Mimicking Titan's upper atmosphere reactivity with a RF-capacitively coupled N2-CH4 plasma

Nathalie Carrasco 1 Thomas Gautier 1 Et-Touhami Es-Sebbar 1 P. Pernot 2 Guy Cernogora 1
1 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
Abstract : Titan is the largest satellite of Saturn. Its upper atmosphere is well-known for the production of a phochemical organic smog. We simulate this ionospheric chemistry with a RF plasma setup. We present here the study of the gas phase composition, neutral and positively charged species, correlated with aerosol production efficiency
Complete list of metadatas

Cited literature [3 references]  Display  Hide  Download

https://hal.archives-ouvertes.fr/hal-00741736
Contributor : Catherine Cardon <>
Submitted on : Monday, October 15, 2012 - 11:12:24 AM
Last modification on : Wednesday, May 22, 2019 - 8:17:27 PM
Long-term archiving on : Wednesday, January 16, 2013 - 3:37:59 AM

File

escampig2012_carrasco.pdf
Files produced by the author(s)

Identifiers

  • HAL Id : hal-00741736, version 1

Citation

Nathalie Carrasco, Thomas Gautier, Et-Touhami Es-Sebbar, P. Pernot, Guy Cernogora. Mimicking Titan's upper atmosphere reactivity with a RF-capacitively coupled N2-CH4 plasma. ESCAMPIG 2012 (Europhysics Conference on the Atomic and Molecular Physics of Ionized Gases), Jul 2012, Viana do Castelo, Portugal. 2 p. ⟨hal-00741736⟩

Share

Metrics

Record views

585

Files downloads

70