Differential rotation and isorotation surfaces in a slowly rotating convective solar envelope

Details Differential rotation and isorotation surfaces in a slowly rotating convective solar envelope Differential rotation and isorotation surfaces in a slowly rotating convective solar envelope

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..741p&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Aug. 1991, p. 741-753. In Russian. In Russian.

Physics

Angular Velocity, Free Convection, Solar Atmosphere, Solar Rotation, Stellar Envelopes, Equations Of Motion, Solar Physics, Velocity Distribution

Scientific paper

It is shown that turbulent convection in a density-stratified medium redistributes the angular momentum such that differential rotation arises. Angular velocity decreases at high latitudes and increases at low ones. The inversion region of the sign of the angular velocity radial gradient belongs to the middle latitudes. It is shown that the solution obtained is not inconsistent with the observations and helioseismological data.

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