中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Brightening of onset arc precedes the dipolarization onset: THEMIS observations of two events on 1 March 2008

文献类型:期刊论文

作者Kan, J. R.; Li, H.; Wang, C.; Frey, H. U.; Kubyshkina, M. V.; Runov, A.; Xiao, C. J.; Lyu, L. H.; Sun, W.
刊名ANNALES GEOPHYSICAE
出版日期2011
卷号29期号:11页码:2045-2059
ISSN号0992-7689
关键词Magnetospheric physics Magnetosphere-ionosphere interactions
通讯作者Li, H (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, Beijing, Peoples R China.
中文摘要We present a new M-I coupling model of substorm during southward IMF based on the THEMIS observations of two events on 1 March 2008. The first event (E-1) was classified as a pseudo-breakup: brightening of the onset arc preceded the first dipolarization onset by similar to 71 +/- 3 s, but the breakup arcs faded within similar to 5 min without substantial poleward expansion and the dipolarization stopped and reversed to thinning. The second event (E-2) was identified as a substorm: brightening of the second onset arc preceded the second dipolarization onset by similar to 80 +/- 3 s, leading to a full-scale expanding auroral bulge during the substorm expansion phase for similar to 20 min. The Alfven travel time from the ionosphere to the dipolarization onset region is estimated at similar to 69.3 s in E-1; at similar to 80.3 s in E-2, which matched well with the observed time delay of the dipolarization onset after the brightening of the onset arc, respectively in E-1 and E-2. Brightening of the onset arc precedes the dipolarization onset suggest that the onset arc brightening is caused by the intense upward field-aligned currents originating from the divergence of the Cowling electrojet in the ionosphere. The Cowling electrojet current loop (CECL) is formed to close the field-aligned currents at all times. The closure current in the Alfven wavefront is anti-parallel to the cross-tail current. Dipolarization onset occurs when the Alfven wavefront incident on the near-Earth plasma sheet to disrupt the cross-tail current in the dipolarization region. Slow MHD waves dominate the disruption of the cross-tail current in the dipolarization region.
英文摘要We present a new M-I coupling model of substorm during southward IMF based on the THEMIS observations of two events on 1 March 2008. The first event (E-1) was classified as a pseudo-breakup: brightening of the onset arc preceded the first dipolarization onset by similar to 71 +/- 3 s, but the breakup arcs faded within similar to 5 min without substantial poleward expansion and the dipolarization stopped and reversed to thinning. The second event (E-2) was identified as a substorm: brightening of the second onset arc preceded the second dipolarization onset by similar to 80 +/- 3 s, leading to a full-scale expanding auroral bulge during the substorm expansion phase for similar to 20 min. The Alfven travel time from the ionosphere to the dipolarization onset region is estimated at similar to 69.3 s in E-1; at similar to 80.3 s in E-2, which matched well with the observed time delay of the dipolarization onset after the brightening of the onset arc, respectively in E-1 and E-2. Brightening of the onset arc precedes the dipolarization onset suggest that the onset arc brightening is caused by the intense upward field-aligned currents originating from the divergence of the Cowling electrojet in the ionosphere. The Cowling electrojet current loop (CECL) is formed to close the field-aligned currents at all times. The closure current in the Alfven wavefront is anti-parallel to the cross-tail current. Dipolarization onset occurs when the Alfven wavefront incident on the near-Earth plasma sheet to disrupt the cross-tail current in the dipolarization region. Slow MHD waves dominate the disruption of the cross-tail current in the dipolarization region.
学科主题空间物理
资助信息National Natural Science Foundation of China [40831060]; Specialized Research Fund for State Key Laboratories in China; ONR [N00014-08-1-0439]; Canadian Space Agency
收录类别SCI ; EI
语种英语
公开日期2014-12-15
源URL[http://ir.nssc.ac.cn/handle/122/3242]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Kan, J. R.,Li, H.,Wang, C.,et al. Brightening of onset arc precedes the dipolarization onset: THEMIS observations of two events on 1 March 2008[J]. ANNALES GEOPHYSICAE,2011,29(11):2045-2059.
APA Kan, J. R..,Li, H..,Wang, C..,Frey, H. U..,Kubyshkina, M. V..,...&Sun, W..(2011).Brightening of onset arc precedes the dipolarization onset: THEMIS observations of two events on 1 March 2008.ANNALES GEOPHYSICAE,29(11),2045-2059.
MLA Kan, J. R.,et al."Brightening of onset arc precedes the dipolarization onset: THEMIS observations of two events on 1 March 2008".ANNALES GEOPHYSICAE 29.11(2011):2045-2059.

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来源:国家空间科学中心

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