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• W2127019216 abstract "The transfer function can be determined by convolution of the pupil function over the aperture. The pupil function itself is a function of the design data of the lens system (i.e., refractive indices, radii of curvature, etc.) Of particular importance, both practically and theoretically, is the frequency response on-axis where only rotationally symmetric aberrations are present. The aberration function is obtained from an integration over the ray-trace data and is curve-fitted by Chebyschev interpolation. Unlike the least-squares method, the Chebyschev approach allows a uniform approximation over the interval. This data is substituted into the transfer function which is numerically evaluated by application of very high-order Gauss quadrature theory." @default.
• W2127019216 created "2016-06-24" @default.
• W2127019216 creator A5049000988 @default.
• W2127019216 date "1962-09-01" @default.
• W2127019216 modified "2023-09-27" @default.
• W2127019216 title "Computation of the Transfer Function of an Optical System from the Design Data for Rotationally Symmetric Aberrations Part I Theory" @default.
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• W2127019216 doi "https://doi.org/10.1364/josa.52.000985" @default.
• W2127019216 hasPublicationYear "1962" @default.
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