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

Authors :: Mikhailov, V. V.
Adriani, O.
Bazilevskaya, G. A.
Barbarino, G. C.
Bellotti, R.
Bogomolov, E. A.
Boezio, M.
Bonvicini, V.
Bongi, M.
Bruno, A.
Vacchi, A.
Vannuccini, E.
Vasilyev, G. I.
Voronov, S. A.
Galper, A. M.
De Santis, C.
Di Felice, V.
Zampa, G.
Zampa, N.
Casolino, M.
Source :: Bulletin of the Russian Academy of Sciences: Physics; Aug2019, Vol. 83 Issue 8, p974-976, 3p
Publication Year :: 2019
Abstract: 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. [ABSTRACT FROM AUTHOR]

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