The Slowly Varying Corona. II. The Components of F 10.7 and Their Use in EUV Proxies
Author:
Funder
AFOSR LRIR
AFOSR
NSF Career Award
PAARE NSF
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab3af9/pdf
Reference94 articles.
1. The Chemical Composition of the Sun
2. Ionospheric evidence for a nonlinear relationship between the solar e.u.v. and 10.7 cm fluxes during an intense solar cycle
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