Magnetoacoustic wave propagation in the solar corona and filament dynamics

Abstract The formation of a S-shaped filament was investigated to determine if and how magnetoacoustic waves in the solar corona can trigger filament excitation. The study investigated how magnetoacoustic waves interact with two magnetic null points in the solar corona. Since the solar corona has a...

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Bibliographic Details
Main Authors: Sabri Somaiyeh, Poedts Stefaan
Format: Article
Language:English
Published: Nature Portfolio 2024-12-01
Series:Scientific Reports
Subjects:
Online Access:https://doi.org/10.1038/s41598-024-80229-0
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