中文

Self-similar turbulent dynamo

混沌动力学 2009-11-10 v3 天体物理学 流体动力学

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.

关键词

引用

@article{arxiv.nlin/0306059,
  title  = {Self-similar turbulent dynamo},
  author = {A. A. Schekochihin and S. C. Cowley and J. L. Maron and J. C. McWilliams},
  journal= {arXiv preprint arXiv:nlin/0306059},
  year   = {2009}
}

备注

revtex, 4 pages, 5 figures; minor changes to match published version