Orthogonal Set of Basis Functions over the Binocular Pupil

TL;DR

This paper introduces a novel orthogonal basis set for modeling wavefront aberrations over two separate, equal-sized circular pupils, extending existing basis functions to more complex pupil geometries in optical systems.

Contribution

It proposes a new orthogonal basis set for two non-overlapping pupils of equal size, derived through Gram-Schmidt orthogonalization of primitive functions, accounting for pupil separation and size ratio.

Findings

Derived explicit overlap integrals for primitive basis functions.

Established a method to generate orthogonal basis functions for dual pupils.

Enhanced modeling capabilities for complex optical pupil configurations.

Abstract

Sets of orthogonal basis functions over two-dimensional circular areas--most often representing pupils in optical applications--are known in the literature for the full circle (Zernike or Jacobi polynomials) and the annulus. This work proposes an orthogonal set if the area is two non-overlapping circular pupils of same size. The major free parameter is the ratio of the pupil radii over the distance between both circles. Increasingly higher order aberrations--as defined for a virtual larger pupil in which both pupils are embedded--are fed into a Gram-Schmidt orthogonalization to implement one unique set of basis functions. The key element is to work out the overlap integrals between a full set of primitive basis functions (products of powers of the distance from the mid-point between both pupils by azimuthal functions of the Fourier type).