

    Maxwell, Shirley; And Others

    1993-01-01

    Describes a project being piloted in a nursery school in east London that offers the opportunity for children between 18 months and 3 years of age from multiethnic communities to learn English. The project encourages parent participation. Profiles one girl who is participating in the project, and suggests that the aims of the project are being…

  16. H2S in the L1157-B1 Bow Shock

    Science.gov (United States)

    Holdship, Jonathan; Viti, Serena; Jimenez-Serra, Izaskun; Lefloch, Bertrand; Codella, Claudio; Podio, Linda; Benedettini, Milena; Fontani, Francesco; Bachiller, Rafael; Tafalla, Mario; Ceccarelli, Cecilia

    2016-08-01

    Sulfur-bearing molecules are highly reactive in the gas phase of the ISM. However, the form in which most of the sulfur is locked onto interstellar dust grains is unknown. By taking advantage of the short time-scales of shocks in young molecular outflows, one could track back the main form of sulfur in the ices. In this paper, six transitions of H2S and its isotopologues in the L1157-B1 bowshock have been detected using data from the Herschel-CHESS survey and the IRAM-30m ASAI large program. These detections are used to calculate the properties of H2S gas in L1157-B1 through use of a rotation diagram and to explore the possible carriers of sulfur on the grains. The isotopologue detections allow the first calculation of the H2S deuteration fraction in an outflow from a low mass protostar. The fractional abundance of H2S in the region is found to be 6.0× 10-7 and the deuteration fraction is 2× 10-2. In order to investigate the form of sulfur on the grains, a chemical model is run with four different networks, each with different branching ratios for the freeze out of sulfur bearing species into molecules such as OCS and H2S. It is found that the model best fits the data when at least half of each sulfur bearing species hydrogenates when freezing. We therefore conclude that a significant fraction of sulfur in L1157-B1 is likely to be locked in H2S on the grains.

  17. Bowing in the Right Direction: Hiland Mountain Correctional Center Women's String Orchestra Programme

    Science.gov (United States)

    Warfield, Duane

    2010-01-01

    The Hiland Mountain Correctional Center, a 400-bed facility for multi-level adult female offenders in Eagle River, Alaska, offers a unique educational programme to its prisoners: an orchestra. Founded in 2003, by volunteer Pati Crofut, orchestra membership grew from eight to 22 female offenders between 2003 and 2009. Crofut has devoted her time…

  18. H2S in the L1157-B1 Bow shock

    CERN Document Server

    Holdship, Jonathan; Jimenez-Serra, Izaskun; Lefloch, Bertrand; Codella, Claudio; Podio, Linda; Benedettini, Milena; Fontani, Francesco; Bachiller, Rafael; Tafalla, Mario; Ceccarelli, Cecilia

    2016-01-01

    Sulfur-bearing molecules are highly reactive in the gas phase of the ISM. However, the form in which most of the sulfur is locked onto interstellar dust grains is unknown. By taking advantage of the short time-scales of shocks in young molecular outflows, one could track back the main form of sulfur in the ices. In this paper, six transitions of H$_2$S and its isotopologues in the L1157-B1 bowshock have been detected using data from the Herschel-CHESS survey and the IRAM-30m ASAI large program. These detections are used to calculate the properties of H$_2$S gas in L1157-B1 through use of a rotation diagram and to explore the possible carriers of sulfur on the grains. The isotopologue detections allow the first calculation of the H$_2$S deuteration fraction in an outflow from a low mass protostar. The fractional abundance of H$_2$S in the region is found to be 6.0$\\times$10$^{-7}$ and the deuteration fraction is 2$\\times$10$^{-2}$. In order to investigate the form of sulfur on the grains, a chemical model is r...

  19. Classification of magnetized star--planet interactions: bow shocks, tails, and inspiraling flows

    CERN Document Server

    Matsakos, Titos; Königl, Arieh

    2015-01-01

    Close-in exoplanets interact with their host stars gravitationally as well as via their magnetized plasma outflows. The rich dynamics that arises may result in distinct observable features. Our objective is to study and classify the morphology of the different types of interaction that can take place between a giant close-in planet (a Hot Jupiter) and its host star, based on the physical parameters that characterize the system. We perform 3D magnetohydrodynamic numerical simulations to model the star--planet interaction, incorporating a star, a Hot Jupiter, and realistic stellar and planetary outflows. We explore a wide range of parameters and analyze the flow structures and magnetic topologies that develop. Our study suggests the classification of star--planet interactions into four general types, based on the relative magnitudes of three characteristic length scales that quantify the effects of the planetary magnetic field, the planetary outflow, and the stellar gravitational field in the interaction region...

  20. Controllable strain-induced uniaxial anisotropy of Fe81Ga19 films deposited on flexible bowed-substrates

    Science.gov (United States)

    Dai, Guohong; Zhan, Qingfeng; Yang, Huali; Liu, Yiwei; Zhang, Xiaoshan; Zuo, Zhenghu; Chen, Bin; Li, Run-Wei

    2013-11-01

    We propose a convenient method to induce a uniaxial anisotropy in magnetostrictive Fe81Ga19 films grown on flexible polyethylene terephthalate (PET) substrates by bending the substrate prior to deposition. A tensile/compressive stress is induced in the Fe81Ga19 films when PET substrates are shaped from concave/convex to flat after deposition. The stressed Fe81Ga19 films exhibit a significant uniaxial magnetic anisotropy due to the internal stress arising from changes in shape of PET substrates. The easy axis is along the tensile stress direction and the coercive field along easy axis is increased with increasing the internal tensile stress. The remanence of hard axis is decreased with increasing the compressive stress, while the coercive field is almost unchanged. A modified Stoner-Wohlfarth model with considering the distribution of easy axes in polycrystalline films is used to account for the magnetic properties tuned by the strain-controlled magnetoelastic anisotropy in flexible Fe81Ga19 films. Our investigations provide a convenient way to induce uniaxial magnetic anisotropy, which is particularly important for fabricating flexible magnetoelectronic devices.

  1. A dynamics of the trainings loadings of highly skilled shooters is from a bow in precompetytion middle cycle

    Directory of Open Access Journals (Sweden)

    Briskin Yu.A.

    2010-08-01

    Full Text Available Quantity indicators of shots of sportsmen in building blocks of a mesocycle are defined. The qualifying determined dynamic of volumes of training loads of sportsmen fixed. Research was conducted with the participation 16 sportsmen of a combined team of Ukraine. The precompetitive mesocycle powered up 3 microcycle (2 failing and 1 regenerative. Duration of 2 first microcycle constituted 5 days (4 training and 1 assigned for "repose" and the third - one training day. It fixed, that the volume of a training load has undulating positive dynamic from the beginning before his completion. Correlations of qualification of sportsmen and volumes of a training load (r = 0,39-0,63 in different building blocks of a mesocycle fixed.

  2. 75 FR 74678 - Medicine Bow-Routt National Forests and Thunder Basin National Grassland; Colorado and Wyoming...

    Science.gov (United States)

    2010-12-01

    ..., mechanical, biological, and cultural weed treatments. The MBRTB is currently treating noxious weeds and..., ] reduces species diversity, increases soil erosion due to a decrease in surface cover, and promotes... Executive Order 13112). Effects analysis of treatments of invasive plants, including cheatgrass...

  3. The CHESS survey of the L1157-B1 bow-shock: high and low excitation water vapor

    CERN Document Server

    Busquet, G; Benedettini, M; Ceccarelli, C; Codella, C; Cabrit, S; Nisini, B; Viti, S; Gómez-Ruiz, A I; Gusdorf, A; di Giorgio, A M; Wiesenfeld, L

    2013-01-01

    Molecular outflows powered by young protostars strongly affect the kinematics and chemistry of the natal molecular cloud through strong shocks resulting in substantial modifications of the abundance of several species. As part of the "Chemical Herschel Surveys of Star forming regions" guaranteed time key program, we aim at investigating the physical and chemical conditions of H20 in the brightest shock region B1 of the L1157 molecular outflow. We observed several ortho- and para-H2O transitions using HIFI and PACS instruments on board Herschel, providing a detailed picture of the kinematics and spatial distribution of the gas. We performed a LVG analysis to derive the physical conditions of H2O shocked material, and ultimately obtain its abundance. We detected 13 H2O lines probing a wide range of excitation conditions. PACS maps reveal that H2O traces weak and extended emission associated with the outflow identified also with HIFI in the o-H2O line at 556.9 GHz, and a compact (~10") bright, higher-excitation ...

  4. Bow has its short, crossbow has its long 弓亦有所短 弩亦有所长

    DEFF Research Database (Denmark)

    wu, zheng; Dai, Zheng

    2009-01-01

    There are two kinds of designer can be hired for a project. They are freelancer designer or designer in company. From designer’s perspective, they would consider about several aspects. The big fame could not equal to a big team. Designer could finish a project individually. The standard of good a...

  5. Experimental and Numerical Analysis of Hull Girder Vibrations and Bow Impact of a Large Ship Sailing in Waves

    Directory of Open Access Journals (Sweden)

    Jialong Jiao

    2015-01-01

    Full Text Available It is of great importance to evaluate the hull structural vibrations response of large ships in extreme seas. Studies of hydroelastic response of an ultra large ship have been conducted with comparative verification between experimental and numerical methods in order to estimate the wave loads response considering hull vibration and water impact. A segmented self-propelling model with steel backbone system was elaborately designed and the experiments were performed in a tank. Time domain numerical simulations of the ship were carried out by using three-dimensional nonlinear hydroelasticity theory. The results from the computational analyses have been correlated with those from model tests.

  6. Guitar with a bow: a jet-like X-ray-emitting feature associated a fast-moving pulsar

    Science.gov (United States)

    Wang, Q. Daniel

    2011-09-01

    The Guitar Nebula is known to be a ram-pressure confined pulsar wind nebula associated with the very fast-moving pulsar B2224+65. Existing observations at two epochs have shown an unexpected 2 arcmin long X-ray-emitting jet-like feature emanating from the pulsar and offset from its proper motion direction by 118 degree. We propose a deep third epoch observation of this system in order to measure the X-ray spectral gradient across the feature as well as to confirm its proper motion, its morphological variation with time, and the presence of a counter jet. We will then critically test scenarios proposed to explain this system, which represents a class of similarly enigmatic objects recently discovered locally and in the central region of our Galaxy.

  7. The Use of Anterolateral Bowing of the Lower Leg in the Diagnostic Criteria for Neurofibromatosis Type 1

    OpenAIRE

    Stevenson, David A.; VISKOCHIL, DAVID H.; Schorry, Elizabeth K.; Crawford, Alvin H; D’Astous, Jacques; Murray, Kathleen A.; Friedman, J M; Armstrong, Linlea; Carey, John C.

    2007-01-01

    Neurofibromatosis type 1 (NF1) is diagnosed clinically based on the presence of 2 of 7 criteria developed by a panel of experts in 1987. The sixth criterion focuses on skeletal findings and is as follows: “A distinctive osseous lesion such as sphenoid dysplasia or thinning of long bone cortex, with or without pseudarthrosis.” The wording for this criterion is misleading. In particular, “thinning of long bone cortex” is not the characteristic radiographic presentation, and no mention of long b...

  8. 76 FR 9320 - Foreign-Trade Zone 274-Butte-Silver Bow, MT; Application for Manufacturing Authority REC Silicon...

    Science.gov (United States)

    2011-02-17

    ... facility (300 employees, 3,450 metric ton capacity) is located within Site 1 of FTZ 274. The facility is used for the manufacturing of polysilicon and silane gas for the photovoltaic industry using domestic... duty orders into the facility and would accept a restriction on such admissions. FTZ procedures...

  9. Network, degeneracy and bow tie. Integrating paradigms and architectures to grasp the complexity of the immune system

    OpenAIRE

    Tieri Paolo; Grignolio Andrea; Zaikin Alexey; Mishto Michele; Remondini Daniel; Castellani Gastone C; Franceschi Claudio

    2010-01-01

    Abstract Recently, the network paradigm, an application of graph theory to biology, has proven to be a powerful approach to gaining insights into biological complexity, and has catalyzed the advancement of systems biology. In this perspective and focusing on the immune system, we propose here a more comprehensive view to go beyond the concept of network. We start from the concept of degeneracy, one of the most prominent characteristic of biological complexity, defined as the ability of struct...

  10. Application of the Bow-Tie model in medication safety risk analysis: Consecutive experience in two hospitals in the Netherlands

    NARCIS (Netherlands)

    P.C. Wierenga; L. Lie-A-Huen; S.E. de Rooij; N.S. Klazinga; H.J. Guchelaar; S.M. Smorenburg

    2009-01-01

    Background: To improve medication safely effectively, one should systematically analyse and assess the risks for medication errors and determine the possible causes. So far, no risk-analysis instrument exists in healthcare that can be used to analyse and visualize risks, causes and consequences of p

  11. Application of the Bow-Tie model in medication safety risk analysis : consecutive experience in two hospitals in the Netherlands

    NARCIS (Netherlands)

    Wierenga, Peter C; Lie-A-Huen, Loraine; de Rooij, Sophia E; Klazinga, Niek S; Guchelaar, Henk-Jan; Smorenburg, Susanne M

    2009-01-01

    BACKGROUND: To improve medication safety effectively, one should systematically analyse and assess the risks for medication errors and determine the possible causes. So far, no risk-analysis instrument exists in healthcare that can be used to analyse and visualize risks, causes and consequences of p

  12. 柱面共形蝶形微带天线%Cylindrical Conformal Bow-Tie Microstrip Antenna

    Institute of Scientific and Technical Information of China (English)

    牛俊伟; 钟顺时

    2003-01-01

    研究了共形于小曲率半径圆柱体的蝶形微带天线,首先计算了平面蝶形微带天线,然后对不同圆柱半径下天线的反射损耗和方向图进行了仿真,与文献结果进行了比较,验证了程序的有效性.表明,当圆柱半径较小于一个波长时,随着圆柱半径的减小,天线谐振频率有所下降,阻抗带宽有所减小,而且方向图有较大变化.

  13. A new rectenna circuit using a bow-tie antenna for the conversion of microwave power to dc power

    Science.gov (United States)

    Tran, Michael; Nguyen, Cam

    1993-01-01

    The novel rectenna circuit presented, which integrated a bowtie antenna with a diode, is capable of broadband, high-efficiency operation, and is insensitive to incident field angle. The device is noted, moreover, to behave as a lowpass filter for dc output. For 2.45 GHz operation, a 79-percent conversion efficiency has been demonstrated.

  14. A Bow-Tie Genetic Architecture for Morphogenesis Suggested by a Genome-Wide RNAi Screen in Caenorhabditis elegans

    OpenAIRE

    Nelson, Matthew D.; Elinor Zhou; Karin Kiontke; Hélène Fradin; Grayson Maldonado; Daniel Martin; Khushbu Shah; Fitch, David H. A.

    2011-01-01

    During animal development, cellular morphogenesis plays a fundamental role in determining the shape and function of tissues and organs. Identifying the components that regulate and drive morphogenesis is thus a major goal of developmental biology. The four-celled tip of the Caenorhabditis elegans male tail is a simple but powerful model for studying the mechanism of morphogenesis and its spatiotemporal regulation. Here, through a genome-wide post-embryonic RNAi-feeding screen, we identified 2...

  15. Flux-based classification of reactions reveals a functional bow-tie organization of complex metabolic networks

    OpenAIRE

    Singh, Shalini; Samal, Areejit; Giri, Varun; Krishna, Sandeep; Raghuram, Nandula; Jain, Sanjay

    2012-01-01

    Unraveling the structure of complex biological networks and relating it to their functional role is an important task in systems biology. Here we attempt to characterize the functional organization of the large-scale metabolic networks of three microorganisms. We apply flux balance analysis to study the optimal growth states of these organisms in different environments. By investigating the differential usage of reactions across flux patterns for different environments, we observe a striking ...

  16. Bow Ties in the Sky I: The Angular Structure of Inverse Compton Gamma-ray Halos in the Fermi Sky

    CERN Document Server

    Broderick, Avery E; Shalaby, Mohamad; Pfrommer, Christoph; Puchwein, Ewald; Chang, Philip; Lamberts, Astrid

    2016-01-01

    Extended inverse Compton halos are generally anticipated around extragalactic sources of gamma rays with energies above 100 GeV. These result from inverse Compton scattered cosmic microwave background photons by a population of high-energy electron/positron pairs produced by the annihilation of the high-energy gamma rays on the infrared background. Despite the observed attenuation of the high-energy gamma rays, the halo emission has yet to be directly detected. Here, we demonstrate that in most cases these halos are expected to be highly anisotropic, distributing the up-scattered gamma rays along axes defined either by the radio jets of the sources or oriented perpendicular to a global magnetic field. We present a pedagogical derivation of the angular structure in the inverse Compton halo and provide an analytic formalism that facilitates the generation of mock images. We discuss exploiting this fact for the purpose of detecting gamma-ray halos in a set of companion papers.

  17. Rupture Analysis of Oil Tankers in a Side Collision:Global Structural Model of Bow Indentation into Ship Side

    OpenAIRE

    Wierzbicki, Tomasz; Simonsen, Bo Cerup

    1996-01-01

    Since the pioneering work of Minorsky in 1958 the collision damage of ships has been extensively studied in literature. In the past few yearsthere has been renewed interest in this type of problem, as exemplified by for example [4], [7]. For a complete review of the subject, the reader is referred to the work by Jones, [4], and subsequent reports of the International Ship Structure Committees. Three main approachesemerged in the literature. The empirically based methods (Minorsky, Woisin), th...

  18. Magnetosheath plasma stability and ULF wave occurrence as a function of location in the magnetosheath and upstream bow shock parameters

    Czech Academy of Sciences Publication Activity Database

    Souček, Jan; Escoubet, C. P.; Grison, Benjamin

    2015-01-01

    Roč. 120, č. 4 (2015), s. 2838-2850. ISSN 2169-9380 R&D Projects: GA ČR(CZ) GAP209/12/2394 Institutional support: RVO:68378289 Keywords : magnetosheath * mirror modes * plasma waves Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 3.440, year: 2013 http://onlinelibrary.wiley.com/doi/10.1002/2015JA021087/full

  19. "It's Just Like an Extra String to Your Bow": Exploring Higher Education Students' Perceptions and Experiences of Extracurricular Activity and Employability

    Science.gov (United States)

    Thompson, Leanne J.; Clark, Gordon; Walker, Marion; Whyatt, J. Duncan

    2013-01-01

    Students' experience of higher education comprises not only their academic studies but also their extracurricular activities. This article reports on the findings from a mixed-methods research project, exploring in detail the nature and value of extracurricular activity engagement and the significance of institutional schemes encouraging…

  20. Responsibility of a Filament Eruption for the Initiation of a Flare, CME, and Blast Wave, and its Possible Transformation into a Bow Shock

    OpenAIRE

    Grechnev, V. V.; Uralov, A. M.; Kuzmenko, I. V.; Kochanov, A. A.; Chertok, I. M.; Kalashnikov, S. S.

    2014-01-01

    Multi-instrument observations of two filament eruptions on 24 February and 11 May 2011 suggest the following updated scenario for eruptive flare, CME and shock wave evolution. An initial destabilization of a filament results in stretching out of magnetic threads belonging to its body and rooted in the photosphere along the inversion line. Their reconnection leads to i) heating of parts of the filament or its environment, ii) initial development of the flare arcade cusp and ribbons, and iii) i...