Mahajan V N
Appl Opt. 1995 Dec 1;34(34):8060-2. doi: 10.1364/AO.34.008060.
The use of Zernike polynomials to calculate the standard deviation of a primary aberration across a circular, annular, or a Gaussian pupil is described. The standard deviation of secondary aberrations is also discussed briefly.
描述了使用泽尼克多项式来计算圆形、环形或高斯光瞳上初级像差的标准差。还简要讨论了次级像差的标准差。