Convective dynamos for rotating stars

Details Convective dynamos for rotating stars Convective dynamos for rotating stars

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982saosr.392a.165g&link_type=abstract

In Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1 p 165-179 (

Statistics

Computation

1

Convective Flow, Dynamo Theory, Stellar Magnetic Fields, Stellar Rotation, Amplitudes, Baroclinic Instability, Computation, Magnetohydrodynamics, Stellar Structure

Scientific paper

Global dynamo theory is applied to the problem of why some stars have
field reversing dynamos, and others do not. It is argued that
convectively driven dynamos are the most likely source of magnetic
fields in stars that have convection zones.

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