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

Size: px
Start display at page:

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

Transcription

1 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 the comression. The balance between this ressure force and gravity yields the hydrostatic balance relation. What actually causes the resistance is the vertical gradient in ressure the ressure acts equally in all directions but it decreases with height, so at height z it is a certain value and at height z+δz it is slightly lower, which will cause the fluid to want to move uwards. But gravity will ull it down and balance will ensue: = ρg. z Hysometric relation: relates a layer thickness to the vertically integrated (over logressure) temerature. Can be in terms of: Height: z ( ) z( ) = R g Geootential height: zφ ( ) zφ ( ) = Geootential: φ ( z ) φ( z1) = R R g o Lecture : Buoyancy, stability, convection and gravity waves T1-radiative equilibrium and observed temerature rofile: The jum at the surface, and as we will see later also the troosheric lase rate are unstable and will lead to convection. T-schematic radiative equilibrium and observed temerature rofile. The trooshere is in Radiative-convective equilibrium. T3-schematic of Radiative-convective equilibrium. Understanding this convection is the toic of this class. In atmoshere we have convection in moist comressible fluid. Much more comlicated than a an of water. We will start from simle to more comlex. Why does convection occur? Horizontally uniform heating of water from below will force a satially uniform temerature decreasing with height. Even though light fluid is on bottom, the gravitational force can be balanced by ressure gradient, according to hydrostatic balance law. Zero net force. So why does convection develo? How come it is satially varying even if balanced state is horizontally homogeneous?

2 Instability: Lets look at the following examle of a ball on a hill-valley: Comonent of gravitational acceleration along the sloe: -gdh/dx Ball at oint A, where dh/dx=0 is in equilibrium stable. What if dislaced an increment δx? Sloe at x A +δx: dh/dx(x A +δx) dh/dx(x A )+(d h/dx ) A δx=(d h/dx ) A δx The equation of motion at δx: d (δx)/dt =-gdh/dx=-g(d h/dx ) A δx σ + t σ t Solution: δ x ( d h t) = C+ e + C e σ = ± ± g dx At the eak (d h/dx ) A<0 so the solution is exonentially growing- a small erturbation will grow. Instability, convection. At the trough (d h/dx ) B>0 so the solution is oscillatory. Energetics: At the trough, the erturbed ball moves uhill- we need to do work since its otential energy increases, and it won't haen. In the absence of an external energy source. At the ridge, the ball moves downhill, decreasing otential energy, and increasing kinetic energy. Motion will continue. Convection in water: Buoyancy: A light object in water will bounce back u. What about a fluid arcel? Fluid arcel: small but finite size, which is thermally isolated from environment and always at same ressure as environment. Assume ρ=ρ(t).

3 Above oint A the fluid is the same in 1, and (arcel). Hence ressure at A1, A, A is the same. Above oint B fluid column is lighter, and ressure is lower. The forces acting on the arcel: (subscrit E for environment and for arcel) Gravity deends on the arcel mass: F g =-gρ δaδz Pressure gradient force- deends on the environmental ressure: F t + F b =-δ E δa= gρ E δa δz Net force on arcel: F g +F t + F b = g(ρ E ρ ) δa δz Divide by the arcel mass ρ δa δz to get the acceleration, which is a reduced form of gravity: Buoyancy: b F tot /m = -g(ρ ρ E )/ ρ If ρ <ρ E, the arcel is ositively buoyant: b>0, and it will accelerate uwards. If ρ >ρ E, the arcel is negatively buoyant: b<0, and it will accelerate downwards. Lets look at a secific density rofile, which we assume deends only on temerature (incomressible water): ρ ref=ρ(1- α[t-t ref ]) Assume that a arcel which is similar to the environment at z1 starts rising, to height z=z1+ Δz, and when it rises it does not exchange energy with the surroundings, thus its temerature remains constant. At z1: ρ = ρ E (z1), T=T E (z1) At z: ρ = ρ E (z1), T=T E (z1) but ρ E = ρ E (z)= ρ E (z1)+ Δz dρ E /dz The arcel's buoyancy is: b(z)=-g(ρ ρ E )/ρ =g/ρ dρ E /dz Δz =g/ρ E(z1) dρ E /dz Δz The buoyancy is ostivie/negative/0 if dρ E /dz is ostivie/negative/0, and the arcel will rise more/sink back/remain still. For the equation of state above, b>0,=0,<0 if dt/dz <0, =0, >0. In the absence of heating and daming, a arcel will be unstable if the density increases with height. Mathematically: the equation of motion for the arcel's dislacement Δz: d (Δz)/dt =b= g/ρ E(z1) dρ E /dz Δz -N Δz N -b/δz =-g/ρ E(z1) dρ E /dz is the buoyancy frequency which we will return to later. if dρ E /dz>0, N <0 and the solution is exonential (instability): N t N t Δ z = Δ e + Δ e 1 If dρ E /dz<0, N >0 and the solution is oscillatory: Δ z = Δ1 cos( Nt) + Δ sin( Nt) We will discuss this case in a bit.

4 Energetics view: The energetics argument of the ball on the hill can't be alied to the arcel, because we are dealing with a continuous fluid, and when the arcel rises, another arcel has to go back down. Thus, we need to examine the initial and final states of the entire fluid, and see what haened to the otential energy: Lets assume the erturbations occurs with a arcel at z1 rising to z, while a arcel at z descends to z1 and besides that all the fluid remains unchanged. The initial otential energy: PE initial =g(ρ 1 z1+ ρ z). The final otential energy: PE final =g(ρ 1 z+ ρ z1) Their difference: PE final - PE initial =-g(ρ -ρ 1 )(z-z1) -g dρ E /dz (z-z1) This yields the same condition if dρ E /dz>0 the arcel's otential energy will be reduced, and its kinetic energy will increase, meaning it will continue moving. If dρ E /dz<0 the arcel's otential energy will increase, on exense of its kinetic energy, and the arcel will sto moving. Note: energetics considerations only show if instability is lausible, but we need an analysis like the one above to determine if instability will arise or not. Water heated from below: We assume a constant known heating rate er meter squared of H (W/m ). This heating will be carried uwards by convection, at a rate H. The heat content of a unit volume of fluid is: ρct where C is the secific heat of water. The heat flux (amount of heat transorted across a unit area) is then ρctw, where w is vertical velocity. W is highly variable in convection, hence we need to integrate over time (a few convective cycles) and sace (over a few convective cells). Assume that over the domain and some time, 1/ the fluid is moving uward with temerature T+ΔT, and half the fluid is moving downward with temerature T. The net integrated flux is: <H> = 1/ ρc(t+δt)w- 1/ ρctw=1/ ρcδt. How do we get w? from energy considerations: Assume all kinetic energy comes from release of otential energy: ΔKE = ΔPE= g Δρ Δz ΔKE= ρ / (u + v + w ) 3/ ρw w /3 g Δρ/ ρ Δz For the equation of state above: ρ ref =ρ(1- α[t-t ref ]), Δρ=ρ ref αδt Plugging in w, and then in <H> we get: <H>=1/ ρ ref C(/3 g αδz) 1/ ΔT 3/ Dry convection in a comressible atmoshere: We need to account for comression due to ressure changes as the arcels rise/descend. Assume that a arcel at z1 has the environmental ressure and temerature: = E (z1), T1=T E (z1), ρ1=/(rt1) The arcel rises to z adiabatically. Its ressure decreases like the environment. What haens to T? Consider a arcel of unit mass: ρv=1. Its exchange of energy with the surroundings follows the law:

5 δq= δu+ δw where δq is the heating from outside, δu is the added internal energy and δw is the work done by the arcel on its surroundings. δq= CvdT+dV where Cv is the secific heat er unit volume (choose this since if dv=0, all δq goes to a change in T. Want to find dt/, so change from dv to using the ideal gas law: dv=d(1/ρ)=-1/ρ dρ, dρ=/(rt)-/(rt )dt dv= -/(ρ RT) + /(ρ RT ) dt =RdT-/ρ δq= (Cv+R)dT-/ρ = CdT - /ρ Note: C>Cv, meaning temerature will change less for a given heating when ressure, rather than volume is ket constant. This is because some of the energy goes towards work due to volume changes. For adiabatic dislacements, δq=0, so CdT = /ρ Where the variables are taken to be the arcel's. From the hydrostatic relation, =-ρ E gdz, so dt/dz= - ρ E /ρ g/c For small dislacements, ρ ρ E, so that their ratio can be taken to be 1, and we get the dry adiabatic lase rate: Γd=-dT/dz=g/C For C=1005J/Kg/K, Γd 10K/km.

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 4

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 4 Atmoshere, Ocean and Climate Dynamics Answers to Chater 4 1. Show that the buoyancy frequency, Eq.(4.22), may be written in terms of the environmental temerature rofile thus N 2 = g µ dte T E dz + Γ d

More information

Ideal Gas Law. September 2, 2014

Ideal Gas Law. September 2, 2014 Ideal Gas Law Setember 2, 2014 Thermodynamics deals with internal transformations of the energy of a system and exchanges of energy between that system and its environment. A thermodynamic system refers

More information

GEF2200 vår 2017 Løsningsforslag sett 1

GEF2200 vår 2017 Løsningsforslag sett 1 GEF2200 vår 2017 Løsningsforslag sett 1 A.1.T R is the universal gas constant, with value 8.3143JK 1 mol 1. R is the gas constant for a secic gas, given by R R M (1) where M is the molecular weight of

More information

ONE. The Earth-atmosphere system CHAPTER

ONE. The Earth-atmosphere system CHAPTER CHAPTER ONE The Earth-atmoshere system 1.1 INTRODUCTION The Earth s atmoshere is the gaseous enveloe surrounding the lanet. Like other lanetary atmosheres, it figures centrally in transfers of energy between

More information

4. A Brief Review of Thermodynamics, Part 2

4. A Brief Review of Thermodynamics, Part 2 ATMOSPHERE OCEAN INTERACTIONS :: LECTURE NOTES 4. A Brief Review of Thermodynamics, Part 2 J. S. Wright jswright@tsinghua.edu.cn 4.1 OVERVIEW This chater continues our review of the key thermodynamics

More information

ATM The thermal wind Fall, 2016 Fovell

ATM The thermal wind Fall, 2016 Fovell ATM 316 - The thermal wind Fall, 2016 Fovell Reca and isobaric coordinates We have seen that for the synotic time and sace scales, the three leading terms in the horizontal equations of motion are du dt

More information

df da df = force on one side of da due to pressure

df da df = force on one side of da due to pressure I. Review of Fundamental Fluid Mechanics and Thermodynamics 1. 1 Some fundamental aerodynamic variables htt://en.wikiedia.org/wiki/hurricane_ivan_(2004) 1) Pressure: the normal force er unit area exerted

More information

Notes on pressure coordinates Robert Lindsay Korty October 1, 2002

Notes on pressure coordinates Robert Lindsay Korty October 1, 2002 Notes on ressure coordinates Robert Lindsay Korty October 1, 2002 Obviously, it makes no difference whether the quasi-geostrohic equations are hrased in height coordinates (where x, y,, t are the indeendent

More information

6.7 Thermal wind in pressure coordinates

6.7 Thermal wind in pressure coordinates 176 CHAPTER 6. THE EQUATIONS OF FLUID MOTION 6.7 Thermal wind in ressure coordinates The thermal wind relation aroriate to the atmoshere is untidy when exressed with height as a vertical coordinate (because

More information

1. Read the section on stability in Wallace and Hobbs. W&H 3.53

1. Read the section on stability in Wallace and Hobbs. W&H 3.53 Assignment 2 Due Set 5. Questions marked? are otential candidates for resentation 1. Read the section on stability in Wallace and Hobbs. W&H 3.53 2.? Within the context of the Figure, and the 1st law of

More information

ESCI 342 Atmospheric Dynamics I Lesson 10 Vertical Motion, Pressure Coordinates

ESCI 342 Atmospheric Dynamics I Lesson 10 Vertical Motion, Pressure Coordinates Reading: Martin, Section 4.1 PRESSURE COORDINATES ESCI 342 Atmosheric Dynamics I Lesson 10 Vertical Motion, Pressure Coordinates Pressure is often a convenient vertical coordinate to use in lace of altitude.

More information

PHYS1001 PHYSICS 1 REGULAR Module 2 Thermal Physics Chapter 17 First Law of Thermodynamics

PHYS1001 PHYSICS 1 REGULAR Module 2 Thermal Physics Chapter 17 First Law of Thermodynamics PHYS1001 PHYSICS 1 REGULAR Module Thermal Physics Chater 17 First Law of Thermodynamics References: 17.1 to 17.9 Examles: 17.1 to 17.7 Checklist Thermodynamic system collection of objects and fields. If

More information

Weather and Climate Laboratory Spring 2009

Weather and Climate Laboratory Spring 2009 MIT OenCourseWare htt://ocw.mit.edu 12.307 Weather and Climate Laboratory Sring 2009 For information about citing these materials or our Terms of Use, visit: htt://ocw.mit.edu/terms. Thermal wind John

More information

Equilibrium Thermodynamics

Equilibrium Thermodynamics Part I Equilibrium hermodynamics 1 Molecular hermodynamics Perhas the most basic equation in atmosheric thermodynamics is the ideal gas law = rr where is ressure, r is the air density, is temerature, and

More information

ATMOS Lecture 7. The First Law and Its Consequences Pressure-Volume Work Internal Energy Heat Capacity Special Cases of the First Law

ATMOS Lecture 7. The First Law and Its Consequences Pressure-Volume Work Internal Energy Heat Capacity Special Cases of the First Law TMOS 5130 Lecture 7 The First Law and Its Consequences Pressure-Volume Work Internal Energy Heat Caacity Secial Cases of the First Law Pressure-Volume Work Exanding Volume Pressure δw = f & dx δw = F ds

More information

Project 3 Convection and Atmospheric Thermodynamics

Project 3 Convection and Atmospheric Thermodynamics 12.818 Project 3 Convection and Atmospheric Thermodynamics Lodovica Illari 1 Background The Earth is bathed in radiation from the Sun whose intensity peaks in the visible. In order to maintain energy balance

More information

Where: Where: f Wave s frequency (Hz) c Speed of light ( ms -1 ) Wavelength (m)

Where: Where: f Wave s frequency (Hz) c Speed of light ( ms -1 ) Wavelength (m) in a direction to both of the fields as shown in Figure 1. In wave model, the electromagnetic radiation is commonly associated with wavelength and frequency, exressed mathematically as: c f...(1) f Wave

More information

Theory of turbomachinery. Chapter 1

Theory of turbomachinery. Chapter 1 Theory of turbomachinery Chater Introduction: Basic Princiles Take your choice of those that can best aid your action. (Shakeseare, Coriolanus) Introduction Definition Turbomachinery describes machines

More information

12.808: Some Physical Properties of Sea Water or, More than you ever wanted to know about the basic state variables of the ocean

12.808: Some Physical Properties of Sea Water or, More than you ever wanted to know about the basic state variables of the ocean 12.88: Some Physical Proerties of Sea Water or, More than you ever wanted to know about the basic state variables of the ocean Salinity Various salt constituents in 1 m 3 of seawater having (t, S) = (2,

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

Conservation of Energy Thermodynamic Energy Equation

Conservation of Energy Thermodynamic Energy Equation Conseration of Energy Thermodynamic Energy Equation The reious two sections dealt with conseration of momentum (equations of motion) and the conseration of mass (continuity equation). This section addresses

More information

The Role of Water Vapor. atmosphere (we will ignore the solid phase here) Refer to the phase diagram in the web notes.

The Role of Water Vapor. atmosphere (we will ignore the solid phase here) Refer to the phase diagram in the web notes. The Role of Water Vaor Water can exist as either a vaor or liquid in the atmoshere (we will ignore the solid hase here) under a variety of Temerature and ressure conditions. Refer to the hase diagram in

More information

Simplifications to Conservation Equations

Simplifications to Conservation Equations Chater 5 Simlifications to Conservation Equations 5.1 Steady Flow If fluid roerties at a oint in a field do not change with time, then they are a function of sace only. They are reresented by: ϕ = ϕq 1,

More information

ATMO 551a Moist Adiabat Fall Change in internal energy: ΔU

ATMO 551a Moist Adiabat Fall Change in internal energy: ΔU Enthalpy and the Moist Adiabat We have described the dry adiabat where an air parcel is lifted rapidly causing the air parcel to expand as the environmental pressure decreases and the air parcel does work

More information

Chapter 4. Convection

Chapter 4. Convection Chapter 4 Convection We learned in Chapters 2 and 3 that terrestrial radiation emanates to space primarily from the upper troposphere, rather than the ground; much of what radiates from the surface is

More information

2.6 Primitive equations and vertical coordinates

2.6 Primitive equations and vertical coordinates Chater 2. The continuous equations 2.6 Primitive equations and vertical coordinates As Charney (1951) foresaw, most NWP modelers went back to using the rimitive equations, with the hydrostatic aroximation,

More information

III. Flow Around Bends: Meander Evolution

III. Flow Around Bends: Meander Evolution III. Flow Around Bends: Meander Evolution 1. Introduction Hooke (1975) [aer available] first detailed data and measurements about what haens around meander bends how flow velocity and shear stress fields

More information

First law of thermodynamics (Jan 12, 2016) page 1/7. Here are some comments on the material in Thompkins Chapter 1

First law of thermodynamics (Jan 12, 2016) page 1/7. Here are some comments on the material in Thompkins Chapter 1 First law of thermodynamics (Jan 12, 2016) age 1/7 Here are some comments on the material in Thomkins Chater 1 1) Conservation of energy Adrian Thomkins (eq. 1.9) writes the first law as: du = d q d w

More information

Liquid water static energy page 1/8

Liquid water static energy page 1/8 Liquid water static energy age 1/8 1) Thermodynamics It s a good idea to work with thermodynamic variables that are conserved under a known set of conditions, since they can act as assive tracers and rovide

More information

Assignment Set 2 - Solutions Due: Wednesday October 6; 1:00 pm

Assignment Set 2 - Solutions Due: Wednesday October 6; 1:00 pm Assignments CE 312 Fluid Mechanics (Fall 21) Assignment Set 2 - s Due: Wednesday October 6; 1: m Question A (7 marks) Consider the situation in the Figure where you see a gate laced under an angle θ=1

More information

MET 4302 Midterm Study Guide 19FEB18

MET 4302 Midterm Study Guide 19FEB18 The exam will be 4% short answer and the remainder (6%) longer (1- aragrahs) answer roblems and mathematical derivations. The second section will consists of 6 questions worth 15 oints each. Answer 4.

More information

References: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr.

References: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr. References: ESCI 340 - Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr. DeCaria Glossary of Meteorology, 2nd ed., American Meteorological Society A Short Course in Cloud

More information

Atmospheric Dynamics: lecture 2

Atmospheric Dynamics: lecture 2 Atmospheric Dynamics: lecture 2 Topics Some aspects of advection and the Coriolis-effect (1.7) Composition of the atmosphere (figure 1.6) Equation of state (1.8&1.9) Water vapour in the atmosphere (1.10)

More information

CHAPTER 19. Fluid Instabilities. In this Chapter we discuss the following instabilities:

CHAPTER 19. Fluid Instabilities. In this Chapter we discuss the following instabilities: CHAPTER 19 Fluid Instabilities In this Chapter we discuss the following instabilities: convective instability (Schwarzschild criterion) interface instabilities (Rayleight Taylor & Kelvin-Helmholtz) gravitational

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

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

Day 3. Fluid Statics. - pressure - forces

Day 3. Fluid Statics. - pressure - forces Day 3 Fluid Statics - ressure - forces we define fluid article: small body of fluid with finite mass but negligible dimension (note: continuum mechanics must aly, so not too small) we consider a fluid

More information

Convection and buoyancy oscillation

Convection and buoyancy oscillation Convection and buoyancy oscillation Recap: We analyzed the static stability of a vertical profile by the "parcel method"; For a given environmental profile (of T 0, p 0, θ 0, etc.), if the density of an

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

Linear Transport Relations (LTR)

Linear Transport Relations (LTR) Linear Transport Relations (LTR) Much of Transport Phenomena deals with the exchange of momentum, mass, or heat between two (or many) objects. Often, the most mathematically simple way to consider how

More information

dn i where we have used the Gibbs equation for the Gibbs energy and the definition of chemical potential

dn i where we have used the Gibbs equation for the Gibbs energy and the definition of chemical potential Chem 467 Sulement to Lectures 33 Phase Equilibrium Chemical Potential Revisited We introduced the chemical otential as the conjugate variable to amount. Briefly reviewing, the total Gibbs energy of a system

More information

The standard atmosphere I

The standard atmosphere I The standard atmoshere I Introduction to eronautical Engineering Prof. dr. ir. Jacco Hoekstra M.T. Salam - CC - BY - S Joe Kittinger ugust 16 th, 1960 31 333 m Felix Baumgartner October 14 th, 2012 38

More information

COMPENDIUM OF EQUATIONS Unified Engineering Thermodynamics

COMPENDIUM OF EQUATIONS Unified Engineering Thermodynamics COMPENDIUM OF EQUAIONS Unified Engineering hermodynamics Note: It is with some reseration that I suly this comendium of equations. One of the common itfalls for engineering students is that they sole roblems

More information

Week 8 lectures. ρ t +u ρ+ρ u = 0. where µ and λ are viscosity and second viscosity coefficients, respectively and S is the strain tensor:

Week 8 lectures. ρ t +u ρ+ρ u = 0. where µ and λ are viscosity and second viscosity coefficients, respectively and S is the strain tensor: Week 8 lectures. Equations for motion of fluid without incomressible assumtions Recall from week notes, the equations for conservation of mass and momentum, derived generally without any incomressibility

More information

THE FIRST LAW OF THERMODYNAMICS

THE FIRST LAW OF THERMODYNAMICS THE FIRST LA OF THERMODYNAMIS 9 9 (a) IDENTIFY and SET UP: The ressure is constant and the volume increases (b) = d Figure 9 Since is constant, = d = ( ) The -diagram is sketched in Figure 9 The roblem

More information

Useful concepts associated with the Bernoulli equation. Dynamic

Useful concepts associated with the Bernoulli equation. Dynamic Useful concets associated with the Bernoulli equation - Static, Stagnation, and Dynamic Pressures Bernoulli eq. along a streamline + ρ v + γ z = constant (Unit of Pressure Static (Thermodynamic Dynamic

More information

Dynamic Meteorology: lecture 2

Dynamic Meteorology: lecture 2 Dynamic Meteorology: lecture 2 Sections 1.3-1.5 and Box 1.5 Potential temperature Radiatively determined temperature (boxes 1.1-1.4) Buoyancy (-oscillations) and static instability, Brunt-Vaisala frequency

More information

ATMO 551a Fall The Carnot Cycle

ATMO 551a Fall The Carnot Cycle What is a arnot ycle and Why do we care The arnot ycle arnot was a French engineer who was trying to understand how to extract usable mechanical work from a heat engine, that is an engine where a gas or

More information

ATMO/OPTI 656b Spring 09. Physical properties of the atmosphere

ATMO/OPTI 656b Spring 09. Physical properties of the atmosphere The vertical structure of the atmosphere. Physical properties of the atmosphere To first order, the gas pressure at the bottom of an atmospheric column balances the downward force of gravity on the column.

More information

Efficiencies. Damian Vogt Course MJ2429. Nomenclature. Symbol Denotation Unit c Flow speed m/s c p. pressure c v. Specific heat at constant J/kgK

Efficiencies. Damian Vogt Course MJ2429. Nomenclature. Symbol Denotation Unit c Flow speed m/s c p. pressure c v. Specific heat at constant J/kgK Turbomachinery Lecture Notes 1 7-9-1 Efficiencies Damian Vogt Course MJ49 Nomenclature Subscrits Symbol Denotation Unit c Flow seed m/s c Secific heat at constant J/kgK ressure c v Secific heat at constant

More information

Convection. If luminosity is transported by radiation, then it must obey

Convection. If luminosity is transported by radiation, then it must obey Convection If luminosity is transported by radiation, then it must obey L r = 16πacr 2 T 3 3ρκ R In a steady state, the energy transported per time at radius r must be equal to the energy generation rate

More information

Lecture contents. Metals: Drude model Conductivity frequency dependence Plasma waves Difficulties of classical free electron model

Lecture contents. Metals: Drude model Conductivity frequency dependence Plasma waves Difficulties of classical free electron model Lecture contents Metals: Drude model Conductivity frequency deendence Plasma waves Difficulties of classical free electron model Paul Karl Ludwig Drude (German: [ˈdʀuːdə]; July, 863 July 5, 96) Phenomenology

More information

f self = 1/T self (b) With revolution, rotaton period T rot in second and the frequency Ω rot are T yr T yr + T day T rot = T self > f self

f self = 1/T self (b) With revolution, rotaton period T rot in second and the frequency Ω rot are T yr T yr + T day T rot = T self > f self Problem : Units : Q-a Mathematically exress the relationshi between the different units of the hysical variables: i) Temerature: ) Fahrenheit and Celsius; 2) Fahrenheit and Kelvin ii) Length: ) foot and

More information

PHYS 432 Physics of Fluids: Instabilities

PHYS 432 Physics of Fluids: Instabilities PHYS 432 Physics of Fluids: Instabilities 1. Internal gravity waves Background state being perturbed: A stratified fluid in hydrostatic balance. It can be constant density like the ocean or compressible

More information

1 atm = 1.01x10 Pa = 760 Torr = 14.7 lb / in

1 atm = 1.01x10 Pa = 760 Torr = 14.7 lb / in Last class we began discussion of ressure in fluids, with ressure defined as, F = ; units N 1 Pa = 1 m 2 There are a number of other ressure units in common use having the following equivalence, 5 2 1

More information

Synoptic Meteorology I: The Geostrophic Approximation. 30 September, 7 October 2014

Synoptic Meteorology I: The Geostrophic Approximation. 30 September, 7 October 2014 The Equations of Motion Synotic Meteorology I: The Geostrohic Aroimation 30 Setember, 7 October 2014 In their most general form, and resented without formal derivation, the equations of motion alicable

More information

Lecture 3: Convection

Lecture 3: Convection EESC V2100 The Climate System spring 2004 Lecture 3: Convection Yochanan Kushnir Lamont Doherty Earth Observatory of Columbia University Palisades, NY 10964, USA kushnir@ldeo.columbia.edu Layers of the

More information

Phase transition. Asaf Pe er Background

Phase transition. Asaf Pe er Background Phase transition Asaf Pe er 1 November 18, 2013 1. Background A hase is a region of sace, throughout which all hysical roerties (density, magnetization, etc.) of a material (or thermodynamic system) are

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 28: Kinetics of Oxidation of Metals: Part 1: rusting, corrosion, and

Lecture 28: Kinetics of Oxidation of Metals: Part 1: rusting, corrosion, and Lecture 8: Kinetics of xidation of etals: Part 1: rusting, corrosion, and the surface rotection, all about chemistry Today s toics hemical rocesses of oxidation of metals: the role layed by oxygen. How

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

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 1 Fundamentals

Chapter 1 Fundamentals Chater Fundamentals. Overview of Thermodynamics Industrial Revolution brought in large scale automation of many tedious tasks which were earlier being erformed through manual or animal labour. Inventors

More information

1. Static Stability. (ρ V ) d2 z (1) d 2 z. = g (2) = g (3) T T = g T (4)

1. Static Stability. (ρ V ) d2 z (1) d 2 z. = g (2) = g (3) T T = g T (4) NCAR (National Center for Atmospheric Research) has an excellent resource for education called COMET-MetEd. There you can find some really great tutorials on SkewT-LogP plots: visit http://www.meted.ucar.edu/mesoprim/skewt/index.htm.

More information

Chapter 7 Energy Principle

Chapter 7 Energy Principle Chater 7: Energy Princile By Dr Ali Jawarneh Hashemite University Outline In this chater we will: Derive and analyse the Energy equation. Analyse the flow and shaft work. Derive the equation for steady

More information

ATMOS 5130 Lecture 9. Enthalpy Conservation Property The Second Law and Its Consequences Entropy

ATMOS 5130 Lecture 9. Enthalpy Conservation Property The Second Law and Its Consequences Entropy ATMOS 5130 Lecture 9 Enthalpy Conservation Property The Second Law and Its Consequences Entropy CLASS Presentation Form group of 2 students Present ~20 minute presentation (~ 10 minute each person) Focus

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

df dz = dp dt Essentially, this is just a statement of the first law in one of the forms we derived earlier (expressed here in W m 3 ) dq p dt dp

df dz = dp dt Essentially, this is just a statement of the first law in one of the forms we derived earlier (expressed here in W m 3 ) dq p dt dp A problem with using entropy as a variable is that it is not a particularly intuitive concept. The mechanics of using entropy for evaluating system evolution is well developed, but it sometimes feels a

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

3 Hydrostatic Equilibrium

3 Hydrostatic Equilibrium 3 Hydrostatic Equilibrium Reading: Shu, ch 5, ch 8 31 Timescales and Quasi-Hydrostatic Equilibrium Consider a gas obeying the Euler equations: Dρ Dt = ρ u, D u Dt = g 1 ρ P, Dɛ Dt = P ρ u + Γ Λ ρ Suppose

More information

Scale analysis of the vertical equation of motion:

Scale analysis of the vertical equation of motion: 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

More information

Hypersonic flow: introduction

Hypersonic flow: introduction Hyersonic flow: introduction Van Dyke: Hyersonic flow is flow ast a body at high ach number, where nonlinearity is an essential feature of the flow. Also understood, for thin bodies, that if is the thickness-to-chord

More information

The thermal wind 1. v g

The thermal wind 1. v g The thermal win The thermal win Introuction The geostrohic win is etermine by the graient of the isobars (on a horizontal surface) or isohyses (on a ressure surface). On a ressure surface the graient of

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

rate~ If no additional source of holes were present, the excess

rate~ If no additional source of holes were present, the excess DIFFUSION OF CARRIERS Diffusion currents are resent in semiconductor devices which generate a satially non-uniform distribution of carriers. The most imortant examles are the -n junction and the biolar

More information

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu Lecture 2: Basic Conservation Laws Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis Conservation Law of Momentum Newton s 2 nd Law of Momentum = absolute velocity viewed

More information

AE301 Aerodynamics I UNIT A: Fundamental Concepts

AE301 Aerodynamics I UNIT A: Fundamental Concepts AE301 Aerodynamics I UNIT A: Fundamental Concets ROAD MAP... A-1: Engineering Fundamentals Reiew A-: Standard Atmoshere A-3: Goerning Equations of Aerodynamics A-4: Airseed Measurements A-5: Aerodynamic

More information

CHAPTER 2 Fluid Statics

CHAPTER 2 Fluid Statics Chater / Fluid Statics CHAPTER Fluid Statics FE-tye Exam Review Problems: Problems - to -9. (C) h (.6 98) (8.5.54) 96 6 Pa Hg. (D) gh 84. 9.8 4 44 76 Pa. (C) h h. 98. 8 Pa w atm x x water w.4 (A) H (.6

More information

Lecture 13 HYDRAULIC ACTUATORS[CONTINUED]

Lecture 13 HYDRAULIC ACTUATORS[CONTINUED] Lecture 1 HYDRAULIC ACTUATORS[CONTINUED] 1.5Acceleration and Deceleration of Cylinder Loads Cylinders are subjected to acceleration and deceleration during their oeration. Cylinders are decelerated to

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

Buoyancy and Coriolis forces

Buoyancy and Coriolis forces Chapter 2 Buoyancy and Coriolis forces In this chapter we address several topics that we need to understand before starting on our study of geophysical uid dynamics. 2.1 Hydrostatic approximation Consider

More information

The Second Law: The Machinery

The Second Law: The Machinery The Second Law: The Machinery Chater 5 of Atkins: The Second Law: The Concets Sections 3.7-3.9 8th Ed, 3.3 9th Ed; 3.4 10 Ed.; 3E 11th Ed. Combining First and Second Laws Proerties of the Internal Energy

More information

What did we learn in Ch. 1? Energy Transfers Link Ch What did we learn in Ch. 3? What did we learn in Ch. 4? Key Combined 1 st +2 nd Law Results

What did we learn in Ch. 1? Energy Transfers Link Ch What did we learn in Ch. 3? What did we learn in Ch. 4? Key Combined 1 st +2 nd Law Results Energy ransfers Link Ch. - Ch. Atmosheric Comosition dry air (N, O, Ar, CO ), Water, (articles) Ch. First and Second Laws Energy Balance (System/Environment) Ch. 3 Stefan-Boltzmann Equation Kirchoff s

More information

13.7 Power Applied by a Constant Force

13.7 Power Applied by a Constant Force 13.7 Power Applied by a Constant Force Suppose that an applied force F a acts on a body during a time interval Δt, and the displacement of the point of application of the force is in the x -direction by

More information

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 8

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 8 Atmosphere, Ocean and Climate Dynamics Answers to Chapter 8 1. Consider a zonally symmetric circulation (i.e., one with no longitudinal variations) in the atmosphere. In the inviscid upper troposphere,

More information

Fluid Dynamics. Type of Flows Continuity Equation Bernoulli Equation Steady Flow Energy Equation Applications of Bernoulli Equation

Fluid Dynamics. Type of Flows Continuity Equation Bernoulli Equation Steady Flow Energy Equation Applications of Bernoulli Equation Tye of Flows Continity Eqation Bernolli Eqation Steady Flow Energy Eqation Alications of Bernolli Eqation Flid Dynamics Streamlines Lines having the direction of the flid velocity Flids cannot cross a

More information

On Gravity Waves on the Surface of Tangential Discontinuity

On Gravity Waves on the Surface of Tangential Discontinuity Alied Physics Research; Vol. 6, No. ; 4 ISSN 96-9639 E-ISSN 96-9647 Published by anadian enter of Science and Education On Gravity Waves on the Surface of Tangential Discontinuity V. G. Kirtskhalia I.

More information

Study of the circulation theory of the cooling system in vertical evaporative cooling generator

Study of the circulation theory of the cooling system in vertical evaporative cooling generator 358 Science in China: Series E Technological Sciences 006 Vol.49 No.3 358 364 DOI: 10.1007/s11431-006-0358-1 Study of the circulation theory of the cooling system in vertical evaorative cooling generator

More information

5. PRESSURE AND VELOCITY SPRING Each component of momentum satisfies its own scalar-transport equation. For one cell:

5. PRESSURE AND VELOCITY SPRING Each component of momentum satisfies its own scalar-transport equation. For one cell: 5. PRESSURE AND VELOCITY SPRING 2019 5.1 The momentum equation 5.2 Pressure-velocity couling 5.3 Pressure-correction methods Summary References Examles 5.1 The Momentum Equation Each comonent of momentum

More information

Temperature and Thermodynamics, Part II. Topics to be Covered

Temperature and Thermodynamics, Part II. Topics to be Covered Teperature and Therodynaics, Part II Topics to be Covered Profiles of Teperature in the Boundary Layer Potential teperature Adiabatic Lapse Rate Theral Stratification 1/8/17 Why are We Interested in Theral

More information

FUGACITY. It is simply a measure of molar Gibbs energy of a real gas.

FUGACITY. It is simply a measure of molar Gibbs energy of a real gas. FUGACITY It is simly a measure of molar Gibbs energy of a real gas. Modifying the simle equation for the chemical otential of an ideal gas by introducing the concet of a fugacity (f). The fugacity is an

More information

The Realm of Hydrogeology

The Realm of Hydrogeology The Real of Hydrogeology In class exercise Stagnant Flow Plot hydraulic head and ressure vs. deth for (also indicate the hydrostatic line) Stagnant flow (no flow) Steady downward flow Steady uward flow

More information

Thermal wind and temperature perturbations

Thermal wind and temperature perturbations Thermal wind and temerature erturbations Robert Lindsay Korty Massachusetts Institute of Technology October 15, 2002 Following the work of Bretherton (1966), we showed in class that a boundary otential

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

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

Physics 556 Stellar Astrophysics Prof. James Buckley. Lecture 9 Energy Production and Scaling Laws

Physics 556 Stellar Astrophysics Prof. James Buckley. Lecture 9 Energy Production and Scaling Laws Physics 556 Stellar Astrophysics Prof. James Buckley Lecture 9 Energy Production and Scaling Laws Equations of Stellar Structure Hydrostatic Equilibrium : dp Mass Continuity : dm(r) dr (r) dr =4πr 2 ρ(r)

More information

The Tropical Atmosphere: Hurricane Incubator

The Tropical Atmosphere: Hurricane Incubator The Tropical Atmosphere: Hurricane Incubator Images from journals published by the American Meteorological Society are copyright AMS and used with permission. A One-Dimensional Description of the Tropical

More information

CHAPTER 2 Fluid Statics

CHAPTER 2 Fluid Statics Chater / Fluid Statics CHAPTER Fluid Statics FE-tye Exam Review Problems: Problems - to -9. (C) h (.6 98) (8.5.54) 96 6 Pa Hg. (D) gh 84. 9.8 4 44 76 Pa. (C) h h. 98. 8 Pa w atm x x water w.4 (A) H (.6

More information

4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017

4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017 4. Atmospheric transport Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017 Forces in the atmosphere: Gravity g Pressure-gradient ap = ( 1/ ρ ) dp / dx for x-direction (also y, z directions)

More information