Detail publikace

Titan's Atmosphere Chemistry Simulation in Atmospheric Glow Discharge

POLÁCHOVÁ, L. HORVÁTH, G. KRČMA, F. KLOHNOVÁ, K. MASON, N. ZÁHORAN, M. MATĚJČÍK, Š.

Originální název

Titan's Atmosphere Chemistry Simulation in Atmospheric Glow Discharge

Anglický název

Titan's Atmosphere Chemistry Simulation in Atmospheric Glow Discharge

Jazyk

en

Originální abstrakt

The formation of products produced in an atmospheric glow discharge fed by a N2-CH4 gas mixture with CH4 contents in range from 0.5% to 2% CH4 has been studied using Fourier Transform Infrared (FTIR). The measurements were carried out in flowing regime at ambient temperature and pressure. Measurements revealed HCN and NH3 to be the major products of the plasma with traces of C2H2. These same molecules were observed by the Cassini-Huygens probe in Titan's atmosphere.

Anglický abstrakt

The formation of products produced in an atmospheric glow discharge fed by a N2-CH4 gas mixture with CH4 contents in range from 0.5% to 2% CH4 has been studied using Fourier Transform Infrared (FTIR). The measurements were carried out in flowing regime at ambient temperature and pressure. Measurements revealed HCN and NH3 to be the major products of the plasma with traces of C2H2. These same molecules were observed by the Cassini-Huygens probe in Titan's atmosphere.

Dokumenty

BibTex


@inproceedings{BUT35613,
  author="Lucie {Töröková} and Gabriel {Horváth} and František {Krčma} and Karolína {Klohnová} and Nigel {Mason} and Miro {Záhoran} and Štefan {Matějčík}",
  title="Titan's Atmosphere Chemistry Simulation in Atmospheric Glow Discharge",
  annote="The formation of products produced in an atmospheric glow discharge fed by a N2-CH4 gas mixture with CH4 contents in range from 0.5% to 2% CH4 has been studied using Fourier Transform Infrared (FTIR). The measurements were carried out in flowing regime at ambient temperature and pressure. Measurements revealed HCN and NH3 to be the major products of the plasma with traces of C2H2. These same molecules were observed by the Cassini-Huygens probe in Titan's atmosphere.",
  booktitle="HAKONE XII - Book of Contributed Papers",
  chapter="35613",
  howpublished="electronic, physical medium",
  year="2010",
  month="september",
  pages="270--274",
  type="conference paper"
}