The wide variation in infrared brightness temperature of Titan is explained in terms of a greenhouse effect. Radiometric observations in the infrared and microwave frequencies indicate an alternate hot atmospheric model. Methane, ammonia, hydrogen atoms, and nitrogen atoms are suggested as main constituents for the Titan atmosphere.
Infrared photometry and spectrophotometry of Titan
1974-01-01
Conference paper
No indication
English
Near-infrared spectrophotometry of Titan
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