The Optical Constants of Olivine in the Near-Infrared as a Function of Iron Content

Details The Optical Constants of Olivine in the Near-Infrared as a Function of Iron Content The Optical Constants of Olivine in the Near-Infrared as a Function of Iron Content

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2745t&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2745

Physics

Scientific paper

Optical constants are important to first-principles modeling of the
spectral properties of planetary surfaces. We derived the optical
constants of olivine as a function of Fo content into 22 parameters by
using the modified Gaussian model.

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