Physics
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996p%26ss...44.1123o&link_type=abstract
Planetary and Space Science, v. 44, p. 1123-1133.
Physics
12
Scientific paper
A local control point network and a DTM (Digital Terrain Model) are derived from Clementine UVVIS multi-look angle images that were obtained on April 30, 1994, covering a small region of the Lunar Orientale Basin (19.5°S to 15°S and 84.5°W to 86.0°W). The nominal camera pointing and spacecraft trajectory data were photogrammetrically adjusted, a procedure which was found to improve estimates of the coordinates of 41 control points significantly to an internally consistent accuracy of 30 m in the horizontal and 50 m in the height direction. The terrain model correlates well with features identified in the image data, two craters, volcanic constructs, and the dark lava-filled Lacus Veris, located in a topographic depression. The terrain model indicates a steep 2000 m drop in elevation within a range of only 6-8 km towards the center of Orientale. Further studies of the lunar topography in this particular region using Clementine stereo data seem well warranted and feasible.
Albertz J.
Cook Anthony C.
Duxbury Tom
Jaumann Ralf
Oberst Jürgen
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