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The ultraviolet absorption spectrum of CO - Applications to planetary atmospheresLaboratory 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.
Document ID
19930049236
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
White, H. P.
(NASA Headquarters Washington, DC United States)
Hua, Xin-Min
(NASA Headquarters Washington, DC United States)
Caldwell, J.
(Inst. for Space and Terrestrial Science North York, Canada)
Chen, F. Z.
(NASA Headquarters Washington, DC United States)
Judge, D. L.
(NASA Headquarters Washington, DC United States)
Wu, C. Y. R.
(Southern California Univ. Los Angeles, CA, United States)
Date Acquired
August 16, 2013
Publication Date
March 25, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: E3
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A33233
Funding Number(s)
CONTRACT_GRANT: NSF DMR-88-21625
CONTRACT_GRANT: NAGW-1924
CONTRACT_GRANT: NSF AST-89-19862
CONTRACT_GRANT: NAS5-30294
Distribution Limits
Public
Copyright
Other

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