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4-Day waves in the Venus atmosphere
Authors:Curt Covey  Gerald Schubert
Institution:1. Department of Earth and Space Sciences, University of California, Los Angeles, California 90024, USA
Abstract: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, we find planetary-scale gravity waves with phase velocities matching the speeds of the uv markings. We propose an upward-propagating wave and waves trapped at cloud levels as candidates to explain the observed uv features.
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