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arxiv: 1701.08996 · v1 · pith:5RXSOVUBnew · submitted 2017-01-31 · ⚛️ physics.flu-dyn · astro-ph.EP· astro-ph.SR· physics.geo-ph

The onset of turbulent rotating dynamos at the low Pm limit

classification ⚛️ physics.flu-dyn astro-ph.EPastro-ph.SRphysics.geo-ph
keywords numberdynamoflowreynoldsturbulentbehaviourevenhigh
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We demonstrate that the critical magnetic Reynolds number $Rm_c$ for a turbulent non-helical dynamo in the low magnetic Prandtl number $Pm$ limit (i.e. $Pm = Rm/Re \ll 1$) can be significantly reduced if the flow is submitted to global rotation. Even for moderate rotation rates the required energy injection rate can be reduced by a factor more than $10^3$. This strong decrease of the onset is attributed to the reduction of the turbulent fluctuations that makes the flow to have a much larger cut-off length-scale compared to a non-rotating flow of the same Reynolds number. The dynamo thus behaves as if it is driven by laminar behaviour (i.e. high $Pm$ behaviour) even at high values of the Reynolds number (i.e. at low values of $Pm$). Our finding thus points into a new paradigm for the design of new liquid metal dynamo experiments.

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