Topographic models for Discovery Rupes, Mercury using digital stereophotogrammetry and photoclinometry

Details Topographic models for Discovery Rupes, Mercury using digital stereophotogrammetry and photoclinometry Topographic models for Discovery Rupes, Mercury using digital stereophotogrammetry and photoclinometry

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1509w&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 509.

Mathematics

1

Mercury Surface, Topography, Stereophotography, Photogrammetry, Tectonics, Mathematical Models, Mariner 10 Space Probe, Satellite Imagery

Scientific paper

Photoclinometric profiles were generated across Discovery Rupes in order to provide an independent check of the DEM. Using recalibrated Mariner 10 images and employing the Lommel-Seeliger/Lamber photometric function, photoclinometric profiles across Discovery Rupes were successfully generated. The horizontal DN, the brightness value of a horizontal surface, was estimated by determining the average of a 9x9 array of pixels. A preliminary comparison of photoclinometric profiles across Discovery and coterminous profiles extracted from the DEM reveals that the difference in maximum relief is less than 10 percent.

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