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data set:
LRO MOON LROC 5 RDR V1.0
Reduced data from Lunar Reconnaissance Orbiter Camera (LROC).
LUNAR RECONNAISSANCE ORBITER - LRO-L-LROC-5-RDR-V1.0 - starting 2009-06-30T00:00:00Z -
data set:
LRO MOON LROC 2 EDR V1.0
Un-calibrated data from Lunar Reconnaissance Orbiter Camera (LROC).
LUNAR RECONNAISSANCE ORBITER - LRO-L-LROC-2-EDR-V1.0 - starting 2009-06-30T00:00:00Z -
data set:
LRO MOON LROC 3 CDR V1.0
Calibrated data from Lunar Reconnaissance Orbiter Camera (LROC).
LUNAR RECONNAISSANCE ORBITER - LRO-L-LROC-3-CDR-V1.0 - starting 2009-07-31T23:59:59.999Z -
bundle:
Watkins 2018 Lunar Boulder Data
The Watkins 2018 Lunar Boulder PDS4 bundle -
instrument host:
LUNAR RECONNAISSANCE ORBITER
Information about the LUNAR RECONNAISSANCE ORBITER instrument host -
collection:
Lunar Topography and Photometric Cube Data V1.0
This package contains topography and photometric data generated by the Gaskell Stereophotoclinometry (SPC) software suite. It focuses on six regions on the Moon. These include wrinkle ridges at Dorsa Aldrovandi, two locations of the lunar swirl within Mare Ingenii, Karpinskiy crater, a swirl within Mare Moscoviense, Reiner Gamma, and Tsiolkovskiy crater. We generated regional Digital Terrain Models (DTM), each about 50 to 100 square kilometers, using Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images from both the right and left cameras. Depending on the location, each vertex of the topography represents heights every 5 to 0.7 meters, with an uncertainty of about one to two vertices. The topography data is provided in both cubes readable by the USGS ISIS program, and as a geoTIFF which can be read by programs such as ArcGIS. We generated photometric data (in cube format) that is aligned to, and has the same horizontal spacing as, the topographic cube data. For each LROC image, four cubes were generated; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. Each cube pixel represents the value at each vertex of the DTM. -
bundle:
Lunar Topography and Photometric Cube Data V1.0
This package contains topography and photometric data generated by the Gaskell Stereophotoclinometry (SPC) software suite. It focuses on six regions on the Moon. These include wrinkle ridges at Dorsa Aldrovandi, two locations of the lunar swirl within Mare Ingenii, Karpinskiy crater, a swirl within Mare Moscoviense, Reiner Gamma, and Tsiolkovskiy crater. We generated regional Digital Terrain Models (DTM), each about 50 to 100 square kilometers, using Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images from both the right and left cameras. Depending on the location, each vertex of the topography represents heights every 5 to 0.7 meters, with an uncertainty of about one to two vertices. The topography data is provided in both cubes readable by the USGS ISIS program, and as a geoTIFF which can be read by programs such as ArcGIS. We generated photometric data (in cube format) that is aligned to, and has the same horizontal spacing as, the topographic cube data. For each LROC image, four cubes were generated; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. Each cube pixel represents the value at each vertex of the DTM. -
collection:
Lunar Topography and Photometric Cube Data V1.0
This package contains topography and photometric data generated by the Gaskell Stereophotoclinometry (SPC) software suite. It focuses on six regions on the Moon. These include wrinkle ridges at Dorsa Aldrovandi, two locations of the lunar swirl within Mare Ingenii, Karpinskiy crater, a swirl within Mare Moscoviense, Reiner Gamma, and Tsiolkovskiy crater. We generated regional Digital Terrain Models (DTM), each about 50 to 100 square kilometers, using Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images from both the right and left cameras. Depending on the location, each vertex of the topography represents heights every 5 to 0.7 meters, with an uncertainty of about one to two vertices. The topography data is provided in both cubes readable by the USGS ISIS program, and as a geoTIFF which can be read by programs such as ArcGIS. We generated photometric data (in cube format) that is aligned to, and has the same horizontal spacing as, the topographic cube data. For each LROC image, four cubes were generated; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. Each cube pixel represents the value at each vertex of the DTM. -
collection:
Lunar_Boulder_data
Collection of lunar boulder data from around small impact craters for regolith production study.
Data Sets and Information