Journal of Geophysical Research Atmospheres · 1978 · 36 citations · 23 references
PhotochemistryPhotosystemsNatural SciencesSpectroscopyAtomic Emission SpectroscopyTotal DissociationCo 2Atmospheric PhotochemistryAtomic PhysicsAtomic Carbon FluorescenceChemistryCarbon CycleQuantum ChemistryEnvironmental PhotochemistryAtomic Carbon EmissionAtomic Fluorescence SpectroscopyHealth Sciences
Atomic carbon fluorescence, C I 1561, 1657, and 1931 Å, has been observed from photodissociation of CO 2 , and the production cross sections have been measured. A line emission source provided the primary photons at wavelengths from threshold to 420 Å. The present results suggest that the excited carbon atoms are produced by total dissociation of CO 2 into three atoms. The cross sections for producing the O I 1304‐Å fluorescence through photodissociation of CO 2 are found to be less than 10 −2 Mb in the wavelength region from 420 to 835 Å. The present data have implications with respect to photochemical processes in the atmospheres of Mars and Venus.
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Mariner 6 and 7 Ultraviolet Spectrometer Experiment: Upper atmosphere data
C. A. Barth, C. W. Hord, J. B. Pearce et al. · Journal of Geophysical Research Atmospheres · 1971 · 247 citations · Full text
Carbon monoxide in the Venus atmosphere
P. Connes, J. Connes, L. D. Kaplan et al. · The Astrophysical Journal · 1968 · 141 citations