A reduced chemical kinetic model for Titan�s atmosphere has been developed. This new model with 18 species and 28 reactions\r\nincludes the mainfeatures of a more complete scheme, respecting the radiative fluxes. It has been verified against three key\r\nelements: a sensitivity analysis, the equilibrium chemical composition using shock tube simulations in CHEMKIN, and the results\r\nof computational fluid dynamics (CFDs) simulations.
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