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Dynamo in Astrophysics

Published online by Cambridge University Press:  19 July 2016

A.A. Ruzmaikin
A.A. Ruzmaikin*
Affiliation:
IZMIRAN, Academy of Sciences Troitsk Moscow Region, 142092 USSR

Abstract

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The fast dynamo acting in a turbulent flow explains the origin of magnetic fields in astrophysical objects. Stellar cycles and large-scale magnetic fields in spiral galaxies reflect the behaviour of a mean magnetic field. Intermittent magnetic structures in clusters of galaxies are associated with random magnetic field.

Type
4. Magnetohydrodynamics of Galactic Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 83 - 89
Copyright
Copyright © Kluwer 1990 

References

Baker, N. and Tamesvary, S. (1966) Tables of stellar envelope models, New York.Google Scholar
Baliunas, S.L. and Vaughan, A.H. (1985) Ann. Rev. Astron. Astrophys. 23, 379–412.Google Scholar
Beck, R. (1986) IEEE Trans. Plasma Sci. 14, 740–747.Google Scholar
Belvedere, G., Paterno, L. and Stix, M. (1980) Astron. Astrophys. 91, 328–330.Google Scholar
Galeev, A.A., Rosner, R. and Vaiana, G.S. (1981) Astrophys. J. 243, 301–308.Google Scholar
Kleeorin, N.I., Ruzmaikin, A.A. and Sokoloff, D.D. (1983) Astrophys. Space Sci. 95, 131–136.Google Scholar
Kleeorin, N.I. and Ruzmaikin, A.A. (1988) in Glagolevsky, Yu.V. and Kopylov, I.M. (eds.), Magnetic Stars, Nauka, Leningrad, pp. 321–328.Google Scholar
Krause, F. and Rädler, K.–H. (1980) Mean–Field Magnetohydrodynamics and Dynamo Theory, Pergamon Press, Oxford.Google Scholar
Moffatt, H.K. (1978) Magnetic Field Generation in Electrically Conducting Fluids, Cambridge Univ. Press, Cambridge.Google Scholar
Molchanov, S.A., Ruzmaikin, A.A. and Sokoloff, D.D. (1983) Geophys. Astrophys. Fluid Dyn. 30, 241–252.Google Scholar
Pallavichini, R., Golub, L., Rosner, R., Vaiana, G.S., Ayres, T. and Linsky, J.L. (1981) Astrophys. J. 248, 279–290.Google Scholar
Parker, E.N. (1979) Cosmic Magnetic Fields, Oxford Univ. Press, Oxford.Google Scholar
Ruzmaikin, A.A. (1981) Comments on Astrophys. 9, 85–91.Google Scholar
Ruzmaikin, A.A., Shukurov, A.M. and Sokoloff, D.D. (1988) Magnetic Fields of Galaxies, Kluwer Academic Publishers, Dordrecht.Google Scholar
Ruzmaikin, A.A., Shukurov, A.M. and Sokoloff, D.D. (1989) Monthly Notices Roy. Astron. Soc. (in press).Google Scholar
Sofue, Y., Fujimoto, M. and Wielebinski, R. (1986) Ann. Rev. Astron. Astrophys. 24, 459–498.Google Scholar
Weiss, N.O., Cattaneo, F. and Jones, C.A. (1984) Geophys. Astrophys. Fluid Dyn. 30, 305.Google Scholar
Wilson, O. (1978) Astrophys. J. 226, 379–396.Google Scholar
Zeldovich, Ya.B. and Ruzmaikin, A.A. (1980) Sov. Phys. JETP 51, 493–497.Google Scholar
Zeldovich, Ya.B., Ruzmaikin, A.A. and Sokoloff, D.D. (1983) Magnetic Fields in Astrophysics, Gordon and Breach, New York, London, Paris.Google Scholar