Speckle phenomenon and its potential for metrology
|
|
- Asher York
- 5 years ago
- Views:
Transcription
1 Joint International Physics Summer School Optics (Olomouc, August 28 September 01, 2017) Speckle phenomenon and its potential for metrology Pavel Horváth* & Petr Šmíd** *Palacký University, Faculty of Science, Regional Centre of Advanced Technologies and Materials, Joint Laboratory of Optics of Palacky University and Institute of Physics AS CR, 17. listopadu 1192/12, Olomouc, Czech Republic **Institute of Physics of the Czech Academy of Sciences, Joint Laboratory of Optics of Palacky University and Institute of Physics AS CR, 17. listopadu 50a, Olomouc, Czech Republic
2 Contents 1. Speckle and its origin. I - 2. Speckle basic properties. 3. Some applications of speckle. 4. Speckle s potential for metrology PA RT Speckle correlation method. Electronic speckle pattern interferometry. 5. Conclusion. PA RT II Pa - ve l Pe tr H or vá t Šm íd h
3 1. Speckle and its origin Speckle field: arises if an object with a rough surface is illuminated by a coherent optical beam. a result of the interference of multiple coherent spherical waves generated by point sources forming the object s surface. Speckle pattern: a chaotic (random) pattern consisting of dark and bright speckles. Illustration of a speckle field origin in case of reflection of coherent light from an object s rough surface.
4 1. Speckle and its origin Condition of speckle field origin: roughness of object s surface ( random changes of height profile Δ ) is on the scale of an optical wavelength λ of incident light: (Δ λ = 500 nm). the rough object introduces path differences greater than one wavelength of used light. The surfaces of most materials comply the condition of roughness: metals, paper, wood, rubber, plant leafs, human tissue... visibility and properties of speckle pattern then depend only on the coherence and polarization of the incident light. Physical origin of speckle (diffuse reflection of light wave from an object s rough surface).
5 2. Speckle basic properties Objective and subjective speckle: FREE SPACE O B SP JE EC C T KL IVE E SU SP BJ E C EC KL T I V E E IMAGE FIELD A) Objective and B) subjective laser speckle pattern recorded by a CMOS camera.
6 2. Speckle basic properties 2-D speckle size in the speckle pattern: The average size d of the objective speckle formed on a screen at a distance L, by reflecting (or scattering) of coherent light from a circular region of a diameter D is given by: L d 1.22 D, where λ is the wavelength of the laser light. Formation of objective speckle.
7 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of the distance L between the object plane and observation plane on the speckle size d! L1 < L2 d1 < d 2 Formation of objective speckle.
8 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of the distance L between the object plane and observation plane on the speckle size d! L1 < L2 d1 < d 2 Formation of objective speckle.
9 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of diameter D of circular illuminated region of the object s surface on the speckle size d! D1 > D2 d1 < d 2 Formation of objective speckle.
10 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of diameter D of circular illuminated region of the object s surface on the speckle size d! D1 > D2 d1 < d 2 Formation of objective speckle.
11 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of wavelength λ of incident laser light on the speckle size d! λ1 < λ2 d1 < d2 Formation of objective speckle.
12 2. Speckle basic properties 2-D speckle size in the speckle pattern: L d 1.22 D Influence of wavelength λ of incident laser light on the speckle size d! λ1 < λ2 d1 < d2 Formation of objective speckle.
13 2. Speckle basic properties 3-D speckle visualization in speckle field: [Source of the pictures: POSPĚCH, M. Shape Analysis of a Speckle in Speckle Pattern. Olomouc, s. Diploma thesis. Palacký University in Olomouc.]
14 3. Some applications of speckle Two-faced of speckle phenomenon: GOOD Dr. Jekyll EVIL Mr. Hyde [Source of the picture: Musical Jekyll & Hyde by composer Frank Wildhorn
15 3. Some applications of speckle Two-faced of speckle phenomenon: GOOD EVIL Unwanted noise during reconstruction of holograms or interferograms: Wide variety of practical applications: optics (measurement of refraction index of liquids), holography, holographic interferometry. mechanics (measurement of object s roughness and deformation), astronomy (detection of binary stars, 0 measurement of diameter of astronomical objects), biology (measurement of biological activity), ecology (detection of air pollution). Images of interferometry fringes. A) corrupted by speckle noise, and B) after speckle reduction.
16 3. Some applications of speckle BIOLOGY / ECOLOGY Monitoring of biological activity of plant using difference image of biospeckle. Optical set-up. Syngonium. Biospeckle difference images of Singonium plant (a) before, (b) two days, and (c) three weeks after giving the artificial acid rain. [Source of the pictures: KADONO, H., TAKAHASHI, G., TOYOOKA, S. Monitoring of biological activity of plant using difference image of biospeckle. In 19th Congress of the ICO, Consortini, A., Righini, G. C., eds., Proc. SPIE, 2002, 4829, pp ]
17 3. Some applications of speckle ASTRONOMY Detection of binary stars by a stellar speckle interferometry. Inventor of the technique: A. Labeyrie (1970). Interferometer = telescope (light is reflected from all parts of telescope mirror into its centre of curvature and then the speckle is arised due to interference). Laboratory simulations showing the principles of stellar speckle interferometry. (A: astronomical objects; B: short exposure photographs; C: diffraction patterns of row B; D: sum of 20 diffraction patterns.) Short exposure photographs of star α Orionis is taken on a 4 m class telescope (exposure time 10 ms; filter bandwith 10 nm). [Source of the pictures: DAINTY, J.C.,Ed., Laser Speckle and Related Phenomena. Springer-Verlag, Berlin, 1984.]
18 3. Some applications of speckle Rayleigh criterion: ASTRONOMY 1,22 D Δa angular resolution of a telescope, D diameter of a telescope mirror, λ operating wavelength. (for D = 4 m, λ = 400 nm Δa = ) Project of hypertelescope Carlina 1 (2004) Balloon altitude: 120 m, Balloon lift: 70 kg, Gondola mass: 12 kg, Mirror segments: zerodur, 250 mm diameter, spherical surface, 70 m curvature radius, Focal length: 35 m. Principle of hypertelescope. Many small mirrors are distibuted on spherical surface (green). Helium balloon carries a gondola that contains focal optics (blue). The red arrows show the light rays. Optical set-up of hypertelescope. [Source of the pictures:
Laser Speckle and Applications in Optics
Laser Speckle and Applications in Optics M. FRANCON Optics Laboratory Faculty of Sciences University of Paris Paris, France Translated by HENRI H. ARSENAULT Department of Physics Laval University Quebec,
More informationSpeckle phenomenon and its potential for metrology
Speckle phenomenon and its potential for metrology PART II Petr Šmíd Institute of Physics of the Academy of Sciences of the Czech Republic, Joint Laboratory of Optics of Palacky University and Institute
More informationOptical Systems Program of Studies Version 1.0 April 2012
Optical Systems Program of Studies Version 1.0 April 2012 Standard1 Essential Understand Optical experimental methodology, data analysis, interpretation, and presentation strategies Essential Understandings:
More informationContents Preface iii 1 Origins and Manifestations of Speckle 2 Random Phasor Sums 3 First-Order Statistical Properties
Contents Preface iii 1 Origins and Manifestations of Speckle 1 1.1 General Background............................. 1 1.2 Intuitive Explanation of the Cause of Speckle................ 2 1.3 Some Mathematical
More informationUNIT-5 EM WAVES UNIT-6 RAY OPTICS
UNIT-5 EM WAVES 2 Marks Question 1. To which regions of electromagnetic spectrum do the following wavelengths belong: (a) 250 nm (b) 1500 nm 2. State any one property which is common to all electromagnetic
More informationPRINCIPLES OF PHYSICAL OPTICS
PRINCIPLES OF PHYSICAL OPTICS C. A. Bennett University of North Carolina At Asheville WILEY- INTERSCIENCE A JOHN WILEY & SONS, INC., PUBLICATION CONTENTS Preface 1 The Physics of Waves 1 1.1 Introduction
More informationA) n L < 1.0 B) n L > 1.1 C) n L > 1.3 D) n L < 1.1 E) n L < 1.3
1. A beam of light passes from air into water. Which is necessarily true? A) The frequency is unchanged and the wavelength increases. B) The frequency is unchanged and the wavelength decreases. C) The
More informationExam 3--PHYS 202--S10
ame: Exam 3--PHYS 202--S0 Multiple Choice Identify the choice that best completes the statement or answers the question A person uses a convex lens that has a focal length of 25 cm to inspect a gem The
More informationOptics.
Optics www.optics.rochester.edu/classes/opt100/opt100page.html Course outline Light is a Ray (Geometrical Optics) 1. Nature of light 2. Production and measurement of light 3. Geometrical optics 4. Matrix
More informationEinstein Classes, Unit No. 102, 103, Vardhman Ring Road Plaza, Vikas Puri Extn., Outer Ring Road New Delhi , Ph. : ,
1 O P T I C S 1. Define resolving power of a telescope & microscope and give the expression for its resolving power. 2. Explain briefly the formation of mirage in deserts. 3. The radii of curvature of
More informationNature of Light Part 2
Nature of Light Part 2 Fresnel Coefficients From Helmholts equation see imaging conditions for Single lens 4F system Diffraction ranges Rayleigh Range Diffraction limited resolution Interference Newton
More informationUse of computer generated holograms for alignment of complex null correctors
Use of computer generated holograms for alignment of complex null correctors Rene Zehnder, James H. Burge and Chunyu Zhao College of Optical Sciences, the University of Arizona 1630 E. University Blvd,
More informationAST 101 Intro to Astronomy: Stars & Galaxies
AST 101 Intro to Astronomy: Stars & Galaxies Telescopes Mauna Kea Observatories, Big Island, HI Imaging with our Eyes pupil allows light to enter the eye lens focuses light to create an image retina detects
More informationLC circuit: Energy stored. This lecture reviews some but not all of the material that will be on the final exam that covers in Chapters
Disclaimer: Chapter 29 Alternating-Current Circuits (1) This lecture reviews some but not all of the material that will be on the final exam that covers in Chapters 29-33. LC circuit: Energy stored LC
More information7. Telescopes: Portals of Discovery Pearson Education Inc., publishing as Addison Wesley
7. Telescopes: Portals of Discovery Parts of the Human Eye pupil allows light to enter the eye lens focuses light to create an image retina detects the light and generates signals which are sent to the
More informationThe Principles of Astronomical Telescope Design
The Principles of Astronomical Telescope Design Jingquan Cheng National Radio Astronomy Observatory Charlottesville, Virginia,.USA " 4y Springer Fundamentals of Optical Telescopes 1 1.1 A Brief History
More informationHypertelescopes without delay lines.
Hypertelescopes without delay lines. V. Borkowski 1, O. Lardière 1, J. Dejonghe 1 and H. Le Coroller 2 1 LISE-Collège de France,Observatory of Haute Provence, France 2 Keck Observatory, Kamuela, Hawaii
More informationGeneral Physics II Summer Session 2013 Review Ch - 16, 17, 18
95.104 General Physics II Summer Session 2013 Review Ch - 16, 17, 18 A metal ball hangs from the ceiling by an insulating thread. The ball is attracted to a positivecharged rod held near the ball. The
More informationActive and adaptive optics for the Carlina Hypertelescope
Bulletin de la Socié Royale des Sciences de Liège - Vol. 74, 1-2-3, 2005, pp. 139-145 Active and adaptive optics for the Carlina Hypertelescope H. Le Coroller 1, V. Borkowski 1, J. Dejonghe 1 and A. Labeyrie
More informationn The visual examination of the image of a point source is one of the most basic and important tests that can be performed.
8.2.11 Star Test n The visual examination of the image of a point source is one of the most basic and important tests that can be performed. Interpretation of the image is to a large degree a matter of
More informationLecture 9: Speckle Interferometry. Full-Aperture Interferometry. Labeyrie Technique. Knox-Thompson Technique. Bispectrum Technique
Lecture 9: Speckle Interferometry Outline 1 Full-Aperture Interferometry 2 Labeyrie Technique 3 Knox-Thompson Technique 4 Bispectrum Technique 5 Differential Speckle Imaging 6 Phase-Diverse Speckle Imaging
More informationChapter 5 Telescopes
Chapter 5 Telescopes Units of Chapter 5 Telescope Design Images and Detectors The Hubble Space Telescope Telescope Size High-Resolution Astronomy Radio Astronomy Interferometry Space-Based Astronomy Full-Spectrum
More informationChapter 6 Telescopes: Portals of Discovery. Agenda. How does your eye form an image? Refraction. Example: Refraction at Sunset
Chapter 6 Telescopes: Portals of Discovery Agenda Announce: Read S2 for Thursday Ch. 6 Telescopes 6.1 Eyes and Cameras: Everyday Light Sensors How does your eye form an image? Our goals for learning How
More informationPHY410 Optics Exam #3
PHY410 Optics Exam #3 NAME: 1 2 Multiple Choice Section - 5 pts each 1. A continuous He-Ne laser beam (632.8 nm) is chopped, using a spinning aperture, into 500 nanosecond pulses. Compute the resultant
More informationVisualization of Convective Structures by Methods of the Hilbert Optics and Phase-Shift Interferometry
Visualization of Convective Structures by Methods of the Hilbert Optics and Phase-Shift Interferometry Yu.N. Dubnishchev 1, 2, V.A. Arbuzov 1, 2, E.V. Arbuzov 3, V.S. Berdnikov 1, O.S. Melekhina 2, and
More informationAstronomy 203 practice final examination
Astronomy 203 practice final examination Fall 1999 If this were a real, in-class examination, you would be reminded here of the exam rules, which are as follows: You may consult only one page of formulas
More informationPrac%ce Quiz 8. These are Q s from old quizzes. I do not guarantee that the Q s on this year s quiz will be the same, or even similar.
Prac%ce Quiz 8 These are Q s from old quizzes. I do not guarantee that the Q s on this year s quiz will be the same, or even similar. A laser beam shines vertically upwards. What laser power is needed
More informationx Contents Segmented Mirror Telescopes Metal and Lightweight Mirrors Mirror Polishing
Contents 1 Fundamentals of Optical Telescopes... 1 1.1 A Brief History of Optical Telescopes.................... 1 1.2 General Astronomical Requirements..................... 6 1.2.1 Angular Resolution.............................
More informationTelescopes (Chapter 6)
Telescopes (Chapter 6) Based on Chapter 6 This material will be useful for understanding Chapters 7 and 10 on Our planetary system and Jovian planet systems Chapter 5 on Light will be useful for understanding
More informationComputer aided measurement of biomechanical characteristics of cadaverous lumbar spines
CEJP 2(3) 2004 504 510 Computer aided measurement of biomechanical characteristics of cadaverous lumbar spines Luděk Bartoněk 1,JiříKeprt 2,Jiří Charamza 3, Lumír Hrabálek 4 1 Department of Experimental
More informationProperties of Thermal Radiation
Observing the Universe: Telescopes Astronomy 2020 Lecture 6 Prof. Tom Megeath Today s Lecture: 1. A little more on blackbodies 2. Light, vision, and basic optics 3. Telescopes Properties of Thermal Radiation
More informationTelescopes. Lecture 7 2/7/2018
Telescopes Lecture 7 2/7/2018 Tools to measure electromagnetic radiation Three essentials for making a measurement: A device to collect the radiation A method of sorting the radiation A device to detect
More informationMetrology and Sensing
Metrology and Sensing Lecture 5: Interferometry I 06--09 Herbert Gross Winter term 06 www.iap.uni-jena.de Preliminary Schedule No Date Subject Detailed Content 8.0. Introduction Introduction, optical measurements,
More informationInterference- Michelson Interferometer. Interference lecture by Dr. T.Vishwam
Interference- Michelson Interferometer Interference lecture by Dr. T.Vishwam * Measurement of the coherence length of a spectral line * Measurement of thickness of thin transparent flakes * Measurement
More informationProbing the orbital angular momentum of light with a multipoint interferometer
CHAPTER 2 Probing the orbital angular momentum of light with a multipoint interferometer We present an efficient method for probing the orbital angular momentum of optical vortices of arbitrary sizes.
More informationChapter 6 Telescopes: Portals of Discovery
Chapter 6 Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How does your eye form an image? How do we record images? How does your eye form an image?
More information1. In Young s double slit experiment, when the illumination is white light, the higherorder fringes are in color.
TRUE-FALSE STATEMENTS: ELECTRICITY: 1. Electric field lines originate on negative charges. 2. The flux of the electric field over a closed surface is proportional to the net charge enclosed by the surface.
More informationDiscussion Review Test #2. Units 12-19: (1) (2) (3) (4) (5) (6)
Discussion Review Test #2 Units 12-19: (1) (2) (3) (4) (5) (6) (7) (8) (9) Galileo used his observations of the changing phases of Venus to demonstrate that a. the sun moves around the Earth b. the universe
More informationLight Pollution. Atmospheric Seeing. Seeing Through the Atmosphere. Atmospheric Absorption of Light
Lec 8: 2 FEB 2012 ASTR 130 - Introductory Astronomy II (Chapter 6) LAST TIME - Optics and Telescopes Basic Functions of a Telescope Reflecting v. Refracting Affects of the Atmosphere TODAY Modern Astronomical
More informationTransmission Electron Microscopy
L. Reimer H. Kohl Transmission Electron Microscopy Physics of Image Formation Fifth Edition el Springer Contents 1 Introduction... 1 1.1 Transmission Electron Microscopy... 1 1.1.1 Conventional Transmission
More informationPhysicsAndMathsTutor.com 1
PhysicsAndMathsTutor.com 1 1. The diagram shows the concave mirror of a Cassegrain reflecting telescope, together with the eyepiece lens. Complete the diagram of the telescope and mark on it the focal
More informationOptical Instruments. Chapter 25. Simple Magnifier. Clicker 1. The Size of a Magnified Image. Angular Magnification 4/12/2011
Optical Instruments Chapter 25 Optical Instruments Analysis generally involves the laws of reflection and refraction Analysis uses the procedures of geometric optics To explain certain phenomena, the wave
More informationThe science of light. P. Ewart
The science of light P. Ewart Oxford Physics: Second Year, Optics Parallel reflecting surfaces t images source Extended source path difference xcos 2t=x Fringes localized at infinity Circular fringe constant
More informationOptical Sciences Center, Rm 704 University of Arizona Tucson, AZ Office Hours: Call for appointment or see after class
Term: Spring 2000 Course #: OPTI 505 Course Title: Diffraction and Interferometry Instructor: James C. Wyant Optical Sciences Center, Rm 704 University of Arizona Tucson, AZ 85721 Phone: 520-621-2448 E-Mail:
More informationApplication of nondiffracting beams to wireless optical communications
Application of nondiffracting beams to wireless optical communications V. Kollárová a, T. Medřík a, R. Čelechovský a, Z. Bouchal a O. Wilfert* b, Z. Kolka b a Faculty of Science, Palacký University, 17.
More informationTechniques for direct imaging of exoplanets
Techniques for direct imaging of exoplanets Aglaé Kellerer Institute for Astronomy, Hawaii 1. Where lies the challenge? 2. Contrasts required for ground observations? 3. Push the contrast limit Recycle!
More informationPrac%ce Quiz 8. These are Q s from old quizzes. I do not guarantee that the Q s on this year s quiz will be the same, or even similar.
Prac%ce Quiz 8 These are Q s from old quizzes. I do not guarantee that the Q s on this year s quiz will be the same, or even similar. A laser beam shines vertically upwards. What laser power is needed
More informationChapter 3 Telescopes 2/19/2014. Lecture Outline. 3.1 Optical Telescopes. 3.1 Optical Telescopes. Units of Chapter Optical Telescopes
Lecture Outline Chapter 3 Telescopes Images can be formed through reflection or refraction. Reflecting mirror Chapter 3 Telescopes Refracting lens Units of Chapter 3 Optical Telescopes Telescope Size High-Resolution
More informationRefraction is the bending of light when it passes from one substance into another. Your eye uses refraction to focus light.
Telescopes Portals of Discovery Chapter 6 Lecture The Cosmic Perspective 6.1 Eyes and Cameras: Everyday Light Sensors How do eyes and cameras work? Seventh Edition Telescopes Portals of Discovery The Eye
More informationPhysics of Light and Optics
Physics of Light and Optics Justin Peatross and Harold Stokes Brigham Young University Department of Physics and Astronomy All Publication Rights Reserved (2001) Revised April 2002 This project is supported
More informationWebster Cash University of Colorado. X-ray Interferometry
Webster Cash University of Colorado X-ray Interferometry Co-Investigators Steve Kahn - Columbia University Mark Schattenburg - MIT David Windt - Lucent (Bell-Labs) Outline of Presentation Science Potential
More informationFACULTY OF SCIENCE DEPARTMENT OF APPLIED PHYSICS AND ENGINEERING MATHEMATICS DATE: 3/12/2015 SESSION 11:30 14:30 DURATION: 3 HOURS MARKS: 110
FACULTY OF SCIENCE DEPARTMENT OF APPLIED PHYSICS AND ENGINEERING MATHEMATICS MODULE CAMPUS PHY1DB1 DFC EXAM DECEMBER 2015 DATE: 3/12/2015 SESSION 11:30 14:30 ASSESSOR(S) INTERNAL MODERATOR DR S.M. RAMAILA
More informationMetrology and Sensing
Metrology and Sensing Lecture 5: Interferometry I 08--6 Herbert Gross Winter term 08 www.iap.uni-jena.de Schedule Optical Metrology and Sensing 08 No Date Subject Detailed Content 6.0. Introduction Introduction,
More informationVersion 087 EX4 ditmire (58335) 1
Version 087 EX4 ditmire (58335) This print-out should have 3 questions. Multiple-choice questions ma continue on the next column or page find all choices before answering. 00 (part of ) 0.0 points A material
More informationBIOSPECKLE SIZE AND CONTRAST MEASUREMENT APPLICATION IN PARTICLE SIZING AND CONCENTRATION ASSESSMENT
BIOPHYSICS BIOSPECKLE SIZE AND CONTRAST MEASUREMENT APPLICATION IN PARTICLE SIZING AND CONCENTRATION ASSESSMENT D. CHICEA Lucian Blaga University, Faculty of Science, Dr. I. Ratiu Street, No. 5 7, 550024,
More informationAstronomy. Optics and Telescopes
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Optics and Telescopes - Refraction, lenses and refracting telescopes - Mirrors and reflecting telescopes - Diffraction limit,
More informationLecture 9: Introduction to Diffraction of Light
Lecture 9: Introduction to Diffraction of Light Lecture aims to explain: 1. Diffraction of waves in everyday life and applications 2. Interference of two one dimensional electromagnetic waves 3. Typical
More informationOPTICAL INSTRUMENTS VERY SHORT ANSWER QUESTIONS
OPTICAL INSTRUMENTS VERY SHORT ANSWER QUESTIONS Q-1. The difference in the focal lengths of the two lenses is larger in which case microscope or telescope? Q-2. What is the formula for angular magnification
More informationMetrology and Sensing
Metrology and Sensing Lecture 5: Interferometry I 017-11-16 Herbert Gross Winter term 017 www.iap.uni-jena.de Preliminary Schedule No Date Subject Detailed Content 1 19.10. Introduction Introduction, optical
More informationTelescopes. Astronomy 320 Wednesday, February 14, 2018
Telescopes Astronomy 320 Wednesday, February 14, 2018 Telescopes gather light and resolve detail A telescope is sometimes called a light bucket. Number of photons collected per second is proportional to
More information1. Give short answers to the following questions. a. What limits the size of a corrected field of view in AO?
Astronomy 418/518 final practice exam 1. Give short answers to the following questions. a. What limits the size of a corrected field of view in AO? b. Describe the visibility vs. baseline for a two element,
More informationTelescopes: Portals of Discovery Pearson Education, Inc.
Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes and cameras work? The Eye Refraction Incoming light ray Air Glass Refraction is the bending
More informationImaging through Kolmogorov model of atmospheric turbulence for shearing interferometer wavefront sensor
Imaging through Kolmogorov model of atmospheric turbulence for shearing interferometer wavefront sensor M.Mohamed Ismail 1 M.Mohamed Sathik 2 1Research Scholar, Department of Computer Science, Sadakathullah
More informationOptical Shop Testing
Optical Shop Testing nd Edition (199 ) Edited by Daniel Malacara 1 OUTLINE Chapter 1. Newton, Fizeau, and Haidinger Interferometer 1.1 1. Fizeau Interferometer 1.3 Haidinger Interferometer 1.4 Absolute
More informationAstronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION
Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION CHAPTER 3 Telescopes Lecture Presentation 3.0 Imaging the universe Our original observations of the universe depended on our eyes! What other
More informationChapter 6 Lecture. The Cosmic Perspective. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Telescopes Portals of Discovery 2014 Pearson Education, Inc. Telescopes Portals of Discovery CofC Observatory 6.1 Eyes and Cameras: Everyday Light Sensors Our goals
More informationChapter 6 Lecture. The Cosmic Perspective Seventh Edition. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Seventh Edition Telescopes Portals of Discovery Telescopes Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes
More informationFourier Transform Spectrograph Development Project
Fourier Transform Spectrograph Development Project NARIT Research Colloquium / Research Project Evaluation 2018 August 2 nd, Flora Creek Hotel, Chiangmai C. Buisset 1, P. Artsang 2, P. Meemon 2, 1 National
More information2. Determine the excess charge on the outer surface of the outer sphere (a distance c from the center of the system).
Use the following to answer question 1. Two point charges, A and B, lie along a line separated by a distance L. The point x is the midpoint of their separation. 1. Which combination of charges will yield
More informationHypertelescope Optical Observatory
Hypertelescope Optical Observatory Antoine Labeyrie Collège de France & Observatoire de la Côte d Azur Laboratoire d Interféromètrie Stellaire et Exoplanétaire simulated direct image of Earth at 3 pc 30mn
More informationElectricity & Optics
Physics 24100 Electricity & Optics Lecture 26 Chapter 33 sec. 1-4 Fall 2017 Semester Professor Koltick Interference of Light Interference phenomena are a consequence of the wave-like nature of light Electric
More informationMichelson Interferometer
Michelson Interferometer Objective Determination of the wave length of the light of the helium-neon laser by means of Michelson interferometer subsectionprinciple and Task Light is made to produce interference
More informationOptics Optical Testing and Testing Instrumentation Lab
Optics 513 - Optical Testing and Testing Instrumentation Lab Lab #6 - Interference Microscopes The purpose of this lab is to observe the samples provided using two different interference microscopes --
More informationASTR 1120 General Astronomy: Stars & Galaxies
ASTR 1120 General Astronomy: Stars & Galaxies!AST CLASS Learning from light: temperature (from continuum spectrum) chemical composition (from spectral lines) velocity (from Doppler shift) "ODA# Detecting
More informationAstr 2310 Thurs. March 3, 2016 Today s Topics
Astr 2310 Thurs. March 3, 2016 Today s Topics Chapter 6: Telescopes and Detectors Optical Telescopes Simple Optics and Image Formation Resolution and Magnification Invisible Astronomy Ground-based Radio
More informationMIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova
MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the
More informationStrain Analysis by Digital Shearography on an Aluminium Plate with a Geometric Defect under Thermal Loading
Journal of Stress Analysis Vol. 1, No. 1, Spring Summer 2016 Strain Analysis by Digital Shearography on an Aluminium Plate with a Geometric Defect under Thermal Loading R. Moharrami, M. Taghiloo, A. Darud
More informationFoundations of Astronomy 13e Seeds. Chapter 6. Light and Telescopes
Foundations of Astronomy 13e Seeds Chapter 6 Light and Telescopes Guidepost In this chapter, you will consider the techniques astronomers use to study the Universe What is light? How do telescopes work?
More informationThe well-composed image was recorded over a period of nearly 2 hours as a series of 30 second long, consecutive exposures on the night of October 5.
Happy Thursday! The well-composed image was recorded over a period of nearly 2 hours as a series of 30 second long, consecutive exposures on the night of October 5. The exposures were made with a digital
More informationExoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges
Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak
More informationMetrology and Sensing
Metrology and Sensing Lecture 5: Interferometry I 07--6 Herbert Gross Winter term 07 www.iap.uni-jena.de Preliminary Schedule No Date Subject Detailed Content 9.0. Introduction Introduction, optical measurements,
More informationLecture 11: Introduction to diffraction of light
Lecture 11: Introduction to diffraction of light Diffraction of waves in everyday life and applications Diffraction in everyday life Diffraction in applications Spectroscopy: physics, chemistry, medicine,
More informationEngineering Physics 1 Prof. G.D. Vermaa Department of Physics Indian Institute of Technology-Roorkee
Engineering Physics 1 Prof. G.D. Vermaa Department of Physics Indian Institute of Technology-Roorkee Module-04 Lecture-02 Diffraction Part - 02 In the previous lecture I discussed single slit and double
More informationIndicate whether each statement is true or false by circling your answer. No explanation for your choice is required. Each answer is worth 3 points.
Physics 5B FINAL EXAM Winter 2009 PART I (15 points): True/False Indicate whether each statement is true or false by circling your answer. No explanation for your choice is required. Each answer is worth
More informationLaboratory Exercise 7 MEASUREMENTS IN ASTRONOMY
Laboratory Exercise 7 MEASUREMENTS IN ASTRONOMY Introduction Part A: The angular resolution of telescopes For astronomical observations, reflecting telescopes have replaced the refracting type of instrument.
More informationLow Coherence Vibration Insensitive Fizeau Interferometer
Low Coherence Vibration Insensitive Fizeau Interferometer Brad Kimbrough, James Millerd, James Wyant, John Hayes 4D Technology Corporation, 3280 E. Hemisphere Loop, Suite 146, Tucson, AZ 85706 (520) 294-5600,
More informationTelescopes: Portals of Discovery
Telescopes: Portals of Discovery How do light and matter interact? Emission Absorption Transmission Transparent objects transmit light Opaque objects block (absorb) light Reflection or Scattering Reflection
More informationMichelson Interferometer. crucial role in Einstein s development of the Special Theory of Relativity.
Michelson Interferometer The interferometer Michelson experiment Interferometer of Michelson and Morley played 0 a crucial role in Einstein s development of the Special Theory of Relativity. Michelson
More informationDiffraction I. Physics 2415 Lecture 37. Michael Fowler, UVa
Diffraction I Physics 2415 Lecture 37 Michael Fowler, UVa Today s Topics Michelson s interferometer The Michelson Morley experiment Single-slit diffraction Eye of a fly Angular resolution Michelson Interferometer
More informationLecture Outlines. Chapter 5. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 5 Astronomy Today 8th Edition Chaisson/McMillan Chapter 5 Telescopes Units of Chapter 5 5.1 Optical Telescopes 5.2 Telescope Size 5.3 Images and Detectors 5.4 High-Resolution Astronomy
More informationBureau International des Poids et Mesures. Rapport BIPM -89/1
Bureau International des Poids et Mesures Rapport BIPM -89/1 Shape Measurements of Standard Length Scales Using Interferometry with Small Angles of Incidence by Lennart Robertsson Abstract An interferometric
More informationOptical Shop Testing. Second Edition. Edited by DANIEL MALACARA. John Wiley & Sons, Inc. A Wiley-Interscience Publication
Optical Shop Testing Second Edition Edited by DANIEL MALACARA A Wiley-Interscience Publication John Wiley & Sons, Inc. New York I Chichester I Brisbane I Toronto I Singapore Contents Preface to the Second
More informationAS750 Observational Astronomy
Lecture 9 0) Poisson! (quantum limitation) 1) Diffraction limit 2) Detection (aperture) limit a)simple case b)more realistic case 3) Atmosphere 2) Aperture limit (More realistic case) Aperture has m pixels
More informationAstronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes
Astronomical Tools Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes Laws of Refraction and Reflection Law of Refraction n 1 sin θ 1
More informationBLUE-PRINT II XII Physics
BLUE-PRINT II XII Physics S.No. UNIT VSA SA I SA II LA Total (1 Mark) (2 Marks) (3Marks) (5 Marks) 1. Electrostatics 1(1) 4(2) 3(1) - 8(4) 2. Current Electricity - 2(1) - 5(1) 7(2) 3. Magnetic Effect of
More informationMicro-fluctuations of Fried s parameter (r 0 )
Micro-fluctuations of Fried s parameter ( ) S. K. Saha and L. Yeswanth Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India e-mail: sks@iiap.res.in; sks@iiap.ernet.in The atmospheric
More informationMore Optical Telescopes
More Optical Telescopes There are some standard reflecting telescope designs used today All have the common feature of light entering a tube and hitting a primary mirror, from which light is reflected
More informationPhys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5
Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5 MULTIPLE CHOICE 1. What is the wavelength of the longest wavelength light visible to the human eye? a. 400 nm b. 4000 nm c. 7000 nm
More informationPH 222-3A Spring 2010
PH -3A Spring 010 Interference Lecture 6-7 Chapter 35 (Halliday/Resnick/Walker, Fundamentals of Physics 8 th edition) 1 Chapter 35 Interference The concept of optical interference is critical to understanding
More informationChapter 16 Holography
Chapter 16 Holography Virtually all recording devices for light respond to light intensity. Problem: How to record, and then later reconstruct both the amplitude and phase of an optical wave. [This question
More information