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Fig. 1


Illustration of the sample trajectories (black points) taken from the 3D radiative-hydrodynamic model atmosphere of HD 189733b (Dobbs-Dixon & Agol 2013); longitudes φ = 0°...315° in steps of Δφ = + 45°, latitudes θ = 0°, + 45°. The sub-stellar point is at φ = 0°, θ = 0°. We assume that the sample trajectories are latitudinal (north-south) symmetric.

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