Evolution of the temperature field in planetary-scale atmospheric processes

Details Evolution of the temperature field in planetary-scale atmospheric processes Evolution of the temperature field in planetary-scale atmospheric processes

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981fizao..17..464k&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana, vol. 17, May 1981, p. 464-469. In Russian.

Physics

Atmospheric Models, Atmospheric Temperature, Baroclinic Waves, Planetary Atmospheres, Temperature Distribution, Adiabatic Equations, Earth Atmosphere, Energy Dissipation, Gas Giant Planets, Heat Transfer, Integral Equations, Nonlinear Equations, Vertical Distribution, Wave Propagation, Wind Velocity

Scientific paper

A nonlinear equation of the evolution of planetary-scale disturbances of
the temperature field is obtained for the vertically averaged baroclinic
atmosphere. In the adiabatic approximation, this equation is reduced to
a simple-wave equation relative to the mean temperature of vertical air
columns. The effect of nonadiabatic factors is also taken into account.

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