Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment

V. V. Mikhailov,O. Adriani,G. A. Bazilevskaya,G. C. Barbarino,R. Bellotti,E. A. Bogomolov, M. Boezio,V. Bonvicini,M. Bongi,A. Bruno,A. Vacchi, E. Vannuccini, G. I. Vasilyev, S. A. Voronov,A. M. Galper,C. De Santis,V. Di Felice,G. Zampa,N. Zampa,M. Casolino,D. Campana,A. V. Karelin, P. Carlson, G. Castellini,F. Cafagna,A. A. Kvashnin,A. N. Kvashnin,S. V. Koldashov, S. A. Koldobskiy,S. Yu. Krutkov,A. A. Leonov,A. G. Mayorov,V. V. Malakhov, M. Martucci, L. Marcelli, W. Menn, M. Merge,E. Mocchiutti,A. Monaco, N. Mori,R. Munini,G. Osteria, B. Panico, P. Papini, P. Picozza,M. Pearce,M. Ricci,S. B. Ricciarini,M. F. Runtso,M. Simon,R. Sparvoli, P. Spillantini,Yu. I. Stozhkov,Yu. T. Yurkin

Bulletin of the Russian Academy of Sciences: Physics（2019）

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摘要

The PAMELA magnetic spectrometer was launched onboard the Resurs-DK1 satellite into a near-polar Earth orbit with an altitude of 350–600 km, in order to study fluxes of cosmic ray particles and antiparticles in the wide energy range of ~80 MeV to hundreds of GeV. The results from observations of electron and positron fluxes in 2006–2016 are presented.

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