Radiative equilibrium temperatures in the stratosphere and mesosphere - A comparison for the stellar occultation and BUV ozone data

Physics

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Atmospheric Heat Budget, Atmospheric Temperature, Mesosphere, Ozone, Radiative Heat Transfer, Stellar Occultation, Stratosphere, Convection, Photochemical Reactions, Solar Radiation, Temperature Profiles, Ultraviolet Spectra

Scientific paper

Recently published ozone densities in the equatorial stratosphere and mesosphere from satellite stellar occultation measurements are appreciably larger than previous independent midlatitude measurements and ozone densities predicted by photochemical theory. Radiative equilibrium temperature profiles with a stratosphere-mesosphere optimized model have been calculated for each of these ozone profiles; it is found that the stellar occultation studies cannot be discounted on energy balance grounds.

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