Fig. 7
From: The turbulent dynamics of Jupiter’s and Saturn’s weather layers: order out of chaos?
Distribution of moist convection in a Jason simulation of Jupiter’s weather layer at a resolution of 0.7° × 0.7° in latitude × longitude (Young and Read 2020), showing (a) the net rate of change of humidity as a function of latitude and pressure, and (b) the fraction of convecting grid points as a function of pressure, showing the confinement of moist convection between ~ 4 bars and 200 hPa