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An adequate kinetic model of photochemical aerosol formation in Titan's atmosphere.
Dimitrov, V; Bar-Nun, A.
  • Dimitrov V; Department of Geophysics and Planetary Sciences, Tel-Aviv University, Israel.
Adv Space Res ; 19(7): 1103-12, 1997.
Article en En | MEDLINE | ID: mdl-11541339
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).
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Banco de datos: MEDLINE Asunto principal: Atmósfera / Saturno / Aerosoles / Hidrocarburos / Modelos Químicos Idioma: En Año: 1997 Tipo del documento: Article
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Banco de datos: MEDLINE Asunto principal: Atmósfera / Saturno / Aerosoles / Hidrocarburos / Modelos Químicos Idioma: En Año: 1997 Tipo del documento: Article