Jaillon Franck, Saint-Jalmes Hervé
Université Claude Bernard Lyon, 1 CNRS UMR 5012-CPE, Laboratoire de Résonance Magnétique Nucléaire, La Doua 3, rue Victor Grignard, 69616 Villeurbanne, France.
J Biomed Opt. 2005 May-Jun;10(3):034016. doi: 10.1117/1.1924715.
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.
提出了一种简单的经验方法,用于从浑浊介质的后向散射偏振图像中确定散射系数μ's。该方法逐像素地使用分别为第二次和第一次后向散射斯托克斯参数图像Q和I的两幅图像的比值。取该图像比值,然后在方位角上对其进行积分,我们得到一个取决于距光入射点距离的函数。该函数有一个最大值。通过蒙特卡罗模拟,对于固定的约化散射系数μ s以及在0到0.8之间变化的各向异性因子g,发现散射系数μ s与该函数最大值位置的倒数之间存在线性关系。