Kattawar G W, Plass G N, Hitzfelder S J
Appl Opt. 1976 Mar 1;15(3):632-47. doi: 10.1364/AO.15.000632.
The complete radiation field including polarization is calculated by the matrix operator method for scattering layers of various optical thicknesses. Results obtained for Rayleigh scattering are compared with those for scattering from a continental haze. Radiances calculated using Stokes vectors show differences as large as 23% compared to the approximate scalar theory of radiative transfer, while the same differences are only of the order of 0.1% for a continental haze phase function. The polarization of the reflected and transmitted radiation is given for a wide range of optical thicknesses of the scattering layer, for various solar zenith angles, and various surface albedos. Two entirely different types of neutral points occur for aerosol phase functions. Rayleigh-like neutral points (RNP) arise from the zero polarization in single scattering that occurs for all phase functions at scattering angles of 0 degrees and 180 degrees . For Rayleigh phase functions, the position of the RNP varies appreciably with the optical thickness of the scattering layer. At low solar elevations there may be four RNP. For a continental haze phase function the position of the RNP in the reflected radiation shows only a small variation with the optical thickness, and the RNP exists in the transmitted radiation only for extremely small optical thicknesses. Another type of neutral point (NRNP) exists for aerosol phase functions. It is associated with the zeros of the single scattered polarization, which occur between the end points of the curve; these are called non-Rayleigh neutral points (NRNP). There may be from zero to four of these neutral points associated with each zero of the single scattering curve. They occur over a range of azimuthal angles, unlike the RNP that are in the principal plane only. The position of these neutral points is given as a function of solar angle and optical thickness.
利用矩阵算子法计算了包括偏振在内的完整辐射场,该辐射场适用于各种光学厚度的散射层。将瑞利散射的结果与大陆霾散射的结果进行了比较。使用斯托克斯矢量计算的辐射亮度与近似标量辐射传输理论相比,差异高达23%,而对于大陆霾相位函数,相同的差异仅为0.1%左右。给出了散射层在各种光学厚度、不同太阳天顶角和不同地表反照率下反射和透射辐射的偏振情况。气溶胶相位函数会出现两种完全不同类型的中性点。类似瑞利的中性点(RNP)源于单次散射中的零偏振,这种零偏振在所有相位函数的0度和180度散射角处都会出现。对于瑞利相位函数,RNP的位置随散射层的光学厚度有明显变化。在低太阳高度时可能有四个RNP。对于大陆霾相位函数,反射辐射中RNP的位置随光学厚度的变化很小,并且RNP仅在极小的光学厚度下才存在于透射辐射中。气溶胶相位函数还存在另一种类型的中性点(NRNP)。它与单次散射偏振的零点相关,这些零点出现在曲线的端点之间;这些被称为非瑞利中性点(NRNP)。与单次散射曲线的每个零点相关的这些中性点可能有零个到四个。它们出现在一系列方位角范围内,这与仅在主平面内的RNP不同。给出了这些中性点的位置作为太阳角度和光学厚度的函数。