Does the braking of the fast plasma flow trigger a substorm?: A study of the August 14, 1996, event

被引:29
作者
Ohtani, S
Yamaguchi, R
Kawano, H
Creutzberg, F
Sigwarth, JB
Frank, LA
Mukai, T
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Kyushu Univ, Dept Earth & Planetary Sci, Fukuoka 8128581, Japan
[3] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[4] KeoMetrics, Ottawa, ON, Canada
[5] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 229, Japan
关键词
D O I
10.1029/2001GL013785
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
[1] In a substorm event of August 14, 1996, the Geotail satellite was at X-GSM similar to -10 R-E aligned with the GOES 8 satellite in the X direction in the premidnight sector. Two Pi2 onsets were identified. Whereas the first onset was associated with a pseudobreakup, an auroral bulge developed following the second onset. At the pseudobreakup Geotail observed a fast (> 900 km/ s) plasma flow along with dipolarization, but the geosynchronous magnetic field became stretched subsequently. In contrast, for the main onset, the magnetic field dipolarized at GOES 8, although the associated total (time- integrated) transport of magnetic flux at Geotail was no stronger than that for the pseudobreakup. It is suggested that the braking of the fast flow does not necessarily cause tail current disruption in a large scale, and there is an additional (or alternative) condition to suffice for an initial brightening to develop to a global substorm.
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页码:16 / 1
页数:4
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