Understanding the Magnetic Field and Plasma-β along Umbral Fan Loops Traced Using 3 Minute Slow Waves

Plasma- β is an important fundamental physical quantity in solar plasma physics, which determines the dominating process in the solar atmosphere, i.e., magnetic or thermodynamic processes. Here, for the first time, we provide variations of magnetic field and plasma- β along magnetically structured l...

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Detalhes bibliográficos

Principais autores:	Ananya Rawat, Girjesh Gupta, Tom Van Doorsselaere, S. Krishna Prasad, Robertus Erdélyi
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal Letters
Assuntos:	Solar atmosphere Sunspots Solar coronal loops Magnetohydrodynamics Solar magnetic fields
Acesso em linha:	https://doi.org/10.3847/2041-8213/ade9be
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