Dynamics of the Radiation Environment in the Near-Earth Space in September–November 2020 according to the Meteor-M and Electro-L Satellite Data
I. N. MyagkovaSkobeltsyn Institute of Nuclear Physics, Moscow State University, 119991, Moscow, RussiaA. V. BogomolovSkobeltsyn Institute of Nuclear Physics, Moscow State University, 119991, Moscow, RussiaV. E. EremeevSkobeltsyn Institute of Nuclear Physics, Moscow State University, 119991, Moscow, RussiaArtem O. ShiryaevBryansk State Technical University, 241035, Bryansk, RussiaE. A. GinzburgFedorov Institute of Applied Geophysics, 129128, Moscow, Russia
2021en
ABI
Abstract
The results of a comparative analysis from Russian satellite data on the radiation environment in the near-Earth space during September–November 2020 are presented. The source of variations in the fluxes and spectra of electrons in the Earth’s outer radiation belt during this period was the high-speed fluxes of the solar wind from the coronal hole. Differences in the response of the Earth’s outer radiation belt to recurrent geomagnetic disturbances at each solar revolution are discussed.
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