Near-simultaneous magnetotail flux rope observations with Cluster and Double Star

被引:17
|
作者
Walsh, A. P.
Fazakerley, A. N.
Wilson, R. J.
Alexeev, I. V.
Henderson, P. D.
Owen, C. J.
Lucek, E.
Carr, C.
Dandouras, I.
机构
[1] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[2] Los Alamos Natl Lab, Los Alamos, NM USA
[3] Imperial Coll London, London SW7 2BZ, England
[4] Ctr Etud Spatiale Rayonnements, Toulouse, France
基金
英国科学技术设施理事会;
关键词
magnetosphere; magnetotail; plasma sheet; storms and substorms;
D O I
10.5194/angeo-25-1887-2007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present observations of three magnetic flux ropes in the tail of the Earth's magnetosphere on 7 August 2004 by the Cluster and Double Star TC-1 spacecraft. The first two flux rope signatures were observed, near-simultaneously, by Cluster and TC-1, which were located at (-16.3, -8.7, 0.10) R-E GSM and (-10.3, -7.11, 0.81) R-E GSM, respectively, a separation of 6.3 R-E. A third signature was observed some four minutes later by two of the four Cluster spacecraft, while the other two spacecraft observed a feature resembling a Travelling Compression Region (TCR). These observations are interpreted as three individual flux ropes existing in the magnetotail, the first two, at least, simultaneously. The formation mechanism of the flux ropes and the consequences of their presence for the structure of the magnetotail on this day are discussed in the context of multiple X-point reconnection.
引用
收藏
页码:1887 / 1897
页数:11
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