Cloud structures for changing C/O = 0.43 (blue), 1.1 (red), and 1.5 (gray) for a prescribed Drift-Phoenix (T_gas, p_gas) structure for a giant gas planet with T_eff = 1600 K, log(g) = 3.0, initial solar element abundances. Left: 1st panel: input T_gas [K] and p_gas [bar], 2nd panel: nucleation rate log J_∗ [cm^-3 s^-1], 3rd panel: cloud particle number density log n_d [cm^-3], and 4th panel: mean cloud particle radius log ⟨ a ⟩ [μm]. Right: changing material composition, V_s/V_tot [%] (relative volume fractions of solid species s), of the cloud particles for different nucleation species.