Geomagnetic Activity as a Reflection of Processes in the Magnetospheric Tail: 2. Plasma Convection Model

被引：1
|
作者：
Krymskii, G. F. [1 ]
Danilov, A. A. [1 ]
Makarov, G. A. [1 ]
机构：
[1] Russian Acad Sci, Shafer Inst Cosmophys Res & Aeron, Siberian Branch, Yakutsk 677980, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2013年 / 53卷 / 05期
关键词：
Solar Wind; Geomagnetic Activity; Plasma Sheet; Dipole Field; Magnetic Tube;
D O I：
10.1134/S0016793213040105
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：
A model of plasma convection in the magnetospheric tail was developed. Although highly simplified, the model adequately describes the main characteristics of the process. We have calculated the physical parameters characterizing the magnetotail, as well as described the convection of fluxtubes in it and the process of electron dropout. The model explains the semiannual variation in magnetic activity.
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页码：604 / 612
页数：9
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