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Height and Energy Evolution of X-Ray Double Sources in a Solar Flare

In the standard model, magnetic reconnection at a vertical current sheet above the flare arcade is key to explaining many aspects of solar eruptions. The supra-arcade region is where the vertical current sheet is supposedly located, and X-ray/extreme-ultraviolet emission therein reflects underlying...

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Autori principali: Hanya Pan, Astrid M. Veronig, Rui Liu
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2026-01-01
Serie:The Astrophysical Journal
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Accesso online:https://doi.org/10.3847/1538-4357/ae372b
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