利用视标和波前数据的NCSF测量

搭建了基于波前像差的神经对比敏感度测定系统,利用Hartman-Shack波前像差传感器测量人眼波前像差,以及高空间频率的对比敏感度测量仪测量全视觉对比敏感度函数,进而得到人眼的神经对比敏感度.和传统激光干涉方法测量神经对比敏感度相比较,本文的测定方法,避免了激光干涉所产生的相干噪音和激光散斑不利因素,并且可以得到白光神经对比敏感度NCSF.对不同人眼分别对绿光和白光视网膜神经对比敏感度进行了测定,测试结果表明:在同等亮度下,绿光的神经对比敏感度远高于白光神经对比敏感度;绿光和白光的对比敏感度曲线的最大值出现在空间频率为8c/deg附近,而其神经对比敏感度曲线的最大值出现在相对高一些12c/deg附近的空间频率上.     

基于波前技术的人眼神经对比敏感度测量

搭建了基于波前像差的神经对比敏感度(NCSF)测试系统。该系统在测试人眼空间对比敏感度(CSF)的同时,利用Hartmann-Shack波前传感器测量人眼波前像差,通过计算进而得到人眼的NCSF。与通过两种设备分别测量全视觉CSF和波前像差获得NCSF相比,该方法避免了不同测试状态下像差波动的影响,简化了测试过程;和传统激光干涉方法测量NCSF相比,该方法避免了激光干涉产生的相干噪音和激光散斑等不利因素,并且通过改变不同亮度不同颜色视标,可以得到不同亮度,不同波长下的NCSF。选用绿光视标对四例正常人眼的NCSF进行了测量,结果表明:该系统可以同时获得人眼的全视觉CSF、屈光系统调制传递函数和NCSF;在同等亮度下,不同人眼的NCSF存在个体差异;对同一个体,NCSF曲线的最大值对应的空间频率比全眼空间CSF曲线的最大值对应的空间频率高一些。     

人眼的高级像差对视功能的影响

准确测量和分析人眼的高级像差有助于更好地改善视觉,具有重要的实验和临床意义。测量了实际人眼的波前像差,分析了高级像差对人眼视功能的影响。像差数据由哈特曼-夏克（Hartmann-Shack）波前传感器分别对不同瞳孔的人眼进行测量而获得,视功能的评价方法采用了调制传递函数（MTF）、对比敏感度函数（CSF）、斯特雷尔（Strehl）比率。由人眼的波前像差数据和视网膜空间像调制度（AIM）曲线直接给出了视锐度值与对比敏感度值。矫正了离焦与像散后．被测者的平均视锐度值达到了1．0,对比敏感度在低频（20c／mm）处约为52,高频（80c／mm）处约为1;矫正了前4阶像差后,平均视锐度值可提高到1．2,对比敏感度在低频（20c／mm）处提高到96,高频（80c／mm）处提高到7。实际人眼各不相同,达到理想成像需矫正高级像差的阶数也不同。矫正了前九阶像差后,均可达到理想成像,斯特雷尔比率值大于0．8。     

基于波前像差的视网膜空间像调制度测定

提出了一种计算复色光下人眼视网膜空间像调制度的方法.利用Hartmann-Shack波前传感器测量的波前像差数据，求得眼睛光学系统的调制传递函数；利用CSV-1000测试仪和VAF-1000视锐度测试仪分别测量同一只眼睛的全眼对比敏感度函数以及视锐度，由调制传递函数、对比敏感度函数以及视锐度之间的关联获得复色光下人眼视网膜空间像调制度曲线.结果表明：视网膜空间像调制度曲线与眼光学系统的调制传递函数无关，并且正常人眼（无视网膜疾病）的视网膜空间像调制度值相近.因此多眼的空间像调制度曲线的统计平均值可以作为标准，用来评判人眼视网膜及视神经疾病.     

人眼亮度和色度对比敏感视觉特性的#br# 测量及其模型研究

为了探讨人眼对比度敏感视觉特性,利用显示器显示11种空间频率、平均亮度为10、60和90 cd/m2的目标光栅,设计实验测量了120名青年的人眼亮度和色度对比敏感度数据,并采用最小二乘法对测量数据进行了分析和拟合,提出了一种多项式调制下的指数形式的人眼亮度和色度对比敏感视觉特性的数学模型,且与国内外典型的模型进行了对比分析。结果表明:随着空间频率f的增加,人眼对比敏感度先增加后减小,当f在3 cpd～4 cpd(周/度)时,人眼最为敏感,其与目前典型的视觉模型基本一致。表明提出的测量方法是有效的、可行的,提出的视觉模型具有一定的科学性;且该测量方法操作简单,视觉模型计算复杂度低,在实际应用中优于典型的测量方法和视觉模型,具有一定的参考价值。     

光学相关论题 视觉光学

R339.142006010793人眼的高级像差对视功能的影响=I mpact of higher-orderwavefront aberrations of human eyes on vision performance[刊,中]/王杨(南开大学现代光学研究所.天津(300071)),王肇圻…∥光学学报.—2005,25(11).—1519-1525测量了实际人眼的波前像差,分析了高级像差对人眼视功能的影响。像差数据由哈特曼-夏克(Hart mann-Shack)波前传感器分别对不同瞳孔的人眼进行测量而获得,视功能的评价方法采用了调制传递函数(MTF)、对比敏感度函数(CSF)、斯特雷尔(Strehl)比率。由人眼的波前像差数据和视网膜空间像调制度(AI M)曲…     

用于人眼视网膜成像照明的激光消散斑技术研究

以近红外激光(808 nm)作为人眼波前像差探测的信号光和视网膜成像的照明光,液晶空间光调制器(LCOS)作为波前校正器,用哈特曼波前探测器探测人眼像差,构建了人眼像差自适应校正的视网膜成像系统.利用模拟眼分析了激光散斑对相机成像的影响和对哈特曼波前探测器进行像差探测的影响,同时验证了利用旋转散射体的方法消除激光散斑的可行性和有效性;用活体人眼进行了激光消散斑前后照明视网膜进行成像的对比实验,并进一步利用自适应光学技术实现了对人眼像差的动态校正和视网膜细胞的连续成像.校正后,系统波前像差的均方根值小于0.1λ.实验表明激光消散斑后可以同时作为人眼像差探测的信号光和视网膜成像的照明光,从而可以进行连续自适应校正和成像.     

基于多尺度叠加的视觉距离模糊算法的研究

为能够模拟观察距离变大时引起的颜色视觉效应,研究了人眼视觉的视锐度特性和对比敏感度特性。通过对人眼视锐度原理的分析,实现了视锐度方法模拟视觉距离增大时的视觉模糊算法;通过对对比敏感度模型测试原理的分析,结合人眼视觉空间频率的多通道特性,实现了基于对比敏感度函数模型模拟视觉距离增大时的视觉模糊算法。视锐度方法可简单模拟视觉距离增大时的模糊效果,可用于观察灰度物体情况。观察彩色物体时,通过使用反差敏感度模型算法,能够模拟视觉感知的多尺度特性、低通和带通滤波特性、局部适应性和颜色感知的叠加性。     

人眼波前像差的动态特性研究

人眼波前像差随时间涨落会引起人眼光学性能和视觉功能的改变.采用改进的HartmannShack波前传感器人眼像差仪对10只屈光度为0D~-5.0D、直径为3mm和6mm的人眼瞳孔的波前像差进行测量,其中每只人眼在5s内连续测量125次,测量频率为25Hz.为确定测量过程中是否引入人为像差,对人造眼3mm和6mm瞳孔的动态波前像差进行测量比对.结果表明:所测量的10只人眼3mm和6mm瞳孔总的Zernike波前像差均方根涨落幅度的平均值分别为0.087μm和0.105μm,均大于Marechal衍射极限;Zernike第3阶到第7阶波前像差均方根涨落幅度随像差阶数的递增而下降,涨落幅度为0.06~0.02μm;人眼波前像差的涨落频率达6Hz.     

基于个性化人眼模型的大视场波像差特性的研究

大视场波前像差对人眼光学系统的影响不容忽视。运用Zemax光学设计软件分别为8只正常人眼构建了个性化的人眼模型,该人眼模型由实际测量的人眼波前像差数据、角膜地形数据及眼内各部分轴向间距数据优化得来,与个体人眼具有相同的光学特性。在此基础上,分析了人眼颞侧方向0°,10°,20°,30°,40°,50°视场的离轴像差随视场角的变化趋势,得出边缘视觉比中央视觉质量差主要来源在于像散与彗差。四阶以上的高阶像差随着视场角的改变,变化不大。将个性化人眼模型计算得到的大视场波前像差值与用哈特曼夏克(Hartmann-Shack)波前传感器实际测量得到的人眼像差值相比较,两者结果相吻合。     

The study of the effects of higher-order aberrations on human contrast sensitivity with white-light retinal aerial image modulation (AIM)

The impact of higher-order aberrations on contrast sensitivity function (CSF) is calculated using individual white-light retinal aerial image modulation (AIM). Wavefront aberrations of 26 eyes are measured with Hartmann-Shack sensor, and the CSFs in natural light are acquired through a range of 2-48 c/deg. The white-light AIM is computed as the ratio of modulation transfer function (MTF) in white-light to CSF. Through manipulating the higher-order aberrations, the affected CSF is predicted by employing the white-light AIM. We find that coma aberration mainly influences CSF at higher spatial frequency and spherical aberration affects CSF in the whole spatial frequency range non-selectively. Additionally, it is spherical aberration rather than coma that impacts the CSF more substantially. Furthermore, the maximum value of area under CSF (AUCSF) is obtained without full correction of higher-order aberration, which indicates that there is compensatory mechanism among aberrations.     

Measurements of retinal aerial image modulation (AIM) for white light based on wave-front aberration of human eye

The aerial image modulation (AIM) curve of retina under the condition of white light is obtained based on the wave-front aberration of human eye. According to the relationship between the wavelength and defocus, we modify the monochromatic wave-front aberration data to calculate the modulation transfer function (MTF) of human eye in the white-light illumination. Combined with the measurement of contrast sensitivity function (CSF) for complete eye and visual acuity (VA) under the same luminance condition, we deduce the AIM curve in natural light. We find that AIM varies slightly at lower and intermediate spatial frequencies among different eyes; at higher frequencies AIM is the predominant factor for VA when the wave-front aberration is not significant. In addition, retinal AIM is expressed in terms of neural contrast sensitivity function (NCSF) which is the clinical valuable for ophthalmologists. Considering the real illumination circumstance, it is of practical significance to obtain the AIM curve and NCSF curve under white-light condition.     

Study on NCSFs of individual color mechanisms of human vision based on wave-front aberrations

Neural contrast sensitivity functions (NCSFs) of isolated color mechanisms are obtained based on the measurements of wave-front aberrations and isoluminant color contrast sensitivity functions (CSFs). Our study indicates that the mean NCSF and CSF of the red mechanism are higher than those of the green mechanism, respectively, while those of the blue mechanism are the lowest. However, the relative heights of the peak of NCSF and CSF between red and green mechanisms vary in subjects. There are some individuals whose peak values of NCSF and/or CSF of green mechanism are higher than that of the red mechanism. On the other hand, we find that the NCSFs and CSFs of isolated color mechanisms all exhibit the similar characteristics and variation tendency. With the statistical average, the NCSFs of the red, green and blue mechanisms are higher than the corresponding CSFs in the whole spatial frequency. The peaks of the NCSFs of isolated color mechanisms, comparing with the corresponding CSFs curves, shift toward higher spatial frequencies, especially for that of blue mechanism which has a largest shift of 3.9 c/deg.     

The study on neural contrast sensitivity function at temporal frequencies

The neural contrast sensitivity function (NCSF) of human eye at temporal frequencies is acquired with a new method in this paper. Firstly the human eye's contrast sensitivity function (CSF) at temporal frequencies is measured by means of travelling-wave stimuli, and the modulation transfer function (MTF) of the eye's optics is obtained by constructing the eye model of the subject. Then the NCSF at temporal frequencies is calculated with the two functions. It is shown that the overall value of the NCSF decreases as the temporal frequency increases. As the temporal frequency increases from 0 cycles per second (c/s) to 1 c/s, 16 c/s and 30 c/s, the NCSF curve changes from the band-pass shape to the low-pass, and then to almost monotonic variation. The attenuation factor of the NCSF, which represents the sensitivity of visual neural system to the temporal frequency, varies little as spatial frequency increases, while that of the CSF declines dramatically in the region of high spatial frequencies. Because it is the NCSF, rather than the CSF, that reflects the characteristics of visual neural system, the investigation of the NCSF at temporal frequency is more essentially.     

Continuous wavelet transform for micro-component profile measurement using vertical scanning interferometry

White-light interferometric techniques have been widely used in three-dimensional (3D) profiling. This paper presents a new method based on vertical scanning interferometry (VSI) for the 3D profile measurement of a micro-component that contains sharp steps. The use of a white-light source in the system overcomes the phase ambiguity problem often encountered in monochromatic interferometry and also reduces speckle noises. A new algorithm based on the continuous wavelet transform (CWT) is used to retrieve the phase of an interferogram. The algorithm accurately determines local fringe peak and improves the vertical resolution of the measurement. The proposed method is highly resistant to noise and is able to achieve high accuracy. A micro-component (lamellar grating) fabricated by sacrificial etching technique is used as a test specimen to verify the proposed method. The measurement uncertainty of the experimental results is discussed.     

用SVGA1薄膜晶体管液晶显示器矫正人眼波像差

在研究了SVGA1薄膜晶体管液晶显示器（TFT LCD）的位相调制特性的基础上,用它作为眼波像差的矫正器件,在用哈特曼-夏克波前传感器的眼像差测量系统中对眼波像差进行了成功的矫正.对于5.2 mm的瞳孔,矫正后人眼波像差的PV值降低了3倍多,并接近瑞利判据的像差容限.对系统的光学传递函数(MTF)的分析说明,经波像差矫正后眼的空间分辨率由17 c/deg提高到38 c/deg.     

基于子谱分析的白光频域OCT

为了提高频域OCT系统轴向分辨率和信噪比,提出了一种采用白光光源的频域OCT系统,研究了所用的CCD相机的横向像素数、白光光源的光谱与系统轴向分辨率之间的关系,建立了一种基于子谱分析的白光频域OCT系统。通过选择所需的白光光源及其接收频段,既能保证最大探测深度和高轴向分辨率,又能提高信噪比。实验结果验证了所提出的光源的相干长度和系统及图像轴向分辨率测量方法,证明了白光频域OCT的可行性。     

Scattering of Solar and Atmospheric Background Radiation from a Target

Light scattering property of environment is very important in theoretical study and application of the remote sensing. What's more, it is valuable for infrared radiation, imaging, and the detection of target and tracking. In this paper, solar and atmospheric background radiation, and their scattering property from target are discussed. BRDF (Biodirectional Reflectance Distribution Function) is a very important quantity that shows the radiation and reflection feature of target. According to electromagnetic radiant and scattering theories, the relationship between laser radar scattering cross section (LRCS) and BRDF is introduced. LOWTRAN model is an effective method of calculating the spectral distribution of solar and atmospheric radiation. Here it is applied to compute solar and atmospheric background radiation scattered from a target. The relative equations are deduced. Thus, the spatial and spectral distribution of scattering light is given. As a special example, for the Lambert's surface, the equations are simplified. As a result, the spatial and spectral distributions scattering radiation of solar and atmospheric background from a rough painted surface are present. The scattering of solar radiation plays a primary role in MIR region, but scattering of atmospheric background radiation is higher in LIR region. At the same time, there is obviously specular reflectance for solar radiation due to coherent scattering from rough surface.