Sizova I M
Appl Opt. 1992 Oct 1;31(28):5930-6. doi: 10.1364/AO.31.005930.
Numerical and analytical simulations of Fraunhofer diffraction by oddly shaped apertures and exponential light amplitudes show that within an accuracy of 20-40%, the dependencies of the normalized encircled energy epsilon on ?, the fraction of the energy transmitted by the aperture within a given polar angle ? are similar in shape when ? is normalized by lambda/rho. Here rho is the size parameter of the aperture geometry (its shape and size) and of the light-amplitude profile. For a small ?, rho = rho(l,eff) = (Sigma(eff)/pi)((1/2)) depends on the effective aperture area Sigma(eff), which is calculated through the axial light intensity. For a large ?, rho = rho(2,eff) = 2Sigma(eff)/Rho(eff) depends on Sigma(eff) and the corresponding perimeter Rho(eff). In the case of a uniform light-amplitude distribution the normalization of rho(1) and rho(2) corresponds to the well-known expansion of epsilon(?) for small and large ?.
对形状不规则的孔径和指数光振幅的夫琅禾费衍射进行的数值和解析模拟表明,在20% - 40%的精度范围内,当用λ/ρ对θ进行归一化时,归一化环围能量ε对θ(在给定极角θ内孔径透射的能量分数)的依赖关系在形状上是相似的。这里ρ是孔径几何形状(其形状和尺寸)以及光振幅分布的尺寸参数。对于小的θ,ρ = ρ(l,eff) = (Σ(eff)/π)^(1/2) 取决于有效孔径面积Σ(eff),它是通过轴向光强计算得出的。对于大的θ,ρ = ρ(2,eff) = 2Σ(eff)/Rho(eff) 取决于Σ(eff) 和相应的周长Rho(eff)。在光振幅分布均匀的情况下,ρ(1) 和ρ(2) 的归一化对应于小θ和大θ时ε(θ) 的著名展开式。