Abstract
Models relevant to numerical studies of the solar cycle are reviewed briefly with discussions of pertinent physical mechanisms. It is suggested that the observed surface activities are secondary in nature and an example of possible non-axisymmetric steady state solutions is given, together with the results of preliminary numerical computations.
The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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Nakagawa, Y. (1971). A Numerical Study of the Solar Cycle. 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_86
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DOI: https://doi.org/10.1007/978-94-010-3117-2_86
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