Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror

A low frequency wavefront aberration correction method for solar telescopes based on secondary mirror movement is proposed to correct dynamic wavefront aberration during the operation of solar telescope. The correction ability of this method is analyzed and validated by numerical simulation and expe...

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Main Authors: Yawei Xiao, Simin Zhao, Junbo Zhang, Linhai Huang, Naiting Gu
Format: Article
Language:English
Published: IEEE 2024-01-01
Series:IEEE Photonics Journal
Subjects:
Online Access:https://ieeexplore.ieee.org/document/10480536/
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author Yawei Xiao
Simin Zhao
Junbo Zhang
Linhai Huang
Naiting Gu
author_facet Yawei Xiao
Simin Zhao
Junbo Zhang
Linhai Huang
Naiting Gu
author_sort Yawei Xiao
collection DOAJ
description A low frequency wavefront aberration correction method for solar telescopes based on secondary mirror movement is proposed to correct dynamic wavefront aberration during the operation of solar telescope. The correction ability of this method is analyzed and validated by numerical simulation and experiments. Theoretical analysis and numerical simulation both indicate the system processes significant aberration correction ability given the correction frequency of the secondary mirror movement is 10 times higher than aberration frequency. After spatiotemporal frequency division of actual wavefront data from solar telescope, the experiment result proves that the proposed correction method based on secondary mirror movement can effectively reduce the overall RMS of dynamic aberrations with high-frequency portion.
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spelling doaj.art-c49bd9a237d34cf7a412d01598f433722024-04-18T23:00:12ZengIEEEIEEE Photonics Journal1943-06552024-01-011631910.1109/JPHOT.2024.338259110480536Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary MirrorYawei Xiao0https://orcid.org/0009-0007-6488-8431Simin Zhao1https://orcid.org/0009-0006-4700-9581Junbo Zhang2https://orcid.org/0009-0003-0672-4827Linhai Huang3https://orcid.org/0000-0003-2380-9091Naiting Gu4https://orcid.org/0000-0003-0030-2802Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, ChinaInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, ChinaInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, ChinaInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, ChinaInstitute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, ChinaA low frequency wavefront aberration correction method for solar telescopes based on secondary mirror movement is proposed to correct dynamic wavefront aberration during the operation of solar telescope. The correction ability of this method is analyzed and validated by numerical simulation and experiments. Theoretical analysis and numerical simulation both indicate the system processes significant aberration correction ability given the correction frequency of the secondary mirror movement is 10 times higher than aberration frequency. After spatiotemporal frequency division of actual wavefront data from solar telescope, the experiment result proves that the proposed correction method based on secondary mirror movement can effectively reduce the overall RMS of dynamic aberrations with high-frequency portion.https://ieeexplore.ieee.org/document/10480536/Imaging systemaberration correctionsecondary mirrorsensitivity matrix methodsolar telescope
spellingShingle Yawei Xiao
Simin Zhao
Junbo Zhang
Linhai Huang
Naiting Gu
Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
IEEE Photonics Journal
Imaging system
aberration correction
secondary mirror
sensitivity matrix method
solar telescope
title Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
title_full Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
title_fullStr Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
title_full_unstemmed Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
title_short Low Spatio-Temporal Frequency Wavefront Aberration Correction Method Based on a Movable Secondary Mirror
title_sort low spatio temporal frequency wavefront aberration correction method based on a movable secondary mirror
topic Imaging system
aberration correction
secondary mirror
sensitivity matrix method
solar telescope
url https://ieeexplore.ieee.org/document/10480536/
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