High-frequency radio signatures of solar eruptive flares

被引：7
|
作者：
Karlicky, M [1 ]
机构：
[1] Acad Sci Czech Republic, Inst Astron, CZ-25165 Ondrejov, Czech Republic
来源：
SPACE SCIENCE REVIEWS | 2003年 / 107卷 / 1-2期
关键词：
radio radiation; solar flares;
D O I：
10.1023/A:1025555218525
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects.
引用
收藏
页码：81 / 88
页数：8
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