Magnetic Reconnection between a Solar Jet and a Filament Channel

Magnetic Reconnection between a Solar Jet and a Filament Channel

The solar corona is highly structured by bunches of magnetic field lines forming either loops, or twisted flux ropes representing prominences/filaments, or very dynamic structures such as jets. The aim of this paper is to understand the interaction between filament channels and jets. We use high-res...

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Bibliographic Details
Main Authors: Garima Karki, Brigitte Schmieder, Pooja Devi, Ramesh Chandra, Nicolas Labrosse, Reetika Joshi, Bernard Gelly
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar active regions
Online Access:https://doi.org/10.3847/1538-4357/ada28e
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