The observed day-to-day variability of Mars atmospheric water vapor

Physics

Scientific paper

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Dust Storms, Mars Atmosphere, Periodic Variations, Polar Caps, Vertical Distribution, Water Vapor, Aerosols, Data Reduction, Ice Clouds, Viking Mars Program, Mars, Atmosphere, Water Vapor, Spacecraft Observations, Viking Missions, Abundance, Aerosols, Distribution, Dust Storms, Polar Regions, Ice Caps, Tharsis Region, Lunae Planum, Clouds, Water Ice, Thermal Properties, Infrared, Wavelengths, Visible Radiation, Seasonal Variations, Cycles, Mawd Instrument, Data Reduction, Analysis, Maps, Haze

Scientific paper

The present evaluation of Viking water column abundance measurements of the Martian atmosphere notes observed changes to be due to atmospheric water vapor vertical column abundance variations, as well as to apparent changes resulting from abundance changes of atmospheric aerosols, relative vertical distribution changes of water vapor and aerosol, or systematic viewing-geometry variations. Variability noted in several major regions by visible and thermal-IR observations is found to very accurately coincide with the occurrence of water ice clouds and hazes.

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