Lecture 6 Introduction to Scattering

Size: px
Start display at page:

Download "Lecture 6 Introduction to Scattering"

Transcription

1 Lecture 6 Introduction to Scattering Collin Roesler 12 July 2017

2 Scattering Theory B = scatterance b= scattering coefficient (m -1 ) B = F b /F o F b F a b = B/Dx F o F t b (m -1 ) = (-1/x) ln(f t /F o ) Dx How is this measurement difference from beam c, a?

3 Geometry of scattering

4 Volume Scattering Function (VSF) b(q, f) = power per unit steradian emanating from a volume illuminated by irradiance b(q,f) = 1 df F o dr dw b = 4p b(q,f) dw What is dw? b = 2p o pb(q,f) sinq dq df

5 Calculate Scattering, b, from the volume scattering function b = 4p b(q,f) dw If there is azimuthal symmetry p b = 2p b(q,f) sinq dq 0 b f = 2p b f = 2p p/2 0 p p/2 b(q,f) sinq dq b(q,f) sinq dq Phase function: b(q,f) ~ = b(q,f)/b These are spectral!

6 Particle parameters that influence scattering Concentration Diameter : wavelength refractive index relative to surrounding medium absorption of radiation through particle Particle shape

7 Electromagnetic Radiation Oscillating magnetic and electric fields Perpendicular to direction of propagation May be polarized

8 Interactions between EM radiation and particles Consider the relationship between particle size and EMR wavelength

9 Interaction of light with small particles: d<<l Rayleigh scatterers Energy from propagating EM wave sets up oscillating dipole in particle

10 Small Particles: Rayleigh scatterers d<<l Propagating EM wave sets up oscillating dipole in particle Oscillating dipole induces EM radiation from particle (scattered radiation)

11 Small Particles: Rayleigh scatterers Angular distribution of radiation is called the volume scattering function (VSF or b(q)) Equal in forward and backward directions

12 Interaction of light with large particles d>> l EMR induces multiple dipole oscillations Some EMR penetrates particle

13 Large particle scattering Diffraction Refraction Reflection Dera, Marine Physics

14 Large Particle Scattering Three effects: refraction, reflection and diffraction

15 Fresnel s Law Quantifies reflection and transmission of EM radiation across an interface between two media with different refractive indices EMR Incident = EMR transmitted + EMR reflected Function of relative indices of refraction and incidence angle

16 Snell s Law: refractive index impact on wave propagation, describes angle of transmission

17 Refraction As EMR crosses an interface (say from water to a particle) it will change celerity If it slows down, the wavelength shortens up Thus it will bend (refract) Once it exits the particle, it will return to its original celerity and wavelength, but likely at a different angle and or phase than original

18 Refraction Change in angle Change in phase

19 Optical cross section Optical cross section for scattering? If every photon incident on the particle scatters geometric cross section Optical/geometric cross section =1 What about for absorbing particle?

20 Diffraction

21 Optical cross section Optical cross section for scattering if you include diffraction? Diffraction can occur 2 radii away Optical/geometric crossection = 2 What about for absorbing particle?

22 Effect of non-sphericity on diffraction (forward scattering pattern) Rectangles/ cylinders Circles/ spheres

23 Basis for design of LISST

24 What influences a particle s refractive index? Variations in particle composition: Stramski et al

25 What influences a particle s refractive index? Highly refractive particles Weakly refractive particles Variations in bulk composition: Twardowski et al

26 Effect of absorption Parameterized by n, the imaginary refractive index relative to surrounding medium Describes attenuation of EM radiation as it passes through particle Reduces scattered radiation

27 Draw absorption

28 Effect of Absorption in the extreme Only diffraction

29 What are the constituent properties that we need to consider Particle size Particle composition Index of refraction (real part) Index of refraction (imaginary part) Particle shape Internal structures

30 What are the particles in the ocean that are responsible for light scattering Water molecules Dissolved matter Inorganic salts Organic matter (CDOM, colloids) Particles Organic Cells and organisms (viruses, bacteria, phytoplankton, to ) Detrital aggregates Inorganic Sediments Minerals Air bubbles

31 Size matters Applicable scattering theory Particle Size Range

32 Particle size in the ocean Stramski and Kiefer 1991

33 Scattering in the ocean: Rayleigh Scattering water molecules

34 Small Particle Scattering follows Rayleigh Theory b( q) b(l) Example for water ~ l -4 VSF q Wavelength (nm)

35 Scattering in the ocean: water Clusters formed from hydrogen bonds between the polar water molecule (Frank-Wen flickering cluster model) A function of temperature (kinetic energy)

36 Scattering in the ocean: dissolved salts Increased b relative to pure water 30% Model of salt dissociation Zhang et al 2009 OptExp

37 Scattering in the ocean: marine viruses Balch et al. 1999

38 Scattering in the ocean: submicron particles (~colloids) Yamasaki et al 1998 Stramski and Wozniak 2005

39 Scattering by CDOM: From Emmanuel Boss Scattering by molecules whose D<<l. Rayleigh scattering: ( ) 4 l l 2 b b( q ) 1 cos ( q ) ( ) No evidence in the literature that scattering is significant (the only place I have ever found significant dissolved scattering (c g >a g ) was in pore water).

40 Scattering in the ocean: phytoplankton Stramski et al. 2001

41 Scattering in the ocean: inorganic minerals Terrestrial dust sources Stramski et al. 2007

42 Void fraction Contribution to bb # bubbles/m 3 /mm Scattering in the ocean: air bubbles Terrill et al Acoustics Size distribution Modeled b Radius (mm) Wind speed (m/s) Terrill et al Radius (mm) Void fraction

43 Scattering in the ocean: air bubbles

44 Mie Theory describes the interaction between EM and particles Homogeneous spheres Size index r ~ d / l Real refractive index relative to surrounding medium (n = m p /m w ) Slows wave propagation Imaginary refractive index relative to surrounding medium (n = m p /m w ) Attenuation of wave propagation

45 VSF of 5 mm particle as a function of refractive index

46 VSF of particles with refractive index 1.05

47 b(q) response to particle size distribution First let s talk about particle size distributions r -3 r -5 Stramski and Kiefer 1989

48 b(q) and response to particle size distribution b(q) / V p Roesler and Boss, 2008

49 b(q) response to index of refraction b(q) / V p Roesler and Boss, 2008

50 Scattering in the ocean: which particles contribute Boss et al., 2004, TOS

51 Consider what information scattering can provide and what do you want to measure b b f b b b(q)

52 Scattering closure Reductionist view (Stramski and Mobley 1997; Mobley and Stramski 1997) Particle-specific volume scattering Particle concentration Add them up

53 Importance of scattering in the ocean Competing forces of absorption and scattering on the downward propagation of light in the ocean

54 Importance of scattering in the ocean Competing forces of absorption and scattering on the downward propagation of light in the ocean Backscattering and the upward propagation of light from the ocean Normalized water-leaving radiance in the Mediterranean Sea (Sept 2003) 412 nm 490 nm

Retrieval of optical and microphysical properties of ocean constituents using polarimetric remote sensing

Retrieval of optical and microphysical properties of ocean constituents using polarimetric remote sensing Retrieval of optical and microphysical properties of ocean constituents using polarimetric remote sensing Presented by: Amir Ibrahim Optical Remote Sensing Laboratory, The City College of the City University

More information

1. Particle Scattering. Cogito ergo sum, i.e. Je pense, donc je suis. - René Descartes

1. Particle Scattering. Cogito ergo sum, i.e. Je pense, donc je suis. - René Descartes 1. Particle Scattering Cogito ergo sum, i.e. Je pense, donc je suis. - René Descartes Generally gas and particles do not scatter isotropically. The phase function, scattering efficiency, and single scattering

More information

Light. Electromagnetic wave with wave-like nature Refraction Interference Diffraction

Light. Electromagnetic wave with wave-like nature Refraction Interference Diffraction Light Electromagnetic wave with wave-like nature Refraction Interference Diffraction Light Electromagnetic wave with wave-like nature Refraction Interference Diffraction Photons with particle-like nature

More information

1.Rayleigh and Mie scattering. 2.Phase functions. 4.Single and multiple scattering

1.Rayleigh and Mie scattering. 2.Phase functions. 4.Single and multiple scattering 5 November 2014 Outline 1.Rayleigh and Mie scattering 2.Phase functions 3.Extinction 4.Single and multiple scattering Luca Lelli luca@iup.physik.uni-bremen.de Room U2080 Phone 0421.218.62097 Scattering

More information

Optical properties of oceanic particles

Optical properties of oceanic particles Optical properties of oceanic particles What physical properties p determine the optical properties p of particles? Size, composition (refractive index), shape, internal structure. These properties interact

More information

Light. Form of Electromagnetic Energy Only part of Electromagnetic Spectrum that we can really see

Light. Form of Electromagnetic Energy Only part of Electromagnetic Spectrum that we can really see Light Form of Electromagnetic Energy Only part of Electromagnetic Spectrum that we can really see Facts About Light The speed of light, c, is constant in a vacuum. Light can be: REFLECTED ABSORBED REFRACTED

More information

Class 11 Introduction to Surface BRDF and Atmospheric Scattering. Class 12/13 - Measurements of Surface BRDF and Atmospheric Scattering

Class 11 Introduction to Surface BRDF and Atmospheric Scattering. Class 12/13 - Measurements of Surface BRDF and Atmospheric Scattering University of Maryland Baltimore County - UMBC Phys650 - Special Topics in Experimental Atmospheric Physics (Spring 2009) J. V. Martins and M. H. Tabacniks http://userpages.umbc.edu/~martins/phys650/ Class

More information

The Importance of Refractive Index When using Laser Diffraction

The Importance of Refractive Index When using Laser Diffraction The Importance of Refractive Index When using Laser Diffraction Mark Bumiller mark.bumiller@horiba.com Fraunhofer Approximation Mie Theory RI 1.60 0.0i, in water, RI 1.33 Mie vs. Fraunhofer 1.E+05 1.E+04

More information

Towards a robust model of planetary thermal profiles

Towards a robust model of planetary thermal profiles Towards a robust model of planetary thermal profiles RT Equation: General Solution: RT Equation: General Solution: Extinction coefficient Emission coefficient How would you express the Source function

More information

MET 4410 Remote Sensing: Radar and Satellite Meteorology MET 5412 Remote Sensing in Meteorology. Lecture 9: Reflection and Refraction (Petty Ch4)

MET 4410 Remote Sensing: Radar and Satellite Meteorology MET 5412 Remote Sensing in Meteorology. Lecture 9: Reflection and Refraction (Petty Ch4) MET 4410 Remote Sensing: Radar and Satellite Meteorology MET 5412 Remote Sensing in Meteorology Lecture 9: Reflection and Refraction (Petty Ch4) When to use the laws of reflection and refraction? EM waves

More information

Monte-Carlo modeling used to simulate propagation of photons in a medium

Monte-Carlo modeling used to simulate propagation of photons in a medium Monte-Carlo modeling used to simulate propagation of photons in a medium Nils Haëntjens Ocean Optics Class 2017 based on lectures from Emmanuel Boss and Edouard Leymarie What is Monte Carlo Modeling? Monte

More information

Lecture 24 EM waves Geometrical optics

Lecture 24 EM waves Geometrical optics Physics 2102 Jonathan Dowling Lecture 24 EM waves Geometrical optics EM spherical waves The intensity of a wave is power per unit area. If one has a source that emits isotropically (equally in all directions)

More information

ISO INTERNATIONAL STANDARD. Particle size analysis Laser diffraction methods Part 1: General principles

ISO INTERNATIONAL STANDARD. Particle size analysis Laser diffraction methods Part 1: General principles INTERNATIONAL STANDARD ISO 13320-1 First edition 1999-11-01 Particle size analysis Laser diffraction methods Part 1: General principles Analyse granulométrique Méthodes par diffraction laser Partie 1:

More information

LECTURE 37: Ray model of light and Snell's law

LECTURE 37: Ray model of light and Snell's law Lectures Page 1 Select LEARNING OBJECTIVES: LECTURE 37: Ray model of light and Snell's law Understand when the ray model of light is applicable. Be able to apply Snell's Law of Refraction to any system.

More information

Chapter 24. Geometric optics. Assignment No. 11, due April 27th before class: Problems 24.4, 24.11, 24.13, 24.15, 24.24

Chapter 24. Geometric optics. Assignment No. 11, due April 27th before class: Problems 24.4, 24.11, 24.13, 24.15, 24.24 Chapter 24 Geometric optics Assignment No. 11, due April 27th before class: Problems 24.4, 24.11, 24.13, 24.15, 24.24 A Brief History of Light 1000 AD It was proposed that light consisted of tiny particles

More information

REMOTE SENSING OF VERTICAL IOP STRUCTURE

REMOTE SENSING OF VERTICAL IOP STRUCTURE REMOTE SENSING OF VERTICAL IOP STRUCTURE W. Scott Pegau College of Oceanic and Atmospheric Sciences Ocean. Admin. Bldg. 104 Oregon State University Corvallis, OR 97331-5503 Phone: (541) 737-5229 fax: (541)

More information

Physics 4C Chapter 33: Electromagnetic Waves

Physics 4C Chapter 33: Electromagnetic Waves Physics 4C Chapter 33: Electromagnetic Waves Our greatest glory is not in never failing, but in rising up every time we fail. Ralph Waldo Emerson If you continue to do what you've always done, you'll continue

More information

dq dt I = Irradiance or Light Intensity is Flux Φ per area A (W/m 2 ) Φ =

dq dt I = Irradiance or Light Intensity is Flux Φ per area A (W/m 2 ) Φ = Radiometry (From Intro to Optics, Pedrotti -4) Radiometry is measurement of Emag radiation (light) Consider a small spherical source Total energy radiating from the body over some time is Q total Radiant

More information

Introduction to Light

Introduction to Light Introduction to Light Light is basic to almost all life on Earth. Light is a form of electromagnetic radiation. Light represents energy transfer from the source to the observer. Images in mirrors Reflection

More information

Chapter 33 cont. The Nature of Light and Propagation of Light (lecture 2) Dr. Armen Kocharian

Chapter 33 cont. The Nature of Light and Propagation of Light (lecture 2) Dr. Armen Kocharian Chapter 33 cont The Nature of Light and Propagation of Light (lecture 2) Dr. Armen Kocharian Polarization of Light Waves The direction of polarization of each individual wave is defined to be the direction

More information

Ch. 22 Properties of Light HW# 1, 5, 7, 9, 11, 15, 19, 22, 29, 37, 38

Ch. 22 Properties of Light HW# 1, 5, 7, 9, 11, 15, 19, 22, 29, 37, 38 Ch. 22 Properties of Light HW# 1, 5, 7, 9, 11, 15, 19, 22, 29, 37, 38 Brief History of the Nature of Light Up until 19 th century, light was modeled as a stream of particles. Newton was a proponent of

More information

SESSION 5: INVESTIGATING LIGHT. Key Concepts. X-planation. Physical Sciences Grade In this session we:

SESSION 5: INVESTIGATING LIGHT. Key Concepts. X-planation. Physical Sciences Grade In this session we: SESSION 5: INVESTIGATING LIGHT Key Concepts In this session we: Explain what light is, where light comes from and why it is important Identify what happens when light strikes the surface of different objects

More information

2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing. Introduction to Remote Sensing

2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing. Introduction to Remote Sensing 2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing Introduction to Remote Sensing Curtis Mobley Delivered at the Darling Marine Center, University of Maine July 2017 Copyright 2017

More information

Light and Electromagnetic Waves. Honors Physics

Light and Electromagnetic Waves. Honors Physics Light and Electromagnetic Waves Honors Physics Electromagnetic Waves EM waves are a result of accelerated charges and disturbances in electric and magnetic fields (Radio wave example here) As electrons

More information

Phys 102 Lecture 17 Introduction to ray optics

Phys 102 Lecture 17 Introduction to ray optics Phys 102 Lecture 17 Introduction to ray optics 1 Physics 102 lectures on light Light as a wave Lecture 15 EM waves Lecture 16 Polarization Lecture 22 & 23 Interference & diffraction Light as a ray Lecture

More information

Physics 202, Lecture 23

Physics 202, Lecture 23 Physics 202, Lecture 23 Today s Topics Lights and Laws of Geometric Optics Nature of Light Reflection and Refraction Law of Reflection Law of Refraction Index of Reflection, Snell s Law Total Internal

More information

Dispersion Polarization

Dispersion Polarization Dispersion Polarization Phys Phys 2435: 22: Chap. 33, 31, Pg 1 Dispersion New Topic Phys 2435: Chap. 33, Pg 2 The Visible Spectrum Remember that white light contains all the colors of the s p e c t r u

More information

Chapter 22. Reflection and Refraction of Light

Chapter 22. Reflection and Refraction of Light Chapter 22 Reflection and Refraction of Light Nature of Light Light has a dual nature. Particle Wave Wave characteristics will be discussed in this chapter. Reflection Refraction These characteristics

More information

Chapter 35. The Nature of Light and the Laws of Geometric Optics

Chapter 35. The Nature of Light and the Laws of Geometric Optics Chapter 35 The Nature of Light and the Laws of Geometric Optics Introduction to Light Light is basic to almost all life on Earth. Light is a form of electromagnetic radiation. Light represents energy transfer

More information

Properties of Light. 1. The Speed of Light 2. The Propagation of Light 3. Reflection and Refraction 4. Polarization

Properties of Light. 1. The Speed of Light 2. The Propagation of Light 3. Reflection and Refraction 4. Polarization Chapter 33 - Light Properties of Light 1. The Speed of Light 2. The Propagation of Light 3. Reflection and Refraction 4. Polarization MFMcGraw-PHY 2426 Chap33-Light - Revised: 6-24-2012 2 Electromagnetic

More information

ISO INTERNATIONAL STANDARD. Particle size analysis Laser diffraction methods. Analyse granulométrique Méthodes par diffraction laser

ISO INTERNATIONAL STANDARD. Particle size analysis Laser diffraction methods. Analyse granulométrique Méthodes par diffraction laser INTERNATIONAL STANDARD ISO 13320 First edition 2009-10-01 Corrected version 2009-12-01 Particle size analysis Laser diffraction methods Analyse granulométrique Méthodes par diffraction laser Reference

More information

Physics 132: Lecture Fundamentals of Physics II Agenda for Today

Physics 132: Lecture Fundamentals of Physics II Agenda for Today Physics 132: Lecture Fundamentals of Physics II Agenda for Today Reflection of light Law of reflection Refraction of light Snell s law Dispersion PHY132 Lecture 17, Pg1 Electromagnetic waves A changing

More information

Lecture 7 Notes: 07 / 11. Reflection and refraction

Lecture 7 Notes: 07 / 11. Reflection and refraction Lecture 7 Notes: 07 / 11 Reflection and refraction When an electromagnetic wave, such as light, encounters the surface of a medium, some of it is reflected off the surface, while some crosses the boundary

More information

Quantifying the Dynamic Ocean Surface Using Underwater Radiometric Measurement

Quantifying the Dynamic Ocean Surface Using Underwater Radiometric Measurement DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Quantifying the Dynamic Ocean Surface Using Underwater Radiometric Measurement Lian Shen Department of Mechanical Engineering

More information

3/10/2019. Models of Light. Waves and wave fronts. Wave fronts and rays

3/10/2019. Models of Light. Waves and wave fronts. Wave fronts and rays Models of Light The wave model: Under many circumstances, light exhibits the same behavior as material waves. The study of light as a wave is called wave optics. The ray model: The properties of prisms,

More information

Physical or wave optics

Physical or wave optics Physical or wave optics In the last chapter, we have been studying geometric optics u light moves in straight lines u can summarize everything by indicating direction of light using a ray u light behaves

More information

Optics. a- Before the beginning of the nineteenth century, light was considered to be a stream of particles.

Optics. a- Before the beginning of the nineteenth century, light was considered to be a stream of particles. Optics 1- Light Nature: a- Before the beginning of the nineteenth century, light was considered to be a stream of particles. The particles were either emitted by the object being viewed or emanated from

More information

Physics 10. Lecture 28A. "If Dracula can t see his reflection in the mirror, how come his hair is always so neatly combed?

Physics 10. Lecture 28A. If Dracula can t see his reflection in the mirror, how come his hair is always so neatly combed? Physics 10 Lecture 28A "If Dracula can t see his reflection in the mirror, how come his hair is always so neatly combed?" --Steven Wright The Nature of Light From now on we will have to treat light as

More information

A Direct Simulation-Based Study of Radiance in a Dynamic Ocean

A Direct Simulation-Based Study of Radiance in a Dynamic Ocean A Direct Simulation-Based Study of Radiance in a Dynamic Ocean Dick K.P. Yue Center for Ocean Engineering Massachusetts Institute of Technology Room 5-321, 77 Massachusetts Ave, Cambridge, MA 02139 phone:

More information

RADIANCE IN THE OCEAN: EFFECTS OF WAVE SLOPE AND RAMAN SCATTERING NEAR THE SURFACE AND AT DEPTHS THROUGH THE ASYMPTOTIC REGION

RADIANCE IN THE OCEAN: EFFECTS OF WAVE SLOPE AND RAMAN SCATTERING NEAR THE SURFACE AND AT DEPTHS THROUGH THE ASYMPTOTIC REGION RADIANCE IN THE OCEAN: EFFECTS OF WAVE SLOPE AND RAMAN SCATTERING NEAR THE SURFACE AND AT DEPTHS THROUGH THE ASYMPTOTIC REGION A Thesis by JULIE MARIE SLANKER Submitted to the Office of Graduate Studies

More information

Ray Optics I. Last time, finished EM theory Looked at complex boundary problems TIR: Snell s law complex Metal mirrors: index complex

Ray Optics I. Last time, finished EM theory Looked at complex boundary problems TIR: Snell s law complex Metal mirrors: index complex Phys 531 Lecture 8 20 September 2005 Ray Optics I Last time, finished EM theory Looked at complex boundary problems TIR: Snell s law complex Metal mirrors: index complex Today shift gears, start applying

More information

HW Chapter 20 Q 2,3,4,5,6,10,13 P 1,2,3. Chapter 20. Classic and Modern Optics. Dr. Armen Kocharian

HW Chapter 20 Q 2,3,4,5,6,10,13 P 1,2,3. Chapter 20. Classic and Modern Optics. Dr. Armen Kocharian HW Chapter 20 Q 2,3,4,5,6,10,13 P 1,2,3 Chapter 20 Classic and Modern Optics Dr. Armen Kocharian Electromagnetic waves and matter: A Brief History of Light 1000 AD It was proposed that light consisted

More information

Chapter 24. Wave Optics. Wave Optics. The wave nature of light is needed to explain various phenomena

Chapter 24. Wave Optics. Wave Optics. The wave nature of light is needed to explain various phenomena Chapter 24 Wave Optics Wave Optics The wave nature of light is needed to explain various phenomena Interference Diffraction Polarization The particle nature of light was the basis for ray (geometric) optics

More information

INTRODUCTION REFLECTION AND REFRACTION AT BOUNDARIES. Introduction. Reflection and refraction at boundaries. Reflection at a single surface

INTRODUCTION REFLECTION AND REFRACTION AT BOUNDARIES. Introduction. Reflection and refraction at boundaries. Reflection at a single surface Chapter 8 GEOMETRICAL OPTICS Introduction Reflection and refraction at boundaries. Reflection at a single surface Refraction at a single boundary Dispersion Summary INTRODUCTION It has been shown that

More information

A Survey of Modelling and Rendering of the Earth s Atmosphere

A Survey of Modelling and Rendering of the Earth s Atmosphere Spring Conference on Computer Graphics 00 A Survey of Modelling and Rendering of the Earth s Atmosphere Jaroslav Sloup Department of Computer Science and Engineering Czech Technical University in Prague

More information

Lecture 1a Overview of Radiometry

Lecture 1a Overview of Radiometry Lecture 1a Overview of Radiometry Curtis Mobley Vice President for Science Senior Scientist Sequoia Scientific, Inc. Bellevue, Washington 98005 USA curtis.mobley@sequoiasci.com IOCCG Course Villefranche-sur-Mer,

More information

Light: Geometric Optics

Light: Geometric Optics Light: Geometric Optics The Ray Model of Light Light very often travels in straight lines. We represent light using rays, which are straight lines emanating from an object. This is an idealization, but

More information

Radiometry (From Intro to Optics, Pedrotti 1-4) Radiometry is measurement of Emag radiation (light) Consider a small spherical source Assume a black

Radiometry (From Intro to Optics, Pedrotti 1-4) Radiometry is measurement of Emag radiation (light) Consider a small spherical source Assume a black Radiometry (From Intro to Optics, Pedrotti -4) Radiometry is measurement of Emag radiation (light) Consider a small spherical source Assume a black body type emitter: uniform emission Total energy radiating

More information

specular diffuse reflection.

specular diffuse reflection. Lesson 8 Light and Optics The Nature of Light Properties of Light: Reflection Refraction Interference Diffraction Polarization Dispersion and Prisms Total Internal Reflection Huygens s Principle The Nature

More information

Chapter 24. Wave Optics. Wave Optics. The wave nature of light is needed to explain various phenomena

Chapter 24. Wave Optics. Wave Optics. The wave nature of light is needed to explain various phenomena Chapter 24 Wave Optics Wave Optics The wave nature of light is needed to explain various phenomena Interference Diffraction Polarization The particle nature of light was the basis for ray (geometric) optics

More information

2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing. Apparent Optical Properties and the BRDF

2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing. Apparent Optical Properties and the BRDF 2017 Summer Course on Optical Oceanography and Ocean Color Remote Sensing Curtis Mobley Apparent Optical Properties and the BRDF Delivered at the Darling Marine Center, University of Maine July 2017 Copyright

More information

Lecture 24: TUE 20 APR 2010 Ch : E&M Waves

Lecture 24: TUE 20 APR 2010 Ch : E&M Waves Physics 2102 Jonathan Dowling Lecture 24: TUE 20 APR 2010 Ch.33.6 10: E&M Waves Radiation Pressure Waves not only carry energy but also momentum. The effect is very small (we don t ordinarily feel pressure

More information

Light & Optical Systems Reflection & Refraction. Notes

Light & Optical Systems Reflection & Refraction. Notes Light & Optical Systems Reflection & Refraction Notes What is light? Light is electromagnetic radiation Ultra-violet + visible + infra-red Behavior of Light Light behaves in 2 ways particles (photons)

More information

Ray Optics. Lecture 23. Chapter 34. Physics II. Course website:

Ray Optics. Lecture 23. Chapter 34. Physics II. Course website: Lecture 23 Chapter 34 Physics II Ray Optics Course website: http://faculty.uml.edu/andriy_danylov/teaching/physicsii Today we are going to discuss: Chapter 34: Section 34.1-3 Ray Optics Ray Optics Wave

More information

2017 Summer Course Optical Oceanography and Ocean Color Remote Sensing. Overview of HydroLight and EcoLight

2017 Summer Course Optical Oceanography and Ocean Color Remote Sensing. Overview of HydroLight and EcoLight 2017 Summer Course Optical Oceanography and Ocean Color Remote Sensing Curtis Mobley Overview of HydroLight and EcoLight Darling Marine Center, University of Maine July 2017 Copyright 2017 by Curtis D.

More information

Phase function effects on oceanic light fields

Phase function effects on oceanic light fields Phase function effects on oceanic light fields Curtis D. Mobley, Lydia K. Sundman, and Emmanuel Boss Numerical simulations show that underwater radiances, irradiances, and reflectances are sensitive to

More information

Lecture PowerPoints. Chapter 24 Physics: Principles with Applications, 7 th edition Giancoli

Lecture PowerPoints. Chapter 24 Physics: Principles with Applications, 7 th edition Giancoli Lecture PowerPoints Chapter 24 Physics: Principles with Applications, 7 th edition Giancoli This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching

More information

Lesson 1 Scattering, Diffraction, and Radiation

Lesson 1 Scattering, Diffraction, and Radiation Lesson 1 Scattering, Diffraction, and Radiation Chen-Bin Huang Department of Electrical Engineering Institute of Photonics Technologies National Tsing Hua University, Taiwan Various slides under courtesy

More information

Properties of Light I

Properties of Light I Properties of Light I Light definition Light Spectrum Wavelength in nm (1nm = 10-7 cm) Visible/White Light Cosmic Gamma X-Rays Ultra Violet Infra Red Micro Waves Radio Waves 1 Theory of Light Two complimentary

More information

Chapter 33. The Nature of Light and Propagation of Light (lecture 1) Dr. Armen Kocharian

Chapter 33. The Nature of Light and Propagation of Light (lecture 1) Dr. Armen Kocharian Chapter 33 The Nature of Light and Propagation of Light (lecture 1) Dr. Armen Kocharian The Nature of Light Before the beginning of the nineteenth century, light was considered to be a stream of particles

More information

Mie scattering off plasmonic nanoparticle

Mie scattering off plasmonic nanoparticle Mie scattering off plasmonic nanoparticle Model documentation COMSOL 2009 Version: COMSOL 3.5a1 (build 3.5.0.608) Contents I. Model Overview II. Model Navigator III. Options and settings IV. Geometry modeling

More information

LIGHT. Speed of light Law of Reflection Refraction Snell s Law Mirrors Lenses

LIGHT. Speed of light Law of Reflection Refraction Snell s Law Mirrors Lenses LIGHT Speed of light Law of Reflection Refraction Snell s Law Mirrors Lenses Light = Electromagnetic Wave Requires No Medium to Travel Oscillating Electric and Magnetic Field Travel at the speed of light

More information

dq dt I = Irradiance or Light Intensity is Flux Φ per area A (W/m 2 ) Φ =

dq dt I = Irradiance or Light Intensity is Flux Φ per area A (W/m 2 ) Φ = Radiometry (From Intro to Optics, Pedrotti -4) Radiometry is measurement of Emag radiation (light) Consider a small spherical source Total energy radiating from the body over some time is Q total Radiant

More information

APPLICATION INFORMATION

APPLICATION INFORMATION A-1994A APPLICATION INFORMATION Particle Characterization USING LASER DIFFRACTION ANALYSIS IN PIGMENT SIZING Introduction Pigments and paints are an important class of industrial materials. They play an

More information

Outline Radiometry of Underwater Image Formation

Outline Radiometry of Underwater Image Formation Outline - Introduction - Features and Feature Matching - Geometry of Image Formation - Calibration - Structure from Motion - Dense Stereo - Radiometry of Underwater Image Formation - Conclusion 1 pool

More information

Electromagnetic waves

Electromagnetic waves Electromagnetic waves Now we re back to thinking of light as specifically being an electromagnetic wave u u u oscillating electric and magnetic fields perpendicular to each other propagating through space

More information

Michelson Interferometer

Michelson Interferometer Michelson Interferometer The Michelson interferometer uses the interference of two reflected waves The third, beamsplitting, mirror is partially reflecting ( half silvered, except it s a thin Aluminum

More information

Today. Participating media. Participating media. Rendering Algorithms: Participating Media and. Subsurface scattering

Today. Participating media. Participating media. Rendering Algorithms: Participating Media and. Subsurface scattering Today Rendering Algorithms: Participating Media and Subsurface Scattering Introduction Rendering participating media Rendering subsurface scattering Spring 2009 Matthias Zwicker Participating media Participating

More information

Kohei Arai 1 Graduate School of Science and Engineering Saga University Saga City, Japan

Kohei Arai 1 Graduate School of Science and Engineering Saga University Saga City, Japan Monte Carlo Ray Tracing Simulation of Polarization Characteristics of Sea Water Which Contains Spherical and Non-Spherical Particles of Suspended Solid and Phytoplankton Kohei Arai 1 Graduate School of

More information

9. Polarization. 1) General observations [Room 310]

9. Polarization. 1) General observations [Room 310] 9. Polarization In this lab we are going to study the various phenomena related to the polarization of light. We will also learn how to analyze, control and transfer the polarization state of light. This

More information

Lecture 17 (Polarization and Scattering) Physics Spring 2018 Douglas Fields

Lecture 17 (Polarization and Scattering) Physics Spring 2018 Douglas Fields Lecture 17 (Polarization and Scattering) Physics 262-01 Spring 2018 Douglas Fields Reading Quiz When unpolarized light passes through an ideal polarizer, the intensity of the transmitted light is: A) Unchanged

More information

f. (5.3.1) So, the higher frequency means the lower wavelength. Visible part of light spectrum covers the range of wavelengths from

f. (5.3.1) So, the higher frequency means the lower wavelength. Visible part of light spectrum covers the range of wavelengths from Lecture 5-3 Interference and Diffraction of EM Waves During our previous lectures we have been talking about electromagnetic (EM) waves. As we know, harmonic waves of any type represent periodic process

More information

WAVE OPTICS-I. A linear source produces cylindrical wavefront. (Draw diagram).

WAVE OPTICS-I. A linear source produces cylindrical wavefront. (Draw diagram). WAVE OPTICS-I Wavefront: It is the locus of points in space which are simultaneously disturbed and are vibrating in same phase. Wavefront can be spherical, plane or cylindrical. Note that the wavefront

More information

PHYSICS 213 PRACTICE EXAM 3*

PHYSICS 213 PRACTICE EXAM 3* PHYSICS 213 PRACTICE EXAM 3* *The actual exam will contain EIGHT multiple choice quiz-type questions covering concepts from lecture (16 points), ONE essay-type question covering an important fundamental

More information

Geometrical Optics INTRODUCTION. Wave Fronts and Rays

Geometrical Optics INTRODUCTION. Wave Fronts and Rays Geometrical Optics INTRODUCTION In this experiment, the optical characteristics of mirrors, lenses, and prisms will be studied based on using the following physics definitions and relationships plus simple

More information

Chapter 24. Wave Optics

Chapter 24. Wave Optics Chapter 24 Wave Optics Wave Optics The wave nature of light is needed to explain various phenomena Interference Diffraction Polarization The particle nature of light was the basis for ray (geometric) optics

More information

Hot Sync. Materials Needed Today

Hot Sync. Materials Needed Today Chapter 11 Lesson 2 Materials Needed Today Please take these materials out of your backpack. Pencil Blank sheet of paper for a lab! Hot Sync Thursday 3/27/14 After learning how light acts. Write a new

More information

Physics 1502: Lecture 28 Today s Agenda

Physics 1502: Lecture 28 Today s Agenda Physics 1502: Lecture 28 Today s Agenda Announcements: Midterm 2: Monday Nov. 16 Homework 08: due next Friday Optics Waves, Wavefronts, and Rays Reflection Index of Refraction 1 Waves, Wavefronts, and

More information

LIGHT SCATTERING THEORY

LIGHT SCATTERING THEORY LIGHT SCATTERING THEORY Laser Diffraction (Static Light Scattering) When a Light beam Strikes a Particle Some of the light is: Diffracted Reflected Refracted Absorbed and Reradiated Reflected Refracted

More information

Algebra Based Physics

Algebra Based Physics Slide 1 / 66 Slide 2 / 66 Algebra Based Physics Geometric Optics 2015-12-01 www.njctl.org Table of ontents Slide 3 / 66 lick on the topic to go to that section Reflection Spherical Mirror Refraction and

More information

Lecture 26, March 16, Chapter 35, Polarization

Lecture 26, March 16, Chapter 35, Polarization Physics 5B Lecture 26, March 16, 2012 Chapter 35, Polarization Simple Spectrometer d sin m Resolving power, to separate two lines closely spaced in wavelength by : R mn Resolving Power Two lines not resolved.

More information

Study of Air Bubble Induced Light Scattering Effect On Image Quality in 193 nm Immersion Lithography

Study of Air Bubble Induced Light Scattering Effect On Image Quality in 193 nm Immersion Lithography Study of Air Bubble Induced Light Scattering Effect On Image Quality in 193 nm Immersion Lithography Y. Fan, N. Lafferty, A. Bourov, L. Zavyalova, B. W. Smith Rochester Institute of Technology Microelectronic

More information

OPTICS MIRRORS AND LENSES

OPTICS MIRRORS AND LENSES Downloaded from OPTICS MIRRORS AND LENSES 1. An object AB is kept in front of a concave mirror as shown in the figure. (i)complete the ray diagram showing the image formation of the object. (ii) How will

More information

Chapter 33 The Nature and Propagation of Light by C.-R. Hu

Chapter 33 The Nature and Propagation of Light by C.-R. Hu Chapter 33 The Nature and Propagation of Light by C.-R. Hu Light is a transverse wave of the electromagnetic field. In 1873, James C. Maxwell predicted it from the Maxwell equations. The speed of all electromagnetic

More information

Chapter 24. Wave Optics

Chapter 24. Wave Optics Chapter 24 Wave Optics Diffraction Huygen s principle requires that the waves spread out after they pass through slits This spreading out of light from its initial line of travel is called diffraction

More information

Fresnel Reflection. angle of transmission. Snell s law relates these according to the

Fresnel Reflection. angle of transmission. Snell s law relates these according to the Fresnel Reflection 1. Reflectivity of polarized light The reflection of a polarized beam of light from a dielectric material such as air/glass was described by Augustin Jean Fresnel in 1823. While his

More information

ESA Training Course Oceanography from Space. Introduction into Hydro Optics

ESA Training Course Oceanography from Space. Introduction into Hydro Optics ESA Training Course Oceanography from Space Introduction into Hydro Optics Roland Doerffer GKSS Institute for Coastal Research September 26, 26 The penetration of light in the sea Source: http://www.malediven.net/haupts.htm

More information

PY106 Class31. Index of refraction. Refraction. Index of refraction. Sample values of n. Rays and wavefronts. index of refraction: n v.

PY106 Class31. Index of refraction. Refraction. Index of refraction. Sample values of n. Rays and wavefronts. index of refraction: n v. Refraction Index of refraction When an EM wave travels in a vacuum, its speed is: c = 3.00 x 10 8 m/s. In any other medium, light generally travels at a slower speed. The speed of light v in a material

More information

Textbook Assignment #1: DUE Friday 5/9/2014 Read: PP Do Review Questions Pg 388 # 1-20

Textbook Assignment #1: DUE Friday 5/9/2014 Read: PP Do Review Questions Pg 388 # 1-20 Page 1 of 38 Page 2 of 38 Unit Packet Contents Unit Objectives Notes 1: Waves Introduction Guided Practice: Waves Introduction (CD pp 89-90) Independent Practice: Speed of Waves Notes 2: Interference and

More information

At the interface between two materials, where light can be reflected or refracted. Within a material, where the light can be scattered or absorbed.

At the interface between two materials, where light can be reflected or refracted. Within a material, where the light can be scattered or absorbed. At the interface between two materials, where light can be reflected or refracted. Within a material, where the light can be scattered or absorbed. The eye sees by focusing a diverging bundle of rays from

More information

Optics and Images. Lenses and Mirrors. Matthew W. Milligan

Optics and Images. Lenses and Mirrors. Matthew W. Milligan Optics and Images Lenses and Mirrors Light: Interference and Optics I. Light as a Wave - wave basics review - electromagnetic radiation II. Diffraction and Interference - diffraction, Huygen s principle

More information

Philpot & Philipson: Remote Sensing Fundamentals Interactions 3.1 W.D. Philpot, Cornell University, Fall 12

Philpot & Philipson: Remote Sensing Fundamentals Interactions 3.1 W.D. Philpot, Cornell University, Fall 12 Philpot & Philipson: Remote Sensing Fundamentals Interactions 3.1 W.D. Philpot, Cornell University, Fall 1 3. EM INTERACTIONS WITH MATERIALS In order for an object to be sensed, the object must reflect,

More information

The sources must be coherent. This means they emit waves with a constant phase with respect to each other.

The sources must be coherent. This means they emit waves with a constant phase with respect to each other. CH. 24 Wave Optics The sources must be coherent. This means they emit waves with a constant phase with respect to each other. The waves need to have identical wavelengths. Can t be coherent without this.

More information

Phys 1020, Day 18: Questions? Cameras, Blmfld Reminders: Next Up: digital cameras finish Optics Note Final Project proposals next week!

Phys 1020, Day 18: Questions? Cameras, Blmfld Reminders: Next Up: digital cameras finish Optics Note Final Project proposals next week! Lights. Action. Phys 1020, Day 18: Questions? Cameras, Blmfld 15.1 Reminders: Next Up: digital cameras finish Optics Note Final Project proposals next week! 1 What have we learned in this section: 1) Lasers

More information

Physics 1C. Lecture 22A. "There are two ways of spreading light: to be the candle or the mirror that reflects it." --Edith Wharton

Physics 1C. Lecture 22A. There are two ways of spreading light: to be the candle or the mirror that reflects it. --Edith Wharton Physics 1C Lecture 22A "There are two ways of spreading light: to be the candle or the mirror that reflects it." --Edith Wharton The Nature of Light An interesting question developed as to the nature of

More information

Basic Optics : Microlithography Optics Part 4: Polarization

Basic Optics : Microlithography Optics Part 4: Polarization Electromagnetic Radiation Polarization: Linear, Circular, Elliptical Ordinary and extraordinary rays Polarization by reflection: Brewster angle Polarization by Dichroism Double refraction (Birefringence)

More information

Modeling Focused Beam Propagation in scattering media. Janaka Ranasinghesagara

Modeling Focused Beam Propagation in scattering media. Janaka Ranasinghesagara Modeling Focused Beam Propagation in scattering media Janaka Ranasinghesagara Teaching Objectives Understand the need of focused beam computational models. Understand the concepts, equations and principles

More information

The branch of physics which studies light

The branch of physics which studies light Mr.V The branch of physics which studies light Geometric model XVI century by W Snell Wave Model XIX century by JC Maxwell Photon Model XX century by Planck, Einstein Models of Light Basic Concept Laws

More information

Wavefronts and Rays. When light or other electromagnetic waves interact with systems much larger than the wavelength, it s a good approximation to

Wavefronts and Rays. When light or other electromagnetic waves interact with systems much larger than the wavelength, it s a good approximation to Chapter 33: Optics Wavefronts and Rays When light or other electromagnetic waves interact with systems much larger than the wavelength, it s a good approximation to Neglect the wave nature of light. Consider

More information

Course Updates. Reminders: 1) Assignment #12 due today. 2) Polarization, dispersion. 3) Last HW (#13 posted) due Monday, May 3rd

Course Updates. Reminders: 1) Assignment #12 due today. 2) Polarization, dispersion. 3) Last HW (#13 posted) due Monday, May 3rd Course Updates http://www.phys.hawaii.edu/~varner/phys272-spr10/physics272.html Reminders: 1) Assignment #12 due today 2) Polarization, dispersion 3) Last HW (#13 posted) due Monday, May 3rd n 1 n 2 Total

More information