VUV photochemistry simulation of planetary upper atmosphere using synchrotron radiation

The coupling of a gas reactor, named APSIS, with a vacuum-ultraviolet (VUV) beamline at the SOLEIL synchrotron radiation facility, for a photochemistry study of gas mixtures, is reported. The reactor may be irradiated windowless with gas pressures up to hundreds of millibar, and thus allows the effe...

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Publié dans:	Journal of synchrotron radiation. - 1994. - 20(2013), Pt 4 vom: 07. Juli, Seite 587-90
Auteur principal:	Carrasco, Nathalie (Auteur)
Autres auteurs:	Giuliani, Alexandre, Correia, Jean Jacques, Cernogora, Guy
Format:	Article en ligne
Langue:	English
Publié:	2013
Accès à la collection:	Journal of synchrotron radiation
Sujets:	Journal Article Titan VUV photochemistry atmosphere planets reactivity