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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Format: | Article |
Language: | English |
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IEEE
2024-01-01
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Series: | IEEE Photonics Journal |
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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. |
first_indexed | 2024-04-24T07:46:08Z |
format | Article |
id | doaj.art-c49bd9a237d34cf7a412d01598f43372 |
institution | Directory Open Access Journal |
issn | 1943-0655 |
language | English |
last_indexed | 2024-04-24T07:46:08Z |
publishDate | 2024-01-01 |
publisher | IEEE |
record_format | Article |
series | IEEE Photonics Journal |
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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