The formation of a steady flow in a fluid by a traveling heat wave, and its influence on the atmospheric circulation of the earth and Mars

Details The formation of a steady flow in a fluid by a traveling heat wave, and its influence on the atmospheric circulation of the earth and Mars The formation of a steady flow in a fluid by a traveling heat wave, and its influence on the atmospheric circulation of the earth and Mars

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..575z&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, July-Aug. 1978, p. 575-582. In Russian.

Physics

Atmospheric Circulation, Earth Atmosphere, Mars Atmosphere, Planetary Rotation, Thermal Radiation, Traveling Waves, Convective Heat Transfer, Diurnal Variations, Environment Simulation, Planetology, Solar Heating, Steady Flow, Venus Atmosphere

Scientific paper

The influence on atmospheric circulation of a flow generated by the
diurnal atmospheric-temperature variation (resulting from the planet's
rotation) is examined. The mean velocity of such flows is evaluated for
different planetary conditions without allowance for the sphericity of
the atmosphere.

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