2021
DOI: 10.1364/ao.441092
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Compensated differential Zernike fitting method for wavefront aberration metrology based on grating lateral shearing

Abstract: Lateral shearing based on the grating is one of the classical configurations when measuring the wavefront aberration of optical systems such as the lithographic projection lens. Because the wavefront under test is spherical, but a detector surface is a plane, the coordinate of the wavefront surface will be distorted on the detector surface. As the numerical aperture (NA) of the optics under test increases, the shear ratios at different positions within the shearing region are significantly different due to the… Show more

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Cited by 6 publications
(2 citation statements)
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“…The Ronchi test measures the aberrations of imaging lenses with the interference patterns produced by a grating. However, the accuracy is limited when the light source does not have good monochromaticity, and strict alignment is needed for the grating [1,4,5]. The star test analyzes the aberrations by examining the images of a point source formed by the lenses under test (LUT) and compares them with the ideal image form, which depends heavily on experience [1].…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…The Ronchi test measures the aberrations of imaging lenses with the interference patterns produced by a grating. However, the accuracy is limited when the light source does not have good monochromaticity, and strict alignment is needed for the grating [1,4,5]. The star test analyzes the aberrations by examining the images of a point source formed by the lenses under test (LUT) and compares them with the ideal image form, which depends heavily on experience [1].…”
Section: Introductionmentioning
confidence: 99%
“…Compared with traditional methods [1][2][3][4][5][6][7][8][9][10], WAMD is more flexible and can achieve sub-wavelength-level accuracy. Although its accuracy cannot achieve the same level as that of interferometry test, it can work in situations where the aberration is too large to be tested by an interferometer [6][7][8].…”
Section: Introductionmentioning
confidence: 99%