ATMOSPHERIC SULFUR PHOTOCHEMISTRY ON HOT JUPITERS

We develop a new 1D photochemical kinetics code to address stratospheric chemistry and stratospheric heating in hot Jupiters. Here we address optically active S-containing species and CO2 at 1200 0 at T > 1200 K. HS is probably more important than S2, as it is generally more abundant than S2 under h... View More