On the Nature of Magnetic Turbulence in Rotating, Shearing Flows
Justin Walker, Geoffroy Lesur, Stanislav Boldyrev

TL;DR
This paper investigates the properties of MRI-driven turbulence in rotating, shearing flows, revealing a dual-component structure with universal fluctuation spectra but system-dependent outer scales, and questions the existence of MRI dynamo at low magnetic Prandtl numbers.
Contribution
It characterizes the dual nature of MRI turbulence, identifies universal spectral properties, and challenges the MRI dynamo's presence at low magnetic Prandtl numbers.
Findings
Turbulence comprises large-scale magnetic fields and small-scale MHD fluctuations.
Fluctuation spectra follow universal power laws: $k^{-2}$ and $k^{-3/2}$.
No sustained dynamo observed at Pm=1 with high Reynolds numbers.
Abstract
The local properties of turbulence driven by the magnetorotational instability (MRI) in rotating, shearing flows are studied in the framework of a shearing-box model. Based on numerical simulations, we propose that the MRI-driven turbulence comprises two components: the large-scale shear-aligned strong magnetic field and the small-scale fluctuations resembling magnetohydrodynamic (MHD) turbulence. The energy spectrum of the large-scale component is close to , whereas the spectrum of the small-scale component agrees with the spectrum of strong MHD turbulence . While the spectrum of the fluctuations is universal, the outer-scale characteristics of the turbulence are not; they depend on the parameters of the system, such as the net magnetic flux. However, there is remarkable universality among the allowed turbulent states -- their intensity and their outer scale…
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