Model VNIR optical constants of igneous powder rocks

Details Model VNIR optical constants of igneous powder rocks Model VNIR optical constants of igneous powder rocks

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..847c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.847

Computer Science

Scientific paper

In this paper we present preliminary results of the determination of the optical constants of complex silicates mixture obtained applying the Hapke radiative transfer model to visible-near infrared reflectance spectra. The selected silicates mixtures are representative of possibly igneous co-genetic rocks. We first calculated optical constants of the end-members represented by plagioclase samples and an assemblages of mafic minerals. The optical constants of the end-members were derived from the known composition of minerals and their grain-size ranges. Subsequently we modeled mixtures between the end-members and we compared the results with the measured spectra of those mixtures.

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