The Internal Solar Angular Velocity: Theory, Observations and Relationship to Solar Magnetic Fields

Author:   B. R. Durney ,  Sofia Sabatino
Publisher:   Springer
Edition:   1987 ed.
Volume:   137
ISBN:  

9789027725233


Pages:   374
Publication Date:   31 July 1987
Format:   Hardback
Availability:   In Print   Availability explained
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The Internal Solar Angular Velocity: Theory, Observations and Relationship to Solar Magnetic Fields


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Author:   B. R. Durney ,  Sofia Sabatino
Publisher:   Springer
Imprint:   Kluwer Academic Publishers
Edition:   1987 ed.
Volume:   137
Dimensions:   Width: 17.00cm , Height: 2.20cm , Length: 24.40cm
Weight:   1.590kg
ISBN:  

9789027725233


ISBN 10:   9027725233
Pages:   374
Publication Date:   31 July 1987
Audience:   College/higher education ,  Professional and scholarly ,  Postgraduate, Research & Scholarly ,  Professional & Vocational
Format:   Hardback
Publisher's Status:   Active
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

Table of Contents

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.

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