Comparison of wind patterns, temperature maps at 10 mbar, cloud latitudinal distributions, and jet acceleration for simulations with Mg₂SiO₄ clouds at super-solar metallicity and particle sizes of 0.1, 1, and 10 μm. The first column is the cloudless simulation, and the following are the cloudy ones. Top row: Zonal mean and time-averaged zonal wind. Black contours are the mass stream function, with solid lines indicating a clockwise circulation and dashed lines an anti-clockwise circulation. Second row: Time-averaged temperature map at the 10 mbar isobaric level. Black contours denote the location of clouds. White vertical dashed lines are the terminators. Third row: Latitude-pressure map of the cloud distribution, averaged in time and longitude. Bottom panel: Vertically integrated jet zonal wind acceleration in zonal and time mean between 5 and 20 mbar. We show the decomposition into residual mean circulation, the eddy contributions, and the net acceleration.