Basic Geometrical Optics
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
The Telescope Lenses, Which Turned the Image Upside Down but Improved the Clarity Dramatically
The image produced by the first refracting telescope was Name right side up. However, the clarity of the image was less than ideal. Johannes Kepler worked to improve the image produced by the refracting telescope. He used two convex The Telescope lenses, which turned the image upside down but improved the clarity dramatically. His design soon became popular By Phyllis Naegeli and remains in use today. Do you like to lie on your back and gaze One problem associated with the refracting telescope was at the stars? What constellations can you the rainbow halo it produced around the object in view. Sir name? Have you ever used a telescope to Isaac Newton did not care for the halo produced by the get a closer look at the universe? Do you refracting telescope. He set out to improve the design, know how a telescope works? which led him to work on the reflecting telescope. The design used a curved mirror to collect light from an object. A telescope is used to see distant objects A secondary flat mirror reflected the image to the side of up close. There are two basic types of the tube where it is viewed through an eyepiece. Newton telescopes - the refracting telescope and also used a shorter, fatter tube allowing magnification to be the reflecting telescope. Each will help increased by using larger mirrors. Newton's design you to see the planets, moon, or stars. Both eliminated the rainbow halo produced by the convex lenses use a tube and have an eyepiece to focus the image for you of the refracting telescope. -
3 Specular Reflection Spectroscopy
3 Specular Reflection Spectroscopy Robert J. Lipert, Brian D. Lamp, and Marc D. Porter 3.1 INTRODUCTION This chapter on specular reflection spectroscopy focuses on applications in the mid-infrared region of the spectrum. Applications in other spectral regions or using other spectroscopic techniques, such as Raman spectros copy, generally follow similar patterns as discussed in this chapter. In the past few decades, infrared spectroscopy (IRS) has developed into an invaluable diagnostic tool for unraveling details about the bonding and molecular structure at surfaces [l, 2, 3, 4, 5, 6]. The importance of IRS derives from five major factors, The first and most critical factor is the role of interfacial phenomena in a vast number of emerging material and surface technologies. Examples include adhesion, catalysis, tribiology, microelec tronics, and electrochemistry [3, 7, 8, 9]. The second factor stems from the Modern Techniques in Applied Molecular Spectroscopy, Edited by Francis M. Mirabella. Techniques in Analytical Chemistry Series. ISBN 0-471-12359-5 © 1998 John Wiley & Sons, Inc. 83 84 Specular Reflection Spectroscopy information-rich content of an IRS spectrum of a surface. That is, the frequencies of the spectroscopic features can be used to identify the chemical composition of a surface and the magnitudes and polarization dependencies of the features used to determine average structural orientations. The third factor arises from advances in the performance of IRS instrumentation. The most important of these advancements are the high throughput and multi plex advantages of Fourier transform interferometry, the development of high sensitivity, low-noise IR detectors, and the improvement in the com putational rates of personal computers and their adaptation to the oper ation of chemical instrumentation. -
Chapter 3 (Aberrations)
Chapter 3 Aberrations 3.1 Introduction In Chap. 2 we discussed the image-forming characteristics of optical systems, but we limited our consideration to an infinitesimal thread- like region about the optical axis called the paraxial region. In this chapter we will consider, in general terms, the behavior of lenses with finite apertures and fields of view. It has been pointed out that well- corrected optical systems behave nearly according to the rules of paraxial imagery given in Chap. 2. This is another way of stating that a lens without aberrations forms an image of the size and in the loca- tion given by the equations for the paraxial or first-order region. We shall measure the aberrations by the amount by which rays miss the paraxial image point. It can be seen that aberrations may be determined by calculating the location of the paraxial image of an object point and then tracing a large number of rays (by the exact trigonometrical ray-tracing equa- tions of Chap. 10) to determine the amounts by which the rays depart from the paraxial image point. Stated this baldly, the mathematical determination of the aberrations of a lens which covered any reason- able field at a real aperture would seem a formidable task, involving an almost infinite amount of labor. However, by classifying the various types of image faults and by understanding the behavior of each type, the work of determining the aberrations of a lens system can be sim- plified greatly, since only a few rays need be traced to evaluate each aberration; thus the problem assumes more manageable proportions. -
EMT UNIT 1 (Laws of Reflection and Refraction, Total Internal Reflection).Pdf
Electromagnetic Theory II (EMT II); Online Unit 1. REFLECTION AND TRANSMISSION AT OBLIQUE INCIDENCE (Laws of Reflection and Refraction and Total Internal Reflection) (Introduction to Electrodynamics Chap 9) Instructor: Shah Haidar Khan University of Peshawar. Suppose an incident wave makes an angle θI with the normal to the xy-plane at z=0 (in medium 1) as shown in Figure 1. Suppose the wave splits into parts partially reflecting back in medium 1 and partially transmitting into medium 2 making angles θR and θT, respectively, with the normal. Figure 1. To understand the phenomenon at the boundary at z=0, we should apply the appropriate boundary conditions as discussed in the earlier lectures. Let us first write the equations of the waves in terms of electric and magnetic fields depending upon the wave vector κ and the frequency ω. MEDIUM 1: Where EI and BI is the instantaneous magnitudes of the electric and magnetic vector, respectively, of the incident wave. Other symbols have their usual meanings. For the reflected wave, Similarly, MEDIUM 2: Where ET and BT are the electric and magnetic instantaneous vectors of the transmitted part in medium 2. BOUNDARY CONDITIONS (at z=0) As the free charge on the surface is zero, the perpendicular component of the displacement vector is continuous across the surface. (DIꓕ + DRꓕ ) (In Medium 1) = DTꓕ (In Medium 2) Where Ds represent the perpendicular components of the displacement vector in both the media. Converting D to E, we get, ε1 EIꓕ + ε1 ERꓕ = ε2 ETꓕ ε1 ꓕ +ε1 ꓕ= ε2 ꓕ Since the equation is valid for all x and y at z=0, and the coefficients of the exponentials are constants, only the exponentials will determine any change that is occurring. -
5 10 15 20 25 30 35 Class 359 Optical: Systems And
CLASS 359 OPTICAL: SYSTEMS AND ELEMENTS 359 - 1 359 OPTICAL: SYSTEMS AND ELEMENTS 1 HOLOGRAPHIC SYSTEM OR ELEMENT 197.1 .Using a periodically moving 2 .Authentication element 3 .Having particular recording 198.1 ..With particular mount or driver medium for element 4 ..Recyclable 199.1 ...Oscillating driver 5 ...Magnetic material 199.2 ....Electrostatically driven 6 ...Sandwich having photoconductor 199.3 ....Electromagnetically driven 7 ...Crystalline material 199.4 ....Electromechanically driven 8 ..Having nonplanar recording 200.1 ...Bearing or shaft for rotary medium surface driver 9 .For synthetically generating a 200.2 ....Specific shaft material or hologram structure (e.g., ceramic ring) 10 .Using modulated or plural 200.3 .....Grooved shaft reference beams 200.4 ....Fluid pressure bearing 11 ..Spatial, phase or amplitude 200.5 .....Dynamic fluid bearing modulation 200.6 ...Electrostatic driver 12 .Copying by holographic means 200.7 ...Electromagnetic driver 13 .Head up display 200.8 ...Electromechanical driver 14 ..Holograph on curved substrate 201.1 ..With multiple scanning elements 15 .Using a hologram as an optical (e.g., plural lenses, lens and element prism, etc.) 16 ..With aberration correction 201.2 ...Reflective element (e.g., 17 ..Scanner mirror, reflector, etc.) 18 ...Flat rotating disk 202.1 ...X-Y scanners 19 ..Lens 203.1 ...Having a common axis or 20 ...Multiple point hologram (e.g., rotation fly-eye lens, etc.) 204.1 ..Utilizing multiple light beams 21 .Having defined page composer 204.2 ...Including modulated light -
Making Your Own Astronomical Camera by Susan Kern and Don Mccarthy
www.astrosociety.org/uitc No. 50 - Spring 2000 © 2000, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Making Your Own Astronomical Camera by Susan Kern and Don McCarthy An Education in Optics Dissect & Modify the Camera Loading the Film Turning the Camera Skyward Tracking the Sky Astronomy Camp for All Ages For More Information People are fascinated by the night sky. By patiently watching, one can observe many astronomical and atmospheric phenomena, yet the permanent recording of such phenomena usually belongs to serious amateur astronomers using moderately expensive, 35-mm cameras and to scientists using modern telescopic equipment. At the University of Arizona's Astronomy Camps, we dissect, modify, and reload disposed "One- Time Use" cameras to allow students to study engineering principles and to photograph the night sky. Elementary school students from Silverwood School in Washington state work with their modified One-Time Use cameras during Astronomy Camp. Photo courtesy of the authors. Today's disposable cameras are a marvel of technology, wonderfully suited to a variety of educational activities. Discarded plastic cameras are free from camera stores. Students from junior high through graduate school can benefit from analyzing the cameras' optics, mechanisms, electronics, light sources, manufacturing techniques, and economics. Some of these educational features were recently described by Gene Byrd and Mark Graham in their article in the Physics Teacher, "Camera and Telescope Free-for-All!" (1999, vol. 37, p. 547). Here we elaborate on the cameras' optical properties and show how to modify and reload one for astrophotography. An Education in Optics The "One-Time Use" cameras contain at least six interesting optical components. -
Spherical Mirror Parabolic Mirror Ray Diagrams for Mirrors
Ray Diagrams for Mirrors September 8, 2015 1:24 PM Light rays travel in straight lines and so when we see one we assume it is coming straight towards us. But as physics students we know that light can be refracted and bent. Plane Mirror Object Image Plane mirrors form images at the same distance to the mirror as the object. This image is a virtual image as it is behind the mirror and impossible to project on a piece of paper in the real world. Question: Do we see more of ourselves as we get closer to the mirror or less? Question: What size of mirror do we need to see all of ourselves? Question: In a plane mirror is the images height larger, smaller or equal to the objects? Plane Mirrors: Are flat reflective surfaces that create a virtual image with the same height as the object and at the same distance from the mirror as the object. Concave Mirrors These are mirrors that are curved with their outer edges closer to you then their centers. Just like a parenthesis ")". They reflect light towards their focal points. The most ideal curved mirror is a Parabolic Mirror but these are extremely difficult to produce accurately. Most Parabolic Mirrors are approximations created from taking a small portion of a spherical mirror. Parabolic Mirror Spherical Mirror Optics Page 1 Parabolic Mirror Spherical Mirror Principal Axis = focal point = center of circle Convex Mirrors Convex Mirrors are just the opposite of a concave mirror. They are like a backwards parenthesis "(". They reflect light away from the mirrors focal point, which is located on the back side of the mirror. -
Reflection Measurements in IR Spectroscopy Author: Richard Spragg Perkinelmer, Inc
TECHNICAL NOTE Reflection Measurements in IR Spectroscopy Author: Richard Spragg PerkinElmer, Inc. Seer Green, UK Reflection spectra Most materials absorb infrared radiation very strongly. As a result samples have to be prepared as thin films or diluted in non- absorbing matrices in order to measure their spectra in transmission. There is no such limitation on measuring spectra by reflection, so that this is a more versatile way to obtain spectroscopic information. However reflection spectra often look quite different from transmission spectra of the same material. Here we look at the nature of reflection spectra and see when they are likely to provide useful information. This discussion considers only methods for obtaining so-called external reflection spectra not ATR techniques. The nature of reflection spectra The absorption spectrum can be calculated from the measured reflection spectrum by a mathematical operation called the Kramers-Kronig transformation. This is provided in most data manipulation packages used with FTIR spectrometers. Below is a comparison between the absorption spectrum of polymethylmethacrylate obtained by Kramers-Kronig transformation of the reflection spectrum and the transmission spectrum of a thin film. Figure 1. Reflection and transmission at a plane surface Reflection takes place at surfaces. When radiation strikes a surface it may be reflected, transmitted or absorbed. The relative amounts of reflection and transmission are determined by the refractive indices of the two media and the angle of incidence. In the common case of radiation in air striking the surface of a non-absorbing medium with refractive index n at normal incidence the reflection is given by (n-1)2/(n+1)2. -
25 Geometric Optics
CHAPTER 25 | GEOMETRIC OPTICS 887 25 GEOMETRIC OPTICS Figure 25.1 Image seen as a result of reflection of light on a plane smooth surface. (credit: NASA Goddard Photo and Video, via Flickr) Learning Objectives 25.1. The Ray Aspect of Light • List the ways by which light travels from a source to another location. 25.2. The Law of Reflection • Explain reflection of light from polished and rough surfaces. 25.3. The Law of Refraction • Determine the index of refraction, given the speed of light in a medium. 25.4. Total Internal Reflection • Explain the phenomenon of total internal reflection. • Describe the workings and uses of fiber optics. • Analyze the reason for the sparkle of diamonds. 25.5. Dispersion: The Rainbow and Prisms • Explain the phenomenon of dispersion and discuss its advantages and disadvantages. 25.6. Image Formation by Lenses • List the rules for ray tracking for thin lenses. • Illustrate the formation of images using the technique of ray tracking. • Determine power of a lens given the focal length. 25.7. Image Formation by Mirrors • Illustrate image formation in a flat mirror. • Explain with ray diagrams the formation of an image using spherical mirrors. • Determine focal length and magnification given radius of curvature, distance of object and image. Introduction to Geometric Optics Geometric Optics Light from this page or screen is formed into an image by the lens of your eye, much as the lens of the camera that made this photograph. Mirrors, like lenses, can also form images that in turn are captured by your eye. 888 CHAPTER 25 | GEOMETRIC OPTICS Our lives are filled with light. -
Chapter 5 Optical Properties of Materials
Chapter 5 Optical Properties of Materials Part I Introduction Classification of Optical Processes refractive index n() = c / v () Snell’s law absorption ~ resonance luminescence Optical medium ~ spontaneous emission a. Specular elastic and • Reflection b. Total internal Inelastic c. Diffused scattering • Propagation nonlinear-optics Optical medium • Transmission Propagation General Optical Process • Incident light is reflected, absorbed, scattered, and/or transmitted Absorbed: IA Reflected: IR Transmitted: IT Incident: I0 Scattered: IS I 0 IT IA IR IS Conservation of energy Optical Classification of Materials Transparent Translucent Opaque Optical Coefficients If neglecting the scattering process, one has I0 IT I A I R Coefficient of reflection (reflectivity) Coefficient of transmission (transmissivity) Coefficient of absorption (absorbance) Absorption – Beer’s Law dx I 0 I(x) Beer’s law x 0 l a is the absorption coefficient (dimensions are m-1). Types of Absorption • Atomic absorption: gas like materials The atoms can be treated as harmonic oscillators, there is a single resonance peak defined by the reduced mass and spring constant. v v0 Types of Absorption Paschen • Electronic absorption Due to excitation or relaxation of the electrons in the atoms Molecular Materials Organic (carbon containing) solids or liquids consist of molecules which are relatively weakly connected to other molecules. Hence, the absorption spectrum is dominated by absorptions due to the molecules themselves. Molecular Materials Absorption Spectrum of Water -
Quantum Metamaterials in the Microwave and Optical Ranges Alexandre M Zagoskin1,2* , Didier Felbacq3 and Emmanuel Rousseau3
Zagoskin et al. EPJ Quantum Technology (2016)3:2 DOI 10.1140/epjqt/s40507-016-0040-x R E V I E W Open Access Quantum metamaterials in the microwave and optical ranges Alexandre M Zagoskin1,2* , Didier Felbacq3 and Emmanuel Rousseau3 *Correspondence: [email protected] Abstract 1Department of Physics, Loughborough University, Quantum metamaterials generalize the concept of metamaterials (artificial optical Loughborough, LE11 3TU, United media) to the case when their optical properties are determined by the interplay of Kingdom quantum effects in the constituent ‘artificial atoms’ with the electromagnetic field 2Theoretical Physics and Quantum Technologies Department, Moscow modes in the system. The theoretical investigation of these structures demonstrated Institute for Steel and Alloys, that a number of new effects (such as quantum birefringence, strongly nonclassical Moscow, 119049, Russia states of light, etc.) are to be expected, prompting the efforts on their fabrication and Full list of author information is available at the end of the article experimental investigation. Here we provide a summary of the principal features of quantum metamaterials and review the current state of research in this quickly developing field, which bridges quantum optics, quantum condensed matter theory and quantum information processing. 1 Introduction The turn of the century saw two remarkable developments in physics. First, several types of scalable solid state quantum bits were developed, which demonstrated controlled quan- tum coherence in artificial mesoscopic structures [–] and eventually led to the devel- opment of structures, which contain hundreds of qubits and show signatures of global quantum coherence (see [, ] and references therein). In parallel, it was realized that the interaction of superconducting qubits with quantized electromagnetic field modes re- produces, in the microwave range, a plethora of effects known from quantum optics (in particular, cavity QED) with qubits playing the role of atoms (‘circuit QED’, [–]).