Prospective of coronal mass ejections, solar flares and geomagnetic storms

被引：0
|
作者：
A. K. Singh
A. Tonk
R. Singh
机构：
[1] University of Lucknow,Department of Physics
来源：
Indian Journal of Physics | 2014年 / 88卷
关键词：
Coronal mass ejections; Solar flares; Solar wind; Geomagnetic storms; Space weather; 96.60.qe; 94.30.Lr;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
On the basis of geomagnetic storm index (minimum Dst index), we have considered nine events of coronal mass ejections (CMEs), solar flares, geomagnetic storms and other parameters during the active period of solar cycle 23 (year 1999–2005). We have examined the physics and phenomenology of CMEs and associated solar flares and their further association with geomagnetic storms. Observational results conclude that coronal mass ejections having faster speed (>1,000 km/s) mostly produce stronger geomagnetic storms.
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收藏
页码：1127 / 1133
页数：6
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