An adequate kinetic model of photochemical aerosol formation in Titan's atmosphere.
The photochemistry of hydrocarbons in Titan's atmosphere is modeled by a comprehensive kinetic scheme, containing 732 elementary reactions and 147 species up to C60. Four groups of the hydrocarbons are considered: Polyacetylenes (PA), Polyvinyles (PV), Vinylacetylenes (VA) and Allenes (Polyenes).
Dimitrov
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Department of Geophysics and Planetary Sciences, Tel-Aviv University, Israel.
Bar-Nun
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D000336:Aerosols / Q000737:chemistry*; D001272:Atmosphere / Q000737:chemistry*; D005118:Extraterrestrial Environment; D006838:Hydrocarbons / Q000737:chemistry*; D007700:Kinetics; D008956:Models, Chemical; D010777:Photochemistry; D018539:Saturn
D000336:Aerosols; D006838:Hydrocarbons