Numerical simulations of separatrix instabilities in collisionless magnetic reconnection

被引:52
作者
Divin, A. [1 ]
Lapenta, G. [1 ]
Markidis, S. [2 ]
Newman, D. L. [3 ]
Goldman, M. V. [3 ]
机构
[1] Katholieke Univ Leuven, Ctr Plasma Astrofys, B-3001 Louvain, Belgium
[2] KTH Royal Inst Technol, PDC Ctr High Performance Comp, Stockholm, Sweden
[3] Univ Colorado, CIPS, Boulder, CO 80309 USA
关键词
SAUSAGE-LIKE INSTABILITY; ELECTRON; PLASMA; ACCELERATION; FIELD;
D O I
10.1063/1.3698621
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
Electron scale dynamics of magnetic reconnection separatrix jets is studied in this paper. Instabilities developing in directions both parallel and perpendicular to the magnetic field are investigated. Implicit particle-in-cell simulations with realistic electron-to-ion mass ratio are complemented by a set of small scale high resolution runs having the separatrix force balance as the initial condition. A special numerical procedure is developed to introduce the force balance into the small scale runs. Simulations show the development of streaming instabilities and consequent formation of electron holes in the parallel direction. A new electron jet instability develops in the perpendicular direction. The instability is closely related to the electron MHD Kelvin-Helmholtz mode and is destabilized by a flow, perpendicular to magnetic field at the separatrix. Tearing instability of the separatrix electron jet is modulated strongly by the electron MHD Kelvin-Helmholtz mode. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.3698621]
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页数:13
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