Trajectory-based Simulation of Far-infrared Collision-induced Absorption Profiles of CH4-N2 for Modeling Titan's Atmosphere

Trajectory-based Simulation of Far-infrared Collision-induced Absorption Profiles of CH for Modeling Titan's AtmosphereDOI: info:10.3847/1538-4365/ac36d3v. 25833
Finenko, Artem A., Bézard, Bruno, Gordon, Iouli E., Chistikov, Daniil N., Lokshtanov, Sergei E., Petrov, Sergey V., and Vigasin, Andrey A. 2022. "Trajectory-based Simulation of Far-infrared Collision-induced Absorption Profiles of CH4-N2 for Modeling Titan's Atmosphere." The Astrophysical Journal Supplement Series, 258 33. https://doi.org/10.3847/1538-4365/ac36d3.
ID: 165500
Type: article
Keywords: SAO