Ultraviolet complex refractive index of Martian dust Laboratory measurements of terrestrial analogs

Details Ultraviolet complex refractive index of Martian dust Laboratory measurements of terrestrial analogs Ultraviolet complex refractive index of Martian dust Laboratory measurements of terrestrial analogs

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icar...25..344e&link_type=abstract

Icarus, vol. 25, June 1975, p. 344-355.

Physics

Optics

5

Atmospheric Models, Dust Storms, Mars Surface, Refractivity, Ultraviolet Photometry, Absorptivity, Analogies, Atmospheric Optics, Atmospheric Refraction, Atmospheric Scattering, Mars Atmosphere, Optical Measurement, Scattering Coefficients

Scientific paper

The optical complex index of refraction of four candidate Martian surface materials has been determined between 0.185 and 0.4 microns using a modified Kubelka-Munk scattering theory. The cadidate materials were limonite, andesite, montmorillonite, and basalt. The effect of scattering has been removed from the results. Also presented are diffuse reflection and transmission data on these samples.

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