Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions

被引：0
|
作者：
N. A. Barkhatov
E. G. Zhulina
E. A. Kalinina
机构：
[1] Nizhni Novgorod State Pedagogical University,
来源：
Geomagnetism and Aeronomy | 2010年 / 50卷
关键词：
Solar Wind; Coronal Mass Ejection; Solar Wind Velocity; Interplanetary Medium; Solar Wind Parameter;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The initial parameters of disturbing fluxes of coronal mass ejections (CMEs) such as loop, front, spike, multiple structure ejection, and structureless ejection, which cannot be determined from direct observations, are determined using the data on the interplanetary coronal mass ejections (ICMEs) registered on the Helios and Pioneer Venus Orbiter spacecraft in the vicinity of Venus. The method of MHD modeling the modified initial parameters of CMEs has been used for this purpose. The ICME parameters have been analyzed in order to determine the types of the solar sources of the considered plasma flows.
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页码：303 / 313
页数：10
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