Intensity on the Venusian disc at distances of 6, 12, 18, and 24 arcsec from the centre, and along its limb (taking the radius of the Venusian disc retrieved along with K₁ by the LMA optimization, 29.29 arcsec), as a function of azimuth. The black curves follow the values from the mean transit image and the red curves the values reproduced in the artificial image by the convolution with K₁. The blue curves represent the intensity obtained in the artificial image by fixing A_i at zero. The intensity fluctuations along the Venusian limb arises from aliasing artefacts.