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The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field

Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms. Particularly, some geomagnetic storms might be induced by solar filament eruptions originating from unexpected surface source regions because o...

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Principais autores: Ye Qiu, Yang Guo, Mingde Ding, Chuan Li, Linggao Kong, Zhen Li
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2025-01-01
coleção:The Astrophysical Journal
Assuntos:
Solar filaments
Solar filament eruptions
Solar magnetic fields
Solar coronal mass ejections
Solar flares
Acesso em linha:https://doi.org/10.3847/1538-4357/adfd54
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