MATH Homework #1 Solution - by Ben Ong

Size: px
Start display at page:

Download "MATH Homework #1 Solution - by Ben Ong"

Transcription

1 MATH 46 - Homewok #1 Solution - by Ben Ong Deivation of the Eule Equations We pesent a fist pinciples deivation of the Eule Equations fo two-dimensional fluid flow in thee-dimensional cylndical cooodinates (, θ, z). We assume no vetical flow (u z = 0) and no vetical vaiations ( / z 0). We define u (, θ, t) and u θ (, θ, t) to be flow components in the ê and ê θ diections espectively. Consevation of mass tells us that the change of mass inside a contol volume has to equal the net flux of mass though the contol volume. The change in mass due to time vaiation in density and volume is given by ] ρ ρ(, θ, t + t) ρ(, θ, t) ( θ) z t ( θ) z (1) t Denoting the flux though sufaces with ê (, θ, z) and ê ( +, θ, z) nomal vectos as flux = ρ(, θ, t) ( u (, θ, t) t ) ( θ) z flux + = ρ( +, θ, t) ( u ( +, θ, t) t )( ( + ) θ ) z We see that the net flux in the ê is Similaly (net flux) (ρu ) t θ z () Thus and flux θ = ρ(, θ, t) ( u θ (, θ, t) t ) z flux θ+ θ = ρ(, θ + θ, t) ( u θ (, θ + θ, t) t ) z (net flux) θ (ρu θ) θ t z (3) θ (net flux) z 0 (4) Combining the fou above equations give the consevation of mass condition ρ t + 1 (ρu ) + 1 (ρu θ ) θ = 0 (5) 1

2 Newton s Law tells us that the net change in momentum is equal to the net impulse. The net change in momentum is affected by (i) momentum flux leaving though the contol volume, and though (ii) time vaiation in density and volume of the contol box. The momentum is given by the poduct of the momentum density and the volume. m(t) = ρ(, θ, t) u (, θ, t)ê (θ) + u θ (, θ, t)ê θ (θ) ]( ( θ) z ) m(t + t) = ρ(, θ, t + t) u (, θ, t + t)ê (θ) + u θ (, θ, t + t)ê θ (θ) ]( ( θ) z ) thus the contibution to the net change fom (ii) is m t { ρ ] } ( ) u ê + u θ ê θ t ( θ) z t (6) Denoting the flux though sufaces with ê (, θ, z) and ê ( +, θ, z) nomal vectos as m() = ρ(, θ, t) u (, θ, t)ê (θ) + u θ (, θ, t)ê θ (θ) ]( (u (, θ, t) t)( θ) z ) m( + ) = ρ( +, θ, t) u ( +, θ, t)ê (θ) + u θ ( +, θ, t)ê θ (θ) ] ( (u ( +, θ, t) t )( ( + ) θ ) z) Thus the net flux out of the two sufaces is appoximated by taking Similaly m( + ) m() lim 0 = m { ρu u ê + u θ ê θ ] } ( t θ z) (7) m(θ) = ρ(, θ, t) u (, θ, t)ê (θ) + u θ (, θ, t)ê θ (θ) ]( (u θ (, θ, t) t) z ) m(θ + θ) = ρ(, θ + θ, t) u (, θ + θ, t)ê (θ + θ) + u θ (, θ + θ, t)ê θ (θ + θ) ] ( (uθ (, θ + θ, t) t ) z) Fom vecto calculus, Substituting into m(θ + θ) gives ê (θ + θ) = ê (θ) + θê θ (θ) (8) ê θ (θ + θ) = ê θ (θ) θê (θ) (9) m(θ + θ) = ρ(, θ + θ, t) u (, θ + θ, t)(ê (θ) + θê θ (θ)) + u θ (, θ + θ, t)(ê θ (θ) θê (θ)) ] ( (uθ (, θ + θ, t) t ) z)

3 Thus m(θ + θ) m(θ) t z = ρ(, θ + θ, t)u (, θ + θ, t)u θ (, θ + θ, t) ρ(, θ, t)u (, θ, t)u θ ((, θ, t) ] ê + ρ(, θ + θ, t)u θ (, θ + θ, t)u θ (, θ + θ, t) ρ(, θ, t)u θ (, θ, t)u θ ((, θ, t) ] ê θ + ρ(, θ + θ, t)u (, θ + θ, t)u θ (, θ + θ, t) ] θê θ ρ(, θ + θ, t)u θ (, θ + θ, t)u θ (, θ + θ, t) ] θê m(θ+ θ) m(θ) Dividing both sides by θ and taking lim θ 0 gives θ { m θ ρuθ (u ê + u θ ê θ ) } ] + ρu θ (u ê θ u θ ê ) t z θ (10) θ Combining equations (6), (7) and (10) gives the net change in momentum t {ρu } + {ρu u } + ] θ {ρu u θ } ρu θ ( θ z t)ê + t {ρu θ} + {ρu θu } + θ ] {ρu θu θ } + ρu u θ ( θ z t)ê θ (11) If you expand the deivatives, and impose consevation of mass (equation (5)), the net change in momentum simplifies to (djm: the two exta tems come fom the CV geomety (8) & (9)) ρ u t u + ρu + 1 ρu θ + ρ u θ t + ρu u θ ρu θ ] ( θ z t)ê u θ + 1 ρu u θ θ θ + ρu u θ ] ( θ z t)ê θ (1) We now need to calculate the net impulse on the system in ode to deive the emaining Eule Equations. Thee ae two contibutions; (i) Fom a given body foce density F (, θ, t) = F (, θ, t)ê + F θ (, θ, t)ê θ + F z (, θ, t)ê z and (ii) fom the intenal pessue. The impulse contibution fom (i) is simply the foce density*volume* t. F (, θ, t) = (F (, θ, t)ê + F θ (, θ, t)ê θ + F z (, θ, t)ê z )( θ z) t (13) 3

4 The foce = (pessue*aea) exeted on the sufaces with ê (, θ, z) and ê ( +, θ, z) nomal vectos is F P = P (, θ, t) ( θ) z ] ê (θ) F + P = P ( +, θ, t) ( + ) θ z ] ê (θ) Thus, the net foce contibution fom the two sufaces Similaly Using equation (9) gives {F P } {P } θ z]ê (θ) P ] + P θ z]ê (θ) (14) F θ P = P (, θ, t) z ] ê θ (θ) F θ+ θ P = P (, θ + θ, t) z ] ê θ (θ + θ) F θ+ θ P = P (, θ + θ, t) z ] (ê θ (θ) θê (θ)) Thus, the contibution fom the two sufaces gives ] P {F P } θ θ êθ(θ) P ê (θ) z θ (15) And the contibution fom sufaces with ê z as nomals is {F P } z 0 (16) Thus the net impulse is (djm: note the amazing cancellation of the non-gadient P tem) F ê + F θ ê θ + F z ê z + P ê + 1 P ] θ êθ θ z t (17) Combining equations (1) and (17) gives us Newton s Law u (ê ) t + u u + u θ u θ u θ = 1 P ] ρ + F (18) u θ (ê θ ) t + u u θ + u θ u θ θ + u u θ = 1 1 ] P ρ θ + F θ (19) (ê z ) 0 = F z (imposes condition on body foce) (0) 4

5 Rotational Flows Given u = ( Ωy, Ωx, 0), find the pessue which poduces a flow solution to the incompessible Eule Equations with F = ρgẑ Incompessible Eule Equations u = 0 (1) u t + ( u ) u P = We notice that equation (1) is automatically satisfied. Expanding () Substituting u = ( Ωy, Ωx, 0), we get Solving (3) gives u t + (uu x + vu y + wu z ) = P x v t + (uv x + vv y + wv z ) = P y w t + (uw x + vw y + ww z ) = P z g + F () Ω x = P x (3) Ω y = P y (4) P z = g (5) P = Ω x + f(y, z) (6) Diffeentiating (6) and compaing with (4) gives Solving (7) gives P y = f (y, z) = Ω y (7) P = Ω (x + y ) + g(z) (8) Diffeentiating (8) and compaing with (5) and solving gives P = Ω (x + y ) gz + constant (9) 5

6 djm:] Since the fluid has voticity, u = (0, 0, Ω) 0, the Benoulli theoem fo iotational flow does not apply. Howeve, the flow is steady and so the Benouilli theoem fo steamlines does apply, but the Benouilli function can have diffeent constant values on diffeent steamlines (cicles aound the axis of otation) and cannot be used to infe the suface geomety. An astonome could make a liquid mio telescope by spinning mecuy on a a paabolic suface. Actually, this is being done at a UBC eseach station in maple Ridge; they have a 6m diamete mio! They need the coect angula velocity to get a unifom coating of the mecuy 6

Classical Mechanics Homework set 7, due Nov 8th: Solutions

Classical Mechanics Homework set 7, due Nov 8th: Solutions Classical Mechanics Homewok set 7, due Nov 8th: Solutions 1. Do deivation 8.. It has been asked what effect does a total deivative as a function of q i, t have on the Hamiltonian. Thus, lets us begin with

More information

Final Review of AerE 243 Class

Final Review of AerE 243 Class Final Review of AeE 4 Class Content of Aeodynamics I I Chapte : Review of Multivaiable Calculus Chapte : Review of Vectos Chapte : Review of Fluid Mechanics Chapte 4: Consevation Equations Chapte 5: Simplifications

More information

Exercise 4: Adimensional form and Rankine vortex. Example 1: adimensional form of governing equations

Exercise 4: Adimensional form and Rankine vortex. Example 1: adimensional form of governing equations Fluid Mechanics, SG4, HT9 Septembe, 9 Execise 4: Adimensional fom and Rankine votex Example : adimensional fom of govening equations Calculating the two-dimensional flow aound a cylinde (adius a, located

More information

Stress, Cauchy s equation and the Navier-Stokes equations

Stress, Cauchy s equation and the Navier-Stokes equations Chapte 3 Stess, Cauchy s equation and the Navie-Stokes equations 3. The concept of taction/stess Conside the volume of fluid shown in the left half of Fig. 3.. The volume of fluid is subjected to distibuted

More information

2.25 Advanced Fluid Mechanics

2.25 Advanced Fluid Mechanics MIT Depatment of Mechanical Engineeing 2.25 Advanced Fluid Mechanics Poblem 4.27 This poblem is fom Advanced Fluid Mechanics Poblems by A.H. Shapio and A.A. Sonin u(,t) pg Gas Liquid, density Conside a

More information

Superposition. Section 8.5.3

Superposition. Section 8.5.3 Supeposition Section 8.5.3 Simple Potential Flows Most complex potential (invicid, iotational) flows can be modeled using a combination of simple potential flows The simple flows used ae: Unifom flows

More information

is the instantaneous position vector of any grid point or fluid

is the instantaneous position vector of any grid point or fluid Absolute inetial, elative inetial and non-inetial coodinates fo a moving but non-defoming contol volume Tao Xing, Pablo Caica, and Fed Sten bjective Deive and coelate the govening equations of motion in

More information

ME 425: Aerodynamics

ME 425: Aerodynamics ME 5: Aeodynamics D ABM Toufique Hasan Pofesso Depatment of Mechanical Engineeing, BUET Lectue- 8 Apil 7 teachebuetacbd/toufiquehasan/ toufiquehasan@mebuetacbd ME5: Aeodynamics (Jan 7) Flow ove a stationay

More information

Do not turn over until you are told to do so by the Invigilator.

Do not turn over until you are told to do so by the Invigilator. UNIVERSITY OF EAST ANGLIA School of Mathematics Main Seies UG Examination 2015 16 FLUID DYNAMICS WITH ADVANCED TOPICS MTH-MD59 Time allowed: 3 Hous Attempt QUESTIONS 1 and 2, and THREE othe questions.

More information

06 - ROTATIONAL MOTION Page 1 ( Answers at the end of all questions )

06 - ROTATIONAL MOTION Page 1 ( Answers at the end of all questions ) 06 - ROTATIONAL MOTION Page ) A body A of mass M while falling vetically downwads unde gavity beaks into two pats, a body B of mass ( / ) M and a body C of mass ( / ) M. The cente of mass of bodies B and

More information

Applied Aerodynamics

Applied Aerodynamics Applied Aeodynamics Def: Mach Numbe (M), M a atio of flow velocity to the speed of sound Compessibility Effects Def: eynolds Numbe (e), e ρ c µ atio of inetial foces to viscous foces iscous Effects If

More information

A 1. EN2210: Continuum Mechanics. Homework 7: Fluid Mechanics Solutions

A 1. EN2210: Continuum Mechanics. Homework 7: Fluid Mechanics Solutions EN10: Continuum Mechanics Homewok 7: Fluid Mechanics Solutions School of Engineeing Bown Univesity 1. An ideal fluid with mass density ρ flows with velocity v 0 though a cylindical tube with cosssectional

More information

Physics Fall Mechanics, Thermodynamics, Waves, Fluids. Lecture 6: motion in two and three dimensions III. Slide 6-1

Physics Fall Mechanics, Thermodynamics, Waves, Fluids. Lecture 6: motion in two and three dimensions III. Slide 6-1 Physics 1501 Fall 2008 Mechanics, Themodynamics, Waves, Fluids Lectue 6: motion in two and thee dimensions III Slide 6-1 Recap: elative motion An object moves with velocity v elative to one fame of efeence.

More information

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion AH Mechanics Checklist (Unit ) AH Mechanics Checklist (Unit ) Cicula Motion No. kill Done 1 Know that cicula motion efes to motion in a cicle of constant adius Know that cicula motion is conveniently descibed

More information

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum 2. Electostatics D. Rakhesh Singh Kshetimayum 1 2.1 Intoduction In this chapte, we will study how to find the electostatic fields fo vaious cases? fo symmetic known chage distibution fo un-symmetic known

More information

(read nabla or del) is defined by, k. (9.7.1*)

(read nabla or del) is defined by, k. (9.7.1*) 9.7 Gadient of a scala field. Diectional deivative Some of the vecto fields in applications can be obtained fom scala fields. This is vey advantageous because scala fields can be handled moe easily. The

More information

Chapter 13 Gravitation

Chapter 13 Gravitation Chapte 13 Gavitation In this chapte we will exploe the following topics: -Newton s law of gavitation, which descibes the attactive foce between two point masses and its application to extended objects

More information

Water Tunnel Experiment MAE 171A/175A. Objective:

Water Tunnel Experiment MAE 171A/175A. Objective: Wate Tunnel Expeiment MAE 7A/75A Objective: Measuement of te Dag Coefficient of a Cylinde Measuement Tecniques Pessue Distibution on Cylinde Dag fom Momentum Loss Measued in Wake it lase Dopple Velocimety

More information

KEPLER S LAWS OF PLANETARY MOTION

KEPLER S LAWS OF PLANETARY MOTION EPER S AWS OF PANETARY MOTION 1. Intoduction We ae now in a position to apply what we have leaned about the coss poduct and vecto valued functions to deive eple s aws of planetay motion. These laws wee

More information

Between any two masses, there exists a mutual attractive force.

Between any two masses, there exists a mutual attractive force. YEAR 12 PHYSICS: GRAVITATION PAST EXAM QUESTIONS Name: QUESTION 1 (1995 EXAM) (a) State Newton s Univesal Law of Gavitation in wods Between any two masses, thee exists a mutual attactive foce. This foce

More information

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3.

As is natural, our Aerospace Structures will be described in a Euclidean three-dimensional space R 3. Appendix A Vecto Algeba As is natual, ou Aeospace Stuctues will be descibed in a Euclidean thee-dimensional space R 3. A.1 Vectos A vecto is used to epesent quantities that have both magnitude and diection.

More information

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j.

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j. 7. We denote the two foces F A + F B = ma,sof B = ma F A. (a) In unit vecto notation F A = ( 20.0 N)ˆ i and Theefoe, Phys 201A Homewok 6 Solutions F A and F B. Accoding to Newton s second law, a = [ (

More information

π(x, y) = u x + v y = V (x cos + y sin ) κ(x, y) = u y v x = V (y cos x sin ) v u x y

π(x, y) = u x + v y = V (x cos + y sin ) κ(x, y) = u y v x = V (y cos x sin ) v u x y F17 Lectue Notes 1. Unifom flow, Souces, Sinks, Doublets Reading: Andeson 3.9 3.12 Unifom Flow Definition A unifom flow consists of a velocit field whee V φ = uî + vθˆ is a constant. In 2-D, this velocit

More information

Sections and Chapter 10

Sections and Chapter 10 Cicula and Rotational Motion Sections 5.-5.5 and Chapte 10 Basic Definitions Unifom Cicula Motion Unifom cicula motion efes to the motion of a paticle in a cicula path at constant speed. The instantaneous

More information

= 4 3 π( m) 3 (5480 kg m 3 ) = kg.

= 4 3 π( m) 3 (5480 kg m 3 ) = kg. CHAPTER 11 THE GRAVITATIONAL FIELD Newton s Law of Gavitation m 1 m A foce of attaction occus between two masses given by Newton s Law of Gavitation Inetial mass and gavitational mass Gavitational potential

More information

PHZ 3113 Fall 2017 Homework #5, Due Friday, October 13

PHZ 3113 Fall 2017 Homework #5, Due Friday, October 13 PHZ 3113 Fall 2017 Homewok #5, Due Fiday, Octobe 13 1. Genealize the poduct ule (fg) = f g +f g to wite the divegence Ö (Ù Ú) of the coss poduct of the vecto fields Ù and Ú in tems of the cul of Ù and

More information

EGN 3353C Fluid Mechanics

EGN 3353C Fluid Mechanics Lectue Look at V ρv na at inlet: only component is in x iection: ( ( ρ u ˆ ˆ ˆ ˆ in, avgi uin, avgi Aini uin, avgmi ρu A m in, avg in at exit: only component is in z iection: ( ( ρ w ˆ ˆ ˆ ˆ out, avgk

More information

PROBLEM SET 5. SOLUTIONS March 16, 2004

PROBLEM SET 5. SOLUTIONS March 16, 2004 Havad-MIT ivision of Health Sciences and Technology HST.54J: Quantitative Physiology: Ogan Tanspot Systems Instuctos: Roge Mak and Jose Venegas MASSACHUSETTS INSTITUTE OF TECHNOLOGY epatments of Electical

More information

Physics 235 Chapter 5. Chapter 5 Gravitation

Physics 235 Chapter 5. Chapter 5 Gravitation Chapte 5 Gavitation In this Chapte we will eview the popeties of the gavitational foce. The gavitational foce has been discussed in geat detail in you intoductoy physics couses, and we will pimaily focus

More information

Math Notes on Kepler s first law 1. r(t) kp(t)

Math Notes on Kepler s first law 1. r(t) kp(t) Math 7 - Notes on Keple s fist law Planetay motion and Keple s Laws We conside the motion of a single planet about the sun; fo simplicity, we assign coodinates in R 3 so that the position of the sun is

More information

AE301 Aerodynamics I UNIT B: Theory of Aerodynamics

AE301 Aerodynamics I UNIT B: Theory of Aerodynamics AE301 Aeodynamics I UNIT B: Theoy of Aeodynamics ROAD MAP... B-1: Mathematics fo Aeodynamics B-2: Flow Field Repesentations B-3: Potential Flow Analysis B-4: Applications of Potential Flow Analysis AE301

More information

Three dimensional flow analysis in Axial Flow Compressors

Three dimensional flow analysis in Axial Flow Compressors 1 Thee dimensional flow analysis in Axial Flow Compessos 2 The ealie assumption on blade flow theoies that the flow inside the axial flow compesso annulus is two dimensional means that adial movement of

More information

Balanced Flow. Natural Coordinates

Balanced Flow. Natural Coordinates Balanced Flow The pessue and velocity distibutions in atmospheic systems ae elated by elatively simple, appoximate foce balances. We can gain a qualitative undestanding by consideing steady-state conditions,

More information

Fluid flow in curved geometries: Mathematical Modeling and Applications

Fluid flow in curved geometries: Mathematical Modeling and Applications Fluid flow in cuved geometies: Mathematical Modeling and Applications D. Muhammad Sajid Theoetical Plasma Physics Division PINSTECH, P.O. Niloe, PAEC, Islamabad Mach 01-06, 010 Islamabad, Paistan Pesentation

More information

PROBLEM SET #3A. A = Ω 2r 2 2 Ω 1r 2 1 r2 2 r2 1

PROBLEM SET #3A. A = Ω 2r 2 2 Ω 1r 2 1 r2 2 r2 1 PROBLEM SET #3A AST242 Figue 1. Two concentic co-axial cylindes each otating at a diffeent angula otation ate. A viscous fluid lies between the two cylindes. 1. Couette Flow A viscous fluid lies in the

More information

Physics 2212 GH Quiz #2 Solutions Spring 2016

Physics 2212 GH Quiz #2 Solutions Spring 2016 Physics 2212 GH Quiz #2 Solutions Sping 216 I. 17 points) Thee point chages, each caying a chage Q = +6. nc, ae placed on an equilateal tiangle of side length = 3. mm. An additional point chage, caying

More information

EELE 3331 Electromagnetic I Chapter 4. Electrostatic fields. Islamic University of Gaza Electrical Engineering Department Dr.

EELE 3331 Electromagnetic I Chapter 4. Electrostatic fields. Islamic University of Gaza Electrical Engineering Department Dr. EELE 3331 Electomagnetic I Chapte 4 Electostatic fields Islamic Univesity of Gaza Electical Engineeing Depatment D. Talal Skaik 212 1 Electic Potential The Gavitational Analogy Moving an object upwad against

More information

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e.,

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e., Stella elaxation Time [Chandasekha 1960, Pinciples of Stella Dynamics, Chap II] [Ostike & Davidson 1968, Ap.J., 151, 679] Do stas eve collide? Ae inteactions between stas (as opposed to the geneal system

More information

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018 Rigid Body Dynamics 2 CSE169: Compute Animation nstucto: Steve Rotenbeg UCSD, Winte 2018 Coss Poduct & Hat Opeato Deivative of a Rotating Vecto Let s say that vecto is otating aound the oigin, maintaining

More information

Physics 1114: Unit 5 Hand-out Homework (Answers)

Physics 1114: Unit 5 Hand-out Homework (Answers) Physics 1114: Unit 5 Hand-out Homewok (Answes) Poblem set 1 1. The flywheel on an expeimental bus is otating at 420 RPM (evolutions pe minute). To find (a) the angula velocity in ad/s (adians/second),

More information

Phases of Matter. Since liquids and gases are able to flow, they are called fluids. Compressible? Able to Flow? shape?

Phases of Matter. Since liquids and gases are able to flow, they are called fluids. Compressible? Able to Flow? shape? Fluids Chapte 3 Lectue Sequence. Pessue (Sections -3). Mechanical Popeties (Sections 5, and 7) 3. Gauge Pessue (Sections 4, and 6) 4. Moving Fluids (Sections 8-0) Pessue Phases of Matte Phase Retains its

More information

Magnetic Field. Conference 6. Physics 102 General Physics II

Magnetic Field. Conference 6. Physics 102 General Physics II Physics 102 Confeence 6 Magnetic Field Confeence 6 Physics 102 Geneal Physics II Monday, Mach 3d, 2014 6.1 Quiz Poblem 6.1 Think about the magnetic field associated with an infinite, cuent caying wie.

More information

Wind Tunnel Experiment MAE 171A/175A. Objective:

Wind Tunnel Experiment MAE 171A/175A. Objective: Wind Tunnel Exeiment MAE 7A/75A Objective: Measue te Aeodynamic Foces and Moments of a Clak Y-4 Aifoil Unde Subsonic Flo Conditions Measuement Tecniques Pessue Distibution on Aifoil Dag fom Momentum Loss

More information

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law AY 7A - Fall 00 Section Woksheet - Solutions Enegy and Keple s Law. Escape Velocity (a) A planet is obiting aound a sta. What is the total obital enegy of the planet? (i.e. Total Enegy = Potential Enegy

More information

F 12. = G m m 1 2 F 21 = F 12. = G m 1m 2. Review. Physics 201, Lecture 22. Newton s Law Of Universal Gravitation

F 12. = G m m 1 2 F 21 = F 12. = G m 1m 2. Review. Physics 201, Lecture 22. Newton s Law Of Universal Gravitation Physics 201, Lectue 22 Review Today s Topics n Univesal Gavitation (Chapte 13.1-13.3) n Newton s Law of Univesal Gavitation n Popeties of Gavitational Foce n Planet Obits; Keple s Laws by Newton s Law

More information

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session.

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session. - 5 - TEST 1R This is the epeat vesion of TEST 1, which was held duing Session. This epeat test should be attempted by those students who missed Test 1, o who wish to impove thei mak in Test 1. IF YOU

More information

6.4 Period and Frequency for Uniform Circular Motion

6.4 Period and Frequency for Uniform Circular Motion 6.4 Peiod and Fequency fo Unifom Cicula Motion If the object is constained to move in a cicle and the total tangential foce acting on the total object is zeo, F θ = 0, then (Newton s Second Law), the tangential

More information

1.2 Differential cross section

1.2 Differential cross section .2. DIFFERENTIAL CROSS SECTION Febuay 9, 205 Lectue VIII.2 Diffeential coss section We found that the solution to the Schodinge equation has the fom e ik x ψ 2π 3/2 fk, k + e ik x and that fk, k = 2 m

More information

1 Fundamental Solutions to the Wave Equation

1 Fundamental Solutions to the Wave Equation 1 Fundamental Solutions to the Wave Equation Physical insight in the sound geneation mechanism can be gained by consideing simple analytical solutions to the wave equation. One example is to conside acoustic

More information

Exercise sheet 8 (Modeling large- and small-scale flows) 8.1 Volcanic ash from the Eyjafjallajökull

Exercise sheet 8 (Modeling large- and small-scale flows) 8.1 Volcanic ash from the Eyjafjallajökull Execise sheet 8 (Modeling lage- and small-scale flows) last edited June 18, 2018 These lectue notes ae based on textbooks by White [13], Çengel & al.[16], and Munson & al.[18]. Except othewise indicated,

More information

Math 124B February 02, 2012

Math 124B February 02, 2012 Math 24B Febuay 02, 202 Vikto Gigoyan 8 Laplace s equation: popeties We have aleady encounteed Laplace s equation in the context of stationay heat conduction and wave phenomena. Recall that in two spatial

More information

/6/4 5 Stuctue-Induced Sediment Scou ef: Eosion and Sedimentation, P.Y. Julien, 998 The Mechanics of Scou in the Maine Envionment, B.M. Sume and J. Fedsoe, Evaluating Scou at Bidges (HEC-8), E.. ichadson

More information

Uniform Circular Motion

Uniform Circular Motion Unifom Cicula Motion Intoduction Ealie we defined acceleation as being the change in velocity with time: a = v t Until now we have only talked about changes in the magnitude of the acceleation: the speeding

More information

Physics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G =

Physics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G = ics Announcements day, embe 9, 004 Ch 1: Gavity Univesal Law Potential Enegy Keple s Laws Ch 15: Fluids density hydostatic equilibium Pascal s Pinciple This week s lab will be anothe physics wokshop -

More information

Is there a magnification paradox in gravitational lensing?

Is there a magnification paradox in gravitational lensing? Is thee a magnification paadox in gavitational ing? Olaf Wucknitz wucknitz@asto.uni-bonn.de Astophysics semina/colloquium, Potsdam, 6 Novembe 7 Is thee a magnification paadox in gavitational ing? gavitational

More information

Institute of Fundamental Sciences-Mathematics,Massey University, Palmerston North,NZ

Institute of Fundamental Sciences-Mathematics,Massey University, Palmerston North,NZ Poceedings20th NZ Geothemal Wokshop 1998 FLUID FLOW A FLASHING CYCLONE SEPARATOR Institute of Fundamental SciencesMathematics,Massey Univesity, Palmeston Noth,NZ SUMMARY In geothemal steamgatheingsystems

More information

Chapter 12. Kinetics of Particles: Newton s Second Law

Chapter 12. Kinetics of Particles: Newton s Second Law Chapte 1. Kinetics of Paticles: Newton s Second Law Intoduction Newton s Second Law of Motion Linea Momentum of a Paticle Systems of Units Equations of Motion Dynamic Equilibium Angula Momentum of a Paticle

More information

Physics 107 TUTORIAL ASSIGNMENT #8

Physics 107 TUTORIAL ASSIGNMENT #8 Physics 07 TUTORIAL ASSIGNMENT #8 Cutnell & Johnson, 7 th edition Chapte 8: Poblems 5,, 3, 39, 76 Chapte 9: Poblems 9, 0, 4, 5, 6 Chapte 8 5 Inteactive Solution 8.5 povides a model fo solving this type

More information

2.25 Advanced Fluid Mechanics

2.25 Advanced Fluid Mechanics MIT Depatment of Mechanical Engineeing.5 Advanced Fluid Mechanics Poblem 6.1 This poblem is fom Advanced Fluid Mechanics Poblems by A.H. Shapio and A.A. Sonin The sketch shows a cicula beaing pad which

More information

Lab 10: Newton s Second Law in Rotation

Lab 10: Newton s Second Law in Rotation Lab 10: Newton s Second Law in Rotation We can descibe the motion of objects that otate (i.e. spin on an axis, like a popelle o a doo) using the same definitions, adapted fo otational motion, that we have

More information

Analysis of the Dynamical Equations Chapter 2. Paul A. Ullrich

Analysis of the Dynamical Equations Chapter 2. Paul A. Ullrich Analysis of the Dynamical Equations Chapte 2 Paul A. Ullich paullich@ucdavis.edu Pat 1: Scale Analysis of the Momentum Equation The Atmospheic Equations Du uv tan Dv + u2 tan Dw c p DT + uw = 1 cos + vw

More information

Gravitation. Chapter 12. PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman. Lectures by James Pazun

Gravitation. Chapter 12. PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman. Lectures by James Pazun Chapte 12 Gavitation PowePoint Lectues fo Univesity Physics, Twelfth Edition Hugh D. Young and Roge A. Feedman Lectues by James Pazun Modified by P. Lam 5_31_2012 Goals fo Chapte 12 To study Newton s Law

More information

Force can be exerted by direct contact between bodies: Contact Force.

Force can be exerted by direct contact between bodies: Contact Force. Chapte 4, Newton s Laws of Motion Chapte IV NEWTON S LAWS OF MOTION Study of Dynamics: cause of motion (foces) and the esistance of objects to motion (mass), also called inetia. The fundamental Pinciples

More information

PHYSICS NOTES GRAVITATION

PHYSICS NOTES GRAVITATION GRAVITATION Newton s law of gavitation The law states that evey paticle of matte in the univese attacts evey othe paticle with a foce which is diectly popotional to the poduct of thei masses and invesely

More information

3-7 FLUIDS IN RIGID-BODY MOTION

3-7 FLUIDS IN RIGID-BODY MOTION 3-7 FLUIDS IN IGID-BODY MOTION S-1 3-7 FLUIDS IN IGID-BODY MOTION We ae almost eady to bein studyin fluids in motion (statin in Chapte 4), but fist thee is one cateoy of fluid motion that can be studied

More information

Transformation of the Navier-Stokes Equations in Curvilinear Coordinate Systems with Maple

Transformation of the Navier-Stokes Equations in Curvilinear Coordinate Systems with Maple Global Jounal of Pue and Applied Mathematics. ISSN 0973-1768 Volume 12, Numbe 4 2016, pp. 3315 3325 Reseach India Publications http://www.ipublication.com/gjpam.htm Tansfomation of the Navie-Stokes Equations

More information

Chapter 7-8 Rotational Motion

Chapter 7-8 Rotational Motion Chapte 7-8 Rotational Motion What is a Rigid Body? Rotational Kinematics Angula Velocity ω and Acceleation α Unifom Rotational Motion: Kinematics Unifom Cicula Motion: Kinematics and Dynamics The Toque,

More information

EM Boundary Value Problems

EM Boundary Value Problems EM Bounday Value Poblems 10/ 9 11/ By Ilekta chistidi & Lee, Seung-Hyun A. Geneal Desciption : Maxwell Equations & Loentz Foce We want to find the equations of motion of chaged paticles. The way to do

More information

PS113 Chapter 5 Dynamics of Uniform Circular Motion

PS113 Chapter 5 Dynamics of Uniform Circular Motion PS113 Chapte 5 Dynamics of Unifom Cicula Motion 1 Unifom cicula motion Unifom cicula motion is the motion of an object taveling at a constant (unifom) speed on a cicula path. The peiod T is the time equied

More information

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE VISUAL PHYSICS ONLIN MODUL 5 ADVANCD MCHANICS GRAVITATIONAL FILD: MOTION OF PLANTS AND SATLLITS SATLLITS: Obital motion of object of mass m about a massive object of mass M (m

More information

A Method of Solving Compressible Navier Stokes Equations in Cylindrical Coordinates Using Geometric Algebra

A Method of Solving Compressible Navier Stokes Equations in Cylindrical Coordinates Using Geometric Algebra Pepints www.pepints.og NOT PEER-REVIEWED Posted: 8 Decembe 08 Aticle A Method of Solving ompessible Navie Stokes Equations in ylindical oodinates Using Geometic Algeba Tey E. Moschandeou,, * London Intenational

More information

= 1. For a hyperbolic orbit with an attractive inverse square force, the polar equation with origin at the center of attraction is

= 1. For a hyperbolic orbit with an attractive inverse square force, the polar equation with origin at the center of attraction is 15. Kepleian Obits Michael Fowle Peliminay: Pola Equations fo Conic Section Cuves As we shall find, Newton s equations fo paticle motion in an invese-squae cental foce give obits that ae conic section

More information

Flux. Area Vector. Flux of Electric Field. Gauss s Law

Flux. Area Vector. Flux of Electric Field. Gauss s Law Gauss s Law Flux Flux in Physics is used to two distinct ways. The fist meaning is the ate of flow, such as the amount of wate flowing in a ive, i.e. volume pe unit aea pe unit time. O, fo light, it is

More information

m1 m2 M 2 = M -1 L 3 T -2

m1 m2 M 2 = M -1 L 3 T -2 GAVITATION Newton s Univesal law of gavitation. Evey paticle of matte in this univese attacts evey othe paticle with a foce which vaies diectly as the poduct of thei masses and invesely as the squae of

More information

Fall 2016 Semester METR 3113 Atmospheric Dynamics I: Introduction to Atmospheric Kinematics and Dynamics

Fall 2016 Semester METR 3113 Atmospheric Dynamics I: Introduction to Atmospheric Kinematics and Dynamics Fall 06 Semeste METR 33 Atmospheic Dynamics I: Intoduction to Atmospheic Kinematics Dynamics Lectue 7 Octobe 3 06 Topics: Scale analysis of the equations of hoizontal motion Geostophic appoximation eostophic

More information

Section 26 The Laws of Rotational Motion

Section 26 The Laws of Rotational Motion Physics 24A Class Notes Section 26 The Laws of otational Motion What do objects do and why do they do it? They otate and we have established the quantities needed to descibe this motion. We now need to

More information

3D-Central Force Problems I

3D-Central Force Problems I 5.73 Lectue #1 1-1 Roadmap 1. define adial momentum 3D-Cental Foce Poblems I Read: C-TDL, pages 643-660 fo next lectue. All -Body, 3-D poblems can be educed to * a -D angula pat that is exactly and univesally

More information

Physics 506 Winter 2006 Homework Assignment #9 Solutions

Physics 506 Winter 2006 Homework Assignment #9 Solutions Physics 506 Winte 2006 Homewok Assignment #9 Solutions Textbook poblems: Ch. 12: 12.2, 12.9, 12.13, 12.14 12.2 a) Show fom Hamilton s pinciple that Lagangians that diffe only by a total time deivative

More information

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased PHYS 0B - HW #7 Sping 2004, Solutions by David Pace Any efeenced euations ae fom Giffiths Poblem statements ae paaphased. Poblem 0.3 fom Giffiths A point chage,, moves in a loop of adius a. At time t 0

More information

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces.

F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces. 4.8. Cental foces The most inteesting poblems in classical mechanics ae about cental foces. Definition of a cental foce: (i) the diection of the foce F() is paallel o antipaallel to ; in othe wods, fo

More information

2 Governing Equations

2 Governing Equations 2 Govening Equations This chapte develops the govening equations of motion fo a homogeneous isotopic elastic solid, using the linea thee-dimensional theoy of elasticity in cylindical coodinates. At fist,

More information

Physics 2001 Problem Set 5 Solutions

Physics 2001 Problem Set 5 Solutions Physics 2001 Poblem Set 5 Solutions Jeff Kissel Octobe 16, 2006 1. A puck attached to a sting undegoes cicula motion on an ai table. If the sting beaks at the point indicated in the figue, which path (A,

More information

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once.

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once. Honos Physics Fall, 2016 Cicula Motion & Toque Test Review Name: M. Leonad Instuctions: Complete the following woksheet. SHOW ALL OF YOUR WORK ON A SEPARATE SHEET OF PAPER. 1. Detemine whethe each statement

More information

3. Magnetostatic fields

3. Magnetostatic fields 3. Magnetostatic fields D. Rakhesh Singh Kshetimayum 1 Electomagnetic Field Theoy by R. S. Kshetimayum 3.1 Intoduction to electic cuents Electic cuents Ohm s law Kichoff s law Joule s law Bounday conditions

More information

1. A stone falls from a platform 18 m high. When will it hit the ground? (a) 1.74 s (b) 1.83 s (c) 1.92 s (d) 2.01 s

1. A stone falls from a platform 18 m high. When will it hit the ground? (a) 1.74 s (b) 1.83 s (c) 1.92 s (d) 2.01 s 1. A stone falls fom a platfom 18 m high. When will it hit the gound? (a) 1.74 s (b) 1.83 s (c) 1.9 s (d).01 s Constant acceleation D = v 0 t + ½ a t. Which, if any, of these foces causes the otation of

More information

Name. Date. Period. Engage Examine the pictures on the left. 1. What is going on in these pictures?

Name. Date. Period. Engage Examine the pictures on the left. 1. What is going on in these pictures? AP Physics 1 Lesson 9.a Unifom Cicula Motion Outcomes 1. Define unifom cicula motion. 2. Detemine the tangential velocity of an object moving with unifom cicula motion. 3. Detemine the centipetal acceleation

More information

Pendulum in Orbit. Kirk T. McDonald Joseph Henry Laboratories, Princeton University, Princeton, NJ (December 1, 2017)

Pendulum in Orbit. Kirk T. McDonald Joseph Henry Laboratories, Princeton University, Princeton, NJ (December 1, 2017) 1 Poblem Pendulum in Obit Kik T. McDonald Joseph Heny Laboatoies, Pinceton Univesity, Pinceton, NJ 08544 (Decembe 1, 2017) Discuss the fequency of small oscillations of a simple pendulum in obit, say,

More information

ECE 3318 Applied Electricity and Magnetism. Spring Prof. David R. Jackson ECE Dept. Notes 13

ECE 3318 Applied Electricity and Magnetism. Spring Prof. David R. Jackson ECE Dept. Notes 13 ECE 338 Applied Electicity and Magnetism ping 07 Pof. David R. Jackson ECE Dept. Notes 3 Divegence The Physical Concept Find the flux going outwad though a sphee of adius. x ρ v0 z a y ψ = D nˆ d = D ˆ

More information

Dynamics of Rotational Motion

Dynamics of Rotational Motion Dynamics of Rotational Motion Toque: the otational analogue of foce Toque = foce x moment am τ = l moment am = pependicula distance though which the foce acts a.k.a. leve am l l l l τ = l = sin φ = tan

More information

ω = θ θ o = θ θ = s r v = rω

ω = θ θ o = θ θ = s r v = rω Unifom Cicula Motion Unifom cicula motion is the motion of an object taveling at a constant(unifom) speed in a cicula path. Fist we must define the angula displacement and angula velocity The angula displacement

More information

to point uphill and to be equal to its maximum value, in which case f s, max = μsfn

to point uphill and to be equal to its maximum value, in which case f s, max = μsfn Chapte 6 16. (a) In this situation, we take f s to point uphill and to be equal to its maximum value, in which case f s, max = μsf applies, whee μ s = 0.5. pplying ewton s second law to the block of mass

More information

Translation and Rotation Kinematics

Translation and Rotation Kinematics Tanslation and Rotation Kinematics Oveview: Rotation and Tanslation of Rigid Body Thown Rigid Rod Tanslational Motion: the gavitational extenal foce acts on cente-of-mass F ext = dp sy s dt dv total cm

More information

A Cross Section surface tension viscosity σ U 2 10 inertia gravity gd

A Cross Section surface tension viscosity σ U 2 10 inertia gravity gd .5 Final Exam 005 SOLUTION Question U A Coss Section Photo emoved fo copyight easons. Souce: Figue 7l in Clanet, C. "Dynamics and stability of wate bells." J. Fluid Mech 40 (00): -47. R d Tooidal im U

More information

arxiv: v1 [physics.flu-dyn] 21 Dec 2018

arxiv: v1 [physics.flu-dyn] 21 Dec 2018 1 axiv:1812.921v1 [physics.flu-dyn] 21 Dec 218 The cicula capillay jump Rajesh K. Bhagat 1, and P. F. Linden 2, 1 Depatment of Chemical Engineeing and Biotechnology, Univesity of Cambidge, Philippa Fawcett

More information

10. Force is inversely proportional to distance between the centers squared. R 4 = F 16 E 11.

10. Force is inversely proportional to distance between the centers squared. R 4 = F 16 E 11. NSWRS - P Physics Multiple hoice Pactice Gavitation Solution nswe 1. m mv Obital speed is found fom setting which gives v whee M is the object being obited. Notice that satellite mass does not affect obital

More information

Raju Ananth Structural Integrity Associates, Inc Hellyer Avenue, Suite 210 San Jose, CA

Raju Ananth Structural Integrity Associates, Inc Hellyer Avenue, Suite 210 San Jose, CA Poceedings of the ASME 1 Pessue Vessels & Piping Confeence PVP1 July 15-19, 1, Toonto, Ontaio, CANADA PVP1-78116 Flow Loads on the Shoud in a Boiling Wate Reacto Due to a Reciculation Outlet Line Beak

More information

Chapter 4. Newton s Laws of Motion

Chapter 4. Newton s Laws of Motion Chapte 4 Newton s Laws of Motion 4.1 Foces and Inteactions A foce is a push o a pull. It is that which causes an object to acceleate. The unit of foce in the metic system is the Newton. Foce is a vecto

More information

Look over Chapter 22 sections 1-8 Examples 2, 4, 5, Look over Chapter 16 sections 7-9 examples 6, 7, 8, 9. Things To Know 1/22/2008 PHYS 2212

Look over Chapter 22 sections 1-8 Examples 2, 4, 5, Look over Chapter 16 sections 7-9 examples 6, 7, 8, 9. Things To Know 1/22/2008 PHYS 2212 PHYS 1 Look ove Chapte sections 1-8 xamples, 4, 5, PHYS 111 Look ove Chapte 16 sections 7-9 examples 6, 7, 8, 9 Things To Know 1) What is an lectic field. ) How to calculate the electic field fo a point

More information

TAMPINES JUNIOR COLLEGE 2009 JC1 H2 PHYSICS GRAVITATIONAL FIELD

TAMPINES JUNIOR COLLEGE 2009 JC1 H2 PHYSICS GRAVITATIONAL FIELD TAMPINES JUNIOR COLLEGE 009 JC1 H PHYSICS GRAVITATIONAL FIELD OBJECTIVES Candidates should be able to: (a) show an undestanding of the concept of a gavitational field as an example of field of foce and

More information

School of Electrical and Computer Engineering, Cornell University. ECE 303: Electromagnetic Fields and Waves. Fall 2007

School of Electrical and Computer Engineering, Cornell University. ECE 303: Electromagnetic Fields and Waves. Fall 2007 School of Electical and Compute Engineeing, Conell Univesity ECE 303: Electomagnetic Fields and Waves Fall 007 Homewok 8 Due on Oct. 19, 007 by 5:00 PM Reading Assignments: i) Review the lectue notes.

More information