L 31 Light and Optics [2] at a Surface • Measurements of the Speed of Light (C) √ Index of Refraction N = C/V > 1

Total Page:16

File Type:pdf, Size:1020Kb

L 31 Light and Optics [2] at a Surface • Measurements of the Speed of Light (C) √ Index of Refraction N = C/V > 1 Reflection and refraction L 31 Light and Optics [2] at a surface • Measurements of the speed of light (c) √ Index of refraction n = c/v > 1 • Index of refraction vmedium = c/n – the bending of light – refraction √ Incident Normal line – total internal reflection √ Light ray reflected • Color (wavelength and frequency, c = λf ) Light ray • Dispersion • rainbows • Atmospheric scattering • blue sky and red sunsets • Law of reflection – mirrors – Image formation refracted Light ray 1 2 Seeing through the window Seeing through a window When the angle of incidence is small, most of the A light ray is offset slightly incident light passes thru the glass, only a small When it passes thru a pane amount is reflected. Of glass. The thinner the Glass, the smaller the offset. r ef lec ted ted smit tran ent incid outside 3 inside 4 Windows behaving as mirrors VISIBLE LIGHT When the angle of incidence is r e f large (grazing l e transmitted c incidence) more t e d light is reflected, the window is like a mirror. t n e Color Î WAVELENGTH OR FREQUENCY d i c n i Wavelength × Frequency = c (speed of light) IN OUT 5 = 3 x 108 m/s 6 1 The index of refraction (n) depends Different colors are refracted (bent) by of the color (wavelength) of the light different amounts this effect is called DISPERSION color Wavelength (nm) n Red 660 1.520 orange 610 1.522 yellow 580 1.523 green 550 1.526 White light red blue 470 1.531 violet 410 1.538 violet contains all Glass prism wavelengths –9 1 nanometer (nm) = 1 × 10 m 7 (colors) 8 The rainbow Why is it a rain BOW ? • Rainbows are caused by dispersion of sunlight The drops must be from water droplets which act as tiny prisms At just the right Angle (42 degrees) Between your eyes And the sun to see The rainbow. This Angle is maintained Along the arc of a Circle. 9 10 Atmospheric scattering Atmospheric scattering: blue sky • Short wavelengths are • Why is the sky blue and sunsets red? scattered more than long • It is due to the way that sunlight is wavelengths scattered by the atmosphere (N and O ) • Blue light (short) is 2 2 scattered 10 times more • ScatteringÆ atoms absorb light energy than red light and re-emit it, but not at the same • The light that we see in wavelength the sky when not looking directly at the sun is • Sunlight contains a full range of scattered blue light wavelengths in the visible region 11 12 2 Atmospheric scattering: red sunset Why are clouds white? • Clouds consist of water droplets and very tiny ice • At sunset, the sun particles is low on the • The water droplets and ice scatter the sunlight horizon • Scattering by water and ice (particles) is very • When looking at the different from scattering by molecules sun it appears red • The atoms are smaller than the wavelength of because much of light, but the ice and water particles are larger the blue light is • Scattering by particles does not favor any scattered out particular wavelength so the white light from the leaving only the red sun is scattered equally Æ clouds are white! 13 14 Mirrors Î reflection The law of reflection • Light does not pass thru metals – it is reflected • The angle of reflection = angle of incidence at the surface • Incident ray, reflected ray and normal all lie • Two types of reflection: diffuse and specular in the same plane normal i r reflected Incident ray ray Diffuse reflection: Specular reflection: Sharp image mirror Fuzzy or no image 15 16 You only need a mirror half as tall as image formation by plane mirrors you are to see your whole self The rays appear to originate from the image behind the Homer’s image Homer mirror. Of course, there is no light behind the mirror Æ this is called a virtual image Mirrors appear to make rooms look larger. 17 18 3 The image of your right Spherical or curved mirrors hand is your left hand Concave mirror Focus AMBULANCE is painted parallel light rays are focused to one point backward so that you see it correctly in your real- view mirror 19 20 Where is the light bulb? convex mirror image of light bulb light bulb F focus f f A concave mirror will form a real image of an object placed at twice its focal length at a distance of twice the focal length. It will be inverted parallel rays diverge from a focus behind and the same size as the object. the mirror 21 22 Dish antennas Magnifying mirrors signal from Homer’s satellite image Homer detector at when something placed within the focus of a concave the focal mirror, an enlarged, upright image is formed. point of the dish this principle is used in a shaving or makeup mirror 23 24 4 Convex mirrors: wide angle view Object Image A convex lens provides a wide angle view. Since it sees more, the images are reduced in size. Passenger side mirrors are often of this type with the warning: “objects appear further than they actually are". Because they appear smaller they look further away. 25 5.
Recommended publications
  • 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.
    [Show full text]
  • Some Diffuse Reflection Problems in Radiation Aerodynamics Stephen Nathaniel Falken Iowa State University
    Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1964 Some diffuse reflection problems in radiation aerodynamics Stephen Nathaniel Falken Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Aerospace Engineering Commons Recommended Citation Falken, Stephen Nathaniel, "Some diffuse reflection problems in radiation aerodynamics " (1964). Retrospective Theses and Dissertations. 3848. https://lib.dr.iastate.edu/rtd/3848 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. This dissertation has been 65-4604 microfilmed exactly as received FALiKEN, Stephen Nathaniel, 1937- SOME DIFFUSE REFLECTION PROBLEMS IN RADIATION AERODYNAMICS. Iowa State University of Science and Technology Ph.D., 1964 Engineering, aeronautical University Microfilms, Inc., Ann Arbor, Michigan SOME DIFFUSE REFLECTIOU PROBLEMS IN RADIATION AERODYNAMICS "by Stephen Nathaniel Falken A Dissertation Submitted to the Graduate Faculty in Partial Fulfillment of The Requirements for the Degree of DOCTOR OF HîILOSOEHï Major Subjects: Aerospace Engineering Mathematics Approved: Signature was redacted for privacy. Cmrg^Vf Major Work Signature was redacted for privacy. Heads of Mgjor Departments Signature was redacted for privacy. De of Gradu^ e College Iowa State University Of Science and Technology Ames, loTfa 196k ii TABLE OF CONTENTS page DEDICATION iii I. LIST OF SYMBOLS 1 II. INTRODUCTION. 5 HI. GENERAL AERODYNAMIC FORCE ANALYSIS 11 IV. THE THEORY OF RADIATION AERODYNAMICS Ik A.
    [Show full text]
  • 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.
    [Show full text]
  • Ap Physics 2 Summary Chapter 21 – Reflection and Refraction
    AP PHYSICS 2 SUMMARY CHAPTER 21 – REFLECTION AND REFRACTION . Light sources and light rays Light Bulbs, candles, and the Sun are examples of extended sources that emit light. Light from such sources illuminates other objects, which reflect the light. We see an object because incident light reflects off of it and reaches our eyes. We represent the travel of light rays (drawn as lines and arrows). Each point of a shining object or a reflecting object send rays in all directions. Law of reflection When a ray strikes a smooth surface such as a mirror, the angle between the incident ray and the normal line perpendicular to the surface equals the angle between the reflected ray and the normal line (the angle of incidence equals the angle of reflection). This phenomenon is called specular reflection. Diffuse reflection If light is incident on an irregular surface, the incident light is reflected in many different directions. This phenomenon is called diffuse reflection. Refraction If the direction of travel of light changes as it moves from one medium to another, the light is said to refract (bend) as it moves between the media. Snell’s law Light going from a lower to a higher index of refraction will bend toward the normal, but going from a higher to a lower index of refraction it will bend away from the normal. Total internal reflection If light tries to move from a more optically dense medium 1 of refractive index n1 into a less optically dense medium 2 of refractive index n2 (n1>n2), the refracted light in medium 2 bends away from the normal line.
    [Show full text]
  • Method for Measuring Solar Reflectance of Retroreflective Materials Using Emitting-Receiving Optical Fiber
    Method for Measuring Solar Reflectance of Retroreflective Materials Using Emitting-Receiving Optical Fiber HiroyukiIyota*, HidekiSakai, Kazuo Emura, orio Igawa, Hideya Shimada and obuya ishimura, Osaka City University Osaka, Japan *Corresponding author email: [email protected] ABSTRACT The heat generated by reflected sunlight from buildings to surrounding structures or pedestrians can be reduced by using retroreflective materials as building exteriors. However, it is very difficult to evaluate the solar reflective performance of retroreflective materials because retroreflective lightcannotbe determined directly using the integrating sphere measurement. To solve this difficulty, we proposed a simple method for retroreflectance measurementthatcan be used practically. A prototype of a specialapparatus was manufactured; this apparatus contains an emitting-receiving optical fiber and spectrometers for both the visible and the infrared bands. The retroreflectances of several types of retroreflective materials are measured using this apparatus. The measured values correlate well with the retroreflectances obtained by an accurate (but tedious) measurement. The characteristics of several types of retroreflective sheets are investigated. Introduction Among the various reflective characteristics, retroreflective materials as shown in Fig.1(c) have been widely used in road signs or work clothes to improve nighttime visibility. Retroreflection was given by some mechanisms:prisms, glass beads, and so on. The reflective performance has been evaluated from the viewpointof these usages only. On the other hand, we have shown thatretroreflective materials reduce the heatgenerated by reflected sunlight(Sakai, in submission). The use of such materials on building exteriors may help reduce the urban heatisland effect. However, itis difficultto evaluate the solar reflective performance of retroreflective materials because retroreflectance cannot be determined using Figure 1.
    [Show full text]
  • 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.
    [Show full text]
  • FTIR Reflection Techniques
    FT-IR Reflection Techniques Vladimír Setnička Overview – Main Principles of Reflection Techniques Internal Reflection External Reflection Summary Differences Between Transmission and Reflection FT-IR Techniques Transmission: • Excellent for solids, liquids and gases • The reference method for quantitative analysis • Sample preparation can be difficult Reflection: • Collect light reflected from an interface air/sample, solid/sample, liquid/sample • Analyze liquids, solids, gels or coatings • Minimal sample preparation • Convenient for qualitative analysis, frequently used for quantitative analysis FT-IR Reflection Techniques Internal Reflection Spectroscopy: Attenuated Total Reflection (ATR) External Reflection Spectroscopy: Specular Reflection (smooth surfaces) Combination of Internal and External Reflection: Diffuse Reflection (DRIFTs) (rough surfaces) FT-IR Reflection Techniques • Infrared beam reflects from a interface via total internal reflectance • Sample must be in optical contact with the crystal • Collected information is from the surface • Solids and powders, diluted in a IR transparent matrix if needed • Information provided is from the bulk matrix • Sample must be reflective or on a reflective surface • Information provided is from the thin layers Attenuated Total Reflection (ATR) - introduced in the 1960s, now widely used - light introduced into a suitable prism at an angle exceeding the critical angle for internal reflection an evanescent wave at the reflecting surface • sample in close contact Single Bounce ATR with IRE
    [Show full text]
  • Reflectance IR Spectroscopy, Khoshhesab
    11 Reflectance IR Spectroscopy Zahra Monsef Khoshhesab Payame Noor University Department of Chemistry Iran 1. Introduction Infrared spectroscopy is study of the interaction of radiation with molecular vibrations which can be used for a wide range of sample types either in bulk or in microscopic amounts over a wide range of temperatures and physical states. As was discussed in the previous chapters, an infrared spectrum is commonly obtained by passing infrared radiation through a sample and determining what fraction of the incident radiation is absorbed at a particular energy (the energy at which any peak in an absorption spectrum appears corresponds to the frequency of a vibration of a part of a sample molecule). Aside from the conventional IR spectroscopy of measuring light transmitted from the sample, the reflection IR spectroscopy was developed using combination of IR spectroscopy with reflection theories. In the reflection spectroscopy techniques, the absorption properties of a sample can be extracted from the reflected light. Reflectance techniques may be used for samples that are difficult to analyze by the conventional transmittance method. In all, reflectance techniques can be divided into two categories: internal reflection and external reflection. In internal reflection method, interaction of the electromagnetic radiation on the interface between the sample and a medium with a higher refraction index is studied, while external reflectance techniques arise from the radiation reflected from the sample surface. External reflection covers two different types of reflection: specular (regular) reflection and diffuse reflection. The former usually associated with reflection from smooth, polished surfaces like mirror, and the latter associated with the reflection from rough surfaces.
    [Show full text]
  • Emission and Reflection from the Ocean and Land Surfaces 1
    Lecture 5 Emission and reflection from the ocean and land surfaces Objectives: 1. Interaction of radiation with the surfaces. 2. Emission from the ocean and land surfaces. 3. Reflection from the ocean and land surfaces. Required reading: G: 4.3, 4.4, 4.5 Additional reading: CNES online tutorial Chapters 5-6 http://ceos.cnes.fr:8100/cdrom-00/ceos1/science/baphygb/intro/content.htm 1. Interaction of radiation and the surfaces. The ocean and land surfaces can modify the atmospheric radiation field by a) reflecting a portion of the incident radiation back into the atmosphere; b) transmitting some incident radiation; c) absorbing a portion of incident radiation (see Lecture 4, Kirchhoff’s law); d) emitting the thermal radiation (see Lecture 4, Kirchhoff’s law); INCIDENT RADIATION REFLECTED RADIATION ABSORBED RADIATION RANSMITTED RADIATION TRANSMITTED RADIATION 1 Conservation of energy requires that monochromatic radiation incident upon any surface, Ii, is either reflected, Ir, absorbed, Ia, or transmitted, It . Thus Ii = Ir + Ia + It [5.1] 1 = Ir / Ii + Ia / Ii + It / Ii = R + A+ T [5.2] where T is the transmission, A is the absorption, and R is the reflection of the surface. In general, T, A, and R are a function of the wavelength: Rλ + Aλ+ Tλ =1 [5.3] Blackbody surfaces (no reflection) and surfaces in LTE (from Kirchhoff’s law): Aλ = ελ [5.4] Opaque surfaces (no transmission): Rλ + Aλ = 1 [5.5] Thus for the opaque surfaces ελ = 1- Rλ [5.6] 2. Emission from the ocean and land surfaces. Emissivity of the surfaces: • In general, emissivity depends on the direction of emission, surface temperature, wavelength and some physical properties of the surface • In the thermal IR (4µm<λ< 100µm), nearly all surfaces are efficient emitters with the emissivity > 0.8 and their emissivity does not depend on the direction.
    [Show full text]
  • Reflection and Refraction
    Fi Reflection and A thi Refraction wa en at th los Th hen you shine a beam of light on a mir- ref rot the light doesn't travel through the dii Wmurmur. but a returned by the mirror's mutate bact into the ad Aben sound aases strike a canyon wall. they return to you as an echo. When a transverse wave transmitted along Changes tn lasaht speed produce a spring reaches a wall. it rrverNes direction In all these situations. refraction. waves remain in one medium rather than enter a new medium. These waves are reflected. In other situations, as when light passes from air into water, waves travel from one medium into another. When waves strike the surface of a medium at an angle, their direction changes as they enter the second medium. These waves are refracted. This is evident when a pencil in a glass of water appears to be bent. Usually waves are partly reflected and partly refracted when they wa fall on a transparent medium. When light shines on water, for exam- refl ple, some of the light is reflected and some is refracted. To under- pet stand this, let's see how reflection occurs. refl dic the 29.1 Reflection When a wave reaches a boundary between two media, some or all of the wave bounces back into the first medium. This is reflection. 21 For example, suppose you fasten a spring to a wall and send a pulse along the spring's length (Figure 29.1). The wall is a very rigid In medium compared with the spring.
    [Show full text]
  • Specular Reflectance – Theory and Applications
    Specular Reflectance – Theory and Applications Specular reflectance sampling in FTIR represents a very important At the reflective substrate, the beam reflects back to the technique useful for the measurement of thin films on reflective surface of the thin film. When the beam exits the thin film it has substrates, the analysis of bulk materials and the measurement of geometrically passed through the film twice and is now represented mono-molecular layers on a substrate material. Often this technique as IA. Infrared energy is absorbed at characteristic wavelengths as provides a means of sample analysis with no sample preparation – this beam passes through the thin film and its spectrum is recorded. keeping the sample intact for subsequent measurements. The specular reflectance spectra produced from relatively thin The basics of the sampling technique involve measurement films on reflective substrates measured at near-normal angle of of the reflected energy from a sample surface at a given angle of incidence are typically of high quality and very similar to spectra incidence. The electromagnetic and physical phenomena which obtained from a transmission measurement. This result is expected occur at and near the surface are dependent upon the angle of as the intensity of IA is high relative to the specular component (IR ). incidence of the illuminating beam, refractive index and thickness of the sample and other sample and experimental conditions. A discussion of all of the physical parameters and considerations surrounding the specular reflectance
    [Show full text]
  • Chapter 22 Reflection and Refraction of Light Wavelength the Distance Between Any Two Crests of the Wave Is Defined As the Wavel
    Chapter 22 Reflection and Refraction of Light Wavelength Dual Nature of Light The distance between any two crests of the • Experiments can be devised that will wave is defined as the wavelength display either the wave nature or the particle nature of light • Nature prevents testing both qualities at the same time Geometric Optics – Using a Ray The Nature of Light Approximation • “Particles” of light are called photons • Light travels in a straight-line path in a • Each photon has a particular energy homogeneous medium until it –E = h ƒ encounters a boundary between two – h is Planck’s constant different media • h = 6.63 x 10-34 J s •The ray approximation is used to – Encompasses both natures of light represent beams of light • Interacts like a particle •A ray of light is an imaginary line drawn • Has a given frequency like a wave along the direction of travel of the light beams Ray Approximation Geometric Optics •A wave front is a surface passing through points of a wave that have the same phase and amplitude • The rays, corresponding to the direction of the wave motion, are perpendicular to the wave fronts Reflection QUICK QUIZ 22.1 Diffuse refection: The objects has irregularities that spread out an initially parallel beam of Which part of the figure below shows specular reflection of light in all directions to produce light from the roadway? diffuse reflection Specular reflection (mirror): When a parallel beam of light is directed at a smooth surface, it is specularly reflected in only one direction. The color of an object we see depends on two things: Law of Reflection The angle of incidence = the angle of reflection The kind of light falling on it and nature of its surface For instance, if white light is used to illuminate an object that absorbs all color other than red, the object will appear red.
    [Show full text]