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Chromospheric and Coronal Heating Mechanisms

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Part of the book series: NATO ASI Series ((ASIC,volume 494))

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

  1. Chen, F.F. (1984), Introduction to Plasma Physics and Controlled Fusion 2ed, Vol 1, Plasma Physics, Plenum Press, New York

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  2. Narain, U., Ulmschneider, P. (1990), Space Sci. Rev. 54, 377 (Paper I)

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  3. Narain, U., Ulmschneider, P. ); (1996), Space Sci. Rev. 75, 453 (Paper II)

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  4. Ulmschneider, P. (1996), in: Cool Stars Stellar Systems and the Sun, ASP Conf. Ser., R. Pallavicini, A.K. Dupree (eds.) in press (Paper III)

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  5. Parker, E.N. (1992), J. Geophys. Res. 97, 4311

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  6. Priest, E.R. (1991), in Mechanisms of Chromospheric and Coronal Heating, Ulmschneider P., Priest E.R., Rosner R., (eds.) Springer, Berlin, p 520

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  7. Strauss, H.R. (1991), Geophys. Res. Let. 18, 77

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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

  • eBook Packages: Springer Book Archive

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