Abstract
I discuss the results of recent measurements of magnetic fields on cool stars and how these measurements relate to stellar “activity”. Special emphasis is given to the correlations between the magnetic field strength, surface filling factor, and the nonthermal emission from the hot outer atmospheres of these stars.
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© 1988 Kluwer Academic Publishers
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Saar, S.H. (1988). The Magnetic Fields on Cool Stars and Their Correlation with Chromospheric and Coronal Emission. In: Pallavicini, R. (eds) Hot Thin Plasmas in Astrophysics. NATO ASI Series, vol 249. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3065-0_9
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DOI: https://doi.org/10.1007/978-94-009-3065-0_9
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