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A semi-analytical model of stellar flares

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Surface Inhomogeneities on Late-Type Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 397))

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References

  • Kopp, R.A., Poletto, G.: 1990, in Mechanisms of Chromospheric and Coronal Heating, P. Ulmschneider. Ed., in press.

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  • Pallavicini, R., Peres, G., Serio, S., Vaiana, G., Acton, L., Leibacher, J., Rosner, R.: 1983, ApJ, 270, 270

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  • Pallavicini, R., Tagliaferri, G., Stella, L.: 1990, A&A, 191, 109

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  • Reale, F., Peres, G., Serio, S., Rosner, R., Schmitt, J.H.M.M.: 1988, ApJ, 328, 256

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Authors and Affiliations

  1. Los Alamos National Laboratory, 87545, Los Alamos, NM, USA

    R. A. Kopp

  2. Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125, Firenze, Italy

    G. Poletto

Authors
  1. R. A. Kopp
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  2. G. Poletto
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Patrick B. Byrne Dermott J. Mullan

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© 1992 Springer-Verlag

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Kopp, R.A., Poletto, G. (1992). A semi-analytical model of stellar flares. In: Byrne, P.B., Mullan, D.J. (eds) Surface Inhomogeneities on Late-Type Stars. Lecture Notes in Physics, vol 397. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55310-X_175

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  • DOI: https://doi.org/10.1007/3-540-55310-X_175

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-55310-6

  • Online ISBN: 978-3-540-47025-0

  • eBook Packages: Springer Book Archive

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