14 March 2016 Equations to estimate the wavefront surface in the Hartmann test for lenses: comparison between two wavefront estimations when the Hartmann screen is close to the test lens
Alejandro Téllez-Quiñones, Daniel Malacara-Doblado, Jorge García-Márquez, D. Asael Gutiérrez-Hernández
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Abstract
When testing lenses with Hartmann methods, a wave aberration function W is typically estimated. This W represents the deviations of the wavefront surface w with respect to an ideal wavefront E. In this test, the distance r from the observation screen to the second lens surface is considered, and, as in the case of W, by considering paraxial approximations, two estimations of w can be directly constructed from Hartmann test data without calculating W. We have compared these two estimations by taking into account small r values; a possible and suitable condition to measure some relatively high-power lenses. The importance of estimating w can be useful for improving some optical measurements as power map reconstructions.
© 2016 Society of Photo-Optical Instrumentation Engineers (SPIE) 0091-3286/2016/$25.00 © 2016 SPIE
Alejandro Téllez-Quiñones, Daniel Malacara-Doblado, Jorge García-Márquez, and D. Asael Gutiérrez-Hernández "Equations to estimate the wavefront surface in the Hartmann test for lenses: comparison between two wavefront estimations when the Hartmann screen is close to the test lens," Optical Engineering 55(3), 034103 (14 March 2016). https://doi.org/10.1117/1.OE.55.3.034103
Published: 14 March 2016
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Cited by 1 scholarly publication.
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KEYWORDS
Wavefronts

Lenses

Error analysis

Optical engineering

Computer simulations

Geometrical optics

Optical spheres

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