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Simulating the spectral properties of iron-bearing regions of Mars using the SPLITS model
2014 IEEE Geoscience and Remote Sensing Symposium
The mineralogy and environmental history of Mars are been extensively investigated through remote sensing observations paired with laboratory and in situ experiments. A significant portion of these experiments is being devoted to the identification and quantification of different iron oxides present in the Martian terrains. Although such experiments can provide valuable information regarding the presence of these minerals, the scope of the resulting observations may be hindered by logistics anddoi:10.1109/igarss.2014.6947111 dblp:conf/igarss/BaranoskiKCM14 fatcat:tqz524qbrzdhdgqorzrgezfnhi