We present a study of the effect of wind-driven advection on the chemical composition of hot Jupiter atmospheres using a fully-consistent 3D hydrodynamics, chemistry and radiative transfer code, the M
We observed the evolution of Jupiter’s polar cyclonic structures over two years between February 2017 and February 2019, using polar observations by the Jovian InfraRed Auroral Mapper, JIRAM, on the J
This data set comprises uncalibratedand calibrated data from the Cassini Composite Infrared Spectrometer(CIRS) instrument. The basic data is comprised of uncalibrated raw...
