Research involving a test of multiplicative transmittance for mixed absorbing gases when their lines are broadened by H2 and He, which are constituents of the atmospheres of the major planets was conducted. The results indicate that the multiplicative law as originally formulated can be applied with confidence. The broadening of individual lines in the CO fundamental by various gases has been investigated. The results indicate that the ratio of the self-broadening ability of CO to the line-broadening ability of foreign gases is greater for lines in the band wings than for lines near the band center when the molecular mass of the broadener is less than that of CO. The results have been interpreted in terms of a phenomenological theory. Studi...
Ices in the atmospheres and on the surfaces of planets are thought to play important roles in the ev...
Accurate data on microwave and millimeter-wave properties of potential planetary atmospheric constit...
Flyby infrared absorption measurements in Martian atmosphere for determination of profiles of carbon...
The initial stages of the research were involved with a test of Burch's law of multiplicative transm...
Collisional broadening of infrared absorption lines with application to planetary atmosphere
Employing the techniques that were described in several publications for measuring infrared lineshif...
The development of high spectral resolution and highly sensitive long infrared wavelength instrument...
This research was supported, in part, by the National Aeronautics and Space Administration.Author In...
This work was supported by a Grant (NSC 1060) from NASA Langley Research Center. Mailing address for...
The aim was to obtain form laboratory measurements the molecular parameters needed to interpret obse...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
We obtain quantitative laboratory spectroscopic measurements of molecular constituents which are of ...
This is a proposal for laboratory measurements of the infrared (λ=1- 20 μm) optical constants of hyd...
A theoretical calculation was made of the CO2 infrared spectra of Earth and Venus atmospheres. The c...
International audienceWe report new optical constants (refractive index, n, and extinction coefficie...
Ices in the atmospheres and on the surfaces of planets are thought to play important roles in the ev...
Accurate data on microwave and millimeter-wave properties of potential planetary atmospheric constit...
Flyby infrared absorption measurements in Martian atmosphere for determination of profiles of carbon...
The initial stages of the research were involved with a test of Burch's law of multiplicative transm...
Collisional broadening of infrared absorption lines with application to planetary atmosphere
Employing the techniques that were described in several publications for measuring infrared lineshif...
The development of high spectral resolution and highly sensitive long infrared wavelength instrument...
This research was supported, in part, by the National Aeronautics and Space Administration.Author In...
This work was supported by a Grant (NSC 1060) from NASA Langley Research Center. Mailing address for...
The aim was to obtain form laboratory measurements the molecular parameters needed to interpret obse...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
We obtain quantitative laboratory spectroscopic measurements of molecular constituents which are of ...
This is a proposal for laboratory measurements of the infrared (λ=1- 20 μm) optical constants of hyd...
A theoretical calculation was made of the CO2 infrared spectra of Earth and Venus atmospheres. The c...
International audienceWe report new optical constants (refractive index, n, and extinction coefficie...
Ices in the atmospheres and on the surfaces of planets are thought to play important roles in the ev...
Accurate data on microwave and millimeter-wave properties of potential planetary atmospheric constit...
Flyby infrared absorption measurements in Martian atmosphere for determination of profiles of carbon...