ON THE STRUCTURE OF THE MAGNETOTAIL CURRENT SHEET

被引:16
|
作者
ASHOURABDALLA, M
ZELENYI, LM
PEROOMIAN, V
RICHARD, RL
机构
[1] RUSSIAN ACAD SCI, SPACE RES INST, MOSCOW 117810, RUSSIA
[2] UNIV CALIF LOS ANGELES, DEPT PHYS, LOS ANGELES, CA USA
关键词
D O I
10.1029/93GL01695
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Results from modeling ion distribution functions in a two-dimensional reduction of the Tsyganenko [1989] magnetic field model have enabled us to calculate the full ion pressure tensor inside the model magnetotail. A thin current sheet is formed in the distant tail and the pressure tensor within this sheet has significant off-diagonal terms. These terms resulting from quasiadiabatic ion trajectories create azimuthally asymmetric distribution functions which are capable of maintaining stress-balance. Outside the current sheet the off-diagonal terms disappear and moderate anisotropy builds up with P(perpendicular-to/P(parallel-to) approximately 0.8. Closer to the Earth rapid isotropization of the distribution occurs.
引用
收藏
页码:2019 / 2022
页数:4
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