A solar dynamo in the overshoot region.

Details A solar dynamo in the overshoot region. A solar dynamo in the overshoot region.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..241p&link_type=abstract

Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 241 - 246

Physics

Solar Interior: Dynamo Theory, Solar Convective Zone: Solar Activity Cycles, Solar Activity: Dynamo Theory

Scientific paper

The overshoot region at the bottom of the convective zone is a favourable site for the solar dynamo. Many physical features of that region are not yet well known. However, it is shown that with the law of rotation suggested by helioseismology and a plausible choice of the mean-field coefficients α and β, it is possible to get realistic butterfly diagrams.

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