Handbook of Visual Optics 3 Geometrical Optics
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Breaking Down the “Cosine Fourth Power Law”
Breaking Down The “Cosine Fourth Power Law” By Ronian Siew, inopticalsolutions.com Why are the corners of the field of view in the image captured by a camera lens usually darker than the center? For one thing, camera lenses by design often introduce “vignetting” into the image, which is the deliberate clipping of rays at the corners of the field of view in order to cut away excessive lens aberrations. But, it is also known that corner areas in an image can get dark even without vignetting, due in part to the so-called “cosine fourth power law.” 1 According to this “law,” when a lens projects the image of a uniform source onto a screen, in the absence of vignetting, the illumination flux density (i.e., the optical power per unit area) across the screen from the center to the edge varies according to the fourth power of the cosine of the angle between the optic axis and the oblique ray striking the screen. Actually, optical designers know this “law” does not apply generally to all lens conditions.2 – 10 Fundamental principles of optical radiative flux transfer in lens systems allow one to tune the illumination distribution across the image by varying lens design characteristics. In this article, we take a tour into the fascinating physics governing the illumination of images in lens systems. Relative Illumination In Lens Systems In lens design, one characterizes the illumination distribution across the screen where the image resides in terms of a quantity known as the lens’ relative illumination — the ratio of the irradiance (i.e., the power per unit area) at any off-axis position of the image to the irradiance at the center of the image. -
Introduction to CODE V: Optics
Introduction to CODE V Training: Day 1 “Optics 101” Digital Camera Design Study User Interface and Customization 3280 East Foothill Boulevard Pasadena, California 91107 USA (626) 795-9101 Fax (626) 795-0184 e-mail: [email protected] World Wide Web: http://www.opticalres.com Copyright © 2009 Optical Research Associates Section 1 Optics 101 (on a Budget) Introduction to CODE V Optics 101 • 1-1 Copyright © 2009 Optical Research Associates Goals and “Not Goals” •Goals: – Brief overview of basic imaging concepts – Introduce some lingo of lens designers – Provide resources for quick reference or further study •Not Goals: – Derivation of equations – Explain all there is to know about optical design – Explain how CODE V works Introduction to CODE V Training, “Optics 101,” Slide 1-3 Sign Conventions • Distances: positive to right t >0 t < 0 • Curvatures: positive if center of curvature lies to right of vertex VC C V c = 1/r > 0 c = 1/r < 0 • Angles: positive measured counterclockwise θ > 0 θ < 0 • Heights: positive above the axis Introduction to CODE V Training, “Optics 101,” Slide 1-4 Introduction to CODE V Optics 101 • 1-2 Copyright © 2009 Optical Research Associates Light from Physics 102 • Light travels in straight lines (homogeneous media) • Snell’s Law: n sin θ = n’ sin θ’ • Paraxial approximation: –Small angles:sin θ~ tan θ ~ θ; and cos θ ~ 1 – Optical surfaces represented by tangent plane at vertex • Ignore sag in computing ray height • Thickness is always center thickness – Power of a spherical refracting surface: 1/f = φ = (n’-n)*c -
Section 10 Vignetting Vignetting the Stop Determines Determines the Stop the Size of the Bundle of Rays That Propagates On-Axis an the System for Through Object
10-1 I and Instrumentation Design Optical OPTI-502 © Copyright 2019 John E. Greivenkamp E. John 2019 © Copyright Section 10 Vignetting 10-2 I and Instrumentation Design Optical OPTI-502 Vignetting Greivenkamp E. John 2019 © Copyright On-Axis The stop determines the size of Ray Aperture the bundle of rays that propagates Bundle through the system for an on-axis object. As the object height increases, z one of the other apertures in the system (such as a lens clear aperture) may limit part or all of Stop the bundle of rays. This is known as vignetting. Vignetted Off-Axis Ray Rays Bundle z Stop Aperture 10-3 I and Instrumentation Design Optical OPTI-502 Ray Bundle – On-Axis Greivenkamp E. John 2018 © Copyright The ray bundle for an on-axis object is a rotationally-symmetric spindle made up of sections of right circular cones. Each cone section is defined by the pupil and the object or image point in that optical space. The individual cone sections match up at the surfaces and elements. Stop Pupil y y y z y = 0 At any z, the cross section of the bundle is circular, and the radius of the bundle is the marginal ray value. The ray bundle is centered on the optical axis. 10-4 I and Instrumentation Design Optical OPTI-502 Ray Bundle – Off Axis Greivenkamp E. John 2019 © Copyright For an off-axis object point, the ray bundle skews, and is comprised of sections of skew circular cones which are still defined by the pupil and object or image point in that optical space. -
Object-Image Real Image Virtual Image
Object-Image • A physical object is usually observed by reflected light that diverges from the object. • An optical system (mirrors or lenses) can 3.1 Images formed by Mirrors and Lenses produce an image of the object by redirecting the light. • Images – Real Image • Image formation by mirrors – Virtual Image • Images formed by lenses Real Image Virtual Image Optical System ing diverging erg converging diverging diverging div Object Object real Image Optical System virtual Image Light appears to come from the virtual image but does not Light passes through the real image pass through the virtual image Film at the position of the real image is exposed. Film at the position of the virtual image is not exposed. Each point on the image can be determined Image formed by a plane mirror. by tracing 2 rays from the object. B p q B’ Object Image The virtual image is formed directly behind the object image mirror. Light does not A pass through A’ the image mirror A virtual image is formed by a plane mirror at a distance q behind the mirror. q = -p 1 Parabolic Mirrors Parabolic Reflector Optic Axis Parallel rays reflected by a parabolic mirror are focused at a point, called the Parabolic mirrors can be used to focus incoming parallel rays to a small area Focal Point located on the optic axis. or to direct rays diverging from a small area into parallel rays. Spherical mirrors Parallel beams focus at the focal point of a Concave Mirror. •Spherical mirrors are much easier to fabricate than parabolic mirrors • A spherical mirror is an approximation of a parabolic Focal point mirror for small curvatures. -
Curriculum Overview Physics/Pre-AP 2018-2019 1St Nine Weeks
Curriculum Overview Physics/Pre-AP 2018-2019 1st Nine Weeks RESOURCES: Essential Physics (Ergopedia – online book) Physics Classroom http://www.physicsclassroom.com/ PHET Simulations https://phet.colorado.edu/ ONGOING TEKS: 1A, 1B, 2A, 2B, 2C, 2D, 2F, 2G, 2H, 2I, 2J,3E 1) SAFETY TEKS 1A, 1B Vocabulary Fume hood, fire blanket, fire extinguisher, goggle sanitizer, eye wash, safety shower, impact goggles, chemical safety goggles, fire exit, electrical safety cut off, apron, broken glass container, disposal alert, biological hazard, open flame alert, thermal safety, sharp object safety, fume safety, electrical safety, plant safety, animal safety, radioactive safety, clothing protection safety, fire safety, explosion safety, eye safety, poison safety, chemical safety Key Concepts The student will be able to determine if a situation in the physics lab is a safe practice and what appropriate safety equipment and safety warning signs may be needed in a physics lab. The student will be able to determine the proper disposal or recycling of materials in the physics lab. Essential Questions 1. How are safe practices in school, home or job applied? 2. What are the consequences for not using safety equipment or following safe practices? 2) SCIENCE OF PHYSICS: Glossary, Pages 35, 39 TEKS 2B, 2C Vocabulary Matter, energy, hypothesis, theory, objectivity, reproducibility, experiment, qualitative, quantitative, engineering, technology, science, pseudo-science, non-science Key Concepts The student will know that scientific hypotheses are tentative and testable statements that must be capable of being supported or not supported by observational evidence. The student will know that scientific theories are based on natural and physical phenomena and are capable of being tested by multiple independent researchers. -
Beam Expander Basics: Not All Spots Are Created Equal
LEARNING – UNDERSTANDING – INTRODUCING – APPLYING Beam Expander Basics: Not All Spots Are Created Equal APPLICATION NOTES www.edmundoptics.com BEAM EXPANDERS A laser beam expander is designed to increase the diameter from well-established optical telescope fundamentals. In such of a collimated input beam to a larger collimated output beam. systems, the object rays, located at infinity, enter parallel to Beam expanders are used in applications such as laser scan- the optical axis of the internal optics and exit parallel to them ning, interferometry, and remote sensing. Contemporary laser as well. This means that there is no focal length to the entire beam expander designs are afocal systems that developed system. THEORY: TELESCOPES Optical telescopes, which have classically been used to view eye, or image created, is called the image lens. distant objects such as celestial bodies in outer space, are di- vided into two types: refracting and reflecting. Refracting tele- A Galilean telescope consists of a positive lens and a negative scopes utilize lenses to refract or bend light while reflecting lens that are also separated by the sum of their focal length telescopes utilize mirrors to reflect light. (Figure 2). However, since one of the lenses is negative, the separation distance between the two lenses is much shorter Refracting telescopes fall into two categories: Keplerian and than in the Keplerian design. Please note that using the Effec- Galilean. A Keplerian telescope consists of positive focal length tive Focal Length of the two lenses will give a good approxima- lenses that are separated by the sum of their focal lengths (Fig- tion of the total length, while using the Back Focal Length will ure 1). -
Laboratory 7: Properties of Lenses and Mirrors
Laboratory 7: Properties of Lenses and Mirrors Converging and Diverging Lens Focal Lengths: A converging lens is thicker at the center than at the periphery and light from an object at infinity passes through the lens and converges to a real image at the focal point on the other side of the lens. A diverging lens is thinner at the center than at the periphery and light from an object at infinity appears to diverge from a virtual focus point on the same side of the lens as the object. The principal axis of a lens is a line drawn through the center of the lens perpendicular to the face of the lens. The principal focus is a point on the principal axis through which incident rays parallel to the principal axis pass, or appear to pass, after refraction by the lens. There are principle focus points on either side of the lens equidistant from the center (See Figure 1a). Figure 1a: Converging Lens, f>0 Figure 1b: Diverging Lens, f<0 In Fig. 1 the object and image are represented by arrows. Two rays are drawn from the top of the object. One ray is parallel to the principal axis which bends at the lens to pass through the principle focus. The second ray passes through the center of the lens and undeflected. The intersection of these two rays determines the image position. The focal length, f, of a lens is the distance from the optical center of the lens to the principal focus. It is positive for a converging lens, negative for a diverging lens. -
Aperture Efficiency and Wide Field-Of-View Optical Systems Mark R
Aperture Efficiency and Wide Field-of-View Optical Systems Mark R. Ackermann, Sandia National Laboratories Rex R. Kiziah, USAF Academy John T. McGraw and Peter C. Zimmer, J.T. McGraw & Associates Abstract Wide field-of-view optical systems are currently finding significant use for applications ranging from exoplanet search to space situational awareness. Systems ranging from small camera lenses to the 8.4-meter Large Synoptic Survey Telescope are designed to image large areas of the sky with increased search rate and scientific utility. An interesting issue with wide-field systems is the known compromises in aperture efficiency. They either use only a fraction of the available aperture or have optical elements with diameters larger than the optical aperture of the system. In either case, the complete aperture of the largest optical component is not fully utilized for any given field point within an image. System costs are driven by optical diameter (not aperture), focal length, optical complexity, and field-of-view. It is important to understand the optical design trade space and how cost, performance, and physical characteristics are influenced by various observing requirements. This paper examines the aperture efficiency of refracting and reflecting systems with one, two and three mirrors. Copyright © 2018 Advanced Maui Optical and Space Surveillance Technologies Conference (AMOS) – www.amostech.com Introduction Optical systems exhibit an apparent falloff of image intensity from the center to edge of the image field as seen in Figure 1. This phenomenon, known as vignetting, results when the entrance pupil is viewed from an off-axis point in either object or image space. -
Lecture 37: Lenses and Mirrors
Lecture 37: Lenses and mirrors • Spherical lenses: converging, diverging • Plane mirrors • Spherical mirrors: concave, convex The animated ray diagrams were created by Dr. Alan Pringle. Terms and sign conventions for lenses and mirrors • object distance s, positive • image distance s’ , • positive if image is on side of outgoing light, i.e. same side of mirror, opposite side of lens: real image • s’ negative if image is on same side of lens/behind mirror: virtual image • focal length f positive for concave mirror and converging lens negative for convex mirror and diverging lens • object height h, positive • image height h’ positive if the image is upright negative if image is inverted • magnification m= h’/h , positive if upright, negative if inverted Lens equation 1 1 1 푠′ ℎ′ + = 푚 = − = magnification 푠 푠′ 푓 푠 ℎ 푓푠 푠′ = 푠 − 푓 Converging and diverging lenses f f F F Rays refract towards optical axis Rays refract away from optical axis thicker in the thinner in the center center • there are focal points on both sides of each lens • focal length f on both sides is the same Ray diagram for converging lens Ray 1 is parallel to the axis and refracts through F. Ray 2 passes through F’ before refracting parallel to the axis. Ray 3 passes straight through the center of the lens. F I O F’ object between f and 2f: image is real, inverted, enlarged object outside of 2f: image is real, inverted, reduced object inside of f: image is virtual, upright, enlarged Ray diagram for diverging lens Ray 1 is parallel to the axis and refracts as if from F. -
Mirror Set for the Optics Expansion
Mirror Holders The mirror holders have the mirrors permanently mounted. Do not remove the Mirror Set mirrors. The convex mirror is fixed in position. The concave mirror can be rotated about a vertical axis in order to offset the image slightly to the half for the Optics screen. Screen Holder Assembly Expansion Kit A half screen is used so that light from a luminous source can pass (Order Code M-OEK) through the open area, reflect from the convex mirror, and then fall on the screen region. The Mirror Set consists of a concave mirror, a convex mirror, and a half screen. When used with components from the Optics Expansion Kit (order code OEK) and a Light Source Assembly (not included with Mirror Set) Vernier Dynamics Track (order code TRACK), basic experiments on mirror optics The light source is part of the Optics Expansion Kit, and is not part of the Mirror Set. can be performed. However, most experiments require the light source, so it is described here for The Mirror Set allows students to investigate image formation from concave and convenience. convex lenses. The light source uses a single white LED. A rotating plate lets you choose various types of light for experiments. The open hole exposes the LED to act as a point Parts included with the Mirror Set source. The other openings are covered by white plastic to Fixed Convex Mirror (–200 mm focal length, shown above at left) create luminous sources. The figure “4” is for studying image Half Screen (shown above, at middle) formation, and is chosen since it is not symmetric left-right or up-down. -
A Practical Guide to Panoramic Multispectral Imaging
A PRACTICAL GUIDE TO PANORAMIC MULTISPECTRAL IMAGING By Antonino Cosentino 66 PANORAMIC MULTISPECTRAL IMAGING Panoramic Multispectral Imaging is a fast and mobile methodology to perform high resolution imaging (up to about 25 pixel/mm) with budget equipment and it is targeted to institutions or private professionals that cannot invest in costly dedicated equipment and/or need a mobile and lightweight setup. This method is based on panoramic photography that uses a panoramic head to precisely rotate a camera and shoot a sequence of images around the entrance pupil of the lens, eliminating parallax error. The proposed system is made of consumer level panoramic photography tools and can accommodate any imaging device, such as a modified digital camera, an InGaAs camera for infrared reflectography and a thermal camera for examination of historical architecture. Introduction as thermal cameras for diagnostics of historical architecture. This article focuses on paintings, This paper describes a fast and mobile methodo‐ but the method remains valid for the documenta‐ logy to perform high resolution multispectral tion of any 2D object such as prints and drawings. imaging with budget equipment. This method Panoramic photography consists of taking a can be appreciated by institutions or private series of photo of a scene with a precise rotating professionals that cannot invest in more costly head and then using special software to align dedicated equipment and/or need a mobile and seamlessly stitch those images into one (lightweight) and fast setup. There are already panorama. excellent medium and large format infrared (IR) modified digital cameras on the market, as well as scanners for high resolution Infrared Reflec‐ Multispectral Imaging with a Digital Camera tography, but both are expensive. -
The F-Word in Optics
The F-word in Optics F-number, was first found for fixing photographic exposure. But F/number is a far more flexible phenomenon for finding facts about optics. Douglas Goodman finds fertile field for fixes for frequent confusion for F/#. The F-word of optics is the F-number,* also known as F/number, F/#, etc. The F- number is not a natural physical quantity, it is not defined and used consistently, and it is often used in ways that are both wrong and confusing. Moreover, there is no need to use the F-number, since what it purports to describe can be specified rigorously and unambiguously with direction cosines. The F-number is usually defined as follows: focal length F-number= [1] entrance pupil diameter A further identification is usually made with ray angle. Referring to Figure 1, a ray from an object at infinity that is parallel to the axis in object space intersects the front principal plane at height Y and presumably leaves the rear principal plane at the same height. If f is the rear focal length, then the angle of the ray in image space θ′' is given by y tan θ'= [2] f In this equation, as in the others here, a sign convention for angles heights and magnifications is not rigorously enforced. Combining these equations gives: 1 F−= number [3] 2tanθ ' For an object not at infinity, by analogy, the F-number is often taken to be the half of the inverse of the tangent of the marginal ray angle. However, Eq. 2 is wrong.