Coronal mass ejections

被引：0

作者：

Pick, M ^{[1
]}

Démoulin, P ^{[1
]}

Maia, D ^{[1
]}

Plunkett, S ^{[1
]}

机构：

[1] Observ Paris Meudon, DASOP, CNRS, UMR 8645, Meudon, France

来源：

9TH EUROPEAN MEETING ON SOLAR PHYSICS: MAGNETIC FIELDS AND SOLAR PROCESSES, VOLS 1 AND 2 | 1999年 / 448卷

关键词：

coronal mass ejections; shocks;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Coronal Mass Ejections (CMEs) are the most spectacular large-scale manifestations of solar activity. Results presented in this review emphasize the importance of coordinated observations over a large spectral domain. The Yohkoh satellite and since 1996, the SOHO mission have provided this opportunity. Radio imaging observations are an important complementary tool. This review includes four main topics: -the observational signatures of CMEs; - the dynamics and energetics of CMEs; - a brief presentation of CME modeling; -the association between coronal shocks, CMEs and flares.

引用

页码：915 / 926

页数：12

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