Published December 29, 2021
| Version 1.0.0.
Dataset
Open
30-m HRSC DTM Mosaic of Gale Crater, Mars
Contributors
Supervisors:
- 1. University College London
- 2. Imperial College London
Description
Digital terrain model (DTM) mosaic of Gale crater, Mars, processed from High-Resolution Stereo Camera (HRSC) stereo images using the modification of DLR-VICAR described by Kim and Muller (2009).
Format: GeoTiff
Projection: Equidistant cylindrical
Datum: Spheroid (r = 3396.190 km)
Bit depth: Float32
Grid-spacing: 30 m/pixel
Terrain reference: 200-m MOLA and HRSC blended global DTM (Fergason et al. 2018)
HRSC source images: H1938_0000, H1927_0000, and H1916_0000
Notes
The first author is now at University of Glasgow. Contact: divya.persaud@glasgow.ac.uk.
Files
hrsc_km09_h1938_h1927_h1916-dtm-mosaic.tif
Files
(311.8 MB)
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Additional details
References
- Deen, R. G. 2015. "VICAR Quick-Start Guide." Jet Propulsion Laboratory.
- Fergason, R. L., T. M. Hare, and J. Laura. 2018. "HRSC and MOLA Blended Digital Elevation Model at 200m V2." Astrogeology PDS Annex, U.S. Geological Survey. 2018. http://bit.ly/HRSC_MOLA_Blend_v0.
- Kim, J.-R. 2010. "HRSC DTM Program."
- Kim, J.-R., and J.-P. Muller. 2009. "Multi-Resolution Topographic Data Extraction from Martian Stereo Imagery." Planetary and Space Science 57 (14–15): 2095–2112. https://doi.org/10.1016/j.pss.2009.09.024.
- Putri, A. R. D., P. Sidiropoulos, J.-P. Muller, H. G. Sebastian, and G. G. Michael. 2019. "A New South Polar Digital Terrain Model of Mars from the High Resolution Stereo Camera (HRSC) Onboard the ESA Mars Express." Planetary and Space Science. https://doi.org/10.1016/j.pss.2019.02.010.