A comparison of pendulum models for large-amplitude longitudinal prominence oscillations

Large-amplitude prominence oscillations offer diagnostic information relevant to understanding the magnetic and plasma structure of solar prominences. Accurate prominence seismology requires the use of reliable models. The so-called pendulum model for large-amplitude longitudinal prominence oscillat...

Ausführliche Beschreibung

Bibliografische Detailangaben

1. Verfasser:	Arregui Iñigo
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	EDP Sciences 2026-04-01
Schriftenreihe:	Astronomy & Astrophysics
Schlagworte:	magnetohydrodynamics (mhd) methods: statistical sun: filaments prominences sun: oscillations
Online-Zugang:	https://www.aanda.org/articles/aa/full_html/2026/04/aa59882-26/aa59882-26.html
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