On the angular velocity distribution in a nonhomogeneously rotating star

Details On the angular velocity distribution in a nonhomogeneously rotating star On the angular velocity distribution in a nonhomogeneously rotating star

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994an....315..171g&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 315, no. 2, p. 171-174

Astronomy and Astrophysics

Astronomy

Angular Momentum, Angular Velocity, Inhomogeneity, Stellar Interiors, Stellar Rotation, Sun, Velocity Distribution, Helioseismology, Turbulence Models, Turbulent Flow, Viscosity

Scientific paper

Some results of the calculations of the angular velocity distribution in the equatorial plane of a nonhomogeneously rotating star, in particular of the Sun, are presented. Hence the hypothesis is advanced of the turbulent viscosity as one of the main factors of the angular momentum transport from a rapidly rotating core through the radiative equilibrium region.

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