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Fig. 2

image

1D trajectory results from the 3D RHD HD 189733b atmosphere simulation used as input for the cloud formation model. Top row: (Tgas, pgas) profiles in steps of longitude Δφ = + 45° at equatorial, θ = 0° and latitude, θ = 45° profiles. Bottom row: smoothed vertical gas velocities vz [km s-1] in steps of longitude Δφ = + 45° at equatorial, θ = 0° and latitude, θ = 45° profiles. Both latitudes show a temperature inversion on the dayside. The sub-stellar point is at φ = 0°, θ = 0°. Solid, dotted and dashed lines indicate dayside, day-night terminator and nightside profiles respectively.

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