Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..185m&link_type=abstract
In ESA, Symposium on Titan p 185-190 (SEE N92-32348 23-91)
Biology
4
Atmospheric Composition, Gas Mixtures, Haze, Optical Properties, Organic Chemistry, Satellite Atmospheres, Solids, Titan, Carbon, Exobiology, Hydrogen, Nitrogen, Spectroscopic Analysis
Scientific paper
The optical properties of the laboratory tholin is considered, and an attempt is made to critically evaluate the analog between laboratory tholin and Titan tholin. The processes that form the solid haze material from the gaseous atmosphere are considered. It is suggested that the N/C ratio may be a useful signature of the processes that determine the haze production rate.
McKay Christopher P.
Toon Brian O.
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