Gyrokinetic simulations of magnetic reconnection

被引:39
|
作者
Pueschel, M. J. [1 ,2 ]
Jenko, F. [1 ]
Told, D. [1 ]
Buechner, J. [2 ]
机构
[1] EURATOM, Max Planck Inst Plasmaphys, D-85748 Garching, Germany
[2] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
关键词
magnetic reconnection; plasma kinetic theory; plasma magnetohydrodynamics; plasma simulation; plasma transport processes; plasma turbulence; Vlasov equation; PLASMA; EQUATIONS; WAVES;
D O I
10.1063/1.3656965
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
Fast magnetic reconnection, believed to be a mechanism for rearranging the magnetic topology and creating energetic particles in many astrophysical and laboratory plasmas, is investigated with the nonlinear gyrokinetic code Gene. After some code-code benchmarking, extensive linear studies are presented, covering all relevant parameter dependencies of two-dimensional slab reconnection. The results are used to ascertain the validity of a fluid model and understand for which parameters it fails to describe the physics correctly. The nonlinear phase is studied for two scenarios: decaying and driven turbulence. In the former case, the initially injected energy is cascading towards the largest scales of the system, whereas a fully turbulent, quasi-stationary state develops if the system is driven through a Krook-type term in the gyrokinetic Vlasov equation. (C) 2011 American Institute of Physics. [doi:10.1063/1.3656965]
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页数:13
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