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

页码：251 / 254

页数：4

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