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442 results on '"Panico, B."'

151. 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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152. Reentrant albedo proton fluxes measured by 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., Carlson, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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.
Abstract: We present a precise measurement of downward going albedo proton fluxes for kinetic energy above similar to 70 MeV performed by the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) experiment at an altitude between 350 and 610 km. On the basis of a trajectory tracing simulation, the analyzed protons were classified into quasi-trapped, concentrating in the magnetic equatorial region, and untrapped spreading over all latitudes, including both short-lived (precipitating) and long-lived (pseudotrapped) components. In addition, features of the penumbra region around the geomagnetic cutoff were investigated in detail. PAMELA results significantly improve the characterization of the high-energy albedo proton populations at low-Earth orbits., QC 20150811
Published: 2015
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153. Force-field parameterization of the galactic cosmic ray spectrum : Validation for Forbush decreases

Author: Usoskin, I. G., Kovaltsov, G. 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, Per, Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Format, 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., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilye, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G., Usoskin, I. G., Kovaltsov, G. 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, Per, Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Format, 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., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilye, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., and Zverev, V. G.
Abstract: A useful parametrization of the energy spectrum of galactic cosmic rays (GCR) near Earth is offered by the so-called force-field model which describes the shape of the entire spectrum with a single parameter, the modulation potential. While the usefulness of the force-field approximation has been confirmed for regular periods of solar modulation, it was not tested explicitly for disturbed periods, when GCR are locally modulated by strong interplanetary transients. Here we use direct measurements of protons and alpha-particles performed by the PAMELA space-borne instrument during December 2006, including a major Forbush decrease, in order to directly test the validity of the force-field parameterization. We conclude that (1) The force-field parametrization works very well in describing the energy spectra of protons and alpha-particles directly measured by PAMELA outside the Earths atmosphere; (2) The energy spectrum of GCR can be well parameterized by the force-field model also during a strong Forbush decrease; (3) The estimate of the GCR modulation parameter, obtained using data from the world-wide neutron monitor network, is in good agreement with the spectra directly measured by PAMELA during the studied interval. This result is obtained on the basis of a single event analysis, more events need to be analyzed., QC 20150626
Published: 2015
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154. PAMELA measurements of the boron and carbon spectra

Author: Mori, N., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., Mori, N., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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.
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., QC 20151102
Published: 2015
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155. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

Author: Karelin, A. V., 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, Per, Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., 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, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Rossetto, Laura, Simon, M., Sparvoli, R., Spillantini, P., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Karelin, A. V., 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, Per, Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., 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, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Rossetto, Laura, Simon, M., Sparvoli, R., Spillantini, P., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
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., QC 20151102
Published: 2015
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156. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

Author: Munini, R., Di Felice, V., 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, Per, 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, Mark, 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, R., Di Felice, V., 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, Per, 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, Mark, 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., and Vos, E. E.
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<0 solar minimum of solar cycle 23, are presented. These fluxes provide important information for the study of charge dependent solar modulation effects., QC 20151102
Published: 2015
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157. 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., Koldashov, S. V., Mayorov, A. G., Mayorova, M. A., Mikhailov, V. V., Aleksandrin, S. Yu, Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, Per, 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, Mark, 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., Malakhov, V. V., Koldashov, S. V., Mayorov, A. G., Mayorova, M. A., Mikhailov, V. V., Aleksandrin, S. Yu, Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, Per, 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, Mark, 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., and Zampa, N.
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= similar to 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., QC 20151102
Published: 2015
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158. Study of deuteron spectra under radiation belt with PAMELA instrument

Author: 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, Per, 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., 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, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., 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, Per, 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., 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, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
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., QC 20151102
Published: 2015
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159. Lithium and beryllium isotopes in the pamela-experiment

Author: Menn, W., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., Menn, W., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., and Vos, E. E.
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 comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anti-coincidence system, a shower tail counter scintillator and a neutron detector. The scientific objectives addressed by the mission are the measurement of the antiprotons and positrons spectra in cosmic rays, the hunt for antinuclei as well as the determination of light nuclei fluxes from hydrogen to oxygen in a wide energy range and with very high statistics. In this paper the identification capability for lithium and beryllium isotopes for two different techniques are presented, combining the rigidity measurement from the magnetic spectrometer with the velocity information derived either with the time-of-flight or with multiple dE/dx measurements in the calorimeter. Preliminary results of the isotopic ratios will be presented., QC 20161117
Published: 2015

160. Measurement of Lithium and Beryllium cosmic-ray abundances by the PAMELA experiment

Author: Vannuccini, E., Mori, N., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Potgieter, M. S., Vos, E. E., Vannuccini, E., Mori, N., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Potgieter, M. S., and Vos, E. E.
Abstract: The PAMELA experiment is collecting particles along a low Earth semi-polar orbit on board of Resurs-DK1 satellite since June 2006. The combined information of a silicon tracking system and a scintillator hodoscope provides redundant light-element identification capabilities, via multiple ionization energy-loss measurements. The instrument design is not optimized for nuclei detection, whose high ionization signal progressively saturates the detectors. However, Li and Be nuclei can still be identified by using the full set of information, which allows to efficiently select the two elements against the background of more abundant elements. The main issues of the analysis aiming to optimize the Li and Be selection are discussed in this paper. Preliminary results on the elemental abundances will be presented at the conference., QC 20161117
Published: 2015

161. Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the pamela-experiment

Author: Menn, W., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., Menn, W., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., and Vos, E. E.
Abstract: The cosmic-ray hydrogen and helium (1H,2H,3He,4He) isotopic composition between 100 MeV/n and 1.4 GeV/n has been measured with the satellite-borne experiment PAMELA, which was launched into low-Earth orbit on-board the Resurs-DK1 satellite on June 15th 2006. The rare isotopes 2H and 3He in cosmic rays are believed to originate mainly from the interaction of high energy protons and helium with the galactic interstellar medium. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C. The isotopic composition was measured between 100 and 1100 MeV/n for hydrogen and between 100 and 1400 MeV/n for helium isotopes using two different detector systems over the 23rd solar minimum from July 2006 to December 2007., QC 20161117
Published: 2015

162. Solar modulation of galactic cosmic ray electrons and positrons over the 23rd solar minimum with the PAMELA experiment

Author: Munini, R., Di Felice, V., Boezio, M., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, Per, 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, Mark, 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, R., Di Felice, V., Boezio, M., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, Per, 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, Mark, 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., and Vos, E. E.
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 time variation of electron and positron spectrum at Earth in great detail, extending the measurement down to 70 MeV and 200 MeV respectively. The spectra have been evaluated with data collected from July 2006 to December 2009, i.e. during the A<0 solar minimum of solar cycle 23, over six-months intervals. These spectra provide important information for the study of CR propagation inside the heliosphere and the investigation of the charge-dependent solar modulation., QC 20161117
Published: 2015

163. Nine years of cosmic rays investigation by the PAMELA experiment

Author: Boezio, M., Martucci, M., Bruno, A., Di Felice, V., Munini, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, Per, 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., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., Boezio, M., Martucci, M., Bruno, A., Di Felice, V., Munini, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, Per, 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., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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.
Abstract: The PAMELA cosmic ray detector was launched on June 15th of 2006 on board the Russian Resurs-DK1 satellite and during nine years of continuous data-taking it has ob- served very interesting features in cosmic rays, namely in the fluxes of protons, helium and electrons. Its discoveries might change our basic vision of the mechanisms of pro- duction, acceleration and propagation of cosmic rays in the Galaxy. Moreover, PAMELA measurements of cosmic antiproton and positron fluxes and positron-to-all-electron ratio have been setting strong constraints to the nature of Dark Matter. Measurements of boron, carbon, lithium and beryllium (together with the isotopic fraction) will also shed new light on the elemental composition of the cosmic radiation. Search for signatures of more exotic processes (such as the ones involving Strange Quark Matter) is also pursued. Furthermore, the instrument is still functional allowing a constant monitoring of the solar activity during its maximum and a detailed and prolonged study of the solar modulation, improving the comprehension of the heliosphere mechanisms. PAMELA is also measur- ing the radiation environment around the Earth, and it detected for the first time the presence of an antiproton radiation belt surrounding our planet. In this highlight paper PAMELA main results will be reviewed., QC 20161117
Published: 2015

164. Magnetospheric effects on high-energy solar particles during the 2012 May 17th event measured with the PAMELA experiment

Author: Martucci, M., Bazilevskaya, G. A., Boezio, M., Bravar, U., Bruno, A., Christian, E. R., De Nolfo, G. A., Lee, M., Mergè, M., Mocchiutti, E., Munini, R., Ricci, M., Ryan, J. M., Stochaj, S., Thakur, N., Adriani, O., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, Per, 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., Mayorov, A. G., Menn, W., Mikhailov, V. V., Monaco, A., Mori, N., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., 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., Martucci, M., Bazilevskaya, G. A., Boezio, M., Bravar, U., Bruno, A., Christian, E. R., De Nolfo, G. A., Lee, M., Mergè, M., Mocchiutti, E., Munini, R., Ricci, M., Ryan, J. M., Stochaj, S., Thakur, N., Adriani, O., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, Per, 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., Mayorov, A. G., Menn, W., Mikhailov, V. V., Monaco, A., Mori, N., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, Picozza, P., 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.
Abstract: The great challenge in constraining scenarios for solar energetic particle (SEP) acceleration is due to the fact that the signatures of acceleration itself are heavily modified by transport within interplanetary space. During transport, SEPs are subject to pitch angle scattering by the turbulent magnetic field, adiabatic focusing, or reflecting magnetic structures. Ground Level Enhancements (GLEs) provide an ideal way to study acceleration with minimal transport. In this work, we present a unique high-energy SEP observation from PAMELA of the 2012 May 17 GLE and interpret the observed pitch angle distributions as a result of local scattering (1 AU) by the Earth's magnetosheath., QC 20161121
Published: 2015

165. Study on CRE arrival distributions with PAMELA experiment

Author: Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Scotti, V., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bottai, S., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Vacchi, A., Zampa, G., Zampa, N., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Donato, C., De Santis, C., Marcelli, L., Mergé, M., Palma, F., Picozza, P., Sparvoli, R., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Giaccari, U., Martucci, M., Menn, W., Simon, M., Ricci, M., Ricciarini, S. B., Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Scotti, V., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bottai, S., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Vacchi, A., Zampa, G., Zampa, N., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Donato, C., De Santis, C., Marcelli, L., Mergé, M., Palma, F., Picozza, P., Sparvoli, R., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Giaccari, U., Martucci, M., Menn, W., Simon, M., Ricci, M., and Ricciarini, S. B.
Abstract: From 2009, several experiments, like PAMELA, FERMI and AMS, have shown a rise in the fraction of positrons versus electrons+positrons. One of the most probable explanation is due to the presence of nearby sources, like SNRs or pulsars. PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) is a ballooon-borne experiment and is collecting data since 15 June 2006. Its quasi-polar orbit permits to perform a survey in each direction of the sky. The study of the arrival distribution of cosmic ray electrons and positrons from different regions allows the exploration of different origins for the excess., QC 20161121
Published: 2015

166. Long-term Monitoring of the TeV Emission from Mrk 421 with the ARGO-YBJ Experiment

Author: Bartoli, B., Bernardini, P., X. J., Bi, Bleve, C., Bolognino, I., Branchini, P., Budano, A., Calabrese, A. K., Camarri, P., Cao, Z., Cappa, A., Cardarelli, R., Catalanotti, S., Cattaneo, C., Celio, P., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. D., Danzengluobu, Dattoli, M., Mitri, I. D., Piazzoli, B. D., Girolamo, T. D., Ding, X. H., Sciascio, G. D., Feng, C. F., Feng, Z., Galeazzi, F., Galeotti, Piero, Giroletti, E., Gou, Q. B., Guo, Y. Q., H. H., He, Hu, H., Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, H. J., Li, J. Y., Li, X. X., Li, Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., X. H., Ma, Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., X. B., Qu, Rossi, E., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, Carlo Francesco, Wang, B., Wang, H., C. Y., Wu, H. R., Wu, Xu, B., Xue, L., Yan, Y. X., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, J., Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., and Collaboration, T. A.
Published: 2011

167. The large-scale anisotropy with the PAMELA calorimeter

Author: Karelin, A., primary, Adriani, O., additional, Barbarino, G., additional, Bazilevskaya, G., additional, Bellotti, R., additional, Boezio, M., additional, Bogomolov, E., 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, Di Felice, V., additional, Formato, V., additional, Galper, A., additional, Koldashov, S., additional, Koldobskiy, S., additional, Krut'kov, S., additional, Kvashnin, A., additional, Leonov, A., additional, Malakhov, V., additional, Marcelli, L., additional, Martucci, M., additional, Mayorov, A., additional, Menn, W., additional, Mergé, 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., additional, Sarkar, R., additional, Simon, M., additional, Scotti, V., additional, Sparvoli, R., additional, Spillantini, P., additional, Stozhkov, Y., additional, Vacchi, A., additional, Vannuccini, E., additional, Vasilyev, G., additional, Voronov, S., additional, Yurkin, Y., additional, Zampa, G., additional, and Zampa, N., additional
Published: 2015
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168. SEARCH FOR ANISOTROPIES IN COSMIC-RAY POSITRONS DETECTED BY THE PAMELA EXPERIMENT

Author: Adriani, O., primary, 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, Donato, C. De, additional, Santis, C. De, additional, Simone, N. De, additional, Felice, V. Di, additional, Formato, V., additional, Galper, A. M., additional, Giaccari, U., 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, 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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169. Search for a positron anisotropy with PAMELA experiment

Author: Panico, B., 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, Giaccari, U., 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, Mori, N., additional, Munini, R., additional, Osteria, G., additional, Palma, F., 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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170. TIME DEPENDENCE OF THEe−FLUX MEASURED BYPAMELADURING THE 2006 JULY–2009 DECEMBER SOLAR MINIMUM

Author: Adriani, O., primary, 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, Donato, C. De, additional, Santis, C. De, additional, Simone, N. De, 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, 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, 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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171. 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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172. 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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173. 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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174. 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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175. 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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176. The PAMELA experiment and cosmic ray observations

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, Danilchenko, I.A., 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, 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, Zampa, N., additional, and Zverev, V.G., additional
Published: 2015
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177. Force-field parameterization of the galactic cosmic ray spectrum: Validation for Forbush decreases

Author: Usoskin, I.G., primary, Kovaltsov, G.A., 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, Carbone, R., 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, Menn, W., additional, Mergé, 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, Pizzolotto, C., additional, Ricci, M., additional, Ricciarini, S.B., additional, Rossetto, L., 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, Zampa, N., additional, and Zverev, V.G., additional
Published: 2015
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178. Reentrant albedo proton fluxes measured by the PAMELA experiment

Author: Adriani, O., primary, 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, Donato, C. De, 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, Menn, W., additional, Mergé, 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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179. PAMELA’S MEASUREMENTS OF MAGNETOSPHERIC EFFECTS ON HIGH-ENERGY SOLAR PARTICLES

Author: Adriani, O., primary, 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, Bruno, A., additional, Cafagna, F., additional, Campana, D., additional, Carbone, R., additional, Carlson, P., additional, Casolino, M., additional, Castellini, G., additional, Christian, E. R., additional, Donato, C. De, additional, Nolfo, G. A. de, additional, Santis, C. De, additional, Simone, N. De, 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, Mergé, 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, Thakur, N., 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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180. TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THE PAMELA EXPERIMENT

Author: Adriani, O., primary, 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, 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, Zampa, N., additional, and Zverev, V. G., additional
Published: 2015
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181. Search for Spatial and Temporary Variations of Galactic Cosmic Ray Positrons in PAMELA Experiment

Author: Mikhailov, V.V., primary, Galper, A.M., additional, Karelin, A.V., additional, Koldashov, S.V., additional, Malakhov, V.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, Carbone, R., 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, Koldobskiy, S., additional, Krutkov, S., additional, Kvashnin, A., additional, Leonov, A., 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, 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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182. Solar Modulation of Galactic Cosmic Rays During 2006-2015 Based on PAMELA and ARINA Data

Author: Mayorova, M.A., primary, Mayorov, A.G., additional, 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, Carbone, R., additional, Carlson, P., additional, Casolino, M., additional, Castellini, G., additional, DeDonato, C., additional, DeSantis, C., additional, DeSimone, N., additional, DiFelice, V., additional, Formato, V., additional, Galper, A.M., additional, Karelin, A.V., additional, Koldashov, S.V., additional, Koldobskiy, S., additional, Kvashnin, A.A., additional, Kvashnin, A.N., additional, Leonov, A., additional, Malakhov, 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, Naumov, P.Yu., additional, Osteria, G., additional, Palma, F., additional, Panico, B., additional, Papini, P., additional, Pearce, M., additional, Picozza, P., additional, Pizzolotto, C., 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, Voronov, S.A., additional, Yurkin, Y.T., additional, Zampa, G., additional, Zampa, N., additional, and Zverev, V.G., additional
Published: 2015
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183. Splash and Re-entrant Albedo Fluxes Measured in the PAMELA Experiment

Author: Mayorov, A.G., primary, Moiseeva, A.I., 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, Carbone, R., additional, Carlson, P., additional, Casolino, M., additional, Castellini, G., additional, DeDonato, C., additional, DeSantis, C., additional, DeSimone, N., additional, DiFelice, V., additional, Formato, V., additional, Galper, A.M., additional, Karelin, A.V., additional, Koldashov, S.V., additional, Koldobskiy, S., additional, Kvashnin, A.A., additional, Kvashnin, A.N., additional, Leonov, A., additional, Malakhov, 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, Osteria, G., additional, Palma, F., additional, Panico, B., additional, Papini, P., additional, Pearce, M., additional, Picozza, P., additional, Pizzolotto, C., 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, Voronov, S.A., additional, Yurkin, Y.T., additional, Zampa, G., additional, Zampa, N., additional, and Zverev, V.G., additional
Published: 2015
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184. 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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., Zverev, V. G., 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, Per, 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., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, Mark, 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.
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., QC 20140915
Published: 2014
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185. A method to detect positron anisotropies with Pamela data

Author: Panico, B, Carlson, Per, Pearce, Mark, Zverev, V. G., et al., Panico, B, Carlson, Per, Pearce, Mark, Zverev, V. G., and et al.
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., QC 20151125
Published: 2014
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186. PAMELA mission : Heralding a new era in cosmic ray physics

Author: Ricciarini, S. 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, Per, Casolino, M., Castellini, G., De Donato, C., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Kheymits, M. D., 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, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Sarkar, R., Simon, M., Scotti, V., 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., Ricciarini, S. 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, Per, Casolino, M., Castellini, G., De Donato, C., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Kheymits, M. D., 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, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Sarkar, R., Simon, M., Scotti, V., 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.
Abstract: After seven years of data taking in space, the experiment PAMELA is showing very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt., QC 20150615
Published: 2014
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187. Back-Tracing and Flux Reconstruction for Solar Events with PAMELA

Author: Bruno, A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bravar, U., Cafagna, F., Campana, D., Carbone, R., 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., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Lee, M., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergé, 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., Zampa, N., Zverev, V. G., Bruno, A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bravar, U., Cafagna, F., Campana, D., Carbone, R., 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., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Lee, M., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergé, 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., Zampa, N., and Zverev, V. G.
Abstract: The PAMELA satellite-borne experiment is providing first direct measurements of Solar Energetic Particles (SEPs) with energies from $\sim$80 MeV to several GeV in near-Earth space. Its unique observational capabilities include the possibility of measuring the flux angular distribution and thus investigating possible anisotropies related to SEP events. This paper focuses on the analysis methods developed to estimate SEP energy spectra as a function of the particle pitch angle with respect to the Interplanetary Magnetic Field (IMF). The crucial ingredient is provided by an accurate simulation of the asymptotic exposition of the PAMELA apparatus, based on a realistic reconstruction of particle trajectories in the Earth's magnetosphere. As case study, the results of the calculation for the May 17, 2012 event are reported., Comment: 25 pages, 9 figures
Published: 2014

188. Trapped proton fluxes at low Earth orbits measured by 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., 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., 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., Zverev, V. G., 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., 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., 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., and Zverev, V. G.
Abstract: We report an accurate measurement of the geomagnetically trapped proton fluxes for kinetic energy above > 70 MeV performed by the PAMELA mission at low Earth orbits (350-610 km). Data were analyzed in the frame of the adiabatic theory of charged particle motion in the geomagnetic field. Flux properties were investigated in detail, providing a full characterization of the particle radiation in the South Atlantic Anomaly region, including locations, energy spectra and pitch angle distributions. PAMELA results significantly improve the description of the Earth's radiation environment at low altitudes placing important constraints on the trapping and interaction processes, and can be used to validate current trapped particle radiation models., Comment: 22 pages, 5 figures
Published: 2014
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189. Energy Spectrum of Cosmic Protons and Helium Nuclei by a Hybrid Measurement at 4300 m a.s.l

Author: Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Chen, S. Z., Chen, T. L., Creti, P., Cui, S. W., Dai, B. Z., D'Amone, A., Danzengluobu, De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Liguori, G., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Panico, B., Perrone, L., Pistilli8, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Collaboration, G. Zizzi for ARGO-YBJ, Bai, Y. X., Chen, M. J., Chen, Y., Feng, S. H., Gao, B., Gu, M. H., Hou, C., Li, X. X., Liu, J. L., Wang, X., Xiao, G., Zhang, B. K., Zhang, S. S., Zhou, B., Collaboration, X. Zuo for LHAASO, Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Chen, S. Z., Chen, T. L., Creti, P., Cui, S. W., Dai, B. Z., D'Amone, A., Danzengluobu, De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Liguori, G., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Panico, B., Perrone, L., Pistilli8, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Collaboration, G. Zizzi for ARGO-YBJ, Bai, Y. X., Chen, M. J., Chen, Y., Feng, S. H., Gao, B., Gu, M. H., Hou, C., Li, X. X., Liu, J. L., Wang, X., Xiao, G., Zhang, B. K., Zhang, S. S., Zhou, B., and Collaboration, X. Zuo for LHAASO
Abstract: The energy spectrum of cosmic Hydrogen and Helium nuclei has been measured, below the so-called "knee", by using a hybrid experiment with a wide field-of-view Cherenkov telescope and the Resistive Plate Chamber (RPC) array of the ARGO-YBJ experiment at 4300 m above sea level. The Hydrogen and Helium nuclei have been well separated from other cosmic ray components by using a multi-parameter technique. A highly uniform energy resolution of about 25% is achieved throughout the whole energy range (100 TeV - 700 TeV). The observed energy spectrum is compatible with a single power law with index gamma=-2.63+/-0.06., Comment: To be published on Chinese Physics C
Published: 2014
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190. A method to detect positron anisotropies with Pamela data

Author: Panico, B., 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, Di Felice, V., additional, Formato, V., additional, Galper, A.M., additional, Giaccari, U., 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, Munini, R., 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, 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, Zampa, N., additional, and Zverev, V.G., additional
Published: 2014
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191. MEASUREMENT OF BORON AND CARBON FLUXES IN COSMIC RAYS WITH THE PAMELA EXPERIMENT

Author: Adriani, O., primary, 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, Danilchenko, I. A., 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, Mori, N., additional, Munini, R., additional, Osteria, G., additional, Palma, F., additional, Panico, B., 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, 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, Zampa, N., additional, and Zverev, V. G., additional
Published: 2014
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192. TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

Author: Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., DAmone, A., Danzengluobu, De Mitri, I., Piazzoli, B. DEttorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., DAmone, A., Danzengluobu, De Mitri, I., Piazzoli, B. DEttorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., and Zizzi, G.
Abstract: The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence level upper limits of the flux from the investigated sky region are shown. Specific upper limits for 663 GeV $\gamma$-ray AGNs inside the ARGO-YBJ field of view are reported. The effect of the absorption of $\gamma$-rays due to the interaction with extragalactic background light is estimated., Comment: 30 pages, 13 figures, Accepted for publication by ApJ
Published: 2013
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193. Observation of TeV gamma-rays from the unidentified source HESS J1841-055 with the ARGO-YBJ experiment

Author: Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. DAli, DAmone, A., Danzengluobu, De Mitri, I., Piazzoli, B. DEttorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. DAli, DAmone, A., Danzengluobu, De Mitri, I., Piazzoli, B. DEttorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Sbano, S. N., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., and Zizzi, G.
Abstract: We report the observation of a very high energy \gamma-ray source, whose position is coincident with HESS J1841-055. This source has been observed for 4.5 years by the ARGO-YBJ experiment from November 2007 to July 2012. Its emission is detected with a statistical significance of 5.3 standard deviations. Parameterizing the source shape with a two-dimensional Gaussian function we estimate an extension \sigma=(0.40(+0.32,-0.22}) degree, consistent with the HESS measurement. The observed energy spectrum is dN/dE =(9.0-+1.6) x 10^{-13}(E/5 TeV)^{-2.32-+0.23} photons cm^{-2} s^{-1} TeV^{-1}, in the energy range 0.9-50 TeV. The integral \gamma-ray flux above 1 TeV is 1.3-+0.4 Crab units, which is 3.2-+1.0 times the flux derived by HESS. The differences in the flux determination between HESS and ARGO-YBJ, and possible counterparts at other wavelengths are discussed., Comment: 17 pages, 4 figures, have been accepted for publication in ApJ
Published: 2013
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194. Long-term Monitoring on Mrk 501 for Its VHE gamma Emission and a Flare in October 2011

Author: Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. DAl, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. DAl, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., and Zizzi, G.
Abstract: As one of the brightest active blazars in both X-ray and very high energy $\gamma$-ray bands, Mrk 501 is very useful for physics associated with jets from AGNs. The ARGO-YBJ experiment is monitoring it for $\gamma$-rays above 0.3 TeV since November 2007. Starting from October 2011 the largest flare since 2005 is observed, which lasts to about April 2012. In this paper, a detailed analysis is reported. During the brightest $\gamma$-rays flaring episodes from October 17 to November 22, 2011, an excess of the event rate over 6 $\sigma$ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the $\gamma$-ray flux above 1 TeV by a factor of 6.6$\pm$2.2 from its steady emission. In particular, the $\gamma$-ray flux above 8 TeV is detected with a significance better than 4 $\sigma$. Based on time-dependent synchrotron self-Compton (SSC) processes, the broad-band energy spectrum is interpreted as the emission from an electron energy distribution parameterized with a single power-law function with an exponential cutoff at its high energy end. The average spectral energy distribution for the steady emission is well described by this simple one-zone SSC model. However, the detection of $\gamma$-rays above 8 TeV during the flare challenges this model due to the hardness of the spectra. Correlations between X-rays and $\gamma$-rays are also investigated., Comment: have been accepted for publication at ApJ
Published: 2012
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195. Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment

Author: Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. D'Alí, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cardarelli, R., Catalanotti, S., Cattaneo, C., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. D'Alí, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., and Zizzi, G.
Abstract: We report the observation of TeV gamma-rays from the Cygnus region using the ARGO-YBJ data collected from 2007 November to 2011 August. Several TeV sources are located in this region including the two bright extended MGRO J2019+37 and MGRO J2031+41. According to the Milagro data set, at 20 TeV MGRO J2019+37 is the most significant source apart from the Crab Nebula. No signal from MGRO J2019+37 is detected by the ARGO-YBJ experiment, and the derived flux upper limits at 90% confidence level for all the events above 600 GeV with medium energy of 3 TeV are lower than the Milagro flux, implying that the source might be variable and hard to be identified as a pulsar wind nebula. The only statistically significant (6.4 standard deviations) gamma-ray signal is found from MGRO J2031+41, with a flux consistent with the measurement by Milagro., Comment: 14 pages, 4 figures
Published: 2012
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196. Long-term monitoring of the TeV emission from Mrk 421 with the ARGO-YBJ experiment

Author: Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cappa, A., Cardarelli, R., Catalanotti, S., Cattaneo, C., Celio, P., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. D'Alí, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Galeotti, P., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Qu, X. B., Rossi, E., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yan, Y. X., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Zizzi, G., Collaboration, The ARGO-YBJ, Bartoli, B., Bernardini, P., Bi, X. J., Bleve, C., Bolognino, I., Branchini, P., Budano, A., Melcarne, A. K. Calabrese, Camarri, P., Cao, Z., Cappa, A., Cardarelli, R., Catalanotti, S., Cattaneo, C., Celio, P., Chen, S. Z., Chen, T. L., Chen, Y., Creti, P., Cui, S. W., Dai, B. Z., Staiti, G. D'Alí, Danzengluobu, Dattoli, M., De Mitri, I., Piazzoli, B. D'Ettorre, Di Girolamo, T., Ding, X. H., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Galeazzi, F., Galeotti, P., Giroletti, E., Gou, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Huang, Q., Iacovacci, M., Iuppa, R., James, I., Jia, H. Y., Labaciren, Li, H. J., Li, J. Y., Li, X. X., Liguori, G., Liu, C., Liu, C. Q., Liu, J., Liu, M. Y., Lu, H., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Martello, D., Mastroianni, S., Montini, P., Ning, C. C., Pagliaro, A., Panareo, M., Panico, B., Perrone, L., Pistilli, P., Qu, X. B., Rossi, E., Ruggieri, F., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Stanescu, C., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, B., Wang, H., Wu, C. Y., Wu, H. R., Xu, B., Xue, L., Yan, Y. X., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, Jilong, Zhang, Jianli, Zhang, L., Zhang, P., Zhang, X. Y., Zhang, Y., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., and Zizzi, G.
Abstract: ARGO-YBJ is an air shower detector array with a fully covered layer of resistive plate chambers. It is operated with a high duty cycle and a large field of view. It continuously monitors the northern sky at energies above 0.3 TeV. In this paper, we report a long-term monitoring of Mrk 421 over the period from 2007 November to 2010 February. This source was observed by the satellite-borne experiments Rossi X-ray Timing Explorer and Swift in the X-ray band. Mrk 421 was especially active in the first half of 2008. Many flares are observed in both X-ray and gamma-ray bands simultaneously. The gamma-ray flux observed by ARGO-YBJ has a clear correlation with the X-ray flux. No lag between the X-ray and gamma-ray photons longer than 1 day is found. The evolution of the spectral energy distribution is investigated by measuring spectral indices at four different flux levels. Hardening of the spectra is observed in both X-ray and gamma-ray bands. The gamma-ray flux increases quadratically with the simultaneously measured X-ray flux. All these observational results strongly favor the synchrotron self-Compton process as the underlying radiative mechanism., Comment: 30 pages, 8 figures
Published: 2011
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197. Measurement of the Cosmic Ray primary spectrum with ARGO-YBJ experiment

Author: Panico, B, primary, Di Sciascio, G, additional, and Iuppa, R, additional
Published: 2013
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198. Observation of Horizontal Air Showers with ARGO-YBJ

Author: Panico, B., primary and Di Sciascio, G., additional
Published: 2012
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199. Measurement of the cosmic rays light component (p+He) primary spectrum with ARGO-YBJ

Author: Panico, B., primary and Di Sciascio, G., additional
Published: 2012
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200. Deuteron spectrum measurements under radiation belt with PAMELA instrument

Author: 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.
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.
Published: 2016
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