SPICAM/Mars-Express : Vertical profiles of aerosols extinction [1], temperature and density of CO2 [2], density of O3 [3] derived from UV occultations. An user manual for the service is available here: http://vo.projet.latmos.ipsl.fr:8080/vo/SPICAM_VESPA_service_user_manual.pdf [1] Määttänen et al. (2013), A complete climatology of the aerosol vertical distribution on Mars from MEx/SPICAM UV solar occultations, Icarus, 223, doi:10.1016/j.icarus.2012.12.001 [2] Forget et al. (2009), Density and temperatures of the upper Martian atmosphere measured by stellar occultations with Mars Express SPICAM, J. Geophys. Res., 114, E01004, doi:10.1029/2008JE003086 [3] Lebonnois et al. (2006), Vertical distribution of ozone on Mars as measured by SPICAM/Mars Express using stellar occultations, J. Geophys. Res., 111, E09S05, doi:10.1029/2005JE002643
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