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5. What kind of ARs may produce more CMEs?

What kind of ARs may produce more CMEs?

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：gcsjsb

【摘 要】

：

Coronal mass ejections(CMEs),as sources of transient events in solar wind,mostly originated from active regions(ARs),are believed to be different phenomena compared with flares in a same eruptive proc

【作 者】

：

Lijuan Liu Yuming Wang Jingxiu Wang Chenglong Shen Pin-zhong Ye Quanhao Zhang Rui Liu S.Wang 

【机 构】

：

CAS Key Laboratory of Geospace Environment,Department of Geophysics and Planetary Sciences,Universit

【出 处】

：

The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

：

2015年5期

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Coronal mass ejections(CMEs),as sources of transient events in solar wind,mostly originated from active regions(ARs),are believed to be different phenomena compared with flares in a same eruptive process.

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