Formation of Polar Crown Filament Magnetic Fields by Supergranular Helicity Injection

Formation of Polar Crown Filament Magnetic Fields by Supergranular Helicity Injection

To understand the magnetic fields of the polar crown filaments (PCFs) at high latitudes near polar regions of the Sun, we perform magnetofrictional numerical simulations on the long-term magnetic evolution of bipolar fields with roughly east–west polarity inversion lines (PILs) in a 3D spherical wed...

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Bibliographic Details
Main Authors: Huanxin Chen, Chun Xia, Hechao Chen
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar prominences
Quiescent solar prominence
Supergranulation
Solar magnetic fields
Magnetohydrodynamical simulations
Online Access:https://doi.org/10.3847/1538-4357/ad3352

Internet

https://doi.org/10.3847/1538-4357/ad3352

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