Solitary structures associated with short large-amplitude magnetic structures (SLAMS) upstream of the Earth's quasi-parallel bow shock -: art. no. L16805

被引:35
作者
Behlke, R
André, M
Bale, SD
Pickett, JS
Cattell, CA
Lucek, EA
Balogh, A
机构
[1] Swedish Inst Space Phys, Uppsala Div, SE-75121 Uppsala, Sweden
[2] Uppsala Univ, Dept Space Phys & Astron, Uppsala, Sweden
[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[4] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[5] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[6] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, England
关键词
D O I
10.1029/2004GL019524
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
For the first time, solitary waves (SWs) have been observed within short large-amplitude magnetic structures (SLAMS) upstream of the Earth's quasi-parallel bow shock. The SWs often occur as bipolar pulses in the electric field data and move parallel to the background magnetic field at velocities of v = 400-1200 km/s. They have peak-to-peak amplitudes in the parallel electric field of up to E-parallel to' = 65 mV/m and parallel scale sizes of L-parallel to similar to 10 lambda(D). The bipolar solitary waves exhibit negative potential structures of \Phi(parallel to)\ = 0.4-2.2 V, i.e., ePhi(parallel to)/kT(e) similar to 0.1. None of the theories commonly used to describe SWs adequately address these negative potential structures moving at velocities above the ion thermal speed in a weakly magnetized plasma.
引用
收藏
页码:L168051 / 4
页数:4
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