1D trajectory results from the 3D RHD HD 189733b atmosphere simulation used as input for the cloud formation model. Top row: (T_gas, p_gas) profiles in steps of longitude Δφ = + 45° at equatorial, θ = 0° and latitude, θ = 45° profiles. Bottom row: smoothed vertical gas velocities v_z [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.