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Fig. 11


Number density of cloud particles nd [cm-3] interpolated across the globe (assuming latitudinal (north-south) symmetry) of HD 189733b. Top row: 10-4 bar, 10-3 bar. Middle row: 10-2 bar, 10-1 bar. Bottom row: 1 bar, 10 bar, respectively. The sub-stellar point is at φ = 0°, θ = 0°. The maximum number of cloud particles occurs on the nightside of the planet. Note: each plot contains a different colour scale.

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