3D surface profiles obtained by shadow analysis

This figure shows 3D surface profiles of selected regions obtained by shadow analysis only (without shape from shading) based on multiple pixel-synchronous images. These examples show that shadow analysis enables us to reconstruct features at the limit of image resolution, for which photoclinometric approaches are hardly suitable. Figure (a) shows the region between lunar craters Hesiodus and Wolf, viewed from the north-east. The result is based on an evaluation of two images taken on April 21, 2002, and on September 30, 2002. Very shallow slopes of the mare surface around the mountain chains which amount to a few tenths of a degree are revealed by bidirectional shadow analysis. Figure (b) shows the eastern face of the Montes Recti mountains along with very shallow ridges of 160 to 180 m altitude, viewed from the east. Reconstruction is based on images obtained on September 30, 2002, and on January 12, 2003, respectively. Figure (c) displays the reconstruction result for the interesting crater Reinhold B, viewed from the south-west, obtained with two images taken on September 30, 2002, and on January 12, 2003. Although the crater floor looks flat, shadow analysis reveals that the altitude difference between the ridge of the eastern (right) crater rim and the centre of the crater floor amounts to 1000 m and is thus 700 m larger than the altitude difference between the ridge of the western (left) rim and the western part of the crater floor, while the ridges of both rims are 300 to 400 m above the level of the environment. This means that the western part of the crater floor is on about the same level as the environment, while its central part is 700 m deeper. Hence, the western half of the crater floor is inclined by an angle of approximately 4 degrees, given the crater diameter of 19 km. Figure (d) shows a cross-section of Reinhold B which additionally contains the results of shadow analysis obtained with a third image (June 09, 2003) obtained at again different illumination conditions (points marked by "a"). Here, an identical ground level east and west of the crater has been assumed.
 

Back to lunar DEM main page