Venusian infrared radiation: Approximate methods for computing spectrum in absorption bands of atmospheric gases

Details Venusian infrared radiation: Approximate methods for computing spectrum in absorption bands of atmospheric gases Venusian infrared radiation: Approximate methods for computing spectrum in absorption bands of atmospheric gases

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986rpspr...2..119m&link_type=abstract

In its USSR Report: Space (JPRS-USP-86-001) p 119-120 (SEE N86-20178 10-88) Transl. into ENGLISH from Kosmicheskiye Issledova

Physics

Absorption Spectra, Atmospheres, Gas Spectroscopy, Infrared Spectra, Planetary Radiation, Venus (Planet), Carbon Dioxide, Spectral Bands, Sulfur Dioxides, Water

Scientific paper

Approximate methods for calculating synthetic spectra in the H2O, CO2, and SO2 absorption bands are described which are used for a quantitative interpretation (chemical analysis and determination of cloud-layer parameters) of results of the Venera 15 and 16 infrared experiment. A simplified version of the line-by-line method is used for H2O; an equidistant-line method is used for CO2; and the overlapping-line method is used for CO2; and the overlapping-line method is used for SO2.

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