The CH4 abundance in the Uranus atmosphere according to spectral geometric albedo data

Details The CH4 abundance in the Uranus atmosphere according to spectral geometric albedo data The CH4 abundance in the Uranus atmosphere according to spectral geometric albedo data

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...18g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, May-June 1987, p. 18-26. In Russian.

Astronomy and Astrophysics

Astronomy

Albedo, Ammonia, Atmospheric Composition, Molecular Spectra, Spectral Reflectance, Uranus Atmosphere, Astronomical Models, Cloud Cover, Optical Thickness, Rayleigh Scattering, Spectrum Analysis

Scientific paper

New data on the geometric albedo of Uranus at 0.5-0.9 microns were analyzed and interpreted within the framework of a model with a semiinfinite scattering-absorbing cloud layer and an above-cloud atmosphere with Rayleigh scattering. The values for the cloud-layer volume density, equivalent width of the atmosphere above the clouds, and relative abundance of methane in the troposphere were varied. The present results suggest that the upper limit to the CH4 relative abundance in the Uranus atmosphere does not exceed 0.01.

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