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Fig. 7

image

Top: dust composition volume fraction Vs/Vtot 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.

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