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Updated: Aug 15, 2026

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Scattering coefficient determination in turbid media with backscattered polarized light
Franck Jaillon1, Hervé Saint-Jalmes
1Université Claude Bernard Lyon, 1 CNRS UMR 5012-CPE, Laboratoire de Résonance Magnétique Nucléaire, La Doua 3, rue Victor Grignard, 69616 Villeurbanne, France.
Abstract:
A simple empirical method is presented to determine the scattering coefficient mu' s from backscattered polarized images of turbid media. It uses the ratio, pixel by pixel, of two images that are the second and the first backscattered Stokes parameter images Q and I, respectively. Taking this image ratio, then integrating it over the azimuth angle, we get a function depending on the distance from the light entrance point. This function has a maximum. Using Monte Carlo simulations, for a fixed reduced scattering coefficient mu s and for an anisotropy factor g varying between 0 and 0.8, it is found a linear relationship between the scattering coefficient mu s and the inverse of the maximum position of this function.

