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First detection of geomagnetically trapped antiprotons 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. 86-89
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • We present the measurement of geomagnetically trapped antiprotons in the South Atlantic Anomaly performed by the PAMELA satellite-bourne experiment. The existence of an antiproton radiation belt, predicted by several models as the product of cosmic ray interactions with the residual terrestrial atmosphere, is evidenced for the first time. PAMELA measured the antiproton spectrum in the kinetic energy range between 60 and 750 MeV, reporting a trapped antiproton flux which exceeds by about 3 orders of magnitude the interplanetary cosmic ray antiproton flux. An estimation of the mean under-cutoff antiproton flux outside radiation belts has been also provided.

Subject headings

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

Keyword

Cosmic rays
Magnetosphere
Radiation belt
SAA
Trapped antiprotons

Publication and Content Type

ref (subject category)
kon (subject category)

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