Physics
Scientific paper
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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