R 1 R 2 R 3. t 1 t 2. n 1 n 2

Similar documents
2.710 Optics Spring 09 Problem Set #3 Posted Feb. 23, 2009 Due Wednesday, March 4, 2009

Mirrors, Lenses &Imaging Systems

Chapters 1 & 2. Definitions and applications Conceptual basis of photogrammetric processing

Image Formation. Light from distant things. Geometrical optics. Pinhole camera. Chapter 36

MASSACHUSETTS INSTITUTE OF TECHNOLOGY. 2.71/2.710 Optics Spring 14 Practice Problems Posted May 11, 2014

Chapter 18 Optical Elements

Lens Design I. Lecture 3: Properties of optical systems II Herbert Gross. Summer term

Lens Design I. Lecture 3: Properties of optical systems II Herbert Gross. Summer term

OPTICAL SYSTEMS OBJECTIVES

Lens Principal and Nodal Points

EE119 Introduction to Optical Engineering Spring 2002 Final Exam. Name:

Chapter 24 Geometrical Optics. Copyright 2010 Pearson Education, Inc.

Algebra Based Physics. Reflection. Slide 1 / 66 Slide 2 / 66. Slide 3 / 66. Slide 4 / 66. Slide 5 / 66. Slide 6 / 66.

Opti 415/515. Introduction to Optical Systems. Copyright 2009, William P. Kuhn

PHYS 160 Astronomy. When analyzing light s behavior in a mirror or lens, it is helpful to use a technique called ray tracing.

Converging Lenses. Parallel rays are brought to a focus by a converging lens (one that is thicker in the center than it is at the edge).

Final Reg Optics Review SHORT ANSWER. Write the word or phrase that best completes each statement or answers the question.

Ch 24. Geometric Optics

Waves & Oscillations

Assignment X Light. Reflection and refraction of light. (a) Angle of incidence (b) Angle of reflection (c) principle axis

2.71 Optics Fall 05 QUIZ 1 Wednesday, Oct. 12, 2005

EE119 Introduction to Optical Engineering Spring 2003 Final Exam. Name:

COURSE NAME: PHOTOGRAPHY AND AUDIO VISUAL PRODUCTION (VOCATIONAL) FOR UNDER GRADUATE (FIRST YEAR)

Optical Zoom System Design for Compact Digital Camera Using Lens Modules

Algebra Based Physics. Reflection. Slide 1 / 66 Slide 2 / 66. Slide 3 / 66. Slide 4 / 66. Slide 5 / 66. Slide 6 / 66.

Sequential Ray Tracing. Lecture 2

University of Rochester Department of Physics and Astronomy Physics123, Spring Homework 5 - Solutions


Area of the Secondary Mirror Obscuration Ratio = Area of the EP Ignoring the Obscuration

Lens Design I Seminar 1

Lecture 4: Geometrical Optics 2. Optical Systems. Images and Pupils. Rays. Wavefronts. Aberrations. Outline

Practice Problems (Geometrical Optics)

Complete the diagram to show what happens to the rays. ... (1) What word can be used to describe this type of lens? ... (1)

Thin Lenses * OpenStax

Understanding Focal Length

CHAPTER 3LENSES. 1.1 Basics. Convex Lens. Concave Lens. 1 Introduction to convex and concave lenses. Shape: Shape: Symbol: Symbol:

GEOMETRICAL OPTICS AND OPTICAL DESIGN

Lenses Design Basics. Introduction. RONAR-SMITH Laser Optics. Optics for Medical. System. Laser. Semiconductor Spectroscopy.

EF 15mm f/2.8 Fisheye. EF 14mm f/2.8l USM. EF 20mm f/2.8 USM

Imaging Instruments (part I)

Performance Factors. Technical Assistance. Fundamental Optics

04. REFRACTION OF LIGHT AT CURVED SURFACES

Lenses, exposure, and (de)focus

Exam Preparation Guide Geometrical optics (TN3313)

Tutorial Zemax 9: Physical optical modelling I

Applied Optics. , Physics Department (Room #36-401) , ,

Lecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.

Aberrations of a lens

Geometrical Optics. Have you ever entered an unfamiliar room in which one wall was covered with a

REFLECTION THROUGH LENS

Types of lenses. Shown below are various types of lenses, both converging and diverging.

Astronomy 80 B: Light. Lecture 9: curved mirrors, lenses, aberrations 29 April 2003 Jerry Nelson

Lens Aperture. South Pasadena High School Final Exam Study Guide- 1 st Semester Photo ½. Study Guide Topics that will be on the Final Exam

Physics 1230: Light and Color. Guest Lecture, Jack again. Lecture 23: More about cameras

Image Formation Fundamentals

Projection. Projection. Image formation. Müller-Lyer Illusion. Readings. Readings. Let s design a camera. Szeliski 2.1. Szeliski 2.

Physics 431 Final Exam Examples (3:00-5:00 pm 12/16/2009) TIME ALLOTTED: 120 MINUTES Name: Signature:

SIGMA 17-70mm F2.8-4 DC MACRO OS HSM 17-70mm F2.8-4 DC MACRO HSM

Projection. Readings. Szeliski 2.1. Wednesday, October 23, 13

Lecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.

General Physics II. Ray Optics

CHAPTER 1 Optical Aberrations

BHARATIYA VIDYA BHAVAN S V M PUBLIC SCHOOL, VADODARA QUESTION BANK

Optical Engineering 421/521 Sample Questions for Midterm 1

6.098 Digital and Computational Photography Advanced Computational Photography. Bill Freeman Frédo Durand MIT - EECS

Image Formation Fundamentals

Refraction of Light. Refraction of Light

An f-number of X may also be displayed as 1:X (instead of f/x), as shown below for the Canon f/2.8 lens.

Physics 1230 Homework 8 Due Friday June 24, 2016

Laboratory experiment aberrations

Section 8. Objectives

Refraction by Spherical Lenses by

Lecture 8. Lecture 8. r 1

R.B.V.R.R. WOMEN S COLLEGE (AUTONOMOUS) Narayanaguda, Hyderabad.

Focal Length of Lenses

OPAC 202 Optical Design and Inst.

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Mechanical Engineering Department. 2.71/2.710 Final Exam. May 21, Duration: 3 hours (9 am-12 noon)

PHYSICS 289 Experiment 8 Fall Geometric Optics II Thin Lenses

Image Formation by Lenses

Department of Physics & Astronomy Undergraduate Labs. Thin Lenses

Thin Lenses. Lecture 25. Chapter 23. Ray Optics. Physics II. Course website:

2. The radius of curvature of a spherical mirror is 20 cm. What is its focal length?

Lab 10: Lenses & Telescopes

Chapter 36. Image Formation

GEOMETRICAL OPTICS Practical 1. Part I. BASIC ELEMENTS AND METHODS FOR CHARACTERIZATION OF OPTICAL SYSTEMS

Instructions. To run the slideshow:

30 Lenses. Lenses change the paths of light.

Chapter 34 Geometric Optics

Chapter 23. Mirrors and Lenses

ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof. Charles A. DiMarzio Northeastern University Fall 2008

2015 EdExcel A Level Physics EdExcel A Level Physics. Lenses

CHAPTER 3 OPTICAL INSTRUMENTS

LIGHT REFLECTION AND REFRACTION

Basic Camera Concepts. How to properly utilize your camera

Name: Lab Partner: Section:

Optical System Design

Actually, you only need to design one monocular of the binocular.

Spherical Mirrors. Concave Mirror, Notation. Spherical Aberration. Image Formed by a Concave Mirror. Image Formed by a Concave Mirror 4/11/2014

Introduction to Optical Modeling. Friedrich-Schiller-University Jena Institute of Applied Physics. Lecturer: Prof. U.D. Zeitner

Geometric optics & aberrations

Transcription:

MASSACHUSETTS INSTITUTE OF TECHNOLOGY 2.71/2.710 Optics Spring 14 Problem Set #2 Posted Feb. 19, 2014 Due Wed Feb. 26, 2014 1. (modified from Pedrotti 18-9) A positive thin lens of focal length 10cm is separated 5cm from a thin negative lens of focal length -10cm. a. Sketch your optical system to scale. b. Find the equivalent focal length of the composite lens, together with the position of the front focal plane, back focal plane and principal planes. You may use ray tracing or matrix methods. c. For an arbitrary object placed in front of the system, please use your findings in b) to find the image. 2. A 25.4mm diameter precision plano-convex achromat doublet lens from Newport is made by N-BK7 and SF5 glass. It has the following specifications: R1=60.741 mm, R2= -89.718 mm, R3= -268.159 mm, t1= 3.8 mm, t2= 2.5 mm, n1= 1.51947 (@λ=532nm), n2= 1.64570 (@λ=633nm). a. What is the optical power of this composite element? b. If a plane wave is incident from the left, where will it focus? R 1 R 2 R 3 t 1 t 2 n 1 n 2 1

3. A Telephoto Lens. For an object placed at infinity, we need to design a composite lens system with the following specifications. - The spacing from the front lens to the rear lens is 120 mm. - The working distance (from the rear lens to image plane) is 100 mm. - The effective focal length (EFL) is 300mm. L1 L2 Image plane d=120 mm BFL=100 mm A.S. a. Assuming all elements are thin lenses, determine the focal length of each individual lens. b. Locate the principle planes of the lens system. c. The aperture stop (A. S.) of this system is located at the front lens. In order for the system to operate at F-number of f/4.0, what should be the diameter of the aperture? d. If two objects are separated by 10-3 radians at infinity, how far apart will their images form on the screen? 4. (modified from Pedrotti 3-5) A optical system is made up of a positive thin lens L1 of diameter 6cm, and focal length f1=6cm, and a negative thin lens L2 of diameter 6cm and focal length f2=-10cm, and an aperture A of diameter 3cm. The aperture A is located 3cm in front of the lens L1, which is located 4cm in front of the lens L2. An object OP, 3cm high, is located 18cm to the left of L1. Pearson Prentice Hall. All rights reserved. This content is excluded from our Creative Commons license. For more information, see http://ocw.mit.edu/fairuse. 2

a. Determine the location and the size of the field stop FS. b. Determine the location and the size of the entrance and exit windows. c. Using the chief ray from object point P to image point P as shown in the example, draw the two marginal rays from P to P, which, together with the chief ray, determine the cone of light that successfully get through the optical system. 5. Camera lens and Image Stabilizer system: Professional or semi-professional cameras are usually designed to be used with interchangeable lenses. In this problem, we will study a simplified model of how the camera works, as well as the mechanism of the Image Stabilizer, which is state-of-art technology to improve the photography quality when shooting with weak light. For simplicity, we assume that the lens with our camera is a prime lens. This means that the focal length of this lens is fixed. As shown in Figure 5a, we want to shoot an image of a flower which is d = 36cm away from us. (More rigorously, the plane normal to the axis near the center of the flower is located distance d from the film plane of the camera.) In today s digital cameras, electronic chips such as CCD or CMOS are placed at the image plane. We assume that the refractive index of the air is n = 1, and the glass used for the lens has ng = 1.5. The lens is assumed to be thin (the distance between the two curved surface is negligible) and symmetric (the curvature of the two refractive surfaces are the same, with radii R = 50mm). In this problem, we only consider the imaging of an on-axis point A on the flower. Figure 5a a. In order to form a sharp image A of A exactly at the film plane, the lens has to be moved longitudinally to a proper position to satisfy the imaging condition (focusing). Calculate the distance between the lens nodal point O (center) and film plane which satisfying the imaging condition (Note: The image is demagnified in camera, which means the valid solution of s satisfies s < d s). 3

Figure 5b b. At dim environments, e.g. indoors or during sunrise, sunset, and at night time, the exposure time must be increased to let the film or CCD/CMOS capture enough photons. However, with long exposure time (> 0.1s), it is usually impossible to keep the hand held camera stationary, resulting in a smeared image. Recently, camera companies developed various techniques to reduce the effect of camera shaking on image quality. In general, these techniques use a micro-gyroscope to detect the shaking of the camera during exposure; then the on-board micro computer drives an actuator to move the lens with respect to the film/ccd/cmos. Ideally the motion should exactly compensate the camera shaking, i.e. freeze the image at the same position on the film/ccd/cmos. CANON s Image Stabilizer (IS) technology moves the lens to achieve this compensation, as shown in Figure 5b. With the lens moved by δ2, the ray is bent and deflected to position A. Assume the camera shaking is a counter clockwise rotation of 1 respect to the lens center, as shown in Figure 5b. In which direction and by how much (δ2) does the IS system have to move the lens to keep the image of A fixed at the same position (A ) on the CCD? 4

MIT OpenCourseWare http://ocw.mit.edu 2.71 / 2.710 Optics Spring 2014 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.