The influence of the angular velocity distribution on the energy transport in the sun's convection zone

Details The influence of the angular velocity distribution on the energy transport in the sun's convection zone The influence of the angular velocity distribution on the energy transport in the sun's convection zone

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...74..107b&link_type=abstract

(ESA and European Physical Society, ESLAB Symposium on Physics of Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-19

Physics

Angular Velocity, Convective Flow, Energy Transfer, Solar Rotation, Astronomical Models, Conservation Equations, Velocity Distribution

Scientific paper

This contribution is a purely exploratory search to investigate the way the distribution of angular velocity inside the Sun's convection zone affects the energy transport. This is related with problems concerning the magnetic activity, whose appearance at the Sun's surface depends on the shape of the isorotation surfaces, and the latitudinal variations in flux. The proposed model is non-linear and axisymmetric

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