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Inhomogeneous models of Titan's aerosol distributionA model of Titan's aerosol is presented which allows the particle size to vary with height. The model assumes a refractive index appropriate to an ethylene polymer and a mass flux independent of height equal to the value derived from laboratory measurements. The free parameters of the model are determined by fitting to the observed geometric albedo at 4000 and 6000 A. A methane spectrum is derived which is in excellent agreement with observations. An aerosol optical depth of about 5 is found in the visible, with the particle radius varying from 0.01 to 8 microns. The presence of an optically thick methane cloud at the temperature minimum is indicated.
Document ID
19840042255
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Podolak, M.
(Tel-Aviv Univ. Ramat-Aviv, Tel-Aviv, Israel)
Bar-Nun, A.
(Tel-Aviv Univ. Ramat-Aviv, Tel-Aviv, Israel)
Noy, N.
(Tel Aviv University Tel Aviv, Israel)
Giver, L. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Icarus
Volume: 57
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
84A25042
Funding Number(s)
CONTRACT_GRANT: NCA2-OR-340-002
Distribution Limits
Public
Copyright
Other

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