Quantitative laboratory spectra and spectral line parameters for the nu2 and nu4 bands of PH3 applicable to spectral radiative models of the atmosphere of Jupiter

Details Quantitative laboratory spectra and spectral line parameters for the nu2 and nu4 bands of PH3 applicable to spectral radiative models of the atmosphere of Jupiter Quantitative laboratory spectra and spectral line parameters for the nu2 and nu4 bands of PH3 applicable to spectral radiative models of the atmosphere of Jupiter

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jqsrt..24..211g&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 24, Sept. 1980, p. 211-218.

Computer Science

3

Absorption Spectra, Atmospheric Composition, Jupiter Atmosphere, Phosphines, Radiative Transfer, Spectral Line Width, Computer Programs, Fourier Transformation, Line Spectra, Spectral Bands, Spectral Resolution, Jupiter, Atmosphere, Models, Spectrum, Phosphine, Parameters, Absorption, Experiments, Comparisons, Data, Wavelengths, Spectroscopy, Analysis, Bands

Scientific paper

Quantitative laboratory PH3 absorption spectra were obtained in the 800-1350/cm region, at approximately 0.05/cm resolution, with gas amounts corresponding to observed PH3 absorptions in the atmosphere of Jupiter. A compilation of spectral line positions, intensities and ground state energies has been generated for the nu2 and nu4 bands of PH3. Line-by-line calculations have been compared with the experimental spectra.

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