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Experimental and theoretical simulations of Titan's VUV photochemistry

2013
A new reactor, named APSIS (Atmospheric Photochemistry SImulated by Synchrotron), has been designed to simulate planetary atmospheric photochemistry [Peng et al. JGR-E. 2013, 118, 778]. We report here a study focusing on Titan's upper atmosphere. A nitrogen-methane gas flow was irradiated by a continuous 60-350 nm VUV beam provided by the DISCO line at
Peng, Z., Carrasco, Nathalie, Pernot, P.
openaire   +1 more source

Theoretical aspects of the photochemistry of adsorbed molecules

Journal of Photochemistry, 1981
Abraham Nitzan, L.E. Brus
openaire   +1 more source

Molecular Photochemistry: Recent Developments in Theory

Angewandte Chemie - International Edition, 2020
Leticia Gonzalez, Sebastian Mai
exaly  

Heterogeneous Photochemistry in the Atmosphere

Chemical Reviews, 2015
Markus Ammann   +2 more
exaly  

Theoretical aspects of the photochemistry of methanol, methylamine, and related materials

Journal of the American Chemical Society, 1983
E Kassab, E M Evleth
exaly  

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