Transport properties of Keplerian flows in extended local domains with no imposed field
Farrukh Nauman, Martin E. Pessah

TL;DR
This study investigates how the transport properties of Keplerian flows in elongated shearing boxes depend on Reynolds number, magnetic Prandtl number, and aspect ratios, revealing that turbulence saturation is sensitive to these parameters.
Contribution
It provides new insights into the dependence of turbulent transport on aspect ratio and dissipation coefficients in extended local domains without imposed magnetic fields.
Findings
Transport coefficients vary with aspect ratio and dissipation parameters.
Turbulent stresses follow a power law with magnetic Prandtl number for Pm > 1.
Saturated turbulence levels are roughly invariant with aspect ratio changes.
Abstract
We compare transport statistics of elongated incompressible shearing boxes for different Reynolds and magnetic Prandtl numbers, and , and aspect ratios, . We find that at fixed aspect ratio and , the turbulent stresses for do not show considerable variation and follow a power law for . This is qualitatively consistent with previous results based on net imposed flux and small box simulations but the power law exponent is different. The saturated level of stresses, the ratio of Maxwell stress to the magnetic energy and Reynolds to Maxwell stress ratio are roughly invariant as is increased. For cases where the boxes are elongated in both the azimuth and vertical direction, the transport coefficient that is times larger than the case with $L_y/L_x =…
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