Dynamics of the Radiation Environment in the Near-Earth Space in September-November 2020 according to the Meteor-M and Electro-L Satellite Data

被引：2

作者：

Myagkova, I. N. ^{[1
]}

Bogomolov, A., V ^{[1
]}

Eremeev, V. E. ^{[1
]}

Shiryaev, A. O. ^{[1
,2
]}

Ginzburg, E. A. ^{[3
]}

机构：

[1] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia

[2] Bryansk State Tech Univ, Bryansk 241035, Russia

[3] Fedorov Inst Appl Geophys, Moscow 129128, Russia

来源：

COSMIC RESEARCH | 2021年 / 59卷 / 06期

关键词：

SOLAR-WIND; BELT; MAGNETOSPHERE; WEATHER; ONBOARD;

D O I：

10.1134/S0010952521060071

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

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.

引用

页码：433 / 445

页数：13

共 18 条

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