Disk-integrated πF_n and P_s as functions of phase angle α for the Jupiter-like model planet with polar hazes as used in Figs. 9 and 10 at: λ = 0.55 μm (black, solid lines), 0.75 μm (red, dotted lines), and 0.95 μm (green, dashed lines). Also shown are the lines for model planets with the clouds but without the hazes: λ = 0.55 μm (blue, dashed-dotted lines), 0.75 μm (grey, dashed-triple-dotted lines), and 0.95 μm (magenta, long-dashed lines).