L = 2 λ 2 = λ (1) In other words, the wavelength of the wave in question equals to the string length,

Size: px
Start display at page:

Download "L = 2 λ 2 = λ (1) In other words, the wavelength of the wave in question equals to the string length,"

Transcription

1 PHY 309 L. Soltions for Problem set # 6. Textbook problem Q.20 at the end of chapter 5: For any standing wave on a string, the distance between neighboring nodes is λ/2, one half of the wavelength. The wave in qestion has three nodes, one at the left end of the string, one in the middle, and one at the right end. Conseqently, the length L of the string is twice the inter-nodal distance, i.e. L 2 λ 2 λ () In other words, the wavelength of the wave in qestion eqals to the string length, λ(this wave) L. (2) By comparison, the fndamental harmonic of the string has only two nodes at the end of the string bt no nodes in the middle. Conseqently, the distance between neighboring nodes of the fndamental harmonic is the length of the whole string, ths λ(fndamental) 2 L λ(fndamental) 2L. (3) Comparing the last two formlae, we immediately see that λ(this wave) λ(fndamental), (4) 2 the wave in qestion has half the wavelength of the fndamental harmonic. Finally, the wavelength and the freqency of any wave are related to the wave speed as f λ. (5) The standing wave in qestion and the fndamental harmonic obtain on the same string, so the wave speed is the same for both waves. Conseqently, eq. (4) for the wavelengths of

2 the two waves imply that their freqencies are related as f(this wave) λ(this wave) 2 2 λ(fndamental) (6) λ(fndamental) 2 f(fndamental), the wave in qestion has twice the freqency of the fndamental harmonic. Indeed, the wave in qestion is the second harmonic of the string. Textbook problem SP.2 at the end of chapter 5: (a) I presme the string is niform, so the linear density m/l is the same for all parts of the string. Since we know the mass of the whole string, the linear density is the ration of that mass to the length of the whole string, m whole L whole kg.25 m kg/m. (7) The playing part of the string between two points where it s fixed to the gitar s deck has a shorter length L 64 cm < L whole, bt it also has a smaller mass m < m whole. We don t know that mass, bt if the string is niform, then the linear density m/l of the playing part shold be the same as the linear density of the whole string, ( m L m whole L whole kg/m. (8) (b) The speed of transverse wave on a string depends on the string s tension force T and linear density m/l, ths T 720 N kg/m 22, 500 m 2 /s 2 50 m/s. (9) 2

3 (c) The fndamental harmonic of the string is a standing wave with two nodes at points where the string is fixed to the deck and no extra nodes in between. Since the distance between nodes of a standing wave is λ/2 one half of the wavelength the fndamental harmonic has λ 2 L (0) where L 64 cm is the length of the playing part of the gitar string, i.e., the distance between the two points where it s fixed to the gitar deck. Therefore, the wavelength of the fndamental harmonic is λ 2L 2 64 cm.28 m. () (d) The freqency of the fndamental harmonic follows from its wavelength λ (fond in part (c)) and wave speed (fond in part (d)): f λ 50 m/s.28 m 7 cycles/s 7 Hz. (2) (e) Higher harmonics of a string are standing waves that have one or more nodes in the middle of the playing part of the string as well as a node at each end (where the string is fixed to the deck). Altogether, the n th harmonic has n + 3, 4, 5,... nodes so the length L of the playing part of the string is divided into n 2, 3, 4,... intervals between the nodes. Since the length of each sch interval is λ/2, the wavelength λ n of the n th harmonic satisfies n λ n 2 L, (3) hence λ n 2L n. (4) For n this formla gives s the wavelength λ 2L of the fndamental harmonic. The 3

4 higher harmonics have shorter wavelengths λ n λ 2L n. (5) The freqencies f n of the higher harmonics follow from their wavelength and the speed of the wave on the string, f n λ n 2L/n n 2L (6) In particlar, the fndamental harmonic # has freqency f 2L, (7) cf. part (d); it is called the fndamental freqency of the string. The higher harmonics have freqencies that are mltiples of the fndamental freqency, f n n f, n 2, 3, 4,... (8) Specifically, the second harmonic jst above the fndamental has one node in the middle of the string, its wavelength λ 2 L λ /2 is a half of the fndamental harmonic s wavelength, and its freqency f 2 2 f is twice the fndamental freqency. For the string in qestion, λ 2.28 m m and f Hz 334 Hz. (9) 4

5 Non-textbook problem #I: The speed of sond in a flid a gas or a liqid is given by a general formla sond B ρ (20) where ρ m/v is the flid s density and B is its blk modls which relates pressre changes to small relative changes of the volme, δp B δv V. (2) When a gas is compressed or rarefied adiabatically fast enogh to prevent the heat from flowing in or ot of the gas its pressre and volme are related as P V γ constant for some adiabatic coefficient γ that depends on the atomic strctre of the gas s molecles: The monoatomic gases sch as helim or argon have γ 5 3, the diatomic gases sch as N 2 or O 2 have γ 7 5.4, while the polyatomic gases sch as carbon dioxide have γ.3. For any sch gas, the adiabatic modls follows from the absolte pressre of the gas, B γ P. (22) Conseqently, the speed of sond in a gas is sond γp ρ. (23) At the reference altitde on Mars (the eqivalent of sea-level on Earth, except Mars does not have any seas), the atmospheric pressre is abot 600 Pascal (less than % of air pressre on Earth, P Earth 00, 000 Pa). Martian atmosphere consists mostly of carbon dioxide (CO 2 ), so its adiabatic coefficient γ is abot.3. And its density dring very cold 5

6 winter nights reaches abot ρ 8 g/m kg/m 3. (24) The speed of sond in Martian atmosphere follows from eq. (23): Note nits: sond γ P ρ Pa m/s. (25) kg/m3 Pa kg/m 3 J/m3 kg/m 3 J/kg (m/s)2. (26) Ths, when we plg into eq. (23) pressre in Pascals and density in kilograms per cbic meter, the speed of sond comes ot in meters per second. Alternative soltion: Sppose I did not give yo the density of Martian atmosphere bt only its temperatre. In this case, yo cold have obtained the density from the ideal gas law P V nrt (27) where T is the absolte temperatre of the gas (in Kelvins), P is its absolte pressre (in Pascals), R 834 J/K/kmol is the niversal gas constant, and n is the amont of gas in kilomols. Here I se kilomols rather than mols becase the mass of n kilomols of gas with moleclar weight is m n (28) in nits of kilograms rather than grams. Hence, the density of gas in kilograms per cbic meter is ρ m V n n RT/P P RT. (29) Note that this density is proportional to the pressre of the gas, so the ratio P / P ρ P RT RT (30) depends only on the temperatre and moleclar weight of the gas, bt does not depend on 6

7 the pressre itself. Conseqently, the speed of sond in the gas sond γp ρ γrt (3) depends only on the the temperatre and chemical formla of the gas bt does not depend on its pressre. Martian atmosphere is made of mostly carbon dioxide CO 2, so it has moleclar weight and adiabatic coefficient γ.3. When this atmosphere is cooled to 70 Kelvin dring a cold winter night on Mars, the speed of sond in it is sond γrt.3 (834 J/K/kmol) (70 K) 44 kg/kmol 460 J/kg 208 m/s. (32) The formla (3) makes clear why the speed of sond on Mars is lower than on Earth: On Mars, the air has lower temperatre than on Earth bt heavier moleclar weight, T Mars < T Earth bt Mars > Earth, hence ( ) γrt Mars < ( ) γrt Earth (33) and therefore the speed of sond ( sond ) γrt on Mars < ( sond ) γrt. (34) on Earth Non-textbook problem #II: Standing waves in pipes are explained in detail in my notes, so I am not going to repeat the theory here. Instead, let me simply refer yo to eqations (notes.33 38) for pipes with two open ends and eqations (notes.43 50) for pipes with one open end and one closed end. 7

8 (a) A pipe with two open ends contains one half-wavelength λ/2 of the lowest harmonic. Conseqently, given the pipe s length L, the lowest harmonic mst have wavelength 2L 2.5 m 3.0 m. (35) In contrast, a pipe with one open end and one closed end contains only one qarterwavelength λ/4 of its own lowest harmonic. pipe is Hence, the lowest harmonic of the second 4L 4.5 m 6.0 m. (36) (b) The n th standing wave mode in a pipe with two open ends fits n half-wavelength intervals inside the pipe, L n λ 2. (notes.35) Hence, the n th harmonic of an open-open pipe of length L has wavelength n 2L n. (37) For the first pipe in qestion, this gives s λ 2L 3.0 m for the first (fndamental) harmonic (cf. eq. (35)), 2 2L 2.5 m (38) for the second harmonic, 3 2L 3.0 m (39) for the third harmonic, etc., etc. 8

9 In contrast, the n th standing wave mode in a pipe with different ends (one open, one closed) fits 2n qarter-wavelength intervals inside the pipe, ths L (2n ) λ 4. (40) Conseqently, the n th harmonic of an open-closed pipe of length L has wavelength n 4L 2n. (4) For the second pipe in qestion which also has L.5 m this gives s λ 4L 6.0 m for the first (fndamental) harmonic (cf. eq. (36)), 2 4L m (42) for the second harmonic, 3 2L 5.2 m (43) for the third harmonic, etc., etc. (c) Given the speed of sond 340 m/s, the freqency f of any sond wave of known wavelength λ can be fond as f /λ. Ths, the first three harmonics of the first pipe (open-open) have freqencies f open open f open open 2 f open open m/s 3.0 m 340 m/s.5 m 340 m/s.0 m 3 Hz, 227 Hz, 340 Hz. Likewise, the first three harmonics of the second pipe (open-closed) have freqencies (44) f open closed f open closed 2 f open closed m/s 6.0 m 340 m/s 2.0 m 340 m/s.2 m 57 Hz, 70 Hz, 283 Hz. (45) 9

10 Textbook qestion Q.2 at the end of chapter 6: Q) Is the electric field of an electromagnetic wave constant in time? A) Hell, no! In any electromagnetic wave, both the electric and the magnetic fields oscillate with the freqency of the wave, E(t) E 0 sin(2πft + φ 0 ), B(t) B0 sin(2πft + φ 0 ), (46) where the amplitdes E 0 and B 0 and the phase φ 0 depend on space coordinates (x, y, z). For different types of waves the space dependence is different for example, a plane wave rnning in x direction has E(t; x, y, z) B(t; x, y, z) ( E 0 sin 2πft 2πx ), λ ( B 0 sin 2πft 2πx ), λ E 0 B 0, E0 and B 0 x axis. while a standing wave has the same phase everywhere bt (x, y, z) dependent amplitdes E ) (x, y, z) and B 0 (x, y, z). Bt the time dependence of the electric and magnetic fields of any EM wave is always as in eq. (46). (47) Textbook qestion Q.4 at the end of chapter 6: Both the microwaves and the light waves are electromagnetic waves, so in vacm they travel at the same speed c , 458 m/s. (48) However, the light waves and the microwaves have very different freqencies and wavelength. The visible light waves have wavelengths in a rather narrow range from abot 700 nanometers for red light to abot 400 nanometers for violet light, i.e., from.4 million to 2.5 million wavelengths in one meter. The freqencies of these waves which obtain from the wavelengths as f c/λ, see the next problem below range from 430 THz for red light to 740 THz for the violet light, i.e., from 430 trillions to 750 trillions cycles per second. 0

11 By comparison, the microwaves have mch longer wavelengths between millimeter and meter, while their freqencies range from 300 MHz to 300 GHz, i.e., from 300 million to 300 billion cycles per second. Textbook problem SP. at the end of chapter 6: (a) Speed of light waves or any other electromagnetic waves in empty space (vacm) is a niversal constant c , 458 m/s m/s (49) (300,000 km/s or abot 86,000 miles/second). Conseqently, in vacm, the wavelength λ of any EM wave is related to its freqency f as λ f c m/s. (50) On the red end of the visible light spectrm, the longest wavelength average hman eye can see is λ red 750 nm (nano-meters). According to eq. (50), this corresponds to lowest visible freqency f red c λ red m/s m Hz, (5) or 400 TeraHertz. On the violet end of the visible light spectrm, the shortest wavelength average hman eye can see is λ red 380 nm (nano-meters). According to eq. (50), this corresponds to highest visible freqency f violet c λ violet m/s m Hz, (52) or 790 TeraHertz.

12 (b) When EM waves propagate throgh some transparent material air, water, glass, whatever, the interactions between the electric and magnetic field and the atoms slow down the EM wave s speed. Ths, in matter, light moves at a slower speed light in material c n < c (53) where n > is the index of refraction of the material. Since the air is rather dilte, its refraction index is little different from to be precise, n air.0003 so the light waves move throgh air at almost the same speed as throgh the vacm, light in air c n air c. (54) Denser materials have higher refraction coefficients, for example n.33 for water and n.5 for many types of glass. Conseqently, the light moves throgh sch materials notably slower than throgh the vacm, light in,water light in,glass c n water c n glass 3 4 c m/s, 2 3 c m/s. (55) PS: The problem ask yo to calclate the speed of light in glass. I have added a similar calclation for the water to illstrate the general rle, bt yo did not have to do it for this homework. (c) When a wave propagates from one medim to another, its freqency does not change it s always the same nmber of cycles per second. For example, if a motor plls a 200 times each second, then the whole string vibrates at freqency f 200 Hz. The vibrating string pshes the air arond it, which creates a sond wave with the same freqency f 200 Hz. And that sond makes yor ear drm vibrates withe the same freqency f 200 Hz. The same works for the light waves: when light moves from one media into another for example, from vacm to glass its freqency does not change. Bt if the speeds of 2

13 light in the two media are different, then the wavelength of the same light wave wold also be different: λ f λ 2 c/n 2 f. (56) The different wavelength make the light change directions as it crosses from one media to another this is called refraction. To calclate the wavelength of light in some material, all we need is the light s freqency f and the speed of light in that material: the wavelength follow from that as λ /f. Ths, given the reslts of parts (a) and (b) of this problem, we immediately have red light λin glass violet light λin glass light in glass f red light light in glass f violet light m/s Hz m/s Hz 500 nm, 253 nm. (57) PS: Since the speed of light in air is almost the same as in vacm, its wavelength in air is almost the same as in vacm. That s why the problem does not specify whether the very red light has wavelength 750 nm in vacm or in air the difference is negligible. Ditto for 380 nm wavelength of the violet light. For simplicity, I assme those wavelength were measred in vacm, bt in practice it wold make very little difference if they were measred in air. 3

PROBLEMS

PROBLEMS PROBLEMS------------------------------------------------ - 7- Thermodynamic Variables and the Eqation of State 1. Compter (a) the nmber of moles and (b) the nmber of molecles in 1.00 cm of an ideal gas

More information

Microscopic Properties of Gases

Microscopic Properties of Gases icroscopic Properties of Gases So far we he seen the gas laws. These came from observations. In this section we want to look at a theory that explains the gas laws: The kinetic theory of gases or The kinetic

More information

Diffraction of light due to ultrasonic wave propagation in liquids

Diffraction of light due to ultrasonic wave propagation in liquids Diffraction of light de to ltrasonic wave propagation in liqids Introdction: Acostic waves in liqids case density changes with spacing determined by the freqency and the speed of the sond wave. For ltrasonic

More information

5. The Bernoulli Equation

5. The Bernoulli Equation 5. The Bernolli Eqation [This material relates predominantly to modles ELP034, ELP035] 5. Work and Energy 5. Bernolli s Eqation 5.3 An example of the se of Bernolli s eqation 5.4 Pressre head, velocity

More information

Momentum Equation. Necessary because body is not made up of a fixed assembly of particles Its volume is the same however Imaginary

Momentum Equation. Necessary because body is not made up of a fixed assembly of particles Its volume is the same however Imaginary Momentm Eqation Interest in the momentm eqation: Qantification of proplsion rates esign strctres for power generation esign of pipeline systems to withstand forces at bends and other places where the flow

More information

PHY 113 C General Physics I 11 AM 12:15 PM TR Olin 101

PHY 113 C General Physics I 11 AM 12:15 PM TR Olin 101 PHY 113 C General Phsics I 11 AM 1:15 PM R Olin 101 Plan for Lectre 16: Chapter 16 Phsics of wave motion 1. Review of SHM. Eamples of wave motion 3. What determines the wave velocit 4. Properties of periodic

More information

EDEXCEL NATIONAL CERTIFICATE/DIPLOMA. PRINCIPLES AND APPLICATIONS of FLUID MECHANICS UNIT 13 NQF LEVEL 3 OUTCOME 3 - HYDRODYNAMICS

EDEXCEL NATIONAL CERTIFICATE/DIPLOMA. PRINCIPLES AND APPLICATIONS of FLUID MECHANICS UNIT 13 NQF LEVEL 3 OUTCOME 3 - HYDRODYNAMICS EDEXCEL NATIONAL CERTIFICATE/DIPLOMA PRINCIPLES AND APPLICATIONS of FLUID MECHANICS UNIT 3 NQF LEVEL 3 OUTCOME 3 - HYDRODYNAMICS TUTORIAL - PIPE FLOW CONTENT Be able to determine the parameters of pipeline

More information

EXERCISES WAVE EQUATION. In Problems 1 and 2 solve the heat equation (1) subject to the given conditions. Assume a rod of length L.

EXERCISES WAVE EQUATION. In Problems 1 and 2 solve the heat equation (1) subject to the given conditions. Assume a rod of length L. .4 WAVE EQUATION 445 EXERCISES.3 In Problems and solve the heat eqation () sbject to the given conditions. Assme a rod of length.. (, t), (, t) (, ),, > >. (, t), (, t) (, ) ( ) 3. Find the temperatre

More information

Second-Order Wave Equation

Second-Order Wave Equation Second-Order Wave Eqation A. Salih Department of Aerospace Engineering Indian Institte of Space Science and Technology, Thirvananthapram 3 December 016 1 Introdction The classical wave eqation is a second-order

More information

ρ u = u. (1) w z will become certain time, and at a certain point in space, the value of

ρ u = u. (1) w z will become certain time, and at a certain point in space, the value of THE CONDITIONS NECESSARY FOR DISCONTINUOUS MOTION IN GASES G I Taylor Proceedings of the Royal Society A vol LXXXIV (90) pp 37-377 The possibility of the propagation of a srface of discontinity in a gas

More information

Cosmic Microwave Background Radiation. Carl W. Akerlof April 7, 2013

Cosmic Microwave Background Radiation. Carl W. Akerlof April 7, 2013 Cosmic Microwave Backgrond Radiation Carl W. Akerlof April 7, 013 Notes: Dry ice sblimation temperatre: Isopropyl alcohol freezing point: LNA operating voltage: 194.65 K 184.65 K 18.0 v he terrestrial

More information

Relativity II. The laws of physics are identical in all inertial frames of reference. equivalently

Relativity II. The laws of physics are identical in all inertial frames of reference. equivalently Relatiity II I. Henri Poincare's Relatiity Principle In the late 1800's, Henri Poincare proposed that the principle of Galilean relatiity be expanded to inclde all physical phenomena and not jst mechanics.

More information

Math 263 Assignment #3 Solutions. 1. A function z = f(x, y) is called harmonic if it satisfies Laplace s equation:

Math 263 Assignment #3 Solutions. 1. A function z = f(x, y) is called harmonic if it satisfies Laplace s equation: Math 263 Assignment #3 Soltions 1. A fnction z f(x, ) is called harmonic if it satisfies Laplace s eqation: 2 + 2 z 2 0 Determine whether or not the following are harmonic. (a) z x 2 + 2. We se the one-variable

More information

sin u 5 opp } cos u 5 adj } hyp opposite csc u 5 hyp } sec u 5 hyp } opp Using Inverse Trigonometric Functions

sin u 5 opp } cos u 5 adj } hyp opposite csc u 5 hyp } sec u 5 hyp } opp Using Inverse Trigonometric Functions 13 Big Idea 1 CHAPTER SUMMARY BIG IDEAS Using Trigonometric Fnctions Algebra classzone.com Electronic Fnction Library For Yor Notebook hypotense acent osite sine cosine tangent sin 5 hyp cos 5 hyp tan

More information

Setting The K Value And Polarization Mode Of The Delta Undulator

Setting The K Value And Polarization Mode Of The Delta Undulator LCLS-TN-4- Setting The Vale And Polarization Mode Of The Delta Undlator Zachary Wolf, Heinz-Dieter Nhn SLAC September 4, 04 Abstract This note provides the details for setting the longitdinal positions

More information

FEA Solution Procedure

FEA Solution Procedure EA Soltion Procedre (demonstrated with a -D bar element problem) EA Procedre for Static Analysis. Prepare the E model a. discretize (mesh) the strctre b. prescribe loads c. prescribe spports. Perform calclations

More information

Two questions from the exam

Two questions from the exam Two qestions from the exam 3. When the sn is located near one of the horizons, an observer looking at the sky directly overhead will view partially polarized light. This effect is de to which of the following

More information

n 1 sin 1 n 2 sin 2 Light and Modern Incident ray Normal 30.0 Air Glass Refracted ray speed of light in vacuum speed of light in a medium c v

n 1 sin 1 n 2 sin 2 Light and Modern Incident ray Normal 30.0 Air Glass Refracted ray speed of light in vacuum speed of light in a medium c v Light and Modern E hf n speed of light in vacm speed of light in a medim c v n sin n sin Incident ray Normal TIP. The reqency Remains the Same The freqency of a wave does not change as the wave passes

More information

EXPT. 5 DETERMINATION OF pk a OF AN INDICATOR USING SPECTROPHOTOMETRY

EXPT. 5 DETERMINATION OF pk a OF AN INDICATOR USING SPECTROPHOTOMETRY EXPT. 5 DETERMITIO OF pk a OF IDICTOR USIG SPECTROPHOTOMETRY Strctre 5.1 Introdction Objectives 5.2 Principle 5.3 Spectrophotometric Determination of pka Vale of Indicator 5.4 Reqirements 5.5 Soltions

More information

BLOOM S TAXONOMY. Following Bloom s Taxonomy to Assess Students

BLOOM S TAXONOMY. Following Bloom s Taxonomy to Assess Students BLOOM S TAXONOMY Topic Following Bloom s Taonomy to Assess Stdents Smmary A handot for stdents to eplain Bloom s taonomy that is sed for item writing and test constrction to test stdents to see if they

More information

Cosmic rays. l Some come from the sun (relatively low energy) and some from catastrophic events elsewhere in the galaxy/universe

Cosmic rays. l Some come from the sun (relatively low energy) and some from catastrophic events elsewhere in the galaxy/universe Special relativity The laws of physics are the same in all coordinate systems either at rest or moving at constant speed with respect to one another The speed of light in a vacm has the same vale regardless

More information

Elements of Coordinate System Transformations

Elements of Coordinate System Transformations B Elements of Coordinate System Transformations Coordinate system transformation is a powerfl tool for solving many geometrical and kinematic problems that pertain to the design of gear ctting tools and

More information

What is fundamental? wwhat is it made of? whow is it all held together? The TWO most fundamental questions about the universe are: Fig. 15.1, p.

What is fundamental? wwhat is it made of? whow is it all held together? The TWO most fundamental questions about the universe are: Fig. 15.1, p. What is fndamental? The TWO most fndamental qestions abot the niverse are: wwhat is it made of? whow is it all held together? Fig. 15.1, p. 467 For Fndamental Elements l The Hnt for the answers to those

More information

University of California, Berkeley Physics H7C Fall 1999 (Strovink) SOLUTION TO FINAL EXAMINATION

University of California, Berkeley Physics H7C Fall 1999 (Strovink) SOLUTION TO FINAL EXAMINATION University of California Berkeley Physics H7C Fall 999 (Strovink SOUTION TO FINA EXAMINATION Directions. Do all six problems (weights are indicated. This is a closed-book closed-note exam except for three

More information

CFD-Simulation thermoakustischer Resonanzeffekte zur Bestimmung der Flammentransferfunktion

CFD-Simulation thermoakustischer Resonanzeffekte zur Bestimmung der Flammentransferfunktion CFD-Simlation thermoakstischer Resonanzeffekte zr Bestimmng der Flammentransferfnktion Ator: Dennis Paschke Technische Universität Berlin Institt für Strömngsmechanik nd Technische Akstik FG Experimentelle

More information

The Cross Product of Two Vectors in Space DEFINITION. Cross Product. u * v = s ƒ u ƒƒv ƒ sin ud n

The Cross Product of Two Vectors in Space DEFINITION. Cross Product. u * v = s ƒ u ƒƒv ƒ sin ud n 12.4 The Cross Prodct 873 12.4 The Cross Prodct In stdying lines in the plane, when we needed to describe how a line was tilting, we sed the notions of slope and angle of inclination. In space, we want

More information

THE INTERNATIONAL SYSTEM OF UNITS (SI) SI Base Units. Quantity Name of unit Symbol

THE INTERNATIONAL SYSTEM OF UNITS (SI) SI Base Units. Quantity Name of unit Symbol Appendix THE INTERNATIONAL SYSTEM OF UNITS (SI) Table 1 SI Base Units Qantity Name of nit Symbol Lengt meter m Mass kilogram kg Time second s Electric crrent ampere A Termodynamic temperatre kelvin K Lminos

More information

III. Demonstration of a seismometer response with amplitude and phase responses at:

III. Demonstration of a seismometer response with amplitude and phase responses at: GG5330, Spring semester 006 Assignment #1, Seismometry and Grond Motions De 30 Janary 006. 1. Calibration Of A Seismometer Using Java: A really nifty se of Java is now available for demonstrating the seismic

More information

MAE 320 Thermodynamics HW 4 Assignment

MAE 320 Thermodynamics HW 4 Assignment MAE 0 Thermodynamics HW 4 Assignment The homework is de Friday, October 7 th, 06. Each problem is worth the points indicated. Copying of the soltion from any sorce is not acceptable. (). Mltiple choice

More information

3.4-Miscellaneous Equations

3.4-Miscellaneous Equations .-Miscellaneos Eqations Factoring Higher Degree Polynomials: Many higher degree polynomials can be solved by factoring. Of particlar vale is the method of factoring by groping, however all types of factoring

More information

Lecture 3. (2) Last time: 3D space. The dot product. Dan Nichols January 30, 2018

Lecture 3. (2) Last time: 3D space. The dot product. Dan Nichols January 30, 2018 Lectre 3 The dot prodct Dan Nichols nichols@math.mass.ed MATH 33, Spring 018 Uniersity of Massachsetts Janary 30, 018 () Last time: 3D space Right-hand rle, the three coordinate planes 3D coordinate system:

More information

m = Average Rate of Change (Secant Slope) Example:

m = Average Rate of Change (Secant Slope) Example: Average Rate o Change Secant Slope Deinition: The average change secant slope o a nction over a particlar interval [a, b] or [a, ]. Eample: What is the average rate o change o the nction over the interval

More information

Study on the impulsive pressure of tank oscillating by force towards multiple degrees of freedom

Study on the impulsive pressure of tank oscillating by force towards multiple degrees of freedom EPJ Web of Conferences 80, 0034 (08) EFM 07 Stdy on the implsive pressre of tank oscillating by force towards mltiple degrees of freedom Shigeyki Hibi,* The ational Defense Academy, Department of Mechanical

More information

Electromagnetic Radiation

Electromagnetic Radiation Electromagnetic Radiation Producing EMR All EMR is produced by accelerating charges Consists of changing electric and magnetic fields Speed of all EMR in vacuum is 3.00 x 10 8 m/s EMR is made up electric

More information

Free electron lasers

Free electron lasers Preparation of the concerned sectors for edcational and R&D activities related to the Hngarian ELI project Free electron lasers Lectre 1.: Introdction, overview and working principle János Hebling Zoltán

More information

Section 7.4: Integration of Rational Functions by Partial Fractions

Section 7.4: Integration of Rational Functions by Partial Fractions Section 7.4: Integration of Rational Fnctions by Partial Fractions This is abot as complicated as it gets. The Method of Partial Fractions Ecept for a few very special cases, crrently we have no way to

More information

FRTN10 Exercise 12. Synthesis by Convex Optimization

FRTN10 Exercise 12. Synthesis by Convex Optimization FRTN Exercise 2. 2. We want to design a controller C for the stable SISO process P as shown in Figre 2. sing the Yola parametrization and convex optimization. To do this, the control loop mst first be

More information

WEAR PREDICTION OF A TOTAL KNEE PROSTHESIS TIBIAL TRAY

WEAR PREDICTION OF A TOTAL KNEE PROSTHESIS TIBIAL TRAY APPLIED PHYSICS MEDICAL WEAR PREDICTION OF A TOTAL KNEE PROSTHESIS TIBIAL TRAY L. CÃPITANU, A. IAROVICI, J. ONIªORU Institte of Solid Mechanics, Romanian Academy, Constantin Mille 5, Bcharest Received

More information

1. INTRODUCTION. A solution for the dark matter mystery based on Euclidean relativity. Frédéric LASSIAILLE 2009 Page 1 14/05/2010. Frédéric LASSIAILLE

1. INTRODUCTION. A solution for the dark matter mystery based on Euclidean relativity. Frédéric LASSIAILLE 2009 Page 1 14/05/2010. Frédéric LASSIAILLE Frédéric LASSIAILLE 2009 Page 1 14/05/2010 Frédéric LASSIAILLE email: lmimi2003@hotmail.com http://lmi.chez-alice.fr/anglais A soltion for the dark matter mystery based on Eclidean relativity The stdy

More information

Lesson 81: The Cross Product of Vectors

Lesson 81: The Cross Product of Vectors Lesson 8: The Cross Prodct of Vectors IBHL - SANTOWSKI In this lesson yo will learn how to find the cross prodct of two ectors how to find an orthogonal ector to a plane defined by two ectors how to find

More information

Phys102 Term: 103 First Major- July 16, 2011

Phys102 Term: 103 First Major- July 16, 2011 Q1. A stretched string has a length of.00 m and a mass of 3.40 g. A transverse sinusoidal wave is travelling on this string, and is given by y (x, t) = 0.030 sin (0.75 x 16 t), where x and y are in meters,

More information

1 The space of linear transformations from R n to R m :

1 The space of linear transformations from R n to R m : Math 540 Spring 20 Notes #4 Higher deriaties, Taylor s theorem The space of linear transformations from R n to R m We hae discssed linear transformations mapping R n to R m We can add sch linear transformations

More information

Vectors in Rn un. This definition of norm is an extension of the Pythagorean Theorem. Consider the vector u = (5, 8) in R 2

Vectors in Rn un. This definition of norm is an extension of the Pythagorean Theorem. Consider the vector u = (5, 8) in R 2 MATH 307 Vectors in Rn Dr. Neal, WKU Matrices of dimension 1 n can be thoght of as coordinates, or ectors, in n- dimensional space R n. We can perform special calclations on these ectors. In particlar,

More information

4 Primitive Equations

4 Primitive Equations 4 Primitive Eqations 4.1 Spherical coordinates 4.1.1 Usefl identities We now introdce the special case of spherical coordinates: (,, r) (longitde, latitde, radial distance from Earth s center), with 0

More information

Lecture 26 Chapter 16 Ideal-dilute solutions and Colligative Properties

Lecture 26 Chapter 16 Ideal-dilute solutions and Colligative Properties Lectre 26 Chapter 16 Ideal-dilte soltions and Colligative Properties nnonce: HW de next Monday Remember Seminars Friday Hledin at 3:00, Bchwalter at 4:00 We ll go over exams on this afternoon Otline: Mixing

More information

Classify by number of ports and examine the possible structures that result. Using only one-port elements, no more than two elements can be assembled.

Classify by number of ports and examine the possible structures that result. Using only one-port elements, no more than two elements can be assembled. Jnction elements in network models. Classify by nmber of ports and examine the possible strctres that reslt. Using only one-port elements, no more than two elements can be assembled. Combining two two-ports

More information

Math 116 First Midterm October 14, 2009

Math 116 First Midterm October 14, 2009 Math 116 First Midterm October 14, 9 Name: EXAM SOLUTIONS Instrctor: Section: 1. Do not open this exam ntil yo are told to do so.. This exam has 1 pages inclding this cover. There are 9 problems. Note

More information

By Dr. Salah Salman. Problem (1)

By Dr. Salah Salman. Problem (1) Chemical Eng. De. Problem ( Solved Problems Samles in Flid Flow 0 A late of size 60 cm x 60 cm slides over a lane inclined to the horizontal at an angle of 0. It is searated from the lane with a film of

More information

Study of the diffusion operator by the SPH method

Study of the diffusion operator by the SPH method IOSR Jornal of Mechanical and Civil Engineering (IOSR-JMCE) e-issn: 2278-684,p-ISSN: 2320-334X, Volme, Isse 5 Ver. I (Sep- Oct. 204), PP 96-0 Stdy of the diffsion operator by the SPH method Abdelabbar.Nait

More information

Reduction of over-determined systems of differential equations

Reduction of over-determined systems of differential equations Redction of oer-determined systems of differential eqations Maim Zaytse 1) 1, ) and Vyachesla Akkerman 1) Nclear Safety Institte, Rssian Academy of Sciences, Moscow, 115191 Rssia ) Department of Mechanical

More information

Modeling Effort on Chamber Clearing for IFE Liquid Chambers at UCLA

Modeling Effort on Chamber Clearing for IFE Liquid Chambers at UCLA Modeling Effort on Chamber Clearing for IFE Liqid Chambers at UCLA Presented by: P. Calderoni own Meeting on IFE Liqid Wall Chamber Dynamics Livermore CA May 5-6 3 Otline his presentation will address

More information

The Bow Shock and the Magnetosheath

The Bow Shock and the Magnetosheath Chapter 6 The Bow Shock and the Magnetosheath The solar wind plasma travels sally at speeds which are faster than any flid plasma wave relative to the magnetosphere. Therefore a standing shock wave forms

More information

Chem 4501 Introduction to Thermodynamics, 3 Credits Kinetics, and Statistical Mechanics. Fall Semester Homework Problem Set Number 10 Solutions

Chem 4501 Introduction to Thermodynamics, 3 Credits Kinetics, and Statistical Mechanics. Fall Semester Homework Problem Set Number 10 Solutions Chem 4501 Introdction to Thermodynamics, 3 Credits Kinetics, and Statistical Mechanics Fall Semester 2017 Homework Problem Set Nmber 10 Soltions 1. McQarrie and Simon, 10-4. Paraphrase: Apply Eler s theorem

More information

DEFINITION OF A NEW UO 2 F 2 DENSITY LAW FOR LOW- MODERATED SOLUTIONS (H/U < 20) AND CONSEQUENCES ON CRITICALITY SAFETY

DEFINITION OF A NEW UO 2 F 2 DENSITY LAW FOR LOW- MODERATED SOLUTIONS (H/U < 20) AND CONSEQUENCES ON CRITICALITY SAFETY DEFINITION OF A NEW UO 2 F 2 DENSITY LAW FOR LOW- MODERATED SOLUTIONS ( < 20) AND CONSEQUENCES ON CRITICALITY SAFETY N. Leclaire, S. Evo, I.R.S.N., France Introdction In criticality stdies, the blk density

More information

PhysicsAndMathsTutor.com

PhysicsAndMathsTutor.com C Integration - By sbstittion PhysicsAndMathsTtor.com. Using the sbstittion cos +, or otherwise, show that e cos + sin d e(e ) (Total marks). (a) Using the sbstittion cos, or otherwise, find the eact vale

More information

1 Differential Equations for Solid Mechanics

1 Differential Equations for Solid Mechanics 1 Differential Eqations for Solid Mechanics Simple problems involving homogeneos stress states have been considered so far, wherein the stress is the same throghot the component nder std. An eception to

More information

Prandl established a universal velocity profile for flow parallel to the bed given by

Prandl established a universal velocity profile for flow parallel to the bed given by EM 0--00 (Part VI) (g) The nderlayers shold be at least three thicknesses of the W 50 stone, bt never less than 0.3 m (Ahrens 98b). The thickness can be calclated sing Eqation VI-5-9 with a coefficient

More information

Obliqe Projection. A body is projected from a point with different angles of projections 0 0, 35 0, 45 0, 60 0 with the horizontal bt with same initial speed. Their respective horizontal ranges are R,

More information

Higher Maths A1.3 Recurrence Relations - Revision

Higher Maths A1.3 Recurrence Relations - Revision Higher Maths A Recrrence Relations - Revision This revision pack covers the skills at Unit Assessment exam level or Recrrence Relations so yo can evalate yor learning o this otcome It is important that

More information

Experimental Study of an Impinging Round Jet

Experimental Study of an Impinging Round Jet Marie Crie ay Final Report : Experimental dy of an Impinging Rond Jet BOURDETTE Vincent Ph.D stdent at the Rovira i Virgili University (URV), Mechanical Engineering Department. Work carried ot dring a

More information

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information Concepts: Properties of Electromagnetic Radiation Chapter 5 Electromagnetic waves Types of spectra Temperature Blackbody radiation Dual nature of radiation Atomic structure Interaction of light and matter

More information

1 JAXA Special Pblication JAXA-SP-1-E Small-scale trblence affects flow fields arond a blff body and therefore it governs characteristics of cross-sec

1 JAXA Special Pblication JAXA-SP-1-E Small-scale trblence affects flow fields arond a blff body and therefore it governs characteristics of cross-sec First International Symposim on Fltter and its Application, 1 11 IEXPERIMENTAL STUDY ON TURBULENCE PARTIAL SIMULATION FOR BLUFF BODY Hiroshi Katschi +1 and Hitoshi Yamada + +1 Yokohama National University,

More information

Replacement of Einstein s Relativity Theory with a New One: Why the Second Postulate is Superfluous?

Replacement of Einstein s Relativity Theory with a New One: Why the Second Postulate is Superfluous? International Jornal of Physics, 16, Vol. 4, No. 5, 14-145 Available online at http://pbs.sciepb.com/ijp/4/5/5 Science and Edcation Pblishing DOI:1.1691/ijp-4-5-5 Replacement of Einstein s Relativity Theory

More information

Oscillation the vibration of an object. Wave a transfer of energy without a transfer of matter

Oscillation the vibration of an object. Wave a transfer of energy without a transfer of matter Oscillation the vibration of an object Wave a transfer of energy without a transfer of matter Equilibrium Position position of object at rest (mean position) Displacement (x) distance in a particular direction

More information

1. Tractable and Intractable Computational Problems So far in the course we have seen many problems that have polynomial-time solutions; that is, on

1. Tractable and Intractable Computational Problems So far in the course we have seen many problems that have polynomial-time solutions; that is, on . Tractable and Intractable Comptational Problems So far in the corse we have seen many problems that have polynomial-time soltions; that is, on a problem instance of size n, the rnning time T (n) = O(n

More information

Simplified Identification Scheme for Structures on a Flexible Base

Simplified Identification Scheme for Structures on a Flexible Base Simplified Identification Scheme for Strctres on a Flexible Base L.M. Star California State University, Long Beach G. Mylonais University of Patras, Greece J.P. Stewart University of California, Los Angeles

More information

Variability sustained pattern formation in subexcitable media

Variability sustained pattern formation in subexcitable media Variability sstained pattern formation in sbexcitable media Erik Glatt, Martin Gassel, and Friedemann Kaiser Institte of Applied Physics, Darmstadt University of Technology, 64289 Darmstadt, Germany (Dated:

More information

CONTENTS. INTRODUCTION MEQ curriculum objectives for vectors (8% of year). page 2 What is a vector? What is a scalar? page 3, 4

CONTENTS. INTRODUCTION MEQ curriculum objectives for vectors (8% of year). page 2 What is a vector? What is a scalar? page 3, 4 CONTENTS INTRODUCTION MEQ crriclm objectives for vectors (8% of year). page 2 What is a vector? What is a scalar? page 3, 4 VECTOR CONCEPTS FROM GEOMETRIC AND ALGEBRAIC PERSPECTIVES page 1 Representation

More information

Q1. A) 53.3 cm/s B) 59.8 cm/s C) 77.5 cm/s D) 35.1 cm/s E) 44.7 cm/s. Ans: 1.6 Q2.

Q1. A) 53.3 cm/s B) 59.8 cm/s C) 77.5 cm/s D) 35.1 cm/s E) 44.7 cm/s. Ans: 1.6 Q2. Coordinator: Dr. W. Al-Basheer Wednesday, July 11, 2018 Page: 1 Q1. A string of 80.0 cm length is fixed at both ends. The string oscillates in the fundamental mode with a frequency of 60.0 Hz and a maximum

More information

(Total 1 mark) IB Questionbank Physics 1

(Total 1 mark) IB Questionbank Physics 1 1. A transverse wave travels from left to right. The diagram below shows how, at a particular instant of time, the displacement of particles in the medium varies with position. Which arrow represents the

More information

Applying Laminar and Turbulent Flow and measuring Velocity Profile Using MATLAB

Applying Laminar and Turbulent Flow and measuring Velocity Profile Using MATLAB IOS Jornal of Mathematics (IOS-JM) e-issn: 78-578, p-issn: 319-765X. Volme 13, Isse 6 Ver. II (Nov. - Dec. 17), PP 5-59 www.iosrjornals.org Applying Laminar and Trblent Flow and measring Velocity Profile

More information

called the potential flow, and function φ is called the velocity potential.

called the potential flow, and function φ is called the velocity potential. J. Szantr Lectre No. 3 Potential flows 1 If the flid flow is irrotational, i.e. everwhere or almost everwhere in the field of flow there is rot 0 it means that there eists a scalar fnction ϕ,, z), sch

More information

Frequency Estimation, Multiple Stationary Nonsinusoidal Resonances With Trend 1

Frequency Estimation, Multiple Stationary Nonsinusoidal Resonances With Trend 1 Freqency Estimation, Mltiple Stationary Nonsinsoidal Resonances With Trend 1 G. Larry Bretthorst Department of Chemistry, Washington University, St. Lois MO 6313 Abstract. In this paper, we address the

More information

Chapter 6. Inverse Circular Functions and Trigonometric Equations. Section 6.1 Inverse Circular Functions y = 0

Chapter 6. Inverse Circular Functions and Trigonometric Equations. Section 6.1 Inverse Circular Functions y = 0 Chapter Inverse Circlar Fnctions and Trigonometric Eqations Section. Inverse Circlar Fnctions. onetoone. range. cos... = tan.. Sketch the reflection of the graph of f across the line =. 7. (a) [, ] é ù

More information

An Interpretation of the Black Energy in Universe by Using a Hydro-Dynamical Analogy with Newton Gravity

An Interpretation of the Black Energy in Universe by Using a Hydro-Dynamical Analogy with Newton Gravity An Interpretation of the Black nergy in Universe by Using a Hydro-Dynamical Analogy with Newton Gravity Corneli BRBNT*,1, Sorin BRBNT *Corresponding athor *,1 POLITHNICA University of Bcharest, Faclty

More information

10.2 Solving Quadratic Equations by Completing the Square

10.2 Solving Quadratic Equations by Completing the Square . Solving Qadratic Eqations b Completing the Sqare Consider the eqation ( ) We can see clearl that the soltions are However, What if the eqation was given to s in standard form, that is 6 How wold we go

More information

Pendulum Equations and Low Gain Regime

Pendulum Equations and Low Gain Regime WIR SCHAFFEN WISSEN HEUTE FÜR MORGEN Sven Reiche :: SwissFEL Beam Dynamics Grop :: Pal Scherrer Institte Pendlm Eqations and Low Gain Regime CERN Accelerator School FELs and ERLs Interaction with Radiation

More information

Geometric Image Manipulation. Lecture #4 Wednesday, January 24, 2018

Geometric Image Manipulation. Lecture #4 Wednesday, January 24, 2018 Geometric Image Maniplation Lectre 4 Wednesda, Janar 4, 08 Programming Assignment Image Maniplation: Contet To start with the obvios, an image is a D arra of piels Piel locations represent points on the

More information

VIBRATION MEASUREMENT UNCERTAINTY AND RELIABILITY DIAGNOSTICS RESULTS IN ROTATING SYSTEMS

VIBRATION MEASUREMENT UNCERTAINTY AND RELIABILITY DIAGNOSTICS RESULTS IN ROTATING SYSTEMS VIBRATIO MEASUREMET UCERTAITY AD RELIABILITY DIAGOSTICS RESULTS I ROTATIG SYSTEMS. Introdction M. Eidkevicite, V. Volkovas anas University of Technology, Lithania The rotating machinery technical state

More information

Using the Biot Savart Law: The Field of a Straight Wire

Using the Biot Savart Law: The Field of a Straight Wire Exective Editor: Nancy Whilton Project Manager: Katie Conley Development Editors: John Mrdzek, Matt Walker Editorial Assistant: arah Kabisch Development Manager: Cathy Mrphy Project Management Team Lead:

More information

Image and Multidimensional Signal Processing

Image and Multidimensional Signal Processing Image and Mltidimensional Signal Processing Professor William Hoff Dept of Electrical Engineering &Compter Science http://inside.mines.ed/~whoff/ Forier Transform Part : D discrete transforms 2 Overview

More information

The Heat Equation and the Li-Yau Harnack Inequality

The Heat Equation and the Li-Yau Harnack Inequality The Heat Eqation and the Li-Ya Harnack Ineqality Blake Hartley VIGRE Research Paper Abstract In this paper, we develop the necessary mathematics for nderstanding the Li-Ya Harnack ineqality. We begin with

More information

Technical Note. ODiSI-B Sensor Strain Gage Factor Uncertainty

Technical Note. ODiSI-B Sensor Strain Gage Factor Uncertainty Technical Note EN-FY160 Revision November 30, 016 ODiSI-B Sensor Strain Gage Factor Uncertainty Abstract Lna has pdated or strain sensor calibration tool to spport NIST-traceable measrements, to compte

More information

STEP Support Programme. STEP III Hyperbolic Functions: Solutions

STEP Support Programme. STEP III Hyperbolic Functions: Solutions STEP Spport Programme STEP III Hyperbolic Fnctions: Soltions Start by sing the sbstittion t cosh x. This gives: sinh x cosh a cosh x cosh a sinh x t sinh x dt t dt t + ln t ln t + ln cosh a ln ln cosh

More information

Numerical verification of the existence of localization of the elastic energy for closely spaced rigid disks

Numerical verification of the existence of localization of the elastic energy for closely spaced rigid disks Nmerical verification of the existence of localization of the elastic energy for closely spaced rigid disks S. I. Rakin Siberian State University of transport Rssia, 6349, Novosibirsk, Dsy Kovalchk street,

More information

Bayes and Naïve Bayes Classifiers CS434

Bayes and Naïve Bayes Classifiers CS434 Bayes and Naïve Bayes Classifiers CS434 In this lectre 1. Review some basic probability concepts 2. Introdce a sefl probabilistic rle - Bayes rle 3. Introdce the learning algorithm based on Bayes rle (ths

More information

Reflections on a mismatched transmission line Reflections.doc (4/1/00) Introduction The transmission line equations are given by

Reflections on a mismatched transmission line Reflections.doc (4/1/00) Introduction The transmission line equations are given by Reflections on a mismatched transmission line Reflections.doc (4/1/00) Introdction The transmission line eqations are given by, I z, t V z t l z t I z, t V z, t c z t (1) (2) Where, c is the per-nit-length

More information

-Electromagnetic. Waves - disturbance that propagates through space & time - usually with transfer of energy -Mechanical.

-Electromagnetic. Waves - disturbance that propagates through space & time - usually with transfer of energy -Mechanical. Waves Waves - disturbance that propagates through space & time - usually with transfer of energy -Mechanical requires a medium -Electromagnetic no medium required Mechanical waves: sound, water, seismic.

More information

Lecture Notes: Finite Element Analysis, J.E. Akin, Rice University

Lecture Notes: Finite Element Analysis, J.E. Akin, Rice University 9. TRUSS ANALYSIS... 1 9.1 PLANAR TRUSS... 1 9. SPACE TRUSS... 11 9.3 SUMMARY... 1 9.4 EXERCISES... 15 9. Trss analysis 9.1 Planar trss: The differential eqation for the eqilibrim of an elastic bar (above)

More information

08/26/09 PHYSICS 223 Exam-2 NAME Please write down your name also on the back side of this exam

08/26/09 PHYSICS 223 Exam-2 NAME Please write down your name also on the back side of this exam 08/6/09 PHYSICS 3 Exam- NAME Please write down your name also on the back side of this exam 1. The figure shows a container-a holding an ideal gas at pressure 3.0 x 10 5 N/m and a temperature of 300K.

More information

Uncertainty Evaluation of Toluene Determination in Room Air by Thermal Desorption Gas Chromatography

Uncertainty Evaluation of Toluene Determination in Room Air by Thermal Desorption Gas Chromatography International Conference on Civil, Transportation and Environment (ICCTE 06) ncertainty Evalation of Tolene Determination in Room Air by Thermal Desorption Gas Chromatography Xiaoyan Wen, a,yanhi Gao,

More information

10.1 Properties of Light

10.1 Properties of Light 10.1 Properties of Light Every time you see, you are using light. You can t see anything in complete darkness! Whether you are looking at a light bulb, or a car, or this book, light brings information

More information

Math 144 Activity #10 Applications of Vectors

Math 144 Activity #10 Applications of Vectors 144 p 1 Math 144 Actiity #10 Applications of Vectors In the last actiity, yo were introdced to ectors. In this actiity yo will look at some of the applications of ectors. Let the position ector = a, b

More information

Homework Book. Wave Properties. Huijia Physics Homework Book 1 Semester 2. Name: Homeroom: Physics Class:

Homework Book. Wave Properties. Huijia Physics Homework Book 1 Semester 2. Name: Homeroom: Physics Class: Homework Book Wave Properties Huijia Physics Homework Book 1 Semester 2 Name: Homeroom: Physics Class: Week 1 Reflection, Refraction, wave equations 1. If the wavelength of an incident wave is 1.5cm and

More information

Lab Manual for Engrd 202, Virtual Torsion Experiment. Aluminum module

Lab Manual for Engrd 202, Virtual Torsion Experiment. Aluminum module Lab Manal for Engrd 202, Virtal Torsion Experiment Alminm modle Introdction In this modle, o will perform data redction and analsis for circlar cross section alminm samples. B plotting the torqe vs. twist

More information

A Decomposition Method for Volume Flux. and Average Velocity of Thin Film Flow. of a Third Grade Fluid Down an Inclined Plane

A Decomposition Method for Volume Flux. and Average Velocity of Thin Film Flow. of a Third Grade Fluid Down an Inclined Plane Adv. Theor. Appl. Mech., Vol. 1, 8, no. 1, 9 A Decomposition Method for Volme Flx and Average Velocit of Thin Film Flow of a Third Grade Flid Down an Inclined Plane A. Sadighi, D.D. Ganji,. Sabzehmeidani

More information

Conceptual Questions. Problems. 852 CHAPTER 29 Magnetic Fields

Conceptual Questions. Problems. 852 CHAPTER 29 Magnetic Fields 852 CHAPTER 29 Magnetic Fields magnitde crrent, and the niform magnetic field points in the positive direction. Rank the loops by the magnitde of the torqe eerted on them by the field from largest to smallest.

More information

Sources of Non Stationarity in the Semivariogram

Sources of Non Stationarity in the Semivariogram Sorces of Non Stationarity in the Semivariogram Migel A. Cba and Oy Leangthong Traditional ncertainty characterization techniqes sch as Simple Kriging or Seqential Gassian Simlation rely on stationary

More information

PhysicsAndMathsTutor.com

PhysicsAndMathsTutor.com . Two smooth niform spheres S and T have eqal radii. The mass of S is 0. kg and the mass of T is 0.6 kg. The spheres are moving on a smooth horizontal plane and collide obliqely. Immediately before the

More information

Physics 202 Homework 7

Physics 202 Homework 7 Physics 202 Homework 7 May 15, 2013 1. On a cello, the string with the largest linear density (0.0156 kg/m) is the C 171 newtons string. This string produces a fundamental frequency of 65.4 Hz and has

More information