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Links to Publicly Available Input Data
- https://pds-geosciences.wustl.edu/missions/mars2020/places.htm
- https://pds-geosciences.wustl.edu/m2020/urn-nasa-pds-mars2020_rover_places
- https://pds-geosciences.wustl.edu/m2020/urn-nasa-pds-mars2020_rover_places/document/Mars2020_Rover_PLACES_PDS_SIS.pdf
To make contextual and orbital tilesets, Landform typically uses the best_interp view which inherits the manually localized solutions for rover end-of-drive locations from the best_tactical view, and also interpolates the other rover positions from the telemetry view between those. Landform does not use PLACES to make tactical tilesets.
- https://astrogeology.usgs.gov/search/map/Mars/Mars2020/JEZ_hirise_soc_006_DTM_MOLAtopography_DeltaGeoid_1m_Eqc_latTs0_lon0_blend40
- https://planetarymaps.usgs.gov/mosaic/mars2020_trn/HiRISE/JEZ_hirise_soc_006_DTM_MOLAtopography_DeltaGeoid_1m_Eqc_latTs0_lon0_blend40.tif
resolution: 1 sample per square meter
- https://astrogeology.usgs.gov/search/map/Mars/Mars2020/JEZ_hirise_soc_006_orthoMosaic_25cm_Eqc_latTs0_lon0_first
- https://planetarymaps.usgs.gov/mosaic/mars2020_trn/HiRISE/JEZ_hirise_soc_007_orthoMosaic_25cm_Ortho_blend120.tif
resolution: 4 samples per square meter
RAS, RZS:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_hazcam_ops_calibrated
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_hazcam_ops_calibrated
XYZ, UVW:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_hazcam_ops_stereo
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_hazcam_ops_stereo
obj:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_hazcam_ops_mesh
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_hazcam_ops_mesh
In contextual tilesets Landform typically uses
- Hazcam left and right eye front and rear radiometrically calibrated visible light images with nonlinear camera models (regex
[FB][LR].*RAS_N.*IMG), though zenith scaled radiance (RZSinstead ofRAS) can also be used - Hazcam left eye front and rear stereo vision point and normal clouds with nonlinear camaera models (regex
[FB]L.*(XYZ|UVW)_N.*IMG)
Landform can also make tactical tilesets from obj format Hazcam wedge meshes.
RAS, RZS:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_navcam_ops_calibrated
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_navcam_ops_calibrated
XYZ, UVW:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_navcam_ops_stereo
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_hazcam_ops_stereo
obj:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_navcam_ops_mesh
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_navcam_ops_mesh
In contextual tilesets Landform typically uses
- Navcam left and right eye radiometrically calibrated visible light images with nonlinear camera models (regex
N[LR].*RAS_N.*IMG), though zenith scaled radiance (RZSinstead ofRAS) can also be used - Navcam left eye stereo vision point and normal clouds with nonlinear camaera models (regex
NL.*(XYZ|UVW)_N.*IMG)
Landform can also make tactical tilesets from obj format Navcam wedge meshes.
RAS, RZS:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_mastcamz_ops_calibrated
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_mastcamz_ops_calibrated
obj:
- https://planetarydata.jpl.nasa.gov/img/data/mars2020/mars2020_mastcamz_ops_mesh
- https://pds-imaging.jpl.nasa.gov/beta/archive-explorer?mission=mars_2020&bundle=mars2020_mastcamz_ops_mesh
In contextual tilesets Landform typically uses
- left and right eye radiometrically calibrated visible light images with nonlinear camera models (regex
Z[LR].*RAS_N.*IMG), though zenith scaled radiance (RZSinstead ofRAS) can also be used
Landform can also make tactical tilesets from obj format Mastcam-Z wedge meshes.