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Dynamics of Large-Scale Magnetic Fields

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Solar Magnetic Fields

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 43))

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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© 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

  • eBook Packages: Springer Book Archive

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