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The Transfer of Large-scale Magnetic Field by Radial Inhomogeneity of the Material Density in the Rotating Convection Zone

Published online by Cambridge University Press:  12 April 2016

V.N. Krivodubskij  and
L.L. Kichatinov
V.N. Krivodubskij
Affiliation:
Kiev University Astronomical Observatory, Observatorna Street 3, Kiev - 53, 252053, Ukraine, USSR
L.L. Kichatinov
Affiliation:
Sib IZMIR, P.O. Box 4026, Irkutsk - 33, 664033, Russia, USSR

Abstract

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The influence of rotation on the transfer of the mean magnetic field of the Sun, caused by the radial inhomogeneity of the solar turbulent plasma density, is investigated. It turns out that the transfer directions of the poloidal and toroidal magnetic fields do not coincide.

Type
Part III Solar magnetism and large-scale flows
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 190 - 192
Copyright
Copyright © Springer-Verlag 1991

References

Kichatinov, L.L.: 1982, Magnitnaya Gidrodinamika 2, 67 Google Scholar
Kichatinov, L.L.: 1990, Astron. Astrophys. (in press)Google Scholar
Krivodubskij, V.N.: 1987, Pis’ma Astron. Zh. 9, 803 (Sov. Astron. Lett. 9, 338)Google Scholar
Spruit, H.C.: 1977, Thesis, University of Utrecht, p.17 Google Scholar
Vainshtein, S.I.: 1983, Magnetic Fields in Outer Space (in Russian), Nauka, Moscow Google Scholar