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Stellar Chromospheres, Coronae, and Winds

  • Chapter
Physics of the Sun

Part of the book series: Geophysics and Astrophysics Monographs ((GAAM,volume 26))

Abstract

The three subjects listed in the title of this chapter were originally defined for phenomena that are observed in the Sun. Observations of other stars have now been made at a wide range of wavelengths and have revealed that one or more of these phenomena are present in stars of every class.

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Authors and Affiliations

  1. Univ. of Wisconsin, Madison, Wisconsin, 53706, USA

    J. P. Cassinelli

  2. High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, 80303, USA

    K. B. MacGregor

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  1. Center for Space Science and Astrophysics, Stanford University, Stanford, California, USA

    Peter A. Sturrock

  2. High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA

    Thomas E. Holzer  & Dimitri M. Mihalas  & 

  3. Astronomy Department, University of California, Los Angeles, California, USA

    Roger K. Ulrich

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Cassinelli, J.P., MacGregor, K.B. (1986). Stellar Chromospheres, Coronae, and Winds. In: Sturrock, P.A., Holzer, T.E., Mihalas, D.M., Ulrich, R.K. (eds) Physics of the Sun. Geophysics and Astrophysics Monographs, vol 26. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5255-3_3

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