Interpretation of the 6818.9-Å methane line in terms of inhomogeneous scattering models for Uranus and Neptune
- 30 April 1978
- Vol. 34 (1), 20-27
- https://doi.org/10.1016/0019-1035(78)90121-5
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- On the 6825 A band of methane as observed in Uranus and NeptuneThe Astrophysical Journal, 1977
- A saturation model of the atmosphere of UranusIcarus, 1977
- The atmosphere of Saturn: An infrared perspectiveIcarus, 1977
- An analysis of Saturn's methane 3ν3 band profiles in terms of an inhomogeneous atmosphereIcarus, 1976
- On the 6825 A band of methaneThe Astrophysical Journal, 1976
- Laboratory band strengths of methane and their application to the atmospheres of Jupiter, Saturn, Uranus, Neptune, and TitanThe Astrophysical Journal, 1976
- Uranian methane abundance, rotational temperature, and effective pressure from the 6800 A bandThe Astrophysical Journal, 1975
- An estimate of the temperature and abundance of CH4 and other molecules in the atmosphere of UranusIcarus, 1975
- The significance of pressure shifts for the interpretation of H2 quadrupole lines in planetary spectraIcarus, 1974
- The temperature dependence of the half widths of some self-and foreign-gas-broadened lines of methaneJournal of Quantitative Spectroscopy and Radiative Transfer, 1973