Do mean-field dynamos in nonrotating turbulent shear-flows exist?

被引:46
作者
Ruediger, G.
Kitchatinov, L. L.
机构
[1] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
[2] Inst Solar Terr Phys, Irkutsk 664033, Russia
关键词
magnetic fields; magnetohydrodynamics; general : physical data and processes;
D O I
10.1002/asna.200610527
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A plane-shear flow in a fluid with forced turbulence is considered. If the fluid is electrically-conducting then a mean electromotive force (EMF) results even without basic rotation and the magnetic diffusivity becomes a highly anisotropic tensor. It is checked whether in this case self-excitation of a large-scale magnetic field is possible (so-called (W) over bar x (J) over bar- dynamo) and the answer is NO. The calculations reveal the cross-stream components of the EMF perpendicular to the mean current having the wrong signs, at least for small magnetic Prandtl numbers. After our results numerical simulations with magnetic Prandtl number of about unity have only a restricted meaning as the Prandtl number dependence of the diffusivity tensor is rather strong. If, on the other hand, the turbulence field is stratified in the vertical direction then a dynamo-active Cc-effect is produced. The critical magnetic Reynolds number for such a self-excitation in a simple shear flow is slightly above 10 like for the other - but much more complicated - flow patterns used in existing dynamo experiments with liquid sodium or gallium. (c) 2006 WILEY VCH Verlag GmbH & Co. KGaA, Weinheim.
引用
收藏
页码:298 / 303
页数:6
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