Current sheet flapping motion and structure observed by Cluster -: art. no. 1327

被引:225
作者
Sergeev, V
Runov, A [1 ]
Baumjohann, W
Nakamura, R
Zhang, TL
Volwerk, M
Balogh, A
Rème, H
Sauvaud, JA
André, M
Klecker, B
机构
[1] St Petersburg State Univ, Inst Phys, St Petersburg, Russia
[2] OAW, Inst Weltraumforsch, A-8042 Graz, Austria
[3] Univ London Imperial Coll Sci Technol & Med, London, England
[4] CNRS, CESR, Toulouse, France
[5] Swedish Inst Space Phys, Uppsala, Sweden
[6] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany
关键词
D O I
10.1029/2002GL016500
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Fast vertical flapping oscillations of the plasma sheet have been observed by Cluster on September 26, 2001. The flapping motion had vertical speeds exceeding 100 km/s, an amplitude in excess of 1 R-E and a quasiperiod of similar to3 min. The current sheet was mostly tilted in the Y-Z plane (with the tilt sometimes exceeding 45degrees). The waves had the properties of a kink mode and propagated toward the dusk flank. The flapping allowed to probe the vertical structure of the plasma sheet. Three different methods gave consistent evidence of a bifurcated structure of the cross-tail current with about half of all current concentrated in two sheets (each similar to500-1000 km thick). The current density peaks at \B-x\similar to0.5 B-L, with a pronounced current density minimum and a plasma density plateau between these peaks.
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