4.6 Article

Extended-aperture Hartmann wavefront sensor with raster scanning

Journal

OPTICS EXPRESS
Volume 29, Issue 21, Pages 34229-34242

Publisher

OPTICAL SOC AMER
DOI: 10.1364/OE.440576

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Funding

  1. National Natural Science Foundation of China [61205192]
  2. National High-tech Research and Development Program [2015AA020944]

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This paper proposes an extended-aperture Hartmann wavefront sensor based on raster scanning, which can achieve a large dynamic range and high spatial resolution simultaneously. The method is not only applicable for HWFS but also for SHWFS, enabling higher accuracy and better power efficiency.
In this paper, we propose an extended-aperture Hartmann wavefront sensor (HWFS) based on raster scanning. Unlike traditional HWFS, where there is a trade-off between the dynamic range and spatial resolution of wavefront measurement, our extended-aperture HWFS breaks the trade-off and thus could achieve a large dynamic range and high spatial resolution simultaneously. By applying a narrow-beam raster-scanning scheme, the detection aperture of our HWFS is extended to 40 x 40 mm(2) without using the enlarging 4f relay system. The spatial resolution of our setup depends on the scanning step, the pinhole size, and the wavelength. The sensitivity and dynamic range can be adjusted flexibly by varying the axial distance between the pinhole plane and the imaging sensor plane, because our decoupled large dynamic range could be reasonable traded-off to achieve better sensitivity. Furthermore, compared with tradition HWFS, our method does not need to compute the positions of a two-dimensional spots array where complicated spots tracking algorithms are necessary to achieve high dynamic range, thus remarkably reduces the spots aliasing issue and the computational cost. It should be noted that this scheme is not only applicable for HWFS but also for Shack-Hartmann wavefront sensor (SHWFS) with microlens array to achieve higher accuracy and better power efficiency. Experiments were performed to demonstrate the capability of our method. (C) 2021 Optical Society of America under the terms of the OSA Open Access Publishing Agreement

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