The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres

Details The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.5491w&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. E3, p. 5491-5497.

Physics

3

Absorption Spectra, Atmospheric Composition, Carbon Monoxide, Planetary Atmospheres, Ultraviolet Absorption, Absorption Cross Sections, Mars Atmosphere, Satellite Atmospheres, Ultraviolet Spectra, Planets, Atmosphere, Ultraviolet, Wavelengths, Absorption, Abundance, Spectra, Carbon Monoxide, Laboratory Studies, Temperature, Pressure, Satellites, Stratosphere, Theoretical Studies, Model, Experiments, Comparisons, Mars, Saturn, Titan, Albedo, Mixing Ratio, Procedure, Calculations, Parameters

Scientific paper

Laboratory gas-phase photoabsorption cross sections of the CO Cameron 0-0 band and the underlying pseudocontinuum have been measured at a temperature of 147 K and pressures of about 200 mbar, conditions similar to ambient in various planetary and satellite stratospheres in the solar system. A theoretical modeling program has also been used to calculate the band's spectrum. Agreement between the theoretical and the experimental spectra is very good. Models suggest that the observations of the CO Cameron band using the Hubble Space Telescope will be straightforward for Mars, but marginal for Titan.

Affiliated with

Also associated with

No associations

Rating

The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ultraviolet absorption spectrum of CO - Applications to planetary atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1446657