Simulated observation for the 1 M_J planet with an integration time of 1 h and an angular resolution of 0.10″. Left: well-mixed case, center: dynamic case, right: radial brightness profiles of the disks in the well-mixed case (dashed black line) and the dynamic case (solid red line). From top to bottom, λ = 350   μm, 850 μm and 1.3 mm (the 2.7 mm image is not shown because it contains only noise). The scale on the images and radial profiles is in arcseconds.