Neutral composition of Titan's atmosphere. A theoretical model

Details Neutral composition of Titan's atmosphere. A theoretical model Neutral composition of Titan's atmosphere. A theoretical model

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..137l&link_type=abstract

In ESA, Symposium on Titan p 137-146 (SEE N92-32348 23-91)

Physics

Atmospheric Composition, Atmospheric Models, Hydrocarbons, Satellite Atmospheres, Titan, Diffusion, Kinetics, Photodissociation, Voyager Project

Scientific paper

Vertical profiles of hydrocarbon densities in the Titan's atmosphere were obtained by means of a theoretical model taking into account condensation, photochemical and dynamical processes and using a fixed aerosols distribution. The model is developed for noontime at the equatorial reqion, in equinox conditions with moderate solar activity and covers the 40 to 1400 km altitude region. A detailed study of the physical and chemical phenomena is performed and an analysis of their relative importance on the obtained concentrations is also carried out.

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