LED Uniform Illumination Using Double Linear Fresnel Lenses for Energy Saving
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Energy Feedback Freeform Lenses for Uniform Illumination of Extended Light Source Leds
Energy feedback freeform lenses for uniform illumination of extended light source LEDs 1 1 2 1 1,* ZONGTAO LI, SHUDONG YU, LIWEI LIN , YONG TANG, XINRUI DING, WEI 1 1 YUAN, BINHAI YU 1 Key Laboratory of Surface Functional Structure Manufacturing of Guangdong High Education Institutes, South China University of Technology, Guangzhou 510640, China 2 Department of Mechanical Engineering, University of California, Berkeley, California 94720, United States *Corresponding author: [email protected] Received XX Month XXXX; revised XX Month, XXXX; accepted XX Month XXXX; posted XX Month XXXX (Doc. ID XXXXX); published XX Month XXXX Using freeform lenses to construct uniform illumination systems is important in light-emitting diode (LED) devices. In this paper, the energy feedback design is used for freeform lens (EFFL) constructions by solving a set of partial differential equations that describe the mapping relationships between the source and the illumination pattern. The simulation results show that the method can overcome the illumination deviation caused by the extended light source (ELS) problem. Furthermore, a uniformity of 95.6% is obtained for chip-on-board (COB) compact LED devices. As such, prototype LEDs manufactured with the proposed freeform lenses demonstrate significant improvements in luminous efficiency and emission uniformity. © 2016 Optical Society of America OCIS codes: (220.4298) Nonimaging optics; (220.2945) Illumination design; (230.3670) Light-emitting diodes. sources (PLSs). For LED applications, the brightness of these LEDs is 1. Introduction not sufficient. Although a module with multiple sources makes it possible to obtain sufficient luminous flux, Kuo found that such a Solid-state lighting devices, especially light-emitting diodes (LEDs), solution would lead to the “multi-shadow” phenomenon, which causes have gained attention recently as a result of their outstanding features the eyes to feel tired [9]. -
Design and Testing of Collimators for Use in Measuring X-Ray Attenuation
DESIGN AND TESTING OF COLLIMATORS FOR USE IN MEASURING X-RAY ATTENUATION By RAJESH PANTHI Master of Science (M.Sc.) in Physics Tribhuvan University Kathmandu, Nepal 2009 Submitted to the Faculty of the Graduate College of the Oklahoma State University in partial fulfillment of the requirements for the Degree of MASTER OF SCIENCE December, 2017 DESIGN AND TESTING OF COLLIMATORS FOR USE IN MEASURING X-RAY ATTENUATION Thesis Approved: Dr. Eric R. Benton Thesis Adviser and Chair Dr. Eduardo G. Yukihara Dr. Mario F. Borunda ii ACKNOWLEDGEMENTS I would like to express the deepest appreciation to my thesis adviser As- sociate Professor Dr. Eric Benton of the Department of Physics at Oklahoma State University for his vigorous guidance and help in the completion of this work. He provided me all the academic resources, an excellent lab environment, financial as- sistantship, and all the lab equipment and materials that I needed for this project. I am grateful for many skills and knowledge that I gained from his classes and personal discussion with him. I would like to thank Adjunct Profesor Dr. Art Lucas of the Department of Physics at Oklahoma State University for guiding me with his wonderful experience on the Radiation Physics. My sincere thank goes to the members of my thesis committee: Professor Dr. Eduardo G. Yukihara and Assistant Professor Dr. Mario Borunda of the Department of Physics at Oklahoma State University for generously offering their valuable time and support throughout the preparation and review of this document. I would like to thank my colleague Mr. Jonathan Monson for helping me to access the Linear Accelerators (Linacs) in St. -
Roland Winston
Science of Nonimaging Optics: The Thermodynamic Connection Roland Winston Schools of Natural Science and Engineering, University of California Merced Director, California Advanced Solar Technologies Institute (UC Solar) [email protected] http://ucsolar.org SinBerBEST) annual meeting for 2013. Singapore Keynote Lecture 1:30 – 2:00 January 9, 2013 Solar Energy 2 Applications 3 The Stefan Boltzmann law s T4 is on page 1 of an optics book--- Something interesting is going on ! What is the best efficiency possible? When we pose this question, we are stepping outside the bounds of a particular subject. Questions of this kind are more properly the province of thermodynamics which imposes limits on the possible, like energy conservation and the impossible, like transferring heat from a cold body to a warm body without doing work. And that is why the fusion of the science of light (optics) with the science of heat (thermodynamics), is where much of the excitement is today. During a seminar I gave some ten years ago at the Raman Institute in Bangalore, the distinguished astrophysicist Venkatraman Radhakrishnan famously asked “how come geometrical optics knows the second law of thermodynamics?” This provocative question from C. V. Raman’s son serves to frame our discussion. Nonimaging Optics 5 During a seminar at the Raman Institute (Bangalore) in 2000, Prof. V. Radhakrishnan asked me: How does geometrical optics know the second law of thermodynamics? A few observations suffice to establish the connection. As is well-known, the solar spectrum fits a black body at 5670 K (almost 10,000 degrees Fahrenheit) Now a black body absorbs radiation at all wavelengths, and it follows from thermodynamics that its spectrum (the Planck spectrum1) is uniquely specified by temperature. -
High Collection Nonimaging Optics
High Collection Nonimaging Optics W. T. WELFORD Optics Section Department of Physics Imperial College of Science, Technology and Medicine University of London London, England R. WINSTON Enrico Fermi Institute and Department of Physics University of Chicago Chicago, Illinois ® ACADEMIC PRESS, INC. Harcourt Brace Jovanovich, Publishers San Diego New York Berkeley Boston London Sydney Tokyo Toronto Contents Preface xi Chapter 1 Concentrators and Their Uses 1.1 Concentrating Collectors 1 1.2 Definition of the Concentration Ratio; the Theoretical Maximum 3 1.3 Uses of Concentrators 6 Chapter 2 Some Basic Ideas in Geometrical Optics 2.1 The Concepts of Geometrical Optics 9 2.2 Formulation of the Ray-Tracing Procedure 10 2.3 Elementary Properties of Image-Forming Optical Systems 14 2.4 Aberrations in Image-Forming Optical Systems 16 2.5 The Effect of Aberrations in an Image-Forming System on the Concentration Ratio 18 2.6 The Optical Path Length and Fermat's Principle 20 2.7 The Generalized Etendue or Lagrange Invariant and the Phase Space Concept 22 2.8 The Skew Invariant 28 2.9 Different Versions of the Concentration Ratio 28 Chapter 3 Some Designs of Image-Forming Concentrators 3.1 Introduction 31 3.2 Some General Properties of Ideal Image-Forming Concentrators 31 V/ Contents 3.3 Can an Ideal Image-Forming Concentrator Be Designed? 39 3.4 Media with Continuously Varying Refractive Index 44 3.5 Another System of Spherical Symmetry 46 3.6 Image-Forming Mirror Systems 48 3.7 Conclusions on Image-Forming Concentrators 50 Chapter 4 Nonimaging -
RX and RXI® for Optical Wireless Communications
Ultra compact optics for optical wireless communications Juan C. Miñano, Pablo Benítez, Rubén Mohedano, José L. Alvarez, Maikel Hernández, Juan C. González*, Kazutoshi Hirohashi**, Satoru Toguchi** IES, E.T.S.I. Telecomunicación, Universidad Politécnica de Madrid, 28040 Madrid, Spain *Universidad Europea de Madrid, Villaviciosa de Odón, Madrid, Spain **HITS (High Speed Infrared Transmission Systems) Laboratories, Inc., 2-16-16 Chuourinkan, Yamato, 242-0007 Japan ABSTRACT Advanced optical design methods [J.C. Miñano, J.C. González, “New method of design of nonimaging concentrators”, Appl. Opt. 31, 1992, pp.3051-3060] using the keys of nonimaging optics lead to some ultra compact designs which combine the concentrating (or collimating) capabilities of conventional long focal length systems with a high collection efficiency [J.C. Miñano, J.C. González, P. Benítez, “A high gain, compact, nonimaging concentrator: the RXI”, Appl. Opt. 34, 1995, pp. 7850-7856 ][ J.C. Miñano, P. Benítez, J.C. González, “RX: a nonimaging concentrator”, Appl. Opt. 34, 1995, pp. 2226- 2235]. One of those designs is the so-called RXI. Its aspect ratio (thickness/aperture diameter) is less than 1/3. Used as a receiver, i.e. placing a photodiode at the proper position, it gets an irradiance concentration of the 95% of the theoretical thermodynamic limit (this means for example, a concentration of 1600 times with an acceptance angle of ±2.14 degrees). When used as an emitter (replacing the aforementioned photodiode by an LED, for instance), similar intensity gains may be obtained within an angle cone almost as wide as the 95% of the thermodynamic limit. In a real device these irradiance (and intensity) gains are reduced by the optical efficiency. -
Repeating Fast Radio Bursts Caused by Small Bodies Orbiting a Pulsar Or a Magnetar Fabrice Mottez1, Philippe Zarka2, and Guillaume Voisin3,1
A&A 644, A145 (2020) Astronomy https://doi.org/10.1051/0004-6361/202037751 & c F. Mottez et al. 2020 Astrophysics Repeating fast radio bursts caused by small bodies orbiting a pulsar or a magnetar Fabrice Mottez1, Philippe Zarka2, and Guillaume Voisin3,1 1 LUTH, Observatoire de Paris, PSL Research University, CNRS, Université de Paris, 5 Place Jules Janssen, 92190 Meudon, France e-mail: [email protected] 2 LESIA, Observatoire de Paris, PSL Research University, CNRS, Université de Paris, Sorbonne Université, 5 Place Jules Janssen, 92190 Meudon, France 3 Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Manchester M19 9PL, UK Received 16 February 2020 / Accepted 1 October 2020 ABSTRACT Context. Asteroids orbiting into the highly magnetized and highly relativistic wind of a pulsar offer a favorable configuration for repeating fast radio bursts (FRB). The body in direct contact with the wind develops a trail formed of a stationary Alfvén wave, called an Alfvén wing. When an element of wind crosses the Alfvén wing, it sees a rotation of the ambient magnetic field that can cause radio-wave instabilities. In the observer’s reference frame, the waves are collimated in a very narrow range of directions, and they have an extremely high intensity. A previous work, published in 2014, showed that planets orbiting a pulsar can cause FRBs when they pass in our line of sight. We predicted periodic FRBs. Since then, random FRB repeaters have been discovered. Aims. We present an upgrade of this theory with which repeaters can be explained by the interaction of smaller bodies with a pulsar wind. -
A High Power Microwave Zoom Antenna with Metal Plate Lenses Julie Lawrance
University of New Mexico UNM Digital Repository Electrical and Computer Engineering ETDs Engineering ETDs 1-28-2015 A High Power Microwave Zoom Antenna With Metal Plate Lenses Julie Lawrance Follow this and additional works at: https://digitalrepository.unm.edu/ece_etds Recommended Citation Lawrance, Julie. "A High Power Microwave Zoom Antenna With Metal Plate Lenses." (2015). https://digitalrepository.unm.edu/ ece_etds/151 This Dissertation is brought to you for free and open access by the Engineering ETDs at UNM Digital Repository. It has been accepted for inclusion in Electrical and Computer Engineering ETDs by an authorized administrator of UNM Digital Repository. For more information, please contact [email protected]. Julie Lawrance Candidate Electrical Engineering Department This dissertation is approved, and it is acceptable in quality and form for publication: Approved by the Dissertation Committee: Dr. Christos Christodoulou , Chairperson Dr. Edl Schamilaglu Dr. Mark Gilmore Dr. Mahmoud Reda Taha i A HIGH POWER MICROWAVE ZOOM ANTENNA WITH METAL PLATE LENSES by JULIE LAWRANCE B.A., Physics, Occidental College, 1985 M.S. Electrical Engineering, 2010 DISSERTATION Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Engineering The University of New Mexico Albuquerque, New Mexico December, 2014 ii A HIGH POWER MICROWAVE ZOOM ANTENNA WITH METAL PLATE LENSES by Julie Lawrance B.A., Physics, Occidental College, 1985 M.S., Electrical Engineering, University of New Mexico, 2010 Ph.D., Engineering, University of New Mexico, 2014 ABSTRACT A high power microwave antenna with true zoom capability was designed and constructed with the use of metal plate lenses. Proof of concept was achieved through experiment as well as simulation. -
Optics Microstructured Optics SMS Design Methods Plastic Optics
www.led-professional.com ISSN 1993-890X Review LpR The technology of tomorrow for general lighting applications. Sept/Oct 2008 | Issue 09 Optics Microstructured Optics SMS Design Methods Plastic Optics LED Driver Circuits Display Report Copyright © 2008 Luger Research & LED-professional. All rights reserved. There are over 20 billion light fixtures using incandescent, halogen, Design of LED or fluorescent lamps worldwide. Many of these fixtures are used for directional light applications but are based on lamps that put Optics out light in all directions. The United States Department of Energy (DOE) states that recessed downlights are the most common installed luminaire type in new residential construction. In addition, the DOE reports that downlights using non-reflector lamps are typically only 50% efficient, meaning half the light produced by the lamp is wasted inside the fixture. In contrast, lighting-class LEDs offer efficient, directional light that lasts at least 50,000 hours. Indoor luminaires designed to take advantage of all the benefits of lighting-class LEDs can exceed the efficacy of any incandescent and halogen luminaire. Furthermore, these LEDs match the performance of even the best CFL (compact fluorescent) recessed downlights, while providing a lifetime five to fifty times longer before requiring maintenance. Lastly, this class of LEDs reduces the environmental impact of light (i.e. no mercury, less power-plant pollution, and less landfill waste). Classical LED optics is composed of primary a optics for collimation and a secondary optics, which produces the required irradiance distribution. Efficient elements for primary optics are concentrators, either using total internal reflection or combined refractive/reflective versions. -
Laser Collimated Beam Sensor LA SERIES ■■General Terms and Conditions
1053 Laser Collimated Beam Sensor LA SERIES ■ General terms and conditions ........... F-17 ■ Sensor selection guide ................. P.967~ FIBER Related Information SENSORS ■ About laser beam........................ P.1403~ ■ General precautions ..................... P.1405 LASER SENSORS PHOTOELECTRIC SENSORS Conforming to Conforming to FDA regulations EMC Directive MICRO (LA-511 only) PHOTOELECTRIC SENSORS AREA SENSORS LIGHT CURTAINS PRESSURE / FLOW SENSORS INDUCTIVE PROXIMITY SENSORS PARTICULAR USE SENSORS SENSOR LA-510 is classified as OPTIONS a Class 1 Laser Product SIMPLE in IEC / JIS standards. WIRE-SAVING LA-511 is a Class I Laser UNITS Product in FDA regulations WIRE-SAVING 21 CFR 1040.10. SYSTEMS Do not look at the laser MEASUREMENT beam through optical SENSORS panasonic-electric-works.net/sunx system such as a lens. STATIC CONTROL DEVICES ENDOSCOPE LASER “Class 1” laser beam sensor safe for your eyes MARKERS PLC / TERMINALS BASIC PERFORMANCE FUNCTIONS HUMAN MACHINE INTERFACES Safe laser beam LA-510 Easy laser beam alignment ENERGY CONSUMPTION VISUALIZATION This laser collimated beam sensor conforms to the Four monitoring LEDs help you to easily align the emitter COMPONENTS Class 1 laser stipulated in IEC 60825-1 and JIS C 6802. and the receiver. FA COMPONENTS Hence, safety measures such as protective gear are not necessary. MACHINE VISION Receiver front face SYSTEMS Precise sensing in wide area “DOWN” lights up UV CURING SYSTEMS Sensing area: 15 × 500 mm 0.591 × 19.685 in Minimum sensing object: ø0.1 mm ø0.004 in “LEFT” lights up The monitoring Repeatability: 10 µm 0.394 mil or less system checks whether the incident Sensing range beam falls evenly on Selection Emitter 500 mm 19.685 in Receiver “RIGHT” lights up Guide all the four receiving Laser “UP” lights up elements in the Displacement receiver window. -
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). -
A Gaussian Beam Shooting Algorithm for Radar Propagation Simulations Ihssan Ghannoum, Christine Letrou, Gilles Beauquet
A Gaussian beam shooting algorithm for radar propagation simulations Ihssan Ghannoum, Christine Letrou, Gilles Beauquet To cite this version: Ihssan Ghannoum, Christine Letrou, Gilles Beauquet. A Gaussian beam shooting algorithm for radar propagation simulations. RADAR 2009 : International Radar Conference ’Surveillance for a safer world’, Oct 2009, Bordeaux, France. hal-00443752 HAL Id: hal-00443752 https://hal.archives-ouvertes.fr/hal-00443752 Submitted on 4 Jan 2010 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A GAUSSIAN BEAM SHOOTING ALGORITHM FOR RADAR PROPAGATION SIMULATIONS Ihssan Ghannoum and Christine Letrou Gilles Beauquet Lab. SAMOVAR (UMR CNRS 5157) Surface Radar Institut TELECOM SudParis THALES Air Systems S.A. 9 rue Charles Fourier, 91011 Evry Cedex, France Hameau de Roussigny, 91470 Limours, France Emails: [email protected] Email: [email protected] [email protected] Abstract— Gaussian beam shooting is proposed as an al- ternative to the Parabolic Equation method or to ray-based techniques, in order to compute backscattered fields in the context of Non-Line-of-Sight ground-based radar. Propagated fields are represented as a superposition of Gaussian beams, which are launched from the emitting antenna and transformed through successive interactions with obstacles. -
Observation and Modeling of Solar Jets
Observation and Modeling of Solar Jets rspa.royalsocietypublishing.org 1 Yuandeng Shen 1 Invited Review Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China The solar atmosphere is full of complicated transients manifesting the reconfiguration of solar magnetic Article submitted to journal field and plasma. Solar jets represent collimated, beam-like plasma ejections; they are ubiquitous in the solar atmosphere and important for the Subject Areas: understanding of solar activities at different scales, Solar Physics, Plasma Physics, magnetic reconnection process, particle acceleration, Space Science coronal heating, solar wind acceleration, as well as other related phenomena. Recent high spatiotemporal Keywords: resolution, wide-temperature coverage, spectroscopic, Flares, Coronal Mass Ejections, and stereoscopic observations taken by ground-based and space-borne solar telescopes have revealed many Magnetic Fields, valuable new clues to restrict the development of Filaments/Prominences, Solar theoretical models. This review aims at providing the Energetic Particles, Magnetic reader with the main observational characteristics of Reconnection, solar jets, physical interpretations and models, as well Magnetohydrodynamic Simulation as unsolved outstanding questions in future studies. Author for correspondence: Yuandeng Shen 1. Introduction e-mail: [email protected] The dynamic solar atmosphere hosts many jetting phenomena that manifest as collimated plasma beams with a width ranging from several hundred to few times 5 10 km [1–5]; they are frequently accompanied by micro- flares, photospheric magnetic flux cancellations, and type III radio bursts, and can occur in all types of solar regions including active regions, coronal holes, and quiet-Sun regions. Since these jetting activities continuously supply mass and energy into the upper atmosphere, they are thought to be one of the important source for heating coronal plasma and accelerating solar wind [1,6–9].