On the nature of kink MHD waves in magnetic flux tubes
M. Goossens, J. Terradas, J. Andries, I. Arregui, J. L. Ballester

TL;DR
This paper investigates the true nature of MHD kink waves in magnetic flux tubes, revealing they are primarily Alfvénic with mixed properties, challenging traditional classifications and emphasizing their robustness across different plasma conditions.
Contribution
The study provides a comprehensive analysis of MHD kink waves, showing they are mainly incompressible and Alfvénic, with implications for their identification and understanding in solar atmospheric phenomena.
Findings
Kink waves are predominantly incompressible with horizontal motions.
The main restoring force for kink waves is magnetic tension.
Kink waves exhibit mixed properties and are not strictly fast or Alfvénic.
Abstract
Magnetohydrodynamic (MHD) waves are often reported in the solar atmosphere and usually classified as slow, fast, or Alfv\'en. The possibility that these waves have mixed properties is often ignored. The goal of this work is to study and determine the nature of MHD kink waves. This is done by calculating the frequency, the damping rate and the eigenfunctions of MHD kink waves for three widely different MHD waves cases: a compressible pressure-less plasma, an incompressible plasma and a compressible plasma with non-zero plasma pressure which allows for MHD radiation. In all three cases the frequency and the damping rate are for practical purposes the same as they differ at most by terms proportional to . In the magnetic flux tube the kink waves are in all three cases, to a high degree of accuracy incompressible waves with negligible pressure perturbations and with mainly…
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Taxonomy
TopicsMagnetic confinement fusion research · Superconducting Materials and Applications · Solar and Space Plasma Dynamics
