Self-similar turbulent dynamo

被引:9
作者
Schekochihin, AA
Cowley, SC
Maron, JL
McWilliams, JC
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Plasma Phys Grp, London SW7 2BW, England
[2] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[3] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
[4] Univ Iowa, Dept Phys & Astron, Ctr Magnet Reconnect Studies, Iowa City, IA 52242 USA
[5] Univ Calif Los Angeles, Dept Atmospher Sci, Los Angeles, CA 90095 USA
关键词
D O I
10.1103/PhysRevLett.92.064501
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The amplification of magnetic fields in a highly conducting fluid is studied numerically. During growth, the magnetic field is spatially intermittent: it does not uniformly fill the volume, but is concentrated in long thin folded structures. Contrary to a commonly held view, intermittency of the folded field does not increase indefinitely throughout the growth stage if diffusion is present. Instead, as we show, the probability-density function (PDF) of the field-strength becomes self-similar. The normalized moments increase with magnetic Prandtl number in a powerlike fashion. We argue that the self-similarity is to be expected with a finite flow scale and system size. In the nonlinear saturated state, intermittency is reduced and the PDF is exponential. Parallels are noted with self-similar behavior recently observed for passive-scalar mixing and for map dynamos.
引用
收藏
页码:645011 / 645014
页数:4
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