Part 1 - Basic Interferometers for Optical Testing
|
|
- Alison Wiggins
- 5 years ago
- Views:
Transcription
1 Part 1 - Basic Interferometers for Optical Testing Two Beam Interference Fizeau and Twyman-Green interferometers Basic techniques for testing flat and spherical surfaces Mach-Zehnder Zehnder,, Scatterplate and Smartt Interferometers Shearing Interferometers Typical Interferograms James C. Wyant Part 1 Page 1 of 43 Two-Beam Interference Fringes I = I 1 + I I 1 I 2 cos(α 1 α 2 ) α 1 α 2 is the phase difference between the two interfering beams α 1 α 2 = ( 2 π )(optical path difference) λ James C. Wyant Part 1 Page 2 of 43
2 Sinusoidal Interference Fringes I = I 1 + I I 1 I 2 cos(α 1 α 2 ) James C. Wyant Part 1 Page 3 of 43 Pioneer Fizeau Interferometer 1862 Light Source Beamsplitter Eye Test Surface Lens Reference Surface James C. Wyant Part 1 Page 4 of 43
3 Typical Interferogram Obtained using Fizeau Interferometer James C. Wyant Part 1 Page 5 of 43 Relationship between Surface Height Error and Fringe Deviation S (x,y) λ Surface height error = ( )( ) 2 S James C. Wyant Part 1 Page 6 of 43
4 Fizeau Fringes Hole Bump 1 Top View Reference Test For a given fringe the separation between the two surfaces is a constant. 1 Top View Reference Test Height error = (λ/2)( /S) S Interferogram S Interferogram James C. Wyant Part 1 Page 7 of 43 Fizeau Fringes for Concave and Convex Surfaces CONCAVE SPHERE CONVEX SPHERE Thick Part of Wedge Thin Part of Wedge Reference Flat Test Sample Reference Flat Test Sample James C. Wyant Part 1 Page 8 of 43
5 Twyman-Green Interferometer (Flat Surfaces) Reference Mirror Laser Beamsplitter Test Mirror Imaging Lens Interferogram James C. Wyant Part 1 Page 9 of 43 Twyman-Green Interferometer (Spherical Surfaces) Laser Beamsplitter Reference Mirror Diverger Lens Imaging Lens Test Mirror Interferogram Incorrect Spacing Correct Spacing James C. Wyant Part 1 Page 10 of 43
6 Typical Interferogram James C. Wyant Part 1 Page 11 of 43 Fizeau Interferometer-Laser Source (Flat Surfaces) Beam Expander Reference Surface Laser Imaging Lens Test Surface Interferogram James C. Wyant Part 1 Page 12 of 43
7 Fizeau Interferometer-Laser Source (Spherical Surfaces) Beam Expander Reference Surface Laser Imaging Lens Interferogram Diverger Lens Test Mirror James C. Wyant Part 1 Page 13 of 43 Testing High Reflectivity Surfaces Beam Expander Reference Surface Laser Imaging Lens Diverger Lens Attenuator Interferogram Test Mirror James C. Wyant Part 1 Page 14 of 43
8 Mach-Zehnder Interferometer Sample Imaging Lens Interferogram Laser Beamsplitter Testing samples in transmission James C. Wyant Part 1 Page 15 of 43 Laser Beam Wavefront Measurement Reference Arm Input Source Pinhole PZT Test Arm Detector Array James C. Wyant Part 1 Page 16 of 43
9 Scatterplate Interferometer Four Terms: Scattered-Scattered Scattered-Direct Direct-Scattered Direct-Direct Source High magnification image. of a scatterplate Interferogram Scatterplate (Near center of curvature of mirror being tested) Scatterplate has inversion symmetry Scatterplate is located at center of curvature of test mirror Direct-scattered and scattered-direct beams produce fringes Mirror Being Tested James C. Wyant Part 1 Page 17 of 43 Microscopic Image of Scatterplate James C. Wyant Part 1 Page 18 of 43
10 Scatterplate Interferometer James C. Wyant Part 1 Page 19 of 43 Scatterplate Interferograms James C. Wyant Part 1 Page 20 of 43
11 Smartt Point Diffraction Interferometer Lens under Test Reference & Aberrated Wavefronts Source PDI Interferogram James C. Wyant Part 1 Page 21 of 43 Lateral Shear Interferometry Measures wavefront slope Shear Plate Source Collimator Lens Interferogram Shear = x James C. Wyant Part 1 Page 22 of 43
12 Lateral Shear Fringes W( x,y)is wavefront being measured Bright fringe obtained when W(x + x,y) W(x, y) = mλ W( x,y) x Average over shear distance ( x) = mλ Measures average value of slope over shear distance James C. Wyant Part 1 Page 23 of 43 Collimation Measurement No wedge in shear plate Not collimated Collimated (one fringe) Vertical wedge in shear plate Not collimated Collimated James C. Wyant Part 1 Page 24 of 43
13 Typical Lateral Shear Interferograms James C. Wyant Part 1 Page 25 of 43 Lateral Shear Interferometer Source Two-frequency grating placed near focus Two sheared images of exit pupil of system under test Lens under test Two diffracted cones of rays at slightly different angles Measures slope of wavefront, not wavefront shape James C. Wyant Part 1 Page 26 of 43
14 Interferogram Obtained using Grating Lateral Shear Interferometer James C. Wyant Part 1 Page 27 of 43 Rotating Grating LSI (Variable Shear) James C. Wyant Part 1 Page 28 of 43
15 Rotating Grating LSI James C. Wyant Part 1 Page 29 of 43 Shearing Interferograms (Different Shear) James C. Wyant Part 1 Page 30 of 43
16 Radial Shear Interferometry Wavefront is interfered with expanded version of itself 2S 1 2S 2 Laser S 1 Radial Shear = R = S 1 S 2 S James C. Wyant Part 1 Page 31 of 43 Analysis of Radial Shear Interferograms Wavefront being measured W ρ,θ ( )= W 020 ρ 2 + W 040 ρ 4 + W 131 ρ 3 cosθ + W 222 ρ 2 cos 2 θ Expanded beam can be written W( Rρ,θ)= W 020 (Rρ) 2 + W 040 (Rρ) 4 + W 131 (Rρ) 3 cosθ +W 222 (Rρ) 2 cos 2 θ Hence, a bright fringe is obtained whenever W( ρ,θ) W( Rρ,θ)= W 020 ρ 2 (1 R 2 ) + W 040 ρ 4 (1 R 4 ) +W 131 ρ 3 (1 R 3 )cosθ + W 222 ρ 2 (1 R 2 )cos 2 θ Same as Twyman- Green if divide each coefficient by (1- R n ) James C. Wyant Part 1 Page 32 of 43
17 Radial Shear Interferogram Variable Sensitivity Test Large shear - results same as for Twyman-Green Small shear - Low sensitivity test James C. Wyant Part 1 Page 33 of 43 Interferograms, Spherical Aberration Paraxial Focus Mid Focus Marginal Focus No Aberration Focal Shift Small Spherical Aberration Larger Spherical Aberration James C. Wyant Part 1 Page 34 of 43
18 Interferograms Small Astigmatism, Sagittal Focus Tilt James C. Wyant Part 1 Page 35 of 43 Interferograms Small Astigmatism, Medial Focus Tilt James C. Wyant Part 1 Page 36 of 43
19 Interferograms, Large Astigmatism, Sagittal Focus, Small Tilt Tilt James C. Wyant Part 1 Page 37 of 43 Interferograms, Large Astigmatism, Medial Focus, Small Tilt Tilt James C. Wyant Part 1 Page 38 of 43
20 Interferograms Small Coma, Large Tilt Tilt James C. Wyant Part 1 Page 39 of 43 Interferograms Large Coma, Small Tilt Tilt James C. Wyant Part 1 Page 40 of 43
21 Interferograms Large Coma, Large Tilt Tilt James C. Wyant Part 1 Page 41 of 43 Interferograms Small Focal Shift Focus Coma Sagittal Astigmatism Medial Astigmatism James C. Wyant Part 1 Page 42 of 43
22 Interferograms Combined Aberrations Spherical Coma Sph + Coma Sph + Astig Sph + Coma + Astig All wavefronts have 1 λ rms departure from bestfitting reference sphere. Astig Coma + Astig James C. Wyant Part 1 Page 43 of 43
n 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 information10.0 Absolute Measurements. Computers make it possible to perform measurements more accurate than the reference surface
10.0 Absolute Measurements Computers make it possible to perform measurements more accurate than the reference surface 10.0 Absolute Measurements n 10.0 Absolute Measurements 10.1 Flat Surfaces 10.2 Spherical
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 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 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 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 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 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 informationWavefront Sensing using Polarization Shearing Interferometer. A report on the work done for my Ph.D. J.P.Lancelot
Wavefront Sensing using Polarization Shearing Interferometer A report on the work done for my Ph.D J.P.Lancelot CONTENTS 1. Introduction 2. Imaging Through Atmospheric turbulence 2.1 The statistics of
More informationAOL Spring Wavefront Sensing. Figure 1: Principle of operation of the Shack-Hartmann wavefront sensor
AOL Spring Wavefront Sensing The Shack Hartmann Wavefront Sensor system provides accurate, high-speed measurements of the wavefront shape and intensity distribution of beams by analyzing the location and
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 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 informationiprom Optical Interferometry Prof. Dr. -Ing. Rainer Tutsch Institut für Produktionsmesstechnik IPROM Technische Universität Braunschweig
Optical Interferometry Prof. Dr. -Ing. Rainer Tutsch Institut für Produktionsmesstechnik IPROM Technische Universität Braunschweig Frontiers of Metrology April 1, 01 I P NSTITUT FÜR RODUKTIONSMESSTECHNIK
More informationFully achromatic nulling interferometer (FANI) for high SNR exoplanet characterization
Fully achromatic nulling interferometer (FANI) for high SNR exoplanet characterization François Hénault Institut de Planétologie et d Astrophysique de Grenoble Université Joseph Fourier Centre National
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 informationLAB DEMONSTRATION OF INTERFEROMETRIC
LAB DEMONSTRATION OF INTERFEROMETRIC MEASUREMENT USING A TEST PLATE AND CGH Presented to: Larry Stepp Eric Hansen The Association of Universities for Research in Astronomy, Inc. Tucson, AZ, 85726 Prepared
More informationOne-Dimensional Analysis of Lateral Shearing Interferograms
One-Dimensional Analysis of Lateral Shearing Interferograms James C. Wyant Optical Sciences Center University of Arizona Introduction Although techniques have been developed for obtaining the entire wavefront
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 informationPolarization Shearing Interferometer (PSI) Based Wavefront Sensor for Adaptive Optics Application. A.K.Saxena and J.P.Lancelot
Polarization Shearing Interferometer (PSI) Based Wavefront Sensor for Adaptive Optics Application A.K.Saxena and J.P.Lancelot Adaptive Optics A Closed loop Optical system to compensate atmospheric turbulence
More informationDirect Phase Measurement
05DirectPhaseMeasurement.nb Optics 513 - James C. Wyant (01) 1 Direct Phase Measurement DP-1 Phase shifting interferometry is used with a Twyman-Green interferometer to measure a spherical mirror. Both
More informationOptical/IR Observational Astronomy Telescopes I: Optical Principles. David Buckley, SAAO. 24 Feb 2012 NASSP OT1: Telescopes I-1
David Buckley, SAAO 24 Feb 2012 NASSP OT1: Telescopes I-1 1 What Do Telescopes Do? They collect light They form images of distant objects The images are analyzed by instruments The human eye Photographic
More informationHigh-Resolution Imagers
40 Telescopes and Imagers High-Resolution Imagers High-resolution imagers look at very small fields of view with diffraction-limited angular resolution. As the field is small, intrinsic aberrations are
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 informationIMPROVING BEAM QUALITY NEW TELESCOPE ALIGNMENT PROCEDURE
IMPROVING BEAM QUALITY NEW TELESCOPE ALIGNMENT PROCEDURE by Laszlo Sturmann Fiber coupled combiners and visual band observations are more sensitive to telescope alignment problems than bulk combiners in
More informationROTATIONAL SHEARING INTERFEROMATER. Introduction. The Interferometer. L. Yeswanth, Optics Group, IIA, Bangalore
ROTATIONAL SHEARING INTERFEROMATER L. Yeswanth, Optics Group, IIA, Bangalore Introduction A rotational shearing interferometer is a modification of the Michelson s interferometer to obtain the spatial
More information* AIT-4: Aberrations. Copyright 2006, Regents of University of California
Advanced Issues and Technology (AIT) Modules Purpose: Explain the top advanced issues and concepts in optical projection printing and electron-beam lithography. AIT-: LER and Chemically Amplified Resists
More informationAstro 500 A500/L-7 1
Astro 500 1 Telescopes & Optics Outline Defining the telescope & observatory Mounts Foci Optical designs Geometric optics Aberrations Conceptually separate Critical for understanding telescope and instrument
More informationTMT Metrology study for M2 and M3
Consultants for Optical Metrology Tucson, Arizona 1 Introduction... 2 2 Requirements for optical test hardware... 3 3 Subaperture interferometry with stitching software... 4 3.1 Fizeau interferometry...
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 informationMoonbows. Friday somebody asked if rainbows can be seen at night.
Moonbows Friday somebody asked if rainbows can be seen at night. Neil Alberding (SFU Physics) Physics 121: Optics, Electricity & Magnetism Spring 2010 1 / 25 Moonbows Friday somebody asked if rainbows
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 informationInternational Journal of Scientific & Engineering Research, Volume 4, Issue 7, July ISSN
International Journal of Scientific & Engineering Research, Volume 4, Issue 7, July-2013 96 Performance and Evaluation of Interferometric based Wavefront Sensors M.Mohamed Ismail1, M.Mohamed Sathik2 Research
More informationLecture 2: Geometrical Optics 1. Spherical Waves. From Waves to Rays. Lenses. Chromatic Aberrations. Mirrors. Outline
Lecture 2: Geometrical Optics 1 Outline 1 Spherical Waves 2 From Waves to Rays 3 Lenses 4 Chromatic Aberrations 5 Mirrors Christoph U. Keller, Utrecht University, C.U.Keller@uu.nl Astronomical Telescopes
More informationDevelopment of surface metrology for the Giant Magellan Telescope primary mirror
Development of surface metrology for the Giant Magellan Telescope primary mirror J. H. Burge a,b, W. Davison a, H. M. Martin a, C. Zhao b a Steward Observatory, University of Arizona, Tucson, AZ 85721,
More information5. Aberration Theory
5. Aberration Theory Last lecture Matrix methods in paraxial optics matrix for a two-lens system, principal planes This lecture Wavefront aberrations Chromatic Aberration Third-order (Seidel) aberration
More informationPS210 - Optical Techniques. Section VI
PS210 - Optical Techniques Section VI Section I Light as Waves, Rays and Photons Section II Geometrical Optics & Optical Instrumentation Section III Periodic and Non-Periodic (Aperiodic) Waves Section
More informationIntroduction to aberrations OPTI518 Lecture 5
Introduction to aberrations OPTI518 Lecture 5 Second-order terms 1 Second-order terms W H W W H W H W, cos 2 2 000 200 111 020 Piston Change of image location Change of magnification 2 Reference for OPD
More informationA Path to Freeform Optics. Kyle Fuerschbach University of Rochester Jannick Rolland University of Rochester Kevin Thompson Synopsys
A Path to Freeform Optics Kyle Fuerschbach University of Rochester Jannick Rolland University of Rochester Kevin Thompson Synopsys Role of Non-Symmetric/Freeform Surfaces in Optical Systems Design Packaging
More informationCHARA Meeting 2017 Pasadena, California
MORE AUTOMATION Laszlo Sturmann M7 ACTUATORS LAB. LASER ALIGNMENT TELESCOPE OPTICAL ALIGNMENT NEW ACTUATORS REMOTELY ACTUATED M7 MOUNT MOTIVATION THE PRECISION OF THE COUDE ALIGNMENT WAS NOT SUFFICIENT
More informationCOMPUTER GENERATED HOLOGRAMS Optical Sciences 627 W.J. Dallas (Monday, August 23, 2004, 12:14 PM)
COMPUTER GENERATED HOLOGRAMS Optical Sciences 67 W.J. Dallas (Monday, August 3, 4, 1:14 PM) PART IV: CHAPTER FOUR OPTICAL TESTING Part IV: Chapter Four Page 1 of 1 Introduction In optical testing an element
More informationFigure measurement of a large optical flat with a Fizeau interferometer and stitching technique
Figure measurement of a large optical flat with a Fizeau interferometer and stitching technique Chunyu Zhao a, Robert A. Sprowl a, Michael Bray b, James H. Burge a a College of Optical Sciences, the University
More informationEuclid/NISP grism qualification model AIT/AIV campaign: optical, mechanical, thermal and vibration tests
Amandine.caillat@lam.fr Euclid/NISP grism qualification model AIT/AIV campaign: optical, mechanical, thermal and vibration tests 18/10/2016 Paper 61 ICSO 2016 - Biarritz Amandine Caillat a, Anne Costille
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 informationLight as Wave Motion p. 1 Huygens' Ideas p. 2 Newton's Ideas p. 8 Complex Numbers p. 10 Simple Harmonic Motion p. 11 Polarized Waves in a Stretched
Introduction p. xvii Light as Wave Motion p. 1 Huygens' Ideas p. 2 Newton's Ideas p. 8 Complex Numbers p. 10 Simple Harmonic Motion p. 11 Polarized Waves in a Stretched String p. 16 Velocities of Mechanical
More informationDevelopment of a cryogenic compact interferometric displacement sensor
Development of a cryogenic compact interferometric displacement sensor Fabián E. Peña Arellano National Astronomical Observatory of Japan Outline of the presentation Motivation: local position sensor for
More informationEM waves and interference. Review of EM wave equation and plane waves Energy and intensity in EM waves Interference
EM waves and interference Review of EM wave equation and plane waves Energy and intensity in EM waves Interference Maxwell's Equations to wave eqn The induced polarization, P, contains the effect of the
More informationThe Diffraction Grating
The Diffraction Grating If one extends the double slit to large number of slits very closely spaced, one gets what is called a diffraction grating. d sin θ. Maxima are still at d sin θ m = mλ, m = 0, 1,
More informationReal Telescopes & Cameras. Stephen Eikenberry 05 October 2017
Lecture 7: Real Telescopes & Cameras Stephen Eikenberry 05 October 2017 Real Telescopes Research observatories no longer build Newtonian or Parabolic telescopes for optical/ir astronomy Aberrations from
More informationLecture 2: Basic Astronomical Optics. Prisms, Lenses, and Mirrors
Lecture 2: Basic Astronomical Optics Prisms, Lenses, and Mirrors Basic Optical Elements Refraction (Lenses) No longer used for large telescopes Widely used for instrument optics Reflection (mirrors) Widely
More informationVågrörelselära och optik
Vågrörelselära och optik Harmonic oscillation: Experiment Experiment to find a mathematical description of harmonic oscillation Kapitel 14 Harmonisk oscillator 1 2 Harmonic oscillation: Experiment Harmonic
More informationOPTI510R: Photonics. Khanh Kieu College of Optical Sciences, University of Arizona Meinel building R.626
OPTI510R: Photonics Khanh Kieu College of Optical Sciences, University of Arizona kkieu@optics.arizona.edu Meinel building R.626 Important announcements Homework #1 is due. Homework #2 is assigned, due
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 informationPhys 2310 Mon. Dec. 11, 2014 Today s Topics. Begin Chapter 9: Interference Reading for Next Time
Phys 30 Mon. Dec., 04 Todays Topics Begin Chapter 9: nterference Reading for Next Time Reading this Week By Wed.: Begin Ch. 9 (9. 9.3) General Considerations, Conditions for nterference, Wavefront-splitting
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 informationIncoherent wind velocity sensing with a two-beam interferometer
U-UR- 0()-4666 Incoherent wind velocity sensing with a two-beam interferometer Ralph R Berggren Los Alamos National f.oborato~, E526 iks Alms, NM87545 Phone 505-667-0593,fhx 505-665-6834, @WQMm@y David
More informationHomogeneity of optical glass
1 Version ebruary 2016 Introduction SCHOTT offers machined optical glasses with homogeneities up to H5 quality. I-Line glasses can even be offered in higher homogeneities. The achievable homogeneity depends
More informationConcave mirrors. Which of the following ray tracings is correct? A: only 1 B: only 2 C: only 3 D: all E: 2& 3
Concave mirrors Which of the following ray tracings is correct? A: only 1 B: only 2 C: only 3 D: all E: 2& 3 1 2 3 c F Point C: geometrical center of the mirror, F: focal point 2 Concave mirrors Which
More informationCorrelation of optical and generation properties of YAG: Nd 3+ rods*
Optica Applicata, Vol. XIV, No., 984 Correlation of optical and generation properties of YAG: Nd 3+ rods* JERZY CZESZKO, SŁAWOMIR KACZMAREK Institute of Quantum Electronics, Military Technical Academy,
More informationPupil matching of Zernike aberrations
Pupil matching of Zernike aberrations C. E. Leroux, A. Tzschachmann, and J. C. Dainty Applied Optics Group, School of Physics, National University of Ireland, Galway charleleroux@yahoo.fr Abstract: The
More informationEdward S. Rogers Sr. Department of Electrical and Computer Engineering. ECE426F Optical Engineering. Final Exam. Dec. 17, 2003.
Edward S. Rogers Sr. Department of Electrical and Computer Engineering ECE426F Optical Engineering Final Exam Dec. 17, 2003 Exam Type: D (Close-book + one 2-sided aid sheet + a non-programmable calculator)
More informationDesigning a Computer Generated Hologram for Testing an Aspheric Surface
Nasrin Ghanbari OPTI 521 Graduate Report 2 Designing a Computer Generated Hologram for Testing an Aspheric Surface 1. Introduction Aspheric surfaces offer numerous advantages in designing optical systems.
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 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 informationPhysical Optics. Lecture 2: Diffraction Herbert Gross.
Physical Optics Lecture : Diffraction 018-04-18 Herbert Gross www.iap.uni-jena.de Physical Optics: Content No Date Subject Ref Detailed Content 1 11.04. Wave optics G Complex fields, wave equation, k-vectors,
More information20. Aberration Theory
0. Aberration Theory Wavefront aberrations ( 파면수차 ) Chromatic Aberration ( 색수차 ) Third-order (Seidel) aberration theory Spherical aberrations Coma Astigmatism Curvature of Field Distortion Aberrations
More informationConstructive vs. destructive interference; Coherent vs. incoherent interference
Constructive vs. destructive interference; Coherent vs. incoherent interference Waves that combine in phase add up to relatively high irradiance. = Constructive interference (coherent) Waves that combine
More information= nm. = nm. = nm
Chemistry 60 Analytical Spectroscopy PROBLEM SET 5: Due 03/0/08 1. At a recent birthday party, a young friend (elementary school) noticed that multicolored rings form across the surface of soap bubbles.
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 informationHolographic Fourier Transform Spectrometer for THz Region N. I. Agladze and A. J. Sievers Laboratory of Atomic and Solid State Physics Cornell Univers
To be published in Optics Letters: Title: Holographic Fourier Transform Spectrometer for THz Region Authors: Nikolay Agladze and Albert Sievers Accepted: 6 January 2010 Posted: 26 January 2010 Doc. ID:
More informationIntroduction to aberrations OPTI 518 Lecture 14
Introduction to aberrations Lecture 14 Topics Structural aberration coefficients Examples Structural coefficients Ж Requires a focal system Afocal systems can be treated with Seidel sums Structural stop
More informationOverview of Aberrations
Overview of Aberrations Lens Design OPTI 57 Aberration From the Latin, aberrare, to wander from; Latin, ab, away, errare, to wander. Symmetry properties Overview of Aberrations (Departures from ideal behavior)
More informationInterferometric Terahertz Wavefront Analysis
IEEE JOURNAL OF SELECTED TOPICS IN QUANTUM ELECTRONICS, VOL. 23, NO. 4, JULY/AUGUST 2017 8400505 Interferometric Terahertz Wavefront Analysis Emmanuel Abraham, Takayuki Ogawa, Mathilde Brossard, and Takeshi
More informationApplications of the Abbe Sine Condition in Multi-Channel Imaging Systems
Applications of the Abbe Sine Condition in Multi-Channel Imaging Systems Barbara Kruse, University of Arizona, College of Optical Sciences May 6, 2016 Abstract Background In multi-channel imaging systems,
More informationMELOS 530 MEASURING EQUIPMENT FOR LENSES AND OPTICAL SYSTEMS. Combinations and Accessories. Indispensable for Quality Control of Optics
Combinations and Accessories Combinations/ Applications Combination 1 235 601 Combination 2 235 602 neg. focal length Combination 3 235 603 neg. focal length Combination 4 235 604 neg. focal length wedge
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 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 information2.71. Final examination. 3 hours (9am 12 noon) Total pages: 7 (seven) PLEASE DO NOT TURN OVER UNTIL EXAM STARTS PLEASE RETURN THIS BOOKLET
2.71 Final examination 3 hours (9am 12 noon) Total pages: 7 (seven) PLEASE DO NOT TURN OVER UNTIL EXAM STARTS Name: PLEASE RETURN THIS BOOKLET WITH YOUR SOLUTION SHEET(S) MASSACHUSETTS INSTITUTE OF TECHNOLOGY
More informationSimple quasi-common path point diffraction interferometer with adjustable fringe contrast and carrier frequency
J. Eur. Opt. Soc.-Rapid, 54 (5) www.jeos.org Simple quasi-common path point diffraction interferometer with adjustable fringe contrast and carrier frequency F. Z. Bai fzbaiim@63.com College of Mechanical
More informationLens Design II. Lecture 1: Aberrations and optimization Herbert Gross. Winter term
Lens Design II Lecture 1: Aberrations and optimization 18-1-17 Herbert Gross Winter term 18 www.iap.uni-jena.de Preliminary Schedule Lens Design II 18 1 17.1. Aberrations and optimization Repetition 4.1.
More informationLaser Optics-II. ME 677: Laser Material Processing Instructor: Ramesh Singh 1
Laser Optics-II 1 Outline Absorption Modes Irradiance Reflectivity/Absorption Absorption coefficient will vary with the same effects as the reflectivity For opaque materials: reflectivity = 1 - absorptivity
More informationInterference. Reminder: Exam 2 and Review quiz, more details on the course website
Chapter 9 Interference Phys 322 Lecture 25 Reminder: Exam 2 and Review quiz, more details on the course website Interferometers Wavefront-splitting interferometers Amplitude-splitting interferometers ed
More informationOptical/IR Observational Astronomy Telescopes I: Telescope Basics. David Buckley, SAAO
David Buckley, SAAO 17 Feb 2010 1 Some other Telescope Parameters 1. Plate Scale This defines the scale of an image at the telescopes focal surface For a focal plane, with no distortion, this is just related
More informationAssignment 3 Due September 27, 2010
Assignment 3 Due September 27, 2010 Text readings Stops section 5.3 Dispersing and Reflecting Prisms [sections 5.5.1 and 5.5.2] Optical systems section 5.7 Lens Aberrations [section 6.3] Be careful about
More informationPhysics 102: Lecture 16 Introduction to Mirrors
Physics 102: Lecture 16 Introduction to Mirrors Physics 102: Lecture 16, Slide 1 Physics 102 recent lectures Light as a wave Lecture 14 EM waves Lecture 15 Polarization Lecture 20 & 21 Interference & diffraction
More informationRevisiting Fizeau s Observations: Spectral study of Na source using Newton s rings. Abstract
Revisiting Fizeau s Observations: Spectral study of Na source using Newton s rings K S Umesh #, Denny Melkay, J Adithya, Sai Prem Shaji, N Ganesh, R Dharmaraj, Rajkumar Jain, S Nanjundan # Author for correspondence:
More informationAbsolute length measurement using multiple-wavelength phase-stepping interferometry
UNIVERSITY OF LONDON 1 IMPERIAL COLLEGE OF SCIENCE,TECHNOLOGY AND MEDICINE DEPARTMENT OF PHYSICS APPLIED OPTICS GROUP Absolute length measurement using multiple-wavelength phase-stepping interferometry
More informationProf. Jose Sasian OPTI 518. Introduction to aberrations OPTI 518 Lecture 14
Introduction to aberrations Lecture 14 Topics Structural aberration coefficients Examples Structural coefficients Ж Requires a focal system Afocal systems can be treated with Seidel sums Structural stop
More informationDesign and Correction of optical Systems
Design and Correction of optical Systems Part 10: Performance criteria 1 Summer term 01 Herbert Gross Overview 1. Basics 01-04-18. Materials 01-04-5 3. Components 01-05-0 4. Paraxial optics 01-05-09 5.
More informationIntroduction to Interferometer and Coronagraph Imaging
Introduction to Interferometer and Coronagraph Imaging Wesley A. Traub NASA Jet Propulsion Laboratory and Harvard-Smithsonian Center for Astrophysics Michelson Summer School on Astrometry Caltech, Pasadena
More informationPHY 2049 SPRING 2001 FINAL EXAM
PHY 049 SPRING 0 FINA EXAM 1 Three charges of the same sign and value q are placed in the corners of an equilateral triangle and free to move One more charge Q is placed in the center of the triangle so
More informationExperiment 3 1. The Michelson Interferometer and the He- Ne Laser Physics 2150 Experiment No. 3 University of Colorado
Experiment 3 1 Introduction The Michelson Interferometer and the He- Ne Laser Physics 2150 Experiment No. 3 University of Colorado The Michelson interferometer is one example of an optical interferometer.
More informationCorrelation of optical and generation properties of YAG: Nd 3+ rods*
Optica Applicata, Vol. XIV, No. 1, 1984 Correlation of optical and generation properties of YAG: Nd 3+ rods* JERZY CZESZKO, SŁAWOMIR KACZMAREK Institute of Quantum Electronics, Military Technical Academy,
More informationAstronomical Optics. Second Edition DANIEL J. SCHROEDER ACADEMIC PRESS
Astronomical Optics Second Edition DANIEL J. SCHROEDER Professor of Physics and Astronomy, Emeritus Department of Physics and Astronomy Beloit College, Beloit, Wisconsin ACADEMIC PRESS A Harcourt Science
More information10 Lecture, 5 October 1999
10 Lecture, 5 October 1999 10.1 Aberration compensation for spherical primaries: the Schmidt camera All-reflecting optical systems are called catoptric; all-refracting systems are called dioptric. Mixed
More informationIntroduction to FT-IR Spectroscopy
Introduction to FT-IR Spectroscopy An FT-IR Spectrometer is an instrument which acquires broadband NIR to FIR spectra. Unlike a dispersive instrument, i.e. grating monochromator or spectrograph, an FT-IR
More informationb) Derive the charge-current continuity equation for free charge-density (, ) and free current-density (, ) from Maxwell s microscopic equations.
Fall 205 Written Comprehensive Exam Opti 50 System of units: MKSA 2Pts a) The charge-current continuity equation is written (, )+ (, ) =0. Explain in a few sentences the physical meaning of the equation
More informationCorrection of Errors in Polarization Based Dynamic Phase Shifting Interferometers
Correction of Errors in Polarization Based Dynamic Phase Shifting Interferometers Bradley Kimbrough 4D Technology Corporation, Tucson Arizona brad.kimbrough@4dtechnology.com 1 Introduction Polarization
More informationOptical/IR Observational Astronomy Telescopes I: Telescope Basics. David Buckley, SAAO
David Buckley, SAAO 27 Feb 2012 1 Some other Telescope Parameters 1. Plate Scale This defines the scale of an image at the telescopes focal surface For a focal plane, with no distortion, this is just related
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 informationPhysics 1302, Exam 3 Review
c V Andersen, 2006 1 Physics 1302, Exam 3 Review The following is a list of things you should definitely know for the exam, however, the list is not exhaustive. You are responsible for all the material
More information