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

✍ Scribed by G. Belvedere; G. Rosa; L. Paternò

Publisher
Springer
Year
1981
Tongue
English
Weight
179 KB
Volume
74
Category
Article
ISSN
0038-0938

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✦ Synopsis

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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