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Coronal Abundances in an Active Region: Evolution and Underlying Chromospheric and Transition Region Properties

The element abundances in the solar corona and solar wind are often different from those of the solar photosphere, typically with a relative enrichment of elements with low first ionization potential (FIP effect). Here, we study the spatial distribution and temporal evolution of the coronal chemical...

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Bibliografiske detaljer
Principais autores: Paola Testa, Juan Martínez-Sykora, Bart De Pontieu
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2023-01-01
Serier:The Astrophysical Journal
Fag:
Online adgang:https://doi.org/10.3847/1538-4357/acb343
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