ATMOSIM: This platform simulates the chemistry of planetary atmospheres.
Two complementary experiments based at LATMOS
This infrastructure is part of a project that has received funding from the European Research Council (ERC)
under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 636829)
Gas phase chemistry is initiated by UV photons. 
Atmospheric aerosol formation simulated by a dusty plasma experiment. 
 VUV photochemistry simulation of planetary upper atmosphere using synchrotron radiation
 PAMPRE: A dusty plasma experiment for Titan's tholins production and study