Similar to Fig. 6, except for i = 90°. The images on the left illustrate the system at ν = 0°, which for i = 90° is precisely in front of the star, i.e., the nightside of the planet is turned toward the observer. To keep the structures in the curves visible, we limited the vertical axis in the graphs for F-. In some cases, the forward-scattering peaks are therefore cut off. The missing peak values are the following: for λ_r = 0°, the lines reach 6.13, 5.37, and 2.25 for γ = 0°, 30°, and 60°, respectively. For λ_r = 30°, they reach 5.36, 4.61, and 1.55, and for λ_r = 30°, 2.38 and 1.65 for γ = 0° and γ = 30°, respectively.