The internal solar angular velocity : theory, observations, and relationship to solar magnetic fields : proceedings of the 8th national solar observatory summer symposium, held in Sunspot, Mexico, August 11-14, 1986

Problems of the Solar Interior.- 1/Observations.- Observations of Solar P-Mode Rotational Splittings.- Latitude and Depth Variation of Solar Rotation.- Observations of Surface Velocity Fields.- Spacelab experiments on convection in a rotating spherical shell with radial gravity.- The Equatorial Rotation Rate in the Solar Convection Zone.- More Evidence for a Solar Latitude Dependent Limb Temperature Variation.- Fine Structure in Solar Oscillation Spectra.- Chromospheric Activity in Open Clusters.- Full-disk solar dopplergrams observed with a one megapixel CCD camera and sodium magneto-optical filter.- Estimates of the solar internal angular velocity obtained with the Mt. Wilson 60-foot solar tower.- Solar Rotation Variations from Sunspot Group Statistics.- The Detection of Global Convection on the Sun by an Analysis of Line Shift Data of the John M. Wilcox Solar Observatory at Stanford University.- 2/Theory: Normal Modes of Oscillations.- Adiabatic Nonradial Oscillations of a Differentially Rotating Star.- Inertial Oscillations and the Rotation Rate Profile of the Sun.- A Spherical Harmonic Decomposition Technique for Analysing Steady Photospheric Flows.- 3/Theory: Radiative Zone.- The solar-stellar connection: Internal rotation in low-mass stars.- Numerical Studies of Solar Evolution with Rotation and Comparison with Stellar Rotation Data.- Magnetic fields and rotation in late-type stars.- Solar Rotation and Age.- Evolution and Internal Rotation of the Sun.- Angular Momentum Transport in the Radiative Interior of the Sun.- Turbulent transport in the radiative zone of a rotating star.- The Generation of Magnetic Fields in the Sun.- Mass Transport by Wave Motion.- Differential Rotation in Stars.- 4/Theory: Convective Zone.- The Generalization of Mixing Length Theory to Rotating Convection Zones and Applications to the Sun.- A Review of What Numerical Simulations Tell Us About the Internal Rotation of the Sun.- Moment closure for thermal convection: a viable approach?.- Magnetic Activity Complexes, Thermal Relaxation Oscillations, and the Dynamics of the Azimuthal Magnetic Field of a Star.- Magnetic Fields and the Rotation of the Solar Convection Zone.- Hydrostatic Adjustment Time of the Solar Subconvective Layer.- Models for a Differentially Rotating Solar Convection Zone.- Beyond the Mixing-Length Theory: A Turbulent Diffusivity Approach.- Mixing-Length, Shears, and Differential Rotation.- Horizontal Reynolds Stress and Radial Rotation Law of the Sun.