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Digital Topography Models for Martian Surfaces
IEEE Geoscience and Remote Sensing Letters, 2005We propose to use an unsupervised automated classification of topographic features on Mars in order to speed up geomorphic and geologic mapping of the planet. We construct a digital topography model (DTM), a multilayer grid that stores various kinds of topographical information for every pixel in a site.
Tomasz F. Stepinski, Ricardo Vilalta
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Martian surface and crust: Review and synthesis
Icarus, 1973The nature of the classical marking of Mars are studied on the basis of Mariner 9 data and some earlier data. The analysis leads to a model of the Martian crust. Evidence for petrologic distinctions between surface materials in dark and light regions is obtained.
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Dielectric Map of the Martian Surface
2005We have undertaken laboratory electromagnetic characterization of the total set of minerals identified by TES [1] on the Martian surface in order to investigate experimentally the dielectric properties of the sediments covering it in the frequency range from 1 to 1000 MHz.
Heggy, Essam, Pommerol, Antoine
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2008
Phenomenal new observations from Earth-based telescopes and Mars-based orbiters, landers, and rovers have dramatically advanced our understanding of the past environments on Mars. These include the first global-scale infrared and reflectance spectroscopic maps of the surface, leading to the discovery of key minerals indicative of specific past climate ...
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Phenomenal new observations from Earth-based telescopes and Mars-based orbiters, landers, and rovers have dramatically advanced our understanding of the past environments on Mars. These include the first global-scale infrared and reflectance spectroscopic maps of the surface, leading to the discovery of key minerals indicative of specific past climate ...
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Some comments on “the composition of the Martian surface”
Icarus, 1965Martian surface composition of either fine or coarse grained silicates coated with finely divided ...
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Polarimetric and photometric simulation of the Martian surface
Icarus, 1969Abstract An approach is presented to obtain a truly rational interpretation of the Martian surface and atmosphere. Polarimetric and photometric properties of ore specimens (limonite, siderite, desert varnish, and serpentine), considered good prospects for the Martian surface, are presented for the colors B(0.48 μ), G(0.54 μ), and I(1.0 μ).
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Surface processes modifying Martian craters
Icarus, 1968Abstract Martian craters, even through many times more abundant than thought from initial inspection of Mariner IV photos, are less numerous, shallower, and have gentler slopes than craters on lunar uplands. This implies more effective action on Mars of some exogenous process or processes of erosion or deposition.
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Antibody–drug conjugates: Smart chemotherapy delivery across tumor histologies
Ca-A Cancer Journal for Clinicians, 2022Javier Cortés +2 more
exaly
Surface Pressures in the Martian Highlands and Lowlands
Nature, 1967CONFLICTING opinions have been expressed on the question of elevation of the Martian dark areas (maria) relative to the bright areas (deserts).
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