Active modes and dynamical balances in MRI-turbulence of Keplerian disks with a net vertical magnetic field
D. Gogichaishvili, G. Mamatsashvili, W. Horton, G. Chagelishvili

TL;DR
This paper analyzes MRI turbulence in Keplerian disks with a net vertical magnetic field, identifying three key active modes and their interactions, revealing the balance of linear and nonlinear processes shaping turbulence dynamics.
Contribution
It introduces a Fourier-space analysis of active modes in MRI turbulence, highlighting the roles of channel, zonal flow, and rest modes and their interplay in the turbulence dynamics.
Findings
Three types of active modes identified: channel, zonal flow, rest modes.
Rest modes collectively dominate energy transfer despite individual insignificance.
Nonlinear transverse cascade redistributes energy, opposing linear MRI growth.
Abstract
We studied dynamical balances in magnetorotational instability (MRI) turbulence with a net vertical field in the shearing box model of disks. Analyzing the turbulence dynamics in Fourier (-)space, we identified three types of active modes that define turbulence characteristics. These modes have lengths similar to the box size, i.e., lie in the small wavenumber region in Fourier space labeled the vital area and are: (i) the channel mode - uniform in the disk plane with the smallest vertical wavenumber,(ii) the zonal flow mode - azimuthally and vertically uniform with the smallest radial wavenumber and (iii) the rest modes. The rest modes comprise those harmonics in the vital area whose energies reach more than of the maximum spectral energy. The rest modes individually are not so significant compared to the channel and zonal flow modes, however, the combined action of…
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