Mathematics – Logic
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mesjj..62...18m&link_type=abstract
Meteorological Society of Japan, Journal (ISSN 0026-1165), vol. 62, Feb. 1984, p. 18-25.
Mathematics
Logic
Atmospheric Circulation, Baroclinic Instability, Flow Stability, Venus Atmosphere, Atmospheric Models, Atmospheric Stratification, Boundary Conditions, Boundary Value Problems, Wind Velocity
Scientific paper
The baroclinic instability in the flow of the thermal wind balance of Venus is modeled analytically to study the Venus upper atmosphere circulation and the effect of the instability on the geostrophic balance. The effects of the boundary condition on the baroclinic instability are examined without using a geostrophic approximation. Attention is given to the characteristics of disturbances at large Rossby numbers and for both weak and strong stratification. A rigid wall is eliminated as the most favorable condition for instability, although values for the growth rate and phase velocity of the disturbances are altered by changing the boundary conditions. Two critical points are defined for the increase in Rossby number, with only one critical point allowed at a time in the baroclinic layer.
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