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Solar Flare Ribbon Fronts. II. Evolution of Heating Rates in Individual Flare Footpoints

Solar flare ribbon fronts appear ahead of the bright structures that normally characterize solar flares, and can persist for an extended period of time in spatially localized patches before transitioning to “regular” bright ribbons. They likely represent the initial onset of flare energy deposition...

Ausführliche Beschreibung

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Bibliografische Detailangaben
Hauptverfasser: Graham S. Kerr, Vanessa Polito, Yan Xu, Joel C. Allred
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2024-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/ad47e1
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