地球极区的磁流体力学慢激波

IMECH-IR > 力学所知识产出(1956-2008)

	地球极区的磁流体力学慢激波
	胡文瑞
Source Publication	科学通报
	1986
Volume	31 Issue:2 Pages:100-103
ISSN	0023-074X
Abstract	<正> 离子在极区电离层被加热和加速以后,逃离地球引力场而形成极风。低能离子通过极风而传送到磁层中,成为磁层粒子的一个重要来源,越来越受到人们的重视。极风的主要成分是H~+、He~+和少量低能的O~+,其中氢离子流量为10~7—5×10~8/厘米~2•秒,氦离子的流量为10~5—10~7/厘米~2•秒。探险号31在极区距地球500—3000公里处测得平行于地磁场的H~+外流速
Keyword	磁流体力学慢激波极区电离层地球地磁场低能离子极风引力场氦离子
Language	中文
Document Type	期刊论文
Identifier	http://dspace.imech.ac.cn/handle/311007/37066
Collection	力学所知识产出(1956-2008)
Corresponding Author	胡文瑞
Recommended Citation GB/T 7714	胡文瑞. 地球极区的磁流体力学慢激波[J]. 科学通报,1986,31,2,:100-103.
APA	胡文瑞.(1986).地球极区的磁流体力学慢激波.科学通报,31(2),100-103.
MLA	胡文瑞."地球极区的磁流体力学慢激波".科学通报 31.2(1986):100-103.

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