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MHD stability of line-tied prominence magnetic fields

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Dynamics of Quiescent Prominences

Part of the book series: Lecture Notes in Physics ((LNP,volume 363))

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References

  1. Low, B. C.: 1981, Astrophys. J. 246, 538.

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  2. De Bruyne, P. and Hood, A. W.: 1989, Solar Phys. 123, 241.

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  3. Bernstein, I. B., Frieman, E. A., Kruskal, M. D., and Kulsrud, R. M.: 1958, Proc. Roy. Soc. London A244, 17.

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  4. De Bruyne, P and Hood, A. W.: 1990, Hvar Obs. Bull., submitted.

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Authors and Affiliations

  1. Department of Mathematical Sciences, University of St. Andrews, KY16 9SS, St. Andrews, Fife, Scotland, U.K.

    P. De Bruyne & A. W. Hood

Authors
  1. P. De Bruyne
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  2. A. W. Hood
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V. Ruždjak E. Tandberg-Hanssen

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© 1990 Springer-Verlag

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De Bruyne, P., Hood, A.W. (1990). MHD stability of line-tied prominence magnetic fields. In: Ruždjak, V., Tandberg-Hanssen, E. (eds) Dynamics of Quiescent Prominences. Lecture Notes in Physics, vol 363. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0025687

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  • DOI: https://doi.org/10.1007/BFb0025687

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-52973-6

  • Online ISBN: 978-3-540-46293-4

  • eBook Packages: Springer Book Archive

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