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Sun-as-a-Star Spectral Line Variability in the 300–2390 nm Wavelength Range
Sergey V. Marchenko, Antje Ludewig, Serena Criscuoli, Khaled Al Moulla, Debi P. Choudhary, Matthew T. DeLand, Greg Kopp, Erwin Loots, Emiel van der Plas and Pepijn Veefkind The Astrophysical Journal 977(1) 33 (2024) https://doi.org/10.3847/1538-4357/ad888f
Modeling Stellar Ca ii H and K Emission Variations. I. Effect of Inclination on the S-index
K. Sowmya, A. I. Shapiro, V. Witzke, N.-E. Nèmec, T. Chatzistergos, K. L. Yeo, N. A. Krivova and S. K. Solanki The Astrophysical Journal 914(1) 21 (2021) https://doi.org/10.3847/1538-4357/abf247
Predictions of Astrometric Jitter for Sun-like Stars. I. The Model and Its Application to the Sun as Seen from the Ecliptic
Kyiv monitoring program of spectral line variations with the 11-year cycle
Nataliia Shchukina, Sergej Osipov, Roman Kostyk and Myroslav Stodilka Proceedings of the International Astronomical Union 13(S340) 31 (2018) https://doi.org/10.1017/S1743921318001369
Are solar brightness variations faculae- or spot-dominated?