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dc.contributor.authorChoi, H.
dc.contributor.authorKang, H.
dc.contributor.authorHuang, Y.
dc.contributor.authorYoo, M.
dc.contributor.authorQuach, H.
dc.contributor.authorKam, J.
dc.contributor.authorKim, D.
dc.date.accessioned2024-03-22T02:46:14Z
dc.date.available2024-03-22T02:46:14Z
dc.date.issued2023-10-04
dc.identifier.citationHeejoo Choi, Hyukmo Kang, Yiyang Huang, Mina Yoo, Henry Quach, John Kam, Daewook Kim, "Advanced deflectometry methods for industrial application," Proc. SPIE 12684, ODS 2023: Industrial Optical Devices and Systems, 1268407 (4 October 2023); https://doi.org/10.1117/12.2678628
dc.identifier.isbn978-151066582-8
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2678628
dc.identifier.urihttp://hdl.handle.net/10150/671545
dc.description.abstractDeflectometry is a versatile optical testing tool used in various fields, from astronomy to industrial applications, due to its non-null testing capability which facilitates precise measurement despite challenging optical surfaces and system layout constraints. In this manuscript, we present novel variational advancements to traditional deflectometry, towards universal functionality and system friendliness. Traditional dark-field illumination is an inspection technique that is sometimes used to detect particles on a specular surface. Problems arise in its repeatability, as an intensity-based measurement is vulnerably dependent on the testing conditions of time, limiting its ability to be used in automated fashion. The first advancement leverages phase algorithms commonly seen in deflectometry; by adding a secondary light source (normal to the surface) and modulating each source's intensity with a time-varying sinusoid. The phase-based information has a higher sensitivity to the light scattered from a defect producing a more robust computational image process method that is now insensitive to the environment. The second advancement is an alignment method to obtain lower-order shape. While deflectometry proves effective in measuring mid-to-high frequency surface shape, it faces challenges when assessing low-order shape measurements like power, astigmatism, and coma due to relative position and alignment error between the unit under test (UUT) and the deflectometry system. To avert the necessity of additional instruments like a coordinate measuring machine, laser trackers, or interferometers, we leveraged computational fiducials and sensitivity matrices to identify and address misalignments effectively. With enhanced capabilities and system-friendly features, our advanced deflectometry techniques provide powerful options in optical testing. By addressing the challenges in low-order shape measurements and incorporating dark field testing, our approaches extend the potential of deflectometry as a valuable tool in optical metrology across a broad spectrum of industries and scientific endeavors. © 2023 SPIE · 0277-786X ·
dc.language.isoen
dc.publisherSPIE
dc.rights© 2023 SPIE. (2023) Published by SPIE.
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectalignment
dc.subjectdark field illumination
dc.subjectdeflectometry
dc.subjectoptical testing
dc.titleAdvanced deflectometry methods for industrial application
dc.typeProceedings
dc.typetext
dc.contributor.departmentWyant College of Optical Sciences, University of Arizona
dc.contributor.departmentLarge Binocular Telescope Observatory, University of Arizona
dc.contributor.departmentDepartment of Astronomy, Steward Observatory, University of Arizona
dc.identifier.journalProceedings of SPIE - The International Society for Optical Engineering
dc.description.noteImmediate access
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal Published Version
dc.source.journaltitleProceedings of SPIE - The International Society for Optical Engineering
refterms.dateFOA2024-03-22T02:46:14Z


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