Total nucleation rate J_* = ∑ J_i (cm⁻³ s⁻¹) for the 1D (T_gas, p_gas)-profiles (Fig. 2) for the hot giant gas planets WASP-43b, and the ultra-hot Jupiters WASP-18b, HAT-P-7b, WASP-103b, and WASP-121bs. The colour code is similar to Fig. 2. The lower right panel shows the day (solid lines) and nightside (dashed lines) averaged seed formation rates, excluding the terminator profiles. All depicted planets show seed formation on the nightside. Only WASP-43b enables the nucleation process on the dayside efficiently.