Aspects of collisionless magnetic reconnection in asymmetric systems

被引:52
|
作者
Hesse, Michael [1 ]
Aunai, Nicolas [1 ]
Zenitani, Seiji [2 ]
Kuznetsova, Masha [1 ]
Birn, Joachim [3 ]
机构
[1] NASA, Goddard Space Flight Ctr, Heliophys Sci Div, Greenbelt, MD 20771 USA
[2] Natl Astron Observ Japan, Tokyo, Japan
[3] Space Sci Inst, Boulder, CO 80301 USA
基金
美国国家科学基金会;
关键词
FIELD; MAGNETOPAUSE;
D O I
10.1063/1.4811467
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Asymmetric reconnection is being investigated by means of particle-in-cell simulations. The research has two foci: the direction of the reconnection line in configurations with nonvanishing magnetic fields; and the question why reconnection can be faster if a guide field is added to an otherwise unchanged asymmetric configuration. We find that reconnection prefers a direction, which maximizes the available magnetic energy, and show that this direction coincides with the bisection of the angle between the asymptotic magnetic fields. Regarding the difference in reconnection rates between planar and guide field models, we demonstrate that a guide field can provide essential confinement for particles in the reconnection region, which the weaker magnetic field in one of the inflow directions cannot necessarily provide. (C) 2013 AIP Publishing LLC.
引用
收藏
页数:7
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