The Temperature-Dependent Damping of Propagating Slow Magnetoacoustic Waves

The rapid damping of slow magnetoacoustic waves in the solar corona has been extensively studied in previous years. Most studies suggest that thermal conduction is a dominant contributor to this damping, albeit with a few exceptions. Employing extreme-ultraviolet (EUV) imaging data from SDO/AIA, we...

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Bibliographic Details
Main Authors: S. Krishna Prasad, David B. Jess, Tom Van Doorsselaere
Format: Article
Language:English
Published: Frontiers Media S.A. 2019-08-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/fspas.2019.00057/full