Thermal inertia and albedo provide information on the distribution of surface materials on Mars. These parameters have been mapped globally on Mars by the Thermal Emission Spectrometer (TES) onboard the Mars Global Surveyor. Two-dimensional clusters of thermal inertia and albedo reflect the thermophysical attributes of the dominant materials on the surface. In this paper three automated, non-deterministic, algorithmic classification methods are employed for defining thermophysical units: Expectation Maximisation of a Gaussian Mixture Model; Iterative Self-Organizing Data Analysis Technique (ISODATA); and Maximum Likelihood. We analyse the behaviour of the thermophysical classes resulting from the three classifiers, operating on the 2007 TES...
abstract: The temperature of a planet's surface depends on numerous physical factors, including ther...
For many regions on Mars the surface composition and its geological history has been debated in lite...
A method for separating the spectral signatures of the Martian surface and atmosphere was developed ...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
© 2014 by the authors. Thermal inertia and albedo provide information on the distribution of surface...
Maps of thermal inertia-albedo units and thermal inertia-elevation units on Mars’ surface have been ...
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, 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...
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 ...
In this paper, we present a new methodology for the simultaneous retrieval of surface and atmospheri...
Albedo and thermal property correlations of the topography of Mars were conducted with emphases upon...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
abstract: The temperature of a planet's surface depends on numerous physical factors, including ther...
For many regions on Mars the surface composition and its geological history has been debated in lite...
A method for separating the spectral signatures of the Martian surface and atmosphere was developed ...
Thermal inertia and albedo provide information on the distribution of surface materials on Mars. The...
© 2014 by the authors. Thermal inertia and albedo provide information on the distribution of surface...
Maps of thermal inertia-albedo units and thermal inertia-elevation units on Mars’ surface have been ...
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, 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...
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 ...
In this paper, we present a new methodology for the simultaneous retrieval of surface and atmospheri...
Albedo and thermal property correlations of the topography of Mars were conducted with emphases upon...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
abstract: The temperature of a planet's surface depends on numerous physical factors, including ther...
For many regions on Mars the surface composition and its geological history has been debated in lite...
A method for separating the spectral signatures of the Martian surface and atmosphere was developed ...