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    Infrared photometry and spectrophotometry of Titan (1974)
    In:  CASI
    Details
    Publication Date: 2016-06-07
    Description: 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.
    Keywords: SPACE SCIENCES
    Type: NASA. Ames Res. Center The Atmos. of Titan; p 12-16
    Format: application/pdf
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