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Trapped protons in SAA measured by the PAMELA experiment

Bruno, A. (author)
Cafagna, F. (author)
Adriani, O. (author)
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Barbarino, G. C. (author)
Bazilevskaya, G. A. (author)
Bellotti, R. (author)
Boezio, M. (author)
Bogomolov, E. A. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Borisov, S. (author)
Bottai, S. (author)
Campana, D. (author)
Carbone, R. (author)
Carlson, Per (author)
KTH,Fysik
Casolino, M. (author)
Castellini, G. (author)
Consiglio, L. (author)
De Pascale, M. P. (author)
De Santis, C. (author)
De Simone, N. (author)
Di Felice, V. (author)
Galper, A. M. (author)
Gillard, William (author)
KTH,Fysik
Grishantseva, L. (author)
Jerse, G. (author)
Karelin, A. V. (author)
Kheymits, M. D. (author)
Koldashov, S. V. (author)
Krutkov, S. Y. (author)
Kvashnin, A. N. (author)
Leonov, A. (author)
Malakhov, V. (author)
Marcelli, L. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Monaco, A. (author)
Mori, N. (author)
Nikonov, N. (author)
Osteria, G. (author)
Palma, F. (author)
Papini, P. (author)
Pearce, Mark (author)
KTH,Fysik
Picozza, P. (author)
Pizzolotto, C. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Rossetto, Laura (author)
KTH,Fysik
Sarkar, R. (author)
Simon, M. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stozhkov, Y. I. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. (author)
Voronov, S. A. (author)
Yurkin, Y. T. (author)
Wu, J. (author)
Zampa, G. (author)
Zampa, N. (author)
Zverev, V. G. (author)
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 (creator_code:org_t)
Institute of High Energy Physics, 2011
2011
English.
In: Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. - : Institute of High Energy Physics. ; , s. 82-85
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • An accurate measurement of under cutoff proton fluxes in the energy range 60 MeV ÷ 3 GeV has been performed by the PAMELA satellite-borne experiment. Thanks to the high identification performances and to the semipolar and elliptic satellite orbit, PAMELA is able to provide information about spectra and composition of particles in different regions of the magnetosphere. Here we present the measurement of the geomagnetically trapped protons from the inner radiation belt (SAA). The fluxes as a function of equatorial pitch angle and McIlwain L-shell are reported.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

Cosmic rays
Magnetosphere
Radiation belt
Saa
Trapped protons

Publication and Content Type

ref (subject category)
kon (subject category)

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