Variation of proton fluxes of galactic cosmic rays during 2012-2020 according to data from the Russian spacecraft in geostationary orbit
E. Bondarev*, A.E. Koziukov, G. Protopopov, P.A. Chubunov, A. Repin, V.I. Denisova and A.V. Tsurgaev
Pre-published on:
July 09, 2021
Published on:
March 18, 2022
Abstract
In this paper, we study the effect of solar modulation over the past decade, and also conduct a comparative analysis with the data provided by the GOES spacecraft.
The measurements were carried out using the Russian spacecraft on the geostationary orbit. The detector has 5 channels for detecting protons with energies E ≥ 3.5 MeV, E ≥ 15 MeV and also with energies E = 13.7-23 MeV, E = 23-42 MeV , E = 42-112 MeV.
DOI: https://doi.org/10.22323/1.395.1308
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