Scale analysis of the vertical equation of motion:

Size: px
Start display at page:

Download "Scale analysis of the vertical equation of motion:"

Transcription

1 Scale analysis of the vertical equation of motion: As we did with the hz eqns, we do for the vertical to estimate the order of magnitude of Dw/ we take the largest of the terms, Dw -- W/T h UW/L W 2 /H w - + u w - + v- w + w w t x y z z-equation Dw/ -2Ωucosφ -(u 2 +v 2 )/a ( ρ) p z -g scaling WU/L f 0 U U 2 /a δp v /(ρh) g value Thus we see that the atmosphere, to the first order, is hydrostatic, p ρg z Even though the atmosphere technically is not at rest, the hydrotatic apx is not a bad estimate. However, the story does not end here, there is more to this than meets the eye in that g and ( ρ) p z nearly cancel each other out (i.e. the -0 scenario). Thus, slight differences between two relatively large terms are responsible for the vertical acceleration. In order to examine these terms in more detail, we introduce the concept of mean and perturbation quantities. Mass Conservation The mass of an air parcel is conserved [no matter how it moves around, deforms, stretches, etc.] Let V be a parcel's volume and ρ it's density. m ρv is the parcel's mass. Mass conservation can be written in many equivalent Lagrangian forms: m const [but dif parcels have dif masses, i.e. dif consts] ρv const ρ(t)v(t) const [ If V increases, ρ must decrease] Dm/ 0 D(ρV)/ 0

2 Use product rule: ρ DV -- V-- Dρ ρ DV -- V Dρ + -- ρv 0 -- DV Dρ -- 0 V ρ These are all equivalent Lagrangian forms. Eulerian forms of mass conservation First lets focus on /V DV/ -- we'll be able to relate it to spatial changes in the wind field. Consider an infinitesimal box-shaped air parcel: z x y Vδxδyδz Thus, from our box we have: air δx δy δz -- DV -- V -- D ( δxδyδz) δxδyδz -- δyδzδx D δxδyδz + δxδzδy D + δxδyδz D δx D D + δy δz D δx δy δz Let s take a look at the time rate of change of the line segment δx: x A δx(t0) x B x A x B δx(δt) Note the following: Translation or rotation of line segment does NOT change the length of the segment! In an infinitesimal time (δt), the v and w components can rotate and translate the line segment but cannot elongate (stretch) it.

3 y x translate tδt t0 rotate elongate u can translate and elongate the segment δx Therefore we have: δx(0) x B x A [initial length] δx(δt) x B x A [length a short time later] Taylor series approximation of x A for small t: dx 0 A x A x A + ---δt + HOT x dt A + u A δt Similarly, dx B 0 x B x B + ---δt + HOT x dt B + u B δt Subtracting, we get x B x A x B x A + ( u B u A )δt δx( δt) δxt ( 0) + ( u B u A )δt Also apply Taylor series for u B, u ~0 u B u A u + ( x x B x A ) + HOT u A + δx ( 0) x Plugging in the expansion about u B into δx(δt) we have u B -u A u δx( δt) δx( 0) + δx ( 0)δt x rearrange (solve for u x )

4 u x δx( δt) δx( 0) δx( 0)δt lim δx( δt) δx( 0) δt 0 δx( 0)δt δx D ---- ( δx) we can show similarly v y ---- Dδy w, and - δy z ---- Dδz ---- δz Hence, we can now relate the three-dimensional wind to the change in volume -- DV -- V u v w u x y z This is 3-D divergence! If u >0 (divergence) air parcel expands (i.e. volume V increases) Now that we have related the change in volume to the velocity, we can rewrite the Lagrangian form of mass conservation as: -- DV Dρ + u Dρ 0 Mass Conservation V ρ ρ If u >0 then Dρ/<0 (which is consistent with above, i.e. divergence and increasing volume and therefore decreasing density). The above expression is a hybrid - part Eularian and part Lagrangian. We can get rid of the mix by multiplying by ρ and expanding the total derivative, ρ ρ + u ρ + ρ u 0 + ρu t t 0 (flux form) where I have used the product rule to condense the last two terms of the first equation above. These two expressions have no total derivatives in them - they are purely Eularian frame. A couple of points... Note that the horizontal divergence provides information on how the area changes but not how the volume changes. For example

5 H u u v + δx D D + δy - D ( δxδy) x y δx δy δxδy - DA H - A H where A H is the horizontal area. CASE I: If u x, v y > 0, we have DA H / > 0 and the area grows δy(0) δy(δt) δx(0) δx(δt) CASE II: If u x 0, and v y < 0, we have compression along the y axis and the area shrinks δy(0) δx(0) δy(δt) δx(δt) CASE III: If u x > 0, v y > 0, and w z > 0, the parcel expands in x, y, and z directions (i.e. the volume increases) and the horizontal area increases. CASE IV: If u x s, v y 2s, and w z 3s, then we have DA H / < 0 (shrinking horizontal area) but growing volume! Thus parcel is stretching in the x and z-directions, and compressing in the y direction. STUDENTS: Show (in 3-D) that ρu ρ u + u ρ

6 Scaling the Mass Conservation Equation As with the vertical equation of motion, we decompose the density into base state (mean) and perturbation quantities, ---- ( ρ + ρ t 0 ) + u ρ ( + ρ 0 ) + ( ρ + ρ 0 ) u 0 where ρ( x, y, z, t) ρ 0 ( z) + ρ ( xyzt,,, ). We know that ρ 0 is a f(z) only rewritten ( ρ 0 t, ρ 0 x, ρ 0 y 0), thus the above equation can be ---- ρ u ρ w dρ ( ρ + ρ t dz 0 ) u 0 multiplying by /ρ 0 we have ---- ρ -- + u ρ ρ 0 t ---- w dρ small ρ u + u 0 ρ 0 dz ρ 0 when comparing the last two terms we know that ρ ρ 0 «0, thus the 4th term is much smaller than the 5th term above. We now have what Holton has, namely ---- ρ -- + u ρ ρ 0 t ---- w dρ u 0 ρ 0 dz

Dynamic Meteorology - Introduction

Dynamic Meteorology - Introduction Dynamic Meteorology - Introduction Atmospheric dynamics the study of atmospheric motions that are associated with weather and climate We will consider the atmosphere to be a continuous fluid medium, or

More information

ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr. DeCaria

ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr. DeCaria ESCI 485 Air/Sea Interaction Lesson 1 Stresses and Fluxes Dr DeCaria References: An Introduction to Dynamic Meteorology, Holton MOMENTUM EQUATIONS The momentum equations governing the ocean or atmosphere

More information

Circulation and Vorticity

Circulation and Vorticity Circulation and Vorticity Example: Rotation in the atmosphere water vapor satellite animation Circulation a macroscopic measure of rotation for a finite area of a fluid Vorticity a microscopic measure

More information

Chapter 4: Fundamental Forces

Chapter 4: Fundamental Forces Chapter 4: Fundamental Forces Newton s Second Law: F=ma In atmospheric science it is typical to consider the force per unit mass acting on the atmosphere: Force mass = a In order to understand atmospheric

More information

Vorticity in natural coordinates

Vorticity in natural coordinates Vorticity in natural coordinates (see Holton pg 95, section 4.2.) Let s consider the vertical vorticity component only, i.e. ζ kˆ ω, we have ω u dl kˆ ω lim --- lim ----------------- curve is in xy plane

More information

Chapter 2. Deriving the Vlasov Equation From the Klimontovich Equation 19. Deriving the Vlasov Equation From the Klimontovich Equation

Chapter 2. Deriving the Vlasov Equation From the Klimontovich Equation 19. Deriving the Vlasov Equation From the Klimontovich Equation Chapter 2. Deriving the Vlasov Equation From the Klimontovich Equation 19 Chapter 2. Deriving the Vlasov Equation From the Klimontovich Equation Topics or concepts to learn in Chapter 2: 1. The microscopic

More information

MATH 56A SPRING 2008 STOCHASTIC PROCESSES 197

MATH 56A SPRING 2008 STOCHASTIC PROCESSES 197 MATH 56A SPRING 8 STOCHASTIC PROCESSES 197 9.3. Itô s formula. First I stated the theorem. Then I did a simple example to make sure we understand what it says. Then I proved it. The key point is Lévy s

More information

From the last time, we ended with an expression for the energy equation. u = ρg u + (τ u) q (9.1)

From the last time, we ended with an expression for the energy equation. u = ρg u + (τ u) q (9.1) Lecture 9 9. Administration None. 9. Continuation of energy equation From the last time, we ended with an expression for the energy equation ρ D (e + ) u = ρg u + (τ u) q (9.) Where ρg u changes in potential

More information

The hydrostatic equilibrium

The hydrostatic equilibrium Chapter 10 The hydrostatic equilibrium 10.1 The force on the infinitesimal parcel Now we will compute the total force acting on an infinitesimal parcel of fluid at rest. Consider a rectangular parallelepiped

More information

z g + F w (2.56) p(x, y, z, t) = p(z) + p (x, y, z, t) (2.120) ρ(x, y, z, t) = ρ(z) + ρ (x, y, z, t), (2.121)

z g + F w (2.56) p(x, y, z, t) = p(z) + p (x, y, z, t) (2.120) ρ(x, y, z, t) = ρ(z) + ρ (x, y, z, t), (2.121) = + dw dt = 1 ρ p z g + F w (.56) Let us describe the total pressure p and density ρ as the sum of a horizontally homogeneous base state pressure and density, and a deviation from this base state, that

More information

Lecture 3: Convective Heat Transfer I

Lecture 3: Convective Heat Transfer I Lecture 3: Convective Heat Transfer I Kerry Emanuel; notes by Paige Martin and Daniel Mukiibi June 18 1 Introduction In the first lecture, we discussed radiative transfer in the climate system. Here, we

More information

Mathematical Concepts & Notation

Mathematical Concepts & Notation Mathematical Concepts & Notation Appendix A: Notation x, δx: a small change in x t : the partial derivative with respect to t holding the other variables fixed d : the time derivative of a quantity that

More information

ρ x + fv f 'w + F x ρ y fu + F y Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ Dv Dt + u2 tanφ + vw a a = 1 p Dw Dt u2 + v 2

ρ x + fv f 'w + F x ρ y fu + F y Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ Dv Dt + u2 tanφ + vw a a = 1 p Dw Dt u2 + v 2 Fundamental Equation in z coordinate p = ρrt or pα = RT Du uv tanφ + uw Dt a a = 1 p ρ x + fv f 'w + F x Dv Dt + u2 tanφ + vw a a = 1 p ρ y fu + F y Dw Dt u2 + v 2 = 1 p a ρ z g + f 'u + F z Dρ Dt + ρ

More information

Lecture 3: 1. Lecture 3.

Lecture 3: 1. Lecture 3. Lecture 3: 1 Lecture 3. Lecture 3: 2 Plan for today Summary of the key points of the last lecture. Review of vector and tensor products : the dot product (or inner product ) and the cross product (or vector

More information

The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh

The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh z = The perturbation pressure, p, can be represented as the sum of a hydrostatic pressure perturbation p h and a nonhydrostatic pressure perturbation p nh, that is, p = p h + p nh. (.1) The former arises

More information

Control Volume. Dynamics and Kinematics. Basic Conservation Laws. Lecture 1: Introduction and Review 1/24/2017

Control Volume. Dynamics and Kinematics. Basic Conservation Laws. Lecture 1: Introduction and Review 1/24/2017 Lecture 1: Introduction and Review Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study of motion without regard for the cause. Dynamics: On the other hand, dynamics

More information

Lecture 1: Introduction and Review

Lecture 1: Introduction and Review Lecture 1: Introduction and Review Review of fundamental mathematical tools Fundamental and apparent forces Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study

More information

1/3/2011. This course discusses the physical laws that govern atmosphere/ocean motions.

1/3/2011. This course discusses the physical laws that govern atmosphere/ocean motions. Lecture 1: Introduction and Review Dynamics and Kinematics Kinematics: The term kinematics means motion. Kinematics is the study of motion without regard for the cause. Dynamics: On the other hand, dynamics

More information

Getting started: CFD notation

Getting started: CFD notation PDE of p-th order Getting started: CFD notation f ( u,x, t, u x 1,..., u x n, u, 2 u x 1 x 2,..., p u p ) = 0 scalar unknowns u = u(x, t), x R n, t R, n = 1,2,3 vector unknowns v = v(x, t), v R m, m =

More information

Where does Bernoulli's Equation come from?

Where does Bernoulli's Equation come from? Where does Bernoulli's Equation come from? Introduction By now, you have seen the following equation many times, using it to solve simple fluid problems. P ρ + v + gz = constant (along a streamline) This

More information

AE/ME 339. K. M. Isaac. 9/22/2005 Topic 6 FluidFlowEquations_Introduction. Computational Fluid Dynamics (AE/ME 339) MAEEM Dept.

AE/ME 339. K. M. Isaac. 9/22/2005 Topic 6 FluidFlowEquations_Introduction. Computational Fluid Dynamics (AE/ME 339) MAEEM Dept. AE/ME 339 Computational Fluid Dynamics (CFD) 1...in the phrase computational fluid dynamics the word computational is simply an adjective to fluid dynamics.... -John D. Anderson 2 1 Equations of Fluid

More information

A Hamiltonian Numerical Scheme for Large Scale Geophysical Fluid Systems

A Hamiltonian Numerical Scheme for Large Scale Geophysical Fluid Systems A Hamiltonian Numerical Scheme for Large Scale Geophysical Fluid Systems Bob Peeters Joint work with Onno Bokhove & Jason Frank TW, University of Twente, Enschede CWI, Amsterdam PhD-TW colloquium, 9th

More information

Pressure in stationary and moving fluid. Lab-On-Chip: Lecture 2

Pressure in stationary and moving fluid. Lab-On-Chip: Lecture 2 Pressure in stationary and moving fluid Lab-On-Chip: Lecture Fluid Statics No shearing stress.no relative movement between adjacent fluid particles, i.e. static or moving as a single block Pressure at

More information

ATM 298, Spring 2013 Lecture 2 The Equa;ons of Fluid Mo;on April 3, Paul A. Ullrich (HH 251)

ATM 298, Spring 2013 Lecture 2 The Equa;ons of Fluid Mo;on April 3, Paul A. Ullrich (HH 251) ATM 298, Spring 2013 Lecture 2 The Equa;ons of Fluid Mo;on April 3, 2013 Paul A. Ullrich (HH 251) paullrich@ucdavis.edu Global Atmospheric Modeling Global atmospheric models were originally constructed

More information

Introduction to Fluid Dynamics

Introduction to Fluid Dynamics Introduction to Fluid Dynamics Roger K. Smith Skript - auf englisch! Umsonst im Internet http://www.meteo.physik.uni-muenchen.de Wählen: Lehre Manuskripte Download User Name: meteo Password: download Aim

More information

Pressure in stationary and moving fluid Lab- Lab On- On Chip: Lecture 2

Pressure in stationary and moving fluid Lab- Lab On- On Chip: Lecture 2 Pressure in stationary and moving fluid Lab-On-Chip: Lecture Lecture plan what is pressure e and how it s distributed in static fluid water pressure in engineering problems buoyancy y and archimedes law;

More information

Chapter 10 Atmospheric Forces & Winds

Chapter 10 Atmospheric Forces & Winds Chapter 10 Atospheric Forces & Winds Chapter overview: Atospheric Pressure o Horizontal pressure variations o Station vs sea level pressure Winds and weather aps Newton s 2 nd Law Horizontal Forces o Pressure

More information

The Equations of Motion in a Rotating Coordinate System. Chapter 3

The Equations of Motion in a Rotating Coordinate System. Chapter 3 The Equations of Motion in a Rotating Coordinate System Chapter 3 Since the earth is rotating about its axis and since it is convenient to adopt a frame of reference fixed in the earth, we need to study

More information

Fundamentals of Atmospheric Modelling

Fundamentals of Atmospheric Modelling M.Sc. in Computational Science Fundamentals of Atmospheric Modelling Peter Lynch, Met Éireann Mathematical Computation Laboratory (Opp. Room 30) Dept. of Maths. Physics, UCD, Belfield. January April, 2004.

More information

Conservation of Mass. Computational Fluid Dynamics. The Equations Governing Fluid Motion

Conservation of Mass. Computational Fluid Dynamics. The Equations Governing Fluid Motion http://www.nd.edu/~gtryggva/cfd-course/ http://www.nd.edu/~gtryggva/cfd-course/ Computational Fluid Dynamics Lecture 4 January 30, 2017 The Equations Governing Fluid Motion Grétar Tryggvason Outline Derivation

More information

Lecture 1: Introduction to Linear and Non-Linear Waves

Lecture 1: Introduction to Linear and Non-Linear Waves Lecture 1: Introduction to Linear and Non-Linear Waves Lecturer: Harvey Segur. Write-up: Michael Bates June 15, 2009 1 Introduction to Water Waves 1.1 Motivation and Basic Properties There are many types

More information

ESS314. Basics of Geophysical Fluid Dynamics by John Booker and Gerard Roe. Conservation Laws

ESS314. Basics of Geophysical Fluid Dynamics by John Booker and Gerard Roe. Conservation Laws ESS314 Basics of Geophysical Fluid Dynamics by John Booker and Gerard Roe Conservation Laws The big differences between fluids and other forms of matter are that they are continuous and they deform internally

More information

wavelength (nm)

wavelength (nm) Blackbody radiation Everything with a temperature above absolute zero emits electromagnetic radiation. This phenomenon is called blackbody radiation. The intensity and the peak wavelength of the radiation

More information

Parcel Model. Atmospheric Sciences September 30, 2012

Parcel Model. Atmospheric Sciences September 30, 2012 Parcel Model Atmospheric Sciences 6150 September 30, 2012 1 Governing Equations for Precipitating Convection For precipitating convection, we have the following set of equations for potential temperature,

More information

On side wall labeled A: we can express the pressure in a Taylor s series expansion: x 2. + higher order terms,

On side wall labeled A: we can express the pressure in a Taylor s series expansion: x 2. + higher order terms, Chapter 1 Notes A Note About Coordinates We nearly always use a coordinate system in this class where the vertical, ˆk, is normal to the Earth s surface and the x-direction, î, points to the east and the

More information

1 Introduction to Governing Equations 2 1a Methodology... 2

1 Introduction to Governing Equations 2 1a Methodology... 2 Contents 1 Introduction to Governing Equations 2 1a Methodology............................ 2 2 Equation of State 2 2a Mean and Turbulent Parts...................... 3 2b Reynolds Averaging.........................

More information

Chapter 1. Governing Equations of GFD. 1.1 Mass continuity

Chapter 1. Governing Equations of GFD. 1.1 Mass continuity Chapter 1 Governing Equations of GFD The fluid dynamical governing equations consist of an equation for mass continuity, one for the momentum budget, and one or more additional equations to account for

More information

2.25 Advanced Fluid Mechanics

2.25 Advanced Fluid Mechanics MIT Department of Mechanical Engineering.5 Advanced Fluid Mechanics Problem 4.05 This problem is from Advanced Fluid Mechanics Problems by A.H. Shapiro and A.A. Sonin Consider the frictionless, steady

More information

Chapter 4 Water Vapor

Chapter 4 Water Vapor Chapter 4 Water Vapor Chapter overview: Phases of water Vapor pressure at saturation Moisture variables o Mixing ratio, specific humidity, relative humidity, dew point temperature o Absolute vs. relative

More information

Goal: Use understanding of physically-relevant scales to reduce the complexity of the governing equations

Goal: Use understanding of physically-relevant scales to reduce the complexity of the governing equations Scale analysis relevant to the tropics [large-scale synoptic systems]* Goal: Use understanding of physically-relevant scales to reduce the complexity of the governing equations *Reminder: Midlatitude scale

More information

2.20 Marine Hydrodynamics Lecture 3

2.20 Marine Hydrodynamics Lecture 3 2.20 Marine Hyroynamics, Fall 2018 Lecture 3 Copyright c 2018 MIT - Department of Mechanical Engineering, All rights reserve. 1.7 Stress Tensor 2.20 Marine Hyroynamics Lecture 3 1.7.1 Stress Tensor τ ij

More information

Convection Heat Transfer

Convection Heat Transfer Convection Heat Transfer Department of Chemical Eng., Isfahan University of Technology, Isfahan, Iran Seyed Gholamreza Etemad Winter 2013 Heat convection: Introduction Difference between the temperature

More information

CHARACTERISTIC OF FLUIDS. A fluid is defined as a substance that deforms continuously when acted on by a shearing stress at any magnitude.

CHARACTERISTIC OF FLUIDS. A fluid is defined as a substance that deforms continuously when acted on by a shearing stress at any magnitude. CHARACTERISTIC OF FLUIDS A fluid is defined as a substance that deforms continuously when acted on by a shearing stress at any magnitude. In a fluid at rest, normal stress is called pressure. 1 Dimensions,

More information

Physics 556 Stellar Astrophysics Prof. James Buckley

Physics 556 Stellar Astrophysics Prof. James Buckley hysics 556 Stellar Astrophysics rof. James Buckley Lecture 8 Convection and the Lane Emden Equations for Stellar Structure Reading/Homework Assignment Read sections 2.5 to 2.9 in Rose over spring break!

More information

Chapter 7: Circulation and Vorticity

Chapter 7: Circulation and Vorticity Chapter 7: Circulation and Vorticity Circulation C = u ds Integration is performed in a counterclockwise direction C is positive for counterclockwise flow!!! Kelvin s Circulation Theorem The rate of change

More information

The total derivative. Chapter Lagrangian and Eulerian approaches

The total derivative. Chapter Lagrangian and Eulerian approaches Chapter 5 The total erivative 51 Lagrangian an Eulerian approaches The representation of a flui through scalar or vector fiels means that each physical quantity uner consieration is escribe as a function

More information

4. The rules of the game

4. The rules of the game ! Revised Friday, November 14, 2014! 1 4. The rules of the game Introduction This chapter gives a quick review of concepts to be used later. Topics covered including the conservation principles for momentum,

More information

The Euler Equation of Gas-Dynamics

The Euler Equation of Gas-Dynamics The Euler Equation of Gas-Dynamics A. Mignone October 24, 217 In this lecture we study some properties of the Euler equations of gasdynamics, + (u) = ( ) u + u u + p = a p + u p + γp u = where, p and u

More information

Models of ocean circulation are all based on the equations of motion.

Models of ocean circulation are all based on the equations of motion. Equations of motion Models of ocean circulation are all based on the equations of motion. Only in simple cases the equations of motion can be solved analytically, usually they must be solved numerically.

More information

Study Guide for Exam #2

Study Guide for Exam #2 Physical Mechanics METR103 November, 000 Study Guide for Exam # The information even below is meant to serve as a guide to help you to prepare for the second hour exam. The absence of a topic or point

More information

OCN-ATM-ESS 587. Simple and basic dynamical ideas.. Newton s Laws. Pressure and hydrostatic balance. The Coriolis effect. Geostrophic balance

OCN-ATM-ESS 587. Simple and basic dynamical ideas.. Newton s Laws. Pressure and hydrostatic balance. The Coriolis effect. Geostrophic balance OCN-ATM-ESS 587 Simple and basic dynamical ideas.. Newton s Laws Pressure and hydrostatic balance The Coriolis effect Geostrophic balance Lagrangian-Eulerian coordinate frames Coupled Ocean- Atmosphere

More information

0.2. CONSERVATION LAW FOR FLUID 9

0.2. CONSERVATION LAW FOR FLUID 9 0.2. CONSERVATION LAW FOR FLUID 9 Consider x-component of Eq. (26), we have D(ρu) + ρu( v) dv t = ρg x dv t S pi ds, (27) where ρg x is the x-component of the bodily force, and the surface integral is

More information

The Hydrostatic Approximation. - Euler Equations in Spherical Coordinates. - The Approximation and the Equations

The Hydrostatic Approximation. - Euler Equations in Spherical Coordinates. - The Approximation and the Equations OUTLINE: The Hydrostatic Approximation - Euler Equations in Spherical Coordinates - The Approximation and the Equations - Critique of Hydrostatic Approximation Inertial Instability - The Phenomenon - The

More information

g (z) = 1 (1 + z/a) = 1 1 ( km/10 4 km) 2

g (z) = 1 (1 + z/a) = 1 1 ( km/10 4 km) 2 1.4.2 Gravitational Force g is the gravitational force. It always points towards the center of mass, and it is proportional to the inverse square of the distance above the center of mass: g (z) = GM (a

More information

Physical Oceanography, MSCI 3001 Oceanographic Processes, MSCI Dr. Katrin Meissner Week 5.

Physical Oceanography, MSCI 3001 Oceanographic Processes, MSCI Dr. Katrin Meissner Week 5. Physical Oceanography, MSCI 3001 Oceanographic Processes, MSCI 5004 Dr. Katrin Meissner k.meissner@unsw.e.au Week 5 Ocean Dynamics Transport of Volume, Heat & Salt Flux: Amount of heat, salt or volume

More information

AE/ME 339. Computational Fluid Dynamics (CFD) K. M. Isaac. Momentum equation. Computational Fluid Dynamics (AE/ME 339) MAEEM Dept.

AE/ME 339. Computational Fluid Dynamics (CFD) K. M. Isaac. Momentum equation. Computational Fluid Dynamics (AE/ME 339) MAEEM Dept. AE/ME 339 Computational Fluid Dynamics (CFD) 9//005 Topic7_NS_ F0 1 Momentum equation 9//005 Topic7_NS_ F0 1 Consider the moving fluid element model shown in Figure.b Basis is Newton s nd Law which says

More information

Propagation of Error Notes

Propagation of Error Notes Propagation of Error Notes From http://facultyfiles.deanza.edu/gems/lunaeduardo/errorpropagation2a.pdf The analysis of uncertainties (errors) in measurements and calculations is essential in the physics

More information

where p oo is a reference level constant pressure (often 10 5 Pa). Since θ is conserved for adiabatic motions, a prognostic temperature equation is:

where p oo is a reference level constant pressure (often 10 5 Pa). Since θ is conserved for adiabatic motions, a prognostic temperature equation is: 1 Appendix C Useful Equations Purposes: Provide foundation equations and sketch some derivations. These equations are used as starting places for discussions in various parts of the book. C.1. Thermodynamic

More information

( ) where the phase! is given by! = kx + mz!"t. We also know

( ) where the phase! is given by! = kx + mz!t. We also know GFD I, Final Exam Solutions 3/7/1 Parker MacCready 1.(a) The expression for the pressure perturbation is found from the vertical momentum equation: Z-MOM w t! 1! p' z b which may be rearranged to give:

More information

Chapter 5. Fundamentals of Atmospheric Modeling

Chapter 5. Fundamentals of Atmospheric Modeling Overhead Slides for Chapter 5 of Fundamentals of Atmospheric Modeling by Mark Z. Jacobson Department of Civil & Environmental Engineering Stanford University Stanford, CA 94305-4020 January 30, 2002 Altitude

More information

Introduction to Synoptic Scale Dynamics

Introduction to Synoptic Scale Dynamics Introduction to Synoptic Scale Dynamics Contents J. H. LaCasce, UiO 1 General dynamics 2 1.1 Derivatives................................. 2 1.2 Continuity equation............................. 3 1.3 Equations

More information

Parcel Model. Meteorology September 3, 2008

Parcel Model. Meteorology September 3, 2008 Parcel Model Meteorology 5210 September 3, 2008 1 Governing Equations for Precipitating Convection For precipitating convection, we have the following set of equations for potential temperature, θ, mixing

More information

The Shallow Water Equations

The Shallow Water Equations The Shallow Water Equations Clint Dawson and Christopher M. Mirabito Institute for Computational Engineering and Sciences University of Texas at Austin clint@ices.utexas.edu September 29, 2008 The Shallow

More information

Quick Recapitulation of Fluid Mechanics

Quick Recapitulation of Fluid Mechanics Quick Recapitulation of Fluid Mechanics Amey Joshi 07-Feb-018 1 Equations of ideal fluids onsider a volume element of a fluid of density ρ. If there are no sources or sinks in, the mass in it will change

More information

The continuity equation

The continuity equation Chapter 6 The continuity equation 61 The equation of continuity It is evient that in a certain region of space the matter entering it must be equal to the matter leaving it Let us consier an infinitesimal

More information

Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic]

Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Entropy 1. (Thermodynamics) a thermodynamic quantity that changes in a

More information

Dust devils, water spouts, tornados

Dust devils, water spouts, tornados Balanced flow Things we know Primitive equations are very comprehensive, but there may be a number of vast simplifications that may be relevant (e.g., geostrophic balance). Seems that there are things

More information

Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere

Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium Goal: Develop a 1D description of the [tropical] atmosphere Vertical temperature profile Total atmospheric mass: ~5.15x10

More information

Chapter 2. Quasi-Geostrophic Theory: Formulation (review) ε =U f o L <<1, β = 2Ω cosθ o R. 2.1 Introduction

Chapter 2. Quasi-Geostrophic Theory: Formulation (review) ε =U f o L <<1, β = 2Ω cosθ o R. 2.1 Introduction Chapter 2. Quasi-Geostrophic Theory: Formulation (review) 2.1 Introduction For most of the course we will be concerned with instabilities that an be analyzed by the quasi-geostrophic equations. These are

More information

Sample Final Questions: Solutions Math 21B, Winter y ( y 1)(1 + y)) = A y + B

Sample Final Questions: Solutions Math 21B, Winter y ( y 1)(1 + y)) = A y + B Sample Final Questions: Solutions Math 2B, Winter 23. Evaluate the following integrals: tan a) y y dy; b) x dx; c) 3 x 2 + x dx. a) We use partial fractions: y y 3 = y y ) + y)) = A y + B y + C y +. Putting

More information

Fluid Dynamics. Massimo Ricotti. University of Maryland. Fluid Dynamics p.1/14

Fluid Dynamics. Massimo Ricotti. University of Maryland. Fluid Dynamics p.1/14 Fluid Dynamics p.1/14 Fluid Dynamics Massimo Ricotti ricotti@astro.umd.edu University of Maryland Fluid Dynamics p.2/14 The equations of fluid dynamics are coupled PDEs that form an IVP (hyperbolic). Use

More information

2. Basic assumptions for stellar atmospheres

2. Basic assumptions for stellar atmospheres . Basic assumptions for stellar atmospheres 1. geometry, stationarity. conservation of momentum, mass 3. conservation of energy 4. Local Thermodynamic Equilibrium 1 1. Geometry Stars as gaseous spheres

More information

3.5 Vorticity Equation

3.5 Vorticity Equation .0 - Marine Hydrodynamics, Spring 005 Lecture 9.0 - Marine Hydrodynamics Lecture 9 Lecture 9 is structured as follows: In paragraph 3.5 we return to the full Navier-Stokes equations (unsteady, viscous

More information

10 Shallow Water Models

10 Shallow Water Models 10 Shallow Water Models So far, we have studied the effects due to rotation and stratification in isolation. We then looked at the effects of rotation in a barotropic model, but what about if we add stratification

More information

2. Basic Assumptions for Stellar Atmospheres

2. Basic Assumptions for Stellar Atmospheres 2. Basic Assumptions for Stellar Atmospheres 1. geometry, stationarity 2. conservation of momentum, mass 3. conservation of energy 4. Local Thermodynamic Equilibrium 1 1. Geometry Stars as gaseous spheres!

More information

Numerical Heat and Mass Transfer

Numerical Heat and Mass Transfer Master Degree in Mechanical Engineering Numerical Heat and Mass Transfer 15-Convective Heat Transfer Fausto Arpino f.arpino@unicas.it Introduction In conduction problems the convection entered the analysis

More information

Chapter 1. Continuum mechanics review. 1.1 Definitions and nomenclature

Chapter 1. Continuum mechanics review. 1.1 Definitions and nomenclature Chapter 1 Continuum mechanics review We will assume some familiarity with continuum mechanics as discussed in the context of an introductory geodynamics course; a good reference for such problems is Turcotte

More information

cos(θ)sin(θ) Alternative Exercise Correct Correct θ = 0 skiladæmi 10 Part A Part B Part C Due: 11:59pm on Wednesday, November 11, 2015

cos(θ)sin(θ) Alternative Exercise Correct Correct θ = 0 skiladæmi 10 Part A Part B Part C Due: 11:59pm on Wednesday, November 11, 2015 skiladæmi 10 Due: 11:59pm on Wednesday, November 11, 015 You will receive no credit for items you complete after the assignment is due Grading Policy Alternative Exercise 1115 A bar with cross sectional

More information

2. Basic assumptions for stellar atmospheres

2. Basic assumptions for stellar atmospheres . Basic assumptions for stellar atmospheres 1. geometry, stationarity. conservation of momentum, mass 3. conservation of energy 4. Local Thermodynamic Equilibrium 1 1. Geometry Stars as gaseous spheres

More information

EATS Notes 1. Some course material will be online at

EATS Notes 1. Some course material will be online at EATS 3040-2015 Notes 1 14 Aug 2015 Some course material will be online at http://www.yorku.ca/pat/esse3040/ HH = Holton and Hakim. An Introduction to Dynamic Meteorology, 5th Edition. Most of the images

More information

13.42 LECTURE 2: REVIEW OF LINEAR WAVES

13.42 LECTURE 2: REVIEW OF LINEAR WAVES 13.42 LECTURE 2: REVIEW OF LINEAR WAVES SPRING 2003 c A.H. TECHET & M.S. TRIANTAFYLLOU 1. Basic Water Waves Laplace Equation 2 φ = 0 Free surface elevation: z = η(x, t) No vertical velocity at the bottom

More information

Gradient, Divergence and Curl in Curvilinear Coordinates

Gradient, Divergence and Curl in Curvilinear Coordinates Gradient, Divergence and Curl in Curvilinear Coordinates Although cartesian orthogonal coordinates are very intuitive and easy to use, it is often found more convenient to work with other coordinate systems.

More information

Mathematical Theory of Non-Newtonian Fluid

Mathematical Theory of Non-Newtonian Fluid Mathematical Theory of Non-Newtonian Fluid 1. Derivation of the Incompressible Fluid Dynamics 2. Existence of Non-Newtonian Flow and its Dynamics 3. Existence in the Domain with Boundary Hyeong Ohk Bae

More information

Linear Momentum, Center of Mass, Conservation of Momentum, and Collision.

Linear Momentum, Center of Mass, Conservation of Momentum, and Collision. PHYS1110H, 2011 Fall. Shijie Zhong Linear Momentum, Center of Mass, Conservation of Momentum, and Collision. Linear momentum. For a particle of mass m moving at a velocity v, the linear momentum for the

More information

Differential equations of mass transfer

Differential equations of mass transfer Differential equations of mass transfer Definition: The differential equations of mass transfer are general equations describing mass transfer in all directions and at all conditions. How is the differential

More information

Ocean currents: some misconceptions and some dynamics

Ocean currents: some misconceptions and some dynamics Ocean currents: some misconceptions and some dynamics Joe LaCasce Dept. Geosciences October 30, 2012 Where is the Gulf Stream? BBC Weather Center Where is the Gulf Stream? Univ. Bergen news website (2011)

More information

CH.5. BALANCE PRINCIPLES. Multimedia Course on Continuum Mechanics

CH.5. BALANCE PRINCIPLES. Multimedia Course on Continuum Mechanics CH.5. BALANCE PRINCIPLES Multimedia Course on Continuum Mechanics Overview Balance Principles Convective Flux or Flux by Mass Transport Local and Material Derivative of a olume Integral Conservation of

More information

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations Needs work : define boundary conditions and fluxes before, change slides 1-2-3 Useful definitions and conservation equations Turbulent Kinetic energy The fluxes are crucial to define our boundary conditions,

More information

R g. o p2. Lecture 2: Buoyancy, stability, convection and gravity waves

R g. o p2. Lecture 2: Buoyancy, stability, convection and gravity waves Lecture : Clarifications of lecture 1: Hydrostatic balance: Under static conditions, only gravity will work on the fluid. Why doesn't all the fluid contract to the ground? Pressure builds u and resists

More information

The equations of fluid motion

The equations of fluid motion Chapter 6 The equations of fluid motion In order to proceed further with our discussion of the circulation of the atmosphere, and later the ocean, we must develop some of the underlying theory governing

More information

Daniel J. Jacob, Models of Atmospheric Transport and Chemistry, 2007.

Daniel J. Jacob, Models of Atmospheric Transport and Chemistry, 2007. 1 0. CHEMICAL TRACER MODELS: AN INTRODUCTION Concentrations of chemicals in the atmosphere are affected by four general types of processes: transport, chemistry, emissions, and deposition. 3-D numerical

More information

EULERIAN DERIVATIONS OF NON-INERTIAL NAVIER-STOKES EQUATIONS

EULERIAN DERIVATIONS OF NON-INERTIAL NAVIER-STOKES EQUATIONS EULERIAN DERIVATIONS OF NON-INERTIAL NAVIER-STOKES EQUATIONS ML Combrinck, LN Dala Flamengro, a div of Armscor SOC Ltd & University of Pretoria, Council of Scientific and Industrial Research & University

More information

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu Lecture 2: Basic Conservation Laws Conservation Law of Momentum Newton s 2 nd Law of Momentum = absolute velocity viewed in an inertial system = rate of change of Ua following the motion in an inertial

More information

1. The vertical structure of the atmosphere. Temperature profile.

1. The vertical structure of the atmosphere. Temperature profile. Lecture 4. The structure of the atmosphere. Air in motion. Objectives: 1. The vertical structure of the atmosphere. Temperature profile. 2. Temperature in the lower atmosphere: dry adiabatic lapse rate.

More information

Linear model for investigation of nonlinear NWP model accuracy. Marko Zirk, University of Tartu

Linear model for investigation of nonlinear NWP model accuracy. Marko Zirk, University of Tartu Linear model for investigation of nonlinear NWP model accuracy Marko Zirk, University of Tartu Introduction A method for finding numerical solution of non-hydrostatic linear equations of atmospheric dynamics

More information

( ) = 1005 J kg 1 K 1 ;

( ) = 1005 J kg 1 K 1 ; Problem Set 3 1. A parcel of water is added to the ocean surface that is denser (heavier) than any of the waters in the ocean. Suppose the parcel sinks to the ocean bottom; estimate the change in temperature

More information

Math background. Physics. Simulation. Related phenomena. Frontiers in graphics. Rigid fluids

Math background. Physics. Simulation. Related phenomena. Frontiers in graphics. Rigid fluids Fluid dynamics Math background Physics Simulation Related phenomena Frontiers in graphics Rigid fluids Fields Domain Ω R2 Scalar field f :Ω R Vector field f : Ω R2 Types of derivatives Derivatives measure

More information

( δx ) = δ dx = δu, etc. Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 2: Analysis Techniques

( δx ) = δ dx = δu, etc. Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 2: Analysis Techniques Course 12.812, General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 2: Analysis Techniques Pressure Coordinates: Most meteorological measurements are made in pressure coordinates, e.g.,

More information

4.1 LAWS OF MECHANICS - Review

4.1 LAWS OF MECHANICS - Review 4.1 LAWS OF MECHANICS - Review Ch4 9 SYSTEM System: Moving Fluid Definitions: System is defined as an arbitrary quantity of mass of fixed identity. Surrounding is everything external to this system. Boundary

More information

Figure 1. adiabatically. The change in pressure experienced by the parcel is. dp = -ρ o gξ

Figure 1. adiabatically. The change in pressure experienced by the parcel is. dp = -ρ o gξ 6. Internal waves Consider a continuously stratified fluid with ρ o (z) the vertical density profile. z p' ξ p ρ ρ ο (z) Figure 1. Figure by MIT OpenCourseWare. At a point P raise a parcel of water by

More information