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arxiv: nlin/0306059 · v3 · submitted 2003-06-28 · 🌊 nlin.CD · astro-ph· physics.flu-dyn

Self-similar turbulent dynamo

classification 🌊 nlin.CD astro-phphysics.flu-dyn
keywords fieldmagneticself-similarfoldedgrowthincreaseintermittencyamplification
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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.

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