Formation of coronal shock waves

被引：0
|
作者：
Vrsnak, B [1 ]
机构：
[1] Fac Geodesy, Hvar Observ, HR-10000 Zagreb, Croatia
来源：
DYNAMIC SUN, PROCEEDINGS | 2001年 / 259卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The evolution of the leading edge of a large amplitude perturbation is studied to investigate the formation of a perpendicular MHD shock wave. The results are applicable to metric and kilometric solar type II bursts.
引用
收藏
页码：251 / 254
页数：4
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