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Sample records for satelite experiment pamela

  1. Random vibration tests of the anticoincidence system of the PAMELA satellite experiment

    CERN Document Server

    Pearce, M; Lundin, M; Lundqvist, J M

    2002-01-01

    PAMELA is a general purpose cosmic ray satellite experiment which will be launched early in 2003. An anticoincidence system surrounds the PAMELA silicon tracker to reject particles not clearly entering the acceptance of the experiment. The engineering model of the PAMELA anticounter system uses plastic scintillator which is read out by Hamamatsu R5900U photomultipliers. The anticounters have been subjected to the random vibration spectrum expected during the launch of PAMELA. The integrated amplitude experienced by the photomultipliers was O(20) g RMS. No degradation to the photomultiplier operation or mechanical assembly was observed.

  2. Data processing and distribution in the PAMELA experiment

    International Nuclear Information System (INIS)

    Casolino, M.; Nagni, M.

    2007-01-01

    YODA is a semi-automated data handling and analysis system for the PAMELA space experiment. The core of the routines have been developed to process a stream of raw data downlinked from the Resurs DK1 satellite (housing PAMELA) to the ground station in Moscow. Raw data consist of scientific data and engineering information. Housekeeping information are analyzed in a short time from download (∼hours) in order to monitor the status of the experiment and for the mission planning. A prototype for the data visualization runs on an APACHE TOMCAT web application server, providing an off-line analysis tool using a browser and part of code for the system maintenance. A quicklook system with GUI interface is used for operator monitoring and fast macrocommand issuing. On a longer timescale scientific data are analyzed, calibrations performed and the database adjourned. The data storage core is composed of CERN's ROOT files structure and MySQL as a relational database. YODA++ is currently being used in the integration and testing of ground PAMELA data

  3. Results from PAMELA

    International Nuclear Information System (INIS)

    Mocchiutti, E.; Adriani, O.; Barbarino, G.C.; Bazilevskaya, G.A.; Bellotti, R.; Boezio, M.; Bogomolov, E.A.; Bonechi, L.; Bongi, M.; Bonvicini, V.; Borisov, S.; Bottai, S.; Bruno, A.; Cafagna, F.; Campana, D.

    2011-01-01

    The PAMELA satellite experiment was launched into low earth orbit on June 15th 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.

  4. Investigations of Forbush decreases in the PAMELA experiment

    Science.gov (United States)

    Lagoida, I. A.; Voronov, S. A.; Mikhailov, V. V.

    2017-01-01

    A phenomenon in cosmic ray physics now called Forbush decrease (FD), or Forbush effect was discovered by S. Forbush in 1937 [1], it is a sudden decrease of galactic cosmic ray (GCR) intensity near the Earth. However, despite of the long term investigations the nature of this phenomenon is still not completely understood. Today this effect is studied mostly by the neutron monitors and muon hodoscopes, which are located on the Earth’s surface. But these monitors can detect only products of GCR interaction with the Earth atmosphere. Satellite detectors allow to obtain more accurate information about the characteristics of FD. Examples of FDs registered by the PAMELA telescope and observed with Oulu neutron monitor are presented. About 10 events with amplitude more than 3% have been registered from 2006 till 2016 with the PAMELA experiment.

  5. Magnetospheric and solar physics observations with the PAMELA experiment

    International Nuclear Information System (INIS)

    Casolino, M.; Adriani, O.; Ambriola, M.; Barbarino, G.C.; Basili, A.; Bazilevskaja, G.A.; Boezio, M.; Bogomolov, E.A.; Bonechi, L.; Bongi, M.; Bonvicini, V.; Bruno, A.; Cafagna, F.; Campana, D.; Carlson, P.; Castellini, G.

    2008-01-01

    PAMELA is a satellite-borne experiment designed to make long duration measurements of the cosmic radiation in Low Earth Orbit. It is devoted to the detection of the cosmic-ray spectra in the 100 MeV-300 GeV range with primary scientific goal the measurement of antiproton and positron spectra over the largest energy range ever achieved. Other tasks include the search for antinuclei with unprecedented sensitivity and the measurement of the light nuclear component of cosmic rays. In addition, PAMELA can investigate phenomena connected with solar and Earth physics. The apparatus consists of: a Time of Flight system, a magnetic spectrometer, an electromagnetic imaging calorimeter, a shower tail catcher scintillator, a neutron detector and an anticoincidence system. In this work we present some measurements of galactic, secondary and trapped particles performed in the first months of operation

  6. Magnetospheric and solar physics observations with the PAMELA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Casolino, M. [INFN, Structure of Rome ' Tor Vergata' and Physics Department of University of Rome ' Tor Vergata' , Via della Ricerca Scientifica 1, I-00133 Rome (Italy)], E-mail: Marco.Casolino@roma2.infn.it; Adriani, O. [INFN, Structure of Florence and Physics Department of University of Florence, Via Sansone 1, I-50019 Sesto Fiorentino, Florence (Italy); Ambriola, M. [INFN, Structure of Bari and Physics Department of University of Bari, Via Amendola 173, I-70126 Bari (Italy); Barbarino, G.C. [INFN, Structure of Naples and Physics Department of University of Naples ' Federico II' , Via Cintia, I-80126 Naples (Italy); Basili, A. [INFN, Structure of Rome ' Tor Vergata' and Physics Department of University of Rome ' Tor Vergata' , Via della Ricerca Scientifica 1, I-00133 Rome (Italy); Bazilevskaja, G.A. [Lebedev Physical Institute, Leninsky Prospekt 53, RU-119991 Moscow (Russian Federation); Boezio, M. [INFN, Structure of Trieste and Physics Department of University of Trieste, Via A. Valerio 2, I-34127 Trieste (Italy); Bogomolov, E.A. [Ioffe Physical Technical Institute, Polytekhnicheskaya 26, RU-194021 St. Petersburg (Russian Federation); Bonechi, L.; Bongi, M. [INFN, Structure of Florence and Physics Department of University of Florence, Via Sansone 1, I-50019 Sesto Fiorentino, Florence (Italy); Bonvicini, V. [INFN, Structure of Trieste and Physics Department of University of Trieste, Via A. Valerio 2, I-34127 Trieste (Italy); Bruno, A.; Cafagna, F. [INFN, Structure of Bari and Physics Department of University of Bari, Via Amendola 173, I-70126 Bari (Italy); Campana, D. [INFN, Structure of Naples and Physics Department of University of Naples ' Federico II' , Via Cintia, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, Albanova University Centre, SE-10691 Stockholm (Sweden); Castellini, G. [IFAC, Via Madonna del Piano 10, I-50019 Sesto Fiorentino, Florence (Italy)] (and others)

    2008-04-01

    PAMELA is a satellite-borne experiment designed to make long duration measurements of the cosmic radiation in Low Earth Orbit. It is devoted to the detection of the cosmic-ray spectra in the 100 MeV-300 GeV range with primary scientific goal the measurement of antiproton and positron spectra over the largest energy range ever achieved. Other tasks include the search for antinuclei with unprecedented sensitivity and the measurement of the light nuclear component of cosmic rays. In addition, PAMELA can investigate phenomena connected with solar and Earth physics. The apparatus consists of: a Time of Flight system, a magnetic spectrometer, an electromagnetic imaging calorimeter, a shower tail catcher scintillator, a neutron detector and an anticoincidence system. In this work we present some measurements of galactic, secondary and trapped particles performed in the first months of operation.

  7. Analysis on H spectral shape during the early 2012 SEPs with the PAMELA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Martucci, M., E-mail: matteo.martucci@roma2.infn.it [University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome (Italy); INFN, Laboratori Nazionali di Frascati, Via Enrico Fermi 40, I-00044 Frascati (Italy); Boezio, M. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bravar, U. [Space Science Center, University of New Hampshire (United States); Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Christian, E.R.; De Nolfo, G.A. [Heliospheric Physics Laboratory, NASA/Goddard Space Flight Center (United States); Mergè, M. [INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome (Italy); University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome (Italy); Mocchiutti, E. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Munini, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); University of Trieste, Department of Physics, I-34147 Trieste (Italy); Ricci, M. [INFN, Laboratori Nazionali di Frascati, Via Enrico Fermi 40, I-00044 Frascati (Italy); Ryan, J.M. [Space Science Center, University of New Hampshire (United States); Sotgiu, A. [University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome (Italy); Stochaj, S. [Electrical and Computer Engineering, New Mexico State University (United States); Thakur, N. [Heliospheric Physics Laboratory, NASA/Goddard Space Flight Center (United States); Adriani, O. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G.C. [University of Naples “Federico II”, Department of Physics, I-80126 Naples (Italy); INFN, Sezione di Naples, I-80126 Naples (Italy); and others

    2014-04-01

    The satellite-borne PAMELA experiment has been continuously collecting data since 2006. This apparatus is designed to study charged particles in the cosmic radiation. The combination of a permanent magnet, a silicon strip tracker and a silicon-tungsten imaging calorimeter, and the redundancy of instrumentation allow very precise studies on the physics of cosmic rays in a wide energy range and with high statistics. This makes PAMELA a very suitable instrument for Solar Energetic Particle (SEP) observations. Not only does it span the energy range between the ground-based neutron monitor data and the observations of SEPs from space, but PAMELA also carries out the first direct measurements of the composition for the highest energy SEP events, including those causing Ground Level Enhancements (GLEs). In particular, PAMELA has registered many SEP events during solar cycle 24, offering unique opportunities to address the question of high-energy SEP origin. A preliminary analysis on proton spectra behaviour during this event is presented in this work.

  8. Analysis on H spectral shape during the early 2012 SEPs with the PAMELA experiment

    International Nuclear Information System (INIS)

    Martucci, M.; Boezio, M.; Bravar, U.; Carbone, R.; Christian, E.R.; De Nolfo, G.A.; Mergè, M.; Mocchiutti, E.; Munini, R.; Ricci, M.; Ryan, J.M.; Sotgiu, A.; Stochaj, S.; Thakur, N.; Adriani, O.; Barbarino, G.C.

    2014-01-01

    The satellite-borne PAMELA experiment has been continuously collecting data since 2006. This apparatus is designed to study charged particles in the cosmic radiation. The combination of a permanent magnet, a silicon strip tracker and a silicon-tungsten imaging calorimeter, and the redundancy of instrumentation allow very precise studies on the physics of cosmic rays in a wide energy range and with high statistics. This makes PAMELA a very suitable instrument for Solar Energetic Particle (SEP) observations. Not only does it span the energy range between the ground-based neutron monitor data and the observations of SEPs from space, but PAMELA also carries out the first direct measurements of the composition for the highest energy SEP events, including those causing Ground Level Enhancements (GLEs). In particular, PAMELA has registered many SEP events during solar cycle 24, offering unique opportunities to address the question of high-energy SEP origin. A preliminary analysis on proton spectra behaviour during this event is presented in this work

  9. The magnetic spectrometer of the PAMELA satellite experiment

    International Nuclear Information System (INIS)

    Adriani, O.; Bonechi, L.; Bongi, M.; Castellini, G.; D'Alessandro, R.; Gabbanini, A.; Grandi, M.; Papini, P.; Ricciarini, S.B.; Spillantini, P.; Straulino, S.; Taccetti, F.; Tesi, M.; Vannuccini, E.

    2003-01-01

    In this paper, we describe in detail the design and the construction of the magnetic spectrometer of the PAMELA experiment, that will be launched during 2003 to do a precise measurement of the energy spectra of the antimatter components in cosmic rays. This paper will mainly focus on the detailed description of the tracking system and on the solutions adopted to deal with the technical challenges that are required to build a very precise detector to be used in the hostile space environment

  10. The PAMELA experiment on satellite and its capability in cosmic rays measurements

    CERN Document Server

    Adriani, O; Barbarino, G C; Barbier, L M; Bartalucci, S; Bazilevskaja, G; Bellotti, R; Bertazzoni, S; Bidoli, V; Boezio, M; Bogomolov, E A; Bonechi, L; Bonvicini, V; Boscherini, M; Bravar, U; Cafagna, F; Campana, D; Carlson, Per J; Casolino, M; Castellano, M; Castellini, G; Christian, E R; Ciacio, F; Circella, M; D'Alessandro, R; De Marzo, C N; De Pascale, M P; Finetti, N; Furano, G; Gabbanini, A; Galper, A M; Giglietto, N; Grandi, M; Grigorieva, A; Guarino, F; Hof, M; Koldashov, S V; Korotkov, M G; Krizmanic, J F; Krutkov, S; Lund, J; Marangelli, B; Marino, L; Menn, W; Mikhailov, V V; Mirizzi, N; Mitchell, J W; Mocchiutti, E; Moiseev, A A; Morselli, A; Mukhametshin, R; Ormes, J F; Osteria, G; Ozerov, J V; Papini, P; Pearce, M; Perego, A; Piccardi, S; Picozza, P; Ricci, M; Salsano, A; Schiavon, Paolo; Scian, G; Simon, M; Sparvoli, R; Spataro, B; Spillantini, P; Spinelli, P; Stephens, S A; Stochaj, S J; Stozhkov, Yu I; Straulino, S; Streitmatter, R E; Taccetti, F; Tesi, M; Vacchi, A; Vannuccini, E; Vasiljev, G; Vignoli, V; Voronov, S A; Yurkin, Y; Zampa, G; Zampa, N

    2002-01-01

    The PAMELA equipment will be assembled in 2001 and installed on board the Russian satellite Resurs. PAMELA is conceived mainly to study the antiproton and positron fluxes in cosmic rays up to high energy (190 GeV for p-bar and 270 GeV for e sup +) and to search antinuclei, up to 30 GeV/n, with a sensitivity of 10 sup - sup 7 in the He-bar/He ratio. The PAMELA telescope consists of: a magnetic spectrometer made up of a permanent magnet system equipped with double sided microstrip silicon detectors; a transition radiation detector made up of active layers of proportional straw tubes interleaved with carbon fibre radiators; and a silicon-tungsten imaging calorimeter made up of layers of tungsten absorbers and silicon detector planes. A time-of-flight system and anti-coincidence counters complete the PAMELA equipment. In the past years, tests have been done on each subdetector of PAMELA; the main results are presented and their implications on the anti-particles identification capability in cosmic rays are discus...

  11. PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA

    Directory of Open Access Journals (Sweden)

    A. Bruno

    2013-12-01

    Full Text Available The PAMELA experiment was launched on board the Resurs-DK1 satellite on June 15th 2006. The apparatus was designed to conduct precision studies of charged cosmic radiation over a wide energy range, from tens of MeV up to several hundred GeV, with unprecedented statistics. In five years of continuous data taking in space, PAMELA accurately measured the energy spectra of cosmic ray antiprotons and positrons, as well as protons, electrons and light nuclei, sometimes providing data in unexplored energetic regions. These important results have shed new light in several astrophysical fields like: an indirect search for Dark Matter, a search for cosmological antimatter (anti-Helium, and the validation of acceleration, transport and secondary production models of cosmic rays in the Galaxy. Some of the most important items of Solar and Magnetospheric physics were also investigated. Here we present the most recent results obtained by the PAMELA experiment.

  12. The PAMELA storage and control unit

    International Nuclear Information System (INIS)

    Casolino, M.; Altamura, F.; Basili, A.; De Pascale, M.P.; Minori, M.; Nagni, M.; Picozza, P.; Sparvoli, R.; Adriani, O.; Papini, P.; Spillantini, P.; Castellini, G.; Boezio, M.

    2007-01-01

    The PAMELA Storage and Control Unit (PSCU) comprises a Central Processing Unit (CPU) and a Mass Memory (MM). The CPU of the experiment is based on a ERC-32 architecture (a SPARC v7 implementation) running a real time operating system (RTEMS). The main purpose of the CPU is to handle slow control, acquisition and store data on a 2 GB MM. Communications between PAMELA and the satellite are done via a 1553B bus. Data acquisition from the sub-detectors is performed via a 2 MB/s interface. Download from the PAMELA MM towards the satellite main storage unit is handled by a 16 MB/s bus. The maximum daily amount of data transmitted to ground is about 20 GB

  13. The PAMELA storage and control unit

    Energy Technology Data Exchange (ETDEWEB)

    Casolino, M. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy)]. E-mail: Marco.Casolino@roma2.infn.it; Altamura, F. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Basili, A. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); De Pascale, M.P. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Minori, M. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Nagni, M. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Picozza, P. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Sparvoli, R. [INFN, Structure of Rome II, Physics Department, University of Rome II ' Tor Vergata' , I-00133 Rome (Italy); Adriani, O. [INFN, Structure of Florence, Physics Department, University of Florence, I-50019 Sesto Fiorentino (Italy); Papini, P. [INFN, Structure of Florence, Physics Department, University of Florence, I-50019 Sesto Fiorentino (Italy); Spillantini, P. [INFN, Structure of Florence, Physics Department, University of Florence, I-50019 Sesto Fiorentino (Italy); Castellini, G. [CNR-Istituto di Fisica Applicata ' Nello Carrara' , I-50127 Florence (Italy); Boezio, M. [INFN, Structure of Trieste, Physics Department, University of Trieste, I-34147 Trieste (Italy)

    2007-03-01

    The PAMELA Storage and Control Unit (PSCU) comprises a Central Processing Unit (CPU) and a Mass Memory (MM). The CPU of the experiment is based on a ERC-32 architecture (a SPARC v7 implementation) running a real time operating system (RTEMS). The main purpose of the CPU is to handle slow control, acquisition and store data on a 2 GB MM. Communications between PAMELA and the satellite are done via a 1553B bus. Data acquisition from the sub-detectors is performed via a 2 MB/s interface. Download from the PAMELA MM towards the satellite main storage unit is handled by a 16 MB/s bus. The maximum daily amount of data transmitted to ground is about 20 GB.

  14. Voices of Experience: Living with HIV. Pamela.

    Centers for Disease Control (CDC) Podcasts

    2009-06-07

    This podcast showcases Pamela, a woman living with HIV, as she tells her story.  Created: 6/7/2009 by Division of HIV and AIDS Prevention (DHAP), National Center for HIV, Hepatitis, STD, and Tuberculosis Prevention ( NCHHSTP).   Date Released: 6/7/2009.

  15. PAMELA: A Satellite Experiment for Antiparticles Measurement in Cosmic Rays

    Science.gov (United States)

    Bongi, M.; Adriani, O.; Ambriola, M.; Bakaldin, A.; Barbarino, G. C.; Basili, A.; Bazilevskaja, G.; Bellotti, R.; Bencardino, R.; Boezio, M.; Bogomolov, E. A.; Bonechi, L.; Bongiorno, L.; Bonvicini, V.; Boscherini, M.; Cafagna, F. S.; Campana, D.; Carlson, P.; Casolino, M.; Castellini, G.; Circella, M.; De Marzo, C. N.; De Pascale, M. P.; Furano, G.; Galper, A. M.; Giglietto, N.; Grigorjeva, A.; Koldashov, S. V.; Korotkov, M. G.; Krut'kov, S. Y.; Lund, J.; Lundquist, J.; Menicucci, A.; Menn, W.; Mikhailov, V. V.; Minori, M.; Mirizzi, N.; Mitchell, J. W.; Mocchiutti, E.; Morselli, A.; Mukhametshin, R.; Orsi, S.; Osteria, G.; Papini, P.; Pearce, M.; Picozza, P.; Ricci, M.; Ricciarini, S. B.; Romita, M.; Rossi, G.; Russo, S.; Schiavon, P.; Simon, M.; Sparvoli, R.; Spillantini, P.; Spinelli, P.; Stochaj, S. J.; Stozhkov, Y.; Straulino, S.; Streitmatter, R. E.; Taccetti, F.; Vacchi, A.; Vannuccini, E.; Vasilyev, G. I.; Voronov, S. A.; Wischnewski, R.; Yurkin, Y.; Zampa, G.; Zampa, N.

    2004-06-01

    PAMELA is a satellite-borne experiment that will study the antiproton and positron fluxes in cosmic rays in a wide range of energy (from 80 MeV up to 190 GeV for antiprotons and from 50 MeV up to 270 GeV for positrons) and with high statistics, and that will measure the antihelium/helium ratio with a sensitivity of the order of 10/sup -8/. The detector will fly on-board a polar orbiting Resurs DK1 satellite, which will be launched into space by a Soyuz rocket in 2004 from Baikonur cosmodrome in Kazakhstan, for a 3-year-long mission. Particle identification and energy measurements are performed in the PAMELA apparatus using the following subdetectors: a magnetic spectrometer made up of a permanent magnet equipped with double-sided microstrip silicon detectors, an electromagnetic imaging calorimeter composed of layers of tungsten absorber and silicon detectors planes, a transition radiation detector made of straw tubes interleaved with carbon fiber radiators, a plastic scintillator time-of-flight and trigger system, a set of anticounter plastic scintillator detectors, and a neutron detector. The features of the detectors and the main results obtained in beam test sessions are presented.

  16. Sistem Receiver Satelit NOAA pada Frekuensi 137,9 MHz

    Directory of Open Access Journals (Sweden)

    Nuhung Suleman

    2017-10-01

    Full Text Available Radio cuaca yang diusulkan terdiri atas rangkaian radio penerima, perangkat lunak untuk translasi data cuaca dari satelit menjadi data cuaca yang mudah dibaca oleh pengguna (nelayan disimpan dalam EPROM yang dapat diintegrasikan pada radio cuaca. Radio cuaca yang diusulkan juga memiliki sistem deteksi penerimaan data satelit cuaca NOAA melalui program aplikasi pewaktu (timer yang dapat mengaktifkan radio cuaca sekitar 5 menit sebelum waktu satelit NOAA melintasi Indonesia. Karena perangkat lunak/aplikasi disimpan dalam EPROM maka tidak diperlukan komputer untuk mengoperasikan radio cuaca.

  17. Positron identification by TRDs in TS93 and PAMELA experiments

    International Nuclear Information System (INIS)

    Bellotti, R.; Cafagna, F.; Castellano, M.; Circella, M.; De Marzo, C.; De Cataldo, G.; Giglietto, N.; Marangelli, B.; Raino, A.; Spinelli, P.

    1997-01-01

    We are involved in a program to study the antimatter components of the cosmic rays in outer space. We present the performances of a transition radiation detector we have built for positron identification during a balloon flight in 1993. The flight (TS93) was dedicated to the measurement of the positron spectrum in the energy range 4-50 GeV. We present also the design and expected performances of a similar detector we intend to build for a future experiment (PAMELA), to be run on a satellite by the end of 1999, in order to complete this program with higher statistics and at higher energies, namely about 200 GeV. (orig.)

  18. A method to detect positron anisotropies with Pamela data

    Energy Technology Data Exchange (ETDEWEB)

    Panico, B. [INFN, Sezione di Naples, I-80126 Naples (Italy); Adriani, O. [University of Florence, Department of Physics and Astronomy, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G.C. [INFN, Sezione di Naples, I-80126 Naples (Italy); University of Naples Federico II”, Department of Physics, I-80126 Naples (Italy); Bazilevskaya, G.A. [Lebedev Physical Institute, RU-119991, Moscow (Russian Federation); Bellotti, R. [University of Bari, Department of Physics, I-70126 Bari (Italy); INFN, Sezione di Bari, I-70126 Bari (Italy); Boezio, M. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E.A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bongi, M. [University of Florence, Department of Physics and Astronomy, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bonvicini, V. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bottai, S. [University of Naples Federico II”, Department of Physics, I-80126 Naples (Italy); Bruno, A. [University of Bari, Department of Physics, I-70126 Bari (Italy); INFN, Sezione di Bari, I-70126 Bari (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M. [INFN, Sezione di Rome Tor Vergata, I-00133 Rome (Italy); RIKEN, Advanced Science Institute, Wako-shi, Saitama (Japan); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); De Donato, C. [INFN, Sezione di Rome Tor Vergata, I-00133 Rome (Italy); and others

    2014-11-15

    The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference.

  19. Ten years of CR physics with PAMELA

    Science.gov (United States)

    Galper, A.; Spillantini, P.

    2017-09-01

    The satellite borne Pamela instrument is dedicated to the precise and high statistics study of CR fluxes on a four decades energy range. Pamela experiment is the last step of the "Russian-Italian Mission" (RIM) program established in 1992 between several Italian and Russian institutes and with the participation of Sweden and Germany. Designed as a cosmic ray observatory at 1 AU, it extensive program is made possible thanks to the outstanding performance of the instrument, the low energy threshold, the quasi-polar orbit and the 10 years duration of the observation. The physics program pays particular attention to the study of particles and antiparticles fluxes and includes search for dark matter, primordial antimatter, new matter in the Universe, study of cosmic-ray propagation, solar physics and solar modulation, and terrestrial magnetosphere. Very important is the discovery of the anomalous increase of the positron flux at energies higher that 50 GeV (the so called "Pamela anomaly"), and the abrupt spectral hardening of H and He, challenging the current paradigm of cosmic-ray acceleration and propagation in the Galaxy.

  20. PAMELA mission: heralding a new era in cosmic ray physics

    Directory of Open Access Journals (Sweden)

    Ricciarini S. B.

    2014-04-01

    Full Text Available After seven years of data taking in space, the experiment PAMELA is showing very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.

  1. Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Formato, V., E-mail: valerio.formato@ts.infn.it [INFN, Sezione di Trieste, I-34149 Trieste (Italy); University of Trieste, Department of Physics, I-34147 Trieste (Italy); Adriani, O. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G.C. [University of Naples “Federico II”, Department of Physics, I-80126 Naples (Italy); INFN, Sezione di Naples, I-80126 Naples (Italy); Bazilevskaya, G.A. [Lebedev Physical Institute, RU-119991, Moscow (Russian Federation); Bellotti, R. [University of Bari, Department of Physics, I-70126 Bari (Italy); INFN, Sezione di Bari, I-70126 Bari (Italy); Boezio, M. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E.A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bongi, M. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bonvicini, V. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bruno, A.; Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Carlson, P. [KTH, Department of Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Oskar Klein Centre for Cosmoparticle Physics (Sweden); Casolino, M. [INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome (Italy); RIKEN, Advanced Science Institute, Wako-shi, Saitama (Japan); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); and others

    2014-04-01

    PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature, with particular focus on the antimatter component. The detector consists of a permanent magnet spectrometer core to provide rigidity and charge sign information, a Time-of-Flight system for velocity and charge information, a Silicon–Tungsten calorimeter and a Neutron detector for lepton/hadron identification. The velocity and rigidity information allow the identification of different isotopes for Z=1 and Z=2 particles in the energy range 100 MeV/n to 1 GeV/n. In this work we will present the PAMELA results on the H and He isotope fluxes based on the data collected during the 23rd solar minimum from 2006 to 2007. Such fluxes carry relevant information helpful in constraining parameters in galactic cosmic rays propagation models complementary to those obtained from other secondary to primary measurements such as the boron-to-carbon ratio.

  2. The instrument PAMELA for antimatter and dark matter search in space

    International Nuclear Information System (INIS)

    Picozza, Piergiorgio; Sparvoli, Roberta

    2010-01-01

    The PAMELA satellite experiment is dedicated to the study of charged particles in cosmic radiation, with a particular focus on antiparticles for the search of antimatter and signals of dark matter, in the energy window from 100 MeV to some hundreds of GeV. PAMELA is installed on board of the Resurs DK1 satellite that was launched from the Baikonur cosmodrome on June 15th, 2006. The PAMELA apparatus comprises a magnetic spectrometer, a time-of-flight system, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. The combination of these devices allows antiparticles to be reliably identified from a large background of other charged particles.

  3. Solar flare activity in 2006 - 2016 according to PAMELA and ARINA spectrometers

    Science.gov (United States)

    Rodenko, S. A.; Borkut, I. K.; Mayorov, A. G.; Malakhov, V. V.; PAMELA Collaboration

    2018-01-01

    From 2006 to 2016 years on the board of RESURS-DK1 satellite PAMELA and ARINA cosmic rays experiments was carried out. The main goal of experiments is measurement of galactic component of cosmic rays; it also registers solar particles accelerated in powerful explosive processes on the sun (solar flares) in wide energy range. The article includes the list of solar events when PAMELA or ARINA spectrometers have registered increasing of proton flux intensities for energies more than 4 MeV.

  4. PAMELA measurements of the boron and carbon spectra

    International Nuclear Information System (INIS)

    Mori, N; Adriani, O; Bongi, M; Barbarino, G C; Bazilevskaya, G A; Bellotti, R; Bruno, A; Boezio, M; Bonvicini, V; Carbone, R; Bogomolov, E A; Bottai, S; Cafagna, F; Campana, D; Carlson, P; Casolino, M; De Donato, C; De Santis, C; De Simone, N; Castellini, G

    2015-01-01

    The satellite-borne PAMELA experiment is aimed at precision measurements of the charged light component of the cosmic-ray spectrum, with a particular focus on antimatter. It consists of a magnetic spectrometer, a time-of-flight system, an electromagnetic calorimeter with a tail catcher scintillating layer, an anticoincidence system and a neutron detector. PAMELA has measured the absolute fluxes of boron and carbon and the B/C ratio, which plays a central role in galactic propagation studies in order to derive the injection spectra at sources from measurements at Earth. In this paper, the data analysis techniques and the final results are presented. (paper)

  5. Excited Dark Matter versus PAMELA/Fermi

    CERN Document Server

    Cline, James M

    2010-01-01

    Excitation of multicomponent dark matter in the galactic center has been proposed as the source of low-energy positrons that produce the excess 511 keV gamma rays that have been observed by INTEGRAL. Such models have also been promoted to explain excess high-energy electrons/positrons observed by the PAMELA, Fermi/LAT and H.E.S.S. experiments. We investigate whether one model can simultaneously fit all three anomalies, in addition to further constraints from inverse Compton scattering by the high-energy leptons. We find models that fit both the 511 keV and PAMELA excesses at dark matter masses M < 400 GeV, but not the Fermi lepton excess. The conflict arises because a more cuspy DM halo profile is needed to match the observed 511 keV signal than is compatible with inverse Compton constraints at larger DM masses.

  6. The PAMELA space mission for antimatter and dark matter searches in space

    International Nuclear Information System (INIS)

    Boezio, M.; Bruno, A.; Adriani, O.; Barbarino, G. C.; Bazilevskaya, G. A.; Bellotti, R.; Bogomolov, E. A.; Bongi, M.; Bonvicini, V.; Borisov, S.; Bottai, S.; Cafagna, F.; Campana, D.; Carbone, R.; Carlson, P.; Casolino, M.; Castellini, G.; Consiglio, L.; De Pascale, M. P.; De Santis, C.

    2012-01-01

    The PAMELA satellite-borne experiment has presented new results on cosmic-ray antiparticles that can be interpreted in terms of DM annihilation or pulsar contribution. The instrument was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectrum in order to search for exotic sources. PAMELA is also searching for primordial antinuclei (anti-helium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. This talk illustrates the most recent scientific results obtained by the PAMELA experiment.

  7. The PAMELA space mission for antimatter and dark matter searches in space

    Energy Technology Data Exchange (ETDEWEB)

    Boezio, M., E-mail: Mirko.Boezio@ts.infn.it [INFN, Sezione di Trieste (Italy); Bruno, A., E-mail: Alessandro.Bruno@ba.infn.it [University of Bari, Department of Physics (Italy); Adriani, O. [University of Florence, Department of Physics (Italy); Barbarino, G. C. [University of Naples ' Federico II' , Department of Physics (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute (Russian Federation); Bellotti, R. [University of Bari, Department of Physics (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute (Russian Federation); Bongi, M. [INFN, Sezione di Florence (Italy); Bonvicini, V. [INFN, Sezione di Trieste (Italy); Borisov, S. [INFN, Sezione di Rome ' Tor Vergata' (Italy); Bottai, S. [INFN, Sezione di Florence (Italy); Cafagna, F. [University of Bari, Department of Physics (Italy); Campana, D.; Carbone, R. [INFN, Sezione di Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics (Sweden); Casolino, M. [INFN, Sezione di Rome ' Tor Vergata' (Italy); Castellini, G. [IFAC (Italy); Consiglio, L. [INFN, Sezione di Naples (Italy); De Pascale, M. P.; De Santis, C. [INFN, Sezione di Rome ' Tor Vergata' (Italy); and others

    2012-12-15

    The PAMELA satellite-borne experiment has presented new results on cosmic-ray antiparticles that can be interpreted in terms of DM annihilation or pulsar contribution. The instrument was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectrum in order to search for exotic sources. PAMELA is also searching for primordial antinuclei (anti-helium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. This talk illustrates the most recent scientific results obtained by the PAMELA experiment.

  8. TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THE PAMELA EXPERIMENT

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [Department of Physics and Astronomy, University of Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [Department of Physics, University of Naples " Federico II," I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991 Moscow (Russian Federation); Bellotti, R.; Bruno, A. [Department of Physics, University of Bari, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M.; De Donato, C.; De Santis, C.; De Simone, N.; Felice, V. Di [INFN, Sezione di Rome " Tor Vergata," I-00133 Rome (Italy); Castellini, G., E-mail: alessandro.bruno@ba.infn.it [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); and others

    2015-01-20

    We report an accurate measurement of the geomagnetically trapped proton fluxes for kinetic energy above ∼70 MeV performed by the PAMELA mission at low Earth orbits (350 ÷ 610 km). Data were analyzed in the frame of the adiabatic theory of charged particle motion in the geomagnetic field. Flux properties were investigated in detail, providing a full characterization of the particle radiation in the South Atlantic Anomaly region, including locations, energy spectra, and pitch angle distributions. PAMELA results significantly improve the description of the Earth's radiation environment at low altitudes, placing important constraints on the trapping and interaction processes, and can be used to validate current trapped particle radiation models.

  9. MEASUREMENTS OF COSMIC-RAY HYDROGEN AND HELIUM ISOTOPES WITH THE PAMELA EXPERIMENT

    International Nuclear Information System (INIS)

    Adriani, O.; Bongi, M.; Barbarino, G. C.; Bazilevskaya, G. A.; Bellotti, R.; Bruno, A.; Boezio, M.; Bonvicini, V.; Formato, V.; Bogomolov, E. A.; Bottai, S.; Cafagna, F.; Campana, D.; Carlson, P.; Casolino, M.; Santis, C. De; Castellini, G.; Donato, C. De; Simone, N. De; Felice, V. Di

    2016-01-01

    The cosmic-ray hydrogen and helium ( 1 H, 2 H, 3 He, 4 He) isotopic composition has been measured with the satellite-borne experiment PAMELA, which was launched into low-Earth orbit on board the Resurs-DK1 satellite on 2006 June 15. The rare isotopes 2 H and 3 He in cosmic rays are believed to originate mainly from the interaction of high-energy protons and helium with the galactic interstellar medium. The isotopic composition was measured between 100 and 1100 MeV/n for hydrogen and between 100 and 1400 MeV/n for helium isotopes using two different detector systems over the 23rd solar minimum from 2006 July to 2007 December

  10. Measurement of boron and carbon fluxes in cosmic rays with the PAMELA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [Department of Physics and Astronomy, University of Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [Department of Physics, University of Naples " Federico II," I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991 Moscow (Russian Federation); Bellotti, R.; Bruno, A. [Department of Physics, University of Bari, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M.; De Donato, C.; De Santis, C.; De Simone, N. [INFN, Sezione di Rome " Tor Vergata," I-00133 Rome (Italy); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); Danilchenko, I. A. [National Research Nuclear University MEPhI, RU-115409 Moscow (Russian Federation); and others

    2014-08-20

    The propagation of cosmic rays inside our galaxy plays a fundamental role in shaping their injection spectra into those observed at Earth. One of the best tools to investigate this issue is the ratio of fluxes for secondary and primary species. The boron-to-carbon (B/C) ratio, in particular, is a sensitive probe to investigate propagation mechanisms. This paper presents new measurements of the absolute fluxes of boron and carbon nuclei as well as the B/C ratio from the PAMELA space experiment. The results span the range 0.44-129 GeV/n in kinetic energy for data taken in the period 2006 July to 2008 March.

  11. MEASUREMENTS OF COSMIC-RAY HYDROGEN AND HELIUM ISOTOPES WITH THE PAMELA EXPERIMENT

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [University of Naples “Federico II,” Department of Physics, I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991, Moscow (Russian Federation); Bellotti, R.; Bruno, A. [University of Bari, Department of Physics, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Formato, V. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M.; Santis, C. De [University of Rome “Tor Vergata,” Department of Physics, I-00133 Rome (Italy); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); Donato, C. De; Simone, N. De; Felice, V. Di [INFN, Sezione di Rome “Tor Vergata,” I-00133 Rome (Italy); and others

    2016-02-10

    The cosmic-ray hydrogen and helium ({sup 1}H, {sup 2}H, {sup 3}He, {sup 4}He) isotopic composition has been measured with the satellite-borne experiment PAMELA, which was launched into low-Earth orbit on board the Resurs-DK1 satellite on 2006 June 15. The rare isotopes {sup 2}H and {sup 3}He in cosmic rays are believed to originate mainly from the interaction of high-energy protons and helium with the galactic interstellar medium. The isotopic composition was measured between 100 and 1100 MeV/n for hydrogen and between 100 and 1400 MeV/n for helium isotopes using two different detector systems over the 23rd solar minimum from 2006 July to 2007 December.

  12. Results from PAMELA, ATIC and FERMI: Pulsars or dark matter?

    Indian Academy of Sciences (India)

    It is well known that dark matter dominates the dynamics of galaxies and clusters of galaxies. Its constituents remain a mystery despite an assiduous search for them over the past three decades. Recent results from the satellite-based PAMELA experiment show an excess in the positron fraction at energies between 10 and ...

  13. MEASUREMENT OF THE ISOTOPIC COMPOSITION OF HYDROGEN AND HELIUM NUCLEI IN COSMIC RAYS WITH THE PAMELA EXPERIMENT

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [Department of Physics, University of Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [Department of Physics, University of Naples ' ' Federico II' ' , I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991, Moscow (Russian Federation); Bellotti, R.; Bruno, A. [Department of Physics, University of Bari, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Borisov, S.; Casolino, M.; De Pascale, M. P. [INFN, Sezione di Rome ' ' Tor Vergata' ' , I-00133 Rome (Italy); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); Danilchenko, I. A. [National Research Nuclear University MEPhI, RU-115409 Moscow (Russian Federation); De Santis, C. [Department of Physics, University of Rome ' ' Tor Vergata' ' , I-00133 Rome (Italy); and others

    2013-06-10

    The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV/n for hydrogen and between 100 and 900 MeV/n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C.

  14. The magnetic spectrometer PAMELA for the study of cosmic antimatter in space

    International Nuclear Information System (INIS)

    Basini, G.; Hof, M.; Barbiellini, G.; Boezio, M.; Bellotti, R.; Cafagna, F.

    1995-01-01

    In the framework of the RIM (Russian Italian mission) program, PAMELA is the experiment devoted to the accurate measurement of the positron and antiproton spectra from the very low energy thresh-old of 100 MeV up to more than 50 GeV, and to hunt antinuclei with sensitivity better than 10 -7 in the helium/helium ratio. A permanent magnet equipped by microstrip silicon sensors, measures the particle momentum with MDR=400 GV/c on GF=25 cm 2 sr. An accurate ToF system, a 19 X o deep imaging calorimeter, an aerogel Cherenkov counter and a TRD detector complement the spectrometer in order an efficient e +- /p +- separation and some light isotope identification capability. The PAMELA experiment will be carried out on a 700 km high polar orbit, on board of the Earth-observation meteor-3A satellite, to be launched at the end of 1988

  15. A Freudian Reading of Samuel Richardson's Pamela

    Directory of Open Access Journals (Sweden)

    Shadi Torabi Sarijaloo

    2016-03-01

    Full Text Available Richardson's Pamela (1740_1 is replete with elements and incidents that make it worthy enough to be viewed from Freud's perspective. The present study focuses upon how Richardson's characters unconsciously attempt to conceal and repress their own conflicting emotions, thoughts, wishes, impulses and how they struggle against their anxiety-ridden situations to regain their psychic balance. Moreover, the repetition of certain occurrences and elements play a crucial role in generating the uncanny effect in Pamela, including the role of double and déjà-vu, the castle-like settings, heroine's intimidating situations and also her master's past secret. In addition, the way Richardson's characters dress for the noteworthy masquerade ball scene and the ambiguous words of Pamela's master are considerably implies something that is affiliated with characters' psyche according to Freud's condensation theory. With regard to Freud's concepts of The 'Tripartite Psyche', 'Anxiety and Ego Defense Mechanisms' and 'Uncanny' the researcher attempts to delve into the heroine and her master's psyche through her letters which reveal the contents of the heroine's unconscious mind.

  16. New type of chromosomal aberrations in microspores of Tradescancia Paludosa in flight experiments on board of space satelites

    Energy Technology Data Exchange (ETDEWEB)

    Delone, N L; Antipov, V V; Parfenov, G P

    1986-01-01

    A new type of chromosomal aberrations - complex nonreciprocal translocations accompanied by spherical fragments, is opened. The results of 30 variants of tests are investigated to establish what factor particularly causes new type of chromosomal aberrations. The experiments have been carried out on boards the space satelites: ''Vostok 3, 4, 5, 6'', ''Voskhod'', ''Kosmos 110'', ''Zond 6, 7'', ''Kosmos 368''. All type of aberrations have been recorded. It is supposed that a new type of aberrations depends on the effect of the sum of dynamic factors. At the same time these aberrations are not the background and escape it by separate bright bursts being independent on the effect of take-off, landing and time of an object staying in weightlessness. There is a type of irradiation causing a special type of aberrations.

  17. New type of chromosomal aberrations in microspores of Tradescancia Paludosa in flight experiments on board of space satelites

    International Nuclear Information System (INIS)

    Delone, N.L.; Antipov, V.V.; Parfenov, G.P.

    1986-01-01

    A new type of chromosomal aberrations - complex nonreciprocal translocations accompanied by spherical fragments, is opened. The results of 30 variants of tests are investigated to establish what factor particularly causes new type of chromosomal aberrations. The experiments have been carried out on boards the space satelites: ''Vostok 3, 4, 5, 6'', ''Voskhod'', ''Kosmos 110'', ''Zond 6, 7'', ''Kosmos 368''. All type of aberrations have been recorded. It is supposed that a new type of aberrations depends on the effect of the sum of dynamic factors. At the same time these aberrations are not the background and escape it by separate bright bursts being independent on the effect of take-off, landing and time of an object staying in weightlessness. There is a type of irradiation causing a special type of aberrations

  18. The magnetic spectrometer PAMELA for the study of cosmic antimatter in space

    Energy Technology Data Exchange (ETDEWEB)

    Basini, G. [INFN, Laboratori Nazionali di Frascati, Rome (Italy); De Pascale, M.P. [Rome Univ. `Tor Vergata` (Italy)]|[INFN, Rome (Italy); Hof, M. [Siegen univ. (Germany). Fachbereich Physik; Golden, R.L. [New Mexico State Univ., Las Cruces, NM (United States). Particle Astrophysics Lab.; Brancaccio, F.; Bocciolini, M. [Florence Univ. (Italy)]|[INFN, Florence (Italy); Barbiellini, G.; Boezio, M. [Trieste Univ. (Italy)]|[INFN, Trieste (Italy); Bellotti, R.; Cafagna, F. [Bari Univ. (Italy)]|[INFN, Bari (Italy)

    1995-09-01

    In the framework of the RIM (Russian Italian mission) program, PAMELA is the experiment devoted to the accurate measurement of the positron and antiproton spectra from the very low energy thresh-old of 100 MeV up to more than 50 GeV, and to hunt antinuclei with sensitivity better than 10{sup -7} in the helium/helium ratio. A permanent magnet equipped by microstrip silicon sensors, measures the particle momentum with MDR=400 GV/c on GF=25 cm{sup 2} sr. An accurate ToF system, a 19 X{sub o} deep imaging calorimeter, an aerogel Cherenkov counter and a TRD detector complement the spectrometer in order an efficient e{sup +-}/p{sup +-} separation and some light isotope identification capability. The PAMELA experiment will be carried out on a 700 km high polar orbit, on board of the Earth-observation meteor-3A satellite, to be launched at the end of 1988.

  19. The Science and First Results of the PAMELA Space Mission

    CERN Multimedia

    CERN. Geneva

    2008-01-01

    On the 15th of June 2006 the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it is collecting data since July 2006. The core of the instrument is a silicon-microstrip magnetic spectrometer combined with a time-of-flight system, a silicon-tungsten electromagnetic calorimeter, a shower tail catcher scintillator, a neutron detector and an anticoincidence system. This telescope allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - 100's GeV) with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectra in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (anti-helium) and performing precise measurements of light nuclei and their isotopes for testing cosmic-ray propagation models. Other objectives are the monitoring of the solar activity, the detection of solar flares and the study of the solar...

  20. Solar Energetic Particle Studies with PAMELA

    Science.gov (United States)

    Bravar, U.; Christian, E. R.; deNolfo, Georgia; Ryan, J. M.; Stochaj, S.

    2011-01-01

    The origin of the high-energy solar energetic particles (SEPs) may conceivably be found in composition signatures that reflect the elemental abundances of the low corona and chromosphere vs. the high corona and solar wind. The presence of secondaries, such as neutrons and positrons, could indicate a low coronal origin of these particles. Velocity dispersion of different species and over a wide energy range can be used to determine energetic particle release times at the Sun. Together with multi-wavelength imaging, in- situ observations of a variety of species, and coverage over a wide energy range provide a critical tool in identifying the origin of SEPs, understanding the evolution of these events within the context of solar active regions, and constraining the acceleration mechanisms at play. The Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA)instrument, successfully launched in 2006 and expected to remain operational until at least the beginning of 2012, measures energetic particles in the same energy range as ground-based neutron monitors, and lower energies as well. It thus bridges the gap between low energy in-situ observations and ground-based Ground Level Enhancements (GLE) observations. It can measure the charge (up to Z=6) and atomic number of the detected particles, and it can identify and measure positrons and detect neutrons-an unprecedented array of data channels that we can bring to bear on the origin of high-energy SEPs. We present prelimiary results on the for the 2006 December 13 solar flare and GLE and the 2011 March 21 solar flare, both registering proton and helium enhancements in PAMELA. Together with multi- spacecraft contextual data and modeling, we discuss the PAMELA results in the context of the different acceleration mechanisms at play.

  1. Identifikasi Kedalaman Laut (Bathymetry berdasarkan Warna Permukaan Laut pada Citra Satelit menggunakan Metode ANFIS

    Directory of Open Access Journals (Sweden)

    Diwan Mukti Pambuko

    2013-10-01

    mengetahui warna permukaan pada posisi tersebut dapat dibuat sebuah sistem yang bisa mengidentifikasi kedalaman laut pada posisi tertentu dari warna pada permukaan laut tersebut. Sistem yang dibangun ini menggunakan data kedalaman laut hasil pengukuran manual dan dipadukan dengan data gambar satelit pada posisi yang sama. Kemudian dilakukan proses learning menggunakan teknik Neuro-Fuzzy dengan metode ANFIS (Adaptive Neuro-Fuzzy Inference System dengan kinerja model identifikasi dapat diketahui dari nilai MAPE (Mean Absolute Percentage Error dan MSE (Mean Square Error. Hasil dari pembuatan model identifikasi, diperoleh sistem yang dapat melakukan identifikasi sangat baik dengan error yang diperoleh pada saat proses pengujian sebesar MAPE 9.0024 % dan MSE 0.0034. Kata kunci: bathymetry, citra satelit, neuro-fuzzy, ANFIS

  2. PAMELA Space Mission: The Transition Radiation Detector

    Science.gov (United States)

    Ambriola, M.; Bellotti, R.; Cafagna, F.; Circella, M.; De Marzo, C.; Giglietto, N.; Marangelli, B.; Mirizzi, N.; Romita, M.; Spinelli, P.

    2003-07-01

    PAMELA telescope is a satellite-b orne magnetic spectrometer built to fulfill the primary scientific objectives of detecting antiparticles (antiprotons and positrons) in the cosmic rays, and to measure spectra of particles in cosmic rays. The PAMELA telescope is currently under integration and is composed of: a silicon tracker housed in a permanent magnet, a time of flight and an anticoincidence system both made of plastic scintillators, a silicon imaging calorimeter, a neutron detector and a Transition Radiation Detector (TRD). The TRD detector is composed of 9 sensitive layers of straw tubes working in proportional mode for a total of 1024 channels. Each layer is interleaved with a radiator plane made of carbon fibers. The TRD detector characteristics will be described along with its performance studied exposing the detector to particle beams of electrons, pions, muons and protons of different momenta at both CERN-PS and CERN-SPS facilities.

  3. Analisa Ketelitian Geometrik Citra Satelit Pleiades 1A Metode Orthorektifikasi Rigorious sebagai Dasar Pembuatan Peta Desa (Studi Kasus: Kelurahan Kenjeran

    Directory of Open Access Journals (Sweden)

    Hanif Khoirul Latif

    2017-01-01

    Full Text Available Peta desa merupakan peta tematik bersifat dasar yang berisi unsur dan informasi batas wilayah, infrastruktur transportasi, toponim, perairan, sarana prasarana, penutup lahan dan penggunaan lahan yang disajikan dalam peta citra, peta sarana dan prasarana, serta peta penutup lahan dan penggunaan lahan. Data citra satelit yang digunakan dalam penelitian ini adalah citra satelit Pleiades 1A. Metode koreksi geometrik yang digunakan dalam penelitian ini adalah orthorektifikasi metode rigorious. Digunakan 8 Ground Control Point (GCP yang didapatkan dari pengukuran GPS geodetik dengan metode statik dengan lama pengamatan 60 menit tiap titik. Digunakan 12 Independence Check Point (ICP. Hasil dari penelitian ini adalah bahwa citra satelit Pleiades 1A Menurut Perka BIG No. 3 Tahun 2016 Tentang Spesifikasi Teknis Penyajian Peta Desa layak untuk digunakan dalam pebuatan peta citra Desa/Kelurahan Kenjeran dengan skala 1:5000 dengan kelas ketelitian 3.

  4. Decaying dark matter and the PAMELA anomaly

    International Nuclear Information System (INIS)

    Ibarra, Alejandro; Tran, David

    2009-01-01

    Astrophysical and cosmological observations do not require the dark matter particles to be absolutely stable. If they are indeed unstable, their decay into positrons might occur at a sufficiently large rate to allow the indirect detection of dark matter through an anomalous contribution to the cosmic positron flux. In this paper we discuss the implications of the excess in the positron fraction recently reported by the PAMELA collaboration for the scenario of decaying dark matter. To this end, we have performed a model-independent analysis of possible signatures by studying various decay channels in the case of both a fermionic and a scalar dark matter particle. We find that the steep rise in the positron fraction measured by PAMELA at energies larger than 10 GeV can naturally be accommodated in several realizations of the decaying dark matter scenario. The data point toward a rather heavy dark matter particle, m DM ∼> 300 GeV, which preferentially decays directly into first or second generation charged leptons with a lifetime τ DM ∼ 10 26 s

  5. The transition radiation detector of the PAMELA space mission

    Science.gov (United States)

    Ambriola, M.; Bellotti, R.; Cafagna, F.; Circella, M.; de Marzo, C.; Giglietto, N.; Marangelli, B.; Mirizzi, N.; Romita, M.; Spinelli, P.

    2004-04-01

    PAMELA space mission objective is to flight a satellite-borne magnetic spectrometer built to fulfill the primary scientific goals of detecting antiparticles (antiprotons and positrons) and to measure spectra of particles in cosmic rays. The PAMELA telescope is composed of: a silicon tracker housed in a permanent magnet, a time-of-flight and an anticoincidence system both made of plastic scintillators, a silicon imaging calorimeter, a neutron detector and a Transition Radiation Detector (TRD). The TRD is composed of nine sensitive layers of straw tubes working in proportional mode for a total of 1024 channels. Each layer is interleaved with a radiator plane made of carbon fibers. The TRD characteristics will be described along with its performances studied at both CERN-PS and CERN-SPS facilities, using electrons, pions, muons and protons of different momenta.

  6. The transition radiation detector of the PAMELA space mission

    International Nuclear Information System (INIS)

    Ambriola, M.; Bellotti, R.; Cafagna, F.; Circella, M.; De Marzo, C.; Giglietto, N.; Marangelli, B.; Mirizzi, N.; Romita, M.; Spinelli, P.

    2004-01-01

    PAMELA space mission objective is to flight a satellite-borne magnetic spectrometer built to fulfill the primary scientific goals of detecting antiparticles (antiprotons and positrons) and to measure spectra of particles in cosmic rays. The PAMELA telescope is composed of: a silicon tracker housed in a permanent magnet, a time-of-flight and an anticoincidence system both made of plastic scintillators, a silicon imaging calorimeter, a neutron detector and a Transition Radiation Detector (TRD). The TRD is composed of nine sensitive layers of straw tubes working in proportional mode for a total of 1024 channels. Each layer is interleaved with a radiator plane made of carbon fibers. The TRD characteristics will be described along with its performances studied at both CERN-PS and CERN-SPS facilities, using electrons, pions, muons and protons of different momenta

  7. The borosilicate glass for 'PAMELA'

    International Nuclear Information System (INIS)

    Schiewer, E.

    1986-01-01

    The low enriched waste concentrate (LEWC) stored at Mol, Belgium, will be solidified in the vitrification plant 'PAMELA'. An alkali-borosilicate glass was developed by the Hahn-Meitner-Institut, Berlin, which dissolves (11 +- 3)wt% waste oxides while providing sufficient flexibility for changes in the process parameters. The development of the glass labelled SM513LW11 is described. Important properties of the glass melt (viscosity, resistivity, formation of yellow phase) and of the glass (corrosion in aqueous solutions, crystallization) are reported. The corrosion data of this glass are similar to those of other HLW-glasses. Less than five wt% of crystalline material are produced upon cooling of large glass blocks. Crystallization does not affect the chemical durability. (Auth.)

  8. Pamela tracking system status report

    CERN Document Server

    Taccetti, F; Bonechi, L; Bongi, M; Boscherini, M; Castellini, G; D'Alessandro, R; Gabbanini, A; Grandi, M; Papini, P; Piccardi, S; Ricciarini, S; Spillantini, P; Straulino, S; Tesi, M; Vannuccini, E

    2002-01-01

    The Pamela apparatus will be launched at the end of 2002 on board of the Resurs DK Russian satellite. The tracking system, composed of six planes of silicon sensors inserted inside a permanent magnetic field was intensively tested during these last years. Results of tests have shown a good signal-to-noise ratio and an excellent spatial resolution, which should allow to measure the antiproton flux in an energy range from 80 MeV up to 190 GeV. The production of the final detector modules is about to start and mechanical and thermal tests on the tracking tower are being performed according to the specifications of the Russian launcher and satellite.

  9. Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24

    Science.gov (United States)

    Martucci, M.; Munini, R.; Boezio, M.; Di Felice, V.; Adriani, O.; Barbarino, G. C.; Bazilevskaya, G. A.; Bellotti, R.; Bongi, M.; Bonvicini, V.; Bottai, S.; Bruno, A.; Cafagna, F.; Campana, D.; Carlson, P.; Casolino, M.; Castellini, G.; De Santis, C.; Galper, A. M.; Karelin, A. V.; Koldashov, S. V.; Koldobskiy, S.; Krutkov, S. Y.; Kvashnin, A. N.; Leonov, A.; Malakhov, V.; Marcelli, L.; Marcelli, N.; Mayorov, A. G.; Menn, W.; Mergè, M.; Mikhailov, V. V.; Mocchiutti, E.; Monaco, A.; Mori, N.; Osteria, G.; Panico, B.; Papini, P.; Pearce, M.; Picozza, P.; Ricci, M.; Ricciarini, S. B.; Simon, M.; Sparvoli, R.; Spillantini, P.; Stozhkov, Y. I.; Vacchi, A.; Vannuccini, E.; Vasilyev, G.; Voronov, S. A.; Yurkin, Y. T.; Zampa, G.; Zampa, N.; Potgieter, M. S.; Raath, J. L.

    2018-02-01

    Precise measurements of the time-dependent intensity of the low-energy (solar activity periods, i.e., from minimum to maximum, are needed to achieve comprehensive understanding of such physical phenomena. The minimum phase between solar cycles 23 and 24 was peculiarly long, extending up to the beginning of 2010 and followed by the maximum phase, reached during early 2014. In this Letter, we present proton differential spectra measured from 2010 January to 2014 February by the PAMELA experiment. For the first time the GCR proton intensity was studied over a wide energy range (0.08–50 GeV) by a single apparatus from a minimum to a maximum period of solar activity. The large statistics allowed the time variation to be investigated on a nearly monthly basis. Data were compared and interpreted in the context of a state-of-the-art three-dimensional model describing the GCRs propagation through the heliosphere.

  10. Decaying dark matter in light of the PAMELA and Fermi LAT data

    International Nuclear Information System (INIS)

    Ibarra, Alejandro; Tran, David

    2009-06-01

    A series of experiments measuring high-energy cosmic rays have recently reported strong indications for the existence of an exotic source of high-energy electrons and positrons. If interpreted in terms of the decay of dark matter particles, the PAMELA measurements of the positron fraction and the Fermi LAT measurements of the total electron plus positron flux restrict the possible decaying dark matter scenarios to a few cases. Pursuing a model-independent approach, we identify some promising scenarios of dark matter decay and calculate the predictions for the diffuse extragalactic gamma-ray flux, including the contributions from inverse Compton scattering with the interstellar radiation field. (orig.)

  11. USA sõjaväe endine hääletoru : esiterroristi jahi kõrval on ka koolid / Pamela Keeton ; interv. Erkki Bahovski

    Index Scriptorium Estoniae

    Keeton, Pamela

    2006-01-01

    Endine USA armee pressiesindaja ja praegune USA Rahuinstituudi avalike suhete juht Pamela Keeton räägib intervjuus reporteri tööst Afganistanis ning leiab, et ajakirjanikud lähenevad sündmuste kajastamisele meedias erinevalt. Lisa: Pamela Keeton CV

  12. Analisis Model Ekstraksi Citra Satelit Untuk Prediksi Tanaman Padi Dengan Pendekatan Model Statistik Dan Kecerdasan Buatan

    OpenAIRE

    Chairuddin, Chairuddin

    2014-01-01

    Keunggulan teknologi inderaja dalam melakukan estimasi melalui objek data citra dengan wahana satelit menjadi salah satu alternatif para pengambil keputusan dalam rangka mendukung dan memperoleh informasi serta solusi terbaik dalam menentukan langkah yang harus diambil untuk menentukan suatu keputusan yang handal. Data citra dapat dimanipulasi dengan serangkaian metode sehingga dapat menghasilkan sebuah informasi yang dibutuhkan terutama dalam melakukan ekstraksi sehingga dapat memprediksi da...

  13. White dwarf axions, PAMELA data, and flipped-SU(5)

    Energy Technology Data Exchange (ETDEWEB)

    Bae, Kyu Jung [Department of Physics and Astronomy and Center for Theoretical Physics, Seoul National University, Seoul 151-747 (Korea, Republic of); Huh, Ji-Haeng [Department of Physics and Astronomy and Center for Theoretical Physics, Seoul National University, Seoul 151-747 (Korea, Republic of)], E-mail: jhhuh@phya.snu.ac.kr; Kim, Jihn E. [Department of Physics and Astronomy and Center for Theoretical Physics, Seoul National University, Seoul 151-747 (Korea, Republic of)], E-mail: jekim@ctp.snu.ac.kr; Kyae, Bumseok [Department of Physics and Astronomy and Center for Theoretical Physics, Seoul National University, Seoul 151-747 (Korea, Republic of)], E-mail: bskyae@gmail.com; Viollier, Raoul D. [Institute of Theoretical Physics and Astrophysics, Department of Physics, University of Cape Town, Private Bag, Rondebosch 7701 (South Africa)

    2009-08-11

    Recently, there are two hints arising from physics beyond the standard model. One is a possible energy loss mechanism due to emission of very weakly interacting light particles from white dwarf stars, with a coupling strength {approx}0.7x10{sup -13}, and another is the high energy positrons observed by the PAMELA satellite experiment. We construct a supersymmetric flipped-SU(5) model, SU(5)xU(1){sub X} with appropriate additional symmetries, [U(1){sub H}]{sub gauge}x[U(1){sub R}xU(1){sub {gamma}}]{sub global}xZ{sub 2}, such that these are explained by a very light electrophilic axion of mass 0.5 meV from the spontaneously broken U(1){sub {gamma}} and two component cold dark matters from Z{sub 2} parity. We show that in the flipped-SU(5) there exists a basic mechanism for allowing excess positrons through the charged SU(5) singlet leptons, but not allowing antiproton excess due to the absence of the SU(5) singlet quarks. We show the discovery potential of the charged SU(5) singlet E at the LHC experiments by observing the electron and positron spectrum. With these symmetries, we also comment on the mass hierarchy between the top and bottom quarks.

  14. Analisis Ketelitian Geometrik Citra Satelit Pleiades 1B dan Geoeye untuk Pembuatan Peta Dasar RDTR Kawasan Pesisir (Studi Kasus: Kecamatan Bulak, Surabaya, Jawa Timur

    Directory of Open Access Journals (Sweden)

    Moh. Mahfudhdin Alawy

    2017-01-01

    Full Text Available Tersedianya berbagai macam citra satelit resolusi tinggi dengan ketelitian yang sangat baik yaitu kurang dari satu meter menunjukkan telah berkembangnya teknologi penginderaan jauh saat ini, hal tersebut menjadi kemajuan pula pada ketelitian berbagai peta dasar yang mengharuskan skala yang tinggi misalkan minimal 1:5000 pada penyusunan peta dasar rencana detil tata ruang baik perkotaan, industri maupun pesisir yang mana akan diulas pada penelitian ini. Tentunya untuk memenuhi skala yang tinggi, citra satelit resolusi tinggi tersebut harus diolah dan dikoreksi geometriknya untuk meminimalisir kesalahan. Data yang digunakan dalam penelitian ini merupakan data citra satelit resolusi tinggi Pleiades 1B tahun 2015 dan Geoeye tahun 2013. Sebagaimana untuk memenuhi ketelitian skala peta yang tinggi yaitu minimal 1:5000, maka pada penelitian ini kedua citra tersebut dilakukan proses koreksi geometrik dengan metode transformasi yang digunakan adalah Affine dan Polynomial Orde 2. Sebagai data penunjang yaitu data Titik Kontrol Tanah (GCP sebanyak 9 titik dan titik Independent Check Point (ICP sebanyak 23 titik yang diukur menggunakan GPS Geodetic serta 21 data pengukuran Jarak Planimetris, data ini digunakan untuk proses koreksi geometrik sampai dengan uji ketelitian geometric yang dilakukan pada masing-masing citra . Pada akhirnya hasil dari penelitian ini menunjukkan bahwa dari kedua citra yang telah dilakukan penelitian memiliki hasil nilai ketelitian yang memenuhi standar ketelitian peta sampai dengan skala 1:5000 pada kelas 1, dengan rincian proses koreksi geometrik  rektifikasi menghasilkan nilai RMS Error yang menunjukkan bahwa metode Polynomial Orde 2 pada citra Pleiades 1B 0,158 dan Geoeye 0,089 memiliki nilai RMS Error yang lebih baik dari metode Affine pada Pleides 1B 0,253 dan Geoeye 0,173, ketelitian geometrik horizontal CE90 citra satelit Geoeye dengan nilai 0,697 yang lebih baik dibandingkan dengan Pleiades 1B yeng memiliki nilai 0

  15. The PAMELA Mission: Heralding a new era in precision cosmic ray physics

    International Nuclear Information System (INIS)

    Adriani, O.; Barbarino, G.C.; Bazilevskaya, G.A.; Bellotti, R.; Boezio, M.; Bogomolov, E.A.; Bongi, M.; Bonvicini, V.; Bottai, S.; Bruno, A.; Cafagna, F.; Campana, D.; Carbone, R.; Carlson, P.; Casolino, M.; Castellini, G.

    2014-01-01

    On the 15th of June 2006, the PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne experiment was launched onboard the Russian Resurs-DK1 satellite by a Soyuz rocket from the Baikonur space centre. The satellite was placed in a quasi-polar 70°inclination orbit at an altitude varying between 350 km and 600 km. New results on the antiparticle component of the cosmic radiation were obtained. The positron energy spectrum and positron fraction were measured from 400 MeV up to 200 GeV revealing a positron excess over the predictions of commonly used propagation models. This can be interpreted either as evidence that the propagation models should be revised or in terms of dark matter annihilation or a pulsar contribution. The antiproton spectrum was measured over the energy range from 60 MeV to 350 GeV. The antiproton spectrum is consistent with secondary production and significantly constrains dark matter models. The energy spectra of protons and helium nuclei were measured up to 1.2 TV. The spectral shapes of these two species are different and cannot be described well by a single power law. For the first time the electron spectrum was measured up to 600 GeV complementing the information obtained from the positron data. Nuclear and isotopic composition was obtained with unprecedented precision. The variation of the low energy proton, electron and positron energy spectra was measured from July 2006 until December 2009 accurately sampling the unusual conditions of the most recent solar minimum activity period (2006–2009). Low energy particle spectra were accurately measured also for various solar events that occurred during the PAMELA mission. The Earth’s magnetosphere was studied measuring the particle radiation in different regions of the magnetosphere. Energy spectra and composition of sub-cutoff and trapped particles were obtained. For the first time a belt of trapped antiprotons was detected in the South Atlantic

  16. The PAMELA Mission: Heralding a new era in precision cosmic ray physics

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G.C. [University of Naples “Federico II”, Department of Physics, I-80126 Naples (Italy); INFN, Sezione di Naples, I-80126 Naples (Italy); Bazilevskaya, G.A. [Lebedev Physical Institute, RU-119991 Moscow (Russian Federation); Bellotti, R. [University of Bari, Department of Physics, I-70126 Bari (Italy); INFN, Sezione di Bari, I-70126 Bari (Italy); Boezio, M. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E.A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bongi, M. [University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence (Italy); INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bonvicini, V. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bruno, A. [University of Bari, Department of Physics, I-70126 Bari (Italy); INFN, Sezione di Bari, I-70126 Bari (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carbone, R. [INFN, Sezione di Naples, I-80126 Naples (Italy); INFN, Sezione di Trieste, I-34149 Trieste (Italy); Carlson, P. [KTH Royal Institute of Technology, Department of Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M. [INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome (Italy); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); and others

    2014-11-30

    On the 15th of June 2006, the PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) satellite-borne experiment was launched onboard the Russian Resurs-DK1 satellite by a Soyuz rocket from the Baikonur space centre. The satellite was placed in a quasi-polar 70°inclination orbit at an altitude varying between 350 km and 600 km. New results on the antiparticle component of the cosmic radiation were obtained. The positron energy spectrum and positron fraction were measured from 400 MeV up to 200 GeV revealing a positron excess over the predictions of commonly used propagation models. This can be interpreted either as evidence that the propagation models should be revised or in terms of dark matter annihilation or a pulsar contribution. The antiproton spectrum was measured over the energy range from 60 MeV to 350 GeV. The antiproton spectrum is consistent with secondary production and significantly constrains dark matter models. The energy spectra of protons and helium nuclei were measured up to 1.2 TV. The spectral shapes of these two species are different and cannot be described well by a single power law. For the first time the electron spectrum was measured up to 600 GeV complementing the information obtained from the positron data. Nuclear and isotopic composition was obtained with unprecedented precision. The variation of the low energy proton, electron and positron energy spectra was measured from July 2006 until December 2009 accurately sampling the unusual conditions of the most recent solar minimum activity period (2006–2009). Low energy particle spectra were accurately measured also for various solar events that occurred during the PAMELA mission. The Earth’s magnetosphere was studied measuring the particle radiation in different regions of the magnetosphere. Energy spectra and composition of sub-cutoff and trapped particles were obtained. For the first time a belt of trapped antiprotons was detected in the South Atlantic

  17. Kajian Dampak Perubahan Garis Pantai Terhadap Penggunaan Lahan Berdasarkan Analisa Penginderaan Jauh Satelit Di Kecamatan Paiton, Kabupaten Probolinggo Jawa Timur

    OpenAIRE

    Prameswari, Siti Rahmi; D. S, Agus Anugroho; Rifai, Azis

    2014-01-01

    Penelitian ini bertujuan untuk mengetahui dampak Perubahan garis pantai terhadap Perubahan lahan pesisir di Kecamatan Paiton dalam jangka waktu 16 tahun dengan menggunakan analisa penginderaan jauh satelit. Penelitian ini menggunakan metode penelitian kuantitatif yakni metode penelitian ilmiah yang sistematis terhadap bagian-bagian dan fenomena serta hubungan-hubungannya yang berkaitan dengan fenomena alam sedangkan metode pengambilan sampel menggunakan metode Purposive Sampling Method yaitu ...

  18. SOLAR MODULATION OF THE LOCAL INTERSTELLAR SPECTRUM WITH VOYAGER 1 , AMS-02, PAMELA , AND BESS

    Energy Technology Data Exchange (ETDEWEB)

    Corti, C.; Bindi, V.; Consolandi, C.; Whitman, K., E-mail: corti@hawaii.edu [Physics and Astronomy Department, University of Hawaii at Manoa, Honolulu, HI 96822 (United States)

    2016-09-20

    In recent years, the increasing precision of direct cosmic rays measurements opened the door to high-sensitivity indirect searches of dark matter and to more accurate predictions for radiation doses received by astronauts and electronics in space. The key ingredients in the study of these phenomena are the knowledge of the local interstellar spectrum (LIS) of galactic cosmic rays and the understanding of how the solar modulation affects the LIS inside the heliosphere. Voyager 1 , AMS-02, PAMELA , and BESS measurements of proton and helium fluxes provide valuable information, allowing us to shed light on the shape of the LIS and the details of the solar modulation during solar cycles 22-24. A new parametrization of the LIS is presented, based on the latest data from Voyager 1 and AMS-02. Using the framework of the force-field approximation, the solar modulation parameter is extracted from the time-dependent fluxes measured by PAMELA and BESS . A modified version of the force-field approximation with a rigidity-dependent modulation parameter is introduced, yielding better fits than the force-field approximation. The results are compared with the modulation parameter inferred by neutron monitors.

  19. Título da página electrónica: Pamela Oliver Homepage

    Directory of Open Access Journals (Sweden)

    José Manuel Mendes

    2012-10-01

    Full Text Available Esta é a página pessoal de Pamela Oliver, professora do Departamento de Sociologia na Universidade de Wisconsin-Madison, nos Estados Unidos. A autora é especialista no estudo dos movimentos sociais e no protesto social, tanto numa vertente quantitativa como qualitativa. Realço nesta página a secção intitulada Protest Dynamics (Dinâmicas de Protesto. Entre os vários artigos disponibilizados, são de especial importância os que se atêm à análise do papel dos media na construção dos aconteciment...

  20. Pamela: una donna goldoniana in Russia con Eleonora Duse

    Directory of Open Access Journals (Sweden)

    Maria Pia Pagani

    2012-01-01

    Full Text Available In Venice (Casa Goldoni Library there is a libretto with a summary of Pamela maiden, which was deliberately prepared for the representation of Eleonora Duse in St. Petersburg, on 11th April 1891. It was printed by the publisher V. K. Travsky – with approval of the Russian censorship issued on 13th March 1891 – at the Typography of the Ministry of Internal Affairs, in limited edition. It was created by an anonymous Russian man of letters to help the public in the comprehension of the plot of the comedy, because the actors played using Italian language.This essay presents the first annotated Italian translation of this libretto, and a reflection about Duse’s first tour in Russia – with particular attention to the diffusion process “outside” the Italian boundaries of this Goldoni’s comedy, which was in her repertory “inside” the national territory since 1880.

  1. Consequences of a dark disk for the Fermi and PAMELA signals in theories with a Sommerfeld enhancement

    International Nuclear Information System (INIS)

    Cholis, Ilias; Goodenough, Lisa

    2010-01-01

    Much attention has been given to dark matter explanations of the PAMELA positron fraction and Fermi electronic excesses. For those theories with a TeV-scale WIMP annihilating through a light force-carrier, the associated Sommerfeld enhancement provides a natural explanation of the large boost factor needed to explain the signals, and the light force-carrier naturally gives rise to hard cosmic ray spectra without excess π 0 -gamma rays or anti-protons. The Sommerfeld enhancement of the annihilation rate, which at low relative velocities v rel scales as 1/v rel , relies on the comparatively low velocity dispersion of the dark matter particles in the smooth halo. Dark matter substructures in which the velocity dispersion is smaller than in the smooth halo have even larger annihilation rates. N-body simulations containing only dark matter predict the existence of such structures, for example subhalos and caustics, and the effects of these substructures on dark matter indirect detection signals have been studied extensively. The addition of baryons into cosmological simulations of disk-dominated galaxies gives rise to an additional substructure component, a dark disk. The disk has a lower velocity dispersion than the spherical halo component by a factor ∼ 6, so the contributions to dark matter signals from the disk can be more significant in Sommerfeld models than for WIMPs without such low-velocity ehancements. We consider the consequences of a dark disk on the observed signals of e + e − , p p-bar and γ-rays as measured by Fermi and PAMELA in models where the WIMP annihilations are into a light boson. We find that both the PAMELA and Fermi results are easily accomodated by scenarios in which a disk signal is included with the standard spherical halo signal. If contributions from the dark disk are important, limits from extrapolations to the center of the galaxy contain significant uncertainties beyond those from the spherical halo profile alone

  2. Kajian Spasial Suhu Permukaan Laut Akibat Air Bahang Pltu Paiton Menggunakan Saluran Termal Satelit Landsat 7/etm+ Di Pantai Bhinor Kabupaten Probolinggo Jawa Timur

    OpenAIRE

    Ismayati, Qorihah; Helmi, Muhammad; Rochaddi, Baskoro

    2013-01-01

    Penelitian bertujuan untuk memetakan secara horisontal suhu permukaan laut di perairan PLTU Paiton Probolinggo dan mengkaji sebaran spasial termal perairan akibat air bahang PLTU Paiton Probolinggo. Pengolahan data citra dilakukan menggunakan perangkat lunak ER Mapper 7.0 dan ArcGIS 9.3. Data yang digunakan dalam penelitian adalah citra Satelit Landsat 7ETM+ tahun 2009 hingga tahun 2012, data arus permukaan dan angin yang diperoleh dari BMKG Maritim Perak Surabaya dan data hasil pengukuran la...

  3. Comparación de anomalías de gravedad derivadas de altimetría satelital con datos de gravedad marina en el margen continental Argentino

    Directory of Open Access Journals (Sweden)

    Ana Carolina Pedraza De Marchi

    Full Text Available En este trabajo se comparan grillas de anomalías de gravedad derivadas de misiones de altimetría satelital con anomalías de gravedad marina a partir de datos de cruceros en el margen continental argentino y zona oceánica adyacente. Se analizan las diferencias entre estas fuentes de datos, ya que es de esperar que éstas sean significativas en zonas costeras o de gradiente horizontal de gravedad abrupto como en el talud continental; se trata de identificar y delimitar dichas zonas. Asimismo se analizan los datos de barco de distintas campañas realizadas en épocas diferentes para organizarlos en una base de datos común, como parte de un proceso de compilación en el que se crearán versiones mejoradas con nuevas correcciones en la medida en que se incorporen más datos en el futuro. Se investiga cuál de las grillas de gravedad derivada de altimetría satelital presenta mejor ajuste con la compilación marina a fin de caracterizarla como la recomendable para su uso en posteriores aplicaciones. Se presentan aquí los resultados de la primera etapa completada en función del alcance los objetivos mencionados.

  4. Ecoepidemiología y epidemiología satelital: nuevas herramientas en el manejo de problemas en salud pública

    Directory of Open Access Journals (Sweden)

    Alfonso J. Rodríguez-Morales

    2005-03-01

    Full Text Available Los recientes avances en la comprensión del ambiente en el cual ocurre la transmisión de muchas enfermedades infecciosas de importancia en salud pública en particular las transmitidas por vectores, ha permitido generar una serie de conceptos y herramientas que están modificando el abordaje de los problemas complejos en salud pública. Así, la ecoepidemiología y más recientemente la epidemiología satelital, brindan un potencial de opciones que se traducen en visiones más integradas de las enfermedades y nuevas posibilidades para prevenirlas y controlarlas. La presente revisión refleja los conceptos en evolución vinculados con estas nuevas ramas de la epidemiología y la salud pública.

  5. Spatial gradients of GCR protons in the inner heliosphere derived from Ulysses COSPIN/KET and PAMELA measurements

    Science.gov (United States)

    Gieseler, J.; Heber, B.

    2016-05-01

    Context. During the transition from solar cycle 23 to 24 from 2006 to 2009, the Sun was in an unusual solar minimum with very low activity over a long period. These exceptional conditions included a very low interplanetary magnetic field (IMF) strength and a high tilt angle, which both play an important role in the modulation of galactic cosmic rays (GCR) in the heliosphere. Thus, the radial and latitudinal gradients of GCRs are very much expected to depend not only on the solar magnetic epoch, but also on the overall modulation level. Aims: We determine the non-local radial and the latitudinal gradients of protons in the rigidity range from ~0.45 to 2 GV. Methods: This was accomplished by using data from the satellite-borne experiment Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) at Earth and the Kiel Electron Telescope (KET) onboard Ulysses on its highly inclined Keplerian orbit around the Sun with the aphelion at Jupiter's orbit. Results: In comparison to the previous A> 0 solar magnetic epoch, we find that the absolute value of the latitudinal gradient is lower at higher and higher at lower rigidities. This energy dependence is therefore a crucial test for models that describe the cosmic ray transport in the inner heliosphere.

  6. Resultados del uso de geodesia satelital para estudios geodinámicos en Colombia

    Directory of Open Access Journals (Sweden)

    Mora-Páez Hector

    2002-08-01

    Full Text Available

    The use of GPS technology provides direct measurements of displacements due to plate motions and intraplate deformation, basic information for understanding kinematic of the movements. Using satelital geodesy techniques, crustal deformation rates in the southwestern Caribbean, southeastern of Central America and northwestern of South America wide plate boundary have been derived from GPS campaigns in 1988, 1990, 1991, 1994, 1996 and 1998 as part of the CASA (Central And South America GPS Project. The zone of study includes the area of complex interaction between the Caribbean, Nazca and South America plates. The same GPS stations have been occupied with the purpose of making comparisons on the position of each site, analyzing distances of separation (baselines and obtaining displacement vectors (magnitude and orientation. Some results are showed using the GIPSY -OASIS II software, that is a precision package for the analysis of GPS data developed by JPL-NASA. INGEOMINAS has built a GPS network called GEORED to be occupied succesively in order to get information about intraplate deformation, under the institutional project named Survey, Compilation and Generation of Geodynamics Information.

    EI uso de la tecnología GPS provee mediciones directas de los desplazamientos debido al movimiento de las placas y la deformación intraplaca, información básica para el entendimiento de la cinemática de los movimientos, Empleando técnicas de geodesia satelital, tasas de deformación de corteza terrestre en el límite amplio de placas al suroeste del Caribe, sureste de América Central y noroeste de Suramérica han sido

  7. VEGETACIÓN DEL PARQUE COPAHUE: APLICACIÓN DE UNA METODOLOGÍA BIOCLIMÁTICA MEDIANTE EL USO DE INFORMACIÓN SATELITAL Y SIG

    Directory of Open Access Journals (Sweden)

    Oscar Peña

    2003-12-01

    Full Text Available La distribución de la vegetación natural se encuentra en intima relación con el comportamiento de los elementos climáticos tal como la temperatura y la humedad. Asimismo la altitud, la orientación (exposición a la radiación y la pendiente modifican dicho comportamiento. El Parque Provincial Copahue, localizado en la Provincia de Neuquen, en la cordillera norpatagónica, presenta características biogeográficas y particularidades ecogeomorfológicas que evidencian el marcado efecto de las variables climáticas. El presente trabajo tiene por objetivo analizar las relaciones de dichas variables mediante la utilización de una metodología bioclimática y el tratamiento digital de imágenes Landsat Tm. Metodológicamente se procedió en tres pasos. El primero consistió en la clasificación supervisada de la imagen satelital. De esto surgió una carta de vegetación del parque. En el segundo paso se digitalizó cartografía 1:100.000 con la que se obtuvo un modelo digital de elevación, mapa de pendiente y de orientación de laderas, de temperaturas y precipitaciones. En el tercero, se confeccionó una base de datos para la aplicación de una metodología bioclimática (Rivas y Martínez.1994 que permitió, mediante la aplicación del SIG delimitar los bioclimas del parque. La información de vegetación obtenida mediante la clasificación digital de la imagen satelital fue cruzada con el mapa bioclimático, el mapa topográfico, de pendiente, orientación y de las variables climáticas consideradas, a fin de conocer el grado de interrelación entre la distribución de la vegetación con las variables físicas tratadas.

  8. TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUM

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [Department of Physics, University of Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [Department of Physics, University of Naples ' ' Federico II' ' , I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991 Moscow (Russian Federation); Bellotti, R.; Bruno, A. [Department of Physics, University of Bari, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Borisov, S.; De Pascale, M. P.; De Santis, C.; De Simone, N. [INFN, Sezione di Rome ' ' Tor Vergata' ' , I-00133 Rome (Italy); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M. [Department of Physics, University of Rome ' ' Tor Vergata' ' , I-00133 Rome (Italy); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); and others

    2013-03-10

    The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation.

  9. Tritium in Meteorites and in Recovered Satellite Material; Tritium dans les meteorites et dans les matieres provenant d'un satellite recupere; Tritij v meteoritakh i v vozvrashchennom sputnike; Tritio en meteoritos y en el material de un satelite recuperado

    Energy Technology Data Exchange (ETDEWEB)

    Fireman, E L [Smithsonian Astrophysical Observatory, Cambridge, MA (United States)

    1962-01-15

    Tritium was measured in separated phases and in whole rock samples of the Bruderheim chondritic meteorite and in samples of lead and iron material of recovered satellites. Radioactive isotopes of argon were also measured. The tritium and argon radioactivity in the Bruderheim meteorite can be reasonably well explained by the interaction of cosmic ray particles of some thousand million volts energy with the meteoritic material. The tritium content of the recovered satellite material was more than a factor of a hundred too large to be explained by the interactions of cosmic rays or by the interactions of solar flare particles with the satellite. The high tritium content of the satellite material must result from a flux of incident tritium particles that stop in the satellite. (author) [French] Tritium dans les meteorites et dans les matieres provenant d'un satellite recupere. On a mesure la teneur en tritium d'echantillons de diverses parties et de l'ensemble de la roche formant la chondrite de Bruderheim, ainsi que celle d'echantillons de plomb et de fer preleves sur des satellites recuperes. On a egalement mesure la teneur en radioargon dans la meteorite de Bruderheim. La presence de tritium et de radioargon peut fort bien s'expliquer par l'interaction d'elements de la meteorite et de rayons cosmiques corpusculaires ayant une energie de l'ordre du milliard de volts. La teneur en tritium des satellites recuperes etait plus de cent fois trop elevee pour pouvoir etre expliquee par une interaction entre les rayons cosmiques ou les particules provenant d'eruptions solaires et le satellite etudie. La forte teneur en tritium des matieres provenant des satellites est certainement due a un flux incident de particules de tritium qui sont retenues dans le satellite. (author) [Spanish] Se midieron las concentraciones de tritio en fases separadas y en muestras enteras de roca del meteorito condritico de Bruderheim, y en muestras de plomo y de hierro de satelites recuperados

  10. Experiencia clínica en monitorización cardiaca extendida con el sistema inalámbrico satelital tipo SEEQ

    Directory of Open Access Journals (Sweden)

    Diego Vanegas-Cadavid

    2018-05-01

    Full Text Available Resumen: Objetivos: Dar a conocer la experiencia clínica con un nuevo sistema de monitorización cardiaca extendida (por 15 días, inalámbrica y satelital en un grupo de pacientes con sospecha de arritmias cardíacas. Metodología: Cohorte de 100 pacientes atendidos en la unidad de Electrofisiología cardiovascular de un centro de referencia, con sospecha de arritmia cardíaca, sin diagnóstico electrocardiográfico causal, a pesar de exámenes previos. Se les aplicó una monitorización cardiaca externa tipo SEEQ (Medtronic por 15 días y se registró el desenlace. Resultados: De un total de 100 sujetos estudiados, 51% eran hombres, con mediana de edad de 60 años (rango: 5 - 91 años. El principal síntoma fueron las palpitaciones (42% y la comorbilidad más prevalente la hipertensión arterial (47%; 98% tenían estudio de Holter previo y 46% dos estudios sin resultado conclusivo que explicara los síntomas. La monitorización tipo SEEQ documentó anormalidad electrocardiográfica significativa en 22% de los pacientes. El implante de marcapaso fue el tratamiento más aplicado y la fibrilación auricular fue la arritmia más frecuente en el 50% de los hallazgos positivos. Hubo una proporción mayor y significativa de diagnósticos positivos en el sexo masculino. Conclusiones: La monitorización cardiaca externa inalámbrica, satelital, extendida por 15 días es una herramienta novedosa que incrementa la probabilidad de documentar una anormalidad electrocardiográfica clínicamente significativa en quienes padecen síntomas cardiovasculares recurrentes. Abstract: Objectives: To present the clinical experience with a new extended (for 15 days, wireless, and satellite cardiac monitoring system in a group of patients with suspicion of cardiac arrhythmia. Method: The study included a cohort of 100 patients seen in the Cardiovascular Electrophysiology Unit of a reference hospital. They were suspected of having a cardiac arrhythmia, with no

  11. Can past gamma-ray bursts explain both INTEGRAL and ATIC/PAMELA/Fermi anomalies simultaneously?

    International Nuclear Information System (INIS)

    Calvez, Antoine; Kusenko, Alexander

    2010-01-01

    Gamma-ray bursts (GRBs) have been invoked to explain both the 511 keV emission from the Galactic bulge and the high-energy positron excess inferred from the ATIC, PAMELA, and Fermi data. While independent explanations can be responsible for these phenomena, we explore the possibility of their common GRB-related origin by modeling the GRB distribution and estimating the rates. For an expected Milky Way long GRB rate, neither of the two signals is generic; the local excess requires a 2% coincidence while the signal from the Galactic center requires a 20% coincidence with respect to the timing of the latest GRB. The simultaneous explanation requires a 0.4% coincidence. Considering the large number of statistical 'trials' created by multiple searches for new physics, the coincidences of a few percent cannot be dismissed as unlikely. Alternatively, both phenomena can be explained by GRB if the Galactic rate is higher than expected. We also show that a similar result is difficult to obtain assuming a simplified short GRB distribution.

  12. Introduction to the AMS Experiment

    CERN Multimedia

    CERN. Geneva

    2015-01-01

    Following the pioneering experiments (ATIC, BESS, CREAM, HEAT, PAMELA, …), using a magnetic spectrometer (AMS) on ISS is a unique way to provide precision long term measurements of primordial high energy charged cosmic rays. AMS was installed on the Station in May 2011. Up to now, 60 billion events have been collected. 40 billion events have been partially analysed. AMS is scheduled to be on the Station until at least 2024. By then AMS will have collected close to 200 billion events. The detector properties and the analysis methods will be introduced.

  13. Proyecto II: Diseño de un plan de marketing de retención y fidelización de clientes para el servicio de televisión satelital en la CNT EP

    OpenAIRE

    Mejía Salazar, Andrés Rafael

    2014-01-01

    Teniendo como base el estudio de mercado realizado en el proyecto de investigación en donde se detectó las causas principales de deserción de los clientes en el servicio de Televisión Satelital en la CNT EP; se realiza un plan de marketing de retención, fidelización y recuperación de clientes. Los puntos clave del plan de marketing se enfocan primeramente en un direccionamiento estratégico del servicio para saber cómo se va a posicionar en corto y mediano plazo el producto de DTH. Se plantea ...

  14. UNIVERSITE DE GENEVE

    CERN Multimedia

    2007-01-01

    Ecole de physique - Département de physique nucléaire et corspusculaire 24, Quai Ernest-Ansermet
1211 GENEVE 4
Tél: (022) 379 62 73 - Fax: (022) 379 69 92 Wednesday 3rd October 2007 PARTICLE PHYSICS SEMINAR at 17:00 - Stückelberg Auditorium The first year in orbit of the PAMELA space experiment by Dr Silvio Orsi, INFN Roma Tor Vergata The satellite-borne PAMELA experiment is designed to study charged particles in the cosmic radiation with a particular focus on antiparticles. PAMELA is mounted on the Resurs DK1 satellite that was launched from the Baikonur cosmodrome in Kazakhstan on June 15th 2006 and has a lifetime of at least 3 years. The PAMELA apparatus comprises a time-of-flight system, a magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. PAMELA is performing indirect dark matter search through a detailed study of the positron and antiproton spectra (50Me...

  15. Automatic classification of pathological myopia in retinal fundus images using PAMELA

    Science.gov (United States)

    Liu, Jiang; Wong, Damon W. K.; Tan, Ngan Meng; Zhang, Zhuo; Lu, Shijian; Lim, Joo Hwee; Li, Huiqi; Saw, Seang Mei; Tong, Louis; Wong, Tien Yin

    2010-03-01

    Pathological myopia is the seventh leading cause of blindness. We introduce a framework based on PAMELA (PAthological Myopia dEtection through peripapilLary Atrophy) for the detection of pathological myopia from fundus images. The framework consists of a pre-processing stage which extracts a region of interest centered on the optic disc. Subsequently, three analysis modules focus on detecting specific visual indicators. The optic disc tilt ratio module gives a measure of the axial elongation of the eye through inference from the deformation of the optic disc. In the texturebased ROI assessment module, contextual knowledge is used to demarcate the ROI into four distinct, clinically-relevant zones in which information from an entropy transform of the ROI is analyzed and metrics generated. In particular, the preferential appearance of peripapillary atrophy (PPA) in the temporal zone compared to the nasal zone is utilized by calculating ratios of the metrics. The PPA detection module obtains an outer boundary through a level-set method, and subtracts this region against the optic disc boundary. Temporal and nasal zones are obtained from the remnants to generate associated hue and color values. The outputs of the three modules are used as in a SVM model to determine the presence of pathological myopia in a retinal fundus image. Using images from the Singapore Eye Research Institute, the proposed framework reported an optimized accuracy of 90% and a sensitivity and specificity of 0.85 and 0.95 respectively, indicating promise for the use of the proposed system as a screening tool for pathological myopia.

  16. Study of Primary Cosmic Ray Electrons In Energy Range 10^11 - 10^13 Ev By Pamela Instrument.

    Science.gov (United States)

    Voronov, S.; Pamela Collaboration

    The main goal of the magnetic spectrometer PAMELA is the study of antiparticle fluxes with energy up to 300 GeV in cosmic rays on board satellite. A modification of instrument was done by introducing of neutron detector. This device was placed under imaging calorimeter and bottom scintillator counter. It consists of two layers of 36 3He gas counters enveloped by a polyethylene moderator. The neutron detector gives additional possibility to identify the antiprotons going in aperture of spectrome- ter and generating the nuclear cascade in tungsten plates of calorimeter. This shower is followed by big number of neutrons in contrast to electromagnetic one caused by elec- tron or positron. From other side the combination of the imaging calorimeter, bottom scintillator and neutron detector constitute the independent instrument with large field of view which gives the possibility to measure the electron-positron cosmic ray com- ponent in energy range 1011-1013 eV with a rejection factor of order 10-4 regarding to nuclear one.

  17. Qualification and characterization programmes for disposal of a glass product resulting from high level waste vitrification in the PAMELA installation of BELGOPROCESS

    International Nuclear Information System (INIS)

    Goeyse, A. de; De, A.K.; Demonie, M.; Iseghem, P. van

    1993-01-01

    In the framework of a general quality assurance and quality control (QA/QC) programme, the quality of a conditioned waste product is achieved in two phases. The first phase is the design of a process and facility which will ensure the required quality of the product. In the second phase the conformance of the product with the preset requirements is verified. NIRAS/ONDRAF, as the agency responsible for the management of all radioactive waste in Belgium (including treatment, conditioning, storage and disposal), controls compliance with the quality requirements during both phases. The purpose of the paper is to describe the different phases of this general procedure in the case of a vitrified HLW product resulting from a vitrification campaign in the PAMELA facility at the BELGOPROCESS site. The active glass product of type SM527 produced during the vitrification of highly enriched waste concentrate (HEWC) (resulting from the reprocessing of highly enriched uranium fuel) has been selected for illustration. During the process qualification phase, the Deutsche Gesellschaft fuer Wiederaufarbeitung von Kernbrennstoffen mbH, responsible for the development of the vitrification process of PAMELA, defined and performed and R and D programmed for each glass product originating from the vitrification of the different HEWC solutions stored at the BELGOPROCESS site. At the end of this qualification phase a data catalogue was prepared. In order to ensure that the active glass product corresponds with the selected product from the data catalogue, the QA/QC handbook for the vitrification process describes all measures to be taken by the waste producer, BELGOPROCESS, during the vitrification. Finally, verification analyses are performed by the characterization of inactive and active samples by an independent laboratory. This phase is called the product quality verification phase. The details of the characterization programmes performed during the different phases and their results

  18. New Fixed-Target Experiments to Search for Dark Gauge Forces

    Energy Technology Data Exchange (ETDEWEB)

    Bjorken, James D.; Essig, Rouven; Schuster, Philip; /SLAC; Toro, Natalia; /Stanford U., ITP

    2010-06-11

    Fixed-target experiments are ideally suited for discovering new MeV-GeV mass U(1) gauge bosons through their kinetic mixing with the photon. In this paper, we identify the production and decay properties of new light gauge bosons that dictate fixed-target search strategies. We summarize existing limits and suggest five new experimental approaches that we anticipate can cover most of the natural parameter space, using currently operating GeV-energy beams and well-established detection methods. Such experiments are particularly timely in light of recent terrestrial and astrophysical anomalies (PAMELA, FERMI, DAMA/LIBRA, etc.) consistent with dark matter charged under a new gauge force.

  19. Analisa Ketelitian Geometrik Citra Resolusi Tinggi Hasil Ortorektifikasi pada Pembuatan Peta Skala 1: 5000

    Directory of Open Access Journals (Sweden)

    Achmad Rizal Al-Amin

    2017-03-01

    Full Text Available Di era teknologi yang berkembang pesat, berbagai metode survei telah banyak digunakan salah satunya dengan cara penginderaan jauh menggunakan satelit. Sebagaimana diketahui bahwa proses perekaman citra satelit diliput dari wahana (satelit yang bergerak di atas permukaan bumi pada ketinggian ratusan kilometer, sehingga menyebabkan citra satelit memiliki distorsi geometrik. Untuk mengurangi pengaruh distorsi geometrik objek pada citra, dilakukan koreksi geometrik dengan cara ortorektifikasi. Pleiades merupakan satelit penghasil citra satelit resolusi tinggi yang dibuat oleh perusahaan Airbus Defence & Space. Citra satelit yang dihasilkan memiliki resolusi spasial 0,5 meter Sebagai acuan bagi kegiatan pemanfaatan ruang yang lebih rinci dari kegiatan pemanfaatan ruang yang diatur dalam Rencana Tata Ruang Wilayah (RTRW, maka dibuat Rencana Detail Tata Ruang (RDTR dengan peta skala 1:5.000 yang telah diatur oleh Badan Informasi Geospasial. Dalam proses ortorektifikasi citra satelit untuk pembuatan peta skala 1 : 5000 ini, digunakan titik kontrol tanah atau Ground Control Point (GCP untuk proses koreksi geometris dan data Digital Elevation Model (DEM. Pada penelitian ini dilakukan proses ortorektifikasi dengan metode polinomial Rational Function menggunakan 21 GCP pada polinomial orde 2. Didapat nilai RMS Error jarak pada citra hasil ortorektifikasi sebesar 0.419 meter, tetapi masih masuk toleransi untuk pembuatan peta skala 1:5000 pada uji statistik T-Test dengan α=5% & α=10%. Didapat juga nilai pixel citra sebelum ortorektifikasi sebesar 0,543592 meter sedangkan setelah ortorektifikasi sebesar 0,500032 meter. Yang berarti, setelah proses ortorektifikasi, nilai pixel sesuai dengan resolusi spasial citra ≈ 0,5 meter.

  20. Fermi/LAT observations of dwarf galaxies highly constrain a dark matter interpretation of excess positrons seen in AMS-02, HEAT, and PAMELA

    Energy Technology Data Exchange (ETDEWEB)

    López, Alejandro [Michigan Center for Theoretical Physics, University of Michigan – Ann Arbor, 450 Church St., Ann Arbor (United States); Savage, Christopher [Nordita (Nordic Institute for Theoretical Physics), KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, Stockholm (Sweden); Spolyar, Douglas; Adams, Douglas Q., E-mail: aolopez@umich.edu, E-mail: chris@savage.name, E-mail: dspolyar@gmail.com, E-mail: doug.q.adams@gmail.com [Oskar Klein Centre for Cosmoparticle Physics, Stockholm University, Roslagstullsbacken 23, Roslagstullsbacken 21, Stockholm (Sweden)

    2016-03-01

    It is shown that a Weakly Interacting Massive dark matter Particle (WIMP) interpretation for the positron excess observed in a variety of experiments, HEAT, PAMELA, and AMS-02, is highly constrained by the Fermi/LAT observations of dwarf galaxies. In particular, this paper examines the annihilation channels that best fit the current AMS-02 data (Boudaud et al., 2014), specifically focusing on channels and parameter space not previously explored by the Fermi/LAT collaboration. The Fermi satellite has surveyed the γ-ray sky, and its observations of dwarf satellites are used to place strong bounds on the annihilation of WIMPs into a variety of channels. For the single channel case, we find that dark matter annihilation into (b b-bar ,e{sup +}e{sup -}, μ{sup +}μ{sup -}, τ{sup +}τ{sup -},4-e or 4-τ ) is ruled out as an explanation of the AMS positron excess (here b quarks are a proxy for all quarks, gauge and Higgs bosons). In addition, we find that the Fermi/LAT 2σ upper limits, assuming the best-fit AMS-02 branching ratios, exclude multichannel combinations into b b-bar and leptons. The tension between the results might relax if the branching ratios are allowed to deviate from their best-fit values, though a substantial change would be required. Of all the channels we considered, the only viable channel that survives the Fermi/LAT constraint and produces a good fit to the AMS-02 data is annihilation (via a mediator) to 4-μ, or mainly to 4-μ in the case of multichannel combinations.

  1. APLIKASI DATA CITRA SATELIT LANDSAT UNTUK PEMANTAUAN DINAMIKA PESISIR MUARA DAS BARITO DAN SEKITARNYA

    Directory of Open Access Journals (Sweden)

    Abdur Rahman

    2016-06-01

    Full Text Available Telah terjadi terjadi kerusakan habitat lingkungan mangrove, abrasi dan akresi yang menyebabkan semakin tingginya muka air  di sepanjang DAS Sungai Barito (DAS Martapura, DAS Alalak dan DAS Kuin, sebab erjadinya proses abrasi dan akresi  yang terjadi di sepanjang garis pantai, terutama DAS Martapura, DAS Alalak dan DAS Kuin. Klasifikasi pemanfaatan lahan dan konversinya serta perubahan pesisir berupa akresi dan abrasi di sepanjang pantai area penelitian di analisis dengan memanfaatkan informasi dari data citra satelit Landsat multi temporal yang di peroleh pada tanggal 29 Juni tahun 1985, dan 03 September 2006. Dominasi pemanfaatan lahan berupa HPH, pertambangan dan pemukiman dengan konversi lahan pada hutan untuk pemanfaatan lain memberikan dampak erosi yang cukup besar dengan ditunjukannya wilayah pesisir yang mengalami peningkatan akresi terutama pada bagian muara sungai (delta. Tren perubahan yang terlihat pada kawasan pesisir di area penelitian selama 21 tahun adalah abrasi sebesar 294,55 m2 di daerah Muara S. Martapura, 75,53 m2 di sekitar muara S. Alalak. Dan perubahan Abrasi sebesar 177,42 m2 , dan akresi sebesar 610,86 m2 di sekitar Muara S. Barito/Kuin. Have happened happened damage of environmental habitat of mangrove, and abrasi of akresi causing its excelsior of face irrigate alongside DAS River of Barito (DAS Martapura, DAS Alalak and of DAS Kuin, because the happening of process of abrasi and of akresi that happened alongside coastline, especially DAS Martapura, DAS Alalak and  DAS Kuin. Classification exploiting of farm and its conversion and also change of coastal area in the form of and akresi of abrasi alongside research area coast in analysis by exploiting information of satellite image data of Landsat temporal multi which in obtaining on 29 June year 1985, and 03 September 2006. Domination exploiting of farm in the form of HPH, settlement and mining with farm conversion at forest for other exploiting give big enough

  2. Le roman anglais du XVIIIe siècle à l’opéra : la sentimentalité, Pamela et The Maid of the Mill The 18th-century Novel as Opera: Sentimentality, Pamela and The Maid of the Mill

    Directory of Open Access Journals (Sweden)

    Michael Burden

    2011-12-01

    Full Text Available Cet article revient sur la notion de sentimentalité et particulièrement sur l’opéra sentimental qui dérive du roman anglais de même nature. L’idée du triomphe ultime du bien, de la possibilité pour une jeune fille pauvre mais honnête de réussir dans la vie et de la bonté comme lien inaltérable unissant les hommes acquit une telle force à la fin du XVIIIe siècle qu’elle a été utilisée pour la définir. Une des œuvres les plus significatives du style sentimental, Pamela, le roman de Richardson, retint l’attention du librettiste Isaac Bickerstaffe (1733-1808, qui le transforma en « opéra anglais » faisant remarquer que son œuvre, « une bagatelle à bien des points de vue, constituait la première pièce sentimentale qui paraisse sur la scène anglaise depuis 40 ans ». Mis en musique par Samuel Arnold (1740-1802 l’opéra présente un genre nouveau, « l’opéra pastiche », qui incorpore la musique de plusieurs compositeurs. Musicalement, l’opéra n’a rien de très original et selon nos critères actuels, l’absence d’un seul compositeur nettement identifiable ou d’une esthétique de composition particulière en fait un objet d’art difficile à jauger. Mais la simplicité de  la musique elle-même constitue un attribut essentiel qui permet à la sentimentalité de l’histoire de s’exprimer et annonce véritablement la naissance d’un nouveau genre d’opéra anglais, le pastiche. De même, les caractéristiques très particulières des représentations théâtrales en Angleterre ont joué un rôle déterminant dans le développement de l’opéra sentimental à Londres.This article returns to the well-known notion of sentimental culture, and specifically, to sentimental opera derived from the English novel.  The notion that goodness must triumph, that a poor but honest girl should ‘make good’, and that such goodness should form a binding force between humans, was such a strong force in

  3. The AFIS experiment: Detecting low energetic antiprotons in a low earth orbit, using an active target detector

    Energy Technology Data Exchange (ETDEWEB)

    Poeschl, Thomas; Gaisbauer, Dominic; Greenwald, Daniel; Hahn, Alexander; Hauptmann, Philipp; Konorov, Igor; Meng, Lingxin; Paul, Stephan [Physics Department E18, Technische Universitaet Muenchen (Germany); Losekamm, Martin [Physics Department E18, Technische Universitaet Muenchen (Germany); Institute of Astronautics, Technische Universitaet Muenchen (Germany); Renker, Dieter [Physics Department E17, Technische Universitaet Muenchen (Germany)

    2014-07-01

    Since the first observation of geomagnetically trapped antiprotons by the PAMELA experiment and the new results on the positron excess by the AMS-02 experiment, the creation and transport of antimatter in the Earth's upper atmosphere attracts more and more attention both at theoretical and experimental side. For this reason the AFIS experiment was initiated to measure the flux of low energetic antiprotons in the South Atlantic Anomaly (SAA). We developed an active target detector made from scintillating fibers connected to silicon photomultipliers which allows to detect antiprotons in the energy interval of about 30 MeV-100 MeV. The stopping curve of incoming antiprotons (Bragg peak) and the signal of outgoing pions created from the annihilation, are used for particle identification as well as triggering. We plan to implement this detector on a 3 unit cubesat satellite in the framework the 'Move2Warp' mission, which is carried out as a student project by the Technische Universitaet Muenchen.

  4. Precision of GNSS instruments by static method comparing in real time

    Directory of Open Access Journals (Sweden)

    Slavomír Labant

    2009-09-01

    Full Text Available Tablet paper describes comparison of measuring accuracy two apparatus from the firm Leica. One of them recieve signals onlyfrom GPS satelites and another instrument is working with GPS and also with GLONASS satelites. Measuring is carry out by RTK staticmethod with 2 minutes observations. Measurement processing is separated to X, Y (position and h (heigh. Adjustment of directobservations is used as a adjusting method.

  5. Analisa Ketelitian Geometrik Citra Pleiades Sebagai Penunjang Peta Dasar RDTR (Studi Kasus: Wilayah Kabupaten Bangkalan, Jawa Timur

    Directory of Open Access Journals (Sweden)

    Wahyu Teo Parmadi

    2017-01-01

    Full Text Available Sebagai upaya perencanaan pembangunan permukiman digunakan bantuan citra satelit resolusi tinggi seperti citra satelit Pleiades. Untuk dapat dimanfaatkan secara optimal, citra satelit harus sudah terbebas dari kesalahan atau distorsi yang terjadi selama proses perekaman data dengan melakukan koreksi. Koreksi citra bertujuan memperbaiki citra agar sesuai mendekati dengan kondisi objek dipermukaan bumi. Koreksi citra meliputi koreksi radiometrik dan geometrik. Untuk mendapatkan posisi geografi yang akurat  dilakukan proses koreksi geometrik. Dalam penelitian ini koreksi geometrik menggunakan metode koreksi non sistematik dimana setiap piksel pada citra diposisikan sesuai koordinat sebenarnya dengan acuan Ground Control Point (GCP sedangkan untuk koreksi topografi dan distorsi perekaman digunakan data Digital Elevation Model (DEM. Data yang digunakan  yaitu data citra satelit Pleiades dan DEM ALOS-PALSAR tahun 2015. Untuk mengetahui ketelitian dari koreksi geometrik dari citra tersebut berdasarkan pada nilai (Root Mean Square Error RMSe yang didapatkan dari perhitungan matematis koreksi geometrik metode Affine dan metode Rigorous Toutin.Hasil dari penelitian ini menunjukkan ketelitian citra terkoreksi geometrik berdasarkan nilai RMSE menggunakan metode Rigorous Toutin lebih baik yaitu sebesar 1,157 m sedangkan menggunakan metode Affine didapatkan nilai ketelitian sebesar 1,749 m. Dari nilai ketelitian ini dapat disimpulkan bahwa Citra Pleiades terkoreksi dapat digunakan sebagai Peta Dasar RDTR skala 1:5000 kelas 3.

  6. Estimate potential evaporation and solar radiation in the Yaqui valley, Sonora, Mexico, using data from satellite; Estimacion de evaporacion y radiacion solar en el valle del Yaqui, Sonora, usando datos de satelite

    Energy Technology Data Exchange (ETDEWEB)

    J Watts, Christopher; Rodriguez, Julio Cesar [Instituto del Medio Ambiente y el Desarrollo sustentable del estado de Sonora (Mexico); Garatuza Payan, Jaime [Instituto Tecnologico de Sonora (Mexico); Henk de Bruin [Universidad Agricola de Wageningen (Netherlands); Stewart, John [Universidad de Southampton (United Kingdom)

    1999-12-01

    The data from tow automatic weather stations in the Yaqui valley were used to estimate potential evaporation using the Makkink formula, based on observed incoming solar radiation and climatological values of air temperature. The usefulness of this formula was assessed by comparison with the Penman-Monteith, Penman and Priestley-Taylor formula and measurements of net radiation. A methodology was presented for estimating incoming solar radiation using visible band data from the GOES satellite. Comparisons against ground-based measurements from two pyranometers installed in the Yaqui valley gave good results, particularly in months with low cloud cover. Images for August 1993 were used to produce a map of the spatial distribution of potential evaporation. [Spanish] Para calcular la evaporacion potencial en el valle del Yaqui, usando la formula de Makkink, se utilizaron datos de dos estaciones meteorologicas automaticas. La mencionada formula se basa en la radiacion solar incidente observada y en ciertos valores climatologicos de temperatura del aire. Se evaluo la utilidad de esta formula, comparandola con las de Penman-Monteith, Pennan y Priestley-Taylor, asi como con mediciones de radiacion neta. Se desarrollo una metodologia para estimar la radiacion solar incidente usando la banda visible del satelite GOES. Se hizo una comparacion con mediciones de dos piranometros instalados en el valla del Yaqui, obteniendose buenos resultados, principalmente en meses con poca nubosidad. Se utilizaron imagenes de agosto de 1993 para producir un mapa de la distribucion espacial de la evaporacion potencial.

  7. A multiwavelength study of superoutbursts in dwarf novae

    International Nuclear Information System (INIS)

    Woerd, H.J. van der.

    1987-01-01

    Dwarf novae are stellar systems consisting of two stars which orbit around each other within a few hours. In dwarf novae one of the stars, which is a bit smaller and less massive than our sun, loses matter to a very compact and degenerated star: a white dwarf. This white dwarf has nearly the same mass as our sun but its radius is about a hundred times smaller. The process of mass transport was studied on the basis of observations with the Exosat-satelite (European X-ray Observatory satelite). 397 refs.; 50 figs.; 21 tabs

  8. 76 FR 61956 - Electronic Tariff Filing System (ETFS)

    Science.gov (United States)

    2011-10-06

    ...] Electronic Tariff Filing System (ETFS) AGENCY: Federal Communications Commission. ACTION: Final rule... with the Commission's Electronic Tariff Filing System (ETFS), Report and Order (Order). This notice is...: Pamela Arluk, Pricing Policy Division, Wireline Competition Bureau, at (202) 418-1520, or email: pamela...

  9. Results from PAMELA, ATIC and FERMI: Pulsars or dark matter?

    Indian Academy of Sciences (India)

    Historically, the first evidence for the unseen or dark matter was found in clusters of galaxies. ..... sensitivity to confirm/rule out the DAMA results. ... γ-ray flux sensitivity over previous experiments largely because of its superior rejection.

  10. Université de Genève | Séminaire de physique corpusculaire | 8 May

    CERN Multimedia

    2013-01-01

    The PAMELA mission: more than six years of Cosmic Rays investigation, Dr Francesco Cafagna, Bari University and INFN.   Wednesday 8 May, 11:15 am Science III, Auditoire 1S081 30, quai Ernest-Ansermet, 1211 Genève 4 Abstract: The PAMELA mission major scientific objective is the measurements of Cosmic Rays energy spectra, with special focus on the antiparticles, i.e. antiprotons and positrons, ones. The PAMELA apparatus is a satellite borne magnetic spectrometer and comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, and shower tail catcher scintillator. It has been more than six years that the PAMELA mission is taking data in space, on board of the russian satellite Resurs-DK. Important results have been obtained on the positron and antiproton abundance and spectra. Moreover new results have been obtained on the composition of the charged cosmic radiation that challenge our current und...

  11. Analisis Ketelitian Geometrik Citra Pleiades 1A untuk Pembuatan Peta Dasar Lahan Pertanian (Studi Kasus: Kecamatan Socah, Kabupaten Bangkalan

    Directory of Open Access Journals (Sweden)

    Andreas Kelvin Pujianto

    2017-01-01

    Full Text Available Penggunaan citra satelit resolusi tinggi lebih tepat dan akurat dibanding citra satelit resolusi rendah. Pada saat ini, beberapa satelit dapat menghasilkan citra dengan resolusi spasial kurang dari 1 m. Selain itu, salah satu keuntungan dari data citra satelit resolusi tinggi untuk deteksi dan inventarisasi sumber daya alam adalah setiap lembar (scene citra ini mencakup wilayah yang sangat luas yaitu sekitar 60–180 km2 (360.000–3.240.000 ha [5]. Interpretasi visual pada citra Pleiades 1A dan survei lapangan telah membuktikan bahwa mayoritas daerah Kecamatan Socah memiliki tutupan lahan berupa lahan pertanian yang lebih banyak dibandingkan dengan kecamatan lainnya di Kabupaten Bangkalan. Alasan tersebut menjadikan Kecamatan Socah sebagai lokasi penelitian. Proses rektifikasi citra menggunakan koordinat titik horizontal (X,Y dari Ground Control Point (GCP yang didapatkan dari pengukuran lapangan menggunakan GPS geodetik dengan metode static dengan lama pengukuran 45 menit tiap baseline. Sedangkan untuk uji ketelitian citra menggunakan pengukuran titik Independent Control Point (ICP yang didapatkan dari pengukuran GPS geodetik dengan metode static dengan lama pengukuran 15 menit. Nilai Root Mean Square Error (RMSE titik ICP dari transformasi affine sebesar 0,645 m, sedangkan polynomial orde-2 sebesar 0,533 m. Masing-masing nilai RMSE titik ICP kemudian dikalikan dengan koefisien Circular Error 90% (CE90 dari Perka BIG no. 15 tahun 2014 maka didapatkan nilai ketelitian geometric sebesar 0,979 m pada affine dan 0,809 m pada polynomial orde-2. Hasil ketelitian geometric dari kedua metode transformasi menunjukkan nilai ≤ 1 m, sehingga citra Pleiades 1A memenuhi syarat untuk dijadikan sebagai peta dasar skala 1:5.000 dengan kategori kelas 1.

  12. Search for Antimatter in Space

    CERN Document Server

    2002-01-01

    PAMELA is a cosmic ray space experiment that will be installed on board of the Russian satellite Resurs-DK1 whose launch is scheduled at the end of 2002. The duration of the mission will be at least three years in a high latitude orbit at an altitude ranging between 350 and 600 Km. \\\\ The observational objectives of the PAMELA experiment are the measurement of the spectra of antiprotons, positrons, particles and nuclei in a wide range of energies, the search for antinuclei and the study of the cosmic ray fluxes during a portion of a solar cycle. The main scientific objectives can be schematically summarized as follows: \\\\ \\\\ a) measurement of the antiproton spectrum in the energy range 80 MeV-190 GeV;\\\\ b) measurement of the positron spectrum in the energy range 50 MeV-270 GeV;\\\\ c) search for antinuclei with a sensitivity of the order $10^{-8}$ in the $\\overline{He}/He$ ratio;\\\\ d) measurement of the nuclei spectra (from H to C) in the energy range 100 MeV/n - 200 GeV/n;\\\\ e) energy spectrum of the electroni...

  13. Physics with the KLOE2 experiment at the φ factory

    International Nuclear Information System (INIS)

    Bloise, C.; Gauzzi, P.

    2009-01-01

    We report on the most debated issues which experimentation at the φ factory can really shed light on with a short-term program of measurements. Recent, very promising improvements in the lattice-QCD calculations call for new precision measurements in the Kaon sector to obtain more stringent results on CKM Unitarity and Lepton Flavour Universality. Neutral Kaon Interferometry can probe Discrete Symmetries, but also Quantum Mechanics at the Planck scale. Current limits obtained by KLOE can be overcome by both, the increase in statistics, and the upgrade of the tracking system with an inner GEM chamber for improving vertex resolution near the beam interaction region. One possible solution to the Dark Mass problem, allowing also to interpret the positron excess measured by the satellite Payload experiment PAMELA, suggests a '' dark '' sector that can really be constrained by the experiments at the Kaon and B-Factories. Low energy QCD phenomenology can receive an important contribution from the new measurements of radiative and non-leptonic decays of K, eta and eta' mesons. Finally, important results on the physics in the continuum can be achieved by new measurements of the hadronic cross section and the study of gamma-gamma processes. Improvements on hadronic cross section at low energy are needed to understand the 3-sigma effect on (g-2) μ and for precision determination of alpha em at the TeV scale while the analysis of the gamma-gamma sample impacts scalar spectroscopy and the underlying physics but also the light-by-light hadronic contribution to (g-2) μ . (authors)

  14. Analisa Ketelitian Geometrik Citra Pleiades 1A dan Worldview-2 untuk Pembuatan Peta Dasar Rencana Detail Tata Ruang Perkotaan (Studi Kasus: Surabaya Pusat

    Directory of Open Access Journals (Sweden)

    Ricko Buana Surya

    2017-01-01

    Full Text Available Perkembangan teknologi penginderaan jauh mulai banyak diterapkan untuk berbagai keperluan, misalnya pembuatan peta Rencana Detail Tata Ruang (RDTR dengan skala 1:5000. Saat ini, ada beberapa satelit yang dapat menghasilkan citra resolusi tinggi dengan resolusi spasial kurang dari 1-2 m. Namun data citra yang diperoleh dari satelit-satelit tersebut harus diolah sedemikian rupa untuk meminimalisasi adanya kesalahan, terutama kesalahan geometrik. Data citra Pleiades 1A tahun 2015 dan citra Worldview-2 tahun 2012. Kedua citra tersebut dikoreksi secara geometrik menggunakan dua metode transformasi yaitu affine dan polynomial orde-2. Proses koreksi geometrik dengan menggunakan 8 titik kontrol tanah (GCP tersebar merata pada keseluruhan area studi yaitu Surabaya Pusat. Koordinat GCP diukur langsung di lapangan menggunakan GPS geodetik dengan metode statik dan lama pengamatan untuk setiap titik sekitar 40 menit. Kemudian citra terkoreksi dilakukan uji ketelitian koordinat dengan menggunakan ICP sebanyak 12 titik. Hasil penelitian ini menunjukkan bahwa nilai RMSE menggunakan metode transformasi polynomial orde-2 lebih baik dibandingkan dengan metode affine. Citra Worldview-2 menghasilkan nilai RMSE lebih kecil dibandingkan dengan citra Pleiades 1A pada kedua metode transformasi yang digunakan. Untuk kelayakan citra sebagai peta dasar, citra Pleiades 1A memenuhi syarat peta skala 1:5000 dan citra Worldview-2 memenuhi syarat peta skala 1:5000.

  15. La televisión satelital

    Directory of Open Access Journals (Sweden)

    Francisco Sacristán Romero

    2014-12-01

    Full Text Available En España, la actividad en el sector de las comunicaciones vía satélite tuvo en el 2005 un crecimiento exponencial de servicios y aplicaciones, ligado a las nuevas vías de explotación comercial del sistema de satélites. El punto de inflexión o referencia que marcó este despegue fue la puesta en órbita del primer satélite HISPASAT (1992.

  16. The determination of parameters of shower initiated in imaging calorimeter by electrons and protons

    International Nuclear Information System (INIS)

    Borisov, S.V.; Voronov, S.A.; Karelin, A.V.; Koldobskij, S.A.; Runtso, M.F.

    2010-01-01

    In this work the report on several methods of shower axis reconstruction and methods of search for the starting point of the shower are presented. They were developed for 'thin' sampling imaging calorimeters. For this purpose we used a Monte-Carlo simulation of interaction of electrons and protons with a silicon-tungsten calorimeter of PAMELA satellite-borne experiment. After some adaptation, these methods could be applied for different types of calorimeters

  17. Ideas as Institutions: Explaining the Air Force’s Struggle With Its Aerospace Concept

    Science.gov (United States)

    2006-04-01

    culled from Pamela S. Tolbert and Lynne G. Zucker’s “The Institutionalism of Institutional Theory ” from the Handbook of Organization Studies, ed...The Institutionalization of Institutional Theory ,” in Handbook of Organization Studies, ed. Stewart R. Clyog, Cynthia Hardy, and Walter R. Nord...Pamela S. Tolbert, published an article in The Handbook of Organization Studies (1996), entitled “The Institutionalization of Institutional Theory .” Both

  18. Measurement of antiproton production in $p$He collisions at $\\sqrt{s_{\\scriptscriptstyle\\rm NN}}=110$ GeV

    CERN Document Server

    The LHCb Collaboration

    2017-01-01

    The antiproton production cross-section in collisions of a 6.5 TeV LHC proton beam on helium at rest is measured by the LHCb experiment using the SMOG internal gas target from a dataset corresponding to an integrated luminosity of 0.4 $\\text{nb}^{-1}$. This is the first direct measurement of antimatter production in $p$He collisions, and has important implications for the interpretation of recent results from the PAMELA and AMS-02 experiments, which measure the antiproton component in cosmic rays outside of the Earth's atmosphere.

  19. Cosmic Ray Experiments and the Implications for Indirect Detection of Dark Matter

    Science.gov (United States)

    Mitchell, John W.; Ormes, Jonathan F.; Streitmatter, Robert E.

    2013-01-01

    Detection of cosmic-ray antiprotons was first reported by Golden et al. in 1979 and their existence was firmly established by the BESS and IMAX collaborations in the early 1990s. Increasingly precise measurements of the antiproton spectrum, most recently from BESS-Polar and PAMELA, have made it an important tool for investigating cosmic-ray transport in the galaxy and heliosphere and for constraining dark-matter models. The history of antiproton measurements will be briefly reviewed. The current status will be discussed, focusing on the results of BESS-Polar II and their implications for the possibility of antiprotons from primordial black hole evaporation. The current results of the BESS-Polar II antihelium search are also presented.

  20. Article

    African Journals Online (AJOL)

    Easy trade

    emphasized its importance as basis for 21st century knowledge acquisition. ... projector, radio satelite systems and all services and applications associated with ... quality education is characterized by effective library which is the reason ...

  1. Diseño y desarrollo de un dispositivo electrónico para transmisión de datos con cobertura universal

    Directory of Open Access Journals (Sweden)

    Hernan Paz Penagos

    2015-01-01

    Full Text Available Este artículo presenta el diseño y desarrollo de un dispositivo electrónico con cobertura celular y satelital para la localización y el rastreo de activos móviles en Colombia (transporte público, transporte de carga. El desarrollo de este producto integra hardware, interfaces de comunicaciones y software, y está alineado con una necesidad detectada en el mercado por la empresa One Solution Position: OSP LTDA. Con esta transferencia tecnológica se busca implementar mejoras en la oferta de servicios inalámbricos para seguimiento de activos móviles mediante una solución dual celular/satelital, versátil, económica, de bajo consumo y ceñida a la normatividad internacional FCC y CE Mark.

  2. Deteksi Non-RTH(Ruang Terbuka Hijau Kota Malang Berbasis Citra Google Earth Dengan Menggunakan Naïve Bayes Classifier

    Directory of Open Access Journals (Sweden)

    Irwan Budi Santoso

    2016-01-01

    Full Text Available Banjir, polusi udara dan naiknya temperatur udara di perkotaan, dewasa ini semakin marak persoalan tersebut tidak lain bersumber dari aktifitas manusia yang tidak terkendali sehingga mengakibatkan kerusakan. Salah satu upaya yang bisa dilakukan untuk membantu menyelesaikan persoalan tersebut adalah adanya fasilitas yang dapat memantau kondisi lingkungan secara riil berupa non-Ruang Terbuka Hijau (non-RTH, melalui komputer. Penyediaan fasilitas tersebut sangatlah mungkin dilakukan dengan memanfaatkan foto satelit seperti yang disediakan oleh Google Earth. Studi kasus dalam penelitian ini adalah kota Malang, dengan metode yang digunakan untuk mendeteksi objek non-RTH dipermukaan bumi kota Malang berdasarkan image atau citra satelit adalah Naïve Bayes Classifier (NBC.Hasil uji coba dengan menggunakan sampel pengujian, menunjukkan tingkat akurasi metode tersebut dalam mendeteksi objek non-RTH kota Malang adalah 81%.

  3. Clinical experience in extended cardiac monitoring with the SEEQ™ satellite wireless system

    Directory of Open Access Journals (Sweden)

    Diego Vanegas-Cadavid

    2018-05-01

    Full Text Available Objectives: To present the clinical experience with a new extended (for 15 days, wireless, and satellite cardiac monitoring system in a group of patients with suspicion of cardiac arrhythmia. Method: The study included a cohort of 100 patients seen in the Cardiovascular Electrophysiology Unit of a reference hospital. They were suspected of having a cardiac arrhythmia, with no electrocardiographic diagnosis of the cause, despite previous examinations. They were subjected to SEEQ-type (Medtronic external cardiac monitoring for 15 days, with the outcomes recorded. Results: Of the total of 100 subjects studied, 51% were male, and the median age was 60 years (range: 5 - 91 years. The main symptoms were palpitation, and the most prevalent comorbidity was arterial hypertension (47%. Almost all (98% of them had a previous Holter study, and 46% had two studies, which were inconclusive in explaining the symptoms. The SEEQ monitoring recorded a significant electrocardiographic abnormality in 22% of the patients. A pacemaker implant was the treatment most applied and atrial fibrillation was the most frequent arrhythmia in 50% of the positive findings. There was a higher and significant percentage of positive diagnoses in males. Conclusions: External, satellite, wireless cardiac monitoring extended for 15 days, is a novel tool that can increase the probability of documenting a clinically significant electrocardiographic abnormality in those patients who suffer recurrent cardiovascular symptoms. Resumen: Objetivos: Dar a conocer la experiencia clínica con un nuevo sistema de monitorización cardiaca extendida (por 15 días, inalámbrica y satelital en un grupo de pacientes con sospecha de arritmias cardíacas. Metodología: Cohorte de 100 pacientes atendidos en la unidad de Electrofisiología cardiovascular de un centro de referencia, con sospecha de arritmia cardíaca, sin diagnóstico electrocardiográfico causal, a pesar de exámenes previos. Se les aplic

  4. A state of the art review of vitrification of high level waste in Europe

    International Nuclear Information System (INIS)

    Heimerl, W.

    This paper gives a review of the state-of-the-art of the development and demonstration of vitrification processes for high level radioactive waste solutions on an industrial scale in four European countries (France, United Kingdom, Federal Republic of Germany and Belgium). Historical development, experiences and operations present status and future plans are presented. Three of the processes which seem to be of major importance are described (AVM-France, HARVEST-United Kingdom, PAMELA Germany/Belgium). (author)

  5. Model-independent implications of the e±, p-bar cosmic ray spectra on properties of Dark Matter

    International Nuclear Information System (INIS)

    Cirelli, M.; Kadastik, M.; Raidal, M.; Strumia, A.

    2009-01-01

    Taking into account spins, we classify all two-body non-relativistic Dark Matter annihilation channels to the allowed polarization states of Standard Model particles, computing the energy spectra of the stable final-state particles relevant for indirect DM detection. We study the DM masses, annihilation channels and cross sections that can reproduce the PAMELA indications of an e + excess consistently with the PAMELA p-bar data and the ATIC/PPB-BETS e + +e - data. From the PAMELA data alone, two solutions emerge: (i) either the DM particles that annihilate into W,Z,h must be heavier than about 10 TeV or (ii) the DM must annihilate only into leptons. Thus in both cases a DM particle compatible with the PAMELA excess seems to have quite unexpected properties. The solution (ii) implies a peak in the e + +e - energy spectrum, which, indeed, seems to appear in the ATIC/PPB-BETS data around 700 GeV. If upcoming data from ATIC-4 and GLAST confirm this feature, this would point to a O(1) TeV DM annihilating only into leptons. Otherwise the solution (i) would be favored. We comment on the implications of these results for DM models, direct DM detection and colliders as well as on the possibility of an astrophysical origin of the excess

  6. Argentine Space Assets.

    Science.gov (United States)

    1997-09-01

    Interview, December 1996. Perea, Mauricio, La CFI Invierte En La Empresa Encargada De Las Comunicaciones Por Satelite En Argentina. Corporacion Financiera...1 Attn: Servicio de Comunicaciones Navales 630 Indiana Avenue NW Washington, D.C. 20004-2989 13. A rgentine N

  7. The actual practice of air cleaning in Belgian nuclear facilities

    Energy Technology Data Exchange (ETDEWEB)

    Goossens, W.R. [PEGO, Mol (Belgium)

    1995-02-01

    With 60% of its power generation from nuclear stations Belgium has 7 nuclear power stations in operation with a total capacity of 5.4 MWe. Enriched uranium is imported and converted to fuel assemblies. The actinides of reprocessed fuel are recycled as MOX fuel. A main waste conditioning operation has been performed in the PAMELA vitrifier. The actual practice of nuclear air cleaning in the Belgian PWR station DOEL-4 and in the PAMELA -vitrification plant for high level liquid waste is reviewed.

  8. International Space Station Systems Engineering. Case Study

    Science.gov (United States)

    2010-01-01

    negotiators to move beyond an impasse.108  Don’t be so ready to chase revolutionary designs over evolutionary designs. A key lesson from Russian...112 2002 Oct. 7 2002 Oct. 18 9A S1 truss delivery Jeffrey S. Ashby, Pamela A. Melroy, David A. Wolf, Piers J. Sellers, Sandra H. Magnus , Fyodor...2002 Oct. 18 9A S1 truss delivery Jeffrey S. Ashby, Pamela A. Melroy, David A. Wolf, Piers J. Sellers, Sandra H. Magnus , Fyodor N. Yurchikhin

  9. Guide to Canadian Aerospace Related Industries,

    Science.gov (United States)

    1984-03-01

    manufacturing per- North America If, is tnus PaissiOre !or PT toc Oer a- exle- sonnel depending upon the product aird customer require- sive range af t...the Brazilian government-owned telecommunications Patrol Frigate. company. The project known as Sistema Brasiliero de Telecomunicacoes por Satelite

  10. Soil moisture mapping for aquarius

    Science.gov (United States)

    Aquarius is the first satellite to provide both passive and active L-band observations of the Earth. In addition, the instruments on Satelite de Aplicaciones Cientificas-D (SAC-D) provide complementary information for analysis and retrieval algorithms. Our research focuses on the retrieval of soil m...

  11. Comparison of three filters in the solution of the Navier-Stokes equation in registration

    DEFF Research Database (Denmark)

    Gramkow, Claus; Bro-Nielsen, Morten

    1997-01-01

    he registration of images is an often encountered problem in e.g. medical imagi ng, satelite imaging, or stereo vision. In most applications a rigid deformation model does not suffce and complex deformations must be estimated. In medical registration Bajcsy et al. [1] have proposed the use...

  12. La comunicación en América Latina. Informe de Argentina

    Directory of Open Access Journals (Sweden)

    Federico Rey Lennon

    2015-01-01

    Full Text Available Se presenta el Informe sobre la comunicación en el Argentina. Abarca la información general sobre los medios, la propiedad de éstos, la inversión publicitaria, los computadores, el Internet, la televisión por cable y satelital.

  13. Planetary gear dynamic response to mesh parametric excitation

    Directory of Open Access Journals (Sweden)

    Vojislav Jovan Batinić

    2013-02-01

    Full Text Available Normal 0 MicrosoftInternetExplorer4 Unutrašnje dinamičke sile i pomeranja po predviđenim stepenima slobode u planetarnim prenosnicima posledica su, prvenstveno, promen-ljivih elastičnih deformacija zubaca u sprezi, vibracija delova prenosnika i odstupanja geometrije ozubljenja usled habanja zubaca i grešaka izrade. U radu se razmatra uticaj vremenski promenljive sprežne krutosti na moguća pomeranja i sile u kontaktima zubaca. Ove funkcije su korišćene kao nelinearni koeficijenti krutosti u sistemu jednačina za ekvivalentni zupčani prenosnik pri utvrđivanju prirode pomeranja i unutrašnjih dinamičkih sila. Rezultati numeričke analize sistema jednačina kojima je opisano dinamičko ponašanje su vremenski - promenljive funkcije pomeranja tačaka sistema i dinamičkih sila u spregama zubaca centralni zupčanik/satelit i satelit/venčanik.

  14. CALCULUL CINETOSTATIC AL MECANISMELOR PLANETARE CILINDRICE

    Directory of Open Access Journals (Sweden)

    Păun ANTONESCU

    2012-05-01

    Full Text Available În lucrare se prezintă o metodă analitică pentru calculul cinetostatic al mecanismului planetarmonomobil cu două roţi dinţate centrale. Se consideră mai întâi cazul general al schemelor cinematice cu douăroţi dinţate solidare tip satelit, în două variante practice (multiplicator şi reductor de turaţie. Este menţionatcazul particular al mecanismelor planetare cu o singură roată satelit cu angrenare dublă (exterioară şiinterioară. Pe baza modelului de analiză cinetostatică a mecanismului planetar monomobil cu două roţi dinţatecentrale, în finalul lucrării se abordează o problemă practică de calcul cinetostatic al unui mecanism planetarcilindric simplu folosit la capul de frezat pentru prelucrarea roţilor dinţate cilindrice cu dinţi curbi înhipocicloidă.

  15. Rancang Bangun Modul PAD (Packet Assembler Dissassembler Menggunakan AX.25 pada Sistem Komunikasi ITS-SAT

    Directory of Open Access Journals (Sweden)

    Pasang Arung Padang

    2013-09-01

    Full Text Available ITS-Sat merupakan jenis satelit piko yang saat ini sedang dikembangkan di Institut Teknologi Sepuluh Nopember. ITS-Sat membutuhkan suatu protokol komunikasi yang mengatur tata cara komunikasi satelit. Protokol AX.25 merupakan protokol komunikasi yang digunakan dalam sistem komunikasi ITS-Sat. Protokol ini berada pada layer data link dalam model OSI Layer. Protokol ini dapat membangun dan memutuskan link serta melakukan pengiriman data. Protokol AX.25 menggabungkan data-data field menjadi suatu frame. Makalah ini mengimplementasikan protokol AX.25 ke dalam modul PAD (Packet Assembler Dissassembler. Protokol AX.25 diimplementasikan ke dalam mikrokontroler yang merupakan otak dari modul PAD dengan menggunakan bahasa pemograman. Modul PAD berfungsi untuk mengkapsulasi data tiap field menjadi sebuah frame AX.25 sebelum dikirim dan kemudian frame AX.25 yang diterima dienkapsulasi kembali menjadi data field. Modul PAD yang dibuat dapat mengirim dan menerima data teks sebanyak 500 karakter. Hasil pengujian menunjukan bahwa modul PAD yang dibuat mampu melakukan komunikasi antar modul PAD dengan baik.

  16. Estimación de pequeñas perturbaciones en satélites geocéntricos como un problema inverso

    Science.gov (United States)

    Zadunaisky, P. E.

    El movimiento geocéntrico de un satélite artificial es simulado automáticamente por un sistema de ecuaciones diferenciales de segundo orden que incluyen dos funciones perturbadoras. La primera representa el segundo término del potencial gravitatorio de la Tierra y la segunda corresponde al frenado atmosférico. Asumiendo como conocidas, por hipótesis o por mediciones, la posición y velocidad del satélite en instantes sucesivos se estiman las perturbaciones a intervalos sucesivos por un método determinístico. Para ilustrar el método y comprobar la precisión de nuestros resultados hemos simulado dos ejemplos incluyendo valores conocidos de las perturbaciones que luego comparamos con los resultados de nuestro método. El método puede aplicarse por ejemplo para el intervalo de una revolución satelital lo cual permitiría el diseño inmediato de una maniobra correctiva de la órbita satelital.

  17. Constraining decaying dark matter with FERMI-LAT gamma rays

    International Nuclear Information System (INIS)

    Maccione, L.

    2011-01-01

    High energy electron sand positrons from decaying dark matter can produce a significant flux of gamma rays by inverse Compton of low energy photons in the interstellar radiation field. This possibility is inevitably related with the dark matter interpretation of the observed PAMELA and FERMI excesses. We will describe a simple and universal method to constrain dark matter models which produce electrons and positrons in their decay by using the FERMI-LAT gamma-ray observations in the energy range between 0.5 GeV and 300 GeV, by exploiting universal response functions that, once convolved with a specific dark matter model, produce the desired constraint. The response functions contain all the astrophysical inputs. Here is discussed the uncertainties in the determination of the response functions and apply them to place constraints on some specific dark matter decay models that can well fit the positron and electron fluxes observed by PAMELA and FERMI LAT, also taking into account prompt radiation from the dark matter decay. With the available data decaying dark matter can not be excluded as source of the PAMELA positron excess.

  18. New Results from Fermi-LAT and Their Implications for the Nature of Dark Matter and the Origin of Cosmic Rays

    Science.gov (United States)

    Moiseev, Alexander

    2009-01-01

    The measured spectrum is compatible with a power law within our current systematic errors. The spectral index (-3.04) is harder than expected from previous experiments and simple theoretical considerations. "Pre-Fermi" diffusive model requires a harder electron injection spectrum (by 0.12) to fit the Fermi data, but inconsistent with positron excess reported by Pamela if it extends to higher energy. Additional component of electron flux from local source(s) may solve the problem; its origin, astrophysical or exotic, is still unclear. Valuable contribution to the calculation of IC component of diffuse gamma radiation.

  19. Dark matter, a hidden universe

    International Nuclear Information System (INIS)

    Trodden, M.; Feng, J.

    2011-01-01

    The main candidates to dark matter are particles called WIMPs for weakly interacting massive particles. 4 experiments (CDMS in Minnesota (Usa), DAMA at Gran Sasso (Italy), CoGeNT in Minnesota (Usa) and PAMELA onboard a Russian satellite) have claimed to have detected them. New clues suggest that it could exist new particles interacting via new forces. The observation that dwarf galaxies are systematically more spherical than massive galaxies might be a sign of the existence of new forces between dark matter components. Dark matter could not be as inert as previously thought. (A.C.)

  20. Infrared studies of asymptotic giant branch stars

    International Nuclear Information System (INIS)

    Willems, F.J.

    1987-01-01

    In this thesis studies are presented of asymptotic giant branch stars, which are thought to be an important link in the evolution of the galaxy. The studies were performed on the basis of data collected by the IRAS, the infrared astronomical satelite. 233 refs.; 33 figs.; 16 tabs

  1. Anoxic and oxic phototrophic primary production during the Precambrian

    DEFF Research Database (Denmark)

    Ebey-Honeycutt, Christina Marie; Bjerrum, Christian J.; Canfield, Donald Eugene

    2009-01-01

    of the mixed layer often lies above the base of the photic zone . Thus, an ecosystem model for the Precambrian should reflect the net primary production (NPP) of oxygenic phototrophs in the mixed layer and anoxygenic phototrophs below (NPPox and NPPred, respectively). Satelite data and a vertically generalized...

  2. Perancangan Dan Realisasi Sistem Transmisi Data GPS Menggunakan Teknologi SMS (Short Messaging Service Sebagai Aplikasi Sistem Personal Tracking

    Directory of Open Access Journals (Sweden)

    DECY NATALIANA

    2017-06-01

    Full Text Available Abstrak Berprinsip pada pengembangan teknologi dan aplikasi dari sistem penjejakan posisi (tracking, maka dibuatlah sistem personal tracking dengan mentransmisikan data GPS (Global Positioning System dengan menggunakan teknologi SMS (Short Messaging Service pada jaringan GSM (Global System for Mobile Communications sebagai media transmisinya.  Dengan sistem GPS akan diperoleh data garis lintang, serta garis bujur dari GPS receiver.  Data tersebut akan diteruskan oleh mikrokontroler untuk dikirim ke ponsel pengamat melalui komunikasi SMS.  Hasil pengujian menunjukkan bahwa device personal tracking berhasil mengirimkan data berupa IMEI, Tanggal satelit, waktu satelit, koordinat longitude, koordinat latitude, dan jumlah satelit yang berhasil ditangkap oleh device ke ponsel pengamat.  Dari data koordinat tersebut pengamat dapat memantau posisi device personal tracking berada dengan bantuan aplikasi pendukung yaitu Google Maps. Kata kunci: GPS, Personal Tracking, SMS, Google Maps.   Abstract Base on technology and application development of tracking, personal tracking system was made by transmiting GPS (Global Positioning System data using SMS (Short Messaging Service technology with GSM (Global System for Mobile Communications network as transmitter media.  BY GPS system, we can get datas such as latitude and longitude of GPS receiver.  Those datas will be processed by microcontroller to be sent from GSM/GPRS module to user cellular phone through SMS communication.  The test result showed that the device can be sending datas such as IMEI, UTC date, UTC time, longitude coordinate, latitude coordinate, and number sattelite which detected by device to user’s phonecell.  From those coordinate, user can be monitoring the device’s position with the Google Maps application. Keywords: GPS, Personal Tracking, SMS, Google Maps.

  3. Albedo and color maps of the Saturnian satellites

    International Nuclear Information System (INIS)

    Buratti, B.J.; Mosher, J.A.; Johnson, T.V.

    1990-01-01

    The paper discusses the production of maps of the albedos and colors of Mimas, Enceladus, Tethys, Dione, and Rhea over the full range of their imaged surfaces. Voyager images were used to prepare maps of the normal reflectances and color ratios (0.58/0.41 micron) of these satelites. 67 refs

  4. Ilmub raamat viikingiajast Saaremaal / Pamela Talzi

    Index Scriptorium Estoniae

    Talzi, Pamela

    2017-01-01

    Saaremaal viikingiaega uurinud arheoloogi, Tallinna ülikooli humanitaarteaduste instituudi ajaloo, arheoloogia ja kunstiajaloo keskuse vanemteaduri Marika Mägi sulest ilmub raamat "Viikingiaegne Eesti"

  5. Solar Energetic Particle Spectra

    Science.gov (United States)

    Ryan, J. M.; Boezio, M.; Bravar, U.; Bruno, A.; Christian, E. R.; de Nolfo, G. A.; Martucci, M.; Mergè, M.; Munini, R.; Ricci, M.; Sparvoli, R.; Stochaj, S.

    2017-12-01

    We report updated event-integrated spectra from several SEP events measured with PAMELA. The measurements were made from 2006 to 2014 in the energy range starting at 80 MeV and extending well above the neutron monitor threshold. The PAMELA instrument is in a high inclination, low Earth orbit and has access to SEPs when at high latitudes. Spectra have been assembled from these high-latitude measurements. The field of view of PAMELA is small and during the high-latitude passes it scans a wide range of asymptotic directions as the spacecraft orbits. Correcting for data gaps, solid angle effects and improved background corrections, we have compiled event-integrated intensity spectra for twenty-eight SEP events. Where statistics permit, the spectra exhibit power law shapes in energy with a high-energy exponential roll over. The events analyzed include two genuine ground level enhancements (GLE). In those cases the roll-over energy lies above the neutron monitor threshold ( 1 GV) while the others are lower. We see no qualitative difference between the spectra of GLE vs. non-GLE events, i.e., all roll over in an exponential fashion with rapidly decreasing intensity at high energies.

  6. Characterization of HLW glass samples Task 3 Characterization of radioactive waste forms a series of final reports (1985-89) No 20

    International Nuclear Information System (INIS)

    Malow, G.; Behrend, U.; Schubert, P.

    1991-01-01

    Due to a delay in the melting of the highly radioactive SON68 glass, a short-term post-investigation of the highly radioactive glass from the Pamela plant in Mol (Belgium) has been carried out, the aim being a check-up of the active LEWC glass SM 513 LW11. The results were compared with those obtained for non-radioactive glass samples. The final report of the present CEC programme shortly describes the planned investigations of the glass R7T7 for the whole period of the research contract and the results of the short-term post-investigation of the Pamela glass. 11 refs.; 9 figs.; 4 tabs

  7. Activity report 1981

    International Nuclear Information System (INIS)

    Delande, E.; Drent, W.

    1982-07-01

    This report reviews the main activities of the Eurochemic company for the fiscal year 1981. These activities are: the plant operation including the safeguards for special nuclear materials, the management of radioactive wastes and the analytical services, new works such as vitrification project, Pamela building and the design for the storage of vitrified wastes. The industrial development concerns the Eurowatt process for solvent treatment, the wet combustion for plutonium bearing solid wastes, the separation of mercury, the incorporation of solid wastes into a polymer concrete matrix and the Pamela process. The health and safety division, the library and documentation service and the administrative matters are also presented. (AF)

  8. Vliv hospodaření na vegetaci a toky energie, vody a látek v malých povodí na Šumavě

    Czech Academy of Sciences Publication Activity Database

    Procházka, J.; Hakrová, P.; Pokorný, Jan; Pecharová, E.; Hezina, T.; Wotavová, K.; Šíma, M.; Pechar, Libor

    2001-01-01

    Roč. 6, - (2001), s. 199-224 ISSN 1211-7420 R&D Projects: GA AV ČR KSK6005114; GA MŠk VS96072; GA MŠk OC 844.20 Institutional research plan: CEZ:AV0Z6005908 Keywords : landscape efficiency * management * matter losses * satelite images * solar energy dissipation Subject RIV: EH - Ecology, Behaviour

  9. Indirect detection of dark matter

    International Nuclear Information System (INIS)

    Pieri, L.

    2008-01-01

    In the Cold Dark Matter scenario, the Dark Matter particle candidate may be a Weakly Interacting Massive Particle (Wimp). Annihilation of two Wimps in local or cosmological structures would result in the production of a number of standard model particles such as photons, leptons and baryons which could be observed with the presently available or future experiments such as the Pamela or Glast satellites or the Cherenkov Telescopes. In this work we review the status-of-the-art of the theoretical and phenomenological studies about the possibility of indirect detection of signals coming from Wimp annihilation.

  10. Asteroids mass determination

    International Nuclear Information System (INIS)

    Hoffmann, M.

    1989-01-01

    Basic methods for asteroid mass determinations and their errors are discussed. New results and some current developments in the astrometric method are reviewed. New methods and techniques, such as electronic imaging, radar ranging and space probes are becoming important for asteroid mass determinations. Mass and density estimations on rotational properties and possible satelites are also discussed

  11. Porcine cumulus and mural granulosa cells secrete cumulus expansion enabling factor (CEEF)

    Czech Academy of Sciences Publication Activity Database

    Procházka, Radek; Nagyová, Eva; Motlík, Jan

    1996-01-01

    Roč. 39, special issue (1996), s. 86 ISSN 0003-9438. [Satelite Symposium of the Central European Conference on Animal Reproduction /1./. Kühlungsborn, 22.09.1996-23.09.1996] R&D Projects: GA ČR GA505/93/2010; GA AV ČR IAA745401 Grant - others:GZ 45379/1-IV/3a/94 Source of funding: AT

  12. Fixed target measurements at LHCb for cosmic rays physics

    CERN Document Server

    AUTHOR|(CDS)2069608

    2018-01-01

    The LHCb experiment has the unique possibility, among the LHC experiments, to be operated in fixed target mode, using its internal gas target. The energy scale achievable at the LHC, combined with the LHCb forward geometry and detector capabilities, allow to explore particle production in a wide Bjorken-$x$ range at the $\\sqrt {s_{NN}} ~$ ~ 100 GeV energy scale, providing novel inputs to nuclear and cosmic ray physics. The first measurement of antiproton production in collisions of LHC protons on helium nuclei at rest is presented. The knowledge of this cross-section is of great importance for the study of the cosmic antiproton flux, and the LHCb results are expected to improve the interpretation of the recent high-precision measurements of cosmic antiprotons performed by the space-borne PAMELA and AMS-02 experiments.

  13. Investigations concerning the source term for the emission of fission products and transuranic elements from the highly radioactive waste in the temperature region between 200 and 11000C

    International Nuclear Information System (INIS)

    Baumgartner, F.; Krebs, K.; Merte, B.

    1984-04-01

    Starting point of these investigations was the research report 290 of the former Institute for Reactor Safety, Cologne. The largely incorrect assumptions made in the chemical statement led to high radioactive doses not only for the closer, but also for the further surroundings of a reprocessing plant in case that the cooling system of the fuel element storage or the storage tank for the highly radioactive waste (HAW) should become inoperative for an extended period of time. However, as a result of this temperature region which we used in our experiments, the investigations concerning the source term of the HAW between 1100 and 1200 0 C became interesting again, because a glass melt of about 1100 0 C is used during the PAMELA-process for the vitrification of the HAW. The aqueous HAW-solution is thereby poured onto a hot glass melt. The solution thereby dries up, the HAW-salt is calcined and finally sinks into the glass melt. From today's point of view an investigation concerning the source term of the fission products and transuranic elements from the HAW at 1100 0 C therefore provides information regarding the fission product- and transuranic element volatilization within the melting furnace during the vitrification process. The results may now therefore also be considered a contribution for the layout of the off-gas purification system during the PAMELA-process

  14. VizieR Online Data Catalog: Local interstellar spectra of cosmic-ray species (Boschini+, 2017)

    Science.gov (United States)

    Boschini, M. J.; Torre, S. D.; Gervasi, M.; Grandi, D.; Johannesson, G.; Kachelriess, M.; La Vacca, G.; Masi, N.; Moskalenko, I. V.; Orlando, E.; Ostapchenko, S. S.; Pensotti, S.; Porter, T. A.; Quadrani, L.; Rancoita, P. G.; Rozza, D.; Tacconi, M.

    2017-11-01

    Local interstellar spectra (LIS) for protons, helium, and antiprotons are built using the most recent experimental results combined with state-of-the-art models for propagation in the Galaxy and heliosphere. Two propagation packages, GALPROP and HelMod, are combined to provide a single framework that is run to reproduce direct measurements of cosmic-ray (CR) species at different modulation levels and at both polarities of the solar magnetic field. To do so in a self-consistent way, an iterative procedure was developed, where the GALPROP LIS output is fed into HelMod, providing modulated spectra for specific time periods of selected experiments to compare with the data; the HelMod parameter optimization is performed at this stage and looped back to adjust the LIS using the new GALPROP run. The parameters were tuned with the maximum likelihood procedure using an extensive data set of proton spectra from 1997 to 2015. The proposed LIS accommodate both the low-energy interstellar CR spectra measured by Voyager 1 and the high-energy observations by BESS, Pamela, AMS-01, and AMS-02 made from the balloons and near-Earth payloads; it also accounts for Ulysses counting rate features measured out of the ecliptic plane. The found solution is in a good agreement with proton, helium, and antiproton data by AMS-02, BESS, and PAMELA in the whole energy range. (3 data files).

  15. Solution of Heliospheric Propagation: Unveiling the Local Interstellar Spectra of Cosmic-ray Species

    Energy Technology Data Exchange (ETDEWEB)

    Boschini, M. J.; Torre, S. Della; Gervasi, M.; Grandi, D.; Vacca, G. La; Pensotti, S.; Rancoita, P. G.; Rozza, D.; Tacconi, M. [INFN, Milano-Bicocca, Milano (Italy); Jóhannesson, G. [Science Institute, University of Iceland, Dunhaga 3, IS-107 Reykjavik (Iceland); Kachelriess, M. [Institutt for fysikk, NTNU, NO-7491 Trondheim (Norway); Masi, N.; Quadrani, L. [INFN, Bologna (Italy); Moskalenko, I. V.; Orlando, E.; Porter, T. A. [Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305 (United States); Ostapchenko, S. S. [Frankfurt Institute of Advanced Studies, Frankfurt (Germany)

    2017-05-10

    Local interstellar spectra (LIS) for protons, helium, and antiprotons are built using the most recent experimental results combined with state-of-the-art models for propagation in the Galaxy and heliosphere. Two propagation packages, GALPROP and HelMod, are combined to provide a single framework that is run to reproduce direct measurements of cosmic-ray (CR) species at different modulation levels and at both polarities of the solar magnetic field. To do so in a self-consistent way, an iterative procedure was developed, where the GALPROP LIS output is fed into HelMod, providing modulated spectra for specific time periods of selected experiments to compare with the data; the HelMod parameter optimization is performed at this stage and looped back to adjust the LIS using the new GALPROP run. The parameters were tuned with the maximum likelihood procedure using an extensive data set of proton spectra from 1997 to 2015. The proposed LIS accommodate both the low-energy interstellar CR spectra measured by Voyager 1 and the high-energy observations by BESS, Pamela, AMS-01, and AMS-02 made from the balloons and near-Earth payloads; it also accounts for Ulysses counting rate features measured out of the ecliptic plane. The found solution is in a good agreement with proton, helium, and antiproton data by AMS-02, BESS, and PAMELA in the whole energy range.

  16. 3rd IAGA/ICMA Workshop on Vertical Coupling in the Atmosphere/Ionosphere System/ Abstract

    Science.gov (United States)

    2007-01-10

    are retrieved from radio occultations made by CHAMP (Challenging Minisatellite Payload) and SAC-C (Satelite de Aplicaciones Cientificas-C) and...commercially available software package, to produce a realistic model of atmospheric electrical phenomena using various current generators...formal description of various spatial grids. Such data storage system organization allows using the same software for data access and data processing and

  17. Sección Portuguesa

    Directory of Open Access Journals (Sweden)

    Revista Chasqui

    2015-01-01

    Full Text Available Editorial Dr. Luis Eladio Proaño; Chasqui entrevistou o Dr. Fausto Izcaray; A Revolução da microelectrônica: consequências para o terceiro mundo;  a educação na sociedade informatizada Héctor Schmucler; Satelites de comunicação: uma perspectiva terceiro-mundista Neville Jayaweera; Controversia entre Sola Pool e Schiller

  18. La radio digital

    Directory of Open Access Journals (Sweden)

    Carlos Eduardo Cortés S.

    2015-01-01

    Full Text Available La radio digital es un producto de la llamada convergencia digital. Las nuevas tecnologías interconectadas permiten la aparición de nuevos modos de audiencia y la implementación de herramientas versátiles. Habla del problema de los estándares, de la radio satelital, la radio digital terrestre, las radios internacionales, la interactividad.

  19. Antenna System for Nano-satelite Mission GOMX-3

    DEFF Research Database (Denmark)

    Tatomirescu, Alexandru; Pedersen, Gert F.; Christiansen, J.

    2016-01-01

    In this paper, we present the antenna design for a nano-satellite mission launched in September, the GOMX-3 mission. Some of the key design challenges are discussed and the chosen solutions are presented. In an effort to minimize development and manufacturing costs for future missions, this study...

  20. Decaying dark matter from dark instantons

    International Nuclear Information System (INIS)

    Carone, Christopher D.; Erlich, Joshua; Primulando, Reinard

    2010-01-01

    We construct an explicit, TeV-scale model of decaying dark matter in which the approximate stability of the dark matter candidate is a consequence of a global symmetry that is broken only by instanton-induced operators generated by a non-Abelian dark gauge group. The dominant dark matter decay channels are to standard model leptons. Annihilation of the dark matter to standard model states occurs primarily through the Higgs portal. We show that the mass and lifetime of the dark matter candidate in this model can be chosen to be consistent with the values favored by fits to data from the PAMELA and Fermi-LAT experiments.

  1. Neutrino signals from dark matter decay

    International Nuclear Information System (INIS)

    Covi, Laura; Grefe, Michael; Ibarra, Alejandro; Tran, David

    2009-12-01

    We investigate different neutrino signals from the decay of dark matter particles to determine the prospects for their detection, and more specifically if any spectral signature can be disentangled from the background in present and future neutrino observatories. If detected, such a signal could bring an independent confirmation of the dark matter interpretation of the dramatic rise in the positron fraction above 10 GeV recently observed by the PAMELA satellite experiment and offer the possibility of distinguishing between astrophysical sources and dark matter decay or annihilation. In combination with other signals, it may also be possible to distinguish among different dark matter decay channels. (orig.)

  2. Neutrino signals from dark matter decay

    Energy Technology Data Exchange (ETDEWEB)

    Covi, Laura; Grefe, Michael [Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany); Ibarra, Alejandro; Tran, David [Technische Univ. Muenchen, Garching (Germany). Physik-Department T30d

    2009-12-15

    We investigate different neutrino signals from the decay of dark matter particles to determine the prospects for their detection, and more specifically if any spectral signature can be disentangled from the background in present and future neutrino observatories. If detected, such a signal could bring an independent confirmation of the dark matter interpretation of the dramatic rise in the positron fraction above 10 GeV recently observed by the PAMELA satellite experiment and offer the possibility of distinguishing between astrophysical sources and dark matter decay or annihilation. In combination with other signals, it may also be possible to distinguish among different dark matter decay channels. (orig.)

  3. KSC-04PD-2218

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Gary Grigg, a survivor of the World Trade Center attack on Sept. 11, 2001, relates his experience as part of KSCs Spaceport Super Safety and Health Day. The event included other guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  4. KSC-04PD-2217

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Gary Grigg, a survivor of the World Trade Center attack on Sept. 11, 2001, relates his experience as part of KSCs Spaceport Super Safety and Health Day. The event included other guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  5. Tight connection between direct and indirect detection of dark matter through Higgs portal couplings to a hidden sector

    International Nuclear Information System (INIS)

    Arina, Chiara; Josse-Michaux, Francois-Xavier; Sahu, Narendra

    2010-01-01

    We present a hidden Abelian extension of the standard model including a complex scalar as a dark matter candidate and a light scalar acting as a long range force carrier between dark matter particles. The Sommerfeld enhanced annihilation cross section of the dark matter explains the observed cosmic ray excesses. The light scalar field also gives rise to potentially large cross sections of dark matter on the nucleon, therefore providing an interesting way to probe this model simultaneously at direct and indirect dark matter search experiments. We constrain the parameter space of the model by taking into account the CDMS-II exclusion limit as well as PAMELA and Fermi LAT data.

  6. Natural SUSY dark matter model

    International Nuclear Information System (INIS)

    Mohanty, Subhendra; Rao, Soumya; Roy, D.P.

    2013-01-01

    The most natural region of cosmologically compatible dark matter relic density in terms of low fine-tuning in a minimal supersymmetric standard model with nonuniversal gaugino masses is the so called bulk annihilation region. We study this region in a simple and predictive SUSY- GUT model of nonuniversal gaugino masses, where the latter transform as a combination of singlet plus a nonsinglet representation of the GUTgroup SU(5). The model prediction for the direct dark matter detection rates is well below the present CDMS and XENON100 limits, but within the reach of a future 1Ton XENON experiment. The most interesting and robust model prediction is an indirect detection signal of hard positron events, which resembles closely the shape of the observed positron spectrum from the PAMELA experiment. (author)

  7. South African Medical Journal - Vol 107, No 1 (2017)

    African Journals Online (AJOL)

    Editorial · EMAIL FREE FULL TEXT EMAIL FREE FULL TEXT DOWNLOAD FULL TEXT DOWNLOAD FULL TEXT. Jacqui Webster, Christelle Crickmore, Karen Charlton, Krisela Steyn, Edelweiss Wentzel-Viljoen, Pamela Naidoo, 20-21 ...

  8. Development of techniques using DNA analysis method for detection/analysis of radiation-induced mutation. Development of an useful probe/primer and improvement of detection efficacy

    International Nuclear Information System (INIS)

    Maekawa, Hideaki; Tsuchida, Kozo; Hashido, Kazuo; Takada, Naoko; Kameoka, Yosuke; Hirata, Makoto

    1999-01-01

    Previously, it was demonstrated that detection of centromere became easy and reliable through fluorescent staining by FISH method using a probe of the sequence preserved in α-satelite DNA. Since it was, however, found inappropriate to detect dicentrics based on the relative amount of DNA probe on each chromosome. A prove which allows homogeneous detection of α-satelite DNA for each chromosome was constructed. A presumed sequence specific to kinetochore, CENP-B box was amplified by PCR method and the product DNA was used as a probe. However, the variation in amounts of probe DNA among chromosomes was decreased by only about 20%. Then, a program for image processing of the results obtained from FISH using α-satelite DNA was constructed to use as a marker for centromere. When compared with detection of abnormal chromosomes stained by the conventional method, calculation efficacy for only detection of centromere was improved by the use of this program. Calculation to discriminate the normal or not was still complicated and the detection efficacy was little improved. Chromosomal abnormalities in lymphocytes were used to detect the effects of radiation. In this method, it is needed to shift the phase of cells into metaphase. The mutation induced by radiation might be often repaired during shifting. To exclude this possibility, DNA extraction was conducted at a low temperature and immediately after exposure to 137 Cs, and a rapid genome detection method was established using the genome DNA. As the model genomes, the following three were used: 1) long chain repeated sequences widely dispersed over chromosome, 2) cluster genes, 3) single copy genes. The effects of radiation were detectable at 1-2 Gy for the long repeated sequences and at 7 Gy for the cluster genes, respectively, whereas no significant effects were observed at any Gy tested for the single copy genes. Amplification was marked in the cells exposed at 1-10 Gy (peak at 4 Gy), suggesting that these regions had

  9. Constraining decaying dark matter with Fermi LAT gamma-rays

    International Nuclear Information System (INIS)

    Zhang, Le; Sigl, Günter; Weniger, Christoph; Maccione, Luca; Redondo, Javier

    2010-01-01

    High energy electrons and positrons from decaying dark matter can produce a significant flux of gamma rays by inverse Compton off low energy photons in the interstellar radiation field. This possibility is inevitably related with the dark matter interpretation of the observed PAMELA and FERMI excesses. The aim of this paper is providing a simple and universal method to constrain dark matter models which produce electrons and positrons in their decay by using the Fermi LAT gamma-ray observations in the energy range between 0.5 GeV and 300 GeV. We provide a set of universal response functions that, once convolved with a specific dark matter model produce the desired constraints. Our response functions contain all the astrophysical inputs such as the electron propagation in the galaxy, the dark matter profile, the gamma-ray fluxes of known origin, and the Fermi LAT data. We study the uncertainties in the determination of the response functions and apply them to place constraints on some specific dark matter decay models that can well fit the positron and electron fluxes observed by PAMELA and Fermi LAT. To this end we also take into account prompt radiation from the dark matter decay. We find that with the available data decaying dark matter cannot be excluded as source of the PAMELA positron excess

  10. Review of The Rise of the Expert Company

    OpenAIRE

    Chalmers, Robert A.

    1989-01-01

    The authors of this book, Edward A. Feigenbaum, Pamela McCorduck, and H. Penny Nii, have given us an absorbing collection of tales about the successful integration of expert systems into mainstream industry.

  11. Download this PDF file

    African Journals Online (AJOL)

    sulaiman.adebowale

    2008-03-04

    Mar 4, 2008 ... who admittedly 'knew little about the music business' when they first .... Numerous stories abound with regard to textbook cases where African ...... Andanda, Pamela, 2004, 'A Golden Chance for Medical Ethics in Kenya',.

  12. 75 FR 68375 - Performance Review Board Appointments

    Science.gov (United States)

    2010-11-05

    ... C. Hildebrandt, Betsy J. Iudicello, Fay S. Jackson, J. Andrew Jacobson, Rachel L. Keable, Edward T..., Donald E. Jr. Malam, Pamela R. Mazer, Bernard J. Moss, Adrianne L. More, Robert S. Nedd, Michael D. O...

  13. Love, lust and the emotional context of multiple and concurrent ...

    African Journals Online (AJOL)

    Love, lust and the emotional context of multiple and concurrent sexual partnerships among young Swazi adults. Allison Ruark, Lunga Dlamini, Nonhlanhla Mazibuko, Edward C Green, Caitlin Kennedy, Amy Nunn, Timothy Flanigan, Pamela J Surkan ...

  14. Peace education: why and how?

    Directory of Open Access Journals (Sweden)

    Pamela Baxter

    2005-01-01

    Full Text Available Pamela Baxter discusses why peace education programmes are so important and Vick Ikobwa presents the methodology and lessons learned from the UNHCR/INEE Peace Education Programme in East Africa and the Horn.

  15. Journal of Language, Technology & Entrepreneurship in Africa - Vol ...

    African Journals Online (AJOL)

    Analysis of Women Small Scale Entrepreneurs Practices during Business Negotiations in Tanzania Agribusiness · EMAIL FREE FULL TEXT EMAIL FREE FULL TEXT DOWNLOAD FULL TEXT DOWNLOAD FULL TEXT. Felix Adamu Nandonde, Pamela John Liana, 28-45 ...

  16. ANALISA PERUBAHAN IONOSFER AKIBAT GEMPA MENTAWAI TAHUN 2010 (Studi Kasus : Kepulauan Mentawai, Sumatra Barat

    Directory of Open Access Journals (Sweden)

    Leni Septiningrum

    2017-01-01

    Full Text Available Gempa merupakan fenomena alam akibat aktifitas tektonik yang sering terjadi di Indonesia. Sepanjang pulau Sumatra merupakan pertumbukan antara lempeng Indo-Australia dan lempeng Eurasia menjadikan Sumatra sebagai daerah paling aktif dengan aktifitas tektoniknya. Pada tahun 2010 tercatat tiga gempa besar yang terjadi, yaitu gempa berkekuatan 6,8 SR pada 5 Maret, disusul 6,5 SR pada 5 Mei dan terakhir 7,8 SR pada 25 Oktober 2010. Post-earthquake anomali merupakan fluktuasi TEC yang terjadi sesaat setelah terjadinya gempa, fenomena ini terjadi 3 menit hingga 1 jam setelah gempa terjadi. Post-earthquake anomali dapat digunakan sebagai early warning sebelum tsunami datang. Pengamatan TEC (Total Electron Content dilakukan dengan menggunakan GPS. Satelit GPS akan secara kontinyu memancarkan sinyal gelombang double frequency pada L band. Pada saat terjadi gempa, sinyal yang dipancarkan oleh satelit GPS akan mengalami delay ketika melewati lapisan ionosfer kira-kira 300 km dari permukaan bumi. Variasi ionosfer diamati pada saat terjadi time-delay ini, sehingga didapat nilai TEC dimana I TECU sama dengan 1016 elektron/m2. Nilai tersebut yang akan menggambarkan besaran gangguan akibat adanya gempa. Pada gempa Mentawai 2010 dengan menggunakan stasiun pengamat GPS pada ketiga kejadian gempa tidak menunjukkan adanya gangguan pada ionosfer, hanya terjadi fluktuasi pada beberapa stasiun pengamat.

  17. Analisa Ketelitian Orthorektifikasi Citra Pleiades untuk Pembuatan Peta Rencana Detail Tata Ruang Terbuka Hijau (Studi Kasus: Kota Surabaya

    Directory of Open Access Journals (Sweden)

    Meika Sumarsono

    2017-01-01

    Full Text Available Surabaya merupakan salah satu kota besar yang mempunyai banyak penduduk sehingga perlu adanya pengembangan RTH yang cukup dalam suatu wilayah agar kondisi lingkungan tetap nyaman salah satunya dengan pembuatan peta RDTR RTH menggunakan citra satelit resolusi tinggi. Namun citra satelit resolusi tinggi perlu dikoreksi secara geometrik dengan orthorektifikasi untuk memposisikan kembali citra sesuai lokasi sebenarnya karena pada saat peliputan data terjadi pergeseran posisi. Penelitian ini mengkaji ketelitian orthorektifikasi citra Pleiades 1A dengan menggunakan metode RPC sebagai peta dasar untuk rekomendasi dalam pembuatan peta RDTR RTH di wilayah Surabaya bagian pusat. Data yang digunakan dalam penelitian ini yaitu citra Pleiades 1A dengan resolusi spasial 0,5 m pankromatik dan 2 m multispektral, DEM ALOS PALSAR dengan ketelitian 12,5 m, Ground Control Point (GCP hasil dari pengukuran di lapangan. Ketelitian geometrik menggunakan metode RPC di mana metode ini menggunakan informasi parameter orientasi dalam yang terdapat di metadata serta dibantu dengan titik kontrol tanah dan DEM. Hasil proses orthorektifikasi dengan menggunakan 8 titik GCP berupa RMSE sebesar 0,36 piksel dan 0,18 m yang memenuhi syarat untuk pembuatan peta dasar skala 1:5000. Hasil orthorektifikasi ini diuji dengan cara tumpang tindih (overlay terhadap peta skala 1:25.000.

  18. The Semi-Submersible Network

    Science.gov (United States)

    2012-12-01

    Hallan Sumergible de las FARC con sistemas por satélite e informáticos,” Semana, September 26, 2011, http://www.semana.com/nacion/hallan-sumergible-farc... sistemas -satelite-informaticos/164832- 3.aspx. 20 Rear Admiral Charles Michel, “Hearing on Border Security Threats to the Homeland: DHS’s Response to... web page on the FARC that provides a detailed description of the terror group’s history, sub-organizations, and their operational locations. In

  19. Densidad de desarrollo alta y baja en Puerto Rico

    Science.gov (United States)

    William A. Gould; Sebastian Martinuzzi; Olga M. Ramos Gonzalez

    2008-01-01

    Este mapa demuestra la distribución de terrenos de alta y baja densidad de desarrollo urbano en Puerto Rico (Martinuzzi et al. 2007). El mapa fue creado mediante el analisis de un mosaico de imagenes de satelite Landsat ETM+ de los años 2000 – 2003. La clasificacion no supervisada ISODATA (“Iterative Self-Organizing Data Analysis Technique”) (ERDAS 2003) fue utilizada...

  20. Uma biblioteca de pontos de controle para imagens MSS Landsat

    OpenAIRE

    Fernando Augusto Mitsuo Ii

    1985-01-01

    O objetivo deste trabalho e desenvolver um sistema para criacao, manutencao e gerenciamento de uma biblioteca de pontos de controle para imagens MSS Landsat. Um ponto de controle e uma caracteristica fisicamente detectavel numa cena, cuja localizacao geodesica e precisamente conhecida. O uso destes pontos e de fundamental importancia num sistema de correcao geometrica de imagens de satelite. A biblioteca permitira que pontos de controle pertencentes a uma dada cena sejam recuperados de uma ma...

  1. Methodological possibilities for using the electron and ion energy balance in thermospheric complex measurements

    International Nuclear Information System (INIS)

    Serafimov, K.B.; Serafimova, M.K.

    1991-01-01

    Combination of ground based measurements for determination of basic thermospheric characteristics is proposed . An expression for the energy transport between components of space plasma is also derived and discussed within the framework of the presented methodology which could be devided into the folowing major sections: 1) application of ionosonde, absorption measurements, TEC-measurements using Faradey radiation or the differential Doppler effect; 2) ground-based airglow measurements; 3) airglow and palsma satelite measurements. 9 refs

  2. La teledeteccion satelital y los sistemas de proteccion ambiental

    Directory of Open Access Journals (Sweden)

    Francisco Sacristan Romero

    2005-07-01

    Full Text Available La Teledetección ofrece grandes posibilidades para la realización de progresos en el conocimiento de la naturaleza, aunque todavía no se ha logrado todo lo que de ella se esperaba debido a que se deben realizar perfeccionamientos en el nivel de resolución espacial, espectral y temporal de los datos. Además, es necesario un mayor rigor científico en la interpretación de los resultados obtenidos, tratando de no extraer conclusiones definitivas de los estudios medioambientales realizados mediante técnicas de Teledetección. Los modelos que se elaboran para interpretar los datos de Teledetección, deberán tener como objetivo eliminar los efectos ocasionados por la variabilidad en las condiciones de captación, la distorsión provocada por la atmósfera, y la influencia de parámetros tales como la posición del Sol, pendiente, exposición, y altitud. En este artículo intentaré desgranar las diversas y múltiples aplicaciones de la técnica de la teledetección al control de los residuos con efectos energéticos y medioambientales. The Teledetection offers great possibilities for the accomplishment of progresses in the knowledge of the nature, although everything has still not been obtained what of her it was expected because they think to make improvements in the level of space resolution, spectral and temporary of the data. In addition, a greater scientific rigor in the interpretation of the obtained results is necessary, treating about not drawing definitive conclusions of the made environmental studies by means of techniques of Teledetection. The models that are elaborated to process the data of Teledetection will have to have like objective to eliminate the effects caused by the variability in the conditions of pick up, the distortion caused by the atmosphere and the influence of parameters such as the position of the Sun, slope, exhibition, and altitude.

  3. Making IT ends meet. Susquehanna Health System outsources Siemens' prized product to nearby hospitals looking for an affordable alternative.

    Science.gov (United States)

    Becker, Cinda

    2004-08-16

    Susquehanna Health System has been offering small, rural hospitals a more affordable information technology system through a unique outsourcing agreement. The system's CIO, Pamela Wirth, left, has advocated the provider-to-provider arrangement, which could draw the ire of some vendors.

  4. Preparing Learners for the Future

    Directory of Open Access Journals (Sweden)

    Olga DeJesus

    2017-12-01

    Full Text Available Book review of “Teaching in a Globally Connected World: Preparing Learners for the Future.” Edited by Ervin F. Sparapani and Pamela L. Ross McClain. Lanham, MD: Hamilton Books, 2016. ISBN: 978-0-7618-6814-9

  5. Remote sensing of severe convective storms over Qinghai-Xizang Plateau

    Science.gov (United States)

    Hung, R. J.; Liu, J. M.; Tsao, D. Y.; Smith, R. E.

    1984-01-01

    The American satellite, GOES-1 was moved to the Indian Ocean at 58 deg E during the First GARP Global Experiment (FGGE). The Qinghai-Xizang Plateau significantly affects the initiation and development of heavy rainfall and severe storms in China, just as the Rocky Mountains influence the local storms in the United States. Satelite remote sensing of short-lived, meso-scale convective storms is particularly important for covering a huge area of a high elevation with a low population density, such as the Qinghai-Xizang Plateau. Results of this study show that a high growth rate of the convective clouds, followed by a rapid collapse of the cloud top, is associated with heavy rainfall in the area. The tops of the convective clouds developed over the Plateau lie between the altitudes of the two tropopauses, while the tops of convective clouds associated with severe storms in the United States usually extend much above the tropopause.

  6. 77 FR 50545 - Members of Senior Executive Service Performance Review Boards

    Science.gov (United States)

    2012-08-21

    ... Strategy (SB/SE) Gregory E. Kane, Deputy Chief Financial Officer, Chief Financial Office (CFO) Sheldon M.... Krieg, IRS Human Capital Officer, Human Capital Office (HCO) Pamela J. LaRue, Chief Financial Officer...) Lauren Buschor, Associate Chief Information Officer (CIO), Enterprise Operations, Information Technology...

  7. An intercultural approach to implementing multilingualism at Rhodes ...

    African Journals Online (AJOL)

    2005-10-06

    Oct 6, 2005 ... Russell H. Kaschula, Pamela Maseko, Lorenzo Dalvit, Thandeka Mapi, Linda Nelani,. Bulelwa Nosilela and .... fashion, trends, pop music) and of verbal and nonverbal symbols. ..... Assisted Language Learning - CALL) and specifically encourages independent learning. The ... Production of and access to.

  8. On the cosmic-ray spectra of three-body lepton-flavor-violating dark matter decays

    International Nuclear Information System (INIS)

    Carone, Christopher D.; Cukierman, Ari; Primulando, Reinard

    2011-01-01

    We consider possible leptonic three-body decays of spin-1/2, charge-asymmetric dark matter. Assuming a general Dirac structure for the four-fermion contact interactions of interest, we study the cosmic-ray electron and positron spectra and show that good fits to the current data can be obtained for both charged-lepton-flavor-conserving and flavor-violating decay channels. We find that different choices for the Dirac structure of the underlying decay operator can be significantly compensated by different choices for the dark matter mass and lifetime. The decay modes we consider provide differing predictions for the cosmic-ray positron fraction at energies higher than those currently probed at the PAMELA experiment; these predictions might be tested at cosmic-ray detectors like AMS-02.

  9. Conception de Réseaux Dynamiques Tolérants aux Pannes

    OpenAIRE

    Huc , Florian

    2008-01-01

    This thesis deals with different aspects of the conception of telecommunication networks. Such networks are a patchwork of various technologies : antenas-satelite links, radio links and optical links, but also onboard networks of satellites. The problematics differ according to the part of the networks on which we focus, to the type of request and to the objective. Paquet requests are studied in the case of grid networks, but this thesis mainly deal with connection requests (either unicast or...

  10. Multilingual Aeronautical Dictionary (Dictionnaire Aeronautique Multilingue)

    Science.gov (United States)

    1980-01-01

    8217See ’aerofoil profile’ DE Bord’Boden-Funkverkehr (ili 20~ AGARD MULTILINGUAL AERONAUTICAL DICTIONARY 10318 air mileage indicator (AMI) ES comunicacion ...Autogenschweissen (nil ES sistema fml autom~tico de comunicacion NE automatische besturing ES soldadura MI autdgena aire-tierra P otooWatmtc FR soudage Wm autogene...AERONAUTICAL DICTIONARY DE Fernmeldesatellit [m) RU 1. maPXWbPOBK& ff1 OTcOKOB RU onPe~ene~me Wn Aesma84HN Komnaca ES satelite Wm do comunicaciones 2

  11. Drawing 1/100,000 scale geological map of Mt. Hakkoda geothermal district

    Energy Technology Data Exchange (ETDEWEB)

    Muraoka, Hirobumi; Takakura, Shin' ichi

    1987-10-01

    Geological map of geothermal district of Mt. Hakkoda was made which included the main volcanos created after Pliocene era. For the purpose, geothermal liquid, terrestial heat sources and its storing structures, were studied with consulting geological map. Aerial and satelite photographs were used for the study of faults, foldings, and dikes,. By the result, stratigragic order of layers, developing process of vocanos, and evoluting process of magma, were summarized for report. (5 figs, 4 tabs, 101 refs)

  12. The Role Of The Military In Myanmars Political Economy

    Science.gov (United States)

    2016-03-01

    MILITARY IN MYANMAR’S POLITICAL ECONOMY by Pamela T. Stein March 2016 Thesis Advisor: Naazneen Barma Second Reader: Zachary Shore THIS......DISTRIBUTION CODE 13. ABSTRACT (maximum 200 words) This thesis examines the role of Myanmar’s military, the Tatmadaw, in the country’s political economy

  13. Editorial | Webster | South African Medical Journal

    African Journals Online (AJOL)

    Jacqui Webster, Christelle Crickmore, Karen Charlton, Krisela Steyn, Edelweiss Wentzel-Viljoen, Pamela Naidoo. Abstract. South Africa's salt reduction strategy: Are we on track, and what lies ahead? Full Text: EMAIL FREE FULL TEXT EMAIL FREE FULL TEXT · DOWNLOAD FULL TEXT DOWNLOAD FULL TEXT.

  14. ISSN 2073-9990 East Cent Afr J Surg

    African Journals Online (AJOL)

    cancer registry at Kilimanjaro Christian Medical Centre in northern Tanzania. Pamela T.K. ... was associated with no other symptoms except night pain and had been gradually growing. He ... healthy for his age and active. X-rays .... osteosarcoma, giant cell tumour, multiple myeloma, metastatic carcinomas, and high-grade.

  15. 78 FR 36508 - Notice of Sugar Purchase and Exchange for Re-Export Program Credits; and Notice of Re-Export...

    Science.gov (United States)

    2013-06-18

    ...; telephone (202) 690-0734. For sugar purchase and general exchange information contact Pamela McKenzie... license balance within certain limits. Sugar exported or transferred is subtracted from the license balance, resulting in a license ``credit;'' sugar imported is added to the balance, resulting in a license...

  16. Research on the Communication Development of Young Children with Deaf-Blindness.

    Science.gov (United States)

    Bullis, Michael, Ed.

    This booklet collects seven papers drawing on research performed through the Communication Skills Center for Young Children with Deaf Blindness of the Oregon State System of Higher Education and its affiliated sites. Papers include: "Research on Vision Assessment" (Pamela Cress); "Use of Microswitch Technology To Facilitate Social…

  17. Decrease Your Risk for Diabetes (A Cup of Health with CDC)

    Centers for Disease Control (CDC) Podcasts

    Nearly 30 million people in the U.S. have diabetes. Almost three times that many may have prediabetes, which puts them at increased risk for developing type 2 diabetes, heart disease, and stroke. In this podcast, Dr. Pamela Allweiss discusses ways to prevent or control diabetes.

  18. Journal of Food Technology in Africa - Vol 5, No 2 (2000)

    African Journals Online (AJOL)

    The Effects of pH and Heat Treatment Processing on the Stability of Natural Food Colours used in Dairy Products · EMAIL FREE FULL TEXT EMAIL FREE FULL TEXT DOWNLOAD FULL TEXT DOWNLOAD FULL TEXT. S. D. Mendi, Bob Peters, Pamela Tiku Kamga, 59-61 ...

  19. TeV Particle Astrophysics 2010, Booklet of abstracts

    International Nuclear Information System (INIS)

    None, C.; Davide Ferella, A.; Pato, M.; Catena, R.; Salucci, P.; Rielage, K.; Kobayashi, K.; Degunda, U.; Estrada, J.; Yue, Q.; Benbow, W.; Maestro, P.; Berghaus, P.; Benzvi, S.; Gallant, Y.; Coniglione, R.; Frey, R.; Besson, D.; Odrowski, S.; Ernenwein, J.P.; Dios Zornosa, J. de; Colnard, C.; Cavalcante de Souza, J.; Fraija, N.; Cerdeno, D.; Moroi, T.; Kumar, J.; Slatyer, T.; Yaguna, C.; Thomson, G.; Tameda, Y.; Taylor, A.; Giacinti, G.; Calvez, A.; Kotera, K.; Shinozaki, K.; Aharonian, F.; Essey, W.; Ahlers, M.; Fargion, D.; Canadas, B.; Boehm, C.; Palomares-Ruiz, S.; Panci, P.; Sanchez-Conde, M.A.; Hensley, B.; Vivier, M.; Hooper, D.; Finkbeiner, D.; Dobler, G.; Malyshev, D.; Mertsch, P.; Giannios, D.; Dalton, M.; Casandijan, J.M.; Mukherjee, R.; Morlino, G.; Ando, S.; Gilmore, R.; Medina, C.; Weitzel, Q.; Caprioli, D.; Vovk, I.; Vincent, S.; Delahaye, T.; Lavalle, J.; Galli, S.; Crocker, R.; Catena, R.; Cholis, I.; Sandick, P.; Rydberg, C.E.; Hulss, J.P.; Danninger, M.; Tran, D.; Spolyar, D.; Belanger, G.; Ronga, F.; Montanino, D.; Fornasa, M.; Regoes, E.; Caprioli, D.; Morlino, G.; Ostapchenko, S.; Kawanaka, N.; Kalli, S.; Whitehorn, N.; Boutayeb, B.; Casanellas, J.; Lopes, I.

    2012-01-01

    The aim of the conference is to bring together theorists and experimentalists working in the fields of Particle Physics, Astrophysics and Cosmology, with a shared interest in physical processes at the TeV energy scale. After decades of theoretical speculation, the exploration of the TeV energy frontier has now in fact begun, with the results provided by ground-based and space-born observatories of gamma-rays (Fermi, HESS, Magic, Veritas, Cangaroo, Milagro), anti-matter (PAMELA, ATIC, HESS and soon AMS-02) and neutrinos (IceCube, Antares), with a large number of ongoing direct Dark Matter search experiments exploiting different detection techniques, and with the TeV particle accelerators Tevatron and the Large Hadron Collider. The physics underlying these experiments involves many intertwined issues, such as the nature of Dark Matter, Physics beyond the Standard Model, the origin of Cosmic Rays and the distribution of Dark and visible matter in the Universe. This document gathers only the abstracts of the papers. (authors)

  20. Generation of auroral hectometer radio emission at the laser cyclotron resonance (ωp≥ωH)

    International Nuclear Information System (INIS)

    Vlasov, V.G.

    1992-01-01

    Generation of auroral hectometer (AHR) and kilometer (AKR) radio emission at a maser cyclotron resonance (MCR) in a relatively dense plasma (ω p ≥ω H ) is theoretically studied. The conclusion is made that availability of two-dimensional small-scale inhomogeneity of plasma density is the basic condition for the AHR generation at the MCR by auroral electron beams. The small-scale inhomogeneity of the auroral plasma, measured on satelites, meets by its parameters the conditions for the generation of auroral radio emission

  1. Cosmic Ray Anomalies from the MSSM?

    Energy Technology Data Exchange (ETDEWEB)

    Cotta, R.C.; /SLAC; Conley, J.A.; /Bonn U.; Gainer, J.S.; /Argonne /Northwestern U.; Hewett, J.L.; Rizzo, T.G.; /SLAC

    2011-08-11

    The recent positron excess in cosmic rays (CR) observed by the PAMELA satellite may be a signal for dark matter (DM) annihilation. When these measurements are combined with those from FERMI on the total (e{sup +} + e{sup -}) ux and from PAMELA itself on the {anti p}p ratio, these and other results are difficult to reconcile with traditional models of DM, including the conventional minimal Supergravity (mSUGRA) version of Supersymmetry even if boosts as large as 10{sup 3-4} are allowed. In this paper, we combine the results of a previously obtained scan over a more general 19-parameter subspace of the Minimal Supersymmetric Standard Model (MSSM) with a corresponding scan over astrophysical parameters that describe the propagation of CR. We then ascertain whether or not a good fit to this CR data can be obtained with relatively small boost factors while simultaneously satisfying the additional constraints arising from gamma ray data. We find that a specific subclass of MSSM models where the Lightest Supersymmetric Particle (LSP) is mostly pure bino and annihilates almost exclusively into {tau} pairs comes very close to satisfying these requirements. The lightest in this set of models is found to be relatively close in mass to the LSP and is in some cases the nLSP. These models lead to a significant improvement in the overall fit to the data by {approx}1 unit of {chi}{sup 2}/dof in comparison to the best fit without Supersymmetry while employing boosts in the range {approx}100-200. The implications of these models for future experiments are discussed.

  2. 77 FR 47814 - Sunshine Act Notice

    Science.gov (United States)

    2012-08-10

    ... Birmingham Hotel, Birmingham Ballroom, 21010 Richard Arrington Jr. Blvd. N., Birmingham, AL 35203. Briefing... Immigration Laws. I. Introductory Remarks by Chairman II. Panel I: Speakers' Remarks III. Panel I: Questions... Pamela Dunston at (202) 376-8105 or at [email protected] at least seven business days before the...

  3. Land Tenure, Gender, and Globalization : Research and Analysis ...

    International Development Research Centre (IDRC) Digital Library (Canada)

    Land Tenure, Gender, and Globalization : Research and Analysis from Africa, Asia, and Latin America. Couverture du livre Land Tenure, Gender, and Globalization : Research and Analysis from Africa. Directeur(s) : Dzodzi Tsikata et Pamela Golah. Maison(s) d'édition : Zubaan, CRDI. 29 août 2009. ISBN : 9788189884727.

  4. Pramana – Journal of Physics | Indian Academy of Sciences

    Indian Academy of Sciences (India)

    We find cosmic ray propagation parameters for which the proton and helium spectra remarkably agree with the PAMELA and CREAM measurements over four decades in energy. Volume 86 Issue 2 February 2016 pp 437-451 Special: Neutrino Physics. Neutrino mass bounds from neutrinoless double beta-decays and ...

  5. Interview with a quality leader: Kate Goonan on performance excellence. Interview by Pamela K. Scarrow.

    Science.gov (United States)

    Goonan, Kathleen Jennison

    2010-01-01

    Kathleen Jennison Goonan, MD, is Executive Director of the Mongan Institute for Health Policy, Center for Performance Excellence (CPE) at Massachusetts General Hospital. CPE guides transformational change in healthcare management and helps leaders, administrators, and practitioners in the healthcare workforce nationwide achieve and sustain performance excellence (http://www.mghcpe.org). An internist trained at the Massachusetts General Hospital, she has more than two decades' experience leading healthcare quality assessment and improvement initiatives. Before joining the CPE in 2002, she held a number of senior executive positions, including Senior Vice President of the Institute for Healthcare Improvement. Dr. Goonan has served as a judge for the Malcolm Baldrige National Quality Award, the Joint Commission's Codman Award, and for the American Hospital Association's McKesson Quest for Quality Award. She teaches extensively about achieving organizational performance excellence. Dr. Goonan co-authored Journey to Excellence: How the Baldrige Health Care Leaders Succeed, authored The Juran Prescription: Clinical Quality Management, and has written numerous articles and book chapters on performance improvement in healthcare. Dr. Goonan was faculty for the Harvard School of Public Health Leadership Development Program for Physicians from Academic Health Centers (1995-2007) and the Institute for Healthcare Improvement (1999-2005).

  6. Charge Asymmetric Cosmic Rays as a probe of Flavor Violating Asymmetric Dark Matter

    DEFF Research Database (Denmark)

    Masina, Isabella; Sannino, Francesco

    2011-01-01

    The recently introduced cosmic sum rules combine the data from PAMELA and Fermi-LAT cosmic ray experiments in a way that permits to neatly investigate whether the experimentally observed lepton excesses violate charge symmetry. One can in a simple way determine universal properties of the unknown...... component of the cosmic rays. Here we attribute a potential charge asymmetry to the dark sector. In particular we provide models of asymmetric dark matter able to produce charge asymmetric cosmic rays. We consider spin zero, spin one and spin one-half decaying dark matter candidates. We show that lepton...... flavor violation and asymmetric dark matter are both required to have a charge asymmetry in the cosmic ray lepton excesses. Therefore, an experimental evidence of charge asymmetry in the cosmic ray lepton excesses implies that dark matter is asymmetric....

  7. Generation of auroral hectometer radio emission at the laser cyclotron resonance ([omega][sub p][>=][omega][sub H]). Generatsiya avroral'nogo gektometrovogo radioizlucheniya na mazernom tsiklotronnom rezonatore ([omega][sub p]>or approx. [omega][sub H])

    Energy Technology Data Exchange (ETDEWEB)

    Vlasov, V G [Irkutskij Politekhnicheskij Inst., Irkutsk (Russian Federation)

    1992-06-01

    Generation of auroral hectometer (AHR) and kilometer (AKR) radio emission at a maser cyclotron resonance (MCR) in a relatively dense plasma ([omega][sub p][>=][omega][sub H]) is theoretically studied. The conclusion is made that availability of two-dimensional small-scale inhomogeneity of plasma density is the basic condition for the AHR generation at the MCR by auroral electron beams. The small-scale inhomogeneity of the auroral plasma, measured on satelites, meets by its parameters the conditions for the generation of auroral radio emission.

  8. Collage with Photoshop.

    Science.gov (United States)

    Sparkman, Russell

    The creative processes of 14 computer graphic artists are recorded in this book. Artists represented include: Joseph Kelter; Glenn Mitsui; Diane Fenster; Steve Lyons; Jeff Brice; Thirst; Pamela Hobbs; Lance Hidy; SKOLOS/WEDELL; Marcolina Design/Dan Marcolina; John Hersey; David Carson; Bert Monroy; and Jack Davis. The narrative provides insight…

  9. The influence of ApoE genotype on the lipid profile and lipoproteins ...

    African Journals Online (AJOL)

    The influence of ApoE genotype on the lipid profile and lipoproteins during normal pregnancy in a Southern African population. Donald Moshen Tanyanyiwa1,2, Adrian David Marais3, Pamela Byrnes3, Sheena Jones3. 1. Division of Human Genetics, Department of Pathology and Institute of Infectious Disease and ...

  10. Making History: SACES Presidential Leadership 1949-1998.

    Science.gov (United States)

    Sheeley, Vernon Lee

    This booklet provides educational, professional, and biographical information on 48 presidents of the Southern Association for Counselor Education and Supervision. A photo of each president is included. All leaders from 1949-1998 are covered. The presidents are: Donna Henderson, Debra Cobia, Pamela Paisley, Larry C. Loesch, Charlotte M. Taylor,…

  11. Disability and the Education System

    Science.gov (United States)

    Aron, Laudan; Loprest, Pamela

    2012-01-01

    Education is important for all children, but even more so for children with disabilities, whose social and economic opportunities may be limited. In this article, Laudan Aron and Pamela Loprest assess how well the nation's education system is serving students with disabilities. Aron and Loprest trace the evolution of the special education system…

  12. Indeterminate HIV-1 Western Blots: Etiology, Natural History, and Psychological Reactions

    Science.gov (United States)

    1992-09-16

    William Lafferty, Departments of Medicine. Laboratori’ Medicine. Epidenrioloý k. .nd Thomas S. Inui, Pamela H. Louie, Carol A. Gates, Biostatistics ...and dentistry . Finally, the psychosoclal onsequences of lWB are considerable.16 1655;LBISOTO2 JAB 13:33 03-17-92 P0003 U3 C9439 0021 11655 JGLM Nov

  13. Uniting the Disparate: Connecting Best Practices and Educational Mandates

    Science.gov (United States)

    Coke, Pamela K.

    2008-01-01

    Pamela K. Coke observes two high school English teachers who carry out practical assessments that supply them with an understanding of student achievement. The strategies used, such as Socratic seminar, book club meetings, and sticky notes, provide constructive information about what students are able to do and help identify ways such practices…

  14. Action Foundations! a Comic (Book) Tale of Defending Educational Studies

    Science.gov (United States)

    Nuñez, Isabel; Konkol, Pamela J.

    2013-01-01

    When defending educational foundations, Isabel Nunez and Pamela Konkol sometimes find themselves responding to the question of "why?"-often phrased, "But WHYYYYY do we have to take a class on this stuff??? (We want to take more methods!)." As distressing as this can be for teacher educators whose own work reveals rather a…

  15. 78 FR 40690 - Sunshine Act Meetings

    Science.gov (United States)

    2013-07-08

    ... ACTION: Revised Notice of Business Meeting. DATE AND TIME: Friday, July 12, 2013; 9:30 a.m. EST PLACE...: A Gender-Based Violation of Civil Rights Report Status Update on the Federal Civil Rights Engagement... Pamela Dunston at (202) 376-8105 or at [email protected] at least seven business days before the...

  16. Advances in Astroparticle Physics (2/5)

    CERN Multimedia

    CERN. Geneva

    2016-01-01

    Astroparticle physics is in an era of rapid progress. New observations challenge theory on several different fronts. We will analyze a few prominent examples, putting special emphasis on the connection with fundamental particle physics. Sessions 2&3: Galactic cosmic rays. What do we learn from new measurements by PAMELA, Fermi, and AMS02?

  17. Advances in Astroparticle Physics (3/5)

    CERN Multimedia

    CERN. Geneva

    2016-01-01

    Astroparticle physics is in an era of rapid progress. New observations challenge theory on several different fronts. We will analyze a few prominent examples, putting special emphasis on the connection with fundamental particle physics. Sessions 2&3: Galactic cosmic rays. What do we learn from new measurements by PAMELA, Fermi, and AMS02?

  18. Pramana – Journal of Physics | Indian Academy of Sciences

    Indian Academy of Sciences (India)

    Home; Journals; Pramana – Journal of Physics; Volume 76; Issue 1. Issue front cover thumbnail. Volume 76, Issue 1. January 2011, pages 1-188. pp 1-22 Topical Review. Results from PAMELA, ATIC and FERMI: Pulsars or dark matter? Debtosh Chowdhury Sudhir K Vempati Chanda J Jog · More Details Abstract Fulltext ...

  19. 75 FR 23820 - Notice of Docketing of Amendment Request for Materials License No. SNM-2506; Northern States...

    Science.gov (United States)

    2010-05-04

    ... INFORMATION CONTACT: Pamela Longmire, Ph.D., Project Manager, Licensing Branch, Division of Spent Fuel Storage... Generating Plant (PINGP), Unit Nos. 1 and 2, site in Goodhue County, Minnesota. The TN-40 cask is currently..., higher burnup spent fuel used in the PINGP reactor as well as associated changes to the ISFSI's technical...

  20. KESESUAIAN LAHAN DAN REVITALISASI TAMBAK BUDIDAYA UDANG DI KAWASAN INDUSTRIALISASI KABUPATEN PROBOLINGGO PROVINSI JAWA TIMUR

    Directory of Open Access Journals (Sweden)

    Utojo Utojo

    2014-12-01

    Full Text Available Penelitian ini bertujuan untuk menentukan kesesuaian lahan tambak budidaya udang di kawasan industrialisasi Kabupaten Probolinggo, Jawa Timur dan mengkaji strategi revitalisasi tambak berdasarkan hasil penelitian remediasi kualitas tanah dan air tambak. Data primer meliputi: topografi, lahan, dan hidrologi pesisir diperoleh melalui survai lapangan. Penentuan stasiun pengamatan dilakukan secara acak dan sistematik. Setiap lokasi pengambilan contoh ditentukan posisi koordinatnya dengan alat Global Positioning System (GPS. Data sekunder yang digunakan berupa data iklim, peta Rupa Bumi Indonesia kawasan Probolinggo skala 1:25.000 dan citra satelit ALOS AVNIR-2 tahun 2010. Data lapangan (topografi, pasang surut, fisika-kimia air dan tanah, data citra satelit ALOS AVNIR-2 dan data sekunder yang lain, dianalisis secara spasial menggunakan Sistem Informasi Geografi (SIG untuk memperoleh tingkat kesesuaian lahan. Berdasarkan hasil analisis kesesuaian lahan tambak dari total luasan tambak 2.143 ha, lahan yang sangat sesuai dan sesuai untuk budidaya udang yaitu 56 ha dan 618 ha. Lahan tersebut tersebar di Kecamatan Tongas dan Pajarakan. Lahan yang cukup sesuai ditemukan sebesar 1.235 ha, dan tersebar di Kecamatan Tongas, Sumberasih, Dringu, Gending, Kraksaan, Pajarakan, dan Paiton. Sedangkan lahan yang tidak sesuai yaitu 234 ha, terdapat di Kecamatan Sumberasih, Gending, dan Kraksaan. Percepatan target peningkatan produksi di tambak budidaya udang kawasan industrialisasi dapat dicapai melalui kesesuaian lahan dan revitalisasi tambak (perbaikan kualitas tanah dan air.

  1. Evaluation of Refractivity Profiles from CHAMP and SAC-C GPS Radio Occultation

    Science.gov (United States)

    Poli, Paul; Ao, Chi On; Joiner, Joanna; delaTorreJuarez, Manuel; Hoff, Raymond

    2002-01-01

    The GeoForschungsZentrum's Challenging Minisatellite Payload for Geophysical Research and Application (CHAMP, Germany-US) and the Comision Nacional de Actividades Especiales' Satelite de Aplicaciones Cientificas-C (SAC-C, Argentina-US) missions are the first missions to carry a second-generation Blackjack Global Positioning System (GPS) receiver. One of the new features of this receiver is its ability to sense the lower troposphere closer to the surface than the proof-of-concept GPS Meteorology experiment (GPS/MET). Since their launch, CHAMP and SAC-C have collected thousands of GPS radio occultations, representing a wealth of measurements available for data assimilation and Numerical Weather Prediction (NWP). In order to evaluate the refractivity data derived by the Jet Propulsion Laboratory (JPL) from raw radio occultation measurements, we use Data Assimilation Office (DAO) 6-hour forecasts as an independent state of the atmosphere. We compare CHAMP and SAC-C refractivity (processed by JPL) with refractivity calculated from the DAO global fields of temperature, water vapor content and humidity. We show statistics of the differences as well as histograms of the differences.

  2. Parametrización y optimización de modelos de inversión para la obtención de humedad del suelo a partir de datos satelitales de Radares de Apertura Sintética

    OpenAIRE

    Barber, Matías Ernesto

    2013-01-01

    Dentro del Plan Espacial Nacional (PEN), la Comisión Nacional de Actividades Espaciales (CONAE) tiene previsto el lanzamiento de la misión satelital SAOCOM, un radar de apertura sintética (SAR) que opera en microondas (λ = 23cm) y cuyo principal objetivo es la estimación de humedad del suelo sobre Pampa Húmeda. El problema de la estimación de variables biogeofísicas a partir de imágenes SAR es un problema mal condicionado, donde con frecuencia existen muchas combinaciones de parámetros de la ...

  3. Efectos de la televisión y las redes sociales en las competencias comunicativas de los estudiantes de la Universidad EAN

    OpenAIRE

    Santos Osorio, Jessica Vanessa; Rueda Duarte, Daniela

    2013-01-01

    Establecer el tipo de impacto que la televisión y las redes sociales tienen en las competencias comunicativas de los estudiantes de la Universidad EAN, es revisar el uso que hacen de la lengua española a nivel escrito y oral. Ya que la transmisión satelital y la Internet, como servicios globales, son ventanas por las que los jóvenes tienen fácil acceso a cualquier tipo de información, en cualquier idioma, y a cualquier sistema de comunicación, como las redes sociales

  4. Modelo de levantamiento de informacion fisica catastral para el Instituto Nacional de Tierras, oficina regional Trujillo

    OpenAIRE

    Castellanos, Víctor

    2011-01-01

    Se identificó la metodología utilizada para el catastro físico de los Asentamientos Campesinos del Estado Trujillo, durante la vigencia del Instituto Agrario Nacional, y la existente actualmente con el Instituto Nacional de Tierras, Ofi cina Regional Trujillo. La evaluación de esta información determinó la propuesta de un modelo de levantamiento con fi nes de densifi cación de redes geodésicas utilizando tecnología satelital GPS, que facilite la actualización catastral de los pred...

  5. Isothermality of the gas in the Coma cluster

    International Nuclear Information System (INIS)

    Hughes, J.P.; Yamashita, K.; Okumura, Y.; Tsunemi, H.; Matsuoka, M.

    1988-01-01

    The high-quality X-ray spectrum of the Coma cluster observed by the Japanese satelite Tenma in conjunction with imaging data from the Einstein Observatory was used to explore the temperature distribution of the cluster gas. It is found that pure polytropic models are inadequate to describe this temperature distribution. Instead, a hybrid model is proposed consisting of a central isothermal region surrounded by a polytropic distribution. It is shown that as much as 75 percent of the global emission may come from the isothermal component. 30 references

  6. Enredados y enchufados para saltar del cerco

    Directory of Open Access Journals (Sweden)

    Víctor Van Oeyen

    2015-01-01

    Full Text Available A partir de la experiencia concreta de la Asociación Latinoamericana de Educación Radiofónica (ALER, se revisan diferentes aspectos que conlleva la relación radio y redes electrónicas. ALRED, sistema satelital de radio de ALER aglutina actualmente 54 emisoras de 14 países que transmiten 7 horas diarias con una programación elaborada entre todas sus afiliadas, a base de un uso democratizador de la tecnología digital. El autor relata diferentes pasos tomados y las lecciones aprendidas en esta experiencia.

  7. Adopting Just-in-Time Teaching in the Context of an Elementary Science Education Methodology Course

    Science.gov (United States)

    Osmond, Pamela; Goodnough, Karen

    2011-01-01

    In this self-study, Pamela, a new science teacher educator, adopted Just-in-Time Teaching (JiTT) in the context of an elementary science education methodology course. JiTT is a teaching and learning strategy involving interaction between web-based study assignments and face-to-face class sessions. Students respond electronically to web-based…

  8. Measurements of Cosmic-Ray Proton and Helium Spectra from the BESS-Polar Long-Duration Balloon Flights Over Antarctica

    Science.gov (United States)

    Abe, K.; Fuke, H.; Haino, S.; Hams, T.; Hasegawa, M.; Horikoshi, A.; Itazaki, A.; Kim, K. C.; Kumazawa, T.; Kusumoto, A.; hide

    2016-01-01

    The BESS-Polar Collaboration measured the energy spectra of cosmic-ray protons and helium during two long-duration balloon flights over Antarctica in December 2004 and December 2007, at substantially different levels of solar modulation. Proton and helium spectra probe the origin and propagation history of cosmic rays in the galaxy, and are essential to calculations of the expected spectra of cosmic-ray antiprotons, positrons, and electrons from interactions of primary cosmic-ray nuclei with the interstellar gas, and to calculations of atmospheric muons and neutrinos. We report absolute spectra at the top of the atmosphere for cosmic-ray protons in the kinetic energy range 0.2-160 GeV and helium nuclei 0.15-80 GeV/nucleon. The corresponding magnetic rigidity ranges are 0.6-160 GV for protons and 1.1-160 GV for helium. These spectra are compared to measurements from previous BESS flights and from ATIC-2, PAMELA, and AMS-02. We also report the ratio of the proton and helium fluxes from 1.1 GV to 160 GV and compare to ratios from PAMELA and AMS-02.

  9. 78 FR 928 - Sunshine Act Meeting

    Science.gov (United States)

    2013-01-07

    ... in the Military I. Introductory Remarks by Chairman II. Panel I--9:30 a.m.-10:55 a.m.: Perspective of.... Panel III--1:15 p.m.-2:45 p.m.: Military Panel Speakers' Remarks and Questions from Commissioners VI... a sign language interpreter should contact Pamela Dunston at (202) 376-8105 or at [email protected

  10. Change Your Shoes, Change Your Life: On Object Play and Transformation in a Woman's Story

    Science.gov (United States)

    Young, Kay

    2012-01-01

    This article asks why adults play dress-up and investigates the role of object play in the making of magical thinking and the reforming of adult identity. The author looks at a wide spectrum of narratives and their genres--the fairy tale "Cinderella," the film comedy "Some Like it Hot", the epistolary novel "Pamela", the film melodrama "Now,…

  11. Prakiraan Daerah Penangkapan Ikan Di Selat Bali Berdasarkan Data Citra Satelit

    Directory of Open Access Journals (Sweden)

    Iqbal Ghazali

    2011-10-01

    Full Text Available Indonesia has a lot of potential marine ecosystem and fisheries, this condition make some many Indonesian get a occupation to be fisherman. However, that is make a problem during his fishing activity, so we have to make some sophisticated technology to support that is activity. At the time, remote sensing technology is the answer for they problem, it is because of that is technology fisherman can be improvement they catcher with more efficient. Determination of fishly ground area by remote sensing technology has some stage before arranging layout Fishly Ground Area Estimation (FGAE map. Procedure to arranging are respectively data searching, data processing, and data analysis, and the last stage is composing of layout of FGAE map.The main purpose of this study is to know about catching area at Bali straits based on image satellite with creating layout of FGAE map. This activity doing descriptive method and the value are based on observation, interview, active participation, and literature search data. At the PDPI making process, the chlorophyl-a data and sea surface temperature getting important parameter, which temperature is the main to parameter to understand of front area and upwelling which is have a lot of nutrient composition. In the other hand, chlorophyl-a is also parameter to know of prosperity area. The data of current, wind speed, wave, and sea surface level are important component as supporting data that will be help to fisherman on determination of fishing ground area at helping fisherman in catching activity. Keywords: Fishing ground, Remote sensing, Bali straits, Chlorophyl-a, Sea surface temperature  

  12. Catullan Voices in Heroides 15: How Sappho Became a Man

    Directory of Open Access Journals (Sweden)

    Judith P. Hallett

    2010-11-01

    Full Text Available This paper examines some echoes of Catullus' poetry in Heroides 15, chiefly but not exclusively from Catullus' poems in the elegiac meter. It argues that these “Catullan voices” strengthen the contention of Pamela Gordon (1997 that Ovid presents his readers with a “mannish Sappho”, a “Roman construction with few roots in the early Greek tradition.”

  13. Effective Measures of Continuing Education

    Science.gov (United States)

    2013-03-01

    00783b5a-f0fe-4f80- 90d6-019695e52d2d (accessed December 23, 2012). 4 Gordon, Robert , “Statement before the Federal Financial Management, Government...2012, 3. 21 Dr. Pamela Raymer , “Recruiting/Retention/Education,” M&RA DCS G-1 Smart Book, January 1, 2013. 22 The National Center for Educational

  14. Coping with Crying in Babies and Toddlers

    Science.gov (United States)

    High, Pamela

    2012-01-01

    Pamela High, MS, MD, co-director of the Infant Behavior, Cry and Sleep Clinic at the Brown Center for the Study of Children at Risk, discusses the phenomena of infant crying and the impact it has on families. In most cases, infant crying will peak and resolve in the early months, but infant irritability can increase the risk of maternal…

  15. Decrease Your Risk for Diabetes (A Cup of Health with CDC)

    Centers for Disease Control (CDC) Podcasts

    2016-11-03

    Nearly 30 million people in the U.S. have diabetes. Almost three times that many may have prediabetes, which puts them at increased risk for developing type 2 diabetes, heart disease, and stroke. In this podcast, Dr. Pamela Allweiss discusses ways to prevent or control diabetes.  Created: 11/3/2016 by MMWR.   Date Released: 11/3/2016.

  16. ¿Por qué el satélite Cóndor?

    Directory of Open Access Journals (Sweden)

    Leonardo Ferrerira

    2015-01-01

    Full Text Available Estados Unidos y Rusia representan el 15 por ciento de la población mundial sin embargo utilizan el 50 por ciento de la órbita geoestacionaria, mientras todo el Tercer Mundo emplea menos del 10 por ciento. Los países del Pacto Andino se encuentran trabajando conjuntamente en el uso compartido de un solo sistemas satelital CONDOR. Pero los críticos norteamericanos consideran que es una manera ineficiente e irracional congestionar el espectro orbital. El artículo se centra en describir este proyecto y la lógica Andina, la soberanía

  17. Sistemas satelitales

    OpenAIRE

    Osorio Avila, Fernando Arturo; Andrade Sigüenza, Edwin Ricardo

    2006-01-01

    En los últimos años, la tecnología satelital ha recobrado gran importancia en el terreno de las comunicaciones. El desarrollo de la fibra óptica parecía que iba a obstaculizar la evolución de los satélites artificiales de comunicación, como consecuencia de sus características de transmisión (Velocidad, Capacidad, Durabilidad…), pero pocos pensaron en los diversos retos que debía enfrentar esta tecnología de comunicación (geográficos, climáticos, y sobretodo financieros). Para cumplir el pr...

  18. Contenido

    OpenAIRE

    -, -

    2016-01-01

    Investigación Satelital – UAPSAT; Indicadores para la gestión del mantenimiento de equipos pesados; Influencia de los parámetros climáticos, soportado en tecnología de información y comunicación, determina un microclima apropiado del invernadero - Cerro de Pasco; Factores condicionantes de la calidad en la Educación Universitaria Peruana; Dificultades de atención y niveles de aprendizaje en estudiantes de Educación General Básica (EGB); Efectos de las técnicas de aprendizaje de la locución en...

  19. X-ray spectroscopy of highly ionised atoms of Ti through Zn in a dense plasma

    International Nuclear Information System (INIS)

    Morita, Shiguro; Fujita, Junji

    1985-01-01

    X-ray spectra for several elements have been observed from a high-temperature plasma produced in a vacuum spark using a curved-crystal spectrometer. The transition wavelengths of the He-like resonance lines for Ti through Zn are determined for the first time under careful experimental treatments. The result is compared with theoretical predictions. The transition wavelengths of the Fe He-like resonance series lines up to 1s6p-1s 2 and the Kβ transition energies of Ti partially M-shell-ionised ions (Ti VI-XIII) are also determined. As a result, several satelite lines are found. (orig.)

  20. Pulsars as the sources of high energy cosmic ray positrons

    International Nuclear Information System (INIS)

    Hooper, Dan; Blasi, Pasquale; Serpico, Pasquale Dario

    2009-01-01

    Recent results from the PAMELA satellite indicate the presence of a large flux of positrons (relative to electrons) in the cosmic ray spectrum between approximately 10 and 100 GeV. As annihilating dark matter particles in many models are predicted to contribute to the cosmic ray positron spectrum in this energy range, a great deal of interest has resulted from this observation. Here, we consider pulsars (rapidly spinning, magnetized neutron stars) as an alternative source of this signal. After calculating the contribution to the cosmic ray positron and electron spectra from pulsars, we find that the spectrum observed by PAMELA could plausibly originate from such sources. In particular, a significant contribution is expected from the sum of all mature pulsars throughout the Milky Way, as well as from the most nearby mature pulsars (such as Geminga and B0656+14). The signal from nearby pulsars is expected to generate a small but significant dipole anisotropy in the cosmic ray electron spectrum, potentially providing a method by which the Fermi gamma-ray space telescope would be capable of discriminating between the pulsar and dark matter origins of the observed high energy positrons

  1. Decaying dark matter in supersymmetric SU(5) models

    International Nuclear Information System (INIS)

    Luo Mingxing; Wang Liucheng; Wu Wei; Zhu Guohuai

    2010-01-01

    Motivated by recent observations from PAMELA, Fermi and H.E.S.S., we consider dark matter decays in the framework of supersymmetric SU(5) grand unification theories. An SU(5) singlet S is assumed to be the main component of dark matters, which decays into visible particles through dimension six operators suppressed by the grand unification scale. Under certain conditions, S decays dominantly into a pair of sleptons with universal coupling for all generations. Subsequently, electrons and positrons are produced from cascade decays of these sleptons. These cascade decay chains smooth the e + +e - spectrum, which permit naturally a good fit to the Fermi-LAT data. The observed positron fraction upturn by PAMELA can be reproduced simultaneously. We have also calculated diffuse gamma-ray spectra due to the e ± excesses and compared them with the preliminary Fermi-LAT data from 0.1 GeV to 10 GeV in the region 0 deg. ≤l≤ 360 deg., 10 deg. ≤|b|≤20 deg. The photon spectrum of energy above 100 GeV, mainly from final state radiations, may be checked in the near future.

  2. MEASUREMENTS OF COSMIC-RAY PROTON AND HELIUM SPECTRA FROM THE BESS-POLAR LONG-DURATION BALLOON FLIGHTS OVER ANTARCTICA

    Energy Technology Data Exchange (ETDEWEB)

    Abe, K.; Itazaki, A.; Kusumoto, A.; Matsukawa, Y.; Orito, R. [Kobe University, Kobe, Hyogo 657-8501 (Japan); Fuke, H. [Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210 (Japan); Haino, S.; Hasegawa, M.; Horikoshi, A.; Kumazawa, T.; Makida, Y.; Matsuda, S.; Matsumoto, K.; Nozaki, M. [High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801 (Japan); Hams, T.; Mitchell, J. W. [NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, MD 20771 (United States); Kim, K. C.; Lee, M. H.; Myers, Z. [IPST, University of Maryland, College Park, MD 20742 (United States); Nishimura, J., E-mail: Kenichi.Sakai@nasa.gov [The University of Tokyo, Bunkyo, Tokyo 113-0033 (Japan); and others

    2016-05-10

    The BESS-Polar Collaboration measured the energy spectra of cosmic-ray protons and helium during two long-duration balloon flights over Antarctica in 2004 December and 2007 December at substantially different levels of solar modulation. Proton and helium spectra probe the origin and propagation history of cosmic rays in the galaxy, and are essential to calculations of the expected spectra of cosmic-ray antiprotons, positrons, and electrons from interactions of primary cosmic-ray nuclei with the interstellar gas, and to calculations of atmospheric muons and neutrinos. We report absolute spectra at the top of the atmosphere for cosmic-ray protons in the kinetic energy range 0.2–160 GeV and helium nuclei in the range 0.15–80 GeV/nucleon. The corresponding magnetic-rigidity ranges are 0.6–160 GV for protons and 1.1–160 GV for helium. These spectra are compared to measurements from previous BESS flights and from ATIC-2, PAMELA, and AMS-02. We also report the ratio of the proton and helium fluxes from 1.1 to 160 GV and compare this to the ratios from PAMELA and AMS-02.

  3. TeV scale singlet dark matter

    International Nuclear Information System (INIS)

    Ponton, Eduardo; Randall, Lisa

    2009-01-01

    It is well known that stable weak scale particles are viable dark matter candidates since the annihilation cross section is naturally about the right magnitude to leave the correct thermal residual abundance. Many dark matter searches have focused on relatively light dark matter consistent with weak couplings to the Standard Model. However, in a strongly coupled theory, or even if the coupling is just a few times bigger than the Standard Model couplings, dark matter can have TeV-scale mass with the correct thermal relic abundance. Here we consider neutral TeV-mass scalar dark matter, its necessary interactions, and potential signals. We consider signals both with and without higher-dimension operators generated by strong coupling at the TeV scale, as might happen for example in an RS scenario. We find some potential for detection in high energy photons that depends on the dark matter distribution. Detection in positrons at lower energies, such as those PAMELA probes, would be difficult though a higher energy positron signal could in principle be detectable over background. However, a light dark matter particle with higher-dimensional interactions consistent with a TeV cutoff can in principle match PAMELA data.

  4. Her Excellency Ms Pamela Hamamoto, Ambassador, Permanent Representative of the United States of America to the United Nations Office and other International Organisations in Geneva

    CERN Multimedia

    Brice, Maximilien

    2015-01-01

    Signature ceremony with Ambassador P. Hamamoto and Director-General R. Heuer - Neutrino Protocol I (CERN- DoE) - Nuclear Physics experiment Protocol I (CERN-DoE) - Experiments Protocol II (CERN-DoE-NSF) - Accelerator Protocol III (CERN-DoE) - Addendum I to Accelerator Protocol III (CERN-DoE)

  5. Kuidas erivajadustega lastega toime tulla teoorias ja praktikas / Pamela Talzi

    Index Scriptorium Estoniae

    Talzi, Pamela

    2016-01-01

    Osilia koolituskeskuses toimuvatest tasuta eripedagoogika kursustest Saare maakonna üldhariduskoolide ja lasteaedade õpetajatele. Projekt sündis Osilia koolituskeskuse ja Tallinna Ülikooli koostöös. Koolituse kohta jagab selgitusi ka Tallinna Ülikooli õpetajate akadeemia koolitusjuht Külli Rauk

  6. A Proven Method for Meeting Export Control Objectives in Postal and Shipping Sectors

    Science.gov (United States)

    2015-02-01

    A Proven Method for Meeting Export Control Objectives in Postal and Shipping Sectors Gregory Crabb, U.S. Postal Inspection Service Julia H...mail fraud, mail theft, identity theft, child exploitation, and prohibited mailings such as bombs and biological and chemical threats...April 2012. http://resources.sei.cmu.edu/library/asset-view.cfm?assetid=10085 [Allen 2014a] Allen, Julia H., Crabb, Gregory; Curtis, Pamela D

  7. Al-Qaeda in Iraq (AQI): An Al-Qaeda Affiliate Case Study

    Science.gov (United States)

    2017-10-01

    123 Jonathan J. Schroden, “Measures for Security in a Counterinsurgency,” Journal of Strategic Studies , 32, issue 5 (2009). 124 Schultz...Security in a Counterinsurgency.” Journal of Strategic Studies . 32, no. 5 (2009). Shanker, Thom. “Qaeda Leaders in Iraq Neutralized, U.S. Says...Case Study Zack Gold With contributions from Pamela G. Faber October 2017 This work was performed under Federal Government

  8. The Role of Culture in Conflict Resolution

    Science.gov (United States)

    2008-03-01

    Grasping the Nettle ; Analyzing Cases of Intractable, Chester A. Crocker, Fen Osler Hampson, and Pamela Aall eds., United States Institute of Peace...considerations in his model.44 Many enduring conflicts are rooted in culturally engrained prejudices and biases against “the other.” Bercovitch makes...Fisher argues that conflicting beliefs, morals and methods of communication, all rooted in culture, influence negotiations in various ways.57 Some

  9. SHORT COMMUNICATION TRITERPENE COMPOUNDS FROM ...

    African Journals Online (AJOL)

    a

    Grison, P.L.; McKey, M.H.; Jaco, M.G.; Jean-Marie, B. Phytochemistry 2002, 61, 61. 3. Sergio, R.P.S.; Hee, B.C.; Young, G.S.; Thawatchai, S.; Vichai, R.; Norman, R.F.; Geoffrey,. A.C.; John, M.P.; Duglas, A.K. Planta Med. 2002, 68, 186. 4. Hong, J.Z.; Pamela, A.T.; Zeynep, A.; Ghee, T.T.; Yoko, S.; Hashimoto, K.; Masaya, N.;.

  10. Possibility of testing the light dark matter hypothesis with the alpha magnetic spectrometer.

    Science.gov (United States)

    Hooper, Dan; Xue, Wei

    2013-01-25

    The spectrum and morphology of gamma rays from the Galactic center and the spectrum of synchrotron emission observed from the Milky Way's radio filaments have each been interpreted as possible signals of ∼ 7-10 GeV dark matter particles annihilating in the inner Galaxy. In dark matter models capable of producing these signals, the annihilations should also generate significant fluxes of ∼ 7-10 GeV positrons which can lead to a distinctive bumplike feature in a local cosmic ray positron spectrum. In this Letter, we show that while such a feature would be difficult to detect with PAMELA, it would likely be identifiable by the currently operating Alpha Magnetic Spectrometer experiment. As no known astrophysical (i.e., nondark matter) sources or mechanisms are likely to produce such a sharp feature, the observation of a positron bump at around 7-10 GeV would significantly strengthen the case for a dark matter interpretation of the reported gamma-ray and radio anomalies.

  11. Antiproton and positron signal enhancement in dark matter mini-spikes scenarios

    International Nuclear Information System (INIS)

    Brun, Pierre; Bertone, Gianfranco; Lavalle, Julien; Salati, Pierre; Taillet, Richard

    2007-04-01

    The annihilation of dark matter (DM) in the Galaxy could produce specific imprints on the spectra of antimatter species in Galactic cosmic rays, which could be detected by upcoming experiments such as PAMELA and AMS02. Recent studies show that the presence of substructures can enhance the annihilation signal by a 'boost factor' that not only depends on energy, but that is intrinsically a statistical property of the distribution of DM substructures inside the Milky Way. We investigate a scenario in which substructures consist of ∼100 'mini-spikes' around intermediate-mass black holes. Focusing on primary positrons and antiprotons, we find large boost factors, up to a few thousand, that exhibit a large variance at high energy in the case of positrons and at low energy in the case of antiprotons. As a consequence, an estimate of the DM particle mass based on the observed cut-off in the positron spectrum could lead to a substantial underestimate of its actual value. (authors)

  12. Sistema de adquisición remota de datos hidrológicos en la cuenca del río Paute

    OpenAIRE

    Flor Garrido, Diana Lucía

    2007-01-01

    Este proyecto está enfocado a proveer alternativas tecnológicas para la transmisión telemática o adquisición remota de datos hidrológicos, con el fin de que la información pueda ser utilizada por el Modelo de predicción de caudales en la cuenca del río Paute, a través del planteamiento de cuatro alternativas de transmisión: radioenlace, spread spectrum, GPRS y satelital. Mediante i) diseño de los perfiles de los trayectos de propagación desde los sitios ii) cálculo de propagación radioeléctri...

  13. Chronotоpical mechanisms of management for development of society

    Directory of Open Access Journals (Sweden)

    O. M. Коrh

    2014-06-01

    On the basis of row of personally conducted theoretically ­ empiric full scale  and sounding expertly ­ analytical researches to the authors it was succeeded to expose the mechanisms of quota each of types of chronotope in the general model of levels of development of subjects of social existence. Coming from principle of the «gold crossing», authors consider that shaky chronotope with situatioonal forces of influence peculiar 68% carriers of marginal levels of development of society. As for the higher and more subzero types of chronotope, then each of them it belong to 16% representatives of nuclear, satelite, and also ballast and deviant levels of development

  14. Numerical study on drop formation through a micro nozzle

    International Nuclear Information System (INIS)

    Kim, Sung Il; Son, Gi Hun

    2005-01-01

    The drop ejection process from a micro nozzle is investigated by numerically solving the conservation equations for mass and momentum. The liquid-gas interface is tracked by a level set method which is extended for two-fluid flows with irregular solid boundaries. Based on the numerical results, the liquid jet breaking and droplet formation behavior is found to depend strongly on the pulse type of forcing pressure and the contact angle at the gas-liquid-solid interline. The negative pressure forcing can be used to control the formation of satelite droplets. Also, various nozzle shapes are tested to investigate their effect on droplet formation

  15. Propiedad y acceso a los medios de comunicación en el mundo

    Directory of Open Access Journals (Sweden)

    Ana Fiol

    2015-01-01

    Full Text Available La globalización genera una clase global de magnates locales de medios con un enorme poder político e influencia en la agenda pública. Prácticamente en todos los países en desarrollo y Europa, la televisión y la radiodifusión fueron monopolio de los Estados. La tecnología y la transnacionalización hicieron posible la transmisión satelital a través de las fronteras, destruyendo los controles oficiales y proveyendo a las audiencias nuevas opciones. Las clases medias y altas acceden a los nuevos medios. Las clases populares, los pobres urbanos, quedan excluidos.

  16. Mediation Outcomes from the Second Sudan Civil War: An Analysis of Abuja and Igad Peace Initiatives

    Science.gov (United States)

    2013-12-01

    Grasping the Nettle : Analyzing Cases of Intractable Conflict, eds. Chester A. Crocker, Fen Osler Hampson, and Pamela Aall (Washington, DC: United...Issues: The Root Causes of Sudan’s Civil Wars (Bloomington, IN: Indiana University, 2003): xi; Ruth Iyob and Gilbert M. Khadiagala, Sudan: The Elusive...however, considered the possibility of a unified identity in the New Sudan.148 Countering the GoS’s assertions that Sudan had historical roots in

  17. ÉTUDE DE CAS — Costa Rica : Du choix pour le consommateur à l ...

    International Development Research Centre (IDRC) Digital Library (Canada)

    17 déc. 2010 ... La CPC s'est adressée aux parties en cause pour obtenir l'information qui lui permettrait d'évaluer le pouvoir de marché de chacune. Une situation atypique, car normalement, c'est la CPC qui a le fardeau de la preuve, souligne Pamela Sittenfeld, directrice générale de la CPC au moment de l'enquête, ...

  18. Unified interpretation of cosmic-ray nuclei and antiproton recent measurements

    International Nuclear Information System (INIS)

    Di Bernardo, Giuseppe; Gaggero, Daniele; Evoli, Carmelo; Grasso, Dario; Maccione, Luca

    2009-09-01

    We use our numerical code, DRAGON, to study the implications and the impact of recent CREAM and PAMELA data on our knowledge of the propagation properties of cosmic ray nuclei with energy >or similar 1 GeV/n in the Galaxy. We will show that B/C (as well as N/O and C/O) and anti p/p data (especially including recent PAMELA results) can consistently be matched within a unique diffusion-reacceleration model. The requirement that light nuclei and anti p data are both reproduced within experimental uncertainties places stringent limits on suitable propagation parameters. In particular, we find the allowed range of the diffusion coefficient spectral index to be 0.38 A ≅15 kms -1 ) is allowed. Furthermore, we do not need to introduce any ad hoc break in the injection spectrum of primary cosmic rays. If antiproton data are not used to constrain the propagation parameters, a larger set of models is allowed. In this case, we determine which combinations of the relevant parameters maximize and minimize the antiproton flux under the condition of still fitting light nuclei data at 95% C.L. These models may then be used to constrain a possible extra antiproton component arising from astrophysical or exotic sources (e.g. dark matter annihilation or decay). (orig.)

  19. Calculation of attenuation by rain using the DAH model and diameter of antennas for the Ka Band in Mexico; Calculo de atenuacion por lluvia usando el modelo DAH y diametro de antena para Banda Ka en Mexico

    Energy Technology Data Exchange (ETDEWEB)

    Landeros-Ayala, S.; Neri-Vela, R; Cruz-Sanchez, H.; Hernandez-Bautista, H. [Universidad Nacional Autonoma de Mexico, Mexico, D.F. (Mexico)

    2002-03-01

    In the last years, the peak in the demand of satellite communication service has caused the saturation in the use of the frequencies corresponding to the band, Cand Ku. Due to this, the engineers have looked for viable alternatives, in order to satisfy the current requisition, as well as the future demand, for which a considerable increment is expected. One of these alternatives is the use of the Ka Band (20Hz/30Hz), that is why the importance of studying the propagation effects that are experienced at these frequencies, especially the attenuation effect by rain, as in this case, where it is significant. The present article has the purpose to describe the use of the Modelo DAH (whose authors are Asoka Dissanayake, Jeremy Allnutt and Fatim Haidara), mixed with the global maps of distribution of rain by Crane, for the calculation of the attenuation by rain in satellite communication systems operated in the Ka Band. Besides, antenna diameters for the systems of communications in Ka Band in different locations of the Mexican Republic, using for it the attenuation margins for rain obtained through the Modelo DAH, and using as references the characteristics of the ANIK F2 satellite and a terrestrial station VSAT, are proposed. [Spanish] En los ultimos anos, el auge en la demanda de servicios de comunicacion por satelite ha provocado la saturacion en los uso de la frecuencia correspondientes a las bandas C y Ku. Debido a esta razon, se han buscado alternativas viables para poder satisfacer la demanda actual, asi como la demanda futura, para la cual se espera un incremento considerable. Una de estas alternativas es el uso de Banda Ka (20Hz/30Hz), de ahi la importancia del estudio sobre los efectos de programacion que se experimentan a esta frecuencia, en especial, el efecto de atencion por lluvias, ya que sen este caso resulta ser significativa. El presente articulo tiene como finalidad describir el uso del Modelo DAH (cuyos autores son Asoka Dissanayake, Jeremy Allnutt y

  20. Linnalood / Andri Ksenofontov ; kommenteerinud R[eet] V[arblane

    Index Scriptorium Estoniae

    Ksenofontov, Andri, 1962-

    2010-01-01

    Erki Kasemetsa näitus "Kohad/Cities Revealed" ja Liina Siibi näitus "Gimme Danger" sarjast "Cityscape" Tallinna Linnagaleriis. Näitus "Jüri Kaarma lugemistuba" Vabaduse Galeriis. Rühmituse Johnson&Johnson näitus "Nothing Left to Save" Draakoni galeriis. Karel Koplimetsa, Sigrid Viiri ja Taaniel Raudsepa kunstiprojekt "OÜ Visible Solutions" Hobusepea galeriis. Inglise kunstniku Pamela June Crooki isikunäitus galeriis Vaal. Peeter Lauritsa fotonäitus "Trickster's Office" ArtDepoo galeriis

  1. Unmet health care needs for persons with environmental sensitivity

    OpenAIRE

    Gibson, Pamela Reed; Kovach, Shannon; Lupfer, Alexis

    2015-01-01

    Pamela Reed Gibson, Shannon Kovach, Alexis LupferDepartment of Psychology, James Madison University, Harrisonburg, VA, USAAbstract: Studies of unmet health care needs have shown that women, people with poor health, and people with lower socioeconomic status are more likely to report having unmet health care needs. In this study, we examined the types of and reasons for unmet health care needs in 465 people with environmental sensitivities. A second area of inquiry involved negative reactions ...

  2. Créer de la valeur pour les petits exploitants agricoles Les 26 et 27 ...

    International Development Research Centre (IDRC) Digital Library (Canada)

    Ida St-Martin

    27 mars 2012 ... formation; des soins de santé; et, par-dessus tout, un accès aux marchés. ... Pamela Anderson, directrice générale, Centre international de la pomme .... Les besoins en matière de sécurité alimentaire varient énormément d'une région à .... Ce débat d'experts met en relief la portée de cette nouvelle vision.

  3. Gender and Work in Capitalist Economies

    OpenAIRE

    Odih, Pamela

    2007-01-01

    From the industrial revolution through to more recent advances in information technology, radical changes in working practices have accelerated rates of production to previously unimaginable levels. The establishment of wage relations, in the second half of the 19th Century, precipitated the rise of the 'employment society' and a movement towards synchronized work. Industrialization epitomized the capitalist definition of work time. \\ud \\ud In Gender and Work in Capitalist Economies, Pamela O...

  4. Hostile Environment? The Development of Sexual Harassment Law in the United States 1971-1991

    OpenAIRE

    Coukos, Pamela

    2011-01-01

    AbstractHostile Environment?The Development of Sexual Harassment Law in the United States 1971 - 1991by Pamela CoukosDoctor of Philosophy in Jurisprudence and Social PolicyUniversity of California, BerkeleyProfessor Lauren B. Edelman, ChairHow did the sexual harassment litigation campaign succeed in defining a new antidiscrimination principle in the midst of the Reagan-era backlash against civil rights? In 1986, the U.S. Supreme Court definitively established sexual harassment as a violation...

  5. Curcumin: a natural substance with potential efficacy in Alzheimer’s disease

    OpenAIRE

    Potter, Pamela

    2013-01-01

    Pamela E Potter Department of Pharmacology, Arizona College of Osteopathic Medicine, Midwestern University, Glendale, AZ, USA Abstract: Curcumin is a component of turmeric, a spice used in many types of cooking. Epidemiological evidence suggesting that populations that eat food with a substantial amount of curcumin were at lower risk of Alzheimer’s disease (AD) led to the idea that this compound might have a neuroprotective effect. Curcumin has substantial antioxidant and anti-infl...

  6. 'Creature' についての共時的・通時的考察 -Richardson の書簡体小説を中心として-

    OpenAIRE

    脇本, 恭子

    2008-01-01

    The present paper aims at examinig the word 'creature' from both synchronic and diachronic perspectives. The first section begins with providing several definitions of 'creature,' along with its etymology, in reference to such major dictionaries as the Oxford English Dictionary and Johnson's A Dictionary of the English Language(1755). In the subsequent three sections, the frequency and the collocation of this word are investigated through Richardson's Pamela and Clarissa as our main linguisti...

  7. Pamela Ngesa A Review of George Gonaís Andrew Mtagwaba ...

    African Journals Online (AJOL)

    Jimmy Gitonga

    The book is divided into three parts. In the first part titled ... particular attention to the role of the Catholic Church, Kailembo's parents and his education in ... job at the ICFTU enhanced his interest in worker welfare, and Dr. Gona emphasizes.

  8. Orbit Geostasioner (GSO dalam Hukum Internasional dan Kepentingan Nasional Indonesia

    Directory of Open Access Journals (Sweden)

    Agus Pramono

    2013-04-01

    Full Text Available Space Treaty 1967 merupakan landasan Hukum Internasional (Ruang Angkasa atas pemanfaatan dan eksploitasi ruang angkasa termasuk bulan dan benda-benda angkasa lainnya. Pemanfaatan dan eksploitasi ruang angkasa tersebut dalam kenyataannya hanya mungkin dilakukan secara optimal oleh negara-negara maju yang memiliki sumber daya dan kemampuan teknologi maju. GSO merupakan salah satu sumber daya alam terbatas yang merupakan tempat strategis untuk penempatan satelit komunikasi. Satelit komunikasi pada dasarnya menjadi wahana utama dan sangat penting dalam mendukung berbagai kegiatan masyarakat dunia umumnya dan kepentingan nasional Indonesia pada khususnya meliputi aspek ekonomi, politik, sosial budaya maupun pertahanan keamanan. Dengan dilandasi semangat kerjasama internasional dalam memanfaatkan GSO untuk tujuan bersama bagi kemanusian dan perdamaian, disepakati prinsip kesetaraan akses di antara negara-negara. Perjuangan Indonesia bersama negara-negara katulistiwa lainnya melalui berbagai fora internasional terus dilanjutkan agar bisa mencapai pengaturan internasional atas pemanfaatan GSO lebih mencerminkan keadilan mengingat letak GSO berada pada posisi di atas ruang angkasa negara-negara katulistiwa. Space treaty 1967 is the international law of space based in utilizing and exploiting of the space including Moon and other space objects. The utilization and exploitation of the space is only conducted by the developed countries, which has the resources and developed technology. Geostasioner is one of the limited natural resources as a strategic place for communication satellite orbite. The communication satellite is the major vehicle to endorse many kind of the world people activities, and especially for the national interest such as economics, politics, social and culture, and also defence. The equal principle among states is based on the international cooperation in utilizing GSO for the human peace. Indonesia with other equatorial countries

  9. GPS, punto de contacto entre la Astronomía y otras disciplinas

    Science.gov (United States)

    Perdomo, R.

    En los primeros años de la pasada década, un grupo de Astrónomos de La Plata iniciaron trabajos de investigación en Geodesia Satelital. En esta presentación se propone repasar sus principales logros y situarlos en el contexto del desarrollo de la disciplina a nivel mundial. Por entonces las aplicaciones prácticas de la disciplina eran indirectas y solo evidentes para los especialistas. Los errores del Posicionamiento Satelital eran de varios metros y en posicionamiento relativo, del orden de medio metro. Estos resultados se lograban al cabo de varios días de medición continuada. En los años siguientes, el sistema GPS alcanzó su nivel operacional y produjo una revolución tanto en lo relacionado con los tiempos de medición como con las precisiones. El grupo de La Plata se desarrolló simultáneamente con GPS, lo que posibilitó su participación actual en diversos temas vigentes: aplicaciones de alta precisión para la materialización de sistemas terrestres de referencia, monitoreo de movimientos de la corteza, contribución con servicios internacionales para la determinación de movimientos tectónicos globales y regionales, monitoreo de la ionósfera a partir de la propagación de las señales, determinación de la ondulación del geoide a escala local, etc. También se generaron muchas aplicaciones prácticas algunas en tiempo real: navegación, apoyo a imágenes aéreas o satelitales, aplicaciones a la agricultura, catastro y ordenamiento territorial, apoyo a relevamientos geofísicos, etc.

  10. Bienestar espiritual de enfermeras y enfermeros en unidades de cuidado intensivo Bem-estar espiritual de enfermeiras e enfermeiros em unidades de cuidado intensivo Spiritual wellness of nurses in intensive care units

    Directory of Open Access Journals (Sweden)

    Luis Sierra Leguía

    2012-01-01

    -estar espiritual alto (46-60 pontos e as práticas que realizam são rezar (69,3 % ou meditar (57,4 %. Para 69,3 %, as crenças espirituais são importantes e 60,4% se sente frequentemente próximo de Deus. Conclusões: verificou-se um bem-estar espiritual alto, evidenciado pelas práticas e crenças espirituais. Para a en-fermagem, a espiritualidade é uma dimensão importante no cuidado porque permite crer na relação da experiência de cuidado.Purpose: To determine the degree of spiritual wellness of nurses serving in Intensive Care Units in Cartagena. Methodology: descriptive study, random sample of 101 female and male nurses with over six months in the work place. Upon the signature of the informed consent forms, a demographic characterization of the group was conducted using Pamela Reed's Spiritual Perspective Scale to measure spiritual beliefs and practices. Data are presented in frequencies and percentages. Results: 94.1 % are women, in average, aged 33.2 years and five-year working experience; 66.3% belong to a religious group. The total score of the scale is 60 points, 98% of the participants had a high spiritual wellness (46-60 points and their common practices are prayers (69.3 % or meditation (57.4 %. 69.3 % agreed to affrm that spiritual beliefs are important and 60.4% use to feel close to God. Conclusions: a high spiritual wellness was observed, substantiated in the spiritual practices and beliefs. In nursing, spirituality is an important dimension of care because it makes easier to believe in the relation of the health-care experience.

  11. Penyajian Data Pelanggan pada Lima Area PT. Telekomunikasi Indonesia, Tbk. Kandatel Pekalongan Menggunakan Google Earth

    Directory of Open Access Journals (Sweden)

    Much Aziz Muslim

    2015-10-01

    Full Text Available Prosedur sistem penyajian data pelanggan di PT. Telekomunikasi Indonesia, Tbk. Kandatel Pekalongan khususnya bidang Divisi Business Services masih menggunakan cara manual, hanya menggunakan media Micorsoft Excel. Dalam hal ini peneliti ingin menerapkannya dalam bentuk aplikasi Google Earth untuk membuat penyajian data pelanggan, karena Google Earth dapat memetakan bumi dari superimposisi gambar yang dikumpulkan dari pemetaan satelit, fotografi udara dan globe GIS tiga dimensi sehingga akan menghasilkan data yang akurat. Penyajian data dengan menggunakan Google Earth dilakukan dengan memanfaatkan bahasa markup HTML. Dengan cara ini, Divisi Business Service akan menjadi lebih mudah ketika menyajikan data-data para pelanggan Telkom yang mencakup lima area yaitu Batang, Pekalongan, Pemalang, Tegal dan Brebes. 

  12. Role of nutrition in performance enhancement and postexercise recovery

    OpenAIRE

    Beck, Kathryn L; Thomson, Jasmine S; Swift, Richard J; von Hurst, Pamela R

    2015-01-01

    Kathryn L Beck,1 Jasmine S Thomson,2 Richard J Swift,1 Pamela R von Hurst11School of Food and Nutrition, Massey Institute of Food Science and Technology, College of Health, Massey University Albany, Auckland, 2School of Food and Nutrition, Massey Institute of Food Science and Technology, College of Health, Massey University Manawatu, Palmerston North, New ZealandAbstract: A number of factors contribute to success in sport, and diet is a key component. An athlete's dietary requirements...

  13. Collection of lectures given on the occasion of the 5th status report of the project of reprocessing and waste treatment

    International Nuclear Information System (INIS)

    1984-09-01

    10 years of R and D work in retrospect with the emphasis being on the development of electrochemical processes for fuel reprocessing (1B-EMMA and 2B-EMMA), vitrification of high-activity wastes by remote control (PAMELA, WA-350), iodine filter development, wet incineration of α-activity wastes, Pu recycling (ALONA), improvement of the chemical flow charts in the planning of the WA-350. Such developments are complemented by processes applied at the HDB. (DG) [de

  14. Is there an association between immunosuppressant therapy medication adherence and depression, quality of life, and personality traits in the kidney and liver transplant population?

    OpenAIRE

    Gorevski, Elizabeth; Succop, Paul; Sachdeva, Jyoti; Cavanaugh, Teresa M; Volek, Paul; Heaton, Pamela; Chisholm-Burns, Marie; Martin-Boone, Jill E

    2013-01-01

    Elizabeth Gorevski,1 Paul Succop,1 Jyoti Sachdeva,1 Teresa M Cavanaugh,1 Paul Volek,1 Pamela Heaton,1 Marie Chisholm-Burns,2 Jill E Martin-Boone1 1University of Cincinnati, Cincinnati, OH, USA, 2University of Tennessee College of Pharmacy, Memphis, TN, USA Objectives: To measure the association of transplant patients' personality, depression, and quality of life with medication adherence in kidney and liver transplant recipients. Methods: A cross-sectional study of liver and kidney t...

  15. Directors General of Europe's research organisations at the EIROforum meeting, CERN 24/10/2001

    CERN Multimedia

    BRICE M.

    2001-01-01

    from left to right: Dr.J. Pamela, EFDA (European Fusion Development Agreement) Associate Leader for JET ( JET-EFDA) Dr. C. Carlile, DG Institut Laue-Langevin (ILL) Dr. A. Mitsos, DG Research, European Commission Prof. L. Maiani, DG CERN Dr. C. Cesarsky, DG European Southern Observatory (ESO) Prof. F. Kafatos, DG European Molecular Biology Laboratory (EMBL) Prof. W.G. Stirling, DG European Snchrotron Radiation Facility (ESRF) Dr.J.P. Poncelet, Director of Strategy and External Relations ESA (European Space Agency)

  16. Information technology Governance standards on mobile applications for fishing zone based onCobIT 5 Framework in Majene

    Science.gov (United States)

    Palalloi, Irfan Andi; Anwar, Azwar; Syarifuddin

    2018-05-01

    Most of the activities of Majene regency society dominant as a fisherman, by and large, they work based on the hereditary experiences of their ancestors. This is proven by fishery industry statistic that highest from other industry with 18,30 % in the distribution of the gross regional domestic product. In each specific case, utilization of technology becomes a necessity that plays a key role. Adoption of technology for fishermen groups in use of GPSequipment has frequently committed by the government also non-profit organization go through training and mentoring. Nowadays there are some modern mobile applications has been developed by government agency assist the group of fishermen handy on managing their fishing activity. Such us ZPPI data row from Lapan Satelite, nelpinwas also known as smart fisheries, infrastructure development for space oceanography (indeso). However, all of them carry out of the risk and problems on the user side. One of them related toaccuracy and reliability. In this research, we elaborate technical factor, governance, through Cobit framework and analyze the best practice standardfor implementing the technology. All in all, the result presented of the governance standard on control and implementing technology under customer dimension in information technology governance on the standard process to ensure benefit delivery for implementing mobile application fishery in DKP Majene regency.

  17. The Sentinel satellites revolutionise environmental observation; Los satelites Sentinel revolucionan la observacion medioambiental

    Energy Technology Data Exchange (ETDEWEB)

    River, A.

    2016-08-01

    Europe has in orbit three Sentinel satellites that are the backbone of the ambitious Copernicus system. Aimed at revolutionising environmental observation from both the scientific and commercial points of view, their objective is to capture massive volumes of data on the Earth with a view to ensuring progress in research into climate change, the oceans and the evolution of ice formations. (Author)

  18. Butterflies (Lepidoptera: Papilionoidea and Hesperoidea) and other protected fauna of Jones Estate, a dying watershed in the Kumaon Himalaya, Uttarakhand, India

    OpenAIRE

    P. Smetacek

    2012-01-01

    Two hundred and forty three species of butterflies recorded from Jones Estate, Uttarakhand between 1951 and 2010 are reported. The ongoing rapid urbanization of Jones Estate micro-watershed will destroy the habitat of 49 species of wildlife protected under Indian law, as well as several species of narrow endemic moths and butterflies. The only known Indian habitat for the butterfly Lister’s Hairstreak Pamela dudgeoni will be destroyed. The effect on the water flow of both the Bhimtal and Sa...

  19. Searching for dark matter signals in the left-right symmetric gauge model with CP symmetry

    International Nuclear Information System (INIS)

    Guo Wanlei; Wu Yueliang; Zhou Yufeng

    2010-01-01

    We investigate the singlet scalar dark matter (DM) candidate in a left-right symmetric gauge model with two Higgs bidoublets in which the stabilization of the DM particle is induced by the discrete symmetries P and CP. According to the observed DM abundance, we predict the DM direct and indirect detection cross sections for the DM mass range from 10 to 500 GeV. We show that the DM indirect detection cross section is not sensitive to the light Higgs mixing and Yukawa couplings except for the resonance regions. The predicted spin-independent DM-nucleon elastic scattering cross section is found to be significantly dependent on the above two factors. Our results show that the future DM direct search experiments can cover the most parts of the allowed parameter space. The PAMELA antiproton data can only exclude two very narrow regions in the two Higgs bidoublets model. It is very difficult to detect the DM direct or indirect signals in the resonance regions due to the Breit-Wigner resonance effect.

  20. Gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV

    CERN Document Server

    Gaggero, Daniele; Marinelli, Antonio; Urbano, Alfredo; Valli, Mauro

    2016-01-01

    As recently shown, Fermi-LAT measurements of the diffuse gamma-ray emission from the Galaxy favor the presence of a smooth softening in the primary cosmic-ray spectrum with increasing Galactocentric distance. This result can be interpreted in terms of a spatial-dependent rigidity scaling of the diffusion coefficient. The DRAGON code was used to build a model based on such feature. That scenario correctly reproduces the latest Fermi-LAT results as well as local cosmic-ray measurements from PAMELA, AMS-02 and CREAM. Here we show that the model, if extrapolated at larger energies, grasps both the gamma-ray flux measured by MILAGRO at 15 TeV and the H.E.S.S. data from the Galactic ridge, assuming that the cosmic-ray spectral hardening found by those experiments at about 250 GeV/n is present in the whole inner Galactic plane region. Moreover, we show as that model also predicts a neutrino emission which may account for a significant fraction, as well as for the correct spectral shape, of the astrophysical flux mea...

  1. Deciphering the Local Interstellar Spectra of Primary Cosmic-Ray Species with HELMOD

    Science.gov (United States)

    Boschini, M. J.; Della Torre, S.; Gervasi, M.; Grandi, D.; Jóhannesson, G.; La Vacca, G.; Masi, N.; Moskalenko, I. V.; Pensotti, S.; Porter, T. A.; Quadrani, L.; Rancoita, P. G.; Rozza, D.; Tacconi, M.

    2018-05-01

    Local interstellar spectra (LIS) of primary cosmic ray (CR) nuclei, such as helium, oxygen, and mostly primary carbon are derived for the rigidity range from 10 MV to ∼200 TV using the most recent experimental results combined with the state-of-the-art models for CR propagation in the Galaxy and in the heliosphere. Two propagation packages, GALPROP and HELMOD, are combined into a single framework that is used to reproduce direct measurements of CR species at different modulation levels, and at both polarities of the solar magnetic field. The developed iterative maximum-likelihood method uses GALPROP-predicted LIS as input to HELMOD, which provides the modulated spectra for specific time periods of the selected experiments for model–data comparison. The interstellar and heliospheric propagation parameters derived in this study are consistent with our prior analyses using the same methodology for propagation of CR protons, helium, antiprotons, and electrons. The resulting LIS accommodate a variety of measurements made in the local interstellar space (Voyager 1) and deep inside the heliosphere at low (ACE/CRIS, HEAO-3) and high energies (PAMELA, AMS-02).

  2. LA TRADUCCIÓN DE VERBOS DE MOVIMIENTO DEL INGLÉS AL ESPAÑOL. UNA APLICACIÓN PRÁCTICA DE LA SEMÁNTICA COMPONENCIAL EN LA FORMACIÓN DE TRADUCTORES

    Directory of Open Access Journals (Sweden)

    Rafael Saldívar Arreola

    2015-01-01

    Full Text Available En el presente artículo se analizan algunos procesos semánticos que están involucrados en la lexicalización de elementos verbales, específicamente en la codificación de trayectoria y modo en verbos de movimiento, en el marco del proceso de la traducción. La base teórica de este análisis parte de la conocida tipología de Talmy (2000, que ubica al inglés como una lengua de marco satelital y al español como una lengua de marco verbal. El análisis presentado toma como base un corpus paralelo español-inglés de traducciones hechas por estudiantes de traducción mexicanos.

  3. LA TRADUCCIÓN DE VERBOS DE MOVIMIENTO DEL INGLÉS AL ESPAÑOL. UNA APLICACIÓN PRÁCTICA DE LA SEMÁNTICA COMPONENCIAL EN LA FORMACIÓN DE TRADUCTORES

    Directory of Open Access Journals (Sweden)

    Rafael Saldívar Arreola

    2015-01-01

    Full Text Available En el presente artículo se analizan algunos procesos semánticos que están involucrados en la lexicalización de elementos verbales, específicamente en la codificación de trayectoria y modo en verbos de movimiento, en el marco del proceso de la traducción. La base teórica de este análisis parte de la conocida tipología de Talmy (2000, que ubica al inglés como una lengua de marco satelital y al español como una lengua de marco verbal. El análisis presentado toma como base un corpus paralelo español- inglés de traducciones hechas por estudiantes de traducción mexicanos.

  4. Statistical distribution of solar soft X-ray bursts

    International Nuclear Information System (INIS)

    Kaufmann, P.; Piazza, L.R.; Schaal, R.E.

    1979-01-01

    Nearly 1000 solar events with fluxes measured in 0.5-3A 0 , 1-8A 0 and 8-20A 0 bands by Explorer 37 (US NRL Solrad) satelite are statistically analysed. The differential distribution of peak fluxes can be represented by power laws with exponents -1.4, -2.2, -2.9 respectively, which are compared to 2-12A 0 results. At the 0.5-3A 0 band there is a suggested peak in the distribution. Autocorrelation analysis of the distribution have shown that in the harder band (0.5-3A 0 ) there is a concentration of events at preferred values multiplied of about 10x10 -5 erg cm -2 S -1 of unknown origin [pt

  5. La teledetección directa por satélites y la solución de controversias

    Directory of Open Access Journals (Sweden)

    Luis Castillo Argañarás

    2014-04-01

    Full Text Available Una de las actividades comerciales espaciales es la teledetección satelital, en este ámbito actúan frecuentemente Estados, organizaciones internacionales y empresas privadas. En 1986, la Asamblea General de la ONU adoptó la Resolución Principios Relativos ala Teleobservación, mientras que en el año 2011, la Corte Permanente de Arbitraje de La Haya adoptó las “Reglas Opcionales para Arbitraje de Controversias, relativas con las actividades del espacio ultraterrestre”. Fundamentos que soportan el desarrollo del presente ensayo cuyo objetivo permite analizar si la Resolución de 1986 regula de manera adecuada las controversias que se plantean y aproximarnos brevemente a las Reglas Opcionales para Arbitraje adoptadas en el año 2011.

  6. No Prejudice in Space

    Energy Technology Data Exchange (ETDEWEB)

    Cotta, R.C.; Gainer, J.S.; Hewett, J.L.; Rizzo, T.G.; /SLAC

    2010-08-26

    might not be sufficient to determine the correct model of the underlying physics. As a first look at the signatures of these models in indirect detection experiments, we examined whether our models could explain the PAMELA excess in the positron to electron ratio at high energies. We find that there are models which fit the PAMELA data rather well, and some of these have significantly smaller boost factors than generally assumed for a thermal relic. The study of the pMSSM presents exciting new possibilities for SUSY phenomenology. The next few years will hopefully see important discoveries both in colliders and in satellite or ground-based astrophysical experiments. It is important that we follow the data and not our existing prejudices; hopefully this sort of relatively model-independent approach to collider and astrophysical phenomenology can be useful in this regard.

  7. No Prejudice in Space

    International Nuclear Information System (INIS)

    2010-01-01

    determine the correct model of the underlying physics. As a first look at the signatures of these models in indirect detection experiments, we examined whether our models could explain the PAMELA excess in the positron to electron ratio at high energies. We find that there are models which fit the PAMELA data rather well, and some of these have significantly smaller boost factors than generally assumed for a thermal relic. The study of the pMSSM presents exciting new possibilities for SUSY phenomenology. The next few years will hopefully see important discoveries both in colliders and in satellite or ground-based astrophysical experiments. It is important that we follow the data and not our existing prejudices; hopefully this sort of relatively model-independent approach to collider and astrophysical phenomenology can be useful in this regard.

  8. R-parity violating right-handed neutrino in gravitino dark matter scenario

    International Nuclear Information System (INIS)

    Endo, Motoi

    2009-06-01

    A decay of the gravitino dark matter is an attractive candidate to explain the current excesses of the PAMELA/ATIC cosmic-ray data. However, R-parity violations are required to be very tiny in low-energy scale. We suggest a R-parity violation in the right-handed neutrino sector. The violation is suppressed by a see-saw mechanism. Although a reheating temperature is constrained from above, the thermal leptogenesis is found to work successfully with a help of the R-parity violating right-handed neutrino. (orig.)

  9. R-parity violating right-handed neutrino in gravitino dark matter scenario

    Energy Technology Data Exchange (ETDEWEB)

    Endo, Motoi [CERN, Geneva (Switzerland). Theory Div., PH Dept.; Shindou, Tetsuo [Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany)

    2009-06-15

    A decay of the gravitino dark matter is an attractive candidate to explain the current excesses of the PAMELA/ATIC cosmic-ray data. However, R-parity violations are required to be very tiny in low-energy scale. We suggest a R-parity violation in the right-handed neutrino sector. The violation is suppressed by a see-saw mechanism. Although a reheating temperature is constrained from above, the thermal leptogenesis is found to work successfully with a help of the R-parity violating right-handed neutrino. (orig.)

  10. On the Energy Spectra of GeV/TeV Cosmic Ray Leptons

    Energy Technology Data Exchange (ETDEWEB)

    Stawarz, Lukasz; /KIPAC, Menlo Park /Jagiellonian U., Astron. Observ.; Petrosian, Vahe; /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., Appl. Phys. Dept.; Blandford, Roger D.; /KIPAC, Menlo Park

    2011-08-19

    protons. The second source discussed here is due to the annihilation of the diffuse Galactic {gamma}-rays on the stellar photon field. We find that high positron fraction increasing with energy, as claimed by the PAMELA experiment, cannot be explained in our model with the conservative set of the model parameters. We are able, however, to reproduce the PAMELA (as well as Fermi and HESS) results assuming high values of the starlight and interstellar gas densities, which would be more appropriate for vicinities of supernova remnants. A possible solution to this problem may be that cosmic rays undergo most of their interactions near their sources due to the efficient trapping in the far upstream of supernova shocks by self-generated, cosmic ray-driven turbulence.

  11. PAMELA’S MEASUREMENTS OF MAGNETOSPHERIC EFFECTS ON HIGH-ENERGY SOLAR PARTICLES

    Energy Technology Data Exchange (ETDEWEB)

    Adriani, O.; Bongi, M. [Department of Physics and Astronomy, University of Florence, I-50019 Sesto Fiorentino, Florence (Italy); Barbarino, G. C. [Department of Physics, University of Naples “Federico II,” I-80126 Naples (Italy); Bazilevskaya, G. A. [Lebedev Physical Institute, RU-119991 Moscow (Russian Federation); Bellotti, R.; Bruno, A. [University of Bari, I-70126 Bari (Italy); Boezio, M.; Bonvicini, V.; Carbone, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Bogomolov, E. A. [Ioffe Physical Technical Institute, RU-194021 St. Petersburg (Russian Federation); Bottai, S. [INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence (Italy); Bravar, U. [Space Science Center, University of New Hampshire, Durham, NH (United States); Cafagna, F. [INFN, Sezione di Bari, I-70126 Bari (Italy); Campana, D. [INFN, Sezione di Naples, I-80126 Naples (Italy); Carlson, P. [KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm (Sweden); Casolino, M.; De Donato, C. [INFN, Sezione di Rome “Tor Vergata,” I-00133 Rome (Italy); Castellini, G. [IFAC, I-50019 Sesto Fiorentino, Florence (Italy); Christian, E. R.; Nolfo, G. A. de, E-mail: georgia.a.denolfo@nasa.gov [Heliophysics Division, NASA Goddard Space Flight Center, Greenbelt, MD (United States); and others

    2015-03-01

    The nature of particle acceleration at the Sun, whether through flare reconnection processes or through shocks driven by coronal mass ejections, is still under scrutiny despite decades of research. The measured properties of solar energetic particles (SEPs) have long been modeled in different particle-acceleration scenarios. The challenge has been to disentangle the effects of transport from those of acceleration. The Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) instrument enables unique observations of SEPs including the composition and angular distribution of the particles about the magnetic field, i.e., pitch angle distribution, over a broad energy range (>80 MeV)—bridging a critical gap between space-based and ground-based measurements. We present high-energy SEP data from PAMELA acquired during the 2012 May 17 SEP event. These data exhibit differential anisotropies and thus transport features over the instrument rigidity range. SEP protons exhibit two distinct pitch angle distributions: a low-energy population that extends to 90° and a population that is beamed at high energies (>1 GeV), consistent with neutron monitor measurements. To explain a low-energy SEP population that exhibits significant scattering or redistribution accompanied by a high-energy population that reaches the Earth relatively unaffected by dispersive transport effects, we postulate that the scattering or redistribution takes place locally. We believe that these are the first comprehensive measurements of the effects of solar energetic particle transport in the Earth’s magnetosheath.

  12. Activity report 1984

    International Nuclear Information System (INIS)

    Drent, W.

    1985-07-01

    For the fiscal year 1984, the technical activities of Eurochemic were: a) the cleaning of the vessels having contained medium level liquid wastes and the incorporation into bitumen of the resulting solution, b) the conditioning of plutonium contaminated solid waste, c) the civil engineering works of Building 29 were completed and the mounting of equipment was begun. The installation will assure the surface storage of the blocks resulting from vitrification, by means of Pamela installation of the high-level liquid wastes. The report includes administrative matters as well as health and safety activity. (AF)

  13. Dark matter and its detection

    International Nuclear Information System (INIS)

    Bi Xiaojun; Qin Bo

    2011-01-01

    We first explain the concept of dark matter,then review the history of its discovery and the evidence of its existence. We describe our understanding of the nature of dark matter particles, the popular dark matter models,and why the weakly interacting massive particles (called WIMPs) are the most attractive candidates for dark matter. Then we introduce the three methods of dark matter detection: colliders, direct detection and indirect detection. Finally, we review the recent development of dark matter detection, including the new results from DAMA, CoGent, PAMELA, ATIC and Fermi. (authors)

  14. KSC-04PD-2219

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. KSC employees learn about a mechanical robot displayed at an exhibit during Spaceport Super Safety and Health Day. The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  15. KSC-04PD-2220

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. KSC Employees stop by the American Red Cross exhibit during Spaceport Super Safety and Health Day. The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  16. KSC-04PD-2224

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Center Director Jim Kennedy kicks off Spaceport Super Safety and Health Day for second shift employees. The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic- great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  17. KSC-04PD-2222

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. KSC employees stop at a table with a display of juices during Spaceport Super Safety and Health Day. The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic- great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  18. Kontribusi Ekonomi Perempuan Penjual Ayam Goreng Gerobak di Beberapa Pasar Satelit di Kota Padang

    Directory of Open Access Journals (Sweden)

    Dwi Yuzaria

    2011-10-01

    Full Text Available Economical contribution of women in merchant-chart-fried chicken business in satellite market in padang city ABSTRACT. As social-economic demands increased, the complexity of family needs grew higher. To fulfill them, woman has to take part in making a living. This research aims to see economical performance of women in running merchant-cart-fried-chicken, identifying the obstacles faced and giving alternatives of solution. This research was conducted by survey method, with respondents of merchant-cart-fried-chicken seller in several markets in Padang city. Sample was taken with proportional allocation of 15 people. Data was analyzed by descriptive analysis method. The research showed that economical performance of women merchant-cart-fried-chicken seller is low with working hour o5 5.07 hours/day. Percentage of women that take part in all activities start from planning to marketing is 32.5%. This is a potential business to develop, with average income 92.259,58 IDR/day and average R/C ratio 1.29. Internal constraints were family relation pattern that scoped women’s part in fulfilling family need, meanwhile the external constraints were the difficulties in acquiring more capital to develop the business and the price fluctuation of chicken as a main raw material. Alternative solution that can be offered was opening the business at home so that women can spare more time to work the business and accessing soft loan with light requirements. The conclusion of the research was that women took part in making a living for the family, however the contribution is low due to patriarchy value as an internal constraint and capital problem as external constraint. The solution offered was taking soft loan and building relation with raw material supplier.

  19. Pengembangan Aplikasi Multimedia untuk Pembelajaran Satelit Astronomi NASA dengan Teknologi Augmented Reality Berbasis Android

    Directory of Open Access Journals (Sweden)

    Dilan Arya Sujati

    2016-04-01

    Full Text Available With the advancement of technology in various aspects of life of today's technology allows developers to create applications that aims to facilitate the public in obtaining information based on mobile. Seeing the importance of the role of astronomy satellites it needs to make a multimedia application with Augmented Reality technology that can provide an overview and brief specifications on astronomy satellite without having to go to the planetarium or observatory.This research is using MDLC (Multimedia Development Life Cycle framework. The process of assembly (pemasangan was performed using Unity and Vuforia library. The result is a book containing related image about NASA’s astronomy satellites which functioned as a marker and an Augmented Reality application based on Android that is capable of displaying NASA’s astronomical satellites on the top of marker that can display brief information about the shape and its parts when touched on the screen. The application that has been made function properly and in accordance with the concept and design. The ideal condition of using the application in places exposed to light with the intensity of 108,3 ± 2,5 lux upwards. In addition the camera is directed to the distance between 10-75 cm of the marker and the angle between 40 ± 0,5 O – 140 ± 0,5 O .. The greater the intensity of the light does not affect the sensitivity of the camera to detect the marker increases. In other words, the marker will not be detected if the distance marker on the camera more than 75 cm and the angle of the camera marker less than 40 ± 0,5 O or more than 140 ± 0,5 O though the light intensity is greater.

  20. Solitary pulmonary nodule: radiologic features and diagnostic approach; Nodulo pulmonar solitario: caracteristicas radiologicas y abordaje diagnostico

    Energy Technology Data Exchange (ETDEWEB)

    Rodriguez Cambronero, Luis Enrique

    2012-07-01

    A literature review is conducted on the solitary pulmonary nodule, to determine the diagnostic methods and specific characteristics. The diagnostic methods used have been: chest radiography, computed tomography, positron emission tomography and magnetic resonance imaging. The radiological features are defined: location, size, definition of contours or edges (margins), densitometric and attenuation characteristics, cavitation, air bronchogram, growth, doubling time, satellite nodules, nutrient vessels [Spanish] Una revision bibliografica es realizada sobre el nodulo pulmonar solitario, para determinar los metodos de diagnostico y caracteristicas especificas. Los metodos de diagnostico utilizados han sido: la radiografia de torax, tomografia computarizada, tomografia por emision de positrones y resonancia magnetica. Las caracteristicas radiologicas son definidas: localizacion, tamano, definicion de los bordes o contornos (margenes), caracteristicas densitometricas y de atenuacion, cavitacion, broncograma aereo, crecimiento, tiempo de duplicacion, nodulos satelite, vasos nutrientes.

  1. Characteristics of ion beam and anode plasma in open-quotes Point Pinch Diodeclose quotes

    International Nuclear Information System (INIS)

    Masugata, K.; Yatsui, K.; Tazima, T.

    1993-01-01

    Diagnostics and evaluation have been carried out on an ion beam and anode plasma in open-quotes Point Pinch Diode.close quotes Mass spectra of ion beam measured by Thomson-parabola spectrometer have shown that the main component are (1) proton and H 2 + , (2) highly ionized carbon and oxygen ions, and (3) singly ionized C, O and molecules such as CO 2 + , OH + , OH 2 + . X-ray and particle pinhole images have shown the size of the electron beam on the plasma to be less than ∼0.5 mm in diameter, in which fine structures are found with size less than 0.05 mm. A K α satelite line of Al V is observed with crystal spectrograph, which indicates the existence of Al 4+ in the plasma

  2. Asymptotic matching of the solar-system gravitational yields

    International Nuclear Information System (INIS)

    Kopejkin, S.M.

    1989-01-01

    In the framework of the general relativity, the structure of the Solar-system gravitational fields is investigated and the relativistic formulae of transformation between nonrotating in the dynamical sense harmonic reference systems - barycentric, planetocentric and topocentric (satelite) ones - are derived by the method of the asymptotic mathing of components of the metric tensor. The derived formulae generalize the linear Poincare transformation in the case of curved space-time. With the help of the asymptotic matching formulae, the relationships between relativistic time scales inside the Solar system have been established, the equations of relativistic precession of the space axis of one reference system with respect to another one have been derived, the equations of translational motion of the center-of-mass of planets (the Sun) and their satellites have been obtained

  3. Behavior of ruthenium, cesium and antimony in high temperature processes for waste conditioning

    International Nuclear Information System (INIS)

    Klein, M.; Weyers, C.; Goossens, W.R.A.

    1985-01-01

    The fission products and the actinides of high level radioactive liquid wastes can be immobilized by incorporation into a glass matrix prior to disposal. The behaviour of so-called semi-volatile products during the vitrification process has been studied by the C.E.N./S.C.K. in Mol since 1979 in the framework of a contract with DWK of Germany in support to the HAW technological program PAMELA. The experiments were performed on laboratory and semi-pilot scale using simulated LEWC solutions tagged with radioisotopes of three suspected volatile fission products, namely ruthenium, cesium and antimony. The releases of these semi-volatile compounds to the off-gases have been investigated for a liquid fed melter as a function of the operational conditions. The study of a wet purification system, comprising in series of a dust scrubber, a condensor, an ejector venturi and an NOsub(x) column, has shown that cesium appears to be the reference isotope for the volatile elements released from the melter. Ruthenium seems not to be a problem from the point of view of gas purification although local radiation problems caused by deposits on metal surfaces cannot be excluded. (Auth.)

  4. Data acquisition. GRAAL experiment. Hybrid reactor experiment. AMS experiment

    International Nuclear Information System (INIS)

    Barancourt, D.; Barbier, G.; Bosson, G.; Bouvier, J.; Gallin-Martel, L.; Meillon, B.; Stassi, P.; Tournier, M.

    1997-01-01

    The main activity of the data acquisition team has consisted in hardware and software developments for the GRAAL experiment with the trigger board, for the 'Reacteurs Hybrides' group with an acquisition board ADCVME8V and for the AMS experiment with the monitoring of the aerogel detector. (authors)

  5. From superWIMPs to decaying dark matter. Models, bounds and indirect searches

    International Nuclear Information System (INIS)

    Weniger, Christoph

    2010-06-01

    Despite lots of observational and theoretical efforts, the particle nature of dark matter remains unknown. Beyond the paradigmatic WIMPs (Weakly Interacting Massive Particles), many theoretically well motivated models exist where dark matter interacts much more weakly than electroweak with Standard Model particles. In this case new phenomena occur, like the decay of dark matter or the interference with the standard cosmology of the early Universe. In this thesis we study some of these aspects of superweakly coupled dark matter in general, and in the special case of hidden U(1) X gauginos that kinetically mix with hypercharge. There, we will assume that the gauge group remains unbroken, similar to the Standard Model U(1) em . We study different kinds of cosmological bounds, including bounds from thermal overproduction, from primordial nucleosynthesis and from structure formation. Furthermore, we study the possible cosmic-ray signatures predicted by this scenario, with emphasis on the electron and positron channel in light of the recent observations by PAMELA and Fermi LAT. Moreover we study the cosmic-ray signatures of decaying dark matter independently of concrete particle-physics models. In particular we analyze in how far the rise in the positron fraction above 10 GeV, as observed by PAMELA, can be explained by dark matter decay. Lastly, we concentrate on related predictions for gamma-ray observations with the Fermi LAT, and propose to use the dipole-like anisotropy of the prompt gamma-ray dark matter signal to distinguish exotic dark matter contributions from the extragalactic gamma-ray background. (orig.)

  6. From superWIMPs to decaying dark matter. Models, bounds and indirect searches

    Energy Technology Data Exchange (ETDEWEB)

    Weniger, Christoph

    2010-06-15

    Despite lots of observational and theoretical efforts, the particle nature of dark matter remains unknown. Beyond the paradigmatic WIMPs (Weakly Interacting Massive Particles), many theoretically well motivated models exist where dark matter interacts much more weakly than electroweak with Standard Model particles. In this case new phenomena occur, like the decay of dark matter or the interference with the standard cosmology of the early Universe. In this thesis we study some of these aspects of superweakly coupled dark matter in general, and in the special case of hidden U(1){sub X} gauginos that kinetically mix with hypercharge. There, we will assume that the gauge group remains unbroken, similar to the Standard Model U(1){sub em}. We study different kinds of cosmological bounds, including bounds from thermal overproduction, from primordial nucleosynthesis and from structure formation. Furthermore, we study the possible cosmic-ray signatures predicted by this scenario, with emphasis on the electron and positron channel in light of the recent observations by PAMELA and Fermi LAT. Moreover we study the cosmic-ray signatures of decaying dark matter independently of concrete particle-physics models. In particular we analyze in how far the rise in the positron fraction above 10 GeV, as observed by PAMELA, can be explained by dark matter decay. Lastly, we concentrate on related predictions for gamma-ray observations with the Fermi LAT, and propose to use the dipole-like anisotropy of the prompt gamma-ray dark matter signal to distinguish exotic dark matter contributions from the extragalactic gamma-ray background. (orig.)

  7. Modulation of Galactic Cosmic Rays in the Inner Heliosphere, Comparing with PAMELA Measurements

    Science.gov (United States)

    Qin, G.; Shen, Z.-N.

    2017-09-01

    We develop a numerical model to study the time-dependent modulation of galactic cosmic rays in the inner heliosphere. In the model, a time-delayed modified Parker heliospheric magnetic field (HMF) and a new diffusion coefficient model, NLGCE-F, from Qin & Zhang, are adopted. In addition, the latitudinal dependence of magnetic turbulence magnitude is assumed to be ˜ (1+{\\sin }2θ )/2 from the observations of Ulysses, and the radial dependence is assumed to be ˜ {r}S, where we choose an expression of S as a function of the heliospheric current sheet tilt angle. We show that the analytical expression used to describe the spatial variation of HMF turbulence magnitude agrees well with the Ulysses, Voyager 1, and Voyager 2 observations. By numerically calculating the modulation code, we get the proton energy spectra as a function of time during the recent solar minimum, it is shown that the modulation results are consistent with the Payload for Antimatter-Matter Exploration and Light-nuclei Astrophysics measurements.

  8. A hadronic explanation of the lepton anomaly

    DEFF Research Database (Denmark)

    Mertsch, Philipp; Sarkar, Subir

    2014-01-01

    The rise in the positron fraction, observed by PAMELA, Fermi-LAT and most recently by AMS-02, has created a lot of interest, fuelled by speculations about an origin in dark matter annihilation in the Galactic halo. However, other channels, e.g. antiprotons or gamma-rays, now severely constrain dark....... This mechanism is guaranteed if hadronic CRs are present and would also lead to observable signatures in other secondary channels like the boron-to-carbon or antiproton-to-proton ratios. If such features were borne out by upcoming AMS-02 data, this would rule out other explanations....

  9. The solidification of high-level liquid wastes in glass and ceramics

    International Nuclear Information System (INIS)

    Krause, H.

    1989-01-01

    In spent nuclear fuel reprocessing a highly radioactive waste solution is produced. It must be converted into a solid product, which binds the radionuclides, be hydrolytic as well as radiation and temperature resistant. Borosilicate glasses fulfil these requirements and, jointly with the barriers of a repository, they prevent inadmissible amounts of radionuclides from escaping into the biocycle. Two techniques were developed for industrial-scale vitrification: a rotary kiln calciner combined with an induction heated metallic melter and the electrode heated ceramic melters. Both techniques were already demonstrated on an industrial scale and under radioactive conditions. (AVM, Marcoule and PAMELA, Mol). (orig./MM) [de

  10. KSC-04PD-2221

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. An exhibit of safety glasses, gloves and protective covers is one of many displayed at KSC during Spaceport Super Safety and Health Day. The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  11. KSC-04PD-2213

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Guest speaker Dr. Pamela Peeke talks to KSC employees during opening ceremonies for Spaceport Super Safety and Health Day at KSC. Other speakers included Navy Com. Stephen E. Iwanowicz , NASAs Dr. Kristine Calderon and Olympic- great Bruce Jenner. Later in the day, employees could visit many vendors exhibits featuring safety and health items. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  12. KSC-04PD-2223

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Astronaut Mark Polansky (left) visits the Life Sciences Lab at KSC where a demonstration of equipment is underway during Spaceport Super Safety and Health Day. . The event included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  13. KSC-04PD-2214

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Olympic champion and motivational speaker Bruce Jenner talks to KSC employees during opening ceremonies for Spaceport Super Safety and Health Day at KSC. Other speakers included Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz and NASAs Dr. Kristine Calderon. Later in the day, employees could visit many vendors exhibits featuring safety and health items. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  14. KSC-04PD-2210

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Center Director Jim Kennedy kicks off Spaceport Super Safety and Health Day with opening ceremonies at the KSC Training Auditorium. Guest speakers included Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Later in the day, employees could visit many vendors exhibits featuring safety and health items. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  15. Dark matter model with non-Abelian gauge symmetry

    International Nuclear Information System (INIS)

    Zhang Hao; Li Chongsheng; Cao Qinghong; Li Zhao

    2010-01-01

    We propose a dark-matter model in which the dark sector is gauged under a new SU(2) group. The dark sector consists of SU(2) dark gauge fields, two triplet dark Higgs fields, and two dark fermion doublets (dark-matter candidates in this model). The dark sector interacts with the standard model sector through kinetic and mass mixing operators. The model explains both PAMELA and Fermi LAT data very well and also satisfies constraints from both the dark-matter relic density and standard model precision observables. The phenomenology of the model at the LHC is also explored.

  16. BiDil: from another vantage point.

    Science.gov (United States)

    Puckrein, Gary

    2006-01-01

    In a recent Health Affairs Web Exclusive, Pamela Sankar and Jonathan Kahn argue against the Food and Drug Administration's approval of BiDil as a new drug for the treatment of heart failure in African Americans. Their paper questions the existence of disparities between African American and other heart-failure patients and the motivations of BiDil's developers and manufacturer. The disparities are confirmed and persistent, however, and BiDil's effectiveness is proven. If the authors' logic were to prevail, patients would be denied life-saving therapy. Continued investigation will likely narrow identification of patients who will benefit.

  17. Los talleres de educación de la sexualidad y la afectividad en los adolescentes como medio de prevención del abuso sexual. (Una propuesta metodológica y teórica

    Directory of Open Access Journals (Sweden)

    Margarita Murillo-Gamboa

    2004-12-01

    Full Text Available Based on the contributions made by Erich Fromm, in regards to the concept of “having and being”, the author proposes the development of a workshop aimed at preventing sexual abuse of adolescents. In this way, she tries to attract youngsters more into the attitude of “being” rather than into that of “having”. Likewise, the participants' concept of sexuality before and after the workshop is discussed. This article is completed whit the supplement (“My sexuality” written by psychologist Pamela Delgado, and addressed to fourth, fifth and sixth graders. It complements the magazine you are reading.

  18. The white dwarf mass-radius relation with Gaia, Hubble and FUSE

    Science.gov (United States)

    Joyce, Simon R. G.; Barstow, Martin A.; Casewell, Sarah L.; Holberg, Jay B.; Bond, Howard E.

    2018-04-01

    White dwarfs are becoming useful tools for many areas of astronomy. They can be used as accurate chronometers over Gyr timescales. They are also clues to the history of star formation in our galaxy. Many of these studies require accurate estimates of the mass of the white dwarf. The theoretical mass-radius relation is often invoked to provide these mass estimates. While the theoretical mass-radius relation is well developed, observational tests of this relation show a much larger scatter in the results than expected. High precision observational tests to confirm this relation are required. Gaia is providing distance measurements which will remove one of the main source of uncertainty affecting most previous observations. We combine Gaia distances with spectra from the Hubble and FUSE satelites to make precise tests of the white dwarf mass-radius relation.

  19. Modelo matemático Two-echelon Capacitated Vehicle Routing Problem para a logística de distribuição de encomendas

    Directory of Open Access Journals (Sweden)

    Karina Pedrini Fraga

    2016-12-01

    Full Text Available Many cities are facing difficulties in urban mobility and therefore are imposing restrictions on the movement of larger trucks. Thus, logistics companies developed a two level logistics strategy based on Urban Distribution Centers (CDU that receives larger trucks and split the cargo to put in small trucks to distribute to customers. To support this type of logistics planning, this paper presents an adaptation of a mathematical model based on the Two-echelon capacitated Vehicle Routing Problem (2E-CVRP to plan the routes from the central depot to the satelites and from these to the clients. The model was applied to the logistics of Correios in the metropolitan area of the Espírito Santo, Brazil, and instances with up to 4 CDU and 25 clients were tested using CPLEX solver 12.6 obtaining routes for deliveries at both levels.

  20. LA DEGRADACIÓN DE TIERRAS MEDIANTE ANÁLISIS FISIOGRÁFICO Y LA APLICACIÓN DE TÉCNICAS DE TELEDETECCIÓN EN LA CUENCA DEL RÍO GUAÑACOS, Resumen DEPARTAMENTO MINAS, NEUQUÉN

    Directory of Open Access Journals (Sweden)

    Ana Paula Salcedo

    2010-12-01

    Full Text Available Este estudio evalúa el estado de degradación en un sector sur del Departamento Minas, Provincia del Neuquén, correspondiente al valle y las planicies circundantes del río Guañacos. El análisis central se realiza mediante la utilización de técnicas de teledetección en el Sistema de Información Geográfica (SIG IDRISI 32, aplicando índices y algoritmos de vegetación específicos sobre imágenes del satélite Landsat 7. Además, se ha realizado un exhaustivo trabajo de campo relevando los indicadores de degradación con el objetivo de profundizar la clasificación e interpretación del medio natural y cotejar los resultados del análisis satelital.

  1. The Experiment Factory: standardizing behavioral experiments

    Directory of Open Access Journals (Sweden)

    Vanessa V Sochat

    2016-04-01

    Full Text Available The administration of behavioral and experimental paradigms for psychology research is hindered by lack of a coordinated effort to develop and deploy standardized paradigms. While several frameworks (de Leeuw (2015; McDonnell et al. (2012; Mason and Suri (2011; Lange et al. (2015 have provided infrastructure and methods for individual research groups to develop paradigms, missing is a coordinated effort to develop paradigms linked with a system to easily deploy them. This disorganization leads to redundancy in development, divergent implementations of conceptually identical tasks, disorganized and error-prone code lacking documentation, and difficulty in replication. The ongoing reproducibility crisis in psychology and neuroscience research (Baker (2015; Open Science Collaboration (2015 highlights the urgency of this challenge: reproducible research in behavioral psychology is conditional on deployment of equivalent experiments. A large, accessible repository of experiments for researchers to develop collaboratively is most efficiently accomplished through an open source framework. Here we present the Experiment Factory, an open source framework for the development and deployment of web-based experiments. The modular infrastructure includes experiments, virtual machines for local or cloud deployment, and an application to drive these components and provide developers with functions and tools for further extension. We release this infrastructure with a deployment (http://www.expfactory.org that researchers are currently using to run a set of over 80 standardized web-based experiments on Amazon Mechanical Turk. By providing open source tools for both deployment and development, this novel infrastructure holds promise to bring reproducibility to the administration of experiments, and accelerate scientific progress by providing a shared community resource of psychological paradigms.

  2. A fussy revisitation of antiprotons as a tool for Dark Matter searches

    International Nuclear Information System (INIS)

    Boudaud, Mathieu; Salati, Pierre; Cirelli, Marco; Giesen, Gaëlle

    2015-01-01

    Antiprotons are regarded as a powerful probe for Dark Matter (DM) indirect detection and indeed current data from PAMELA have been shown to lead to stringent constraints. However, in order to exploit their constraining/discovery power properly and especially in anticipation of the exquisite accuracy of upcoming data from AMS-02, great attention must be put into effects (linked to their propagation in the Galaxy) which may be perceived as subleading but actually prove to be quite relevant. Using a semi-analytic code for rapidity, we revisit the computation of the astrophysical background and of the DM antiproton fluxes. Like in the fully numerical standard calculations, we include the effects of: diffusive reacceleration, energy losses including tertiary component and solar modulation (in a force field approximation). We show that their inclusion can somewhat modify the current bounds, even at large DM masses, and that a wrong interpretation of the data may arise if they are not taken into account. At the present level of accuracy of the data from PAMELA, the inclusion of the above effects amounts to changing the constraints, with respect to the case in which they are neglected, of up to about 40% at a DM mass of 1 TeV and 30% at 10 TeV . When the AMS-02 level of precision is reached, including them would strengthen (lessen) the bounds on the annihilation cross section by up to a factor of 15 below (above) a DM mass of 300 GeV. The numerical results for the astrophysical background are provided in terms of fit functions; the results for Dark Matter are incorporated in the new release of the PPPC4DMID

  3. A fussy revisitation of antiprotons as a tool for Dark Matter searches

    Energy Technology Data Exchange (ETDEWEB)

    Boudaud, Mathieu; Salati, Pierre [LAPTh, Université Savoie Mont Blanc, CNRS, BP 110, 74941 Annecy-le-Vieux (France); Cirelli, Marco; Giesen, Gaëlle, E-mail: mathieu.boudaud@lapth.cnrs.fr, E-mail: marco.cirelli@cea.fr, E-mail: gaelle.giesen@cea.fr, E-mail: pierre.salati@lapth.cnrs.fr [Institut de Physique Théorique, CNRS, URA 2306 and CEA/Saclay, F-91191 Gif-sur-Yvette (France)

    2015-05-01

    Antiprotons are regarded as a powerful probe for Dark Matter (DM) indirect detection and indeed current data from PAMELA have been shown to lead to stringent constraints. However, in order to exploit their constraining/discovery power properly and especially in anticipation of the exquisite accuracy of upcoming data from AMS-02, great attention must be put into effects (linked to their propagation in the Galaxy) which may be perceived as subleading but actually prove to be quite relevant. Using a semi-analytic code for rapidity, we revisit the computation of the astrophysical background and of the DM antiproton fluxes. Like in the fully numerical standard calculations, we include the effects of: diffusive reacceleration, energy losses including tertiary component and solar modulation (in a force field approximation). We show that their inclusion can somewhat modify the current bounds, even at large DM masses, and that a wrong interpretation of the data may arise if they are not taken into account. At the present level of accuracy of the data from PAMELA, the inclusion of the above effects amounts to changing the constraints, with respect to the case in which they are neglected, of up to about 40% at a DM mass of 1 TeV and 30% at 10 TeV . When the AMS-02 level of precision is reached, including them would strengthen (lessen) the bounds on the annihilation cross section by up to a factor of 15 below (above) a DM mass of 300 GeV. The numerical results for the astrophysical background are provided in terms of fit functions; the results for Dark Matter are incorporated in the new release of the PPPC4DMID.

  4. Bounds on Cross-sections and Lifetimes for Dark Matter Annihilation and Decay into Charged Leptons from Gamma-ray Observations of Dwarf Galaxies

    Energy Technology Data Exchange (ETDEWEB)

    Essig, Rouven; /SLAC; Sehgal, Neelima; Strigari, Louis E.; /KIPAC, Menlo Park

    2009-06-19

    We provide conservative bounds on the dark matter cross-section and lifetime from final state radiation produced by annihilation or decay into charged leptons, either directly or via an intermediate particle {phi}. Our analysis utilizes the experimental gamma-ray flux upper limits from four Milky Way dwarf satellites: HESS observations of Sagittarius and VERITAS observations of Draco, Ursa Minor, and Willman 1. Using 90% confidence level lower limits on the integrals over the dark matter distributions, we find that these constraints are largely unable to rule out dark matter annihilations or decays as an explanation of the PAMELA and ATIC/PPB-BETS excesses. However, if there is an additional Sommerfeld enhancement in dwarfs, which have a velocity dispersion {approx} 10 to 20 times lower than that of the local Galactic halo, then the cross-sections for dark matter annihilating through {phi}'s required to explain the excesses are very close to the cross-section upper bounds from Willman 1. Dark matter annihilation directly into {tau}'s is also marginally ruled out by Willman 1 as an explanation of the excesses, and the required cross-section is only a factor of a few below the upper bound from Draco. Finally, we make predictions for the gamma-ray flux expected from the dwarf galaxy Segue 1 for the Fermi Gamma-ray Space Telescope. We find that for a sizeable fraction of the parameter space in which dark matter annihilation into charged leptons explains the PAMELA excess, Fermi has good prospects for detecting a gamma-ray signal from Segue 1 after one year of observation.

  5. Pengaruh Jumlah Kelas dan Skema Klasifikasi terhadap Akurasi Informasi Penggunaan Lahan Hasil Klasifikasi Berbasis Objek dengan Teknik Support Vector Machine di Sebagian Kabupaten Kebumen Provinsi Jawa Tengah

    Directory of Open Access Journals (Sweden)

    Aria Jaka Dwiputra

    2016-10-01

    Full Text Available Produksi peta penggunaan lahan dari data geospasial satelit harus memperhatikan resolusi spasial yang digunakan, dengan menggunakan ilmu penginderaan jauh secara digital akurasi informasi geospasial tematik yang diperoleh dari data geospasial satelit dapat diukur secara kuantitatif. Jumlah kelas penggunaan lahan, skema klasifikasi, dan teknik ekstraksi informasi akan berpengaruh dalam overall accuracy.Penelitian ini menggunakan tiga variasi jumlah kelas dan skema klasifikasi yaitu 4, 7, dan 10 kelas penggunaan lahan. Tiga variasi tersebut diekstraksi dari citra ALOS AVNIR – 2 dengan resolusi 10 meter menggunakan metode klasifikasi berbasis objek dengan pendekatan support vector machine. Sesuatu yang lain dari klasifikasi berbasis objek adalah proses segmentasi yang mengelompokkan objek tutupan lahan dalam satu bagian, dan algoritma SVM mengklasifikasikan citra segmentasi dengan memanfaatkan empat tipe kernel yaitu linier, radial basis function, sigmoid, dan polynomial. Hasil ekstraksi informasi penggunaan lahan untuk jumlah kelas empat menggunakan klasifikasi berbasis objek dengan pendekatan support vector machine memiliki akurasi sebesar 87.2666% serta nilai koefesien kappa 0.8048 dan tipe kernel yang dipakai adalah kernel Linier. Hasil ekstraksi informasi penggunaan lahan untuk jumlah kelas tujuh menggunakan klasifikasi berbasis objek dengan pendekatan support vector machine memiliki akurasi sebesar 79.8021% serta nilai koefesien kappa 0.7293 dan tipe kernel yang dipakai adalah kernel Linier. Hasil ekstraksi informasi penggunaan lahan untuk jumlah kelas sepuluh menggunakan klasifikasi berbasis objek dengan pendekatan support vector machine memiliki akurasi sebesar 73.3377% serta nilai koefesien kappa 0.6466 dan tipe kernel yang dipakai adalah kernel Linier. Hasil ekstraksi informasi penggunaan lahan untuk jumlah kelas sepuluh menggunakan klasifikasi berbasis objek dengan pendekatan support vector machine dan ditambah dengan data bantu berupa

  6. Teledetección satelital cuantitativa para estimar el área basal del bosque de Nothofagus pumilio (Nothofagaceae: El rol del índice de área foliar como información auxiliar Quantitative remote sensing to estimate basal area in Nothofagus pumilio (Nothofagaceae forest: The role of leaf area index as ancillary information

    Directory of Open Access Journals (Sweden)

    GASTÓN M DÍAZ

    2011-12-01

    Full Text Available Los bosques de lenga (Nothofagus pumilio son el recurso forestal más importante de la región andino patagónica argentina, sin embargo, para implementar planes de manejo en pos de prevenir o revertir su degradación es necesario disponer de mayor información sobre su estructura. Una alternativa para obtener esa información es relacionar datos satelitales con las características del bosque a través de modelos físicos y estadísticos. Pero, ¿cuál es el método más eficaz? El índice de área foliar (IAF se encuentra relacionado con la reflectividad del dosel vegetal a través del modelo de transferencia radiativa PROSAIL, lo que permite desarrollar técnicas de teledetección satelital para estimar el IAF con bases físicas, en vez de con modelos estadísticos. De ese modo se puede aprovechar la relación empírico-biológica existente entre el IAF y la estructura del bosque para estimar el área basal. El objetivo principal fue comparar la exactitud de tres métodos para estimar el área basal de la lenga con datos SPOT-5. Los métodos comparados fueron: estadístico directo (ED, estadístico de dos pasos (E2P y físico-estadístico de dos pasos (FE2P. La exactitud fue evaluada con 24 parcelas no involucradas en el ajuste o calibración de los modelos. No se hallaron diferencias significativas en la exactitud de la alternativa físico-estadística en comparación con las netamente estadísticas. Sin embargo, en base al análisis conjunto de los resultados y lo reportado por otros investigadores, se concluye que la ventaja de utilizar modelos físicos radica en la mayor robustez de la estimación y no en la mayor exactitud.Lenga forests (Nothofagus pumilio are the most important forest resource of the Argentinean Andean Patagonia, however, more information about their structure is needed to implement forest management policies and practices in order to prevent their degradation and revert it. One option to obtain this kind of information

  7. Customer experience

    OpenAIRE

    Koperdáková, Zuzana

    2016-01-01

    Bachelor thesis deals with the theme of customer experience and terms related to this topic. The thesis consists of three parts. The first part explains the terms generally, as the experience or customer loyalty. The second part is dedicated to medotology used for Customer Experience Management. In the third part is described application of Customer Experience Management in practice, particularly in the context Touch Point Analyses in GE Money Bank.

  8. Effect of Electrodynamic Forces on the Attitude Stabilization of a Satellite in Ecliptic orbits

    Science.gov (United States)

    Abdel-Aziz, Yehia

    This work is based on the previous paper of the author [1]. The present paper is devoted to the investigation of the attitude dynamics of an ecliptic satellite moving in the magnetic field of the Earth. Eelectrodynamic forces result from the motion of a charged satelite relative to the magnetic field of the Earth. The torque due to electrodynamic effect of the Lorentz forces on the attitude stabilization of the satellite is studied with the detailed model of the Earth's magnetic field. A method for estimating the stable and unstable regions of the equilibrium positions based on Euler's equation is also discussed. The results show that Lorentz forces can affect the stablization of the satellite, in particular for highly eccentric orbits and also for large satellte. [1] Abdel-Aziz, Y. A. Attitude Stabilization of a Rigid Spacecraft in the Geomagnetic Field. AdSpR 40, 18-24, 2007.

  9. Líneas ciclo trónicas en el espectro de rayos y pulsado

    Directory of Open Access Journals (Sweden)

    Jorge Paez

    2016-03-01

    Full Text Available If the magnetic Bremsstrahlung process is responsable for the lines observes in the spectra of two y-ray bursts, GB880205 and GB870303 detected by the spectrometer of the GINGA satelite, then the fundamental and primary harmonics (transition between the excited Landau levels N=2,1 to the ground-state N´=0 may be identified as the cause of those features detected in those y-ray bursts. We use the transition rate for this process in order to prove our asseveration. We suppose that this process is occurring under the presence of an external magnetic field of order 2*10 12 Gauss. The numerical results for the energy average of the emitted photons are: 22.41 Kev and 43.86 Kev. These energies correspond to the fundamental and primary harmonics transition respectively. Subjet headings: y-rays- magnetic fields- radiation mechanisms.

  10. PROPUESTA INICIAL PARA EL DESARROLLO DE UNA METODOLOGÍA PARA LA IMPLEMENTACIÓN DE IPTv6 SOBRE IMS

    Directory of Open Access Journals (Sweden)

    Jean Paul Granados Cárdenas

    2013-09-01

    Full Text Available La televisión digital ha evolucionado continuamente desde su presentación digital terrestre (DVB-T, pasando por el estándar satelital (DVB-S hasta llegar a su presentación actual conocida como IPTV (Internet Protocolo Television que ofrece múltiples servicios multimedia tales como voz, video y datos, transportados con ciertos niveles de calidad de servicio, seguridad, interactividad y confianza gracias a la utilización de la pila de protocolos TCP/IP. En tal sentido el artículo pone a disposición de la comunidad académica una propuesta  metodológica inicial que pretende servir de guía en la implementación de este tipo de sistemas sobre una plataforma de libre distribución conocida como IMS (IP Multimedia Subsystem para redes de área local tipo IPv6.

  11. Fermi LAT Search for Dark Matter in Gamma-Ray Lines and the Inclusive Photon Spectrum

    Science.gov (United States)

    Ackermann, M.; Ajello, M.; Albert, A.; Baldini, L.; Barbiellini, G.; Bechtol, K.; Bellazzini, R.; Berenji, B.; Blandford, R. D.; Bloom, E. D.; hide

    2012-01-01

    Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.

  12. A New Type of Accelerator for Charged Particle Cancer Therapy

    CERN Document Server

    Edgecock, Rob

    2013-01-01

    acceleration of protons and light ions for the treatment of certain cancers. They have unique features as they combine techniques from the existing types of accelerators, cyclotrons and synchrotrons, and hence look to have advantages over both for this application. However, these unique features meant that it was necessary to build one of these accelerators to show that it works and to undertake a detailed conceptual design of a medical machine. Both of these have now been done. This paper will describe the concepts of this type of accelerator, show results from the proof-of-principle machine (EMMA) and described the medical machine (PAMELA).

  13. Gamma ray constraints on decaying dark matter

    DEFF Research Database (Denmark)

    Cirelli, M.; Moulin, E.; Panci, P.

    2012-01-01

    We derive new bounds on decaying dark matter from the gamma ray measurements of (i) the isotropic residual (extragalactic) background by Fermi and (ii) the Fornax galaxy cluster by H.E.S.S. We find that those from (i) are among the most stringent constraints currently available, for a large range...... of dark matter masses and a variety of decay modes, excluding half-lives up to similar to 10(26) to few 10(27) seconds. In particular, they rule out the interpretation in terms of decaying dark matter of the e(+/-) spectral features in PAMELA, Fermi and H.E.S.S., unless very conservative choices...

  14. Dark matter through the axion portal

    International Nuclear Information System (INIS)

    Nomura, Yasunori; Thaler, Jesse

    2009-01-01

    Motivated by the galactic positron excess seen by PAMELA and ATIC/PPB-BETS, we propose that dark matter is a TeV-scale particle that annihilates into a pseudoscalar 'axion'. The positron excess and the absence of an antiproton or gamma ray excess constrain the axion mass and branching ratios. In the simplest realization, the axion is associated with a Peccei-Quinn symmetry, in which case it has a mass around 360-800 MeV and decays into muons. We present a simple and predictive supersymmetric model implementing this scenario, where both the Higgsino and dark matter obtain masses from the same source of TeV-scale spontaneous symmetry breaking.

  15. KSC-04PD-2211

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. During opening ceremonies for Spaceport Super Safety and Health Day at KSC, members of the astronaut corps and KSC employees enjoy the humor of guest speaker Dr. Pamela Peeke. Other speakers included Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic- great Bruce Jenner. Later in the day, employees could visit many vendors exhibits featuring safety and health items. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  16. KSC-04PD-2208

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Employees at KSC take time to look at safety equipment on display during Spaceport Super Safety and Health Day. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The day-long event also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  17. KSC-04PD-2207

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Inside a tent, employees at KSC look over an exhibit of safety equipment during Spaceport Super Safety and Health Day. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The day-long event also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  18. KSC-04PD-2205

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Inside a tent, employees at KSC look over an exhibit of special equipment during Spaceport Super Safety and Health Day. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The day-long event also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  19. KSC-04PD-2204

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Inside a tent, employees look over an exhibit of safety equipment. The exhibits were part of Spaceport Super Safety and Health Day, which also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The annual event was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  20. KSC-04PD-2212

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Col.David Nuckles, chief of Safety with the 45th Space Wing, talks to guests and employees during opening ceremonies for Spaceport Super Safety and Health Day at KSC. Guest speakers included Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Later in the day, employees could visit many vendors exhibits featuring safety and health items. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  1. KSC-04PD-2203

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Inside a tent, employees look over an exhibit of work shoes. The exhibits were part of Spaceport Super Safety and Health Day, which also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The annual event was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  2. KSC-04PD-2206

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Employees at KSC walk through a tent filled with vendors exhibits during Spaceport Super Safety and Health Day. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The day-long event also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  3. ‘The Life and Times of Uncle Warwick’

    Directory of Open Access Journals (Sweden)

    Helen R. Haines

    2006-11-01

    Full Text Available Recently, I had the privilege of hosting a session in honour of Dr. Warwick Bray at the 71st Annual Meeting of the Society for American Archaeology, in San Juan, Puerto Rico. The following is a forward to Pamela J. Smith’s interview which introduces the reader to this wonderfully modest and endearingly understated man. His modest nature is exemplified in the title for my introduction which comes from a letter Warwick sent me in response to my request for his curriculum vitae – a document he humourously paralleled to children’s book ‘The Life and Times of Uncle Wiggley’.

  4. Simulator experiments: effects of NPP operator experience on performance

    International Nuclear Information System (INIS)

    Beare, A.N.; Gray, L.H.

    1984-01-01

    During the FY83 research, a simulator experiment was conducted at the control room simulator for a GE Boiling Water Reactor (BWR) NPP. The research subjects were licensed operators undergoing requalification training and shift technical advisors (STAs). This experiment was designed to investigate the effects of senior reactor operator (SRO) experience, operating crew augmentation with an STA and practice, as a crew, upon crew and individual operator performance, in response to anticipated plant transients. Sixteen two-man crews of licensed operators were employed in a 2 x 2 factorial design. The SROs leading the crews were split into high and low experience groups on the basis of their years of experience as an SRO. One half of the high- and low-SRO experience groups were assisted by an STA. The crews responded to four simulated plant casualties. A five-variable set of content-referenced performance measures was derived from task analyses of the procedurally correct responses to the four casualties. System parameters and control manipulations were recorded by the computer controlling the simulator. Data on communications and procedure use were obtained from analysis of videotapes of the exercises. Questionnaires were used to collect subject biographical information and data on subjective workload during each simulated casualty. For four of the five performance measures, no significant differences were found between groups led by high (25 to 114 months) and low (1 to 17 months as an SRO) experience SROs. However, crews led by low experience SROs tended to have significantly shorter task performance times than crews led by high experience SROs. The presence of the STA had no significant effect on overall team performance in responding to the four simulated casualties. The FY84 experiments are a partial replication and extension of the FY83 experiment, but with PWR operators and simulator

  5. Extracting Insights from Experience Designers to Enhance User Experience Design

    OpenAIRE

    Kremer, Simon; Lindemann, Udo

    2016-01-01

    User Experience (UX) summarizes how a user expects, perceives and assesses an encounter with a product. User Experience Design (UXD) aims at creating meaningful experiences. While UXD is a rather young discipline with-in product development and traditional processes predominate, other disciplines traditionally focus on creating experiences. We engaged with experience de-signers from the fields of arts, movies, sports, music and event management. By analyzing their working processes via interv...

  6. Employing Tropospheric Numerical Weather Prediction Model for High-Precision GNSS Positioning

    Science.gov (United States)

    Alves, Daniele; Gouveia, Tayna; Abreu, Pedro; Magário, Jackes

    2014-05-01

    In the past few years is increasing the necessity of realizing high accuracy positioning. In this sense, the spatial technologies have being widely used. The GNSS (Global Navigation Satellite System) has revolutionized the geodetic positioning activities. Among the existent methods one can emphasize the Precise Point Positioning (PPP) and network-based positioning. But, to get high accuracy employing these methods, mainly in real time, is indispensable to realize the atmospheric modeling (ionosphere and troposphere) accordingly. Related to troposphere, there are the empirical models (for example Saastamoinen and Hopfield). But when highly accuracy results (error of few centimeters) are desired, maybe these models are not appropriated to the Brazilian reality. In order to minimize this limitation arises the NWP (Numerical Weather Prediction) models. In Brazil the CPTEC/INPE (Center for Weather Prediction and Climate Studies / Brazilian Institute for Spatial Researches) provides a regional NWP model, currently used to produce Zenithal Tropospheric Delay (ZTD) predictions (http://satelite.cptec.inpe.br/zenital/). The actual version, called eta15km model, has a spatial resolution of 15 km and temporal resolution of 3 hours. In this paper the main goal is to accomplish experiments and analysis concerning the use of troposphere NWP model (eta15km model) in PPP and network-based positioning. Concerning PPP it was used data from dozens of stations over the Brazilian territory, including Amazon forest. The results obtained with NWP model were compared with Hopfield one. NWP model presented the best results in all experiments. Related to network-based positioning it was used data from GNSS/SP Network in São Paulo State, Brazil. This network presents the best configuration in the country to realize this kind of positioning. Actually the network is composed by twenty stations (http://www.fct.unesp.br/#!/pesquisa/grupos-de-estudo-e-pesquisa/gege//gnss-sp-network2789/). The

  7. Beyond the Standard Model: The Weak Scale, Neutrino Mass, and the Dark Sector

    International Nuclear Information System (INIS)

    Weiner, Neal

    2010-01-01

    The goal of this proposal was to advance theoretical studies into questions of collider physics at the weak scale, models and signals of dark matter, and connections between neutrino mass and dark energy. The project was a significant success, with a number of developments well beyond what could have been anticipated at the outset. A total of 35 published papers and preprints were produced, with new ideas and signals for LHC physics and dark matter experiments, in particular. A number of new ideas have been found on the possible indirect signals of models of dark matter which relate to the INTEGRAL signal of astrophysical positron production, high energy positrons seen at PAMELA and Fermi, studies into anomalous gamma rays at Fermi, collider signatures of sneutrino dark matter, scenarios of Higgs physics arising in SUSY models, the implications of galaxy cluster surveys for photon-axion conversion models, previously unconsidered collider phenomenology in the form of 'lepton jets' and a very significant result for flavor physics in supersymmetric theories. Progress continues on all fronts, including development of models with dramatic implications for direct dark matter searches, dynamics of dark matter with various excited states, flavor physics, and consequences of modified missing energy signals for collider searches at the LHC.

  8. Cosmic ray modulation and radiation dose of aircrews during the solar cycle 24/25

    Science.gov (United States)

    Miyake, Shoko; Kataoka, Ryuho; Sato, Tatsuhiko

    2017-04-01

    Weak solar activity and high cosmic ray flux during the coming solar cycle are qualitatively anticipated by the recent observations that show the decline in the solar activity levels. We predict the cosmic ray modulation and resultant radiation exposure at flight altitude by using the time-dependent and three-dimensional model of the cosmic ray modulation. Our galactic cosmic ray (GCR) model is based on the variations of the solar wind speed, the strength of the heliospheric magnetic field, and the tilt angle of the heliospheric current sheet. We reproduce the 22 year variation of the cosmic ray modulation from 1980 to 2015 taking into account the gradient-curvature drift motion of GCRs. The energy spectra of GCR protons obtained by our model show good agreement with the observations by the Balloon-borne Experiment with a Superconducting magnetic rigidity Spectrometer (BESS) and the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) except for a discrepancy at the solar maximum. Five-year annual radiation dose around the solar minimum at the solar cycle 24/25 will be approximately 19% higher than that in the last cycle. This is caused by the charge sign dependence of the cosmic ray modulation, such as the flattop profiles in a positive polarity.

  9. NEW EVIDENCE FOR CHARGE-SIGN-DEPENDENT MODULATION DURING THE SOLAR MINIMUM OF 2006 TO 2009

    Energy Technology Data Exchange (ETDEWEB)

    Di Felice, V. [INFN, Sezione di Roma “Tor Vergata,” I-00133 Rome (Italy); Munini, R. [INFN, Sezione di Trieste, I-34149 Trieste (Italy); Vos, E. E.; Potgieter, M. S. [Centre for Space Research, North-West University, 2520 Potchefstroom (South Africa)

    2017-01-01

    The PAMELA space experiment, in orbit since 2006, has measured cosmic rays (CRs) through the most recent period of minimum solar activity with the magnetic field polarity as A  < 0. During this entire time, galactic electrons and protons have been detected down to 70 MV and 400 MV, respectively, and their differential variation in intensity with time has been monitored with unprecedented accuracy. These observations are used to show how differently electrons and protons responded to the quiet modulation conditions that prevailed from 2006 to 2009. It is well known that particle drifts, as one of four major mechanisms for the solar modulation of CRs, cause charge-sign-dependent solar modulation. Periods of minimum solar activity provide optimal conditions in which to study these drift effects. The observed behavior is compared to the solutions of a three-dimensional model for CRs in the heliosphere, including drifts. The numerical results confirm that the difference in the evolution of electron and proton spectra during the last prolonged solar minimum is attributed to a large extent to particle drifts. We therefore present new evidence of charge-sign-dependent solar modulation, with a perspective on its peculiarities for the observed period from 2006 to 2009.

  10. The experience sampling method: Investigating students' affective experience

    Science.gov (United States)

    Nissen, Jayson M.; Stetzer, MacKenzie R.; Shemwell, Jonathan T.

    2013-01-01

    Improving non-cognitive outcomes such as attitudes, efficacy, and persistence in physics courses is an important goal of physics education. This investigation implemented an in-the-moment surveying technique called the Experience Sampling Method (ESM) [1] to measure students' affective experience in physics. Measurements included: self-efficacy, cognitive efficiency, activation, intrinsic motivation, and affect. Data are presented that show contrasts in students' experiences (e.g., in physics vs. non-physics courses).

  11. Simulator experiments: effects of NPP operator experience on performance

    International Nuclear Information System (INIS)

    Beare, A.N.; Gray, L.H.

    1985-01-01

    Experiments are being conducted on nuclear power plant (NPP) control room training simulators by the Oak Ridge National Laboratory, its subcontractor, General Physics Corporation, and participating utilities. The experiments are sponsored by the Nuclear Regulatory Commission's (NRC) Human Factors and Safeguards Branch, Division of Risk Analysis and Operations, and are a continuation of prior research using simulators, supported by field data collection, to provide a technical basis for NRC human factors regulatory issues concerned with the operational safety of nuclear power plants. During the FY83 research, a simulator experiment was conducted at the control room simulator for a GE boiling water reactor (BWR) NPP. The research subjects were licensed operators undergoing requalification training and shift technical advisors (STAs). This experiment was designed to investigate the effects of (a) senior reactor operator (SRO) experience, (b) operating crew augmentation with an STA and (c) practice, as a crew, upon crew and individual operator performance, in response to anticipated plant transients. The FY84 experiments are a partial replication and extension of the FY83 experiment, but with PWR operators and simulator. Methodology and results to date are reported

  12. Experiment WA1 (CDHS Neutrino Experiment)

    CERN Multimedia

    CERN PhotoLab

    1977-01-01

    Experiment WA1, also known under CDHS (CERN, Dortmund, Heidelberg, Saclay; spokesman Jack Steinberger), was the first neutrino experiment on the SPS, in its West Area. Magnetized iron (with a toroidal field) forms the core of the detector. On its outside we see drift chambers and photomultipliers (detecting the light from the plastic scintillators further in). Peter Schilly is wearing a white coat. See also CERN Annual Report 1976, p.57.

  13. TRIO experiment

    International Nuclear Information System (INIS)

    Clemmer, R.G.; Finn, P.A.; Malecha, R.F.

    1984-09-01

    The TRIO experiment is a test of in-situ tritium recovery and heat transfer performance of a miniaturized solid breeder blanket assembly. The assembly (capsule) was monitored for temperature and neutron flux profiles during irradiation and a sweep gas flowed through the capsule to an anaytical train wherein the amounts of tritium in its various chemical forms were determined. The capsule was designed to operate at different temperatures and sweep gas conditions. At the end of the experiment the amount of tritium retained in the solid was at a concentration of less than 0.1 wppM. More than 99.9% of tritium generated during the experiment was successfully recovered. The results of the experiment showed that the tritium inventories at the beginning and at the end of the experiment follow a relationship which appears to be characteristic of intragranular diffusion

  14. Pixel Experiments

    DEFF Research Database (Denmark)

    Petersen, Kjell Yngve; Søndergaard, Karin; Augustesen, Christina

    2015-01-01

    Pixel Experiments The term pixel is traditionally defined as any of the minute elements that together constitute a larger context or image. A pixel has its own form and is the smallest unit seen within a larger structure. In working with the potentials of LED technology in architectural lighting...... for using LED lighting in lighting design practice. The speculative experiments that have been set-up have aimed to clarify the variables that can be used as parameters in the design of lighting applications; including, for example, the structuring and software control of light. The experiments also...... elucidate and exemplify already well-known problems in relation to the experience of vertical and horizontal lighting. Pixel Experiments exist as a synergy between speculative test setups and lighting design in practice. This book is one of four books that is published in connection with the research...

  15. Pemanfaatan Data ARR (Automatic Rainfall Recorder) untuk Peningkatan Efektifitas Model Hujan Satelit (Studi Kasus DAS Indragiri)

    OpenAIRE

    Hendra, Yuli; Fauzi, Manyuk; Sutikno, Sigit

    2015-01-01

    The availability of data on hydrological modeling always become a problem considering the incompleteness and the imprecision of data. As the development of technology, many models of hidrology using data acquired from the satellite have emerged. The accuracy and the model correlation was still unachieved from the previous research using satellite data. This problems was caused by the unstable weather conditions thus the process of recording and dowloading of the satellite data become less opt...

  16. PEMETAAN SUHU PERMUKAAN LAUT (SPL MENGGUNAKAN CITRA SATELIT ASTER DI PERAIRAN LAUT JAWA BAGIAN BARAT MADURA

    Directory of Open Access Journals (Sweden)

    Dyah Ayu Sulistyo Rini

    2010-10-01

    Full Text Available Oceanographical temperature in Java Sea is very important to be considered. This research was combines in-site observation technique, Geographical Information System (GLS and remote sensing in order to get accurate, present and updateable data. The aim of this research is to determine the distribution of sea-surface temperature and accuration-test value in Java Sea especially on western coast of Madura using ASTER satellite imagery. This research were used software of ENVI 4.5, ILWIS 3.3, and ArcGIS 9.3 and also changed the radian value until °C. Result showed that using ASTER satellite imagery within band 10 range between 32 "C-35 "C. Band 11,between 24.9"C 25,2"C. Band 12 between 16,7"C to 17"C. Band while band 13 abd 14 between 30.7, band 28. Band 11 is more accurate compared to Band 10, 12, 13. 14, the RMS Error on band 11 showed lower value compared to the other band.Keywords: Sea-surface Temperature. ASTER satellite imagery. Java Sea, Western coast of Madura

  17. Use of modeled and satelite soil moisture to estimate soil erosion in central and southern Italy.

    Science.gov (United States)

    Termite, Loris Francesco; Massari, Christian; Todisco, Francesca; Brocca, Luca; Ferro, Vito; Bagarello, Vincenzo; Pampalone, Vincenzo; Wagner, Wolfgang

    2016-04-01

    This study presents an accurate comparison between two different approaches aimed to enhance accuracy of the Universal Soil Loss Equation (USLE) in estimating the soil loss at the single event time scale. Indeed it is well known that including the observed event runoff in the USLE improves its soil loss estimation ability at the event scale. In particular, the USLE-M and USLE-MM models use the observed runoff coefficient to correct the rainfall erosivity factor. In the first case, the soil loss is linearly dependent on rainfall erosivity, in the second case soil loss and erosivity are related by a power law. However, the measurement of the event runoff is not straightforward or, in some cases, possible. For this reason, the first approach used in this study is the use of Soil Moisture For Erosion (SM4E), a recent USLE-derived model in which the event runoff is replaced by the antecedent soil moisture. Three kinds of soil moisture datasets have been separately used: the ERA-Interim/Land reanalysis data of the European Centre for Medium-range Weather Forecasts (ECMWF); satellite retrievals from the European Space Agency - Climate Change Initiative (ESA-CCI); modeled data using a Soil Water Balance Model (SWBM). The second approach is the use of an estimated runoff rather than the observed. Specifically, the Simplified Continuous Rainfall-Runoff Model (SCRRM) is used to derive the runoff estimates. SCRMM requires soil moisture data as input and at this aim the same three soil moisture datasets used for the SM4E have been separately used. All the examined models have been calibrated and tested at the plot scale, using data from the experimental stations for the monitoring of the erosive processes "Masse" (Central Italy) and "Sparacia" (Southern Italy). Climatic data and runoff and soil loss measures at the event time scale are available for the period 2008-2013 at Masse and for the period 2002-2013 at Sparacia. The results show that both the approaches can provide better results than the USLE. Specifically, the SM4E model has proven to be particularly effective at Masse, providing the best soil loss estimations, especially when the modeled soil moisture is used. In this case, the RSR index (ratio between the Root Mean Square Error and the Observed Standard deviation) is equal to 0.94. Instead, the SCRRM is able to better estimate the event runoff at Sparacia than at Masse, thus resulting in good performances of the USLE-derived models using the estimated runoff; however, even at Sparacia the SM4E with modeled soil moisture gives the better soil loss estimates, with RSR = 0.54. These results open an interesting scenario in the use of empirical models to determine soil loss at a large scale, since soil moisture is a not only a simple in situ measurement, but only a widely available information on a global scale from remote sensing.

  18. ARC EMCS Experiments (Seedling Growth-2) Experiment Status

    Science.gov (United States)

    Heathcote, David; Steele, Marianne

    2015-01-01

    Presentation of the status of the ARC ISS (International Space Station) Experiment, Seedling Growth-2 to the Payload Operations Investigator Working Group meeting at MSFC, Huntsville AL. The experiment employs the European Modular Cultivation System (ECMS).

  19. Policy Debate | Ecuador’s Yasuní-ITT Initiative : What Can We Learn from its Failure?

    Directory of Open Access Journals (Sweden)

    Pamela L. Martin

    2014-05-01

    Full Text Available Editor’s note: This paper is a contribution to the ‘Policy Debate’ section of International Development Policy. In this section, academics, policy-makers and practioners engage in a dialogue on global development challenges. Papers are copy-edited but not peer-reviewed. Instead, the initial thematic contribution is followed by critical comments and reactions from scholars and/or policy-makers.In her article ‘Pay to Preserve: The Global Politics of Ecuador’s Yasuní-ITT Proposal’, published in DevPol’s special issue on  Energy and Development in 2011, Pamela L. Martin, Associate Professor of Politics at the Coastal Carolina University in Conway, South Carolina, provided a favourable outlook on Ecuador’s innovative environmental governance mechanism. Accordingly, its unique potential lay in its objective of contributing towards sustainable development and social justice and in case of success, the author even predicted a possible replication in other developing countries. Despite its benefits, the initiative was abandoned in 2013. In this paper, Martin revisits the initiative and analyses the reasons for its failure, namely President Correa’s public pursuit of a Plan B, entering into negotiations with oil firms interested to explore the ITT reserves. Moreover, the initiative was in stark competition with the national REDD+ programme, the mainstream policy approach to reduce emissions from deforestation and forest degradation against payments, which is being negotiated under the United Nations Framework Convention on Climate Change (UNFCCC.Pamela L. Martin’s article is followed by a response by Dr. Imme Scholz, Deputy Director of the German Development Institute/Deutsches Institut für Entwicklungspolitik (DIE. She examines why Germany, as the largest European donor, withdrew its support for the Yasuní-ITT Initiative.Readers who are intetested are invited to contribute to this policy debate on our blog .Download the whole

  20. Constraints on particle dark matter from cosmic-ray antiprotons

    International Nuclear Information System (INIS)

    Fornengo, N.; Vittino, A.; Maccione, L.

    2014-01-01

    Cosmic-ray antiprotons represent an important channel for dark matter indirect-detection studies. Current measurements of the antiproton flux at the top of the atmosphere and theoretical determinations of the secondary antiproton production in the Galaxy are in good agreement, with no manifest deviation which could point to an exotic contribution in this channel. Therefore, antiprotons can be used as a powerful tool for constraining particle dark matter properties. By using the spectrum of PAMELA data from 50 MV to 180 GV in rigidity, we derive bounds on the dark matter annihilation cross section (or decay rate, for decaying dark matter) for the whole spectrum of dark matter annihilation (decay) channels and under different hypotheses of cosmic-rays transport in the Galaxy and in the heliosphere. For typical models of galactic propagation, the constraints are strong, setting a lower bound on the dark matter mass of a ''thermal'' relic at about 40–80 GeV for hadronic annihilation channels. These bounds are enhanced to about 150 GeV on the dark matter mass, when large cosmic-rays confinement volumes in the Galaxy are considered, and are reduced to 3–4 GeV for annihilation to light quarks (no bound for heavy-quark production) when the confinement volume is small. Bounds for dark matter lighter than few tens of GeV are due to the low energy part of the PAMELA spectrum, an energy region where solar modulation is relevant: to this aim, we have implemented a detailed solution of the transport equation in the heliosphere, which allowed us not only to extend bounds to light dark matter, but also to determine the uncertainty on the constraints arising from solar modulation modelling. Finally, we estimate the impact of soon-to-come AMS-02 data on the antiproton constraints

  1. TRACY transient experiment databook. 2) ramp withdrawal experiment

    International Nuclear Information System (INIS)

    Nakajima, Ken; Yamane, Yuichi; Ogawa, Kazuhiko; Aizawa, Eiju; Yanagisawa, Hiroshi; Miyoshi, Yoshinori

    2002-03-01

    This is a databook of TRACY ''ramp withdrawal'' experiments. TRACY is a reactor to perform supercritical experiments using low-enriched uranyl nitrate aqueous solution. The excess reactivity of TRACY is 3$ at maximum, and it is inserted by feeding the solution to a core tank or by withdrawing a control rod, which is called as the transient rod, from the core. In the ramp withdrawal experiment, the supercritical experiment is initiated by withdrawing the transient rod from the core in a constant speed using a motor drive system. The data in the present databook consist of datasheets and graphs. Experimental conditions and typical values of measured parameters are tabulated in the datasheet. In the graph, power and temperature profiles are plotted. Those data are useful for the investigation of criticality accidents with fissile solutions, and for validation of criticality accident analysis codes. (author)

  2. Experiment prediction for Loft Nonnuclear Experiment L1-4

    International Nuclear Information System (INIS)

    White, J.R.; Berta, V.T.; Holmstrom, H.L.O.

    1977-04-01

    A computer analysis, using the WHAM and RELAP4 computer codes, was performed to predict the LOFT system thermal-hydraulic response for Experiment L1-4 of the nonnuclear (isothermal) test series. Experiment L1-4 will simulate a 200 percent double-ended offset shear in the cold leg of a four-loop large pressurized water reactor. A core simulator will be used to provide a reactor vessel pressure drop representative of the LOFT nuclear core. Experiment L1-4 will be initiated with a nominal isothermal primary coolant temperature of 282.2 0 C, a pressurizer pressure of 15.51 MPa, and a primary coolant flow of 270.9 kg/s. In general, the predictions of saturated blowdown for Experiment Ll-4 are consistent with the expected system behavior, and predicted trends agree with results from Semiscale Test S-01-4A, which simulated the Ll-4 experiment conditions

  3. Learning and Experience

    DEFF Research Database (Denmark)

    Olesen, Henning Salling

    2017-01-01

    Abstract: This chapter introduces a psycho-societal approach to theorizing learning, combining a materialist theory of socialization with a hermeneutic interpretation methodology. The term "approach" indicates the intrinsic connection between theory, empirical research process and epistemic subject....... Learning is theorized as dynamic subjective experience of (socially situated) realities, counting on individual subjectivity as well as subjective aspects of social interaction. This psycho-societal theory of subjective experiences conceptualizes individual psychic development as interactional experience...... of societal relations, producing an inner psycho-dynamic as a conscious and unconscious individual resource in future life. The symbolization of immediate sensual experiences form an individual life experience of social integration, language use being the medium of collective, social experience (knowledge...

  4. Albedos and spectral signatures determination and it connection to geological processes: Simile between Earth and other solar system bodies

    Science.gov (United States)

    Suarez, J.; Ochoa, L.; Saavedra, F.

    2017-07-01

    Remote sensing has always been the best investigation tool for planetary sciences. In this research have been used data of Surface albedo, electromagnetic spectra and satelital imagery in search of understanding glacier dynamics in some bodies of the solar system, and how it's related to their compositions and associated geological processes, this methodology is very common in icy moons studies. Through analytic software's some albedos map's and geomorphological analysis were made that allow interpretation of different types of ice in the glacier's and it's interaction with other materials, almost all the images were worked in the visible and infrared ranges of the spectrum; spectral data were later used to connect the reflectance whit chemical and reologic properties of the compounds studied. It have been concluded that the albedo analysis is an effective tool to differentiate materials in the bodies surfaces, but the application of spectral data is necessary to know the exact compounds of the glaciers and to have a better understanding of the icy bodies.

  5. Manual of program operation for data analysis from radiometer system

    International Nuclear Information System (INIS)

    Silva Mello, L.A.R. da; Migliora, C.G.S.

    1987-12-01

    This manual describes how to use the software to retrieve and analyse data from radiometer systems and raingauges used in the 12 GHz PROPAGATION MEASUREMENTS/CANADA - TELEBRAS COOPERATION PROGRAM. The data retrieval and analisys is being carried out by CETUC, as part of the activities of the project Simulacao de Enlaces Satelite (SES). The software for these tasks has been supplied by the Canadian Research Centre (CRC), together with the measurement equipment. The two following sections describe the use of the data retrieval routines and the data analysis routines of program ATTEN. Also, a quick reference guide for commands that can be used when a microcomputer is local or remotely connected to a radiometer indoor unit is included as a last section. A more detailed description of these commands, their objectives and cautions that should de taken when using them can be found in the manual ''12 GHz Propagation Measurements System - Volume 1 - Dual Slope Radiometer and Data Aquisition System'', supplied by Diversitel Communications Inc. (author) [pt

  6. Dinámica metropolitana en México

    Directory of Open Access Journals (Sweden)

    Jorge Isauro Rionda-Ramírez

    2007-01-01

    Full Text Available Actualmente, el crecimiento de las ciudades es tema relevante ante el evidente cambio de patrones tanto en la demografía como en el crecimiento y desarrollo urbanos. Las ciudades medias, la acentuada precarización del campo, el rápido ascenso industrial urbano y la inminente terciarización de las áreas urbanas, la metropolización de las grandes ciudades así como los fenómenos de conurbación, desarrollo satelital y periférico, la desconcentración industrial y, sobre todo, la marginación, son elementos que no deben dejarse de lado en los programas de investigación social del país. El presente trabajo denota el carácter y algunas de las características más sobresalientes de este fenómeno para el caso de México y, en especial, en materia de desarrollo regional.

  7. Method for the determination of spectroradiometric corrections of data from multichannel aerospatial spectrometers

    International Nuclear Information System (INIS)

    Bakalova, K.P.; Bakalov, D.D.

    1984-01-01

    Various factors in the aerospatial conditions of operation may lead to changes in the transmission characteristics of the electron-optical medium or environment of spectrometers for remote sensing of the Earth. Consequently, the data obtained need spectroradiometric corrections. In the paper, a unified approach to the determination of these corrections is suggested. The method uses measurements of standard sources with a smooth emission spectrum that is much wider than the width of the channels, such as a lamp with an incandescent filament, Sun and other natural objects, without special spectral reference standards. The presence of additional information about the character of changes occuring in the measurements may considerably simplify the determination of corrections through setting appropriate values of a coefficient and the spectral shift. The method has been used with the Spectrum-15 and SMP-32 spectrometers on the Salyut-7 orbital station and the 'Meteor-Priroda' satelite of the Bulgaria-1300-ii project

  8. District heating by the Bohunice nuclear power plant

    International Nuclear Information System (INIS)

    Metke, E.; Skvarka, P.

    1984-01-01

    Technical and economical aspects of district heating by the electricity generating nuclear plants in Czechoslovakia are discussed. As a first stage of the project, 240 MW thermal power will be supplied using bleeding lines steam from the B-2 nuclear power plant at Jaslovske Bohunice to heat up water at a central station to 130 grad C. The maximal thermal power that can be produced for district heating by WWER type reactors with regular condensation turbines is estimated to be: 465 MW for a WWER-440 reactor with two 220 MWe turbines and 950 MW for a WWER-1000 reactor with a Skoda made 1000 MWe turbine using a three-stage scheme to heat up water from 60 grad C to 150 grad C. The use of satelite heating turbines connected to the steam collector is expected to improve the efficiency. District heating needs will de taken into account for siting of the new power plants

  9. Electron-nuclear γ transition spectrum of a nucleus in a multicharged atomic ion

    International Nuclear Information System (INIS)

    Ivanov, L.N.; Letokhov, V.S.

    1987-01-01

    The nuclear emission of absorption spectrum of an atom possesses a set of electron satelites which are due to an alternation of the state of the electron shell. It is shown that the mechanism of formation of the satellites might be different for neutral atoms and high-charge ions. In the first case (loose electron shell) a ''shaking'' of the shell resulting from the interaction between the nucleus and γ quantum is predominant. In the second case (rigid electron shell) the mechanism involves a direct interaction between the γ quantum and electrons. The second mechanism is important in the case of dipole nuclear transitions and dominates at γ quantum energies p 2λ (λ is the nuclear transition multipole order, μ p ∼ 1/2 π is the relative proton mass and z the core mass). In the spectrum of the plasma source the electron satellites corresponding to the γ quantum emission and absorption lines are not overlapped by the Doppler contour of the γ line

  10. Morphology of auroral zone radio wave scintillation

    International Nuclear Information System (INIS)

    Rino, C.L.; Matthews, S.J.

    1980-01-01

    This paper describes the morphology of midnight sector and morning sector auroral zone scintillation observations made over a two-year period using the Wideband satelite, which is in a sun-synchronous, low-altitude orbit. No definitive seasonal variation was found. The nighttime data showed the highest scintillation ocurrence levels, but significant amounts of morning scintillation were observed. For the most part the scintillation activity followed the general pattern of local magnetic activity. The most prominent feature in the nightime data is a localized amplitude and phase scintillation enhancement at the point where the propagation vector lies within an L shell. A geometrical effect due to a dynamic slab of sheetlike structures in the F region is hypothesized as the source of his enhancement. The data have been sorted by magnetic activity, proximity to local midnight, and season. The general features of the data are in agreement with the accepted morphology of auroral zone scintillation

  11. TRACY transient experiment databook. 3) Ramp feed experiment

    Energy Technology Data Exchange (ETDEWEB)

    Nakajima, Ken; Yamane, Yuichi; Ogawa, Kazuhiko; Aizawa, Eiju; Yanagisawa, Hiroshi; Miyoshi, Yoshinori [Japan Atomic Energy Research Inst., Tokai, Ibaraki (Japan). Tokai Research Establishment

    2002-03-01

    This is a databook of TRACY ''ramp feed'' experiments. TRACY is a reactor to perform supercritical experiments using low-enriched uranyl nitrate aqueous solution. The excess reactivity of TRACY is 3$ at maximum, and it is inserted by feeding the solution to a core tank or by withdrawing a control rod, which is called as the transient rod, from the core. In the ramp feed experiment, the supercritical experiment is initiated by feeding the fuel solution to the core tank in a constant feed rate. The data in the present databook consist of datasheets and graphs. Experimental conditions and typical values of measured parameters are tabulated in the datasheet. In the graph, power and temperature profiles are plotted. Those data are useful for the investigation of criticality accidents with fissile solutions, and for validation of criticality accident analysis codes. (author)

  12. The difference between traditional experiments and CFD validation benchmark experiments

    Energy Technology Data Exchange (ETDEWEB)

    Smith, Barton L., E-mail: barton.smith@usu.edu

    2017-02-15

    Computation Fluid Dynamics provides attractive features for design, and perhaps licensing, of nuclear power plants. The most important of these features is low cost compared to experiments. However, uncertainty of CFD calculations must accompany these calculations in order for the results to be useful for important decision making. In order to properly assess the uncertainty of a CFD calculation, it must be “validated” against experimental data. Unfortunately, traditional “discovery” experiments are normally ill-suited to provide all of the information necessary for the validation exercise. Traditionally, experiments are performed to discover new physics, determine model parameters, or to test designs. This article will describe a new type of experiment; one that is designed and carried out with the specific purpose of providing Computational Fluid Dynamics (CFD) validation benchmark data. We will demonstrate that the goals of traditional experiments and validation experiments are often in conflict, making use of traditional experimental results problematic and leading directly to larger predictive uncertainty of the CFD model.

  13. The difference between traditional experiments and CFD validation benchmark experiments

    International Nuclear Information System (INIS)

    Smith, Barton L.

    2017-01-01

    Computation Fluid Dynamics provides attractive features for design, and perhaps licensing, of nuclear power plants. The most important of these features is low cost compared to experiments. However, uncertainty of CFD calculations must accompany these calculations in order for the results to be useful for important decision making. In order to properly assess the uncertainty of a CFD calculation, it must be “validated” against experimental data. Unfortunately, traditional “discovery” experiments are normally ill-suited to provide all of the information necessary for the validation exercise. Traditionally, experiments are performed to discover new physics, determine model parameters, or to test designs. This article will describe a new type of experiment; one that is designed and carried out with the specific purpose of providing Computational Fluid Dynamics (CFD) validation benchmark data. We will demonstrate that the goals of traditional experiments and validation experiments are often in conflict, making use of traditional experimental results problematic and leading directly to larger predictive uncertainty of the CFD model.

  14. Decaying Dark Atom Constituents and Cosmic Positron Excess

    DEFF Research Database (Denmark)

    Belotsky, K.; Khlopov, M.; Kouvaris, C.

    2014-01-01

    We present a scenario where dark matter is in the form of dark atoms that can accommodate the experimentally observed excess of positrons in PAMELA and AMS-02 while being compatible with the constraints imposed on the gamma-ray ux from Fermi/LAT. This scenario assumes that the dominant component...... of dark matter is in the form of a bound state between a helium nucleus and a -2 particle and a small component is in the form of a WIMP-like dark atom compatible with direct searches in underground detectors. One of the constituents of this WIMP-like state is a +2 metastable particle with a mass of 1 Te...... baryons in the universe to be close to -3....

  15. Tell Your Story to No One: ‘Re-Servicing’ Virtue in the Magdalen House

    Directory of Open Access Journals (Sweden)

    Sylvia Greenup

    2015-03-01

    Full Text Available Thearticle probes the amphibious character of the ‘slippery’ servant-maid who methodically migrates between servitude and prostitution. It focuses in particular on the revision of the servant-maid/prostitute in the 1759 novel The Histories of Some of the Penitents in the Magdalen House, published concomitantly with the opening of the Magdalen Hospital for Penitent Prostitutes as an aid in its object of re-training fallen women for domestic service. The literary re-imagining of Histories is analysed here through its engagement with the most significant topoi in master-servant relations recurring in both anti-servant literature and domestic conduct manuals as well as within the larger context of the so-called Pamela controversy. 

  16. Dark matter through the axion portal

    Science.gov (United States)

    Nomura, Yasunori; Thaler, Jesse

    2009-04-01

    Motivated by the galactic positron excess seen by PAMELA and ATIC/PPB-BETS, we propose that dark matter is a TeV-scale particle that annihilates into a pseudoscalar “axion.” The positron excess and the absence of an antiproton or gamma ray excess constrain the axion mass and branching ratios. In the simplest realization, the axion is associated with a Peccei-Quinn symmetry, in which case it has a mass around 360-800 MeV and decays into muons. We present a simple and predictive supersymmetric model implementing this scenario, where both the Higgsino and dark matter obtain masses from the same source of TeV-scale spontaneous symmetry breaking.

  17. KSC-04PD-2201

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Employees at KSC stroll among several tents featuring vendors exhibits of safety- and health-related products. The exhibits were part of Spaceport Super Safety and Health Day, which also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building (seen here) and the O&C Building. The annual event was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  18. The Challenging Experience Questionnaire: Characterization of challenging experiences with psilocybin mushrooms.

    Science.gov (United States)

    Barrett, Frederick S; Bradstreet, Matthew P; Leoutsakos, Jeannie-Marie S; Johnson, Matthew W; Griffiths, Roland R

    2016-12-01

    Acute adverse psychological reactions to classic hallucinogens ("bad trips" or "challenging experiences"), while usually benign with proper screening, preparation, and support in controlled settings, remain a safety concern in uncontrolled settings (such as illicit use contexts). Anecdotal and case reports suggest potential adverse acute symptoms including affective (panic, depressed mood), cognitive (confusion, feelings of losing sanity), and somatic (nausea, heart palpitation) symptoms. Responses to items from several hallucinogen-sensitive questionnaires (Hallucinogen Rating Scale, the States of Consciousness Questionnaire, and the Five-Dimensional Altered States of Consciousness questionnaire) in an Internet survey of challenging experiences with the classic hallucinogen psilocybin were used to construct and validate a Challenging Experience Questionnaire. The stand-alone Challenging Experience Questionnaire was then validated in a separate sample. Seven Challenging Experience Questionnaire factors (grief, fear, death, insanity, isolation, physical distress, and paranoia) provide a phenomenological profile of challenging aspects of experiences with psilocybin. Factor scores were associated with difficulty, meaningfulness, spiritual significance, and change in well-being attributed to the challenging experiences. The factor structure did not differ based on gender or prior struggle with anxiety or depression. The Challenging Experience Questionnaire provides a basis for future investigation of predictors and outcomes of challenging experiences with classic hallucinogens. © The Author(s) 2016.

  19. A Multi-frequency analysis of dark matter annihilation interpretations of recent anti-particle and γ-ray excesses in cosmic structures

    Energy Technology Data Exchange (ETDEWEB)

    Beck, G.; Colafrancesco, S., E-mail: geoff.m.beck@gmail.com, E-mail: sergio.colafrancesco@wits.ac.za [School of Physics, University of the Witwatersrand, Private Bag 3, WITS-2050, Johannesburg (South Africa)

    2016-05-01

    The Fermi-LAT observation of a γ-ray excess from the galactic-centre, as well as the PAMELA, AMS, and AMS-2 anti-particle excesses, and the recent indications of a Fermi-LAT γ-ray excess in the Reticulum II dwarf galaxy have all been variously put forward as possible indirect signatures of supersymmetric neutralino dark matter. These are of particular interest as the neutralino annihilation models which fit these observations must have observable consequences across the frequency spectrum, from radio to γ-ray emission. Moreover, since dark matter is expected to be a major constituent of cosmic structure, these multi-frequency consequences should be common to such structures across the mass spectrum, from dwarf galaxies to galaxy clusters. Thus, in this work we make predictions for the multi-frequency spectra of three well-known sources dominated by dark matter on cluster, galaxy and dwarf galaxy scales, e.g. the Coma cluster, the galaxy M81, and the Draco dwarf galaxy, using models favoured by dark matter interpretations of the aforementioned observations. We pay special attention to the consequences for these models when their cross-sections are renormalised to reproduce the recent γ-ray excess observed in the Reticulum II dwarf galaxy, as well as using cross-sections from the Fermi-LAT dwarf galaxy limits, which throw a dark matter interpretation of this excess into doubt. We find that the multi-frequency data of Coma and Draco are in conflict with the dark matter interpretation of the AMS, PAMELA and Fermi positron excess. Additionally, models derived from Fermi-LAT galactic centre observations, and AMS-2 re-analysis, present similar but less extensive conflicts. Using the sensitivity projections for the Square Kilometre Array, the Cherenkov Telescope Array, as well as the ASTROGAM and ASTRO-H satellites, we determine the detection prospects for a subset of neutralino models that remain consistent with Planck cosmological constraints. Although the SKA has

  20. Particle physics experiments

    International Nuclear Information System (INIS)

    Stuart, G.W.

    1986-01-01

    The report of the Rutherford Appleton Laboratory describes the work carried out in 1985 on experiments approved by the Particle Physics Experiments Selection Panel. The contents consist of unedited contributions from each experiment. (author)

  1. Sharing ESA's knowledge and experience - the Erasmus Experiment Archive

    Science.gov (United States)

    Isakeit, Dieter; Sabbatini, Massimo; Carey, William

    2004-11-01

    The Erasmus Experiment Archive is an electronic database, that collects all experiments performed to date in the faciliteis that fall under the responsibility of the ESA (human spaceflight, microgravity, exploration).

  2. Design of modern experiments

    International Nuclear Information System (INIS)

    Park, Sung Hweon

    1984-03-01

    This book is for researchers and engineers, which is written to focus on practical design of experiments. It gives descriptions of conception of design of experiments, basic statistics theory, one way design of experiment, two-way layout without repetition, two-way layout with repetition, partition, a correlation analysis and regression analysis, latin squares, factorial design, design of experiment by table of orthogonal arrays, design of experiment of response surface, design of experiment on compound, Evop, and design of experiment of taguchi.

  3. Classic experiments

    CERN Multimedia

    CERN. Geneva; Franklin, M

    2001-01-01

    These will be a set of lectures on classic particle physics experiments, with emphasis on how the emasurements are made. I will discuss experiments made to measure the electric charge distribution of particles, to measure the symmetries of the weak decays, to measure the magnetic moment of the muon. As well as experiments performed which discovered new particles or resonances, like the tAU2and the J/Psi. The coverage will be general and should be understandable to someone knowing little particle physics.

  4. Researching experiences

    DEFF Research Database (Denmark)

    Gjedde, Lisa; Ingemann, Bruno

    In the beginning was - not the word - but the experience. This phenomenological approach provides the basis for this book, which focuses on how a person-in-situation experiences and constructs meaning from a variety of cultural visual events. This book presents video-based processual methods......, dialogue, moods, values and narratives have been investigated qualitatively with more than sixty informants in a range of projects. The processual methodological insights are put into a theoretical perspective and also presented as pragmatic dilemmas. Researching Experiences is relevant not only...

  5. Particle physics experiments 1986

    International Nuclear Information System (INIS)

    Stuart, G.W.

    1987-01-01

    The paper presents research work carried out in 1986 on 52 elementary particle experiments approved by the Particle Physics Experiments Selection Panel. Most of the experiments were collaborative and involved research groups from different countries. About half of the experiments were conducted at CERN, the remaining experiments employed the accelerators: LAMPT, LEP, PETRA, SLAC, and HERA. The contents consist of unedited contributions from each experiment. (U.K.)

  6. Pixel Experiments

    DEFF Research Database (Denmark)

    Petersen, Kjell Yngve; Søndergaard, Karin; Augustesen, Christina

    2015-01-01

    Pixel Experiments The term pixel is traditionally defined as any of the minute elements that together constitute a larger context or image. A pixel has its own form and is the smallest unit seen within a larger structure. In working with the potentials of LED technology in architectural lighting...... lighting design in practice, one quickly experiences and realises that there are untapped potentials in the attributes of LED technology. In this research, speculative studies have been made working with the attributes of LEDs in architectural contexts, with the ambition to ascertain new strategies...... for using LED lighting in lighting design practice. The speculative experiments that have been set-up have aimed to clarify the variables that can be used as parameters in the design of lighting applications; including, for example, the structuring and software control of light. The experiments also...

  7. Simulated experiments

    International Nuclear Information System (INIS)

    Bjerknes, R.

    1977-01-01

    A cybernetic model has been developed to elucidate some of the main principles of the growth regulation system in the epidermis of the hairless mouse. A number of actual and theoretical biological experiments have been simulated on the model. These included simulating the cell kinetics as measured by pulse labelling with tritiated thymidine and by continuous labelling with tritiated thymidine. Other simulated experiments included steady state, wear and tear, painting with a carcinogen, heredity and heredity and tumour. Numerous diagrams illustrate the results of these simulated experiments. (JIW)

  8. Organic chemistry experiment

    International Nuclear Information System (INIS)

    Mun, Seok Sik

    2005-02-01

    This book deals with organic chemistry experiments, it is divided five chapters, which have introduction, the way to write the experiment report and safety in the laboratory, basic experiment technic like recrystallization and extraction, a lot of organic chemistry experiments such as fischer esterification, ester hydrolysis, electrophilic aromatic substitution, aldol reaction, benzoin condensation, wittig reaction grignard reaction, epoxidation reaction and selective reduction. The last chapter introduces chemistry site on the internet and way to find out reference on chemistry.

  9. Experiment Databases

    Science.gov (United States)

    Vanschoren, Joaquin; Blockeel, Hendrik

    Next to running machine learning algorithms based on inductive queries, much can be learned by immediately querying the combined results of many prior studies. Indeed, all around the globe, thousands of machine learning experiments are being executed on a daily basis, generating a constant stream of empirical information on machine learning techniques. While the information contained in these experiments might have many uses beyond their original intent, results are typically described very concisely in papers and discarded afterwards. If we properly store and organize these results in central databases, they can be immediately reused for further analysis, thus boosting future research. In this chapter, we propose the use of experiment databases: databases designed to collect all the necessary details of these experiments, and to intelligently organize them in online repositories to enable fast and thorough analysis of a myriad of collected results. They constitute an additional, queriable source of empirical meta-data based on principled descriptions of algorithm executions, without reimplementing the algorithms in an inductive database. As such, they engender a very dynamic, collaborative approach to experimentation, in which experiments can be freely shared, linked together, and immediately reused by researchers all over the world. They can be set up for personal use, to share results within a lab or to create open, community-wide repositories. Here, we provide a high-level overview of their design, and use an existing experiment database to answer various interesting research questions about machine learning algorithms and to verify a number of recent studies.

  10. Understanding patient experience

    DEFF Research Database (Denmark)

    Andersen, Tariq O.; Andersen, Pernille R. D.; Kornum, Anders C.

    2017-01-01

    , safety) arise from getting feedback on symptoms and from continuous and comforting interaction with clinicians. With this paper, we aim to sensitise UX researchers and designers of patient-centred e-health by proposing three UX dimensions: connectedness, comprehension, and compassion.......The term 'patient experience' is currently part of a global discourse on ways to improve healthcare. This study empirically explores what patient experience is in cardiac remote monitoring and considers the implications for user experience (UX). Through interviews around the deployment of a mobile...... app that enables patients to collaborate with clinicians, we unpack experiences in six themes and present narratives of patients' lifeworlds. We find that patients' emotions are grounded in negative feelings (uncertainty, anxiety, loss of hope) and that positive experiences (relief, reassurance...

  11. Linking consumer experiences

    DEFF Research Database (Denmark)

    Smed, Karina Madsen

    become part of the individual self, worldview, and behaviour. This paper seeks to explore links between consumer experiences through the exploration of narrative sequences in travel blogs. Findings indicate that non-consumption is a central element to the bloggers and also indicative of a community......Consumers consume products in various ways serving a number of purposes. Much attention has been paid to experiences attached to consumption, sometimes very explicitly, e.g. in tourism, the essence of which is experiences of various sorts, but often also implicitly as internalised experiences...

  12. Analytical chemistry experiment

    International Nuclear Information System (INIS)

    Park, Seung Jo; Paeng, Seong Gwan; Jang, Cheol Hyeon

    1992-08-01

    This book deals with analytical chemistry experiment with eight chapters. It explains general matters that require attention on experiment, handling of medicine with keep and class, the method for handling and glass devices, general control during experiment on heating, cooling, filtering, distillation and extraction and evaporation and dry, glass craft on purpose of the craft, how to cut glass tube and how to bend glass tube, volumetric analysis on neutralization titration and precipitation titration, gravimetric analysis on solubility product, filter and washing and microorganism experiment with necessary tool, sterilization disinfection incubation and appendixes.

  13. The Experiment

    Science.gov (United States)

    Mariana Nicoara, Floare

    2016-04-01

    My name is Nicoara Floarea and I am teacher at Secondary School Calatele and I teach students from preparatory class and the second grade . They are six-eight years old. In my activity, for introducing scientific concepts to my students, I use various and active methods or traditional methods including experiments. The experiment stimulates students' curiosity, their creativity, the understanding and knowledge taught accessibility. I propose you two such experiments: The life cycle of the plants (long-term experiment, with rigorous observation time):We use beans, wheat or other; They are grown in pots and on the cotton soaked with water,keeping under students' observation protecting them ( just soak them regularly) and we waiting the plants rise. For discussions and comments of plant embryo development we use the plants which rose on the cotton soaked with water plants at the end of the first week. Last school year we had in the pot climbing beans which in May made pods. They were not too great but our experiment was a success. The students could deduce that there will develop those big beans which after drying will be planted again. The influence of light on plants (average duration experiment with the necessary observation time): We use two pots in which plants are of the same type (two geraniums), one of them is situated so as to get direct sunlight and other plant we put in a closed box. Although we wet both plants after a week we see that the plant that benefited from sunlight has turned strain in direct sunlight, developing normally in return the plant out of the box I have yellowed leaves, photosynthesis does not She has occurred . Students will understand the vital role of the Sun in plants' life, both in the classroom and in nature. The experiment is a method of teaching students extremely pleasant, with a remarkable percentage of acquiring more knowledge.

  14. Experiments in computing: a survey.

    Science.gov (United States)

    Tedre, Matti; Moisseinen, Nella

    2014-01-01

    Experiments play a central role in science. The role of experiments in computing is, however, unclear. Questions about the relevance of experiments in computing attracted little attention until the 1980s. As the discipline then saw a push towards experimental computer science, a variety of technically, theoretically, and empirically oriented views on experiments emerged. As a consequence of those debates, today's computing fields use experiments and experiment terminology in a variety of ways. This paper analyzes experimentation debates in computing. It presents five ways in which debaters have conceptualized experiments in computing: feasibility experiment, trial experiment, field experiment, comparison experiment, and controlled experiment. This paper has three aims: to clarify experiment terminology in computing; to contribute to disciplinary self-understanding of computing; and, due to computing's centrality in other fields, to promote understanding of experiments in modern science in general.

  15. PERENCANAAN RUTE PERJALANAN DI JAWA TIMUR DENGAN DUKUNGAN GIS MENGGUNAKAN METODE DIJKSTRA S

    Directory of Open Access Journals (Sweden)

    Kartika Gunadi

    2002-01-01

    Full Text Available Many people need geographical information nowadays, such as: the distance between areas, information about some areas, information about nature resources in that area, to search for accident area, and others geographical information. Geographical Information System (GIS is only one from many others solution to seek for geographical information. This research aim is to make software that can give some geographical information for shortest path between towns in East Java. Others information that can be gain is information about governmental, population, tourism places, mountains, special food, handicraft, and traditional art. This software is designed with database not using satellite, so much cheaper compare with using satellite. This software use Dijkstra's method to seek the shortest path from one node to another node in the picture, so this program can't give alternative path. GIS can give answer for anything that related with geographical situation. Peoples can use GIS power to reach for a better life. Abstract in Bahasa Indonesia : Informasi mengenai geografi semakin dibutuhkan oleh banyak pihak, misalnya informasi untuk mengetahui jarak antara satu daerah dengan daerah lain, informasi seputar daerah yang diinginkan, informasi tentang sumber daya alam yang dicari, informasi untuk menemukan lokasi kecelakaan dengan cepat, dan banyak informasi mengenai geografi lainnya. Geographical Information Systems (GIS merupakan salah satu solusi untuk mendapatkan informasi geografi tersebut. Tujuan perancangan adalah membuat suatu perangkat lunak yang dapat memberikan informasi geografi mengenai rute jalan terpendek antara kota yang satu dengan kota yang lainnya di Jawa Timur. Sedangkan informasi lainnya yang dapat diperoleh antara lain informasi mengenai pemerintahan, jumlah penduduk, tempat wisata, nama gunung, makanan khas, kerajinan, dan `kesenian tradisional yang berasal dari suatu daerah. Program ini dirancang tanpa menggunakan satelit namun hanya

  16. Particle physics experiments 1982

    International Nuclear Information System (INIS)

    Rousseau, M.D.; Stuart, G.

    1983-01-01

    Work carried out in 1982 on 52 experiments approved by the Particle Physics Experiments Selection Panel is described. Each experiment is listed under title, collaboration, technique, accelerator, year of running, status and spokesman. Unedited contributions are given from each experiment. (U.K.)

  17. Framework of product experience

    NARCIS (Netherlands)

    Desmet, P.; Hekkert, P.

    2007-01-01

    In this paper, we introduce a general framework for product experience that applies to all affective responses that can be experienced in human-product interaction. Three distinct components or levels of product experiences are discussed: aesthetic experience, experience of meaning, and emotional

  18. Experience in Design and Learning Approaches – Enhancing the Framework for Experience

    Directory of Open Access Journals (Sweden)

    Merja L.M. Bauters

    2017-06-01

    Full Text Available In design and learning studies, an increasing amount of attention has been paid to experience. Many design approaches relate experience to embodiment and phenomenology. The growth in the number of applications that use the Internet of Things (IoT has shifted human interactions from mobile devices and computers to tangible, material things. In education, the pressure to learn and update skills and knowledge, especially in work environments, has underlined the challenge of understanding how workers learn from reflection while working. These directions have been fuelled by research findings in the neurosciences, embodied cognition, the extended phenomenological–cognitive system and the role of emotions in decision-making and meaning making. The perspective on experience in different disciplines varies, and the aim is often to categorise experience. These approaches provide a worthwhile view of the importance of experience in learning and design, such as the recent emphasis on conceptual and epistemological knowledge creation. In pragmatism, experience plays a considerable role in research, art, communication and reflection. Therefore, I rely on Peirce’s communicative theory of signs and Dewey’s philosophy of experience to examine how experience is connected to reflection and therefore how it is necessarily tangible.

  19. Popper's Thought Experiment Reinvestigated

    Science.gov (United States)

    Richardson, Chris; Dowling, Jonathan

    2012-02-01

    Karl Popper posed an interesting thought experiment in 1934. With it, he meant to question the completeness of quantum mechanics. He claimed that the notion of quantum entanglement leads to absurd scenarios that cannot be true in real life and that an implementation of his thought experiment would not give the results that QM predicts. Unfortunately for Popper, it has taken until recently to perform experiments that test his claims. The results of the experiments do not refute QM as Popper predicted, but neither do they confirm what Popper claimed QM predicted. Kim and Shih implemented Popper's thought experiment in the lab. The results of the experiment are not clear and have instigated many interpretations of the results. The results show some correlation between entangled photons, but not in the way that Popper thought, nor in the way a simple application of QM might predict. A ghost-imaging experiment by Strekalov, et al. sheds light on the physics behind Popper's thought experiment, but does not try to directly test it. I will build the physics of Popper's thought experiment from the ground up and show how the results of both of these experiments agree with each other and the theory of QM, but disprove Popper.

  20. Adaptive structures flight experiments

    Science.gov (United States)

    Martin, Maurice

    The topics are presented in viewgraph form and include the following: adaptive structures flight experiments; enhanced resolution using active vibration suppression; Advanced Controls Technology Experiment (ACTEX); ACTEX program status; ACTEX-2; ACTEX-2 program status; modular control patch; STRV-1b Cryocooler Vibration Suppression Experiment; STRV-1b program status; Precision Optical Bench Experiment (PROBE); Clementine Spacecraft Configuration; TECHSAT all-composite spacecraft; Inexpensive Structures and Materials Flight Experiment (INFLEX); and INFLEX program status.

  1. Experiment-o-mania

    Science.gov (United States)

    Drndarski, Marina

    2015-04-01

    Every 21st century student is expected to develop science literacy skills. As this is not part of Serbian national curriculum yet, we decided to introduce it with this project. Experiment-o-mania provides students to experience science in different and exciting way. It makes opportunity for personalized learning offering space and time to ask (why, where, how, what if) and to try. Therefore, we empower young people with skills of experimenting, and they love science back. They ask questions, make hypothesis, make problems and solve them, make mistakes, discuss about the results. Subsequently this raises the students' interest for school curriculum. This vision of science teaching is associated with inquiry-based learning. Experiment-o-mania is the unique and recognizable teaching methodology for the elementary school Drinka Pavlović, Belgrade, Serbia. Experiment-o-mania implies activities throughout the school year. They are held on extra class sessions, through science experiments, science projects or preparations for School's Days of science. Students learn to ask questions, make observations, classify data, communicate ideas, conduct experiments, analyse results and make conclusions. All science teachers participate in designing activities and experiments for students in Experiment-o-mania teaching method. But they are not alone. Teacher of fine arts, English teachers and others also take part. Students have their representatives in this team, too. This is a good way to blend knowledge among different school subject and popularize science in general. All the experiments are age appropriate and related to real life situations, local community, society and the world. We explore Fibonacci's arrays, saving energy, solar power, climate change, environmental problems, pollution, daily life situations in the country or worldwide. We introduce great scientists as Nikola Tesla, Milutin Milanković and sir Isaac Newton. We celebrate all relevant international days, weeks

  2. Inner heliosphere spatial gradients of GCR protons and alpha particles in the low GeV range

    Science.gov (United States)

    Gieseler, J.; Boezio, M.; Casolino, M.; De Simone, N.; Di Felice, V.; Heber, B.; Martucci, M.; Picozza, P.

    2013-12-01

    The spacecraft Ulysses was launched in October 1990 in the maximum phase of solar cycle 22, reached its final, highly inclined (80.2°) Keplerian orbit around the Sun in February 1992, and was finally switched off in June 2009. The Kiel Electron Telescope (KET) aboard Ulysses measures electrons from 3 MeV to a few GeV and protons and helium in the energy range from 6 MeV/nucleon to above 2 GeV/nucleon. In order to investigate the radial and latitudinal gradients of galactic cosmic rays (GCR), it is essential to know their intensity variations for a stationary observer in the heliosphere because the Ulysses measurements reflect not only the spatial but also the temporal variation of the energetic particle intensities. This was accomplished in the past with the Interplanetary Monitoring Platform-J (IMP 8) until it was lost in 2006. Fortunately, the satellite-borne experiment PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) was launched in June 2006 and can be used as a reliable 1 AU baseline for measurements of the KET aboard Ulysses. With these tools at hand, we have the opportunity to determine the spatial gradients of GCR protons and alpha particles at about 0.1 to 1 GeV/n in the inner heliosphere during the extended minimum of solar cycle 23. We then compare these A0 cycle.

  3. Channeling experiment

    International Nuclear Information System (INIS)

    Abelin, H.; Birgersson, L.; Widen, H.; Aagren, T.; Moreno, L.; Neretnieks, I.

    1990-07-01

    Channeling of water flow and tracer transport in real fractures in a granite body at Stripa have been investigated experimentally. The experimental site was located 360 m below the ground level. Two kinds of experiments were performed. In the single hole experiments, 20 cm diameter holes were drilled about 2.5 m into the rock in the plane of the fracture. Specially designed packers were used to inject water into the fracture in 5 cm intervals all along the fracture trace in the hole. The variation of the injection flowrates along the fracture were used to determine the transmissivity variations in the fracture plane. Detailed photographs were taken from inside the hole and the visual fracture aperture was compared with the injection flowrates in the same locations. Geostatistical methods were used to evaluate the results. Five holes were measured in great detail. In addition 7 holes were drilled and scanned by simpler packer systems. A double hole experiment was performed where two parallel holes were drilled in the same fracture plane at nearly 2 m distance. Pressure pulse tests were made between the holes in both directions. Tracers were injected in 5 locations in one hole and monitored for in many locations in the other hole. The single hole experiment and the double hole experiment show that most of the fracture planes are tight but that there are open sections which form connected channels over distances of at least 2 meters. It was also found in the double hole experiment that the investigated fracture was intersected by at least one fracture between the two holes which diverted a large amount of the injected tracers to several distant locations at the tunnel wall. (authours)

  4. The ERASMUS experiment archive

    Science.gov (United States)

    Isakeit, Dieter; Sabbatini, Massimo; Carey, William

    2005-08-01

    The Erasmus Experiment Archive is an electronic database, accessible through the Internet, that collects in a single reference repository scientific, technical and operational information regarding the experiments performed in the experiment facilities which fall under the responsibility of the ESA Directorate of Human Spaceflight, Microgravity and Exploration. The archive is operated, filled with content and kept up-to-date by the Erasmus User Centre. which forms part of the Directorate. The archive shares its records and is interoperable with similar experiment archives of the partner agencies NASA USA) and JAXA (Japan) through a mutually agreed standard for experiment records called the International Distributed Experiment Archive (IDEA).

  5. Estimating solar resources in Mexico using cloud cover data

    Energy Technology Data Exchange (ETDEWEB)

    Renne, David; George, Ray; Brady, Liz; Marion, Bill [National Renewable Energy Laboratory, Colorado (United States); Estrada Cajigal, Vicente [Cuernavaca, Morelos (Mexico)

    2000-07-01

    Laboratory (Laboratorio Nacional de Energia Renovable)) a Mexico para desarrollar una base de datos solares. Una fuente importante de datos de entrada al modelo CSR es una base de datos de cubrimiento de nubes de la superficie terrestre proveniente de satelite, llamada Real Time Nephanalysis (RTNEPH)(Nefanalisis de Tiempo Real). El RTNEPH es desarrollado por la Fuerza Aerea de los Estados Unidos y distribuido por el Centro Nacional de Datos Climaticos de los Estados Unidos. El RTNEPH combina observaciones de rutina en tierra de cubrimiento de nubes realizadas cada tres horas en los centros nacionales de temperatura a traves del mundo con una informacion de cubrimiento de nubes proveniente de satelite elaborada por los satelites climaticos polares en orbita. Los datos son digitalizados geoespacialmente de tal manera que la informacion cubrimiento de nubes multiestratificadas este disponible en una cuadricula de aproximadamente 40 Km por cada cuadro. El desarrollo de esta base de datos es un proyecto en curso que actualmente cubre mas de 20 anos de observaciones. Para el analisis de Norte America (incluyendo Mexico) utilizamos un histograma de 8 anos resumido sobre la RTNEPH que proporciona un promedio mensual de informacion de cubrimiento de nubes por el periodo de 1985 a 1992. El modelo CSR tambien toma en cuenta el debilitamiento del haz de luz solar debido a aerosoles, trazas de gases atmosfericos, y vapor de agua. El modelo CSR proporciona informacion solar promediada mensualmente de manera directa y normal, horizontal global y difusa para cada una de las celdas de 40 Km de la red. De esta informacion es tambien posible producir estimados de los recursos solares para varios tipos de colectores solares y varias orientaciones, tal como los colectores de plato plano orientados hacia la inclinacion de la latitud, o concentrando colectores de energia solar. Los resultados de los modelos se despliegan al usar el software Geographic Information System (Sistema de Informacion

  6. Review of experiments

    International Nuclear Information System (INIS)

    Chang, C.; Yodh, G.; Cutts, D.; Lanou, R.; Engels, E.; Kramer, M.; Danby, G.

    1977-01-01

    A study was made to examine the effects which raising the ISA from 200 x 200 GeV to 400 x 400 GeV would have on the ''canonical'' experiments. These were ''canonical'' in the sense that they span the full range of foreseeable physics and have served as topics in previous Summer Studies and Workshops which resulted in quite explicit hardware designs and experimental goals. The study results indicate that all of the ''canonical'' experiments survive. Some are actually improved, some are unaffected, and some require changes which are suggested. In general, the 90 0 experiments are relatively unaffected. The single arm small angle spectrometer, the wide aperture (FATS-WASP) spectrometer and the Coulomb interference experiment have the largest number of modifications suggested. No uniqueness to these solutions are claimed, and there may be more desirable radical approaches. It is, however, felt that the 400 x 400 GeV ISA not only permits the work on conceptual experiments from previous Summer Studies to be taken over entirely, but indicates areas of improvement in many of them. Specifics of the individual experiments are discussed

  7. Diagnostics for pellet experiments

    International Nuclear Information System (INIS)

    Johnson, R.R.

    1978-01-01

    The target diagnostics which are being used and planned in current laser driven ICF Experiments are described. Most of these diagnostics can be easily applied to future ion-beam fusion experiments. The status of laser fusion diagnostics has been much improved in the last 5 years and further improvements can be expected and should be available when the first ICF experiments using ion beams are performed. As an example, x-ray temporal and spatial resolutions are now approximately 5 psec and 3 μm, which is approximately a factor of 4 better than the resolution reported in the first implosion experiments. As one plans ahead for ion-beam fusion experiments it should be emphasized that high yield experiments are easier to diagnose provided adequate shielding is employed. However, in the event that the first high yield experiments fail it will be necessary to have diagnostics available to determine where the problems lie. In laser fusion it is interesting to note that higher laser powers are required now for breakeven experiments than first anticipated, mainly because some aspects of the laser-interaction physics were not recognized until the experiments were carefully diagnosed. Thus as has been pointed out, it may be necessary to increase the energy of the ion-beam driver to enable us to do breakeven experiments with high confidence

  8. Reproducible computational biology experiments with SED-ML--the Simulation Experiment Description Markup Language.

    Science.gov (United States)

    Waltemath, Dagmar; Adams, Richard; Bergmann, Frank T; Hucka, Michael; Kolpakov, Fedor; Miller, Andrew K; Moraru, Ion I; Nickerson, David; Sahle, Sven; Snoep, Jacky L; Le Novère, Nicolas

    2011-12-15

    The increasing use of computational simulation experiments to inform modern biological research creates new challenges to annotate, archive, share and reproduce such experiments. The recently published Minimum Information About a Simulation Experiment (MIASE) proposes a minimal set of information that should be provided to allow the reproduction of simulation experiments among users and software tools. In this article, we present the Simulation Experiment Description Markup Language (SED-ML). SED-ML encodes in a computer-readable exchange format the information required by MIASE to enable reproduction of simulation experiments. It has been developed as a community project and it is defined in a detailed technical specification and additionally provides an XML schema. The version of SED-ML described in this publication is Level 1 Version 1. It covers the description of the most frequent type of simulation experiments in the area, namely time course simulations. SED-ML documents specify which models to use in an experiment, modifications to apply on the models before using them, which simulation procedures to run on each model, what analysis results to output, and how the results should be presented. These descriptions are independent of the underlying model implementation. SED-ML is a software-independent format for encoding the description of simulation experiments; it is not specific to particular simulation tools. Here, we demonstrate that with the growing software support for SED-ML we can effectively exchange executable simulation descriptions. With SED-ML, software can exchange simulation experiment descriptions, enabling the validation and reuse of simulation experiments in different tools. Authors of papers reporting simulation experiments can make their simulation protocols available for other scientists to reproduce the results. Because SED-ML is agnostic about exact modeling language(s) used, experiments covering models from different fields of research

  9. Reproducible computational biology experiments with SED-ML - The Simulation Experiment Description Markup Language

    Science.gov (United States)

    2011-01-01

    Background The increasing use of computational simulation experiments to inform modern biological research creates new challenges to annotate, archive, share and reproduce such experiments. The recently published Minimum Information About a Simulation Experiment (MIASE) proposes a minimal set of information that should be provided to allow the reproduction of simulation experiments among users and software tools. Results In this article, we present the Simulation Experiment Description Markup Language (SED-ML). SED-ML encodes in a computer-readable exchange format the information required by MIASE to enable reproduction of simulation experiments. It has been developed as a community project and it is defined in a detailed technical specification and additionally provides an XML schema. The version of SED-ML described in this publication is Level 1 Version 1. It covers the description of the most frequent type of simulation experiments in the area, namely time course simulations. SED-ML documents specify which models to use in an experiment, modifications to apply on the models before using them, which simulation procedures to run on each model, what analysis results to output, and how the results should be presented. These descriptions are independent of the underlying model implementation. SED-ML is a software-independent format for encoding the description of simulation experiments; it is not specific to particular simulation tools. Here, we demonstrate that with the growing software support for SED-ML we can effectively exchange executable simulation descriptions. Conclusions With SED-ML, software can exchange simulation experiment descriptions, enabling the validation and reuse of simulation experiments in different tools. Authors of papers reporting simulation experiments can make their simulation protocols available for other scientists to reproduce the results. Because SED-ML is agnostic about exact modeling language(s) used, experiments covering models from

  10. The Belle II Experiment

    CERN Document Server

    Kahn, J

    2017-01-01

    Set to begin data taking at the end of 2018, the Belle II experiment is the next-generation B-factory experiment hosted at KEK in Tsukuba, Japan. The experiment represents the cumulative effort from the collaboration of experimental and detector physics, computing, and software development. Taking everything learned from the previous Belle experiment, which ran from 1998 to 2010, Belle II aims to probe deeper than ever before into the field of heavy quark physics. By achieving an integrated luminosity of 50 ab−1 and accumulating 50 times more data than the previous experiment across its lifetime, along with a rewritten analysis framework, the Belle II experiment will push the high precision frontier of high energy physics. This paper will give an overview of the key components and development activities that make the Belle II experiment possible.

  11. Virtual neutron scattering experiments

    DEFF Research Database (Denmark)

    Overgaard, Julie Hougaard; Bruun, Jesper; May, Michael

    2016-01-01

    We describe how virtual experiments can be utilized in a learning design that prepares students for hands-on experiments at large-scale facilities. We illustrate the design by showing how virtual experiments are used at the Niels Bohr Institute in a master level course on neutron scattering....... In the last week of the course, students travel to a large-scale neutron scattering facility to perform real neutron scattering experiments. Through student interviews and survey answers, we argue, that the virtual training prepares the students to engage more fruitfully with experiments by letting them focus...... on physics and data rather than the overwhelming instrumentation. We argue that this is because they can transfer their virtual experimental experience to the real-life situation. However, we also find that learning is still situated in the sense that only knowledge of particular experiments is transferred...

  12. Experiments in physical chemistry

    CERN Document Server

    Wilson, J M; Denaro, A R

    1968-01-01

    Experiments in Physical Chemistry, Second Edition provides a compilation of experiments concerning physical chemistry. This book illustrates the link between the theory and practice of physical chemistry. Organized into three parts, this edition begins with an overview of those experiments that generally have a simple theoretical background. Part II contains experiments that are associated with more advanced theory or more developed techniques, or which require a greater degree of experimental skill. Part III consists of experiments that are in the nature of investigations wherein these invest

  13. Federal Republic of Germany R and D programme: A special issue of the journal radioactive waste management and the nuclear fuel cycle

    International Nuclear Information System (INIS)

    Merz, E.R.

    1986-01-01

    This book examines the issues of radioactive waste management and the nuclear fuel cycle in the Federal Republic of Germany. Topics considered include the challenges of waste handling and disposal, the borosilicate glass for Pamela, the treatment and conditioning of transuranelement bearing wastes in the Federal Republic of Germany, conditioning of low and intermediate level wastes, volume reduction of low level solid radioactive waste by incineration and compaction in the Federal Republic of Germany, MAW test emplacement in boreholes, treatment and disposal of special radioactive wastes comprising tritium, carbon 14, krypton 85 and iodine 129, and the German Project: ''Safety Studies for Nuclear Waste Management: Development of Safety Assessment Methodology for Final Disposal of Nuclear Waste in a Salt Dome

  14. Gamma-ray constraints on hadronic and leptonic activities of decaying dark matter

    International Nuclear Information System (INIS)

    Chen, Chuan-Ren; Mandal, Sourav K.; Takahashi, Fuminobu

    2010-01-01

    While the excess in cosmic-ray electrons and positrons reported by PAMELA and Fermi may be explained by dark matter decaying primarily into charged leptons, this does not necessarily mean that dark matter should not have any hadronic decay modes. In order to quantify the allowed hadronic activities, we derive constraints on the decay rates of dark matter into WW, ZZ, hh, q q-bar and gg using the Fermi and HESS gamma-ray data. We also derive gamma-ray constraints on the leptonic e + e − , μ + μ − and τ + τ − final states. We find that dark matter must decay primarily into μ + μ − or τ + τ − in order to simultaneously explain the reported excess and meet all gamma-ray constraints

  15. KSC-04PD-2216

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. This panel comprising former and current Safety and Mission Assurance (S&MA) management talk about identifying and comparing safety challenges of the past, present and future during Spaceport Super Safety and Health Day (SS&H) at KSC. Larry Crawford, left, is director of S&MA. SS&H Day included guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. In addition, many vendors exhibits were on display for employees. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  16. Particle physics experiments 1983

    International Nuclear Information System (INIS)

    Stuart, G.W.

    1983-01-01

    The report describes work carried out in 1983 on experiments approved by the Particle Physics Experiments Selection Panel. The contents consist of unedited contributions from each experiment. (author)

  17. The Information Science Experiment System - The computer for science experiments in space

    Science.gov (United States)

    Foudriat, Edwin C.; Husson, Charles

    1989-01-01

    The concept of the Information Science Experiment System (ISES), potential experiments, and system requirements are reviewed. The ISES is conceived as a computer resource in space whose aim is to assist computer, earth, and space science experiments, to develop and demonstrate new information processing concepts, and to provide an experiment base for developing new information technology for use in space systems. The discussion covers system hardware and architecture, operating system software, the user interface, and the ground communication link.

  18. Nova target experiments

    International Nuclear Information System (INIS)

    Drake, R.P.

    1985-11-01

    The Nova laser, at the Lawrence Livermore National Laboratory, provides unique opportunities for target experiments. It has unprecedented energy on target and significant flexibility. The paper presented by John Hunt described the capabilities and the status of Nova. This paper discusses plans for future experiments using Nova, and the present status of target experiments. We plan to perform high-quality physics experiments that exploit the unique capabilities of Nova. Because this is our goal, we are fielding an extensive array of well-characterized target diagnostics to measure the emissions from the target. The first section of this paper discusses the basic target diagnostics. We are also taking care to quantify the performance of the laser

  19. Velocity Feedback Experiments

    Directory of Open Access Journals (Sweden)

    Chiu Choi

    2017-02-01

    Full Text Available Transient response such as ringing in a control system can be reduced or removed by velocity feedback. It is a useful control technique that should be covered in the relevant engineering laboratory courses. We developed velocity feedback experiments using two different low cost technologies, viz., operational amplifiers and microcontrollers. These experiments can be easily integrated into laboratory courses on feedback control systems or microcontroller applications. The intent of developing these experiments was to illustrate the ringing problem and to offer effective, low cost solutions for removing such problem. In this paper the pedagogical approach for these velocity feedback experiments was described. The advantages and disadvantages of the two different implementation of velocity feedback were discussed also.

  20. The International Heat Pipe Experiment. [international cooperation zero g experiment

    Science.gov (United States)

    Mcintosh, R.; Ollendorf, S.; Harwell, W.

    1976-01-01

    The aims of the experiment are outlined. Flight experiments included in this program were provided by NASA, Goddard Space Flight Center, ESA (European Space Agency), the German Ministry of Technology, Hughes Aircraft Company and NASA, Ames Research Center.

  1. Virtual neutron scattering experiments

    DEFF Research Database (Denmark)

    Overgaard, Julie Hougaard; Bruun, Jesper; May, Michael

    2017-01-01

    . In the last week of the course, students travel to a large-scale neutron scattering facility to perform real neutron scattering experiments. Through student interviews and survey answers, we argue, that the virtual training prepares the students to engage more fruitfully with experiments by letting them focus......We describe how virtual experiments can be utilized in a learning design that prepares students for hands-on experiments at large-scale facilities. We illustrate the design by showing how virtual experiments are used at the Niels Bohr Institute in a master level course on neutron scattering...

  2. Explicating Experience: Development of a Valid Scale of Past Hazard Experience for Tornadoes.

    Science.gov (United States)

    Demuth, Julie L

    2018-03-23

    People's past experiences with a hazard theoretically influence how they approach future risks. Yet, past hazard experience has been conceptualized and measured in wide-ranging, often simplistic, ways, resulting in mixed findings about its relationship with risk perception. This study develops a scale of past hazard experiences, in the context of tornadoes, that is content and construct valid. A conceptual definition was developed, a set of items were created to measure one's most memorable and multiple tornado experiences, and the measures were evaluated through two surveys of the public who reside in tornado-prone areas. Four dimensions emerged of people's most memorable experience, reflecting their awareness of the tornado risk that day, their personalization of the risk, the intrusive impacts on them personally, and impacts experienced vicariously through others. Two dimensions emerged of people's multiple experiences, reflecting common types of communication received and negative emotional responses. These six dimensions are novel in that they capture people's experience across the timeline of a hazard as well as intangible experiences that are both direct and indirect. The six tornado experience dimensions were correlated with tornado risk perceptions measured as cognitive-affective and as perceived probability of consequences. The varied experience-risk perception results suggest that it is important to understand the nuances of these concepts and their relationships. This study provides a foundation for future work to continue explicating past hazard experience, across different risk contexts, and for understanding its effect on risk assessment and responses. © 2018 Society for Risk Analysis.

  3. Particle physics experiments 1987

    International Nuclear Information System (INIS)

    Stuart, G.W.

    1988-01-01

    This report describes work carried out in 1987 on experiments approved by the Particle Physics Experiments Selection Panel (United Kingdom). The contents consist of unedited contributions from each experiment. (author)

  4. Understanding customer experience.

    Science.gov (United States)

    Meyer, Christopher; Schwager, Andre

    2007-02-01

    Anyone who has signed up for cell phone service, attempted to claim a rebate, or navigated a call center has probably suffered from a company's apparent indifference to what should be its first concern: the customer experiences that culminate in either satisfaction or disappointment and defection. Customer experience is the subjective response customers have to direct or indirect contact with a company. It encompasses every aspect of an offering: customer care, advertising, packaging, features, ease of use, reliability. Customer experience is shaped by customers' expectations, which largely reflect previous experiences. Few CEOs would argue against the significance of customer experience or against measuring and analyzing it. But many don't appreciate how those activities differ from CRM or just how illuminating the data can be. For instance, the majority of the companies in a recent survey believed they have been providing "superior" experiences to customers, but most customers disagreed. The authors describe a customer experience management (CEM) process that involves three kinds of monitoring: past patterns (evaluating completed transactions), present patterns (tracking current relationships), and potential patterns (conducting inquiries in the hope of unveiling future opportunities). Data are collected at or about touch points through such methods as surveys, interviews, focus groups, and online forums. Companies need to involve every function in the effort, not just a single customer-facing group. The authors go on to illustrate how a cross-functional CEM system is created. With such a system, companies can discover which customers are prospects for growth and which require immediate intervention.

  5. Particle physics experiments 1989

    International Nuclear Information System (INIS)

    Bairstow, R.

    1990-01-01

    This report describes work carried out in 1989 on experiments approved by the Particle Physics Experiments Selection Panel of Rutherford Appleton Laboratory. The contents consist of unedited contributions from each experiment. (author)

  6. Experiment data report for LOFT Boron dilution Experiment L6-6

    International Nuclear Information System (INIS)

    Stitt, B.D.; Divine, J.M.

    1982-06-01

    Selected pertinent and uninterpreted data from the sixth anticipated transient experiment (Experiment L6-6) conducted in the Loss-of-Fluid Test (LOFT) facility are presented. Experiment L6-6 simulated a boron dilution accident by injecting demineralized water into the primary coolant system (PCS) at a rate of 0.47 L/s while the reactor was in a cold shutdown condition with the control rods withdrawn. System pressure was maintained at approximately 285 kPa throughout the experiment. The experiment was divided into two parts. In the first part, L6-6A, a recirculation flow of 4.7 L/s was maintained through the PCS and criticality was achieved 7416 +- 10 s after the initiation of the dilution flow. The second part, L6-6B, was identical to L6-6A except that a recirculation flow of 9.5 L/s was maintained and criticality occurred at 8058 +- 10 s

  7. LDR structural experiment definition

    Science.gov (United States)

    Russell, R. A.

    1988-01-01

    A system study to develop the definition of a structural flight experiment for a large precision segmented reflector on the Space Station was accomplished by the Boeing Aerospace Company for NASA's Langley Research Center. The objective of the study was to use a Large Deployable Reflector (LDR) baseline configuration as the basis for focusing an experiment definition, so that the resulting accommodation requirements and interface constraints could be used as part of the mission requirements data base for Space Station. The primary objectives of the first experiment are to construct the primary mirror support truss and to determine its structural and thermal characteristics. Addition of an optical bench, thermal shield and primary mirror segments, and alignment of the optical components, would occur on a second experiment. The structure would then be moved to the payload point system for pointing, optical control, and scientific optical measurement for a third experiment. Experiment 1 will deploy the primary support truss while it is attached to the instrument module structure. The ability to adjust the mirror attachment points and to attach several dummy primary mirror segments with a robotic system will also be demonstrated. Experiment 2 will be achieved by adding new components and equipment to experiment one. Experiment 3 will demonstrate advanced control strategies, active adjustment of the primary mirror alignment, and technologies associated with optical sensing.

  8. Stimulated Brillouin scattering experiments

    International Nuclear Information System (INIS)

    Slater, D.C.; Berger, R.L.; Busch, G.; Kinzer, C.M.; Mayer, F.J.; Powers, L.V.; Tanner, D.J.

    1981-01-01

    This report describes two experiments in which SBS would be expected to play an important role. In the first experiment, we find a clear signature of the Brillouin backscatter of a short (100 psec) pulse from a long (approx. 50 μm) gradient length gas target plasma. The second experiment used much longer (approx. 1 nsec) pulses on spherical glass shell targets. These experiments were done with both narrow ( 30A) bandwidth laser light. Using one-dimensional, spherically symmetric fluid simulations, we have attempted to model many of the laser-plasma interaction processes which combine to determine the amount of absorbed energy in the long-pulse experiments. These simulations indicate that modest laser bandwidths are successful in reducing the level of SBS at the irradiances ( 15 W/cm 2 ) used in these experiments

  9. Unstable gravitino dark matter prospects for indirect and direct detection

    International Nuclear Information System (INIS)

    Grefe, Michael

    2011-11-01

    We confront the signals expected from unstable gravitino dark matter with observations of indirect dark matter detection experiments in all possible cosmic-ray channels. For this purpose we calculate in detail the gravitino decay widths in theories with bilinear violation of R parity, particularly focusing on decay channels with three particles in the final state. Based on these calculations we predict the fluxes of gamma rays, charged cosmic rays and neutrinos expected from decays of gravitino dark matter. Although the predicted spectra could in principal explain the anomalies observed in the cosmic ray positron and electron fluxes as measured by PAMELA and Fermi LAT, we find that this possibility is ruled out by strong constraints from gamma-ray and antiproton observations. Therefore, we employ current data of indirect detection experiments to place strong constraints on the gravitino lifetime and the strength of R-parity violation. In addition, we discuss the prospects of forthcoming searches for a gravitino signal in the spectrum of cosmic-ray antideuterons, finding that they are in particular sensitive to rather low gravitino masses. Finally, we discuss in detail the prospects for detecting a neutrino signal from gravitino dark matter decays, finding that the sensitivity of neutrino telescopes like IceCube is competitive to observations in other cosmic ray channels, especially for rather heavy gravitinos. Moreover, we discuss the prospects for a direct detection of gravitino dark matter via R-parity violating inelastic scatterings off nucleons. We find that, although the scattering cross section is considerably enhanced compared to the case of elastic gravitino scattering, the expected signal is many orders of magnitude too small in order to hope for a detection in underground detectors. (orig.)

  10. Unstable gravitino dark matter prospects for indirect and direct detection

    Energy Technology Data Exchange (ETDEWEB)

    Grefe, Michael

    2011-11-15

    We confront the signals expected from unstable gravitino dark matter with observations of indirect dark matter detection experiments in all possible cosmic-ray channels. For this purpose we calculate in detail the gravitino decay widths in theories with bilinear violation of R parity, particularly focusing on decay channels with three particles in the final state. Based on these calculations we predict the fluxes of gamma rays, charged cosmic rays and neutrinos expected from decays of gravitino dark matter. Although the predicted spectra could in principal explain the anomalies observed in the cosmic ray positron and electron fluxes as measured by PAMELA and Fermi LAT, we find that this possibility is ruled out by strong constraints from gamma-ray and antiproton observations. Therefore, we employ current data of indirect detection experiments to place strong constraints on the gravitino lifetime and the strength of R-parity violation. In addition, we discuss the prospects of forthcoming searches for a gravitino signal in the spectrum of cosmic-ray antideuterons, finding that they are in particular sensitive to rather low gravitino masses. Finally, we discuss in detail the prospects for detecting a neutrino signal from gravitino dark matter decays, finding that the sensitivity of neutrino telescopes like IceCube is competitive to observations in other cosmic ray channels, especially for rather heavy gravitinos. Moreover, we discuss the prospects for a direct detection of gravitino dark matter via R-parity violating inelastic scatterings off nucleons. We find that, although the scattering cross section is considerably enhanced compared to the case of elastic gravitino scattering, the expected signal is many orders of magnitude too small in order to hope for a detection in underground detectors. (orig.)

  11. AGS experiments: 1985, 1986, 1987

    International Nuclear Information System (INIS)

    Depken, J.C.

    1987-01-01

    This report contains: Experimental areas layout, table of beam parameters and fluxes, experiment schedule ''as run,'' experiment long range schedule, a listing of experiments by number, two-page summaries of each experiment, also ordered by number, and publications of AGS experiments, 1982-1987

  12. Collaborative experience

    DEFF Research Database (Denmark)

    Mortensen, Thomas Bøtker

    -Doerr, 1996) and has been shown to have a positive effect to the outcome of collaborative R&D (Sampson, 2005). Anand & Khanna (2000), furthermore, hypothesized that research joint ventures are more ambiguous than marketing joint ventures and even more the licensing and showed that the effect of collaborative......Literature review: Collaborative experience has been shown to have a positive effect on the collaborative outcome in general (Anand & Khanna, 2000; Kale, Dyer & Singh, 2002). Furthermore, it has been linked to the ability to exploit the network of the firm for learning (Powell, Koput and Smith...... experience was largest the higher the hypothesized ambiguity. Theoretically contribution: This research project aims at contributing to existing literature by arguing, that collaborative experience is a moderating variable which moderates the effects on collaborative outcome from the level of complexity...

  13. Memorable Experiences with Sad Music—Reasons, Reactions and Mechanisms of Three Types of Experiences

    Science.gov (United States)

    Peltola, Henna-Riikka

    2016-01-01

    Reactions to memorable experiences of sad music were studied by means of a survey administered to a convenience (N = 1577), representative (N = 445), and quota sample (N = 414). The survey explored the reasons, mechanisms, and emotions of such experiences. Memorable experiences linked with sad music typically occurred in relation to extremely familiar music, caused intense and pleasurable experiences, which were accompanied by physiological reactions and positive mood changes in about a third of the participants. A consistent structure of reasons and emotions for these experiences was identified through exploratory and confirmatory factor analyses across the samples. Three types of sadness experiences were established, one that was genuinely negative (Grief-Stricken Sorrow) and two that were positive (Comforting Sorrow and Sweet Sorrow). Each type of emotion exhibited certain individual differences and had distinct profiles in terms of the underlying reasons, mechanisms, and elicited reactions. The prevalence of these broad types of emotional experiences suggested that positive experiences are the most frequent, but negative experiences were not uncommon in any of the samples. The findings have implications for measuring emotions induced by music and fiction in general, and call attention to the non-pleasurable aspects of these experiences. PMID:27300268

  14. Experimenting with a design experiment

    Directory of Open Access Journals (Sweden)

    Bakker, Judith

    2012-12-01

    Full Text Available The design experiment is an experimental research method that aims to help design and further develop new (policy instruments. For the development of a set of guidelines for the facilitation of citizens’ initiatives by local governments, we are experimenting with this method. It offers good opportunities for modeling interventions by testing their instrumental validity –the usefulness for the intended practical purposes. At the same time design experiments are also useful for evaluating the empirical validity of theoretical arguments and the further development of these arguments in the light of empirical evidence (by using e.g. the technique of pattern matching. We describe how we have applied this methodology in two cases and discuss our research approach. We encountered some unexpected difficulties, especially in the cooperation with professionals and citizens. These difficulties complicate the valid attribution of causal effects to the use of the new instrument. However, our preliminary conclusion is that design experiments are useful in our field of study

    El experimento de diseño es un método de investigación experimental que tiene como objetivo diseñar y desarrollar posteriormente nuevas herramientas (políticas. En este artículo experimentamos con este método para desarrollar un conjunto de directrices que permitan a los gobiernos locales facilitar las iniciativas ciudadanas. El método ofrece la oportunidad de modelar las intervenciones poniendo a prueba su validez instrumental (su utilidad para el fin práctico que se proponen. Al mismo tiempo, los experimentos de diseño son útiles también para evaluar la validez empírica de las discusiones teóricas y el posterior desarrollo de esas discusiones a la luz de la evidencia empírica (usando, por ejemplo, técnicas de concordancia de patrones. En este trabajo describimos cómo hemos aplicado este método a dos casos y discutimos nuestro enfoque de

  15. Conducting interactive experiments online.

    Science.gov (United States)

    Arechar, Antonio A; Gächter, Simon; Molleman, Lucas

    2018-01-01

    Online labor markets provide new opportunities for behavioral research, but conducting economic experiments online raises important methodological challenges. This particularly holds for interactive designs. In this paper, we provide a methodological discussion of the similarities and differences between interactive experiments conducted in the laboratory and online. To this end, we conduct a repeated public goods experiment with and without punishment using samples from the laboratory and the online platform Amazon Mechanical Turk. We chose to replicate this experiment because it is long and logistically complex. It therefore provides a good case study for discussing the methodological and practical challenges of online interactive experimentation. We find that basic behavioral patterns of cooperation and punishment in the laboratory are replicable online. The most important challenge of online interactive experiments is participant dropout. We discuss measures for reducing dropout and show that, for our case study, dropouts are exogenous to the experiment. We conclude that data quality for interactive experiments via the Internet is adequate and reliable, making online interactive experimentation a potentially valuable complement to laboratory studies.

  16. LDR structural experiment definition

    Science.gov (United States)

    Russell, Richard A.; Gates, Richard M.

    1988-01-01

    A study was performed to develop the definition of a structural flight experiment for a large precision segmented reflector that would utilize the Space Station. The objective of the study was to use the Large Deployable Reflector (LDR) baseline configuration for focusing on experiment definition activity which would identify the Space Station accommodation requirements and interface constraints. Results of the study defined three Space Station based experiments to demonstrate the technologies needed for an LDR type structure. The basic experiment configurations are the same as the JPL baseline except that the primary mirror truss is 10 meters in diameter instead of 20. The primary objectives of the first experiment are to construct the primary mirror support truss and to determine its structural and thermal characteristics. Addition of the optical bench, thermal shield and primary mirror segments and alignment of the optical components occur on the second experiment. The structure will then be moved to the payload pointing system for pointing, optical control and scientific optical measurement for the third experiment.

  17. AGS experiments---1987, 1988, 1989

    International Nuclear Information System (INIS)

    Depken, J.C.

    1989-04-01

    This report contains: Experimental Areas Layout; Table of Beam Parameters and Fluxes; Experiment Schedule ''as run''; Experiment Long Range Schedule; A listing of experiments by number; Two-page summaries of each experiment begin here, also ordered by number; Publications of AGS experiments; and List of experimenters

  18. AGS experiments, 1988, 1989, 1990

    International Nuclear Information System (INIS)

    Depken, J.C.

    1991-04-01

    This report contains: experimental areas layout; table of beam parameters and fluxes; experiment schedule ''as run''; experiment long range schedule; a listing of experiments by number; two-page summaries of each experiment begin here, also ordered by number; publications of AGS experiments; and list of experimenters

  19. Aesthetic experience of dance performances

    Directory of Open Access Journals (Sweden)

    Vukadinović Maja

    2012-01-01

    Full Text Available In this study the aesthetic experience of dance performances is investigated. The study includes construction of an instrument for measuring the aesthetic experience of dance performances and an investigation of the structure of both dancers’ and spectators’ aesthetic experience. The experiments are carried out during eight different performances of various dance forms, including classical ballet, contemporary dance, flamenco and folklore. Three factors of aesthetic experience of dance performances are identified: Dynamism, Exceptionality and Affective Evaluation. The results show that dancers’ aesthetic experience has a somewhat different factorial structure from that of the spectators’. Unlike spectators’ aesthetic experience, dancers’ aesthetic experience singles out the Excitement factor. The results are discussed within the context of dancers’ proprioception and spectators’ exteroception since these findings confirm the idea of a significant role of proprioception in dancers’ aesthetic experience.

  20. Magnetic resonance on oriented 131I nuclei in iron

    International Nuclear Information System (INIS)

    Visser, D.

    1981-01-01

    In this thesis experiments are described on 131 I implanted into iron single crystals. It is shown that the magnetization behaviour of iron single crystals in an external magnetic field agrees with the macroscopic theory of domain structure in ferromagnets. This knowledge is used to give the influence of the external field on NMR measurements on the iodine. The iodine atoms that end up in regular lattice sites after the implantation give rise to a strong resonance. The discovery of much smaller satelite resonance, due to I nuclei experiencing a hyperfine field of 92% of that of atoms in regular lattice sites is reported. The splitting of this resonance by quadrupole interaction has enabled it to be identified as due to an implanted iodine atom with a missing nearest neighbour iron atom. The author has measured the relaxation of the iodine nuclei in iron single crystals for different crystallographic orientations. For the first time it is shown that the relaxation rate depends strongly on the magneto-crystalline anisotropy; a high rate results at a low external field. This behaviour can not be explained with the relaxation mechanisms discussed in the literature up till now. It is very likely that the low-field spin-lattice relaxation is largely determined by spin wave interactions, which are strongly field dependent. The anisotropic dispersion relation for these waves are derived, including the dependence on the state of magnetization of the sample. Finally a simple method is given to measure the power saturation of an NMR-ON resonance, from which the fraction of nuclei contributing to this resonance can be derived. (Auth.)

  1. The Challenging Experience Questionnaire: Characterization of challenging experiences with psilocybin mushrooms

    Science.gov (United States)

    Barrett, Frederick S.; Bradstreet, Matthew P.; Leoutsakos, Jeannie-Marie S.; Johnson, Matthew W.; Griffiths, Roland R.

    2017-01-01

    Acute adverse psychological reactions to classic hallucinogens (“bad trips”, or “challenging experiences”), while usually benign with proper screening, preparation, and support in controlled settings, remain a safety concern in uncontrolled settings (such as illicit use contexts). Anecdotal and case reports suggest potential adverse acute symptoms including affective (panic, depressed mood), cognitive (confusion, feelings of losing sanity), and somatic (nausea, heart palpitation) symptoms. Responses to items from several hallucinogen-sensitive questionnaires (Hallucinogen Rating Scale, the States of Consciousness Questionnaire, and the 5-Dimensional Altered States of Consciousness questionnaire) in an internet survey of challenging experiences with the classic hallucinogen psilocybin were used to construct and validate a Challenging Experience Questionnaire (CEQ). The stand-alone CEQ was then validated in a separate sample. Seven CEQ factors (grief, fear, death, insanity, isolation, physical distress, and paranoia) provide a phenomenological profile of challenging aspects of experiences with psilocybin. Factor scores were associated with the difficulty, meaningfulness, spiritual significance, and change in well-being attributed to the challenging experiences. The factor structure did not differ based on gender or prior struggle with anxiety or depression. The CEQ provides a basis for future investigation of predictors and outcomes of challenging experiences with psilocybin, and should be explored as a measure of challenging experiences with the broad class of classic hallucinogens. PMID:27856683

  2. Experiment prediction for LOFT nuclear experiments L5-1/L8-2

    International Nuclear Information System (INIS)

    Chen, T.H.; Modro, S.M.

    1982-01-01

    The LOFT Experiments L5-1 and L8-2 simulated intermediate break loss-of-coolant accidents with core uncovery. This paper compares the predictions with the measured data for these experiments. The RELAP5 code was used to perform best estimate double-blind and single-blind predictions. The double-blind calculations are performed prior to the experiment and use specified nominal initial and boundary conditions. The single-blind calculations are performed after the experiment and use measured initial and boundary conditions while maintaining all other parameters constant, including the code version. Comparisons of calculated results with experimental results are discussed; the possible causes of discrepancies are explored and explained. RELAP5 calculated system pressure, mass inventory, and fuel cladding temperature agree reasonably well with the experiment results, and only slight changes are noted between the double-blind and single-blind predictions

  3. Space Experiment Module (SEM)

    Science.gov (United States)

    Brodell, Charles L.

    1999-01-01

    The Space Experiment Module (SEM) Program is an education initiative sponsored by the National Aeronautics and Space Administration (NASA) Shuttle Small Payloads Project. The program provides nationwide educational access to space for Kindergarten through University level students. The SEM program focuses on the science of zero-gravity and microgravity. Within the program, NASA provides small containers or "modules" for students to fly experiments on the Space Shuttle. The experiments are created, designed, built, and implemented by students with teacher and/or mentor guidance. Student experiment modules are flown in a "carrier" which resides in the cargo bay of the Space Shuttle. The carrier supplies power to, and the means to control and collect data from each experiment.

  4. Radiochemical solar neutrino experiments

    International Nuclear Information System (INIS)

    Rich, R.; Spiro, M.

    1993-01-01

    This review covers the three presently running radiochemical solar neutrino experiments, namely the Chlorine, SAGE, and GALLEX experiments. The focus of the review is on a discussion of statistical consistency checks of the available data. The chlorine radiochemical experiment is conceptually simple and shows no strong indication of any statistical anomalies. It still forms the basis of the solar neutrino problem. Each of the two gallium experiments show internal statistical consistency. SAGE's recent preliminary results are consistent with the published GALLEX results. If this convergence is confirmed by a more definitive analysis, this would suggest that the combined result of the two gallium experiments, SAGE and GALLEX, be used for comparisons with theoretical expectations. 5 refs., 15 figs

  5. Inverse Cerenkov experiment

    International Nuclear Information System (INIS)

    Kimura, W.D.

    1993-01-01

    The final report describes work performed to investigate inverse Cherenkov acceleration (ICA) as a promising method for laser particle acceleration. In particular, an improved configuration of ICA is being tested in a experiment presently underway on the Accelerator Test Facility (ATF). In the experiment, the high peak power (∼ 10 GW) linearly polarized ATF CO 2 laser beam is converted to a radially polarized beam. This is beam is focused with an axicon at the Cherenkov angle onto the ATF 50-MeV e-beam inside a hydrogen gas cell, where the gas acts as the phase matching medium of the interaction. An energy gain of ∼12 MeV is predicted assuming a delivered laser peak power of 5 GW. The experiment is divided into two phases. The Phase I experiments, which were completed in the spring of 1992, were conducted before the ATF e-beam was available and involved several successful tests of the optical systems. Phase II experiments are with the e-beam and laser beam, and are still in progress. The ATF demonstrated delivery of the e-beam to the experiment in Dec. 1992. A preliminary ''debugging'' run with the e-beam and laser beam occurred in May 1993. This revealed the need for some experimental modifications, which have been implemented. The second run is tentatively scheduled for October or November 1993. In parallel to the experimental efforts has been ongoing theoretical work to support the experiment and investigate improvement and/or offshoots. One exciting offshoot has been theoretical work showing that free-space laser acceleration of electrons is possible using a radially-polarized, axicon-focused laser beam, but without any phase-matching gas. The Monte Carlo code used to model the ICA process has been upgraded and expanded to handle different types of laser beam input profiles

  6. The Game Experience Questionnaire

    NARCIS (Netherlands)

    IJsselsteijn, W.A.; de Kort, Y.A.W.; Poels, K.

    2013-01-01

    This document contains the English version of the Game Experience Questionnaire. The development and testing of the Game Experience Questionnaire is described in project Deliverable 3.3. The Game Experience Questionnaire has a modular structure and consists of : 1. The core questionnaire 2. The

  7. Do entheogen-induced mystical experiences boost the immune system? Psychedelics, peak experiences, and wellness.

    Science.gov (United States)

    Roberts, T B

    1999-01-01

    Daily events that boost the immune system (as indicated by levels of salivary immunoglobulin A), some instances of spontaneous remission, and mystical experiences seem to share a similar cluster of thoughts, feelings, moods, perceptions, and behaviors. Entheogens--psychedelic drugs used in a religious context--can also produce mystical experiences (peak experiences, states of unitive consciousness, intense primary religious experiences) with the same cluster of effects. When this happens, is it also possible that such entheogen-induced mystical experiences strengthen the immune system? Might spontaneous remissions occur more frequently under such conditions? This article advances the so called "Emxis hypothesis"--that entheogen-induced mystical experiences influence the immune system.

  8. Results of recent LOFT experiments

    International Nuclear Information System (INIS)

    Leach, L.P.; Hanson, D.J.; Batt, D.L.

    1982-01-01

    Five experiments were performed in the Loss-of-Fluid Test (LOFT) facility during the past year. The experiments conducted spanned a wide range of potential accident scenarios, including large and small break loss-of-coolant accidents (LOCAs), control rod withdrawal accidents, uncontrolled boron dilution, and anticipated transients without scram (ATWS). This summary describes these experiments and presents results available from the experiments and experiment prediction calculations. A brief overview is given for the remaining experiment planned in the LOFT Program

  9. CANDU operating experience

    International Nuclear Information System (INIS)

    McConnell, L.G.; Woodhead, L.W.; Fanjoy, G.R.; Thurygill, E.W.

    1980-05-01

    The CANDU-PHW program is based upon 38 years of heavy water reactor experience with 35 years of operating experience. Canada has had 72 reactor years of nuclear-electric operations experience with 10 nuclear units in 4 generating stations during a period of 18 years. All objectives have been met with outstanding performance: worker safety, public safety, environmental emissions, reliable electricity production, and low electricity cost. The achievement has been realized through total teamwork involving all scientific disciplines and all project functions (research, design, manufacturing, construction, and operation). (auth)

  10. Experience as Excursion

    DEFF Research Database (Denmark)

    Svabo, Connie; Shanks, Michael

    2014-01-01

    researchers and practitioners to travel – making it possible to follow experiences as they are enacted across and between places, modes of transportation, mobile mediation and assemblages of things. Drawing on the nomadic metaphysics of philosopher Michel Serres, the journeying, shifting and propagating...... qualities of experience are highlighted as part of a suggestion that design may indeed relate as much to metaphysics as to mechanics, materials science, and the psychology of the consumer and user. An Experience Design is sketched out as the choreography of temporary and shifting engagements across...

  11. Neutrino oscillation experiments

    International Nuclear Information System (INIS)

    Camilleri, L.

    1996-01-01

    Neutrino oscillation experiments (ν μ →ν e and ν μ →ν τ ) currently being performed at accelerators are reviewed. Future plans for short and long base-line experiments are summarized. (author) 10 figs., 2 tabs., 29 refs

  12. Experiment, right or wrong

    CERN Document Server

    Franklin, Allan

    2008-01-01

    In Experiment, Right or Wrong, Allan Franklin continues his investigation of the history and philosophy of experiment presented in his previous book, The Neglect of Experiment. In this new study, Franklin considers the fallibility and corrigibility of experimental results and presents detailed histories of two such episodes: 1) the experiment and the development of the theory of weak interactions from Fermi's theory in 1934 to the V-A theory of 1957 and 2) atomic parity violation experiments and the Weinberg-Salam unified theory of electroweak interactions of the 1970s and 1980s. In these episodes Franklin demonstrates not only that experimental results can be wrong, but also that theoretical calculations and the comparison between experiment and theory can also be incorrect. In the second episode, Franklin contrasts his view of an "evidence model" of science in which questions of theory choice, confirmation, and refutation are decided on the basis of reliable experimental evidence, with that proposed by the ...

  13. What Public Experience May Be – On Publicity, Communication and the Expression of Lived Experiences

    Directory of Open Access Journals (Sweden)

    Samuel Mateus

    2016-09-01

    Full Text Available The idea of public experience is often invoked in different social and academic contexts. However, it seldom deserved a reflection that specifically sought to deepen its meaning from the point of view of social life. In this article we contribute to the understanding of the uniqueness of the public form of experience. We believe that one of the best ways through which we can observe the public experience is by the objectification, performance and dramatization of the culture, i.e., the “expression of lived experiences”. There is, in publicity, the possibility of simultaneous allocation of individual and collective experiences, and it is in this sense that we can see how culture influences the shaping of experience itself. Public experience is characterized by the weaving and intertwining of singular experiences that are pluralized and plural lived experiences that are singularized, in a process where individual and society interpenetrate. The relationship between experience and publicity arises from this symbolic communion contained in the systems of thought and action of societies. The decisive role of the principle of publicity to experience consists, according with the hypothesis we wish to put forward, in making available and communicating the social world of symbolic (cultural activity. Public experience is, then, envisaged as the experience of a common world where both singular and plural definitions of the individual (taken as society converge through lived experiences and, particularly, through their expression, which can take different symbolic forms.

  14. Implanted-tritium permeation experiments

    International Nuclear Information System (INIS)

    Longhurst, G.R.; Holland, D.F.; Casper, L.A.; Hsu, P.Y.; Miller, L.G.; Schmunk, R.E.; Watts, K.D.; Wilson, C.J.; Kershner, C.J.; Rogers, M.L.

    1982-04-01

    In fusion reactors, charge exchange neutral atoms of tritium coming from the plasma will be implanted into the first wall and other interior structures. EG and G Idaho is conducting two experiments to determine the magnitude of permeation into the coolant streams and the retention of tritium in those structures. One experiment uses an ion gun to implant deuterium. The ion gun will permit measurements to be made for a variety of implantation energies and fluxes. The second experiment utilizes a fission reactor to generate a tritium implantation flux by the 3 He(n,p) 3 H reaction. This experiment will simulate the fusion reactor radiation environment. We also plan to verify a supporting analytical code development program, in progress, by these experiments

  15. The JESSICA experiment. Pt I. Improvements of the JESSICA-experiment

    Energy Technology Data Exchange (ETDEWEB)

    Nuenighoff, K.; Conrad, H.; Filges, D.; Goldenbaum, F.; Neef, R.D.; Pohl, Ch.; Schaal, H.; Stelzer, H.; Tietze-Jaensch, H.; Paul, N.; Wohlmuther, W. [Forschungszentrum Juelich GmbH, Juelich (Germany); Ninaus, W. [Technische Univ. Graz, Inst. fuer Technische Physik, Graz (Austria); Smirnov, A. [Joint Inst. of Nuclear Research, Dubna (Russian Federation)

    2004-03-01

    In this article we like to report on the progress of the JESSICA experiment. The experimental setup is described and the experimental method is presented. Proton beam monitoring and results from water and polyethylene will also be mentioned. In the end we give an outlook to the upcoming experiments with further cold moderator materials. (orig.)

  16. The JESSICA experiment. Part I. Improvements of the JESSICA-experiment

    International Nuclear Information System (INIS)

    Nuenighoff, K.; Conrad, H.; Filges, D.; Goldenbaum, F.; Neef, R.D.; Pohl, Ch.; Schaal, H.; Stelzer, H.; Tietze-Jaensch, H.; Paul, N.; Wohlmuther, W.; Ninaus, W.; Smirnov, A.

    2004-01-01

    In this article we like to report on the progress of the JESSICA experiment. The experimental setup is described and the experimental method is presented. Proton beam monitoring and results from water and polyethylene will also be mentioned. In the end we give an outlook to the upcoming experiments with further cold moderator materials. (orig.)

  17. The French experience

    CERN Document Server

    Bougard, Marie-Thérèse

    2003-01-01

    Developed for beginners, The French Experience 1 course book is designed to accompany the French Experience 1 CDs (9780563472582) but can also be used on its own to develop your reading and writing skills. You’ll gain valuable insights into French culture too.

  18. Neutrino oscillation experiments

    Energy Technology Data Exchange (ETDEWEB)

    Camilleri, L [European Organization for Nuclear Research, Geneva (Switzerland)

    1996-11-01

    Neutrino oscillation experiments ({nu}{sub {mu}}{yields}{nu}{sub e} and {nu}{sub {mu}}{yields}{nu}{sub {tau}}) currently being performed at accelerators are reviewed. Future plans for short and long base-line experiments are summarized. (author) 10 figs., 2 tabs., 29 refs.

  19. Future of neutrino experiments

    Indian Academy of Sciences (India)

    them are under construction. The next generation double beta decay experiments are sensitive to the inverted mass hierarchy. In order to explore the normal mass hierarchy, the sensitivity of the experiments still needs to be improved substantially. For example, see [32] for more details of the double beta decay experiments.

  20. AGS experiments - 1982, 1983, 1984

    International Nuclear Information System (INIS)

    Bunce, G.

    1983-01-01

    The report contains layouts of experimental areas, a table of beam parameters and fluxes, the experiment schedule as run, the experiment long range schedule, a listing of experiments by number, and a section of two-page summaries of each experiment

  1. Faktor-Faktor yang Mempengaruhi Pendapatan Rumah tangga Miskin di Sekitar Taman Nasional Bukit Dua Belas (Studi Kasus Desa-Desa Penyangga TNBD di Kecamatan Maro Sebo Ulu, Kabupaten Batang Hari

    Directory of Open Access Journals (Sweden)

    Rudi Syaf

    2013-10-01

    Full Text Available Poverty and forestry has inter-connected one another. Most of the poor people live in the urban area are closely interacted with forest. This fact has been showed in some studies which are clearly stated that poor people are mostly found nearby forest area. Bukit Dua Belas national park as one of national park in Jambi province had experienced drastical forest degradation for the last 20 years. Based on the data alalysis from Citra Satelite, the total of degraded forest area is approximately 69,825 ha or in average is 3,492 ha per year. It happens because of massive encroachment which is done by the local people in a purpose to open communities’ farming. The primary objective of this research is to analyze which factors has contributed to communities’ impovorishment around TNBD. The result of this study shows that the distance of farming, size of land,  the management and the status of land are the potential factor affecting the communities’ income significantly.   Keywords: national park, forestry, forest degradation, poor people

  2. Modulation of galactic and anomalous cosmic rays in the inner heliosphere

    Science.gov (United States)

    Heber, B.

    Our knowledge on how galactic and anomalous cosmic rays are modulated in the inner heliosphere has been dramatically enlarged due to measurements provided by several missions launched in the past ten years. The current paradigma of singly charged anomalous cosmic rays has been confirmed by recent measurements from the SAMPEX and ACE satelite. Ulysses explored the inner heliosphere at polar regions during the last solar minimum period and is heading again to high heliographic latitudes during the time of the conference in July, 2000. The Sun approaches maximum activity when the spacecraft is at high heliographic latitudes giving us for the first time the possibility to explore modulation of cosmic rays in the inner three-dimensional heliosphere during such conditions. Ulysses electron measurements in addition to the 1 AU ICE electron and IMP helium measurements allows us to investigate charge sign dependent modulation over a full 22-year solar magnetic cycle. Implications of these observations for our understanding of different modulation processes in the inner three-dimensional heliosphere are presented.

  3. Experience Supporting the Integration of LHC Experiments Software Framework with the LCG Middleware

    CERN Document Server

    Santinelli, Roberto

    2006-01-01

    The LHC experiments are currently preparing for data acquisition in 2007 and because of the large amount of required computing and storage resources, they decided to embrace the grid paradigm. The LHC Computing Project (LCG) provides and operates a computing infrastructure suitable for data handling, Monte Carlo production and analysis. While LCG offers a set of high level services, intended to be generic enough to accommodate the needs of different Virtual Organizations, the LHC experiments software framework and applications are very specific and focused on the computing and data models. The LCG Experiment Integration Support team works in close contact with the experiments, the middleware developers and the LCG certification and operations teams to integrate the underlying grid middleware with the experiment specific components. The strategical position between the experiments and the middleware suppliers allows EIS team to play a key role at communications level between the customers and the service provi...

  4. User Experience Dimensions

    DEFF Research Database (Denmark)

    Lykke, Marianne; Jantzen, Christian

    2016-01-01

    The present study develops a set of 10 dimensions based on a systematic understanding of the concept of experience as a holistic psychological. Seven of these are derived from a psychological conception of what experiencing and experiences are. Three supplementary dimensions spring from the obser...

  5. Social experience infrastructure

    DEFF Research Database (Denmark)

    Kvistgaard, Peter

    2006-01-01

    and explorative fashion to share with others thoughts and ideas concerning the development of new ways to construct/reconstruct recreational spaces with a better coherence with regard to designing experiences. This article claims that it is possible to design recreational spaces with good social experience...

  6. Materials science experiments in space

    Science.gov (United States)

    Gelles, S. H.; Giessen, B. C.; Glicksman, M. E.; Margrave, J. L.; Markovitz, H.; Nowick, A. S.; Verhoeven, J. D.; Witt, A. F.

    1978-01-01

    The criteria for the selection of the experimental areas and individual experiments were that the experiment or area must make a meaningful contribution to the field of material science and that the space environment was either an absolute requirement for the successful execution of the experiment or that the experiment can be more economically or more conveniently performed in space. A number of experimental areas and individual experiments were recommended for further consideration as space experiments. Areas not considered to be fruitful and others needing additional analysis in order to determine their suitability for conduct in space are also listed. Recommendations were made concerning the manner in which these materials science experiments are carried out and the related studies that should be pursued.

  7. Urban Experiments and Concrete Utopias

    DEFF Research Database (Denmark)

    Andersson, Lasse

    2009-01-01

    The paper explores how concrete urban experiments can challenge the pecuniary version of the experience city and stimulate a locally rooted and democratic version of an experience based city using heterotopias and concrete utopias as the link between top down planning and bottom up experiments...... administrations with public participation in order to shape a cultural agenda. The second part of the paper looks at two cases: NDSM in Amsterdam and Platform4 in Aalborg suggesting that it is concrete urban experiments like these that can create a link between visions and local reality in the Experience city...

  8. Experiments as politics

    NARCIS (Netherlands)

    Spears, R; Smith, HJ

    The purpose of this paper is to illustrate the political nature of laboratory experiments. Such experiments can be construed as paradigms of power, open to construction and debate, where different agents and interests are involved in a process of struggle over both (re)presentation and substance.

  9. THX Experiment Overview

    Science.gov (United States)

    Wernet, Mark; Wroblewski, Adam; Locke, Randy; Georgiadis, Nick

    2016-01-01

    This presentation provides an overview of experiments conducted at NASA GRC to provide turbulent flow measurements needed for new turbulence model development and validation. The experiments include particle image velocimetry (PIV) and hot-wire measurements of mean flow velocity and temperature fields, as well as fluctuating components.

  10. Activity Coefficients of Acetone-Chloroform Solutions: An Undergraduate Experiment. Undergraduate Experiment.

    Science.gov (United States)

    Ozog, J. Z.; Morrison, J. A.

    1983-01-01

    Presents information, laboratory procedures, and results of an undergraduate experiment in which activity coefficients for a two-component liquid-vapor system are determined. Working in pairs, students can perform the experiment with 10 solutions in a given three-hour laboratory period. (Author/JN)

  11. Experiments on ferrimagnetism

    International Nuclear Information System (INIS)

    Kraftmakher, Yaakov

    2013-01-01

    Ferrimagnetism undoubtedly deserves a proper place in the undergraduate laboratory on electricity and magnetism. Four student experiments on ferrimagnetism are considered: (i) the hysteresis loops and permeability of a ‘soft’ ferrite; (ii) the differential permeability versus a dc bias; (iii) the frequency dependence of the complex permeability and (iv) the electromagnetic interference suppression by ferrite chokes and beads. Two ferrite cores taken off a low-frequency choke and a power cord are used. The measurements are simple and straightforward and show the important properties of ferrites and their applications. The values of the permeability of the ferrite core determined in experiments (i)–(iii) are in reasonable agreement. The frequency dependence of the complex permeability of the ferrites is similar to that given by the manufacturers. The capability of absorbing electromagnetic waves in a definite frequency range shown in experiment (iv) demonstrates one of the principles of Stealth technology. The equipment necessary for the experiments can be found in many student laboratories. (paper)

  12. [The AMY experiment

    International Nuclear Information System (INIS)

    1989-01-01

    The AMY experiment is one of three major experiments at TRISTAN which is studying the states the matter produced in electron positron annihilations in the center of mass energy range of 50--65GeV. It provides information between the lower energy facilities such as PEP and PETRA and the new facilities SLC and LEP which are designed to operate in the region of the Z 0 mass near 90GeV. In the region of the AMY experiment, interaction cross sections are near their minimum of about 100pb, making it difficult to acquire large data samples during typical running cycles. This last year has seen an accumulation of about 10---12pb -1 of integrated luminosity in the energy range from 58 to 61.7GeV. Despite this limited data sample, the AMY experiment has been extremely active in attempting to extract the minimum amount of information from the data. Some of the most significant results are discussed in this paper. 9 refs

  13. Olkiluoto 3 Experience

    International Nuclear Information System (INIS)

    Tiippana, Petteri

    2011-01-01

    This paper discusses the experience from the Olkiluoto 3 nuclear power plant project from regulator's point of view. There are certain factors that have affected greatly the project progress. First, Olkiluoto 3 nuclear power plant is the first European Pressurised Reactor (EPR) being constructed. Secondly, construction of the unit started after a fairly long break in nuclear power plant construction in Europe, which had resulted in loss of experienced and qualified engineering and manufacturing resources. These factors have to be kept in mind when evaluating the experience from Olkiluoto 3. Experience discussed in this paper have to do with the licensing and regulatory oversight process, completion of the design prior to construction, experience and know-how of the participating organisations, quality management in a nuclear construction project, advanced manufacturing and construction technologies, turnkey contract with regard to licensee's responsibility, safety culture aspects in a nuclear construction project, and the role and importance of regulator's oversight. (author)

  14. Aura, Self, and Aesthetic Experience

    OpenAIRE

    Marshall Battani

    2011-01-01

    Aesthetic experiences are generated in encounters with cultural objects and such experiences are marked by the free play of cognitive and numinous experience unstructured by concepts. Kant’s famous three types of pleasure, made infamous in social theory by Pierre Bourdieu, are examined in relation to the critical theoretical concept of aura, the social psychology of “flow,” and cognitive explanations of perception to explain experience in aesthetic fields. Theories of aesthetic experience de...

  15. Experience and Its Generation

    Institute of Scientific and Technical Information of China (English)

    Chen Youqing

    2006-01-01

    Experience iS an activity that arouses emotions and generates meanings based on vivid sensation and profound compreh ension.It iS emotional,meaningful,and personal,playing a key role in the course of forming and developing one'S qualities.The psychological process of experience generation consists of such links as sensing things,arousing emotions,promoting comprehension and association,generating insights and meanings,and deepening emotional responses.Undergoing things personally by means of direct sensation,taking part in activities,and living life are the most important preconditions of experience generation.Emotional influence,situational edification,and arts edification ale extemal factors that induce experience generation.

  16. The G0 Experiment

    International Nuclear Information System (INIS)

    Nakahara, Kazutaka

    2007-01-01

    The G0 experiment measures the parity-violating asymmetries in elastic electron-proton and quasi-elastic electron-deuteron scattering over the momentum transfers 0.12 ≤ Q2 ≤ 1.0 GeV2. These asymmetries are sensitive to the strange-quark contribution to the charge and magnetization distributions of the proton. The experiment is conducted at Jefferson Laboratory using a toroidal spectrometer designed to detect forward scattered recoil protons and backward scattered elastic and quasi-elastic electrons. The forward angle experiment was completed in 2004, and the backward angle phase of the experiment is currently taking place

  17. ATLAS Experiment Brochure

    CERN Multimedia

    AUTHOR|(INSPIRE)INSPIRE-00085461

    2016-01-01

    ATLAS is one of the four major experiments at the Large Hadron Collider at CERN. It is a general-purpose particle physics experiment run by an international collaboration, and is designed to exploit the full discovery potential and the huge range of physics opportunities that the LHC provides.

  18. Peak Experience Project

    Science.gov (United States)

    Scott, Daniel G.; Evans, Jessica

    2010-01-01

    This paper emerges from the continued analysis of data collected in a series of international studies concerning Childhood Peak Experiences (CPEs) based on developments in understanding peak experiences in Maslow's hierarchy of needs initiated by Dr Edward Hoffman. Bridging from the series of studies, Canadian researchers explore collected…

  19. Experience with technology dynamics of user experience with mobile media devices

    CERN Document Server

    al-Azzawi, Ali

    2013-01-01

    With a focus on gaining an empirically derived understanding of the underlying psychological dimensions and processes behind people’s experiences with technology, this book contributes to the debate of user experience (UX) within several disciplines, including HCI, design and marketing. It analyses UX dynamics at various time scales, and explores the very nature of time and meaning in the context of UX.Experience with Technology uses personal construct theory (PCT) as a theoretical and methodological starting point to this project. Major case-studies are described that examine people’s exp

  20. AGS Experiments: 1989, 1990, 1991

    Energy Technology Data Exchange (ETDEWEB)

    Depken, J.C.

    1992-02-01

    This report contains: Experimental areas layout; table of beam parameters and fluxes; experiment schedule ``as run``; proposed 1992 schedule; a listing of experiments by number; two-page summaries of each experiment begin here, also ordered by number; publications of AGS Experiments begin here; and list of AGS Experimenters begins here.

  1. AGS Experiments: 1989, 1990, 1991

    International Nuclear Information System (INIS)

    Depken, J.C.

    1992-02-01

    This report contains: Experimental areas layout; table of beam parameters and fluxes; experiment schedule ''as run''; proposed 1992 schedule; a listing of experiments by number; two-page summaries of each experiment begin here, also ordered by number; publications of AGS Experiments begin here; and list of AGS Experimenters begins here

  2. AGS Experiments: 1989, 1990, 1991

    Energy Technology Data Exchange (ETDEWEB)

    Depken, J.C.

    1992-02-01

    This report contains: Experimental areas layout; table of beam parameters and fluxes; experiment schedule as run''; proposed 1992 schedule; a listing of experiments by number; two-page summaries of each experiment begin here, also ordered by number; publications of AGS Experiments begin here; and list of AGS Experimenters begins here.

  3. Welcome to the experience economy.

    Science.gov (United States)

    Pine, B J; Gilmore, J H

    1998-01-01

    First there was agriculture, then manufactured goods, and eventually services. Each change represented a step up in economic value--a way for producers to distinguish their products from increasingly undifferentiated competitive offerings. Now, as services are in their turn becoming commoditized, companies are looking for the next higher value in an economic offering. Leading-edge companies are finding that it lies in staging experiences. To reach this higher level of competition, companies will have to learn how to design, sell, and deliver experiences that customers will readily pay for. An experience occurs when a company uses services as the stage--and goods as props--for engaging individuals in a way that creates a memorable event. And while experiences have always been at the heart of the entertainment business, any company stages an experience when it engages customers in a personal, memorable way. The lessons of pioneering experience providers, including the Walt Disney Company, can help companies learn how to compete in the experience economy. The authors offer five design principles that drive the creation of memorable experiences. First, create a consistent theme, one that resonates throughout the entire experience. Second, layer the theme with positive cues--for example, easy-to-follow signs. Third, eliminate negative cues, those visual or aural messages that distract or contradict the theme. Fourth, offer memorabilia that commemorate the experience for the user. Finally, engage all five senses--through sights, sounds, and so on--to heighten the experience and thus make it more memorable.

  4. Nitrogen-detected CAN and CON experiments as alternative experiments for main chain NMR resonance assignments

    International Nuclear Information System (INIS)

    Takeuchi, Koh; Heffron, Gregory; Sun, Zhen-Yu J.; Frueh, Dominique P.; Wagner, Gerhard

    2010-01-01

    Heteronuclear direct-detection experiments, which utilize the slower relaxation properties of low γ nuclei, such as 13 C have recently been proposed for sequence-specific assignment and structural analyses of large, unstructured, and/or paramagnetic proteins. Here we present two novel 15 N direct-detection experiments. The CAN experiment sequentially connects amide 15 N resonances using 13 C α chemical shift matching, and the CON experiment connects the preceding 13 C' nuclei. When starting from the same carbon polarization, the intensities of nitrogen signals detected in the CAN or CON experiments would be expected four times lower than those of carbon resonances observed in the corresponding 13 C-detecting experiment, NCA-DIPAP or NCO-IPAP (Bermel et al. 2006b; Takeuchi et al. 2008). However, the disadvantage due to the lower γ is counteracted by the slower 15 N transverse relaxation during detection, the possibility for more efficient decoupling in both dimensions, and relaxation optimized properties of the pulse sequences. As a result, the median S/N in the 15 N observe CAN experiment is 16% higher than in the 13 C observe NCA-DIPAP experiment. In addition, significantly higher sensitivity was observed for those residues that are hard to detect in the NCA-DIPAP experiment, such as Gly, Ser and residues with high-field C α resonances. Both CAN and CON experiments are able to detect Pro resonances that would not be observed in conventional proton-detected experiments. In addition, those experiments are free from problems of incomplete deuterium-to-proton back exchange in amide positions of perdeuterated proteins expressed in D 2 O. Thus, these features and the superior resolution of 15 N-detected experiments provide an attractive alternative for main chain assignments. The experiments are demonstrated with the small model protein GB1 at conditions simulating a 150 kDa protein, and the 52 kDa glutathione S-transferase dimer, GST.

  5. The Cryogenic Test Bed experiments: Cryogenic heat pipe flight experiment CRYOHP (STS-53). Cryogenic two phase flight experiment CRYOTP (STS-62). Cryogenic flexible diode flight experiment CRYOFD

    Science.gov (United States)

    Thienel, Lee; Stouffer, Chuck

    1995-09-01

    This paper presents an overview of the Cryogenic Test Bed (CTB) experiments including experiment results, integration techniques used, and lessons learned during integration, test and flight phases of the Cryogenic Heat Pipe Flight Experiment (STS-53) and the Cryogenic Two Phase Flight Experiment (OAST-2, STS-62). We will also discuss the Cryogenic Flexible Diode Heat Pipe (CRYOFD) experiment which will fly in the 1996/97 time frame and the fourth flight of the CTB which will fly in the 1997/98 time frame. The two missions tested two oxygen axially grooved heat pipes, a nitrogen fibrous wick heat pipe and a 2-methylpentane phase change material thermal storage unit. Techniques were found for solving problems with vibration from the cryo-collers transmitted through the compressors and the cold heads, and mounting the heat pipe without introducing parasitic heat leaks. A thermally conductive interface material was selected that would meet the requirements and perform over the temperature range of 55 to 300 K. Problems are discussed with the bi-metallic thermostats used for heater circuit protection and the S-Glass suspension straps originally used to secure the BETSU PCM in the CRYOTP mission. Flight results will be compared to 1-g test results and differences will be discussed.

  6. Feel Experience Dan Think Experience Marketing Pengaruhnya Terhadap Loyalitas Konsumen Melalui Kepuasan Konsumen Sebagai Variabel Intervening

    Directory of Open Access Journals (Sweden)

    Asti Hidayati

    2017-12-01

      Key Word: feel experience, think experience marketing, customer loyalty, customer satisfaction   Abstrak : Penelitian ini bertujuan untuk mengetahui pengaruh langsung dan pengaruh tidak langsung feel experience dan think experience marketing terhadap loyalitas konsumen melalui kepuasan konsumen sebagai variabel intervening. Metode penelitian yang digunakan adalah metode kuantitatif. Jumlah sampel dalam penelitian ini sebanyak 100 responden, teknik pengambilan sampel menggunakan teknik sampling insidental. Teknik penarikan data menggunakan kuesioner. Teknik analisis data dilakukan dengan menggunakan analisis jalur (Path Analysis. Hasil penelitian ini menunjukkan bahwa feel experience mempunyai pengaruh langsung terhadap loyalitas konsumen. Think experience marketing mempunyai pengaruh tidak langsung terhadap loyalitas konsumen.    Kata  kunci: feel experience, think experience marketing, loyalitas konsumen, kepuasan konsumen

  7. Galactic signatures of decaying dark matter

    International Nuclear Information System (INIS)

    Zhang, Le; Sigl, Guenter

    2009-05-01

    If dark matter decays into electrons and positrons, it can affect Galactic radio emissions and the local cosmic ray fluxes. We propose a new, more general analysis of constraints on dark matter. The constraints can be obtained for any decaying dark matter model by convolving the specific dark matter decay spectrum with a response function. We derive this response function from full-sky radio surveys at 408 MHz, 1.42 GHz and 23 GHz, as well as from the positron flux recently reported by PAMELA. We discuss the influence of astrophysical uncertainties on the response function, such as from propagation and from the profiles of the dark matter and the Galactic magnetic field. As an application, we find that some widely used dark matter decay scenarios can be ruled out under modest assumptions. (orig.)

  8. Cosmic Ray Signatures of Decaying Dark Matter

    International Nuclear Information System (INIS)

    Ibarra, Alejandro

    2011-01-01

    Astrophysical and cosmological observations do not require the dark matter particles to be absolutely stable. If they are indeed unstable, their decay into Standard Model particles might occur at a sufficiently large rate to allow the indirect detection of dark matter through an anomalous contribution to the high energy cosmic ray fluxes. We analyze the implications of the excess in the total electron plus positron flux and the positron fraction reported by the Fermi and PAMELA collaborations, respectively, for the scenario of decaying dark matter. We also discuss the constraints on this scenario from measurements of other cosmic ray species and the predictions for the diffuse gamma ray flux and the neutrino flux. In particular, we expect a sizable dipole-like anisotropy which may be observed in the near future by the Fermi-LAT.

  9. The PyZgoubi framework and the simulation of dynamic aperture in fixed-field alternating-gradient accelerators

    International Nuclear Information System (INIS)

    Tygier, S.; Appleby, R.B.; Garland, J.M.; Hock, K.; Owen, H.; Kelliher, D.J.; Sheehy, S.L.

    2015-01-01

    We present PyZgoubi, a framework that has been developed based on the tracking engine Zgoubi to model, optimise and visualise the dynamics in particle accelerators, especially fixed-field alternating-gradient (FFAG) accelerators. We show that PyZgoubi abstracts Zgoubi by wrapping it in an easy-to-use Python framework in order to allow simple construction, parameterisation, visualisation and optimisation of FFAG accelerator lattices. Its object oriented design gives it the flexibility and extensibility required for current novel FFAG design. We apply PyZgoubi to two example FFAGs; this includes determining the dynamic aperture of the PAMELA medical FFAG in the presence of magnet misalignments, and illustrating how PyZgoubi may be used to optimise FFAGs. We also discuss a robust definition of dynamic aperture in an FFAG and show its implementation in PyZgoubi

  10. The PyZgoubi framework and the simulation of dynamic aperture in fixed-field alternating-gradient accelerators

    Energy Technology Data Exchange (ETDEWEB)

    Tygier, S., E-mail: sam.tygier@hep.manchester.ac.uk [Cockcroft Accelerator Group, The University of Manchester (United Kingdom); Appleby, R.B., E-mail: robert.appleby@manchester.ac.uk [Cockcroft Accelerator Group, The University of Manchester (United Kingdom); Garland, J.M. [Cockcroft Accelerator Group, The University of Manchester (United Kingdom); Hock, K. [University of Liverpool (United Kingdom); Owen, H. [Cockcroft Accelerator Group, The University of Manchester (United Kingdom); Kelliher, D.J.; Sheehy, S.L. [STFC Rutherford Appleton Laboratory (United Kingdom)

    2015-03-01

    We present PyZgoubi, a framework that has been developed based on the tracking engine Zgoubi to model, optimise and visualise the dynamics in particle accelerators, especially fixed-field alternating-gradient (FFAG) accelerators. We show that PyZgoubi abstracts Zgoubi by wrapping it in an easy-to-use Python framework in order to allow simple construction, parameterisation, visualisation and optimisation of FFAG accelerator lattices. Its object oriented design gives it the flexibility and extensibility required for current novel FFAG design. We apply PyZgoubi to two example FFAGs; this includes determining the dynamic aperture of the PAMELA medical FFAG in the presence of magnet misalignments, and illustrating how PyZgoubi may be used to optimise FFAGs. We also discuss a robust definition of dynamic aperture in an FFAG and show its implementation in PyZgoubi.

  11. Galactic signatures of decaying dark matter

    Energy Technology Data Exchange (ETDEWEB)

    Zhang, Le; Sigl, Guenter [Hamburg Univ. (Germany). II. Inst. fuer Theoretische Physik; Redondo, Javier [Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany)

    2009-05-15

    If dark matter decays into electrons and positrons, it can affect Galactic radio emissions and the local cosmic ray fluxes. We propose a new, more general analysis of constraints on dark matter. The constraints can be obtained for any decaying dark matter model by convolving the specific dark matter decay spectrum with a response function. We derive this response function from full-sky radio surveys at 408 MHz, 1.42 GHz and 23 GHz, as well as from the positron flux recently reported by PAMELA. We discuss the influence of astrophysical uncertainties on the response function, such as from propagation and from the profiles of the dark matter and the Galactic magnetic field. As an application, we find that some widely used dark matter decay scenarios can be ruled out under modest assumptions. (orig.)

  12. HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess

    Energy Technology Data Exchange (ETDEWEB)

    Hooper, Dan [Fermilab; Cholis, Ilias [Johns Hopkins U.; Linden, Tim [Ohio State U., CCAPP; Fang, Ke [Maryland U.

    2017-11-17

    Recent measurements of the Geminga and B0656+14 pulsars by the gamma-ray telescope HAWC (along with earlier measurements by Milagro) indicate that these objects generate significant fluxes of very high-energy electrons. In this paper, we use the very high-energy gamma-ray intensity and spectrum of these pulsars to calculate and constrain their expected contributions to the local cosmic-ray positron spectrum. Among models that are capable of reproducing the observed characteristics of the gamma-ray emission, we find that pulsars invariably produce a flux of high-energy positrons that is similar in spectrum and magnitude to the positron fraction measured by PAMELA and AMS-02. In light of this result, we conclude that it is very likely that pulsars provide the dominant contribution to the long perplexing cosmic-ray positron excess.

  13. Gamma ray constraints on flavor violating asymmetric dark matter

    DEFF Research Database (Denmark)

    Masina, I.; Panci, P.; Sannino, F.

    2012-01-01

    We show how cosmic gamma rays can be used to constrain models of asymmetric Dark Matter decaying into lepton pairs by violating flavor. First of all we require the models to explain the anomalies in the charged cosmic rays measured by PAMELA, Fermi and H.E.S.S.; performing combined fits we...... determine the allowed values of the Dark Matter mass and lifetime. For these models, we then determine the constraints coming from the measurement of the isotropic gamma-ray background by Fermi for a complete set of lepton flavor violating primary modes and over a range of DM masses from 100 GeV to 10 Te......V. We find that the Fermi constraints rule out the flavor violating asymmetric Dark Matter interpretation of the charged cosmic ray anomalies....

  14. KSC-04PD-2209

    Science.gov (United States)

    2004-01-01

    KENNEDY SPACE CENTER, FLA. Lockheed Martin representatives explain some of the activities they are working on for safe Return to Flight of the Space Shuttle. The exhibit was one of many presented to KSC employees during Spaceport Super Safety and Health Day. Vendors exhibits were set up in the parking areas outside the Vehicle Assembly Building and the O&C Building. The day-long event also featured presentations by guest speakers Dr. Pamela Peeke, Navy Com. Stephen E. Iwanowicz, NASAs Dr. Kristine Calderon and Olympic-great Bruce Jenner. Super Safety and Health Day was initiated at KSC in 1998 to increase awareness of the importance of safety and health among the government and contractor workforce. The theme for this years event was Safety and Health: A Winning Combination.

  15. Experiment prediction for LOFT nuclear experiments L5-1 and L8-2

    International Nuclear Information System (INIS)

    Chen, T.H.; Modro, S.M.

    1983-01-01

    The LOFT Experiments L5-1 and L8-2 simulated intermediate break loss-of-coolant accidents with core uncovery. This paper compares the predictions with the measured data for these experiments. The RELAP5 code was used to perform best estimate double-blind and single-blind predictions. The double-blind calculations are performed prior to the experiment and use specified nominal initial and boundary conditions. The single-blind calculations are performed after the experiment and use measured initial and boundary conditions while maintaining all other parameters constant, including the code version. Comparisons of calculated results with experimental results are discussed; the possible causes of discrepancies are explored and explained. RELAP5 calculated system pressure, mass inventory, and fuel cladding temperature agree reasonably well with the experiment results, and only slight changes are noted between the double-blind and single-blind predictions

  16. Dashboard for the LHC experiments

    International Nuclear Information System (INIS)

    Andreeva, J; Cirstoiu, C; Miguel, M D F D; Ivanchenko, A; Gaidioz, B; Herrala, J; Janulis, M; Maier, G; Maguire, E J; Rivera, R P; Rocha, R; Saiz, P; Sidorova, I; Belov, S; Berejnoj, A; Kodolova, O; Chen, Y; Chen, T; Chiu, S; Munro, C

    2008-01-01

    In this paper we present the Experiment Dashboard monitoring system, which is currently in use by four Large Hadron Collider (LHC) experiments. The goal of the Experiment Dashboard is to monitor the activities of the LHC experiments on the distributed infrastructure, providing monitoring data from the virtual organization (VO) and user perspectives. The LHC experiments are using various Grid infrastructures (LCG/EGEE, OSG, NDGF) with correspondingly various middleware flavors and job submission methods. Providing a uniform and complete view of various activities like job processing, data movement and publishing, access to distributed databases regardless of the underlying Grid flavor is the challenging task. In this paper we will describe the Experiment Dashboard concept, its framework and main monitoring applications

  17. Free-electron laser experiments in the microwave tokamak experiment

    International Nuclear Information System (INIS)

    Allen, S.L.; Brown, M.D.; Byers, J.A.; Casper, T.A.; Cohen, B.I.; Cohen, R.H.; Cummings, J.C.; Fenstermacher, M.E.; Foote, J.H.; Hooper, E.B.; Jong, R.A.; Langdon, A.B.; Lasinski, B.F.; Lasnier, C.J.; Matsuda, Y.; Meyer, W.H.; Moller, J.M.; Nexsen, W.E.; Rice, B.W.; Rognlien, T.D.; Smith, G.R.; Stallard, B.W.; Thomassen, K.I.; Throop, A.L.; Turner, W.C.; Wood, R.D.; Cook, D.R.; Makowski, M.A.; Oasa, K.; Ogawa, T.

    1990-08-01

    Microwave pulses have been injected from a free electron-laser (FEL) into the Microwave Tokamak Experiment (MTX) at up to 0.2 GW at 140 GHz in short pulses (10-ns duration) with O-mode polarization. The power transmitted through the plasma was measured in a first experimental study of high power pulse propagation in the plasma; no nonlinear effects were found at this power level. Calculations indicate that nonlinear effects may be found at the higher power densities expected in future experiments. 9 refs., 2 figs

  18. Tracking System : Suaineadh satellite experiment

    OpenAIRE

    Brengesjö, Carl; Selin, Martine

    2011-01-01

    The purpose of this bachelor thesis is to present a tracking system for the Suaineadh satellite experiment. The experiment is a part of the REXUS (Rocket EXperiments for University Students) program and the objective is to deploy a foldable web in space. The assignment of this thesis is to develop a tracking system to find the parts from the Suaineadh experiment that will land on Earth. It is important to find the parts and recover all the data that the experiment performed during the travel ...

  19. Sampling Participants' Experience in Laboratory Experiments: Complementary challenges for more complete data collection

    Directory of Open Access Journals (Sweden)

    Alan eMcAuliffe

    2016-05-01

    Full Text Available Speelman and McGann's (2013 examination of the uncritical way in which the mean is often used in psychological research raises questions both about the average's reliability and its validity. In the present paper, we argue that interrogating the validity of the mean involves, amongst other things, a better understanding of the person's experiences, the meaning of their actions, at the time that the behaviour of interest is carried out. Recently emerging approaches within Psychology and Cognitive Science have argued strongly that experience should play a more central role in our examination of behavioural data, but the relationship between experience and behaviour remains very poorly understood. We outline some of the history of the science on this fraught relationship, as well as arguing that contemporary methods for studying experience fall into one of two categories. Wide approaches tend to incorporate naturalistic behaviour settings, but sacrifice accuracy and reliability in behavioural measurement. Narrow approaches maintain controlled measurement of behaviour, but involve too specific a sampling of experience, which obscures crucial temporal characteristics. We therefore argue for a novel, mid-range sampling technique, that extends Hurlburt's Descriptive Experience Sampling, and adapts it for the controlled setting of the laboratory. This Controlled Descriptive Experience Sampling may be an appropriate tool to help calibrate both the mean and the meaning of an experimental situation with one another.

  20. Particle physics experiments 1988

    International Nuclear Information System (INIS)

    Bairstow, R.

    1989-01-01

    This report describes work carried out in 1988 on experiments approved by the Particle Physics Experiments Selection Panel. The contents consist of unedited contributions from each experiment. More than forty projects at different accelerators (SPS, ISIS, PETRA, LAMPF, LEP, HERA, BNL, ILL, LEAR) are listed. Different organisations collaborate on different projects. A brief progress report is given. References to published articles are given. (author)

  1. Overview of Experiments for Physics of Fast Reactors from the International Handbooks of Evaluated Criticality Safety Benchmark Experiments and Evaluated Reactor Physics Benchmark Experiments

    Energy Technology Data Exchange (ETDEWEB)

    Bess, J. D.; Briggs, J. B.; Gulliford, J.; Ivanova, T.; Rozhikhin, E. V.; Semenov, M. Yu.; Tsibulya, A. M.; Koscheev, V. N.

    2017-07-01

    Overview of Experiments to Study the Physics of Fast Reactors Represented in the International Directories of Critical and Reactor Experiments John D. Bess Idaho National Laboratory Jim Gulliford, Tatiana Ivanova Nuclear Energy Agency of the Organisation for Economic Cooperation and Development E.V.Rozhikhin, M.Yu.Sem?nov, A.M.Tsibulya Institute of Physics and Power Engineering The study the physics of fast reactors traditionally used the experiments presented in the manual labor of the Working Group on Evaluation of sections CSEWG (ENDF-202) issued by the Brookhaven National Laboratory in 1974. This handbook presents simplified homogeneous model experiments with relevant experimental data, as amended. The Nuclear Energy Agency of the Organization for Economic Cooperation and Development coordinates the activities of two international projects on the collection, evaluation and documentation of experimental data - the International Project on the assessment of critical experiments (1994) and the International Project on the assessment of reactor experiments (since 2005). The result of the activities of these projects are replenished every year, an international directory of critical (ICSBEP Handbook) and reactor (IRPhEP Handbook) experiments. The handbooks present detailed models of experiments with minimal amendments. Such models are of particular interest in terms of the settlements modern programs. The directories contain a large number of experiments which are suitable for the study of physics of fast reactors. Many of these experiments were performed at specialized critical stands, such as BFS (Russia), ZPR and ZPPR (USA), the ZEBRA (UK) and the experimental reactor JOYO (Japan), FFTF (USA). Other experiments, such as compact metal assembly, is also of interest in terms of the physics of fast reactors, they have been carried out on the universal critical stands in Russian institutes (VNIITF and VNIIEF) and the US (LANL, LLNL, and others.). Also worth mentioning

  2. The OLYMPUS experiment

    Energy Technology Data Exchange (ETDEWEB)

    Milner, R.; Hasell, D.K. [Massachusetts Institute of Technology, Cambridge, MA (United States); Kohl, M. [Hampton Univ., Hampton, VA (United States); Collaboration: The OLYMPUS Collaboration; and others

    2013-12-15

    The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross sections, with the goal of determining the contribution of two-photon exchange to the elastic cross section. Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, {mu}{sub p}G{sup p}{sub E}/G{sup p}{sub M}, made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01 GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately 25 -75 . Symmetric Moeller/Bhabha calorimeters at 1.29 and telescopes of GEM and MWPC detectors at 12 served as luminosity monitors. A total luminosity of approximately 4.5 fb{sup -1} was collected over two running periods in 2012. This paper provides details on the accelerator, target, detectors, and operation of the experiment.

  3. Magnetized gun experiments

    International Nuclear Information System (INIS)

    Jarboe, T.R.; Henins, I.; Hoida, H.W.; Marshall, J.; Sherwood, A.R.

    1981-01-01

    In the Los Alamos Magnetized Gun Experiment we are attempting to produce a compact torus in a manner similar to an earlier experiment of Alfven. In our experiment a solenoidal coil is placed inside the inner electrode of a coaxial plasma gun. This coil produces an axial magnetic field inside the inner electrode which diverges and becomes a largely radial field in front of the gun muzzle. The idea is that when the gun is fired, the plasma escaping from the gun stretches these radial fields along the axial direction away from the gun, and these field lines can reconnect behind the plasma forming the poloidal field of the compact torus. The magnetic field generated by the gun current becomes the toroidal field and the major axis of the compact torus will be the same as the axis of the coaxial gun. Recent interest in this possible method of compact torus generation was stimulated by C. Hartman, and the approach is also being pursued in the field-reversed plasma gun experiment at LLL

  4. The OLYMPUS experiment

    International Nuclear Information System (INIS)

    Milner, R.; Hasell, D.K.; Kohl, M.

    2013-12-01

    The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross sections, with the goal of determining the contribution of two-photon exchange to the elastic cross section. Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, μ p G p E /G p M , made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01 GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately 25 -75 . Symmetric Moeller/Bhabha calorimeters at 1.29 and telescopes of GEM and MWPC detectors at 12 served as luminosity monitors. A total luminosity of approximately 4.5 fb -1 was collected over two running periods in 2012. This paper provides details on the accelerator, target, detectors, and operation of the experiment.

  5. The OLYMPUS experiment

    Science.gov (United States)

    Milner, R.; Hasell, D. K.; Kohl, M.; Schneekloth, U.; Akopov, N.; Alarcon, R.; Andreev, V. A.; Ates, O.; Avetisyan, A.; Bayadilov, D.; Beck, R.; Belostotski, S.; Bernauer, J. C.; Bessuille, J.; Brinker, F.; Buck, B.; Calarco, J. R.; Carassiti, V.; Cisbani, E.; Ciullo, G.; Contalbrigo, M.; D'Ascenzo, N.; De Leo, R.; Diefenbach, J.; Donnelly, T. W.; Dow, K.; Elbakian, G.; Eversheim, D.; Frullani, S.; Funke, Ch.; Gavrilov, G.; Gläser, B.; Görrissen, N.; Hauschildt, J.; Henderson, B. S.; Hoffmeister, Ph.; Holler, Y.; Ice, L. D.; Izotov, A.; Kaiser, R.; Karyan, G.; Kelsey, J.; Khaneft, D.; Klassen, P.; Kiselev, A.; Krivshich, A.; Lehmann, I.; Lenisa, P.; Lenz, D.; Lumsden, S.; Ma, Y.; Maas, F.; Marukyan, H.; Miklukho, O.; Movsisyan, A.; Murray, M.; Naryshkin, Y.; O'Connor, C.; Perez Benito, R.; Perrino, R.; Redwine, R. P.; Rodríguez Piñeiro, D.; Rosner, G.; Russell, R. L.; Schmidt, A.; Seitz, B.; Statera, M.; Thiel, A.; Vardanyan, H.; Veretennikov, D.; Vidal, C.; Winnebeck, A.; Yeganov, V.

    2014-03-01

    The OLYMPUS experiment was designed to measure the ratio between the positron-proton and electron-proton elastic scattering cross-sections, with the goal of determining the contribution of two-photon exchange to the elastic cross-section. Two-photon exchange might resolve the discrepancy between measurements of the proton form factor ratio, μpGEp/GMp, made using polarization techniques and those made in unpolarized experiments. OLYMPUS operated on the DORIS storage ring at DESY, alternating between 2.01 GeV electron and positron beams incident on an internal hydrogen gas target. The experiment used a toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight detectors to measure rates for elastic scattering over the polar angular range of approximately 25°-75°. Symmetric Møller/Bhabha calorimeters at 1.29° and telescopes of GEM and MWPC detectors at 12° served as luminosity monitors. A total luminosity of approximately 4.5 fb-1 was collected over two running periods in 2012. This paper provides details on the accelerator, target, detectors, and operation of the experiment.

  6. AGS experiments -- 1991, 1992, 1993

    International Nuclear Information System (INIS)

    Depken, J.C.

    1994-04-01

    This report contains: (1) FY 1993 AGS schedule as run; (2) FY 1994--95 AGS schedule; (3) AGS experiments ≥ FY 1993 (as of 30 March 1994); (4) AGS beams 1993; (5) AGS experimental area FY 1991 physics program; (6) AGS experimental area FY 1992 physics program; (7) AGS experimental area FY 1993 physics program; (8) AGS experimental area FY 1994 physics program (planned); (9) a listing of experiments by number; (10) two-page summaries of each experiment; (11) listing of publications of AGS experiments; and (12) listing of AGS experiments

  7. AGS experiments: 1990, 1991, 1992

    International Nuclear Information System (INIS)

    Depken, J.C.

    1993-04-01

    This report contains a description of the following: AGS Experimental Area - High Energy Physics FY 1993 and Heavy Ion Physics FY 1993; Table of Beam Parameters and Fluxes; Experiment Schedule ''as run''; Proposed 1993 Schedule; A listing of experiments by number; Two-page summaries of each experiment begin here, also ordered by number; Publications of AGS Experiments; and List of AGS Experimenters

  8. Molybdenum solar neutrino experiment

    International Nuclear Information System (INIS)

    Wolfsberg, K.; Cowan, G.A.; Bryant, E.A.

    1984-01-01

    The goal of the molybdenum solar neutrino experiment is to deduce the 8 B solar neutrino flux, averaged over the past several million years, from the concentration of 98 Tc in a deeply buried molybdenum deposit. The experiment is important to an understanding of stellar processes because it will shed light on the reason for the discrepancy between theory and observation of the chlorine solar neutrino experiment. Possible reasons for the discrepancy may lie in the properties of neutrinos (neutrino oscillations or massive neutrinos) or in deficiencies of the standard solar model. The chlorine experiment only measures the 8 B neutrino flux in current times and does not address possible temporal variations in the interior of the sun, which are also not considered in the standard model. In the molybdenum experiment, we plan to measure 98 Tc (4.2 Myr), also produced by 8 B neutrinos, and possibly 97 Tc (2.6 Myr), produced by lower energy neutrinos

  9. Undergraduate reactor control experiment

    International Nuclear Information System (INIS)

    Edwards, R.M.; Power, M.A.; Bryan, M.

    1992-01-01

    A sequence of reactor and related experiments has been a central element of a senior-level laboratory course at Pennsylvania State University (Penn State) for more than 20 yr. A new experiment has been developed where the students program and operate a computer controller that manipulates the speed of a secondary control rod to regulate TRIGA reactor power. Elementary feedback control theory is introduced to explain the experiment, which emphasizes the nonlinear aspect of reactor control where power level changes are equivalent to a change in control loop gain. Digital control of nuclear reactors has become more visible at Penn State with the replacement of the original analog-based TRIGA reactor control console with a modern computer-based digital control console. Several TRIGA reactor dynamics experiments, which comprise half of the three-credit laboratory course, lead to the control experiment finale: (a) digital simulation, (b) control rod calibration, (c) reactor pulsing, (d) reactivity oscillator, and (e) reactor noise

  10. Cryogenics for LHC experiments

    CERN Multimedia

    2001-01-01

    Cryogenic systems will be used by LHC experiments to maximize their performance. Institutes around the world are collaborating with CERN in the construction of these very low temperature systems. The cryogenic test facility in hall 180 for ATLAS magnets. High Energy Physics experiments have frequently adopted cryogenic versions of their apparatus to achieve optimal performance, and those for the LHC will be no exception. The two largest experiments for CERN's new flagship accelerator, ATLAS and CMS, will both use large superconducting magnets operated at 4.5 Kelvin - almost 270 degrees below the freezing point of water. ATLAS also includes calorimeters filled with liquid argon at 87 Kelvin. For the magnets, the choice of a cryogenic version was dictated by a combination economy and transparency to emerging particles. For the calorimeters, liquid argon was selected as the fluid best suited to the experiment's physics requirements. High Energy Physics experiments are the result of worldwide collaborations and...

  11. Penggunaan Citra Satelit untuk Mengetahui Persebaran Dacrycarpus imbricatus (Blume de Laub. di Bukit Tapak, Cagar Alam Batukahu Bali

    Directory of Open Access Journals (Sweden)

    Rajif Iryadi

    2017-07-01

    Full Text Available Pleaides image is an important asset to obtain data and information with regard to the structure of the vegetation in the forest that are difficult to measure directly as the area is inaccessible and has a large coverage. Dacrycarpus imbricatus (Blume de Laub. is the one of typical plants on the Tapak Hill which has the conservation and economic values. This study aimed to determine the location and distribution of D. imbricatus using Pleaides satellite image that had a high spatial resolution. The determination of site characteristics was conducted by visual interpretation of high resolution satellite imagery Pleiades 2014 and elevation spatial data. Pleaides accuracy in the identification cover of D. imbricatus reached 96.83% and total accuracy mapping reached 93.38% with kappa coefficient of 88.64%. The distribution of D. imbricatus in Tapak Hill showed actual habitat range narrower than of its potential, which was distributed on the elevation of 1,321 – 1,800 m asl with a percentage of 89,52% from its total cover. About 79.29% of the coverage laid on the slope of 25.1 to 55%, whereas the rest on the slope of >25%. This information is important related to sustainability and conservation efforts for this gymnosperm plant in Tapak Hill.

  12. Fourier Imaging X-ray Spectrometer (FIXS) for the Argentinian, Scout-launched satelite de Aplicaciones Cienficas-1 (SAC-1)

    International Nuclear Information System (INIS)

    Dennis, B.R.; Crannell, C.J.; Desai, U.D.

    1988-01-01

    The Fourier Imaging X-ray Spectrometer (FIXS) is one of four instruments on SAC-1, the Argentinian satellite being proposed for launch by NASA on a Scout rocket in 1992/3. The FIXS is designed to provide solar flare images at X-ray energies between 5 and 35 keV. Observations will be made on arcsecond size scales and subsecond time scales of the processes that modify the electron spectrum and the thermal distribution in flaring magnetic structures

  13. MENENTUKAN VARIABILITAS SPASIAL ALBEDOPADA WILAYAH BALI MENGGUNAKAN DATA SATELIT MODIS BRDF MCD43A1 TAHUN 2005 - 2012

    Directory of Open Access Journals (Sweden)

    Ni Wayan Meri Monika Sari

    2015-02-01

    Full Text Available A research has been conducted to determine the variability of the albedo in Bali using MODIS BRDF MCD43A1 satellite data started from 2005 until 2012. The data used in this study is MODIS BRDF MCD43A1 data and MODIS Aerosol Optical Depth data. From MODIS BRDF MCD43A1 data, black sky and white sky albedo were calculated. The results of black sky and white sky albedo combined together and with MODISAerosol Optical Depth data to find the blue sky albedo (actual albedo, then monthly average of blue sky albedoused todetermine the spatial albedo variability in Bali. Spatial annual variability of actual albedo in Bali during 2005 – 2012 reached the highest peak in 2008 and lowest in 2010. Monthly average of actual albedo started from September-October while the lowest is in January - February.  Keywords: Albedo, MODIS BRDF MCD43A1, MODIS Aerosol Optical Depth, Black Sky albedo, White Sky Albedo, Blue Sky Albedo (Actual Albedo

  14. ALGUNAS APLICACIONES RECIENTES DE LA TÉCNICA DE RADIO OCULTAMIENTO SATELITAL EN EL ESTUDIO DE PROCESOS ATMOSFÉRICOS

    Directory of Open Access Journals (Sweden)

    Alejandro de la Torre

    2013-12-01

    Full Text Available In the last years, the use of radio occultation (RO technique to observe the terrestrial atmosphere and the climate takes advantage of the occultation of the Sun, the Moon, the stars and principally of artificial satellites of low height (LEO. In the latter case, crossed signs between LEO and GPS satellites are used. The application of RO's technology using transmitters of the GPS system in high orbits and recipients on board of low orbit satellites, has provided profiles of atmospheric refractivity very precise. The basic idea of a RO is to observe how waves emitted by a GPS are propagated in the atmosphere. The ray trajectory associated to a radio wave between a GPS and a LEO, while these are hiding themselves mutually due to the interposition of the Earth, is deviated due to refractivity gradients. The ray bending angle is obtained from a change in the phase (Doppler shift of the signal received by the LEO. Assuming spherical symmetry, the deviation information may be inverted by an Abel transformation to obtain a vertical profile of the index of refraction. From atmospheric profiles of refractivity and an atmospheric model, several parameters are obtained: from temperature (T, pressure, geopotential height and water vapor to minor species as aerosols, cloud liquid water and ionospheric electron density. The enormous advantage offered by the coverage in the whole planet, above the continental and oceanic territories, the 1K T resolution, the long term stability and mainly the absence of any restriction imposed by climatic conditions, makes the GPS RO technique unique among different remote sensing atmospheric systems. Up to now, hundreds of thousands of soundings have been processed, from the first satellites to recent (SAC-C, CHAMP, GRACE, COSMIC, TerraSAR-X, MetOp. In the present work, examples of global and regional water vapor and atmospheric wave energy distributions will be shown. It will be put on special emphasis on the mountainous regions of the Andes Range at middle latitudes and the Antarctic Peninsula and case studies will be analyzed. This analysis will be complemented by WRF model simulations and with measured T profiles in the regions of interest. In particular it will be shown: i the spatial distribution of stationary gravity waves, ii their propagation in the lower and middle atmospheres, and iii the possible relevance of mountain waves as a triggering mechanism of seep convection processes with hail production. Key words: satellite radio occultation, gravity waves.

  15. ALGUNAS APLICACIONES RECIENTES DE LA TÉCNICA DE RADIO OCULTAMIENTO SATELITAL EN EL ESTUDIO DE PROCESOS ATMOSFÉRICOS

    Directory of Open Access Journals (Sweden)

    Pedro

    2013-12-01

    Full Text Available SOME RECENT APPLICATIONS OF RADIO OCCULTATIONTECHNIQUE IN ATMOSPHERIC PROCESES Abstract In the last years, the use of radio occultation (RO technique to observe the terrestrial atmosphere and the climate takes advantage of the occultation of the Sun, the Moon, the stars and principally of artificial satellites of low height (LEO. In the latter case, crossed signs between LEO and GPS satellites are used. The application of RO's technology using transmitters of the GPS system in high orbits and recipients on board of low orbit satellites, has provided profiles of atmospheric refractivity very precise. The basic idea of a RO is to observe how waves emitted by a GPS are propagated in the atmosphere. The ray trajectory associated to a radio wave between a GPS and a LEO, while these are hiding themselves mutually due to the interposition of the Earth, is deviated due to refractivity gradients. The ray bending angle is obtained from a change in the phase (Doppler shift of the signal received by the LEO. Assuming spherical symmetry, the deviation information may be inverted by an Abel transformation to obtain a vertical profile of the index of refraction. From atmospheric profiles of refractivity and an atmospheric model, several parameters are obtained: from temperature (T, pressure, geopotential height and water vapor to minor species as aerosols, cloud liquid water and ionospheric electron density. The enormous advantage offered by the coverage in the whole planet, above the continental and oceanic territories, the 1K T resolution, the long term stability and mainly the absence of any restriction imposed by climatic conditions, makes the GPS RO technique unique among different remote sensing atmospheric systems. Up to now, hundreds of thousands of soundings have been processed, from the first satellites to recent (SAC-C, CHAMP, GRACE, COSMIC, TerraSAR-X, MetOp. In the present work, examples of global and regional water vapor and atmospheric wave energy distributions will be shown. It will be put on special emphasis on the mountainous regions of the Andes Range at middle latitudes and the Antarctic Peninsula and case studies will be analyzed. This analysis will be complemented by WRF model simulations and with measured T profiles in the regions of interest. In particular it will be shown: i the spatial distribution of stationary gravity waves, ii their propagation in the lower and middle atmospheres, and iii the possible relevance of mountain waves as a triggering mechanism of seep convection processes with hail production. Key words: satellite radio occultation, gravity waves.

  16. Critical experiment study on uranyl nitrate solution experiment facility

    International Nuclear Information System (INIS)

    Zhu Qingfu; Shi Yongqian; Wang Jinrong

    2005-01-01

    The Uranyl Nitrate Solution Experiment Facility was constructed for the research on nuclear criticality safety. In this paper, the configuration of the facility is introduced; a series of critical experiments on uranyl nitrate solution is described later, which were performed for various uranium concentrations under different conditions, i.e. with or without neutron absorbers in the core and with or without water-reflector outside the core. Critical volume and the minimum 235U critical mass for different uranium concentrations are presented. Finally, theoretical analysis is made on the experimental results. (authors)

  17. Touch massage, a rewarding experience.

    Science.gov (United States)

    Lindgren, Lenita; Jacobsson, Maritha; Lämås, Kristina

    2014-12-01

    This study aims to describe and analyze healthy individuals' expressed experiences of touch massage (TM). Fifteen healthy participants received whole body touch massage during 60 minutes for two separate occasions. Interviews were analyzed by narrative analysis. Four identifiable storyline was found, Touch massage as an essential need, in this storyline the participants talked about a desire and need for human touch and TM. Another storyline was about, Touch massage as a pleasurable experience and the participants talked about the pleasure of having had TM. In the third storyline Touch massage as a dynamic experience, the informants talked about things that could modulate the experience of receiving TM. In the last storyline, Touch massage influences self-awareness, the participants described how TM affected some of their psychological and physical experiences. Experiences of touch massage was in general described as pleasant sensations and the different storylines could be seen in the light of rewarding experiences. © The Author(s) 2014.

  18. Physical experience enhances science learning.

    Science.gov (United States)

    Kontra, Carly; Lyons, Daniel J; Fischer, Susan M; Beilock, Sian L

    2015-06-01

    Three laboratory experiments involving students' behavior and brain imaging and one randomized field experiment in a college physics class explored the importance of physical experience in science learning. We reasoned that students' understanding of science concepts such as torque and angular momentum is aided by activation of sensorimotor brain systems that add kinetic detail and meaning to students' thinking. We tested whether physical experience with angular momentum increases involvement of sensorimotor brain systems during students' subsequent reasoning and whether this involvement aids their understanding. The physical experience, a brief exposure to forces associated with angular momentum, significantly improved quiz scores. Moreover, improved performance was explained by activation of sensorimotor brain regions when students later reasoned about angular momentum. This finding specifies a mechanism underlying the value of physical experience in science education and leads the way for classroom practices in which experience with the physical world is an integral part of learning. © The Author(s) 2015.

  19. 1. Introduction. 2. Laboratory experiments. 3. Field experiments. 4. Integrated field-laboratory experiments. 5. Panel recommendations

    International Nuclear Information System (INIS)

    Anon.

    1975-01-01

    Some recommendations for the design of laboratory and field studies in marine radioecology are formulated. The difficulties concerning the comparability of various experimental methods used to measure the fluxes of radionuclides through marine organisms and ecosystems, and also the use of laboratory results to make predictions for the natural environment are discussed. Three working groups were established during the panel meeting, to consider laboratory experiments, field studies, and the design and execution of integrated laboratory and field studies respectively. A number of supporting papers dealing with marine radioecological experiments were presented

  20. Poetic Experience

    Directory of Open Access Journals (Sweden)

    Shahab Yar Khan

    2014-01-01

    Full Text Available Nature of poetic experience is hereby redefined. The present article initially deals with the perennial nature of true poetic experience and its essential relevance to the world. It attempts to elaborate the process through which a poet is uplifted in a creative moment beyond terrestrial boundaries and is aligned with the ‘state of Perfection'. The role of successive generations of audiences in rediscovering the meaning of a poetic image is defined as life principle of all great poetry. Shakespeare is discussed as the ultimate example of this principle since his popularity remains an irreversible phenomenon