Comparison of Damping Mechanisms for Transverse Waves in Solar Coronal Loops
We present a method to assess the plausibility of alternative mechanisms to explain the damping of magnetohydrodynamic transverse waves in solar coronal loops. The considered mechanisms are resonant absorption of kink waves in the Alfvén continuum, phase mixing of Alfvén waves, and wave leakage. Our methods make use of Bayesian inference and model
Montes-Solís, M. et al.
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2017