Study of transmitted light through the atmosphere of Titan

Details Study of transmitted light through the atmosphere of Titan Study of transmitted light through the atmosphere of Titan

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..397t&link_type=abstract

In ESA, Symposium on Titan p 397-399 (SEE N92-32348 23-91)

Statistics

Computation

Atmospheric Composition, Atmospheric Models, Light Transmission, Photochemical Reactions, Satellite Atmospheres, Titan, Aerosols, Albedo, Mathematical Models, Monte Carlo Method, Rayleigh Scattering

Scientific paper

A temperature pressure density model of Titan's atmosphere was used to describe the structure of the atmosphere and the major components identified. The optical depth was calculated for Rayleigh and Mie scattering and a Monte Carlo model developed. The history of one photon and the calculations performed on it are outlined. Results of computation with a ground albedo equal to 0.5 are presented together with calculated Boud and geometric albedos.

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