o-.rr rcdels give the deperrdence of the angular velocity at the Sunis equator on the depth of the convecÈion zcne. In order to drive differential rotation we ccnsidered two different rnechanisxns: latirude depe:rience of the n:xj"ng length and the anisoircpy of :ie turbulent viscosity. lie studied also the influence of boundary conditions at the botton of the ccnvection zone on our rcdels.
Models of solar differential rotation
Pidatella, Rosa Maria;Belvedere, G.;
1984-01-01
Abstract
o-.rr rcdels give the deperrdence of the angular velocity at the Sunis equator on the depth of the convecÈion zcne. In order to drive differential rotation we ccnsidered two different rnechanisxns: latirude depe:rience of the n:xj"ng length and the anisoircpy of :ie turbulent viscosity. lie studied also the influence of boundary conditions at the botton of the ccnvection zone on our rcdels.File in questo prodotto:
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