Abstract
This review summarizes the many contact points between solar and stellar physics stressing the similarities and differences between phenomena observed on the Sun and on stars with outer convective mantles. Topics discussed include: 1) the relationship between convection, rotation and magnetic fields as a source of magnetic activity in late-type stars; 2) the observation of solar-type phenomena (spots, plages, activity cycles etc.) on other stars; 3) the structuring and heating of high temperature coronae; 4) the observation and interpretation of radio emission from the Sun and late-type stars.
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Pallavicini, R. (1985). The Solar-Stellar Connection. In: Hjellming, R.M., Gibson, D.M. (eds) Radio Stars. Astrophysics and Space Science Library, vol 116. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5420-5_27
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