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astro-ph.SR2024
Magnetic Reconnection between a Solar Jet and a Filament Channel
Garima Karki, Brigitte Schmieder, Pooja Devi +4
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…
astro-ph.SR2024
Direct evidence of hybrid nature of EUV waves and the reflection of the fast-mode wave
Ramesh Chandra, P. F. Chen, Pooja Devi
We performed an analysis of the extreme-ultraviolet (EUV) wave event on 2022 March 31. The event originated from active region (AR) 12975 located at N13W52 in the field of view of…