Simulating the density of organic species in the atmosphere of Titan with a coupled ion-neutral photochemical model

V. Vuitton 1 V. Yelle 2 S.J. Klippenstein 3 S.M. Hörst 4 P. Lavvas 5
1 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble
2 LPL - Lunar and Planetary Laboratory [Tucson]
3 Chemical Sciences and Engineering Division [Argonne]
4 Morton K. Blaustein Department of Earth and Planetary Sciences [Baltimore]
5 GSMA - Groupe de spectrométrie moléculaire et atmosphérique - UMR 7331
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https://hal.univ-reims.fr/hal-02104659
Contributor : Barbara Groupe de Spectrométrie Moléculaire Et Atmosphérique <>
Submitted on : Friday, April 19, 2019 - 3:56:02 PM
Last modification on : Friday, December 6, 2019 - 4:58:20 PM

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V. Vuitton, V. Yelle, S.J. Klippenstein, S.M. Hörst, P. Lavvas. Simulating the density of organic species in the atmosphere of Titan with a coupled ion-neutral photochemical model. Icarus, Elsevier, 2019, 324, pp.120-197. ⟨10.1016/j.icarus.2018.06.013⟩. ⟨hal-02104659⟩

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