Effect of magnetic twist on nonlinear transverse kink oscillations
J. Terradas, N. Magyar, T. Van Doorsselaere

TL;DR
This paper investigates how magnetic twist influences nonlinear transverse kink oscillations in solar magnetic tubes, showing that twist delays shear instabilities and affects their development depending on the inhomogeneous layer thickness.
Contribution
It provides a comprehensive analysis of magnetic twist effects on nonlinear kink oscillations, including energy transfer and shear instability development in different layer configurations.
Findings
Twist delays shear instability onset.
Effect of twist is stronger with thicker inhomogeneous layers.
Moderate twist has limited impact on thin layers.
Abstract
Magnetic twist is thought to play an important role in many structures of the solar atmosphere. One of the effects of twist is to modify the properties of the eigenmodes of magnetic tubes. In the linear regime standing kink solutions are characterized by a change in polarization of the transverse displacement along the twisted tube. In the nonlinear regime, magnetic twist affects the development of shear instabilities that appear at the tube boundary when it is oscillating laterally. These Kelvin-Helmholtz instabilities (KHI) are produced either by the jump in the azimuthal component of the velocity at the edge of the sharp boundary between the internal and external part of the tube, or either by the continuous small length-scales produced by phase-mixing when there is a smooth inhomogeneous layer. In this work the effect of twist is consistently investigated by solving the…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics
