Mimicking Titan's upper atmosphere reactivity with a RF-capacitively coupled N2-CH4 plasma - Archive ouverte HAL Access content directly
Conference Papers Year : 2012

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

Nathalie Carrasco
Thomas Gautier
P. Pernot
Guy Cernogora
  • Function : Author

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
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Dates and versions

hal-00741736 , version 1 (15-10-2012)

Identifiers

  • HAL Id : hal-00741736 , version 1

Cite

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⟩
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