Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24

被引：0
|
作者：
D. G. Rodkin
Yu. S. Shugai
V. A. Slemzin
V. A. Veselovskii
机构：
[1] Russian Academy of Sciences,Lebedev Physical Institute
[2] Moscow State University,Skobeltsyn Institute of Nuclear Physics
来源：
Bulletin of the Lebedev Physics Institute | 2016年 / 43卷
关键词：
Sun; solar wind; coronal mass ejection; coronal hole; active region;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The interaction of the interplanetary coronal mass ejection (ICME) and the high-speed solar wind flux (HSSWF) associated with the coronal hole (CH) is considered. By the examples of two events at the maximum of solar cycle 24 from June 4 to June 16 and from June 30 to July 10, 2012 it is shown that the temperature-dependent parameters of the SW ionic composition appear closer to the values in the HSSWF than in the ICME due to mixing of fluxes in the corona when the ICME source is near the CH boundary.
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页码：287 / 290
页数：3
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