Top: dust composition volume fraction V_s/V_tot as a function of pressure at θ = 0° (Left) and θ = 45° (Right) in Δφ = + 45° longitude intervals. Grain composition is generally dominated by silicate-oxides including MgSiO₃[s] apart from localised regions such as 10^-2...10^-1 bar at φ = 0°, 45°, θ = 0°. Fe[s] dominates at 10^-2...10^-1 bar at φ = 0°, θ = 45°. Fe[s] grains remain at the cloud base as the most thermally stable element. Bottom: key showing line-style and colour of our considered dust species.