Section 9 Stops and Pupils

Total Page:16

File Type:pdf, Size:1020Kb

Section 9 Stops and Pupils 9-1 I and Instrumentation Design Optical OPTI-502 © Copyright 2019 John E. Greivenkamp E. John 2019 © Copyright Section 9 Stops and Pupils 9-2 I and Instrumentation Design Optical OPTI-502 Stops and Pupils Greivenkamp E. John 2019 © Copyright The aperture stop is the aperture in the system that limits the bundle of light that propagates through the system from the axial object point. The stop can be one of the lens apertures or a separate aperture (iris diaphragm) placed in the system, however, the stop is always a physical or real surface. The beam of light that propagates through an axially symmetric system from a on-axis point is shaped like a spindle. The entrance pupil (EP) is the image of the stop into object space, and the exit pupil (XP) is the image of the stop into image space. The pupils define the cones of light entering and exiting the optical system from any object point. XP EP Object Image z Stop There is a stop or pupil in each optical space. The EP is in the system object space, and the XP is in the system image space. Intermediate pupils are formed in other spaces. 9-3 I and Instrumentation Design Optical OPTI-502 Aperture Stop Greivenkamp E. John 2019 © Copyright The limiting aperture of the system may not be obvious. There are two common methods to determine which aperture in a system serves as the system stop: The first method is to image each potential stop into object space (use the optical surfaces between the potential stop and the object). The candidate pupil with the smallest angular size from the perspective of the axial object point corresponds to the stop. An analogous procedure can also be done in image space. Four apertures exist in this EP4 optical system. A EP3 EP1 1 EP2 A3 A 4 Each aperture is imaged into A2 object space to produced four potential EPs. z O EP2 has the smallest angular subtense as viewed from O. Aperture 2 is the system stop. Note: All of the potential EPs are in object space. EP4 and EP2 are virtual. Since lens A1 is the first optical element, its aperture is in object space, and A1 serves as EP1. 9-4 I and Instrumentation Design Optical OPTI-502 Aperture Stop Greivenkamp E. John 2019 © Copyright The second method to determine which aperture serves as the system stop is to trace a ray through the system from the axial object point with an arbitrary initial angle. At each aperture or potential stop, form the ratio of the aperture radius ak to the height of this ray at that surface y k . The stop is the aperture with the minimum ratio: a Aperture Stop Minimum k y k A 4 A6 A A3 1 A5 A2 a y 4 4 u0 z ak Scaled Ray: u0 is arbitrary Min yk The limiting ray is found by scaling the aa uukk yy initial ray: jjyy jj kkMIN MIN 9-5 I and Instrumentation Design Optical OPTI-502 Limiting Apertures Greivenkamp E. John 2019 © Copyright Large changes in object position may cause different apertures to serve as the limiting aperture or system stop. The EP with the smallest angular subtense can change. A different aperture would then become the system stop. However when designing a system, it is usually critical that the stop surface does not change over the range of possible object positions that the system will be used with. O1 O2 z EP1 EP2 9-6 I and Instrumentation Design Optical OPTI-502 Pupils Greivenkamp E. John 2019 © Copyright The pupil locations can be found by tracing a ray that goes through the center of the stop. The intersections of this ray with the axis in image space and object space determine the location of the exit and entrance pupils. L1 L2 z EP Stop XP The rays are extended to the axis to locate the pupil. The EP and the XP are often virtual. The EP is in the system object space, and the XP is L1 L2 in the system image space. z XP EP Stop 9-7 I and Instrumentation Design Optical OPTI-502 Intermediate Space Pupils Greivenkamp E. John 2019 © Copyright Intermediate pupils are formed in each optical space for multi-element systems. If there are N elements, there are N+1 pupils (including the stop). L2 L 1 L3 z Int. Pupil XP EP Stop 9-8 I and Instrumentation Design Optical OPTI-502 Marginal and Chief Rays Greivenkamp E. John 2019 © Copyright Rays confined to the y-z plane are called meridional rays. The marginal ray and the chief ray are two special meridional rays that together define the properties of the object, images, and pupils. The marginal ray starts at the axial object position, goes through the edge of the entrance pupil, and defines image locations and pupil sizes. It propagates to the edge of the stop and to the edge of the exit pupil. The chief ray starts at the edge of the object, goes through the center of the entrance pupil, and defines image heights and pupil locations. It goes through the center of the stop and the center of the exit pupil. y marginal ray height y chief ray height u marginal ray angle u chief ray angle Marginal Ray Object EP y y u u z Chief Ray 9-9 I and Instrumentation Design Optical OPTI-502 Images and Pupils Greivenkamp E. John 2019 © Copyright The heights of the marginal ray and the chief ray can be evaluated at any z in any optical space. Image When the marginal ray crosses the axis, an image is located, and the size of the image is yh given by the chief ray height in that plane. y0 z Whenever the chief ray crosses the axis, a Pupil pupil or the stop is located, and the pupil radius is given by the marginal ray height in yh that plane. PUPIL y0 z Intermediate images and pupils are often virtual. The chief ray is the axis of the unvignetted beam from a point at the edge of the field, and the radius of that beam at any cross section is equal to the marginal ray height in that plane. 9-10 I and Instrumentation Design Optical OPTI-502 On-Axis Ray Bundle Greivenkamp E. John 2019 © Copyright The stop limits the ray bundle from the axial object point. The marginal ray is at the edge of the on-axis ray bundle. The EP defines the ray bundle in object space from the axial object point. The ray bundle that will propagate through the system fills the EP. The XP defines the ray bundle converging to the axial image point in image space. The ray bundle emerging from the system appears to come from a filled XP. XP EP Object z Image Stop The stop and the intermediate image (not shown) define the ray bundle in the intermediate optical space. In any additional optical spaces, the intermediate pupils and images will define the ray bundles. 9-11 I and Instrumentation Design Optical OPTI-502 Ray Bundles Greivenkamp E. John 2019 © Copyright The pupils are the image of the stop and do not change position or size with an off-axis object. The EP and the XP also define the skewed ray bundles that enter and exit the optical system for an off-axis object point. The off-axis ray bundle that will propagate through the system fills the EP. The off-axis ray bundle emerging from the system appears to come from a filled XP. The skewed ray bundles are centered on the chief ray for that object point. XP EP Object z Image Stop 9-12 I and Instrumentation Design Optical OPTI-502 Vignetting Greivenkamp E. John 2019 © Copyright For an off-axis object point, the beam of light through the system is shaped like a spindle of skew cone-shaped sections as long as no aperture other than the stop limits the beam. If the beam is intercepted by one or more additional apertures, vignetting occurs. The top and or bottom of the ray bundle is clipped, and the beam of light propagating through the system no longer has a circular profile. For example, reducing the lens diameters in the previous example produces vignetting at the top of the first lens and the bottom of the second lens. Vignetting Object z Image XP Appearance: Stop Vignetting XP Vignetting Apertures Vignetted XP 9-13 I and Instrumentation Design Optical OPTI-502 Field of View Greivenkamp E. John 2019 © Copyright The Field of View FOV of an optical system is determined by the object size or the image size depending on the situation: - the maximum angular size of the object as seen from the entrance pupil - the maximum object height - the maximum image height - the maximum angular size of the image as seen from the exit pupil Field of View FOV: the diameter of the object/image Half Field of View HFOV: the radius of the object/image Full Field of View FFOV is sometimes used instead of FOV to emphasize that this is a diameter measure. 9-14 I and Instrumentation Design Optical OPTI-502 Field of View – Object Measures Greivenkamp E. John 2019 © Copyright EP HFOV 1/2 L h tan1/2 z L 1/2 h h u tan 1/ 2 L Since the EP is the reference position for the FOV, this defining ray becomes the chief ray of the system in object space. For distant objects, the apparent angular size of the object as viewed from the EP or from the front principal plane P or the nodal point N are approximately the same.
Recommended publications
  • 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.
    [Show full text]
  • Geometrical Irradiance Changes in a Symmetric Optical System
    Geometrical irradiance changes in a symmetric optical system Dmitry Reshidko Jose Sasian Dmitry Reshidko, Jose Sasian, “Geometrical irradiance changes in a symmetric optical system,” Opt. Eng. 56(1), 015104 (2017), doi: 10.1117/1.OE.56.1.015104. Downloaded From: https://www.spiedigitallibrary.org/journals/Optical-Engineering on 11/28/2017 Terms of Use: https://www.spiedigitallibrary.org/terms-of-use Optical Engineering 56(1), 015104 (January 2017) Geometrical irradiance changes in a symmetric optical system Dmitry Reshidko* and Jose Sasian University of Arizona, College of Optical Sciences, 1630 East University Boulevard, Tucson 85721, United States Abstract. The concept of the aberration function is extended to define two functions that describe the light irra- diance distribution at the exit pupil plane and at the image plane of an axially symmetric optical system. Similar to the wavefront aberration function, the irradiance function is expanded as a polynomial, where individual terms represent basic irradiance distribution patterns. Conservation of flux in optical imaging systems is used to derive the specific relation between the irradiance coefficients and wavefront aberration coefficients. It is shown that the coefficients of the irradiance functions can be expressed in terms of wavefront aberration coefficients and first- order system quantities. The theoretical results—these are irradiance coefficient formulas—are in agreement with real ray tracing. © 2017 Society of Photo-Optical Instrumentation Engineers (SPIE) [DOI: 10.1117/1.OE.56.1.015104] Keywords: aberration theory; wavefront aberrations; irradiance. Paper 161674 received Oct. 26, 2016; accepted for publication Dec. 20, 2016; published online Jan. 23, 2017. 1 Introduction the normalized field H~ and aperture ρ~ vectors.
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Nikon Binocular Handbook
    THE COMPLETE BINOCULAR HANDBOOK While Nikon engineers of semiconductor-manufactur- FINDING THE ing equipment employ our optics to create the world’s CONTENTS PERFECT BINOCULAR most precise instrumentation. For Nikon, delivering a peerless vision is second nature, strengthened over 4 BINOCULAR OPTICS 101 ZOOM BINOCULARS the decades through constant application. At Nikon WHAT “WATERPROOF” REALLY MEANS FOR YOUR NEEDS 5 THE RELATIONSHIP BETWEEN POWER, Sport Optics, our mission is not just to meet your THE DESIGN EYE RELIEF, AND FIELD OF VIEW The old adage “the better you understand some- PORRO PRISM BINOCULARS demands, but to exceed your expectations. ROOF PRISM BINOCULARS thing—the more you’ll appreciate it” is especially true 12-14 WHERE QUALITY AND with optics. Nikon’s goal in producing this guide is to 6-11 THE NUMBERS COUNT QUANTITY COUNT not only help you understand optics, but also the EYE RELIEF/EYECUP USAGE LENS COATINGS EXIT PUPIL ABERRATIONS difference a quality optic can make in your appre- REAL FIELD OF VIEW ED GLASS AND SECONDARY SPECTRUMS ciation and intensity of every rare, special and daily APPARENT FIELD OF VIEW viewing experience. FIELD OF VIEW AT 1000 METERS 15-17 HOW TO CHOOSE FIELD FLATTENING (SUPER-WIDE) SELECTING A BINOCULAR BASED Nikon’s WX BINOCULAR UPON INTENDED APPLICATION LIGHT DELIVERY RESOLUTION 18-19 BINOCULAR OPTICS INTERPUPILLARY DISTANCE GLOSSARY DIOPTER ADJUSTMENT FOCUSING MECHANISMS INTERNAL ANTIREFLECTION OPTICS FIRST The guiding principle behind every Nikon since 1917 product has always been to engineer it from the inside out. By creating an optical system specific to the function of each product, Nikon can better match the product attri- butes specifically to the needs of the user.
    [Show full text]
  • 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.
    [Show full text]
  • Technical Aspects and Clinical Usage of Keplerian and Galilean Binocular Surgical Loupe Telescopes Used in Dentistry Or Medicine
    Surgical and Dental Ergonomic Loupes Magnification and Microscope Design Principles Technical Aspects and Clinical Usage of Keplerian and Galilean Binocular Surgical Loupe Telescopes used in Dentistry or Medicine John Mamoun, DMD1, Mark E. Wilkinson, OD2 , Richard Feinbloom3 1Private Practice, Manalapan, NJ, USA 2Clinical Professor of Opthalmology at the University of Iowa Carver College of Medicine, Department of Ophthalmology and Visual Sciences, Iowa City, IA, USA, and the director, Vision Rehabilitation Service, University of Iowa Carver Family Center for Macular Degeneration 3President, Designs for Vision, Inc., Ronkonkoma, NY Open Access Dental Lecture No.2: This Article is Public Domain. Published online, December 2013 Abstract Dentists often use unaided vision, or low-power telescopic loupes of 2.5-3.0x magnification, when performing dental procedures. However, some clinically relevant microscopic intra-oral details may not be visible with low magnification. About 1% of dentists use a surgical operating microscope that provides 5-20x magnification and co-axial illumination. However, a surgical operating microscope is not as portable as a surgical telescope, which are available in magnifications of 6-8x. This article reviews the technical aspects of the design of Galilean and Keplerian telescopic binocular loupes, also called telemicroscopes, and explains how these technical aspects affect the clinical performance of the loupes when performing dental tasks. Topics include: telescope lens systems, linear magnification, the exit pupil, the depth of field, the field of view, the image inverting Schmidt-Pechan prism that is used in the Keplerian telescope, determining the magnification power of lens systems, and the technical problems with designing Galilean and Keplerian loupes of extremely high magnification, beyond 8.0x.
    [Show full text]
  • TELESCOPE to EYE ADAPTION for MAXIMUM VISION at DIFFERENT AGES. the Physiological Change of the Human Eye with Age Is Surely
    TELESCOPE TO EYE ADAPTION FOR MAXIMUM VISION AT DIFFERENT AGES. The physiological change of the human eye with age is surely contributing to the poorer shooting performance of older shooters. This is regardless of the fact that the refractive deviation of the eyes is generally faithfully corrected with lenses or surgery (laser procedures) and hopefully optometrically restored again to 6/6 effectiveness. Also, blurred eye lenses (cataracts) get replaced in the over sixty group. So, what then is the reason for seeing “poorer” through the telescope after the above? The table below speaks volumes about this. The iris opening (pupil size) of the eye determines the amount of light (the eye pupil in mm diameter) that enters the eye under specific light conditions. This amount of light, actually photons in the sight spectrum that contains the energy to activate the retina photoreceptors, again determines the clarity of the information / image interpreted by the brain via the retina's interaction. As we grow older, less light is entering the eye because the iris dilator muscle adaptability weakens as well as slows down. Average eye pupil diameter change versus age Day iris Night iris Age in years opening in opening in mm mm 20 4.7 8 30 4.3 7 40 3.9 6 50 3.5 5 60 3.1 4.1 70 2.7 3.2 80 2.3 2.5 The following calculations, based on the values in the table above, show how drastic these eye pupil changes are on our sight due to the less light that enters the eye.
    [Show full text]
  • Part 4: Filed and Aperture, Stop, Pupil, Vignetting Herbert Gross
    Optical Engineering Part 4: Filed and aperture, stop, pupil, vignetting Herbert Gross Summer term 2020 www.iap.uni-jena.de 2 Contents . Definition of field and aperture . Numerical aperture and F-number . Stop and pupil . Vignetting Optical system stop . Pupil stop defines: 1. chief ray angle w 2. aperture cone angle u . The chief ray gives the center line of the oblique ray cone of an off-axis object point . The coma rays limit the off-axis ray cone . The marginal rays limit the axial ray cone stop pupil coma ray marginal ray y field angle image w u object aperture angle y' chief ray 4 Definition of Aperture and Field . Imaging on axis: circular / rotational symmetry Only spherical aberration and chromatical aberrations . Finite field size, object point off-axis: - chief ray as reference - skew ray bundels: y y' coma and distortion y p y'p - Vignetting, cone of ray bundle not circular O' field of marginal/rim symmetric view ray RAP' chief ray - to distinguish: u w' u' w tangential and sagittal chief ray plane O entrance object exit image pupil plane pupil plane 5 Numerical Aperture and F-number image . Classical measure for the opening: plane numerical aperture (half cone angle) object in infinity NA' nsinu' DEnP/2 u' . In particular for camera lenses with object at infinity: F-number f f F# DEnP . Numerical aperture and F-number are to system properties, they are related to a conjugate object/image location 1 . Paraxial relation F # 2n'tanu' . Special case for small angles or sine-condition corrected systems 1 F # 2NA' 6 Generalized F-Number .
    [Show full text]
  • 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.
    [Show full text]
  • Lens Tutorial Is from C
    �is version of David Jacobson’s classic lens tutorial is from c. 1998. I’ve typeset the math and fixed a few spelling and grammatical errors; otherwise, it’s as it was in 1997. — Jeff Conrad 17 June 2017 Lens Tutorial by David Jacobson for photo.net. �is note gives a tutorial on lenses and gives some common lens formulas. I attempted to make it between an FAQ (just simple facts) and a textbook. I generally give the starting point of an idea, and then skip to the results, leaving out all the algebra. If any part of it is too detailed, just skip ahead to the result and go on. It is in 6 parts. �e first gives formulas relating object (subject) and image distances and magnification, the second discusses f-stops, the third discusses depth of field, the fourth part discusses diffraction, the fifth part discusses the Modulation Transfer Function, and the sixth illumination. �e sixth part is authored by John Bercovitz. Sometime in the future I will edit it to have all parts use consistent notation and format. �e theory is simplified to that for lenses with the same medium (e.g., air) front and rear: the theory for underwater or oil immersion lenses is a bit more complicated. Object distance, image distance, and magnification �roughout this article we use the word object to mean the thing of which an image is being made. It is loosely equivalent to the word “subject” as used by photographers. In lens formulas it is convenient to measure distances from a set of points called principal points.
    [Show full text]