Abstract
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.
This is a preview of subscription content, log in via an institution to check access.
References
Kichatinov, L.L.: 1982, Magnitnaya Gidrodinamika 2, 67
Kichatinov, L.L.: 1990, Astron. Astrophys. (in press)
Krivodubskij, V.N.: 1987, Pis'ma Astron. Zh. 9, 803 (Sov. Astron. Lett. 9, 338)
Spruit, H.C.-1977, Thesis, University of Utrecht, p.17
Vainshtein S.I.: 1983, Magnetic Fields in Outer Space (in Russian), Nauka, Moscow
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1991 Springer-Verlag
About this paper
Cite this paper
Krivodubskij, V.N., Kichatinov, L.L. (1991). The transfer of large-scale magnetic field by radial inhomogeneity of the material density in the rotating convection zone. In: Tuominen, I., Moss, D., Rüdiger, G. (eds) The Sun and Cool Stars: activity, magnetism, dynamos. Lecture Notes in Physics, vol 380. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53955-7_127
Download citation
DOI: https://doi.org/10.1007/3-540-53955-7_127
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-53955-1
Online ISBN: 978-3-540-46483-9
eBook Packages: Springer Book Archive