Scaling of asymmetric magnetic reconnection: General theory and collisional simulations

被引:402
作者
Cassak, P. A. [1 ]
Shay, M. A. [1 ]
机构
[1] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
D O I
10.1063/1.2795630
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
A Sweet-Parker-type scaling analysis for asymmetric antiparallel reconnection (in which the reconnecting magnetic field strengths and plasma densities are different on opposite sides of the dissipation region) is performed. Scaling laws for the reconnection rate, outflow speed, the density of the outflow, and the structure of the dissipation region are derived from first principles. These results are independent of the dissipation mechanism. It is shown that a generic feature of asymmetric reconnection is that the X-line and stagnation point are not colocated, leading to a bulk flow of plasma across the X-line. The scaling laws are verified using two-dimensional resistive magnetohydrodynamics numerical simulations for the special case of asymmetric magnetic fields with symmetric density. Observational signatures and applications to reconnection in the magnetosphere are discussed. (C) 2007 American Institute of Physics.
引用
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页数:11
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