Resonantly Damped Kink Magnetohydrodynamic Waves in a Partially Ionized Filament Thread
R. Soler, R. Oliver, and J. L. Ballester

TL;DR
This study investigates how resonant absorption dampens kink magnetohydrodynamic waves in partially ionized solar filament threads, showing that ionization degree has minimal impact on damping at observed wavelengths.
Contribution
First analytical and numerical study of resonant absorption damping of kink MHD waves in partially ionized filament threads.
Findings
Resonant absorption efficiently damps kink waves at typical filament wavelengths.
Partial ionization does not significantly affect resonant damping.
Damping times align with observational data.
Abstract
Transverse oscillations of solar filament and prominence threads have been frequently reported. These oscillations have the common features of being of short period (2-10 min) and being damped after a few periods. Kink magnetohydrodynamic (MHD) wave modes have been proposed as responsible for the observed oscillations, whereas resonant absorption in the Alfven continuum and ion-neutral collisions are the best candidates to be the damping mechanisms. Here, we study both analytically and numerically the time damping of kink MHD waves in a cylindrical, partially ionized filament thread embedded in a coronal environment. The thread model is composed of a straight and thin, homogeneous filament plasma, with a transverse inhomogeneous transitional layer where the plasma physical properties vary continuously from filament to coronal conditions. The magnetic field is homogeneous and parallel to…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
