4-day waves in the Venus atmosphere

Details 4-day waves in the Venus atmosphere 4-day waves in the Venus atmosphere

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...47..130c&link_type=abstract

Icarus, vol. 47, July 1981, p. 130-138.

Physics

16

Albedo, Gravity Waves, Planetary Waves, Planetology, Ultraviolet Radiation, Venus Atmosphere, Atmospheric Circulation, Atmospheric Models, Atmospheric Temperature, Planetary Radiation, Wave Propagation, Wind Profiles, Venus, Atmosphere, Waves, Ultraviolet, Wavelengths, Models, Velocities, Theoretical Studies, Winds, Thermal Properties, Structure, Pioneer Venus, Gravity Waves, Clouds, Features, Resonance, Data, Albedo, Circulation

Scientific paper

Ultraviolet albedo contrasts in the Venus atmosphere are probably large-scale atmospheric waves propagating slowly with respect to the rapid cloud-top zonal winds. Using a simple theoretical model and profiles of mean wind and thermal structure based on Pioneer Venus data, planetary-scale gravity waves with phase velocities matching the speeds of the UV markings are found. An upward-propagating wave, and waves trapped at cloud levels are proposed as candidates to explain the observed UV features.

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