English

Resistive instabilities in sinusoidal shear flows with a streamwise magnetic field

Fluid Dynamics 2022-10-19 v1 Earth and Planetary Astrophysics Solar and Stellar Astrophysics Plasma Physics

Abstract

We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be unstable to the Kelvin-Helmholtz instability in the hydrodynamic case. The same is true in ideal MHD, where dissipation is neglected, provided the magnetic field strength does not exceed a critical threshold beyond which magnetic tension stabilizes the flow. Here, we demonstrate that including viscosity and resistivity introduces two new modes of instability. One of these modes, which we call a resistively-unstable Alfv\'en wave due to its connection to shear Alfv\'en waves, exists for any nonzero magnetic field strength as long as the magnetic Prandtl number Pm<1Pm < 1. We present a reduced model for this instability that reveals its excitation mechanism to be the negative eddy viscosity of periodic shear flows described by Dubrulle & Frisch (1991). Finally, we demonstrate numerically that this mode saturates in a quasi-stationary state dominated by counter-propagating solitons.

Keywords

Cite

@article{arxiv.2204.10875,
  title  = {Resistive instabilities in sinusoidal shear flows with a streamwise magnetic field},
  author = {Adrian E. Fraser and Imogen G. Cresswell and Pascale Garaud},
  journal= {arXiv preprint arXiv:2204.10875},
  year   = {2022}
}

Comments

23 pages, 10 figures, submitted to JFM

R2 v1 2026-06-24T10:56:16.520Z