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Plasma physics and astrophysics

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Festkörperprobleme 11

Part of the book series: Advances in Solid State Physics ((ASSP,volume 11))

Zusammenfassung

Wir veranschaulichen die Bedeutung des astrophysischen Plasmas mit einer Besprechung einiger astrophysischen Probleme.

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References

  • We have not referred to literature in the body of the text, as we have only given a bird's eye view of the field. For those readers who want to study the field any further we give here a—highly prejudiced and personal—selected list. General coverage can be found in: Plasma Astrophysics (Ed. P. A. Sturrock), Academic Press 1967.

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  • Transactions of the International Astronomical Union, Vol. XIV A, Reports on Astronomy, Report by Commission 43 (Plasmas and Magnetohydrodynamics in Astrophysics).

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  • H. Alfvén and C-G. Fälthammer, Cosmical Electrodynamics, Oxford University Press, 1963. For solar and planetary phenomena we refer to: V. V. Zheleznyakov, Radio Emission of the Sun and Planets, Pergamon, 1970. For cosmic rays we refer to

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  • V. L. Ginzburg and S. I. Syrovatskii, The Origin of Cosmic Rays, Pergamon, 1964. For pulsars we refer to

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  • V. L. Ginzburg and V. V. Zheleznyakov, Comments Ap. Space Phys. 2, 167 and 197 (1970). D. ter Haar, Phys. Repts, 1 (1971) (in press).

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  • We finally refer to the following books and review articles which we have found useful: Oscillations in a Plasma, Pergamon, 1967.

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  • V. L. Ginzburg, The Propagation of Electromagnetic Waves in Plasma, Pergamon, 1970.

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  • S. F. Smerd, Proc. Astron. Soc, Australia 1, 124 (1968).

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  • V. N. Tsytovich, Soviet Phys.—Uspekhi, 12, 42 (1969).

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O. Madelung

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© 1971 Friedr. Vieweg + Sohn GmbH, Verlag

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ter Haar, D. (1971). Plasma physics and astrophysics. In: Madelung, O. (eds) Festkörperprobleme 11. Advances in Solid State Physics, vol 11. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0107692

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  • DOI: https://doi.org/10.1007/BFb0107692

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-528-08017-4

  • Online ISBN: 978-3-540-75328-5

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