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

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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Bibliographic Details
Main Authors: Ananya Rawat, Girjesh Gupta, Tom Van Doorsselaere, S. Krishna Prasad, Robertus Erdélyi
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar atmosphere
Sunspots
Solar coronal loops
Magnetohydrodynamics
Solar magnetic fields
Online Access:https://doi.org/10.3847/2041-8213/ade9be
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https://doi.org/10.3847/2041-8213/ade9be

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