Cardinal planes/points in paraxial optics

Slides:



Advertisements
Similar presentations
Option G: Electromagnetic Waves G2: Optical Instruments.
Advertisements

Hecht 5.2, 6.1 Monday September 16, 2002
Chapter 31: Images and Optical Instruments
1© Manhattan Press (H.K.) Ltd. Final image at infinity Eye-ring Eye-ring 12.6 Refracting telescope.
How to Draw and Read Ray Diagrams Draw the image forming device(s), i.e., lens(es), mirror(s), on the optical axis A. Draw a principal plane (line) H for.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Telescopes. Introduction  A telescope is designed to form on the retina of the eye a larger image of an object than would be created if the object were.
Optical Instruments Physics 2415 Lecture 34 Michael Fowler, UVa.
1 Cardinal planes/points in paraxial optics Wednesday September 18, 2002.
Lecture 25-1 Locating Images Real images form on the side of a mirror where the objects are, and virtual images form on the opposite side. only using the.
Ch. 18 Mirrors and Lenses Milbank High School. Sec Mirrors Objectives –Explain how concave, convex, and plane mirrors form images. –Locate images.
Geometric Optics of thick lenses and Matrix methods
Physics 1502: Lecture 30 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Friday Optics –Mirrors –Lenses –Eye.
Homework Set 4: From “Seeing the Light” Chapter 3: (starting page 101) P9, P10, P11, PM3 From “Seeing the Light” Chapter 4: P2, P5, P7, P13 Due: Monday,
Lenses We will only consider “thin” lenses where the thickness of the lens is small compared to the object and image distances. Eugene Hecht, Optics, Addison-Wesley,
Copyright © 2008 Pearson Education Inc., publishing as Pearson Addison-Wesley PowerPoint ® Lectures for University Physics, Twelfth Edition – Hugh D. Young.
C F V Light In Side S > 0 Real Object Light Out Side S ’ > 0 Real Image C This Side, R > 0 S < 0 Virtual Object S ’ < 0 Virtual Image C This Side, R
Copyright © 2008 Pearson Education Inc., publishing as Pearson Addison-Wesley PowerPoint ® Lectures for University Physics, Twelfth Edition – Hugh D. Young.
By Bhaskar Department of Physics K L University. Lecture 07 (25 Aug) Interference in Thin Films.
Convex Lens A convex lens curves outward; it has a thick center and thinner edges.
Lenses.
Example: An object 3 cm high is placed 20 cm from (a) a convex and (b) a concave spherical mirror, each of 10 cm focal length. Determine the position.
Copyright © 2009 Pearson Education, Inc. Chapter 33 Lenses and Optical Instruments.
Lecture 14 Images Chp. 35 Opening Demo Topics –Plane mirror, Two parallel mirrors, Two plane mirrors at right angles –Spherical mirror/Plane mirror comparison.
Chapter 18 Mirrors and Lenses Lenses A. Types of Lenses A. Types of Lenses B. Convex Lenses B. Convex Lenses C. Concave Lenses C. Concave Lenses.
Images and Optical Instruments. Definitions Real Image - Light passes through the image point. Virtual Image - Light does not pass through the image point.
Chapter 12 Optical Instruments Physics Beyond 2000.
LIGHT: Geometric Optics. The Ray Model of Light Light travels in straight lines under a wide variety of circumstances Light travels in straight line paths.
Dr. Andrew Tomasch 2405 Randall Lab
Engineering Optics Understanding light? Reflection and refraction Geometric optics (
Review for Test #1  Responsible for: - Chapters 35 and 36 and section Notes from class - Problems worked in class - Homework assignments  Test.
Today’s agenda: Death Rays. You must know when to run from Death Rays. Refraction at Spherical Surfaces. You must be able to calculate properties of images.
1 32 Optical Images image formation reflection & refraction mirror & lens equations Human eye Spherical aberration Chromatic aberration.
12.1 Characteristics of Lenses. Today we will learn about...  the different types of lenses, the characteristics of the image formed by each of those.
Today’s agenda: Death Rays. You must know when to run from Death Rays. Refraction at Spherical Surfaces. You must be able to calculate properties of images.
Thin-lens equation: 1/f = 1/d 0 + 1/d i. Magnification equation: h i /h o = d i /d o.
Notes 2-5 OPTICAL TOOLS. Cameras: How do they work? Light from object travels through one or more convex lenses Lens focuses light Puts an image on film.
Chapter 18-2 Lenses.
Physics 203/204 4: Geometric Optics Images formed by refraction Lens Makers Equation Thin lenses Combination of thin lenses Aberration Optical Instruments.
Thin Lenses A lens is an optical device consisting of two refracting surfaces The simplest lens has two spherical surfaces close enough together that we.
Physics 1202: Lecture 23 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Optical Instruments.
Physics 1202: Lecture 22 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Chapter 18 Mirrors and Lenses. Objectives 18.1 Explain how concave, convex, and plane mirrors form images 18.1 Locate images using ray diagrams, and calculate.
Cardinal planes and matrix methods
Matrix methods, aberrations & optical systems
GEOMETRICAL OPTICS. Laws of Reflection Laws of Refraction.
Lenses, mirrors and refractive surfaces
Geometric Optics: Mirrors and Lenses. Mirrors with convex and concave spherical surfaces. Note that θ r = θ i for each ray.
1 Matrix methods in paraxial optics Wednesday September 25, 2002.
Chapter 33 Lenses and Optical Instruments The Thin Lens Equation; Magnification Example 33-2: Image formed by converging lens. What are (a) the.
17.1 Reflection and Refraction. Chapter 17 Objectives  Describe the functions of convex and concave lenses, a prism, and a flat mirror.  Describe how.
Lens Applications & Technologies. airglass airglass.
Lecture 25-1 Locating Images Real images form on the side of a mirror where the objects are, and virtual images form on the opposite side. only using the.
Lecture 2: Reflection of Light: Mirrors (Ch 25) & Refraction of Light: Lenses (Ch 26)
18. Images Images in plane mirrors
Ch. 30 Lenses.
Refraction at Spherical Surfaces.
A. WAVE OPTICS B. GEOMETRIC OPTICS Light Rays
SPHERICAL MIRROR EQUATIONS
17.3 Optical Systems 1.
lens that causes light rays parallel to central axis to converge
Lecture 2: Basic Astronomical Optics
12.1 Characteristics of Lenses
Newton’s rings in reflected light
Mirrors, Plane and Spherical Spherical Refracting Surfaces
Ch.6 Lens (透鏡).
SPHERICAL MIRROR EQUATIONS
Lenses.
Presentation transcript:

Cardinal planes/points in paraxial optics Friday September 20, 2002

Find power of combined system Combination of two systems: e.g. two spherical interfaces, two thin lenses … n H1 H1’ n2 H’ h’ n’ 1. Consider F’ and F2’ H2 H2’ y’ y Y θ θ F2 F’ F2’ d ƒ2’ ƒ2 ƒ’ Find power of combined system

Summary I II H H’ H1 H1’ H2 H2’ F’ F n2 n’ n d h h’ ƒ ƒ’

Summary

Thick Lens In air n = n’ =1 Lens, n2 = 1.5 n n2 n’ R1 = - R2 = 10 cm d = 3 cm Find ƒ1,ƒ2,ƒ, h and h’ Construct the principal planes, H, H’ of the entire system R1 R2 H1,H1’ H2,H2’

Principal planes for thick lens (n2=1.5) in air Equi-convex or equi-concave and moderately thick  P1 = P2 ≈ P/2 H H’ H H’

Principal planes for thick lens (n2=1.5) in air Plano-convex or plano-concave lens with R2 =   P2 = 0 H H’ H H’

Principal planes for thick lens (n=1.5) in air For meniscus lenses, the principal planes move outside the lens R2 = 3R1 (H’ reaches the first surface) H H’ H H’ H H’ H H’ Same for all lenses

Examples: Two thin lenses in air ƒ1 ƒ2 n = n2 = n’ = 1 Want to replace Hi, Hi’ with H, H’ d h h’ H1 H1’ H2 H2’

Examples: Two thin lenses in air ƒ1 ƒ2 n = n2 = n’ = 1 F F’ d ƒ’ ƒ s s’

Huygen’s eyepiece ƒ1=2ƒ2 and d=1.5ƒ2 In order for a combination of two lenses to be independent of the index of refraction (i.e. free of chromatic aberration) Example, Huygen’s Eyepiece ƒ1=2ƒ2 and d=1.5ƒ2 Determine ƒ, h and h’

Huygen’s eyepiece H1 H’ H2 H h’ = -ƒ2 h=2ƒ2 d=1.5ƒ2

Two separated lenses in air f1’=2f2’ H’ H H’ H F’ F’ F F f’ f’ d = f2’ d = 0.5 f2’

Two separated lenses in air f1’=2f2’ Principal points at  H’ H F’ F f’ d = 3f2’ d = 2f2’ e.g. Astronomical telescope

Two separated lenses in air f1’=2f2’ e.g. Compound microscope H H’ F’ F f’ d = 5f2’

Two separated lenses in air f1’=-2f2’ e.g. Galilean telescope d = -f2’ Principal points at 

Two separated lenses in air f1’=-2f2’ H H’ F F’ f’ e.g. Telephoto lens d = -1.5f2’