Catastrophic onset of fast magnetic reconnection with a guide field

被引:41
作者
Cassak, P. A. [2 ]
Drake, J. F.
Shay, M. A.
机构
[1] Univ Maryland, College Pk, MD 20742 USA
[2] Univ Delaware, Dept Phys & Astron, Sharp Lab 217, Newark, DE 19716 USA
基金
美国国家科学基金会;
关键词
D O I
10.1063/1.2734948
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
It was recently shown that the slow (collisional) Sweet-Parker and the fast (collisionless) Hall magnetic reconnection solutions simultaneously exist for a wide range of resistivities; reconnection is bistable [Cassak, Shay, and Drake, Phys. Rev. Lett., 95, 235002 (2005)]. When the thickness of the dissipation region becomes smaller than a critical value, the Sweet-Parker solution disappears and fast reconnection ensues, potentially explaining how large amounts of magnetic free energy can accrue without significant release before the onset of fast reconnection. Two-fluid numerical simulations extending the previous results for anti-parallel reconnection (where the critical thickness is the ion skin depth) to component reconnection with a large guide field (where the critical thickness is the thermal ion Larmor radius) are presented. Applications to laboratory experiments of magnetic reconnection and the sawtooth crash are discussed. (C) 2007 American Institute of Physics.
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页数:4
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