2017
DOI: 10.1016/j.optcom.2017.06.017
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Deflectometry using a Hartmann screen to measure tilt, decentering and focus errors in a spherical surface

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Cited by 6 publications
(2 citation statements)
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“…In the past few years, various deflectometric methods and systems have been proposed to achieve accurate optical testing, including the astronomical telescope mirrors [6], spherical surfaces [7], aspheric mirrors [8,9], specular freeform mirrors [10] and precision x-ray mirrors [11]. Compared to interferometrical methods, the deflectometry is much lower in cost due to its simple system configuration, simply consisting of a projection screen, CCD camera and test object.…”
Section: Introductionmentioning
confidence: 99%
“…In the past few years, various deflectometric methods and systems have been proposed to achieve accurate optical testing, including the astronomical telescope mirrors [6], spherical surfaces [7], aspheric mirrors [8,9], specular freeform mirrors [10] and precision x-ray mirrors [11]. Compared to interferometrical methods, the deflectometry is much lower in cost due to its simple system configuration, simply consisting of a projection screen, CCD camera and test object.…”
Section: Introductionmentioning
confidence: 99%
“…For high lateral resolution and avoiding aliasing effects, a dense grid is desirable. A dense grid, however, masks the original Makyoh image, thus hindering the observation of the morphology: the method can no longer be strictly treated as 'Makyoh topography', rather, we obtain a variation of the well known deflectometry [10] methods. (We note here that in this 'deflectomery mode', the mask does not need to be a grid; any two-dimensional periodic pattern, e.g., a Hartmann mask is suitable.)…”
Section: Introduction and Basic Conceptsmentioning
confidence: 99%