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Properties of haze in the atmosphere of TritonVoyager UV spectrometer measurements of CH4 and haze of the Triton atmosphere combined with the haze brightness profile determined by the narrow angle camera are used to infer a haze optical thickness of 0.024 at 1500 A and 0.0078 in the spectral range of the narrow angle camera centered at 4700A, rho/gamma = 0.36 +/- 0.1 g/cu cm (gamma is the quantum yield of condensate), and values of r(c) varying from 0.1 +/- 0.02 micron at 30 km to 0.15 +/- 0.03 micron near the surface. Other auxiliary properties of the haze are also determined. The value found for rho/gamma corresponds to a packing coefficient of 0.6 gamma if C2H4 is the main condensible species.
Document ID
19920068976
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Krasnopolsky, V. A.
(NASA Headquarters Washington, DC United States)
Sandel, B. R.
(NASA Headquarters Washington, DC United States)
Herbert, F.
(Arizona, University Tucson, United States)
Date Acquired
August 15, 2013
Publication Date
July 25, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: E7 J
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
92A51600
Funding Number(s)
CONTRACT_GRANT: NAGW-610
CONTRACT_GRANT: NAGW-2441
Distribution Limits
Public
Copyright
Other

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