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  • Bruno, A. (author)

Trapped protons in SAA measured by the PAMELA experiment

  • Article/chapterEnglish2011

Publisher, publication year, extent ...

  • Institute of High Energy Physics,2011
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:kth-164997
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-164997URI
  • https://doi.org/10.7529/ICRC2011/V06/0963DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:kon swepub-publicationtype

Notes

  • QC 20150422
  • 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 and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Cafagna, F. (author)
  • Adriani, O. (author)
  • 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, PerKTH,Fysik(Swepub:kth)u1ua4u32 (author)
  • 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, WilliamKTH,Fysik(Swepub:kth)u171jmfw (author)
  • 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, MarkKTH,Fysik(Swepub:kth)u17jptna (author)
  • Picozza, P. (author)
  • Pizzolotto, C. (author)
  • Ricci, M. (author)
  • Ricciarini, S. B. (author)
  • Rossetto, LauraKTH,Fysik(Swepub:kth)u1tv6cqb (author)
  • 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)
  • KTHFysik (creator_code:org_t)

Related titles

  • In:Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011: Institute of High Energy Physics, s. 82-85

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