First Insights into the Applicability and Importance of Different 3D Magnetic Field Extrapolation Approaches for Studying the Preeruptive Conditions of Solar Active Regions

The three-dimensional (3D) coronal magnetic field has not yet been directly observed. However, for a better understanding and prediction of magnetically driven solar eruptions, 3D models of solar active regions are required. This work aims to provide insight into the significance of different extrap...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Marianna B. Korsós, Robert Jarolim, Robertus Erdélyi, Astrid M. Veronig, Huw Morgan, Francesca Zuccarello
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Solar flares Solar active region magnetic fields Solar active regions
Online Access:	https://doi.org/10.3847/1538-4357/ad18bd