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Thermal convection of an internally heated infinite Prandtl number fluid in a spherical shellA Galerkin technique is used to study the finite-amplitude axisymmetric steady convective motions of an infinite Prandtl number Boussinesq fluid in a spherical shell. Two types of heating are considered: in one case, convection is driven both by internal heat sources in the fluid and by an externally imposed temperature drop across the shell boundaries; in the other case, only internal heat sources drive convection and the lower boundary of the shell is adiabatic. Two distinct classes of axisymmetric steady states are found to be possible: states characterized by temperature and radial velocity fields that are symmetric about an equatorial plane; and a class of solutions that does not possess any symmetry properties about the equatorial plane.
Document ID
19810028553
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schubert, G.
(California, University Los Angeles, Calif., United States)
Zebib, A.
(Rutgers University Piscataway, N.J., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1980
Publication Information
Publication: Geophysical and Astrophysical Fluid Dynamics
Volume: 15
Issue: 1-2,
Subject Category
Geophysics
Accession Number
81A12957
Funding Number(s)
CONTRACT_GRANT: NSG-7601
CONTRACT_GRANT: NGR-05-007-317
CONTRACT_GRANT: NSF EAR-77-15198
Distribution Limits
Public
Copyright
Other

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