Fundamental scales in the kinematic phase of the turbulent dynamo
arXiv:2204.00828 · doi:10.1093/mnras/stac969 10.1093/mnras/stac969 10.1093/mnras/stac969 10.1093/mnras/stac969
Abstract
The turbulent dynamo is a powerful mechanism that converts turbulent kinetic energy to magnetic energy. A key question regarding the magnetic field amplification by turbulence, is, on what scale, , do magnetic fields become most concentrated? There has been some disagreement about whether is controlled by the viscous scale, (where turbulent kinetic energy dissipates), or the resistive scale, (where magnetic fields dissipate). Here we use direct numerical simulations of magnetohydrodynamic turbulence to measure characteristic scales in the kinematic phase of the turbulent dynamo. We run -simulations with hydrodynamic Reynolds numbers of , and magnetic Reynolds numbers of , to explore the dependence of on and . Using physically motivated models for the kinetic and magnetic energy spectra, we measure , and , making sure that the obtained scales are numerically converged. We determine the overall dissipation scale relations and , where is the turbulence driving wavenumber and is the magnetic Prandtl number. We demonstrate that the principle dependence of is on . For plasmas where , we find that , with the proportionality constant related to the power-law `Kazantsev' exponent of the magnetic power spectrum. Throughout this study, we find a dichotomy in the fundamental properties of the dynamo where , compared to . We report a minimum critical hydrodynamic Reynolds number, for bonafide turbulent dynamo action.
arXiv comment15 pages, 10 figures; accepted for publication in MNRAS, 2022 April 4
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