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Convective instability when the temperature gradient and rotation vector are oblique to gravity. II - Real fluids with effects of diffusionThe linear stability analysis of Hathaway et al. (1979) is repeated for Boussinesq fluids with viscous and thermal diffusion. The fluid is confined between plane parallel boundaries and the rotation vector is oblique to gravity; this tilted rotation vector introduces a preference for roll-like disturbances whose axes are oriented north-south. The presence of a latitudinal temperature gradient produces a thermal wind shear which favors axisymmetric convective rolls if the gradient exceeds some critical value. The axisymmetric rolls are similar in many respects to the cloud bands on Jupiter provided they extend to a depth of about 15,000 km.
Document ID
19810028550
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hathaway, D. H.
(Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Toomre, J.
(Colorado, University; Joint Institute for Laboratory Astrophysics, Boulder, Colo., United States)
Gilman, P. A.
(High Altitude Observatory Boulder, Colo., 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
Lunar And Planetary Exploration
Report/Patent Number
AFGL-TR-82-0087
AD-A112461
Accession Number
81A12954
Funding Number(s)
CONTRACT_GRANT: F19628-77-C-0104
CONTRACT_GRANT: NAS8-31958
CONTRACT_GRANT: NSG-7511
Distribution Limits
Public
Copyright
Other

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