A shallow water model for magnetohydrodynamic flows with turbulent Hartmann layers

TL;DR

This paper introduces a new shallow water model for magnetohydrodynamic flows with turbulent Hartmann layers, successfully matching experimental dissipation levels and revealing turbulence effects on flow dynamics.

Contribution

The authors develop a simplified shallow water model incorporating turbulent Hartmann layers using Prandtl's mixing length, improving upon previous laminar assumptions.

Findings

Model accurately predicts experimental angular momentum and velocity.

Turbulence in Hartmann layers explains dissipation discrepancies.

Turbulent friction limits large-scale turbulence.

Abstract

We establish a shallow water model for flows of electrically conducting fluids in homogeneous static magnetic fields that are confined between two parallel planes where turbulent Hartmann layers are present. This is achieved by modelling the wall shear stress in these layers using the Prandtl's mixing length model, as did the authors of Albousssi\`ere \& Lingwood (Phys. Fluids, 2000). The idea for this new model arose from the failure of previous shallow water models that assumed a laminar Hartmann layer to recover the correct amount of dissipation found in some regimes of the MATUR experiment. This experiment, conducted by the authors of Messadek \& Moreau (J. Fluid Mech. 2002), consisted of a thin layer of mercury electrically driven in differential rotation in a transverse magnetic field. Numerical Simulations of our new model in the configuration of this experiment allowed us to recover experimental values of both the global angular momentum and the local velocity up to a few percent when the Hartmann layer was in a sufficiently well developed turbulent state. We thus provide an evidence that the unexplained level of dissipation observed in MATUR in these specific regimes was caused by turbulence in the Hartmann layers. A parametric analysis of the flow, made possible by the simplicity of our model, also revealed that turbulent friction in the Hartmann layer prevented quasi-2D turbulence from becoming more intense and limited the size of the large scales.