Gyro-induced acceleration of magnetic reconnection

被引:37
作者
Comisso, L. [1 ,2 ]
Grasso, D. [1 ,2 ]
Waelbroeck, F. L. [3 ]
Borgogno, D. [1 ]
机构
[1] Politecn Torino, Dipartimento Energia, I-10129 Turin, Italy
[2] CNR, Ist Sistemi Complessi, I-00185 Rome, Italy
[3] Univ Texas Austin, Inst Fus Studies, Austin, TX 78712 USA
关键词
COLLISIONLESS RECONNECTION; IMPULSIVE RECONNECTION; NONLINEAR DYNAMICS; M=1 MODES; INSTABILITIES; COLLAPSE;
D O I
10.1063/1.4821840
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
The linear and nonlinear evolution of magnetic reconnection in collisionless high-temperature plasmas with a strong guide field is analyzed on the basis of a two-dimensional gyrofluid model. The linear growth rate of the reconnecting instability is compared to analytical calculations over the whole spectrum of linearly unstable wave numbers. In the strongly unstable regime (large Delta'), the nonlinear evolution of the reconnecting instability is found to undergo two distinctive acceleration phases separated by a stall phase in which the instantaneous growth rate decreases. The first acceleration phase is caused by the formation of strong electric fields close to the X-point due to ion gyration, while the second acceleration phase is driven by the development of an open Petschek-like configuration due to both ion and electron temperature effects. Furthermore, the maximum instantaneous growth rate is found to increase dramatically over its linear value for decreasing diffusion layers. This is a consequence of the fact that the peak instantaneous growth rate becomes weakly dependent on the microscopic plasma parameters if the diffusion region thickness is sufficiently smaller than the equilibrium magnetic field scale length. When this condition is satisfied, the peak reconnection rate asymptotes to a constant value. (C) 2013 AIP Publishing LLC.
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页数:14
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