Computer Science
Scientific paper
Apr 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icar...42...68m&link_type=abstract
Icarus, vol. 42, Apr. 1980, p. 68-70.
Computer Science
Albedo, Brightness Temperature, Neptune (Planet), Uranus (Planet), Atmospheric Models, Neptune Atmosphere, Opacity, Uranus Atmosphere, Planets, Uranus, Neptune, Brightness Temperature, Albedo, Comparisons, Phosphine, Opacity, Atmosphere, Methane, Absorption, Thermal Emissions, Reflectance, Observations, Gases, Vapor Pressure, Coefficients, Models, Wavelengths, Hydrogen, Element Ratios, Isotopes
Scientific paper
Five-micron brightness temperatures and brightness temperature upper limits for Uranus and Neptune have been obtained which are substantially lower than those of Jupiter and Saturn and which correspond to a geometric albedo of approximately 0.01, in agreement with results reported by Gillett and Rieke (1977). Phosphine and CH3D, which are observed at 5 microns on Jupiter and Saturn, are discussed as possible sources of opacity at 5 microns in the atmospheres of Uranus and Neptune.
Beichman Charles Arnold
Macy William W.
Sinton William M.
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