On the ortho-para equilibrium of H2 in the atmospheres of the Jovian planets
- 31 January 1978
- Vol. 33 (1), 210-216
- https://doi.org/10.1016/0019-1035(78)90034-9
Abstract
No abstract availableKeywords
Funding Information
- National Aeronautics and Space Administration
This publication has 9 references indexed in Scilit:
- The atmosphere of Saturn: An infrared perspectiveIcarus, 1977
- The aerosol distribution in Uranus' atmosphere - Interpretation of the hydrogen spectrumThe Astrophysical Journal, 1976
- Spatially resolved spectroscopy of Jupiter. I - H2 quadrupole 4-0 S/1/ lineThe Astrophysical Journal, 1976
- Spectroscopic photoelectric imaging Fabry-Perot interferometer: its development and preliminary observational resultsApplied Optics, 1976
- The significance of pressure shifts for the interpretation of H2 quadrupole lines in planetary spectraIcarus, 1974
- Collision-Narrowed Curves of Growth for H2Applied to New Photoelectric Observations of JupiterJournal of the Atmospheric Sciences, 1969
- Quadrupole Transitions in the H2, HD and D2MoleculesJournal of the Atmospheric Sciences, 1969
- The Interpretation of Intensities in Diatomic Molecular SpectraThe Astrophysical Journal Supplement Series, 1967
- Molecular hydrogen features in the spectra of Saturn and UranusIcarus, 1966