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1. Gamma-Ray Burst Observations by the High-Energy Particle Detector on board the China Seismo-Electromagnetic Satellite between 2019 and 2021.

Author

Palma, F., Martucci, M., Neubüser, C., Sotgiu, A., Follega, F. M., Ubertini, P., Bazzano, A., Rodi, J. C., Ammendola, R., Badoni, D., Bartocci, S., Battiston, R., Beolè, S., Bertello, I., Burger, W. J., Campana, D., Cicone, A., Cipollone, P., Coli, S., and Conti, L.

Subjects
PARTICLE detectors, PARTICLE board, GAMMA ray bursts, PHOTON flux, MONTE Carlo method, COSMIC rays
Abstract

In this paper we report the detection of five strong gamma-ray bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satellite, operational since 2018 on a Sun-synchronous polar orbit at a ∼507 km altitude and 97° inclination. HEPD-01 was designed to detect high-energy electrons in the energy range 3–100 MeV, protons in the range 30–300 MeV, and light nuclei in the range 30–300 MeV n−1. Nonetheless, Monte Carlo simulations have shown HEPD-01 is sensitive to gamma-ray photons in the energy range 300 keV–50 MeV, even if with a moderate effective area above ∼5 MeV. A dedicated time correlation analysis between GRBs reported in literature and signals from a set of HEPD-01 trigger configuration masks has confirmed the anticipated detector sensitivity to high-energy photons. A comparison between the simultaneous time profiles of HEPD-01 electron fluxes and photons from GRB190114C, GRB190305A, GRB190928A, GRB200826B, and GRB211211A has shown a remarkable similarity, in spite of the different energy ranges. The high-energy response, with peak sensitivity at about 2 MeV, and moderate effective area of the detector in the actual flight configuration explain why these five GRBs, characterized by a fluence above ∼3 × 10−5 erg cm−2 in the energy interval 300 keV–50 MeV, have been detected. [ABSTRACT FROM AUTHOR]

Published
2024
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4. Cosmic Rays Investigation by the PAMELA experiment

Author

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

Published
2020
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5. Time dependence of the proton and helium flux measured by PAMELA

Author

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

Published
2020
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6. Cosmic ray electrons and positrons over decade with the PAMELA experiment

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Kleymenova, S O, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2019
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7. Eastâ€"West Proton Flux Anisotropy Observed with the PAMELA Mission.

Author

Bruno, A., Martucci, M., Cafagna, F. S., Sparvoli, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Campana, D., Carlson, P., Casolino, M., Castellini, G., Santis, C. De, Galper, A. M., Koldashov, S. V., and Koldobskiy, S.

Subjects
ANISOTROPY, PROTONS, ASTROPHYSICS, COSMIC rays, ANTIMATTER
Abstract

We present a study of the eastâ€"west anisotropy of trapped-proton fluxes in low-Earth orbit based on the measurements of the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) experiment. The differential intensities of eastward- and westward-traveling protons detected in the South Atlantic Anomaly region were estimated as a function of equatorial pitch angle and drift shell, for six energy bins between 80 MeV and 2 GeV. We found that, as a consequence of the strong atmospheric gradient coupled with the large gyroradius in this energy range, the intensities of eastward fluxes exceed those of westward fluxes by a factor of ∼10â€"20. However, the reported directional asymmetry also depends on the sign of the local flux gradient, resulting in more intense westward fluxes beyond the radial distances where the inner belt peaks. PAMELA observations can be used to improve the description of the near-Earth radiation environment at lowest altitudes and highest trapping energies, where current theoretical and empirical models are affected by the largest uncertainties. [ABSTRACT FROM AUTHOR]

Published
2021
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9. Galactic Cosmic-Ray Hydrogen Spectra in the 40–250 MeV Range Measured by the High-energy Particle Detector (HEPD) on board the CSES-01 Satellite between 2018 and 2020.

Author

Bartocci, S., Battiston, R., Burger, W. J., Campana, D., Carfora, L., Castellini, G., Conti, L., Contin, A., De Donato, C., De Persio, F., De Santis, C., Diego, P., Follega, F. M., Iuppa, R., Lazzizzera, I., Marcelli, N., Martucci, M., Masciantonio, G., Mergé, M., and Osteria, G.

Subjects
PARTICLE detectors, HYDROGEN as fuel, HYDROGEN, ARTIFICIAL satellites
Abstract

The High-energy Particle Detector (HEPD) on board the China Seismo-Electromagnetic Satellite (CSES-01)—launched on 2018 February 2—is a light and compact payload suitable for measuring electrons (3–100 MeV), protons (30–250 MeV), and light nuclei (up to a few hundreds of MeV). The Sun-synchronous orbit and large acceptance allow HEPD to measure cosmic-ray particles near the ±65° latitude limit for a fair amount of time per day. In this work, three semiannual galactic hydrogen energy spectra between ∼40 and 250 MeV are presented, including a comparison with theoretical spectra from HelMod, a 2D Monte Carlo model developed to simulate the solar modulation of cosmic rays throughout the heliosphere. To our knowledge, these are the first hydrogen energy spectra below 250 MeV measured at 1 au between 2018 and 2020. [ABSTRACT FROM AUTHOR]

Published
2020
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10. Time Dependence of the Flux of Helium Nuclei in Cosmic Rays Measured by the PAMELA Experiment between 2006 July and 2009 December.

Author

Marcelli, N., Boezio, M., Lenni, A., Menn, W., Munini, R., Aslam, O. P. M., Bisschoff, D., Ngobeni, M. D., Potgieter, M. S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., and Carlson, P.

Subjects
HELIUM, COSMIC rays, THRESHOLD energy, HELIOSPHERE, THREE-dimensional modeling, MEASURING instruments
Abstract

Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. The PAMELA experiment, with its long flight duration (2006 June 15–2016 January 23) and the low energy threshold (80 MeV/n) is an ideal detector for cosmic-ray solar modulation studies. In this paper, the helium nuclei spectra measured by the PAMELA instrument from 2006 July to 2009 December over a Carrington rotation time basis are presented. A state-of-the-art three-dimensional model for cosmic-ray propagation inside the heliosphere was used to interpret the time-dependent measured fluxes. Proton-to-helium flux ratio time profiles at various rigidities are also presented in order to study any features that could result from the different masses and local interstellar spectra shapes. [ABSTRACT FROM AUTHOR]

Published
2020
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11. First observations of speed of light tracks by a fluorescence detector looking down on the atmosphere

Author

Abdellaoui, G., primary, Abe, S., additional, Jr., J.H. Adams, additional, Ahriche, A., additional, Allard, D., additional, Allen, L., additional, Alonso, G., additional, Anchordoqui, L., additional, Anzalone, A., additional, Arai, Y., additional, Asano, K., additional, Attallah, R., additional, Attoui, H., additional, Pernas, M. Ave, additional, Bacholle, S., additional, Bakiri, M., additional, Baragatti, P., additional, Barrillon, P., additional, Bartocci, S., additional, Bayer, J., additional, Beldjilali, B., additional, Belenguer, T., additional, Belkhalfa, N., additional, Bellotti, R., additional, Belov, A., additional, Belov, K., additional, Benmessai, K., additional, Bertaina, M., additional, Biermann, P.L., additional, Biktemerova, S., additional, Bisconti, F., additional, Blanc, N., additional, Błȩcki, J., additional, Blin-Bondil, S., additional, Bobik, P., additional, Bogomilov, M., additional, Bozzo, E., additional, Bruno, A., additional, Caballero, K.S., additional, Cafagna, F., additional, Campana, D., additional, Capdevielle, J-N., additional, Capel, F., additional, Caramete, A., additional, Caramete, L., additional, Carlson, P., additional, Caruso, R., additional, Casolino, M., additional, Cassardo, C., additional, Castellina, A., additional, Catalano, C., additional, Catalano, O., additional, Cellino, A., additional, Chikawa, M., additional, Chiritoi, G., additional, Christl, M.J., additional, Connaughton, V., additional, Conti, L., additional, Cordero, G., additional, Cotto, G., additional, Crawford, H.J., additional, Cremonini, R., additional, Csorna, S., additional, Cummings, A., additional, Dagoret-Campagne, S., additional, Donato, C. De, additional, Taille, C. de la, additional, Santis, C. De, additional, Peral, L. del, additional, Martino, M. Di, additional, Damian, A. Diaz, additional, Djemil, T., additional, Dutan, I., additional, Ebersoldt, A., additional, Ebisuzaki, T., additional, Engel, R., additional, Eser, J., additional, Fenu, F., additional, Fernández-González, S., additional, Fernández-Soriano, J., additional, Ferrarese, S., additional, Flamini, M., additional, Fornaro, C., additional, Fouka, M., additional, Franceschi, A., additional, Franchini, S., additional, Fuglesang, C., additional, Fujii, T., additional, Fujimoto, J., additional, Fukushima, M., additional, Galeotti, P., additional, García-Ortega, E., additional, Garipov, G., additional, Gascón, E., additional, Genci, J., additional, Giraudo, G., additional, Alvarado, C. González, additional, Gorodetzky, P., additional, Greg, R., additional, Guarino, F., additional, Guzmán, A., additional, Hachisu, Y., additional, Haiduc, M., additional, Harlov, B., additional, Haungs, A., additional, Carretero, J. Hernández, additional, Cruz, W. Hidber, additional, Ikeda, D., additional, Inoue, N., additional, Inoue, S., additional, Isgrò, F., additional, Itow, Y., additional, Jammer, T., additional, Jeong, S., additional, Joven, E., additional, Judd, E.G., additional, Jung, A., additional, Jochum, J., additional, Kajino, F., additional, Kajino, T., additional, Kalli, S., additional, Kaneko, I., additional, Karadzhov, Y., additional, Karczmarczyk, J., additional, Katahira, K., additional, Kawai, K., additional, Kawasaki, Y., additional, Kedadra, A., additional, Khales, H., additional, Khrenov, B.A., additional, Kim, Jeong-Sook, additional, Kim, Soon-Wook, additional, Kleifges, M., additional, Klimov, P.A., additional, Kolev, D., additional, Krantz, H., additional, Kreykenbohm, I., additional, Kudela, K., additional, Kurihara, Y., additional, Kusenko, A., additional, Kuznetsov, E., additional, Barbera, A. La, additional, Lachaud, C., additional, Lahmar, H., additional, Lakhdari, F., additional, Larson, R., additional, Larsson, O., additional, Lee, J., additional, Licandro, J., additional, Campano, L. López, additional, Maccarone, M.C., additional, Mackovjak, S., additional, Mahdi, M., additional, Maravilla, D., additional, Marcelli, L., additional, Marcos, J.L., additional, Marini, A., additional, Marszał, W., additional, Martens, K., additional, Martín, Y., additional, Martinez, O., additional, Martucci, M., additional, Masciantonio, G., additional, Mase, K., additional, Mastafa, M., additional, Matev, R., additional, Matthews, J.N., additional, Mebarki, N., additional, Medina-Tanco, G., additional, Mendoza, M.A., additional, Menshikov, A., additional, Merino, A., additional, Meseguer, J., additional, Meyer, S.S., additional, Mimouni, J., additional, Miyamoto, H., additional, Mizumoto, Y., additional, Monaco, A., additional, Ríos, J.A. Morales de los, additional, Moretto, C., additional, Nagataki, S., additional, Naitamor, S., additional, Napolitano, T., additional, Naslund, W., additional, Nava, R., additional, Neronov, A., additional, Nomoto, K., additional, Nonaka, T., additional, Ogawa, T., additional, Ogio, S., additional, Ohmori, H., additional, Olinto, A.V., additional, Orleański, P., additional, Osteria, G., additional, Pagliaro, A., additional, Painter, W., additional, Panasyuk, M.I., additional, Panico, B., additional, Pasqualino, G., additional, Parizot, E., additional, Park, I.H., additional, Pastircak, B., additional, Patzak, T., additional, Paul, T., additional, Pérez-Grande, I., additional, Perfetto, F., additional, Peter, T., additional, Picozza, P., additional, Pindado, S., additional, Piotrowski, L.W., additional, Piraino, S., additional, Placidi, L., additional, Plebaniak, Z., additional, Pliego, S., additional, Pollini, A., additional, Polonski, Z., additional, Popescu, E.M., additional, Prat, P., additional, Prévôt, G., additional, Prieto, H., additional, Puehlhofer, G., additional, Putis, M., additional, Rabanal, J., additional, Radu, A.A., additional, Reyes, M., additional, Rezazadeh, M., additional, Ricci, M., additional, Frías, M.D. Rodríguez, additional, Rodencal, M., additional, Ronga, F., additional, Roudil, G., additional, Rusinov, I., additional, Rybczyński, M., additional, Sabau, M.D., additional, Cano, G. Sáez, additional, Sagawa, H., additional, Sahnoune, Z., additional, Saito, A., additional, Sakaki, N., additional, Salazar, H., additional, Balanzar, J.C. Sanchez, additional, Sánchez, J.L., additional, Santangelo, A., additional, Sanz-Andrés, A., additional, Palomino, M. Sanz, additional, Saprykin, O., additional, Sarazin, F., additional, Sato, M., additional, Schanz, T., additional, Schieler, H., additional, Scotti, V., additional, Selmane, S., additional, Semikoz, D., additional, Serra, M., additional, Sharakin, S., additional, Shimizu, H.M., additional, Shinozaki, K., additional, Shirahama, T., additional, Spataro, B., additional, Stan, I., additional, Sugiyama, T., additional, Supanitsky, D., additional, Suzuki, M., additional, Szabelska, B., additional, Szabelski, J., additional, Tajima, N., additional, Tajima, T., additional, Takahashi, Y., additional, Takami, H., additional, Takeda, M., additional, Takizawa, Y., additional, Talai, M.C., additional, Tenzer, C., additional, Thomas, S.B., additional, Tibolla, O., additional, Tkachev, L., additional, Tokuno, H., additional, Tomida, T., additional, Tone, N., additional, Toscano, S., additional, Traïche, M., additional, Tsenov, R., additional, Tsunesada, Y., additional, Tsuno, K., additional, Tubbs, J., additional, Turriziani, S., additional, Uchihori, Y., additional, Vaduvescu, O., additional, Valdés-Galicia, J.F., additional, Vallania, P., additional, Vankova, G., additional, Vigorito, C., additional, Villaseñor, L., additional, Vlcek, B., additional, Ballmoos, P. von, additional, Vrabel, M., additional, Wada, S., additional, Watanabe, J., additional, Jr., J. Watts, additional, Weber, M., additional, Muñoz, R. Weigand, additional, Weindl, A., additional, Wiencke, L., additional, Wille, M., additional, Wilms, J., additional, Włodarczyk, Z., additional, Yamamoto, T., additional, Yang, J., additional, Yano, H., additional, Yashin, I.V., additional, Yonetoku, D., additional, Yoshida, S., additional, Young, R., additional, Zgura, I.S, additional, Zotov, M.Yu., additional, and Marchi, A. Zuccaro, additional

Published
2018
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12. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C., additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V., additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2017
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13. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

Author

Mayorov, A G, primary, Adriani, O, additional, Aleksandrin, S Y, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Kvashnin, A A, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, M A, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Naumov, P Yu, additional, Osteria, G, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Rodenko, S A, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2017
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14. The PAMELA experiment: a decade of Cosmic Ray Physics in space

Author

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

Published
2017
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15. The measurement of the dipole anisotropy of protons and helium cosmic rays with the PAMELA experiment

Author

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

Published
2016
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16. H, He, Li and Be Isotopes in the PAMELA-Experiment

Author

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

Published
2016
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17. The May 17, 2012 solar event: back-tracing analysis and flux reconstruction with PAMELA

Author

Bruno, A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A., additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bravar, U, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Christian, E C, additional, De Donato, C, additional, de Nolfo, G A, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Lee, M, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Ryan, J M, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stochaj, S, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2016
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18. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment

Author

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

Published
2016
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19. Trapped positrons observed by PAMELA experiment

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Santis, C, additional, De Simone, N, additional, Felice, V. Di, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2016
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20. Study of deuteron spectra under radiation belt with PAMELA instrument

Author

Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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21. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

Author

Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V., additional, Galper, A M, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M., additional, Menn, W, additional, Merge, M., additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R., additional, Osteria, G, additional, Palma, F, additional, Panico, B., additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V., additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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22. PAMELA measurements of the boron and carbon spectra

Author

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

Published
2015
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23. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

Author

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

Published
2015
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24. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data

Author

Malakhov, V V, primary, Koldashov, S V, additional, Mayorov, A G, additional, Mayorova, M A, additional, Mikhailov, V V, additional, Aleksandrin, S Yu, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Krutkov, S Yu, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Marcelli, L, additional, Martucci, M, additional, Menn, W, additional, Merge, M, additional, Mocchuuitti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacci, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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25. Study of solar modulation of galactic cosmic rays with the PAMELA and ARINA spectrometers in 2006-2012

Author

Bzheumikhova, M A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, Pascale, M P De, additional, Santis, C De, additional, Simone, N De, additional, Felice, V Di, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Losev, D S, additional, Malakhov, V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Sidorov, A V, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Ulitin, A A, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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26. The PAMELA experiment: light-nuclei selection with stand-alone detectors

Author

Carbone, R, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Giaccari, U, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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27. A search algorithm for finding Cosmic-Ray anisotropy with the PAMELA calorimeter

Author

Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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28. Cosmic ray electron and positron spectra measured with PAMELA

Author

Mikhailov, Vladimir, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Jerse, G, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Yu Krutkov, S, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Malvezzi, V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Yu T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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29. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment

Author

Mayorov, A G, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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30. Cosmic Ray Study with the PAMELA Experiment

Author

Picozza, P, primary, Marcelli, L, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Wu, J, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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31. Search for cosmic ray electron-positron anisotropies with the Pamela data

Author

Campana, D, primary, Giaccari, U, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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32. Galactic deuteron spectrum measured in PAMELA experiment

Author

Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, Y V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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34. PAMELA and indirect dark matter searches

Author

Boezio, M, primary, Pearce, M, additional, Picozza, P, additional, Sparvoli, R, additional, Spillantini, P, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, Santis, C De, additional, Simone, N De, additional, Felice, V Di, additional, Galper, A M, additional, Grishantseva, L, additional, Gillard, W, additional, Hofverberg, P, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malvezzi, V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Papini, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2009
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35. Performance of the PAMELA Si-W imaging calorimeter in space

Author

Bonvicini, V, primary, Boezio, M, additional, Mocchiutti, E, additional, Vacchi, A, additional, Zampa, G, additional, Zampa, N, additional, Bellotti, R, additional, Bruno, A, additional, Cafagna, F, additional, Adriani, O, additional, Bonechi, L, additional, Bongi, M, additional, Bottai, S, additional, Fedele, D, additional, Papini, P, additional, Ricciarini, S, additional, Spillantini, P, additional, Taddei, E, additional, Vannuccini, E, additional, Castellini, G, additional, Ricci, M, additional, Basilevskaja, G A, additional, Kvashnin, A N, additional, Stozhkov, Y I, additional, Galper, A M, additional, Grishantseva, L, additional, Koldashov, S V, additional, Leonov, A, additional, Mikhailov, V V, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zverev, V G, additional, Barbarino, G, additional, Rosa, G De, additional, Osteria, G, additional, Campana, D, additional, Casolino, M, additional, Pascale, M P De, additional, Malvezzi, V, additional, Marcelli, L, additional, Minori, M, additional, Picozza, P, additional, Sparvoli, R, additional, Bogomolov, E A, additional, Krutkov, S Y, additional, Vasilyev, G, additional, Menn, W, additional, Simon, M, additional, Carlson, P, additional, Hofverberg, P, additional, Orsi, S, additional, and Pearce, M, additional

Published
2009
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37. MEASUREMENT OF THE ISOTOPIC COMPOSITION OF HYDROGEN AND HELIUM NUCLEI IN COSMIC RAYS WITH THE PAMELA EXPERIMENT.

Author

ADRIANI, O., BARBARINO, G. C., BAZILEVSKAYA, G. A., BELLOTTI, R., BOEZIO, M., BOGOMOLOV, E. A., BONGI, M., BONVICINI, V., BORISOV, S., BOTTAI, S., BRUNO, A., CAFAGNA, F., CAMPANA, D., CARBONE, R., CARLSON, P., CASOLINO, M., CASTELLINI, G., DANILCHENKO, I. A., DE PASCALE, M. P., and DE SANTIS, C.

Subjects
HYDROGEN isotopes, HELIUM isotopes, GALACTIC nuclei, COSMIC rays, EXPERIMENTS
Abstract

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

Published
2013
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38. TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUM.

Author

ADRIANI, O., BARBARINO, G. C., BAZILEVSKAYA, G. A., BELLOTTI, R., BOEZIO, M., BOGOMOLOV, E. A., BONGI, M., BONVICINI, V., BORISOV, S., BOTTAI, S., BRUNO, A., CAFAGNA, F., CAMPANA, D., CARBONE, R., CARLSON, P., CASOLINO, M., CASTELLINI, G., DE PASCALE, M. P., DE SANTIS, C., and DE SIMONE, N.

Subjects
COSMIC rays, EARTH (Planet), SOLAR magnetic fields, HELIOSPHERE, SUN, PROTONS, SOLAR wind
Abstract

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

Published
2013
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40. OBSERVATIONS OF THE 2006 December 13 AND 14 SOLAR PARTICLE EVENTS IN THE 80 MeV n-1-3 GeV n-1 RANGE FROM SPACE WITH THE PAMELA DETECTOR.

Author

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

Subjects
SOLAR energetic particles, SPACE spectrometry, SOLAR energy, PROTON spectra, HELIUM spectra
Abstract

We present the space spectrometer PAMELA observations of proton and helium fluxes during the 2006 December 13 and 14 solar particle events. This is the first direct measurement of the solar energetic particles in space with a single instrument in the energy range from ~80 MeV n-1 up to ~3 GeV n-1. For the December 13 event, measured energy spectra of solar protons and helium are compared with results obtained by neutron monitors and other detectors. Our measurements show a spectral behavior different from those derived from the neutron monitor network. No satisfactory analytical fitting was found for the energy spectra. During the first hours of the December 13 event, solar energetic particles spectra were close to the exponential form, demonstrating rather significant temporal evolution. Solar He with energy up to 1 GeV n-1 was recorded on December 13. For the December 14 event, energy of solar protons reached 600 MeV, whereas the maximum energy of He was below 100 MeV n-1. The spectra were slightly bent in the lower energy range and preserved their form during the second event. Differences in the particle flux appearance and temporal evolution of these two events may argue for special conditions leading to the acceleration of solar particles up to relativistic energies. [ABSTRACT FROM AUTHOR]

Published
2011
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42. MEASUREMENT OF BORON AND CARBON FLUXES IN COSMIC RAYS WITH THE PAMELA EXPERIMENT.

Author

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., Donato, C. De, Santis, C. De, and Simone, N. De

Subjects
COSMIC rays, GALAXIES, BORON, FLUX (Energy), CARBON, KINETIC energy
Abstract

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

Published
2014
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44. Neutrino Astronomy with the MACRO Detector.

Author

Ambrosio, M., Antolini, R., Auriemma, G., Bakari, D., Baldini, A., Barbarino, G. C., Barish, B. C., Battistoni, G., Bellotti, R., Bemporad, C., Bernardini, P., Bilokon, H., Bisi, V., Bloise, C., Bower, C., Brigida, M., Bussino, S., Cafagna, F., Calicchio, M., and Campana, D.

Published
2001
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45. 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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