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551. The JEM-EUSO instrument

Author

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

Subjects
Ciencias Físicas, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, law.invention, Telescope, Optics, cosmic rays, law, International Space Station, Cosmic rays, Physics, International space station, UHECR, Astronomy and Astrophysics, Space and Planetary Science, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Celestial sphere, Astronomy and Astrophysic, Astronomía, Refracting telescope, Focal surface, business, Event (particle physics), CIENCIAS NATURALES Y EXACTAS
Abstract

In this paper we describe the main characteristics of the JEM-EUSO instrument. The Extreme Universe Space Observatory on the Japanese Experiment Module (JEM-EUSO) of the International Space Station (ISS) will observe Ultra High-Energy Cosmic Rays (UHECR) from space. It will detect UV-light of Extensive Air Showers (EAS) produced by UHECRs traversing the Earth?s atmosphere. For each event, the detector will determine the energy, arrival direction and the type of the primary particle. The advantage of a space-borne detector resides in the largefield of view, using a target volume of about 10 12 tons of atmosphere, far greater than what is achievable from ground. Another advantage is a nearly uniform sampling of the whole celestial sphere. The corresponding increase in statistics will help to clarify the origin and sources of UHECRs and characterize the environment traversed during their production and propagation. JEM-EUSO is a 1.1 ton refractor telescope using an optics of 2.5 m diameter Fresnel lenses to focus the UV-light from EAS on a focal surface composed of about 5000 multi-anode photomultipliers, for a total of 3x10^5 channels. A multi-layer parallel architecture handles front-end acquisition, selecting and storing valid triggers. Each processing level filters the events with increasingly complex algorithms using FPGAs and DSPs to reject spurious events and reduce thedata rate to a value compatible with downlink constraints. 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 Alcala; 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: Bobik, P.. Institute of Experimental Physics; Eslovaquia Fil: Bogomilov, M.. University of Sofia; Bulgaria 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: Casolino, Marco. RIKEN; Japón Fil: Kajino, Fumiyoshi. National Astronomical Observatory; Japón Fil: Piotrowski, Lech Wiktor. RIKEN; Japón Fil: The JEM-EUSO Collaboration.

Published
2015

552. A balloon-borne prototype for demonstrating the concept of JEM-EUSO

Author

E. Parizot, J. Szabelski, M. D. Rodríguez Frías, Toshikazu Ebisuzaki, G. Osteria, A. Ebersoldt, A. Jung, K. Tusno, P. Danto, M. Dupieux, P. Picozza, Andrea Santangelo, S. Dagoret, J. Evrard, G. Medina-Tanco, G. Roudil, P. von Ballmoos, M. Ricci, James H. Adams, H. Prieto, Y. Takizawa, P. Gorodetzky, Guillaume Prévôt, Inkyu Park, G. Distratis, F. Cafagna, Pierre Barrillon, Marco Casolino, J. Bayer, Valentina Scotti, A. Haungs, Yoshiya Kawasaki, B. Mot, M. E. Bertaina, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), 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), 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), Centre National d'Études Spatiales [Toulouse] (CNES), AstroParticule et Cosmologie (APC (UMR_7164)), 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), APC - Astrophysique des Hautes Energies (APC - AHE), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-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)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), JEM-EUSO, 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), 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), 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)-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)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Von Ballmoos, P., Santangelo, A., Adams, J. H., Barrillon, P., Bayer, J., Bertaina, M., Cafagna, F., Casolino, M., Dagoret, S., Danto, P., Distratis, G., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Evrard, J., Gorodetzky, P., Haungs, A., Jung, A., Kawasaki, Y., Medina-Tanco, G., Mot, B., Osteria, G., Parizot, E., Park, I. H., Picozza, P., Prévôt, G., Prieto, H., Ricci, M., Rodríguez Frías, M. D., Roudil, G., Scotti, V., Szabelski, J., Takizawa, Y., Tusno, K., 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), 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), 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)-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)-Dipartimento di Astronomia, Universita degli Studi di Bologna, and Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)

Subjects
Atmospheric Science, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, Aerospace Engineering, Cosmic ray, Balloon, 01 natural sciences, 7. Clean energy, law.invention, Telescope, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], law, Observatory, 0103 physical sciences, Ultraviolet light, Cosmic-ray observatory, 010303 astronomy & astrophysics, Stratospheric balloon, Remote sensing, Physics, Balloon-borne instrumentation, 010308 nuclear & particles physics, Extragalactic cosmic-rays, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Ultra-high energy cosmic rays, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Geophysics, Pathfinder, Space and Planetary Science, Physics::Space Physics, General Earth and Planetary Sciences, Astrophysics::Earth and Planetary Astrophysics
Abstract

EUSO-BALLOON has been conceived as a pathfinder for JEM-EUSO, a mission concept for a space-borne wide-field telescope monitoring the Earth's nighttime atmosphere with the objective of recording the ultraviolet light from tracks initiated by ultra-high energy cosmic rays. Through a series of stratospheric balloon flights performed by the French Space Agency CNES, EUSO-BALLOON will serve as a test-bench for the key technologies of JEM-EUSO. EUSO-BALLOON shall perform an end-to-end test of all subsystems and components, and prove the global detection chain while improving our knowledge of the atmospheric and terrestrial ultraviolet background. The balloon-instrument also has the potential to detect for the first time UV-light generated by atmospheric air-shower from above, marking a milestone in the development of UHECR science, and paving the way for any future large scale, space-based ultra-high energy cosmic ray observatory. © 2013 COSPAR. Published by Elsevier Ltd. All rights reserved.

Published
2014

553. Performance of the EUSO-Balloon electronics

Author

J. Karczmarczyk, H. Miyamoto, L. Santiago, C. Blaksley, J. Rojas, S. Dagoret, J. Bayer, C. de la Taille, C. Moretto, S. Blin, Valentina Scotti, S. Bacholle, J. Szabelski, F. Cafagna, G. Osteria, Claudio Fornaro, F. Perfetto, J. A. Rabanal Reina, Pierre Barrillon, G. A. Medina Tanco, P. Gorodetzky, P. Prat, A. Jung, Inkyu Park, Guillaume Prévôt, H. Silva, 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)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11), JEM-EUSO, 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Barrillon, P., Bacholle, S., Bayer, J., Blaksley, C., Blin, S., Cafagna, F., Dagoret, S., Fornaro, C., Gorodetzky, P., Jung, A., Karczmarczyk, J., De La Taille, C., Tanco, G. Medina, Miyamoto, H., Moretto, C., Osteria, G., Park, I., Perfetto, F., Prévôt, G., MARTIN PRATS, MARIA ANGELES, Reina, J. Rabanal, Rojas, J., Santiago, L., Scotti, V., Silva, H., Szabelski, J., Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-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)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)

Subjects
architecture, Computer science, Photodetector, 02 engineering and technology, algorithms, Balloon, 01 natural sciences, Analogue electronic circuit, law.invention, Data processing system, Telescope, law, Front-end electronics for detector readout, 0103 physical sciences, Detector control systems (detector and experiment monitoring and slowcontrol systems, architecture, hardware, algorithms, databases), 0202 electrical engineering, electronic engineering, information engineering, hardware, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Electronics, Instrumentation, Mathematical Physics, Control and monitor systems online, 010308 nuclear & particles physics, business.industry, Detector control systems (detector and experiment monitoring and slow- control systems, Electrical engineering, 020207 software engineering, Analogue electronic circuits, electronics: readout, photon: detector, databases), business, performance
Abstract

International audience; The 24th of August 2014, the EUSO-Balloon instrument went for a night flight for several hours, 40 km above Timmins (Canada) balloon launching site, concretizing the hard work of an important part of the JEM-EUSO collaboration started 3 years before. This instrument consists of a telescope made of two lenses and a complex electronic chain divided in two main sub-systems: the PDM (Photo Detector Module) and the DP (Data Processor). Each of them is made of several innovative elements developed and tested in a short time. This paper presents their performances before and during the flight.

Published
2016

554. EUSO-BALLOON a pathfinder for detecting UHECR's from the edge of space

Author

G. Osteria, A. Ebersoldt, S. Dagoret, Katsuhiko Tsuno, Pierre Barrillon, G. Distratis, A. Jung, G. Roudil, Andrea Santangelo, Guillaume Prévôt, F. Cafagna, Toshikazu Ebisuzaki, G. Medina-Tanco, J. Bayer, B. Mot, Valentina Scotti, E. Parizot, P. Picozza, Marco Casolino, Yoshiya Kawasaki, M. Dupieux, P. Gorodetzky, M. E. Bertaina, A. Haungs, M. D. Rodríguez Frías, J. Szabelski, P. von Ballmoos, M. Ricci, Il Han Park, Y. Takizawa, James H. Adams, H. Prieto, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-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)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), 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), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), 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)-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)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), 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), K.-H. Kampert, M. Fukushima, R. Engel, B. Pattison, JEM-EUSO, Von Ballmoos, P., Dagoret, S., Santangelo, A., Adams, J. H., Barrillon, P., Bayer, J., Bertaina, M., Cafagna, F., Casolino, M., Distratis, G., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Gorodetzky, P., Haungs, A., Jung, A., Kawasaki, Y., Medina-Tanco, G., Mot, B., Osteria, G., Parizot, E., Park, I. H., Picozza, P., Prévôt, G., Prieto, H., Ricci, M., Frías, M. D. R., Roudil, G., Scotti, V., Szabelski, J., Takizawa, Y., Tsuno, K., 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), 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), 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)-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)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), 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), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), 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)-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)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)

Subjects
Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 010308 nuclear & particles physics, business.industry, QC1-999, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics, Balloon, 7. Clean energy, 01 natural sciences, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Pathfinder, Observatory, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Enhanced Data Rates for GSM Evolution, Aerospace engineering, Experimental methods, business, 010303 astronomy & astrophysics, Stratospheric balloon
Abstract

EUSO-Balloon has been conceived as a pathfinder mission for JEM-EUSO, to perform an end-to-end test of the subsystems and components, and to prove the global detection chain while improving our knowledge of the atmospheric and terrestrial UV background. Through a series of stratospheric balloon flights performed by the French Space Agency CNES, EUSO-BALLOON will serve as an evolutive test-bench for all the key technologies of JEM-EUSO. EUSO-Balloon also has the potential to detect Extensive Air Showers from above, marking a key milestone in the development of UHECR science, and paving the way for any future large scale, space-based UHECR observatory. © Owned by the authors, published by EDP Sciences, 2013.

Published
2012

557. Dataset of night-time emissions of the Earth in the near UV range (290-430 nm), with 6.3 km resolution in the latitude range -51.6<L<+51.6 degrees, acquired on board the International Space Station with the Mini-EUSO detector.

Author

Marcelli L, Bolmgren K, Barghini D, Battisti M, Blaksley C, Blin S, Belov A, Bertaina M, Bianciotto M, Bisconti F, Cambiè G, Capel F, Casolino M, Churilo I, Crisconio M, Taille C, Ebisuzaki T, Eser J, Fenu F, Franceschi MA, Fuglesang C, Golzio A, Gorodetzky P, Kasuga H, Kajino F, Klimov P, Kuznetsov V, Manfrin M, Mascetti G, Marszal W, Miyamoto H, Murashov A, Napolitano T, Ohmori H, Olinto A, Parizot E, Picozza P, Piotrowski LW, Plebaniak Z, Prevot G, Reali E, Romoli G, Ricci M, Sakaki N, Shinozaki K, Szabelski J, Takizawa Y, Vagelli V, Valentini G, Vrabel M, and Wiencke L

Abstract

The data presented in this article are related to the research paper entitled " Observation of night-time emissions of the Earth in the near UV range from the International Space Station with the Mini-EUSO detector " (Remote Sensing of Environment, Volume 284, January 2023, 113336, https://doi.org/10.1016/j.rse.2022.113336). The data have been acquired with the Mini-EUSO detector, an UV telescope operating in the range 290-430 nm and located inside the International Space Station. The detector was launched in August 2019, and it has started operations from the nadir-facing UV-transparent window in the Russian Zvezda module in October 2019. The data presented here refer to 32 sessions acquired between 2019-11-19 and 2021-05-06. The instrument consists of a Fresnel-lens optical system and a focal surface composed of 36 multi-anode photomultiplier tubes, each with 64 channels, for a total of 2304 channels with single photon counting sensitivity. The telescope, with a square field-of-view of 44°, has a spatial resolution on the Earth surface of 6.3 km and saves triggered transient phenomena with a temporal resolution of 2.5 µs and 320 µs. The telescope also operates in continuous acquisition at a 40.96 ms scale. In this article, large-area night-time UV maps obtained processing the 40.96 ms data, taking averages over regions of some specific geographical areas (e.g., Europe, North America) and over the entire globe, are presented. Data are binned into 0.1 °  × 0.1 ° or 0.05 °  × 0.05 ° cells (depending on the scale of the map) over the Earth's surface. Raw data are made available in the form of tables (latitude, longitude, counts) and .kmz files (containing the .png images). These are - to the best of our knowledge - the highest sensitivity data in this wavelength range and can be of use to various disciplines., Competing Interests: The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper., (© 2023 The Author(s).)

Published
2023
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558. A Review of the EUSO-Balloon Pathfinder for the JEM-EUSO Program.

Author

Adams JH Jr, Ahmad S, Allard D, Anzalone A, Bacholle S, Barrillon P, Bayer J, Bertaina M, Bisconti F, Blaksley C, Blin-Bondil S, Bobík P, Cafagna F, Campana D, Capel F, Casolino M, Cassardo C, Catalano C, Cremonini R, Dagoret-Campagne S, Danto P, Del Peral L, de la Taille C, Díaz Damian A, Dupieux M, Ebersoldt A, Ebisuzaki T, Eser J, Evrard J, Fenu F, Ferrarese S, Fornaro C, Fouka M, Gorodetzky P, Guarino F, Guzman A, Hachisu Y, Haungs A, Judd E, Jung A, Karczmarczyk J, Kawasaki Y, Klimov PA, Kuznetsov E, Mackovjak S, Manfrin M, Marcelli L, Medina-Tanco G, Mercier K, Merino A, Mernik T, Miyamoto H, Morales de Los Ríos JA, Moretto C, Mot B, Neronov A, Ohmori H, Olinto AV, Osteria G, Panico B, Parizot E, Paul T, Picozza P, Piotrowski LW, Plebaniak Z, Pliego S, Prat P, Prévôt G, Prieto H, Putis M, Rabanal J, Ricci M, Rojas J, Rodríguez Frías MD, Roudil G, Sáez Cano G, Sahnoun Z, Sakaki N, Sanchez JC, Santangelo A, Sarazin F, Scotti V, Shinozaki K, Silva H, Soriano JF, Suino G, Szabelski J, Toscano S, Tabone I, Takizawa Y, von Ballmoos P, Wiencke L, Wille M, and Zotov M

Abstract

EUSO-Balloon is a pathfinder for JEM-EUSO , the mission concept of a spaceborne observatory which is designed to observe Ultra-High Energy Cosmic Ray (UHECR)-induced Extensive Air Showers (EAS) by detecting their UltraViolet (UV) light tracks "from above." On August 25, 2014, EUSO-Balloon was launched from Timmins Stratospheric Balloon Base (Ontario, Canada) by the balloon division of the French Space Agency CNES. After reaching a floating altitude of 38 km, EUSO-Balloon imaged the UV light in the wavelength range ∼290-500 nm for more than 5 hours using the key technologies of JEM-EUSO . The flight allowed a good understanding of the performance of the detector to be developed, giving insights into possible improvements to be applied to future missions. A detailed measurement of the photoelectron counts in different atmospheric and ground conditions was achieved. By means of the simulation of the instrument response and by assuming atmospheric models, the absolute intensity of diffuse light was estimated. The instrument detected hundreds of laser tracks with similar characteristics to EASs shot by a helicopter flying underneath. These are the first recorded laser tracks measured from a fluorescence detector looking down on the atmosphere. The reconstruction of the direction of the laser tracks was performed. In this work, a review of the main results obtained by EUSO-Balloon is presented as well as implications for future space-based observations of UHECRs., (© The Author(s) 2022.)

Published
2022
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562. Charged-pion production in noninclusive proton-nucleus interactions at 0.8 and 1.6 GeV incident energies.

Author

Lemaire M, Trzaska M, Alard JP, Augerat J, Bachelier D, Bastid N, Boyard J, Cavata C, Charmensat P, Dupieux P, Gorodetzky P, Gosset J, Hennino T, Jourdain J, Le Merdy A, L'Hôte D, Lucas B, Marroncle J, Montarou G, Parizet M, Poitou J, Qassoud D, Radvanyi P, Ramstein B, Rahmani A, Roy-Stephan M, Valette O, Zupranski P, Cugnon J, and Vandermeulen J

Published
1991
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563. Exclusive measurements of mean pion multiplicities in 4He-nucleus reactions from 200 to 800 MeV/nucleon.

Author

L'Hôte D, Alard JP, Augerat J, Babinet R, Brochard F, Fodor Z, Fraysse L, Girard J, Gorodetzky P, Gosset J, Laspalles C, Lemaire MC, Lucas B, Montarou G, Parizet MJ, Poitou J, Racca C, Schimmerling W, Tamain JC, Terrien Y, Valero J, Cugnon J, and Vandermeulen J

Subjects
Carbon, Copper, Energy Transfer, Ions, Lead, Monte Carlo Method, Nuclear Physics, Helium, Mesons, Models, Theoretical, Protons, Radiometry
Abstract

Mean multiplicities of pi+ and pi- in 4He collisions with C, Cu, and Pb at 200, 600, and 800 MeV/u, and with C and Pb at 400 MeV/u have been measured using the large solid angle detector Diogene. The independence of pion multiplicity on projectile incident energy, target mass and proton multiplicity is studied in comparison with intra-nuclear cascade predictions. The discrepancy between experimental results and theory is pointed out and discussed.

Published
1987
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564. Nuclear collective flow and charged-pion emission in Ne-nucleus collisions at E/A = 800 MeV.

Author

Gosset J, Valette O, Alard JP, Augerat J, Babinet R, Bastid N, Brochard F, De Marco N, Dupieux P, Fodor Z, Fraysse L, Gorodetzky P, Lemaire MC, L'Hôte D, Lucas B, Marroncle J, Montarou G, Parizet MJ, Poitou J, Racca C, Rahmani A, Schimmerling W, and Terrien Y

Subjects
Elementary Particles, Lead, Nuclear Physics, Energy Transfer, Mesons, Models, Theoretical, Neon
Abstract

Triple-differential cross sections of charged pions were measured for collisions of Ne projectiles at E/A = 800 MeV with NaF, Nb, and Pb targets. The reaction plane was estimated event by event from the light-baryon momentum distribution. For heavy targets, preferential emission of charged pions away from the interaction zone towards the projectile side was observed in the transverse direction. Such a preferential emission, which is not predicted by cascade calculations, may be attributed to a stronger pion absorption by the heavier spectator remnant.

Published
1989
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565. Proton-proton correlations at small relative momentum in neon-nucleus collisions at E/A=400 and 800 MeV.

Author

Dupieux P, Alard JP, Augerat J, Babinet R, Bastid N, Brochard F, Charmensat P, De Marco N, Fanet H, Fodor Z, Fraysse L, Girard J, Gorodetzky P, Gosset J, Laspalles C, Lemaire MC, L'Hôte D, Lucas B, Marroncle J, Montarou G, Parizet MJ, Poitou J, Qassoud D, Racca C, and Schimmerling W

Subjects
Carbon, Elementary Particles, Lead, Models, Theoretical, Niobium, Particle Accelerators, Sodium Fluoride, Energy Transfer, Neon, Nuclear Physics, Protons
Abstract

Proton-proton small angle correlations have been measured in neon-nucleus collisions, using the 4 pi detector Diogene, at 400 and 800 MeV per nucleon incident energies. Values of the size of the emitting region are obtained by comparison with the Koonin formula, taking into account the biases of the apparatus. The dependence of the density on target mass and incident energy is also analysed.

Published
1988
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