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Dynamo Driven Mean Magnetic Field in Accretion Disks of Compact Astrophysical Objects and its Manifestations

Published online by Cambridge University Press:  19 July 2016

G.D. Chagelishvili
Affiliation:
Abastumani Astrophysical Observatory Academy of Sciences of Georgian SSR Pavlov str. 2a 380060 Tbilisi, USSR
R.G. Chanishvili
Affiliation:
Abastumani Astrophysical Observatory Academy of Sciences of Georgian SSR Pavlov str. 2a 380060 Tbilisi, USSR
J.G. Lominadze
Affiliation:
Abastumani Astrophysical Observatory Academy of Sciences of Georgian SSR Pavlov str. 2a 380060 Tbilisi, USSR
Z.A. Sokhadze
Affiliation:
Abastumani Astrophysical Observatory Academy of Sciences of Georgian SSR Pavlov str. 2a 380060 Tbilisi, USSR

Abstract

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The simplest case of the nonlinear turbulent dynamo mechanism is proposed. It is shown that under certain conditions the generated mean magnetic field can become stronger than the small-scale one. Some manifestations (the model of Cyg X-1 bimodal behaviour, asymmetric accretion onto the magnetized rotating compact star) of this mean field are discussed.

Type
7. Magnetic Fields in Galactic Nuclei
Copyright
Copyright © Kluwer 1990 

References

Chagelishvili, G.D. and Lominadze, J.G. (1984) Proc. Course and Workshop Plasma Astrophysics, Varenna, Italy, ESA SP-207.Google Scholar
Chagelishvili, G.D., Lominadze, J.G. and Sokhadze, Z.A. (1986a) Proc. Joint Int. School and Workshop Plasma Astrophysics, Sukhumi, USSR, ESA SP–251, 523529.Google Scholar
Chagelishvili, G.D., Chanishvili, R.G. and Lominadze, J.G. (1986b) Proc. Joint Int. Course and Workshop Plasma Astrophysics, Sukhumi, USSR, ESA SP–251, 563.Google Scholar
Chagelishvili, G.D., Chanishvili, R.G. and Lominadze, J.G. (1988) Adv. Space Res. 8 (2), 217.Google Scholar
Moffatt, H.K. (1978) Magnetic Field Generation in Electrically Conducting Fluids, Cambridge University Press.Google Scholar
Shakura, N.I. and Sunyaev, R.A. (1973) Astron. Astrophys. 24, 337359.Google Scholar
Weinstein, S.I., Zel'dovich, Ya.B. and Ruzmaikin, A.A. (1980) Turbulent Dynamo in Astrophysics, NAUKA, Moscow.Google Scholar