Small f/number, “fast” system, little depth of focus, tight tolerances on placement of components Large f/number, “slow” system, easier tolerances,

Slides:



Advertisements
Similar presentations
Flat Mirrors Consider an object placed in front of a flat mirror
Advertisements

Lab 10: Lenses 1.Focal Length 2.Magnification 3.Lens Equation 4.Depth of Field 5.Spherical Aberrations and Curved Focal Plane 6.Chromatic Aberration 7.Astigmatism.
Lens Aberrations Aberration: a departure from the paraxial limit.
Chapter 31 Images.
In all cameras, light enters through the lens and hits the recording medium. (In film cameras, the film plane, in digital cameras (for our purposes),
Announcements No lab tonight due to Dark Sky Observing Night last night Homework: Chapter 6 # 1, 2, 3, 4, 5 & 6 First Quarter Observing Night next Wednesday.
Aperture Pupil (stop) Exit Pupil Entrance Pupil.
Optical Theory II ABERRATIONS Copyright Ellen Stoner, MALS, ABOM, NCLC.
Geometric Optics of thick lenses and Matrix methods
3. Geometrical Optics. Geometric optics—process of light ray through lenses and mirrors to determine the location and size of the image from a given object.
Optics 1----by Dr.H.Huang, Department of Applied Physics
Telescope Optics: A Primer for Amateur Astronomers Part 2: Optical aberrations Marc Baril West Hawaii Astronomy Club, October 13, 2009.
Announcements. Projection Today’s Readings Nalwa 2.1.
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,
Optical Center Eugene Hecht, Optics, Addison-Wesley, Reading, MA, 1998.
Fig Spherical aberration for a lens
Fiber Optics Defining Characteristics: Numerical Aperture Spectral Transmission Diameter.
Physics 52 - Heat and Optics Dr. Joseph F. Becker Physics Department San Jose State University © 2005 J. F. Becker San Jose State University Physics 52.
Image Formation III Chapter 1 (Forsyth&Ponce) Cameras “Lenses”
The Camera : Computational Photography Alexei Efros, CMU, Fall 2008.
Physics 1230: Light and Color Ivan I. Smalyukh, Instructor Office: Gamow Tower, F Phone: Lectures: Tuesdays.
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science Mirrors and Lenses.
Factors affecting the depth of field for SEM Afshin Jooshesh.
© 2010 Pearson Education, Inc. Conceptual Physics 11 th Edition Chapter 28: REFLECTION & REFRACTION Reflection Principle of Least Time Law of Reflection.
1© Manhattan Press (H.K.) Ltd. Terms used for lenses Images in lenses Images in lenses 12.2 Converging and diverging lenses Lens formula Lens formula.
Visual Angle How large an object appears, and how much detail we can see on it, depends on the size of the image it makes on the retina. This, in turns,
Notes on Chapter 30 Lenses
Can YOU determine the general characteristics of the “image” 1.Its location (closer than, further than or the same distance as the object and the mirror)
Optical Instruments, Camera A single lens camera consists basically of an opaque box, converging lens and film. Focusing depends on the object distance.
Real Camera Real-time Rendering of Physically Based Optical Effects in Theory and Practice Yoshiharu Gotanda tri-Ace, Inc.
Fundamental of Optical Engineering Lecture 3.  Aberration happens when the rays do not converge to a point where it should be. We may distinguish the.
Magnifiers, Projectors, CamerasPaul Avery (PHY 3400)1 Magnifiers, Projectors, Cameras Applied Optics Paul Avery University of Florida
Recap from Wednesday Two strategies for realistic rendering capture real world data synthesize from bottom up Both have existed for 500 years. Both are.
Introduction to Engineering Camera Lab #3 - 1 Agenda Do parts I and II of the lab Record data Answer questions.
Chapter 34 Lecture Eight: Images: II. Image Formed by a Thin Lens A thin lens is one whose thickness is small compared to the radii of curvature For a.
Geometric Optics. An object inside the focus casts a virtual image that is only focused by the eye.
Background Research. material selection for launching of telescope; must be soft, able to absorb vibration, fit within the appropriate temperature range.
Geometrical Optics Chapter 24 + Other Tidbits 1. On and on and on …  This is a short week.  Schedule follows  So far, no room available for problem.
Light and Reflection Curved Mirrors. Concave Spherical Mirrors Concave spherical mirror – an inwardly curved, spherical mirrored surface that is a portion.
25.4: Spherical Mirrors. Concave Mirror Light rays near and parallel to the principal axis are reflected from a concave mirror and converge at the focal.
Optical Density - a property of a transparent medium that is an inverse measure of the speed of light through the medium. (how much a medium slows the.
1 32 Optical Images image formation reflection & refraction mirror & lens equations Human eye Spherical aberration Chromatic aberration.
Chapter 25 Optical Instruments 25-1 The Camera The basic parts of a camera are the light-tight box, lens, and shutter. Shutter speed refers to the speed.
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.
1. What is depth of field? 2. Everything else equal, what effect will each of the following have on depth of field (larger, smaller?): -Larger aperture.
October 13, IMAGE FORMATION. October 13, CAMERA LENS IMAGE PLANE OPTIC AXIS LENS.
CSE 185 Introduction to Computer Vision Cameras. Camera models –Pinhole Perspective Projection –Affine Projection –Spherical Perspective Projection Camera.
Aperture What is it and how does it affect your pictures?
Film/Sensor Where the light is recorded Lens Bends the light Trajectory of light Subject Source of light Focusing A look at the overall camera system.
Thin-lens equation: 1/f = 1/d 0 + 1/d i. Magnification equation: h i /h o = d i /d o.
3.30. Image location by ray tracing Consider a real object that is placed in front of a convex lens. The location of the image can be found by considering.
Physics 203/204 4: Geometric Optics Images formed by refraction Lens Makers Equation Thin lenses Combination of thin lenses Aberration Optical Instruments.
ABERRATIONS Lecturer in PHYSICS Silver Jubilee Govt.,College(A),
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.
Prof. Charles A. DiMarzio Northeastern University Fall 2003 July 2003
Lesson 1: The Art and Physics of Photography Basic Photography MITSAA Spring 2003 Rob Zehner.
Lenses Properties, Characteristics & Ray Diagrams.
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.
Chapter 2: The Lens. Focal Length is the distance between the center of a lens and the film plane when focused at infinity.
Matrix methods, aberrations & optical systems
Image Formation III Chapter 1 (Forsyth&Ponce) Cameras “Lenses” Guido Gerig CS-GY 6643, Spring 2016 (slides modified from Marc Pollefeys, UNC Chapel Hill/
Properties of Telescopes. Magnification Magnification is how much larger an image in a telescope is when compared to when the object is seen by the naked.
A light beam striking a boundary between two media can be partly transmitted and partly reflected at the boundary.
Chapter 13: Mirrors and Lenses Section 1 : Mirrors Section 2: Lenses Section 3: Optical Instruments.
Spherical Aberration. Rays emanating from an object point that are incident on a spherical mirror or lens at different distances from the optical axis,
Refraction & lenses. Types Of Lenses Image Formation via Refraction by thin lenses Thin lenses are those whose thickness is small compared to their radius.
July © Chuck DiMarzio, Northeastern University ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof.
25 Optical Instruments Digital Camera with Zoom Lens.
Lab 10: Lenses Focal Length Magnification Lens Equation Depth of Field
Chapter 5 Telescopes: Refracting , Reflecting, Cassegrain.
Presentation transcript:

Small f/number, “fast” system, little depth of focus, tight tolerances on placement of components Large f/number, “slow” system, easier tolerances, nearly parallel rays through filter F/number = focal length ÷ aperture Also, reciprocal of “relative aperture”

Same primary mirror, but very different f/numbers

Primary is f/2.63, but system is f/31.2 !!

Spherical aberration—focal length depends on radius where ray strikes mirror/lens.

Note circle of least confusion, the “best” focus Image of a point source is usually a bright dot surrounded by a halo of light Effect on extended image is to soften the contrast and blur the details

Chromatic aberration

The primary “monochromatic” aberrations are: Spherical aberration Comatic aberration (“coma”) Astigmatism Petzval field curvature Distortion

Coma Affected by where the light rays hit the lens/mirror Same focal plane, but different magnification Coma varies with the shape of the lens, and the position of any apertures/stops. Size of coma patch varies linearly with its distance from the axis

Astigmatism Image of a point source is not a point, but takes the form of two separate lines Between the astigmatic foci, the image is an elliptical or circular blur Circle of least confusion increases in diameter as the object moves further off-axis Image loses definition around its edges

Field curvature

Schmidt camera

Distortion

Example: If we increase aperture diameter by 50%, and reduce field of view by 50%, then ‘y’ is 1.5x the original, ‘h’ is 0.5x the original Coma increases by Curvature reduced to 0.25 of previous amount Blurs due to astigmatism or curvature will of of original size y = distance of image from optical axis h = distance of object from optical axis