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Attitude correction of secondary mirror in large telescope using coma and imaging point position
Y. Zhu; J. Wang; T. Chen; X. Wu and H. Li
2022
发表期刊Guangxue Jingmi Gongcheng/Optics and Precision Engineering
ISSN1004924X
卷号30期号:23页码:3090-3096
摘要A secondary mirror mount in a large telescope introduces different attitude errors at different elevationsreducing the accuracy of the imaging device. In particularlarge SiC telescopes suffer from this problem. Without correction of the secondary mirror attitude, a large error of imaging point position was introduced that result in an overload of the precision tracking system. By considering the optical design parameters of the telescopea secondary mirror correction method based on the coma-free pointCFPand center of curvature was developed. Stewart platform is used to correct the attitude of secondary mirror based on the telescope elevation. The alignment error before the precision tracking system is reduced from 12. 85to 1. 80as a result of the attitude correction of the secondary mirror. The correction method is simple and effectiveallowing for coarse alignment of the precision tracking system and preserving the accuracy of the imaging system. 2022 Chinese Academy of Sciences. All rights reserved.
DOI10.37188/OPE.20223023.3090
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条目标识符http://ir.ciomp.ac.cn/handle/181722/66431
专题中国科学院长春光学精密机械与物理研究所
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Y. Zhu,J. Wang,T. Chen,et al. Attitude correction of secondary mirror in large telescope using coma and imaging point position[J]. Guangxue Jingmi Gongcheng/Optics and Precision Engineering,2022,30(23):3090-3096.
APA Y. Zhu,J. Wang,T. Chen,&X. Wu and H. Li.(2022).Attitude correction of secondary mirror in large telescope using coma and imaging point position.Guangxue Jingmi Gongcheng/Optics and Precision Engineering,30(23),3090-3096.
MLA Y. Zhu,et al."Attitude correction of secondary mirror in large telescope using coma and imaging point position".Guangxue Jingmi Gongcheng/Optics and Precision Engineering 30.23(2022):3090-3096.
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