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1. Spectra of solar neutrons with energies of ~10–1000 MeV in the PAMELA experiment in the flare events of 2006–2015

Author: Alfonso Monaco, C. De Santis, R. Sparvoli, Roberto Bellotti, A. M. Galper, M. Merge, Yu. T. Yurkin, G. A. Bazilevskaya, A. N. Kvashnin, S. Bottai, V. Di Felice, Per Carlson, M. Bongi, F. Cafagna, G. Castellini, Sergey Koldashov, Alexey Leonov, Matteo Martucci, V. Bonvicini, V. V. Malakhov, Andrea Vacchi, E. A. Bogomolov, N. Zampa, D. Campana, L. Marcelli, M. Simon, Yuri Stozhkov, Mark Pearce, S. B. Ricciarini, O. Adriani, A. Bruno, Marco Casolino, Sergey Koldobskiy, A. V. Karelin, Marco Ricci, W. Menn, M. F. Runtso, G. C. Barbarino, Riccardo Munini, S. A. Voronov, P. Spillantini, P. Papini, Nicola Mori, A. G. Mayorov, E. Vannuccini, S. Y. Krutkov, G. Zampa, Beatrice Panico, G. Osteria, P. Picozza, G. I. Vasilyev, E. Mocchiutti, V. V. Mikhailov, Mirko Boezio, A. A. Kvashnin, Bogomolov, E. A., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Karelin, A. V., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Pearce, M., Ricci, M., Ricciarini, S. B., Runtso, M. F., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., and Yurkin, Y. T.
Subjects: Physics Solar flare, Solar neutrons, Space experiments: Neutrons, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Hadron, General Physics and Astronomy, Flux, Astrophysics, 01 natural sciences, Spectral line, law.invention, Nuclear physics, Physics and Astronomy (all), Space experiment, law, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Neutron detection, Neutron, Nuclear Experiment, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Settore FIS/01, Physics, Solar flare, Physics::Space Physics, Flare
Abstract: The first results from measuring the spectra of solar neutrons with energies of ~10-1000 MeV in the solar flares of 2006-2015 observed by the PAMELA international space experiment are presented. The PAMELA neutron detector with 3He counters and a moderator with an area of 0.18 m2 allows us to estimate the flux of solar neutrons during solar flares. Solar neutrons with energies of ~10-1000 MeV likely occurred in 21 out of the 24 analyzed flares of 2006-2015. © 2017, Allerton Press, Inc.
Published: 2017

2. Secondary positrons and electrons in near-Earth space in the PAMELA experiment

Author: A. G. Mayorov, Alfonso Monaco, S. Y. Krutkov, D. Campana, Alexey Leonov, Matteo Martucci, M. Merge, Marco Casolino, Sergey Koldobskiy, Yu. T. Yurkin, G. C. Barbarino, M. Bongi, N. Zampa, V. Bonvicini, P. Picozza, G. Zampa, Beatrice Panico, L. Marcelli, Andrea Vacchi, E. Mocchiutti, V. Di Felice, A. Bruno, A. A. Kvashnin, M. F. Runtso, S. A. Voronov, Sergey Koldashov, M. Simon, Mirko Boezio, Riccardo Munini, A. V. Karelin, Yuri Stozhkov, V. V. Malakhov, O. Adriani, W. Menn, G. A. Bazilevskaya, G. Osteria, P. Spillantini, S. Bottai, G. Castellini, Roberto Bellotti, A. M. Galper, E. A. Bogomolov, Marco Ricci, A. N. Kvashnin, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, G. I. Vasilyev, Nicola Mori, C. De Santis, V. V. Mikhailov, R. Sparvoli, Per Carlson, F. Cafagna, Mikhailov, V. V., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Karelin, A. V., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Pearce, M., Ricci, M., Ricciarini, S. B., Runtso, M. F., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., and Yurkin, Y. T.
Subjects: Settore FIS/01, Physics, PAMELA detector, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, Magnetosphere, Cosmic ray, Astrophysics, Electron, 01 natural sciences, law.invention, Atmosphere, Physics and Astronomy (all), symbols.namesake, Atmosphere of Earth, Positron, law, Van Allen radiation belt, Physics::Space Physics, 0103 physical sciences, symbols, Cosmology, Earth (planet), Earth atmosphere, Orbits, Positrons, Radiation belts Different mechanisms, Electron flux, Magnetic spectrometers, Near-earth spaces, Secondary particles, Trapped particle, Astrophysics::Earth and Planetary Astrophysics, 010306 general physics
Abstract: Fluxes of electrons and positrons with energies above ~100 MeV in the near-Earth space are measured with the PAMELA magnetic spectrometer aboard the Resurs DK-1 satellite launched on June 15, 2006, into a quasipolar orbit with an altitude of 350–600 km and an inclination of 70°. Calculating the trajectories of detected electrons and positrons in the magnetosphere of the Earth allows us to determine their origin and isolate particles produced during interaction between cosmic rays and the residual atmosphere. Spatial distributions of albedo, quasitrapped, and trapped (in the radiation belt) positrons and electrons are presented. The ratio of positron and electron fluxes suggests that the fluxes of trapped particles of the radiation belt and quasitrapped secondary particles have different mechanisms of formation.
Published: 2017

3. EUSO-TA - First results from a ground-based EUSO telescope

Author: N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, M. Haiduc, Lech Wiktor Piotrowski, S. Bartocci, J. A. Morales de los Ríos, N. Belkhalfa, Susumu Inoue, S. Yoshida, J. Szabelski, S. B. Thomas, K. Kudela, M. D. Rodríguez Frías, Naoto Sakaki, Z. Plebaniak, Thomas Schanz, Michiyuki Chikawa, M. Di Martino, A. Marini, Toshikazu Ebisuzaki, G. Roudil, B. Harlov, J. F. Valdés-Galicia, G. Osteria, Carlo Vigorito, L. G. Tkachev, Josef Jochum, S. Naitamor, G. Vankova, A. Caramete, Livio Conti, K. Martens, D. Maravilla, L. López Campano, J. Fernández-Soriano, R. Matev, Yoshihiko Mizumoto, Sebastián Franchini, S. Biktemerova, A. Ebersoldt, Daisuke Ikeda, A. Zuccaro Marchi, Hajime Takami, Masaki Fukushima, E. G. Judd, O. Larsson, H. J. Crawford, M. Serra, Jörn Wilms, J. Karczmarczyk, M. Ave Pernas, D. Kolev, H. Krantz, Mohammed Bakiri, Luis A. Anchordoqui, I. Kaneko, O. A. Saprykin, Estíbaliz Gascón, S. Turriziani, A. Belov, Valerie Connaughton, L. Marcelli, Konstantin Belov, A. Anzalone, T. Napolitano, Toshitaka Kajino, Francesco Fenu, N. Tone, Christer Fuglesang, Humberto Ibarguen Salazar, K. Benmessai, A. Guzmán, C. Lachaud, Daisuke Yonetoku, J. Blecki, José Meseguer, Angel Sanz-Andrés, Shinsuke Abe, P. Galeotti, R. Attallah, J. Hernández Carretero, H. Tokuno, B. Beldjilali, Takayuki Tomida, Santiago Pindado, S. Jeong, T. Shirahama, Y. Tsunesada, Junpei Fujimoto, M. Yu. Zotov, Silvia Ferrarese, Katsuaki Asano, Alfonso Monaco, H. Attoui, E. M. Popescu, B. A. Khrenov, A. Pagliaro, J. Genci, L. Villaseñor, C. Tenzer, T. Sugiyama, Piergiorgio Picozza, R. Tsenov, Satoshi Wada, N. Mebarki, W. Painter, Piotr Orleanski, T. Paul, A. Pollini, Pavel Klimov, B. Panico, Y. Karadzhov, Isabel Pérez-Grande, F. Sarazin, Zbigniew Wlodarczyk, Marc Weber, F. Bisconti, C. González Alvarado, Tokonatsu Yamamoto, E. Bozzo, T. Ogawa, M. C. Talai, J.N. Capdevielle, G. Sáez Cano, Angela V. Olinto, Javier Licandro, M. Rezazadeh, Andrea Santangelo, A. Kusenko, Katsuhiko Tsuno, Yoshio Arai, I. Kreykenbohm, Pierre Sokolsky, G. Masciantonio, Y. Martín, S. Selmane, John Belz, L. Placidi, M. Kleifges, P. L. Biermann, Tomás Belenguer, Yoshitaka Itow, N. Tajima, Giuseppe Giraudo, M. Takeda, M. A. Mendoza, G. Medina-Tanco, Shigehiro Nagataki, Barbara Szabelska, T. Peter, O. Martinez, Gordon Thomson, Toshiyuki Nonaka, F. Ronga, Gustavo Alonso, J. Watanabe, J. Tubbs, I. Rusinov, I. V. Yashin, M. Fouka, Osvaldo Catalano, M. Martucci, Fausto Guarino, J. Yang, P. von Ballmoos, M. Ricci, H. Miyamoto, M. Sanz Palomino, S. E. Csorna, Amine Ahriche, Simona Toscano, A. Bruno, Jeong-Sook Kim, Kenji Shinozaki, L. Caramete, Marcos Reyes, Roberto Bellotti, K. Mase, Gali Garipov, Joowon Lee, M. Flamini, B. Vlcek, T. Patzak, James H. Adams, H. Prieto, N. Blanc, R. Cremonini, S. Dagoret-Campagne, Francesca Capel, Y. Takizawa, S. Mackovjak, J. L. Marcos, E. Kuznetsov, G. Puehlhofer, D. Supanitsky, R. Weigand Muñoz, P. Gorodetzky, Shoichi Ogio, Johannes Eser, P. Baragatti, Austin Cummings, M. Wille, Y. Uchihori, A. La Barbera, Guillaume Prévôt, S. Blin-Bondil, R. Greg, I. Stan, G. Cordero, Malek Mustafa, J. Mimouni, M. Bogomilov, Z. Polonski, D. Campana, H. Khales, L. Allen, F. Lakhdari, F. Kajino, Maciej Rybczyński, Inkyu Park, M. Putis, S. S. Meyer, A. Weindl, Mark Christl, O. Tibolla, S. Pliego, K. Kawai, Akinori Saito, Ovidiu Vaduvescu, Claudio Cassardo, Dmitri Semikoz, Andrés Merino, P. Carlson, Yuichiro Tameda, John N. Matthews, M. Traïche, F. Cafagna, E. Joven, Y. Hachisu, F. Perfetto, Bruno Spataro, B. Pastirčák, Pierre Barrillon, Eduardo García-Ortega, Sergei A. Sharakin, Piero Vallania, R. Young, Yukihiro Takahashi, José Luis Sánchez, M. D. Sabau, M. Suzuki, Marco Casolino, Claudio Fornaro, Mikhail Panasyuk, A. Neronov, Sergio Fernández-González, J. Bayer, M. C. Maccarone, Valentina Scotti, C. de la Taille, A. Kedadra, I. Dutan, I. S. Zgura, G. Cotto, K. Katahira, M. Mahdi, C. De Donato, Soon-Wook Kim, Yoshimasa Kurihara, G. Chiritoi, H. Schieler, A. Jung, A. Haungs, S. Piraino, H. Lahmar, Antonella Castellina, Mitsuteru Sato, T. Jammer, J. Rabanal, G. Abdellaoui, Hajime Yano, Heungsu Shin, R. Nava, Ralph Engel, Takahiro Fujii, Rossella Caruso, Toshiki Tajima, Hitoshi Ohmori, K. S. Caballero, Hiroyuki Sagawa, Yoshiya Kawasaki, A. Radu, A. Menshikov, Hirohiko M. Shimizu, T. Djemil, D. Allard, Alberto Cellino, S. Kalli, J. Watts, M. E. Bertaina, C. De Santis, L. R. Wiencke, M. Vrabel, P. Prat, Ken'ichi Nomoto, Z. Sahnoune, W. Hidber Cruz, S. Bacholle, Francesco Isgrò, W. Marszał, J. C. Sanchez Balanzar, AstroParticule et Cosmologie (APC (UMR_7164)), 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), 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), Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), 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), 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 de Paris (UP), 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), École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), 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)-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)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), 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), Abdellaoui, G., Abe, S., Adams, J., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Ave Pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Belz, J. W., Benmessai, K., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blanc, N., Blecki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Cordero, G., Cotto, G., Crawford, H. J., Cremonini, R., Csorna, S., Cummings, A., Dagoret-Campagne, S., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Fernández-Soriano, J., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., González Alvarado, C., Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández Carretero, J., Hidber Cruz, W., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kolev, D., Krantz, H., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., López Campano, L., Maccarone, M. C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J., Marini, A., Marszal, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Mustafa, M., Matev, R., Matthews, J., Mebarki, N., Medina-Tanco, G., Mendoza, M. A., Menshikov, A., Merino, A., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Morales de los Ríos, J. A., Nagataki, S., Naitamor, S., Napolitano, T., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonski, Z., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A. A., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez Frías, M. D., Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M., Sáez Cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sanchez Balanzar, J. C., Sánchez, J. L., Santangelo, A., Sanz-Andrés, A., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H. M., Shin, H. S., Shinozaki, K., Shirahama, T., Sokolsky, P., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tameda, Y., Tenzer, C., Thomas, S. B., Thomson, G. B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts, J., Weber, M., Weigand Muñoz, R., Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S., Zotov, M. Yu., Zuccaro Marchi, A., 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: Fresnel lens, Photomultiplier, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Night sky, JEM-EUSO, Cosmic ray, Field of view, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, cosmic rays, EAS, UHECR, Astronomy and Astrophysics, Aeronáutica, law.invention, Telescope, law, 0103 physical sciences, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, cosmic ray, Astrophysique, Physics, Fresnel len, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomie, Astronomía, Limiting magnitude, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: EUSO-TA is a ground-based telescope, installed at the Telescope Array (TA) site in Black Rock Mesa, Utah, USA. This is the first detector to successfully use a Fresnel lens based optical system and multi-anode photomultipliers (64 channels per tube, 2304 channels encompassing a 10.6° × 10.6° field of view) for detection of Ultra High Energy Cosmic Rays (UHECR). The telescope is located in front of one of the fluorescence detectors of the TA experiment. Since its installation in 2013, the detector has observed several ultra-high energy cosmic ray events and, in addition, meteors. The limiting magnitude of 5.5 on summed frames (∼ 3 ms) has been established. Measurements of the UV night sky emission in different conditions and moon phases and positions have been completed. The performed observations serve as a proof of concept for the future application of this detector technology., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2018

4. Measuring the albedo deuteron flux in the PAMELA satellite experiment

Author: Alfonso Monaco, G. Osteria, M. Merge, Nicola Mori, D. Campana, S. A. Voronov, Matteo Martucci, Per Carlson, Roberta Sparvoli, N. Zampa, Yu. T. Yurkin, Marco Casolino, Laura Rossetto, S. Y. Krutkov, G. I. Vasilyev, E. A. Bogomolov, A. G. Mayorov, F. Palma, R. Carbone, C. Pizzolotto, Valerio Formato, M. Simon, Riccardo Munini, L. Marcelli, Sergey Koldobskiy, W. Menn, C. De Santis, G. C. Barbarino, A. Vacchi, Marco Ricci, Mark Pearce, S. B. Ricciarini, V. V. Malakhov, C. De Donato, A. Bruno, A.A. Kvashnin, V. Di Felice, P. Papini, G. Zampa, Beatrice Panico, Yuri Stozhkov, Valentina Scotti, E. Vannuccini, P. Picozza, P. Spillantini, Alexey Leonov, N. De Simone, V. G. Zverev, Mirko Boezio, V. Bonvicini, O. Adriani, Sergey Koldashov, E. Mocchiutti, V. V. Mikhailov, Ritabrata Sarkar, S. Bottai, G. A. Bazilevskaya, G. Castellini, M. Bongi, F. Cafagna, I. A. Danilchenko, A. V. Karelin, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, S., Koldobskiya, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, I. A., Danilchenko, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. A., Kvashnin, A. N., Kvashnin, A., Leonov, V. V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Merge, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Stozhkov, Y. u. I., A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Yurkin, Y. u. T., G., Zampa, N., Zampa, V. G., Zverev, Koldobskiy, S., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Danilchenko, I. A., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. A., Kvashnin, A. N., Leonov, A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, L., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Zampa, G., Zampa, N., and Zverev, V. G.
Subjects: deuteron, Nuclear Theory, General Physics and Astronomy, Geomagnetism, Solar radiation Artificial Earth satellites, Energy interval, High-precision, Instrument setup, Cosmic ray, Spectral line, Latitude, law.invention, Physics and Astronomy (all), cosmic rays, PAMELA, law, Nuclear Experiment, Physics::Atmospheric and Oceanic Physics, Settore FIS/01, Physics, PAMELA detector, Astronomy, Albedo, Earth's magnetic field, Physics::Space Physics, PAMELA, cosmic rays, albedo particles, deuteron, Satellite, Astrophysics::Earth and Planetary Astrophysics, Nucleon, albedo particles
Abstract: The results of measuring albedo deuteron fluxes in the vicinity of the Earth are presented. The data were obtained in the PAMELA experiment conducted aboard the Resurs DK-1 artificial Earth satellite. High-precision detectors of the instrument setup allow us to identify albedo deuterons and measure their spectra in the energy interval from 70 to 600 MeV/nucleon at altitudes of 350-600 km for different geomagnetic latitudes.
Published: 2015

5. Deuteron spectrum measurements under radiation belt with PAMELA instrument

Author: V. G. Zverev, Yu. T. Yurkin, V. Bonvicini, Y. I. Stozhkov, R. Carbone, Sergey Koldobskiy, V. Di Felice, G. C. Barbarino, O. Adriani, W. Menn, N. Zampa, G. A. Bazilevskaya, Matteo Martucci, S. A. Voronov, M. Simon, Riccardo Munini, L. Marcelli, P. Papini, Piero Spillantini, E. A. Bogomolov, A. Vacchi, A. Bruno, Laura Rossetto, Alfonso Monaco, V. V. Malakhov, A. G. Mayorov, M. Merge, Per Carlson, G. Castellini, A. A. Kvashnin, S. Y. Krutkov, N. De Simone, Mark Pearce, S. B. Ricciarini, Sergey Koldashov, R. Sparvoli, E. Mocchiutti, Alexey Leonov, P. Picozza, Marco Ricci, S. Bottai, F. Cafagna, C. Pizzolotto, I. A. Danilchenko, Ritabrata Sarkar, D. Campana, V. V. Mikhailov, E. Vannuccini, G. I. Vasilyev, G. Zampa, Beatrice Panico, Marco Casolino, Valerio Formato, G. Osteria, Nicola Mori, C. De Santis, C. De Donato, Valentina Scotti, F. Palma, Mirko Boezio, A. V. Karelin, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, Massimo Bongi, Koldobskiy, S. A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Danilchenko, I. A., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. A., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, L., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., and Zverev, V. G.
Subjects: Albedo, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Cosmic ray, Radiation, 01 natural sciences, law.invention, Nuclear physics, symbols.namesake, law, Deuteron, PAMELA experiment, Radiation belt, 0103 physical sciences, Nuclear Experiment, 010303 astronomy & astrophysics, Settore FIS/01, Physics, Range (particle radiation), PAMELA detector, 010308 nuclear & particles physics, Van Allen radiation belt, symbols, Satellite, Nucleon
Abstract: In this work the results of data analysis of the deuteron albedo radiation obtained in the PAMELA experiment are presented. PAMELA is an international space experiment carried out on board of the satellite Resurs DK-1. The high precision detectors allow to register and identify cosmic ray particles in a wide energy range. The albedo deuteron spectrum in the energy range 70 - 600 MeV/nucleon has been measured. © 2015 Elsevier B.V..
Published: 2016

6. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

Author: Alfonso Monaco, A. N. Kvashnin, M. Merge, V. V. Mikhailov, P. Carlson, A. G. Mayorov, G. I. Vasiliev, R. Sparvoli, N. De Simone, G. Zampa, Beatrice Panico, M. Simon, N. Zampa, Sergey Koldashov, G. A. Bazilevskaya, Yu. T. Yurkin, C. De Santis, Yu. I. Stozhkov, V. V. Malakhov, S. Yu. Krutkov, P. Picozza, Roberto Bellotti, Mark Pearce, S. B. Ricciarini, F. Palma, A. M. Galper, P. Papini, Giuseppe Osteria, E. Vannuccini, Matteo Martucci, S. A. Koldobsky, E. Mocchiutti, F. Cafagna, A. V. Karelin, Mirko Boezio, D. Campana, S. Bottai, Maria Teresa Ricci, S. A. Voronov, Marco Casolino, C. De Donato, Nicola Mori, E. A. Bogomolov, Riccardo Munini, M. Bongi, P. Spillantini, O. Adriani, W. Menn, V. Di Felice, V. Bonvicini, G. C. Barbarino, G. Castellini, L. Marcelli, A. Vacchi, A. Bruno, Alexey Leonov, Mikhailov, V. V., Adriani, O., Barbarino, G., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F. S., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobsky, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Papini, P., Palma, F., Panico, B., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasiliev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Physics, Settore FIS/01, History, Antiparticle, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Polar orbit, Cosmic ray, Astrophysics, Electron, Cosmology, Electrons, Magnetic polarity, Orbits, Positrons, Computer Science Applications, Education, law.invention, Physics and Astronomy (all), Positron, law, Physics::Space Physics, Satellite, Astrophysics::Earth and Planetary Astrophysics
Abstract: Magnetic spectrometer PAMELA was launched onboard a satellite Resurs-DK1 into low-Earth polar orbit with altitude 350-600 km to study cosmic ray antiparticle fluxes in a wide energy range from ~ 100 MeV to hundreds GeV. This paper presents the results of observations of temporal variations of the positron and electron fluxes in the 2006-2015. The ratio of the positron and electron fluxes below 2 GV shows sharp increasing since 2014 due to changing of the polarity of the solar magnetic field.
Published: 2017

7. Solar modulation of cosmic deuteron fluxes in the PAMELA experiment

Author: Roberto Bellotti, A. M. Galper, V. V. Mikhailov, V. Bonvicini, Andrea Vacchi, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, M. Simon, G. Zampa, Beatrice Panico, Riccardo Munini, N. Zampa, Mirko Boezio, A. V. Karelin, R. Sparvoli, Marco Ricci, Per Carlson, Alfonso Monaco, F. Cafagna, A. N. Kvashnin, Yu. T. Yurkin, M. Merge, G. Osteria, Massimo Bongi, Sergey Koldobskiy, G. C. Barbarino, V. V. Malakhov, A. G. Mayorov, G. A. Bazilevskaya, V. Di Felice, S. Bottai, O. Adriani, E. Mocchiutti, W. Menn, A. A. Kvashnin, G. I. Vasilyev, S. Y. Krutkov, Matteo Martucci, M. F. Runtso, S. A. Voronov, P. Picozza, C. De Santis, Nicola Mori, P. Spillantini, D. Campana, Marco Casolino, Sergey Koldashov, L. Marcelli, A. Bruno, Alexey Leonov, Yuri Stozhkov, G. Castellini, E. A. Bogomolov, Koldobskiy, S. A., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Karelin, A. V., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldashov, S. V., Krutkov, S. Y., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Pearce, M., Ricci, M., Ricciarini, S. B., Runtso, M. F., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., and Yurkin, Y. T.
Subjects: Physics, COSMIC cancer database, PAMELA detector, 010308 nuclear & particles physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Settore FIS/04, General Physics and Astronomy, Cosmic ray, Cosmic ray measurement, Cosmic rays, Deuterium, Modulation, Solar energy Energy interval, Galactic cosmic rays, High precision detections, Measurements of, Solar activity, Solar modulation, Astrophysics, Solar energy, 01 natural sciences, Spectral line, law.invention, Physics and Astronomy (all), law, 0103 physical sciences, Physics::Space Physics, Coronal mass ejection, Satellite, Astrophysics::Earth and Planetary Astrophysics, business, Nucleon, 010303 astronomy & astrophysics
Abstract: The preliminary results from measurements of deuteron fluxes in galactic cosmic rays (GCR) in the vicinity of the Earth in 2006–2009 are presented. The results are obtained by analyzing data from the PAMELA experiment aboard the Resurs DK-1 satellite. High-precision detection instruments provided an opportunity to identify GCR deuterons and measure their spectrum in the energy interval of 90–650MeV/nucleon. Spectra averaged over six-month intervals from the summer of 2006 to the summer of 2009 (the solar activity minimum) are presented. The influence of solar modulation on the observed spectrum is clearly seen in the results.
Published: 2017

8. Modulation of electrons and positrons in 2006â2015 in the PAMELA experiment

Author: E. Mocchiutti, O. Adriani, W. Menn, A. G. Mayorov, A. N. Kvashnin, A. V. Karelin, R. Sparvoli, Mark Pearce, S. B. Ricciarini, Sergey Koldobskiy, P. Papini, G. Castellini, E. Vannuccini, Yu. T. Yurkin, G. C. Barbarino, V. V. Malakhov, Mirko Boezio, Marco Ricci, C. De Santis, N. Zampa, M. Bongi, Matteo Martucci, V. Di Felice, V. Bonvicini, S. Bottai, Roberto Bellotti, A. M. Galper, Andrea Vacchi, G. Zampa, Beatrice Panico, S. Y. Krutkov, A. A. Kvashnin, G. I. Vasilyev, Per Carlson, M. Simon, F. Cafagna, L. Marcelli, G. A. Bazilevskaya, G. Osteria, A. Bruno, Nicola Mori, P. Picozza, V. V. Mikhailov, Riccardo Munini, P. Spillantini, D. Campana, M. F. Runtso, S. A. Voronov, Marco Casolino, Sergey Koldashov, Alfonso Monaco, M. Merge, Yuri Stozhkov, Alexey Leonov, E. A. Bogomolov, Mikhailov, V. V., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Karelin, A. V., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Pearce, M., Ricci, M., Ricciarini, S. B., Runtso, M. F., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., and Yurkin, Y. T.
Subjects: Physics, Settore FIS/01, Antiparticle, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, Cosmic ray, Electron, Astrophysics, 01 natural sciences, law.invention, Physics and Astronomy (all), Positron, law, 0103 physical sciences, Physics::Space Physics, Coronal mass ejection, Interplanetary magnetic field, 010306 general physics, 010303 astronomy & astrophysics, Cosmic rays, Cosmology, Magnetic polarity, Orbits, Positrons, Solar energy Magnetic spectrometers, Solar activity, Solar magnetic fields, Temporal variation, Time interval, Wide energy range
Abstract: The PAMELA magnetic spectrometer was launched aboard the Resurs DK-1 satellite into a nearpolar circumterrestrial orbit with an altitude of 350–600 km to study fluxes of the particles and antiparticles of cosmic rays in the wide energy range of ~80 MeV to several hundred gigaelectronvolts. The results from observations of temporal variations in electron and positron fluxes in 2006–2015 are presented. The ratio of electron and positron fluxes measured in this time interval reveals a dependence on the rigidity of particles, the solar activity, and the polarity of the solar magnetic field.
Published: 2017

9. Cosmic ray oriented performance studies for the JEM-EUSO first level trigger

Author: H. Sato, T. Djemil, Alberto Cellino, Octavian Micu, Javier Licandro, M. D. Rodríguez Frías, Z. Plebaniak, N. Guardone, Katsuhiko Tsuno, A. Belov, L. R. Wiencke, N. Tone, G. Cordero, A. Anzalone, T. Napolitano, Michiyuki Chikawa, Katsuaki Asano, A. Ebersoldt, Daisuke Yonetoku, I. S. Zgura, Roberto Bellotti, M. Mahdi, T. Pierog, Yoshimasa Kurihara, H. Schieler, E. M. Popescu, Antonella Castellina, Mitsuteru Sato, T. Jammer, K. S. Caballero, Hiroyuki Sagawa, Christer Fuglesang, J. Watanabe, G. Roudil, K. Mase, Graciela B. Gelmini, G. Chiritoi, Y. Hachisu, F. Perfetto, Y. Yamamoto, B. Pastirčák, J. Geary, H. Khales, José Meseguer, Angel Sanz-Andrés, Osvaldo Catalano, Santiago Pindado, Junpei Fujimoto, B. A. Khrenov, S. Pliego, Thomas J. Weiler, Pierre Barrillon, Eduardo García-Ortega, Sergei A. Sharakin, Massimiliano Bonamente, James H. Adams, Y. Tsunesada, H. Lahmar, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, Satoshi Wada, T. Ogawa, M. Yu. Zotov, J. Genci, Piergiorgio Picozza, N. Mebarki, Mohammed Bakiri, C. Catalano, K. Benmessai, M. Suzuki, Valentina Scotti, Hitoshi Ohmori, G. Abdellaoui, Francesco Isgrò, Daisuke Ikeda, Belkacem Benadda, W. Painter, P. Gorodetzky, Yoshiya Kawasaki, E. Kuznetsov, Yoshihiko Mizumoto, R. Bechini, M. C. Talai, C. De La Taille, K. Shinozaki, A. Radu, F.J. Ronga, Alfonso Monaco, Shinsuke Abe, B. Nadji, E. Parizot, A. Guzmán, Toshitaka Kajino, K. Kawai, Ralph Engel, I. Kreykenbohm, Hajime Takami, Angela V. Olinto, Andrea Santangelo, D. Maravilla, S. Blin-Bondil, D. Allard, Vladimir Andreev, Masaki Fukushima, R. Nava, V. S. Morozenko, Akinori Saito, Maxim Gonchar, Hirohiko M. Shimizu, M. A. Mendoza, E. G. Judd, D. Kang, G. Castellini, Andreas A. Berlind, M. Rezazadeh, S. Selmane, Alexander Kusenko, K. Higashide, C. Moretto, P. Galeotti, Y. Martín, M. E. Bertaina, L. Villaseñor, C. De Santis, J. Yang, Rossella Caruso, J. Karczmarczyk, Shigeto Watanabe, Ken'ichi Nomoto, K. Słomińska, H. Attoui, C. Tenzer, F Dulucq, N. Inoue, S. Bacholle, John N. Matthews, Francesca Capel, J. F. Valdés-Galicia, L. G. Tkachev, H. Tahi, G. Vankova, Tokonatsu Yamamoto, Guillaume Prévôt, L. del Peral, A. Franceschi, Pavol Bobik, T. Sugiyama, Hajime Yano, Tadeusz Wibig, B. Mot, S. Dagoret-Campagne, S. Bartocci, E. Bozzo, M. Serra, Luis A. Anchordoqui, T. Shibata, M. Traïche, S. Mackovjak, J. Fernández-Soriano, D. Supanitsky, T. Batsch, Toshio Murakami, R. Young, M. Sakata, S. Biktemerova, Toshikazu Ebisuzaki, Yukihiro Takahashi, José Luis Sánchez, S. Ahmad, C. Lachaud, F. Cafagna, H. J. Crawford, O. Larsson, S. Messaoud, K. Kudela, G. Modestino, E. Joven, M. Rahmani, Giuseppe Giraudo, R. Weigand Muñoz, T. Shirahama, S. A. Djenas, S. Kalli, I. Kaneko, A. Haungs, S. Piraino, J. Watts, Hanna Rothkaehl, J. Mimouni, J. A. Morales de los Ríos, Toshiyuki Nonaka, Ovidiu Vaduvescu, M. Karus, L. Santiago Crúz, M. Bogomilov, Josef Jochum, F. Bisconti, M. Lacombe, Claudio Cassardo, Shoichi Ogio, M. Flamini, Silvia Ferrarese, C. Pennypacker, Marco Casolino, Claudio Fornaro, Susumu Inoue, Tomás Belenguer, J. Błȩcki, L. Mehrad, M. Vrabel, P. Prat, Piotr Orleanski, Ke Fang, Mikhail Panasyuk, F. Kajino, Andrés Merino, Y. Takizawa, M. Fouka, P. L. Biermann, Z. Sahnoune, D. Kolev, H. Lim, J. C. Sanchez, Maciej Rybczyński, G. Sáez Cano, D. Monnier-Ragaigne, A. Segreto, W. Aouimeur, A. Neronov, M. C. Maccarone, B. Harlov, I. Rusinov, P. Carlson, T. Mernik, A. Jung, H. W. Park, R. Boudaoud, M. Dupieux, I. V. Yashin, Carlo Vigorito, Domenico Finco, A. Kedadra, T. Paul, Valerie Connaughton, Marcos Reyes, R. Guehaz, N. Blanc, M. Ave Pernas, T. Nakamura, Yoshio Arai, L. Marcelli, I. Dutan, L. Placidi, A. Sobey, Francesco Fenu, Piero Vallania, S. E. Csorna, G. Masciantonio, G. Medina-Tanco, J. L. Marcos, M. D. Sabau, Johannes Eser, H. Prieto, R. Cremonini, H. Ikeda, Naoto Sakaki, G. Cotto, Markus Roth, C. De Donato, L. López Campano, Sergio Fernández-González, Takayuki Tomida, Nicusor Arsene, J. Bayer, A. Insolia, M. Kleifges, N. Tajima, M. Takeda, Soon-Wook Kim, J. Rabanal, J. Hernández Carretero, Fausto Guarino, P. von Ballmoos, M. Ricci, A. Bruno, M. Unger, Shigehiro Nagataki, K. Katahira, Isabel Pérez-Grande, F. Sarazin, Zbigniew Wlodarczyk, Marc Weber, R. Matev, Simona Toscano, Michael S. Briggs, M. Haiduc, Lech Wiktor Piotrowski, S. Yoshida, J. Szabelski, Estíbaliz Gascón, O. Martinez, T. Patzak, M. Nagata, Dmitry V. Naumov, J.N. Capdevielle, I. Stan, A. Caramete, K. Martens, Konstantin Belov, Joowon Lee, F. Tajima, A. Acheli, J. N. Albert, Thomas Schanz, M. Wille, Livio Conti, Y. Uchihori, A. Zuccaro Marchi, Jörn Wilms, O. A. Saprykin, Sug Whan Kim, F. Kanouni, Sebastián Franchini, Gali Garipov, R. Attallah, D. Campana, F. Lakhdari, Barbara Szabelska, Inkyu Park, M. Putis, Y. Miyazaki, A. Weindl, T. Peter, B. Vlcek, Mark Christl, Gustavo Alonso, O. Tibolla, Jeong Sook Kim, C. González Alvarado, P. Baragatti, H. Miyamoto, M. Manfrin, Yoshitaka Itow, L. Caramete, M. Sanz Palomino, Y. Karadzhov, Amine Ahriche, Humberto Ibarguen Salazar, G. Contino, H. Tokuno, W. Hidber, R. Tsenov, R. Forza, A. Pollini, Pavel Klimov, B. Panico, M. Mignone, M. Di Martino, A. Marini, G. Osteria, D.V. Semikoz, T. Tymieniecka, J. Sledd, M. Nagano, Abdellaoui, G., Abe, S., Acheli, A., Adams, J. H., Ahmad, S., Ahriche, A., Albert, J. N., Allard, D., Alonso, G., Anchordoqui, L., Andreev, V., Anzalone, A., Aouimeur, W., Arai, Y., Arsene, N., Asano, K., Attallah, R., Attoui, H., Ave pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, A., Belov, K., Benadda, B., Benmessai, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blanc, N., Błȩcki, J., Blin Bondil, S., Bobik, P., Bogomilov, M., Bonamente, M., Boudaoud, R., Bozzo, E., Briggs, M. S., Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J. N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Castellini, G., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Contino, G., Cordero, G., Cotto, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., De donato, C., De la taille, C., De santis, C., Del peral, L., Di martino, M., Djemil, T., Djenas, S. A., Dulucq, F., Dupieux, M., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fang, K., Fenu, F., Fernández González, S., Fernández Soriano, J., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Forza, R., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujimoto, J., Fukushima, M., Galeotti, P., García Ortega, E., Garipov, G., Gascón, E., Geary, J., Gelmini, G., Genci, J., Giraudo, G., Gonchar, M., González alvarado, C., Gorodetzky, P., Guardone, N., Guarino, Fausto, Guehaz, R., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández carretero, J., Hidber, W., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Jammer, T., Joven, E., Judd, E. G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Kang, D., Kanouni, F., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., 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., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., Lim, H., López campano, L., Maccarone, M. C., Mackovjak, S., Mahdi, M., Manfrin, M., Maravilla, D., Marcelli, L., Marcos, J. L., Marini, A., Martens, K., Martín, Y., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Matthews, J. N., Mebarki, N., Medina Tanco, G., Mehrad, L., Mendoza, M. A., Merino, A., Mernik, T., Meseguer, J., Messaoud, S., Micu, O., Mignone, M., Mimouni, J., 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., Nadji, B., 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., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Pérez Grande, I., Perfetto, Francesco, Peter, T., Picozza, P., Pierog, T., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Putis, M., Rabanal, J., Radu, A. A., Rahmani, M., Reardon, P., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sanchez, J. C., Sánchez, J. L., Santangelo, A., Santiago crúz, L., Sanz Andrés, A., Sanz palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, Valentina, Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Sledd, J., Słomińska, K., Sobey, A., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tahi, H., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., Von ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weigand muñoz, R., Weindl, A., 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, S., Young, R., Zgura, I. S., Zotov, M. Y. u., Zuccaro marchi, A., Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), 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), 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 de Paris (UP), 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), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-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), 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), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), 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), 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: Nuclear and High Energy Physics, data analysis method, Instrumentation, Astrophysics::High Energy Astrophysical Phenomena, Night sky, measurement methods, satellite, JEM-EUSO, FPGA, Nightglow background, Trigger system, Cosmic ray, 01 natural sciences, law.invention, Aeronáutica, Telescope, nightglow background, law, 0103 physical sciences, International Space Station, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, background: suppression, Remote sensing, Physics, detector: wide-angle, trigger system, laser: pulsed, showers: atmosphere, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, trigger, Astronomía, Satellite, background: fluctuation, FPGA, JEM-EUSO, Nightglow background, Trigger system, Nuclear and High Energy Physics, Instrumentation, Neutrino, Energy (signal processing), performance
Abstract: 著者人数: 368名 (JAXA職員: 池田, 博一 ; 鈴木, 睦 ; 矢野, 創), Accepted: 2017-05-29, 資料番号: SA1170117000
Published: 2017

10. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

Author: Alfonso Monaco, S. Bottai, A. G. Mayorov, P. Picozza, M. Merge, Maria Teresa Ricci, Sergey Koldobskiy, G. C. Barbarino, P. Yu. Naumov, A. V. Karelin, P. Spillantini, Alexey Leonov, R. Sparvoli, Mark Pearce, S. B. Ricciarini, Nicola Mori, S. A. Voronov, M. Simon, P. Papini, E. Vannuccini, N. Zampa, G. A. Bazilevskaya, L. Marcelli, E. A. Bogomolov, G. Osteria, D. Campana, A. Vacchi, Laura Rossetto, V. V. Malakhov, Yu. T. Yurkin, A. Bruno, V. V. Mikhailov, O. Adriani, M. A. Mayorova, Marco Casolino, Roberto Bellotti, A. M. Galper, Matteo Martucci, W. Menn, G. I. Vasilyev, V. Di Felice, A. A. Kvashnin, Mirko Boezio, G. Castellini, G. Zampa, Beatrice Panico, Riccardo Munini, C. De Santis, S. A. Rodenko, F. Cafagna, M. Bongi, Per Carlson, V. Bonvicini, Y. Stozhkov, Sergey Aleksandrin, E. Mocchiutti, and S. V. Koldashov
Subjects: Settore FIS/01, Physics, History, Scintillation, PAMELA detector, Spectrometer, Cosmic rays, Cosmology, Magnetic polarity, Modulation, Solar energy, Spectrometers Galactic cosmic rays, Magnetic spectrometers, Solar activity, Solar magnetic fields, Solar modulation, Transient periods, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Computer Science Applications, Education, Magnetic field, law.invention, Physics and Astronomy (all), law, Physics::Space Physics, Nuclear Experiment
Abstract: Solar modulation of galactic protons with energies from 50 MeV up to dozens of GeV during July '06 - January '16 studied based on a data of the magnetic spectrometer PAMELA and scintillation spectrometer ARINA. This period is interesting because it covers the end of 23rd and current 24th cycles of solar activity, including the abnormally long transient period and change of the polarity of solar magnetic field. © Published under licence by IOP Publishing Ltd.
Published: 2017

11. Geomagnetically trapped, albedo and solar energetic particles: Trajectory analysis and flux reconstruction with PAMELA

Author: G. Zampa, Beatrice Panico, Roberto Bellotti, A. M. Galper, Matteo Martucci, G. A. de Nolfo, Alfonso Monaco, A. G. Mayorov, Alexey Leonov, M. Merge, Valentina Scotti, N. Zampa, G. A. Bazilevskaya, V. Bonvicini, Y. I. Stozhkov, E. Mocchiutti, Ritabrata Sarkar, S. Bottai, Sergey Koldashov, R. Sparvoli, Sergey Koldobskiy, A. V. Karelin, Marco Ricci, V. V. Malakhov, G. C. Barbarino, G. Osteria, G. I. Vasilyev, G. Castellini, S. Y. Krutkov, James M. Ryan, V. Di Felice, C. De Santis, C. De Donato, Mirko Boezio, P. Picozza, Nicola Mori, F. Palma, M. Simon, V. V. Mikhailov, Riccardo Munini, F. Cafagna, E. C. Christian, O. Adriani, A. N. Kvashnin, W. Menn, Yu. T. Yurkin, L. Marcelli, M. Bongi, A. Vacchi, A. Bruno, Mark Pearce, S. B. Ricciarini, Steven Stochaj, P. Papini, E. Vannuccini, S. A. Voronov, E. A. Bogomolov, Per Carlson, N. De Simone, P. Spillantini, D. Campana, Marco Casolino, Bruno, A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., Christian, E. C., De Donato, C., de Nolfo, G. A., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Ryan, J. M., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stochaj, S., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Atmospheric Science, Solar energetic particles, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Aerospace Engineering, FOS: Physical sciences, Space weather, 01 natural sciences, law.invention, Physics::Geophysics, symbols.namesake, Physics - Space Physics, law, 0103 physical sciences, Albedo particles, Cosmic-rays, 010303 astronomy & astrophysics, Ring current, 0105 earth and related environmental sciences, Physics, Geomagnetic storm, Settore FIS/01, PAMELA detector, Astronomy, Geomagnetic cutoff, Radiation belts, Space and Planetary Science, Astronomy and Astrophysics, Space Physics (physics.space-ph), Geophysics, Earth's magnetic field, Van Allen radiation belt, Health threat from cosmic rays, Physics::Space Physics, symbols, General Earth and Planetary Sciences, Astrophysics::Earth and Planetary Astrophysics
Abstract: The PAMELA satellite experiment is providing comprehensive observations of the interplanetary and magnetospheric radiation in the near-Earth environment. Thanks to its identification capabilities and the semi-polar orbit, PAMELA is able to precisely measure the energetic spectra and the angular distributions of the different cosmic-ray populations over a wide latitude region, including geomagnetically trapped and albedo particles. Its observations comprise the solar energetic particle events between solar cycles 23 and 24, and the geomagnetic cutoff variations during magnetospheric storms. PAMELA's measurements are supported by an accurate analysis of particle trajectories in the Earth's magnetosphere based on a realistic geomagnetic field modeling, which allows the classification of particle populations of different origin and the investigation of the asymptotic directions of arrival., Comment: Accepted for publication in Advances in Space Research, 2016. 21 pages, 7 figures
Published: 2017

12. Searching for cosmic ray anisotropy using the calorimeter in the PAMELA experiment

Author: A. V. Karelin, Nicola Mori, W. Menn, Y. Wu, Andrea Vacchi, S. V. Borisov, G. A. Bazilevskaya, Giovanna Jerse, M. F. Runtso, A. M. Galper, R. Belotti, S. A. Voronov, A. N. Kvashnin, A. G. Mayorov, P. Picozza, C. Pizzolotto, Mirko Boezio, G. I. Vasilyev, R. Carbone, P. Spillantini, A. Bruno, L. Consiglio, Sergey Koldobskiy, G. C. Barbarino, C. De Santis, Mark Pearce, S. B. Ricciarini, Alfonso Monaco, N. De Simone, Laura Rossetto, Yu. T. Yurkin, P. Papini, E. Vannuccini, G. Castellini, Yu. I. Stozhkov, Giuseppe Osteria, Gianluigi Zampa, S. Bottai, V. V. Malakhov, V. G. Zverev, M. P. De Pascale, S. Yu. Krutkov, M. Bongi, E. A. Bogomolov, N. Zampa, Roberta Sparvoli, A. A. Leonov, Lorenzo Bonechi, D. Campana, Marco Casolino, L. Marcelli, O. Adriani, V. V. Mikhailov, P. Carlson, F. Cafagna, I. A. Danilchenko, S. V. Koldashov, Marco Ricci, E. Mocchiutti, M. Simon, V. Di Felice, V. Malvezzi, V. Bonvicini, A., Karelin, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Belotti, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S. h., Borisov, S., Bottai, A., Bruno, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Wu, A., Galper, I., Danilchenko, M. D., Pascale, C. D., Santi, N. D., Simone, V. D., Felice, G., Jerse, V., Zverev, G., Zampa, N., Zampa, F., Cafagna, D., Campana, R. h., Carbone, P., Carlson, M., Casolino, G., Castellini, A., Kvashnin, S., Koldashov, S., Koldobskiy, Consiglio, Lucia, S., Krutkov, A., Leonov, V., Malvezzi, L., Marcelli, A., Mayorov, V., Malakhov, W., Menn, V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, M., Runtso, M., Simon, R., Sparvoli, P., Spillantini, Y., Stozhkov, and Y., Yurkin
Subjects: Physics, Range (particle radiation), Scintillation, genetic structures, Calorimeter (particle physics), PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, Cosmic ray, Electron, Radiation, law.invention, Nuclear physics, Physics and Astronomy (all), Calorimeters, law, A-particles, Cosmic ray anisotropy, Cosmic ray spectra, Electron component, Experiment study, Nuclear components, Position sensitive, Secondary particle, High Energy Physics::Experiment, Anisotropy, Cosmic rays, Experiment, Anisotropy
Abstract: The satellite-borne PAMELA experiment studies cosmic ray spectra over a wide range of energies. The instrument was placed in orbit in June 2006 and remains there to the present day. A position-sensitive calorimeter is one of the main parts of the PAMELA instrument. The calorimeter data are used to determine the energy of particles that interact within it, separate the electron component of the detected radiation from the nuclear component, and reconstruct the tracks of particles passing through the instrument. The special calorimeter and S4 scintillation shower detector triggers enables us to expand our statistics considerably. Using the calorimeter data in generating these triggers means we can study the anisotropy of cosmic rays with energies in excess of tens of GeV. This method of anisotropy detection is based on reconstructing the direction of a particle's arrival from the axis of the secondary particle cascade in the calorimeter. ?????? 2013 Allerton Press, Inc.
Published: 2013

13. The high energy cosmic ray particle spectra measurements with the PAMELA calorimeter

Author: A. G. Mayorov, C. De Santis, Alfonso Monaco, Yu. T. Yurkin, Valerio Formato, M. Merge, Sergey Koldashov, R. Carbone, Sergey Koldobskiy, G. C. Barbarino, Alexey Leonov, Roberto Bellotti, F. Cafagna, P. Picozza, Ritabrata Sarkar, A. M. Galper, Matteo Martucci, M. Simon, G. Osteria, A. N. Kvashnin, O. Adriani, W. Menn, V. V. Malakhov, L. Marcelli, Mark Pearce, S. B. Ricciarini, V. G. Zverev, A. Vacchi, Nicola Mori, S. A. Voronov, G. Castellini, E. Mocchiutti, A. Bruno, E. A. Bogomolov, P. Papini, E. Vannuccini, Laura Rossetto, M. P. De Pascale, Marco Ricci, Riccardo Munini, M. Bongi, S. Yu. Krutkov, S. Bottai, N. De Simone, A. V. Karelin, G. I. Vasilyev, Mirko Boezio, V. V. Mikhailov, Ugo Giaccari, P. Carlson, M. D. Kheymits, G. Zampa, N. Zampa, G. A. Bazilevskaya, R. Sparvoli, V. Di Felice, V. Bonvicini, P. Spillantini, and Marco Casolino
Subjects: Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, helium, Scintillator, 01 natural sciences, law.invention, Nuclear physics, law, 0103 physical sciences, calorimeter, Calorimeter, Electrons and positrons, Helium, Protons, Neutron detection, Ultra-high-energy cosmic ray, electrons and positrons, 010306 general physics, 010303 astronomy & astrophysics, Physics, Range (particle radiation), protons, Spectrometer, PAMELA detector, Calorimeter (particle physics), Settore FIS/04
Abstract: Up until now there has been limited, contradictive data on the high energy range of the cosmic ray electron-positron, proton and helium spectra. Due to the limitations of the use of a magnetic spectrometer, over 8 years experimental data was processed using information from a sampling electro-magnetic calorimeter, a neutron detector and scintillator detectors. The use of these devices allowed us to successfully obtain the high energy cosmic ray particle spectra measurements. The results of this study clarify previous findings and greaten our understanding of the origin of cosmic rays.
Published: 2016

14. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment

Author: A. V. Karelin, V. Formato, S. A. Voronov, Yu. T. Yurkin, M. Merge, S. Y. Krutkov, P. Picozza, Sergey Koldashov, G. Osteria, R. Sparvoli, E. A. Bogomolov, V. V. Mikhailov, Per Carlson, Andrea Vacchi, O. Adriani, Mirko Boezio, Massimo Bongi, W. Menn, V. Di Felice, L. Marcelli, Roberto Bellotti, A. M. Galper, G. Zampa, Beatrice Panico, A. Bruno, V. V. Malakhov, Matteo Martucci, A. N. Kvashnin, D. Campana, Sergey Koldobskiy, G. C. Barbarino, N. Zampa, V. Bonvicini, Valentina Scotti, G. A. Bazilevskaya, Riccardo Munini, Y. I. Stozhkov, N. De Simone, Piero Spillantini, Marco Casolino, F. Cafagna, A. G. Mayorov, G. Castellini, F. Palma, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, Maria Teresa Ricci, C. De Donato, Ritabrata Sarkar, E. Mocchiutti, M. Simon, A. A. Leonov, S. Bottai, G. I. Vasilyev, Nicola Mori, C. De Santis, Alfonso Monaco, Koldobskiy, S. A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Felice, V. D., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Physics, History, Earth's orbit, PAMELA detector, Settore FIS/04, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Astrophysics, Cosmic ray measurement, Cosmology, Deuterium, Orbits, Solar radiation Cosmic-ray particles, Albedo, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), law, Re entrant, Nuclear Experiment, Trajectory (fluid mechanics)
Abstract: The results of trajectory reconstruction for re-entrant albedo deuteron fluxes obtained in the PAMELA experiment are presented in this work. PAMELA is an international experiment aimed on measurements of cosmic ray particle fluxes in wide energy range. In particular, analysis of PAMELA data gives possibility to identify deuterons. Classification of re-entrant albedo deuterons with energies from 70 to 400 MeV/nucleon depending on theirs reconstructed lifetimes and generation zones is presented here at first time.
Published: 2016

15. Measurement of the high-energy electron and positron spectrum in the PAMELA experiment

Author: S. A. Voronov, Roberto Bellotti, G. I. Vasil’ev, Alfonso Monaco, A. N. Kvashnin, S. Bottai, P. Spillantini, C. De Santis, Laura Rossetto, G. Zampa, Mark Pearce, S. B. Ricciarini, G. Osteria, V. V. Mikhailov, P. Carlson, Petter Hofverberg, N. N. Nikonov, Nicola Mori, P. Papini, S. V. Borisov, G. A. Bazilevskaya, V. Di Felice, P. Picozza, E. Vannuccini, R. Carbone, Juan Wu, N. De Simone, V. Malvezzi, Yu. T. Yurkin, L. Consiglio, Mirko Boezio, F. Cafagna, William Gillard, O. Adriani, W. Menn, M. Simon, L. Marcelli, A. Vacchi, A. A. Leonov, V. Bonvicini, A. Bruno, M. P. De Pascale, S. Yu. Krutkov, D. Campana, Marco Casolino, N. Zampa, Lorenzo Bonechi, G. Castellini, Roberta Sparvoli, E. Mocchiutti, S. V. Koldashov, Marco Ricci, L. A. Grishantseva, A. M. Galper, Giovanna Jerse, V. G. Zverev, Yu. I. Stozhkov, and A. V. Karelin
Subjects: Physics, Range (particle radiation), Proton, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Electron, Settore FIS/04 - Fisica Nucleare e Subnucleare, Electronic, Optical and Magnetic Materials, law.invention, Nuclear physics, Positron, law, Antiproton, Physics::Space Physics, Physics::Accelerator Physics, High Energy Physics::Experiment, Nuclear Experiment
Abstract: The PAMELA magnetic spectrometer onboard the Resurs DK1 satellite no. 1 was put into (Earth) orbit on June 15, 2006; measurements continue at the present time. The scientific objective of the spectrometer is the study of antiproton, proton, positron, electron and light nucleus fluxes in cosmic rays. In this paper, we present the technique for measuring electron and positron spectra in the energy range from 20 to 800 GeV.
Published: 2010

16. The EUSO-Balloon pathfinder

Author: N. Tone, Daisuke Yonetoku, H. Ikeda, K. Mase, Francesco Isgrò, B. Keilhauer, Francesco Fenu, I. V. Yashin, Frederic Jean Ronga, L. Santiago Crúz, M. Yu. Zotov, Silvia Ferrarese, L. Marcelli, Susana Briz, I. Kreykenbohm, Vladimir Andreev, F. Dulucq, D. Ikeda, F. Sarazin, Andreas A. Berlind, A. Bruno, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, D. Kolev, Karl Mannheim, Valerie Connaughton, H. H. Silva Lopez, Marc Weber, K. Shinozaki, G. Masciantonio, Hitoshi Ohmori, Tomás Belenguer, G. Castellinic, H. Prieto, R. Cremonini, P. L. Biermann, Yoshiya Kawasaki, R. Nava, Michael S. Briggs, A. J. de Castro, N. Sakaki, I. Rusinov, S. Ahmad, Markus Roth, M. D. Rodríguez Frías, Alberto Cellino, Fausto Guarino, P. von Ballmoos, M. Ricci, L. Valore, I. Rodríguez, D. Allard, Rossella Caruso, T. Patzak, Toshiyuki Nonaka, Alfonso Monaco, M. E. Bertaina, Thomas J. Weiler, Yoshihiko Mizumoto, Taka Tomida, Z. Plebaniak, J. Blümer, Marcos Reyes, Tokonatsu Yamamoto, G. Roudil, M. Putis, A. Sobey, T. Murakami, O. Martinez, T. Shirahama, S. Sánchez, G. Catalano, Ken'ichi Nomoto, J. Karczmarczyk, J. N. Albert, Thomas Schanz, B. A. Khrenov, H. Miyamoto, S. Perez Cano, H. J. Crawford, L. R. Wiencke, G. Giraudo, A. Insolia, M. Kleifges, Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, M. Flamini, Hanna Rothkaehl, Michiyuki Chikawa, Y. Takizawa, Livio Conti, M. Serra, A. Haungs, C. De Donato, Soon-Wook Kim, B. Harlov, Luis A. Anchordoqui, S. Piraino, Carlo Vigorito, T. Batsch, Hajime Yano, S. Falk, K. Kudela, Yoshimasa Kurihara, H. Schieler, M. Nagata, Piotr Orleanski, J. Geary, J. S. Kim, T. Shibata, I. Kaneko, K. Kawai, Akinori Saito, A. Zuccaro Marchi, V. S. Morozenko, Jörn Wilms, Roberto Bellotti, Dmitry V. Naumov, Y. Karadzhov, Mitsuteru Sato, N. De Simone, R. Young, O. A. Saprykin, M. Sakata, B. Mot, Javier Licandro, J.N. Capdevielle, Z. Włodarczyk, P. Picozza, Andrii Neronov, J. Lee, James H. Adams, J. Błȩcki, G. Distratis, A. Ebersoldt, J. F. Valdés-Galicia, L. Villaseñor, Yukihiro Takahashi, R. Bechini, Piero Vallania, R. Tsenov, H. Lim, N. Tajima, M. C. Maccarone, M. D. Sabau, Toshikazu Ebisuzaki, M. Suzuki, L. G. Tkachev, G. Sáez-Cano, A. Jung, S. Csorna, T. Pierog, J. Watanabe, Gali Garipov, Shigehiro Nagataki, Yoshiki Tsunesada, Simona Toscano, A. Pollini, Pavel Klimov, D. Supanitsky, M. Takeda, F. Cafagna, T. Paul, K. Yoshida, Marco Casolino, Claudio Fornaro, J. Bayer, G. Modestino, E. Joven, K. Higashide, Lech Wiktor Piotrowski, G. Vankova, Shigeto Watanabe, C. de la Taille, Ovidiu Vaduvescu, M. Lacombe, K. Katahira, Claudio Cassardo, Massimiliano Bonamente, M. Rybczyński, Valentina Scotti, H. Sato, Shoichi Ogio, Dmitri Semikoz, Yoshitaka Itow, Graciela B. Gelmini, Hajime Takami, A. Guzman, Jianyi Yang, Masaki Fukushima, C. Lachaud, E. Kuznetsov, G. Medina-Tanco, S. Biktemerova, T. Mernik, Y. Hachisu, Y. Arai, S. Dagoret-Campagne, D. Maravilla, G. Cordero, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, David B. Cline, T. Nakamura, Y. Yamamoto, Katsuaki Asano, Alexander Kusenko, C. González Alvarado, J. A. Morales de los Ríos, Pierre Barrillon, S. Yoshida, J. Szabelski, K. Słomińska, E. G. Judd, Sergei A. Sharakin, Katsuhiko Tsuno, Susumu Inoue, Guillaume Prévôt, Satoshi Wada, M. Di Martino, A. Marini, A. Dell’Oro, Toshitaka Kajino, T. Ogawa, G. Osteria, C. Blaksley, T. Tymieniecka, J. Sledd, M. Sanz Palomino, Angela V. Olinto, Fernando López, Andrea Santangelo, R. Matev, M. Bogomilov, F. Tajima, F. Kajino, Ralph Engel, C. Moretto, P. Galeotti, M. Ave Pernas, H. W. Park, P. Gorodetzky, C. Tenzer, T. Sugiyama, Tadeusz Wibig, Ke Fang, Frederic Trillaud, M. Wille, M. Nagano Murakami, Y. Uchihori, J. Hernández Carretero, M. Unger, M. Dupieux, Barbara Szabelska, T. Peter, M. I. Panasyuk, S. Selmane, A. Anzalone, T. Napolitano, K. Belov, C. Catalano, D. Monnier-Ragaigne, A. Segreto, N. Blanc, S. Blin-Bondil, J. Fujimoto, P. Bobik, Hiroyuki Sagawa, Maxim Gonchar, Hirohiko M. Shimizu, P. Baragatti, J. Watts, C. Pennypacker, B. Pastircak, P. Prat, I. Fernández-Gómez, M. Karus, Domenico Finco, D. Campana, Inkyu Park, Y. Miyazaki, Mark Christl, O. Tibolla, APC - Astrophysique des Hautes Energies (APC - AHE), 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)-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), 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), 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., FernÃ¡ndez GÃ³mez, 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., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez 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 RÃos, 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., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, 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 LÃ³pez, 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., ValdÃ©s 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., 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, and 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)
Subjects: Ciencias Físicas, JEM-EUSO, cosmic-rays, Cosmic ray, 01 natural sciences, law.invention, Telescope, Observatory, law, 0103 physical sciences, International Space Station, Ultraviolet light, Air-fluorescence, Balloon experiment, UHECR, Astronomy and Astrophysics, Space and Planetary Science, 010303 astronomy & astrophysics, Remote sensing, Physics, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astronomy and Astrophysic, Near space, Astronomía, Pathfinder, [SDU]Sciences of the Universe [physics], Temporal resolution, UHECR, Air-fluorescence, JEM-EUSO, Balloon experiment, EUSO-Balloon, 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: 2015-06-11, 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: SA1150237000
Published: 2015

17. Measuring the spectra of high-energy cosmic-ray particles in the PAMELA experiment

Author: L. Marcelli, A. Bruno, M. Simon, M. Bongi, V. Di Felice, A. G. Mayorov, V. Bonvicini, P. Spillantini, Marco Ricci, Roberta Sparvoli, O. Adriani, W. Menn, Mark Pearce, S. B. Ricciarini, S. Bottai, V. Malvezzi, P. Papini, E. Vannuccini, E. Mocchiutti, V. V. Mikhailov, P. Carlson, S. A. Voronov, D. Campana, V. V. Malakhov, Matteo Martucci, V. G. Zverev, P. Picozza, F. Cafagna, G. Castellini, Marco Casolino, Alexey Leonov, E. A. Bogomolov, Sergey Koldashov, Lorenzo Bonechi, Giuseppe Osteria, G. A. Bazilevskaya, N. Zampa, R. Sarkar, Andrea Vacchi, R. Carbone, Sergey Koldobskiy, G. C. Barbarino, Alfonso Monaco, F. Palma, M. Merge, Mirko Boezio, Roberto Bellotti, Yu. T. Yurkin, A. M. Galper, N. De Simone, A. N. Kvashnin, A. V. Karelin, S. Yu. Krutkov, Nicola Mori, G. I. Vasilyev, C. De Santis, C. De Donato, Gianluigi Zampa, Karelin, A. V., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Zverev, V. G., Zampa, G., Zampa, N., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y. u., Leonov, A. A., Malvezzi, V., Marcelli, L., Martucci, M., Mayorov, A. G., Malakhov, V. V., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sarkar, R., Sparvoli, R., Spillantini, P., and Yurkin, Y. u. T.
Subjects: Physics, PAMELA detector, Spectrometer, Calorimeter (particle physics), Physics::Instrumentation and Detectors, Settore FIS/04, General Physics and Astronomy, chemistry.chemical_element, Cosmic ray, Electron, law.invention, Nuclear physics, Physics and Astronomy (all), chemistry, law, Scintillation counter, Calorimeters, Cosmic ray measurement, Energy spectra, Helium nuclei, Neutron detection, Helium
Abstract: The available data on the energy spectra of electrons, protons, and helium nuclei in the high-energy region are fragmentary, a situation made worse by their scarcity. Due to limitations imposed on the use of the magnetic spectrometer in the PAMELA satellite experiment, the calorimeter must be used for measurements performed in the high-energy region. The processing of experimental data accumulated in more than eight years of measurements with the calorimeter, neutron detector, and scintillation counters allows the spectra of high-energy particles to be obtained, greatly expanding our understanding of the nature of primary cosmic rays.
Published: 2015

18. 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., FernÃ¡ndez GÃ³mez, 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., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez 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 RÃos, 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. RodrÃguez, Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A, Santiago CrÃºz, 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 LÃ³pez, 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., ValdÃ©s 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)
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
Published: 2015

19. The PAMELA experiment and cosmic ray observations

Author: G. Castellini, P. Spillantini, Mirko Boezio, Alexey Leonov, Roberto Bellotti, A. M. Galper, Ritabrata Sarkar, N. Zampa, G. A. Bazilevskaya, G. Zampa, Beatrice Panico, A. N. Kvashnin, Matteo Martucci, S. Y. Krutkov, S. Bottai, F. Palma, Yu. T. Yurkin, M. Simon, Valerio Formato, M. Bongi, V. Di Felice, A. G. Mayorov, Roberta Sparvoli, P. Picozza, V. V. Malakhov, Valentina Scotti, A. V. Karelin, R. Carbone, Sergey Koldobskiy, Alfonso Monaco, G. C. Barbarino, I. A. Danilchenko, Marco Ricci, V. G. Zverev, M. Merge, O. Adriani, G. I. Vasilyev, W. Menn, E. Mocchiutti, V. V. Mikhailov, V. Bonvicini, Y. I. Stozhkov, F. Cafagna, G. Osteria, Mark Pearce, S. B. Ricciarini, Nicola Mori, C. De Santis, P. Papini, E. Vannuccini, C. De Donato, Riccardo Munini, L. Marcelli, A. Vacchi, A. Bruno, D. Campana, Marco Casolino, Sergey Koldashov, Per Carlson, N. De Simone, S. A. Voronov, E. A. Bogomolov, N., Mori, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, I. A., Danilchenko, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S. A., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A. A., Leonov, V. V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergè, V. V., Mikhailov, E., Mocchiutti, A., Monaco, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, M. L., Rosetto, R., Sarkar, V. M., Simon, Sparvoli, Y. I., Stozhkov, P., Vacchi, E., Vannuccini, G. I., Vasil’Ev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, V. G., Zverev, Mori, N., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Danilchenko, I. A., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergé, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., and Zverev, V. G.
Subjects: Physics, Space experiments, Range (particle radiation), Nuclear and High Energy Physics, PAMELA detector, Physics::Instrumentation and Detectors, Cosmic rays, Settore FIS/04, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, law.invention, Space experiment, law, Physics::Space Physics, High Energy Physics::Experiment, Ultra-high-energy cosmic ray, space experiments
Abstract: The \PAMELA\ space experiment is aimed at precise measurements of the charged light component of the cosmic ray spectrum in the energy range spanning from the sub-GeV region to the TeV region, with a particular focus on antimatter. The instrument consists of a magnetic spectrometer, an electromagnetic sampling calorimeter,a time-of-flight system, an anticoincidence shield, a tail-catcher scintillator and a neutron detector. Launched in June 2006 and hosted on the Resurs-DK1 satellite, \PAMELA\ has been taking data for more than eight years, providing scientific results with unprecedented statistics and a continuous monitoring of the sun activity and the heliosphere.
Published: 2015

20. Calibration aspects of the JEM-EUSO mission

Author: Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, Katsuaki Asano, Alfonso Monaco, M. Rybczyński, Alberto Cellino, R. Tsenov, Taka Tomida, H. Sato, P. Baragatti, Gali Garipov, A. Pollini, Pavel Klimov, G. Cordero, L. R. Wiencke, Tokonatsu Yamamoto, Barbara Szabelska, David B. Cline, Yoshimasa Kurihara, H. Schieler, Mitsuteru Sato, Silvia Ferrarese, M. Di Martino, G. Giraudo, A. Marini, T. Peter, Satoshi Wada, R. Matev, T. Ogawa, E. G. Judd, G. Catalano, Katsuhiko Tsuno, G. Osteria, T. Tymieniecka, J. Sledd, C. Lachaud, M. I. Panasyuk, B. A. Khrenov, H. Miyamoto, M. Suzuki, S. Dagoret-Campagne, D. Campana, Valentina Scotti, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, M. Ave Pernas, S. Falk, Graciela B. Gelmini, Y. Hachisu, Inkyu Park, F. Dulucq, Angela V. Olinto, Y. Arai, Fernando López, Andrea Santangelo, Massimiliano Bonamente, Y. Yamamoto, Francesco Isgrò, A. Guzmán, B. Keilhauer, J. N. Albert, Dmitri Semikoz, Pierre Barrillon, Sergei A. Sharakin, Y. Miyazaki, Thomas Schanz, J. Geary, Y. Karadzhov, Roberto Bellotti, R. Young, J. Watts, M. Sakata, Yoshitaka Itow, Andreas A. Berlind, M. D. Rodríguez Frías, E. Kuznetsov, Toshikazu Ebisuzaki, C. Pennypacker, Frederic Jean Ronga, Toshiyuki Nonaka, Z. Plebaniak, James H. Adams, B. Pastircak, N. De Simone, J. Blümer, M. Putis, Mark Christl, O. Tibolla, Livio Conti, P. Prat, L. Villaseñor, A. Zuccaro Marchi, P. L. Biermann, T. Mernik, I. Kreykenbohm, H. Ikeda, M. Flamini, Vladimir Andreev, F. Tajima, Michiyuki Chikawa, J. Hernández Carretero, P. Gorodetzky, I. Rusinov, I. Fernández-Gómez, A. Sobey, Ralph Engel, Yoshihiko Mizumoto, M. Unger, A. Insolia, M. Kleifges, Alexander Kusenko, Thomas J. Weiler, C. Blaksley, G. Sáez-Cano, Y. Takizawa, M. Wille, Jörn Wilms, D. Kolev, I. V. Yashin, S. Perez Cano, M. Nagano Murakami, Y. Uchihori, M. Karus, O. A. Saprykin, S. Ahmad, T. Shibata, L. Marcelli, K. Słomińska, Marcos Reyes, J. F. Valdés-Galicia, L. G. Tkachev, Domenico Finco, T. Murakami, Kenji Shinozaki, J. Karczmarczyk, R. Bechini, M. Serra, N. Inoue, Luis A. Anchordoqui, Ke Fang, J. Błȩcki, L. del Peral, A. Franceschi, E. Parizot, S. Sánchez, Pavol Bobik, Valerie Connaughton, H. H. Silva Lopez, S. Csorna, T. Batsch, A. Bruno, G. Vankova, Frederic Trillaud, Hiroyuki Sagawa, K. Mase, Karl Mannheim, Michael S. Briggs, A. J. de Castro, D. Maravilla, H. Lim, K. Kawai, Akinori Saito, S. Biktemerova, Francesco Fenu, M. C. Maccarone, Shigeto Watanabe, T. Patzak, I. Kaneko, Hajime Yano, Z. Włodarczyk, Piero Vallania, J. A. Morales de los Ríos, M. D. Sabau, M. Dupieux, Tomás Belenguer, Hanna Rothkaehl, Maxim Gonchar, Hirohiko M. Shimizu, G. Distratis, D. Supanitsky, Susumu Inoue, D. Ikeda, Lech Wiktor Piotrowski, D. Monnier-Ragaigne, A. Segreto, C. González Alvarado, N. Tone, F. Sarazin, Simona Toscano, J. Bayer, A. Ebersoldt, S. Selmane, Marc Weber, Daisuke Yonetoku, F. Cafagna, G. Modestino, E. Joven, Shoichi Ogio, P. Picozza, J. Lee, Guillaume Prévôt, S. Yoshida, J. Szabelski, C. de la Taille, M. Yu. Zotov, A. Jung, Javier Licandro, Susana Briz, A. Anzalone, T. Napolitano, H. J. Crawford, Yoshiki Tsunesada, T. Paul, K. Katahira, K. Yoshida, O. Martinez, B. Mot, Yukihiro Takahashi, N. Blanc, G. Castellinic, Markus Roth, R. Nava, Hajime Takami, M. Bogomilov, N. Sakaki, Patrick J. Reardon, T. Pierog, J. Watanabe, Toshiki Tajima, G. Siemieniec-Oziȩbło, Fausto Guarino, P. von Ballmoos, M. Ricci, L. Valore, Masaki Fukushima, M. Sanz Palomino, T. Nakamura, G. Medina-Tanco, M. Takeda, K. Belov, Marco Casolino, Claudio Fornaro, C. Catalano, Rossella Caruso, F. Kajino, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, I. Rodríguez, H. W. Park, T. Shirahama, D. Allard, M. E. Bertaina, Piotr Orleanski, C. De Donato, Soon-Wook Kim, Ken'ichi Nomoto, J. S. Kim, V. S. Morozenko, A. Haungs, S. Piraino, J. Fujimoto, S. Blin-Bondil, L. Santiago Crúz, H. Prieto, R. Cremonini, Jianyi Yang, M. Nagata, Dmitry V. Naumov, J.N. Capdevielle, Andrii Neronov, G. Roudil, B. Harlov, Carlo Vigorito, K. Kudela, N. Tajima, Shigehiro Nagataki, A. Dell’Oro, Toshitaka Kajino, K. Higashide, C. Moretto, P. Galeotti, C. Tenzer, T. Sugiyama, Tadeusz Wibig, 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., FernÃ¡ndez GÃ³mez, 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., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez 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 RÃos, 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., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, 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 LÃ³pez, 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., ValdÃ©s 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., and Zuccaro Marchi, A.
Subjects: Photon, Ciencias Físicas, JEM-EUSO, Phase (waves), Air-Shower fluorescence telescope, Calibration, Space-Based experiment, Astronomy and Astrophysics, Space and Planetary Science, computer science, law.invention, Telescope, Optics, law, Transmittance, observations and techniques, space-based experiment, Remote sensing, Physics, business.industry, Detector, air-shower fluorescence telescope, Albedo, Astronomy and Astrophysic, calibration, chemistry and earth sciences, Air-Shower fluorescence telescope, JEM-EUSO, Calibration, Space-Based experiment, Astronomía, astronomy, statistics for engineering, Focal surface, business, physics, CIENCIAS NATURALES Y EXACTAS
Abstract: he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper. 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.. INAF - 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 (UAH); España 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.. Universita’ di Torino; 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: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos 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.
Published: 2015

21. New Upper Limit on Strange Quark Matter Abundance in Cosmic Rays with the PAMELA Space Experiment

Author: S. Y. Krutkov, Yu. T. Yurkin, V. V. Malakhov, Alexey Leonov, S. Bottai, A. G. Mayorov, V. Formato, Ritabrata Sarkar, Mark Pearce, S. B. Ricciarini, S. A. Voronov, P. Picozza, P. Papini, Valentina Scotti, E. Vannuccini, Matteo Martucci, Roberto Bellotti, G. I. Vasilyev, A. M. Galper, E. A. Bogomolov, P. Spillantini, L. Marcelli, A. Vacchi, Per Carlson, A. N. Kvashnin, C. De Donato, Mirko Boezio, M. Simon, O. Adriani, C. De Santis, A. Bruno, Sergey Koldobskiy, G. C. Barbarino, G. Castellini, Roberta Sparvoli, W. Menn, N. De Simone, Riccardo Munini, A. V. Karelin, M. Bongi, E. Mocchiutti, V. V. Mikhailov, F. Palma, G. Osteria, V. Bonvicini, Nicola Mori, Marco Ricci, Y. I. Stozhkov, N. Zampa, G. A. Bazilevskaya, G. Zampa, Beatrice Panico, V. Di Felice, F. Cafagna, Alfonso Monaco, M. Merge, D. Campana, Marco Casolino, Sergey Koldashov, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S. A., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A. A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergè, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, V. M., Simon, Sparvoli, P., Spillantini, Y. I., Stozhkov, P., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Koldobskiy, S, Krutkov, S. Y, Kvashnin, A. N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Mergè, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S. A, Yurkin, Y. T, Zampa, G, and Zampa, N.
Subjects: Physics, Quark matter, Space experiments, Cosmic rays, Spectrometers, Strange quark, PAMELA, Cosmic rays, Strange matter, PAMELA detector, Strangelet, Astrophysics::High Energy Astrophysical Phenomena, Settore FIS/01 - Fisica Sperimentale, General Physics and Astronomy, Cosmic ray, Astrophysics, law.invention, Physics and Astronomy (all), Strange matter, Rigidity (electromagnetism), Quark star, law, PAMELA, State of matter
Abstract: In this work we present results of a direct search for strange quark matter (SQM) in cosmic rays with the PAMELA space spectrometer. If this state of matter exists it may be present in cosmic rays as particles, called strangelets, having a high density and an anomalously high mass-to-charge (A/Z) ratio. A direct search in space is complementary to those from ground-based spectrometers. Furthermore, it has the advantage of being potentially capable of directly identifying these particles, without any assumption on their interaction model with Earth's atmosphere and the long-term stability in terrestrial and lunar rocks. In the rigidity range from 1.0 to ∼1.0×10^{3} GV, no such particles were found in the data collected by PAMELA between 2006 and 2009. An upper limit on the strangelet flux in cosmic rays was therefore set for particles with charge 1≤Z≤8 and mass 4≤A≤1.2×10^{5}. This limit as a function of mass and as a function of magnetic rigidity allows us to constrain models of SQM production and propagation in the Galaxy.
Published: 2015

22. 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.
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
Published: 2015

23. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data

Author: Yu. T. Yurkin, Mark Pearce, S. B. Ricciarini, V. Di Felice, Roberta Sparvoli, G. Zampa, Beatrice Panico, P. Papini, E. Vannuccini, D. Campana, G. C. Barbarino, Valentina Scotti, Valerio Formato, Yu. I. Stozhkov, A. M. Galper, Mirko Boezio, S. Yu. Krutkov, Alexey Leonov, N. Zampa, G. A. Bazilevskaya, S. Bottai, A. G. Mayorov, A. N. Kvashnin, Ritabrata Sarkar, M. A. Mayorova, Marco Casolino, P. Spillantini, V. V. Mikhailov, A. V. Karelin, E. Mocchuuitti, M. Simon, V. V. Malakhov, Sergey Koldashov, Riccardo Munini, G. Osteria, G. Castellini, Matteo Martucci, F. Palma, A. A. Kvashnin, Massimo Bongi, O. Adriani, L. Marcelli, F. Cafagna, W. Menn, N. De Simone, A. Bruno, Maria Teresa Ricci, P. Picozza, V. Bonvicini, Per Carlson, A. Vacci, S. A. Voronov, E. A. Bogomolov, S. Yu. Aleksandrin, G. I. Vasilyev, C. De Santis, C. De Donato, Alfonso Monaco, M. Merge, Nicola Mori, Malakhov, V. V, Koldashov, S. V, Mayorov, A. G, Mayorova, M. A, Mikhailov, V. V, Aleksandrin, S. Yu, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, A. M, Karelin, A. V, Krutkov, S. Yu, Kvashnin, A. A, Kvashnin, A. N, Leonov, A. A, Marcelli, L, Martucci, M, Menn, W, Merge, M, Mocchuuitti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Yu I, Vacci, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Yu T, Zampa, G, Zampa, N., V., Malakhov, S. V., Koldashov, A. G., Mayorov, M. A., Mayorova, V. V., Mikhailov, Aleksandrin, S. Y. u., O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. Y., Krutkov, A. A., Kvashnin, A. N., Kvashnin, A., Leonov, L., Marcelli, M., Martucci, W., Menn, M., Mergé, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, and N., Zampa
Subjects: History, High energy, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Proton flux, radiation belt, Education, law.invention, satellite experiment, symbols.namesake, law, PAMELA, Cosmic rays, radiation belt, proton, PAMELA, Cosmic rays, Physics, PAMELA detector, Settore FIS/04, Astronomy, Computer Science Applications, Proton (rocket family), Van Allen radiation belt, Physics::Space Physics, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Satellite, Time variations, proton
Abstract: The PAMELA and the ARINA experiments are carried out on the board of satellite RESURS-DK1 since 2006 up to now. Main goal of the PAMELA instrument is measurements of high energy antiparticles in cosmic rays while the ARINA instrument is intended studying high energy charged particle bursts in the magnetosphere. Both of these experiments have a possibility to study trapped particles in the inner radiation belt. Complex of these two instruments covers proton energy range from 30 MeV up to trapping limit (E= ~2 GeV). Continuous measurements with the PAMELA and the ARINA spectrometers include falling and rising phases of 23/24 solar cycles and maximum of 24th one. In this report we present temporal profiles of proton flux in the inner zone of the radiation belt (1.11 < L < 1.18, 0.18 < B < 0.22G). Dependence of proton fluxes on a magnitude of the solar activity was studied for various phases of 23/24 solar cycles. At that it was shown that proton fluxes at the solar minimum are several times greater than at the solar maximum.
Published: 2015

24. Search for Spatial and Temporary Variations of Galactic Cosmic Ray Positrons in PAMELA Experiment

Author: C. De Santis, Sergey Koldashov, E. A. Bogomolov, Alexey Leonov, Ritabrata Sarkar, P. Spillantini, Mirko Boezio, G. Castellini, E. Vannuccini, M. Simon, V. Bonvicini, M. Bongi, R. Sparvoli, R. Carbone, V. Formato, Sergey Koldobskiy, S. A. Voronov, D. Campana, S. Y. Krutkov, G. C. Barbarino, L. Marcelli, A. Vacchi, Yuri Stozhkov, Mark Pearce, A. V. Karelin, G. I. Vasilyev, Marco Casolino, S. B. Ricciarini, A. Bruno, V. Scotti, V. V. Malakhov, O. Adriani, N. De Simone, V. V. Mikhailov, F. Palma, E. Mocchiutti, P. Carlson, W. Menn, P. Picozza, Alfonso Monaco, G. Osteria, Nicola Mori, P. Papini, Marco Ricci, S. Bottai, M. Merge, F. Cafagna, N. Zampa, Riccardo Munini, G. A. Bazilevskaya, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, G. Zampa, Beatrice Panico, C. De Donato, Matteo Martucci, Yu. T. Yurkin, V. Di Felice, A. G. Mayorov, Mikhailov, V. V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Malakhov, V. V., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Koldobskiy, S., Krutkov, S., Kvashnin, A., Leonov, A., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Settore FIS/01, Physics, Annihilation, Spectrometer, PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, electrons, Astronomy, Cosmic ray, Astrophysics, anisotropy, Physics and Astronomy(all), law.invention, Physics and Astronomy (all), Positron, Pulsar, law, cosmic ray, positons, Neutron detection, High Energy Physics::Experiment
Abstract: The PAMELA experiment is gathering data since 2006 on board the Resurs DK1 satellite (orbit with inclination 70.4°, the altitude 350-600km). The instrument consists magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter, neutron detector and shower scintillator that gives possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Results of the experiment indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10GeV. This excess might be originated through dark matter annihilation or in local astrophysical objects such as pulsars producing possible spatial and season variations. Electron and positron events have been analyzed searching for spatial and temporal variations from June 2006 till January 2014.
Published: 2015

25. Ground-based tests of JEM-EUSO components at the Telescope Array site, 'EUSO-TA'

Author: Hiroyuki Sagawa, A. Bruno, M. Rybczyński, Alfonso Monaco, G. Cordero, N. Tone, O. Martinez, C. Tenzer, L. Tkachev, Y. Uchihori, E. Kuznetsov, Ovidiu Vaduvescu, K. Nomoto, I. Kreykenbohm, Maxim Gonchar, R. Matev, T. Mernik, G. Catalano, M. Lacombe, Claudio Cassardo, A. Anzalone, T. Batsch, Roberto Bellotti, K. Mannheim, M. Serra, M. Yu. Zotov, Susana Briz, Satoshi Wada, T. Ogawa, C. De Santis, S. Blin-Bondil, Y. Kawasaki, R. Young, N. Inoue, K. Higashide, I. V. Yashin, T. Tajima, J. Bayer, T. Nonaka, Angela V. Olinto, Fernando López, Andrea Santangelo, A. Pollini, Pavel Klimov, M. Di Martino, S. Falk, V. Andreev, G. Giraudo, T. Kajino, T. Tymieniecka, J. Sledd, F. Tajima, R. Tsenov, J. Yang, D. Cline, A. Dell’Oro, I. Kaneko, B. Szabelska, G. Medina-Tanco, F. Guarino, F. Ronga, D. Yonetoku, T. Wibig, T. Napolitano, S. Nagataki, Tomás Belenguer, J. Blümer, S. Watanabe, P. Orleański, G. Masciantonio, Silvia Ferrarese, Mitsuteru Sato, H. Tokuno, H. Schieler, A. J. de Castro, M. Fukushima, Z. Plebaniak, M. J. Christl, R. Bechini, A. Insolia, J. Błȩcki, I. Rodríguez, H. Lim, M. C. Maccarone, B. Keilhauer, J. N. Capdevielle, L. Santiago Crúz, L. Wiencke, J. Watts, C. Pennypacker, C. González Alvarado, G. Osteria, M. I. Panasyuk, P. L. Biermann, H. Sato, M. Nagano Murakami, T. Sugiyama, L. Anchordoqui, I. H. Park, B. Pastircak, K. Asano, A. Guzman, S. Ogio, Francesco Isgrò, J. Fujimoto, B. A. Khrenov, H. Miyamoto, F. Kajino, I. Rusinov, Frederic Trillaud, G. Modestino, P. Reardon, M. Chikawa, L. Valore, P. Vallania, A. Jung, G. Siemieniec-Oziȩbło, A. Marini, H. Ikeda, G. Prévôt, H. J. Crawford, D. Supanitsky, S. Perez Cano, M. Suzuki, M. Ricci, K. Shinozaki, N. Tajima, B. Mot, M. Karus, L. Villaseñor, T. Pierog, M. D. Rodríguez Frías, M. Kleifges, C. Moretto, P. Bobik, S. Biktemerova, H. W. Park, T. Paul, F. Dulucq, R. Nava, J. H. Adams, P. Galeotti, Y. Yamamoto, N. Sakaki, K. Tsuno, M. Nagata, Yukihiro Takahashi, M. Bogomilov, K. Belov, S. Sánchez, A. Ebersoldt, E. G. Judd, Domenico Finco, Rossella Caruso, Dmitry V. Naumov, K. Yoshida, M. Weber, Y. Karadzhov, M. Sanz Palomino, D. Allard, P. Barrillon, M. E. Bertaina, E. Joven, G. Distratis, J. F. Valdés-Galicia, Marco Casolino, D. Monnier-Ragaigne, A. Segreto, T. Shibata, D. Maravilla, K. Kawai, Y. Kurihara, H. Prieto, S. Csorna, G. Castellinic, Akinori Saito, G. Sáez-Cano, H. Rothkaehl, C. Catalano, Y. Hachisu, Claudio Fornaro, Y. Arai, T. Tomida, Gali Garipov, N. Blanc, H. H. Silva Lopez, C. De Donato, M. D. Sabau, M. Putis, A. Sobey, G. Roudil, D. Semikoz, K. Słomińska, H. Takami, J. Licandro, M. Bonamente, T. Peter, T. Nakamura, P. Gorodetzky, J. S. Kim, V. S. Morozenko, B. Harlov, S. Selmane, Carlo Vigorito, Hajime Yano, K. Kudela, P. Prat, S. Piraino, S. Ahmad, M. Unger, G. Vankova, M. Sakata, A. Neronov, C. Lachaud, S. Dagoret-Campagne, R. Cremonini, M. Reyes, L. Marcelli, Z. Włodarczyk, D. Kolev, J. N. Albert, Thomas Schanz, T. Yamamoto, T. Patzak, I. Fernández-Gómez, F. Cafagna, P. von Ballmoos, G. Gelmini, P. Baragatti, Toshikazu Ebisuzaki, M. Ave Pernas, F. Sarazin, Livio Conti, Sergei A. Sharakin, A. Zuccaro Marchi, A. A. Berlind, Jörn Wilms, Simona Toscano, O. A. Saprykin, H. M. Shimizu, J. Geary, V. Scotti, Ke Fang, T. Murakami, N. De Simone, C. de la Taille, K. Katahira, A. Kusenko, J. Karczmarczyk, M. Dupieux, Y. Miyazaki, L. del Peral, A. Franceschi, E. Parizot, J. A. Morales de los Ríos, Susumu Inoue, M. S. Briggs, Y. Tsunesada, P. Picozza, H. Salazar, K. Mase, O. Tibolla, J. Hernández Carretero, D. Campana, J. Lee, H. Ohmori, M. Wille, A. Cellino, M. Roth, Lech Wiktor Piotrowski, T. Shirahama, S. Yoshida, R. Engel, S. W. Kim, J. Watanabe, M. Takeda, A. Haungs, T. J. Weiler, V. Connaughton, M. Flamini, Y. Takizawa, C. Blaksley, J. Szabelski, Y. Mizumoto, Francesco Fenu, Y. Itow, D. Ikeda, 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: Physics::Instrumentation and Detectors, Ciencias Físicas, Astrophysics::High Energy Astrophysical Phenomena, JEM-EUSO, Telescope array, EUSO-TA, Ultra high energy cosmic ray, law.invention, Telescope, Light source, Optics, law, Calibration, Electronics, Ultra high energy cosmic rays, Astronomy and Astrophysics, Space and Planetary Science, Physics, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysic, Astronomía, Air shower, High Energy Physics::Experiment, business, CIENCIAS NATURALES Y EXACTAS
Abstract: We are conducting tests of optical and electronics components of JEM-EUSO at the Telescope Array site in Utah with a ground-based "EUSO-TA" detector. The tests will include an engineering validation of the detector, cross-calibration of EUSO-TA with the TA fluorescence detector and observations of air shower events. Also, the proximity of the TA?s Electron Light Source will allow for convenient use of this calibration device. In this paper, we report initial results obtained with the EUSO-TA telescope. 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.. INAF - 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 (UAH); España Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. Lomonosov Moscow State University; Rusia Fil: Bayer, J.. University of Tubingen; Alemania Fil: Bechini, R.. Universita’ di Torino; 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: Blacki, 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: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos 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: Kawasaki, Yoshiya. RIKEN; Japón Fil: Piotrowski, Lech Wiktor. RIKEN; Japón Fil: Kawasaki, Yoshiya. Yoshiya; Japón Fil: Piotrowski, Lech Wiktor. Yoshiya; Japón Fil: The JEM-EUSO Collaboration ·.
Published: 2015

26. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

Author: L. Marcelli, A. Vacchi, S. Bottai, A. Bruno, E. Mocchiutti, D. Campana, Mirko Boezio, Maria Teresa Ricci, Marco Casolino, F. Cafagna, A. V. Karelin, Riccardo Munini, Etienne Vos, G. Osteria, M. S. Potgieter, O. Adriani, Massimo Bongi, Matteo Martucci, Alexey Leonov, W. Menn, V. V. Mikhailov, V. Formato, Valentina Scotti, N. Zampa, G. A. Bazilevskaya, C. De Santis, Roberto Bellotti, A. M. Galper, Sergey Koldashov, A. N. Kvashnin, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, V. Bonvicini, Y. I. Stozhkov, A. G. Mayorov, M. Simon, Sergey Koldobskiy, F. Palma, G. C. Barbarino, V. Di Felice, Nicola Mori, V. V. Malakhov, C. De Donato, G. I. Vasilyev, Roberta Sparvoli, S. Y. Krutkov, P. Picozza, P. Spillantini, Alfonso Monaco, M. Merge, Ritabrata Sarkar, S. A. Voronov, E. A. Bogomolov, N. De Simone, G. Castellini, Per Carlson, Yu. T. Yurkin, G. Zampa, Beatrice Panico, Munini, R, Di Felice, V, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Koldobskiy, S, Krutkov, S. Y, Kvashnin, A. N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Merge, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S. A, Yurkin, Y. T, Zampa, G, Zampa, N, Potgieter, M. S, Vos, E. E., Munini, Riccardo, V., Di Felice, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, M. S., Potgieter, and E. E., Vos
Subjects: Solar minimum, electron, History, Antiparticle, Astrophysics::High Energy Astrophysical Phenomena, solar minimum, Solar cycle 23, Cosmic ray, Astrophysics, Solar Modulation, electron, solar minimum, PAMELA, Education, law.invention, Physics and Astronomy (all), law, PAMELA, Cosmology, Modulation, Solar energy Apparatus design, Charged components, Electron spectrum, Galactic cosmic rays, Solar minima, Solar modulation, Solar modulation effects, Coronal mass ejection, Physics, PAMELA detector, Settore FIS/04, Computer Science Applications, Solar cycle, Solar Modulation, Antimatter, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING
Abstract: The satellite-borne PAMELA experiment has been continuously collecting data since 15th June 2006, when it was launched from the Baikonur cosmodrome to detect the charged component of cosmic rays over a wide energy range and with unprecedented statistics. The apparatus design is particularly suited for particle and antiparticle identification. The PAMELA experiment has measured the electron spectrum at Earth in great detail, extending up to about 100 GeV and down to about 200 MeV. The galactic cosmic ray electron spectra for 2007 and 2009, i.e. measured during the A
Published: 2015

27. PAMELA measurements of the boron and carbon spectra

Author: Alexey Leonov, A. G. Mayorov, Ritabrata Sarkar, G. Zampa, Beatrice Panico, S. Y. Krutkov, Yu. T. Yurkin, A. V. Karelin, C. De Santis, N. Zampa, G. A. Bazilevskaya, P. Picozza, P. Spillantini, Valerio Formato, C. De Donato, G. Osteria, Riccardo Munini, D. Campana, R. Carbone, O. Adriani, Alfonso Monaco, Sergey Koldobskiy, V. Di Felice, G. C. Barbarino, W. Menn, V. Bonvicini, V. V. Malakhov, Marco Casolino, Roberto Bellotti, Valentina Scotti, G. Castellini, A. M. Galper, L. Marcelli, Y. I. Stozhkov, A. Vacchi, S. Bottai, A. Bruno, M. Merge, N. De Simone, M. Bongi, A. N. Kvashnin, Mark Pearce, S. B. Ricciarini, Sergey Koldashov, Nicola Mori, P. Papini, Matteo Martucci, E. Vannuccini, Mirko Boezio, S. A. Voronov, G. I. Vasilyev, Per Carlson, E. A. Bogomolov, F. Palma, V. V. Mikhailov, Maria Teresa Ricci, F. Cafagna, M. Simon, Roberta Sparvoli, E. Mocchiutti, N., Mori, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, Mori, N, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Koldobskiy, S, Krutkov, S. Y, Kvashnin, A. N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Mergé, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, and Zampa, N.
Subjects: History, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, chemistry.chemical_element, Cosmic ray, Spectral line, Education, law.invention, Nuclear physics, Physics and Astronomy (all), cosmic rays, law, PAMELA, Boron, Cosmic ray measurement, Cosmology, High energy physics Anticoincidence systems, Boron and carbons, Cosmic ray spectra, Data analysis techniques, Electromagnetic calorimeter, Injection spectra, Magnetic spectrometers, Time of flight systems, Neutron detection, Physics, carbon boron, Spectrometer, PAMELA detector, Settore FIS/04, PAMELA, cosmic rays, carbon boron, fluxes, fluxes, Computer Science Applications, chemistry, Antimatter, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Carbon
Abstract: The satellite-borne PAMELA experiment is aimed at precision measurements of the charged light component of the cosmic-ray spectrum, with a particular focus on antimatter. It consists of a magnetic spectrometer, a time-of-flight system, an electromagnetic calorimeter with a tail catcher scintillating layer, an anticoincidence system and a neutron detector. PAMELA has measured the absolute fluxes of boron and carbon and the B/C ratio, which plays a central role in galactic propagation studies in order to derive the injection spectra at sources from measurements at Earth. In this paper, the data analysis techniques and the final results are presented.
Published: 2015

28. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

Author: S. Bottai, Roberta Sparvoli, Sergey Koldobskiy, A. V. Karelin, G. C. Barbarino, Alfonso Monaco, Yu. T. Yurkin, D. Campana, G. Osteria, Riccardo Munini, M. Merge, L. Marcelli, A. Vacchi, Per Carlson, Marco Casolino, A. Bruno, F. Palma, V. V. Malakhov, S. Y. Krutkov, Sergey Koldashov, Massimo Bongi, S. A. Voronov, Roberto Bellotti, G. Zampa, Beatrice Panico, R. Carbone, A. M. Galper, E. A. Bogomolov, N. Zampa, G. A. Bazilevskaya, Valentina Scotti, A. N. Kvashnin, P. Picozza, G. Castellini, Laura Rossetto, Mirko Boezio, Mark Pearce, S. B. Ricciarini, Alexey Leonov, N. De Simone, P. Papini, E. Vannuccini, Ritabrata Sarkar, Valerio Formato, V. V. Mikhailov, M. Simon, O. Adriani, W. Menn, Matteo Martucci, F. Cafagna, Maria Teresa Ricci, Piero Spillantini, A. G. Mayorov, G. I. Vasilyev, C. De Santis, C. De Donato, Nicola Mori, E. Mocchiutti, V. Di Felice, V. Bonvicini, A. V., Karelin, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, A. G., Mayorov, V., Malakhov, L., Marcelli, M., Martucci, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, L., Rossetto, M., Simon, R., Sparvoli, P., Spillantini, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, Karelin, A. V, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V., Galper, A. M, Koldashov, S. V, Koldobskiy, S. A, Krutkov, S. Y, Kvashnin, A. N, Leonov, A. A, Mayorov, A. G, Malakhov, V. V, Marcelli, L, Martucci, M., Menn, W, Merge, M., Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R., Osteria, G, Palma, F, Panico, B., Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V., Rossetto, L, Simon, M, Sparvoli, R, Spillantini, P, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, and Zampa, N.
Subjects: electron, History, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Cosmic rays, positron, electron, PAMELA, Cosmic ray, Particle detector, Education, law.invention, Nuclear physics, Physics and Astronomy (all), Positron, law, PAMELA, Neutron detection, Ultra-high-energy cosmic ray, Cosmic rays, Physics, Calorimeter (particle physics), PAMELA detector, Settore FIS/04, Computer Science Applications, Antimatter, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, positron, High Energy Physics::Experiment, Calorimeters, Cosmic ray measurement, Cosmology, Electron energy levels, Positrons, Tellurium compounds Cosmic ray electrons, Energy ranges, High-energy cosmic rays, High-energy electron, High-energy range
Abstract: At present the existing data on the cosmic ray electron energy spectra in the high energy range are fragmented, and the situation is exacerbated by their small number. In the satellite PAMELA experiment measurements at high energies are carried out by the calorimeter. The experimental data accumulated for more than 8 years of measurements, with the information of the calorimeter, the neutron detector and the scintillation counters made it possible to obtain the total spectrum of high-energy electrons and positrons in energy range 0.3-3 TeV.
Published: 2015

29. Searching for anisotropy of positrons and electrons in the PAMELA experiment

Author: N. Zampa, Alfonso Monaco, Mark Pearce, S. B. Ricciarini, C. De Santis, Giuseppe Osteria, G. A. Bazilevskaya, P. Picozza, P. Papini, V. G. Zverev, E. Vannuccini, C. De Donato, Alexey Leonov, P. Spillantini, R. Carbone, V. Malvezzi, M. Merge, F. Palma, Sergey Koldobskiy, Sergey Koldashov, Ritabrata Sarkar, Nicola Mori, S. A. Voronov, Roberta Sparvoli, G. C. Barbarino, S. Bottai, G. Zampa, Beatrice Panico, Yu. I. Stozhkov, O. Adriani, Mirko Boezio, V. V. Malakhov, Lorenzo Bonechi, V. Bonvicini, D. Campana, L. Marcelli, G. I. Vasilyev, V. V. Mikhailov, G. Castellini, M. Bongi, A. Vacchi, P. Carlson, A. Bruno, Roberto Bellotti, Marco Casolino, A. M. Galper, E. A. Bogomolov, E. Mocchiutti, F. Cafagna, A. N. Kvashnin, A. V. Karelin, Yu. T. Yurkin, Riccardo Munini, W. Menn, M. Simon, V. Di Felice, Marco Ricci, N. De Simone, S. Yu. Krutkov, A. G. Mayorov, Matteo Martucci, V. V., Mikhailov, O., Adriani, G. C., Barbarino, G., A., R., Bellotti, M., Boezio, E., A., L., Bonechi, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, A. M., Galper, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V. G., Zverev, G., Zampa, N., Zampa, F., Cafagna, D., Campana, R., Carbone, A. V., Karelin, P., Carlson, M., Casolino, G., Castellini, A. N., Kvashnin, S. V., Koldashov, S. A., Koldobskiy, Krutkov, S. Y. u., A. A., Leonov, V., Malvezzi, L., Marcelli, M., Martucci, A. G., Mayorov, V., Malakhov, W., Menn, M., Merge, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palm, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, M., Simon, R., Sarkar, R., Sparvoli, P., Spillantini, Stozhkov, Y. u. I., Yurkin, Y. u. T., Mikhailov, V. V., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Zverev, V. G., Zampa, G., Zampa, N., Cafagna, F., Campana, D., Carbone, R., Karelin, A. V., Carlson, P., Casolino, M., Castellini, G., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Leonov, A. A., Malvezzi, V., Marcelli, L., Martucci, M., Mayorov, A. G., Malakhov, V., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sarkar, R., Sparvoli, R., and Spillantini, P.
Subjects: Physics, positrons, Annihilation, PAMELA detector, Settore FIS/04, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, electrons, General Physics and Astronomy, Cosmic ray, Astrophysics, Electron, anisotropy, law.invention, Physics and Astronomy (all), Positron, Pulsar, cosmic rays, law, PAMELA, Positron sources, Anisotropy, Electrons, PAMELA, cosmic rays, anisotropy, positrons, electrons
Abstract: The PAMELA experiment has been under way aboard the Resurs DK-1 satellite since June 2006. The results have revealed an increase in the ratio of the positron intensity to the total electron and positron intensity at energies in excess of 10 GeV. This increase suggests an additional source of cosmic rays that is associated with either some astrophysical objects (e.g., pulsars) or the probable annihilation of particles of dark matter. Local positron sources can produce notable anisotropy in their flux. The results from the search for anisotropy of positrons and electrons in the events detected by the PAMELA experiment in the 2006-2013 timeframe are described in detail in this work.
Published: 2015

30. 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., FernÃ¡ndez GÃ³mez, 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., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez 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 RÃos, 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., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, 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 LÃ³pez, 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., ValdÃ©s 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.
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
Published: 2015

31. 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

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

Author: Alfonso Monaco, P. Spillantini, M. Merge, R. Carbone, Mirko Boezio, Sergey Koldobskiy, G. C. Barbarino, D. Campana, A. G. Mayorov, V. V. Mikhailov, P. Carlson, F. Cafagna, V. Di Felice, N. De Simone, M. Simon, G. Castellini, Marco Casolino, A. A. Leonov, L. Marcelli, A. Vacchi, S. A. Voronov, A. Bruno, Roberta Sparvoli, Sergey Koldashov, V. Bonvicini, Ritabrata Sarkar, Matteo Martucci, E. A. Bogomolov, Y. I. Stozhkov, S. Bottai, Riccardo Munini, Roberto Bellotti, V. V. Malakhov, Mark Pearce, S. B. Ricciarini, A. M. Galper, C. De Donato, P. Papini, A. N. Kvashnin, E. Vannuccini, V. G. Zverev, P. Picozza, G. Zampa, Marco Ricci, N. Zampa, G. A. Bazilevskaya, M. Bongi, Valerio Formato, A. V. Karelin, O. Adriani, Y. Krutkov, W. Menn, E. Mocchiutti, C. Pizzolotto, Y. T. Yurkin, G. I. Vasilyev, C. De Santis, G. Osteria, Nicola Mori, M. P. De Pascale, F. Palma, Valentina Scotti, Formato, V. p., Adriani, O. b., Barbarino, Giancarlo, Bazilevskaya, G., Bellotti, R. g., Boezio, M., Bogomolov, E., Bongi, M. b., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P. k., Casolino, M. m., Castellini, G., C. k., L, M. o., De, C. o., De, Simone, N. D., Felice, V. D., Galper, A., Karelin, A., Koldashov, S., Koldobskiy, S., Krutkov, Y., Kvashnin, A., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M. r., Mayorov, A., Menn, W., Merg��, M. o., Mikhailov, V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R. p., Osteria, Giuseppe, Palma, F. o., Papini, P., Pearce, M. k., Picozza, P. o., Pizzolotto, C. u., Ricci, M., Ricciarini, S., Sarkar, R., Simon, M., Scotti, V. d., Sparvoli, R. o., Spillantini, P. b., Stozhkov, Y., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S., Yurkin, Y., Zampa, G., Zampa, N., Zverev, V., Formato, V., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Carlson, P., Casolino, M., De Donato, C., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Kvashnin, A. N., Martucci, M., Mayorov, A. G., Mergè, M., Mikhailov, V. V., Munini, Riccardo, Osteria, G., Palma, F., Pearce, M., Picozza, P., Pizzolotto, C., Ricciarini, S. B., Scotti, V., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Voronov, S. A., Yurkin, Y. T., and Zverev, V. G.
Subjects: Nuclear and High Energy Physics, Hydrogen, Astrophysics::High Energy Astrophysical Phenomena, Flux, chemistry.chemical_element, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Cosmic ray propagation, Isotopes, PAMELA, Instrumentation, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, law, Isotopes of helium, Physics, Cosmic ray measurement, Isotopes, PAMELA detector, Cosmic ray propagation, Galactic cosmic rays, Helium isotopes, Magnet spectrometers, PAMELA, Propagation models, Satellite-borne experiment, Time-of-flight system, Detector, Astronomy, Cosmic rays, Experiments, Galaxies, Isotopes, Rigidity, chemistry, Antimatter, Physics::Space Physics, Satellite
Abstract: PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature, with particular focus on the antimatter component. The detector consists of a permanent magnet spectrometer core to provide rigidity and charge sign information, a Time-of-Flight system for velocity and charge information, a Silicon-Tungsten calorimeter and a Neutron detector for lepton/hadron identification. The velocity and rigidity information allow the identification of different isotopes for Z=1 and Z=2 particles in the energy range 100 MeV/n to 1 GeV/n. In this work we will present the PAMELA results on the H and He isotope fluxes based on the data collected during the 23rd solar minimum from 2006 to 2007. Such fluxes carry relevant information helpful in constraining parameters in galactic cosmic rays propagation models complementary to those obtained from other secondary to primary measurements such as the boron-to-carbon ratio. �� 2013 Elsevier B.V.
Published: 2014

33. New measurements of the energy spectra of high-energy cosmic-ray protons and helium nuclei with the calorimeter in the PAMELA experiment

Author: V. Bonvicini, P. Spillantini, S. Bottai, S. Yu. Krutkov, V. G. Zverev, N. De Simone, Alfonso Monaco, N. Zampa, R. Sarkar, C. Pizzolotto, Nicola Mori, M. Simon, Yu. T. Yurkin, A. A. Leonov, Mark Pearce, S. B. Ricciarini, Roberta Sparvoli, O. Adriani, P. Papini, W. Menn, V. Di Felice, E. Vannuccini, S. A. Voronov, Per Carlson, V. Malvezzi, P. Picozza, A. M. Galper, F. Cafagna, Mirko Boezio, Marco Ricci, G. I. Vasilyev, M. Merge, M. Bongi, G. A. Bazilevskaya, R. Carbone, Sergey Koldobskiy, G. C. Barbarino, C. De Santis, A. Bruno, Matteo Martucci, C. De Donato, F. Palma, Gianluigi Zampa, V. V. Mikhailov, Andrea Vacchi, Yu. I. Stozhkov, L. Marcelli, Giuseppe Osteria, A. G. Mayorov, E. Mocchiutti, G. Castellini, V. V. Malakhov, L. Boneci, E. A. Bogomolov, Roberto Bellotti, A. N. Kvashnin, Sergey Koldashov, D. Campana, A. V. Karelin, Marco Casolino, A., Karelin, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Bellotti, M., Boezio, E., Bogomolov, L., Boneci, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, A., Galper, C. D., Donato, C. D., Santi, N. D., Simone, V. D., Felice, V., Zverev, G., Zampa, N., Zampa, F., Cafagna, D., Campana, R. h., Carbone, P., Carlson, M., Casolino, G., Castellini, A., Kvashnin, S., Koldashov, S., Koldobskiy, S., Krutkov, A., Leonov, V., Malvezzi, L., Marcelli, M., Martucci, A., Mayorov, V., Malakhov, W., Menn, M., Merge, V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y., Stozhkov, and Y., Yurkin
Subjects: Physics, PAMELA detector, Solid-state physics, Calorimeter (particle physics), Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, General Physics and Astronomy, chemistry.chemical_element, Cosmic ray, Alpha particle, respiratory system, Spectral line, law.invention, Nuclear physics, Physics and Astronomy (all), chemistry, Energy spectra, Event selection, Helium nuclei, Measurements of, Position sensitive, Satellite-borne experiment, law, Protons, Nucleon, Nuclear Experiment, Helium, Calorimeters, Cosmic rays, Experiments, Helium, Spectroscopy
Abstract: New measurements of the energy spectra of cosmic-ray protons and helium nuclei with significantly increased statistics owing to an improvement of the event selection technique and the involvement of all data over the period 2006?????????2013 in the analysis have been made at energies above 0.8 TeV/nucleon with a position-sensitive calorimeter based on data from the PAMELA satellite-borne experiment.
Published: 2014

34. The PAMELA experiment and antimatter in the universe

Author: A. M. Galper, Valerio Formato, V. Bonvicini, S. A. Voronov, Ritabrata Sarkar, Riccardo Munini, Y. I. Stozhkov, V. V. Malakhov, C. De Donato, G. Castellini, E. A. Bogomolov, P. Picozza, C. Pizzolotto, Y. T. Yurkin, F. Palma, Mark Pearce, S. B. Ricciarini, Roberto Bellotti, P. Papini, E. Vannuccini, Marco Ricci, G. Zampa, G. I. Vasilyev, P. Spillantini, A. Vacchi, M. P. De Pascale, A. G. Mayorov, A. N. Kvashnin, A. V. Karelin, Y. Krutkov, A. Bruno, G. Osteria, Valentina Scotti, V. G. Zverev, Nicola Mori, Alfonso Monaco, E. Mocchiutti, L. Marcelli, C. De Santis, V. Di Felice, Mirko Boezio, M. Simon, M. Merge, Per Carlson, A. A. Leonov, Matteo Martucci, Roberta Sparvoli, N. Zampa, G. A. Bazilevskaya, S. Bottai, Sergey Koldashov, N. De Simone, V. V. Mikhailov, D. Campana, F. Cafagna, Marco Casolino, O. Adriani, W. Menn, M. Bongi, R. Carbone, Sergey Koldobskiy, G. C. Barbarino, Boezio, M., Carbone, R., Adriani, O., Barbarino, Giancarlo, Bazilevskaya, G., Bellotti, R. h., Bogomolov, E., Bongi, M. c., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M. l., Castellini, G., Donato, C. D., M. n., De, C. n., De, Simone, N. D., Felice, V. D., Formato, V. o., Galper, A., Karelin, A., Koldashov, S., Koldobskiy, S., Krutkov, Y., Kvashnin, A., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M. q., Mayorov, A., Menn, W., Merg??????, M. n., Mikhailov, V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R. o., Osteria, Giuseppe, Palma, F. n., Papini, P., Pearce, M., Picozza, P. n., Pizzolotto, C. t., Ricci, M., Ricciarini, S. m., Sarkar, R., Scotti, V. e., Simon, M., Sparvoli, R. o., Spillantini, P. c., Stozhkov, Y., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S., Yurkin, Y., Zampa, G., Zampa, N., Zverev, V., Ariani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Casolino, M., De Donato, C., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Kvashnin, A. N., Martucci, M., Mayorov, A. G., Mergè, M., Mikhailov, V. V., Munini, Riccardo, Osteria, G., Palma, F., Piccozza, P., Pizzolotto, C., Ricciarini, S. B., Scotti, V., Sparsoli, R., Spillantini, P., Stozhkov, Y. I., Voronov, S. A., Yurkin, Y. T., and Zverev, V. G.
Subjects: Antiparticle, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Antiparticles, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, law.invention, law, Atomic and Molecular Physics, Physical and Theoretical Chemistry, Astroparticle physics, Physics, Cosmic-ray, PAMELA detector, Astrophysics::Instrumentation and Methods for Astrophysics, Space experiment, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Interstellar medium, Antiproton, Antimatter, and Optics
Abstract: On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The primary scientific goal is the measurement of the antiproton and positron energy spectra. Antiparticles are a natural component of the cosmic radiation being produced in the interaction between cosmic rays and the interstellar matter. They have been shown to be extremely interesting for understanding the propagation mechanisms of cosmic rays. Furthermore, novel sources of primary cosmic-ray antiparticles of either astrophysical or exotic origin (e.g. annihilation of dark matter particles) can also be probed. In this paper we review the PAMELA antiparticle results and their significance for the field of astroparticle physics. © 2014 Springer International Publishing Switzerland.
Published: 2014

35. A method to detect positron anisotropies with Pamela data

Author: R. Carbone, Sergey Koldobskiy, G. C. Barbarino, V. Di Felice, P. Spillantini, A. M. Galper, M. Simon, Roberto Bellotti, A. A. Leonov, V. G. Zverev, Per Carlson, E. Mocchiutti, Riccardo Munini, A. N. Kvashnin, A. G. Mayorov, S. Y. Krutkov, N. Zampa, G. A. Bazilevskaya, V. V. Malakhov, Maria Teresa Ricci, V. Bonvicini, Y. I. Stozhkov, Valerio Formato, S. B. Ricciarini, Roberta Sparvoli, C. Pizzolotto, S. A. Voronov, P. Picozza, Alfonso Monaco, G. Zampa, Beatrice Panico, Mark Pearce, E. A. Bogomolov, Y. T. Yurkin, A. V. Karelin, F. Palma, S. Bottai, M. Merge, G. Castellini, G. Osteria, Mirko Boezio, P. Papini, E. Vannuccini, Ritabrata Sarkar, Matteo Martucci, V. V. Mikhailov, N. De Simone, F. Cafagna, C. De Donato, Nicola Mori, G. I. Vasilyev, C. De Santis, O. Adriani, W. Menn, M. Bongi, L. Marcelli, A. Vacchi, A. Bruno, D. Campana, Marco Casolino, Sergey Koldashov, V. Scotti, Ugo Giaccari, Panico, B., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Giaccari, U., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G., and Munini, Riccardo
Subjects: Physics, PAMELA, cosmic ray, anisotropy, positron, electrons, Nuclear and High Energy Physics, Annihilation, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Flux, Cosmic ray, Astrophysics, Electron, Atomic and Molecular Physics, and Optics, law.invention, Nuclear physics, Positron, Pulsar, law, Atomic and Molecular Physics, Anisotropy, Electrons, and Optics
Abstract: The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference. © 2014 Elsevier B.V.
Published: 2014

36. PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA

Author: S. V. Borisov, G. Zampa, S. A. Voronov, N. De Simone, P. Spillantini, E. A. Bogomolov, A. V. Karelin, C. De Santis, William Gillard, Giovanna Jerse, L. Marcelli, A. G. Mayorov, A. Vacchi, Laura Rossetto, V. V. Mikhailov, V. G. Zverev, G. C. Barbarino, G. Osteria, F. Palma, O. Adriani, R. Carbone, S. Bottai, V. Di Felice, N. N. Nikonov, W. Menn, L. Consiglio, Alfonso Monaco, Juan Wu, Roberta Sparvoli, N. Zampa, G. A. Bazilevskaya, S. Y. Krutkov, M. D. Kheymits, L. A. Grishantseva, M. Bongi, V. V. Malakhov, C. Pizzolotto, M. P. De Pascale, Nicola Mori, V. Bonvicini, Y. T. Yurkin, D. Campana, F. Cafagna, A. Bruno, Y. I. Stozhkov, Maria Teresa Ricci, P. Picozza, Roberto Bellotti, Per Carlson, Mirko Boezio, Marco Casolino, E. Mocchiutti, G. I. Vasilyev, A. N. Kvashnin, M. Simon, S. V. Koldashov, A. A. Leonov, A. M. Galper, Ritabrata Sarkar, G. Castellini, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, A., Bruno, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. g., Bellotti, M., Boezio, E., Bogomolov, M., Bongi, V., Bonvicini, S. k., L., S., Bottai, F., Cafagna, D., Campana, R. k., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. k., De, C. k., De, N. k., De, V. D., Felice, A., Galper, W., Gillard, L., Grishantseva, G. o., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. c., Monaco, N. c., Mori, N. j., K., Osteria, Giuseppe, F. k., Palma, P., Papini, M., Pearce, P. k., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. k., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Yurkin, J., Wu, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, Antimatter, Cosmic rays, Dark matter, Solar modulation, Trapped radiation, Engineering (all), PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, General Engineering, Astronomy, Magnetosphere, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy, law.invention, Positron, Antiproton, law, lcsh:TA1-2040, lcsh:Engineering (General). Civil engineering (General)
Abstract: The PAMELA experiment was launched on board the Resurs-DK1 satellite on June 15th 2006. The apparatus was designed to conduct precision studies of charged cosmic radiation over a wide energy range, from tens of MeV up to several hundred GeV, with unprecedented statistics. In five years of continuous data taking in space, PAMELA accurately measured the energy spectra of cosmic ray antiprotons and positrons, as well as protons, electrons and light nuclei, sometimes providing data in unexplored energetic regions. These important results have shed new light in several astrophysical fields like: an indirect search for Dark Matter, a search for cosmological antimatter (anti-Helium), and the validation of acceleration, transport and secondary production models of cosmic rays in the Galaxy. Some of the most important items of Solar and Magnetospheric physics were also investigated. Here we present the most recent results obtained by the PAMELA experiment. �� Czech Technical University in Prague, 2013.
Published: 2013

37. Spectra of primary cosmic-ray positrons and electrons in the PAMELA experiment

Author: Yu. T. Yurkin, Roberta Sparvoli, R. Sarkar, A. Bruno, M. Simon, Yu. I. Stozhkov, G. Jerse, C. Pizzolotto, V. Di Felice, N. De Simone, Lorenzo Bonechi, D. Campana, M. Bongi, V. Bonvicini, M. P. De Pascale, Marco Casolino, S. Yu. Krutkov, V. G. Zverev, L. A. Grishantseva, P. Picozza, N. Zampa, P. Spillantini, V. V. Malakhov, S. Bottai, Giuseppe Osteria, F. Cafagna, G. A. Bazilevskaya, E. Mocchiutti, A. A. Leonov, V. Malvezzi, O. Adriani, V. V. Mikhailov, A. V. Karelin, F. Palma, P. Carlson, S. V. Koldashov, Juan Wu, Marco Ricci, Mirko Boezio, A. N. Kvashnin, A. G. Mayorov, L. Marcelli, R. Carbone, S. A. Voronov, Sergey Koldobskiy, Laura Rossetto, G. C. Barbarino, G. Castellini, Andrea Vacchi, C. De Santis, E. A. Bogomolov, Alfonso Monaco, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, A. M. Galper, Gianluigi Zampa, L. Consiglio, R. Belotti, G. I. Vasilyev, Nicola Mori, W. Menn, V. V., Mikhailov, O., Adriani, G. A., Bazilevskaya, Barbarino, Giancarlo, R., Belotti, E. A., Bogomolov, M., Boezio, V., Bonvicini, M., Bongi, L., Bonechi, S., Bottai, A., Bruno, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, J., Wu, A. M., Galper, L. A., Grishantseva, C., Santi, N., Simone, G., Jerse, V., Felice, G., Zampa, N., Zampa, V. G., Zverev, M., Casolino, D., Campana, P., Carlson, R., Carbone, A. V., Karelin, G., Castellini, F., Cafagna, A. N., Kvashnin, S. V., Koldashov, S. A., Koldobskiy, Consiglio, Lucia, Krutkov, S. Y. u., A. A., Leonov, V. V., Malakhov, A. G., Mayorov, V., Malvezzi, L., Marcelli, W., Menn, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, F., Palma, P., Papini, M. P., Pascale, C., Pizzolotto, P., Picozza, M., Pearce, L., Rossetto, M., Ricci, S., Ricciarini, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Stozhkov, Y. u. I., and Yurkin, Y. u. T.
Subjects: Physics, Range (particle radiation), Spectrometer, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, General Physics and Astronomy, Cosmic ray, Electron, Spectral line, law.invention, Nuclear physics, Physics and Astronomy (all), Positron, law, Satellite
Abstract: The PAMELA experiment is being conducted aboard the Russian satellite Resurs-DK 1, which was launched into a near-Earth circumpolar orbit on June 15, 2006. The instrument, which includes a magnetic spectrometer and an electromagnetic calorimeter (16X 0), allows us to measure the fluxes of cosmic-ray electrons and positrons over a wide range of energies from ~100 MeV to hundreds of GeV. This work presents the measurement data collected from July 2006 through January 2010 on the spectra of primary cosmic-ray electrons and positrons. At low energies, this spectrum is in good agreement with a diffusion model that includes reacceleration and damping. At high energies, the measured spectrum is harder than the one predicted. © 2013 Allerton Press, Inc.
Published: 2013

38. The PAMELA experiment: light-nuclei selection with stand-alone detectors

Author: V. Malvezzi, C. Pizzolotto, P. Spillantini, E. Mocchiutti, C. De Santis, S. Y. Krutkov, V. Di Felice, Matteo Martucci, Ugo Giaccari, Juan Wu, N. Zampa, G. A. Bazilevskaya, V. Bonvicini, P. Picozza, Y. I. Stozhkov, S. V. Koldashov, A. G. Mayorov, Mark Pearce, S. B. Ricciarini, Alfonso Monaco, G. Castellini, G. I. Vasilyev, Lorenzo Bonechi, V. V. Malakhov, M. Simon, A. A. Leonov, P. Papini, E. Vannuccini, Riccardo Munini, L. A. Grishantseva, O. Adriani, Ritabrata Sarkar, W. Menn, M. P. De Pascale, Nicola Mori, Giovanna Jerse, A. Bianco, Maria Teresa Ricci, S. A. Voronov, Valerio Formato, A. M. Galper, D. Campana, M. Bongi, N. N. Nikonov, F. Cafagna, N. De Simone, Marco Casolino, E. A. Bogomolov, V. V. Mikhailov, Laura Rossetto, Y. T. Yurkin, S. V. Borisov, A. V. Karelin, Mirko Boezio, R. Carbone, G. C. Barbarino, G. Osteria, Per Carlson, Roberto Bellotti, A. N. Kvashnin, F. Palma, Andrea Vacchi, L. Marcelli, A. Bruno, V. G. Zverev, S. Bottai, Roberta Sparvoli, M. D. Kheymits, G. Zampa, A D Erlykin, R P Kokoulin, A S Lidvansky, L I Meroshnichenko, M I Panasyuk, A D Panov A W Wolfendale, R., Carbone, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, A., Bianco, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, Formato, Valerio, A. M., Galper, U., Giaccari, L., Grishantseva, Jerse, Giovanna, A. V., Karelin, M. D., Kheymit, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, V. V., Mikhailov, Mocchiutti, Emiliano, A., Monaco, N., Mori, Munini, Riccardo, N., Nikonov, G., Osteria, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, Vacchi, Andrea, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, V. G., Zverev, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. h., Bellotti, A. i., Bianco, E., Bogomolov, S. l., M, A. h., Bruno, M. l., De, C. D., Santi, N. D., Simone, V. D., Felice, V. i., Formato, A., Galper, G. i., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, M. p., Martucci, A., Mayorov, V., Mikhailov, E., Mocchiutti, A. h., Monaco, R. i. n, N. k. l, Osteria, Giuseppe, F. l., Palma, P. l., Picozza, C. r., S, S., Ricciarini, R. l., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, S., Voronov, Y., Yurkin, and V., Zverev
Subjects: Physics, History, Analysis strategies, Dark matter, Energy ranges, Light nuclei, Magnetic spectrometers, Measurements of, Precise measurements, Propagation models, Space experiments, Time-of-flight system, COSMIC cancer database, Spectrometer, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galaxy, Cosmic Rays, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Cosmic ray measurement, Positron, Antiproton, law, Nuclear Experiment, Cosmic rays, Detectors, Experiments, Galaxies, Isotope
Abstract: Launched on the 15th of June 2006, the space experiment PAMELA is providing data showing interesting features in cosmic rays that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. PAMELA is also testing cosmic rays acceleration and propagation models through precise measurements of light nuclei and their isotopes. The determination of fluxes and secondary-to-primary ratios is possible for nuclei up to Oxygen in the energy range 200MeV/n – 150 GeV/n. To investigate this important item, PAMELA can use measurements from three main detectors: the magnetic spectrometer, the calorimeter and the Time-of-Flight system. Analysis strategy and performance for nuclei studies using the detectors in stand-alone configuration will be discussed in this work.
Published: 2013

39. Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment

Author: S. V. Koldashov, Marco Ricci, Andrea Vacchi, L. A. Grishantseva, M. F. Runtso, S. A. Voronov, S. Y. Krutkov, M. Simon, N. N. Nikonov, G. Zampa, P. Spillantini, D. Campana, A. A. Leonov, P. Picozza, Mark Pearce, S. B. Ricciarini, N. Zampa, Laura Rossetto, M. Bongi, V. G. Zverev, Marco Casolino, P. Papini, E. Vannuccini, G. Castellini, N. De Simone, Y. T. Yurkin, C. Pizzolotto, V. V. Mikhailov, A. V. Karelin, Mirko Boezio, Roberta Sparvoli, V. Di Felice, W. Malvezzi, R. Carbone, I. A. Danilchenko, Lorenzo Bonechi, E. A. Bogomolov, Sergey Koldobskiy, G. C. Barbarino, V. V. Malakhov, O. Adriani, Giovanna Jerse, M. P. De Pascale, E. Mocchiutti, W. Menn, V. Bonvicini, Roberto Bellotti, L. Consiglio, G. Osteria, S. Bottai, A. M. Galper, Per Carlson, A. N. Kvashnin, Ritabrata Sarkar, F. Cafagna, Nicola Mori, Alfonso Monaco, Yuri Stozhkov, C. De Santis, S. V. Borisov, G. I. Vasilyev, William Gillard, L. Marcelli, G. A. Bazilevskaya, Juan Wu, A. Bruno, A. G. Mayorov, F. Palma, O., Adriani, G. A., Bazilevskaya, Barbarino, Giancarlo, R., Bellotti, M., Boezio, E. A., Bogomolov, V., Bonvicini, M., Bongi, L., Bonechi, S. V., Borisov, S., Bottai, A., Bruno, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, J., Wu, A. M., Galper, L. A., Grishantseva, I. A., Danilchenko, W., Gillard, G., Jerse, G., Zampa, N., Zampa, V. G., Zverev, M., Casolino, D., Campana, R., Carbone, A. V., Karelin, P., Carlson, G., Castellini, F., Cafagna, A. N., Kvashnin, S. V., Koldashov, S. A., Koldobskiy, S. Y., Krutkov, Consiglio, Lucia, A. A., Leonov, A. G., Mayorov, V. V., Malakhov, W., Malvezzi, L., Marcelli, W., Menn, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N. N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, C., Pizzolotto, M. P., Pascale, P., Picozza, M., Pearce, M., Ricci, S., Ricciarini, L., Rossetto, M. F., Runtso, C., Santi, R., Sarkar, M., Simon, N., Simone, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, V., Felice, and Y. T., Yurkin
Subjects: Physics, Antiparticle, Annihilation, Solid-state physics, PAMELA detector, Physics and Astronomy (miscellaneous), Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, Nuclear physics, Antiproton, law, High Energy Physics::Experiment, Nuclear Experiment
Abstract: It is interesting to measure the antiproton galactic component in cosmic rays in order to study the mechanisms by which particles and antiparticles are generated and propagate in the Galaxy and to search for new sources of, e. g., annihilation or decay of dark matter hypothetical particles. The antiproton spectrum and the ratio of the fluxes of primary cosmic ray antiprotons to protons with energies of 60 MeV to 350 GeV found from the data obtained from June 2006 to January 2010 in the PAMELA experiment are presented. The usage of the advanced data processing method based on the data classification mathematical model made it possible to increase statistics and analyze the region of higher energies than in the earlier works. © 2012 Pleiades Publishing, Ltd.
Published: 2013

40. Cosmic ray electron and positron spectra measured with PAMELA

Author: Alfonso Monaco, S. A. Voronov, Maria Teresa Ricci, V. Bonvicini, G. I. Vasiliev, Y. I. Stozhkov, Roberta Sparvoli, E. A. Bogomolov, P. Picozza, Per Carlson, Laura Rossetto, Giovanna Jerse, L. Consiglio, Ritabrata Sarkar, P. Spillantini, S. V. Borisov, V. V. Malakhov, C. Pizzolotto, V. Di Felice, S. Bottai, Mark Pearce, S. B. Ricciarini, V. Malvezzi, V. G. Zverev, Lorenzo Bonechi, R. Carbone, C. De Santis, M. P. De Pascale, S. Yu. Krutkov, G. C. Barbarino, F. Cafagna, L. Marcelli, A. Vacchi, A. G. Mayorov, G. Zampa, D. Campana, N. De Simone, P. Papini, A. Bruno, Marco Casolino, E. Vannuccini, V. V. Mikhailov, G. Castellini, Juan Wu, Y. T. Yurkin, A. V. Karelin, Giuseppe Osteria, F. Palma, M. Simon, A. A. Leonov, M. Bongi, N. Zampa, G. A. Bazilevskaya, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, O. Adriani, W. Menn, S. A. Koldobsky, Mirko Boezio, Nicola Mori, S. V. Koldashov, E. Mocchiutti, V., Mikhailov, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Bellotti, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. m., De, C. D., Santi, N. D., Simone, V. D., Felice, A., Galper, G., Jerse, A., Karelin, S., Koldashov, S., Koldobsky, S. Y., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, A., Mayorov, W., Menn, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, P., Papini, F. m., Palma, M., Pearce, P. m., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. m., Sparvoli, P., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasiliev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, History, Antiparticle, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Polar orbit, Cosmic ray, Astrophysics, Electrons, Positrons, Tungsten, Particle detector, Cosmic ray electrons, Electromagnetic calorimeter, Magnetic spectrometers, Polar orbit, Propagation models, Wide energy range, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), Positron, law, Antimatter, Cosmic rays
Abstract: The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.
Published: 2013

41. Antiprotons of galactic cosmic radiation in the PAMELA experiment

Author: S. Pizzolotto, Ritabrata Sarkar, S. V. Borisov, D. Campana, Marco Casolino, Laura Rozetto, V. Bonvicini, Lorenzo Bonechi, M. F. Runtso, L. Consiglio, M. D. Kheimits, S. A. Voronov, Roberta Sparvoli, William Gillard, N. De Simone, Yu. I. Stozhkov, G. Jerse, N. N. Nikonov, Per Carlson, G. Castellini, O. Adriani, L. Marcelli, A. Vacchi, Mirko Boezio, P. Picozza, S. Bottai, W. Menn, A. Bruno, N. Zampa, Alfonso Monaco, E. A. Bogomolov, M. Bongi, C. De Santis, V. V. Mikhailov, Yu. T. Yurkin, M. Simon, A. G. Mayorov, V. V. Malakhov, V. Di Felice, R. Carbone, I. A. Danilchenko, V. Malvezzi, Sergey Koldobskiy, G. C. Barbarino, A. M. Galper, L. A. Grishantseva, V. G. Zverev, A. A. Leonov, R. Belotti, F. Cafagna, F. Palma, Juan Wu, A. N. Kvashnin, A. V. Karelin, G. A. Bazilevskaia, G. I. Vasilyev, G. Osteria, Nicola Mori, M. P. De Pascale, S. Yu. Krutkov, S. V. Koldashov, Marco Ricci, E. Mocchiutti, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, P. Spilantini, G. Zampa, A. G., Mayorov, O., Adriani, Barbarino, Giancarlo, G. A., Bazilevskaia, R., Belotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S. V., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, I. A., Danilchenko, M. P., Pascale, C., Santi, N., Simone, V., Felice, A. M., Galper, W., Gillard, L. A., Grishantseva, G., Jerse, A. V., Karelin, M. D., Kheimit, S. V., Koldashov, S. A., Koldobskiy, Krutkov, S. Y. u., A. N., Kvashnin, A. A., Leonov, V. V., Malakhov, V., Malvezzi, L., Marcelli, W., Menn, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N. N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, S., Pizzolotto, M., Ricci, S., Ricciarini, L., Rozetto, M. F., Runtso, R., Sarkar, M., Simon, R., Sparvoli, P., Spilantini, Stozhkov, Y. u. I., A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, J., Wu, Yurkin, Y. u. T., G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, Calorimeter (particle physics), PAMELA detector, Physics::Instrumentation and Detectors, Hadron, Dark matter, General Physics and Astronomy, Cosmic ray, Electron, Astrophysics, Flux ratio, law.invention, Nuclear physics, Physics and Astronomy (all), Antiproton, law, High Energy Physics::Experiment
Abstract: A method for antiproton selection against a background of electrons, based on a mathematical model of data classification using variations in interparticle interaction in a calorimeter, and a metho ...
Published: 2013

42. Search for cosmic ray electron-positron anisotropies with the Pamela data

Author: Riccardo Munini, S. Y. Krutkov, A. V. Karelin, G. Osteria, D. Campana, V. Malvezzi, Marco Casolino, A. Bianco, Alfonso Monaco, A. M. Galper, V. G. Zverev, M. P. De Pascale, Mark Pearce, S. B. Ricciarini, S. V. Koldashov, P. Picozza, P. Papini, E. Vannuccini, Roberta Sparvoli, L. Marcelli, A. Bruno, Y. T. Yurkin, Roberto Bellotti, A. N. Kvashnin, Maria Teresa Ricci, P. Spillantini, V. Di Felice, F. Cafagna, V. Bonvicini, Y. I. Stozhkov, Matteo Martucci, Lorenzo Bonechi, Juan Wu, M. Simon, A. A. Leonov, F. Palma, E. Mocchiutti, V. V. Malakhov, Ugo Giaccari, C. De Santis, S. Bottai, M. D. Kheymits, N. Zampa, C. Pizzolotto, G. A. Bazilevskaya, V. V. Mikhailov, N. N. Nikonov, Andrea Vacchi, Mirko Boezio, Giovanna Jerse, A. G. Mayorov, M. Bongi, R. Carbone, G. C. Barbarino, G. Zampa, L. A. Grishantseva, O. Adriani, W. Menn, G. I. Vasilyev, Nicola Mori, S. V. Borisov, S. A. Voronov, E. A. Bogomolov, Laura Rossetto, Ritabrata Sarkar, Valerio Formato, G. Castellini, Per Carlson, N. De Simone, D., Campana, U., Giaccari, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. g., Bellotti, A. i., Bianco, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S. l., M, S., Bottai, A. g., Bruno, F., Cafagna, R., Carbone, P., Carlson, M., Casolino, G., Castellini, M. l., De, C. D., Santi, N. D., Simone, V. D., Felice, V. i., Formato, A., Galper, L., Grishantseva, G. i., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, M. p., Martucci, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. g., Monaco, N., Mori, R. i. n, N. k. l, Osteria, Giuseppe, F. l., Palma, P., Papini, M., Pearce, P. l., Picozza, C. r., S, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. l., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, V., Zverev, A D Erlykin, R P Kokoulin, A S Lidvansky, L I Meroshnichenko, M I Panasyuk, A D Panov and A W Wolfendale, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, A., Bianco, E. A., Bogomolov, S., Borisov, A., Bruno, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, Formato, Valerio, A. M., Galper, Jerse, Giovanna, A. V., Karelin, M. D., Kheymit, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, M., Martucci, A. G., Mayorov, V. V., Mikhailov, Mocchiutti, Emiliano, A., Monaco, Munini, Riccardo, N., Nikonov, G., Osteria, F., Palma, P., Picozza, C., Pizzolotto, S. B., Ricciarini, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, Vacchi, Andrea, S. A., Voronov, Y. T., Yurkin, and V. G., Zverev
Subjects: Physics, History, Angular distribution, Anisotropy, Positron, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Isotropy, Flux, Cosmic ray, Electron, Astrophysics, Cosmic Rays, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Angular scale, Arrival direction, Cosmic ray electrons, Directional Analysis, Strong anisotropy, Nuclear physics, Positron, law, Anisotropy, Directional analysis
Abstract: Using data taken by the Pamela experiment during 5 years of operation we studied the anisotropy in the arrival direction of cosmic ray electrons and positrons with energy above 40 GeV. We report on a study of anisotropy in the e�� flux at different angular scales extending from 30��up to 90��, furthermore a directional analysis has been performed around the Sun direction. The observed distribution of arrival directions is consistent with the isotropic expectation at any angular scale used in this study and no significant evidence of strong anisotropies has been observed, also the analysis around the Sun direction did not show any significant excess.
Published: 2013

43. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment

Author: S. Bottai, C. Pizzolotto, S. V. Borisov, S. A. Voronov, Sergey Koldobskiy, D. Campana, Roberto Bellotti, G. C. Barbarino, S. Y. Krutkov, V. G. Zverev, Marco Casolino, G. Castellini, E. A. Bogomolov, A. N. Kvashnin, E. Mocchiutti, Roberta Sparvoli, Laura Rossetto, V. Di Felice, M. Simon, Mark Pearce, S. B. Ricciarini, N. Zampa, G. A. Bazilevskaya, Alfonso Monaco, P. Picozza, A. A. Leonov, N. N. Nikonov, Ritabrata Sarkar, O. Adriani, P. Spillantini, P. Papini, R. Carbone, Lorenzo Bonechi, V. V. Malakhov, W. Menn, Per Carlson, E. Vannuccini, Giovanna Jerse, V. V. Mikhailov, N. De Simone, M. Bongi, S. V. Koldashov, V. Bonvicini, Y. I. Stozhkov, Maria Teresa Ricci, M. P. De Pascale, Y. T. Yurkin, A. V. Karelin, F. Cafagna, G. Osteria, A. G. Mayorov, L. Consiglio, William Gillard, A. M. Galper, L. Marcelli, A. Vacchi, M. D. Kheymits, A. Bruno, G. Zampa, G. I. Vasilyev, Juan Wu, Nicola Mori, C. De Santis, F. Palma, Mirko Boezio, A., Mayorov, O. b., Adriani, G, Barbarino, Giancarlo, Bazilevskaya, R. g., Bellotti, M., Boezio, E., Bogomolov, L. b., Bonechi, M., Bongi, V., Bonvicini, S. k., L., S., Bottai, A. g., Bruno, F., Cafagna, D., Campana, R. k., Carbone, P., Carlson, M. r., Casolino, G., Castellini, L., Consiglio, M. k., De, C. k., De, N. k., De, V. D., Felice, A., Galper, W., Gillard, G. o., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Koldobskiy, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, W., Menn, V., Mikhailov, E., Mocchiutti, A., Monaco, N. b., Mori, N. j., K., Osteria, Giuseppe, F. k., Palma, P., Papini, M., Pearce, P. k., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R. k., Sparvoli, P. b., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, History, Antiparticle, Experiments, Intelligent systems, Proton, Calorimeter (particle physics), PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Antiproton flux, Classification algorithm, Energy ranges, Galactic cosmic radiations, Monte Carlo Simulation, Training sample, Cosmic ray, Particle detector, Particle identification, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), law, Antiproton, Antimatter, Nuclear Experiment, Cosmic rays
Abstract: The new method based on the classification algorithms was developed to separate antiprotons and electrons in the PAMELA experiment. Training samples based on Monte-Carlo simulation of particle's interactions in the PAMELA imaging Si/W calorimeter were used to achieve rejection factor and to keep high antiproton efficiency. With comparison to the previous publication the number of events was increased 1.5 times. Information collected from the mission start in 2006 till January 2010 was used in the analysis. 2800 events were found in the energy range from 60 MeV to 350 GeV. The flux of antiprotons in galactic cosmic radiation obtained with new method is presented.
Published: 2013

44. Cosmic ray study with the PAMELA experiment

Author: N. De Simone, P. Spillantini, M. D. Kheymits, Nicola Mori, S. Bottai, Alfonso Monaco, Giovanna Jerse, A. G. Mayorov, Roberto Bellotti, G. Zampa, Mark Pearce, S. B. Ricciarini, A. M. Galper, R. Carbone, S. A. Voronov, P. Papini, E. Vannuccini, O. Adriani, D. Campana, W. Menn, G. C. Barbarino, A. N. Kvashnin, V. V. Malakhov, E. A. Bogomolov, A. V. Karelin, L. Marcelli, A. Vacchi, A. Bruno, S. V. Borisov, G. I. Vasilyev, S. Y. Krutkov, C. Pizzolotto, F. Palma, E. Mocchiutti, Laura Rossetto, M. Bongi, N. N. Nikonov, Roberta Sparvoli, Marco Casolino, V. V. Mikhailov, P. Carlson, G. Osteria, Juan Wu, C. De Santis, S. V. Koldashov, V. Di Felice, V. Bonvicini, G. Castellini, Y. I. Stozhkov, L. A. Grishantseva, Mirko Boezio, F. Cafagna, M. P. De Pascale, Y. T. Yurkin, P. Picozza, Ritabrata Sarkar, V. G. Zverev, N. Zampa, G. A. Bazilevskaya, Maria Teresa Ricci, M. Simon, A. A. Leonov, P. b., Picozza, L., Marcelli, O. d., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. i., Bellotti, M., Boezio, E., Bogomolov, M., Bongi, V., Bonvicini, S. b., L, S., Bottai, A. i., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M. b., N, G., Castellini, M. b., De, C. b., De, N. D., Simone, V. D., Felice, A., Galper, L., Grishantseva, G. q., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. i., Monaco, N., Mori, N. b., K, Osteria, Giuseppe, F. b., Palma, P., Papini, M., Pearce, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R. b., Sparvoli, P. d., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Yurkin, J., Wu, G., Zampa, N., Zampa, and V., Zverev
Subjects: History, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Settore FIS/04 - Fisica Nucleare e Subnucleare, Education, law.invention, symbols.namesake, Physics and Astronomy (all), Positron, law, Experiments, Galaxies, Protons, Radiation belts, Solar energy, Cosmic rays, Physics, COSMIC cancer database, PAMELA detector, Astronomy, Computer Science Applications, Dark matter, Data collection, Heliospheres, Measurements of, Particle detection, Radiation environments, Solar activity, Solar modulation, Antiproton, Van Allen radiation belt, Physics::Space Physics, symbols, Heliosphere
Abstract: In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.
Published: 2013

45. The PAMELA space experiment

Author: Yu. T. Yurkin, N. Zampa, G. A. Bazilevskaya, V. Bonvicini, R. Carbone, G. I. Vasilyev, V. Malvezzi, Y. I. Stozhkov, Juan Wu, M. Bongi, Giancarlo Barbarino, V. V. Malakhov, M. Simon, Mark Pearce, S. B. Ricciarini, N. De Simone, V. Di Felice, C. Pizzolotto, F. Cafagna, P. Papini, Piero Spillantini, G. Zampa, E. Vannuccini, S. V. Borisov, Marco Ricci, V. G. Zverev, J. C. Stockton, G. Osteria, A. G. Mayorov, Andrea Vacchi, S. Y. Krutkov, G. Castellini, Nicola Mori, V. V. Mikhailov, L. Consiglio, A. V. Karelin, Roberta Sparvoli, O. Adriani, Alexey Leonov, C. De Santis, F. Palma, E. Mocchiutti, W. Menn, S. Bottai, M. P. De Pascale, P. Picozza, Alfonso Monaco, Per Carlson, Mirko Boezio, S. J. Stochaj, N. N. Nikonov, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, S. A. Voronov, E. A. Bogomolov, Laura Rossetto, Giovanna Jerse, L. A. Grishantseva, Sergey Koldashov, Lorenzo Bonechi, D. Campana, Marco Casolino, Ritabrata Sarkar, William Gillard, L. Marcelli, A. Bruno, W., Menn, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Bellotti, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. D., Pascale, C. D., Santi, N. D., Simone, V. D., Felice, A., Galper, W., Gillard, L., Grishantseva, G., Jerse, A., Karelin, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, A., Mayorov, V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R., Sparvoli, P., Spillantini, S., Stochaj, J., Stockton, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, Atmospheric Science, Antimatter, Cosmic rays, Satellite-borne experiment, Aerospace Engineering, Space and Planetary Science, PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Cosmic ray, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, Nuclear physics, Space experiment, Geophysics, law, General Earth and Planetary Sciences
Abstract: On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus is comprised of a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV to 100's GeV) with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectra in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (anti-helium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. Moreover, PAMELA is investigating phenomena connected with solar and earth physics. After 4 years of operation in flight, PAMELA is now delivering coherent results about spectra and chemical composition of the charged cosmic radiation, allowing scenarios of production and propagation of cosmic rays to be fully established and understood. © 2011 COSPAR. Published by Elsevier Ltd. All rights reserved.
Published: 2013
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46. PAMELA Measurements of Cosmic-ray Proton and Helium Spectra

Author: Alfonso Monaco, P. Papini, Roberto Bellotti, C. Pizzolotto, A. N. Kvashnin, M. P. De Pascale, N. Zampa, G. A. Bazilevskaya, L. Consiglio, G. Castellini, Y. I. Stozhkov, M. Bongi, A. G. Mayorov, L. A. Grishantseva, Y. T. Yurkin, G. Osteria, A. V. Karelin, S. Bottai, O. Adriani, W. Menn, M. Simon, Giovanna Jerse, A. A. Leonov, Nicola Mori, V. Bonvicini, V. G. Zverev, G. Zampa, Mark Pearce, S. V. Borisov, E. Vannuccini, G. C. Barbarino, V. Di Felice, S. V. Koldashov, Marco Ricci, Juan Wu, V. Malvezzi, G. I. Vasilyev, Roberta Sparvoli, N. De Simone, Ritabrata Sarkar, C. De Santis, E. Mocchiutti, Per Carlson, Andrea Vacchi, A. M. Galper, F. Cafagna, William Gillard, L. Marcelli, A. Bruno, V. V. Mikhailov, S. B. Ricciarini, S. A. Voronov, E. A. Bogomolov, Laura Rossetto, V. V. Malakhov, Mirko Boezio, R. Carbone, Lorenzo Bonechi, P. Spillantini, S. Y. Krutkov, F. Palma, D. Campana, Marco Casolino, P. Picozza, N. N. Nikonov, O., Adriani, Barbarino, Giancarlo, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, A. M., Galper, W., Gillard, L., Grishantseva, G., Jerse, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, A. G., Mayorov, W., Menn, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S. A., Voronov, Y. T., Yurkin, J., Wu, G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Multidisciplinary, Proton, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, chemistry.chemical_element, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy, Spectral line, law.invention, Settore FIS/04 - Fisica Nucleare e Subnucleare, Supernova, chemistry, law, Antimatter, Astrophysics - High Energy Astrophysical Phenomena, Helium, Astrophysics::Galaxy Astrophysics
Abstract: Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in the Galaxy. We report precision measurements of the proton and helium spectra in the rigidity range 1 GV-1.2 TV performed by the satellite-borne experiment PAMELA. We find that the spectral shapes of these two species are different and cannot be well described by a single power law. These data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy. More complex processes of acceleration and propagation of cosmic rays are required to explain the spectral structures observed in our data., Comment: 13 pages, 4 figures, link to SOM (with tables) in the references. This manuscript has been accepted for publication in Science. This version has not undergone final editing. Please refer to the complete version of record at http://www.sciencemag.org/ [www.sciencemag.org]
Published: 2011
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47. Results from PAMELA

Author: Alfonso Monaco, A. V. Karelin, William Gillard, Mirko Boezio, L. Marcelli, D. Campana, A. Vacchi, Per Carlson, Marco Casolino, N. N. Nikonov, A. Bruno, G. Osteria, V. V. Malakhov, V. G. Zverev, M. F. Runtso, S. V. Borisov, R. Carbone, Lorenzo Bonechi, F. Cafagna, O. Adriani, L. A. Grishantseva, S. A. Voronov, W. Menn, Roberto Bellotti, G. Zampa, A. M. Galper, N. Zampa, G. A. Bazilevskaya, A. N. Kvashnin, E. A. Bogomolov, Roberta Sparvoli, S. Bottai, Mark Pearce, S. B. Ricciarini, P. Papini, Laura Rossetto, E. Vannuccini, M. Bongi, M. P. De Pascale, G. C. Barbarino, L. Consiglio, F. Palma, G. Castellini, C. Pizzolotto, Giovanna Jerse, Y. T. Yurkin, G. I. Vasilyev, V. V. Mikhailov, C. De Santis, N. De Simone, O. Maksumov, Ritabrata Sarkar, Juan Wu, Nicola Mori, A. G. Mayorov, M. Simon, A. A. Leonov, Maria Teresa Ricci, S. Y. Krutkov, P. Picozza, P. Spillantini, V. Malvezzi, E. Mocchiutti, S. V. Koldashov, V. Di Felice, V. Bonvicini, Y. I. Stozhkov, E., Mocchiutti, O., Adriani, Barbarino, Giancarlo, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, L., Consiglio, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, A. M., Galper, W., Gillard, L., Grishantseva, G., Jerse, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, O., Maksumov, V., Malakhov, V., Malvezzi, L., Marcelli, A. G., Mayorov, W., Menn, A., Monaco, V. V., Mikhailov, N., Mori, N. N., Nikonov, G., Osteria, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, M., Runtso, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, Nuclear and High Energy Physics, genetic structures, Spectrometer, Calorimeter (particle physics), PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Atomic and Molecular Physics, and Optics, law.invention, Settore FIS/04 - Fisica Nucleare e Subnucleare, Nuclear physics, Low earth orbit, law, Magnet, Atomic and Molecular Physics, Physics::Space Physics, Satellite, Astrophysics::Earth and Planetary Astrophysics, and Optics
Abstract: The PAMELA satellite experiment was launched into low earth orbit on June 15(th) 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter al ...
Published: 2011

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

Author: M. Simon, O. Adriani, A. A. Leonov, L. Consiglio, Mirko Boezio, W. Menn, N. Zampa, G. A. Bazilevskaya, V. G. Zverev, L. A. Grishantseva, A. V. Karelin, S. Bottai, P. Spillantini, Juan Wu, V. Di Felice, Alfonso Monaco, M. D. Kheymits, S. A. Voronov, V. Bonvicini, E. Mocchiutti, Roberta Sparvoli, M. Bongi, Y. I. Stozhkov, E. A. Bogomolov, C. Pizzolotto, D. Campana, Laura Rossetto, S. V. Koldashov, Mark Pearce, S. B. Ricciarini, Giovanna Jerse, Marco Ricci, F. Cafagna, A. M. Galper, F. Palma, G. I. Vasilyev, Ritabrata Sarkar, A. G. Mayorov, P. Papini, E. Vannuccini, G. Zampa, S. Y. Krutkov, Marco Casolino, V. V. Mikhailov, P. Carlson, G. Osteria, N. De Simone, M. P. De Pascale, G. C. Barbarino, P. Picozza, S. V. Borisov, Nicola Mori, William Gillard, C. De Santis, N. N. Nikonov, G. Castellini, R. Carbone, V. V. Malakhov, L. Marcelli, A. Vacchi, Y. T. Yurkin, A. Bruno, Roberto Bellotti, A. N. Kvashnin, M., Boezio, A., Bruno, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Bellotti, E., Bogomolov, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. d., Pascale, C. d., Santi, N. d., Simone, V. D., Felice, A., Galper, W., Gillard, L., Grishantseva, G., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Yurkin, J., Wu, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, Particle physics, Antiparticle, Antimatter, Nuclear and High Energy Physics, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Astronomy, Cosmic rays, Atomic and Molecular Physics, and Optics, Condensed Matter Physics, Physical and Theoretical Chemistry, Cosmic ray, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, Pulsar, law, Antiproton, Atomic and Molecular Physics, and Optics
Abstract: The PAMELA satellite-borne experiment has presented new results on cosmic-ray antiparticles that can be interpreted in terms of DM annihilation or pulsar contribution. The instrument was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectrum in order to search for exotic sources. PAMELA is also searching for primordial antinuclei (anti-helium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. This talk illustrates the most recent scientific results obtained by the PAMELA experiment.
Published: 2011

49. Measuring fluxes of the protons and helium nuclei of high-energy cosmic rays

Author: R. Carbone, M. F. Runtso, O. Adriani, C. Pizzolotto, S. A. Voronov, Sergey Koldobskiy, W. Menn, A. G. Mayorov, G. C. Barbarino, P. Spillantini, E. A. Bogomolov, Mark Pearce, S. B. Ricciarini, S. V. Borisov, P. Papini, F. Cafagna, V. Malvezzi, M. Bongi, Laura Rossetto, E. Vannuccini, Yu. T. Yurkin, S. Bottai, Andrea Vacchi, N. De Simone, Juan Wu, M. P. De Pascale, S. Yu. Krutkov, Alfonso Monaco, A. V. Karelin, Nicola Mori, V. Bonvicini, V. V. Mikhailov, P. Carlson, Lorenzo Bonechi, G. Castellini, Petter Hofverberg, V. G. Zverev, Mirko Boezio, G. I. Vasilyev, P. Picozza, I. A. Danilchenko, Yu. I. Stozhkov, Giovanna Jerse, Roberto Bellotti, L. Marcelli, M. Simon, A. A. Leonov, D. Campana, A. N. Kvashnin, V. Di Felice, Marco Casolino, N. N. Nikonov, Roberta Sparvoli, E. Mocchiutti, S. V. Koldashov, Marco Ricci, L. A. Grishantseva, C. De Santis, Gianluigi Zampa, Giuseppe Osteria, N. Zampa, G. A. Bazilevskaya, V. V. Malakhov, A. M. Galper, A. Bruno, and L. Consiglio
Subjects: Physics, Calorimeter (particle physics), PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Nuclear Theory, General Physics and Astronomy, chemistry.chemical_element, Cosmic ray, Alpha particle, Spectral line, law.invention, Nuclear physics, Physics and Astronomy (all), chemistry, law, Ultra-high-energy cosmic ray, Nuclear Experiment, Helium
Abstract: Techniques for measuring helium nuclei and proton energy spectra in circumterrestrial space were developed on the basis of simulated data and data from the position-sensitive silicon-tungsten calorimeter in the PAMELA satellite experiment. The thickness of the calorimeter is 0.6 nuclear interaction lengths. In this work, the experimental results for the measured energy spectra of the protons and helium nuclei of cosmic rays with energies above 50 GeV are presented. © 2011 Allerton Press, Inc.
Published: 2011
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50. Study of deuteron spectra under radiation belt with PAMELA instrument

Author: S. A. Voronov, L. Marcelli, A. Vacchi, A. Bruno, Valerio Formato, Roberta Sparvoli, E. A. Bogomolov, P. Spillantini, S. Y. Krutkov, P. Picozza, A. A. Kvashnin, Mirko Boezio, N. De Simone, Nicola Mori, D. Campana, G. Castellini, A. G. Mayorov, N. Zampa, G. A. Bazilevskaya, Alexey Leonov, Yu. T. Yurkin, C. De Santis, Per Carlson, Marco Casolino, C. De Donato, Ritabrata Sarkar, S. Bottai, O. Adriani, V. Di Felice, F. Palma, Roberto Bellotti, Riccardo Munini, W. Menn, A. M. Galper, Sergey Koldashov, G. Zampa, Mark Pearce, S. B. Ricciarini, Beatrice Panico, A. N. Kvashnin, Maria Teresa Ricci, Sergey Koldobskiy, M. Bongi, V. V. Malakhov, G. C. Barbarino, G. I. Vasilyev, Valentina Scotti, P. Papini, E. Vannuccini, Alfonso Monaco, M. Simon, A. V. Karelin, G. Osteria, M. Merge, Matteo Martucci, F. Cafagna, V. V. Mikhailov, V. Bonvicini, Y. I. Stozhkov, E. Mocchiutti, Koldobskiy, S. A, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Krutkov, S. Y, Kvashnin, A. A, Kvashnin, A. N, Leonov, A. A, Malakhov, V. V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Merge’, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, Zampa, N., S., Koldobskiy, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. A., Kvashnin, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, and N., Zampa
Subjects: deuteron, History, Proton, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Cosmology, Deuterium, Geomagnetism, Radiation belts, Solar radiation Cosmic-ray particles, Energy ranges, High-precision, Measurements of, Proton flux, Wide energy range, Cosmic ray, Astrophysics, radiation belt, Radiation, Spectral line, Education, law.invention, Nuclear physics, Physics and Astronomy (all), symbols.namesake, cosmic rays, PAMELA, law, PAMELA, cosmic rays, deuteron, radiation belt, Nuclear Experiment, Settore FIS/01, Physics, PAMELA detector, Albedo, Computer Science Applications, Van Allen radiation belt, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, symbols, Astrophysics::Earth and Planetary Astrophysics
Abstract: This paper presents the results of measurements of proton and deuteron fluxes of albedo radiation in the Earth vicinity, obtained in the PAMELA experiment. PAMELA is an international experiment meant to study cosmic rays. PAMELA is carried out on board the satellite Resurs-DK1. High-precision equipment of the experiment allows registration and identification of cosmic ray particles of different varieties in a wide energy range. The albedo deuteron spectrum and albedo deuteron-to-proton fluxes ratio in the energy range 70 – 600 MeV/nucleon at altitude of 350 – 600 km for different geomagnetic latitudes is presented.
Published: 2015

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