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    A new approach to wavefront sensing: AI software with an autostigmatic microscope

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    Author
    Baudat, G.
    Parks, R.E.
    Anjakos, B.
    Affiliation
    Wyant College of Optical Sciences, The University of Arizona
    Steward Observatory, The University of Arizona
    Issue Date
    2023-10-04
    Keywords
    Artificial intelligence
    autostigmatic microscope
    field-dependent wavefront sensing
    low cost fast wavefront sensing
    machine learning
    multi-source wavefront sensing
    wavefront sensing
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Gaston Baudat, Robert E. Parks, Benjamin Anjakos, "A new approach to wavefront sensing: AI software with an autostigmatic microscope," Proc. SPIE 12672, Applied Optical Metrology V, 126720L (4 October 2023); https://doi.org/10.1117/12.2676411
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    © 2023 SPIE.
    Collection Information
    This 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.
    Abstract
    The use of artificial intelligence (AI) software for wavefront sensing has been demonstrated in previous studies [1], [3]. In this work, we have developed a novel approach to wavefront sensing by coupling an AI software with an Autostigmatic Microscope (AM). The resulting system offers optical component and system testing capabilities similar to those of an interferometer used in double pass, but with several advantages. The AM is smaller, lighter, and less expensive than commercially available interferometers, while the AI software is capable of reading out Zernike coefficients, providing real-time feedback for alignment. Our AI software uses an artificial neural network (NN) that is trained to output the Zernike coefficients, or any other relevant figures of merit, exclusively from synthetic data. The synthetic data includes random Zernike coefficients for a parametric description of the wavefront, noise, and a defocus error to avoid any stringent accuracy requirement. Once trained, the NN yields Zernike coefficients from a single frame of defocused intensity. The feedforward architecture of the NN enables swift output of Zernike coefficients, eliminating the need for iteration or optimization during run time. Using the software with an AM allows for paraxial alignment of the object in the test cavity, with the real-time Zernike coefficients guiding the item into optimal alignment. This double pass test is not possible with most other types of wavefront sensors, as they are designed for single-pass use. Our results demonstrate that the test results obtained compare well with modeled results, and that errors in the AM can be removed by calibration, as in the case of interferometer transmission spheres. Furthermore, the simple defocused image of a source provides non-ambiguous phase retrieval, which competes with traditional wavefront sensors such as Shack-Hartmann (SH) sensors or interferometers. The AI software provides high dynamic range, sensitivity and precision [3]. This novel approach to wavefront sensing has significant potential for use in a wide range of applications in the field of optics. © 2023 SPIE. All rights reserved.
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    978-151066558-3
    DOI
    10.1117/12.2676411
    Version
    Final Published Version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2676411
    Scopus Count
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    UA Faculty Publications

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