The influence of the angular velocity distribution on the energy transport in the Sun's convection zone |
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| Authors: | G. Belvedere G. La Rosa L. Paternò |
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| Affiliation: | (1) Istituto di Astronomia dell' Università di Catania, Italy;(2) Osservatorio Astrofisico di Catania, Italy;(3) Osservatorio Astrofisico di Catania, Italy;(4) Istituto di Fisica della Facoltà di Ingegneria dell' Università di Catania, Italy |
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| Abstract: | 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.Proceedings of the 14th ESLAB Symposium on Physics of Solar Variations, 16–19 September 1980, Scheveningen, The Netherlands. |
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