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Collective Plasma Phenomena and their Role in the Dynamics of the Interstellar Medium

Published online by Cambridge University Press:  14 August 2015

B. B. Kadomtsev  and
V. N. Tsytovich
B. B. Kadomtsev
Affiliation:
Fizicheskij Institut P. N. Lebedev, Akademiya Nauk S.S.S.R., Moskva, S.S.S.R.
V. N. Tsytovich
Affiliation:
Fizicheskij Institut P. N. Lebedev, Akademiya Nauk S.S.S.R., Moskva, S.S.S.R.

Extract

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The First Symposium on cosmical gas dynamics clearly demonstrated that magnetic fields play an essential role in the dynamics of the interstellar matter. The Symposium emphasized that the behavior of interstellar gas should be described not by traditional gas dynamics but with the help of magneto-gas dynamics. As we now realize this was only the first step, since in plasmas a very broad range of phenomena can occur which are coupled not with large-scale magneto-gas dynamic motions but rather with more subtle collective plasma motions. To describe properly the dynamics of an ensemble of charged particles we should use not only average characteristics such as density, pressure and mean velocity, but also more detailed features of the particle distribution function.

Type
Part I: Description and General Theory of the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 39: Interstellar Gas Dynamics , 1970 , pp. 108 - 132
Copyright
Copyright © Reidel 1970 

References

Ginzburg, V. L.: 1965, Astron. Zh. 42, 1129 (1966, Soviet Astron. 9, 877).Google Scholar
Ginzburg, V. L. and Syrovat-skii, S. I.: 1963, The Origin of Cosmic Rays, Izd. Akad. Nauk SSSR, Moscow (translation 1964, Pergamon Press, Oxford).Google Scholar
Kadomtsev, B. B.: 1964, Plasma Turbulence, Izd. Akad. Nauk SSSR, Moscow (translation 1965, Academic Press, New York).Google Scholar
Kaplan, S. A. and Tsytovich, V. N.: 1968, Astron. Zh. 45, 777 (1969, Soviet Astron. 12, 618).Google Scholar
Kaplan, S. A. and Tsytovich, V. N.: 1969, Usp. Fiz. Nauk 97, 77 (1969, Soviet Phys. Usp., under translation).CrossRefGoogle Scholar
Lerche, I.: 1967, Astrophys. J. 147, 689.CrossRefGoogle Scholar
Liperovskii, V. A. and Tsytovich, V. N.: 1969, Zh. Eksp. Teor. Fiz. 57, 301 (1969, Soviet Phys. JETP, under translation).Google Scholar
Melrose, D. B.: 1967, Preprint Belfer Graduate School, New York.Google Scholar
Pikel'ner, S. B.: 1968, Ann. Rev. Astron. Astrophys. 6, 165.CrossRefGoogle Scholar
Pikel'ner, S. B. and Tsytovich, V. N.: 1968, Zh. Eksp. Teor. Fiz. 55, 977 (1969, Soviet Phys. JETP 28, 507).Google Scholar
Pikel'ner, S. B. and Tsytovich, V. N.: 1969, Astron. Zh. 46, 8 (1969, Soviet Astron. 13, 5).Google Scholar
Spitzer, L.: 1962, Physics of Fully Ionized Gases, 2nd ed., Interscience, New York.Google Scholar
Stix, T.: 1962, Theory of Plasma Waves, McGraw-Hill, New York.Google Scholar
Tsytovich, V. N.: 1963, Zh. Eksp. Teor. Fiz. 44, 946 (1963, Soviet Phys. JETP 17, 643).Google Scholar
Tsytovich, V. N.: 1965, Astron. Zh. 42, 33 (1965, Soviet Astron. 9, 24).Google Scholar
Tsytovich, V. N.: 1966a, Astron. Zh. 43, 528 (1966a, Soviet Astron. 10, 419).Google Scholar
Tsytovich, V. N.: 1966b, Usp. Fiz. Nauk 89, 89 (1966b, Soviet Phys. Usp. 9, 370).CrossRefGoogle Scholar
Tsytovich, V. N.: 1967, Nonlinear Effects in Plasmas, Izd. Akad. Nauk SSSR, Moscow.CrossRefGoogle Scholar
Tsytovich, V. N.: 1969, Lebedev Physical Institute, preprint.Google Scholar
Tsytovich, V. N. and Chikhachev, A. S.: 1969, Astron. Zh. 46, 486 (1970, Soviet Astron., under translation).Google Scholar
Tverskoy, B. A.: 1967, Zh. Eksp. Teor. Fiz. 53, 1417 (1968, Soviet Phys. JETP 26, 821).Google Scholar
Wentzel, D. G.: 1968, Astrophys. J. 152, 987.CrossRefGoogle Scholar