A technique to deduce atmospheric temperature and constituent profiles from a planet's limb radiance profile

Computer Science

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Atmospheric Composition, Atmospheric Temperature, Planetary Atmospheres, Radiance, Temperature Distribution, Atmospheric Models, Carbon Dioxide, Limbs, Mars Atmosphere, Vertical Distribution, Water Vapor, Weighting Functions

Scientific paper

The concept is described of deducing the temperature and constituent profile of a planetary atmosphere from orbiter measurements of the planet's IR limb-radiance profile. Expressions are derived for the weighting functions associated with the limb-radiance profile for a Goody random-band model. Analysis of the weighting functions for the Martian atmosphere indicates that a limb radiance profile in the 15-micron CO2 band can be used to determine the Martian atmospheric temperature profile from 20 to 60 km. Simulation of the Martian limb-radiance profile in the rotational water-vapor band indicates that Martian water-vapor mixing ratios can be inferred from limb-radiance observations in a water-vapor band.

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