Infrared laboratory studies of synthetic planetary atmospheres

Details Infrared laboratory studies of synthetic planetary atmospheres Infrared laboratory studies of synthetic planetary atmospheres

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ksu..rept.....w&link_type=abstract

Semiannual Status Report, 1 Jun. - 30 Nov. 1977 Kansas State Univ., Manhattan. Dept. of Physics.

Physics

Atmospheric Models, Infrared Spectroscopy, Optical Properties, Planetary Atmospheres, Spectral Line Width, Absorption Spectra, Concentration (Composition), Liquefied Gases, Ozonosphere, Quantitative Analysis, Venus Clouds

Scientific paper

Topics covered include: the broadening of individual lines in the CO fundamental by various gases; total band absorptance as a function of absorber thickness and total effect pressure at various temperatures for bands of CO and N2O; nitric acid vapor content in the region of the ozone layer; optical properties of solid NH3; HSO4 concentration in Venus clouds; Burch's law of multiplicative transmittance for mixing absorbing gases when their lines are broadened by helium and hydrogen; ling strength and self-broadening parameters in the v3 fundamental of CO2 and N2O; optical constants of liquid ammonia, liquid methane, saturated hydrocarbons, ammonium hydride and ammonium salts.

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