Cool (T_eff,P = 800 K), the transient (T_eff,P = 1600 K), the hot (T_eff,P = 2400 K) exoplanet atmospheres (log₁₀ɡ = 3 [cgs]) with an F type host star. 2D equatorial plane slices (θ = 0°) for the 1D profiles extracted from the 3D GCM models (Baeyens et al. 2022) show the main cloud formation properties: local gas temperature [K] (first row), total nucleation rate log₁₀( J_* / cm⁻³ s⁻¹) (second row), surface averaged mean particle size log₁₀ (〈a〉_A/ µm) overlayed with f_e = 10⁻⁷ (solid line; f_e = 10⁻⁶ (dashed); third row), mean molecular weight (fourth row). The outer limit for the pressure is fixed at 10^−3.5 bar for all models.