Improvement of Valley Network 3D Geometry from HRSC DEMs Compared to MOLA Data

Details Improvement of Valley Network 3D Geometry from HRSC DEMs Compared to MOLA Data Improvement of Valley Network 3D Geometry from HRSC DEMs Compared to MOLA Data

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3152a&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3152

Computer Science

Scientific paper

Here we compare the organization of valley networks in three regions
(Huygens impact crater, Aeolis region and West Echus plateau) using MOLA
and HRSC DEMs, and HRSC nadir images in order to quantify the difference
of geometry between these datasets.

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