Radiative-transfer intensities for λ_obs = 1.6 μm. The max(I) for the logarithmic colour scale is taken for each plot individually, after application of an artificial coronagraph of radius 10 AU. The (τ = 1)-surfaces from r = 0 and z = ∞ are indicated by dotted orange and blue lines, respectively. Rows: inclinations , columns: results without (first and fourth) and with (second and third) dusty wind outflow; ‘fixed’ model on the left, ‘variable’ one on the right. The wind signature is most noticeable at high inclinations, revealing a chimney-like structure with a distinctly narrower opening angle than the disk surface; it remains clearly less bright than said disk surface. The ‘variable’ dust scale height yields a much fainter outflow signal.