Abstract
A discussion is given of the dynamics of large-scale solar magnetic fields as a joint action of a transport by a regular velocity field, by a generalized diffusion, by coming to the surface and sinking and by sources of origin and destruction of magnetic fields. Also these processes are discussed using the observed picture of magnetic field dynamics.
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References
Bumba, V. and Howard, R. F.: 1965, Astrophys. J. 141,1502
Leighton, R. B.: 1964, Astrophys. J. 140,1547
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© 1971 International Astronomical Union
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Kuklin, G.V. (1971). Dynamics of Large-Scale Magnetic Fields. In: Howard, R. (eds) Solar Magnetic Fields. International Astronomical Union / Union Astronomique Internationale, vol 43. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3117-2_87
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DOI: https://doi.org/10.1007/978-94-010-3117-2_87
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3119-6
Online ISBN: 978-94-010-3117-2
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