Large scale dynamo action precedes turbulence in shearing box simulations of the magnetorotational instability
Pallavi Bhat, Fatima Ebrahimi, and Eric G. Blackman

TL;DR
This study reveals that large scale magnetic fields grow during the early MRI phase in shearing box simulations, driven by linear modes before turbulence develops, challenging previous assumptions about the turbulence-dynamo relationship.
Contribution
It demonstrates the presence of large scale dynamo action in MRI simulations during the linear growth phase, prior to turbulence, using both horizontal and vertical averaging methods.
Findings
Large scale fields grow during MRI's early phase.
Growth driven by linear fluctuations, not turbulence.
Vertical averaging reveals feedback of MRI modes on initial fields.
Abstract
We study the dynamo generation (exponential growth) of large scale (planar averaged) fields in unstratified shearing box simulations of the magnetorotational instability (MRI). In contrast to previous studies restricted to horizontal (-) averaging, we demonstrate the presence of large scale fields when either horizontal or vertical (-) averaging is employed. By computing planar averaged fields and power spectra, we find large scale dynamo action in the early MRI growth phase---a previously unidentified feature. Fast growing horizontal low modes and fiducial vertical modes over a narrow range of wave numbers amplify these planar averaged fields in the MRI growth phase, before turbulence sets in. The large scale field growth requires linear fluctuations but not nonlinear turbulence (as defined by mode-mode coupling) and grows as a direct global mode of the MRI. Only by…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Aeolian processes and effects
