High dispersion spectroscopic observations of Venus near superior conjunction. IV - Results for the carbon dioxide bands in the IV-N photographic region

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Atmospheric Composition, Carbon Dioxide, High Dispersion Spectrographs, Spectroscopic Analysis, Venus Atmosphere, Abundance, Annual Variations, Atmospheric Radiation, Atmospheric Scattering, Bandwidth, Conjunction, Line Spectra, Spectral Line Width, Venus, Spectroscopy, Observations, Carbon Dioxide, Bands, Data, Abundance, Phase Angles, Comparisons, Atmosphere, Clouds, Procedure

Scientific paper

Phase curves for the CO2 bands at 7883, 7820, and 8689 A are presented. While the weaker bands at 7820 and 7883 A show a definite 'inverse phase effect,' the band at 8689 A shows a more normal phase curve; it also exhibited much larger day-to-day variations in the CO2 abundance near superior conjunction in 1971. Because the variation of the phase curves with band strength is comparable to temporal variations on Venus, simultaneous observations of strong and weak bands are still needed to determine the dependence on band strength accurately.

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