Kelvin-Helmholtz instability in solar H-alpha surges
I. Zhelyazkov, T. V. Zaqarashvili, R. Chandra, A. K. Srivastava, T., Mishonov

TL;DR
This paper investigates the conditions under which Kelvin-Helmholtz instability occurs in solar H-alpha surges, modeling the surge as a twisted magnetic flux tube and analyzing the stability of MHD waves.
Contribution
It presents a detailed MHD model of a solar surge as a twisted flux tube and identifies the specific wave modes and flow velocities that lead to KH instability.
Findings
KH instability occurs at flow velocities of 25-50 km/s
Only high negative mode number MHD waves become unstable
Instability occurs at sub-Alfvenic flow speeds
Abstract
We study the evolutionary conditions for Kelvin-Helmholtz (KH) instability in a H-alpha solar surge observed in NOAA AR 8227 on 1998 May 30. The jet with speeds in the range of 45-50 km/s, width of 7 Mm, and electron number density of 3.83 x 10^{10} cm^{-3} is assumed to be confined in a twisted magnetic flux tube embedded in a magnetic field of 7 G. The temperature of the plasma flow is of the order of 10^5 K while that of its environment is taken to be 2 x 10^6 K. The electron number density of surrounding magnetized plasma has a typical for the TR/lower corona region value of 2 x 10^{9} cm^{-3}. Under these conditions, the Alfven speed inside the jet is equal to 78.3 km/s. We model the surge as a moving magnetic flux tube for two magnetic field configurations: (i) a twisted tube surrounded by plasma with homogeneous background magnetic field, and (ii) a twisted tube which environment…
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