Sub-stellar (T_gas, p_gas)-profiles from the Carone (blue, extended inner boundary) and the Parmentier (red, standard inner boundary) GCM runs for WASP-43b. The comparison to the thermal stability curves (supersaturation ratio S = 1 for solar element abundances) of selected solid materials shows that the local temperature differences at p_gas ≈ 1 bar support our finding for the cloud particle material composition differences between the two models (Fig. 14). We note that the S = 1 curves do not represent our full kinetic model approach and are provided here for the purpose of visualisation.