A SCENARIO FOR THE LARGE-SCALE MAGNETIC-FIELD EVOLUTION IN CMES

被引：2

作者：

SOMOV, BV

机构：

来源：

JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY | 1991年 / 43卷

关键词：

D O I：

10.5636/jgg.43.Supplement1_31

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

This report gives a summary of the principal properties of coronal mass ejections (CMEs) from the view-point of magnetic field transport through the solar corona. The origin of a coronal streamer system is discussed in the context of a large-scale magnetic field configuration pre-existing to CMEs. Reconnection driven by the solar wind is highlighted for its non-steady character as well as for its key role in the global dynamics of plasma flows in the corona.

引用

页码：31 / 36

页数：6

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