3D Magnetohydrodynamic Wave Propagation and Energy Transport in a Simulated Solar Vortex

3D Magnetohydrodynamic Wave Propagation and Energy Transport in a Simulated Solar Vortex

Magnetic flux tubes in the presence of background rotational flows are abundant throughout the solar atmosphere and may act as conduits for MHD waves to transport energy throughout the solar atmosphere. Here we investigate the contribution from MHD waves to the Poynting flux in a 3D numerical simula...

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Bibliographic Details
Main Authors: Samuel J. Skirvin, Viktor Fedun, Gary Verth, Istvan Ballai
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Magnetohydrodynamics
Solar atmosphere
Solar chromosphere
Solar oscillations
Online Access:https://doi.org/10.3847/1538-4357/adce73
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