Ghost interference and diffraction based on the beam splitter

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三阶鬼成像的可见度研究

三阶鬼成像的可见度研究

三阶鬼成像的可见度研究于佳意;常锋;姚治海;徐聪;董博;王晓茜【摘要】Ghost imaging,also called correlation imaging,has attracted much attention in recent years. It has in estima-ble development prospects in many fields. This article put forward a new experiment scheme of third-order ghost imag-ing according to a research of third-order ghost imaging. We got the visibility range of both the original and new scheme by calculating the third-order correlation functions. Then,we compared these two kinds of schemes,and anal-ysed the similarities and differences between them. The result showed that,the new imaging scheme could improve the image quality and visibility. This conclusion was verified by numerical simulation.%鬼成像又称为关联成像,近年来受到广泛的关注,在很多领域上都具有广阔的发展前景。

通过对热光三阶鬼成像进行研究,提出一种新的三阶鬼成像实验方案。

通过计算三阶关联函数,导出三阶关联函数原始方案与新方案的可见度取值范围,将两种方案进行比较,分析它们的异同。

光学术语中英文对照

光学术语中英文对照

平面镜 Flat Mirrors球面凹面镜,球面凸面镜 Spherical Concave and Convex Mirrors 抛物面镜,椭圆面镜 Off-Axis Paraboloids and Ellipsoids Mirrors 非球面镜 Aspheric Mirrors多面镜 Polygonal Mirrors热镜 Hot Mirrors冷镜 Cold Mirrors玻璃,玻璃/陶瓷面镜 Glass and Glass-Ceramic Mirrors双色向面镜 Dichroic Mirror金属面镜 Metal Mirrors多层面镜 Multilayer Mirrors半涂银面镜 Half-Silvered Mirrors激光面镜 Laser Mirrors天文用面镜 Astronomical Mirrors棱镜系列术语中英文对照Nicol棱镜 Nicol PrismsGlan-Thomson棱镜 Glan-Thomson PrismsWollaston棱镜 Wollaston PrismsRochon棱镜 Rochon Prisms直角棱镜 Right-Angle; Rectangular Prisms五面棱镜 Pentagonal Prisms脊角棱镜 Roof Prisms双棱镜 Biprisms直视棱镜 Direct Vision Prisms微小棱镜 Micro Prisms滤光镜系列术语中英文对照尖锐滤光镜 Sharp Cut (off) Filters色温变换滤光镜,日光滤光镜 Colour Conversion/Daylight Filters 干涉滤光镜 Interference Filters中性密度滤光镜 Neutral Density Filters空间/光学匹配滤光镜 Spatial/Optical Matched Filters双色向滤光镜 Dichroic Filters偏光滤光镜 Polarizing Filters排除频带滤光镜 Rejection Band Filters可调式滤光镜 Turnable Filter超窄频滤光镜 Ultra Narrowband Filters色吸收滤光镜 Absorption Filters红外吸收/反射滤光镜 Infrared Absorbing/Reflecting Filters 红外透过滤光镜 Infrared Transmitting Filters紫外吸收滤光镜 Ultraviolet Absorbing Filters紫外透过滤光镜 Ultraviolet Transmitting Filters针孔滤光镜 Pinhole Filters有色玻璃滤光镜 Colored-Glass Filters塑胶滤光镜 Plastic Filters照像用滤光镜 Photographic Filters全像滤光镜 Holographic Filters微小干涉滤光镜 Micro Interference Filters光学词汇Iris – aperture stop虹膜孔径光珊retina视网膜Color Blind 色盲weak color 色弱Myopia – near-sighted 近视Sensitivity to Light感光灵敏度boost推进lag behind落后于Hyperopic – far-sighted 远视Dynamic Range 动态范围critical fusion frequency 临界融合频率CFF临界闪变频率visual sensation视觉Chromaticity Diagram色度图Color Temperature色温HSV Model色彩模型(hue色度saturation饱和度 value纯度CIE Model 相干红外能量模式Complementary Colors补色Bar Pattern条状图形Heat body 热稠化approximate近似violet紫罗兰Body Curve人体曲线Color Gamut色阶adjacent邻近的normal illumination法线照明Primary colors红黄蓝三原色Color saturation色饱和度Color Triangle颜色三角Color Notation颜色数标法Color Difference色差TV Signal Processing电视信号处理Gamma Correction图像灰度校正Conversion Tables换算表out of balance失衡wobble摇晃back and forth前后clear (white) panel白光板vibrant震动fuzzy失真quantum leap量子越迁SVGA (800x600)derive from起源自culprit犯人render呈递inhibit抑制,约束stride大幅前进blemish污点obstruction障碍物scratch刮伤substance物质实质主旨residue杂质criteria标准parameter参数adjacent邻近的接近的asynchrony异步cluster串群mutually互助得algorithm运算法则Chromatic Aberrations色差Fovea小凹Visual Acuity视觉灵敏度Contrast Sensitivity对比灵敏度Temporal (time) Response反应时间rendition表演,翻译animation活泼又生气ghost重影Parallax视差deficient缺乏的不足的Display panel显示板NG.( Narrow Gauge)窄轨距dichroic mirror二色性的双色性的Brewster Angle布鲁斯特角Polarized Light极化光Internal reflection内反射Birefringence 双折射Extinction Ratio 消光系数Misalignment 未对准Quarter Waveplates四分之一波片blemish污点瑕疵Geometric几何学的ripple波纹capacitor电容器parallel平行的他tantalum钽(金属元素)exsiccate使干燥exsiccate油管,软膏furnace炉子镕炉electrolytic电解的,由电解产生的module模数analog类似物out of the way不恰当pincushion针垫拉lateral侧面得rectangle长方形fixture固定设备control kit工具箱DVI connector DVI数局线Vertical垂直的horizontal 水平的interlace隔行扫描mullion竖框直楞sawtooth锯齿toggle套索钉keypad数字按键键盘tangential切线diagnostic tool诊断工具sagittal direction径向的cursor position光标位置ray aberration光线相差weighting factor权种因子variables变量for now暂时,目前.眼下check box复选框Airy disk艾里斑exit pupil出[射光]瞳optical path difference光称差with respect to关于diffraction limited衍射极限wavefront aberration波阵面相差spherical aberration球面象差paraxial focus傍轴焦点chromatic aberration象差local coordinate system局部坐标系统coordinate system坐标系orthogonal直角得,正交的conic sections圆锥截面account for解决,得分parabolic reflector拋物面反射镜radius of curvature曲率半径spherical mirror球面镜geometrical aberration几何相差incident radiation入射辐射global coordinate总体坐标in terms of根据按照reflected beam反射束FYI=for your information供参考Constructive interference相长干涉phase difference相差achromatic singlet消色差透镜Interferometer干涉仪boundary constraint边界约束,池壁效应radii半径Zoom lenses变焦透镜Beam splitters分束器discrete不连续的,分离的objective/eye lens物镜/目镜mainframe主机rudimentary根本的,未发展的photographic照相得摄影得taxing繁重的,费力得algebra代数学trigonometry三角学geometry几何学calculus微积分学philosophy哲学lagrange invariant拉格朗日不变量spherical球的field information场信息Standard Lens标准透镜Refracting Surface折射面astigmatism散光HDTV高清晰度电视DLV ( Digital Light Valve)数码光路真空管,简称数字光阀diffraction grating衍射光珊field angle张角paraxial ray trace equations近轴光线轨迹方称back focal length后焦距principal plane主平面vertex顶点,最高点astigmatism散光,因偏差而造成的曲解或错判medial中间的,平均的variance不一致conic圆锥的,二次曲线field of view视野collimator瞄准仪convolution回旋.盘旋,卷积fuzzy失真,模糊aberrated异常的asymmetry不对称得indicative可表示得parabolic拋物线得suffice足够,使满足specification规格,说明书straightforward易懂的,直接了当的solidify凝固,巩固.Constraints 约束,限制metrology度量衡field coverage视场,视野dictate口述, 口授, 使听写, 指令, 指示, 命令, 规定irradiance发光, 光辉,辐照度aerial空气得,空中得halide卤化物的monochromatic单色的,单频的polychromatic多色的aspherical非球面的spherical球面的alignment列队,结盟power(透镜)放大率equiconvergence 同等收敛EFL(effective focal length)有效焦距workhorse广为应用的设备biconvex两面凸的global optimization整体最优化concave凹得,凹面得cylindrical圆柱得solid model实体模型Modulation Transfer Function调制传递函数in the heat of在最激烈的时候protocol协议,规定triplet三重态sanity心智健全zinc锌,涂锌的selenide 硒化物,硒醚miscellaneous各色各样混在一起, 混杂的, 多才多艺的versus与...相对polynomial多项式的coefficient系数explicit function显函数distinct清楚的,截然不同的emanate散发, 发出, 发源rudimentary根本的,未发展的intersection角差点PRTE=paraxial ray trace equation旁轴光线轨迹方程 achromats 消色差透镜cardinal points基本方位separations分色片dashed 虚线blow up放大overlay覆盖,覆盖图 multiplayer 多层的humidity 湿度float glass浮法玻璃square one 出发点,端点square up to 准备开打,坚决地面对reflecting telescope 反射式望远镜 diagnostic tools诊断工具Layout plots规划图Modulation transfer function调制转换功能FFT快速傅里叶变换Point spread function点传播功能wavelength波长angle角度absorption吸收system aperture系统孔径lens units透镜单位wavelength range 波长范围singlet lens单业透镜spectrum光谱diffraction grating 衍射光栅asphere半球的LDE=Lens data editor Surface radius of curvature表面曲率半径surface thickness表面厚度material type 材料种类semi-diameter半径focal length焦距aperture type孔径类型aperture value孔径值field of view视场microns微米F, d, and C= blue hydrogen, yellow helium, red hydrogen lines, primary wavelength主波长sequential mode连续模式object surface物表面The front surface of the lens透镜的前表面stop 光阑The back surface of the lens透镜的后表面The image surface 像表面symmetric相对称的biconvex两面凸的The curvature is positive if the center of curvature of the surface is to the right of the vertex. It is negative if the center of curvature is to the left of the vertex.如果曲率中心在最高点的右边,曲率值为正,如果曲率中心在最高点的左边,则曲率为负image plane像平面Ray Aberration光线相差tangential direction切线方向sagittal direction径向paraxial focus旁轴的Marginal边缘的spherical aberration球面像差Optimization Setup最优化调整variable变量mathematical sense数学角度MFE= Merit Function Editor, Adding constraints增加约束focal length焦矩长度operand操作数the effective focal length有效焦矩primary wavelength主波长initiate开始spot diagram位图表Airy disk艾里斑axial chromatic aberration轴向色差with respect to关于至于exit pupil出射光瞳OPD=optical path difference光学路径差diffraction limited衍射极限chromatic aberration色差chromatic focal shift色焦距变换paraxial focus傍轴焦点axial spherical aberration轴向球差(longitudinal spherical aberration 纵向球差:沿光轴方向度量的球差)lateral spherical aberration垂轴球差(在过近轴光线像点A‵的垂轴平面内度量的球差)coma、comatic aberration彗差meridional coma子午彗差sagittal coma弧矢彗差astigmatism像散local coordinate system 本地坐标系统meridional curvature of field子午场曲sagittal curvature of field弧矢场曲decentered lens偏轴透镜orthogonal 直角的垂直的conic section圆锥截面account for说明,占有,得分stigmatic optical system无散光的光学系统Newtonian telescope牛顿望远镜parabolic reflector抛物面镜foci焦距chromatic aberration,色差superpose重迭parabola抛物线spherical mirror球面镜RMS=Root Mean Square均方根wavefront 波阵面spot size光点直径Gaussian quadrature高斯积分rectangular array矩阵列grid size磨粒度PSF=Point Spread Function点扩散函数FFT=Fast Fourier Transform Algorithm快速傅里叶变换Cross Section横截面Obscurations昏暗local coordinates局部坐标系统vignette把…印为虚光照Arrow key键盘上的箭头键refractive折射reflective反射in phase同相的协调的Ray tracing光线追迹diffraction principles衍射原理order effect式样提出的顺序效果energy distribution能量分配Constructive interference相长干涉dispersive色散的Binary optics二元光学phase advance相位提前achromatic single消色差单透镜diffractive parameter衍射参数Zoom lenses变焦透镜Athermalized lenses绝热透镜Interferometers干涉计Beam splitter分束器Switchable component systems可开关组件系统common application通用symmetry对称boundary constraint边界约束multi-configuration (MC) MC Editor (MCE) perturbation动乱,动摇index accuracy折射率准确性index homogeneity折射率同种性index distribution折射率分配abbe number离差数Residual 剩余的Establishing tolerances建立容差figure of merit质量因子tolerance criteria公差标准Modulation Transfer Function (MTF)调制传递函数boresight视轴,瞄准线Monte Carlo蒙特卡洛Tolerance operands误差操作数conic constant ]MC1"{_qT .ueg g 圆锥常数astigmatic aberration像散误差Mechanical tilt机械倾斜,机械倾角Tolerance Data Editor (TDE)公差资料编辑器compensator补偿棱镜estimated system performance预估了的系统性能iteratively反复的,重迭的statistical dependence统计相关性sequential ray trace model连续光线追迹模型imbed埋葬,埋入multiple多样的,多重的,若干的Non-Sequential Components 不连续的组件Corner cube角隅棱镜,三面直角透镜Sensitivity Analysis灵敏度分析Faceted reflector有小面的反射镜emit发射,发出nest嵌套overlap交迭outer lens外透镜brute force强力seidel像差系数aspect ratio长宽比MRA边缘光线角MRH边缘光线高度asynchronous不同时的,异步 Apodization factor变迹因子hexapolar六角形dithered高频脉冲衍射调制传递函数(DMTF),衍射实部传递函数(DRTF),衍射虚部传递函数(DITF),衍射相位传递函数(DPTF),方波传递函数(DSWM)logarithmic对数的parity 奇偶 % Uc,I e ,17]3NnoClongitudinal aberrations 纵向像差赛得系数: 球差(SPHA,SI),彗差(COMA,S2),像散(ASTI,S3),场曲(FCUR,S4),畸变(DIST,S5),轴向色差(CLA,CL)和横向色差(CTR,CT).横向像差系数:横向球差(TSPH),横向弧矢彗差(TSCO),横向子午彗差(TTCO),横向弧矢场曲(TSFC),横向子午场曲(TTFC),横向畸变(TDIS)横向轴上色差(TLAC)。

和哥哥一起做实验作文

和哥哥一起做实验作文

和哥哥一起做实验作文English Response:In the realm of scientific exploration, curiosity and collaboration dance in harmonious synchrony. With my brother as my intrepid partner, I embarked on an extraordinary experimental journey that ignited our imaginations and expanded our understanding of the world around us.The experiment, meticulously designed, sought to unravel the secrets of sound wave propagation. Armed with an array of scientific instruments, including a frequency generator, speakers, and a microphone, we meticulously set up our laboratory, eager to unravel the mysteries that lay ahead.As the experiment commenced, we generated different frequencies of sound waves through the speakers. The microphone, acting as our sensory instrument, captured thevariations in sound intensity as the waves traversed our experimental setup. With each adjustment, we meticulously recorded and analyzed the data, our eyes fixed upon the computer screens that revealed the intricate patterns of sound propagation.Throughout the experiment, my brother and I shared insights, ideas, and observations. Our collaboration was a testament to the power of teamwork in scientific exploration. We discussed our findings, challenged each other's assumptions, and remained open to unexpected outcomes.The experiment culminated in a series of fascinating discoveries. We observed that the frequency of the sound wave influenced its propagation speed, and that higher frequencies traveled faster than lower frequencies. Additionally, we noticed that obstacles in the path of the sound waves caused reflections and diffractions, creating complex patterns of interference and reinforcement.Chinese Response:和哥哥一起做实验是我难忘的经历。

光双缝衍射的量子理论

光双缝衍射的量子理论

光双缝衍射的量子理论陶莹;刘晓静;王清才;陈万金;王岩;郭义庆【摘要】通过求解光的相对论波动方程,得到光在缝中的波函数,再由基尔霍夫定律得到光的衍射波函数,从而得到光的双缝衍射强度表达式,结果表明,理论结果与光的双缝衍射实验数据符合较好.【期刊名称】《吉林大学学报(理学版)》【年(卷),期】2011(049)004【总页数】6页(P750-755)【关键词】量子理论;光衍射;基尔霍夫定律;相对论波动方程【作者】陶莹;刘晓静;王清才;陈万金;王岩;郭义庆【作者单位】吉林师范大学教育技术与传播学院,吉林四平136000;吉林师范大学物理学院,吉林四平136000;吉林师范大学物理学院,吉林四平136000;吉林师范大学物理学院,吉林四平136000;吉林师范大学物理学院,吉林四平136000;中国科学院高能物理研究所,北京100049【正文语种】中文【中图分类】O413由于光具有波动性和粒子性, 因而在一定条件下会产生干涉和衍射现象[1-4]. 文献[5-8]利用量子理论方法研究了电子和中子的衍射, 所得结果与实验相符. 目前, 光衍射理论的描述主要用经典电磁理论, 该理论可描述光的衍射现象. 但由于光子具有波动性和粒子性, 因此对光衍射的精确描述应采用量子理论[9-10]. 本文用量子理论新方法, 通过求解光的波函数ψ(r,t), 得到光的相对衍射强度. 其中波函数模的平方表示光子在空间出现的几率密度, 而光的相对衍射强度正比于波函数模的平方. 本文在文献[10]的基础上, 增加了反射波的贡献. 通过理论推导得到衍射强度与缝长度、宽度、厚度、光波长以及衍射角间的解析关系.1 单缝中光的波函数φ(r,t)光的双缝衍射如图1所示. 假设双缝的宽度均为a, 长度均为b, 厚度为c′. 取x轴沿缝宽方向, y轴沿缝长方向. 在t时刻, 假设入射光沿z轴方向入射, 则波函数可表示为(1)图1 光的双缝衍射Fig.1 Light double-slit diffraction其中: φ0j=Aj·exp{ipz/ћ}(j=x,y,z); A为常矢量.光的含时相对论量子波动方程为[11]iћћ▽×φ(r,t)+Vφ(r,t),(2)其中: c为光速;势能在缝中V=0.光的相对论波动方程为iћћ▽×φ(r,t),(3)将式(3)两边对时间求导可得▽(▽·φ(r,t)-▽2φ(r,t))].(4)由于则有▽·φ(r,t)=0,(5)由式(4),(5)可得(6)当φ(r,t)在一定频率下变化时,φ(r,t)=φ(r)e-iωt,(7)将式(7)代入式(6)可得(8)其中波函数φ(x,y,z)满足边界条件: φ(0,y,z)=φ(b,y,z)=0,(9)φ(x,0,z)=φ(x,a,z)=0,(10)光子波函数(11)将式(11)代入式(8)~(10)可得(12)φj(0,y,z)=φj(b,y,z)=0,(13)φj(x,0,z)=φj(x,a,z)=0,(14)对式(12)中φj(r)进行分离变量:φj(x,y,z)=Xj(x)Yj(y)Zj(z),(15)可得式(12)的一般解为(16)其中: 第一项为透射波函数; 第二项为反射波函数. 由波函数在z=0处连续φ0(x,y,z;t)|z=0=φ(x,y,z;t)|z=0,(17)φ0j(x,y,z)|z=0=φj(x,y,z)|z=0 (j=x,y,z)(18)可得(19)由波函数导数在z=0处连续或得(20)将式(19),(20)进行傅里叶变换可得:(21)(22)由式(21)和(22)可得(23)(24)其中将式(23)和(24)代入式(16)可得(25)将式(25)代入式(11)可得(26)2 光的衍射波函数ψ(r,t)由基尔霍夫公式可知ψj(r,t)满足[12] (27)图2 光的单缝衍射Fig.2 Light single-slit diffraction总的衍射波函数为(28)光的单缝衍射如图2所示. 其中: r′为单缝中z=c′平面上的一点(常数c′为单缝厚度); x为衍射空间的任意一点; n为垂直于单缝表面的单位矢量. k2沿r方向, 且k2=kr/r. 由图2可得:(29)(30)这里k2=kr/r. 将式(25),(29)和(30)代入式(27)可得(31)其中: 设k2与x轴夹角为π/2-α, 与y轴夹角为π/2-β, α和β即为衍射波偏离yz 面和xz面的角, 因此有k2x=ksin α, k2y=ksin β,(32)n·k2=kcos θ,(33)这里θ为k2与z轴的夹角, 且θ,α,β满足(34)将式(32),(33)代入式(31)可得(35)将式(35)代入式(28)可得(36)式(36)即为光通过第一个缝后的光衍射波函数.3 光的双缝衍射波函数由式(36)可得光通过第一个缝后的波函数为(37)通过坐标变换(38)可得光通过第二个缝后的波函数为(39)则双缝衍射总的波函数为ψ(x,y,z;t)=c1ψ1(x,y,z;t)+c2ψ2(x,y,z;t),(40)其中c1,c2为态叠加系数. 由于因此在显示屏上观察到光的双缝衍射强度I∝.4 结果与讨论图3 理论结果与实验数据比较Fig.3 Comparison between theoretical result and experimental data理论结果与实验数据比较如图3所示, 其中曲线为理论计算结果, 黑点为实验数据. 为方便与实验数据[13]进行比较, 将衍射角β转换为距离s, 由于衍射角非常小, 因此在理论计算中, 与yz面的衍射夹角α=0, 普朗克常数ħ=1.055×10-34 J·s, 态叠加系数c1=0.964, c2=0.264, 缝的长度b=3.0×10-3 m, 缝厚c′=1×10-3 m. 由图3可见, 理论计算结果与实验数据符合较好.综上所述, 本文利用光的相对论量子理论方法研究了光的双缝衍射, 给出了光的衍射强度与缝长、缝宽、缝厚、光的波长及衍射角间的关系, 并将光的衍射强度与实验数据进行比较, 结果表明, 理论计算结果与实验数据符合较好.参考文献【相关文献】[1] Pittman T B, Shih Y H, Strekalov D V, et al. Optical Imaging by Means of Two-Photon Quantum Entanglement [J]. Phys Rev A, 1995, 52(5): R3429-R3432.[2] Brown R H, Twiss R Q. A Test of a New Type of Stellar Interferometer on Sirius [J]. Nature, 1956, 178: 1046-1048.[3] Haner A B, Isenor N R. Intensity Correlations from Pseudothermal Light Sources [J]. American Journal of Physics, 1970, 38(6): 748-751.[4] ZHAI Yu-hua, CHEN Xi-hao, ZHANG Da, et al. Two-Photon Interference with True Thermal Light [J]. Phys Rev A, 2005, 72(4): 043805.[5] WU Xiang-yao, ZHANG Bai-jun, LI Hai-bo, et al. Quantum Theory of Electronic Double-Slit Diffraction [J]. Chin Phys Lett, 2007, 24(10): 2741-2744.[6] WU Xiang-yao, ZHANG Bai-jun, HUA Zhong, et al. Quantum Theory Approach for Neutron Single and Double-Slit Diffraction [J]. Int J Theor Phys, 2010, 49: 2191-2199. [7] LIU Xiao-jing, ZHANG Bai-jun, LI Hai-bo, et al. Quantum Theory of Neutron Double-Slit Diffraction [J]. Acta Phys Sin, 2010, 59(6): 4117-4122. (刘晓静, 张佰军, 李海波, 等. 应用量子理论方法研究中子双缝衍射 [J]. 物理学报, 2010, 59(6): 4117-4122.)[8] WU Xiang-yao, ZHANG Bai-jun, LIU Xiao-jing, et al. Quantum Theory for Neutron Diffraction [J]. International Journal of Modern Physics B, 2009, 23(15): 3255-3264.[9] WU Xiang-yao, LIU Xiao-jing, WU Yi-heng, et al. Quantum Wave Equation of Photon [J].Int J Theor Phys, 2010, 49: 194-200.[10] WU Xiang-yao, ZHANG Bai-jun, YANG Jing-hai, et al. Quantum Theory of Light Diffraction [J]. Journal of Modern Optics, 2010, 57(20): 2082-2091.[11] Smith B J, Raymer M G. Photon Wave Functions, Wave-Packet Quantization of Light, and Coherence Theory [J]. New J Phys, 2007, 9: 414.[12] Schwartz M. Principles of Electrodynamics [M]. Oxford: Oxford University Press, 1972.[13] Strekalov D V, Sergienko A V, Klyshko D N, et al. Observation of Two-Photon “Ghost” Interference and Diffraction [J]. Phys Rev Lett, 1995, 74(18): 3600-3603.。

哈里德 物理学基础 学习指导 36 Diffraction

哈里德 物理学基础 学习指导 36 Diffraction
diffraction maximum? T\rtor: The edge of the maximum is where the minima are. Student: So I need to find the minimum corresponding to m
T\rtor:
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Yes.
Student: And they are NhomakorabeatC
EXAMPLE
Light of wavelength 570 nm goes through a slit of width 30 pm. What is the width of the central diffraction maximum on a screen 1.5 m away?
What's the "central diffraction maximum?" At the middle of the pattern on the screen, light from all points in the slit travels the same distance, so they all interfere constructively, and the light is the brightest. If you move away from the center to the spot where o sin 0 - ), then the light from the bottom half of the slit cancels the light from the top half and
A more interesting question is what to do with a single slit. It may seem that with only one source, there should be no interference. But light from the far edge of the slit has to go a little further than light from the near edge of the slit. To deal with one slit properly, we need to divide it into an infinite number of slits.

光的折射实验说明作文英语100字

光的折射实验说明作文英语100字

光的折射实验说明作文英语100字全文共6篇示例,供读者参考篇1The Bending of Light: A Wondrous Experiment with RefractionHave you ever noticed how things can look a bit bent or distorted when you look at them through water? Maybe you've seen a pencil or straw dipped halfway into a glass of water and it seemed broken or bent at the surface. That's because of something called refraction - the bending of light as it passes from one material into another.In our science class, we did a super cool experiment to see refraction in action. Miss Wilson told us we were going to investigate how light bends when it goes from the air into water.I was really excited because I love hands-on experiments where we get to use special science equipment.First, Miss Wilson had us gather around the demonstration table at the front of the class. She had a large rectangular glass container filled with water, and next to it was a bright light source that shone a beam of light across the surface of the water.We could clearly see the beam of light traveling through the air above the water."What do you think will happen when the light beam hits the water?" Miss Wilson asked us. Some of my classmates guessed that the light would just keep going straight through the water. But I raised my hand and said I thought the light would bend or change direction when it hit the water. Miss Wilson smiled and told me I was right!She then carefully adjusted the light source so that the beam struck the surface of the water at an angle. As soon as the beam hit the water, we could all see it bend and take a different path through the water! It was like the light beam was being pushed in a new direction as it went from the air into the denser water. We all gasped and marveled at how clearly we could observe the refraction happening right before our eyes.Miss Wilson then explained that refraction occurs because light travels at different speeds through different materials. In the air, light travels extremely fast. But when it enters a denser substance like water, the light slows down slightly. This causes the wavefronts of the light beam to tilt and bend as they cross the boundary from one material into the other at an angle.We learned that the amount of bending or refraction depends on two main factors: the angle that the light beam strikes the surface, and the properties of the two materials the light is traveling between. The greater the difference in density between the materials, the more dramatic the amount of refraction.After the demonstration, we split up into small groups and each group got their own plastic container of water to experiment with. We took turns shining a laser pointer through the air and into the water at different angles to observe the refraction. We traced the paths of the light beams with our fingers on the sides of the containers. It was amazing to see how drastically the light could bend when it hit the water at very steep angles!My favorite part was when Miss Wilson brought out some other objects for us to shine the laser through - things like glass blocks, plastic sheets, and even an old glass diamond ring that belonged to her grandmother. We could really see how the light refracted differently depending on the densities and shapes of the objects.When I got home that day, I couldn't wait to show my parents what I had learned about refraction. I filled up a clearglass with water and shone a flashlight through it at an angle. Just like in class, the beam bent and distorted as it went from the air into the water. My dad pointed out that this is why pencils and other objects always look a bit wonky and bent when you view them underwater in a pool or lake - because the light is refracting!I feel like I really understand refraction now after doing those hands-on experiments. Whenever I see light bending or taking weird paths, I think about how it must be traveling between different materials of varying densities. Refraction is one of the coolest optical effects, and I'm glad we got to investigate it so thoroughly in class. Who knew that a simple thing like light could be capable of such wondrous bending and redirection? Science is awesome!篇2The Awesome Refraction Experiment!Have you ever looked into a glass of water and noticed how the pencil or straw looks kind of bent and weird? That's because of something called refraction - the bending of light waves as they pass from one material into another. My science teachershowed us a really cool experiment to see refraction in action, and I'm going to tell you all about it!First, we gathered our materials. We needed a glass baking dish or shallow pan, some water, a plastic or paper protractor to measure angles, and a bright flashlight or laser pointer. My teacher let me be in charge of filling the baking dish about halfway with water. I was very careful not to spill any!Next, we positioned the dish on a flat surface and shined the light from the flashlight through the side of the dish at an angle. The light beam entered the water at one angle, but when it passed through into the water, it bent and traveled at a different angle! My teacher called the initial angle the "angle of incidence" and the new angle in the water the "angle of refraction."Using the protractor, we carefully measured both of those angles for several trials. We had to hold the protractor right next to the dish and look very closely to get accurate measurements. It was kind of tricky, but totally worth it to see the science up close.As we took more measurements, a pattern started to emerge. The angle of refraction was always smaller than the angle of incidence when the light passed from air into water. But when we shined the light from water into air, the opposite happened - theangle of refraction became larger than the angle of incidence! Woah, how crazy is that?My teacher explained that this happens because of the different properties of the materials the light is traveling through. Light actually travels at different speeds through different substances. It travels fastest through empty space and air, but slows down a little in water and even more in glass or certain other materials.When light passes from a fast medium like air into a slower one like water, the wavefronts get a little disrupted and the beam bends toward the normal line (an imaginary line perpendicular to the surface). The denser the new material, the more the light slows and the more it refracts or bends. This causes the beam to follow a different angle of refraction than the original angle of incidence.In the reverse situation, when light passes from a slower medium like water to a faster one like air, the wavefront gets disrupted in a different way and the light bends away from the normal line. The beam emerges at a larger angle of refraction compared to the angle it entered the water at.Seeing this happen with my own eyes was amazing! I felt like a real scientist measuring the angles so precisely. My teachersaid that refraction is not only fascinating, but also has tons of practical applications.For example, lenses in glasses, telescopes, cameras, and microscopes all work by refracting and bending light in very precise ways to help us see better. Rainbows are another example - the colors we see are produced by the refraction and dispersion of sunlight through water droplets in the atmosphere. Isn't that so cool?At the end, my teacher let me play around by shining the laser through different objects like glasses, plastic containers, and even gelatin to observe the refraction effects. I tried bending the laser beams in all kinds of crazy directions! I felt like I had laser superpowers or something.Overall, the refraction experiment was one of the highlights of our optics unit. I had so much fun getting hands-on experience with this fundamental principle of light. Who knew that a simple glass dish, water, and a flashlight could demonstrate such an awesome phenomenon? I can't wait until we get to learn about other properties of light like reflection, interference, and diffraction. The world of optics is so incredibly fascinating!篇3The Light Refraction ExperimentHi everyone! Today I want to tell you all about the super cool light refraction experiment we did in science class. It was so much fun and I learned a ton about how light behaves.First, let me explain what refraction is. Refraction happens when light travels from one transparent material into another transparent material at an angle. As the light crosses the boundary between the two materials, it actually bends and changes direction a little bit. Crazy, right?Our experiment was all about seeing this refraction effect in action. The materials we used were a glass block, a laser pointer, and a piece of paper with a line drawn on it. Oh, and we also had a protractor to measure angles.The first step was to put the glass block on the paper, lining it up so one edge was right on the line. Then we shone the laser pointer through the side of the block at an angle. When the laser beam went into the glass, it bent! We could clearly see the beam was no longer traveling in a straight line after it entered the glass.Using the protractor, we measured the angle that the beam made going into the glass. We called this the "angle of incidence." Then we measured the angle that the refracted (bent) beam made on the other side of the glass block. This was called the "angle of refraction."We tried shining the laser at a bunch of different incident angles and measured the refraction angles each time. The results were really neat! When the incident angle was small, the refraction angle was also small. But as we increased the incident angle, the refraction angle got bigger too. However, there was a limit. No matter how big we made the incident angle, the refraction angle never got larger than about 42 degrees in the glass we used.Our teacher explained that this maximum refraction angle of 42 degrees is called the "critical angle" for that type of glass. If we made the incident angle any bigger than the critical angle, the light would actually get trapped inside the glass by total internal reflection instead of refracting out the other side.Total internal reflection is another really awesome property of light interacting with transparent materials. Basically, if the incident angle is greater than the critical angle, the light gets completely reflected back into the material it's traveling through,rather than passing through to the next medium. Fiber optic cables used for telecommunications and endoscopes used by doctors both rely on this total internal reflection effect.After trying out lots of different angles, we graphed our incident angle and refraction angle data. The graph showed a curved relationship, where the refraction angles got increasingly bigger compared to the incident angles as the incident angle increased.This curve is described by an equation called Snell's Law, named after the mathematician who first studied it deeply. Snell's Law states that the ratio of the sine of the incident angle to the sine of the refracted angle is a constant, which depends on the two materials the light travels between.By measuring the angles very precisely and calculating the sines, we were able to determine the constant value for the pair of materials used in our glass block. It matched up with the textbook value, which was really exciting!The best part was when we got to take the glass blocks home. My friend and I spent hours shining laser pointers and flashlight beams through the blocks and watching the refraction effects. We even tried making some cool light art by refracting the beams in different ways.I had so much fun with this experiment and feel like I really understand refraction and Snell's Law now. Who knew that the simple act of light bending as it goes from one material to another could be so fascinating and lead to all sorts of useful applications? Science is awesome!Well, that's the story of our thrilling light refraction lab. Let me know if you have any other questions! I'm officially a refraction expert now after conquering this experiment. Thanks for reading, friends!篇4The Awesome Light Refraction ExperimentHave you ever noticed how a pencil looks bent when you put it in a glass of water? Well, that's because of something called refraction! Refraction is when light bends as it moves from one material to another. It's kind of like when you're walking on the street and you suddenly step onto the grass, your path changes a little bit. Light does the same thing!In our science class, we did a really cool experiment to see refraction happening right before our eyes. Ms. Johnson, our teacher, told us we were going to learn about how light travelsand what happens when it goes from one material to another. We were all super excited because we love doing experiments!First, Ms. Johnson told us a little bit about light. She said that light travels in straight lines, called rays. When light hits something, like a window or a piece of paper, it either gets reflected (bounces back) or it passes through the material. If it passes through, that's called transmission. But sometimes, when light goes from one material to another, like from air to water, it bends or refracts.Then, Ms. Johnson showed us how to set up the experiment. We each got a clear plastic container filled with water, a pencil, and a piece of paper with a straight line drawn on it. We were supposed to put the pencil in the water, but hold it at an angle, not straight up and down.When I put the pencil in the water, it looked like it was broken! The part of the pencil in the water looked like it was bent at a weird angle from the part of the pencil that was still in the air. It was so cool!Ms. Johnson explained that the reason the pencil looked bent was because of refraction. When the light from the pencil traveled from the air into the water, it slowed down a little bitand changed direction slightly. That's what made the pencil look bent!But that's not all we did. Next, we had to put the piece of paper with the straight line behind the container of water. When we looked through the side of the container, the line looked like it was broken or offset! Again, this was because of refraction. The light from the line was bending as it went from the air into the water and back into the air on the other side of the container.We even got to try looking at the container from different angles, and the amount of bending or refraction changed depending on the angle. It was so much fun to see refraction happening right in front of us!After the experiment, Ms. Johnson taught us more about why refraction happens. She said that light travels at different speeds in different materials. In air, light travels really fast, but in water or glass, it slows down a little bit. When light has to go from one material to another, it has to kind of "adjust" its speed and direction, which is what causes the bending or refraction.She also told us that refraction is what makes things look distorted or wavy when you look at them through water or glass. It's also why rainbows happen! When sunlight hits raindrops in the sky, it refracts or bends as it goes from the air into the waterdroplets and back out into the air. This separates the white sunlight into all the different colors of the rainbow. Isn't that amazing?I loved doing the light refraction experiment. It was so much fun to see something that happens all the time in the real world, like light bending, right there in our classroom. Science is the best!篇5Experiment on Light RefractionHave you ever noticed how a pencil looks bent when you put it in a glass of water? Or how the bottom of a swimming pool appears closer than it really is? That's because light bends or refracts when it travels from one medium to another, like from air to water or water to air. This bending of light is called refraction, and it's what we're going to explore in this fun experiment!Before we start, let me explain what refraction is in simple terms. Light travels in waves, and when these waves move from one medium to another, like air to water, their speed changes. This change in speed causes the light waves to bend or refract. The denser the new medium is, the more the light will bend.Now, let's get started with the experiment! You'll need a few things:A glass of waterA pencil or strawA flashlight or strong light sourceFirst, fill the glass about three-quarters full with water. Now, place the pencil or straw into the water at an angle, so part of it is in the water and part is out. Look at the pencil from the side of the glass. What do you notice?The part of the pencil in the water appears bent or broken! This is because the light coming from the pencil is refracting or bending as it travels from the water (a denser medium) into the air (a less dense medium).Next, turn off the lights in the room and shine the flashlight onto the pencil in the water at an angle. You should see the light beam bending as it enters the water and then bending again as it exits the water.Isn't that cool? You're seeing refraction in action!But why does this happen? Well, when light travels from one medium to another, like from air to water, its speed changes. In adenser medium like water, light slows down a bit. This change in speed causes the light waves to bend or refract.Here's a simple way to understand it: Imagine you're running on a flat surface, and then you suddenly step onto a muddy patch. Your feet would sink into the mud, and you'd have to change direction slightly to keep going forward. That's similar to what happens to light when it moves from one medium to another with a different density.You can try this experiment with other transparent materials too, like glass or plastic. You'll notice that the amount of bending or refraction depends on the density of the material. The denser the material, the more the light will bend.Refraction is not just a cool optical illusion; it has many practical applications in our daily lives. Lenses in glasses, cameras, telescopes, and microscopes all rely on refraction to help us see better. Even rainbows are formed due to the refraction and dispersion of sunlight through raindrops!I hope this experiment has helped you understand refraction better. Next time you see a pencil in a glass of water or notice the bottom of a pool looking closer than it is, you'll know it's all thanks to the bending of light!篇6The Awesome Refraction Experiment!Have you ever looked into a glass of water and noticed how the pencil or straw looks kind of bent or broken? That's because of something called refraction! Refraction is when a light ray changes direction as it goes from one transparent material into another. The light ray bends and that makes things look different than they really are.In my science class, we did a really cool experiment to see refraction happening right before our eyes. My teacher Ms. Martin told us we were going to learn about how light behaves when it travels through different materials. I thought that sounded pretty interesting!First, Ms. Martin explained what refraction is all about. She said that when light travels from one medium to another with a different density, like from air into water, the light ray changes direction a little bit. The denser the new medium is, the more the light will bend.To show us what she meant, Ms. Martin had us do an experiment. She gave each of us a rectangular plastic container and told us to fill it about 3/4 full with water. Then we got aplastic circular plate to put on top. Using a pencil, we traced a line across the diameter of the plate. This was going to help us see the refraction.Next, Ms. Martin turned off the classroom lights and used a bright flashlight to shine the beam through the side of the container. When the beam hit the water, we could see it refracting and bending downwards! The line we traced on the plate helped us compare where the refracted beam hit versus where it would have gone if there was no water there. So cool!After that, we got to play around with the refraction effect some more. Ms. Martin had us partially submerge a pencil into the water at an angle. Because of refraction, the pencil looked like it had a weird bent or broken section underwater! The part in the water seemed offset from the part in the air. Wild!Then we tried the same thing but used a glass instead of the container. We could see the refraction effect even better through the curved glass surface. Things looked all distorted and wavy. It was like the pencil was made of rubber!My favorite part was making our own simple rainbow using refraction. We angled the flashlight beam through the glass of water just right. As the light entered and exited the water, it refracted and the white beam separated into the colors of therainbow! You could see red, orange, yellow, green, blue, indigo, and violet. Making a rainbow out of just a glass of water was pure magic.After the experiments, Ms. Martin explained that refraction happens because light waves travel at different speeds through different materials. For example, light goes slower through water than air. So when the light beam enters the water, it refracts and bends towards the normal line. The denser the material, the more the light slows down and the more it refracts.Refraction is why a pool looks shallower than it really is when you view it from the side. It's also why the sun appears to be positioned higher in the sky than its true position. And rainbows? Those beautiful rainbow arcs are caused by refraction and dispersion of sunlight through millions of raindrops!I had so much fun learning about refraction through our hands-on experiments. Who knew some simple water and light could reveal one of the awesome ways light behaves in the world around us? I can't wait until our next science exploration. Maybe we'll learn more about light or dig into another physics concept. Science rocks!。

白光干涉_精品文档

白光干涉_精品文档

白光干涉引言白光干涉是一种以白光为光源的干涉现象。

干涉现象是指两束或多束光波相互叠加形成干涉条纹的现象。

白光由许多不同波长的光波组成,因此在干涉中会出现一整套彩色的干涉条纹。

白光干涉广泛应用于光学领域,也为研究光的性质和干涉现象提供了重要的实验手段。

白光干涉的原理白光干涉的原理可以通过杨氏双缝干涉实验来解释。

在杨氏双缝干涉实验中,一束光通过一块有两个狭缝的屏幕后,会形成一组干涉条纹。

当白光通过这两个狭缝时,不同波长的光波会以不同的角度散射,因此在干涉条纹中可以观察到彩色的条纹。

干涉条纹的形成是由于光波的相干性。

相干性指的是两个光波的相位关系的稳定性。

当两束光波的相位差满足一定条件时,它们会相互干涉形成明暗相间的条纹。

在白光干涉中,不同波长的光波会产生不同的相位差,从而形成彩色的干涉条纹。

应用白光干涉在很多领域都有重要的应用。

以下是一些常见的应用:1. 厚度测量:白光干涉可以用来测量透明物体的厚度。

通过测量干涉条纹的间距或颜色的变化,可以推断出透明物体的厚度。

这在材料科学和工程中具有重要意义。

2. 反射率测量:白光干涉也可以用来测量材料的反射率。

通过分析反射光的干涉条纹,可以推断出材料的光学性质。

这对于研究透明材料的折射率和反射率具有重要意义。

3. 光学薄膜:白光干涉在光学薄膜的设计和表征中起着关键作用。

薄膜的干涉效应可以用来实现光学滤波器、反射镜和分光器等光学器件。

通过精确控制薄膜的厚度和折射率,可以实现对特定波长光的选择性传输或反射。

4. 激光干涉:白光干涉在激光器技术中也有重要应用。

激光干涉可以用来调谐激光器的输出波长和稳定性。

通过调整反射镜或干涉仪的位置,可以实现对激光器输出光波的准确控制。

结论白光干涉是一种以白光为光源的干涉现象。

它通过不同波长的光波的干涉叠加,形成彩色的干涉条纹。

白光干涉在光学领域的应用十分广泛,例如厚度测量、反射率测量、光学薄膜设计和激光器技术等。

这些应用不仅丰富了人们对光的认识,也为光学科学的发展做出了重要贡献。

光学专业英语

光学专业英语

Iris – aperture stop虹膜孔俓光珊retina视网膜[ˈrɛtnə]Color Blind 色盲weak color 色弱Myopia – near-sighted 近视(Myopia[maɪˈopiə])Sensitivity to Light感光灵敏度(Sensitivity [ˌsɛnsɪˈtɪvɪti])boost推进[bust]lag behind落后于Hyperopic – far-sighted 远视Dynamic Range 动态范围(Dynamic[daiˈnæmik])critical fusion frequency 临界融合频率(critical[ˈkrɪtɪkəl])fusionˈfjuʒən]CFF临界闪变频率visual sensation视觉Chromaticity Diagram色度图 Chromaticity[ˌkroməˈtɪsɪti]Color Temperature色温HSV Model色彩模型(hue色度[hju]saturation饱和度value纯度CIE Model 相干红外能量模式Complementary Colors补色Bar Pattern条状图形Heat body 热稠化approximate近似violet紫罗兰Body Curve人体曲线Color Gamut色阶adjacent邻近的normal illumination法线照明Primary colors红黄蓝三原色Color saturation色饱和度Color Triangle颜色三角Color Notation颜色数标法Color Difference色差TV Signal Processing电视信号处理Gamma Correction图像灰度校正Conversion Tables换算表out of balance失衡wobble摇晃back and forth前后clear (white) panel白光板vibrant震动fuzzy失真quantum leap量子越迁SVGA (800x600)derive from起源自culprit犯人render呈递inhibit抑制,约束stride大幅前进blemish污点obstruction障碍物scratch刮伤substance物质实质主旨residue杂质criteria标准parameter参数adjacent邻近的接近的asynchrony异步cluster串群mutually互助得algorithm运算法则Chromatic Aberrations色差Fovea小凹Visual Acuity视觉灵敏度Contrast Sensitivity对比灵敏度Temporal (time) Response反应时间rendition表演,翻译animation活泼又生气ghost重影Parallax视差deficient缺乏的不足的Display panel显示板NG.( Narrow Gauge)窄轨距dichroic mirror二色性的双色性的Brewster Angle布鲁斯特角Polarized Light极化光Internal reflection内反射Birefringence 双折射Extinction Ratio 消光系数Misalignment 未对准Quarter Waveplates四分之一波片blemish污点瑕疵Geometric几何学的ripple波纹capacitor电容器parallel平行的他tantalum钽(金属元素)exsiccate使干燥exsiccate油管,软膏furnace炉子镕炉electrolytic电解的,由电解产生的module模数analog类似物out of the way不恰当pincushion针垫拉lateral侧面得rectangle长方形fixture固定设备control kit工具箱DVIconnector DVI数局线Vertical垂直的horizontal 水平的interlace隔行扫描mullion竖框直楞sawtooth锯齿[ˈsɔtuθ]toggle套索钉keypad数字按键键盘tangential切线diagnostic tool诊断工具sagittal direction径向的sagittal[ˈsædʒɪtl]cursor position光标位置3Yw'/#p3`ray aberration光线相差weighting factor权种因子variables变量for now暂时,目前.眼下check box复选框Airy disk艾里斑exit pupil出[射光]瞳optical path difference光称差with respect to关于diffraction limited衍射极限wavefront aberration波阵面相差spherical aberration球面象差paraxial focus傍轴焦点chromatic aberration象差local coordinate system局部坐标系统coordinate system坐标系orthogonal直角得,正交的conic sections圆锥截面account for解决,得分parabolic reflector拋物面反射镜radius of curvature曲率半径spherical mirror球面镜geometrical aberration几何相差incident radiation入射辐射global coordinate总体坐标in terms of根据按照reflected beam反射束FYI=for your information供参考Constructive interference相长干涉phase difference相差achromatic singlet消色差透镜Interferometer干涉仪boundary constraint边界约束,池壁效radii半径Zoom lenses变焦透镜Beam splitters分束器discrete不连续的,分离的objective/eye lens物镜/目镜mainframe主机rudimentary根本的,未发展的photographic照相得摄影得taxing繁重的,费力得algebra代数学trigonometry三角学geometry几何学calculus微积分学philosophy哲学lagrange invariant拉格朗日不变量spherical球的field information场信息Standard Lens标准透镜Refracting Surface折射面astigmatism散光HDTV高清晰度电视DLV ( Digital Light Valve)数码光路真空管,简称数字光阀diffraction grating衍射光珊field angle张角paraxial ray trace equations近轴光线轨迹方称back focal length后焦距principal plane主平面vertex顶点,最高点astigmatism散光,因偏差而造成的曲解或错判medial中间的,平均的variance不一致conic圆锥的,二次曲线field of view视野collimator瞄准仪convolution回旋.盘旋,卷积fuzzy失真,模糊aberrated异常的[ˈæbəˌretɪd]asymmetry不对称得[eˈsɪmɪtri]indicative可表示得[ɪnˈdɪkətɪv]parabolic拋物线得[ˌpærəˈbɑlɪk]suffice足够,使满足specification规格,说明书[ˌspɛsəfɪˈkeʃən]straightforward易懂的,直接了当的[stretˈfɔrwəd],solidify凝固,巩固.Constraints 约束,限制metrology度量衡field coverage视场,视野dictate口述, 口授, 使听写, 指令, 指示, 命令, 规定irradiance发光, 光辉,辐照度aerial空气得,空中得halide卤化物的monochromatic单色的,单频的polychromatic多色的aspherical非球面的spherical球面的alignment列队,结盟power(透镜)放大率equiconvergence 同等收敛EFL(effective focal length)有效焦距workhorse广为应用的设备biconvex两面凸的global optimization整体最优化concave凹得,凹面得cylindrical圆柱得solid model实体模型Modulation Transfer Function调制传递函数in the heat of在最激烈的时候protocol协议,规定triplet三重态sanity心智健全zinc锌,涂锌的selenide 硒化物,硒醚miscellaneous各色各样混在一起, 混杂的, 多才多艺的versus与...相对polynomial多项式的coefficient系数explicit function显函数" wYgi%distinct清楚的,截然不同的emanate散发, 发出, 发源rudimentary根本的,未发展的intersection角差点PRTE=paraxial ray trace equation旁轴光线轨迹方程achromats 消色差透镜cardinal points基本方位separations分色dashed虚线blow up放大overlay覆盖,覆盖图multiplayer 多层的humidity 湿度float glass浮法玻璃square one 出发点,端点square up to 准备开打,坚决地面对reflecting telescope 反射式望远镜diagnostic tools诊断工具Layout plots规划图Modulation transfer function调制转换功能FFT快速傅里叶变换Point spread function点传播功能wavelength波长angle角度absorption吸收system aperture系统孔径lens units透镜单位wavelength range波长范围singlet lens单业透镜spectrum光谱diffraction grating衍射光栅asphere半球的LDE=Lens data editor Surface radius of curvature表面曲率半径surface thickness表面厚度material type材料种类semi-diameter半径focal length焦距aperture type孔径类型aperture value孔径值field of view视场microns微米F, d, and C= blue hydrogen, yellow helium, red hydrogen lines, primary wavelength主波长sequential mode连续模式object surface物表面The front surface of the lens透镜的前表面stop光阑The back surface of the lens透镜的后表面The image surface像表面symmetric相对称的biconvex两面凸的The curvature is positive if the center of curvature of the surface is to the right of the vertex. It is negative if the center of curvature is to the left of the vertex.如果曲率中心在最高点的右边,曲率值为正,如果曲率中心在最高点的左边,则曲率为负image plane像平面Ray Aberration光线相差tangential direction切线方向sagittal direction径向paraxial focus旁轴的Marginal边缘的spherical aberration球面像差Optimization Setup最优化调整variable变量mathematical sense数学角度MFE= Merit Function Editor, Adding constraints增加约束focal length焦矩长度operand操作数the effective focal length有效焦矩primary wavelength主波长initiate开始spot diagram位图表Airy disk艾里斑axial chromatic aberration轴向色差with respect to关于至于exit pupil出射光瞳OPD=optical path difference光学路径差diffraction limited衍射极限chromatic aberration色差chromatic focal shift色焦距变换paraxial focus傍轴焦点axial spherical aberration轴向球差(longitudinal spherical aberration 纵向球差:沿光轴方向度量的球差) lateral spherical aberration垂轴球差(在过近轴光线像点A‵的垂轴平面内度量的球差)coma、comatic aberration彗差meridional coma子午彗差sagittal coma弧矢彗差astigmatism像散local coordinate system本地坐标系统meridional curvature of field子午场曲sagittal curvature of field弧矢场曲decentered lens偏轴透镜orthogonal直角的垂直的conic section圆锥截面account for说明,占有,得分stigmatic optical system无散光的光学系统Newtonian telescope牛顿望远镜parabolic reflector抛物面镜foci焦距chromatic aberration,色差superpose重迭parabola抛物线spherical mirror球面镜RMS=Root Mean Square均方根wavefront波阵面spot size光点直径Gaussian quadrature高斯积分rectangular array矩阵列grid size磨粒度PSF=Point Spread Function点扩散函数FFT=Fast Fourier Transform Algorithm快速傅里叶变换Cross Section横截面Obscurations昏暗local coordinates局部坐标系统vignette把…印为虚光照Arrow key键盘上的箭头键refractive折射reflective反射in phase同相的协调的Ray tracing光线追迹diffraction principles衍射原理order effect式样提出的顺序效果energy distribution能量分配Constructive interference相长干涉dispersive色散的Binary optics二元光学phase advance相位提前achromatic single消色差单透镜diffractive parameter衍射参数Zoom lenses变焦透镜Athermalized lenses绝热透镜Interferometers干涉计Beam splitter分束器Switchable component systems可开关组件系统common application通用symmetry对称boundary constraint边界约束multi-configuration (MC) MC Editor (MCE) perturbation动乱,动摇index accuracy折射率准确性index homogeneity折射率同种性index distribution折射率分配abbe number离差数Residual剩余的Establishing tolerances建立容差figure of merit质量因子tolerance criteria公差标准Modulation Transfer Function (MTF)调制传递函数boresight视轴,瞄准线Monte Carlo蒙特卡洛Tolerance operands误差操作数conic constant ]MC1"{_qT 圆锥常数astigmatic aberration像散误差Mechanical tilt机械倾斜,机械倾角Tolerance Data Editor (TDE)公差资料编辑器compensator补偿棱镜estimated system performance预估了的系统性能iteratively反复的,重迭的statistical dependence统计相关性sequential ray trace model连续光线追迹模型imbed埋葬,埋入multiple多样的,多重的,若干的Non-Sequential Components不连续的组件Corner cube角隅棱镜,三面直角透镜Sensitivity Analysis灵敏度分析Faceted reflector有小面的反射镜emit发射,发出nest嵌套overlap交迭outer lens外透镜brute force强力seidel像差系数aspect ratio长宽比MRA边缘光线角MRH边缘光线高度asynchronous不同时的,异步Apodization factor变迹因子hexapolar六角形dithered高频脉冲衍射调制传递函数(DMTF),衍射实部传递函数(DRTF),衍射虚部传递函数(DITF),衍射相位传递函数(DPTF),方波传递函数(DSWM)logarithmic对数的parity奇偶% Uc,I e longitudinal aberrations 纵向像差赛得系数:球差(SPHA,SI)彗差(COMA,S2),像散(ASTI,S3),场曲(FCUR,S4),畸变(DIST,S5),轴向色差(CLA,CL)和横向色差(CTR,CT).横向像差系数:横向球差(TSPH),横向弧矢彗差(TSCO),横向子午彗差(TTCO),横向弧矢场曲(TSFC),横向子午场曲(TTFC),横向畸变(TDIS)横向轴上色差(TLAC)。

迈克尔逊干涉仪翻译

迈克尔逊干涉仪翻译

Mach–Zehnder interferometerIn physics, the Mach–Zehnder interferometer is a device used to determine the relative phase shift variations between two collimated beams derived by splitting light from a single source. The interferometer has been used, among other things, to measure phase shifts between the two beams caused by a sample or a change in length of one of the paths. The apparatus is named after the physicists Ludwig Mach (the son of Ernst Mach) and Ludwig Zehnder: Zehnder's proposal in an 1891 article[1] was refined by Mach in an 1892 article.[2]IntroductionThe Mach–Zehnder interferometer is a highly configurable instrument. In contrast to the well-known Michelson interferometer, each of the well-separated light paths is traversed only once.If it is decided to produce fringes in white light, then, since white light has a limited coherence length, on the order of micrometers, great care must be taken to simultaneously equalize the optical paths over all wavelengths or no fringes will be visible. As seen in Fig. 1, a compensating cell made of the same type of glass as the test cell (so as to have equal optical dispersion) would be placed in the path of the reference beam to match the test cell. Note also the precise orientation of the beam splitters. The reflecting surfaces of the beam splitters would be oriented so that the test and reference beams pass through an equal amount of glass. In this orientation, the test and reference beams each experience two front-surface reflections, resulting in the same number of phase inversions. The result is that light traveling an equal optical path length in the test and reference beams produces a white light fringe of constructive interference.[3][4]Figure 2. Localized fringes result when an extended source is used in a 迈克尔逊interferometer. By appropriately adjusting the mirrors and beam splitters, the fringes can be localized in any desired plane.Collimated sources result in a nonlocalized fringe pattern. Localized fringes result when an extended source is used. In Fig. 2, we see that the fringes can be adjusted so that they are localized in any desired plane.[5]:18 In most cases, the fringes would be adjusted to lie in the same plane as the test object, so that fringes and test object can be photographed together.The Mach–Zehnder interferometer's relatively large and freely accessible working space, and its flexibility in locating the fringes has made it the interferometer of choice for visualizing flow in wind tunnels[6][7] and for flow visualization studies in general. It is frequently used in the fields of aerodynamics, plasma physics and heat transfer to measure pressure, density, and temperature changes in gases.[5]:18,93–95Mach–Zehnder interferometers are used in electro-optic modulators, electronic devices used in various fibre-optic communications applications. 迈克尔逊modulators are incorporated in monolithic integrated circuits and offer well-behaved, high-bandwidth electro-optic amplitude and phase responses over a multiple GHz frequency range.Mach–Zehnder interferometers are also used to study one of the most counterintuitive predictions of quantum mechanics, the phenomenon known as quantum entanglement.[8][9]The possibility to easily control the features of the light in the reference channel without disturbing the light in the object channel popularized the Mach–Zehnder configuration in holographic interferometry. In particular, optical heterodyne detection with an off-axis, frequency-shifted reference beam ensures good experimental conditions for shot-noise limited holography with video-rate cameras,[10] vibrometry,[11] and laser Doppler imaging of blood flow.[12]How it worksSet-upA collimated beam is split by a half-silvered mirror. The two resulting beams (the "sample beam" and the "reference beam") are each reflected by a mirror. The two beams then pass a second half-silvered mirror and enter two detectors.PropertiesThe Fresnel equations for reflection and transmission of a wave at a dielectric imply that there is a phase change for a reflection when a wave reflects off a change from low to high refractive index but not when it reflects off a change from high to low.A 180 degree phase shift occurs upon reflection from the front of a mirror, since the medium behind the mirror (glass) has a higher refractive index than the medium the light is traveling in (air). No phase shift accompanies a rear surface reflection, since the medium behind the mirror (air) has a lower refractive index than the medium the light is traveling in (glass).Figure 3.Effect of a sample on the phase of the output beams in a Mach–Zehnder interferometer. The speed of light is slower in media with an index of refraction greater than that of a vacuum, which is 1. Specifically, its speed is: v = c/n, where c is the speed of light in vacuum and n is the index of refraction. This causes a phase shift increase proportional to (n − 1) × length traveled. If k is the constant phase shift incurred by passing through a glass plate on which a mirror resides, a total of 2k phase shift occurs when reflecting off the rear of a mirror. This is because light traveling toward the rear of a mirror will enter the glass plate, incurring k phase shift, and then reflect off the mirror with no additional phase shift since only air is now behind the mirror, and travel again back through the glass plate incurring an additional k phase shift.The rule about phase shifts applies to beamsplitters constructed with a dielectric coating, and must be modified if a metallic coating is used, or when different polarizations are taken into account. Also, in real interferometers, the thicknesses of the beamsplitters may differ, and the path lengths are not necessarily equal. Regardless, in the absence of absorption, conservation of energy guarantees that the two paths must differ by a half wavelength phase shift. Also note thatbeamsplitters that are not 50/50 are frequently employed to improve the interferometer's performance in certain types of measurement.[3]Observing the effect of a sampleIn Fig. 3, in the absence of a sample, both the sample beam SB and the reference beam RB will arrive in phase at detector 1, yielding constructive interference. Both SB and RB will have undergone a phase shift of (1×wavelength + k) due to two front-surface reflections and one transmission through a glass plate.At detector 2, in the absence of a sample, the sample beam and reference beam will arrive with a phase difference of half a wavelength, yielding complete destructive interference. The RB arriving at detector 2 will have undergone a phase shift of (0.5×wavelength + 2k) due to one front-surface reflection and two transmissions. The SB arriving at detector 2 will have undergone a (1×wavelength + 2k) phase shift due to two front-surface reflections and one rear-surface reflection. Therefore, when there is no sample, only detector 1 receives light.If a sample is placed in the path of the sample beam, the intensities of the beams entering the two detectors will change, allowing the calculation of the phase shift caused by the sample.ApplicationsThe versatility of the Mach–Zehnder configuration has led to its being used in a wide range of fundamental research topics in quantum mechanics, including studies on counterfactual definiteness, quantum entanglement, quantum computation, quantum cryptography, quantum logic, Elitzur-Vaidman bomb tester, the quantum eraser experiment, the quantum Zeno effect, and neutron diffraction. In optical telecommunications it is used as an electro-optic modulator for phase as well as amplitude modulation of light.迈克尔逊干涉仪在物理学中,迈克尔逊干涉仪是用于确定通过分离来自单个光源的光而得到的两个准直光束之间的相对相移变化的装置。

光场强度分布对鬼成像成像质量的影响

光场强度分布对鬼成像成像质量的影响

光场强度分布对鬼成像成像质量的影响王志峰;姚治海;高超;王晓茜【摘要】鬼成像的优越性使其应用前景非常广泛,而其成像质量是决定鬼成像实用化的重要因素之一.在鬼成像系统中,光源性质是影响鬼成像成像质量的重要因素.通过数值模拟与实验,验证了光场的空间结构的分布与一阶统计分布对鬼成像的成像质量的影响.并通过对比度和衬噪比这两个指标来衡量鬼成像的成像质量,发现光场的一阶统计性质对成像质量的影响尤为明显.将光场的统计分布调制为均匀分布时,能够显著提高了图像的对比度和衬噪比,因此可以只通过调节光场的一阶统计分布而提高鬼成像的成像质量.%The superiority of ghost imaging makes its application prospect very broad;and the image quality is one of the important factors to determine the practical application of ghost imaging. Through the numerical simulation and ex-periment,the distribution of the spatial structure of the light field and the influence of the first-order statistical distribu-tion on the imaging quality of the ghost imaging are verified. The influence of the first-order statistical properties of the optical field on the image quality is especially obvious according to the visibility and CNR of the image. When the statistical distribution of the light field is modulated into a uniform distribution,the visibility and CNR of the image can be improved obviously;so that the image quality of the ghost imaging can be improved only by adjusting the first-order statistical distribution of the light field.【期刊名称】《长春理工大学学报(自然科学版)》【年(卷),期】2018(041)001【总页数】5页(P22-25,29)【关键词】鬼成像;空间分布;统计分布;成像质量【作者】王志峰;姚治海;高超;王晓茜【作者单位】长春理工大学理学院,长春130022;长春理工大学理学院,长春130022;长春理工大学理学院,长春130022;长春理工大学理学院,长春130022【正文语种】中文【中图分类】O438鬼成像,又称为关联成像,是近些年兴起的新型成像技术[1-4]。

光电信息专业英语单词句子中英翻译

光电信息专业英语单词句子中英翻译

词汇Ray Optics射线光学Refraction 折射Reflection 反射Index of Refraction 折射率Optical spectrum 光谱Dispersion 色散lens 透镜Total Internal Reflection全内反射Prisms棱镜right isosceles triangles正等腰三角形Spherical refracting surface 球面折射面sign convention符号法则paraxial approximation近轴近似aberration像差chromatic aberration色差collimated平行的;使平行critical angle临界角defect缺点,缺陷incident入射的inclination倾斜角;偏向magnitude数量级virtual image 虚像Diffraction 衍射Interference 干涉aperture 孔径complex exponential function复指数函数complex conjugate复共轭monochromatic单色的optical path difference 光程差polarization 偏振resonator谐振器resolution分辨率Holography 全息术wavelength 波长microscope 显微镜beam splitter 分束器Rainbow holography彩虹全息术Volume holograms 体全息图Computer-generated holography 计算机全息术Spatial Filtering空间滤波gratings光栅harmonics interferogram谐波干涉图pupil function 光瞳函数principal maxima 主极大值Mode Locking 波模锁定;振荡型同步Transverse modes 横向模式Laser rangefinder激光测距仪navigation 导航Photodetector光电检测器photomultiplier光电倍增管Photon 光子Optical Fiber Communication 光纤通信fiber 纤维Optical Loss 光学损失Group集体velocity 速度nonlinearity非线性anomalous-dispersion反常色散Stimulated Raman Scattering 受激拉曼散射Self-Phase Modulation 相位调制效应Cross-Phase Modulation 交叉相位调制bandwidth 带宽optical switches光开关Photodetectors光电探测器crystal 晶体Birefringence 双折射electron 电子Mechanical and thermal strength 机械和热强度surface 表面Bandgap 能带carrier concentration 载体浓度discharge 放电photovoltaic 光伏Optical Thin Film Technology光学薄膜技术Photolithography 光刻, biophotonics生物光子学,3D Display Technology 3 d显示技术,Infrared Detection Technology红外探测技术exposure 曝光irradiation 辐照nanoparticle纳米颗粒句子We treat light beams as rays that propagate along straight lines, except at interfaces between dissimilar materials, where the rays may be bent or refracted. This approach, which had been assumed to be completely accurate before the discovery of the wave nature of light, leads to a great many useful results regarding lens optics and optical instruments.我们将光束处理为沿着直线传播的光线,除了在不同材料之间的界面处,其中光线可以被弯曲或折射。

光学术语中英文对照

光学术语中英文对照

透镜系列术语中英文对照单透镜Simple (Single) Lenses球透镜Ball Lenses歪像透镜Anamorphic Lenses圆锥透镜Conical Lenses柱状透镜,环形透镜Cylindrical & Toroidal Lenses非球面透镜Aspheric Lenses反射折射透镜Catadioptric Lenses绕射极限透镜Diffraction-Limited LensesGRIN透镜GRIN Lenses (Graduated Refractive Index Rod)微小透镜阵列Micro Lens Arrays准直透镜Collimator Lenses聚光透镜Condenser Lenses多影像透镜Multiple Image Lenses傅利叶透镜Fourier Lenses菲涅尔透镜Fresnel Lenses替续透镜Relay Lenses大口径透镜(直径150mm以上) Large Aperture Lenses (150mm) 复合透镜Complex Lenses红外线透镜Infrared Lenses紫外线透镜Ultraviolet Lenses激光透镜Laser Lenses望远镜对物镜Telescope Objectives Lenses显微镜对物镜Microscope Objectives Lenses接目镜Eyepieces Lenses向场透镜Field Lenses望远镜头Telephoto Lenses广角镜头Wide Angle Lenses可变焦伸缩镜头Variable Focal Length Zoom LensesCCTV镜头CCTV Lenses影印机镜头Copy Machine Lenses传真机镜头Facsimile Lenses条码扫描器镜头Bar Code Scanner Lenses影像扫描器镜头Image Scanner Lenses光碟机读取头透镜Pick-up Head LensesAPS相机镜头APS Camera Lenses数位相机镜头Digital Still Camera Lenses液晶投影机镜头Liquid Crystal Projector Lenses镜面系列术语中英文对照平面镜Flat Mirrors球面凹面镜,球面凸面镜Spherical Concave and Convex Mirrors 抛物面镜,椭圆面镜Off-Axis Paraboloids and Ellipsoids Mirrors 非球面镜Aspheric Mirrors多面镜Polygonal Mirrors热镜Hot Mirrors冷镜Cold Mirrors玻璃,玻璃/瓷面镜Glass and Glass-Ceramic Mirrors双色向面镜Dichroic Mirror金属面镜Metal Mirrors多层面镜Multilayer Mirrors半涂银面镜Half-Silvered Mirrors激光面镜Laser Mirrors天文用面镜Astronomical Mirrors棱镜系列术语中英文对照Nicol棱镜Nicol PrismsGlan-Thomson棱镜Glan-Thomson PrismsWollaston棱镜Wollaston PrismsRochon棱镜Rochon Prisms直角棱镜Right-Angle; Rectangular Prisms五面棱镜Pentagonal Prisms脊角棱镜Roof Prisms双棱镜Biprisms直视棱镜Direct Vision Prisms微小棱镜Micro Prisms滤光镜系列术语中英文对照尖锐滤光镜Sharp Cut (off) Filters色温变换滤光镜,日光滤光镜Colour Conversion/Daylight Filters 干涉滤光镜Interference Filters中性密度滤光镜Neutral Density Filters空间/光学匹配滤光镜Spatial/Optical Matched Filters双色向滤光镜Dichroic Filters偏光滤光镜Polarizing Filters排除频带滤光镜Rejection Band Filters可调式滤光镜Turnable Filter超窄频滤光镜Ultra Narrowband Filters色吸收滤光镜Absorption Filters红外吸收/反射滤光镜Infrared Absorbing/Reflecting Filters红外透过滤光镜Infrared Transmitting Filters紫外吸收滤光镜Ultraviolet Absorbing Filters紫外透过滤光镜Ultraviolet Transmitting Filters针孔滤光镜Pinhole Filters有色玻璃滤光镜Colored-Glass Filters塑胶滤光镜Plastic Filters 照像用滤光镜Photographic Filters全像滤光镜Holographic Filters微小干涉滤光镜Micro Interference Filters光学词汇Iris – aperture stop虹膜孔径光珊retina视网膜Color Blind 色盲weak color 色弱Myopia – near-sighted 近视Sensitivity to Light感光灵敏度boost推进lag behind落后于Hyperopic – far-sighted 远视Dynamic Range 动态围critical fusion frequency 临界融合频率CFF临界闪变频率visual sensation视觉Chromaticity Diagram色度图Color Temperature色温HSV Model色彩模型(hue色度saturation饱和度value纯度CIE Model 相干红外能量模式Complementary Colors补色Bar Pattern条状图形Heat body 热稠化approximate近似violet紫罗兰Body Curve人体曲线Color Gamut色阶adjacent邻近的normal illumination法线照明Primary colors红黄蓝三原色Color saturation色饱和度Color Triangle颜色三角Color Notation颜色数标法Color Difference色差TV Signal Processing电视信号处理Gamma Correction图像灰度校正Conversion Tables换算表out of balance失衡wobble摇晃back and forth前后clear (white) panel白光板vibrant震动fuzzy失真quantum leap量子越迁SVGA (800x600)derive from起源自culprit犯人render呈递inhibit抑制,约束stride大幅前进blemish污点obstruction障碍物scratch刮伤substance物质实质主旨residue杂质criteria标准parameter参数adjacent邻近的接近的asynchrony异步cluster串群mutually互助得algorithm运算法则Chromatic Aberrations色差Fovea小凹Visual Acuity视觉灵敏度Contrast Sensitivity对比灵敏度Temporal (time) Response反应时间rendition表演,翻译animation活泼又生气ghost重影Parallax视差deficient缺乏的不足的Display panel显示板NG.( Narrow Gauge)窄轨距dichroic mirror二色性的双色性的Brewster Angle布鲁斯特角Polarized Light极化光Internal reflection反射Birefringence 双折射Extinction Ratio 消光系数Misalignment 未对准Quarter Waveplates四分之一波片blemish污点瑕疵Geometric几何学的ripple波纹capacitor电容器parallel平行的他tantalum钽(金属元素) exsiccate使干燥exsiccate油管,软膏furnace炉子镕炉electrolytic电解的,由电解产生的module模数analog类似物out of the way不恰当pincushion针垫拉lateral侧面得rectangle长方形fixture固定设备control kit工具箱DVI connector DVI数局线Vertical垂直的horizontal 水平的interlace隔行扫描mullion竖框直楞sawtooth锯齿toggle套索钉keypad数字按键键盘tangential切线diagnostic tool诊断工具sagittal direction径向的cursor position光标位置ray aberration光线相差weighting factor权种因子variables变量for now暂时,目前.眼下check box复选框Airy disk艾里斑exit pupil出[射光]瞳optical path difference光称差with respect to关于diffraction limited衍射极限wavefront aberration波阵面相差spherical aberration球面象差paraxial focus傍轴焦点chromatic aberration象差local coordinate system局部坐标系统coordinate system坐标系orthogonal直角得,正交的conic sections圆锥截面account for解决,得分parabolic reflector拋物面反射镜radius of curvature曲率半径spherical mirror球面镜geometrical aberration几何相差incident radiation入射辐射global coordinate总体坐标in terms of根据按照reflected beam反射束FYI=for your information供参考Constructive interference相长干涉phase difference相差achromatic singlet消色差透镜Interferometer干涉仪boundary constraint边界约束,池壁效应radii半径Zoom lenses变焦透镜Beam splitters分束器discrete不连续的,分离的objective/eye lens物镜/目镜mainframe主机rudimentary根本的,未发展的photographic照相得摄影得taxing繁重的,费力得algebra代数学trigonometry三角学geometry几何学calculus微积分学philosophy哲学lagrange invariant拉格朗日不变量spherical球的field information场信息Standard Lens标准透镜Refracting Surface折射面astigmatism散光HDTV高清晰度电视DLV ( Digital Light Valve)数码光路真空管,简称数字光阀diffraction grating衍射光珊field angle角paraxial ray trace equations近轴光线轨迹方称back focal length后焦距principal plane主平面vertex顶点,最高点astigmatism散光,因偏差而造成的曲解或错判medial中间的,平均的variance不一致conic圆锥的,二次曲线field of view视野collimator瞄准仪convolution回旋.盘旋,卷积fuzzy失真,模糊aberrated异常的asymmetry不对称得indicative可表示得parabolic拋物线得suffice足够,使满足specification规格,说明书straightforward易懂的,直接了当的solidify凝固,巩固.Constraints 约束,限制metrology度量衡field coverage视场,视野dictate口述, 口授, 使听写, 指令, 指示, 命令, 规定irradiance发光, 光辉,辐照度aerial空气得,空中得halide卤化物的monochromatic单色的,单频的polychromatic多色的aspherical非球面的spherical球面的alignment列队,结盟power(透镜)放大率equiconvergence 同等收敛EFL(effective focal length)有效焦距workhorse广为应用的设备biconvex两面凸的global optimization整体最优化concave凹得,凹面得cylindrical圆柱得solid model实体模型Modulation Transfer Function调制传递函数in the heat of在最激烈的时候protocol协议,规定triplet三重态sanity心智健全zinc锌,涂锌的selenide 硒化物,硒醚miscellaneous各色各样混在一起, 混杂的, 多才多艺的versus与...相对polynomial多项式的coefficient系数explicit function显函数distinct清楚的,截然不同的emanate散发, 发出, 发源rudimentary根本的,未发展的intersection角差点PRTE=paraxial ray trace equation旁轴光线轨迹方程achromats 消色差透镜cardinal points基本方位separations分色片dashed虚线blow up 放大overlay覆盖,覆盖图multiplayer 多层的humidity 湿度float glass 浮法玻璃square one 出发点,端点square up to 准备开打,坚决地面对reflecting telescope 反射式望远镜diagnostic tools诊断工具Layout plots规划图Modulation transfer function调制转换功能FFT快速傅里叶变换Point spread function点传播功能wavelength波长angle角度absorption吸收system aperture系统孔径lens units透镜单位wavelength range波长围singlet lens单业透镜spectrum光谱diffraction grating衍射光栅asphere半球的LDE=Lens data editor Surface radius of curvature表面曲率半径surface thickness表面厚度material type材料种类semi-diameter半径focal length焦距aperture type孔径类型aperture value孔径值field of view视场microns微米F, d, and C= blue hydrogen, yellow helium, red hydrogen lines, primary wavelength主波长sequential mode连续模式object surface物表面The front surface of the lens透镜的前表面stop光阑The back surface of the lens透镜的后表面The image surface像表面symmetric相对称的biconvex两面凸的The curvature is positive if the center of curvature of the surface is to the right of the vertex. It is negative if the center of curvature is to the left of the vertex.如果曲率中心在最高点的右边,曲率值为正,如果曲率中心在最高点的左边,则曲率为负image plane像平面Ray Aberration光线相差tangential direction切线方向sagittal direction径向paraxial focus旁轴的Marginal 边缘的spherical aberration球面像差Optimization Setup最优化调整variable变量mathematical sense数学角度MFE= Merit Function Editor, Adding constraints增加约束focal length焦矩长度operand操作数theeffective focal length有效焦矩primary wavelength主波长initiate开始spot diagram位图表Airy disk艾里斑axial chromatic aberration轴向色差with respect to关于至于exit pupil出射光瞳OPD=optical path difference 光学路径差diffraction limited衍射极限chromatic aberration色差chromatic focal shift色焦距变换paraxial focus傍轴焦点axial spherical aberration轴向球差(longitudinal spherical aberration 纵向球差:沿光轴方向度量的球差)lateral spherical aberration垂轴球差(在过近轴光线像点A‵的垂轴平面度量的球差)coma、comatic aberration彗差meridional coma子午彗差sagittal coma弧矢彗差astigmatism像散local coordinate system本地坐标系统meridional curvature of field子午场曲sagittal curvature of field弧矢场曲decentered lens偏轴透镜orthogonal直角的垂直的conic section圆锥截面account for说明,占有,得分stigmatic optical system无散光的光学系统Newtonian telescope牛顿望远镜parabolic reflector抛物面镜foci焦距chromatic aberration,色差superpose重迭parabola抛物线spherical mirror球面镜RMS=Root Mean Square均方根wavefront波阵面spot size光点直径Gaussian quadrature 高斯积分rectangular array矩阵列grid size磨粒度PSF=Point Spread Function点扩散函数FFT=Fast Fourier Transform Algorithm快速傅里叶变换Cross Section横截面Obscurations昏暗local coordinates局部坐标系统vignette把…印为虚光照Arrow key键盘上的箭头键refractive折射reflective反射in phase同相的协调的Ray tracing光线追迹diffraction principles衍射原理order effect式样提出的顺序效果energy distribution 能量分配Constructive interference相长干涉dispersive色散的Binary optics二元光学phase advance相位提前achromatic single消色差单透镜diffractive parameter衍射参数Zoom lenses变焦透镜Athermalized lenses绝热透镜Interferometers干涉计Beam splitter分束器Switchable component systems可开关组件系统common application通用symmetry 对称boundary constraint边界约束multi-configuration (MC) MC Editor (MCE) perturbation动乱,动摇index accuracy折射率准确性index homogeneity折射率同种性index distribution折射率分配abbe number 离差数Residual剩余的Establishing tolerances建立容差figure of merit 质量因子tolerance criteria公差标准Modulation Transfer Function (MTF)调制传递函数boresight视轴,瞄准线Monte Carlo蒙特卡洛Tolerance operands误差操作数conic constant ]MC1"{_qT .ueg g圆锥常数astigmatic aberration像散误差Mechanical tilt机械倾斜,机械倾角Tolerance Data Editor (TDE)公差资料编辑器compensator补偿棱镜estimated system performance预估了的系统性能iteratively反复的,重迭的statistical dependence统计相关性sequential ray trace model连续光线追迹模型imbed埋葬,埋入multiple多样的,多重的,若干的Non-Sequential Components不连续的组件Corner cube角隅棱镜,三面直角透镜Sensitivity Analysis灵敏度分析Faceted reflector有小面的反射镜emit发射,发出nest嵌套overlap交迭outer lens外透镜brute force 强力seidel像差系数aspect ratio长宽比MRA边缘光线角MRH边缘光线高度asynchronous不同时的,异步Apodization factor变迹因子hexapolar六角形dithered高频脉冲衍射调制传递函数(DMTF),衍射实部传递函数(DRTF),衍射虚部传递函数(DITF),衍射相位传递函数(DPTF),方波传递函数(DSWM)logarithmic对数的parity奇偶% Uc,I e ,17]3NnoClongitudinal aberrations 纵向像差赛得系数: 球差(SPHA,SI),彗差(COMA,S2),像散(ASTI,S3),场曲(FCUR,S4),畸变(DIST,S5),轴向色差(CLA,CL)和横向色差(CTR,CT).横向像差系数:横向球差(TSPH),横向弧矢彗差(TSCO),横向子午彗差(TTCO),横向弧矢场曲(TSFC),横向子午场曲(TTFC),横向畸变(TDIS)横向轴上色差(TLAC)。

光的原理科普英语作文600字

光的原理科普英语作文600字

光的原理科普英语作文600字## The Nature of Light: A Comprehensive Exploration.Light, an ever-present and indispensable force in our world, holds an enigmatic allure that has captivated scientists and philosophers alike for centuries. Its intricate nature and far-reaching implications have fueled countless investigations, leading to a profound understanding of its fundamental properties.Electromagnetic Radiation: Unveiling Light's True Form.Light belongs to the vast spectrum of electromagnetic radiation, a continuum of waves that propagate through space and matter. These waves, characterized by their wavelength and frequency, encompass a wide range from radio waves to gamma rays. Light falls within the visible spectrum, perceived by the human eye as vibrant hues.Wave-Particle Duality: A Paradox Unveiled.The nature of light poses a unique paradox. It exhibits both wave-like and particle-like properties, a duality that has been a subject of intense scientific debate. As a wave, light demonstrates interference and diffraction patterns, reminiscent of ripples in a pond. However, when interacting with matter, it behaves as a stream of discrete particles called photons.Light and Matter: A Symphony of Interactions.Light's interaction with matter is a complex and dynamic process. When light strikes an object, it can be absorbed, reflected, refracted, or scattered. Absorption occurs when light energy is transferred to the object, leading to a rise in temperature or the excitation of electrons. Reflection occurs when light bounces off a surface, preserving its direction and obeying the laws of specular reflection. Refraction, on the other hand, involves the bending of light as it passes from one medium to another, such as from air to glass. Scattering occurs when light encounters irregularities in the medium,redirecting its path in various directions.Light and Vision: Illuminating the World.The human eye, a remarkable sensory organ, has evolved to perceive light and convert it into visual information. When light enters the eye, it is focused onto the retina, where specialized cells called photoreceptors detect its presence and intensity. Different types of photoreceptors respond to specific wavelengths of light, enabling us to perceive color and contrast.Applications of Light: Shaping Our World.The practical applications of light are virtually endless. From its use in illumination to its role inoptical devices and telecommunications, light has played a pivotal role in shaping human society. Artificial light sources, such as incandescent bulbs and LEDs, extend our ability to work and engage in activities beyond the constraints of daylight hours. Optical fibers transmit vast amounts of data at lightning speeds, powering the internetand modern communication networks. Lasers, highly focused and coherent beams of light, have revolutionized manufacturing, medicine, and research.Conclusion.Light, a fundamental aspect of our universe, is a multifaceted phenomenon that continues to fascinate and inspire. Its wave-particle duality, its interactions with matter, and its myriad applications have shaped our understanding of the world and empowered us to harness its potential for the betterment of humanity. The study of light remains an ongoing endeavor, with new discoveries constantly expanding our knowledge and opening up new avenues of exploration.。

如何探究科学奥秘英语作文关于光的

如何探究科学奥秘英语作文关于光的

如何探究科学奥秘英语作文关于光的英文回答:Light, an enigmatic force that permeates our universe, has long captivated scientists and philosophers alike. Its elusive nature and its profound implications for our understanding of the cosmos have propelled countless expeditions into its enigmatic realm.One of the earliest and most foundational explorations into the mysteries of light was undertaken by Isaac Newton in the 17th century. Through his groundbreaking experiments with prisms, Newton demonstrated that white light is composed of a spectrum of colors, each with its unique wavelength. This discovery shattered the prevailing belief that light was an indivisible entity and laid the groundwork for modern optics.In the 19th century, the wave theory of light gained prominence, championed by scientists such as Thomas Youngand Augustin-Jean Fresnel. This theory proposed that light propagates as a wave through a hypothetical medium called the luminiferous ether. Experiments involving interference and diffraction provided compelling evidence supporting the wave model.However, in the early 20th century, Albert Einstein's theory of relativity and Max Planck's quantum theory challenged the wave theory's dominance. Einstein's work demonstrated that light exhibits particle-like properties, known as photons, which carry discrete packets of energy. Planck's theory introduced the concept of wave-particle duality, suggesting that light can behave both as a wave and as a particle.Modern research in optics continues to push the boundaries of our understanding of light's nature. Scientists are exploring the potential of quantum optics, a field that harnessers the principles of quantum mechanics to manipulate and control light at the quantum level. This work holds promise for advancements in fields as diverse as computing, imaging, and cryptography.In addition to its fundamental properties, light also plays a crucial role in countless natural phenomena. It enables us to see, provides sustenance to plants through photosynthesis, and shapes the dynamics of our planet's atmosphere and oceans. By unraveling the mysteries of light, we gain a deeper appreciation for the interconnectedness of the universe and the limitless possibilities it holds.中文回答:光,一种弥漫我们宇宙的神秘力量,长期以来一直吸引着科学家和哲学家。

大学物理之光的波动性与粒子性简述

大学物理之光的波动性与粒子性简述

大学物理之光的波动性与粒子性简述Light, a fundamental aspect of our universe, exhibits both wave-like and particle-like properties. This dual nature of light has been a subject of intense debate and exploration since the dawn of modern physics.Firstly, the wave nature of light is evidenced by its ability to undergo interference and diffraction. These phenomena occur whenlight waves encounter obstacles or pass through apertures, resultingin patterns that can only be explained by treating light as a wave. The wavelength of light determines its color and plays a crucial role in optics and electromagnetic radiation.On the other hand, the particle nature of light is demonstrated bythe photoelectric effect. This phenomenon occurs when light hits a metal surface and ejects electrons, which can be measured as a current. The energy of the ejected electrons is dependent on the frequency of the incident light, rather than its intensity, as would be expected if light were a mere wave. This observation led to the quantum theory of light, in which light is treated as a stream of particles, known as photons.The wave-particle duality of light remains a fascinating and elusive aspect of physics. It challenges our intuitive understanding of the world and continues to inspire new research and experiments in the field of quantum physics. As we delve deeper into the mysteries of light, we gain insights into the fundamental nature of reality itself.。

每一件事都有两面性英语作文

每一件事都有两面性英语作文

每一件事都有两面性英语作文The Dual Nature of Everything.The world is a canvas upon which we paint our experiences, and every stroke, every dot, and every line has a dual nature. Nothing exists in absolute black or white; everything has a shade of grey. This essay explores the intricate dualities that exist in every aspect of life, from the smallest particle to the vastest expanse of the universe.In the realm of physics, the dual nature of matter is perhaps the most intriguing. Light, for instance, behaves as both a particle and a wave. Depending on the experimental setup, physicists can observe light's wave-like properties, such as interference and diffraction, or its particle-like qualities, like the photoelectric effect. Similarly, electrons, fundamental building blocks of atoms, exhibit both wave-like and particle-like characteristics. This duality is not just a theoretical abstraction; it hasprofound practical implications in fields like quantum computing and nanotechnology.The dual nature of emotions is another fascinating aspect. Joy and sorrow, anger and calm, love and hate these emotions exist in a constant state of flux, intertwined and influencing each other. We experience the sweetness of joy only after tasting the bitterness of sorrow, and the intensity of anger is often followed by a profound calm. Love and hate, too, are often two sides of the same coin; they can transform into each other depending on the context and our perspective.The dual nature of human beings is also evident in our thoughts and actions. We are simultaneously rational and irrational, logical and emotional, selfish and altruistic. We make decisions based on logic and reason, but we are also swayed by emotions and impulses. We strive for self-improvement and yet are drawn to comfort zones that hinder our growth. This duality is not a weakness but a strength, as it allows us to navigate the complexities of life with flexibility and adaptability.Moreover, the dual nature of society is reflected inits structures and institutions. On the one hand, societyis ordered and structured, with laws, norms, and valuesthat govern our behavior. On the other hand, it is dynamic and ever-changing, constantly evolving to adapt to new technologies, ideas, and globalizations. This dual natureis seen in the balance between tradition and innovation, between conservatism and progressivism, between individualism and collectivism.The dual nature of everything also extends to the universe itself. The vastness and infinity of space are counterbalanced by the minuteness and finiteness of matter. The orderly motion of planets and stars is contrasted by the random and chaotic motion of particles at the quantum level. The beautiful harmony of the cosmos is mirrored by the brutal violence of natural disasters and astrophysical events.In conclusion, the dual nature of everything is a fundamental aspect of existence. It is a reminder that lifeis not black and white, but a rainbow of colors that blend into each other. Understanding and appreciating this dual nature helps us navigate the complexities of life with greater wisdom and compassion. It encourages us to embrace the paradoxes and contradictions that make us unique and to find balance in the ever-shifting landscape of the universe.。

结构光学教学大纲

结构光学教学大纲

结构光学教学大纲一、导言结构光学是现代光学领域中的一个重要分支,旨在研究和设计能够控制光的传播和分布的结构。

本课程旨在系统介绍结构光学的基本理论、原理和应用,使学生能够掌握结构光学的核心概念和基本技术。

二、课程目标1. 熟悉结构光学的基本概念和原理;2. 掌握结构光学的设计方法和工具;3. 能够应用结构光学进行光学元件和系统的设计和优化;4. 了解结构光学在现代光学技术中的应用。

三、课程内容1. 结构光学基础(1)光的基本性质(2)相干光和非相干光(3)衍射和干涉(4)波前调制2. 结构光学元件(1)衍射光栅(2)微透镜阵列(3)光子晶体(4)金属光栅3. 结构光学设计(1)光学色彩(2)非球面透镜设计(3)多层光学膜设计(4)结构光学元件设计软件介绍4. 结构光学应用(1)光通信(2)激光加工(3)生物医学成像(4)光学传感器四、教学方法1. 理论讲授:通过课堂讲解,系统介绍结构光学的基本理论和原理;2. 实践操作:安排实验课程,让学生亲自操作结构光学元件,加深理解和掌握实际操作技能;3. 论文阅读与讨论:指定相关结构光学领域的论文,引导学生掌握前沿技术和发展趋势。

五、考核方式1. 课堂作业:包括理论计算和实验报告;2. 期末考试:考察学生对结构光学基本概念和设计方法的掌握程度;3. 课程设计:设计结构光学元件并完成实际优化。

六、参考教材1. 《Structure of Light: The Science of VLSI Photonic Integrated Circuits》2. 《Introduction to Photonics and Optical Communications》3. 《Principles of Optics: Electromagnetic Theory of Propagation, Interference and Diffraction of Light》七、结语通过本课程的学习,学生将全面了解结构光学的基本理论和设计方法,培养实际操作技能,为将来的光学研究和工作奠定良好的基础。

射频和无线电波的关系

射频和无线电波的关系

射频和无线电波的关系Radio frequency (RF) and radio waves are intricately linked concepts in the field of electromagnetic waves. RF refers to a specific range of frequencies within the electromagnetic spectrum, typically defined as those frequencies that fall within the range of about 300 kHz to 300 GHz. This range corresponds to wavelengths ranging from one meter to one millimeter.射频(RF)和无线电波是电磁波领域中紧密相关的概念。

射频指的是电磁频谱中特定频率范围,通常定义为大约300千赫兹到300吉赫兹之间的频率。

这个范围对应的波长从一米到一毫米不等。

Radio waves, on the other hand, are a type of electromagnetic radiation that falls within the RF range. They are produced by oscillating electric and magnetic fields and propagate through space at the speed of light. Radio waves are capable of carrying information, making them crucial for wireless communication technologies such as radio, television, and mobile telephony.而无线电波则是一种属于射频范围内的电磁波。

鬼成像文献综述

鬼成像文献综述

鬼成像发展历史及现状学号:1011010430 姓名:陈超一,引言近年来,量子通信作为一门新兴学科得到了迅猛的发展。

它巨大的科学意义和潜在应用价值不仅引起物理学家、信息科学家的兴趣,而且也引起各国政府、军事部门、金融银行和企业厂商的重视。

它的未来发展势将对整个基础科学和工程科学,包括计算机科技、通讯科技、材料工程、精密测量技术、量子基础科学及信息论科学带来一次巨大的变革。

在对非线性晶体的自发参量下转换过程产生的双光子纠缠态进行的理论和实验的研究中,发现了一些新的光学现象,如鬼成像[1]等。

这些奇特的物理效应更新了我们对光现象的认识的传统观念,为开拓新的光信息技术提供了可能。

由于光源具有量子纠缠特性,人们自然将之归于量子纠缠态的非定域性。

在鬼成像系统中,纠缠光子对在空间上是分离的,鬼成像技术可以通过测量这两个相关光源而获得物体的像,而单独测量某一光源只能获得有限的信息。

鬼成像技术以其独特的非定域成像方式引起人们极大的研究热情,并在军事、医疗以及搜救等领域有着不可估量的应用价值。

在军事上,鬼成像传感器可以使直升机或无人机获得能评估投下的炸弹所造成的破坏程度的图像,可以在硝烟弥漫的战场上辨别敌我。

除此之外,在医学领域和搜救行动中也能利用这种成像技术并且能避免云雾和烟等使常规成像技术无能为力的气象条件的干扰,从而获得更清晰的图像。

作为量子通信和量子信息领域分支的鬼成像,以其独特的成像方式以及潜在的应用价值受到越来越多的关注。

二,发展历史及成果(一)鬼成像基本知识如图2.1所示,所谓鬼成像就是由同一个光源发出的两束光,其中一束通过物体照射探测器(称为信号光),另一束光(称为闲置光)的光路上不包含任何物体,最后对这两束光进行符合计数,符合测量的结果重现了物体,这种成像称为关联成像或鬼成像。

鬼成像按阶数可分为二阶、三阶、甚至更高阶,按光源可分为真热光源(完全非相干光)、赝热光源、双光子纠缠光源和部分相干光光源。

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k

input-output theory, applied to the beam splitter, yields the following canonical transformation [17] b− → k c− → k r = t =
1 √ . 2
=
r t −t r

where the parameters r and t satisfy r 2 + t2 = 1. For a 50 − 50% beam splitter, characteristic functions for the output modes and for the input modes
Ghost interference and diffraction based on the beam splitter
arXiv:quant-ph/9707030v1 16 Jul 1997
Lu-Ming Duan and Guang-Can Guo∗ Department of Physics and Nonlinear Science Center, University of Science and Technology of China, Hefei 230026, People’s Republic of China
† † ∗ ∗ χ(n) b− → , c− →; ξ − →, ξ − → = exp i ξ − → c− → b− → →+ξ − k k 1k 2k 1k k 2k k
Fig. 1 2
In Fig. 1, L1 , L2 and L3 are convex lenses. The line thermal light source S is put at the focal plane of lens L1 , so after L1 the beam has considerably large angular uncertainty. The beam is split by a beam splitter (BS) into two correlated beams, the signal beam and the idler beam. A single- or double-slit is inserted into the signal beam. After lens L2 , the signal light is coupled to a fiber. The input tip of the fiber is fixed on the axis at the focal plane of L2 . The idler light, passing through lens L3 , is coupled to another fiber. The horizontal transverse coordinate x of the fiber input tip is scanned by an encoder driver at the focal plane of L3 . After a delay τ , the idler light and the signal light are superposed and then detected by a photon-counting detector D . The visibility of the interference fringe gives the first-order correlation between the signal and the idler beams. By scanning the fiber input tip in the idler beam, an interference-diffraction pattern of the slit inserted into the signal beam will occur in the first-order correlation. In the following, we derive the interference-diffraction pattern of the slit in the first-order correlation. In this scheme, the input light of the beam splitter is a multi-mode thermal optical field. Different modes of the thermal light are − → 2 2 − k2 independent of each other. The mode with angular k = kx , ky , ω − kx y c2
is denoted by a− → , whose corresponding output modes, the signal mode and the k idler mode, are denoted by b− → , respectively. Another corresponding input → and c− k k mode of the beam splitter, which is in the vacuum state, is denoted by a− → . The
PACS numbers: 42.50.Dv, 03.65.Bz

Electronic address: gcguo@
1
Quantum correlation was recognized as one of the most striking features of quantum mechanics ever since Einstein, Podolsky, and Rosen proposed their famous gedanken experiment [1]. In various applications of non-classical features, such as in quantum cryptography [2-4] and in teleportation [5,6], correlations of states play an essential role . In recent years, quantum correlation has been confirmed in a number of two-photon correlation experiments [7-15]. Among those, the ghost interference-diffraction [15] is a remarkable example. In the original observation [15] of ghost diffraction, a correlated two-photon state is generated in the beta barium borate (BBO) crystal by the process of spontaneous parametric down-conversion (SPDC). The SPorthogonal polarization components (usually called signal and idler), is split by a polarization beam splitter into two beams, and detected by two distant pointlike photon counting detectors for coincidences. A Young’s double-slit or single-slit aperture is inserted into the signal beam. Surprisingly, an interferencediffraction pattern is observed in the coincidence counts by scanning the detector in the idler beam. This is called the ghost interference-diffraction, whose most striking feature is that the slit is inserted into the signal beam and in the idler beam ”appears” the interference-diffraction pattern. The ghost interference-diffraction results from quantum correlation. In the original experiment [15], the correlation is produced by the SPDC process. Beam splitters can also be used to generate quantum correlation [16]. In this letter, we propose a simple scheme for observing the ghost interference and diffraction. The scheme is based on the correlation generated by a beam splitter. We use the thermal light source and measure the first-order correlation between the signal and the idler beams. This is contrast to the original experiment, where one in fact measures the second-order correlation. (Note that for a correlated twophoton state the coincidence counting rate is proportional to the second-order correlation function between the signal and the idler beams.) The probable experimental setup for this scheme is illustrated in Fig. 1.
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