Thermal inertia was estimated at high resolution from a data set within Gale Crater collected by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument on board the Mars Reconnaissance Orbiter. This result was then analysed alongside observations from the Curiosity rover to characterize surface properties within the scene, especially in and around the Glen Torridon region within Gale Crater. This data set consists of the CRISM scene (scene id FRT00021C92) processed to single-scattering albedo using the WUSTL hyperspectral processing pipeline (see https://www.hou.usra.edu/meetings/lpsc2019/pdf/2094.pdf, https://www.hou.usra.edu/meetings/lpsc2019/pdf/2690.pdf for details), related summary products derived from single-scat...
Physical properties of terrains encountered by the Curiosity rover during the rst 360 sols of operat...
AbstractMars Reconnaissance Orbiter Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) hyp...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
Thermal inertia was estimated at high resolution from a data set within Gale Crater collected by the...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
International audienceThe analysis of particle physical properties (grain size, shape and internal s...
The analysis of particle physical properties (grain size, shape and internal structure) and its orga...
Sediment/regolith history and mantling of underlying bedrock are important processes to understand f...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
<p>The most significant mobility challenges that planetary rovers encounter are compounded by loose,...
Thermal inertia, which represents the resistance to change in temperature of the upper few centimete...
The analysis of the surface texture from the particle (grain size, shape and internal structure) to ...
The Thermal Emission Imaging System (THEMIS) inertia mosaic of Jezero Crater was created following t...
Analysis of the Martian surface today can provide insight into the processes that may have affected ...
Physical properties of terrains encountered by the Curiosity rover during the rst 360 sols of operat...
AbstractMars Reconnaissance Orbiter Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) hyp...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
Thermal inertia was estimated at high resolution from a data set within Gale Crater collected by the...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
International audienceThe analysis of particle physical properties (grain size, shape and internal s...
The analysis of particle physical properties (grain size, shape and internal structure) and its orga...
Sediment/regolith history and mantling of underlying bedrock are important processes to understand f...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
<p>The most significant mobility challenges that planetary rovers encounter are compounded by loose,...
Thermal inertia, which represents the resistance to change in temperature of the upper few centimete...
The analysis of the surface texture from the particle (grain size, shape and internal structure) to ...
The Thermal Emission Imaging System (THEMIS) inertia mosaic of Jezero Crater was created following t...
Analysis of the Martian surface today can provide insight into the processes that may have affected ...
Physical properties of terrains encountered by the Curiosity rover during the rst 360 sols of operat...
AbstractMars Reconnaissance Orbiter Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) hyp...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...