Internal rotation, convection and dynamos

Details Internal rotation, convection and dynamos Internal rotation, convection and dynamos

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094...77k&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Computer Science

2

Star Formation, Interplanetary Magnetic Fields, Magnetohydrodynamics And Plasmas

Scientific paper

The large-scale magnetic field and activity cycle of the Sun are believed to be the result of an advection-dominated dynamo, which is an extension of the well-known αΩ. dynamo in which a large-scale meridional flow plays a key part. We present a model of stellar rotation based on the mean field approach of magnetohydrodynamics. The model reproduces the observed solar internal rotation and surface meridional flow. We compare its predictions with the observations available so far. We also address the generation of magnetic fields in lower main sequence stars.

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