Characterization and Compensation of Stray Light Effects in Time of Flight Based Range Sensors

Total Page:16

File Type:pdf, Size:1020Kb

Characterization and Compensation of Stray Light Effects in Time of Flight Based Range Sensors Characterization and compensation of Stray light effects in Time of flight based range sensors Jonas Holmlund Master’s Thesis in Engineering Physics, Department of Physics, Umeå University, 2013 Department of physics Linnaeus väg 20 901 87 Umeå Sweden www.physics.umu.se Characterization and compensation of Stray light effects in Time of flight based range sensors Jonas Holmlund [email protected] MAY 2013 Supervisors: Emil Jonze Jonas Sjöberg Examiner: Ove Axner Abstract Recently much work has been done with the development of 3D real-time imagers, including the Time-of-flight (ToF) camera. This type of camera uses the principle of time of flight, in order to perform a distance measurement to every point in the field of view of the camera. This is done by sending a light signal towards the objects of the observed scene of the camera, where the light is reflected and returns to the camera. The signal is detected at the camera sensor, usually a CCD- or CMOS-chip with an array of pixels, where a distance measurement is made at every pixel, creating a 3D image of the whole scene. The problem is that some of the signal light travels through the optical system of the camera in a way that was not meant in the design. This light is called stray light. The measurement of the distance to different points within the field of view of the camera depends on the amount of light and the distance traveled by the light that reaches each and every one of the sensor pixels. This means that the effects of stray light will directly affect the accuracy of the depth data for the images when stray light spreads to different parts of the sensor. The purpose of this master thesis work was to devise a method, using computer software, that can be used in order to study stray light effects in order to reduce these effects. This has been done by running simulations of light emitted from predefined observed scenes entering a simulated model of the optical system of a ToF camera, using Zemax. The ray tracing data obtained in Zemax was then treated in Matlab, creating simulated ToF images, displaying the same stray light effects as real ToF images. A short analysis of the optical system was made using the simulated model. The results suggest that the reflective surface at the sensor, as well as an additional band-pass filter sometimes used to prevent light from external sources to enter the camera, were fundamental sources of stray light. Two algorithms, designed to correct the errors caused by stray light, were tested and evaluated. One used the properties of the evaluated incoming signal to approximate the contribution from stray light and subtract this contribution from the detected signal. The other method used filtering, approximating the distribution of light spread across the sensor in order to create an appropriate filter. Both methods show some promise, and could be used to decrease the effects of stray light, but the results can differ from case to case. The choice of certain weighting factors, when applying the algorithms, show different results when applied to different cases, where no optimized factors that work well for all measurement situations was found. Thus it is recommended that both methods are investigated and optimized further before being implemented in practice. Sammanfattning Den senaste tiden har mycket arbete utförts kring utvecklingen av 3D-sensorer som kan konstruera 3D-bilder i realtid. Detta inkluderar Time-of-Flight-kameror (TOF-kameror). Dessa kameror använder time-of-flight för att mäta avståndet till varje punkt i kamerans synfält. Kameran skickar en ljussignal mot objekten i kamerans synfält, vid vilka signalen reflekteras och återvänder till kameran. Signalen registreras vid en sensor i kameran, vanligen ett CCD- eller CMOS-chip konstruerad med en serie pixlar, där avståndet beräknas vid varje pixel. På så sätt erhålls en 3D-bild av hela omgivningen inom ToF-kamerans synfält på en gång. Ett problem är att en del av ljuset färdas genom kamerans linssystem på ett sätt som inte är beräknat eller förutsett vid designen av kameran. Detta ljus kallas för ströljus. Avståndsmätningen vid varje pixel beror både på hur mycket ljus som når pixlarna och hur långt detta ljus färdats. Detta gör att ströljus kan spridas över sensorn och påverkar direkt avståndsmätningen vid pixlarna. Syftet med detta exjobb är att komma på en metod, för att med hjälp av olika dataprogram, som kan användas för att studera ströljuseffekter, med målet att kunna bearbeta dessa effekter. Med programmet Zemax har simuleringar kunnat köras där ljus från olika objekt skickats in i en simulerad modell av kamerans linssystem. Data från dessa simuleringar har överförts till Matlab och behandlats för att göra simulerade ToF-bilder som visar samma inverkan av ströljus som riktiga ToF-bilder. En enkel optisk analys av det optiska systemet gjordes med modellen. Resultaten tyder på att de reflektiva ytorna hos glaset som täcker sensorns pixlar, kamerans inre hölje samt ett band- pass-filter, som ibland används för att filtrera ljus från övriga källor från att nå sensorn, är fundamentala källor till ströljus. Två algoritmer som designats för att korrigera de fel som uppstår p.g.a. ströljus testades och analyserades. Ena metoden använde signalljusets egenskaper för att bedöma hur mycket ströljuset bidrar till varje beräknat avståndsvärde för att subtrahera detta bidrag från den registrerade signalen. Den andra metoden använde sig utav approximationer för hur ljuset sprids över sensorn för att designa ett lämpligt filter som kan reducera ströljusets inverkan. Båda metoderna visade sig potentiellt kunna förbättra kamerans prestanda, men resultaten varierar något från fall till fall. Valet av värdet på vissa viktningsfaktorer som används för att justera algoritmernas effekter, gav varierande resultat beroende på mätsituationen. Inga optimerade värden, som fungerade bra för varenda mätsituation som testades, kunde bestämmas under projektet. Därför rekommenderas att vidare undersökning av dessa två algoritmer bör göras innan de tillämpas i praktiken. Preface This master’s thesis work was done in co-operation with the organizations Adopticum and Optronic, stationed in Skellefteå, Sweden. I would like to thank the people at Adopticum, particularly my supervisors Emil Jonze and Jonas Sjöberg, for giving me a lot of support and encouragement during my whole time of working with this thesis. I would also like to thank Emil Hällstig at Optronic, for presenting me the opportunity of doing this master’s thesis work as well as additional support during the project. Many thanks go to Bo Lindberg at Lens-Tech AB, who has offered a lot of help and teachings, valuable for the project. Also, I want to thank Ove Axner, at Umeå University, for taking the role as my examiner for this project. This has been a great experience for me. I’ve taken a big step towards the life outside the university. I’m looking forward to see what the future holds. Jonas Holmlund Table of Contents 1 INTRODUCTION .................................................................................................... 3 1.1 Background...................................................................................................................................................... 3 1.2 The purpose of this thesis ............................................................................................................................... 3 1.3 Restrictions ...................................................................................................................................................... 4 2 THEORY ............................................................................................................. 5 2.1 Time of flight ................................................................................................................................................... 5 2.1.1 The Time of Flight principle ...................................................................................................................... 5 2.1.2 Continuous wave modulation .................................................................................................................... 6 2.2 The camera – How it works ............................................................................................................................ 9 2.2.1 Components ............................................................................................................................................... 9 2.2.2 The sensor ................................................................................................................................................ 11 2.2.3 Partial reflection ....................................................................................................................................... 15 2.2.4 Other sources of error .............................................................................................................................. 18 3 METHOD ........................................................................................................... 21 3.1 General approach .......................................................................................................................................... 21 3.1.1 Running simulations ................................................................................................................................ 21 3.1.2 Treating data using Matlab .....................................................................................................................
Recommended publications
  • Boenig-Liptsin / Entrepreneurs of the Mind / 1 Citizen's Mind
    Margo Boenig-Liptsin SIGCIS Workshop, November 9, 2014 Work in !rogress Session "orking draft – please do not cite (ear SIGCIS Workshop !articipants) *hank you $or reading this partial draft of one of my dissertation 'hapters) I-m submitting to your review a draft of a 'hapter $rom the mi##&e of my dissertation, therefore to contextualize the "riting that you "i&& be reading, I inc&ude be&ow an abstract of my "hole dissertation project and a chapter out&ine. 2s you "i&& see, this early draft of Chapter 2 is based primari&y on empirical research of my three national cases1 I haven't yet integrated into it any secondary &iterature. I "ould be very gratef,& $or your suggestions of re$erences that you $eel "ould be interesting $or me to incorporate/refect upon, especial&y $rom the &iterature on the history of computing, given the topi's that I am exploring in this chapter or in the dissertation as a "hole. *his early draft is also missing complete $ootnotes—they are current&y 0ust notes $or mysel$ and references that I need to tidy up. I-m gratef,& $or al& of your comments, "hich "i&& no doubt make the next #raft of this signifcant&y better) Best "ishes, Margo (issertation abstract Making the Citi/en of the Information 2ge7 2 comparative study of computer &iteracy programs $or 'hi&dren, 1960s-1990s My dissertation is a comparative history of the frst computer &iteracy programs $or chi&dren. *he project examines how programs to introduce 'hi&dren to computers in the 9nited States, :rance, and the Soviet 9nion $rom the 1960s to 1990s embodied political, epistemic, and moral debates about the kind of citi/en required $or &i$e in the 21st century.
    [Show full text]
  • Stray Light Correction on Array Spectroradiometers for Optical Radiation Risk Assessment in the Workplace a Barlier-Salsi
    Stray light correction on array spectroradiometers for optical radiation risk assessment in the workplace A Barlier-Salsi To cite this version: A Barlier-Salsi. Stray light correction on array spectroradiometers for optical radiation risk assessment in the workplace. Journal of the Society for Radiological Protection, Institute of Physics (IOP), 2014, J. Radiol.Prot., 34 (4), pp.doi:10.1088/0952-4746/34/4/915. 10.1088/0952-4746/34/4/915. hal- 01148941 HAL Id: hal-01148941 https://hal.archives-ouvertes.fr/hal-01148941 Submitted on 5 May 2015 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. Stray light correction on array spectroradiometers for optical radiation risk assessment in the workplace A Barlier-Salsi Institut national de recherche et de sécurité (INRS) E-mail: [email protected] Abstract. The European directive 2006/25/EC requires the employer to assess and if necessary measure the levels of exposure to optical radiation in the workplace. Array spectroradiometers can measure optical radiation from various types of sources; however poor stray light rejection affects their accuracy. A stray light correction matrix, using a tunable laser, was developed at the National Institute of Standards and Technology (NIST).
    [Show full text]
  • Cpp-Skript SS18.Pdf
    Programmierung mit C++ für Computerlinguisten CIS, LMU München Max Hadersbeck Mitarbeiter Daniel Bruder, Ekaterina Peters, Jekaterina Siilivask, Kiran Wallner, Stefan Schweter, Susanne Peters, Nicola Greth — Version Sommersemester 2018 — Inhaltsverzeichnis 1 Einleitung1 1.1 Prozedurale und objektorientierte Programmiersprachen . .1 1.2 Encapsulation, Polymorphismus, Inheritance . .1 1.3 Statische und dynamische Bindung . .2 1.4 Die Geschichte von C++ . .2 1.5 Literaturhinweise . .3 2 Traditionelle und objektorientierte Programmierung4 2.1 Strukturiertes Programmieren . .4 2.2 Objektorientiertes Programmieren . .5 3 Grundlagen7 3.1 Installation von Eclipse und Übungsskript . .7 3.2 Starten eines C++ Programms . .7 3.3 Allgemeine Programmstruktur . .8 3.4 Kommentare in Programmen . 10 3.5 Variablen . 11 3.5.1 Was sind Variablen? . 11 3.5.2 Regeln für Variablen . 12 3.5.3 Grundtypen von Variablen . 12 3.5.4 Deklaration und Initialisierung von Variablen . 13 3.5.5 Lebensdauer von Variablen . 14 3.5.6 Gültigkeit von Variablen . 15 3.6 Namespace . 16 3.6.1 Defaultnamespace . 16 3.7 Zuweisen von Werten an eine Variable . 17 3.8 Einlesen und Ausgeben von Variablenwerten . 19 3.8.1 Einlesen von Daten . 19 3.8.2 Zeichenweises Lesen und Ausgeben von Daten . 21 3.8.3 Ausgeben von Daten . 22 3.8.4 Arbeit mit Dateien . 23 3.8.4.1 Textdateien unter Unix ................... 23 3.8.4.2 Textdateien unter Windows ................ 24 3.8.4.3 Lesen aus einer Datei . 25 3.8.4.4 Lesen aus einer WINDOWS Textdatei . 26 i ii Inhaltsverzeichnis 3.8.4.5 Schreiben in eine Datei . 26 3.9 Operatoren .
    [Show full text]
  • Landsat 9 Thermal Infrared Sensor 2 Preliminary Stray Light Assessment
    TIRS-2 Instrument Project Thermal Infrared Sensor-2 Landsat 9 Thermal Infrared Sensor 2 Preliminary Stray Light Assessment Joel McCorkel (NASA Goddard) Matt Montanaro (NASA Goddard) June Tveekrem (NASA Goddard) John Stauder (Space Dynamics Lab) Allen Lunsford (NASA Goddard) Eric Mentzell (NASA Goddard) Jason Hair (NASA Goddard) Dennis Reuter (NASA Goddard) 1 Stray Light Assessment Objective for TIRS-2 • Landsat 8 / Thermal Infrared Sensor – 1 (TIRS-1) has significant stray light in its optical system. • Landsat 9 / TIRS-2 is a near-replica of TIRS-1. • Stray light effects on TIRS-1 imagery have now been corrected in the ground processing system. • To prevent the problem with TIRS-2, the instrument has built-in mitigations to drastically reduce stray light. • Major effort to model and test the design changes in TIRS-2. • Results of the initial scattering measurements in thermo-vacuum conditions along with results of the optical scattering model are presented here. 2 Stray Light Problem on Landsat 8 / TIRS-1 • Landsat 8 / TIRS-1 instrument found to have a stray light issue where off-axis radiance scatters onto the focal plane. • Demonstrated through on-orbit out-of-field scans of the Moon. Moon position 15-deg Field-of-View & approx. size Detector A Detector B k-- bandlO ~ bandll Detector C Scattered Signal 3 Lunar Scans for TIRS-1 • Flagged lunar locations where scatter was recorded by the detectors. • Discovered that there 40 is a strong scattering 30 source in the optical system approximately 20 13-deg off-axis. 10 , 0)Q) I 0. • Very weak 22-deg "a;" o· Ol C: scatter also observed <:I'.: (not indicated here) Strong -30 13-deg scatter -40 Band 10 Band 11 -50 ~-~-~-~-~ -50 ~-~-~-~-~ -20 -10 0 10 20 -20 -10 0 10 20 Angle [D eg] Ang le [Deg] 4 Cause of Scattering for TIRS-1 • Detailed optical models pin-pointed scattering surface in the telescope.
    [Show full text]
  • The Space Infrared Interferometric Telescope (SPIRIT): High- Resolution Imaging and Spectroscopy in the Far-Infrared
    Leisawitz, D. et al., J. Adv. Space Res., in press (2007), doi:10.1016/j.asr.2007.05.081 The Space Infrared Interferometric Telescope (SPIRIT): High- resolution imaging and spectroscopy in the far-infrared David Leisawitza, Charles Bakera, Amy Bargerb, Dominic Benforda, Andrew Blainc, Rob Boylea, Richard Brodericka, Jason Budinoffa, John Carpenterc, Richard Caverlya, Phil Chena, Steve Cooleya, Christine Cottinghamd, Julie Crookea, Dave DiPietroa, Mike DiPirroa, Michael Femianoa, Art Ferrera, Jacqueline Fischere, Jonathan P. Gardnera, Lou Hallocka, Kenny Harrisa, Kate Hartmana, Martin Harwitf, Lynne Hillenbrandc, Tupper Hydea, Drew Jonesa, Jim Kellogga, Alan Koguta, Marc Kuchnera, Bill Lawsona, Javier Lechaa, Maria Lechaa, Amy Mainzerg, Jim Manniona, Anthony Martinoa, Paul Masona, John Mathera, Gibran McDonalda, Rick Millsa, Lee Mundyh, Stan Ollendorfa, Joe Pellicciottia, Dave Quinna, Kirk Rheea, Stephen Rineharta, Tim Sauerwinea, Robert Silverberga, Terry Smitha, Gordon Staceyf, H. Philip Stahli, Johannes Staguhn j, Steve Tompkinsa, June Tveekrema, Sheila Walla, and Mark Wilsona a NASA’s Goddard Space Flight Center, Greenbelt, MD b Department of Astronomy, University of Wisconsin, Madison, Wisconsin, USA c California Institute of Technology, Pasadena, CA, USA d Lockheed Martin Technical Operations, Bethesda, Maryland, USA e Naval Research Laboratory, Washington, DC, USA f Department of Astronomy, Cornell University, Ithaca, USA g Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA h Astronomy Department, University of Maryland, College Park, Maryland, USA i NASA’s Marshall Space Flight Center, Huntsville, Alabama, USA j SSAI, Lanham, Maryland, USA ABSTRACT We report results of a recently-completed pre-Formulation Phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25 - 400 µm.
    [Show full text]
  • A Python Implementation for Racket
    PyonR: A Python Implementation for Racket Pedro Alexandre Henriques Palma Ramos Thesis to obtain the Master of Science Degree in Information Systems and Computer Engineering Supervisor: António Paulo Teles de Menezes Correia Leitão Examination Committee Chairperson: Prof. Dr. José Manuel da Costa Alves Marques Supervisor: Prof. Dr. António Paulo Teles de Menezes Correia Leitão Member of the Committee: Prof. Dr. João Coelho Garcia October 2014 ii Agradecimentos Agradec¸o... Em primeiro lugar ao Prof. Antonio´ Leitao,˜ por me ter dado a oportunidade de participar no projecto Rosetta com esta tese de mestrado, por todos os sabios´ conselhos e pelos momentos de discussao˜ e elucidac¸ao˜ que se proporcionaram ao longo deste trabalho. Aos meus pais excepcionais e a` minha mana preferida, por me terem aturado e suportado ao longo destes quase 23 anos e sobretudo pelo incondicional apoio durante estes 5 anos de formac¸ao˜ superior. Ao pessoal do Grupo de Arquitectura e Computac¸ao˜ (Hugo Correia, Sara Proenc¸a, Francisco Freire, Pedro Alfaiate, Bruno Ferreira, Guilherme Ferreira, Inesˆ Caetano e Carmo Cardoso), por todas as sug- estoes˜ e pelo inestimavel´ feedback em artigos e apresentac¸oes.˜ Aos amigos em Tomar (Rodrigo Carrao,˜ Hugo Matos, Andre´ Marques e Rui Santos) e em Lisboa (Diogo da Silva, Nuno Silva, Pedro Engana, Kaguedes, Clara Paiva e Odemira), por terem estado pre- sentes, duma forma ou doutra, nos essenciais momentos de lazer. A` Fundac¸ao˜ para a Cienciaˆ e Tecnologia (FCT) e ao INESC-ID pelo financiamento e acolhimento atraves´ da atribuic¸ao˜ de uma bolsa de investigac¸ao˜ no ambitoˆ dos contratos Pest-OE/EEI/LA0021/2013 e PTDC/ATP-AQI/5224/2012.
    [Show full text]
  • Stray Light Measurement on Lenscheck™ Lens Measurement Systems
    Stray Light Measurement on LensCheck™ Lens Measurement Systems Optikos is seeing continued interest in measuring stray light from our customers’ products and anticipates substantial growth in suppliers and end-users specifying and testing stray light performance. This is encouraging as it shows an increasing appreciation for the significance of stray light in optical imaging systems. The LensCheck instrument is an ideal and affordable instrument for enabling measurement of both Veiling Glare Index and Glare Spread Function. Optikos LensCheck™ systems are designed to meet the increasing demand to measure the effects of stray light on optical imaging systems. Although unwanted light in a camera may pose a minor issue for the casual photographer, the resulting degradation in system performance in many industrial and automotive applications can represent significant financial costs, cause serious safety issues, or make or break a successful product launch. Manufacturers are asking vision systems to take on more and more challenging imaging tasks across non-ideal imaging environments. Many applications require imaging scenes with extraordinarily high dynamic range content. For example, automotive cameras must be able to identify a pedestrian or traffic light at night while also imaging an on-coming car’s headlights. This performance must be determined while viewing through protective windows that may be scratched or covered with debris. Windows, debris, optical elements, and even the sensor can result in unintended radiation striking the detector. This light can potentially overwhelm the desired signal and introduce computational errors. Above is an example of a ghost reflection that would be characterized in a GSF measurement. The designers, manufacturers and consumers of these lens and camera systems require a quantitative measurement of stray light.
    [Show full text]
  • Non-Destructive Characterization of Anti-Reflective Coatings on PV Modules
    1 Non-destructive Characterization of Anti-Reflective Coatings on PV Modules Todd Karin ∗, David Miller y, Anubhav Jain ∗ ∗Lawrence Berkeley National Laboratory, Berkeley, CA, U.S.A yNational Renewable Energy Laboratory, Golden, CO, U.S.A Abstract—Anti-reflective coatings (ARCs) are used on the vast example, multi-layer coatings composed of hard materials with majority of solar photovoltaic (PV) modules to increase power a high mechanical modulus have been found to be significantly production. However, ARC longevity can vary from less than 1 more durable to abrasion [7]. Because there are no pores, the year to over 15 years depending on coating quality and deploy- ment conditions. A technique that can quantify ARC degradation permeability of water is reduced, preventing moisture ingress non-destructively on commercial modules would be useful both and subsequent damage in the event of glass corrosion [8] of for in-field diagnostics and accelerated aging tests. In this paper, the underlying substrate and/or additional strain in the event we demonstrate that accurate measurements of ARC spectral of freezing. reflectance can be performed using a modified commercially- Although the single-layer ARCs on the market today can available integrating-sphere probe. The measurement is fast, accurate, non-destructive and can be performed outdoors in have an expected lifetime of 15 years [1], ARC lifetime full-sun conditions. We develop an interferometric model that depends on the coating deposition process [9] and deploy- estimates coating porosity, thickness and fractional area coverage ment conditions including heat, humidity, soiling and fre- from the measured reflectance spectrum for a uniform single- quency/method of cleaning.
    [Show full text]
  • Stray Light Measurement
    Stray Light Measurement on LensCheck™ Systems Haskell Kent, Roy Youman July 1, 2020 Copyright ©2020 Optikos Corporation Contents Section 1. Background .......................................................................................................................................... iv Section 2. What is Stray Light? .............................................................................................................................. v Section 3. How OpTest® Software Measures Stray Light .................................................................................... vi 3.1 Veiling Glare Index .................................................................................................................................... vi 3.2 How does the VGI measurement work with LensCheck and OpTest® 7?............................................... vii 3.3 What lenses can I test with the Stray Light Kit? ........................................................................................ ix 3.4 What are the limitations of the Stray Light Kit? ......................................................................................... ix 3.5 Glare Spread Function (GSF) .................................................................................................................... ix 3.6 How does the LensCheck’s new GSF measurement work with OpTest 7? ............................................... x 3.7 On what lenses can I measure GSF? ........................................................................................................
    [Show full text]
  • Telescope Stray Light Telescope Stray Light
    TELESCOPE STRAY LIGHT – FUNDAMENTAL OPTICAL PLUMBING & EARLY EXPERIENCE WITH SOFIA SOFIA SCIENCE CENTER PATRICK WADDELL 15FEB2017 1 STRAY LIGHT ENGINEERING: SUCCESSFUL SYSTEMS (STRUCTURES & COATINGS) FOR MILLENNIA 2 STRAY LIGHT ENGINEERING: NON-TRANSMISSIVE SOLUTIONS THROUGH MID- 20TH CENTURY 3 STRAY LIGHT FOR OPTICAL ASTRONOMY , DETECTING AND ANALYZING SCIENCE TARGETS AND TARGET FEATURES REQUIRES DIRECT SOURCE MEASUREMENT, USU ALLY T O SO ME QU ALITY, SUC H AS AT OR ABOVE A SPECIFIC S/N. DEF. STRAY LIGHT IS LIGHT CAPTURED & MEASURED WITHIN A SYSTEM THAT IS NOT FROM THE INTENDED SOURCE(S) BASED ON THE SENSOR DESIGN. THIS UNINTENDED SIGNAL CONTRIBUTES AMPLITUDE ERRORS, A MPLITUUUCUOOS(OSSO/SODE RELATED FLUCT U ATIO N NO I S E ( P O I SSON /SH O T NOISE), AND COMPLEX CALIBRATION PROBLEMS, SUCH AS CAUSTICS, AND VARIABLE CONTRIBUTIONS. 4 STRAY LIGHT STRAY LIGHT SOURCE EXAMPLES: . BRIGHT OBJECTS NEAR THE LINE OF SIGHT, MOON, PLANETS, ETC . SKY GLOW . THERMAL RADIATION ( IR A PPLICATIONS) . MICRO-ROUGH AND/OR CONTAMINATED OPTICAL SURFACES; “TURNED” EDGES . REFLECTIONS FROM BAFFLES & STRUCTURES . TRANSMISSIVE OPTICS INTERNAL REFLECTIONS; GRATING ORDER SEPARATION . DESIGN FLAWS THAT PERMIT LIGHT TO ENTER AND HIT DETECTORS DIRECTLY 5 STRAY LIGHT TO ACHIEVE THE DESIRED SCIENCE A NUMBER OF MEANS ARE EMPLOYED TO CONTROL BACKGROUND SIGNAL CONTRIBUTION: . BLOCKING: DESIGN & INCLUDE EFFECTIVE BAFFLES & STRUCTURES; DEFLECTION WITH SPECIAL OPTICS . ATTENUATING/SCATTERING: PROVIDE SURFACES WITH ABSORBING COATINGS, ALSO DIFFUSE/LAMBERTIAN – NON-SPECULAR PROPERTIES . REAL TIME MODULATION: CHOPPING & NODDING . MODEL BEFORE COMMITTING TO BUILD TO REDUCE PERFORMANCE RISKS: ASAP, APART/PADE, ZEMAX 6 STRAY LIGHT – THE SDSS 2.5M INDUSTRIAL SCALE IMAGING AND SPECTROMETRY IMAGING WAS THE DRIVER, DEFINED SYSTEM CHALLENGES: .
    [Show full text]
  • Correction of Stray Light in Spectrographs: Implications for Remote Sensing
    Correction of stray light in spectrographs: implications for remote sensing Yuqin Zong, Steven W. Brown, B. Carol Johnson, Keith R. Lykke, and Yoshi Ohno National Institute of Standards and Technology, Gaithersburg, MD 20899 ABSTRACT Spectrographs are used in a variety of applications in the field of remote sensing for radiometric measurements due to the benefits of measurement speed, sensitivity, and portability. However, spectrographs are single grating instruments that are susceptible to systematic errors arising from stray radiation within the instrument. In the application of measurements of ocean color, stray light of the spectrographs has led to significant measurement errors. In this work, a simple method to correct stray-light errors in a spectrograph is described. By measuring a set of monochromatic laser sources that cover the instrument’s spectral range, the instrument’s stray-light property is characterized and a stray-light correction matrix is derived. The matrix is then used to correct the stray-light error in measured raw signals by a simple matrix multiplication, which is fast enough to be implemented in the spectrograph’s firmware or software to perform real-time corrections: an important feature for remote sensing applications. The results of corrections on real instruments demonstrated that the stray-light errors were reduced by one to two orders of magnitude, to a level of approximately 10-5 for a broadband source measurement, which is a level less than one count of a 15-bit resolution instrument. As a stray-light correction example, the errors in measurement of solar spectral irradiance using a high- quality spectrograph optimized for UV measurements are analyzed; the stray-light correction leads to reduction of errors from a 10 % level to a 1 % level in the UV region.
    [Show full text]
  • The Improvement on the Performance of DMD Hadamard Transform Near-Infrared Spectrometer by Double Filter Strategy and a New Hadamard Mask
    micromachines Article The Improvement on the Performance of DMD Hadamard Transform Near-Infrared Spectrometer by Double Filter Strategy and a New Hadamard Mask Zifeng Lu 1,2, Jinghang Zhang 1, Hua Liu 1,2,*, Jialin Xu 3 and Jinhuan Li 1,2 1 Center for Advanced Optoelectronic Functional Materials Research, and Key Laboratory for UV-Emitting Materials and Technology of Ministry of Education, Northeast Normal University, 5268 Renmin Street, Changchun 130024, China; [email protected] (Z.L.); [email protected] (J.Z.); [email protected] (J.L.) 2 Demonstration Center for Experimental Physics Education, Northeast Normal University, 5268 Renmin Street, Changchun 130024, China 3 Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China; [email protected] * Correspondence: [email protected]; Tel.: +86-180-0443-0180 Received: 7 December 2018; Accepted: 15 February 2019; Published: 23 February 2019 Abstract: In the Hadamard transform (HT) near-infrared (NIR) spectrometer, there are defects that can create a nonuniform distribution of spectral energy, significantly influencing the absorbance of the whole spectrum, generating stray light, and making the signal-to-noise ratio (SNR) of the spectrum inconsistent. To address this issue and improve the performance of the digital micromirror device (DMD) Hadamard transform near-infrared spectrometer, a split waveband scan mode is proposed to mitigate the impact of the stray light, and a new Hadamard mask of variable-width stripes is put forward to improve the SNR of the spectrometer. The results of the simulations and experiments indicate that by the new scan mode and Hadamard mask, the influence of stray light is restrained and reduced.
    [Show full text]