不同导星数量和排布情况下地表层自适应光学系统的性能分析

大气与环境光学学报 ›› 2022, Vol. 17 ›› Issue (5): 485-493.

• 大气光学 • 下一篇

不同导星数量和排布情况下地表层自适应光学系统的性能分析

赵梓旭1,2,3 , 马晓燠2,3∗ , 饶长辉1,2,3

1 中国科学院大学, 北京 100049; 2 中国科学院自适应光学重点实验室, 四川成都 610209; 3 中国科学院光电技术研究所, 四川成都 610209

收稿日期:2021-04-06 修回日期:2022-04-25 出版日期:2022-09-28 发布日期:2022-10-17
通讯作者: E-mail: maxiaoyu001@126.com E-mail:maxiaoyu001@126.com
作者简介:赵梓旭 (1996 - ), 吉林公主岭人, 硕士研究生, 主要从事地表层自适应光学方面的研究。 E-mail: zhaozixu ucas@163.com
基金资助:
Supported by the National Natural Science Foundation of China′ s Major Scientific Research Instrument (Free Application) Project (国家自然科学基金重大科研仪器 (自由申请) 项目支持, 11727805)

Performance analysis of ground layer adaptive optics system under different number and arrangement of guide stars

ZHAO Zixu 1,2,3 , MA Xiaoyu 2,3∗ , RAO Changhui 1,2,3

1 University of Chinese Academy of Sciences, Beijing 100049, China; 2 Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China; 3 Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China

Received:2021-04-06 Revised:2022-04-25 Published:2022-09-28 Online:2022-10-17

摘要/Abstract

摘要： 基于频谱滤波理论和经典大气湍流 7 层模型, 通过地表层自适应光学 (GLAO) 系统的理论滤波器模型, 结合有限导星条件下的误差传递函数 (ETF), 探究了不同导星数量与不同导星排布情况下地表层自适应光学系统的性能。研究结果表明 6 颗导星呈中心 1 颗、其余 5 颗在视场边缘均匀环形分布时, 系统校正性能较优。该研究结果对正在研制的一米新真空太阳望远镜多层共轭自适应光学 (MCAO) 系统 (含有 GLAO 系统) 具有重要指导作用和参考价值。

关键词: 地表层自适应光学, 导星, 性能分析, 太阳望远镜

Abstract: Based on the theory of spectral filtering and the classical 7-layer model of atmospheric turbulence, the performance of the adaptive optics system on ground layer under different number of guide stars and different guide star arrangements is explored by using the theoretical filter model of the Ground Layer Adaptive Optics (GLAO) system and the error transfer function (ETF) under the condition of finite guide stars. The results show that when 1 guide star is in the center and the other 5 guide stars are evenly distributed around the edge of the field of view, the calibration performance of the system is the best. The research results have important guiding role and reference value for the multi-conjugate adaptive optics (MCAO) system (including GLAO system) of the one-meter new vacuum solar telescope being developed.

Key words: ground layer adaptive optics, guide star, performance analysis, solar telescope

中图分类号:

O439
P111.21

赵梓旭, 马晓燠, ∗, 饶长辉, . 不同导星数量和排布情况下地表层自适应光学系统的性能分析[J]. 大气与环境光学学报, 2022, 17(5): 485-493.

ZHAO Zixu , , MA Xiaoyu , ∗ , RAO Changhui , . Performance analysis of ground layer adaptive optics system under different number and arrangement of guide stars[J]. Journal of Atmospheric and Environmental Optics, 2022, 17(5): 485-493.

参考文献 J

[1]	Hubin N, Arsenault R, Conzelmann R, et al. Ground layer adaptive optics [J]. Comptes Rendus Physique, 2005, 6(10): 1099-
	1109.
[2]	Marchetti E, Brast R, Delabre B, et al. MAD on sky results in star-oriented mode [C]. SPIE Astronomical Telescopes +
	Instrumentation. Proc SPIE 7015, Adaptive Optics Systems, Marseille, France. 2008, 7015: 61-72.
[3]	Rimmele T R, Woeger F, Marino J, et al. Solar multiconjugate adaptive optics at the dunn solar telescope [C]. SPIE Astronomical Telescopes + Instrumentation. Proc SPIE 7736, Adaptive Optics Systems II, San Diego, California, USA. 2010, 7736:
10	86-1092.
[4]	Ren D Q, Jolissaint L, Zhang X, et al. Solar ground-layer adaptive optics [J]. Publications of the Astronomical Society of the
	Pacific, 2015, 127(951): 469-478.
[5]	Baranec C, Lloyd-Hart M, Milton N M. Ground-layer wave front reconstruction from multiple natural guide stars [J]. The
	Astrophysical Journal Letters, 2007, 661(2): 1332-1338.
[6]	Hart M, Milton N M, Baranec C, et al. A ground-layer adaptive optics system with multiple laser guide stars [J]. Nature, 2010,
46	6(7307): 727-729.
[7]	Rao C H, Gu N T, Rao X J, et al. First light of the 1.8-m solar telescope—CLST [J]. Science China Physics, Mechanics &
	Astronomy, 2020, 63(10): 109631.
[8]	Zhang L Q. Solar Multi-Conjugate Adaptive Optics for High Resolution Imaging [D]. Chengdu: Institute of Optics and Electronics, University of Chinese Academy of Sciences, 2014.
	张兰强. 太阳高分辨力成像多层共轭自适应光学技术研究 [D]. 成都: 中国科学院大学 (光电技术研究所), 2014.
[9]	Tokovinin A. Seeing improvement with ground-layer adaptive optics [J]. Publications of the Astronomical Society of the
	Pacific, 2004, 116(824): 941-951.
[10]	Liu Z, Xu J. 1-meter near-infrared solar telescope [J]. Astronomical Society of India Conference Series, 2011, 2: 9-17.
[11]	Ellerbroek B L, Rigaut F J. Scaling multiconjugate adaptive optics performance estimates to extremely large telescopes [C].
	Astronomical Telescopes and Instrumentation. Proc SPIE 4007, Adaptive Optical Systems Technology, Munich, Germany.
20	00, 4007: 1088-1099.
[12]	Wang Z Y, Zhang L Q, Rao C H. Characterizing daytime wind profiles with the wide-field Shack-Hartmann wavefront sensor
[J]	Monthly Notices of the Royal Astronomical Society, 2019, 483(4): 4910-4921

不同导星数量和排布情况下地表层自适应光学系统的性能分析

Performance analysis of ground layer adaptive optics system under different number and arrangement of guide stars

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