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51. Theory of isotropic magnetic turbulence in gases

Published online by Cambridge University Press:  18 July 2016

S. A. Kaplan
S. A. Kaplan*
Affiliation:
Astronomical Observatory, University of L'vov, U.S.S.R.

Abstract

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A system of spectral equations of magnetic turbulence in gases differing from that given by Chandrasekhar is suggested. The solution of this system is examined. Correlation and structure functions of the turbulence of interstellar gases, determined according to the data on radial velocities of interstellar clouds from Adams's catalogue, are given. For motions of a scale less than the fundamental one (l less than 80 pc) the spectral function F(k) is about k–1·71, which agrees with the theoretical conclusions.

Type
Part VII: Additional Contributions
Information
Symposium - International Astronomical Union , Volume 6: Electromagnetic Phenomena in Cosmical Physics , 1958 , pp. 504 - 512
Copyright
Copyright © Cambridge University Press 1958 

References

1. Kaplan, S. A. Circ. Lvov astron. obs. no. 25, 1953.Google Scholar
2. Kaplan, S. A. C.R. Acad. Sci. U.R.S.S. 94, 33, 1954; J. Exp. Theor. Phys. 27, 699, 1954.Google Scholar
3. Heisenberg, W. Z. Phys. 124, 628, 1948.Google Scholar
4. Batchelor, G. K. Proc. Roy. Soc. A , 201, 405, 1950.Google Scholar
5. Kaplan, S. A. A.J. U.S.S.R. 32, 255, 1955.Google Scholar
6. Chandrasekhar, S. Proc. Roy. Soc. A , 233, 322 and 390, 1955.Google Scholar
7. Chandrasekhar, S. Proc. Roy. Soc. A , 204, 435, 1951.Google Scholar
8. Millionschchikov, M. D. C.R. Acad. Sci. U.R.S.S. 32, 611 and 615, 1941.Google Scholar