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Ultraviolet observations of Titan from OAO-2High altitude deposition of energy in Titan's atmosphere can have a significant effect on the spectral distribution of emitted thermal radiation from the satellite. This reasoning led to the prediction of emission peaks at wavelengths corresponding to allowed bands of CH4 and trace photolysis products such as C2H6. Intermediate resolution infrared spectrophotometry has encouraged this interpretation of the infrared properties of Titan, and provided the basis for initial, detailed model.
Document ID
19740012374
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Caldwell, J. J. (Princeton Univ. NJ, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Publication Information
Publication: NASA. Ames Res. Center The Atmos. of Titan
Subject Category
Space Sciences
Accession Number
74N20487
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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