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Solar Flare Activity from 2006 to 2016 according to Data from the PAMELA and ARINA Spectrometers.

Solar Flare Activity from 2006 to 2016 according to Data from the PAMELA and ARINA Spectrometers.

Authors :
Rodenko, S. A.
Troitskaya, I. K.
Mayorov, A. G.
Malakhov, V. V.
Source :
Physics of Atomic Nuclei. Sep2018, Vol. 81 Issue 5, p634-637. 4p.
Publication Year :
2018

Abstract

In the period from 2006 to 2016, experiments based on the use of the PAMELA and ARINA spectrometers and aimed at detecting cosmic rays were performed on board the RESURS-DK1 satellite. Although the main goal of these experiments was to study the galactic component of cosmic rays, the instruments in question also detected, over a broad energy range, solar particles accelerated in powerful explosive processes on the Sun (solar flares). A list of solar events in which the PAMELA and ARINA spectrometers detected, in various years of their operation, an increase in the intensities of fluxes of solar protons whose energies were above 45 MeV is presented among other things. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
10637788
Volume :
81
Issue :
5
Database :
Academic Search Index
Journal :
Physics of Atomic Nuclei
Publication Type :
Academic Journal
Accession number :
132371891
Full Text :
https://doi.org/10.1134/S1063778818050162