Finite Plasma β Three-dimensional Magnetic Field Extrapolation Based on the Magnetohydrodynamic Relaxation Method

The three-dimensional (3D) magnetic field in the solar atmosphere provides crucial information to help understand explosive phenomena such as solar flares and coronal mass ejections. Since it is still hard to determine the 3D magnetic field from direct observation, a nonlinear force-free field (NLFF...

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Bibliografische Detailangaben

Hauptverfasser:	Daiki Yamasaki, Takahiro Miyoshi, Satoshi Inoue
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2026-01-01
Schriftenreihe:	The Astrophysical Journal Supplement Series
Schlagworte:	Solar magnetic fields Solar corona Solar chromosphere Magnetohydrodynamics
Online-Zugang:	https://doi.org/10.3847/1538-4365/ae34ae
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