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行星际强磁场结构中的亚阿尔文波速流
Alternative TitleA Sun-ALFVENIC FLOW IN THE STRONG INTERPLANETARY MAGNETIC FIELD STRUCTURE
章公亮; 北京8701信箱
Department空间天气学国家重点实验室
Source Publication空间科学学报
1996
Volume16Issue:2Pages:92-96
ISSN0254-6124
Language中文
Keyword行星际亚阿尔文波速流 强磁场结构 太阳风高速流 行星际扰动组合结构
Abstract1982年11月23日开始的极高速太阳风流追赶强磁场结构的事件,形成了高密度前鞘-强磁场本体-高密度后鞘-高速流的组合结构.本文分析了此组合结构的磁流体动力学特征,发现在强磁场本体内出现行星际亚阿尔文波速流,并推论了其可能的成因.
Other AbstractOn November 23, 1982, an extremely high-speed stream was overtaking a strong magnetic field structure, resulting in an interplanetary combinative structire including high-density front sheath, main part with strong magnetic field and low density, high density rear sheath, and extremely high-speed streams. The MHD characteristics of the combinative structure are analyzed in this paper. A sub-Alfvenic flow is found inside the main part of the strong magnetic field structure, the formation of which is also discussed.
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1261
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
章公亮,北京8701信箱. 行星际强磁场结构中的亚阿尔文波速流[J]. 空间科学学报,1996,16(2):92-96.
APA 章公亮,&北京8701信箱.(1996).行星际强磁场结构中的亚阿尔文波速流.空间科学学报,16(2),92-96.
MLA 章公亮,et al."行星际强磁场结构中的亚阿尔文波速流".空间科学学报 16.2(1996):92-96.
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