Critical-layer instability of shallow water magnetohydrodynamic shear flows

TL;DR

This paper investigates the instability mechanisms in shallow water magnetohydrodynamic shear flows caused by the interaction of critical levels where wave phase velocity matches Alfvén speeds, highlighting the role of magnetic field curvature.

Contribution

It provides a comprehensive analysis of critical-layer instability in shallow water MHD flows, deriving a general differential equation and elucidating the magnetic field's influence on stability criteria.

Findings

Critical layers can generate instability when they coalesce.

Magnetic field curvature influences the instability mechanism.

The study combines asymptotic and numerical solutions for analysis.

Abstract

In this paper, the instability of shallow water shear flow with a sheared parallel magnetic field is studied. Waves propagating in such magnetic shear flows encounter critical levels where the phase velocity relative to the basic flow $c-U(y)$ matches the Alfv\'en wave velocities $\pm B(y)/\sqrt{\mu\rho}$, based on the local magnetic field $B(y)$, the magnetic permeability $\mu$ and the mass density of the fluid $\rho$. It is shown that when the two critical levels are close to each other, the critical layer can generate an instability. The instability problem is solved, combining asymptotic solutions at large wavenumbers and numerical solutions, and the mechanism of instability explained using the conservation of momentum. For the shallow water MHD system, the paper gives the general form of the local differential equation governing such coalescing critical layers for any generic field and flow profiles, and determines precisely how the magnetic field modifies the purely hydrodynamic stability criterion based on the potential vorticity gradient in the critical layer. The curvature of the magnetic field profile, or equivalently the electric current gradient, $J' = - B''/\mu$ in the critical layer is found to play a complementary role in the instability.