Quantitative laboratory spectra and spectral line parameters for the v2 and v4 bands of PH3 applicable to spectral radiative models of the atmosphere of Jupiter
- 30 September 1980
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 24 (3) , 211-218
- https://doi.org/10.1016/0022-4073(80)90063-1
Abstract
No abstract availableKeywords
This publication has 6 references indexed in Scilit:
- Infrared Observations of the Jovian System from Voyager 2Science, 1979
- High-resolution spectra of Jupiter in the 744-980 inverse centimeter spectral rangeThe Astrophysical Journal, 1979
- ν2 and ν4 fundamentals of phosphine occurring at 8–12 μmJournal of Molecular Spectroscopy, 1974
- Infrared determination of C for phosphine via perturbation-allowed Δ |k − l|= ± 3 transitions in the 3ν2 bandThe Journal of Chemical Physics, 1973
- Coriolis interactions about X-Y axes in symmetric topsJournal of Molecular Spectroscopy, 1966
- Absolute Infrared Intensities of Vibration Bands in Ammonia and PhosphineThe Journal of Chemical Physics, 1956