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- W1661926741 abstract "We have begun to create a comprehensive set of thermal infrared (TIR, approx. 1650-200/cm, approx. 6-50 microns) spectra of palagonitic and hydrothermally altered soils that exhibit a range of mineralogical and chemical compositions for use in analyzing MGS TES data. Palagonite, a phyllosilicate-poor hydrolytically altered tephra, has been suggested as a possible component of the martian soil/dust based on visible and near infrared (VNIR) spectral similarities with martian dusty regions. The chemistry and crystallinity of altered tephras are highly variable depending on the parent material and local environmental conditions, and are important indicators of alteration processes." @default.
- W1661926741 created "2016-06-24" @default.
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- W1661926741 date "2003-01-01" @default.
- W1661926741 modified "2023-09-26" @default.
- W1661926741 title "Thermal Emission Spectra of Altered Tephras and Constraints on the Composition of Martian Dust" @default.
- W1661926741 hasPublicationYear "2003" @default.
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