On the problem of electron loss in the outer radiation belt during a magnetic storm

被引：0

作者：

Lazutin, L. L. ^{[1
]}

机构：

[1] Moscow MV Lomonosov State Univ, Skobelitsyn Res Inst Nucl Phys, Moscow, Russia

来源：

GEOMAGNETISM AND AERONOMY | 2016年 / 56卷 / 05期

关键词：

DAWN-DUSK ASYMMETRY; RELATIVISTIC ELECTRONS; GEOMAGNETIC STORMS; MAGNETOSPHERE; PARTICLE; BOUNDARY; DYNAMICS; TIME; ACCELERATION; MODEL;

D O I：

10.1134/S0016793216040095

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

An abrupt change in the latitudinal profile of energetic electrons in the Earth's outer radiation belt during magnetic storms is explained in many publications by a loss of electrons at L = 4-7 resulting from their departure to the atmosphere or to the magnetopause. In the present work, the loss of electrons is explained primarily by adiabatic transformation of the magnetic drift trajectories. For this purpose, the effect of dawnto- dusk asymmetry measured by low-orbit SERVIS-1 and KORONAS-F satellites is involved.

引用

页码：545 / 556

页数：12

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