Dynamics of nonlinearly interacting magnetic electron drift vortex modes in a nonuniform plasma

被引:3
|
作者
Eliasson, B. [1 ,2 ]
Shukla, P. K. [1 ,2 ,3 ,4 ]
Pavlenko, V. P. [5 ]
机构
[1] Ruhr Univ Bochum, Inst Theoret Phys 4, D-44780 Bochum, Germany
[2] Umea Univ, Dept Phys, SE-90187 Umea, Sweden
[3] Univ Strathclyde, Dept Phys, SUPA, Glasgow G4 0NG, Lanark, Scotland
[4] Univ KwaZulu Natal, Sch Phys, ZA-4000 Durban, South Africa
[5] Uppsala Univ, Dept Phys & Astron, SE-75120 Uppsala, Sweden
基金
瑞典研究理事会;
关键词
LARGE-SCALE STRUCTURE; WEIBEL INSTABILITY; FIELDS; TURBULENCE; WAVES; GENERATION;
D O I
10.1063/1.3103785
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 simulation study of dynamical evolution of nonlinearly interacting two-dimensional magnetic electron drift vortex (MEDV) modes in a nonuniform plasma is presented. Depending on the equilibrium density and temperature gradients, the system can either be stable or unstable. The unstable system reveals spontaneous generation of magnetic fields from noise level, and large-scale magnetic field structures are formed. When the system is linearly stable, one encounters MEDV mode turbulence in which there is a competition between zonons (zonal flows) and streamers. For large MEDV mode amplitudes, one encounters the formation of localized and small-scale magnetic vortices and vortex pairs with scale sizes of the order of the electron skin depth. The MEDV turbulence exhibits nonuniversal (non-Kolmogorov-type) spectra for different sets of plasma parameters. The relevance of this work to laboratory and cosmic plasmas is briefly mentioned. (C) 2009 American Institute of Physics. [DOI: 10.1063/1.3103785]
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页数:8
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