Methane abundance in the atmosphere of Uranus

Author:

Teifel V.G.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference24 articles.

1. Geometric albedo of Uranus at λ 0.5–1.1 μm;Atai;Astron. Tzirkular,1979

2. The spectrum of Uranus at λ 0.47–1.00 μm: A comparison with the simplest models of the CH4 absorption bands formation;Atai;Astron. Vestnik,1981

3. The atmosphere of Uranus;Belton;Astrophys. J.,1971

4. Application of the methane band-model parameters to the visible and near-infrared spectrum of Uranus;Benner;Icarus,1980

5. Monochromatic brightness coefficients of the major planets;Bugaenko;Astron. Vestnik,1972

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1. Empirical rovibrational energy levels for methane;Journal of Quantitative Spectroscopy and Radiative Transfer;2024-04

2. Planetary research in Kazakhstan;Planetary and Space Science;2001-11

3. The upper atmosphere of Uranus: EUV occultations observed by Voyager 2;Journal of Geophysical Research: Space Physics;1987-12-30

4. The atmosphere of Uranus: Results of radio occultation measurements with Voyager 2;Journal of Geophysical Research: Space Physics;1987-12-30

5. Uranus' (3-0) H2 quadrupole line profiles;Icarus;1987-04

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