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国家自然科学基金(11204299)

作品数:7 被引量:26H指数:2
相关作者:李大禹宣丽刘永刚高明黄涛更多>>
相关机构:中国科学院长春光学精密机械与物理研究所沈阳师范大学更多>>
发文基金:国家自然科学基金更多>>
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7 条 记 录,以下是 1-7
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Multiple-object Shack–Hartmann wavefront sensor design for a wide field of view on the retina被引量:1
2015年
In order to detect the aberration from a wide field of view(FOV) on the retina with adaptive optics, we present a multiple-object Shack–Hartmann wavefront sensor(MOSHWFS) design. The simulated results indicate that the wavefront from our MOSHWFS can be reconstructed for multiple objects, and the measurement error can be less than λ∕7 with an MOSHWFS with an FOV of 6.7°, for maximum eye aberration. The experimental result with two objects indicates that the measurement error can be less than λ∕14, with the root mean square of the reference wavefront as 0.798λ and 0.895λ, respectively.
杨乐宝胡立发李大禹曹召良穆全全马骥宣丽
关键词:哈特曼波前传感器传感器设计自适应光学
A high precision phase reconstruction algorithm for multi-laser guide stars adaptive optics
2016年
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.
何斌胡立发李大禹徐焕宇张杏云王少鑫王玉坤杨程亮曹召良穆全全鲁兴海宣丽
关键词:自适应光学相位失真
Configuration optimization of laser guide stars and wavefront correctors for multi-conjugation adaptive optics被引量:1
2016年
Multi-conjugation adaptive optics(MCAOs) have been investigated and used in the large aperture optical telescopes for high-resolution imaging with large field of view(FOV).The atmospheric tomographic phase reconstruction and projection of three-dimensional turbulence volume onto wavefront correctors,such as deformable mirrors(DMs) or liquid crystal wavefront correctors(LCWCs),is a very important step in the data processing of an MCAO's controller.In this paper,a method according to the wavefront reconstruction performance of MCAO is presented to evaluate the optimized configuration of multi laser guide stars(LGSs) and the reasonable conjugation heights of LCWCs.Analytical formulations are derived for the different configurations and are used to generate optimized parameters for MCAO.Several examples are given to demonstrate our LGSs configuration optimization method.Compared with traditional methods,our method has minimum wavefront tomographic error,which will be helpful to get higher imaging resolution at large FOV in MCAO.
宣丽何斌胡立发李大禹徐焕宇张杏云王少鑫王玉坤杨程亮曹召良穆全全鲁兴海
关键词:自适应光学光学望远镜三维湍流
Determining the imaging plane of a retinal capillary layer in adaptive optical imaging
2016年
Even in the early stage,endocrine metabolism disease may lead to micro aneurysms in retinal capillaries whose diameters are less than 10 μm.However,the fundus cameras used in clinic diagnosis can only obtain images of vessels larger than 20 μm in diameter.The human retina is a thin and multiple layer tissue,and the layer of capillaries less than10 μm in diameter only exists in the inner nuclear layer.The layer thickness of capillaries less than 10 μm in diameter is about 40 μm and the distance range to rod&cone cell surface is tens of micrometers,which varies from person to person.Therefore,determining reasonable capillary layer(CL) position in different human eyes is very difficult.In this paper,we propose a method to determine the position of retinal CL based on the rod&cone cell layer.The public positions of CL are recognized with 15 subjects from 40 to 59 years old,and the imaging planes of CL are calculated by the effective focal length of the human eye.High resolution retinal capillary imaging results obtained from 17 subjects with a liquid crystal adaptive optics system(LCAOS) validate our method.All of the subjects' CLs have public positions from 127 μm to 147 μm from the rod&cone cell layer,which is influenced by the depth of focus.
杨乐宝胡立发李大禹曹召良穆全全马骥宣丽
关键词:自适应光学系统视锥细胞眼底照相机CLS
大视场液晶自适应视网膜成像系统被引量:7
2013年
设计了大视场眼底自适应成像系统,用于扩大现有视网膜自适应成像系统的视场。对人眼等晕角视场下的自适应像差校正成像进行分析,确定了波前探测与成像校正两个过程对视场的不同要求。在共光源像差探测及成像光学系统中,采用切变视场光阑的方式先后在波前探测和自适应校正成像过程中进行小-大视场切换,避免了大视场中眼波像差探测失真问题,使成像区域由200μm扩展到500μm。利用人眼等晕角大视场使眼底液晶自适应成像系统在不降低成像质量的前提下将成像区域扩展了2.5倍,大幅提升了该自适应成像系统在临床上应用的可行性。
刘丽丽黄涛蔡敏高明封文江
关键词:自适应光学大视场
液晶自适应光学在天文学研究中的应用展望被引量:18
2015年
液晶波前校正器作为一种高单元密度的新型波前校正器件,通过相息图的衍射可以轻松实现十微米的波前位相校正量。因此,基于液晶波前校正器的自适应光学(LCAO)系统是21世纪天文观测领域非常有希望普及的系统。但是液晶波前校正器存在响应速度慢(〉10ms)、能量利用率低的双重问题,国际上一直处于探索研究中。本课题组不但解决了能量问题,而且在速度方面不断取得进步,所研制的LCAO系统与1.23m口径望远镜连接,清晰观测到土星及其环绕的光环带,分辨出4.8和5.5视星等的α-Com双星,成像分辨率达到1.8倍衍射极限分辨率;目前系统延迟时间只有2ms,可以说已达到工程应用水平,在装备8~10m级大口径天文学望远镜方面极具应用潜力。
宣丽李大禹刘永刚
关键词:液晶波前校正器自适应光学望远镜
Design of the Rotation Angle Measurement System for the Atmospheric Dispersion Corrector (ADC)
2017年
In order to measure the rotation angle error of the worm and gear mechanisms in the atmospheric dispersion corrector( ADC),a novel measurement system based on the autocollimator is designed in this paper.Based on the position relations between the shaft and spot converged by rays of autocollimator,the rotation angle can be calculated quickly and conveniently using a brief algorithm. An optical wedge is introduced to the measurement system for suppressing the awful measuring error caused by the axial wobbly error. The measurement system can measure the shaft rotation angle at any rotation position,which is the novel usage of the two-dimensional autocollimator. Its optical layout is very simple. Only an optical wedge and two plane mirrors are needed besides the autocollimator. The measurement accuracy of the proposed method is less than±0.5 arcmin. In the measurement of two worms and gears mechanisms in ADC,the rotation angle error are±0.05° and ±0.07° respectively,which all satisfies the design demand( ±0.1°). The proposed measurement system can be also suits for some engineering fields.
Wenjie LiQuanquan MuShaoxin WangChengliang YangHaiping WangZhaoliang CaoLi Xuan
关键词:OPTICALROTATIONAUTOCOLLIMATORAXISOPTICALWEDGE
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