第2讲几何光学和眼睛PPT讲稿.ppt
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1、第第2讲几何光学和眼几何光学和眼睛睛第1页,共53页,编辑于2022年,星期一Magnification Power透镜的透镜的放大倍率放大倍率Often,positive lenses are rated with a single magnification,such as 4x.In principle,any positive lens can be used at an infinite number of possible magnifications.However,when a viewer adjusts the object distance so that the ima
2、ge appears to be essentially at infinity(which is a comfortable viewing distance for most individuals(明视距离明视距离),the magnification is given by the relationship:Object under observationThus,a 25-mm focal-length positive lens would be a 10 x magnifier!那么,那么,50 x的镜头的焦距是多少?(提问)的镜头的焦距是多少?(提问)Magnification
3、=250 mm/f 第2页,共53页,编辑于2022年,星期一Virtual Images 虚像虚像When the object is less than one focal length away from a lens,no image occurs,but a virtual image is said to occur if you look back through the lens.Objectf 0Virtual imagefdof第3页,共53页,编辑于2022年,星期一fIt depends on how much of the lens is used,that is,t
4、he aperture 孔径光阑.Only one plane(平面)is imaged(i.e.,is in focus)at a time.But wed like objects near this plane to at least be almost in focus.The range of distances in acceptable focus is called the depth of field.Out-of-focus planeFocal planeObjectImageSize of blur in out-of-focus planeApertureThe sm
5、aller the aperture,the more the depth of field 通过孔径越小,焦深就越大.Depth of Field 焦深焦深孔径(光阑)第4页,共53页,编辑于2022年,星期一The pinhole camera 针孔照相机针孔照相机You can make an entire room into a camera this way by cutting a small hole in a wall and looking at the opposite wall.This is called the camera obscura.ObjectImagePi
6、nholeIf all light rays are directed through a pinhole,it forms an image with an infinite depth of field.The first person to mention this idea was Aristotle.The concept of the focal length is inappropriate for a pinhole lens.The magnification is still di/do.意大利Torino都灵大教堂耶稣裹尸布造假事件思考:针孔照相机的优点是什么?什么情况下
7、会用针孔照相机?我们常用的照相机为什么不用针孔照相机?(提问)第5页,共53页,编辑于2022年,星期一都灵的主教堂都灵的主教堂圣乔瓦尼大教堂圣乔瓦尼大教堂(Duono di San Giovsnni,Piazza San Giovanni)第6页,共53页,编辑于2022年,星期一如何发现裹尸布是造假的?如何发现裹尸布是造假的?第7页,共53页,编辑于2022年,星期一The F-number,“f/#”,of a lens is the ratio of its focal length and its diameter.f/#=f/dffd1fd2f/#=1f/#=2Large f-nu
8、mber lenses collect more light but are harder to engineer.F-number光圈光圈F值值f完整的照相机光圈是:f1,f1.4,f2,f2.8,f4,f5.6,f8,f11,f16,f22,f32,f44,f64第8页,共53页,编辑于2022年,星期一Another measure of a lens size is the numerical aperture.Its the product of the medium refractive index and the marginal ray angle.NA =n sin(a)Hi
9、gh-numerical-aperture lenses are bigger.faNumerical Aperture 数值孔径数值孔径Why this definition?Because the magnification can be shown to be the ratio of the NA on the two sides of the lens.第9页,共53页,编辑于2022年,星期一F/#and NA光圈光圈F值与数值孔径之间的关系值与数值孔径之间的关系In many cases,the best coupling you can get occurs when you
10、match the f/#between optical systems.Realistic f/#s:lens 2fibers 1.5数值孔径匹配的重要性。例题:把数值孔径2.0的光学系统耦合到数值孔径为1.5的光学系统中,光通量耦合效率是多少?第10页,共53页,编辑于2022年,星期一And this arrangementmaps position to angle:Lenses can also map angle to position.From the object to the image,we have:1)A distance f2)A lens of focal leng
11、th f3)A distance f出射角和入射光源位置有关没有放大率,位置只和入射角有关第11页,共53页,编辑于2022年,星期一Prism 棱镜棱镜顶角棱镜的全内反射棱镜的全内反射可作指纹读取器可作指纹读取器偏向角Deviation angleApex angle第12页,共53页,编辑于2022年,星期一FTIR and fingerprintingSee TIR from a fingerprint valley and FTIR from a ridge.第13页,共53页,编辑于2022年,星期一Prism pair for dispersion compensation棱镜对可
12、以用来补偿色散棱镜对可以用来补偿色散The minimum deviation angle when Brewster incidenceThe apex angle at Brewster incidence第14页,共53页,编辑于2022年,星期一Dispersion of plane glass and prism第15页,共53页,编辑于2022年,星期一Telescopes望远镜望远镜A telescope should image an object,but,because the object will have a very small solid angle,it shou
13、ld also increase its solid angle significantly,so it looks bigger.So wed like D to be large and use two lenses to square the effect.where M=-di/doSo use di do for both lenses.Note that this is easy for the first lens,as the object is really far away!M1M2Image plane#1Image plane#2Keplerian telescope第
14、16页,共53页,编辑于2022年,星期一Telescope Terminology 望远镜术语望远镜术语第17页,共53页,编辑于2022年,星期一Telescopes(contd)The Galilean Telescope:one negative and one positive lensesThe merit?f1 0The analysis of this telescope is a homework problem!第18页,共53页,编辑于2022年,星期一The Cassegrain Telescope卡塞格林望远镜卡塞格林望远镜Telescopes must collec
15、t as much light as possible from the generally very dim objects many light-years away.Its easier to create large mirrors than large lenses(only the surface needs to be very precise).ObjectIt may seem like the image will have a hole in it,but only if its out of focus.If a 45-mirror reflects the beam
16、to the side before the smaller mirror,its called a Newtonian telescope.牛顿望远镜第19页,共53页,编辑于2022年,星期一No discussion of telescopes would be complete without a few pretty pictures.NGC 6543-Cats Eye Nebula 星云-one of the most complex planetary nebulae ever seenGalaxy Messier 81Uranus 天王星 is surrounded by it
17、s four major rings and by 10 of its 17 known satellites 第20页,共53页,编辑于2022年,星期一Microscopes显显微镜微镜Image plane#2Microscopes work on the same principle as telescopes,except that the object is really close and we wish to magnify it.When two lenses are used,its called a compound microscope.Standard distanc
18、es are s=250 mm for the eyepiece and s=160 mm for the objective,where s is the image distance beyond one focal length.In terms of s,the magnification of each lens is given by:The magnification of the microscope is the M1M2Image plane#1Eye-pieceObjectivef1f2第21页,共53页,编辑于2022年,星期一If an optical system
19、lacks cylindrical symmetry,we must analyze its x-and y-directions separately:Cylindrical lenses 柱透镜柱透镜A spherical lens focuses in both transverse directions.A cylindrical lens focuses in only one transverse direction.When using cylindrical lenses,we must perform two separate ray-matrix analyses,one
20、for each transverse direction.第22页,共53页,编辑于2022年,星期一Large-angle reflection off a curved mirror also destroys cylindrical symmetry 反射镜的入射角过大会导致柱面不对称反射镜的入射角过大会导致柱面不对称Optic axis before reflectionOptic axis after reflectionThe optic axis makes a large angle with the mirror normal,and rays make an angle
21、with respect to it.Rays that deviate from the optic axis in the plane of incidence are called“tangential子午面.”Rays that deviate from the optic axis to the plane of incidence are called“sagittal弧矢面.“(We need a 3D display to show one of these.)tangential ray第23页,共53页,编辑于2022年,星期一Ray Matrix for Off-Axis
22、 Reflection from a Curved Mirror 反射镜离轴反射矩阵反射镜离轴反射矩阵If the beam is incident at a large angle,q,on a mirror with radius of curvature,R:where Re=R cosq for tangential rays 子午and Re=R/cosq for sagittal rays 弧矢ROptic axistangential ray 子午q第24页,共53页,编辑于2022年,星期一Aberrations 像差像差Aberrations are distortions
23、that occur in images,usually due to imperfections in lenses,some unavoidable,some avoidable.They include:Chromatic aberration 色差Spherical aberration 球差Astigmatism 像散Coma 慧差Curvature of field 场弯曲Pincushion and Barrel distortion 畸变Aberrations cant be modeled with ray matrices.Designers beat them by ma
24、king lenses with multiple elements,that is,several lenses in a row.Some zoom lenses can have as many as a dozen or so lenses.栅(枕)形畸变桶形畸变第25页,共53页,编辑于2022年,星期一Chromatic Aberration 色差色差Because the lens material has a different refractive index for each wavelength,the lens will have a different focal l
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