Reflection and Image Formation by Mirrors
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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 Diffuse Reflecting Power of Various Substances 1
. THE DIFFUSE REFLECTING POWER OF VARIOUS SUBSTANCES 1 By W. W. Coblentz CONTENTS Page I. Introduction . 283 II. Summary of previous investigations 288 III. Apparatus and methods 291 1 The thermopile 292 2. The hemispherical mirror 292 3. The optical system 294 4. Regions of the spectrum examined 297 '. 5. Corrections to observations 298 IV. Reflecting power of lampblack 301 V. Reflecting power of platinum black 305 VI. Reflecting power of green leaves 308 VII. Reflecting power of pigments 311 VIII. Reflecting power of miscellaneous substances 313 IX. Selective reflection and emission of white paints 315 X. Summary 318 Note I. —Variation of the specular reflecting power of silver with angle 319 of incidence I. INTRODUCTION In all radiometric work involving the measurement of radiant energy in absolute value it is necessary to use an instrument that intercepts or absorbs all the incident radiations; or if that is impracticable, it is necessary to know the amount that is not absorbed. The instruments used for intercepting and absorbing radiant energy are usually constructed in the form of conical- shaped cavities which are blackened with lampblack, the expecta- tion being that, after successive reflections within the cavity, the amount of energy lost by passing out through the opening is reduced to a negligible value. 1 This title is used in order to distinguish the reflection of matte surfaces from the (regular) reflection of polished surfaces. The paper gives also data on the specular reflection of polished silver for different angles of incidence, but it seemed unnecessary to include it in the title. -
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. -
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 -
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. -
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. -
Multidisciplinary Design Project Engineering Dictionary Version 0.0.2
Multidisciplinary Design Project Engineering Dictionary Version 0.0.2 February 15, 2006 . DRAFT Cambridge-MIT Institute Multidisciplinary Design Project This Dictionary/Glossary of Engineering terms has been compiled to compliment the work developed as part of the Multi-disciplinary Design Project (MDP), which is a programme to develop teaching material and kits to aid the running of mechtronics projects in Universities and Schools. The project is being carried out with support from the Cambridge-MIT Institute undergraduate teaching programe. For more information about the project please visit the MDP website at http://www-mdp.eng.cam.ac.uk or contact Dr. Peter Long Prof. Alex Slocum Cambridge University Engineering Department Massachusetts Institute of Technology Trumpington Street, 77 Massachusetts Ave. Cambridge. Cambridge MA 02139-4307 CB2 1PZ. USA e-mail: [email protected] e-mail: [email protected] tel: +44 (0) 1223 332779 tel: +1 617 253 0012 For information about the CMI initiative please see Cambridge-MIT Institute website :- http://www.cambridge-mit.org CMI CMI, University of Cambridge Massachusetts Institute of Technology 10 Miller’s Yard, 77 Massachusetts Ave. Mill Lane, Cambridge MA 02139-4307 Cambridge. CB2 1RQ. USA tel: +44 (0) 1223 327207 tel. +1 617 253 7732 fax: +44 (0) 1223 765891 fax. +1 617 258 8539 . DRAFT 2 CMI-MDP Programme 1 Introduction This dictionary/glossary has not been developed as a definative work but as a useful reference book for engi- neering students to search when looking for the meaning of a word/phrase. It has been compiled from a number of existing glossaries together with a number of local additions. -
Curved Mirror - Wikipedia
2018/11/5 Curved mirror - Wikipedia Curved mirror A curved mirror is a mirror with a curved reflecting surface. The surface may be either convex (bulging outwards) or concave (bulging inwards). Most curved mirrors have surfaces that are shaped like part of a sphere, but other shapes are sometimes used in optical devices. The most common non-spherical type are parabolic reflectors, found in optical devices such as reflecting telescopes that need to image distant objects, since spherical mirror systems, like spherical lenses, suffer from spherical aberration. Distorting mirrors are used for entertainment. They have convex and concave regions that produce deliberately distorted images. Contents Convex mirrors Uses of convex mirror Image Concave mirrors Reflections in a spherical convex Uses mirror. The photographer is seen Image reflected at top right Mirror shape Analysis Mirror equation, magnification, and focal length Ray tracing Ray transfer matrix of spherical mirrors See also References External links Convex mirrors A convex mirror, diverging mirror, or fish eye mirror is a curved mirror in which the reflective surface bulges toward the light source.[1] Convex mirrors reflect light outwards, therefore they are not used to focus light. Such mirrors always form a virtual image, since the focal point (F) and the centre of curvature (2F) are both imaginary points "inside" the mirror, that cannot be reached. As a result, images formed by these mirrors cannot be projected on a screen, since the image is inside the mirror. The image is smaller than the object, but gets larger as the object approaches the mirror. A collimated (parallel) beam of light diverges (spreads out) after reflection from a convex mirror, since the normal to the surface differs with each spot on the mirror. -
Physics I Notes Chapter 14: Light, Reflection, and Color
Physics I Notes Chapter 14: Light, Reflection, and Color Characteristics of light • Light is an electromagnetic wave . As shown below, an electromagnetic wave is a transverse wave consisting of mutually perpendicular oscillating electric and magnetic fields. Electromagnetic waves are ultimately produced by an accelerating charge. A changing electric field produces a changing magnetic field which in turn produces a changing electric field and so on. Because of this relationship between the changing electric and magnetic fields, an electromagnetic wave is a self- propagating wave that can travel through a vacuum or a material medium since electric and magnetic fields can exist in either one. Animation of e.m. wave with vibrating charge Scroll down after webpage loads for animation. http://www.phy.ntnu.edu.tw/ntnujava/index.php?topic=35.0 • All electromagnetic waves travel at the speed of light. Electromagnetic waves are distinguished from each other by their differences in wavelengths and frequencies (wavelength is inversely related to frequency) . c=f λλλ c = speed of light = 3.0 x 10 8 m/s in a vacuum = 300,000 km/s = 186,000 miles/s A light year is the distance that light travels in one year in a vacuum. So haw many miles would that be? What would a light-minute be? • The electromagnetic spectrum is a continuum of all electromagnetic waves arranged according to frequency and wavelength. Visible light is only a small portion of the entire electromagnetic spectrum. Page 1 of 8 • Brightness or intensity of light decreases by the square of the distance from the source (inverse square law). -
Near-Field Fourier Ptychography: Super- Resolution Phase Retrieval Via Speckle Illumination
Near-field Fourier ptychography: super- resolution phase retrieval via speckle illumination HE ZHANG,1,4,6 SHAOWEI JIANG,1,6 JUN LIAO,1 JUNJING DENG,3 JIAN LIU,4 YONGBING ZHANG,5 AND GUOAN ZHENG1,2,* 1Biomedical Engineering, University of Connecticut, Storrs, CT, 06269, USA 2Electrical and Computer Engineering, University of Connecticut, Storrs, CT, 06269, USA 3Advanced Photon Source, Argonne National Laboratory, Argonne, IL 60439, USA. 4Ultra-Precision Optoelectronic Instrument Engineering Center, Harbin Institute of Technology, Harbin 150001, China 5Shenzhen Key Lab of Broadband Network and Multimedia, Graduate School at Shenzhen, Tsinghua University, Shenzhen, 518055, China 6These authors contributed equally to this work *[email protected] Abstract: Achieving high spatial resolution is the goal of many imaging systems. Designing a high-resolution lens with diffraction-limited performance over a large field of view remains a difficult task in imaging system design. On the other hand, creating a complex speckle pattern with wavelength-limited spatial features is effortless and can be implemented via a simple random diffuser. With this observation and inspired by the concept of near-field ptychography, we report a new imaging modality, termed near-field Fourier ptychography, for tackling high- resolution imaging challenges in both microscopic and macroscopic imaging settings. The meaning of ‘near-field’ is referred to placing the object at a short defocus distance with a large Fresnel number. In our implementations, we project a speckle pattern with fine spatial features on the object instead of directly resolving the spatial features via a high-resolution lens. We then translate the object (or speckle) to different positions and acquire the corresponding images using a low-resolution lens. -
Improving Design Processes Through Structured Reflection
Improving Design Processes through Structured Reflection A Domain-independent Approach Copyright 2001 by Isabelle M.M.J. Reymen, Eindhoven, The Netherlands. All rights reserved. No part of this publication may be stored in a retrieval system, transmitted, or reproduced, in any form or by any means, including but not limited to photocopy, photograph, magnetic or other record, without prior agreement and written permission of the author. CIP-DATA LIBRARY TECHNISCHE UNIVERSITEIT EINDHOVEN Reymen, Isabelle M.M.J. Improving design processes through structured reflection : a domain-independent approach / by Isabelle M.M.J. Reymen. – Eindhoven : Eindhoven University of Technology, 2001. Proefschrift. - ISBN 90-386-0831-4 NUGI 841 Subject headings : design research / design theory ; domain independence / design method ; reflection / design process ; description / multidisciplinary engineering design Stan Ackermans Institute, Centre for Technological Design The work in this thesis has been carried out under the auspices of the research school IPA (Institute for Programming research and Algorithmics). IPA Dissertation Series 2001-4 Printed by University Press Facilities, Technische Universiteit Eindhoven Cover Design by Cliff Hasham Improving Design Processes through Structured Reflection A Domain-independent Approach PROEFSCHRIFT ter verkrijging van de graad van doctor aan de Technische Universiteit Eindhoven, op gezag van de Rector Magnificus, prof.dr. M. Rem, voor een commissie aangewezen door het College voor Promoties in het openbaar te verdedigen op dinsdag 3 april 2001 om 16.00 uur door Isabelle Marcelle Marie Jeanne Reymen geboren te Elsene, België Dit proefschrift is goedgekeurd door de promotoren: prof.dr.Dipl.Ing. D.K. Hammer en prof.dr.ir. P. Kroes To Twan vi Preface After I finished my Master's thesis at the Department of Architecture, Urban Design, and Planning (ASRO) of the Faculty of Applied Sciences at the Katholieke Universiteit Leuven (KULeuven) in Belgium, prof.