Generation of near-Earth reconnection by divergent flows in the plasma sheet

被引:11
|
作者
Lin, Y [1 ]
Swift, DW
机构
[1] Auburn Univ, Dept Phys, Allison Lab 206, Auburn, AL 36849 USA
[2] Univ Alaska, Inst Geophys, Fairbanks, AK 99775 USA
关键词
magnetic reconnection; divergent flow; magnetotail plasma sheet; hybrid simulation;
D O I
10.1029/2002JA009308
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] A global two-dimensional hybrid simulation is carried out to study the evolution of the near-Earth plasma sheet. It is shown that reconnection X lines and plasmoids can be generated by diverging flows in the plasma sheet. These diverging flows can be caused by variations in the Maxwell stress due to variations of B-x and B-z components of the magnetic field outside the current sheet. In addition, the flow acceleration/deceleration in the plasma sheet can also be caused by variations in the local plasma mass density. Comparison runs have been made with a Harris model current sheet with zero B-z, and no evidence of reconnection is found. The results indicate that divergent plasma flow is a sufficient condition for reconnection even in a dissipation-less plasma.
引用
收藏
页数:9
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