Abstract
The present work discusses the basic physical mechanisms which produce the heating of stellar chromospheres and coronae. As extensive reviews on this subject have been published elsewhere (Narain & Ulmschneider [2], (Paper I), Narain & Ulmschneider [3] (Paper II) as well as Ulmschneider [4] (Paper III)) the present paper concentrates on the physics of the heating processes. For additional literature as well as for additional reviews see Papers I to III. Section 2 discusses the necessity of chromospheric and coronal heating and describes the elementary heating processes. Section 3 outlines the hydrodynamic heating mechanisms and Section 4 the magnetic heating mechanisms.
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References
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© 1997 Kluwer Academic Publishers
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Ulmschneider, P. (1997). Chromospheric and Coronal Heating Mechanisms. In: Mouradian, Z., Stavinschi, M. (eds) Theoretical and Observational Problems Related to Solar Eclipses. NATO ASI Series, vol 494. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5492-5_17
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DOI: https://doi.org/10.1007/978-94-011-5492-5_17
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-4619-7
Online ISBN: 978-94-011-5492-5
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