Replication Data for: Analysis of the topographic roughness of the Moon using the Wavelet Leaders Method and the Lunar Digital Elevation Model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera

This repository contains the data generated by Lemelin et al. (2019)* regarding the analysis of the topographic roughness of the Moon using the Wavelet Leaders Method and the Lunar Digital Elevation Model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera. Near global mosaics (+/- 60 degrees in latitude) of the Holder exponent values and the correlation coefficient can be found for the three scaling regimes analysed. Local mosaics of the Holder exponent values for the smallest scaling regime, and for the intermediate scaling regime (in some cases) can be found for the seven regions of interest analysed at a higher spatial resolution than the global product. The definition of the scaling regimes can be found in Lemelin et al. (2019). These data products are stored as geotiffs using the GCS_Moon_2000 (datum D_Moon_2000) coordinate system. The data used to generate figures 7 and 8 in Lemelin et al. (2019) can also be found here as an excel table. Data products: • global holder exponents scales j=0-1 (geotiff): 65 Mb • global holder exponents scales j=2-6 (geotiff): 65 Mb • global holder exponents scales j=7-9 (geotiff): 65 Mb • global correl coeffs scales j=0-1 (geotiff): 65 Mb • global correl coeffs scales j=2-6 (geotiff): 65 Mb • global correl coeffs scales j=7-9 (geotiff): 65 Mb • holder Aristarchus scales j=0-2: 33 Mb • holder Copernicus scales j=0-2: 16 Mb • holder Tycho scales j=0-2: 16 Mb • holder Orientale scales j=0-2: 263 Mb • holder Orientale scales j=3-7: 263 Mb • holder Crisium scales j=0-2: 263 Mb • holder Crisium scales j=3-7: 263 Mb • holder Rima Ariadeus scales j=0-2: 33 Mb • holder Rima Ariadeus scales j=3-7: 33Mb • holder Schiller-Schickard scales j=0-2: 66 Mb • data table used to generate the plots in figures 7&8: 43 Kb *Lemelin, M., Daly, M., and Deliège, A. (2019) Analysis of the topographic roughness of the Moon using the Wavelet Leaders Method and the Lunar Digital Elevation Model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera, Journal of Geophysical Research - Planets.