Solar dynamo models with realistic internal rotation

Arnab Rai, Choudhuri and Dibyendu, Nandy (2002) Solar dynamo models with realistic internal rotation. In: Euroconference/IAU Colloquium 188 on Magnetic Coupling of the Solar Atmosphere, JUN 11-15, 2002, Santorini, Greece.

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Abstract

Solar dynamo models based on differential 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.

Item Type:	Conference Paper
Publisher:	ESA Publications Division C/O Estec
Additional Information:	Copyright of this article belongs to ESA Publications Division C/O Estec.
Department/Centre:	Division of Physical & Mathematical Sciences > Physics
Date Deposited:	16 Mar 2012 12:10
Last Modified:	16 Mar 2012 12:10
URI:	http://eprints.iisc.ac.in/id/eprint/43971

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