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24 results on '"Panasyuk, M"'

1. Data acquisition system for the TUNKA-133 array

Author

Budnev, N. M., Chvalaev, O. B., Gress, O. A., Kalmykov, N. N., Kozhin, V. A., Korosteleva, E. E., Kuzmichev, L. A., Lubsandorzhiev, B. K., Mirgazov, R. R., Navarra, G., Panasyuk, M. I., Pankov, L. V., Prosin, V. V., Ptuskin, V. S., Semeney, Y. A., Skurikhin, A. V., Shaibonov, B. A., Spiering, Ch., Wischnewski, R., Yashin, I. V., Zablotsky, A. Z., and Zagorodnikov, A. V. more...

Subjects
Astrophysics
Abstract

The new EAS Cherenkov array TUNKA-133, with about 1 km**2 sensitive area, is being installed in the Tunka Valley. The investigated energy range is 10**15-10**18 eV. It will consist of 133 optical detectors based on EMI9350 PMTs. Optical detectors are grouped into 19 clusters with 7 detectors each. The detectors are connected to the cluster box with RG-58 cables. Every PMT signal is digitized in the cluster box with 200 MHz FADC. The cluster boxes are connected to the data acquisition center with a 1 Gb/s optical link. A detailed description of the data acquisition system (DAQ) is presented., Comment: 5 pages, 4 figures, Proceedings of the 10th ICATPP Conference,Como Italy, 8-12 October 2007 more...

Published
2008
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2. Tunka-133 EAS Cherenkov Array: Status of 2007

Author

Budnev, N. M., Chvalaev, O. V., Gress, O. A., Kalmykov, N. N., Kozhin, V. A., Korosteleva, E. E., Kuzmichev, L. A., Lubsandorzhiev, B. K., Mirgazov, R. R., Navarra, G., Panasyuk, M. I., Pankov, L. V., Prosin, V. V., Ptuskin, V. S., Semeney, Y. A., Skurikhin, A. V., Shaibonov, B. A., Spiering, Ch., Wieschnewski, R., Yashin, I. V., Zablotsky, A. V., and Zagorodnikov, A. V. more...

Subjects
Astrophysics
Abstract

The new EAS Cherenkov array Tunka-133, with about 1 km**2 sensitive area, is being installed in the Tunka Valley since the end of 2005. This array will permit a detailed study of the cosmic ray energy spectrum and the mass composition in the energy range of 10**15-10**18 eV with a unique method. The array will consist of 19 clusters, each composed of 7 optical detectors. The first cluster started operation in October 2006. We describe the data acquisition system and present preliminary results from data taken with the first cluster., Comment: 4 pages, 4 figures, Proceedings of 30th ICRC, Merinda, Mexico, July 2007 more...

Published
2008

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3. Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)

Author

Panov, A. D., Sokolskaya, N. V., Adams, Jr., J. H., Ahn, H. S., Bashindzhagyan, G. L., Batkov, K. E., Chang, J., Christl, M., Fazely, A. R., Ganel, O., Gunasingha, R. M., Guzik, T. G., Isbert, J., Kim, K. C., Kouznetsov, E. N., Panasyuk, M. I., Schmidt, W. K. H., Seo, E. S., Watts, J., Wefel, J. P., Wu, J., and Zatsepin, V. I. more...

Subjects
Astrophysics
Abstract

The ATIC balloon-borne experiment measures the energy spectra of elements from H to Fe in primary cosmic rays from about 100 GeV to 100 TeV. ATIC is comprised of a fully active bismuth germanate calorimeter, a carbon target with embedded scintillator hodoscopes, and a silicon matrix that is used as the main charge detector. The silicon matrix produces good charge resolution for protons and helium but only partial resolution for heavier nuclei. In the present paper, the charge resolution of ATIC was improved and backgrounds were reduced in the region from Be to Si by using the upper layer of the scintillator hodoscope as an additional charge detector. The flux ratios of nuclei B/C, C/O, N/O in the energy region from about 10 GeV/nucleon to 300 GeV/nucleon obtained from this high-resolution, high-quality charge spectra are presented, and compared with existing theoretical predictions., Comment: 4 pages,2 figures, a paper for 30-th International Cosmic Rays Conference more...

Published
2007

4. The results of ATIC-2 experiment for elemental spectra of cosmic rays

Author

Panov, A. D., Adams, J. H., Ahn, H. S., Bashindzhagyan, G. L., Batkov, K. E., Chang, J., Christl, M., Fazely, A. R., Ganel, O., Gunashingha, R. M., Guzik, T. G., Isbert, J., Kim, K. C., Kouznetsov, E. N., Panasyuk, M. I., Schmidt, W. K. H., Seo, E. S., Sokolskaya, N. V., Watts, John W., Wefel, J. P., Wu, J., and Zatsepin, V. I. more...

Subjects
Astrophysics
Abstract

The results of ATIC-2 baloon experiment (2002-2003) for energy spectra of protons, He, C, O, Ne, Mg, Si, Fe, some groups of nuclei, and all-particle spectrum in primary cosmic rays are presented in energy region 50GeV--200TeV. The conclusion is that the spectra of protons and helium nuclei are essentially different (the spectrum of protons is steeper) and the spectra of protons and heavy nuclei have no-power form., Comment: 7 pages, 3 figures, report on 29-th Russian Cosmic Rays Conference, to be published in Bull.Russ.Acad.Sci., Phys more...

Published
2006

5. The Tunka Experiment: Towards a 1-km^2 EAS Cherenkov Light Array in the Tunka Valley

Author

Budnev, N. M., Chernov, D. V., Gress, O. A., Kalmykov, N. N., Kozhin, V. A., Korosteleva, E. E., Kuzmichev, L. A., Lubsandorzhiev, B. K., Navarra, G., Panasyuk, M. I., Pankov, L. V., Parfenov, Yu. V., Prosin, V. V., Ptuskin, V. S., Semeney, Yu. A., Shirokov, A. V., Skurikhin, A. V., Spiering, C., Wischnewski, R., and Yashin, I. V. more...

Subjects
Astrophysics
Abstract

The project of an EAS Cherenkov array in the Tunka valley/Siberia with an area of about 1 km2 is presented. The new array will have a ten times bigger area than the existing Tunka-25 array and will permit a detailed study of the cosmic ray energy spectrum and the mass composition in the energy range from 10^15 to 10^18 eV., Comment: 4 pages, 2 figures, ICRC2005, rus-kuzmichev-LA-abs1-he15-poster more...

Published
2005

6. The Tunka Experiment: Towards a 1-km^2 Cherenkov EAS Array in the Tunka Valley

Author

Chernov, D., Kalmykov, N., Korosteleva, E., Kuzmichev, L., Prosin, V., Panasyuk, M., Shirokov, A., Yashin, I., Budnev, N., Gress, O., Pankov, L., Parfenov, Yu., Semeney, Yu., Lubsandorzhiev, B., Pohil, P., Ptuskin, V., Spiering, Ch., Wischnewski, R., and Navarra, G. more...

Subjects
Astrophysics
Abstract

The project of an EAS Cherenkov array in the Tunka valley/Siberia with an area of about 1 km^2 is presented. The new array will have a ten times bigger area than the existing Tunka-25 array and will permit a detailed study of the cosmic ray energy spectrum and the mass composition in the energy range from 10^15 to 10^18 eV., Comment: 3 pages, 2 figures, to be published in IJMPA more...

Published
2004
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7. The Cosmic Ray Electron Excess

Author

Chang, J, Adams, J. H, Ahn, H. S, Bashindzhagyan, G. L, Christl, M, Ganel, O, Guzik, T. G, Isbert, J, Kim, K. C, Kuznetsov, E. N, Panasyuk, M. I, Panov, A. D, Schmidt, W. K. H, Seo, E. S, Sokolskaya, N. V, Watts, J. W, Wefel, J. P, Wu, J, and Zatsepin, V. I more...

Subjects
Astrophysics
Abstract

This slide presentation reviews the possible sources for the apparent excess of Cosmic Ray Electrons. The presentation reviews the Advanced Thin Ionization Calorimeter (ATIC) instrument, the various parts, how cosmic ray electrons are measured, and shows graphs that review the results of the ATIC instrument measurement. A review of Cosmic Ray Electrons models is explored, along with the source candidates. Scenarios for the excess are reviewed: Supernova remnants (SNR) Pulsar Wind nebulae, or Microquasars. Each of these has some problem that mitigates the argument. The last possibility discussed is Dark Matter. The Anti-Matter Exploration and Light-nuclei Astrophysics (PAMELA) mission is to search for evidence of annihilations of dark matter particles, to search for anti-nuclei, to test cosmic-ray propagation models, and to measure electron and positron spectra. There are slides explaining the results of Pamela and how to compare these with those of the ATIC experiment. Dark matter annihilation is then reviewed, which represent two types of dark matter: Neutralinos, and kaluza-Kline (KK) particles, which are next explained. The future astrophysical measurements, those from GLAST LAT, the Alpha Magnetic Spectrometer (AMS), and HEPCAT are reviewed, in light of assisting in finding an explanation for the observed excess. Also the Compact Muon Solenoid (CMS) experiment at the Large Hadron Collider (LHC) could help by revealing if there are extra dimensions. more...

Published
2008
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8. All-Particle Spectrum Measured by the ATIC Experiment

Author

Ahn, H. S, Adams, J. H, Bashindzhagyan, G, Batkov, K. E, Chang, J, Christl, M, Fazely, A. R, Ganel, O, Gunasingha, R. M, Guzik, T. G, Isbert, J, Kouznetsov, E, Panasyuk, M, Panov, A, Schmidt, W. K. H, Seo, E. S, Sinai, R, Sokolskaya, N. V, Wang, J. Z, Wefel, J. P, Wu, J, and Zatsepin, V more...

Subjects
Astrophysics
Abstract

The Advanced Thin Ionization Calorimeter (ATIC), a balloon-borne experiment, is designed to investigate the composition and energy spectra of cosmic rays of charge Z = 1 to 26 over the energy range - 10(exp 11) - 10(exp 14) ev. The instrument consists of a silicon matrix charge detector, plastic-scintillator strip hodoscopes interleaved with graphite interaction targets, and an 18 radiation length deep, fully active bismuth germanate (BGO) calorimeter. ATIC has had two successful long duration balloon (LDB) flights launched from McMurdo Station, Antarc't'ica in 2000 and 2002. In this paper, we present the all-particle spectrum extracted from data collected during the ATIC flights, and compare it with results from other experiments at both lower and higher energies. more...

Published
2007

9. Relative Fluxes of Primary Particles in B-C-N-O Group from the ATIC Experiment (Science Flight)

Author

Panov, A. D, Adams, J. H., Jr, Ahn, H. S, Bashindzhagyan, G. L, Chang, J, Christl, M, Fazely, A. R, Ganel, O, Gunashingha, R. M, Guzik, T. G, Isbert, J, Kim, K. C, Kouznetsov, E. N, Panasyuk, M. I, Schmidt, W. K. H, Seo, E. S, Sokolskaya, N. V, Watts, John W, Wefel, J. P, Wu, J, and Zatsepin, V. I more...

Subjects
Astrophysics
Abstract

The ATIC balloon-born experiment measures the energy spectra of elements from H to Fe in primary cosmic rays from about 100 GeV to 100 TeV. ATIC is comprised of a fully active bismuth germinate calorimeter, a carbon target with embedded scintillator hodoscopes, and a silicon matrix that is used as a main charge detector. The silicon matrix produces good charge resolution for the protons and helium but only a partial resolution for heavier nuclei. In the present paper a charge resolution of ATIC device was improved and backgrounds were reduced in the region from Be to Si by means of the upper layer of the scintillator hodoscope that was used as charge detector together with silicon matrix. Relative fluxes of nuclei B, C, N, O in the energy region from about 20 GeV/nucleon to 200 GeV/nucleon that were obtained from new high-resolution and high-quality charge spectra of nuclei are presented. more...

Published
2007

10. A Neutron Detector for the Electron Calorimeter (ECAL) Long Duration Balloon Experiment

Author

Adams, J. H., Jr, Bashindzhagyan, G. L, Binns, W. R, Chang, J, Cherry, M. L, Christl, M. J, Guzik, t. G, Isbert, J, Israel, M. H, Korotkova, N, Panasyuk, M. I, Panov, A, Sokolskaya, N. V, Watts, J. W, Wefel, J. P, and Zatsepin, V more...

Subjects
Astrophysics
Abstract

The highest energy measurements of cosmic ray electrons extend just beyond 1 TeV. High energy electrons are of particular interest because energy losses during interstellar propagation insure that they arrive primarily from nearby sources. This may produce observable structure in their spectrum. Further, it is predicted that electrons and positrons result from the annihilation of many exotic particles deposited as dark matter candidates. These electrons may appear as excesses in the cosmic ray electron spectrum from 200 GeV to 1000 GeV. A new long duration balloon experiment, ECAL, is being planned to provide direct cosmic ray electron measurements from approx.50 GeV to >1 TeV. To make these measurements ECAL must discriminate strongly against showers from protons and heavier ions. One of the techniques used to make this discrimination may be based on measuring the secondary neutrons produced by events in the instrument. The neutron detector configuration and technique will be discussed along with its expected performance based on Monte Carlo simulations. more...

Published
2007

11. Revised Energy Spectra for Primary Elements, H - Si, above 50 GeV from the ATIC-2 Science Flight

Author

Wefel, J. P, Adams, J. H., Jr, Ahn, H. S, Bashindzhagyan, G. L, Chang, J, Christl, M, Fazely, A. R, Ganel, O, Gunashingha, R. M, Guzik, T. G, Isbert, J, Kim, K. C, Kouznetsov, E. N, Panasyuk, M. I, Panov, A. D, Schmidt, W. K. H, Seo, E. S, Sokolskaya, N. V, Watts, J. W, Wu, J, and Zatsepin, V. I more...

Subjects
Astrophysics
Abstract

The Advanced Thin Ionization Calorimeter (ATIC) long duration balloon experiment had a successful science flight accumulating 18 days of data (12/02 - 1/03) during a single circumnavigation in Antarctica. ATIC measures the energy spectra of elements from H to Fe in primary cosmic rays using a fully active Bismuth Germanate calorimeter preceded by a carbon target, with embedded scintillator hodoscopes, and a silicon matrix charge detector at the top. Preliminary results from ATIC have been reported in previous conferences. The revised results reported here are derived from a new analysis of the data with improved charge resolution, lower background and revised energy calibration. The raw energy deposit spectra are de-convolved into primary energy spectra and extrapolated to the top of the atmosphere. We compare these revised results to previous data and comment upon the astrophysical interpretation of the results. more...

Published
2007

12. The Mechanism Responsible for High Concentrations of Be-7 in the Near Space

Author

Panasyuk, M. I, Nymmik, R. A, Kuzhevskii, B. M, Kulikauskas, V. S, Zhuravlev, D. A, Phillips, G. W, Share, G. H, King, S. E, August, R. A, Tylka, A. J, and Whitaker, Ann F

Subjects
Astrophysics
Abstract

In 1990 an unexpectedly high concentration of Be-7 was discovered on the LDEF satellite surface, facing in the RAM direction. The search for an explanation of this high concentration of Be-7 which is in thermal equilibrium in the upper atmosphere, led the researchers to the hypothesis of Be-7 transport by vertical turbulent fluxes from deeper layers in the Earth's atmosphere, where Be-7 is produced as a result of nuclear reactions between solar energetic protons (which penetrated there after a solar flare) and terrestrial atmosphere elements. The experiments carried out during 1995-1999 on 'Resource F1' and 'Cosmos' satellites not only confirmed the existence of high Be-7 concentrations at altitudes of about 200 km, but also permitted to establish correlation between the concentration of Be-7 in the upper atmosphere and flare activity on the Sun. More detailed analysis of the whole set of experimental data on Be-7 measurements at satellite altitudes showed, that the appearance of high Be-7 concentrations in the upper atmosphere of the Earth is a more complicated phenomenon. Two more mechanisms , explaining the observed effect can be indicated. Firstly, the observed concentrations could be associated with direct penetration of energetic Be-7 nuclei, originating in flares, into the terrestrial atmosphere. Calculations show, that in solar cosmic rays the flux of Be-7 nuclei should be maximum in comparison to the fluxes of other Beryllium isotopes. Secondly, the high concentration of Be-7 in the upper atmosphere of the Earth could be explained by solar wind penetration through the polar zones. Theoretical analysis of active processes including flares, occurring in the solar atmosphere, leads to the conclusion, that radioactive Beryllium is constantly present in the solar atmosphere, and, possibly, is the main isotope of solar Beryllium. more...

Published
2001

13. An excess of cosmic ray electrons at energies of 300–800 GeV.

Author

Chang, J., Adams, J. H., Ahn, H. S., Bashindzhagyan, G. L., Christl, M., Ganel, O., Guzik, T. G., Isbert, J., Kim, K. C., Kuznetsov, E. N., Panasyuk, M. I., Panov, A. D., Schmidt, W. K. H., Seo, E. S., Sokolskaya, N. V., Watts, J. W., Wefel, J. P., Wu, J., and Zatsepin, V. I. more...

Subjects
GALACTIC cosmic rays, COMPTON electrons, SYNCHROTRONS, PULSARS, QUASARS, DARK matter, RELATIVISTIC particles, KALUZA-Klein theories, ASTROPHYSICS
Abstract

Galactic cosmic rays consist of protons, electrons and ions, most of which are believed to be accelerated to relativistic speeds in supernova remnants. All components of the cosmic rays show an intensity that decreases as a power law with increasing energy (for example as E-2.7). Electrons in particular lose energy rapidly through synchrotron and inverse Compton processes, resulting in a relatively short lifetime (about 105 years) and a rapidly falling intensity, which raises the possibility of seeing the contribution from individual nearby sources (less than one kiloparsec away). Here we report an excess of galactic cosmic-ray electrons at energies of ∼300–800 GeV, which indicates a nearby source of energetic electrons. Such a source could be an unseen astrophysical object (such as a pulsar or micro-quasar) that accelerates electrons to those energies, or the electrons could arise from the annihilation of dark matter particles (such as a Kaluza–Klein particle with a mass of about 620 GeV). [ABSTRACT FROM AUTHOR] more...

Published
2008
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14. Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)

Author

Panov, A. D., Sokolskaya, N. V., Adams Jr, J. H., Ahn, H. S., Bashindzhagyan, G. L., Batkov, K. E., Chang, J., Christl, M., Fazely, A. R., Ganel, O., Gunasingha, R. M., Guzik, T. G., Isbert, J., Kim, K. C., Kouznetsov, E. N., Panasyuk, M. I., Schmidt, W. K. H., Eun-Suk Seo, Watts, J., Wefel, J. P., Wu, J., and Zatsepin, V. I. more...

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), FOS: Physical sciences, High Energy Physics::Experiment, Astrophysics, Nuclear Experiment
Abstract

The ATIC balloon-borne experiment measures the energy spectra of elements from H to Fe in primary cosmic rays from about 100 GeV to 100 TeV. ATIC is comprised of a fully active bismuth germanate calorimeter, a carbon target with embedded scintillator hodoscopes, and a silicon matrix that is used as the main charge detector. The silicon matrix produces good charge resolution for protons and helium but only partial resolution for heavier nuclei. In the present paper, the charge resolution of ATIC was improved and backgrounds were reduced in the region from Be to Si by using the upper layer of the scintillator hodoscope as an additional charge detector. The flux ratios of nuclei B/C, C/O, N/O in the energy region from about 10 GeV/nucleon to 300 GeV/nucleon obtained from this high-resolution, high-quality charge spectra are presented, and compared with existing theoretical predictions., Comment: 4 pages,2 figures, a paper for 30-th International Cosmic Rays Conference more...

15. The orbital TUS detector simulation.

Author

Grinyuk, A., Grebenyuk, V., Khrenov, B., Klimov, P., Lavrova, M., Panasyuk, M., Sharakin, S., Shirokov, A., Tkachenko, A., Tkachev, L., and Yashin, I.

Subjects
*COSMIC rays, *ATMOSPHERIC radiation, *DETECTORS, *ALGORITHMS, *ASTROPHYSICS
Abstract

The TUS space experiment is aimed at studying energy and arrival distribution of UHECR at E > 7 × 10 19 eV by using the data of EAS fluorescent radiation in atmosphere. The TUS mission was launched at the end of April 2016 on board the dedicated “Lomonosov” satellite. The TUSSIM software package has been developed to simulate performance of the TUS detector for the Fresnel mirror optical parameters, the light concentrator of the photo detector, the front end and trigger electronics. Trigger efficiency crucially depends on the background level which varies in a wide range: from 0.2 × 10 6 to 15 × 10 6 ph/( m 2 μ s sr) at moonless and full moon nights respectively. The TUSSIM algorithms are described and the expected TUS statistics is presented for 5 years of data collection from the 500 km solar-synchronized orbit with allowance for the variability of the background light intensity during the space flight. [ABSTRACT FROM AUTHOR] more...

Published
2017
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16. A telescope for observation from space of extreme lightnings in the upper atmosphere

Author

Nam, S., Artikova, S., Chung, T., Garipov, G., Jeon, J.A., Jeong, S., Jin, J.Y., Khrenov, B.A., Kim, J.E., Kim, M., Kim, Y.K., Klimov, P., Lee, J., Lee, H.Y., Na, G.W., Oh, S.J., Panasyuk, M., Park, I.H., Park, J.H., and Park, Y.-S. more...

Subjects
*ASTROPHYSICS, *SPACE telescopes, *MICROELECTROMECHANICAL systems, *COSMIC rays
Abstract

Abstract: A new type of telescope with a wide field-of-view and functions of fast zoom-in has been introduced. Two kinds of MEMS (Micro-Electro-Mechanical Systems) micromirrors, digital and analog, are used for reflectors of the telescope, placed at different focal lengths. We apply this technology to the observation from space of TLE (Transient Luminous Events), extremely large transient sparks occurring at the upper atmosphere. TLE are one type of important backgrounds to be understood for future space observation of UHECR (Ultra-High Energy Cosmic Rays). The launch of the payload carried by a Russian microsatellite is foreseen in the middle of 2008. [Copyright &y& Elsevier] more...

Published
2008
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17. The ATIC long duration balloon project

Author

Guzik, T.G., Adams, J.H., Ahn, H.S., Bashindzhagyan, G., Chang, J., Christl, M., Fazely, A.R., Ganel, O., Granger, D., Gunasingha, R., Han, Y.J., Isbert, J.B., Kim, H.J., Kim, K.C., Kim, S.K., Kouznetsov, E., Panasyuk, M., Panov, A., Price, B., and Samsonov, G. more...

Subjects
*BALLOONS, *SPACE shuttles, *ASTROPHYSICS, *ASTRONOMY
Abstract

Long Duration Balloon (LDB) scientific experiments, launched to circumnavigate the south pole over Antarctica, have particular advantages compared to Shuttle or other Low Earth Orbit (LEO) missions in terms of cost, weight, scientific “duty factor” and work force development. The Advanced Thin Ionization Calorimeter (ATIC) cosmic-ray astrophysics experiment is a good example of a university-based project that takes full advantage of current LDB capability. The ATIC experiment is currently being prepared for its first LDB science flight that will investigate the charge composition and energy spectra of primary cosmic-rays over the energy range from about 1010 to 1014 eV. The instrument is built around a fully active, Bismuth–Germanate (BGO) ionization calorimeter to measure the energy deposited by cascades formed by particles interacting in a thick carbon target. A highly segmented silicon matrix, located above the target, provides good incident charge resolution plus rejection of “backscattered” particles from the cascade. Trajectory reconstruction is based on the cascade profile in the BGO calorimeter, plus information from the three pairs of scintillator hodoscope layers in the target section above it. A full evaluation of the experiment was performed during a test flight occurring between 28 December 2000 and 13 January 2001 where ATIC was carried to an altitude of ∼37 km above Antarctica by a ∼850,000 m3 helium filled balloon for one circumnavigation of the continent. All systems behaved well, the detectors performed as expected, >43 GB of engineering and cosmic-ray event data were returned and these data are now undergoing preliminary data analysis. During the coming 2002–2003 Antarctica summer season, we are preparing for an ATIC science flight with ∼15 to 30 days of data collection in the near-space environment of Long Duration Balloon (LDB) float altitudes. [Copyright &y& Elsevier] more...

Published
2004
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18. JEM-EUSO observational technique and exposure

Author

G. Castellinic, Markus Roth, Thomas J. Weiler, S. Perez Cano, Fausto Guarino, P. von Ballmoos, M. Ricci, Roberto Bellotti, Andreas A. Berlind, K. Kawai, M. Di Martino, A. Marini, Graciela B. Gelmini, Akinori Saito, G. Osteria, T. Tymieniecka, Barbara Szabelska, T. Peter, J. Sledd, Y. Hachisu, Y. Arai, P. L. Biermann, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, M. Nagata, James H. Adams, J. Fujimoto, Dmitri Semikoz, O. Martinez, Dmitry V. Naumov, Y. Yamamoto, M. I. Panasyuk, I. V. Yashin, L. Marcelli, J.N. Capdevielle, H. Ikeda, Andrii Neronov, D. Kolev, Silvia Ferrarese, I. Rusinov, T. Mernik, Gali Garipov, Yoshihiko Mizumoto, Katsuaki Asano, Guillaume Prévôt, Kenji Shinozaki, A. Bruno, H. Sato, Pierre Barrillon, Valerie Connaughton, H. H. Silva Lopez, T. Batsch, T. Shibata, S. Selmane, T. Murakami, J. Karczmarczyk, Karl Mannheim, Michael S. Briggs, A. J. de Castro, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, M. Bogomilov, Pavol Bobik, Y. Karadzhov, Yoshitaka Itow, G. Distratis, Marcos Reyes, Sergei A. Sharakin, R. Young, M. Sakata, A. Anzalone, N. Tajima, T. Napolitano, David B. Cline, T. Patzak, Piero Vallania, Hanna Rothkaehl, S. Blin-Bondil, M. D. Sabau, Satoshi Wada, T. Ogawa, F. Kajino, Shigehiro Nagataki, M. Serra, F. Cafagna, G. Modestino, Luis A. Anchordoqui, E. G. Judd, Katsuhiko Tsuno, H. W. Park, J. A. Morales de los Ríos, F. Tajima, E. Joven, Massimiliano Bonamente, R. Bechini, Ralph Engel, J. Watts, K. Belov, P. Gorodetzky, Humberto Ibarguen Salazar, C. Catalano, J. Lee, C. Lachaud, S. Dagoret-Campagne, Tomás Belenguer, B. A. Khrenov, Angela V. Olinto, Fernando López, Andrea Santangelo, C. De Santis, H. Tokuno, H. Miyamoto, E. Kuznetsov, C. Pennypacker, Piergiorgio Picozza, Toshikazu Ebisuzaki, L. Santiago Crúz, J. Bayer, M. Wille, I. Kreykenbohm, Vladimir Andreev, B. Pastircak, S. Sánchez, M. Ave Pernas, Alexander Kusenko, J. Błȩcki, M. Nagano Murakami, Frederic Trillaud, Y. Uchihori, Susumu Inoue, J. N. Albert, C. Blaksley, I. Kaneko, Toshiyuki Nonaka, P. Prat, K. Słomińska, C. de la Taille, Alfonso Monaco, Thomas Schanz, Shigeto Watanabe, Ke Fang, I. Fernández-Gómez, H. Prieto, R. Cremonini, B. Mot, R. Tsenov, K. Katahira, S. Ahmad, Livio Conti, N. Tone, Z. Włodarczyk, H. Lim, M. C. Maccarone, J. F. Valdés-Galicia, L. G. Tkachev, M. Dupieux, F. Dulucq, A. Pollini, Pavel Klimov, Patrick J. Reardon, Toshiki Tajima, A. Zuccaro Marchi, M. Karus, D. Monnier-Ragaigne, A. Segreto, Daisuke Yonetoku, S. Csorna, G. Vankova, H. J. Crawford, Taka Tomida, Jörn Wilms, Yukihiro Takahashi, G. Siemieniec-Oziȩbło, Yoshimasa Kurihara, O. A. Saprykin, A. Dell’Oro, Toshitaka Kajino, H. Schieler, N. Blanc, G. Masciantonio, Hitoshi Ohmori, Domenico Finco, J. Hernández Carretero, D. Supanitsky, M. Yu. Zotov, M. Unger, S. Biktemerova, Yoshiya Kawasaki, K. Higashide, C. Moretto, Tokonatsu Yamamoto, P. Galeotti, Susana Briz, G. Catalano, Hiroyuki Sagawa, C. González Alvarado, Mitsuteru Sato, Shoichi Ogio, C. Tenzer, Marco Casolino, Claudio Fornaro, M. Putis, D. Allard, A. Guzmán, A. Sobey, M. E. Bertaina, D. Campana, C. De Donato, A. Insolia, M. Kleifges, Soon-Wook Kim, Ken'ichi Nomoto, T. Sugiyama, A. Ebersoldt, Tadeusz Wibig, M. Sanz Palomino, Maxim Gonchar, Inkyu Park, Hirohiko M. Shimizu, J. Geary, S. Falk, A. Haungs, S. Piraino, Hajime Yano, N. De Simone, Y. Miyazaki, G. Roudil, L. Villaseñor, M. Suzuki, B. Harlov, Carlo Vigorito, K. Kudela, J. S. Kim, G. Sáez-Cano, Mark Christl, O. Tibolla, V. S. Morozenko, Yoshiki Tsunesada, M. Rybczyński, Lech Wiktor Piotrowski, A. Jung, T. Paul, K. Yoshida, P. Baragatti, G. Cordero, Valentina Scotti, Hajime Takami, Masaki Fukushima, G. Medina-Tanco, S. Yoshida, J. Szabelski, T. Nakamura, R. Nava, N. Sakaki, R. Matev, M. D. Rodríguez Frías, Z. Plebaniak, J. Blümer, L. Valore, Rossella Caruso, Michiyuki Chikawa, Simona Toscano, Alberto Cellino, L. R. Wiencke, K. Mase, G. Giraudo, Francesco Fenu, D. Ikeda, I. Rodríguez, F. Sarazin, Marc Weber, M. Flamini, Y. Takizawa, T. Shirahama, Francesco Isgrò, Piotr Orleanski, B. Keilhauer, Frederic Jean Ronga, Javier Licandro, T. Pierog, J. Watanabe, M. Takeda, D. Maravilla, Jianyi Yang, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blümer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmán, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., López, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prévôt, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodríguez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sánchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseñor, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A. more...

Subjects
Aperture, Ciencias Físicas, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Extensive air shower, JEM-EUSO, ultra-high energy cosmic rays, Cosmic ray, Astrophysics, Atmosphere, Altitude, International Space Station, Nadir, Extensive air showers, extensive air showers, Ultra-high energy cosmic ray, Physics::Atmospheric and Oceanic Physics, media_common, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Ultra-high energy cosmic rays, Astronomy and Astrophysic, Universe, Astronomía, Tilt (optics), Space and Planetary Science, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, CIENCIAS NATURALES Y EXACTAS
Abstract

Designed as the first mission to explore the ultra-high energy universe from space, JEM-EUSO observes the Earth’s atmosphere at night to record the ultraviolet tracks generated by the extensive air showers. We present the expected geometrical aperture and annual exposure in the nadir and tilt modes for ultra-high energy cosmic rays observation as a function of the altitude of the International Space Station. Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia Fil: Fenu, F.. University of Tubingen; Alemania Fil: Shinozaki, K.. RIKEN; Japón Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos Fil: Ahmad, S.. Ecole Polytechnique; Francia Fil: Albert, J. N.. Univ Paris-Sud; Francia Fil: Allard, D.. Univ Paris Diderot; Francia Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos Fil: Andreev, V.. University of California; Estados Unidos Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón Fil: Asano, K.. Tokyo Institute of Technology; Japón Fil: Ave Pernas, M.. Universidad de Alcalá; España Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. National Centre for Nuclear Research; Polonia Fil: Bayer, J.. University of Tubingen; Alemania Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belov, K.. University of California; Estados Unidos Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia Fil: Blaksley, C.. Univ Paris Diderot; Francia Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: The JEM-EUSO Collaboration. more...

Published
2014
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19. JEM-EUSO: Meteor and nuclearite observations

Author

K. Mannheim, P. Reardon, T. Nonaka, Toshikazu Ebisuzaki, M. Kleifges, M. S. Briggs, Y. Tsunesada, P. Picozza, H. Salazar, A. Marini, F. Guarino, G. Siemieniec-Oziȩbło, M. Nagata, Dmitry V. Naumov, I. H. Park, R. Young, M. D. Rodríguez Frías, G. Distratis, Satoshi Wada, Hiroyuki Sagawa, M. Flamini, Y. Takizawa, C. Blaksley, Tomás Belenguer, Frederic Trillaud, Silvia Ferrarese, S. Ogio, J. Fujimoto, I. V. Yashin, T. Ogawa, J. Szabelski, M. I. Panasyuk, L. Wiencke, H. Sato, A. Guzman, D. Allard, M. E. Bertaina, E. Kuznetsov, F. Tajima, J. Błȩcki, J. N. Capdevielle, L. Santiago Crúz, H. Ohmori, H. Ikeda, I. Kreykenbohm, T. Batsch, N. Inoue, K. Higashide, J. Yang, D. Cline, Gali Garipov, Y. Mizumoto, L. Villaseñor, R. Bechini, C. Tenzer, P. Bobik, S. Biktemerova, Ke Fang, Y. Hachisu, R. Tsenov, M. Nagano Murakami, A. Haungs, M. Wille, H. Lim, M. C. Maccarone, Maxim Gonchar, M. Serra, E. G. Judd, T. Murakami, J. Karczmarczyk, H. J. Crawford, Angela V. Olinto, Fernando López, Andrea Santangelo, S. Blin-Bondil, C. Lachaud, V. Andreev, Ovidiu Vaduvescu, M. Lacombe, A. Kusenko, T. J. Weiler, P. Prat, S. Piraino, S. Dagoret-Campagne, A. Cellino, Y. Arai, S. Watanabe, D. Yonetoku, T. Wibig, Y. Miyazaki, G. Vankova, M. Ave Pernas, H. Prieto, C. De Donato, G. Giraudo, T. Kajino, J. N. Albert, P. Orleański, G. Masciantonio, Thomas Schanz, H. Schieler, M. Bonamente, A. J. de Castro, Claudio Cassardo, M. Fukushima, Z. Plebaniak, T. Tomida, M. Dupieux, J. Licandro, D. Maravilla, S. Sánchez, B. Mot, T. Paul, F. Dulucq, V. Connaughton, S. Ahmad, M. Unger, F. Ronga, I. Rodríguez, T. Peter, M. Chikawa, P. Vallania, Livio Conti, A. Zuccaro Marchi, A. A. Berlind, H. Takami, I. Kaneko, B. Szabelska, M. Sakata, M. Reyes, T. Napolitano, K. Mase, O. Tibolla, M. Weber, C. De Santis, L. Marcelli, A. Insolia, T. Patzak, Jörn Wilms, Alfonso Monaco, D. Monnier-Ragaigne, A. Segreto, Yukihiro Takahashi, Francesco Fenu, J. S. Kim, J. Hernández Carretero, V. S. Morozenko, O. A. Saprykin, D. Campana, Y. Itow, L. Anchordoqui, J. Lee, H. Rothkaehl, G. Sáez-Cano, E. Joven, J. F. Valdés-Galicia, L. del Peral, A. Franceschi, E. Parizot, B. Keilhauer, T. Shibata, M. Rybczyński, G. Osteria, M. J. Christl, P. Gorodetzky, C. Catalano, N. Blanc, D. Semikoz, S. Csorna, Hajime Yano, C. González Alvarado, Marco Casolino, T. Tajima, Claudio Fornaro, G. Cordero, F. Kajino, D. Ikeda, L. Valore, C. Moretto, H. H. Silva Lopez, M. D. Sabau, M. Putis, Francesco Isgrò, Roberto Bellotti, O. Martinez, G. Catalano, V. Scotti, K. Shinozaki, A. Sobey, K. Asano, J. Bayer, Lech Wiktor Piotrowski, H. W. Park, R. Nava, J. H. Adams, K. Belov, Y. Karadzhov, G. Prévôt, A. Ebersoldt, J. Watts, C. de la Taille, C. Pennypacker, B. Pastircak, K. Katahira, Y. Kawasaki, D. Supanitsky, N. Sakaki, R. Matev, B. A. Khrenov, H. Miyamoto, T. Pierog, Rossella Caruso, G. Castellinic, M. Sanz Palomino, S. Falk, A. Pollini, S. Yoshida, A. Neronov, Z. Włodarczyk, Sergei A. Sharakin, N. Tone, I. Fernández-Gómez, F. Cafagna, M. Ricci, P. von Ballmoos, D. Kolev, Pavel Klimov, J. A. Morales de los Ríos, L. Tkachev, S. Perez Cano, G. Gelmini, P. Galeotti, M. Yu. Zotov, M. Bogomilov, Y. Kurihara, Simona Toscano, A. Bruno, M. Karus, Susana Briz, S. Selmane, K. Kawai, Akinori Saito, K. Tsuno, T. Mernik, S. Nagataki, R. Cremonini, Y. Uchihori, J. Blümer, Domenico Finco, K. Słomińska, P. L. Biermann, A. Anzalone, T. Nakamura, Susumu Inoue, M. Di Martino, K. Nomoto, I. Rusinov, T. Tymieniecka, J. Sledd, G. Medina-Tanco, F. Sarazin, H. M. Shimizu, J. Geary, N. De Simone, Mitsuteru Sato, G. Modestino, M. Suzuki, A. Jung, K. Yoshida, P. Barrillon, T. Yamamoto, M. Roth, P. Baragatti, T. Shirahama, R. Engel, S. W. Kim, J. Watanabe, M. Takeda, N. Tajima, Y. Yamamoto, G. Roudil, B. Harlov, Carlo Vigorito, K. Kudela, A. Dell’Oro, H. Tokuno, T. Sugiyama, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blümer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmán, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., López, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prévôt, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodríguez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sánchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseñor, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A. more...

Subjects
Meteor (satellite), Solar System, JEM-EUSO, Meteors, Nuclearites, Space detectors, Astronomy and Astrophysics, Space and Planetary Science, Ciencias Físicas, Cosmic ray, Astrophysics, Primary (astronomy), Meteor, Space detector, Physics, Nuclearite, Meteoroid, Astronomy, Astronomy and Astrophysic, Speed of light (cellular automaton), Astronomía, Trajectory, Satellite, CIENCIAS NATURALES Y EXACTAS
Abstract

Meteor and fireball observations are key to the derivation of both the inventory and physical characterization of small solar system bodies orbiting in the vicinity of the Earth. For several decades, observation of these phenomena has only been possible via ground-based instruments. The proposed JEM-EUSO mission has the potential to become the first operational space-based platform to share this capability. In comparison to the observation of extremely energetic cosmic ray events, which is the primary objective of JEM-EUSO, meteor phenomena are very slow, since their typical speeds are of the order of a few tens of km/sec (whereas cosmic rays travel at light speed). The observing strategy developed to detect meteors may also be applied to the detection of nuclearites, which have higher velocities, a wider range of possible trajectories, but move well below the speed of light and can therefore be considered as slow events for JEM-EUSO. The possible detection of nuclearites greatly enhances the scientific rationale behind the JEM-EUSO mission. Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Cellino, A.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Ronga, F.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos Fil: Ahmad, S.. Ecole Polytechnique; Francia Fil: Albert, J. N.. Univ Paris-Sud; Francia Fil: Allard, D.. Univ Paris Diderot; Francia Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos Fil: Andreev, V.. University of California; Estados Unidos Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón Fil: Asano, K.. Tokyo Institute of Technology; Japón Fil: Ave Pernas, M.. Universidad de Alcalá; España Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. National Centre for Nuclear Research; Polonia Fil: Bayer, J.. University of Tubingen; Alemania Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA; España Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belov, K.. University of California; Estados Unidos Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia Fil: Blaksley, C.. Univ Paris Diderot; Francia Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM; Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Blin Bondil, S.. Ecole Polytechnique; Francia Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: The JEM-EUSO Collaboration. more...

Published
2015
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20. The JEM-EUSO mission : an introduction

Author

J. Karczmarczyk, A. Haungs, T. Murakami, Tomás Belenguer, Piero Vallania, M. D. Sabau, M. Serra, J. Bayer, C. de la Taille, K. Katahira, Luis A. Anchordoqui, T. Batsch, D. Supanitsky, Hanna Rothkaehl, R. Nava, N. Sakaki, Y. Karadzhov, I. Kaneko, K. Mase, J. Watts, L. Valore, Rossella Caruso, H. J. Crawford, C. Pennypacker, I. Rodríguez, Shoichi Ogio, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, D. Allard, G. Castellini, M. E. Bertaina, Ken'ichi Nomoto, Silvia Ferrarese, Toshiyuki Nonaka, P. Prat, R. Young, M. Sakata, A. Guzmán, I. V. Yashin, T. Shirahama, T. Shibata, Alberto Cellino, P. Picozza, J. Lee, I. Fernández-Gómez, P. Baragatti, L. Marcelli, Ralph Engel, M. Karus, G. Sáez Cano, M. Nagata, A. Ebersoldt, L. Villaseñor, A. Bruno, Jeong-Sook Kim, L. R. Wiencke, J. Błȩcki, Karl Mannheim, D. Ikeda, D. Monnier-Ragaigne, A. Segreto, F. Tajima, Lech Wiktor Piotrowski, M. Rybczyński, Michael S. Briggs, A. J. de Castro, F. Sarazin, Domenico Finco, H. Lim, Frederic Trillaud, P. Gorodetzky, Dmitry V. Naumov, R. Bechini, Marc Weber, Katsuaki Asano, G. Cordero, M. C. Maccarone, Piotr Orleanski, N. Blanc, S. Piraino, J.N. Capdevielle, T. Patzak, S. Yoshida, J. Szabelski, Francesco Fenu, Yoshiki Tsunesada, Hiroyuki Sagawa, M. Wille, Andrii Neronov, Y. Uchihori, R. Matev, G. Giraudo, M. Suzuki, Satoshi Wada, H. Sato, C. De Donato, Markus Roth, J. N. Albert, T. Ogawa, Hajime Takami, B. A. Khrenov, G. Distratis, Fausto Guarino, O. Martinez, Masaki Fukushima, Thomas Schanz, Soon-Wook Kim, Takuji Nakamura, Jianyi Yang, Yoshitaka Itow, Shigeto Watanabe, H. Miyamoto, D. Maravilla, P. von Ballmoos, M. Ricci, K. Shinozaki, Angela V. Olinto, Fernando López, Andrea Santangelo, S. Selmane, Livio Conti, J. Fujimoto, A. Anzalone, Barbara Szabelska, T. Peter, David B. Cline, A. Zuccaro Marchi, Maxim Gonchar, Hirohiko M. Shimizu, M. D. Rodríguez Frías, F. Cafagna, G. Modestino, E. Joven, D. Campana, Francesco Isgrò, F. Dulucq, Z. Plebaniak, J. Blümer, Valentina Scotti, B. Keilhauer, Graciela B. Gelmini, M. Flamini, P. L. Biermann, Jörn Wilms, Javier Licandro, M. I. Panasyuk, J. F. Valdés-Galicia, L. G. Tkachev, O. A. Saprykin, Michiyuki Chikawa, B. Mot, Y. Hachisu, Inkyu Park, Frederic Jean Ronga, M. Dupieux, S. Csorna, T. Napolitano, S. Perez Cano, Y. Takizawa, L. Santiago Crúz, M. Putis, Humberto Ibarguen Salazar, Y. Arai, G. Vankova, I. Rusinov, A. Sobey, Y. Miyazaki, S. Blin-Bondil, C. De Santis, H. Tokuno, Y. Yamamoto, A. Insolia, M. Kleifges, Yukihiro Takahashi, B. Pastirčák, E. G. Judd, T. Pierog, M. Ave Pernas, Katsuhiko Tsuno, H. Prieto, R. Cremonini, S. Biktemerova, J. Watanabe, Pierre Barrillon, Mark Christl, O. Tibolla, Osvaldo Catalano, Gali Garipov, K. Kawai, I. Kreykenbohm, Sergei A. Sharakin, R. Tsenov, Vladimir Andreev, Marcos Reyes, Marco Casolino, Claudio Fornaro, K. Belov, C. Catalano, A. Pollini, J. Hernández Carretero, Pavel Klimov, M. Unger, C. Lachaud, S. Dagoret-Campagne, M. Di Martino, A. Marini, Toshikazu Ebisuzaki, T. J. Weiler, G. Osteria, S. Sánchez, S. Ahmad, Yoshimasa Kurihara, T. Tymieniecka, J. Sledd, H. Schieler, Mitsuteru Sato, C. González Alvarado, Alfonso Monaco, C. Blaksley, N. Tone, Ke Fang, M. Nagano, Taka Tomida, Daisuke Yonetoku, Roberto Bellotti, Andreas A. Berlind, M. Sanz Palomino, Tokonatsu Yamamoto, James H. Adams, M. Yu. Zotov, D. Kolev, Valerie Connaughton, H. H. Silva Lopez, Susana Briz, S. Falk, H. Ikeda, V. S. Morozenko, Hajime Yano, A. Dell’Oro, Toshitaka Kajino, K. Higashide, C. Moretto, P. Galeotti, C. Tenzer, T. Sugiyama, Tadeusz Wibig, K. Kudela, G. Roudil, B. Harlov, Carlo Vigorito, N. Tajima, M. Takeda, Shigehiro Nagataki, Guillaume Prévôt, M. Bogomilov, F. Kajino, H. W. Park, Massimiliano Bonamente, E. Kuznetsov, Alexander Kusenko, K. Słomińska, Akinori Saito, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, Dmitri Semikoz, Sug-Whan Kim, T. Mernik, Z. Włodarczyk, Simona Toscano, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, J. A. Morales de los Ríos, Susumu Inoue, A. Jung, T. Paul, K. Yoshida, G. Medina-Tanco, J. Geary, N. De Simone, Yoshihiko Mizumoto, Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali del Sud (LNS), Istituto Nazionale di Fisica Nucleare (INFN), Division of Biology, Kansas State University, Kansas State University, CTC, Università degli studi di Bari Aldo Moro = University of Bari Aldo Moro (UNIBA), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Universities Space Research Association (USRA), Regione Emilia Romagna, Servizio Tecnico Bacini Enza e sinistra Secchia, Institute for Data Processing and Electronics (IPE), Karlsruhe Institute of Technology (KIT), Institute for Ecology, Universität Greifswald - University of Greifswald, Tokushima research center, Department of Physics and Astronomy [UCLA, Los Angeles], University of California [Los Angeles] (UCLA), University of California (UC)-University of California (UC), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (INFN, Sezione di Torino), Institute of Applied Biotechnology and Basic Sciences, Rzeszow University, Department of Mechanical System (Hiroshima University), Hiroshima University, Nagoya University, Department of Pathology, Ludwig-Maximilians-Universität München (LMU), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Institute of Experimental Physics of Kosice, Slovak Academy of Sciences (SAS), KEK (High energy accelerator research organization), iMagX/MIRO, Université Catholique de Louvain = Catholic University of Louvain (UCL), Instituto de Astrofisica de Canarias (IAC), The Open University of Japan [Chiba] (OUJ), Tohoku University [Sendai], Department of Earth and Planetary Science [Tokyo], Graduate School of Science [Tokyo], The University of Tokyo (UTokyo)-The University of Tokyo (UTokyo), Department of Electrical Engineering and Computer Sciences, University of Hyogo, INTEGRAL Science Data Center (ISDC), Geneva Observatory, Université de Genève = University of Geneva (UNIGE)-Université de Genève = University of Geneva (UNIGE), Service de dermatologie et vénéréologie (CHUV Lausanne), Centre Hospitalier Universitaire Vaudois [Lausanne] (CHUV), Laboratoire de Physique Théorique et Modèles Statistiques (LPTMS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Institute for Surgical Technology and Biomechanics [Bern] (ISTB), University of Bern, Centre IRMf de Marseille, Université de la Méditerranée - Aix-Marseille 2, Space Research Centre of Polish Academy of Sciences (CBK), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Centre d'étude spatiale des rayonnements (CESR), Center for Mathematics and Physics, University of Aizu, Centre de recherche sur la Paléobiodiversité et les Paléoenvironnements (CR2P), Muséum national d'Histoire naturelle (MNHN)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Colorado School of Mines, Department of Physics (Department of Physics), Tokyo Metropolitan University [Tokyo] (TMU), Department of Radiation-Oncology, Università degli Studi di Firenze = University of Florence (UniFI), Graduate School of Materials Science, Nara Institute os Science and Technology, Observatoire océanologique de Banyuls (OOB), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, Vrije Universiteit Brussel (VUB), Laboratoire de Génie Electrique de Grenoble (G2ELab), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institute of Sensor and Actuator Systems, Vienna University of Technology (TU Wien), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Luxembourg Institute of Science and Technology (LIST), Dr. Karl-Remeis-Sternwarte, Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU)-Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Kyoto University, University of Connecticut (UCONN), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), National Institute for Nuclear Physics (INFN), University of Bari and INFN section of Bari, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), University of California-University of California, Université Catholique de Louvain (UCL), The University of Tokyo, University of Geneva [Switzerland]-University of Geneva [Switzerland], Polska Akademia Nauk (PAN), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS), Tokyo Metropolitan University [Tokyo], University of Florence (UNIFI), High Energy Accelerator Research Organization (KEK), University of Tsukuba, Vrije Universiteit [Brussels] (VUB), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Technical University of Vienna [Vienna] (TU WIEN), PSL Research University (PSL)-PSL Research University (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Kyoto University [Kyoto], Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellini, G., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, Jeong Sook, Kim, Soon Wook, Kim, Sug Whan, Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Nagano, M., Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrã­guez, I., Frã­as, M. D. Rodríguez, Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A, Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., Zuccaro Marchi, A., École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Università degli studi di Bari Aldo Moro (UNIBA), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), The University of Tokyo (UTokyo), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Firenze = University of Florence [Firenze] (UNIFI), Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology, Centre National de la Recherche Scientifique (CNRS)-Université de Lille-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC) more...

Subjects
Photon, Aperture, Ciencias Físicas, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, ultra-high energy cosmic rays, Astrophysics, law.invention, Telescope, Atmosphere, law, International Space Station, Neutrino, Ultra-high energy cosmic rays, Neutrinos, Neutrinos, Ultra-high energy cosmic ray, ComputingMilieux_MISCELLANEOUS, media_common, Physics, [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, neutrinos, Astronomy and Astrophysics, Ultra-high energy cosmic rays, Astronomy and Astrophysic, Universe, Astronomía, Space and Planetary Science, Physics::Space Physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], CIENCIAS NATURALES Y EXACTAS
Abstract

注記: The JEM-EUSO Collaboration 288名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2015-10-19, Note: The JEM-EUSO Collaboration 288members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150231000 more...

Published
2015
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21. Performances of JEM–EUSO : energy and X_{max} reconstruction

Author

I. V. Yashin, L. Marcelli, B. A. Khrenov, H. Miyamoto, Kenji Shinozaki, A. Bruno, Karl Mannheim, Michael S. Briggs, A. J. de Castro, D. Supanitsky, Shoichi Ogio, M. Rybczyński, F. Dulucq, Graciela B. Gelmini, Andreas A. Berlind, A. Jung, Massimiliano Bonamente, Javier Licandro, T. Paul, N. Tone, Daisuke Yonetoku, M. Ave Pernas, F. Tajima, H. Sato, David B. Cline, Gali Garipov, C. De Donato, Soon-Wook Kim, G. Cordero, M. Yu. Zotov, K. Yoshida, Susana Briz, S. Selmane, Y. Hachisu, Y. Arai, Y. Yamamoto, Piero Vallania, M. D. Sabau, Alfonso Monaco, Taka Tomida, J. Bayer, E. Kuznetsov, J. Hernández Carretero, P. Baragatti, Hiroyuki Sagawa, D. Kolev, J. S. Kim, M. Putis, A. Sobey, A. Insolia, M. Kleifges, C. de la Taille, E. G. Judd, K. Katahira, M. Unger, T. Pierog, J. Watanabe, M. Wille, M. Nagano Murakami, Y. Uchihori, M. Takeda, J. F. Valdés-Galicia, P. Gorodetzky, G. Distratis, V. S. Morozenko, C. Lachaud, Katsuhiko Tsuno, G. Castellinic, Katsuaki Asano, J. Fujimoto, Tokonatsu Yamamoto, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, S. Dagoret-Campagne, Pierre Barrillon, L. G. Tkachev, S. Csorna, Valerie Connaughton, Toshikazu Ebisuzaki, T. Shibata, I. Kreykenbohm, D. Allard, M. E. Bertaina, Alexander Kusenko, G. Vankova, H. H. Silva Lopez, Jianyi Yang, Vladimir Andreev, R. Matev, J. N. Albert, M. Di Martino, Markus Roth, G. Medina-Tanco, Ken'ichi Nomoto, Francesco Isgrò, A. Marini, D. Campana, M. Nagata, Thomas Schanz, Hajime Yano, Fausto Guarino, P. von Ballmoos, M. Ricci, Satoshi Wada, G. Catalano, P. Prat, A. Haungs, S. Piraino, K. Słomińska, B. Keilhauer, G. Prévôt, S. Biktemerova, T. Ogawa, Yoshihiko Mizumoto, T. Patzak, Lech Wiktor Piotrowski, R. Nava, Inkyu Park, Dmitry V. Naumov, R. Bechini, N. Sakaki, Livio Conti, Ke Fang, S. Ahmad, T. Murakami, J. Karczmarczyk, A. Zuccaro Marchi, Y. Karadzhov, L. Valore, F. Cafagna, Frederic Jean Ronga, Sergei A. Sharakin, G. Modestino, Rossella Caruso, Angela V. Olinto, Fernando López, Jörn Wilms, E. Joven, G. Osteria, Andrea Santangelo, T. Tymieniecka, J. Sledd, D. Maravilla, Y. Miyazaki, A. Dell’Oro, Toshitaka Kajino, S. Yoshida, J. Szabelski, Silvia Ferrarese, O. A. Saprykin, P. L. Biermann, Maxim Gonchar, S. Falk, S. Blin-Bondil, Hirohiko M. Shimizu, R. Young, M. Sakata, I. Rusinov, M. Dupieux, Z. Włodarczyk, Hanna Rothkaehl, Shigeto Watanabe, Mark Christl, O. Tibolla, J. N. Capdevielle, L. Santiago Crúz, A. Anzalone, T. Napolitano, Thomas J. Weiler, K. Higashide, C. Moretto, J. Geary, P. Galeotti, Alberto Cellino, A. Guzmán, S. Perez Cano, C. González Alvarado, Marcos Reyes, P. Picozza, J. Błȩcki, Roberto Bellotti, H. Prieto, J. Lee, Simona Toscano, Barbara Szabelska, T. Peter, C. Tenzer, I. Rodríguez, H. Lim, L. R. Wiencke, R. Cremonini, M. C. Maccarone, N. De Simone, T. Sugiyama, J. Watts, S. Sánchez, Tadeusz Wibig, T. Shirahama, Toshiyuki Nonaka, C. Pennypacker, James H. Adams, Andrii Neronov, B. Pastircak, H. Ikeda, L. Villaseñor, G. Giraudo, G. Sáez-Cano, N. Inoue, I. Fernández-Gómez, K. Kawai, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, M. Sanz Palomino, M. Bogomilov, D. Monnier-Ragaigne, A. Segreto, M. Karus, M. I. Panasyuk, Akinori Saito, M. Suzuki, Piotr Orleanski, Domenico Finco, K. Belov, C. Catalano, F. Kajino, J. A. Morales de los Ríos, Yoshitaka Itow, Ovidiu Vaduvescu, G. Roudil, M. Lacombe, Tomás Belenguer, Claudio Cassardo, B. Harlov, Susumu Inoue, H. W. Park, Carlo Vigorito, K. Kudela, H. J. Crawford, Valentina Scotti, Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, N. Tajima, T. Mernik, Shigehiro Nagataki, R. Tsenov, A. Pollini, Pavel Klimov, Yoshimasa Kurihara, H. Schieler, Ralph Engel, Mitsuteru Sato, Frederic Trillaud, B. Mot, Yukihiro Takahashi, Marco Casolino, Claudio Fornaro, M. Flamini, Y. Takizawa, C. Blaksley, K. Mase, M. D. Rodríguez Frías, Z. Plebaniak, J. Blümer, Michiyuki Chikawa, D. Ikeda, A. Ebersoldt, F. Sarazin, Marc Weber, Yoshiki Tsunesada, O. Martinez, N. Blanc, Francesco Fenu, D. Semikoz, Hajime Takami, Masaki Fukushima, T. Nakamura, M. Serra, Luis A. Anchordoqui, T. Batsch, I. Kaneko, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blümer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmán, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., López, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prévôt, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodríguez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sánchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseñor, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A. more...

Subjects
reconstruction, Ciencias Físicas, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, JEM-EUSO, X (max) reconstruction, ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, Cosmic ray, X_{max} reconstruction, Astrophysics, law.invention, Energy reconstruction, JEM–EUSO, Xmax reconstruction, Astronomy and Astrophysics, Space and Planetary Science, Telescope, law, International Space Station, Ultra-high-energy cosmic ray, max, media_common, energy reconstruction, Physics, Resolution (electron density), Astrophysics::Instrumentation and Methods for Astrophysics, X-max reconstruction, Astronomy, Universe, Astronomía, JEM-EUSO, Energy reconstruction, X-max reconstruction, Event (particle physics), CIENCIAS NATURALES Y EXACTAS, Energy (signal processing)
Abstract

注記: The JEM-EUSO Collaboration 288名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2014-10-13, Note: The JEM-EUSO Collaboration 288members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150235000 more...

Published
2015
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22. Ultra high energy photons and neutrinos with JEM-EUSO

Author

M. Weber, D. Monnier-Ragaigne, A. Segreto, H. Rothkaehl, C. Catalano, B. Mot, S. Watanabe, N. Blanc, M. Bonamente, S. Ahmad, M. Unger, D. Semikoz, M. Sakata, M. Reyes, L. Marcelli, Yukihiro Takahashi, I. Rodríguez, M. Serra, R. Bechini, M. Rybczyński, C. González Alvarado, T. Murakami, J. Karczmarczyk, F. Kajino, Marco Casolino, Claudio Fornaro, S. Ogio, L. Valore, I. Kaneko, B. Szabelska, G. Cordero, T. Shirahama, S. Blin-Bondil, G. Siemieniec-Oziȩbło, H. Ikeda, H. W. Park, L. Villaseñor, V. Andreev, Roberto Bellotti, M. J. Christl, T. Paul, F. Dulucq, H. Sato, D. Yonetoku, A. Guzman, O. Martinez, K. Mannheim, T. Wibig, A. Bruno, E. G. Judd, K. Mase, O. Tibolla, M. S. Briggs, Y. Tsunesada, R. Engel, F. Guarino, P. Picozza, H. Salazar, A. Marini, M. Chikawa, A. Jung, J. Watts, C. Pennypacker, P. Vallania, F. Tajima, D. Campana, J. Lee, T. Shibata, M. D. Sabau, Silvia Ferrarese, B. Pastircak, D. Allard, R. Matev, M. Sanz Palomino, A. Ebersoldt, M. E. Bertaina, K. Yoshida, M. Putis, A. Sobey, A. Neronov, A. Haungs, I. H. Park, D. Maravilla, J. Fujimoto, M. Karus, C. Tenzer, H. H. Silva Lopez, Gali Garipov, K. Shinozaki, R. Nava, J. H. Adams, Frederic Trillaud, Y. Uchihori, L. Wiencke, M. Nagata, Domenico Finco, N. Sakaki, P. Barrillon, Z. Włodarczyk, Y. Kurihara, Lech Wiktor Piotrowski, D. Kolev, G. Castellinic, Hiroyuki Sagawa, Rossella Caruso, Alfonso Monaco, S. Selmane, P. von Ballmoos, P. Prat, S. Piraino, G. Vankova, S. Sánchez, Dmitry V. Naumov, T. J. Weiler, S. Yoshida, E. Kuznetsov, H. Prieto, P. Bobik, S. Biktemerova, I. V. Yashin, R. Cremonini, C. Lachaud, S. Dagoret-Campagne, C. De Donato, S. W. Kim, G. Catalano, G. Gelmini, L. del Peral, A. Franceschi, E. Parizot, Maxim Gonchar, T. Nakamura, M. Nagano Murakami, Toshikazu Ebisuzaki, I. Kreykenbohm, T. Batsch, Y. Kawasaki, J. Watanabe, M. Takeda, G. Sáez-Cano, R. Tsenov, T. Patzak, Simona Toscano, S. Falk, J. S. Kim, T. Nonaka, V. S. Morozenko, J. N. Albert, K. Tsuno, J. A. Morales de los Ríos, V. Connaughton, Ke Fang, N. Inoue, Thomas Schanz, R. Young, M. D. Rodríguez Frías, Francesco Fenu, Tomás Belenguer, M. Roth, H. Ohmori, P. Reardon, Y. Itow, A. Kusenko, K. Higashide, G. Modestino, P. Orleański, Susumu Inoue, Livio Conti, P. Gorodetzky, A. Zuccaro Marchi, A. A. Berlind, G. Masciantonio, E. Joven, A. J. de Castro, M. Suzuki, Jörn Wilms, M. I. Panasyuk, J. Błȩcki, J. Yang, D. Cline, G. Giraudo, J. F. Valdés-Galicia, M. Kleifges, O. A. Saprykin, H. Lim, M. Dupieux, M. Fukushima, Z. Plebaniak, A. Insolia, M. C. Maccarone, T. Kajino, V. Scotti, S. Csorna, F. Ronga, M. Wille, F. Sarazin, T. Napolitano, D. Ikeda, C. de la Taille, B. Keilhauer, H. M. Shimizu, K. Katahira, K. Słomińska, J. Geary, L. Anchordoqui, Y. Karadzhov, G. Distratis, H. J. Crawford, N. De Simone, K. Asano, B. A. Khrenov, A. Cellino, G. Osteria, H. Miyamoto, J. N. Capdevielle, L. Santiago Crúz, Y. Hachisu, C. Moretto, Y. Arai, Francesco Isgrò, M. Ricci, M. Ave Pernas, M. Flamini, J. Licandro, G. Prévôt, K. Belov, T. Pierog, P. Galeotti, Sergei A. Sharakin, K. Nomoto, Y. Takizawa, C. Blaksley, J. Hernández Carretero, Mitsuteru Sato, J. Szabelski, Y. Mizumoto, T. Peter, T. Yamamoto, P. Baragatti, Y. Miyazaki, M. Di Martino, T. Tymieniecka, J. Sledd, G. Medina-Tanco, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, T. Mernik, A. Anzalone, C. De Santis, T. Tajima, Satoshi Wada, J. Bayer, T. Ogawa, A. Pollini, Pavel Klimov, Angela V. Olinto, Fernando López, Andrea Santangelo, H. Schieler, A. Dell’Oro, H. Tokuno, T. Sugiyama, P. L. Biermann, I. Rusinov, D. Supanitsky, S. Perez Cano, N. Tone, L. Tkachev, N. Tajima, Y. Yamamoto, M. Bogomilov, M. Yu. Zotov, Susana Briz, G. Roudil, B. Harlov, Carlo Vigorito, K. Kudela, S. Nagataki, J. Blümer, K. Kawai, Akinori Saito, T. Tomida, H. Takami, Hajime Yano, I. Fernández-Gómez, F. Cafagna, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blümer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmán, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., López, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prévôt, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodríguez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sánchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseñor, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A. more...

Subjects
space observation, Ciencias Físicas, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Neutrino, Neutrinos, Photons, Space observation, Astronomy and Astrophysics, Space and Planetary Science, photons, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, neutrinos, Astronomy and Astrophysic, Solar neutrino problem, Photon, Astronomía, Cosmic neutrino background, Neutrino detector, Physics::Space Physics, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino astronomy, CIENCIAS NATURALES Y EXACTAS
Abstract

Ultra high energy photons and neutrinos are carriers of very importantastrophysical information. They may be produced at the sites of cosmic ray acceleration or during the propagation of the cosmic rays in the intergalactic medium. In contrast to charged cosmic rays, photon and neutrino arrival directions point to the production site because they are not deflected by the magnetic fields of the Galaxy or the intergalactic medium. In this work we study the characteristics of the longitudinal development of showers initiated by photons and neutrinos at the highestenergies. These studies are relevant for development of techniques for neutrino and photon identification by the JEM-EUSO telescope. In particular, we study the possibility of observing the multi-peak structure of very deep horizontal neutrino showers with JEM-EUSO. We also discuss the possibility to determine the flavor content of the incident neutrino flux by taking advantage of the different characteristics of thelongitudinal profiles generated by different type of neutrinos. This is of grate importance for the study of the fundamental properties of neutrinos at the highest energies. Regarding photons, we discuss the detectability of the cosmogenic component by JEM-EUSO and also estimate the expected upper limits on the photon fraction which can be obtained from the future JEM-EUSO data for the case in which there are no photons in the samples. Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Medina Tanco, G.. Universidad Nacional Autónoma de México; México Fil: Guzman, A.. University of Tubingen; Alemania Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos Fil: Ahmad, S.. Ecole Polytechnique; Francia Fil: Albert, J. N.. Univ Paris-Sud; Francia Fil: Allard, D.. Univ Paris Diderot; Francia Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos Fil: Andreev, V.. University of California; Estados Unidos Fil: Anzalone, A.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón Fil: Asano, K.. Tokyo Institute of Technology; Japón Fil: Ave Pernas, M.. Universidad de Alcalá; España Fil: Baragatti, P.. UTIU, Dipartimento di Ingegneria; Italia Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. National Centre for Nuclear Research; Polonia Fil: Bayer, J.. University of Tubingen; Alemania Fil: Bechini, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belov, K.. University of California; Estados Unidos Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia Fil: Blaksley, C.. Univ Paris Diderot; Francia Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania Fil: The JEM-EUSO Collaboration. more...

Published
2015

23. Science of atmospheric phenomena with JEM-EUSO

Author

Yoshihiko Mizumoto, Toshiyuki Nonaka, T. Murakami, A. Guzmán, J. Karczmarczyk, J. Watts, C. Pennypacker, B. Pastircak, P. Prat, I. Fernández-Gómez, M. Karus, Domenico Finco, Hiroyuki Sagawa, M. Suzuki, M. Flamini, Hanna Rothkaehl, D. Monnier-Ragaigne, A. Segreto, Maxim Gonchar, Hirohiko M. Shimizu, L. Villaseñor, Y. Takizawa, Javier Licandro, P. Picozza, Alberto Cellino, Roberto Bellotti, J. Lee, F. Dulucq, Lech Wiktor Piotrowski, Valentina Scotti, J. N. Albert, N. Blanc, Thomas Schanz, Toshikazu Ebisuzaki, G. Sáez-Cano, M. Rybczyński, Andreas A. Berlind, L. R. Wiencke, James H. Adams, H. Ikeda, M. Di Martino, S. Yoshida, J. Szabelski, A. Marini, T. Pierog, J. Watanabe, G. Cordero, M. Takeda, G. Castellinic, Livio Conti, C. De Donato, A. Zuccaro Marchi, G. Giraudo, Soon-Wook Kim, Katsuaki Asano, S. Blin-Bondil, Markus Roth, A. Dell’Oro, Toshitaka Kajino, A. Haungs, S. Piraino, Jörn Wilms, D. Kolev, G. Osteria, Massimiliano Bonamente, O. A. Saprykin, Fausto Guarino, P. von Ballmoos, M. Ricci, J. Słomiński, T. Tymieniecka, H. Sato, J. Sledd, Valerie Connaughton, H. H. Silva Lopez, E. Kuznetsov, M. Putis, P. Baragatti, K. Higashide, C. Moretto, P. Galeotti, A. Sobey, Barbara Szabelska, R. Matev, Satoshi Wada, M. Nagata, T. Ogawa, Alexander Kusenko, A. Insolia, M. Kleifges, Gali Garipov, Ralph Engel, David B. Cline, J. F. Valdés-Galicia, L. G. Tkachev, S. Csorna, C. Tenzer, J. S. Kim, D. Maravilla, Yoshimasa Kurihara, T. Peter, H. Schieler, T. Sugiyama, G. Vankova, O. Martinez, K. Słomińska, V. S. Morozenko, Mitsuteru Sato, Francesco Isgrò, Angela V. Olinto, Tadeusz Wibig, Fernando López, Andrea Santangelo, E. G. Judd, B. Keilhauer, Katsuhiko Tsuno, Alfonso Monaco, Graciela B. Gelmini, D. Campana, T. Shibata, Taka Tomida, C. Blaksley, Frederic Trillaud, Y. Hachisu, Dmitry V. Naumov, Y. Arai, I. Kreykenbohm, Vladimir Andreev, Tokonatsu Yamamoto, K. Mase, R. Young, Frederic Jean Ronga, I. Rodríguez, Tomás Belenguer, S. Biktemerova, M. Sakata, C. Lachaud, Inkyu Park, S. Dagoret-Campagne, B. Mot, Y. Yamamoto, T. Shirahama, J.N. Capdevielle, Francesco Fenu, G. Catalano, S. Ahmad, N. Tajima, Piero Vallania, Y. Miyazaki, M. D. Sabau, Shigehiro Nagataki, J. Fujimoto, S. Falk, R. Bechini, Yukihiro Takahashi, M. Ave Pernas, C. González Alvarado, Pierre Barrillon, Ke Fang, Mark Christl, O. Tibolla, Marco Casolino, Claudio Fornaro, Z. Włodarczyk, Humberto Ibarguen Salazar, D. Ikeda, F. Sarazin, Piotr Orleanski, Silvia Ferrarese, H. J. Crawford, J. Bayer, Sergei A. Sharakin, J. Hernández Carretero, Mikhail Panasyuk, M. Unger, C. De Santis, Marc Weber, Shigeto Watanabe, J. Błȩcki, H. Tokuno, C. de la Taille, G. Roudil, B. Harlov, H. Lim, Carlo Vigorito, M. C. Maccarone, K. Kudela, M. Sanz Palomino, K. Katahira, L. Santiago Crúz, Jianyi Yang, M. Dupieux, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, R. Nava, Y. Karadzhov, N. Sakaki, M. Serra, Luis A. Anchordoqui, L. Valore, Rossella Caruso, Yoshiya Kawasaki, Simona Toscano, T. Batsch, H. Prieto, R. Cremonini, R. Tsenov, D. Allard, Guillaume Prévôt, Andrii Neronov, S. Selmane, M. E. Bertaina, A. Pollini, Pavel Klimov, I. Kaneko, Ken'ichi Nomoto, F. Tajima, Yoshitaka Itow, P. Gorodetzky, A. Anzalone, M. Bogomilov, T. Napolitano, M. Wille, M. Nagano Murakami, Y. Uchihori, K. Belov, F. Kajino, A. Ebersoldt, C. Catalano, H. W. Park, Yoshiki Tsunesada, Hajime Takami, Masaki Fukushima, T. Nakamura, N. Tone, Daisuke Yonetoku, M. Yu. Zotov, Susana Briz, M. D. Rodríguez Frías, Z. Plebaniak, J. Blümer, Michiyuki Chikawa, Hajime Yano, P. L. Biermann, D. Supanitsky, I. Rusinov, J. Geary, N. De Simone, Marcos Reyes, Shoichi Ogio, A. Jung, T. Paul, K. Yoshida, S. Sánchez, B. A. Khrenov, H. Miyamoto, G. Medina-Tanco, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, J. A. Morales de los Ríos, Susumu Inoue, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, Dmitri Semikoz, T. Mernik, I. V. Yashin, L. Marcelli, Thomas J. Weiler, S. Perez Cano, Kenji Shinozaki, A. Bruno, Karl Mannheim, Michael S. Briggs, A. J. de Castro, K. Kawai, T. Patzak, Akinori Saito, G. Distratis, F. Cafagna, G. Modestino, E. Joven, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrã­guez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., Zuccaro Marchi, A., and Słomiński, J. more...

Subjects
Atmospheric physics, Ciencias Físicas, Space Shuttle, Cosmic ray, Elves, Jets - Atmospheric phenomena, Sprites, Transient Luminous Events, Astronomy and Astrophysics, Space and Planetary Science, Astrophysics, ELVES, Elve, Transient Luminous Events, Elves, Sprites, Jets - Atmospheric phenomena, law.invention, Telescope, purl.org/becyt/ford/1 [https], law, International Space Station, Ultra-high-energy cosmic ray, Astrophysique, Physics, Astronomy, purl.org/becyt/ford/1.3 [https], Astronomie, Astronomy and Astrophysic, Sciences de l'espace, Astronomía, Moment (physics), Sprite, Satellite, Transient Luminous Event, CIENCIAS NATURALES Y EXACTAS
Abstract

注記: The JEM-EUSO Collaboration 289名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2014-11-17, Note: The JEM-EUSO Collaboration 289members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150236000 more...

Published
2015
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24. Gamma-ray burst investigation via polarimetry and spectroscopy (GRIPS)

Author

R. Bellazini, Andreas Zoglauer, M. I. Panasyuk, René Hudec, L. G. Balasz, R. Marcinkowski, V. M. Lipunov, Mark Pearce, Felix Ryde, Andrei M. Bykov, Elena Pian, D. Hartmann, Guido Barbiellini, Andrew W. Strong, A. Majczyna, Zsolt Bagoly, Sandra Savaglio, J. Kiener, István T. Horváth, B. K. Lubsandorgiev, R. V. Poleschuk, Sheila McBreen, Vincent Tatischeff, Karl Mannheim, G. Wrochna, A. M. Chernenko, Martino Marisaldi, G. Bisnovaty-Kogan, A. Pollo, Attila Mészáros, A. F. Iyudin, A. G. Zabrodskij, J. Uvarov, S. Larsson, W. Dröge, S. E. Boggs, A. M. Cherepashuk, Gottfried Kanbach, Andreas von Kienlin, Norbert Langer, S. I. Svertilov, Dmitry Bisikalo, L. M. Zeleny, G. Dicocco, Jochen Greiner, Werner Collmar, Roland Diehl, B. McBreen, Lorraine Hanlon, Claudio Labanti, Cornelia B. Wunderer, Boris Shustov, E. Orlando, Marco Ajello, M. Gierlik, D. A. Varshalovich, Alexei Pozanenko, G. G. Lichti, L. B. Bezrukov, Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Greiner, J., Iyudin, A., Kanbach, G., Zoglauer, A., Diehl, R., Ryde, F., Hartmann, D., v. Kienlin, A., Mcbreen, S., Ajello, M., Bagoly, Z., Balasz, L. G., Barbiellini, G., Bellazini, R., Bezrukov, L., Bisikalo, D. V., Bisnovaty-Kogan, G., Boggs, S., Bykov, A., Cherepashuk, A. M., Chernenko, A., Collmar, W., Dicocco, G., Droege, W., Gierlik, M., Hanlon, L., Horvath, I., Hudec, R., Kiener, J., Labanti, C., Langer, N., Larsson, S., Lichti, G., Lipunov, V. M., Lubsandorgiev, B. K., Majczyna, A., Mannheim, K., Marcinkowski, R., Marisaldi, M., Mcbreen, B., Meszaros, A., Orlando, E, Panasyuk, M. I., Pearce, M., Pian, E., Poleschuk, R. V., Pollo, A., Pozanenko, A., Savaglio, S., Shustov, B., Strong, A., Svertilov, S., Tatischeff, V., Uvarov, J., Varshalovich, D. A., Wunderer, C. B., Wrochna, G., Zabrodskij, A. G., and Zeleny, L. M. more...

Subjects
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, education, Early universe, ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, Polarimetry, Astrophysics, Compton and pair creation telescope, 7. Clean energy, 01 natural sciences, Primary (astronomy), Nucleosynthesis, Observatory, 0103 physical sciences, Nuclear astrophysics, Hardware_ARITHMETICANDLOGICSTRUCTURES, Spectroscopy, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, health care economics and organizations, ComputingMethodologies_COMPUTERGRAPHICS, media_common, Physics, 010308 nuclear & particles physics, gamma-ray bursts, Astrophysics::Instrumentation and Methods for Astrophysics, nucleosynthesis, Astronomy, Astronomy and Astrophysics, social sciences, early universe, Universe, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 95.55.Ka * 98.70.Rz * 26.30.-k, Space and Planetary Science, Compton and Pair creation telescope, Gamma-ray bursts, Gamma-ray burst
Abstract

The primary scientific goal of the GRIPS mission is to revolutionize our understanding of the early universe using gamma-ray bursts. We propose a new generation gamma-ray observatory capable of unprecedented spectroscopy over a wide range of gamma-ray energies (200 keV-50 MeV) and of polarimetry (200-1000 keV). The gamma-ray sensitivity to nuclear absorption features enables the measurement of column densities as high as 10(28)cm (-aEuro parts per thousand 2). Secondary goals achievable by this mission include direct measurements of all types of supernova interiors through gamma-rays from radioactive decays, nuclear astrophysics with massive stars and novae, and studies of particle acceleration near compact stars, interstellar shocks, and clusters of galaxies. more...

Published
2009
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