Paper
19 September 2013 Diffractive imaging analysis of large-aperture segmented telescope based on partial Fourier transform
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Proceedings Volume 8905, International Symposium on Photoelectronic Detection and Imaging 2013: Laser Sensing and Imaging and Applications; 890516 (2013) https://doi.org/10.1117/12.2033702
Event: ISPDI 2013 - Fifth International Symposium on Photoelectronic Detection and Imaging, 2013, Beijing, China
Abstract
Large-aperture segmented primary mirror will be widely used in next-generation space-based and ground-based telescopes. The effects of intersegment gaps, obstructions, position and figure errors of segments, which are all involved in the pupil plane, on the image quality metric should be analyzed using diffractive imaging theory. Traditional Fast Fourier Transform (FFT) method is very time-consuming and costs a lot of memory especially in dealing with large pupil-sampling matrix. A Partial Fourier Transform (PFT) method is first proposed to substantially speed up the computation and reduce memory usage for diffractive imaging analysis. Diffraction effects of a 6-meter segmented mirror including 18 hexagonal segments are simulated and analyzed using PFT method. The influence of intersegment gaps and position errors of segments on Strehl ratio is quantitatively analyzed by computing the Point Spread Function (PSF). By comparing simulation results with theoretical results, the correctness and feasibility of PFT method is confirmed.
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Bing Dong, Shun Qin, and Xinqi Hu "Diffractive imaging analysis of large-aperture segmented telescope based on partial Fourier transform", Proc. SPIE 8905, International Symposium on Photoelectronic Detection and Imaging 2013: Laser Sensing and Imaging and Applications, 890516 (19 September 2013); https://doi.org/10.1117/12.2033702
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Cited by 2 scholarly publications.
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KEYWORDS
Pulmonary function tests

Image segmentation

Segmented mirrors

Telescopes

Space telescopes

Fourier transforms

Mirrors

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