Dissipative Instability of Magnetohydrodynamic Sausage Waves in a Compressional Cylindrical Plasma: Effect of Flow Shear and Viscosity Shear
D. J. Yu

TL;DR
This paper investigates how flow shear and viscosity influence the stability of MHD sausage waves in a cylindrical plasma, revealing conditions under which dissipative instability occurs and deriving analytical dispersion relations.
Contribution
It provides an analytical dispersion relation for slow sausage modes considering viscosity and flow shear, highlighting the nonlinear effects on growth rates.
Findings
Growth rate proportional to axial wavenumber and flow shear for slow surface modes
Peak growth rate at certain axial wavenumber for slow body modes
Nonlinear development of growth rate with increasing flow shear and viscosities
Abstract
The shear flow influences the stability of magnetohydrodynamic (MHD) waves. In the presence of a dissipation mechanism, flow shear may induce a MHD wave instability below the threshold of the Kelvin-Helmholtz instability (KHI), which is called dissipative instability (DI). This phenomenon is also called negative energy wave instability (NEWI) because it is closely related to the backward wave which has negative wave energy. Considering viscosity as a dissipation mechanism, we derive an analytical dispersion relation for the slow sausage modes in a straight cylinder with a discontinuous boundary. It is assumed that the steady flow is inside and dynamic and bulk viscosities are outside the circular flux tube under photospheric condition. When the two viscosities are weak, it is found that for the slow surface mode, the growth rate is proportional to the axial wavenumber and flow shear,…
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