Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993p%26ss...41..495d&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 41, no. 7, p. 495-504
Astronomy and Astrophysics
Astronomy
40
Abundance, Emission Spectra, Fluorescence, Infrared Spectra, Near Infrared Radiation, Oxygen, Radiance, Venus (Planet), Venus Atmosphere, Water Vapor, Astronomical Spectroscopy, Carbon Monoxide, Galileo Spacecraft, Infrared Spectroscopy, Spaceborne Astronomy
Scientific paper
The spectroscopic data of the Near-Infrared Mapping Spectrometer (NIMS), recorded during the Galileo flyby of Venus, are analysed to retrieve the water vapor abundance variations in the lower atmosphere of Venus at night. The 1.18 micrometer spectral window, which probes altitude levels below 20 km, is used for this purpose. Constraints on the CO2 continuum and far-wing opacity from existing ground-based high-resolution observations are included in the modelling of the NIMS spectra. The NIMS measurements can be fitted with a water vapor mixing ratio of 30 +/- 15 ppm, in agreement with analyses of ground-based nightside observations. The water vapor abundance shows no horizontal variations exceeding 20% over a wide latitude range (40 deg S, 50 deg N) on the nightside of Venus. Within the same selection of NIMS spectra, a large enhancement in the O2 fluorescence emission at 1.27 micrometer is observed at a latitude of 40 deg S, over a spatial area about 100 km wide.
Bezard Bruno
Calcutt Simon B.
Collard A. D.
Drossart Pierre
Encrenaz Th.
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