The structure of the Uranian atmosphere: Constraints from the geometric albedo spectrum and H2 and CH4 line profiles
- 31 March 1986
- Vol. 65 (2-3) , 406-441
- https://doi.org/10.1016/0019-1035(86)90146-6
Abstract
No abstract availableKeywords
This publication has 40 references indexed in Scilit:
- Interpretation of the 6818.9-Å methane feature observed on Jupiter, Saturn, and UranusIcarus, 1983
- High-resolution observations of the 6815-Å band of methane in the major planetsIcarus, 1983
- Line positions and strengths in the H2 quadrupole spectrumThe Astrophysical Journal, 1982
- Application of methane band-model parameters to the visible and near-infrared spectrum of UranusIcarus, 1980
- Determination of the H2 4-0 S/1/ quadrupole line strength and pressure shiftThe Astrophysical Journal, 1980
- Intensity and pressure shift of the H2 /4,0/ S/1/ quadrupole lineThe Astrophysical Journal, 1978
- Theory of line shape in pressure-induced absorptionCanadian Journal of Physics, 1976
- Limb Brightening on Uranus: a PredictionThe Astrophysical Journal, 1973
- The Atmosphere of UranusThe Astrophysical Journal, 1971
- Quadrupole Transitions in the H2, HD and D2MoleculesJournal of the Atmospheric Sciences, 1969