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Estimates of the Albedo of Powderlike Surfaces in the Geometrical Optics Approximation

机译:几何光学近似中粉末状表面反照率的估计

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Results of computer simulation of light scattering by powderlike media composed of large semitransparent particles of different shapes are presented. The geometrical optics approach is used. The cases of particles of spherical, cubic, and random shapes are considered. The one-dimensional geometrical optics model of light scattering by powderlike media, which finds application in investigations of planetary surfaces, meteorites, and lunar samples, is briefly described. The numerical simulation allowed us to estimate the error of this model, which turned out to be within the limits of several percent. The albedo calculated by using the one-dimensional model is shown to be closest to the "three-dimensional" reflectance of the surfaces at a phase angle of about 60°. This albedo also approximates fairly well the integrated reflectance, which in laboratory measurements is determined with the help of an integrating sphere.
机译:给出了由粉末状介质散射的计算机模拟结果,该粉末状介质由不同形状的大半透明颗粒组成。使用了几何光学方法。考虑球形,立方和随机形状的粒子的情况。简要描述了粉末状介质散射光的一维几何光学模型,该模型可用于研究行星表面,陨石和月球样品。数值模拟使我们能够估计该模型的误差,结果证明误差在百分之几的范围内。通过一维模型计算出的反照率显示出在约60°的相角处最接近表面的“三维”反射率。该反照率也相当好地近似了积分反射率,该积分反射率在实验室测量中是借助积分球确定的。

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