Properties of interplanetary coronal mass ejections

被引：131
|
作者：
Gopalswamy, Nat [1 ]
机构：
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源：
SPACE SCIENCE REVIEWS | 2006年 / 124卷 / 1-4期
关键词：
coronal mass ejections; interplanetary CMEs; solar wind; magnetic clouds; shocks; solar flares; geomagnetic storms;
D O I：
10.1007/s11214-006-9102-1
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs.
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收藏
页码：145 / 168
页数：24
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