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Abstract
During the Clementine Mission both oblique and vertical multispectral images were collected. The oblique and vertical images from a single spectral band collected during the same orbit form a stereo pair that can be used to derive the topography. These stereo pairs were used to derive the topography of an area surrounding the lunar South Pole (90°S - 64°S latitude) and North Pole (90°N - 64°N latitude). In addition, during the Clementine mission laser altimeter data were collected. A goal was to match the photogrammetric topographic data to the topographic data collected by the laser altimeter. This required developing some innovative techniques to deal with mismatches between the photogrammetric topographic data set and the laser altimetry topographic data.
| Publication type | Conference Paper |
|---|---|
| Publication Subtype | Conference Paper |
| Title | Combining lunar photogrammetric topographic data with Clementine LIDAR data |
| Year Published | 2001 |
| Language | English |
| Publisher | English |
| Contributing office(s) | Astrogeology Science Center |
| Description | 3 p. |
| Larger Work Type | Book |
| Larger Work Subtype | Conference publication |
| Larger Work Title | Planetary Mapping: ISPRS Working Group IV/9 Workshop Proceedings |
| Conference Title | Planetary Mapping: ISPRS Working Group IV/9 Workshop |
| Conference Date | 2001 |
| Google Analytic Metrics | Metrics page |