Solar dynamo models with realistic internal rotation

Details Solar dynamo models with realistic internal rotation Solar dynamo models with realistic internal rotation

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505...91c&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Physics

Solar Dynamo, Solar Rotation, Meridional Circulation

Scientific paper

Solar dynamo models based on differetial rotation inferred from
helioseismology tend to produce rather strong magnetic activity at high
solar latitudes, in contrast to the observed fact that sunspots appear
at low latitudes. We show that a meridional circulation penetrating
below the tachocline can solve this problem.

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