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1.	Aad, G, et al. (author) 2015 swepub:Mat__t
2.	Karelin, A. V., et al. (author) Measuring the spectra of high-energy cosmic-ray particles in the PAMELA experiment 2015 In: Bulletin of the Russian Academy of Sciences: Physics. - 1062-8738. ; 79:3, s. 289-293 Journal article (peer-reviewed)abstract The available data on the energy spectra of electrons, protons, and helium nuclei in the high-energy region are fragmentary, a situation made worse by their scarcity. Due to limitations imposed on the use of the magnetic spectrometer in the PAMELA satellite experiment, the calorimeter must be used for measurements performed in the high-energy region. The processing of experimental data accumulated in more than eight years of measurements with the calorimeter, neutron detector, and scintillation counters allows the spectra of high-energy particles to be obtained, greatly expanding our understanding of the nature of primary cosmic rays.
3.	Mikhailov, V. V., et al. (author) Searching for anisotropy of positrons and electrons in the PAMELA experiment 2015 In: Bulletin of the Russian Academy of Sciences: Physics. - 1062-8738. ; 79:3, s. 298-301 Journal article (peer-reviewed)abstract The PAMELA experiment has been under way aboard the Resurs DK-1 satellite since June 2006. The results have revealed an increase in the ratio of the positron intensity to the total electron and positron intensity at energies in excess of 10 GeV. This increase suggests an additional source of cosmic rays that is associated with either some astrophysical objects (e.g., pulsars) or the probable annihilation of particles of dark matter. Local positron sources can produce notable anisotropy in their flux. The results from the search for anisotropy of positrons and electrons in the events detected by the PAMELA experiment in the 2006–2013 timeframe are described in detail in this work.

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Type of publication: journal article (2)

Type of content: peer-reviewed (2)

Author/Editor: Simon, M. (3); Casolino, M. (2); Vacchi, A. (2); Bonvicini, V. (2); Zampa, G. (2); Malvezzi, V. (2); show more...; Pearce, Mark (2); Carlson, Per (2); Bruno, A. (2); Bellotti, R. (2); Cafagna, F. (2); Campana, D. (2); De Donato, C. (2); De Santis, C. (2); Marcelli, L. (2); Martucci, M. (2); Monaco, A. (2); Osteria, G. (2); Picozza, P. (2); Ricci, M. (2); Castellini, G. (2); Adriani, O. (2); Barbarino, G. C. (2); Bazilevskaya, G. A. (2); Boezio, M. (2); Bogomolov, E. A. (2); Bonechi, L. (2); Bongi, M. (2); Bottai, S. (2); Carbone, R. (2); De Simone, N. (2); Di Felice, V. (2); Galper, A. M. (2); Koldashov, S. V. (2); Krutkov, S. Y. (2); Kvashnin, A. N. (2); Menn, W. (2); Mikhailov, V. V. (2); Mocchiutti, E. (2); Mori, N. (2); Papini, P. (2); Ricciarini, S. B. (2); Sparvoli, R. (2); Spillantini, P. (2); Vannuccini, E. (2); Voronov, S. A. (2); Yurkin, Y. T. (2); Zampa, N. (2); Zverev, V. G. (2); Karelin, A. V. (2); show less...

University: Royal Institute of Technology (2)

Language: English (3)

Research subject (UKÄ/SCB): Natural sciences (2)

Year: 2015 (3)

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