Wavefront aberration function is modified and expressed by combination of Bi-Zernike polynomials in rotationally symmetric optical systems. The field and pupil parameters of wavefront aberration function are separated and described respectively by orthonormal Zernike polynomials.

© 2013 Optical Society of America

PDF Article


You do not have subscription access to this journal. Citation lists with outbound citation links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.

Contact your librarian or system administrator
Login to access OSA Member Subscription

Supplementary Material (1)

» Media 1: PDF (544 KB)