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CIE Technical Note 004:2016
TECHNICAL NOTE The Use of Terms and Units in Photometry – Implementation of the CIE System for Mesopic Photometry CIE TN 004:2016 CIE TN 004:2016 CIE Technical Notes (TN) are short technical papers summarizing information of fundamental importance to CIE Members and other stakeholders, which either have been prepared by a TC, in which case they will usually form only a part of the outputs from that TC, or through the auspices of a Reportership established for the purpose in response to a need identified by a Division or Divisions. This Technical Note has been prepared by CIE Technical Committee 2-65 of Division 2 “Physical Measurement of Light and Radiation" and has been approved by the Board of Administration as well as by Division 2 of the Commission Internationale de l'Eclairage. The document reports on current knowledge and experience within the specific field of light and lighting described, and is intended to be used by the CIE membership and other interested parties. It should be noted, however, that the status of this document is advisory and not mandatory. Any mention of organizations or products does not imply endorsement by the CIE. Whilst every care has been taken in the compilation of any lists, up to the time of going to press, these may not be comprehensive. CIE 2016 - All rights reserved II CIE, All rights reserved CIE TN 004:2016 The following members of TC 2-65 “Photometric measurements in the mesopic range“ took part in the preparation of this Technical Note. The committee comes under Division 2 “Physical measurement of light and radiation”. -
Fundametals of Rendering - Radiometry / Photometry
Fundametals of Rendering - Radiometry / Photometry “Physically Based Rendering” by Pharr & Humphreys •Chapter 5: Color and Radiometry •Chapter 6: Camera Models - we won’t cover this in class 782 Realistic Rendering • Determination of Intensity • Mechanisms – Emittance (+) – Absorption (-) – Scattering (+) (single vs. multiple) • Cameras or retinas record quantity of light 782 Pertinent Questions • Nature of light and how it is: – Measured – Characterized / recorded • (local) reflection of light • (global) spatial distribution of light 782 Electromagnetic spectrum 782 Spectral Power Distributions e.g., Fluorescent Lamps 782 Tristimulus Theory of Color Metamers: SPDs that appear the same visually Color matching functions of standard human observer International Commision on Illumination, or CIE, of 1931 “These color matching functions are the amounts of three standard monochromatic primaries needed to match the monochromatic test primary at the wavelength shown on the horizontal scale.” from Wikipedia “CIE 1931 Color Space” 782 Optics Three views •Geometrical or ray – Traditional graphics – Reflection, refraction – Optical system design •Physical or wave – Dispersion, interference – Interaction of objects of size comparable to wavelength •Quantum or photon optics – Interaction of light with atoms and molecules 782 What Is Light ? • Light - particle model (Newton) – Light travels in straight lines – Light can travel through a vacuum (waves need a medium to travel in) – Quantum amount of energy • Light – wave model (Huygens): electromagnetic radiation: sinusiodal wave formed coupled electric (E) and magnetic (H) fields 782 Nature of Light • Wave-particle duality – Light has some wave properties: frequency, phase, orientation – Light has some quantum particle properties: quantum packets (photons). • Dimensions of light – Amplitude or Intensity – Frequency – Phase – Polarization 782 Nature of Light • Coherence - Refers to frequencies of waves • Laser light waves have uniform frequency • Natural light is incoherent- waves are multiple frequencies, and random in phase. -
Variable Star Photometry with a DSLR Camera
Variable star photometry with a DSLR camera Des Loughney Introduction now be studied. I have used the method to create lightcurves of stars with an amplitude of under 0.2 magnitudes. In recent years it has been found that a digital single lens reflex (DSLR) camera is capable of accurate unfiltered pho- tometry as well as V-filter photometry.1 Undriven cameras, Equipment with appropriate quality lenses, can do photometry down to magnitude 10. Driven cameras, using exposures of up to 30 seconds, can allow photometry to mag 12. Canon 350D/450D DSLR cameras are suitable for photome- The cameras are not as sensitive or as accurate as CCD try. My experiments suggest that the cameras should be cameras primarily because they are not cooled. They do, used with quality lenses of at least 50mm aperture. This however, share some of the advantages of a CCD as they allows sufficient light to be gathered over the range of have a linear response over a large portion of their range1 exposures that are possible with an undriven camera. For and their digital data can be accepted by software pro- bright stars (over mag 3) lenses of smaller aperture can be grammes such as AIP4WIN.2 They also have their own ad- used. I use two excellent Canon lenses of fixed focal length. vantages as their fields of view are relatively large. This makes One is the 85mm f1.8 lens which has an aperture of 52mm. variable stars easy to find and an image can sometimes in- This allows undriven photometry down to mag 8. -
Chapter 4 Introduction to Stellar Photometry
Chapter 4 Introduction to stellar photometry Goal-of-the-Day Understand the concept of stellar photometry and how it can be measured from astro- nomical observations. 4.1 Essential preparation Exercise 4.1 (a) Have a look at www.astro.keele.ac.uk/astrolab/results/week03/week03.pdf. 4.2 Fluxes and magnitudes Photometry is a technique in astronomy concerned with measuring the brightness of an astronomical object’s electromagnetic radiation. This brightness of a star is given by the flux F : the photon energy which passes through a unit of area within a unit of time. The flux density, Fν or Fλ, is the flux per unit of frequency or per unit of wavelength, respectively: these are related to each other by: Fνdν = Fλdλ (4.1) | | | | Whilst the total light output from a star — the bolometric luminosity — is linked to the flux, measurements of a star’s brightness are usually obtained within a limited frequency or wavelength range (the photometric band) and are therefore more directly linked to the flux density. Because the measured flux densities of stars are often weak, especially at infrared and radio wavelengths where the photons are not very energetic, the flux density is sometimes expressed in Jansky, where 1 Jy = 10−26 W m−2 Hz−1. However, it is still very common to express the brightness of a star by the ancient clas- sification of magnitude. Around 120 BC, the Greek astronomer Hipparcos ordered stars in six classes, depending on the moment at which these stars became first visible during evening twilight: the brightest stars were of the first class, and the faintest stars were of the sixth class. -
Lamp Catalog Ce
BRAT LE ING LAMP CATALOG CE YEARS 19 46 - 2016 CONTENTS CONTENTS COMPACT FLUORESCENT BUILDING A LEGACY ... 4-5 LED LAMPS 10-17 LAMPS 18-23 MAKE THE SWITCH. 6 Decorative Lamps ........................11 Twist Lamps. .19 General Purpose Lamps .................12 Covered Lamps .........................20 UNDERSTAND LIGHT ..... 7 Reflector Lamps ........................13 Reflector Lamps ........................20 LAMP PACKAGING ........ 8 Specialty General Purpose Lamps ........14 Pin Base Lamps. 21 Specialty Halogen Alternative Lamps .....14 Color Temperature ......................22 HOW TO Filament Lamps .........................15 Compact Fluorescent Lamp Base Types ..23 USE THIS CATALOG. 9 Linear Lamps ...........................16 Compact Fluorescent Lamp Shapes ......23 Recessed LED Downlights ...............16 LED Lamp Components .................17 LED Lamp Base Types ...................17 LED Lamp Shapes .......................17 To better serve you, Westinghouse Lighting reserves the right to make changes and/or improvements (both visually and technically) to the products in this catalog without notice. As a result, some products and/or product information may change during the life of this catalog. Visit our website for the latest specifications. www.westinghouselighting.com 1 CONTENTS INCANDESCENT LAMPS 24-47 Glowescent® Lamps (Spun Satin) .........25 BR38 Indoor/Outdoor Lamps ............37 Flicker Flame Lamps ....................25 C7 Lamps ..............................38 F15 and Decorative Specialty Lamps ......25 S6, S11 -
1 CMGT 235 – Electrical and Mechanical Systems Discussion No
CMGT 235 – Electrical and Mechanical Systems Discussion No. 25 Unit 3 - Electrical Systems Fall 2020 Commercial Building Electrical Systems - Lighting Systems Lighting Terminology Lamp Types Watts vs. Lumens Light Emitting Diode - LED 40W bulb: at least 450 lumens Fluorescent - FL 60W bulb: at least 800 lumens Compact Fluorescent (CFL) 75W bulb: at least 1,100 lumens Incandescent (INC) 100W bulb: at least 1,500 lumens Halogens High Intensity Discharge (HID) Fact: The more lumens of light you get per watt of High Pressure Sodium (HPS) electricity, the more efficient the bulb is. Metal Halide (MH) Mercury Vapor (MV) A 10W LED can easily outshine a 12W competitor if it Low Pressure Sodium converts watts to lumens more efficiently. Efficiency = lumens / watts 1 Light Emitting Diode – LED https://www.youtube.com/watch?v=oPYrldvk2is Energy-efficient LED bulbs are available in a variety of shapes and sizes. LEDs deliver quality light across a broad spectrum of color temperatures from warm ambient light to the bright white look of daylight, to suit any indoor or outdoor application. LED light bulbs, or light emitting diodes, are low heat, long lasting, energy efficient lighting alternatives for your home or business. The availability and selection of LED light bulbs has expanded greatly. No longer are LEDs just for exit signs. LEDs are available in almost all base and shape configurations. A Group: A15, A19, A21, and A25 From top left to bottom right: A19 LED filament bulbs in ceiling fan fixture, A21 LED bulbs in bedroom lamps, A19 gold-tint LED filament bulb in porch light fixture, A19 LED fireworks bulbs in string lights Standard/arbitrary (A) bulbs are the most widely used and thought of when it comes to household lighting. -
Basics of Photometry Photometry: Basic Questions
Basics of Photometry Photometry: Basic Questions • How do you identify objects in your image? • How do you measure the flux from an object? • What are the potential challenges? • Does it matter what type of object you’re studying? Topics 1. General Considerations 2. Stellar Photometry 3. Galaxy Photometry I: General Considerations 1. Garbage in, garbage out... 2. Object Detection 3. Centroiding 4. Measuring Flux 5. Background Flux 6. Computing the noise and correlated pixel statistics I: General Considerations • Object Detection How do you mathematically define where there’s an object? I: General Considerations • Object Detection – Define a detection threshold and detection area. An object is only detected if it has N pixels above the threshold level. – One simple example of a detection algorithm: • Generate a segmentation image that includes only pixels above the threshold. • Identify each group of contiguous pixels, and call it an object if there are more than N contiguous pixels I: General Considerations • Object Detection I: General Considerations • Object Detection Measuring Flux in an Image • How do you measure the flux from an object? • Within what area do you measure the flux? The best approach depends on whether you are looking at resolved or unresolved sources. Background (Sky) Flux • Background – The total flux that you measure (F) is the sum of the flux from the object (I) and the sky (S). F = I + S = #Iij + npix " sky / pixel – Must accurately determine the level of the background to obtaining meaningful photometry ! (We’ll return to this a bit later.) Photometric Errors Issues impacting the photometric uncertainties: • Poisson Error – Recall that the statistical uncertainty is Poisson in electrons rather than ADU. -
An Introduction to Photometry and Photometric Measurements Henry
An introduction to photometry and photometric measurements Henry Joy McCracken Institut d’Astrophysique de Paris What is photometry? • Photometry is concerned with obtaining quantitative physical measurements of astrophysical objects using electromagnetic radiation. • The challenge is to relate instrumental measurements (like electrons counted in an electronic detector) to physically meaningful quantities like flux and flux density • The ability to make quantitative measurements transformed astronomy from a purely descriptive science to one with great explanative power. To print higher-resolution math symbols, click the Hi-Res Fonts for Printing button on the jsMath control panel. Brightness and Flux Density Astronomers learn about an astronomical source by measuring the strength of its radiation as a function of direction on the sky (by mapping or imaging) and frequency (spectroscopy), plus other quantities (time, polarization) that we ignore for now. We need precise and quantitative definitions to describe the strength of radiation and how it varies with distance between the source and the observer. The concepts of brightness and flux density are deceptively simple, but they regularly trip up experienced astronomers. It is very important to understand them clearly because they are so fundamental. We start with the simplest possible case of radiation traveling from a source through empty space (so there is no absorption, scattering, or emission along the way) to an observer. In the ray-optics approximation, radiated energy flows in straight lines. This approximation is valid only for systems much larger than the wavelength of the radiation, a criterion easily met by astronomical sources. You may find it helpful to visualize electromagnetic radiation as a stream of light particles (photons), essentially bullets that travel in straight lines at the speed of light. -
Lamps & Fixtures
January 2019 LED Catalog Lamps & Fixtures · Winter 2018 selection. solutions. simplicity. eiko.com Contents LitespanLED® Replacement Lamps ...................................................... 2 HID Replacement Lamps.....................................................................................................................................2 Linear Tubes.............................................................................................................................................................. 5 A19/A21 Replacement Lamps .......................................................................................................................... 9 Filament Dimmable Decorative Lamps ......................................................................................................12 PL CFL Replacement Lamps ........................................................................................................................... 14 PLL Replacement Lamps .................................................................................................................................. 16 BR Replacement Lamps .....................................................................................................................................17 PAR Replacement Lamps ................................................................................................................................. 18 MR Replacement Lamps ................................................................................................................................ -
Light Bulb Cross Reference Chart
Light Bulb Cross Reference Chart Which Tray line-ups so modishly that Avram abjure her litholapaxy? Presented and toiling Richmond massagesqueue her railerthat kumquats bays half-wittedly duplicates or restrictedlyclamor unchangeably, and chords issteaming. Tedie unexalted? Uncursed Harland Here is measured by the chart and the same socket which are offered in it, volts and life tests are. Light Bulbs Etc Inc 0 items 000 Your shopping cart should empty Categories Incandescent Bulbs LED Products. Headlight bulb cross reference DodgeForumcom. Cross reference neon tubing chart for signage Light Sources. Replacement Bulb Cross Reference Chart Petco. Sylvania in candelabra and levering screwdrivers as auxiliary lighting, wiko and socket. Bulbs that is logged at the chart. Filament wire reduces thermal protector wiring, light to reference chart for ordering the lights better downroad, and any auto tale? These are bulbs that answer will remind in the charge with chance of them playing to key role in. Did a light? Austin machine and money for the amount of a cross reference. The light bulb cross referenced on the locking tab designs are. We will never guarantee a bulb reference from the lighting regulations within these cookies may be taken into consideration should be inadequate contact is copyrighted property of. 3157 Bulb Guide Today sulfur is tri cents LED precise and level one's a replacement for american car or motorcycle bulbs 3157 Bulb Cross Reference 3157 T25 3155. Looking for as rich text field within the lighting technologies including optimized energy costs. Auto Headlight Bulbs Cross Reference Guide LED-Colight. Light transparent cross reference Harley to regular Harley Davidson. -
Effect of Different Welding Methods on Flip-Chip LED (FC-LED) Filament Properties
applied sciences Article Effect of Different Welding Methods on Flip-Chip LED (FC-LED) Filament Properties Mengtian Li 1, Jun Zou 2,3,4,*, Wengjuan Wu 2,*, Mingming Shi 2, Bobo Yang 2,5, Wenbo Li 3 and Bin Guo 6 1 School of Material Science and Engineering, Shanghai Institute of Technology, Shanghai 201418, China; [email protected] 2 School of Science, Shanghai Institute of Technology, Shanghai 201418, China; [email protected] (M.S.); [email protected] (B.Y.) 3 Zhejiang Emitting Optoelectronic Technology Co., Ltd., Jiaxing 314100, China; [email protected] 4 Institute of New Materials & Industrial Technology, WenZhou University, Wenzhou 325000, China 5 Institute of Beyond Lighting, Academy for Engineering and Technology, Fudan University, Shanghai 200433, China 6 School of Electronics and Information Engineering, Changchun University of Science and Technology, Changchun 130022, China; [email protected] * Correspondence: [email protected] (J.Z.); [email protected] (W.W.) Received: 22 October 2018; Accepted: 7 November 2018; Published: 15 November 2018 Abstract: This paper investigates the effect of two different welding methods, direct welding (DW) and vacuum furnace welding (VFW), on flip-chip light-emitting diode (FC-LED) filament properties. Shearing force, SEM, steady-state voltage, steady-state luminous flux, and change of photoelectric performance with aging time were employed to characterize the differences in filament properties between the two welding methods. The shearing test revealed that the average shearing force of the VFW group was higher than that of the DW group, but the two groups followed the standard. Furthermore, the microstructure of the VFW group fault was more smoother, and the voids were fewer and smaller based on the SEM test results. -
Radiometry and Photometry
Radiometry and Photometry Wei-Chih Wang Department of Power Mechanical Engineering National TsingHua University W. Wang Materials Covered • Radiometry - Radiant Flux - Radiant Intensity - Irradiance - Radiance • Photometry - luminous Flux - luminous Intensity - Illuminance - luminance Conversion from radiometric and photometric W. Wang Radiometry Radiometry is the detection and measurement of light waves in the optical portion of the electromagnetic spectrum which is further divided into ultraviolet, visible, and infrared light. Example of a typical radiometer 3 W. Wang Photometry All light measurement is considered radiometry with photometry being a special subset of radiometry weighted for a typical human eye response. Example of a typical photometer 4 W. Wang Human Eyes Figure shows a schematic illustration of the human eye (Encyclopedia Britannica, 1994). The inside of the eyeball is clad by the retina, which is the light-sensitive part of the eye. The illustration also shows the fovea, a cone-rich central region of the retina which affords the high acuteness of central vision. Figure also shows the cell structure of the retina including the light-sensitive rod cells and cone cells. Also shown are the ganglion cells and nerve fibers that transmit the visual information to the brain. Rod cells are more abundant and more light sensitive than cone cells. Rods are 5 sensitive over the entire visible spectrum. W. Wang There are three types of cone cells, namely cone cells sensitive in the red, green, and blue spectral range. The approximate spectral sensitivity functions of the rods and three types or cones are shown in the figure above 6 W. Wang Eye sensitivity function The conversion between radiometric and photometric units is provided by the luminous efficiency function or eye sensitivity function, V(λ).