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Fig. 6


Joint-PDF distributions of the brightness temperature in K2V (left), K3 (center), and K2R (right) for different combinations of the radiative transfer geometry (1.5D or 3D) and the line scattering (CRD or XRD). Intensities are calculated using Model 1 atmosphere at μ = 1. The red line is y = x. The correlation coefficient r is given on each panel. Contours encompass 50% (white) and 90% (black) of the pixels. Each column in the Joint PDF is scaled to maximum contrast. The short black lines at the univariate histograms (each panel’s top and right) show mean values.

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