Ion dynamics of magnetic reconnection in the magnetotail

被引：1
|
作者：
Hishino, M [1 ]
Nishida, A [1 ]
Mukai, T [1 ]
Kokubun, S [1 ]
Yamamoto, T [1 ]
机构：
[1] NAGOYA UNIV, STE LAB, AICHI 46401, JAPAN
来源：
RECONNECTION IN THE SOLAR CORONA AND MAGNETOSPHERIC SUBSTORMS | 1997年 / 19卷 / 12期
关键词：
D O I：
10.1016/S0273-1177(97)00084-7
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
We discuss the kinetic processes of plasma thermalization, acceleration, and mixing in magnetic reconnection. Non-Maxwellian, gyrotropic ion distribution functions such as anisotropic ion beams in the plasma sheet boundary layer (PSBL) and counter-streaming ions (CSIs) in the plasma sheet are often observed during a plasmoid passage of a satellite in the Earth's magnetotail. Non-gyrotropic ion distribution functions are also sometimes observed just after the passage of the plasmoid. We study the behavior of non-Maxwellian ion distribution functions observed by GEOTAIL. We further stud!: theoretically the ion dynamics by using a particle-in-cell simulation, and discuss the role of non-Maxwellian distribution functions in magnetic reconnection. (C) 1997 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：1827 / 1835
页数：9
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