Multiple Subaperture Interferometric Testing of Full Spheres

Rick A. Williams, O. Kwon
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Abstract

The objectives of this work are to develop nondestructive, optical test techniques to estimate optical path difference (OPD) errors of full spheres (e.g., gyroscopes, ball hearings, micro-balloons). We propose to use a multiple subaperture interferometric test modeled after analogous techniques used in full aperture testing of large optical systems1. A spherical harmonic base set of polynomials for full sphere descriptions is developed, together with the numerical methods for fitting these polynomials to obtain the aberration coefficients over the spherical surface. The physical interpretation of the lower order terms with respect to OPD errors for a spherical body are discussed and demonstrated using three-dimensional graphics representations. A computer simulation of the multiple subaperture technique for full spheres is utilized in an analysis of test accuracy as a function of various test design parameters (subaperture size, number of subapertures, subaperture tilt errors, inter-subaperture phasing errors, etc.). The results of the simulation suggest that optical testing of full spheres is feasable and has the potential for increased speed, accuracy, and surface preservation as compared to direct physical methods.
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全球体的多子孔径干涉检测
这项工作的目标是发展非破坏性的光学测试技术,以估计全球体(如陀螺仪,球耳,微型气球)的光程差(OPD)误差。我们建议采用类似于大型光学系统全孔径测试技术的多子孔径干涉测试方法。提出了一种用于全球面描述的球谐基多项式集,并给出了拟合这些多项式的数值方法,以获得球面上的像差系数。讨论了球面OPD误差的低阶项的物理解释,并使用三维图形表示进行了演示。利用全球面多子孔径技术的计算机模拟,分析了测试精度与各种测试设计参数(子孔径大小、子孔径数量、子孔径倾斜误差、子孔径间相位误差等)的关系。模拟结果表明,与直接的物理方法相比,全球体的光学测试是可行的,并且具有提高速度,精度和表面保存的潜力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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