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Modeling Time-variable Elemental Abundances in Coronal Loop Simulations

Numerous recent X-ray observations of coronal loops in both active regions and solar flares have shown clearly that elemental abundances vary with time. Over the course of a flare, they have been found to move from coronal values toward photospheric values near the flare peak, before slowly returnin...

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Auteurs principaux: Jeffrey W. Reep, John Unverferth, Will T. Barnes, Sherry Chhabra
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2024-01-01
Collection:The Astrophysical Journal Letters
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Accès en ligne:https://doi.org/10.3847/2041-8213/ad64c3
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