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Cosmic–ray positron energy spectrum measured by PAMELA

Mocchiutti, E. (author)
Adriani, O. (author)
Barbarino, G. C. (author)
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Bazilevskaya, G. A. (author)
Bellotti, R. (author)
Bianco, A. (author)
Boezio, M. (author)
Bogomolov, E. A. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Bottai, S. (author)
Bruno, A. (author)
Cafagna, F. (author)
Campana, D. (author)
Carbone, R. (author)
Carlson, P. (author)
Casolino, M. (author)
Castellini, G. (author)
Donato, C. D. E. (author)
Pascale, M. P. D. E. (author)
Santis, C. D. E. (author)
Simone, N. D. E. (author)
Felice, V. D. I. (author)
Formato, V. (author)
Galper, A. M. (author)
Karelin, A. V. (author)
Koldashov, S. V. (author)
Koldobskiy, S. (author)
Krutkov, Y. (author)
Kvashnin, A. N. (author)
Leonov, A. (author)
Malakhov, V. (author)
Marcelli, L. (author)
Martucci, M. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Mergè, M. (author)
Mikhailov, V. V. (author)
Monaco, A. (author)
Mori, N. (author)
Munini, R. (author)
Osteria, G. (author)
Palma, F. (author)
Papini, P. (author)
Pearce, Mark, 1970- (author)
KTH,Partikel- och astropartikelfysik
Picozza, P. (author)
Pizzolotto, C. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Rossetto, Laura (author)
KTH
Sarkar, R. (author)
Scotti, V. (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)
Zampa, G. (author)
Zampa, N. (author)
Zverev, V. G. (author)
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 (creator_code:org_t)
Sociedade Brasileira de Fisica, 2013
2013
English.
In: Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013. - : Sociedade Brasileira de Fisica. - 9788589064293
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range. One of PAMELA’s main goal is the study of the antimatter component of cosmic rays. The experiment, housed on board the Russian satellite Resurs–DK1, was launched on June 15th 2006 and it is still taking data. In this work we present the measurement of galactic positron energy spectrum in the energy range between 500 MeV and few hundred GeV. 

Subject headings

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

Keyword

Cosmic–Rays
Neural Networks
PAMELA
Positrons
Cosmic rays
Electrons
Spectroscopy
Energy ranges
Positron energy
Satellite-borne experiment
Wide energy range
Cosmology

Publication and Content Type

ref (subject category)
kon (subject category)

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