LINKING SEDIMENT THERMAL INERTIA TO DEPOSITIONAL CONTEXT ON EARTH AND MARS: DATA
- Ari Koeppel
Publication date
April 2023
DOIAbstract
Thermophysical, grain, and spectroscopic data collected from Mars-analog field sites on Earth
Thermophysical, grain, and spectroscopic data collected from Mars-analog field sites on Earth
We study the Martian fine-grained dark material by focussing on a global selection of impact craters...
The heat flux and thus temperature gradient of the Martian crust is critical for comparison with mea...
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...
The final copy of this dissertation has been examined by the signatories, and we find that both the ...
Thermal inertia, which represents the resistance to change in temperature of the upper few centimete...
Sediment/regolith history and mantling of underlying bedrock are important processes to understand f...
As Viking Lander 1 touched down on Mars one of its footpads fully penetrated a patch of loose fine-g...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
Orbital thermal infrared (TIR) remote sensing is an important tool for characterizing geologic surfa...
Thermal Emission Spectrometer (TES) are well suited for determining the subpixel abundance of rocks ...
International audienceThe thermophysical structure of the martian surface is the result of various p...
Analysis of the Martian surface today can provide insight into the processes that may have affected ...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
Thermal anomalies associated with ore-mineralization (Pb-Cu-Zn and Fe) were studied using thermal in...
We study the Martian fine-grained dark material by focussing on a global selection of impact craters...
The heat flux and thus temperature gradient of the Martian crust is critical for comparison with mea...
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...
The final copy of this dissertation has been examined by the signatories, and we find that both the ...
Thermal inertia, which represents the resistance to change in temperature of the upper few centimete...
Sediment/regolith history and mantling of underlying bedrock are important processes to understand f...
As Viking Lander 1 touched down on Mars one of its footpads fully penetrated a patch of loose fine-g...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
Orbital thermal infrared (TIR) remote sensing is an important tool for characterizing geologic surfa...
Thermal Emission Spectrometer (TES) are well suited for determining the subpixel abundance of rocks ...
International audienceThe thermophysical structure of the martian surface is the result of various p...
Analysis of the Martian surface today can provide insight into the processes that may have affected ...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
Thermal anomalies associated with ore-mineralization (Pb-Cu-Zn and Fe) were studied using thermal in...
We study the Martian fine-grained dark material by focussing on a global selection of impact craters...
The heat flux and thus temperature gradient of the Martian crust is critical for comparison with mea...
Thermal inertia was estimated at high resolution from a data set within Gale Crater collected by the...
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