Characterization and Compensation of Stray Light Effects in Time of Flight Based Range Sensors
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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Margo Boenig-Liptsin SIGCIS Workshop, November 9, 2014 Work in !rogress Session "orking draft – please do not cite (ear SIGCIS Workshop !articipants) *hank you $or reading this partial draft of one of my dissertation 'hapters) I-m submitting to your review a draft of a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. -
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). -
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 . -
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. -
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. -
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. -
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. -
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. -
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? ........................................................................................................ -
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: . -
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. -
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.