Visible Light-Based Human Visual System Conceptual Model
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1 LIGHT PHYSICS Light and Lighting Francesco Anselmo Light Intro Light Animates and Reveals Architecture
1 LIGHT PHYSICS Light and Lighting Francesco Anselmo Light intro Light animates and reveals architecture. Architecture cannot fully exist without light, since without light there would be nothing to see. Yet in architectural design light is usually either expected from nature or developed as an add-on attachment very late in the design process. The course explores the symbiotic relationship between architecture and light. As much as light can reveal architecture, architecture can animate light, making it bounce, scatter, refract, altering its spectrum and colour perception, absorbing it or reflecting it, modulating its path and strength in both space and time. It aims at developing a sensibility and intuition to the qualities of light, whilst giving the physical and computational tools to explore and validate design ideas. 4 7 1 2 5 3 6 1 LIGHT PHYSICS 4 LIGHT ELECTRIC 7 LIGHT CONNECTED 2 LIGHT BIOLOGY 5 LIGHT ARCHITECTURE 3 LIGHT NATURAL 6 LIGHT VIRTUAL Reading list Books Free online resources Bachelard, Gaston. The poetics of space, Beacon Press 1992 • http://hyperphysics.phy-astr.gsu.edu/hbase/ligcon.html Banham, Reyner. The architecture of the well-tempered Environment, Chicago University Press 1984 • http://thedaylightsite.com/ Bazerman, Charles. The languages of Edison’s light, MIT Press 2002 Berger, John. Ways of seeing, Pearson Education, Limited, 2002 • http://issuu.com/lightonline/docs/handbook-of-lighting-design Berger, John. About looking, Bloomsbury Publishing 2009 • http://www.radiance-online.org/ Bluhm, Andreas. Light! The industrial age 1750-1900, Carnegie Museum of Art 2000 Boyce, Peter R. Human Factors in Lighting, Taylor & Francis 2003 Calvino, Italo. -
7. Gamma and X-Ray Interactions in Matter
Photon interactions in matter Gamma- and X-Ray • Compton effect • Photoelectric effect Interactions in Matter • Pair production • Rayleigh (coherent) scattering Chapter 7 • Photonuclear interactions F.A. Attix, Introduction to Radiological Kinematics Physics and Radiation Dosimetry Interaction cross sections Energy-transfer cross sections Mass attenuation coefficients 1 2 Compton interaction A.H. Compton • Inelastic photon scattering by an electron • Arthur Holly Compton (September 10, 1892 – March 15, 1962) • Main assumption: the electron struck by the • Received Nobel prize in physics 1927 for incoming photon is unbound and stationary his discovery of the Compton effect – The largest contribution from binding is under • Was a key figure in the Manhattan Project, condition of high Z, low energy and creation of first nuclear reactor, which went critical in December 1942 – Under these conditions photoelectric effect is dominant Born and buried in • Consider two aspects: kinematics and cross Wooster, OH http://en.wikipedia.org/wiki/Arthur_Compton sections http://www.findagrave.com/cgi-bin/fg.cgi?page=gr&GRid=22551 3 4 Compton interaction: Kinematics Compton interaction: Kinematics • An earlier theory of -ray scattering by Thomson, based on observations only at low energies, predicted that the scattered photon should always have the same energy as the incident one, regardless of h or • The failure of the Thomson theory to describe high-energy photon scattering necessitated the • Inelastic collision • After the collision the electron departs -
Download the DIA Color Chart
DEMI-PERMANENT HAIRCOLOR 2 COMPLIMENTARY LINES OF HAIRCOLOR Each with its own benefit & expertise both provide maximum creativity & freedom ADVANCED ALKALINE TECHNOLOGY GENTLE ACID TECHNOLOGY HIGH PERFORMANCE HIGH PERFORMANCE • Demi-permanent crème • Luminous demi-permanent gel-crème • Rich tones, exceptional softness • Zero lift • Covers up to 70% grey • Intense care for the hair THE PROCESS THE PROCESS • Lifts (up to 1.5 Levels with 15-vol), then deposits • Zero lift, deposit only BEFORE COLOR DURING COLOR AFTER COLOR BEFORE COLOR DURING COLOR AFTER COLOR On natural hair, the cuticle The alkaline agents slightly open DIA Richesse has the ability to lighten up On color-treated & DIA Light has an acid The cationic polymers in scales are closed. the hair fiber allowing colorants to 1.5 levels, cover up to 70% white hair sensitized hair, the cuticle pH close to the natural pH of the hair. DIA Light have a resurfacing to penetrate the cuticle. & create rich, profound tones. scales are already open. effect on the cuticle, leaving There is no lift with gentle penetration the hair with amazing shine. of colorants for long lasting color. ADVANCED ALKALINE TECHNOLOGY ADVANCED ALKALINE TECHNOLOGY HIGH PERFORMANCE • Demi-permanent crème • Rich tones, exceptional softness • Covers up to 70% grey THE PROCESS • Lifts (up to 1.5 Levels with 15-vol), then deposits BEFORE COLOR DURING COLOR AFTER COLOR On natural hair, the cuticle The alkaline agents slightly open DIA Richesse has the ability to lighten scales are closed. the hair fiber allowing colorants up to 1.5 levels, cover up to 70% white to penetrate the cuticle. -
WHITE LIGHT and COLORED LIGHT Grades K–5
WHITE LIGHT AND COLORED LIGHT grades K–5 Objective This activity offers two simple ways to demonstrate that white light is made of different colors of light mixed together. The first uses special glasses to reveal the colors that make up white light. The second involves spinning a colorful top to blend different colors into white. Together, these activities can be thought of as taking white light apart and putting it back together again. Introduction The Sun, the stars, and a light bulb are all sources of “white” light. But what is white light? What we see as white light is actually a combination of all visible colors of light mixed together. Astronomers spread starlight into a rainbow or spectrum to study the specific colors of light it contains. The colors hidden in white starlight can reveal what the star is made of and how hot it is. The tool astronomers use to spread light into a spectrum is called a spectroscope. But many things, such as glass prisms and water droplets, can also separate white light into a rainbow of colors. After it rains, there are often lots of water droplets in the air. White sunlight passing through these droplets is spread apart into its component colors, creating a rainbow. In this activity, you will view the rainbow of colors contained in white light by using a pair of “Rainbow Glasses” that separate white light into a spectrum. ! SAFETY NOTE These glasses do NOT protect your eyes from the Sun. NEVER LOOK AT THE SUN! Background Reading for Educators Light: Its Secrets Revealed, available at http://www.amnh.org/education/resources/rfl/pdf/du_x01_light.pdf Developed with the generous support of The Charles Hayden Foundation WHITE LIGHT AND COLORED LIGHT Materials Rainbow Glasses Possible white light sources: (paper glasses containing a Incandescent light bulb diffraction grating). -
Light, Color, and Atmospheric Optics
Light, Color, and Atmospheric Optics GEOL 1350: Introduction To Meteorology 1 2 • During the scattering process, no energy is gained or lost, and therefore, no temperature changes occur. • Scattering depends on the size of objects, in particular on the ratio of object’s diameter vs wavelength: 1. Rayleigh scattering (D/ < 0.03) 2. Mie scattering (0.03 ≤ D/ < 32) 3. Geometric scattering (D/ ≥ 32) 3 4 • Gas scattering: redirection of radiation by a gas molecule without a net transfer of energy of the molecules • Rayleigh scattering: absorption extinction 4 coefficient s depends on 1/ . • Molecules scatter short (blue) wavelengths preferentially over long (red) wavelengths. • The longer pathway of light through the atmosphere the more shorter wavelengths are scattered. 5 • As sunlight enters the atmosphere, the shorter visible wavelengths of violet, blue and green are scattered more by atmospheric gases than are the longer wavelengths of yellow, orange, and especially red. • The scattered waves of violet, blue, and green strike the eye from all directions. • Because our eyes are more sensitive to blue light, these waves, viewed together, produce the sensation of blue coming from all around us. 6 • Rayleigh Scattering • The selective scattering of blue light by air molecules and very small particles can make distant mountains appear blue. The blue ridge mountains in Virginia. 7 • When small particles, such as fine dust and salt, become suspended in the atmosphere, the color of the sky begins to change from blue to milky white. • These particles are large enough to scatter all wavelengths of visible light fairly evenly in all directions. -
Photon Cross Sections, Attenuation Coefficients, and Energy Absorption Coefficients from 10 Kev to 100 Gev*
1 of Stanaaros National Bureau Mmin. Bids- r'' Library. Ml gEP 2 5 1969 NSRDS-NBS 29 . A111D1 ^67174 tioton Cross Sections, i NBS Attenuation Coefficients, and & TECH RTC. 1 NATL INST OF STANDARDS _nergy Absorption Coefficients From 10 keV to 100 GeV U.S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS T X J ". j NATIONAL BUREAU OF STANDARDS 1 The National Bureau of Standards was established by an act of Congress March 3, 1901. Today, in addition to serving as the Nation’s central measurement laboratory, the Bureau is a principal focal point in the Federal Government for assuring maximum application of the physical and engineering sciences to the advancement of technology in industry and commerce. To this end the Bureau conducts research and provides central national services in four broad program areas. These are: (1) basic measurements and standards, (2) materials measurements and standards, (3) technological measurements and standards, and (4) transfer of technology. The Bureau comprises the Institute for Basic Standards, the Institute for Materials Research, the Institute for Applied Technology, the Center for Radiation Research, the Center for Computer Sciences and Technology, and the Office for Information Programs. THE INSTITUTE FOR BASIC STANDARDS provides the central basis within the United States of a complete and consistent system of physical measurement; coordinates that system with measurement systems of other nations; and furnishes essential services leading to accurate and uniform physical measurements throughout the Nation’s scientific community, industry, and com- merce. The Institute consists of an Office of Measurement Services and the following technical divisions: Applied Mathematics—Electricity—Metrology—Mechanics—Heat—Atomic and Molec- ular Physics—Radio Physics -—Radio Engineering -—Time and Frequency -—Astro- physics -—Cryogenics. -
Chapter 30: Quantum Physics ( ) ( )( ( )( ) ( )( ( )( )
Chapter 30: Quantum Physics 9. The tungsten filament in a standard light bulb can be considered a blackbody radiator. Use Wien’s Displacement Law (equation 30-1) to find the peak frequency of the radiation from the tungsten filament. −− 10 1 1 1. (a) Solve Eq. 30-1 fTpeak =×⋅(5.88 10 s K ) for the peak frequency: =×⋅(5.88 1010 s−− 1 K 1 )( 2850 K) =× 1.68 1014 Hz 2. (b) Because the peak frequency is that of infrared electromagnetic radiation, the light bulb radiates more energy in the infrared than the visible part of the spectrum. 10. The image shows two oxygen atoms oscillating back and forth, similar to a mass on a spring. The image also shows the evenly spaced energy levels of the oscillation. Use equation 13-11 to calculate the period of oscillation for the two atoms. Calculate the frequency, using equation 13-1, from the inverse of the period. Multiply the period by Planck’s constant to calculate the spacing of the energy levels. m 1. (a) Set the frequency T = 2π k equal to the inverse of the period: 1 1k 1 1215 N/m f = = = =4.792 × 1013 Hz Tm22ππ1.340× 10−26 kg 2. (b) Multiply the frequency by Planck’s constant: E==×⋅ hf (6.63 10−−34 J s)(4.792 × 1013 Hz) =× 3.18 1020 J 19. The light from a flashlight can be considered as the emission of many photons of the same frequency. The power output is equal to the number of photons emitted per second multiplied by the energy of each photon. -
Physics, Chapter 40: Light As a Wave Motion
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Robert Katz Publications Research Papers in Physics and Astronomy 1-1958 Physics, Chapter 40: Light as a Wave Motion Henry Semat City College of New York Robert Katz University of Nebraska-Lincoln, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/physicskatz Part of the Physics Commons Semat, Henry and Katz, Robert, "Physics, Chapter 40: Light as a Wave Motion" (1958). Robert Katz Publications. 177. https://digitalcommons.unl.edu/physicskatz/177 This Article is brought to you for free and open access by the Research Papers in Physics and Astronomy at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Robert Katz Publications by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. 40 Light as a Wave Motion 40-1 Wave Versus Particle Let us recount some of the characteristics of the motion of particles and the propagation of waves, with a view toward analyzing the behavior of light. In accordance with Newton's first law, a particle moves in a straight-line path in the absence of external forces. Thus we might infer, as Newton suggested, that light is composed of particles, and that, in a continuous medium, there is no deflecting force on the light particles. At the interface between two media, light may be propagated in a straight line parallel to the interface. Thus even at an interface there is no force on the particles of light unless the light passes through the interface, and in that event the force acting must be perpendicular to the interface. -
The Basic Interactions Between Photons and Charged Particles With
Outline Chapter 6 The Basic Interactions between • Photon interactions Photons and Charged Particles – Photoelectric effect – Compton scattering with Matter – Pair productions Radiation Dosimetry I – Coherent scattering • Charged particle interactions – Stopping power and range Text: H.E Johns and J.R. Cunningham, The – Bremsstrahlung interaction th physics of radiology, 4 ed. – Bragg peak http://www.utoledo.edu/med/depts/radther Photon interactions Photoelectric effect • Collision between a photon and an • With energy deposition atom results in ejection of a bound – Photoelectric effect electron – Compton scattering • The photon disappears and is replaced by an electron ejected from the atom • No energy deposition in classical Thomson treatment with kinetic energy KE = hν − Eb – Pair production (above the threshold of 1.02 MeV) • Highest probability if the photon – Photo-nuclear interactions for higher energies energy is just above the binding energy (above 10 MeV) of the electron (absorption edge) • Additional energy may be deposited • Without energy deposition locally by Auger electrons and/or – Coherent scattering Photoelectric mass attenuation coefficients fluorescence photons of lead and soft tissue as a function of photon energy. K and L-absorption edges are shown for lead Thomson scattering Photoelectric effect (classical treatment) • Electron tends to be ejected • Elastic scattering of photon (EM wave) on free electron o at 90 for low energy • Electron is accelerated by EM wave and radiates a wave photons, and approaching • No -
Photons Outline
1 Photons Observational Astronomy 2019 Part 1 Prof. S.C. Trager 2 Outline Wavelengths, frequencies, and energies of photons The EM spectrum Fluxes, filters, magnitudes & colors 3 Wavelengths, frequencies, and energies of photons Recall that λν=c, where λ is the wavelength of a photon, ν is its frequency, and c is the speed of light in a vacuum, c=2.997925×1010 cm s–1 The human eye is sensitive to wavelengths from ~3900 Å (1 Å=0.1 nm=10–8 cm=10–10 m) – blue light – to ~7200 Å – red light 4 “Optical” astronomy runs from ~3100 Å (the atmospheric cutoff) to ~1 µm (=1000 nm=10000 Å) Optical astronomers often refer to λ>8000 Å as “near- infrared” (NIR) – because it’s beyond the wavelength sensitivity of most people’s eyes – although NIR typically refers to the wavelength range ~1 µm to ~2.5 µm We’ll come back to this in a minute! 5 The energy of a photon is E=hν, where h=6.626×10–27 erg s is Planck’s constant High-energy (extreme UV, X-ray, γ-ray) astronomers often use eV (electron volt) as an energy unit, where 1 eV=1.602176×10–12 erg 6 Some useful relations: E (erg) 14 ⌫ (Hz) = 1 =2.418 10 E (eV) h (erg s− ) ⇥ ⇥ c hc 1 1 1 λ (A)˚ = = = 12398.4 E− (eV− ) ⌫ ⌫ E (eV) ⇥ Therefore a photon with a wavelength of 10 Å has an energy of ≈1.24 keV 7 If a photon was emitted from a blackbody of temperature T, then the average photon energy is Eav~kT, where k = 1.381×10–16 erg K–1 = 8.617×10–5 eV K–1 is Boltzmann’s constant. -
Liquicolor Permanente Shades 07-10-12.Pdf
LIQUICOLOR PERMANENTE INTENSE INTENSE INTENSE INTENSE GOLD RED NEUTRAL (RN) INTENSE RED (RR) RED VIOLET (RV) RED VIOLET (RRV) BASE INTENSE NEUTRAL (NN) NEUTRAL (N) ASH (A) ASH (A) ASH (AA) ASH (AA) NEUTRAL(GN) GOLD (G) REDPELIRROJO NEUTRAL (RN) RED (R) INTENSEPELIRROJO RED (RR) REDPELIRROJO VIOLET (RV) REDPELIRROJO VIOLET (RRV) NEUTRAL INTENSO NEUTRAL CENIZO CENIZO CENIZO INTENSO CENIZO INTENSO DORADO NEUTRAL GOLDDORADO (G) PELIRROJONEUTRAL PELIRROJORED (R) PELIRROJOINTENSO PELIRROJOVIOLETA VIOLETAPELIRROJO INTENSO LEVEL/NIVEL DORADO NEUTRAL PELIRROJO INTENSO VIOLETA VIOLETA INTENSO 12 HIGH-LIFT BLONDE 12N/HL-N 12A/HL-V 12AA-B/HL-B 12AA-BV 12G / HL-G HIGH LIFT HIGH LIFT HIGH LIFT ULTRA HIGH LIFT ULTRA HIGH LIFT GOLDEN BLONDE NEUTRAL BLONDE COOL BLONDE COOL BLONDE BLUE COOL BLONDE BLUE VIOLET 10 LIGHTEST BLONDE RUBIO CLARÍSIMO 10N/12B1 10GN/12G2 OUR FIRST NN 10G / 12G LIGHTEST NEUTRAL BLONDE LIGHTEST GOLD LIQUID COLOR LIGHTEST GOLDEN BLONDE blondest beige NEUTRAL BLONDE blondest blonde blondest gold 9 VERY LIGHT BLONDE RUBIO MUY CLARO 9NN 9N/89N 9A/26D 9A-N/40D 9AA/20D 9AA-BV/30D VERY LIGHT RICH VERY LIGHT VERY LIGHT VERY LIGHT COOL VERY LIGHT ULTRA VERY LIGHT ULTRA COOL NEUTRAL BLONDE NEUTRAL BLONDE COOL BLONDE NEUTRAL BLONDE COOL BLONDE BLONDE BLUE VIOLET lightest neutral blonde winter wheat topaz arctic blonde flaxen blonde 8 LIGHT BLONDE RUBIO CLARO 8NN 8N/88N 8A / 28D 8GN/27G 8RN / 71RG 8R / 29R LIGHT RICH LIGHT LIGHT COOL BLONDE LIGHT GOLD NEUTRAL LIGHT RED NEUTRAL LIGHT RED BLONDE NEUTRAL BLONDE NEUTRAL BLONDE autumn mist BLONDE -
Light Search and Rescue Operations
Light Search and Rescue Operations CERT Basic Training Unit 5 Search and Rescue ● Consists of three separate operations . Sizeup: Using 9-step, continual model . Search: Locating victims and documenting . Rescue: Extricating victims CERT Basic Training 5-1 Unit 5: Light Search and Rescue Operations Deciding to Attempt Rescue ● Decision based on three factors . The risks involved for the rescuer . Greatest good for the greatest number . Resources and manpower available CERT Basic Training 5-2 Unit 5: Light Search and Rescue Operations Goals of Search and Rescue ● Rescue greatest number in shortest amount of time ● Get walking wounded out first ● Rescue lightly trapped victims next ● Keep the rescuer safe CERT Basic Training 5-3 Unit 5: Light Search and Rescue Operations Effective Search and Rescue ● Depends on: . Effective sizeup . Rescuer safety . Victim safety CERT Basic Training 5-4 Unit 5: Light Search and Rescue Operations Unit Objectives ● Identify sizeup requirements ● Describe most common search techniques ● Use safe techniques for debris removal ● Use safe techniques for victim extrication ● Describe ways to protect rescuers CERT Basic Training 5-5 Unit 5: Light Search and Rescue Operations Unit Topics ● Safety During Search and Rescue Operations ● Conducting Interior and Exterior Searches ● Conducting Rescue Operations CERT Basic Training 5-6 Unit 5: Light Search and Rescue Operations CERT Sizeup 1. Gather Facts 2. Assess Damage 3. Consider Probabilities REMEMBER: 4. Assess Your Situation CERT SIZEUP IS A 5. Establish Priorities CONTINUAL PROCESS 6. Make Decisions 7. Develop Plan of Action 8. Take Action 9. Evaluate Progress CERT Basic Training 5-7 Unit 5: Light Search and Rescue Operations Sizeup: Step 1 Gather Facts ● Time of event and day of the week ● Construction type/terrain ● Occupancy ● Weather ● Hazards CERT Basic Training 5-8 Unit 5: Light Search and Rescue Operations Sizeup: Step 2 Assess and Communicate Damage The CERT mission changes if: .