Canonical transformations to warped surfaces: Correction of aberrated optical images

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Published under licence by IOP Publishing Ltd
, , Citation Eisso J Atzema et al 1997 J. Phys. A: Math. Gen. 30 5793 DOI 10.1088/0305-4470/30/16/020

0305-4470/30/16/5793

Abstract

The projection of optical images on warped screens is a canonical transformation of phase space between flat and warped evolution-parameter surfaces. In mechanics, the evolution parameter is time; in geometric optics it is the optical axis of coordinate space. We consider the specific problem of bringing to focus an axis-symmetric aberrating optical system by warping the output screen. The solution for the surface curvature coefficients is given in terms of the Lie aberration coefficients of the system; a linear optimization strategy applies.

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10.1088/0305-4470/30/16/020