A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera
We present an improved lunar digital elevation model (DEM) covering latitudes within ±60°, at a horizontal resolution of 512 pixels per degree (~60 m at the equator) and a typical vertical accuracy ~3 to 4 m. This DEM is constructed from ~4.5×109geodetically-accurate topographic heights from the Lun...
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Elsevier BV
2018
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Online Access: | http://hdl.handle.net/1721.1/118411 https://orcid.org/0000-0003-2652-8017 |
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author | Barker, M.K. Neumann, G.A. Haruyama, J. Mazarico, Erwan Matias Zuber, Maria Smith, David Edmund |
author2 | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
author_facet | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Barker, M.K. Neumann, G.A. Haruyama, J. Mazarico, Erwan Matias Zuber, Maria Smith, David Edmund |
author_sort | Barker, M.K. |
collection | MIT |
description | We present an improved lunar digital elevation model (DEM) covering latitudes within ±60°, at a horizontal resolution of 512 pixels per degree (~60 m at the equator) and a typical vertical accuracy ~3 to 4 m. This DEM is constructed from ~4.5×109geodetically-accurate topographic heights from the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter, to which we co-registered 43,200 stereo-derived DEMs (each 1°×1°) from the SELENE Terrain Camera (TC) (~1010pixels total). After co-registration, approximately 90% of the TC DEMs show root-mean-square vertical residuals with the LOLA data of <5 m compared to ~ 50% prior to co-registration. We use the co-registered TC data to estimate and correct orbital and pointing geolocation errors from the LOLA altimetric profiles (typically amounting to <10 m horizontally and <1 m vertically). By combining both co-registered datasets, we obtain a near-global DEM with high geodetic accuracy, and without the need for surface interpolation. We evaluate the resulting LOLA + TC merged DEM (designated as "SLDEM2015") with particular attention to quantifying seams and crossover errors. |
first_indexed | 2024-09-23T08:53:18Z |
format | Article |
id | mit-1721.1/118411 |
institution | Massachusetts Institute of Technology |
last_indexed | 2024-09-23T08:53:18Z |
publishDate | 2018 |
publisher | Elsevier BV |
record_format | dspace |
spelling | mit-1721.1/1184112024-05-15T02:51:40Z A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera Barker, M.K. Neumann, G.A. Haruyama, J. Mazarico, Erwan Matias Zuber, Maria Smith, David Edmund Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Mazarico, Erwan Matias Zuber, Maria Smith, David E. We present an improved lunar digital elevation model (DEM) covering latitudes within ±60°, at a horizontal resolution of 512 pixels per degree (~60 m at the equator) and a typical vertical accuracy ~3 to 4 m. This DEM is constructed from ~4.5×109geodetically-accurate topographic heights from the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter, to which we co-registered 43,200 stereo-derived DEMs (each 1°×1°) from the SELENE Terrain Camera (TC) (~1010pixels total). After co-registration, approximately 90% of the TC DEMs show root-mean-square vertical residuals with the LOLA data of <5 m compared to ~ 50% prior to co-registration. We use the co-registered TC data to estimate and correct orbital and pointing geolocation errors from the LOLA altimetric profiles (typically amounting to <10 m horizontally and <1 m vertically). By combining both co-registered datasets, we obtain a near-global DEM with high geodetic accuracy, and without the need for surface interpolation. We evaluate the resulting LOLA + TC merged DEM (designated as "SLDEM2015") with particular attention to quantifying seams and crossover errors. United States. National Aeronautics and Space Administration. Lunar Reconnaissance Orbiter Project and Planetary Geology and Geophysics Program 2018-10-10T13:38:21Z 2018-10-10T13:38:21Z 2015-08 2015-06 2018-10-05T15:15:54Z Article http://purl.org/eprint/type/JournalArticle 00191035 http://hdl.handle.net/1721.1/118411 Barker, M.K., E. Mazarico, G.A. Neumann, M.T. Zuber, J. Haruyama, and D.E. Smith. “A New Lunar Digital Elevation Model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera.” Icarus 273 (July 2016): 346–355. https://orcid.org/0000-0003-2652-8017 http://dx.doi.org/10.1016/J.ICARUS.2015.07.039 Icarus Creative Commons Attribution-NonCommercial-NoDerivs License http://creativecommons.org/licenses/by-nc-nd/4.0/ application/pdf Elsevier BV Elsevier |
spellingShingle | Barker, M.K. Neumann, G.A. Haruyama, J. Mazarico, Erwan Matias Zuber, Maria Smith, David Edmund A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title | A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title_full | A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title_fullStr | A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title_full_unstemmed | A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title_short | A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera |
title_sort | new lunar digital elevation model from the lunar orbiter laser altimeter and selene terrain camera |
url | http://hdl.handle.net/1721.1/118411 https://orcid.org/0000-0003-2652-8017 |
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