How typical are atypical current sheets? -: art. no. L03108

被引:83
作者
Asano, Y
Nakamura, R
Baumjohann, W
Runov, A
Vörös, Z
Volwerk, M
Zhang, TL
Balogh, A
Klecker, B
Réme, H
机构
[1] OAW, Inst Weltraumforsch, A-8042 Graz, Austria
[2] Univ London Imperial Coll Sci Technol & Med, London SW7 2BZ, England
[3] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[4] CNRS, CESR, F-31028 Toulouse, France
关键词
D O I
10.1029/2004GL021834
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Using multi-satellite Cluster magnetic field data, we statistically examined how often an atypical, i.e., non-Harris type, current sheet is formed. We found that a cross-tail current sheet with an off-equatorial current density maximum, indicating bifurcation, is frequently formed in thin current sheets with a half thickness of similar to1500 km. The occurrence of off-equatorial current density maxima is correlated with the occurrence of fast plasma flows, namely if fast plasma flows occur nearby, one is more likely to observe off-equatorial current density maxima. We also found that many of the center-peaked current sheets exhibit a feature different from a normal Harris sheet: namely a very intense current concentrated near the equatorial plane, embedded in a broader current sheet with lower current density.
引用
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页码:1 / 4
页数:4
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