Synoptic Meteorology I. Some Thermodynamic Concepts

Size: px
Start display at page:

Download "Synoptic Meteorology I. Some Thermodynamic Concepts"

Transcription

1 Synotic Meteoroloy I Some hermodynamic Concets

2 Geootential Heiht Geootential Heiht (h): the otential enery of a nit mass lifted from srface to. Φ d 0 -Since constant in the trooshere, we can write Φ Δ m m m 2 2 s s 2 J k We can now define eootential heiht!

3 Geootential Heiht h 1 Φ d (no nits) eootential meters (m) m 2 /s 2 m 2 s -2 denotes a otential enery Ultimately, h is emloyed to ensre NO v in horiontal flow.

4 Geootential Heiht Here s how it works: i. Earth is an oblate sheroid R R e R e > R

5 Geootential Heiht ii. As sch, increases as yo travel S -> N (yo re decreasin distance from the center of mass) iii. Frther, srfaces at a constant heiht above the earth (sea level) will also be misshaen. 10,000m 000m MS * So, ravity chanes, y on those srfaces!

6 Geootential Heiht lower over ole eootential srface srface A v hiher over eqator v On a srface, is not always a (arallel allel to local kˆ ) If we assme it is, then we se a v that does not oint to the center of Earth s mass. Doin so, artificially introdces an eqatorward acceleration, A v (Moral: Use h).

7 Geootential Heiht On a constant heiht srface (above MS) N 0 o 10,000m ole > eqator * is not always to (a ball on this srface tends to the eqator) On a eootential srface N 0 o Φ constant

8 Geootential Heiht On a eootential srface N 0oΦ constant ball is at rest eootential srface NO comonent of v actin alone the srface v does not affect horiontal flow On constant srfaces, we se lines of constant h (m), e.., 5640 m at 500 mb. A constant srface does not eqal a eootential srface, BU v is to each heiht line.

9 Geootential Heiht m ,021m 10,000m 9.78 o 9.84 o o Δ N h o m 9970m s ,000m m 10,000m 45 o Δ h ,000m s m 10,021m 0o Δ h ,000m s o o 9.79

10 Geostrohic Winds y f ρ 1 x f v ρ 1 - coordinates f Φ 1 v y f y f Φ 1 - coordinates x f x f v

11 Geostrohic Winds Qick Conversion Rle (or h) 1. relace 1/ρ with 2. exchane with (eometric heiht) or h (eootential heiht) *We se eootential heihts to et Δh more accrately from RAOBS. Δh R 9.8 v ln U eliminated variable, Δ R v ln U

12 Hysometric Eqation Derivin the hysometric eqation or thickness eqation assme a hydrostatic atmoshere ρ and introdce the eqation of state: ρ 1 R 2 Rd

13 Hysometric Eqation Now, sbstitte 2 into 1 R d R l d 1 Now, assme d R l d 1 d R l d d R ln

14 Hysometric Eqation [ ] ) ( ln ln R R d ) ( ln ln R R d ) ( ln R d R ) ( ln d R ) ( ln and that brins s to...

15 Hysometric Eqation R d Δ ln he Hysometric Eqation! Ex 1: 287 Δ J KK 9.81 km ks m 2 s 2 2 (269 K ) ln m 2 s m mb mb msl 297 (75 o F) (- 24 o F) 269.5

16 Hysometric Eqation Ex. 2: 287 Δ Δ J KK R d ln (285 K ) 1000 ln m s mb mb K K K 5779 km ks m s m known 500mb (1000mb) known

17 Hysometric Eqation Ex. 3: Δ R d Δ ln Δ R d R d e Δ 450 m,, ln e ( 450 ) ( 303 ) R Δ ha e ha d 954 ha known Δknown MS

18 Hysometric Eqation So Hysometric Eqation is Vital for: 1. Redcin Station ressre to sea level. 2. Determinin heihts of er-level ressre srfaces.

19 Hysometric Eqation *Crcial Qestion* Δ R d constant constant R d ln If we fix and, then Δ is deendent only on. Δ α

20 Hysometric Eqation cold 5160 thickness attern warm thickness stron radient of stron radient of r lare Δ

21 hickness and hermal Wind hickness and thermal wind: 1. hels exlain how winds chane in vertical 2. assmes eostrohic atmoshere tells s somethin abot vertical strctre of 3. tells s somethin abot vertical strctre of atmoshere

22 hickness and hermal Wind v v v V V - V V r V r V shear of V r eostrohic cold wind V r 1 kˆ V v R f d ln kˆ n- 3 n- 2 n-1 n warm thickness thermal wind blows ll to thickness contors

23 hickness and hermal Wind chanes in the wind in the vertical (vertical wind shear) α the mean thermal radient over the layer V r r V r V V r V r V r V V r

24 hickness and hermal Wind With mltile ressre levels: backin conterclockwise (cold air always to left) V v V300 cold V r V r 850 warm * backin with heiht mean layer V is casin cold advection

25 hickness and hermal Wind Veerin- clockwise chane of wind warm V v 850 r V cold V r 300 * veerin with heiht mean layer V is casin warm advection

26 otential emeratre Consider the First aw of hermo dh C d- α d 1 First aw states that, for a closed system, no heat may be added to/removed from a system (arcel). dh 0 C d α d 2 Now, eqation of state ives s ρr or ρ /R or α R/ 3

27 otential emeratre Sbstitte 3 into 2 to et C d R d Next, divide by to et C d R d d Now divide throh by C to et Rd J/k K C 1005 J/k K d Rd C d

28 otential emeratre We then et θ d Rd C 1000 d d θ tem at 1000mb Τ tem at some ressre level ln θ -ln Rd ln 1000 ln C ln θ Rd C ln 1000

29 otential emeratre ake exonent of both sides θ Rd C 1000 let θ 1000 Rd C θ κ 1000 θ otential tem. tem. a arcel will have if broht down to 1000mb from some level, havin some tem.,.

30 otential emeratre Examle θ 1000 κ Given, θ 28 o C301K, what will be at 850 mb? 301K K K 14.3oC

Synoptic Meterorology I. Some Thermodynamic Concepts

Synoptic Meterorology I. Some Thermodynamic Concepts Synotic Meteroroloy I Some hermoynamic Concets Geootential Heiht Geootential Heiht (h): the otential enery of a nit mass lifte from srface to. Φ 0 -Since constant in the trooshere, we can write Φ m m m

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

1 such that v k g. v g. u g

1 such that v k g. v g. u g Mesoscale Meteoroloy: Quasi-Geostrohic Theory 4, 6 February 7 Wait this is a mesoscale class why do we care about a tenet o synotic meteoroloy?? On the synotic-scale, scale analysis o the orcin terms in

More information

Comments on Vertical Vorticity Advection

Comments on Vertical Vorticity Advection Comments on Vertical Vorticity Advection It shold be fairly intitive that ositive maima in vertical vorticity are associated with cyclones, and ths ositive cyclonic vorticity advection might be a sefl

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

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

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

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

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

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

Hydrostatic Equation and Thermal Wind. Meteorology 411 Iowa State University Week 5 Bill Gallus

Hydrostatic Equation and Thermal Wind. Meteorology 411 Iowa State University Week 5 Bill Gallus Hydrostatic Equation and Thermal Wind Meteorology 411 Iowa State University Week 5 Bill Gallus Hydrostatic Equation In the atmosphere, vertical accelerations (dw/dt) are normally fairly small, and we can

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

Ground Rules. PC1221 Fundamentals of Physics I. Position and Displacement. Average Velocity. Lectures 7 and 8 Motion in Two Dimensions

Ground Rules. PC1221 Fundamentals of Physics I. Position and Displacement. Average Velocity. Lectures 7 and 8 Motion in Two Dimensions PC11 Fndamentals of Physics I Lectres 7 and 8 Motion in Two Dimensions A/Prof Tay Sen Chan 1 Grond Rles Switch off yor handphone and paer Switch off yor laptop compter and keep it No talkin while lectre

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

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

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

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

The homework problem (pucks_on_ice) illustrates several important points:

The homework problem (pucks_on_ice) illustrates several important points: Ekman laers, friction & eostrohic flow The homework roblem (ucks_on_ice) illustrates several imortant oints: 1. Particles move erendicular to the alied force, to the riht in the northern hemishere, to

More information

1. THE MOMENTUM EQUATIONS FOR SYNOPTIC-SCALE FLOW IN THE ROTATING COORDINATE SYSTEM

1. THE MOMENTUM EQUATIONS FOR SYNOPTIC-SCALE FLOW IN THE ROTATING COORDINATE SYSTEM NOTES FO THE THEOY OF WKD 35. THE MOMENTUM EQUATIONS FO SYNOPTIC-SCALE FLOW IN THE OTATING COODINATE SYSTEM Scalin o the momentm eqations or snotic scale circlation (>000km dimension) reslted in the elimination

More information

CC-32 Trigonometric Identities

CC-32 Trigonometric Identities CC-32 Common Core State Standards MACC.92.F-TF.3.8 Prove the Pythagorean identity sin2(x) + cos2(x) and se it to find sin(x), cos(x), or tan(x), given sin(x), cos(x), or tan(x), and the qadrant of the

More information

4 Primitive Equations

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

More information

STATIC, STAGNATION, AND DYNAMIC PRESSURES

STATIC, STAGNATION, AND DYNAMIC PRESSURES STATIC, STAGNATION, AND DYNAMIC PRESSURES Bernolli eqation is g constant In this eqation is called static ressre, becase it is the ressre that wold be measred by an instrment that is static with resect

More information

Chapter 2 Introduction to the Stiffness (Displacement) Method. The Stiffness (Displacement) Method

Chapter 2 Introduction to the Stiffness (Displacement) Method. The Stiffness (Displacement) Method CIVL 7/87 Chater - The Stiffness Method / Chater Introdction to the Stiffness (Dislacement) Method Learning Objectives To define the stiffness matrix To derive the stiffness matrix for a sring element

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

In the last lecture we have seen the electronic transitions and the vibrational structure of these electronic transitions.

In the last lecture we have seen the electronic transitions and the vibrational structure of these electronic transitions. Title: Term vales of the electronic states of the molecle Pae-1 In the beinnin of this modle, we have learnt the formation of the molecle from atoms. We have also learnt the moleclar orbital and the electronic

More information

A Simulation-based Spatial Decision Support System for a New Airborne Weather Data Acquisition System

A Simulation-based Spatial Decision Support System for a New Airborne Weather Data Acquisition System A Simlation-based Satial Decision Sort System for a New Airborne Weather Data Acqisition System Erol Ozan Deartment of Engineering Management Old Dominion University Norfol, VA 23529 Pal Kaffmann Deartment

More information

Chapter 6 Momentum Transfer in an External Laminar Boundary Layer

Chapter 6 Momentum Transfer in an External Laminar Boundary Layer 6. Similarit Soltions Chapter 6 Momentm Transfer in an Eternal Laminar Bondar Laer Consider a laminar incompressible bondar laer with constant properties. Assme the flow is stead and two-dimensional aligned

More information

The Vorticity Equation

The Vorticity Equation The Vorticit Eqation Potential orticit Circlation theorem is reall good Circlation theorem imlies a consered qantit dp dt 0 P g 2 PV or barotroic lid General orm o Ertel s otential orticit: P g const Consider

More information

Chapter 1: Differential Form of Basic Equations

Chapter 1: Differential Form of Basic Equations MEG 74 Energ and Variational Methods in Mechanics I Brendan J. O Toole, Ph.D. Associate Professor of Mechanical Engineering Howard R. Hghes College of Engineering Universit of Nevada Las Vegas TBE B- (7)

More information

Lecture 5. Differential Analysis of Fluid Flow Navier-Stockes equation

Lecture 5. Differential Analysis of Fluid Flow Navier-Stockes equation Lectre 5 Differential Analsis of Flid Flo Naier-Stockes eqation Differential analsis of Flid Flo The aim: to rodce differential eqation describing the motion of flid in detail Flid Element Kinematics An

More information

STEP Support Programme. STEP III Hyperbolic Functions: Solutions

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

More information

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

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

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

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

More information

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 atmosphere in motion: forces and wind. AT350 Ahrens Chapter 9

The atmosphere in motion: forces and wind. AT350 Ahrens Chapter 9 The atmosphere in motion: forces and wind AT350 Ahrens Chapter 9 Recall that Pressure is force per unit area Air pressure is determined by the weight of air above A change in pressure over some distance

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

5. The Bernoulli Equation

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

More information

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

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

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

L = 2 λ 2 = λ (1) In other words, the wavelength of the wave in question equals to the string length, PHY 309 L. Soltions for Problem set # 6. Textbook problem Q.20 at the end of chapter 5: For any standing wave on a string, the distance between neighboring nodes is λ/2, one half of the wavelength. The

More information

EE2 Mathematics : Functions of Multiple Variables

EE2 Mathematics : Functions of Multiple Variables EE2 Mathematics : Fnctions of Mltiple Variables http://www2.imperial.ac.k/ nsjones These notes are not identical word-for-word with m lectres which will be gien on the blackboard. Some of these notes ma

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

Geopotential tendency and vertical motion

Geopotential tendency and vertical motion Geopotential tendency and vertical motion Recall PV inversion Knowin the PV, we can estimate everythin else! (Temperature, wind, eopotential ) In QG, since the flow is eostrophic, we can obtain the wind

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

Rossby waves (waves in vorticity)

Rossby waves (waves in vorticity) Rossb waes (waes in orticit) Stationar (toograhicall orced) waes NCEP Reanalsis Z500 Janar mean 2 3 Vorticit eqation z w z w z w t 2 1 Change in relatie (ertical comonent o) orticit at a oint, Adection

More information

1 Differential Equations for Solid Mechanics

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

More information

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

OPTIMUM EXPRESSION FOR COMPUTATION OF THE GRAVITY FIELD OF A POLYHEDRAL BODY WITH LINEARLY INCREASING DENSITY 1

OPTIMUM EXPRESSION FOR COMPUTATION OF THE GRAVITY FIELD OF A POLYHEDRAL BODY WITH LINEARLY INCREASING DENSITY 1 OPTIMUM EXPRESSION FOR COMPUTATION OF THE GRAVITY FIEL OF A POLYHERAL BOY WITH LINEARLY INCREASING ENSITY 1 V. POHÁNKA2 Abstract The formla for the comptation of the gravity field of a polyhedral body

More information

Homework 1. System dynamics can be expressed in nonlinear state-space form as

Homework 1. System dynamics can be expressed in nonlinear state-space form as Hoework arane s eqation and soe iortant systes This Hoework irst ives an eale o indin the dynaics o a certain canonical syste, then asks yo to do the sae or two other canonical systes odelin Physical Systes

More information

= 0, no work has been added

= 0, no work has been added hater Practice Problems (P1) Enery Balance: Eqn 7 d u z u z u z m U m m Q + + + + + + & + + & lets lets E + S (P) closed system, no mass flow m & m& 0, valve stuck revent any steam from o m& 0, no chane

More information

STATISTICAL MECHANICS

STATISTICAL MECHANICS STATISTICAL MECHAICS PD Dr. Christian Holm PART Entropy and Temperature Fundamental assumption a closed system is equally likely to be in any of its accessible micro- states, and all accessible micro-

More information

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 3

Atmosphere, Ocean and Climate Dynamics Answers to Chapter 3 Atmosphere, Ocean and Climate Dynamics Answers to Chapter 3 1. Use the hydrostatic equation to show that the mass of a vertical column of air of unit cross-section, extendin from the round to reat heiht,

More information

2 Dynamical basics, part 1

2 Dynamical basics, part 1 Contents 1 Dynamical basics, art 1 3 1.1 What drives the atmosheric circulation?........................ 7 1.2 Conservation laws..................................... 8 1.3 Large-scale circulation: Basic

More information

ESCI 343 Atmospheric Dynamics II Lesson 1 Ageostrophic Wind

ESCI 343 Atmospheric Dynamics II Lesson 1 Ageostrophic Wind ESCI 343 Atmospheric Dynamics II Lesson 1 Aeostrophic Wind References: An Introduction to Dynamic Meteoroloy (3 rd edition), J.R. Holton THE QG MOMENTUM EQUATIONS The QG momentum equations are derived

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

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

DO NOT TURN OVER UNTIL TOLD TO BEGIN

DO NOT TURN OVER UNTIL TOLD TO BEGIN ame HEMIS o. For Internal Stdents of Royal Holloway DO OT TUR OVER UTIL TOLD TO BEGI EC5040 : ECOOMETRICS Mid-Term Examination o. Time Allowed: hor Answer All 4 qestions STATISTICAL TABLES ARE PROVIDED

More information

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

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

More information

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

(! g. + f ) Dt. $% (" g. + f ) + f

(! g. + f ) Dt. $% ( g. + f ) + f The QG Vorticity equation The complete derivation of the QG vorticity equation can be found in Chapter 6.2.. Please read this section and keep in mind that extra approximations have been made besides those

More information

By Dr. Salah Salman. Problem (1)

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

More information

Aorangi (Mt. Cook) we typically view the state of the troposphere on "isobaric surfaces" (surfaces of constant pressure) rather

Aorangi (Mt. Cook) we typically view the state of the troposphere on isobaric surfaces (surfaces of constant pressure) rather Ch3 (ctd.) EAS270_Ch3_BehaviourAtmos_B.odp JDW, EAS UAlberta, last mod. 19 Sept. 2016 Atmospheric "behaviour" Aorani (Mt. Cook) "ride" we typically view the state of the troposphere on "isobaric surfaces"

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

Motion in Two Dimension (Projectile Motion)

Motion in Two Dimension (Projectile Motion) Phsics Motion in Two Dimension (Projectile Motion) www.testprepkart.com Table of Content. Introdction.. Projectile. 3. Assmptions of projectile motion. 4. Principle of phsical independence of motions.

More information

Net Force on a Body Completely in a Fluid. Natural Convection Heat Transfer. Net Buoyancy Force and Temperature

Net Force on a Body Completely in a Fluid. Natural Convection Heat Transfer. Net Buoyancy Force and Temperature Natral Conection eat ranfer Net Force on a Bo Comletel in a Fli he net force alie to a bo comletel bmere in a fli i Bo F W F net bo bo boanc V bo fli fli V V bo bo W F boanc Fli q he bo can be a blk of

More information

Change of Variables. (f T) JT. f = U

Change of Variables. (f T) JT. f = U Change of Variables 4-5-8 The change of ariables formla for mltiple integrals is like -sbstittion for single-ariable integrals. I ll gie the general change of ariables formla first, and consider specific

More information

4 Exact laminar boundary layer solutions

4 Exact laminar boundary layer solutions 4 Eact laminar bondary layer soltions 4.1 Bondary layer on a flat plate (Blasis 1908 In Sec. 3, we derived the bondary layer eqations for 2D incompressible flow of constant viscosity past a weakly crved

More information

FEA Solution Procedure

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

More information

Physics 111 P 2 A = P 1. A + mg = P 1. A + ρ( AΔh)g. Wednesday, 8-9 pm in NSC 118/119 Sunday, 6:30-8 pm in CCLIR 468.

Physics 111 P 2 A = P 1. A + mg = P 1. A + ρ( AΔh)g. Wednesday, 8-9 pm in NSC 118/119 Sunday, 6:30-8 pm in CCLIR 468. ics Announcements day, ember 11, 011 C5: Fluids Pascal s Principle Archimede s Principle Fluid Flows Continuity Equation Bernoulli s Equation Toricelli s Theorem Wednesday, 8-9 pm in NSC 118/119 Sunday,

More information

Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 8: Lorenz Energy Cycle

Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 8: Lorenz Energy Cycle Course.8, General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 8: Lorenz Enery Cycle Enery Forms: As we saw in our discussion of the heat budet, the enery content of the atmosphere per

More information

5 Shallow water Q-G theory.

5 Shallow water Q-G theory. 5 Shallow water Q-G theory. So far we have discussed the fact that lare scale motions in the extra-tropical atmosphere are close to eostrophic balance i.e. the Rossby number is small. We have examined

More information

2.3. PBL Equations for Mean Flow and Their Applications

2.3. PBL Equations for Mean Flow and Their Applications .3. PBL Equations for Mean Flow and Their Applications Read Holton Section 5.3!.3.1. The PBL Momentum Equations We have derived the Reynolds averaed equations in the previous section, and they describe

More information

Modelling Turbulence Effect in Formation of Zonal Winds

Modelling Turbulence Effect in Formation of Zonal Winds The Oen Atmosheric Science Journal 8 49-55 49 Modelling Turbulence Effect in Formation of Zonal Winds Oen Access J. Heinloo and A. Toomuu * Marine Systems Institute Tallinn University of Technology Akadeemia

More information

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

PHYSICS 218 SOLUTION TO HW 8. Created: November 20, :15 pm Last updated: November 21, 2004

PHYSICS 218 SOLUTION TO HW 8. Created: November 20, :15 pm Last updated: November 21, 2004 Created: November 20, 2004 7:5 pm Last updated: November 2, 2004. Schroeder.6 (a) The three forces actin on the slab of thickness dz are ravity and the pressure from above and below. To achieve equilibrium

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

Geodesics as gravity

Geodesics as gravity Geodesics as ravity February 8, 05 It is not obvious that curvature can account for ravity. The orbitin path of a planet, for example, does not immediately seem to be the shortest path between points.

More information

Part 3. Atmospheric Thermodynamics The Gas Laws

Part 3. Atmospheric Thermodynamics The Gas Laws Part 3. Atmosheric Thermoynamics The Gas Laws Eq. of state V = mrt mass gas constant for 1 kg of a gas For ry air ρ = m/ = ρrt or α = RT where α = 1/ ρ = ρ R T, where R a R M * = uniersal gas constant

More information

Final Examination, MEA 443 Fall 2003, Lackmann

Final Examination, MEA 443 Fall 2003, Lackmann Place an X here to count it double! Name: Final Eamination, MEA 443 Fall 003, Lackmann If ou wish to have the final eam count double, and dro our lowest score in an of the three semester eams, mark an

More information

[ K] McAlpine, hmwk #5, ATMS 611. J.D. McAlpine ATMS 611 HMWK #5

[ K] McAlpine, hmwk #5, ATMS 611. J.D. McAlpine ATMS 611 HMWK #5 McAline, hmwk 5, ATMS 6 J.D. McAline ATMS 6 HMWK 5 3.43 Rainro evaorating (is 2 C) : 8 C, calculate mixing ratio of - sat. mixing ratio at 2 C is 8.7 g/kg (assume wet-bulb temerature) - L e = 2.25*0 6

More information

Propagation of error for multivariable function

Propagation of error for multivariable function Proagation o error or mltiariable nction No consider a mltiariable nction (,,, ). I measrements o,,,. All hae ncertaint,,,., ho ill this aect the ncertaint o the nction? L tet) o (Eqation (3.8) ± L ),...,,

More information

Turbulence and boundary layers

Turbulence and boundary layers Trblence and bondary layers Weather and trblence Big whorls hae little whorls which feed on the elocity; and little whorls hae lesser whorls and so on to iscosity Lewis Fry Richardson Momentm eqations

More information

Midterm Feb. 17, 2009 Physics 110B Secret No.=

Midterm Feb. 17, 2009 Physics 110B Secret No.= Midterm Feb. 17, 29 Physics 11B Secret No.= PROBLEM (1) (4 points) The radient operator = x i ê i transforms like a vector. Use ɛ ijk to prove that if B( r) = A( r), then B( r) =. B i = x i x i = x j =

More information

KINEMATICS PREVIOUS EAMCET BITS ENGINEERING PAPER

KINEMATICS PREVIOUS EAMCET BITS ENGINEERING PAPER KINEMATICS PREVIOUS EAMCET BITS ENGINEERING PAPER. A body is projected vertically upwards at time t = 0 and is seen at a heiht at time t and t seconds durin its fliht. The maximum heiht attained is [ =

More information

Reduction of over-determined systems of differential equations

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

More information

Multiplication and division. Explanation and worked examples. First, we ll look at work you should know at this level.

Multiplication and division. Explanation and worked examples. First, we ll look at work you should know at this level. x Mltilication and division Exlanation and worked examles Level First, we ll look at work yo shold know at this level. Work ot these mltilication and division sms: a) ) 96 c) 8 d) 6 Soltions: a) 9 6 Yo

More information

2E1252 Control Theory and Practice

2E1252 Control Theory and Practice 2E1252 Control Theory and Practice Lectre 11: Actator satration and anti wind-p Learning aims After this lectre, yo shold nderstand how satration can case controller states to wind p know how to modify

More information

Mechanics Cycle 3 Chapter 12++ Chapter 12++ Revisit Circular Motion

Mechanics Cycle 3 Chapter 12++ Chapter 12++ Revisit Circular Motion Chapter 12++ Revisit Circular Motion Revisit: Anular variables Second laws for radial and tanential acceleration Circular motion CM 2 nd aw with F net To-Do: Vertical circular motion in ravity Complete

More information

g L Simple Pendulum, cont Simple Pendulum Period of Simple Pendulum Equations of Motion for SHM: 4/8/16 k m

g L Simple Pendulum, cont Simple Pendulum Period of Simple Pendulum Equations of Motion for SHM: 4/8/16 k m Simple Pendulum The simple pendulum is another example of simple harmonic motion The force is the component of the weiht tanent to the path of motion F t = - m sin θ Simple Pendulum, cont In eneral, the

More information

u P(t) = P(x,y) r v t=0 4/4/2006 Motion ( F.Robilliard) 1

u P(t) = P(x,y) r v t=0 4/4/2006 Motion ( F.Robilliard) 1 y g j P(t) P(,y) r t0 i 4/4/006 Motion ( F.Robilliard) 1 Motion: We stdy in detail three cases of motion: 1. Motion in one dimension with constant acceleration niform linear motion.. Motion in two dimensions

More information

LECTURE NOTES - VI. Prof. Dr. Atıl BULU

LECTURE NOTES - VI. Prof. Dr. Atıl BULU LECTURE NOTES - VI «FLUID MECHANICS» Istanbl Technical Uniersit College of Ciil Engineering Ciil Engineering Deartment Hdralics Diision CHAPTER 6 TWO-DIMENSIONAL IDEAL FLOW 6. INTRODUCTION An ideal flid

More information

OSCILLATIONS

OSCILLATIONS OSCIAIONS Important Points:. Simple Harmonic Motion: a) he acceleration is directly proportional to the displacement of the body from the fixed point and it is always directed towards the fixed point in

More information

Lecture: Corporate Income Tax - Unlevered firms

Lecture: Corporate Income Tax - Unlevered firms Lectre: Corporate Income Tax - Unlevered firms Ltz Krschwitz & Andreas Löffler Disconted Cash Flow, Section 2.1, Otline 2.1 Unlevered firms Similar companies Notation 2.1.1 Valation eqation 2.1.2 Weak

More information

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

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

More information

ERTH 465 Fall Lab 3. Vertical Consistency and Analysis of Thickness

ERTH 465 Fall Lab 3. Vertical Consistency and Analysis of Thickness Name Date ERTH 465 Fall 2015 Lab 3 Vertical Consistency and Analysis of Thickness 1. All labs are to be kept in a three hole binder. Turn in the binder when you have finished the Lab. 2. Show all work

More information

Module 4. Analysis of Statically Indeterminate Structures by the Direct Stiffness Method. Version 2 CE IIT, Kharagpur

Module 4. Analysis of Statically Indeterminate Structures by the Direct Stiffness Method. Version 2 CE IIT, Kharagpur Modle Analysis of Statically Indeterminate Strctres by the Direct Stiffness Method Version CE IIT, Kharagr Lesson The Direct Stiffness Method: Trss Analysis (Contined) Version CE IIT, Kharagr Instrctional

More information

PhysicsAndMathsTutor.com

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

More information

Lesson 16 Electric Potential

Lesson 16 Electric Potential Physics 30 Lesson 16 Electric Potential I. Gravitational otential energy revisited There are many similarities between gravitational otential energy and electric otential energy. To hel us understand electric

More information