Meta-Lens Doublet in the Visible Region Benedikt Groever, Wei Ting Chen, and Federico Capasso* Harvard John A
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Chapter 3 (Aberrations)
Chapter 3 Aberrations 3.1 Introduction In Chap. 2 we discussed the image-forming characteristics of optical systems, but we limited our consideration to an infinitesimal thread- like region about the optical axis called the paraxial region. In this chapter we will consider, in general terms, the behavior of lenses with finite apertures and fields of view. It has been pointed out that well- corrected optical systems behave nearly according to the rules of paraxial imagery given in Chap. 2. This is another way of stating that a lens without aberrations forms an image of the size and in the loca- tion given by the equations for the paraxial or first-order region. We shall measure the aberrations by the amount by which rays miss the paraxial image point. It can be seen that aberrations may be determined by calculating the location of the paraxial image of an object point and then tracing a large number of rays (by the exact trigonometrical ray-tracing equa- tions of Chap. 10) to determine the amounts by which the rays depart from the paraxial image point. Stated this baldly, the mathematical determination of the aberrations of a lens which covered any reason- able field at a real aperture would seem a formidable task, involving an almost infinite amount of labor. However, by classifying the various types of image faults and by understanding the behavior of each type, the work of determining the aberrations of a lens system can be sim- plified greatly, since only a few rays need be traced to evaluate each aberration; thus the problem assumes more manageable proportions. -
Synopsis of Technical Report
Tzu-Yu Wu October 26, 2011 Opti 521 – Fall 2011 Introductory to opto-mechanical engineering Synopsis of Technical Report J.M. Sasian. ”Design, assembly, and testing of an objective lens for a free-space photonic switching system”, Optical Engineering 32(8), 1871-1878 (August 1993) 1. Introduction In this paper, the design, lens tolerancing, assembly and testing of a lens with a high numerical aperture over a small field of view are discussed. Although this object lens is specifically designed for a free-space photonic switching system, the concepts in aberration corrections and the approaches to reach a high NA within small field of view are applicable in many applications such as microscope objective lens, laser scan lenses. It also serves as a nice guide for a lens designer to understand the whole process of making a lens system which is not only limited to lens design but included tolerancing, lens ordering, the strategy to maintain the budget, assembly and testing details, and the approximate time required for each task. 2. Summary of the synopsis This synopsis mainly focuses on the general concepts in lens design of a fast objective lens with small field of view. It starts with a brief introduction on the lens requirement and lists the common aberration correction methods. Some explanations in aberration corrections are referenced from “Introduction to Lens Design with practical ZEMAX examples” by Joseph M Geary. Lens tolerancing, assembly and testing are included. Details in phonic switching system are neglected. Interested reader can refer the original paper for more details. 3. Lens requirement Lens requirements Focal length: 15mm Focal ratio: 1.5 Field of View: 7 degrees Wavelength: 850 nm Mapping: F-sin( ) ±1.0 Image surface: Flat Performance: Strehl휃 ratio> 0.95휇푚 over the full field Telecentricity: In the image space Lenses: Glass all spherical surfaces Page 1 of 5 4. -
United States Patent (19) 11 Patent Number: 5,838,480 Mcintyre Et Al
USOO583848OA United States Patent (19) 11 Patent Number: 5,838,480 McIntyre et al. (45) Date of Patent: Nov. 17, 1998 54) OPTICAL SCANNING SYSTEM WITH D. Stephenson, “Diffractive Optical Elements Simplify DIFFRACTIVE OPTICS Scanning Systems”, Laser Focus World, pp. 75-80, Jun. 1995. 75 Inventors: Kevin J. McIntyre, Rochester; G. Michael Morris, Fairport, both of N.Y. 73 Assignee: The University of Rochester, Primary Examiner James Phan Rochester, N.Y. Attorney, Agent, or Firm M. Lukacher; K. Lukacher 57 ABSTRACT 21 Appl. No.: 639,588 22 Filed: Apr. 29, 1996 An improved optical System having diffractive optic ele ments is provided for Scanning a beam. This optical System (51) Int. Cl. ............................................... GO2B 26/08 includes a laser Source for emitting a laser beam along a first 52 U.S. Cl. .......................... 359/205; 359/206; 359/207; path. A deflector, Such as a rotating polygonal mirror, 359/212; 359/216; 359/17 intersects the first path and translates the beam into a 58 Field of Search ..................................... 359/205-207, Scanning beam which moves along a Second path in a Scan 359/212-219, 17, 19,563, 568-570,900 plane. A lens System (F-0 lens) in the Second path has first 56) References Cited and Second elements for focusing the Scanning beam onto an image plane transverse to the Scan plane. The first and U.S. PATENT DOCUMENTS Second elements each have a cylindrical, non-toric lens. One 4,176,907 12/1979 Matsumoto et al. .................... 359/217 or both of the first and second elements also provide a 5,031,979 7/1991 Itabashi. -
Characterisation Studies on the Optics of the Prototype Fluorescence Telescope FAMOUS
Characterisation studies on the optics of the prototype fluorescence telescope FAMOUS von Hans Michael Eichler Masterarbeit in Physik vorgelegt der Fakultät für Mathematik, Informatik und Naturwissenschaften der Rheinisch-Westfälischen Technischen Hochschule Aachen im März 2014 angefertigt im III. Physikalischen Institut A bei Prof. Dr. Thomas Hebbeker Erstgutachter und Betreuer Zweitgutachter Prof. Dr. Thomas Hebbeker Prof. Dr. Christopher Wiebusch III. Physikalisches Institut A III. Physikalisches Institut B RWTH Aachen University RWTH Aachen University Abstract In this thesis, the Fresnel lens of the prototype fluorescence telescope FAMOUS, which is built at the III. Physikalisches Institut of the RWTH Aachen, is characterised. Due to the usage of silicon photomultipliers as active detector component, an adequate optical performance is required. The optical performance and transmittance of the used Fresnel lens and the qualification for the operation in the fluorescence telescope FAMOUS is examined in several series of measurements and simulations. Zusammenfassung In dieser Arbeit wird die Fresnel-Linse des Prototyp-Fluoreszenz-Teleskops FAMOUS charakterisiert, welches am III. Physikalischen Institut der RWTH Aachen gebaut wird. Durch die Verwendung von Silizium-Photomultipliern als aktive Detektorkomponente werden besondere Anforderungen an die Optik des Teleskops gestellt. In verschiedenen Messreihen und Simulationen wird untersucht, ob die Abbildungsqualität und die Transmission der verwendeten Fresnel-Linse für die Verwendung in diesem Fluoreszenz- Teleskop geeignet ist. Contents 1. Introduction 1 2. Cosmic rays 3 2.1 Energy spectrum . 4 2.2 Sources of cosmic rays . 6 2.3 Extensive air showers . 7 3. Fluorescence light detection 11 3.1 Fluorescence yield . 11 3.2 The Pierre Auger fluorescence detector . 14 3.3 FAMOUS . -
Tessar and Dagor Lenses
Tessar and Dagor lenses Lens Design OPTI 517 Prof. Jose Sasian Important basic lens forms Petzval DB Gauss Cooke Triplet little stress Stressed with Stressed with Low high-order Prof. Jose Sasian high high-order aberrations aberrations Measuring lens sensitivity to surface tilts 1 u 1 2 u W131 AB y W222 B y 2 n 2 n 2 2 1 1 1 1 u 1 1 1 u as B y cs A y 1 m Bstop ystop n'u' n 1 m ystop n'u' n CS cs 2 AS as 2 j j Prof. Jose Sasian Lens sensitivity comparison Coma sensitivity 0.32 Astigmatism sensitivity 0.27 Coma sensitivity 2.87 Astigmatism sensitivity 0.92 Coma sensitivity 0.99 Astigmatism sensitivity 0.18 Prof. Jose Sasian Actual tough and easy to align designs Off-the-shelf relay at F/6 Coma sensitivity 0.54 Astigmatism sensitivity 0.78 Coma sensitivity 0.14 Astigmatism sensitivity 0.21 Improper opto-mechanics leads to tough alignment Prof. Jose Sasian Tessar lens • More degrees of freedom • Can be thought of as a re-optimization of the PROTAR • Sharper than Cooke triplet (low index) • Compactness • Tessar, greek, four • 1902, Paul Rudolph • New achromat reduces lens stress Prof. Jose Sasian Tessar • The front component has very little power and acts as a corrector of the rear component new achromat • The cemented interface of the new achromat: 1) reduces zonal spherical aberration, 2) reduces oblique spherical aberration, 3) reduces zonal astigmatism • It is a compact lens Prof. Jose Sasian Merte’s Patent of 1932 Faster Tessar lens F/5.6 Prof. -
Applied Physics I Subject Code: PHY-106 Set: a Section: …………………………
Test-1 Subject: Applied Physics I Subject Code: PHY-106 Set: A Section: ………………………….. Max. Marks: 30 Registration Number: ……………… Max. Time: 45min Roll Number: ………………………. Question 1. Define systematic and random errors. (5) Question 2. In an experiment in determining the density of a rectangular block, the dimensions of the block are measured with a vernier caliper with least count of 0.01 cm and its mass is measured with a beam balance of least count 0.1 g, l = 5.12 cm, b = 2.56 cm, t = 0.37 cm and m = 39.3 g. Report correctly the density of the block. (10) Question 3. Derive a relation to overcome chromatic aberration for an optical system consisting of two convex lenses. (5) Question 4. An achromatic doublet of focal length 20 cm is to be made by placing a convex lens of borosilicate crown glass in contact with a diverging lens of dense flint glass. Assuming nr = 1.51462, nb = ′ ′ 1.52264, 푛푟 = 1.61216, and 푛푏 = 1.62901, calculate the focal length of each lens; here the unprimed and the primed quantities refer to the borosilicate crown glass and dense flint glass, respectively. (10) Test-1 Subject: Applied Physics I Subject Code: PHY-106 Set: B Section: ………………………….. Max. Marks: 30 Registration Number: ……………… Max. Time: 45min Roll Number: ………………………. Question 1. Distinguish accuracy and precision with example. (5) Question 2. Obtain an expression for chromatic aberration in the image formed by paraxial rays. (5) Question 3. It is required to find the volume of a rectangular block. A vernier caliper is used to measure the length, width and height of the block. -
Carl Zeiss Oberkochen Large Format Lenses 1950-1972
Large format lenses from Carl Zeiss Oberkochen 1950-1972 © 2013-2019 Arne Cröll – All Rights Reserved (this version is from October 4, 2019) Carl Zeiss Jena and Carl Zeiss Oberkochen Before and during WWII, the Carl Zeiss company in Jena was one of the largest optics manufacturers in Germany. They produced a variety of lenses suitable for large format (LF) photography, including the well- known Tessars and Protars in several series, but also process lenses and aerial lenses. The Zeiss-Ikon sister company in Dresden manufactured a range of large format cameras, such as the Zeiss “Ideal”, “Maximar”, Tropen-Adoro”, and “Juwel” (Jewel); the latter camera, in the 3¼” x 4¼” size, was used by Ansel Adams for some time. At the end of World War II, the German state of Thuringia, where Jena is located, was under the control of British and American troops. However, the Yalta Conference agreement placed it under Soviet control shortly thereafter. Just before the US command handed the administration of Thuringia over to the Soviet Army, American troops moved a considerable part of the leading management and research staff of Carl Zeiss Jena and the sister company Schott glass to Heidenheim near Stuttgart, 126 people in all [1]. They immediately started to look for a suitable place for a new factory and found it in the small town of Oberkochen, just 20km from Heidenheim. This led to the foundation of the company “Opton Optische Werke” in Oberkochen, West Germany, on Oct. 30, 1946, initially as a full subsidiary of the original factory in Jena. -
Optical Systems for Laser Scanners1 to Provide Yet Another Perspective
2 OpticalSystemsforLaserScanners Stephen F. Sagan NeoOptics Lexington, Massachusetts, USA CONTENTS 2.1 Introduction .......................................................................................................................... 70 2.2 Laser Scanner Configurations ............................................................................................71 2.2.1 Objective Scanning..................................................................................................71 2.2.2 Post-objective Scanning ..........................................................................................72 2.2.3 Pre-objective Scanning............................................................................................72 2.3 Optical Design and Optimization: Overview .................................................................72 2.4 Optical Invariants ................................................................................................................ 74 2.4.1 The Diffraction Limit .............................................................................................. 76 2.4.2 Real Gaussian Beams .............................................................................................. 76 2.4.3 Truncation Ratio ....................................................................................................... 77 2.5 Performance Issues .............................................................................................................. 79 2.5.1 Image Irradiance ......................................................................................................79 -
Engineering an Achromatic Bessel Beam Using a Phase-Only Spatial Light Modulator and an Iterative Fourier Transformation Algorithm
Optics Communications 383 (2017) 64–68 Contents lists available at ScienceDirect Optics Communications journal homepage: www.elsevier.com/locate/optcom Engineering an achromatic Bessel beam using a phase-only spatial light modulator and an iterative Fourier transformation algorithm Marie Walde a, Aurélie Jost a, Kai Wicker a,b,c, Rainer Heintzmann a,c,n a Institut für Physikalische Chemie (IPC), Abbe Center of Photonics, Friedrich-Schiller-Universität, Jena, Germany b Carl Zeiss AG, Corporate Research and Technology, Jena, Germany c Leibniz Institute of Photonic Technology (IPHT), Jena, Germany article info abstract Article history: Bessel illumination is an established method in optical imaging and manipulation to achieve an extended Received 12 June 2016 depth of field without compromising the lateral resolution. When broadband or multicolour imaging is Received in revised form required, wavelength-dependent changes in the radial profile of the Bessel illumination can complicate 13 August 2016 further image processing and analysis. Accepted 21 August 2016 We present a solution for engineering a multicolour Bessel beam that is easy to implement and Available online 2 September 2016 promises to be particularly useful for broadband imaging applications. A phase-only spatial light mod- Keywords: ulator (SLM) in the image plane and an iterative Fourier Transformation algorithm (IFTA) are used to Bessel beam create an annular light distribution in the back focal plane of a lens. The 2D Fourier transformation of Spatial light modulator such a light ring yields a Bessel beam with a constant radial profile for different wavelength. Non-diffracting beams & 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND Iterative Fourier transform algorithm Frequency filtering license (http://creativecommons.org/licenses/by-nc-nd/4.0/). -
Utilization of a Curved Focal Surface Array in a 3.5M Wide Field of View Telescope
Utilization of a curved focal surface array in a 3.5m wide field of view telescope Lt. Col. Travis Blake Defense Advanced Research Projects Agency, Tactical Technology Office E. Pearce, J. A. Gregory, A. Smith, R. Lambour, R. Shah, D. Woods, W. Faccenda Massachusetts Institute of Technology, Lincoln Laboratory S. Sundbeck Schafer Corporation TMD M. Bolden CENTRA Technology, Inc. ABSTRACT Wide field of view optical telescopes have a range of uses for both astronomical and space-surveillance purposes. In designing these systems, a number of factors must be taken into account and design trades accomplished to best balance the performance and cost constraints of the system. One design trade that has been discussed over the past decade is the curving of the digital focal surface array to meet the field curvature versus using optical elements to flatten the field curvature for a more traditional focal plane array. For the Defense Advanced Research Projects Agency (DARPA) 3.5-m Space Surveillance Telescope (SST)), the choice was made to curve the array to best satisfy the stressing telescope performance parameters, along with programmatic challenges. The results of this design choice led to a system that meets all of the initial program goals and dramatically improves the nation’s space surveillance capabilities. This paper will discuss the implementation of the curved focal-surface array, the performance achieved by the array, and the cost level-of-effort difference between the curved array versus a typical flat one. 1. INTRODUCTION Curved-detector technology for applications in astronomy, remote sensing, and, more recently, medical imaging has been a component in the decision-making process for fielded systems and products in these and other various disciplines for many decades. -
Lens/Mirrors
Refractive Optical Design Systems Any lens system is a tradeoff of many factors Add optical elements (lens/mirrors) to balance these Many different types of lens systems used Want to look at each from the following Performance Requirements Resolution of the lens – how good at seeing fine details Also compensation to reduce lens aberrations Field of View: How much of a object is seen in the image from the lens system F# - that is how fast is the lens i.e. how good is the lens at low light exposures Packaging requirements- can you make it rugged & portable Spectral Range – what wavelengths do you want to see Also how to prevent chromatic aberrations Single Element Poor image quality with spherical lens Creates significant aberrations especially for small f# Aspheric lens better but much more expensive (2-3x higher $) Very small field of view High Chromatic Aberrations – only use for a high f# Need to add additional optical element to get better images However fine for some applications eg Laser with single line Where just want a spot, not a full field of view Landscape Lens Single lens but with aperture stop added i.e restriction on lens separate from the lens Lens is “bent” around the stop Reduces angle of incidence – thus off axis aberrations Aperture either in front or back Simplest cameras use this Achromatic Doublet Typically brings red and blue into same focus Green usually slightly defocused Chromatic blur 25x less than singlet (for f#=5 lens) Cemented achromatic doublet poor at low f# Slight improvement -
Lens Design OPTI 517 Seidel Aberration Coefficients
Lens Design OPTI 517 Seidel aberration coefficients Prof. Jose Sasian OPTI 517 Fourth-order terms 2 2 W H, W040 W131H W222 H 2 W220 H H W311H H H W400 H H Spherical aberration Coma Astigmatism (cylindrical aberration!) Field curvature Distortion Piston Prof. Jose Sasian OPTI 517 Coordinate system Prof. Jose Sasian OPTI 517 Spherical aberration h 2 h 4 Z 2r 8r 3 u h y1 y 2r W n'[PB'] n'[PA' ] n'[PB'] n[PB] We have a spherical surface of radius of curvature r, a ray intersecting the surface at point P, intersecting the reference sphere at B’, intersecting the wavefront in object space at B and in image space at A’, and passing in image space by the point Q’’ in the optical axis. The reference sphere in object space is centered at Q and in image space is centered at Q’ Question: how do we draw the first order Prof. Jose Sasian OPTI 517 marginal ray in image space? [PQ]2 s Z 2 h 2 s 2 2sZ Z 2 h 2 2 4 4 2 h h h h 2s 3 2 2r 8r 4r [PB] [OQ] [PQ] s 2 1 2 2 s h 2 1 1 h 4 1 1 h 4 1 1 2 2 s r 8r s r 8s s r 2 4 2 h s h s s 1 1 1 u s 2 r 4r 2 s 2 r h y1 y 2r Prof. Jose Sasian OPTI 517 Spherical aberration ' ' [PB] [OQ] [PQ] [PB'] [OQ ] [PQ ] 2 2 2 4 y 2 u 1 1 y 4 1 1 y u 1 1 y 1 1 1 y 1 y ' 2 ' 2 2 2r s r 8r s r 2 2r s r 8r s r 4 2 4 2 y 1 1 y 1 1 8s ' s ' r 8s s r W n '[PB'] n[PB] y 2 u 1 1 1 1 1 y n ' n ' 2 r s r s r y 4 1 1 1 1 n ' n 2 ' 8r s r s r 2 2 y 4 n ' 1 1 n 1 1 ' ' 8 s s r s s r Prof.