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Electron distribution functions in the diffusion region of asymmetric magnetic reconnection
被引:70
|作者:
Bessho, N.
[1
,2
]
Chen, L. -J.
[1
,2
]
Hesse, M.
[2
]
机构:
[1] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[2] NASA, Goddard Space Flight Ctr, Heliophys Sci Div, Greenbelt, MD USA
基金:
美国国家科学基金会;
关键词:
magnetic reconnection;
asymmetric reconnection;
electron distribution function;
PIC simulation;
stagnation point;
diffusion region;
ACCELERATION;
D O I:
10.1002/2016GL067886
中图分类号:
P [天文学、地球科学];
学科分类号:
07 ;
摘要:
We study electron distribution functions in a diffusion region of antiparallel asymmetric reconnection by means of particle-in-cell simulations and analytical theory. At the electron stagnation point, the electron distribution comprises a crescent-shaped population and a core component. The crescent-shaped distribution is due to electrons coming from the magnetosheath toward the stagnation point and accelerated mainly by electric field normal to the current sheet. Only a part of magnetosheath electrons can reach the stagnation point and form the crescent-shaped distribution that has a boundary of a parabolic curve. The penetration length of magnetosheath electrons into the magnetosphere is derived. We expect that satellite observations can detect crescent-shaped electron distributions during magnetopause reconnection.
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页码:1828 / 1836
页数:9
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