Analysis of the effect of a mean velocity field on a mean field dynamo

被引:1
|
作者
Kandus, Alejandra [1 ]
机构
[1] Univ Estadual Santa Cruz, Dept Ciencias Exactas & Technol, Lab Astrofis Teor & Observ, BR-45662000 Salobrinho, BA, Brazil
关键词
magnetic fields; MHD; turbulence;
D O I
10.1111/j.1365-2966.2007.11863.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study semi-analytically and in a consistent manner the generation of a mean velocity field (U) over bar by helical magnetohydrodynamical (MHD) turbulence, and the effect that this field can have on a mean field dynamo. Assuming a prescribed, maximally helical small-scale velocity field, we show that large-scale flows can be generated in MHD turbulent flows via small-scale Lorentz force. These flows back-react on the mean electromotive force of a mean field dynamo through new terms, leaving the original alpha and beta terms explicitly unmodified. Cross-helicity plays the key role in interconnecting all the effects. In the minimal tau closure that we chose to work with, the effects are stronger for large relaxation times.
引用
收藏
页码:1356 / 1364
页数:9
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