Understanding the Relationship between Solar Coronal Abundances and F10.7 cm Radio Emission

Sun-as-a-star coronal plasma composition, derived from full-Sun spectra, and the F10.7 radio flux (2.8 GHz) have been shown to be highly correlated ( r = 0.88) during solar cycle 24. However, this correlation becomes nonlinear during increased solar magnetic activity. Here we use cotemporal, high sp...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Andy S. H. To, Alexander W. James, T. S. Bastian, Lidia van Driel-Gesztelyi, David M. Long, Deborah Baker, David H. Brooks, Samantha Lomuscio, David Stansby, Gherardo Valori
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Subjects:	Solar corona Solar magnetic fields Solar radio emission Solar abundances
Online Access:	https://doi.org/10.3847/1538-4357/acbc1b