Paper
5 February 1996 Polychromatic merit functions in terms of the Wigner distribution function
Author Affiliations +
Proceedings Volume 2730, Second Iberoamerican Meeting on Optics; (1996) https://doi.org/10.1117/12.231077
Event: Second Iberoamerican Meeting on Optics, 1995, Guanajuato, Mexico
Abstract
A method for the calculation of the axial illuminance and chromaticity as polychromatic merit functions of optical imaging systems is presented. We show that the Wigner distribution function of the pupil of the system allows us to obtain all the monochromatic components needed for the calculation of these parameters. From this single phase-space representation, the merit functions can be obtained in a polar fashion for a variable spherical and longitudinal chromatic aberrations. Numerical examples for an axially apodizing filter are shown.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Walter D. Furlan, Genaro Saavedra, Enrique Silvestre-Mora, Maria Josefa Yzuel, and Pedro Andres "Polychromatic merit functions in terms of the Wigner distribution function", Proc. SPIE 2730, Second Iberoamerican Meeting on Optics, (5 February 1996); https://doi.org/10.1117/12.231077
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Wigner distribution functions

Point spread functions

Imaging systems

Colorimetry

Optical imaging

Chromatic aberrations

Computing systems

Back to Top