This website contains the derived data in the manuscript Meter-scale topographic roughness of the Moon: The effect of small impact craters by Yuzhen Cai and Wenzhe Fa that is published in Journal of Geophysical Research: Planets
The nature of the lunar crust provides crucial information on the Moon’s origin and subsequent evolu...
Impact bombardment during the first billion years after the formation of the Moon produced at least ...
International audienceWe have analyzed the Bouguer anomaly (BA) of~1200 complex craters in the lunar...
The datasets related to the work of Millimeter- to Decimeter-Scale Surface Slope and Roughness of th...
The datasets related to the work of of Morphological Characterization of Decimeter- to Hectometer-Sc...
This work seeks to understand past and present surface conditions on the Moon using two different bu...
Impact craters are essential and dominant features of the lunar surface. Under the presence of a ver...
[1] The acquisition of new global elevation data from the Lunar Orbiter Laser Altimeter, carried on ...
We analyze and compare the surface roughness of the Moon, Mercury and Mars by characterizing the sca...
We report the surface roughness analysis of the lunar highlands for the baseline range 0.15-100km. W...
We report roughness measurement results at the baseline scale from 0.15 to 100 km, using the digital...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
Impact cratering produces characteristic variations in the topographic power spectral density (PSD) ...
This website contains the derived data in the manuscript Regolith Properties in the Chang'E-5 Landin...
Landscape evolution on the Moon is driven by a relatively small number of physical mechanisms, makin...
The nature of the lunar crust provides crucial information on the Moon’s origin and subsequent evolu...
Impact bombardment during the first billion years after the formation of the Moon produced at least ...
International audienceWe have analyzed the Bouguer anomaly (BA) of~1200 complex craters in the lunar...
The datasets related to the work of Millimeter- to Decimeter-Scale Surface Slope and Roughness of th...
The datasets related to the work of of Morphological Characterization of Decimeter- to Hectometer-Sc...
This work seeks to understand past and present surface conditions on the Moon using two different bu...
Impact craters are essential and dominant features of the lunar surface. Under the presence of a ver...
[1] The acquisition of new global elevation data from the Lunar Orbiter Laser Altimeter, carried on ...
We analyze and compare the surface roughness of the Moon, Mercury and Mars by characterizing the sca...
We report the surface roughness analysis of the lunar highlands for the baseline range 0.15-100km. W...
We report roughness measurement results at the baseline scale from 0.15 to 100 km, using the digital...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
Impact cratering produces characteristic variations in the topographic power spectral density (PSD) ...
This website contains the derived data in the manuscript Regolith Properties in the Chang'E-5 Landin...
Landscape evolution on the Moon is driven by a relatively small number of physical mechanisms, makin...
The nature of the lunar crust provides crucial information on the Moon’s origin and subsequent evolu...
Impact bombardment during the first billion years after the formation of the Moon produced at least ...
International audienceWe have analyzed the Bouguer anomaly (BA) of~1200 complex craters in the lunar...
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