Light Reflectors and Optical Resonators

Similar documents
OPTICAL COMMUNICATIONS

34. Even more Interference Effects

Wavepackets. Outline. - Review: Reflection & Refraction - Superposition of Plane Waves - Wavepackets - ΔΔk Δx Relations

1. Consider the biconvex thick lens shown in the figure below, made from transparent material with index n and thickness L.

Problem 8.0 Make Your Own Exam Problem for Midterm II by April 13

Electromagnetic Waves in Materials

Calculating Thin Film Stack Properties. Polarization Properties of Thin Films

OPSE FINAL EXAM Fall 2016 YOU MUST SHOW YOUR WORK. ANSWERS THAT ARE NOT JUSTIFIED WILL BE GIVEN ZERO CREDIT.

Massachusetts Institute of Technology Physics 8.03 Practice Final Exam 3

Chapter 35 Physical Optics: Light as a wave

Optics.

Calculating Thin Film Stack Properties

Physics 214 Course Overview

Sub-wavelength electromagnetic structures

ECE 484 Semiconductor Lasers

LECTURE 23: LIGHT. Propagation of Light Huygen s Principle

Fresnel Equations cont.

EECS 117. Lecture 22: Poynting s Theorem and Normal Incidence. Prof. Niknejad. University of California, Berkeley

LECTURE 23: LIGHT. Propagation of Light Huygen s Principle

Some Topics in Optics

Chapter 2 Basic Optics

Summary of Beam Optics

2.71. Final examination. 3 hours (9am 12 noon) Total pages: 7 (seven) PLEASE DO NOT TURN OVER UNTIL EXAM STARTS PLEASE RETURN THIS BOOKLET

Edward S. Rogers Sr. Department of Electrical and Computer Engineering. ECE318S Fundamentals of Optics. Final Exam. April 16, 2007.

4. The interaction of light with matter

Massachusetts Institute of Technology Physics 8.03SC Fall 2016 Homework 9

Lecture 7: Optical Spectroscopy. Astrophysical Spectroscopy. Broadband Filters. Fabry-Perot Filters. Interference Filters. Prism Spectrograph

4. What is the speed (in cm s - 1 ) of the tip of the minute hand?

Chapter 1 - The Nature of Light

Lecture 2: Thin Films. Thin Films. Calculating Thin Film Stack Properties. Jones Matrices for Thin Film Stacks. Mueller Matrices for Thin Film Stacks

New Aspects of Old Equations: Metamaterials and Beyond (Part 2) 신종화 KAIST 물리학과

Formula Sheet. ( γ. 0 : X(t) = (A 1 + A 2 t) e 2 )t. + X p (t) (3) 2 γ Γ +t Γ 0 : X(t) = A 1 e + A 2 e + X p (t) (4) 2

Plane Waves Part II. 1. For an electromagnetic wave incident from one medium to a second medium, total reflection takes place when

3 December Lesson 5.5

1 The formation and analysis of optical waveguides

Refractive Index Measurement by Gain- or Loss-Induced Resonance

Edward S. Rogers Sr. Department of Electrical and Computer Engineering. ECE426F Optical Engineering. Final Exam. Dec. 17, 2003.

Exam 3 Solutions. Answer: 1830 Solution: Because of equal and opposite electrical forces, we have conservation of momentum, m e

Lecture 9. Transmission and Reflection. Reflection at a Boundary. Specific Boundary. Reflection at a Boundary

Group Velocity and Phase Velocity

Chapter 33. Electromagnetic Waves

Impact of the Opto-Geometric Parameters on the Band Diagram and Transmission and Reflection Spectrum of the Bragg Structure

Surface Plasmon Wave

10 (4π 10 7 ) 2σ 2( = (1 + j)(.0104) = = j.0001 η c + η j.0104

PRINCIPLES OF PHYSICAL OPTICS

Today in Physics 218: stratified linear media II

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Electrical Engineering and Computer Science

A) n 1 > n 2 > n 3 B) n 1 > n 3 > n 2 C) n 2 > n 1 > n 3 D) n 2 > n 3 > n 1 E) n 3 > n 1 > n 2

Waves. Daniel S. Weile. ELEG 648 Waves. Department of Electrical and Computer Engineering University of Delaware. Plane Waves Reflection of Waves

Electromagnetic spectra

Lecture Outline. Scattering From a Dielectric Slab Anti Reflection Layer Bragg Gratings 8/9/2018. EE 4347 Applied Electromagnetics.

ElectroMagnetic Radiation (EMR) Lecture 2-3 August 29 and 31, 2005

OPSE FINAL EXAM Fall 2015 YOU MUST SHOW YOUR WORK. ANSWERS THAT ARE NOT JUSTIFIED WILL BE GIVEN ZERO CREDIT.

Electricity & Optics

Lecture 8 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell

Waves & Oscillations

ECE357H1F ELECTROMAGNETIC FIELDS FINAL EXAM. 28 April Examiner: Prof. Sean V. Hum. Duration: hours

Electricity & Magnetism Study Questions for the Spring 2018 Department Exam December 4, 2017

PS210 - Optical Techniques. Section VI

PHYS 4400, Principles and Varieties of Solar Energy Instructor: Randy J. Ellingson The University of Toledo

LC circuit: Energy stored. This lecture reviews some but not all of the material that will be on the final exam that covers in Chapters

Today in Physics 218: Fresnel s equations

Final examination. 3 hours (9am 12 noon) Total pages: 7 (seven) PLEASE DO NOT TURN OVER UNTIL EXAM STARTS PLEASE RETURN THIS BOOKLET

Numerical modeling of thin film optical filters

= nm. = nm. = nm

Electromagnetic Waves. Chapter 33 (Halliday/Resnick/Walker, Fundamentals of Physics 8 th edition)

1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light

General Appendix A Transmission Line Resonance due to Reflections (1-D Cavity Resonances)

( z) ( ) ( )( ) ω ω. Wave equation. Transmission line formulas. = v. Helmholtz equation. Exponential Equation. Trig Formulas = Γ. cos sin 1 1+Γ = VSWR

LASERS. Amplifiers: Broad-band communications (avoid down-conversion)

Chapter 3. Design for manufacture of Fabry-Perot cavity sensors

Today in Physics 218: stratified linear media I

III. Spherical Waves and Radiation

Lab 4: Spectrometer Tuesday and Wednesday, April 12, 13 Due: Friday, April 22, 2011

ORE Open Research Exeter

Electromagnetic Waves Across Interfaces

Massachusetts Institute of Technology Physics 8.03 Fall 2004 Final Exam Thursday, December 16, 2004

Describe the forces and torques exerted on an electric dipole in a field.

1. Reminder: E-Dynamics in homogenous media and at interfaces

Outline of College Physics OpenStax Book

Physics of Light and Optics

Electric field enhancement in metallic and multilayer dielectric gratings

PH 222-3A Spring 2010

1. In Young s double slit experiment, when the illumination is white light, the higherorder fringes are in color.

Preview from Notesale.co.uk Page 1 of 38

A longitudinal wave travels through a medium from left to right.

INTRODUCTION TO MICROWAVE REMOTE SENSING. Dr. A. Bhattacharya

Introduction to Photonic Crystals

Experiment 6: Interferometers

Properties of waves. Question. Ch 22, : Waves & interference. Question. Phase difference & interference

OPTICAL Optical properties of multilayer systems by computer modeling

Problem 8.18 For some types of glass, the index of refraction varies with wavelength. A prism made of a material with

Introduction to Seismology Spring 2008

Waves in Linear Optical Media

PAP Physics Spring Exam Review

The Electromagnetic Properties of Materials

Laser Optics-II. ME 677: Laser Material Processing Instructor: Ramesh Singh 1

A) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface

1. (P2.2D) Describe the acceleration and speed of an object that is experiencing uniform circular motion.

Brewster Angle and Total Internal Reflection

Transcription:

Light Reflectors and Optical Resonators Outline Review of Wave Reflection Reflection and Interference Fiber for Telecommunications Optical Resonators 1

Reflection of a Normally Incident EM Wave from a Perfect Conductor E i =ˆxE ( H i =ˆ y η Reflected wave e jkz oe jkz E o o ) e jkz E H H E Incident wave e jkz x E z Standing wave pattern of the E-field kz = 2π kz = π H 2E o 0 z Image by Theogeo http://www. flickr.com/photos/theogeo/1102 816166/ on flickr Standing wave pattern of the H-field 2 kz = 3π/2 kz = π/2 2(E o /η o ) z

Reflection & Transmission of EM Waves at Boundaries E 1 = E i + E r E 2 = E t H 1 = H i + H r Medium 1 Medium 2 H 2 = H r 3

Reflection of EM Waves at Boundaries E 1 (z =0)=E 2 (z =0) Eo i + E r o = E t o H 1 (z =0)=H 2 (z =0) E r μ Eo i E r o E t η = o η = 1 η 1 η2 ɛ r = o η 2 η 1 E = t Eo i t = η 2 + η o 2η 2 = 1 Eo i η 2 + η 1 REFLECTION COEFFICIENT (note that sign of r depends on the relative values of η 2 and η 1 ) TRANSMISION COEFFICIENT 4

x MEDIUM 1 MEDIUM 2 Examples of Light Reflection z The im age below indicates the standing wave patterns ( E i + E r ) resulting when an incident wave in medium 1 with amplitude equal to 1 V/m is incident on an interface. Label the graphs (a)-(g) to match them with the description detailed below. c 2.0 2.0 2.0 2.0 e 1.6 E y,total a) Plot of with medium 1 being air, medium 2, n 2 =2. Normal incidence. E y,total b) Plot of with medium 1 having n 1 = 2, medium 2 being air. Normal incidence. E y,total c) Plot of with medium 1 being air, medium 2 being a perfect conductor 1.33 0.67 1.33 0.67 b a 0.95 2.85 0.32 f g H y,total d) Plot of with medium 1 being air, medium 2 being a perfect conductor E y,total e) Plot of with medium 1 having n 1 =2, medium 2 being air. Angle of incidence greater than critical angle. E y,total f) Plot of with angle of incidence equal to the Brewster angle. 2.0 d 2.0 E y,total g) Plot of with angle of incidence equal to the Brewster angle. Medium 2 is air. 5

Remote Sensing of the Environment using radar E 0 E 5 ε = εo μ = μ o σ =0 1 T 12 E 1 E 4 d 2 ε =3.5ε o μ = μ o σ =10 6 S/m E 2 E 3 T 21 EXAMPLE: MEASUREMENT OF THICKNESS OF POLAR ICE CAPS 6

Reflectometry measurement of distance to a target by identifying the nodes in the standing wave pattern transmitter receiver Conducting surface d 1 d 7

Today s Culture Moment Ice is more reflective than water 70-80% of sunlight reflected by snow 10% reflected by ocean water 20% reflected by vegetation and dark soil 8

The Greenhouse Effect Sunlight is reradiated as heat and trapped by greenhouse gasses such as carbon dioxide. Too much carbon dioxide, however, causes the planet to heat up more than usual. Celsius 19 18 17 16 15 14 13 56.79 F Future Temperatures? 57.97 F 1880 1920 1960 2000 2040 2080 Year 9

Deploy Aluminum Rafts over Dead Ocean Areas? Net excess energy input into planet Earth 1.6 W/m 2. Illuminance on ground level is ~1000 W/m 2 We need to reflect 1.6/1000 of energy back to Balance the Energy IN/OUT Oceans are 90% absorptive (10% reflective) Aluminum is 88% reflective on the shiny side and 80% reflective on the dull side. (Frosted silica might also be able to be used as a reflector) How much of ocean area do we need to cover with 80% reflective sheets of aluminum to balance the energy IN/OUT? (1.6/1000) / (80% - 10%) = 0.23% (of the Earth s surface area) Earth surface area = 5100 million km 2 We need to cover = 1.2 million km 2 equivalent to ~100 years of today s Aluminum production (assuming 50 μm thick Al foil) Dead ocean zones = 0.24 million km 2 Ice fields: North Pole = 9 to 12 million km² Greenland ice sheet = 1.7 million km² South Pole = 14 million km² Image is in the public domain 10

METAL REFLECTION Three Ways to Make a Mirror Kyle Hounsell. All rights reserved. This content is excluded from our Creative Commons license. For more information, see http://ocw.mit.edu/fairuse MULTILAYER REFLECTION Image is in the public domain Image is in the public domain: http://en.wikipedia.org/wiki/ File:Dielectric_laser_mirror_from_a_dye_las er.jpg TOTAL INTERNAL REFLECTION 11

Dielectric Mirrors can be >99% reflective n hi n lo Simple dielectric mirrors consist of stacked of layers of high and low refractive index. The layers are chosen such the path-length differences of reflections from low to high index layers are integer multiples of wavelengths. Similarly, reflections from low-index layers have path length difference of half a wavelength, but add constructively because of 180 degree phase shift from the reflection. For normal incidence, these optimized thicknesses are a quarter of a wavelength d 1 d 2 1 b 2 d 1 = λ/(4nhi) n N LO R = b = Π i=0 1+ b n d 2 = λ/(4nlo) HI Thin layers with a high refractive index n HI are interleaved with thicker layers with a lower refractive index n LO. The path lengths l A and l B differ by exactly one wavelength, which leads to constructive interference. Source: wikipedia.com 12

Opals are an example of dielectric mirrors Colors with λ =2dsin(α) have constructive interference Image is in the public domain Precious opal consists of spheres of silica of fairly regular size, packed into close-packed planes that are stacked together with characteristic dimensions of several hundred nm. λ Silica spheres α d Unique Opals. All rights reserved. This content is excluded from our Creative Commons license. For more information, see http://ocw.mit.edu/fairuse. 13

Fiber to the Home 2.4 Gbps shared by up to 128 users Small Businesses 10-100 Mbps service rates 2.4 Gbps out 1.2 Gbps in 1 OLT 2 Splitter 4 3 20 km reach Splitter 1 2 3 4 Splitter New Buried Development Splitter Time Division Multiplexing 14 Image by Dan Tentler http://www.flickr.com/ photos/vissago/4634464205/ on flickr

Fiber to the Home Time Division Multiplexing 2.4 Gbps shared by up to 128 users Small Businesses 10-100 Mbps service rates Splitter Splitter 2 3 2.4 Gbps out 1.2 Gbps in 1 2 OLT (located in Verizon's central switching office) 3 4 20 km reach 1 4 Splitter Splitter An (Optical Network Terminal) is a media converter that is installed by Verizon either outside or inside your premises, during FiOS installation. The converts fiber-optic light signals to copper/electric signals. Three wavelengths of light are used between the and the OLT (Optical Line Terminal): λ = 1310 nm voice/data transmit λ = 1490 nm voice/data receive λ = 1550 nm video receive Each is capable of delivering: Multiple POTS (plain old telephone service) lines, Internet data, Video 15

Fiber to the Home Image by uuzinger http://www.flickr.com/photos/uuzinger/ 411425461/ on flickr Image by uuzinger http://www.flickr.com/photos/uuzinger/ 411425452/ on flickr Bandwidths & Services POTS Upstream Downstream 1310 nm 1490 nm Voice and Voice and Data Data 1550 nm Video Data Video Channels downstream to each home λ = 1490 and λ = 1550 nm Channel upstream from each home λ = 1310 nm Power & Battery Image of by Josh Bancroft http://www.flickr.com/photos/joshb/87167324/ on flickr 16

Passive Optical Network Optical (PON) Assembly TO Can Laser Single mode fiber TO Can PINS Ball lens Channels downstream to each home λ = 1490 and λ = 1550 nm λ Channel upstream from each home λ = 1310 nm Thin film filters Transmission Upstream Downstream 1310 1490 1550 Wavelength (nm) 17

Separating Wavelengths Dispersion Image by Ian Mackenzie http://www.flickr.com/photos/ madmack/136237003/ on flickr Diffraction Sunlight diffracted through a 20 μm slit Image by wonker http://www.flickr.com/photos/wonker/ 2505350820/ on flickr 18 Image is in the public domain

Resonators STANDING WAVE RESONATORS H E E o E H z kz = 2π kz = π z Terminate the standing wave with a second wall to form a resonator 19

Thin Film Interference E i Image by Yoko Nekonomania http://www. flickr.com/photos/nekonomania/4827035737/ on flickr 3 t 12 (r 21 ) t 21 E i e jβ 22L t 12 r 21 t 21 E i e jβ 22L r 12 E i E i t 12E i t12r 21 r 21 t 21 E i e t 12 t 21 E i e jβ 22L jβ22l 20

Optical Resonator E i E t = [ t 12 t 21e jβ 2L + t 12 e jβ 2L r 21e jβ 2L jβ 2 L r 21 e t 21... ] Ei [ ( jβl 2 = t 12 t 21 e 1+r 12 r 21 e 2jβL + ( r r e 2jβL ) )]... t 12 t 21 e jβ 2L = E 1 r 12 r 21 e 2jβL i 12 21 E i 21

Fabry-Perot Resonance t 12 t 21 e jkl t = 1 r12 r 21 e 2jkL Transmission t 2 1 0.8 0.6 0.4 0.2 0 1.5 1.52 1.54 1.56 1.58 Wavelength [μm] max{e 2jk 2L } =1 Fabry-Perot Resonance: maximum transmission min{e 2jk 2L } = 1 minimum transmission 22

Total Internal Reflection Beyond the critical angle, θ c, a ray within the higher index medium cannot escape at shallower angles n 2 sinθ 2 = n 1 sinθ 1 θ c = sin 1 (n 1 /n 2 ) TOTAL INTERNAL REFLECTION For glass, the critical internal angle is 42 For water, it is 49 Image is in the public domain INCOMING RAY HUGS SURFACE n 1 =1.0 42 n 2 =1.5 23

Waveguide Transport Light Between Mirrors Metal waveguides Dielectric waveguides So what kind of waveguide are the optical fibers? Image by Dan Tentler http://www.flickr.com/ photos/vissago/4634464205/ on flickr 24

Fabry-Perot Modes Constructive Interference r 21 = n 2 n 1 n 2 + n 1 Standing Wave E-field λ o1 = 2n 1L m E r = re i ( ) 1 1 Δλ o =2n L m m +1 2 2n 2 L = m(m +1) λ o2 = 2n 2L m +1 λ o =1μm, n 2 =35,. L = 300μm λ 1 =1μm m = 2100 Δλ =5Å 25

Plane Waves in Lossy Materials E y =Re{ A 1 e j(ωtkz) } +Re{ A 2 e j(ωtkz) } Ey(z,t) =A 1 e α/ 2z cos(ωt kz)+a 2 e +α/2z cos(ωt + kz) Field strength [a.u.] 1.0 0.5 0-0.5-1.0 e ( α/2)z α =2κβ = 2κω c = 4πκ λ 1 2 3 4 5 6 Propagation distance [cm] 26

Resonators with Internal Loss Image is in the public domain r = ñ 1 ñ 1 ñ 2 + 2 n 2ñ1 t = ñ1 + 2 n E t jkl jk r L αl t 1t 2 e t 1 t 2 e e = = Ei 1 r 1r 2e 2j kl 1 r 1r 2e 2jk rl e 2αL...the EM wave loss is what heats the water inside the food 27

Laser Using Fabre-Perot Cavity Resonant modes Gain profile Image is in the public domain 28

Resonators with Internal Gain What if it was possible to make a material with negative absorption so the field grew in magnitude as it passed through a material? Field strength [a.u.] 1.0 0.5 0-0.5 E(z) = E i e gz e gz -1.0 1 2 3 4 5 6 Propagation distance [cm] Resonance: Et t1t 2 e jkl t 1t 2e jkrl e αl = = E 2jkL i 1 r e 2jkL 1r 2 1 r 1r 2e 2jk rl e 2αL e =1 29

Lasers: Something for Nothing (almost) at resonance e 2jkL =1 Et t 1 t 2e jkl t 1 t 2 e jkrl e αl = = E i 1 r 1r e 2jkL 2 1 r 1r 2e 2jk rl e 2αL singularity at 1=r 1 r 2 e ΓgL e αil 1=R1R 2 e 2ΓgL 2α i L e E t E i Image is in the public domain 30

MIT OpenCourseWare http://ocw.mit.edu 6.007 Electromagnetic Energy: From Motors to Lasers Spring 2011 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.