Computer Science
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr......128k&link_type=abstract
Akademiia Nauk SSSR, Izvestiia, Mekhanika Zhidkosti i Gaza, Jan.-Feb. 1975, p. 128-137. In Russian.
Computer Science
Atmospheric Boundary Layer, Atmospheric Circulation, Free Convection, Planetary Atmospheres, Rotating Spheres, Temperature Gradients, Atmospheric Models, Environment Simulation, Heat Sources, Hydrodynamics, Latitude
Scientific paper
The convective stability of a fluid flow generated in a rotating spherical layer, due to a nonuniform temperature distribution at one of the boundaries of the layer is analyzed. The problem studied may simulate large-scale motions in atmospheres of large planets which contain internal heat sources and which absorb solar radiation at the cloud cover. It is shown that depending on the relationship between the parameters responsible for the rotation and for the nonuniform temperature distribution, the layer will become stable or unstable as compared to a fixed layer of equal thickness and with the same but uniform distribution of the applied heat flow.
Iavorskaia I. M.
Keller B. S.
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