南开大学光学工程内部课件Sep_16th

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光学-课件全集

光学-课件全集

a
n1
i1
a1
D B
n2
A
i2
n1 C
a2
d
由折射定律和几何关系可得出:
n1siin 1n2siin 2
AD AB siin1
AC C Bd/coi2s AB2dtain2
1、非相干叠加 独立光源的两束光或同一光源的不同部位所发出 的光的位相差“瞬息万变”
1
0
cosdt0
II1I2
叠加后光强等与两光束单独照射时的光强之和,
无干涉现象
2、相干叠加 满足相干条件的两束光叠加后
II1I22I1I2co s
位相差恒定,有干涉现象
若 I1 I2
§1.1.5 相干与不相干叠加
矢量合成方法
x1A 1cots (1)0
x 2 A 2 co t s 2) ( 0

A
AA 12A2 22A 1A2co2s0 (1)0
A2
y2
y2
y
0arcA A 1 1tc sa io1 1 n n s0 0 A A 2 2c sio2 n 2s 0 0O
3、光强 光波是电磁波。 光波中参与与物质相互作用(感光作用、生理
作用)的是 A 矢量,称为光矢量。 A 矢量的振动称为光振动。
光强:在光学中,通常把平均能流密度称为光强, 用 I 表示。
I A2
机械波的独立性和叠加性
发生干涉的条件: 1、频率相同 2、观察时间内波动不中断 3、相遇出振动方向几乎在同一直线上 干涉现行的特性:
2d
k0,1,2…
干涉加强
干涉减弱
明纹位置
暗纹位置
两相邻明(或暗)条纹间的距离称为条纹间距。

南开大学光学工程内部课件Sep 7th

南开大学光学工程内部课件Sep 7th

Brief history of optics (cont’ed)
平面镜 (《经下》19/—/42· —) 经:景迎日。说在转。 影子可以由反射(迎)太阳(的光线)形 成。理由在于翻转
经说:景,日之光反烛人,则景在日与人之间。
如果太阳之间
Brief history of optics (cont’ed)

母国光 战元龄著 《光学》 人民教育出版社
参考书目
ftp://202.113.227.137 Username: optics Password: optics-nk
/opt/index/
/course/optics/
《淮南万毕术》,公元前120左右,淮南王刘安及 其门客的著作。记录了用冰制作透镜的方法: “削冰令圆,举以向日,以艾承其影,则火生。” 还记录了潜望镜的雏形:“取大镜高悬,置水盆 于其下,则见四邻矣。”
Brief history of optics (cont’ed)

谭峭《化书》,约公元940年(南 唐)。书中有一段十分有趣的记 录:小人常有四镜。一名圭,一 名珠,一名砥,一名盂。圭视者 大,珠视者小,砥视者正,盂视 者倒。观彼之器,查我之型,由 是无大小,无短长,无妍丑,无 美恶。描述的很有可能是四种透 镜的成像性质。圭是双凹发散透 镜,珠是双凸透镜,砥是平凹透 镜,盂是平凸透镜。
一个受到光照射的人,看起来就好像他在发射出(光线)一样。人的下 部成为(像的)上部,而人的上部成为(像的)下部。人的脚(好像发 出)光在下方被遮蔽(即照到了针孔的下方),(但另一些光线)在上 方成像。人的头(好像发出)光在上方被遮蔽(即照到了针孔的上方), (但另一些光线)在下方成像。在(离开光源、反射体或像)较远或较 近的某个位置上,有一个距激光的点(端)(即针孔),结果像就只被 允许通过聚集之处(库)的光线所形成

南开大学光学工程内部课件Oct 19th

南开大学光学工程内部课件Oct 19th

E1 (r , t ) E01 exp i(k1 r t 1 ) E2 (r , t ) E02 exp i(k2 r t 2 ).
Two plane waves meet at P
Superposition of two beams

The transmitted light is incident onto a screen containing two narrow slits
Young’s Double Slit Experiment

The symmetric narrow slits, S1 and S2 act as the two light sources The waves from the two slits come from the same source S0 and therefore are always in phase.
m


= 0, ±1, ±2, …
Interference Equations

Y:measured vertically from the zeroth order maximum Assumptions


L >>d,
d >>λ

y =LtanθLsinθ
I I1 I 2 2 I1I 2 cos(kd sin ) I1 I 2 2 I1I 2 cos(kdy / L)

Other Coherent Sources

Currently, it is much more common to use a laser as a coherent source The laser produces an intense, coherent,

南开大学光学工程内部课件Nov-16th

南开大学光学工程内部课件Nov-16th

If the primary wave was simply to propagate
from S to P, it is
E
0
e i[t k ( r0 )]
r0
The two equations must be exactly the same. So we introduce a /2 phase difference between the primary wave and the secondary wave to make the two equations so.
dS d 2 ( sin )
Fresnel Dif2 2( r0 )cos
So
dS 2 rdr. Constant!!! r0
We have
El
(1)l 1
2Kl A r0
equation (a) becomes
E E1 Em
2
2
Fresnel Diffraction
From equation (b) we have
E
E1

E2 2

E m 1 2

Em
Since K() goes from 1 to 0 over a great many zones, we can neglect any variation between adjacent zones, i.e. │E1│= │E2│, │Em-1│= │Em│. So

Em 2
)
Em 2
(a)
or
E
E1

E2 2
(
E2 2

E3

E4 2

南开大学光学工程内部课件Lecture 2

南开大学光学工程内部课件Lecture 2
—— Range Instrumentation prism, right.
BM 60 90 right
Ray Tracing
Reflection from Flat Surface
—— Range Instrumentation prism, left, roof.
BM 100 90 left roof
CR 180 roof
Ray Tracing
Reflection from Flat Surface
—— Rhomb prism. It has two reflective faces 斜方棱镜,又名菱形棱镜
BC 0 (Rhomb)
Ray Tracing
Reflection from Flat Surface
Reflection from Flat Surface
—— Isosceles prism, three reflective faces, roof
CR 45 roof (Schmidt)
Ray Tracing
Reflection from Flat Surface
—— Isosceles prism, three reflective faces, roof

Reflection Prism
—— Isosceles prism (Classification code: R), single reflective face. 等腰棱镜(代号:D), 一次反射型
The Dove Prism (AR45)
Ray Tracing
Reflection from Flat Surface
• In fact, if the UV and IR are included, most any substance will sow some absorption. So anomalous dispersion exist somewhere throughout the spectrum

南开大学光学——绪论

南开大学光学——绪论

常胜江 办公地点:伯苓楼3区303
电话:23504571
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Nankai University
光在各向同性介质界面上的 反射和折射
晶体的光学性质 光与物质的相互作用
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CHANG Sheng Jiang, Institute of Modern Optics, Nankai University
主要参考书:
1. 新概念物理教程-光学,赵凯华; ----高等教育出版社, 2. 光学 (上下册), 赵凯华,钟锡华 ; ----北京大学出版社; 3. 光学, 母国光等. ----高等教育出版社;
2
光与物质相互作用的性质及特点
1. 线性作用过程:
-----非强光光场的线性叠加等;
2. 非线性作用过程: -----强激光与大气相互作用过程;
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CHANG Sheng Jiang, Institute of Modern Optics, Nankai University Nankai University
认为光是纵波,是一种在弹性媒质中传播的机械波;
------成功解释了光的反射和折射等现象;
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CHANG Sheng Jiang, Institute of Modern Optics, Nankai University
2. 托马斯 杨 和菲涅尔 (19世纪初) :
发现并解释了干涉、衍射现象,把波动理论大大推 向前进; -----通过偏振现象确认光是一种横波; -----初步测定了波长;


光学课程需要回答的问题:
1 2 3
光的本质是什么? 光与物质相互作用的性质及特点 光学能做什么?
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《光学基本知识讲座》课件

《光学基本知识讲座》课件

光学在军事中的应用
总结词
光学技术在军事侦察和武器系统中的应用
详细描述
光学技术在军事领域的应用包括红外侦察、 激光雷达、瞄准和测距等。这些技术提高了 军事侦察和武器系统的精度和效率,对现代
战争的胜负具有关键作用。
04
光学发展历程
光学发展史简介
古代光学
古代文明对光的研究和利用,如反射、折射等简单光 学现象的发现和应用。
全息摄影技术
总结词
全息摄影原理及应用
详细描述
全息摄影技术利用光的干涉和衍射原理,记 录并重现三维物体的光波信息。全息照片具 有立体感和视角任选的特性,广泛应用于产 品展示、艺术创作和安全识别等领域。
光学在医学中的应用
总结词
光学在医学诊断和治疗中的应用
详细描述
光学技术在医学领域具有广泛的应用 ,如光学显微镜用于细胞观察,激光 用于手术切割和眼科治疗,以及光学 成像技术用于无创检测和诊断。
文艺复兴时期
科学方法的兴起,对光的本质和传播方式的研究逐渐 深入。
19世纪
光学理论体系逐渐完善,如波动光学和几何光学的发 展。
光学重大发明和发现
01
02
03
牛顿的棱镜实验
揭示了白光是由不同颜色 的光组成,奠定了光谱学 的基础。
干涉现象的发现
为波动光学的建立提供了 重要依据。
激光的发明
开创了光学的新领域,对 科技、工业、医疗等领域 产生了深远影响。
实验材料
光源、衍射板、屏幕等 。
Hale Waihona Puke 实验步骤将光源对准衍射板中心 ,调整光源与衍射板距 离;观察衍射现象并记
录。
注意事项
注意保护眼睛,避免直 接照射光源;调整仪器

南开大学结构化学课件1.pdf

南开大学结构化学课件1.pdf

普朗克因提出量子化概念获得1918年Nobel物理奖。
Nankai University
黑体辐射研究中理论发展过程
实验数据
黑体模型 Kirchhoff 经典理论
经验关系式 Wien
数学模型
众多实验 证明
量子力学 诞生
量子假说 Planck
Planck 数学模型
Rayleigh-Jeans 数学模型 紫外灾难
“The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decima”
麦克斯韦尔(J. C. Maxwell) 1856-1865年 电磁理论 光是一种电磁波。
赫兹(Gustav Hertz) 1887 年,实验验证电磁波
光的波动说似乎已确定无疑
Nankai University
1. 麦克斯韦尔电磁学说:光是一种电磁波,可以用电场
Nankai University
玻尔1913年基于卢瑟福(Ernest Rutherford)提出的原子模型,综合Planck和
Einstein的量子论,提出了关于原子结构的模型
①经典轨道加定态条件
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Refraction at curved surface
Similar, the second or image focus is the axial point Fi where the image is formed when S0= . And the second or image focal length fi as equal to Si in the special case, we have
Why are focusing instruments necessary?
Refraction at curved surface
Imaging In order to image S at location P, the time it takes for each and every portion of a wavefront leaving S to converge at point P must be identical. So:
which followed with
n1 n2 1 n2 S i n1 S0 ( ) SM 2 MS ' R MS ' SM
Refraction at curved surface
Discussion Sign convention for spherical refraction surfaces and thin lenses
Refraction at curved surface
Fermat’s Principle maintains that the optical path length (OPLSS’) will be stationary (实际上,物与像之间根据费马原 理具有等光程性), i.e.:
1 d (OPLSS ' ) 2 2 d {n1 [ R ( S 0 R ) 2 R( S 0 R ) cos ] 2 } d d
Imaging by a Flat refracting surface

The image formed by a flat refracting surface is on the same side of the surface as the object The image is virtual The image forms between the object and the surface The rays bend away from the normal since n1 > n2 L
The emerging wavefront segment corresponding to paraxial rays from a point source S is essentially spherical and will form a “perfect” image at its center point located at S’.

Refraction at curved surface
n1
Yo
i
V
M
n2
S

u
S0

R
i
C Si
n
u
Yi

S’
The upper figure depicts a wave from the point source S impinging on a spherical interface of radius R centered at C. Here we assume n2>n1.
n1 n2 n2 n1 P S0 S i R
(1)
Refraction at curved surface
P is called optical power. We could have this formula with Snell’s law rather than Fermat’s Principle.
Refraction at curved surface
Perfect reshaping between converging (diverging) wave and flat wave

With the help of ellipsoidal or hyperboloidal surface, we can reshape precisely converging (diverging) waves into plane wave or vice versa

Lens—Type of lenses

Type of lenses
We limit ourselves centered systems of spherical surfaces (for which all the nonplanar surfaces are centered on a common axis, or in other words, all surfaces are rotationally symmetric about a common axis)
Lens
第一章第6节
Lens—What is a lens
What is a lens In traditional sense, a lens is an optical system consisting of two or more refractive interfaces where at least one of these is curved.
d {n2 [ R ( S i R ) 2 R( S i R ) cos ] 2 } d
2 2
1
0
Refraction at curved surface
So we have:
n1 R( S0 R) sin n2 R( Si R) sin 0 2 SM 2 MS '
s’
s
Refraction at curved surface
Refraction at a spherical surface Image we have a point source S (in other words, we have a point object S) whose spherical waves arrive at a spherical boundary of two transparent media. We prefer that the wave traveling in the second medium converges to a point S’. In fact, it is also the basic requirement of optical instruments.
Refraction at curved surface

Focus and focal length If an point is located at F0, where
n1 f0 R n2 n1
according to equation (1), it is imaged at infinity (Si=). The location F0 is called first or object focus. And the special object distance is defined as the first or object focal length.
Lens—Type of lenses
1. Simple lens and compound lens: Simple lens —— consist of one element, i.e., it only has two refracting surfaces Compound lens —— more than one elements. 2. Thin and thick lens: —— if its thickness is effectively negligible or not
Lens—Thin-lens equations
The simplest case —— thin-lens equations Let’s now locate the conjugate points for a lens of index nl surrounded by a medium of index nm. It is the simplest cБайду номын сангаасse of a lens.
Lens—Type of lenses
3. Convex (converging or positive) lens and concave (diverging or negative) lens: With the assumption that the refractive index of the lens is larger than that of the environment of the lens, convex lens is thicker at the center and so tends to decrease the radius of wavefronts. On the other hand, concave lens is thinner at the center and tends to cause the wavefronts to be more diverging than it was upon entry.
n2 fi R n2 n1
Refraction at curved surface
Refraction at curved surface

Refraction at aspherical surfaces
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