Relative intensity against position angle from G-band observations (symbols) at the Dutch Open Telescope on La Palma (Spain) and modeling in this work at 0.43 μm (solid) for the egress during the 2004 Venus transit. The intensities and position angle are defined by Tanga et al. (2012). To reproduce the peak in brightness away from the South Pole, we needed to shift the reference h_cloud-latitude profile by about 20°. For a color version of the figure, see the electronic journal.