As Fig. 6, but in Galactic disk regions for VVV representative fields at the furthest (left panel, at VVV field d115, centered at l = 295°̣44, b = 1°̣63) and closest (right panel, at VVV field d076, centered at l = 349°̣41, b = −0°̣56) longitudes from the Galactic bulge available to the VVV observations. In the CMD in the left panel, we are able to clearly identify the MS and RC of the Galactic disk, even though extinction at low latitudes broaden sequences from further away stars, while in the CMD in the right panel, confusion increases as the Galactic bulge populations become more dominant. A series of online movies show the CMDs for all the different VVV disk fields.