Wave Phenomena Physics 15c
|
|
- Noreen Townsend
- 5 years ago
- Views:
Transcription
1 Wave Phenomena Phyi 15 Leture 18 EM Wave in Matter (H&L Setion 9.7)
2 What We Did Lat Time! Reviewed refletion and refration! Total internal refletion i more ubtle than it look! Imaginary wave extend a few λ beyond the urfae! Studied how to reate EM wave! Aelerated harge radiate EM wave! Power given by Larmor formula! Proportional to (aeleration)! Intability of atom " QM! Polarization parallel to the aeleration! Explain Brewter angle µ q inθ r ET a( t ) 4π r µ qa P 6π a
3 Oillating Charge! Now we onider an oillating harge x i t x e ω! Tranvere omponent of E at (r,θ) i! What thi ign? i t a x ω xe ω! a point oppoite to x # Thi i where the minu ame from! But E T point oppoite to a! It more appropriate to write!! θ µ q inθ µ qω x r inθ ET a( t ) e 4π r 4π r E T point the ame diretion a x E T + r iω t q µ qω x inθ e 4π r E T r iω t
4 Power! Trivial to alulate power denity! NB: Mut take the real part before alulating a! S µ q ω x in θ 16π r 4 o r ( t ) { ω } Time average! Eay enough to alulate total power of radiation! Integrate over a phere at ditane r 4 π π µ q ω x π 3 P dφ S r inθdθ in θdθ 16π 4 µ q ω x 1π S 4 µ q ω x in θ 3π r Inreae with frequeny a ω 4
5 Rayleigh Sattering! Sunlight paing through the air make air moleule oillate! Inoming light ha a broad petrum! All frequenie are more or le equal E q F qe! Moleule radiate power aording to 4 µ q ω x P 1π! More power i aborbed and re-emitted at higher frequenie! Thi i why the ky look blue
6 Sunrie/Sunet! Air atter blue light! Sunlight loe blue a it travere atmophere! It turn red
7 Polarization! Sunlight ontain two polarization Viewed from right! Only one aue radiation that reahe the oberver! Sattered light (what you ee in the blue ky) i polarized! Photographer ue polarizing filter to deepen the olor of the ky
8 Goal for Today! We know an aelerated harge radiate EM wave! Matter i made of harged partile! EM wave paing through matter aelerate them! They radiate EM wave in return! What happen in the end?! It hould explain how EM wave behave in matter! In partiular, why doe it travel lower?! We put together many harge and aelerate them! And try to figure out what happen to the EM field around
9 Sheet of Charge! Imagine an infinite array of harge making a heet! All harge are oillating together a x i t x e ω E? z y x! What kind of EM radiation would they make at a ditane z from the heet?! Suppoe that there are n harge of +q per unit area
10 Sheet of Charge! Conider a little piee! Charge of thi piee i q n dxdy! E due to thi piee i dx dy z r y dx dy x µ qnω x inθ iω t Edxdy T e dxdy 4π r! Conider a imilar piee at x! y-z omponent anel r x θ x E r x We only need x omponent µ qnω x in θ iω t Edxdy x Edxdy T inθ e dxdy 4π r r
11 Radiation From the Sheet! Integrating E x over dxdy i pain r x + y + z r + + µ qnω x + + in θ iω t x Edxdy e dxdy 4π r! Calulation i diffiult, but irrelevant! We know that! E i parallel to the x axi! E doe not depend on x or y inθ y + r z Solution mut be plane wave in ±z diretion! Atual olution i Proportional to veloity in oppoite diretion E (, t z) x iω t iµ qnωx e µ qn z vt ( ) z
12 Wall of Charge! Imagine the heet ha a thikne dz! Denity of harge i n per unit volume " n dz per unit area! Plane EM wave are arriving from z! Suppoe E in move the harge a x qe k in Fore Spring ontant! Thi i impliti iω qe iωt! Veloity i v e k! We an alulate radiation from the heet z i t Ein Ee ω dz z
13 Radiation From the Wall! Charge in the wall radiate µ qn dz iωµ q n E z v t dze e z rad ( > ) ( ) k! Add thi to the inoming wave iωµ q n Ein + Erad 1+ dz Ee k! For mall dz, we an ue e α! E jut after the wall (z dz) i z iω t 1+ α +" z iω t dz z iωµ q n 1 dz µ q n dz iω t iω + dz k k iωt in + rad z dz ( ) E E e E e E e e E in
14 Thin " Thik Wall! Paing the thin wall hange the E field Ez i t E e ω! Add more wall Ez i t E e ω z Ndz 1 µ iω + iωt Ez dz Ee e E E e e z Ndz Ee q n k dz 1 µ q n iω + Ndz iωt k 1 µ q n iω t + z k Multiply the ame fator N time! Solution look jut like plane wave Propagation of plane EM wave through a thik wall of harged partile
15 Phae Veloity Ezt (, ) Ee 1 µ q n iω t z + k! We an alulate the phae veloity by ( ) 1 µ q n t C t + k z ont. C z 1 + µ! Differentiate: qn! That i n 1+ Index of refration!! We found k! p i maller than OK with Relativity! p i ontant No diperion q n dz p 1 µ q n µ q n q n dt + k 1+ k 1+ ε k ε k
16 Quik Summary! We tarted from aelerated harged partile! Eah of them radiate EM wave! Matter i denely populated by thoe! Inoming EM wave make them oillate! Colletive radiation from a thin heet make plane wave! Phae of the EM wave i hifted lightly by adding it! Aumulating the phae hift over finite thikne make plane wave again, but with modified phae veloity! We end up with a lower peed of light! We found origin of refration!
17 Corretion! There wa a mall omiion in the above diuion! Thin heet radiate EM wave in both ide! I ignored the bakward-going wave! Bakward wave ompliate analyi! But the onluion hange little! We till find plane wave with modified phae veloity! Index of refration turn out n + true 1 qn ε k intead of n 1+ qn approx. ε k! For material with mall n, n true n approx.
18 Maxwell Equation! Now we go bak to Maxwell equation E ρ ε B E t B 1 E B + µ J t! Movement of the harge in matter " Current q! We aumed E q E x v k k t! Uual trik with BAC-CAB rule give u 1 E µ qn E E + t k t J qn v Simple wave equation
19 Plane Wave Solution 1 µ qn +! Wave equation redue to! Diperion relation i! We found the ame olution E i( kx ωt) E E E k e t 1 µ qn k E ω + k k ω qn 1 + εk 1+! We ued the hort-ut by truting Maxwell J term! It an be made even impler p ω k qn ε k n 1+ E qn ε k Same n true
20 Maxwell Equation! Take the equation! We are auming q J qn v v k! We ould define ε E B ε µ + µ J t E t εµ E t qn ε + B k E µ qn E B εµ + t k t qn E ε + µ k t! We aborbed the J term into the matter permittivity ε! Now it eay to get ε n 1+ ε qn ε k
21 Quik Summary Again! We took three approahe to get the ame anwer! Miroopi: what doe eah eletron do?! Gave u a glimpe of really why light goe lower! Integration wa too tough! Current denity in vauum! Repreent eletron olletive movement by J! Wave equation i eay enough to olve! Permittivity of matter! Aborb J by replaing ε with ε! Solution i totally trivial! They repreent different level of abtration
22 Realiti Example! In the previou analyi, we ued a impliti model for the movement of the harge x qe k! Let try omething more realiti! We diu plama firt! I know it ound unfamiliar! But it a lot impler tuff than mot matter! Then we talk about more ordinary inulator! I ll take air for an example
23 Plama! Imagine a pae filled with free eletron! We neutralize the eletron ga by adding poitive ion! The ion are heavy Ignore their movement! Suh a mixture i alled a plama! You an make them by heating tuff up really hot! It rather eay to analyze! Eah eletron equation of motion i i t q m!! x qe qee ω x E e mω! Current denity iq n J qn v E mω e iωt iω t
24 Plama Frequeny! Wave Equation i 1 E J µ t t E + ω qn ω ω p! Diperion relation i k 1 1 εmω ω qn! ω p i alled the plama frequeny ε m! Plama i a diperive medium:! ω p i a ut-off frequeny iq n J qn v E mω ω µ qn k E E+ E m 1 ω p! For ω < ω p, k beome imaginary " Wave diappear p ω k ω e iωt
25 Phae and Group Veloitie ω ω( k) ωp + k ω k p 1 ω ω p ω p k g dω 1 ω p ω dk ω Slope p Slope g ω p! p i greater than, but g remain le than! I hope you remember thi from Leture #1
26 Ionophere! Sunlight ionize air in the upper atmophere! Ionophere ha free eletron denity n ~ 1 1 /m 3! Varie with unpot, eaon, day/night, latitude, et qn 7 ω p rad/ ε m ω p 6 ν p 9 1 Hz π! Viible light (ν ~ 1 14 Hz) pae through eaily! Shortwave radio (ν ~ 5 MHz) i refleted! You an hear BBC, Deuthe Welle, Voie of Ruia
27 Inulator! Unlike in plama or in metal, eletron in inulator are bound to the moleule! Binding fore i imilar to a pring! Ret of the moleule muh heavier " Ignore the movement! Equation of motion qe m kx i t m!! x qee ω k x! Fored oillation We know the olution i t e ω x x mω x qe k x qe q k mω E x m( ω ω )! Current denity i iω q n k iωt J qnv E e ω m( ω ω ) m M
28 Diperion Relation! Wave Equation i 1 E J µ t t E +! Diperion relation i k ω! It diperive again ω p k 1 + ρω ( ω ω ) ω µ qn ω k E E E m ω ω qn ω ω ρ εm( ω ω ) ω ω n 1 + ρω ( ω ω ) iω q n m( ω ω ) J qn v E ρ Idential to the LC tranmiion line diued in Leture #1 e qn ε k iωt
29 Example: Air! Air i a mixture of N, O, H O, Ar, et! Many reonane exit in UV and horter wavelength! Thing are impler in viible light p 1 + ρω ( ω ω ) + ρ 1! At STP, n 1.3 " ρ.6 n 1+ ρ 1+ ρ! ρ i proportional to denity n! Uing the ideal ga formula PV nmolrt P(atm) n + Index of refration of air T (K) 1 for low-freq. EM wave 1 ρ qn ε k
30 Mirage! In a hot day, air temperature i higher near the ground 73 P(atm) n 1+.3 T (K) 1! Light travel fater! Refration make light bend upward! You may ee the ground reflet light a if there i a path of water low fat ool hot T
31 Summary! Studied miroopi origin of refration in matter! Started from EM radiation due to aelerated harge! Uniform ditribution of uh harge make EM wave appear to low down! Three level of deribing EM wave in matter! Point harge in vauum! Current denity in vauum! Permittivity (and permeability) of matter! Analyzed EM wave in plama and in inulator n ω ω plama 1 p! Plama refletive for ω < ω p n 1 + ρω ( ω ω ) inulator ω p qn ε m
Wave Phenomena Physics 15c. Lecture 17 EM Waves in Matter
Wave Phenomena Physics 15c Lecture 17 EM Waves in Matter What We Did Last Time Reviewed reflection and refraction Total internal reflection is more subtle than it looks Imaginary waves extend a few beyond
More information@(; t) p(;,b t) +; t), (; t)) (( whih lat line follow from denition partial derivative. in relation quoted in leture. Th derive wave equation for ound
24 Spring 99 Problem Set 5 Optional Problem Phy February 23, 999 Handout Derivation Wave Equation for Sound. one-dimenional wave equation for ound. Make ame ort Derive implifying aumption made in deriving
More informationc = ω k = 1 v = ω k = 1 ²µ
3. Electromagtic Wave 3.5. Plama wave A plama i an ionized ga coniting of charged particle (e.g., electron and ion). Variou wave can be excited eaily in a plama. Wave phenomena have been an important ubject
More informationThe Laws of Electromagnetism Maxwell s Equations Displacement Current Electromagnetic Radiation
The letromagneti petrum The Law of letromagnetim Maxwell quation Diplaement Current letromagneti Radiation Maxwell quation of letromagnetim in Vauum (no harge, no mae) lane letromagneti Wave d d z y (x,
More informationTHE SOLAR SYSTEM. We begin with an inertial system and locate the planet and the sun with respect to it. Then. F m. Then
THE SOLAR SYSTEM We now want to apply what we have learned to the olar ytem. Hitorially thi wa the great teting ground for mehani and provided ome of it greatet triumph, uh a the diovery of the outer planet.
More informationWhere Standard Physics Runs into Infinite Challenges, Atomism Predicts Exact Limits
Where Standard Phyi Run into Infinite Challenge, Atomim Predit Exat Limit Epen Gaarder Haug Norwegian Univerity of Life Siene Deember, 07 Abtrat Where tandard phyi run into infinite hallenge, atomim predit
More informationUVa Course on Physics of Particle Accelerators
UVa Coure on Phyi of Partile Aelerator B. Norum Univerity of Virginia G. A. Krafft Jefferon Lab 3/7/6 Leture x dx d () () Peudoharmoni Solution = give β β β () ( o µ + α in µ ) β () () β x dx ( + α() α
More informationEinstein's Energy Formula Must Be Revised
Eintein' Energy Formula Mut Be Reied Le Van Cuong uong_le_an@yahoo.om Information from a iene journal how that the dilation of time in Eintein peial relatie theory wa proen by the experiment of ientit
More informationTo determine the biasing conditions needed to obtain a specific gain each stage must be considered.
PHYSIS 56 Experiment 9: ommon Emitter Amplifier A. Introdution A ommon-emitter oltage amplifier will be tudied in thi experiment. You will inetigate the fator that ontrol the midfrequeny gain and the low-and
More informationLaplace Transformation
Univerity of Technology Electromechanical Department Energy Branch Advance Mathematic Laplace Tranformation nd Cla Lecture 6 Page of 7 Laplace Tranformation Definition Suppoe that f(t) i a piecewie continuou
More informationGeneration of EM waves
Generation of EM waves Susan Lea Spring 015 1 The Green s funtion In Lorentz gauge, we obtained the wave equation: A 4π J 1 The orresponding Green s funtion for the problem satisfies the simpler differential
More informationRiemann s Functional Equation is Not Valid and its Implication on the Riemann Hypothesis. Armando M. Evangelista Jr.
Riemann Functional Equation i Not Valid and it Implication on the Riemann Hypothei By Armando M. Evangelita Jr. On November 4, 28 ABSTRACT Riemann functional equation wa formulated by Riemann that uppoedly
More informationPhysics 218, Spring February 2004
Physis 8 Spring 004 0 February 004 Today in Physis 8: dispersion in onduting dia Semilassial theory of ondutivity Condutivity and dispersion in tals and in very dilute ondutors : group veloity plasma frequeny
More informationGreen s function for the wave equation
Green s funtion for the wave equation Non-relativisti ase January 2019 1 The wave equations In the Lorentz Gauge, the wave equations for the potentials are (Notes 1 eqns 43 and 44): 1 2 A 2 2 2 A = µ 0
More informationEELE 3332 Electromagnetic II Chapter 10
EELE 333 Electromagnetic II Chapter 10 Electromagnetic Wave Propagation Ilamic Univerity of Gaza Electrical Engineering Department Dr. Talal Skaik 01 1 Electromagnetic wave propagation A changing magnetic
More informationMechanics Physics 151
Mechanic Phyic 151 Lecture 7 Scattering Problem (Chapter 3) What We Did Lat Time Dicued Central Force Problem l Problem i reduced to one equation mr = + f () r 3 mr Analyzed qualitative behavior Unbounded,
More informationDeepak Rajput
General quetion about eletron and hole: A 1a) What ditinguihe an eletron from a hole? An) An eletron i a fundamental partile wherea hole i jut a onept. Eletron arry negative harge wherea hole are onidered
More informationNonlinear Dynamics of Single Bunch Instability in Accelerators *
SLAC-PUB-7377 Deember 996 Nonlinear Dynami of Single Bunh Intability in Aelerator * G. V. Stupakov Stanford Linear Aelerator Center Stanford Univerity, Stanford, CA 9439 B.N. Breizman and M.S. Pekker Intitute
More informationConstant Force: Projectile Motion
Contant Force: Projectile Motion Abtract In thi lab, you will launch an object with a pecific initial velocity (magnitude and direction) and determine the angle at which the range i a maximum. Other tak,
More informationPHYS 110B - HW #6 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased
PHYS B - HW #6 Spring 4, Solution by David Pace Any referenced equation are from Griffith Problem tatement are paraphraed. Problem. from Griffith Show that the following, A µo ɛ o A V + A ρ ɛ o Eq..4 A
More informationUniform Acceleration Problems Chapter 2: Linear Motion
Name Date Period Uniform Acceleration Problem Chapter 2: Linear Motion INSTRUCTIONS: For thi homework, you will be drawing a coordinate axi (in math lingo: an x-y board ) to olve kinematic (motion) problem.
More informationRiemann s Functional Equation is Not a Valid Function and Its Implication on the Riemann Hypothesis. Armando M. Evangelista Jr.
Riemann Functional Equation i Not a Valid Function and It Implication on the Riemann Hypothei By Armando M. Evangelita Jr. armando78973@gmail.com On Augut 28, 28 ABSTRACT Riemann functional equation wa
More informationBogoliubov Transformation in Classical Mechanics
Bogoliubov Tranformation in Claical Mechanic Canonical Tranformation Suppoe we have a et of complex canonical variable, {a j }, and would like to conider another et of variable, {b }, b b ({a j }). How
More informationClass XII - Physics Electromagnetic Waves Chapter-wise Problems
Class XII - Physis Eletromagneti Waves Chapter-wise Problems Multiple Choie Question :- 8 One requires ev of energy to dissoiate a arbon monoxide moleule into arbon and oxygen atoms The minimum frequeny
More informationThermochemistry and Calorimetry
WHY? ACTIVITY 06-1 Thermohemitry and Calorimetry Chemial reation releae or tore energy, uually in the form of thermal energy. Thermal energy i the kineti energy of motion of the atom and moleule ompriing
More informationMAE 101A. Homework 3 Solutions 2/5/2018
MAE 101A Homework 3 Solution /5/018 Munon 3.6: What preure gradient along the treamline, /d, i required to accelerate water upward in a vertical pipe at a rate of 30 ft/? What i the anwer if the flow i
More informationEE 333 Electricity and Magnetism, Fall 2009 Homework #11 solution
EE 333 Eetriity and Magnetim, Fa 009 Homework #11 oution 4.4. At the interfae between two magneti materia hown in Fig P4.4, a urfae urrent denity J S = 0.1 ŷ i fowing. The magneti fied intenity H in region
More informationChapter 26 Lecture Notes
Chapter 26 Leture Notes Physis 2424 - Strauss Formulas: t = t0 1 v L = L0 1 v m = m0 1 v E = m 0 2 + KE = m 2 KE = m 2 -m 0 2 mv 0 p= mv = 1 v E 2 = p 2 2 + m 2 0 4 v + u u = 2 1 + vu There were two revolutions
More informationPHY 108: Optical Physics. Solution to Midterm Test
PHY 108: Optial Physis Solution to Midterm Test TA: Xun Jia 1 May 14, 2008 1 Email: jiaxun@physis.ula.edu Spring 2008 Physis 108 Xun Jia (May 14, 2008) Problem #1 For a two mirror resonant avity, the resonane
More informationPhysics 218, Spring February 2004
Physis 8 Spring 004 8 February 004 Today in Physis 8: dispersion Motion of bound eletrons in matter and the frequeny dependene of the dieletri onstant Dispersion relations Ordinary and anomalous dispersion
More informationPhysics 486. Classical Newton s laws Motion of bodies described in terms of initial conditions by specifying x(t), v(t).
Physis 486 Tony M. Liss Leture 1 Why quantum mehanis? Quantum vs. lassial mehanis: Classial Newton s laws Motion of bodies desribed in terms of initial onditions by speifying x(t), v(t). Hugely suessful
More informationELECTROMAGNETIC WAVES
ELECTROMAGNETIC WAVES Now we will study eletromagneti waves in vauum or inside a medium, a dieletri. (A metalli system an also be represented as a dieletri but is more ompliated due to damping or attenuation
More informationLecture 23 Date:
Lecture 3 Date: 4.4.16 Plane Wave in Free Space and Good Conductor Power and Poynting Vector Wave Propagation in Loy Dielectric Wave propagating in z-direction and having only x-component i given by: E
More informationTutorial 8: Solutions
Tutorial 8: Solutions 1. * (a) Light from the Sun arrives at the Earth, an average of 1.5 10 11 m away, at the rate 1.4 10 3 Watts/m of area perpendiular to the diretion of the light. Assume that sunlight
More informationName Solutions to Test 1 September 23, 2016
Name Solutions to Test 1 September 3, 016 This test onsists of three parts. Please note that in parts II and III, you an skip one question of those offered. Possibly useful formulas: F qequb x xvt E Evpx
More informationLecture 15 - Current. A Puzzle... Advanced Section: Image Charge for Spheres. Image Charge for a Grounded Spherical Shell
Lecture 15 - Current Puzzle... Suppoe an infinite grounded conducting plane lie at z = 0. charge q i located at a height h above the conducting plane. Show in three different way that the potential below
More informationCritical Percolation Probabilities for the Next-Nearest-Neighboring Site Problems on Sierpinski Carpets
Critial Perolation Probabilitie for the Next-Nearet-Neighboring Site Problem on Sierpinki Carpet H. B. Nie, B. M. Yu Department of Phyi, Huazhong Univerity of Siene and Tehnology, Wuhan 430074, China K.
More informationGeneral Equilibrium. What happens to cause a reaction to come to equilibrium?
General Equilibrium Chemial Equilibrium Most hemial reations that are enountered are reversible. In other words, they go fairly easily in either the forward or reverse diretions. The thing to remember
More informationLecture 16. Kinetics and Mass Transfer in Crystallization
Leture 16. Kineti and Ma Tranfer in Crytallization Crytallization Kineti Superaturation Nuleation - Primary nuleation - Seondary nuleation Crytal Growth - Diffuion-reation theory - Srew-diloation theory
More informationProblem 1. Construct a filtered probability space on which a Brownian motion W and an adapted process X are defined and such that
Stochatic Calculu Example heet 4 - Lent 5 Michael Tehranchi Problem. Contruct a filtered probability pace on which a Brownian motion W and an adapted proce X are defined and uch that dx t = X t t dt +
More informationME2142/ME2142E Feedback Control Systems
Root Locu Analyi Root Locu Analyi Conider the cloed-loop ytem R + E - G C B H The tranient repone, and tability, of the cloed-loop ytem i determined by the value of the root of the characteritic equation
More informationCHAPTER 24: ELECTROMAGNETIC WAVES
College Phyi Student Manual Chapter 4 CHAPTER 4: ELECTROMAGNETC WAVES 4. MAXWELL S EQUATONS: ELECTROMAGNETC WAVES PREDCTED AND OSERVED. Veriy that the orret value or the peed o light i obtained when nuerial
More information1. Basic introduction to electromagnetic field. wave properties and particulate properties.
Lecture Baic Radiometric Quantitie. The Beer-Bouguer-Lambert law. Concept of extinction cattering plu aborption and emiion. Schwarzchild equation. Objective:. Baic introduction to electromagnetic field:
More informationDISCHARGE MEASUREMENT IN TRAPEZOIDAL LINED CANALS UTILIZING HORIZONTAL AND VERTICAL TRANSITIONS
Ninth International Water Tehnology Conferene, IWTC9 005, Sharm El-Sheikh, Egypt 63 DISCHARGE MEASUREMENT IN TRAPEZOIDAL LINED CANALS UTILIZING HORIZONTAL AND VERTICAL TRANSITIONS Haan Ibrahim Mohamed
More informationPhysics Exam 3 Formulas
Phyic 10411 Exam III November 20, 2009 INSTRUCTIONS: Write your NAME on the front of the blue exam booklet. The exam i cloed book, and you may have only pen/pencil and a calculator (no tored equation or
More informationWavetech, LLC. Ultrafast Pulses and GVD. John O Hara Created: Dec. 6, 2013
Ultrafast Pulses and GVD John O Hara Created: De. 6, 3 Introdution This doument overs the basi onepts of group veloity dispersion (GVD) and ultrafast pulse propagation in an optial fiber. Neessarily, it
More informationSound Propagation through Circular Ducts with Spiral Element Inside
Exerpt from the Proeeding of the COMSOL Conferene 8 Hannover Sound Propagation through Cirular Dut with Spiral Element Inide Wojieh Łapka* Diviion of Vibroaouti and Sytem Biodynami, Intitute of Applied
More informationChapter 7: 17, 20, 24, 25, 32, 35, 37, 40, 47, 66 and 79.
hapter 7: 17, 0,, 5,, 5, 7, 0, 7, 66 and 79. 77 A power tranitor mounted on the wall diipate 0.18 W. he urface temperature of the tranitor i to be determined. Aumption 1 Steady operating condition exit.
More informationGNSS Solutions: What is the carrier phase measurement? How is it generated in GNSS receivers? Simply put, the carrier phase
GNSS Solution: Carrier phae and it meaurement for GNSS GNSS Solution i a regular column featuring quetion and anwer about technical apect of GNSS. Reader are invited to end their quetion to the columnit,
More informationELECTROMAGNETIC WAVES AND PHOTONS
CHAPTER ELECTROMAGNETIC WAVES AND PHOTONS Problem.1 Find the magnitude and direction of the induced electric field of Example.1 at r = 5.00 cm if the magnetic field change at a contant rate from 0.500
More informationCherenkov Radiation. Bradley J. Wogsland August 30, 2006
Cherenkov Radiation Bradley J. Wogsland August 3, 26 Contents 1 Cherenkov Radiation 1 1.1 Cherenkov History Introdution................... 1 1.2 Frank-Tamm Theory......................... 2 1.3 Dispertion...............................
More informationLecture #1: Quantum Mechanics Historical Background Photoelectric Effect. Compton Scattering
561 Fall 2017 Leture #1 page 1 Leture #1: Quantum Mehanis Historial Bakground Photoeletri Effet Compton Sattering Robert Field Experimental Spetrosopist = Quantum Mahinist TEXTBOOK: Quantum Chemistry,
More informationPlasmonic Waveguide Analysis
Plamoni Waveguide Analyi Sergei Yuhanov, Jerey S. Crompton *, and Kyle C. Koppenhoeer AltaSim Tehnologie, LLC *Correponding author: 3. Wilon Bridge Road, Suite 4, Columbu, O 4385, je@altaimtehnologie.om
More informationEP225 Note No. 5 Mechanical Waves
EP5 Note No. 5 Mechanical Wave 5. Introduction Cacade connection of many ma-pring unit conitute a medium for mechanical wave which require that medium tore both kinetic energy aociated with inertia (ma)
More informationLecture 17. Phys. 207: Waves and Light Physics Department Yarmouk University Irbid Jordan
Leture 17 Phys. 7: Waves and Light Physis Departent Yarouk University 1163 Irbid Jordan Dr. Nidal Ershaidat http://taps.yu.edu.jo/physis/courses/phys7/le5-1 Maxwell s Equations In 187, Jaes Clerk Maxwell's
More informationGreen s function for the wave equation
Green s funtion for the wave equation Non relativisti ase 1 The wave equations In the Lorentz Gauge, the wave equations for the potentials in Lorentz Gauge Gaussian units are: r 2 A 1 2 A 2 t = 4π 2 j
More informationChapter 4. Simulations. 4.1 Introduction
Chapter 4 Simulation 4.1 Introdution In the previou hapter, a methodology ha been developed that will be ued to perform the ontrol needed for atuator haraterization. A tudy uing thi methodology allowed
More information4. (12) Write out an equation for Poynting s theorem in differential form. Explain in words what each term means physically.
Eletrodynamis I Exam 3 - Part A - Closed Book KSU 205/2/8 Name Eletrodynami Sore = 24 / 24 points Instrutions: Use SI units. Where appropriate, define all variables or symbols you use, in words. Try to
More informationChapter 6 Control Systems Design by Root-Locus Method. Lag-Lead Compensation. Lag lead Compensation Techniques Based on the Root-Locus Approach.
hapter 6 ontrol Sytem Deign by Root-Lou Method Lag-Lead ompenation Lag lead ompenation ehnique Baed on the Root-Lou Approah. γ β K, ( γ >, β > ) In deigning lag lead ompenator, we onider two ae where γ
More information22.01 Fall 2015, Problem Set 6 (Normal Version Solutions)
.0 Fall 05, Problem Set 6 (Normal Version Solutions) Due: November, :59PM on Stellar November 4, 05 Complete all the assigned problems, and do make sure to show your intermediate work. Please upload your
More informationDepartment of Mechanical Engineering Massachusetts Institute of Technology Modeling, Dynamics and Control III Spring 2002
Department of Mechanical Engineering Maachuett Intitute of Technology 2.010 Modeling, Dynamic and Control III Spring 2002 SOLUTIONS: Problem Set # 10 Problem 1 Etimating tranfer function from Bode Plot.
More informationME 375 FINAL EXAM Wednesday, May 6, 2009
ME 375 FINAL EXAM Wedneday, May 6, 9 Diviion Meckl :3 / Adam :3 (circle one) Name_ Intruction () Thi i a cloed book examination, but you are allowed three ingle-ided 8.5 crib heet. A calculator i NOT allowed.
More informationMicrowave instability of coasting ion beam with space charge in small isochronous ring
SLAC-PUB-56 Mirowave intability of oating ion beam with pae harge in mall iohronou ring Yingjie Li* Department of Phyi, Mihigan State Univerity, Eat Laning, MI 4884, USA Lanfa Wang SLAC National Aelerator
More informationF = c where ^ı is a unit vector along the ray. The normal component is. Iν cos 2 θ. d dadt. dp normal (θ,φ) = dpcos θ = df ν
INTRODUCTION So far, the only information we have been able to get about the universe beyond the solar system is from the eletromagneti radiation that reahes us (and a few osmi rays). So doing Astrophysis
More informationWe consider the nonrelativistic regime so no pair production or annihilation.the hamiltonian for interaction of fields and sources is 1 (p
.. RADIATIVE TRANSITIONS Marh 3, 5 Leture XXIV Quantization of the E-M field. Radiative transitions We onsider the nonrelativisti regime so no pair prodution or annihilation.the hamiltonian for interation
More informationTMA4125 Matematikk 4N Spring 2016
Norwegian Univerity of Science and Technology Department of Mathematical Science TMA45 Matematikk 4N Spring 6 Solution to problem et 6 In general, unle ele i noted, if f i a function, then F = L(f denote
More informationThe statistical properties of the primordial fluctuations
The tatitical propertie of the primordial fluctuation Lecturer: Prof. Paolo Creminelli Trancriber: Alexander Chen July 5, 0 Content Lecture Lecture 4 3 Lecture 3 6 Primordial Fluctuation Lecture Lecture
More informationPY Modern Physics
PY 351 - Modern Physis Assignment 6 - Otober 19, 2017. Due in lass on Otober 26, 2017. Assignment 6: Do all six problems. After a base of 4 points (to make the maximum sore equal to 100), eah orret solution
More informationTowards a nonsingular inflationary Universe
Toward a noningular inflationary Univere Taotao Qiu Intitute of Atrophyi, Central China Normal Univerity 014-1-19 Baed on Phy.Rev. D88 (013) 04355, JCAP 1110: 036, 011, JHEP 0710 (007) 071, 1 and reent
More informationAP Physics Charge Wrap up
AP Phyic Charge Wrap up Quite a few complicated euation for you to play with in thi unit. Here them babie i: F 1 4 0 1 r Thi i good old Coulomb law. You ue it to calculate the force exerted 1 by two charge
More informationPulsed Magnet Crimping
Puled Magnet Crimping Fred Niell 4/5/00 1 Magnetic Crimping Magnetoforming i a metal fabrication technique that ha been in ue for everal decade. A large capacitor bank i ued to tore energy that i ued to
More informationLecture 7: Testing Distributions
CSE 5: Sublinear (and Streaming) Algorithm Spring 014 Lecture 7: Teting Ditribution April 1, 014 Lecturer: Paul Beame Scribe: Paul Beame 1 Teting Uniformity of Ditribution We return today to property teting
More informationPhysics 41 Homework Set 3 Chapter 17 Serway 7 th Edition
Pyic 41 Homework Set 3 Capter 17 Serway 7 t Edition Q: 1, 4, 5, 6, 9, 1, 14, 15 Quetion *Q17.1 Anwer. Te typically iger denity would by itelf make te peed of ound lower in a olid compared to a ga. Q17.4
More informationRadiation processes and mechanisms in astrophysics 3. R Subrahmanyan Notes on ATA lectures at UWA, Perth 22 May 2009
Radiation proesses and mehanisms in astrophysis R Subrahmanyan Notes on ATA letures at UWA, Perth May 009 Synhrotron radiation - 1 Synhrotron radiation emerges from eletrons moving with relativisti speeds
More informationExam 1 Solutions. +4q +2q. +2q +2q
PHY6 9-8-6 Exam Solution y 4 3 6 x. A central particle of charge 3 i urrounded by a hexagonal array of other charged particle (>). The length of a ide i, and charge are placed at each corner. (a) [6 point]
More informationONE-PARAMETER MODEL OF SEAWATER OPTICAL PROPERTIES
Oean Opti XIV CD-ROM, Kailua-Kona, Hawaii, 0- November 998 (publihed by Offie of Naval Reearh, November 998) INTRODUCTION ONE-PARAMETER MODEL OF SEAWATER OPTICAL PROPERTIES Vladimir I Haltrin Naval Reearh
More informationDIFFERENTIAL EQUATIONS
DIFFERENTIAL EQUATIONS Laplace Tranform Paul Dawkin Table of Content Preface... Laplace Tranform... Introduction... The Definition... 5 Laplace Tranform... 9 Invere Laplace Tranform... Step Function...4
More informationPlasma Processes. m v = ee. (2)
Plasma Processes In the preceding few lectures, we ve focused on specific microphysical processes. In doing so, we have ignored the effect of other matter. In fact, we ve implicitly or explicitly assumed
More informationMath 273 Solutions to Review Problems for Exam 1
Math 7 Solution to Review Problem for Exam True or Fale? Circle ONE anwer for each Hint: For effective tudy, explain why if true and give a counterexample if fale (a) T or F : If a b and b c, then a c
More informationLECTURE 22. Collective effects in multi-particle beams: Parasitic Losses. Longitudinal impedances in accelerators (continued)
LECTURE Collective effect in multi-particle beam: Longitudinal impedance in accelerator Tranvere impedance in accelerator Paraitic Loe /7/0 USPAS Lecture Longitudinal impedance in accelerator (continued)
More informationTheoretical Computer Science. Optimal algorithms for online scheduling with bounded rearrangement at the end
Theoretical Computer Science 4 (0) 669 678 Content lit available at SciVere ScienceDirect Theoretical Computer Science journal homepage: www.elevier.com/locate/tc Optimal algorithm for online cheduling
More informationThe Laplace Transform , Haynes Miller and Jeremy Orloff
The Laplace Tranform 8.3, Hayne Miller and Jeremy Orloff Laplace tranform baic: introduction An operator take a function a input and output another function. A tranform doe the ame thing with the added
More informationEcon 455 Answers - Problem Set 4. where. ch ch ch ch ch ch ( ) ( ) us us ch ch us ch. (world price). Combining the above two equations implies: 40P
Fall 011 Eon 455 Harvey Lapan Eon 455 Anwer - roblem et 4 1. Conider the ae of two large ountrie: U: emand = 300 4 upply = 6 where h China: emand = 300 10 ; upply = 0 h where (a) Find autarky prie: U:
More informationSocial Studies 201 Notes for March 18, 2005
1 Social Studie 201 Note for March 18, 2005 Etimation of a mean, mall ample ize Section 8.4, p. 501. When a reearcher ha only a mall ample ize available, the central limit theorem doe not apply to the
More informationLecture 2: Computer Arithmetic: Adders
CMU 8-447 S 9 L2-29 8-447 Leture 2: Computer Arithmeti: Adder Jame C. Hoe Dept of ECE, CMU January 4, 29 Announement: No la on Monday Verilog Refreher next Wedneday Review P&H Ch 3 Handout: Lab and HW
More informationParticle-wave symmetry in Quantum Mechanics And Special Relativity Theory
Partile-wave symmetry in Quantum Mehanis And Speial Relativity Theory Author one: XiaoLin Li,Chongqing,China,hidebrain@hotmail.om Corresponding author: XiaoLin Li, Chongqing,China,hidebrain@hotmail.om
More informationLinear Motion, Speed & Velocity
Add Important Linear Motion, Speed & Velocity Page: 136 Linear Motion, Speed & Velocity NGSS Standard: N/A MA Curriculum Framework (006): 1.1, 1. AP Phyic 1 Learning Objective: 3.A.1.1, 3.A.1.3 Knowledge/Undertanding
More informationLet s consider nonrelativistic electrons. A given electron follows Newton s law. m v = ee. (2)
Plasma Processes Initial questions: We see all objects through a medium, which could be interplanetary, interstellar, or intergalactic. How does this medium affect photons? What information can we obtain?
More informationPID CONTROL. Presentation kindly provided by Dr Andy Clegg. Advanced Control Technology Consortium (ACTC)
PID CONTROL Preentation kindly provided by Dr Andy Clegg Advaned Control Tehnology Conortium (ACTC) Preentation Overview Introdution PID parameteriation and truture Effet of PID term Proportional, Integral
More informationSingular perturbation theory
Singular perturbation theory Marc R. Rouel June 21, 2004 1 Introduction When we apply the teady-tate approximation (SSA) in chemical kinetic, we typically argue that ome of the intermediate are highly
More informationMath Skills. Scientific Notation. Uncertainty in Measurements. Appendix A5 SKILLS HANDBOOK
ppendix 5 Scientific Notation It i difficult to work with very large or very mall number when they are written in common decimal notation. Uually it i poible to accommodate uch number by changing the SI
More informationFI 3221 ELECTROMAGNETIC INTERACTIONS IN MATTER
6/0/06 FI 3 ELECTROMAGNETIC INTERACTION IN MATTER Alexander A. Ikandar Phyic of Magnetim and Photonic CATTERING OF LIGHT Rayleigh cattering cattering quantitie Mie cattering Alexander A. Ikandar Electromagnetic
More informationChapter 9 Review. Block: Date:
Science 10 Chapter 9 Review Name: KEY Block: Date: 1. A change in velocity occur when the peed o an object change, or it direction o motion change, or both. Thee change in velocity can either be poitive
More informationHeat transfer and absorption of SO 2 of wet flue gas in a tube cooled
Heat tranfer and aborption of SO of wet flue ga in a tube ooled L. Jia Department of Power Engineering, Shool of Mehanial, Eletroni and Control Engineering, Beijing Jiaotong Univerity, Beijing 00044, China
More informationInverse Kinematics 1 1/21/2018
Invere Kinemati 1 Invere Kinemati 2 given the poe of the end effetor, find the joint variable that produe the end effetor poe for a -joint robot, given find 1 o R T 3 2 1,,,,, q q q q q q RPP + Spherial
More informationEnergy-Work Connection Integration Scheme for Nonholonomic Hamiltonian Systems
Commun. Theor. Phy. Beiing China 50 2008 pp. 1041 1046 Chinee Phyial Soiety Vol. 50 No. 5 November 15 2008 Energy-Wor Connetion Integration Sheme for Nonholonomi Hamiltonian Sytem WANG Xian-Jun 1 and FU
More information22.54 Neutron Interactions and Applications (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E')
22.54 Neutron Interations and Appliations (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E') Referenes -- J. R. Lamarsh, Introdution to Nulear Reator Theory (Addison-Wesley, Reading, 1966),
More informationMASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.286: The Early Universe December 21, 2013 Prof. Alan Guth QUIZ 3 SOLUTIONS
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physis Department Physis 8.286: The Early Universe Deember 2, 203 Prof. Alan Guth QUIZ 3 SOLUTIONS Quiz Date: Deember 5, 203 PROBLEM : DID YOU DO THE READING? (35
More informationThe Electric Potential Energy
Lecture 6 Chapter 28 Phyic II The Electric Potential Energy Coure webite: http://aculty.uml.edu/andriy_danylov/teaching/phyicii New Idea So ar, we ued vector quantitie: 1. Electric Force (F) Depreed! 2.
More informations much time does it take for the dog to run a distance of 10.0m
ATTENTION: All Diviion I tudent, START HERE. All Diviion II tudent kip the firt 0 quetion, begin on #.. Of the following, which quantity i a vector? Energy (B) Ma Average peed (D) Temperature (E) Linear
More information