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行星际磁场北向时磁层顶区磁场重联的全球模式
Alternative TitleA GLOBAL MODEL OF MAGNETIC RECONNECTION AT MAGNETOPAUSE FOR NORTHWARD IMF
张洪; 刘振兴; 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:4Pages:274-281
ISSN0254-6124
Language中文
Keyword行星际磁场 磁层顶 磁场重联
Abstract在对背阳面磁层顶区局域磁场重联模拟的基础上提出了一个行星际磁场北向时磁层顶磁场重联的全球模式.行星际磁场北向时磁层顶磁场重联导致近地尾瓣的能量被输送到远磁尾,太阳风能量不在磁尾储存,向阳面磁层顶变厚,磁层受到一系列扰动.
Other AbstractA 2D compressible model is used to simulate the local the nightside magnetopause for northward IMF.Based globe magnetic reconnection model for northward IMF is on magnetic reconnection the simulation result,at proposed.As results of mag-netic reconnection at magnetopause for northward IMF,the magnetic energy in tail lobe is transported to far magnetotail,dayside magnetopause become thicker, and the magnetosphere is disturbed.
Indexed ByCSCD
Funding Project中国科学院空间科学与应用研究中心
Citation statistics
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1444
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
张洪,刘振兴,北京8701信箱. 行星际磁场北向时磁层顶区磁场重联的全球模式[J]. 空间科学学报,1996,16(4):274-281.
APA 张洪,刘振兴,&北京8701信箱.(1996).行星际磁场北向时磁层顶区磁场重联的全球模式.空间科学学报,16(4),274-281.
MLA 张洪,et al."行星际磁场北向时磁层顶区磁场重联的全球模式".空间科学学报 16.4(1996):274-281.
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