Coronal mass ejections to the interplanetary medium

被引：0
|
作者：
Pick, M [1 ]
机构：
[1] Observ Paris, CNRS, Dept Astron Solaire, UMR 8645, F-92195 Meudon, France
来源：
SOLAR-TERRESTRIAL MAGNETIC ACTIVITY AND SPACE ENVIRONMENT | 2002年 / 14卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Wepresent some recent results on CME development obtained from joint observations, more particularly on observations coordinated with spectral and imaging radio measurements. We also briefly discuss the origin of energetic particles measured in the interplanetary medium. In addition to the CME bow shock, coronal sites of particle acceleration that are related to large scale reconfiguration associated with CME development, contribute to populating significantly the interplanetary medium with energetic particles over several hours.
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页码：149 / 156
页数：8
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