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The 8-13 micron observations of TitanNarrow band observations of Titan at selected wavelengths in the 8-13 micron range show evidence for a strong temperature inversion and the existence of at least one more spectroscopically active component in the atmosphere in addition to H2 and CH4.
Document ID
19740012382
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Gillett, F. C. (Kitt Peak National Observatory Tucson, AZ, United States)
Forrest, W. J. (Kitt Peak National Observatory Tucson, AZ, United States)
Merrill, K. M. (Kitt Peak National Observatory Tucson, AZ, 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
74N20495
Funding Number(s)
CONTRACT_GRANT: NGL-05-005-003
Distribution Limits
Public
Copyright
Public Use Permitted.

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