A mean-field approach to the propagation of field patterns in stratified magneto rotational turbulence
Oliver Gressel

TL;DR
This paper develops a mean-field model to explain cyclic magnetic field patterns in stratified magneto-rotational turbulence, revealing multiple dynamo mechanisms and successfully reproducing observed field behaviors.
Contribution
It introduces a mean-field approach with closure parameters derived via the test field method to explain field pattern propagation and saturation in MRI turbulence.
Findings
Identifies two distinct dynamo mechanisms in stratified MRI turbulence.
Successfully reproduces observed magnetic field patterns and parity in simulations.
Provides insights into the saturation process of MRI-induced turbulence.
Abstract
Local shearing box simulations of stratified magneto rotational turbulence invariably exhibit cyclic field patterns which propagate away from the disc midplane. A common explanation for this is magnetic buoyancy. The recent analysis by Shi et al. however shows that the flow is buoyantly stable below one disc scale height H, necessitating an alternative explanation in this region. We here conduct and analyse direct numerical simulations to explain the observed behaviour by means of a mean-field description. Apart from the mean radial and azimuthal field, we monitor the small-scale current helicity, which we propose as a key indicator for saturation. Reconstructing the horizontally averaged field, we demonstrate that the problem can be reduced to a one-dimensional induction equation. By means of the so-called test field method, we then determine the underlying closure parameters. Our…
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