UV-VIS-NIR Reflectance Spectra of Intimate Mixtures of Synthetic CaCO3 and Amorphous SiO2: 0.35-2.5 µm; Implications for the Spectral Identification of Shocked Assemblages on Mars

Details UV-VIS-NIR Reflectance Spectra of Intimate Mixtures of Synthetic CaCO3 and Amorphous SiO2: 0.35-2.5 µm; Implications for the Spectral Identification of Shocked Assemblages on Mars UV-VIS-NIR Reflectance Spectra of Intimate Mixtures of Synthetic CaCO3 and Amorphous SiO2: 0.35-2.5 µm; Implications for the Spectral Identification of Shocked Assemblages on Mars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2110c&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2110

Computer Science

1

Scientific paper

A comparison of the spectroscopic features generated in shock
metamorphosed and melted/recrystallized carbonates from the Haughton
impact structure with spectroscopic features in an intimate mixture
suite of synthetic calcite and amorphous silica.

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