Matches in SemOpenAlex for { <https://semopenalex.org/work/W3190913080> ?p ?o ?g. }
- W3190913080 endingPage "845" @default.
- W3190913080 startingPage "845" @default.
- W3190913080 abstract "Recent satellite observations and the deconvolution of remote sensing data have shown the existence of various carbonate minerals in different solar system bodies. Emissivity, from 403 to 803 K, and reflectance spectra at 300 and 193 K of selected carbonates minerals with different ratios of Na:Ca and water amounts were respectively collected at 3–20 μm and at 1–16 μm. All reflectance spectra show absorption features in the 1.9–2.5 and 3.4–4.0 μm areas due to overtone and a combination of CO32− and fundamental vibrational models at ≈9.09, 11.35, 7.06, and 14.7 μm. The increase of the Na:Ca ratio in anhydrous samples produces a shift of the absorption features in the 3.4–4.0 μm area toward shorter wavelengths, and the peak at 3.9 μm doubles in the presence of a CO32− oxygen group shared with two cations in minerals having more complex structures. The comparison of the bands at ≈669 and ≈794 cm−1 in the emissivity spectra collected at high temperatures indicates that around 600 K, phase transitions occurred in natrite and thermonatrite. The reflectance spectra measured at 193 K reveal a fine structure compared to spectra collected at room temperature. The comparison of laboratory results with the spectrum of Ceres’s brightest crater Occator from the Dawn mission, taken as a case study, showed how the anhydrous samples, shortite and nyerereite, studied in this work can also be hypothesized for Ceres’s surface beyond that already suggested (trona, natrite, thermonatrite)." @default.
- W3190913080 created "2021-08-16" @default.
- W3190913080 creator A5058324077 @default.
- W3190913080 creator A5059498892 @default.
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- W3190913080 creator A5062302776 @default.
- W3190913080 creator A5072188855 @default.
- W3190913080 creator A5075618186 @default.
- W3190913080 creator A5084635796 @default.
- W3190913080 date "2021-08-05" @default.
- W3190913080 modified "2023-09-30" @default.
- W3190913080 title "NIR-MID Reflectance and Emissivity Study at Different Temperatures of Sodium Carbonate Minerals: Spectra Characterization and Implication for Remote Sensing Identification" @default.
- W3190913080 cites W1638771311 @default.
- W3190913080 cites W191739862 @default.
- W3190913080 cites W1964370137 @default.
- W3190913080 cites W1967226936 @default.
- W3190913080 cites W1968630458 @default.
- W3190913080 cites W1973740431 @default.
- W3190913080 cites W1974297322 @default.
- W3190913080 cites W1975479777 @default.
- W3190913080 cites W1978558455 @default.
- W3190913080 cites W1981520460 @default.
- W3190913080 cites W1983475289 @default.
- W3190913080 cites W1983690826 @default.
- W3190913080 cites W1986067510 @default.
- W3190913080 cites W1986530877 @default.
- W3190913080 cites W1986947350 @default.
- W3190913080 cites W1987076206 @default.
- W3190913080 cites W1993397335 @default.
- W3190913080 cites W2006479510 @default.
- W3190913080 cites W2009866352 @default.
- W3190913080 cites W2013235808 @default.
- W3190913080 cites W2013593997 @default.
- W3190913080 cites W2015713046 @default.
- W3190913080 cites W2016260972 @default.
- W3190913080 cites W2016376046 @default.
- W3190913080 cites W2016873947 @default.
- W3190913080 cites W2018753133 @default.
- W3190913080 cites W2032410888 @default.
- W3190913080 cites W2035143991 @default.
- W3190913080 cites W2041632711 @default.
- W3190913080 cites W2045139855 @default.
- W3190913080 cites W2060709501 @default.
- W3190913080 cites W2066045775 @default.
- W3190913080 cites W2069409503 @default.
- W3190913080 cites W2069698695 @default.
- W3190913080 cites W2076120657 @default.
- W3190913080 cites W2076609619 @default.
- W3190913080 cites W2078222544 @default.
- W3190913080 cites W2083001970 @default.
- W3190913080 cites W2083870523 @default.
- W3190913080 cites W2085362480 @default.
- W3190913080 cites W2094939710 @default.
- W3190913080 cites W2095814622 @default.
- W3190913080 cites W2100489794 @default.
- W3190913080 cites W2102920959 @default.
- W3190913080 cites W2120468983 @default.
- W3190913080 cites W2131109655 @default.
- W3190913080 cites W2132216432 @default.
- W3190913080 cites W2136954203 @default.
- W3190913080 cites W2137152051 @default.
- W3190913080 cites W2161736871 @default.
- W3190913080 cites W2192394225 @default.
- W3190913080 cites W2287533622 @default.
- W3190913080 cites W2301557771 @default.
- W3190913080 cites W2321039488 @default.
- W3190913080 cites W2324966600 @default.
- W3190913080 cites W2468294605 @default.
- W3190913080 cites W2511139331 @default.
- W3190913080 cites W2514424123 @default.
- W3190913080 cites W2558961138 @default.
- W3190913080 cites W2567618975 @default.
- W3190913080 cites W2576889528 @default.
- W3190913080 cites W2606286065 @default.
- W3190913080 cites W2739631214 @default.
- W3190913080 cites W2748959038 @default.
- W3190913080 cites W2755779991 @default.
- W3190913080 cites W2780544899 @default.
- W3190913080 cites W2791129288 @default.
- W3190913080 cites W2792396913 @default.
- W3190913080 cites W2806826649 @default.
- W3190913080 cites W2886455253 @default.
- W3190913080 cites W2886667211 @default.
- W3190913080 cites W2888476524 @default.
- W3190913080 cites W2897083338 @default.
- W3190913080 cites W2903541436 @default.
- W3190913080 cites W2923854211 @default.
- W3190913080 cites W2972803007 @default.
- W3190913080 cites W2999869065 @default.
- W3190913080 cites W3000975969 @default.
- W3190913080 cites W3008547805 @default.
- W3190913080 cites W3023383796 @default.
- W3190913080 cites W3028431305 @default.
- W3190913080 cites W3048696055 @default.
- W3190913080 cites W3091112064 @default.
- W3190913080 cites W4205232972 @default.
- W3190913080 cites W4255650847 @default.
- W3190913080 doi "https://doi.org/10.3390/min11080845" @default.