Modelling the Directionality of Light Scattered in Translucent Materials
|
|
- Blake Martin
- 5 years ago
- Views:
Transcription
1 Modelling the Directionality of Light Scattered in Translucent Materials Jeppe Revall Frisvad Joint work with Toshiya Hachisuka, Aarhus University Thomas Kjeldsen, The Alexandra Institute March 2014
2 Materials (scattering and absorption of light) Optical properties (index of refraction, n(λ) = n (λ) + i n (λ)). Reflectance distribution functions, S(x i, ω i ; x o, ω o ). BSSRDF n 1 x i x o n 2 BRDF n 1 n 2
3 Subsurface scattering Behind the rendering equation [Nicodemus et al. 1977]: n 1 dl r (x o, ω o ) dφ i (x i, ω i ) = S(x i, ω i ; x o, ω o ). x i xo An element of reflected radiance dl r is proportional to an element of incident flux dφ i. S (the BSSRDF) is the factor of proportionality. d 2 Φ Using the definition of radiance L =, we have cos θ da dω L r (x o, ω o ) = S(x i, ω i ; x o, ω o )L i (x i, ω i ) cos θ dω i da. References A 2π - Nicodemus, F. E., Richmond, J. C., Hsia, J. J., Ginsberg, I. W., and Limperis, T. Geometrical considerations and nomenclature for reflectance. Tech. rep., National Bureau of Standards (US), n 2
4
5 BRDF [Jensen et al. 2001] BSSRDF
6 [Donner and Jensen 2006]
7 Splitting up the BSSRDF Bidirectional Scattering-Surface Reflectance Distribution Function: S = S(x i, ω i ; x o, ω o ). Away from sources and boundaries, we can use diffusion. Splitting up the BSSRDF where S = T 12 (S (0) + S (1) + S d )T 21. T 12 and T 21 are Fresnel transmittance terms (using ω i, ω o ). S (0) is the direct transmission part (using Dirac δ-functions). S (1) is the single scattering part (using all arguments). Sd is the diffusive part (multiple scattering, using x o x i ). We distribute the single scattering to the other terms using the delta-eddington approximation: S = T 12 (S δe + S d )T 21, and generalize the model such that S d = S d (x i, ω i ; x o ).
8 Diffusion theory Think of multiple scattering as a diffusion process. In diffusion theory, we use quantities that describe the light field in an element of volume of the scattering medium. Total flux, or fluence, is defined by y dz φ(x) = L(x, ω) dω. dy 4π dx x z We find an expression for φ by solving the diffusion equation (D 2 σ a )φ(x) = q(x) + 3D Q(x), where σ a and D are absorption and diffusion coefficients, while q and Q are zeroth and first order source terms. x
9 Deriving a BSSRDF Assume that emerging light is diffuse due to a large number of scattering events: S d (x i, ω i ; x o, ω o ) = S d (x i, ω i ; x o ). Integrating emerging diffuse radiance over outgoing directions, we find S d = C φ(η) φ C E (η) D n o φ, where Φ 4πC φ (1/η) Φ is the flux entering the medium at xi. no is the surface normal at the point of emergence x o. Cφ and C E depend on the relative index of refraction η and are polynomial fits of different hemispherical integrals of the Fresnel transmittance. This connects the BSSRDF and the diffusion theory. To get an analytical model, we use a special case solution for the diffusion equation (an expression for φ). Then, all we need to do is to find φ (do the math) and deal with boundary conditions (build a plausible model).
10 Point source diffusion or ray source diffusion standard dipole Point source diffusion [Bothe 1941; 1942] φ(r) = Φ e σ trr 4πD r, where r = x o x i and σ tr = σ a /D is the effective transport coefficient. our model Ray source diffusion [Menon et al. 2005a; 2005b] φ(r, θ) = Φ 4πD e σ trr r ( 1 + 3D 1+σ trr r cos θ ), where θ is the angle between the refracted ray and x o x i.
11 Our BSSRDF when disregarding the boundary d Using x = x o x i, r = x, cos θ = x ω 12 /r, we take the gradient of φ(r, θ) (the expression for ray source diffusion) and insert to find S d (x, ω 12, r) = 1 C E (η) ( 1 e σtrr 4C φ (1/η) 4π 2 r 3 [ 3D(1 + σ tr r) ω 12 n o C φ (η) ( r 2 D + 3(1 + σ trr) x ω 12 ) ((1 + σ tr r) + 3D 3(1+σtrr)+(σtrr)2 r 2 x ω 12 ) x n o )], which would be the BSSRDF if we neglect the boundary.
12 Dipole configuration (method of mirror images) d We place the real ray source at the boundary and reflect it in an extrapolated boundary to place the virtual ray source. Distance to the extrapolated boundary [Davison 1958]: d e = D/ 1 3Dσ a. In case of a refractive boundary (η 1 η 2 ), the distance is Ad e with A = 1 C E(η) 2C φ (η).
13 Modified tangent plane d The dipole assumes a semi-infinite medium. We assume that the boundary contains the vector x o x i and that it is perpendicular to the plane spanned by n i and x o x i. The normal of the assumed boundary plane is then n i = x o x i x o x i n i (x o x i ) n i (x o x i ), or n i = n i if x o = x i. and the virtual source is given by x v = x i +2Ad e n i, d v = x v x i, ω v = ω 12 2( ω 12 n i ) n i.
14 Distance to the real source (handling the singularity) z-axis zr real source n dr d n 2 n 1 r z = 0 incident light ω i -z v dv virtual source ω o observer standard dipole d r = r 2 + z 2 r. our model d r = r? Emergent radiance is an integral over z of a Hankel transform of a Green function which is Fourier transformed in x and y. Approximate analytic evaluation is possible if r is corrected to R 2 = r 2 + (z + d e ) 2. The resulting model for z = 0 corresponds to the standard dipole where z = z r and d e is replaced by the virtual source.
15 r2 + d 2 e Distance to the real source (handling the singularity) d e β n o x i θ r x o ω 12 n o θ 0 Since we neither have normal incidence nor x o in the tangent plane, we modify the distance correction: R 2 = r 2 + z 2 + d 2 e 2z d e cos β. It is possible to reformulate the integral over z to an integral along the refracted ray. We can approximate this integral by choosing an offset D along the refracted ray. Then z = D cos θ 0.
16 Our BSSRDF when considering boundary conditions Our final distance to the real source becomes { dr 2 r = 2 + Dµ 0 (Dµ 0 2d e cos β) for µ 0 > 0 (frontlit) r 2 + 1/(3σ t ) 2 otherwise (backlit), with µ 0 = cos θ 0 = n o ω 12 and r r cos β = sin θ = 2 (x ω 12 ) 2 r 2 + de 2 r 2 + de 2. The diffusive part of our BSSRDF is then S d (x i, ω i ; x o ) = S d (x o x i, ω 12, d r ) S d (x o x v, ω v, d v ), while the full BSSRDF is as before: S = T 12 (S δe + S d )T 21.
17 Previous Models Previous models are based on the point source solution of the diffusion equation and have the problems listed below. 1. Ignore incoming light direction: Standard dipole [Jensen et al. 2001]. Multipole [Donner and Jensen 2005]. Quantized diffusion [d Eon and Irving 2011]. 2. Require precomputation: Precomputed BSSRDF [Donner et al. 2009, Yan et al. 2012]. 3. Rely on numerical integration: Photon diffusion [Donner and Jensen 2007, Habel et al. 2013]. Using ray source diffusion, we can get rid of those problems.
18 Results (Grapefruit Bunnies) ours reference dipole quantized
19 Results (marble Bunnies) ours reference dipole quantized
20 Results (Simple Scene) Path traced single scattering was added to the existing models but not to ours. Faded bars show quality measurements when single scattering is not added. The four leftmost materials scatter light isotropically RMSE dipole btpole qntzd ours apple marble potato skin1 choc milk soy milk w. grape milk (r.) SSIM skin1 choc apple marble potato milk soy milk w. grape milk (r.)
21 Results (2D plots, 30 Oblique Incidence) quantized ours Our model is significantly different when the angle of incidence changes when the direction toward the point of emergence changes.
22 Results (2D plots, 45 Oblique Incidence) quantized ours Our model is significantly different when the angle of incidence changes when the direction toward the point of emergence changes.
23 Results (2D plots, 60 Oblique Incidence) quantized ours Our model is significantly different when the angle of incidence changes when the direction toward the point of emergence changes.
24 Results (Diffuse Reflectance Curves) dipole btpole qntzd ours ptrace dipole btpole qntzd ours ptrace R d (x) Our model comes closer than the existing analytical models to measured and simulated diffuse reflectance curves.
25 Results (Image Based Lighting) quantized ours
26 The 3Shape Buddha! (scanned with a TRIOS Scanner) matte milk-coloured mini milk
27 Conclusion First BSSRDF which... Considers the direction of the incident light. Requires no precomputation. Provides a fully analytical solution. Much more accurate than previous models. Incorporates single scattering in the analytical model. Future work: Consider the direction of the emergent light. Real-time approximations. Directional multipole and quadpole extensions. Directional photon diffusion. Anisotropic media (skewed dipole).
Classical and Improved Diffusion Theory for Subsurface Scattering
Classical and Improved Diffusion Theory for Subsurface Scattering Ralf Habel 1 Per H. Christensen 2 Wojciech Jarosz 1 1 Disney Research Zürich 2 Pixar Animation Studios Technical report, June 2013 Abstract
More informationFundametals 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 Realistic Rendering
More informationFundamental Stellar Parameters
Fundamental Stellar Parameters Radiative Transfer Specific Intensity, Radiative Flux and Stellar Luminosity Observed Flux, Emission and Absorption of Radiation Radiative Transfer Equation, Solution and
More informationOptical Imaging Chapter 5 Light Scattering
Optical Imaging Chapter 5 Light Scattering Gabriel Popescu University of Illinois at Urbana-Champaign Beckman Institute Quantitative Light Imaging Laboratory http://light.ece.uiuc.edu Principles of Optical
More informationp(θ,φ,θ,φ) = we have: Thus:
1. Scattering RT Calculations We come spinning out of nothingness, scattering stars like dust. - Jalal ad-din Rumi (Persian Poet, 1207-1273) We ve considered solutions to the radiative transfer equation
More informationIllumination, Radiometry, and a (Very Brief) Introduction to the Physics of Remote Sensing!
Illumination, Radiometry, and a (Very Brief) Introduction to the Physics of Remote Sensing! Course Philosophy" Rendering! Computer graphics! Estimation! Computer vision! Robot vision" Remote sensing! lhm
More informationMean Intensity. Same units as I ν : J/m 2 /s/hz/sr (ergs/cm 2 /s/hz/sr) Function of position (and time), but not direction
MCRT: L5 MCRT estimators for mean intensity, absorbed radiation, radiation pressure, etc Path length sampling: mean intensity, fluence rate, number of absorptions Random number generators J Mean Intensity
More informationOptics.
Optics www.optics.rochester.edu/classes/opt100/opt100page.html Course outline Light is a Ray (Geometrical Optics) 1. Nature of light 2. Production and measurement of light 3. Geometrical optics 4. Matrix
More informationGoal: The theory behind the electromagnetic radiation in remote sensing. 2.1 Maxwell Equations and Electromagnetic Waves
Chapter 2 Electromagnetic Radiation Goal: The theory behind the electromagnetic radiation in remote sensing. 2.1 Maxwell Equations and Electromagnetic Waves Electromagnetic waves do not need a medium to
More informationThe Radiative Transfer Equation
The Radiative Transfer Equation R. Wordsworth April 11, 215 1 Objectives Derive the general RTE equation Derive the atmospheric 1D horizontally homogenous RTE equation Look at heating/cooling rates in
More informationMultiple-source optical diffusion approximation for a multilayer scattering medium
Multiple-source optical diffusion approximation for a multilayer scattering medium Joseph. Hollmann 1 and ihong V. Wang 1,2, * 1 Optical Imaging aboratory, Department of Biomedical Engineering, Texas A&M
More informationLecture Notes Prepared by Mike Foster Spring 2007
Lecture Notes Prepared by Mike Foster Spring 2007 Solar Radiation Sources: K. N. Liou (2002) An Introduction to Atmospheric Radiation, Chapter 1, 2 S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology:
More informationWave Propagation in Uniaxial Media. Reflection and Transmission at Interfaces
Lecture 5: Crystal Optics Outline 1 Homogeneous, Anisotropic Media 2 Crystals 3 Plane Waves in Anisotropic Media 4 Wave Propagation in Uniaxial Media 5 Reflection and Transmission at Interfaces Christoph
More informationIntroduction to Computer Vision Radiometry
Radiometry Image: two-dimensional array of 'brightness' values. Geometry: where in an image a point will project. Radiometry: what the brightness of the point will be. Brightness: informal notion used
More informationSTOCHASTIC & DETERMINISTIC SOLVERS
STOCHASTIC & DETERMINISTIC SOLVERS Outline Spatial Scales of Optical Technologies & Mathematical Models Prototype RTE Problems 1-D Transport in Slab Geometry: Exact Solution Stochastic Models: Monte Carlo
More informationLecture notes 5: Diffraction
Lecture notes 5: Diffraction Let us now consider how light reacts to being confined to a given aperture. The resolution of an aperture is restricted due to the wave nature of light: as light passes through
More informationMATH 228: Calculus III (FALL 2016) Sample Problems for FINAL EXAM SOLUTIONS
MATH 228: Calculus III (FALL 216) Sample Problems for FINAL EXAM SOLUTIONS MATH 228 Page 2 Problem 1. (2pts) Evaluate the line integral C xy dx + (x + y) dy along the parabola y x2 from ( 1, 1) to (2,
More information1. (a) (5 points) Find the unit tangent and unit normal vectors T and N to the curve. r (t) = 3 cos t, 0, 3 sin t, r ( 3π
1. a) 5 points) Find the unit tangent and unit normal vectors T and N to the curve at the point P 3, 3π, r t) 3 cos t, 4t, 3 sin t 3 ). b) 5 points) Find curvature of the curve at the point P. olution:
More informationWaves & Oscillations
Physics 42200 Waves & Oscillations Lecture 25 Propagation of Light Spring 2013 Semester Matthew Jones Midterm Exam: Date: Wednesday, March 6 th Time: 8:00 10:00 pm Room: PHYS 203 Material: French, chapters
More informationMonte Carlo Methods:
Short Course on Computational Monte Carlo Methods: Fundamentals Shuang Zhao Assistant Professor Computer Science Department University of California, Irvine Shuang Zhao 1 Teaching Objective Introducing
More informationProtocol for drain current measurements
Protocol for drain current measurements 1 Basics: the naive model of drain current A beam of intensity I (number of photons per unit area) and cross section impinges with a grazing angle Φ on a sample.
More informationElectromagnetic fields and waves
Electromagnetic fields and waves Maxwell s rainbow Outline Maxwell s equations Plane waves Pulses and group velocity Polarization of light Transmission and reflection at an interface Macroscopic Maxwell
More informationLecture 3: Asymptotic Methods for the Reduced Wave Equation
Lecture 3: Asymptotic Methods for the Reduced Wave Equation Joseph B. Keller 1 The Reduced Wave Equation Let v (t,) satisfy the wave equation v 1 2 v c 2 = 0, (1) (X) t2 where c(x) is the propagation speed
More informationHigh-Resolution. Transmission. Electron Microscopy
Part 4 High-Resolution Transmission Electron Microscopy 186 Significance high-resolution transmission electron microscopy (HRTEM): resolve object details smaller than 1nm (10 9 m) image the interior of
More information2 Feynman rules, decay widths and cross sections
2 Feynman rules, decay widths and cross sections 2.1 Feynman rules Normalization In non-relativistic quantum mechanics, wave functions of free particles are normalized so that there is one particle in
More information6. X-ray Crystallography and Fourier Series
6. X-ray Crystallography and Fourier Series Most of the information that we have on protein structure comes from x-ray crystallography. The basic steps in finding a protein structure using this method
More information6. LIGHT SCATTERING 6.1 The first Born approximation
6. LIGHT SCATTERING 6.1 The first Born approximation In many situations, light interacts with inhomogeneous systems, in which case the generic light-matter interaction process is referred to as scattering
More information(a) Show that the amplitudes of the reflected and transmitted waves, corrrect to first order
Problem 1. A conducting slab A plane polarized electromagnetic wave E = E I e ikz ωt is incident normally on a flat uniform sheet of an excellent conductor (σ ω) having thickness D. Assume that in space
More informationTRANSFER OF RADIATION
TRANSFER OF RADIATION Under LTE Local Thermodynamic Equilibrium) condition radiation has a Planck black body) distribution. Radiation energy density is given as U r,ν = 8πh c 3 ν 3, LTE), tr.1) e hν/kt
More informationA radiative transfer framework for rendering materials with anisotropic structure
A radiative transfer framework for rendering materials with anisotropic structure Expanded Technical Report Wenzel Jakob Adam Arbree Jonathan T. Moon Kavita Bala Steve Marschner Cornell University The
More informationMath 234. What you should know on day one. August 28, You should be able to use general principles like. x = cos t, y = sin t, 0 t π.
Math 234 What you should know on day one August 28, 2001 1 You should be able to use general principles like Length = ds, Area = da, Volume = dv For example the length of the semi circle x = cos t, y =
More informationNeutron Diffusion Theory: One Velocity Model
22.05 Reactor Physics - Part Ten 1. Background: Neutron Diffusion Theory: One Velocity Model We now have sufficient tools to begin a study of the second method for the determination of neutron flux as
More informationUniversity of Illinois at Chicago Department of Physics. Electricity & Magnetism Qualifying Examination
University of Illinois at Chicago Department of Physics Electricity & Magnetism Qualifying Examination January 7, 28 9. am 12: pm Full credit can be achieved from completely correct answers to 4 questions.
More informationMATH 280 Multivariate Calculus Fall Integrating a vector field over a surface
MATH 280 Multivariate Calculus Fall 2011 Definition Integrating a vector field over a surface We are given a vector field F in space and an oriented surface in the domain of F as shown in the figure below
More informationIn Situ Imaging of Cold Atomic Gases
In Situ Imaging of Cold Atomic Gases J. D. Crossno Abstract: In general, the complex atomic susceptibility, that dictates both the amplitude and phase modulation imparted by an atom on a probing monochromatic
More informationLecture 8 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell
Lecture 8 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell 1. Scattering Introduction - Consider a localized object that contains charges
More informationAT622 Section 2 Elementary Concepts of Radiometry
AT6 Section Elementary Concepts of Radiometry The object of this section is to introduce the student to two radiometric concepts intensity (radiance) and flux (irradiance). These concepts are largely geometrical
More informationJackson 7.6 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell
Jackson 7.6 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell PROBLEM: A plane wave of frequency ω is incident normally from vacuum on a semi-infinite slab of material
More informationLecture 2 Solutions to the Transport Equation
Lecture 2 Solutions to the Transport Equation Equation along a ray I In general we can solve the static transfer equation along a ray in some particular direction. Since photons move in straight lines
More informationFundamentals of Rendering - Radiometry / Photometry
Fundamentals of Rendering - Radiometry / Photometry Image Synthesis Torsten Möller Today The physics of light Radiometric quantities Photometry vs/ Radiometry 2 Reading Chapter 5 of Physically Based Rendering
More informationFundamentals of Rendering - Radiometry / Photometry
Fundamentals of Rendering - Radiometry / Photometry CMPT 461/761 Image Synthesis Torsten Möller Today The physics of light Radiometric quantities Photometry vs/ Radiometry 2 Reading Chapter 5 of Physically
More informationAstro 305 Lecture Notes Wayne Hu
Astro 305 Lecture Notes Wayne Hu Set 1: Radiative Transfer Radiation Observables From an empiricist s point of view there are 4 observables for radiation Energy Flux Direction Color Polarization Energy
More informationPhysics Dec The Maxwell Velocity Distribution
Physics 301 7-Dec-2005 29-1 The Maxwell Velocity Distribution The beginning of chapter 14 covers some things we ve already discussed. Way back in lecture 6, we calculated the pressure for an ideal gas
More informationHigh-Order Similarity Relations in Radiative Transfer: Supplementary Document
High-Order Similarity Relations in Radiative Transfer: Supplementary Document Shuang hao Ravi Ramamoorthi Kavita Bala Cornell University University of California, Berkeley Cornell University Overview This
More informationWaves & Oscillations
Physics 42200 Waves & Oscillations Lecture 32 Electromagnetic Waves Spring 2016 Semester Matthew Jones Electromagnetism Geometric optics overlooks the wave nature of light. Light inconsistent with longitudinal
More informationThe mathematics of scattering and absorption and emission
The mathematics of scattering and absorption and emission The transmittance of an layer depends on its optical depth, which in turn depends on how much of the substance the radiation has to pass through,
More informationMonte Carlo method projective estimators for angular and temporal characteristics evaluation of polarized radiation
Monte Carlo method projective estimators for angular and temporal characteristics evaluation of polarized radiation Natalya Tracheva Sergey Ukhinov Institute of Computational Mathematics and Mathematical
More informationMagnetic Neutron Reflectometry. Moses Marsh Shpyrko Group 9/14/11
Magnetic Neutron Reflectometry Moses Marsh Shpyrko Group 9/14/11 Outline Scattering processes Reflectivity of a slab of material Magnetic scattering Off-specular scattering Source parameters Comparison
More informationThe linear equations can be classificed into the following cases, from easier to more difficult: 1. Linear: u y. u x
Week 02 : Method of C haracteristics From now on we will stu one by one classical techniques of obtaining solution formulas for PDEs. The first one is the method of characteristics, which is particularly
More informationA Dielectric Invisibility Carpet
A Dielectric Invisibility Carpet Jensen Li Prof. Xiang Zhang s Research Group Nanoscale Science and Engineering Center (NSEC) University of California at Berkeley, USA CLK08-09/22/2008 Presented at Center
More informationSummary of Beam Optics
Summary of Beam Optics Gaussian beams, waves with limited spatial extension perpendicular to propagation direction, Gaussian beam is solution of paraxial Helmholtz equation, Gaussian beam has parabolic
More informationBasic Optical Concepts. Oliver Dross, LPI Europe
Basic Optical Concepts Oliver Dross, LPI Europe 1 Refraction- Snell's Law Snell s Law: Sin( φi ) Sin( φ ) f = n n f i n i Media Boundary φ i n f φ φ f angle of exitance 90 80 70 60 50 40 30 20 10 0 internal
More informationHeriot-Watt University
Heriot-Watt University Distinctly Global www.hw.ac.uk Thermodynamics By Peter Cumber Prerequisites Interest in thermodynamics Some ability in calculus (multiple integrals) Good understanding of conduction
More information1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light
1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light 1. Double-Slit Eperiment reading: Chapter 22 2. Single-Slit Diffraction reading: Chapter 22 3. Diffraction Grating reading: Chapter
More informationZero variance-based sampling schemes (a.k.a. path guiding) Jaroslav Křivánek Charles University, Prague Render Legion/Chaos Group
Zero variance-based sampling schemes (a.k.a. path guiding) Jaroslav Křivánek Charles University, Prague Render Legion/Chaos Group Path guiding The idea Zero-variance path sampling in volumes A theoretical
More information2 The Radiative Transfer Equation
9 The Radiative Transfer Equation. Radiative transfer without absorption and scattering Free space or homogeneous space I (r,,) I (r,,) r -r d da da Figure.: Following a pencil of radiation in free space
More informationLecture 3: Specific Intensity, Flux and Optical Depth
Lecture 3: Specific Intensity, Flux and Optical Depth We begin a more detailed look at stellar atmospheres by defining the fundamental variable, which is called the Specific Intensity. It may be specified
More informationClassical electric dipole radiation
B Classical electric dipole radiation In Chapter a classical model was used to describe the scattering of X-rays by electrons. The equation relating the strength of the radiated to incident X-ray electric
More informationTo remain at 0 K heat absorbed by the medium must be removed in the amount of. dq dx = q(l) q(0) dx. Q = [1 2E 3 (τ L )] σ(t T 4 2 ).
294 RADIATIVE HEAT TRANSFER 13.7 Two infinite, isothermal plates at temperatures T 1 and T 2 are separated by a cold, gray medium of optical thickness τ L = L (no scattering). (a) Calculate the radiative
More informationAVAZ inversion for fracture orientation and intensity: a physical modeling study
AVAZ inversion for fracture orientation and intensity: a physical modeling study Faranak Mahmoudian*, Gary F. Margrave, and Joe Wong, University of Calgary. CREWES fmahmoud@ucalgary.ca Summary We present
More informationQuantum Field Theory Spring 2019 Problem sheet 3 (Part I)
Quantum Field Theory Spring 2019 Problem sheet 3 (Part I) Part I is based on material that has come up in class, you can do it at home. Go straight to Part II. 1. This question will be part of a take-home
More informationRadiative transfer equations with varying refractive index: a mathematical perspective
Radiative transfer equations with varying refractive index: a mathematical perspective Guillaume Bal November 23, 2005 Abstract This paper reviews established mathematical techniques to model the energy
More informationIntroduction to Condensed Matter Physics
Introduction to Condensed Matter Physics Diffraction I Basic Physics M.P. Vaughan Diffraction Electromagnetic waves Geometric wavefront The Principle of Linear Superposition Diffraction regimes Single
More informationPHYS 102 Exams. PHYS 102 Exam 3 PRINT (A)
PHYS 102 Exams PHYS 102 Exam 3 PRINT (A) The next two questions pertain to the situation described below. A metal ring, in the page, is in a region of uniform magnetic field pointing out of the page as
More informationOPTICAL Optical properties of multilayer systems by computer modeling
Workshop on "Physics for Renewable Energy" October 17-29, 2005 301/1679-15 "Optical Properties of Multilayer Systems by Computer Modeling" E. Centurioni CNR/IMM AREA Science Park - Bologna Italy OPTICAL
More informationChapter 9 Electro-optic Properties of LCD
Chapter 9 Electro-optic Properties of LCD 9.1 Transmission voltage curves TVC stands for the transmittance-voltage-curve. It is also called the electro-optic curve. As the voltage is applied, θ(z) and
More informationOffset Spheroidal Mirrors for Gaussian Beam Optics in ZEMAX
Offset Spheroidal Mirrors for Gaussian Beam Optics in ZEMAX Antony A. Stark and Urs Graf Smithsonian Astrophysical Observatory, University of Cologne aas@cfa.harvard.edu 1 October 2013 This memorandum
More informationNotes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015)
Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015) Interaction of x-ray with matter: - Photoelectric absorption - Elastic (coherent) scattering (Thomson Scattering) - Inelastic (incoherent) scattering
More informationlim = F F = F x x + F y y + F z
Physics 361 Summary of Results from Lecture Physics 361 Derivatives of Scalar and Vector Fields The gradient of a scalar field f( r) is given by g = f. coordinates f g = ê x x + ê f y y + ê f z z Expressed
More informationAnalysis of Scattering of Radiation in a Plane-Parallel Atmosphere. Stephanie M. Carney ES 299r May 23, 2007
Analysis of Scattering of Radiation in a Plane-Parallel Atmosphere Stephanie M. Carney ES 299r May 23, 27 TABLE OF CONTENTS. INTRODUCTION... 2. DEFINITION OF PHYSICAL QUANTITIES... 3. DERIVATION OF EQUATION
More information1. Consider the biconvex thick lens shown in the figure below, made from transparent material with index n and thickness L.
Optical Science and Engineering 2013 Advanced Optics Exam Answer all questions. Begin each question on a new blank page. Put your banner ID at the top of each page. Please staple all pages for each individual
More informationECE 484 Semiconductor Lasers
ECE 484 Semiconductor Lasers Dr. Lukas Chrostowski Department of Electrical and Computer Engineering University of British Columbia January, 2013 Module Learning Objectives: Understand the importance of
More informationMultipole moments. November 9, 2015
Multipole moments November 9, 5 The far field expansion Suppose we have a localized charge distribution, confined to a region near the origin with r < R. Then for values of r > R, the electric field must
More informationPC4262 Remote Sensing Scattering and Absorption
PC46 Remote Sensing Scattering and Absorption Dr. S. C. Liew, Jan 003 crslsc@nus.edu.sg Scattering by a single particle I(θ, φ) dφ dω F γ A parallel beam of light with a flux density F along the incident
More informationBasic Properties of Radiation, Atmospheres, and Oceans
Basic Properties of Radiation, Atmospheres, and Oceans Jean-Sébastian Tempel Department of Physics and Technology University of Bergen 16. Mai 2007 phys264 - Environmental Optics and Transport of Light
More informationInteraction X-rays - Matter
Interaction X-rays - Matter Pair production hν > M ev Photoelectric absorption hν MATTER hν Transmission X-rays hν' < hν Scattering hν Decay processes hν f Compton Thomson Fluorescence Auger electrons
More informationRadiative heat transfer
Radiative heat transfer 22 mars 2017 Energy can be transported by the electromagnetic field radiated by an object at finite temperature. A very important example is the infrared radiation emitted towards
More informationSolution Set 1 Phys 4510 Optics Fall 2013
Solution Set Phys 450 Optics Fall 203 Due date: Tu, September 7, in class Reading: Fowles 2.2-2.4, 2.6-2.7. Derive the formulas: and (see Fowles problem.6) v g = v φ λ dv φ dλ = λ 0 dn (2) v g v φ c dλ
More informationPHYS 508 (2015-1) Final Exam January 27, Wednesday.
PHYS 508 (2015-1) Final Exam January 27, Wednesday. Q1. Scattering with identical particles The quantum statistics have some interesting consequences for the scattering of identical particles. This is
More informationMultiple Integrals and Vector Calculus (Oxford Physics) Synopsis and Problem Sets; Hilary 2015
Multiple Integrals and Vector Calculus (Oxford Physics) Ramin Golestanian Synopsis and Problem Sets; Hilary 215 The outline of the material, which will be covered in 14 lectures, is as follows: 1. Introduction
More informationLaser Cross Section (LCS) (Chapter 9)
Laser Cross Section (LCS) (Chapter 9) EC4630 Radar and Laser Cross Section Fall 010 Prof. D. Jenn jenn@nps.navy.mil www.nps.navy.mil/jenn November 011 1 Laser Cross Section (LCS) Laser radar (LADAR), also
More informationLecture 4. Diffusing photons and superradiance in cold gases
Lecture 4 Diffusing photons and superradiance in cold gases Model of disorder-elastic mean free path and group velocity. Dicke states- Super- and sub-radiance. Scattering properties of Dicke states. Multiple
More informationSimplified Collector Performance Model
Simplified Collector Performance Model Prediction of the thermal output of various solar collectors: The quantity of thermal energy produced by any solar collector can be described by the energy balance
More informationPractice Final Solutions
Practice Final Solutions Math 1, Fall 17 Problem 1. Find a parameterization for the given curve, including bounds on the parameter t. Part a) The ellipse in R whose major axis has endpoints, ) and 6, )
More informationRadiation processes and mechanisms in astrophysics I. R Subrahmanyan Notes on ATA lectures at UWA, Perth 18 May 2009
Radiation processes and mechanisms in astrophysics I R Subrahmanyan Notes on ATA lectures at UWA, Perth 18 May 009 Light of the night sky We learn of the universe around us from EM radiation, neutrinos,
More informationLecture Pure Twist
Lecture 4-2003 Pure Twist pure twist around center of rotation D => neither axial (σ) nor bending forces (Mx, My) act on section; as previously, D is fixed, but (for now) arbitrary point. as before: a)
More informationPlasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi
Plasma Physics Prof. V. K. Tripathi Department of Physics Indian Institute of Technology, Delhi Lecture No. # 09 Electromagnetic Wave Propagation Inhomogeneous Plasma (Refer Slide Time: 00:33) Today, I
More informationSupplementary Information for Negative refraction in semiconductor metamaterials
Supplementary Information for Negative refraction in semiconductor metamaterials A.J. Hoffman *, L. Alekseyev, S.S. Howard, K.J. Franz, D. Wasserman, V.A. Poldolskiy, E.E. Narimanov, D.L. Sivco, and C.
More informationTHREE-DIMENSIONAL INTEGRAL NEUTRON TRANSPORT CELL CALCULATIONS FOR THE DETERMINATION OF MEAN CELL CROSS SECTIONS
THREE-DIMENSIONAL INTEGRAL NEUTRON TRANSPORT CELL CALCULATIONS FOR THE DETERMINATION OF MEAN CELL CROSS SECTIONS Carsten Beckert 1. Introduction To calculate the neutron transport in a reactor, it is often
More informationMathieu Hébert, Thierry Lépine
1 Introduction to Radiometry Mathieu Hébert, Thierry Lépine Program 2 Radiometry and Color science IOGS CIMET MINASP 3DMT Introduction to radiometry Advanced radiometry (2 nd semester) x x x x x o o Color
More informationRecent Advances on the Effective Optical Properties of Turbid Colloids. Rubén G. Barrera Instituto de Física, UNAM Mexico
Recent Advances on the Effective Optical Properties of Turbid Colloids Rubén G. Barrera Instituto de Física, UNAM Mexico In In collaboration with: Augusto García Edahí Gutierrez Celia Sánchez Pérez Felipe
More informationChapter 9. Electromagnetic waves
Chapter 9. lectromagnetic waves 9.1.1 The (classical or Mechanical) waves equation Given the initial shape of the string, what is the subsequent form, The displacement at point z, at the later time t,
More informationLecture 2: Thin Films. Thin Films. Calculating Thin Film Stack Properties. Jones Matrices for Thin Film Stacks. Mueller Matrices for Thin Film Stacks
Lecture 2: Thin Films Outline Thin Films 2 Calculating Thin Film Stack Properties 3 Jones Matrices for Thin Film Stacks 4 Mueller Matrices for Thin Film Stacks 5 Mueller Matrix for Dielectrica 6 Mueller
More informationCHAPTER 9 ELECTROMAGNETIC WAVES
CHAPTER 9 ELECTROMAGNETIC WAVES Outlines 1. Waves in one dimension 2. Electromagnetic Waves in Vacuum 3. Electromagnetic waves in Matter 4. Absorption and Dispersion 5. Guided Waves 2 Skip 9.1.1 and 9.1.2
More informationChapter 10. Interference of Light
Chapter 10. Interference of Light Last Lecture Wave equations Maxwell equations and EM waves Superposition of waves This Lecture Two-Beam Interference Young s Double Slit Experiment Virtual Sources Newton
More informationRadiation in the atmosphere
Radiation in the atmosphere Flux and intensity Blackbody radiation in a nutshell Solar constant Interaction of radiation with matter Absorption of solar radiation Scattering Radiative transfer Irradiance
More informationJim Lambers MAT 280 Summer Semester Practice Final Exam Solution. dy + xz dz = x(t)y(t) dt. t 3 (4t 3 ) + e t2 (2t) + t 7 (3t 2 ) dt
Jim Lambers MAT 28 ummer emester 212-1 Practice Final Exam olution 1. Evaluate the line integral xy dx + e y dy + xz dz, where is given by r(t) t 4, t 2, t, t 1. olution From r (t) 4t, 2t, t 2, we obtain
More informationClassical Field Theory: Electrostatics-Magnetostatics
Classical Field Theory: Electrostatics-Magnetostatics April 27, 2010 1 1 J.D.Jackson, Classical Electrodynamics, 2nd Edition, Section 1-5 Electrostatics The behavior of an electrostatic field can be described
More informationROINN NA FISICE Department of Physics
ROINN NA FISICE Department of 1.1 Astrophysics Telescopes Profs Gabuzda & Callanan 1.2 Astrophysics Faraday Rotation Prof. Gabuzda 1.3 Laser Spectroscopy Cavity Enhanced Absorption Spectroscopy Prof. Ruth
More informationSection 22. Radiative Transfer
OPTI-01/0 Geometrical and Instrumental Optics Copyright 018 John E. Greivenkamp -1 Section Radiative Transfer Radiometry Radiometry characterizes the propagation of radiant energy through an optical system.
More information