Feb 1, 1998byBrummell, Nicholas H.; Hurlburt, Neal E.; Toomre, Jur
The effects of rotation on turbulent, compressible convection within stellar envelopes are studied through three-dimensional numerical simulations conducted within a local f-plane model. This work seeks to understand the types of differential rotation that can be established in convective envelopes of stars like the Sun, for which recent helioseismic observations suggest an angular velocity profile with depth and latitude at variance with many theoretical predictions. This paper analyzes the... Topics: AEROSOLS, SULFURIC ACID, ASHES, COAGULATION, DILUTION, DROP SIZE, MASS RATIOS, NUCLEATION, OZONE...