Titan's atmosphere as observed by Cassini/VIMS solar occultations: CH${}_4$, CO and evidence for C${}_2$H${}_6$ absorption

L. Maltagliati, B. Bézard, S. Vinatier +6

We present an analysis of the VIMS solar occultations dataset, which allows us to extract vertically resolved information on the characteristics of Titan's atmosphere between 100-7…