Currently, sci.esa.int is under review and not being updated. For the latest information and news from ESA science missions and scientific results, please visit esa.int. For a comprehensive overview of ESA’s Science Programme and its missions, please refer to science.esa.int. For in-depth technical information aimed at ESA's scientific communities, you may also wish to consult cosmos.esa.int.

Asset Publisher

Back An Adequate Kinetic Model of Photochemical Aerosol Formation in Titan's Atmosphere

An Adequate Kinetic Model of Photochemical Aerosol Formation in Titan's Atmosphere

Publication date: 02 April 1997

Authors: Dimitrov, V. and Bar-Nun, A.

Journal: Advances in Space Research
Volume: 19
Issue: 7
Page: pp. 1103-1112
Year: 1997

Copyright: Elsevier

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).

Link to publication
Last Update: Sep 1, 2019 9:36:09 AM
12-Apr-2026 01:07 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/WvPprdA

Images And Videos

Related Publications

Related Links

See Also

Documentation