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Figure 1- Histogram measuring the displacement of the  coordinates of named lunar features derived from the Clementine images (ULCN2005) to coordinates derived from LOLA hill shade images and a global LROC WAC mosaic (LRO reference frame)
Figure 2- ULCN 2005 control points (green dots) overlaid  the frames were used for registration.on UVVIS image footprints (colored polygons)
Figure 4- Result of orientation correction. The left column is a set of ratio images derived from a pair of a map projected images (UVVIS: LUA2293F.102 and WAC: M123397685C) before (top) and after (bottom) applying the orientation correction

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