期刊文献+

A high precision phase reconstruction algorithm for multi-laser guide stars adaptive optics

A high precision phase reconstruction algorithm for multi-laser guide stars adaptive optics
下载PDF
导出
摘要 Adaptive optics(AO) systems are widespread and considered as an essential part of any large aperture telescope for obtaining a high resolution imaging at present.To enlarge the imaging field of view(FOV),multi-laser guide stars(LGSs) are currently being investigated and used for the large aperture optical telescopes.LGS measurement is necessary and pivotal to obtain the cumulative phase distortion along a target in the multi-LGSs AO system.We propose a high precision phase reconstruction algorithm to estimate the phase for a target with an uncertain turbulence profile based on the interpolation.By comparing with the conventional average method,the proposed method reduces the root mean square(RMS) error from 130 nm to 85 nm with a 30% reduction for narrow FOV.We confirm that such phase reconstruction algorithm is validated for both narrow field AO and wide field AO. Adaptive optics(AO) systems are widespread and considered as an essential part of any large aperture telescope for obtaining a high resolution imaging at present.To enlarge the imaging field of view(FOV),multi-laser guide stars(LGSs) are currently being investigated and used for the large aperture optical telescopes.LGS measurement is necessary and pivotal to obtain the cumulative phase distortion along a target in the multi-LGSs AO system.We propose a high precision phase reconstruction algorithm to estimate the phase for a target with an uncertain turbulence profile based on the interpolation.By comparing with the conventional average method,the proposed method reduces the root mean square(RMS) error from 130 nm to 85 nm with a 30% reduction for narrow FOV.We confirm that such phase reconstruction algorithm is validated for both narrow field AO and wide field AO.
出处 《Chinese Physics B》 SCIE EI CAS CSCD 2016年第9期83-87,共5页 中国物理B(英文版)
基金 Project supported by the National Natural Science Foundation of China(Grant Nos.11174274,11174279,61205021,11204299,61475152,and 61405194) State Key Laboratory of Applied Optics,Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences
关键词 laser guide star adaptive optics phase reconstruction liquid crystal wavefront corrector laser guide star adaptive optics phase reconstruction liquid crystal wavefront corrector
  • 相关文献

参考文献25

  • 1Booth M J 2014 Light Sci. Appl. 3 e165.
  • 2Xuan L, Li D Y and Liu Y G 2015 Chin. J. Liq. Cryst. Disp. 30 1 (in Chinese).
  • 3Min L, Yao L S, Wang Y K, Wang S X, Liu Y G, Peng Z H and Xuan L 2015 Chin. J. Liq. Cryst. Disp. 30 32.
  • 4Wang Y C, Zhang Z D and Zhou X 2015 Chin. J. Liq. Cryst. Disp. 30 949 (in Chinese).
  • 5Yu Y, Zhou X and Zhang Z D 2015 Chin. J. Liq. Cryst. Disp. 30 213 (in Chinese).
  • 6Chen Y C, Xuan L, Yao L S and Peng Z H 2016 Chin. J. Liq. Cryst. Disp. 31 (in Chinese).
  • 7Zhou Q, Lu J F and Yin J P 2013 Chin. J. Liq. Cryst. Disp. 28 349 (in Chinese).
  • 8McCall S and Passner A 1978 Adaptive Optics and Short Wavelength Sources 1 149.
  • 9Fried D L 1995 J. Opt. Soc. Am. A 12 939.
  • 10Foy R and Labeyrie A 1985 Astron. Astrophys. 152 L29.

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部