6.7 Thermal wind in pressure coordinates
|
|
- Egbert Montgomery
- 5 years ago
- Views:
Transcription
1 176 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 of ρ variations), but becomes simle when exressed in ressure coordinates.. To roceed in coordinates, we write the hydrostatic relation thus: z = 1 gρ. and take, for examle, the -derivative of the x-comonent of (6.58) yielding = g 2 z f y = g µ z = 1 µ 1. f y f y ρ Since 1/ρ = RT/, itsderivativeat constant ressure is µ 1 = R µ T, y ρ y whence = R µ T. (6.62) f y Similarly, for v we find v = R µ T. (6.63) f x Thus, horizontal gradients of temerature must be accomanied by vertical gradients of wind. (In height coordinates, one can obtain a similar relationshi, but it is a bit messier, because of the ρ factors in (6.57).) Eqs. (6.62) and (6.63) exress the thermal wind relationshi in ressure coordinates. To see how, consider Fig.(6.40). Suose, for simlicity, = 0 is constant at sea level (z =0), and that there is a monotonic decrease of temerature with y (so T/ y < 0) within the atmoshere. Then geostrohic balance tells us that u =0at z =0. Now, hydrostatic balance tells us that, at oints α and β aloft, the ressure is (x, y, z) = 0 g Z z 0 ρdz.
2 6.7. THERMAL WIND IN PRESSURE COORDINATES 177 Figure 6.40: Since beneath oint α (on the left) the air is warm and therefore light (low density), while is cold and dense beneath oint β, it follows that α > β. Aloft, therefore, there must be a geostrohic flow, out of the aer and therefore westerly (if we are in the northern hemishere), with low ressure on its left. Thus, a northward decrease of temerature imlies westerly winds increasing with height (i.e., / < 0), consistent with (6.62). In articular, if temerature decreases oleward (as we have seen it does), then T/ y < 0 in the northern hemishere, T/ y > 0 in the southern hemishere, so f 1 T/ y < 0 in both. Then (6.62) tells us that / < 0: so, with increasing height (decreasing ressure), winds must become increasingly eastward (westerly) in both hemisheres (see Fig.??) which is just what we observe in Fig Thermal wind exressed in terms of otential temerature The thermal wind can also be written in terms of otential temerature, θ, defined in eq(4.7) of chater 4. From eq(4.7) we note that: µ µ k µ T θ = y o y and so, for examle, eq(6.62) can be exressed thus:
3 178 CHAPTER 6. THE EQUATIONS OF FLUID MOTION Figure 6.41: = R T f θ µ θ = 1 y fρθ µ θ. (6.64) y (and similarly for v ) where the equation of state has been used. Thus the vertical (geostrohic) wind shear in ressure coordinates is directly roortional to the meridional gradient of θ on ressure surfaces. The connection between meridional otential temerature gradients and vertical wind shear is readily seen in the zonal-average climatology - see, for examle, fig.5.16 and fig.5.6. Be sure to check out that eq(6.64) also makes quantitative sense. The atmoshere is also close to thermal wind balance on the large scale at any instant. Fig.(6.42) lots the otential temerature on the 500mb surface on Nov 6th, 2001, zero hours GMT. Note the strong meridional gradients in middle latitudes associated with the jet stream. These gradients are also evident in fig.(6.43), a vertical cross section of otential temerature, θ, and zonal wind, u, through the atmoshere at 90 Wextendingfrom20 Nto70 N at the same time as in fig(6.42). The vertical coordinate is ressure. Note that, in accord with eq(6.64), the wind increases with height where θ surfaces sloe uward and decreases with height where θ surfaces sloe downwards. The vertical wind shear is very strong in regions where the θ surfaces steely sloe; the vertical wind shear is very weak where the θ surfaces are almost horizontal.
4 6.7. THERMAL WIND IN PRESSURE COORDINATES 179 Figure 6.42: The otential temerature, θ, on the 500mb surface on 6th November 2001 at 00 GMT.
5 180 CHAPTER 6. THE EQUATIONS OF FLUID MOTION Figure 6.43: A cross section of zonal wind, u, and otential temerature, θ, through the atmoshere at 90 W extending from 20 Nto70 Non6th November 2001 at 00 GMT.
6 6.7. THERMAL WIND IN PRESSURE COORDINATES 181 Summary of key equations 9 (x, y, z) ³ coordinates (x, y, z) ³ coordinates (x, y, ) ³ coordinates,,,, x y z x y z,, x y (incomressible - OCEAN) (com. erfect gas - ATMOS) Continuity: ρ t u =0 u =0 Hydrostatic balance z = gρ z = gρ z = 1 gρ Geostrohic balance fu = 1bz ρ fu = 1bz ρ fu =gbz z Thermal wind balance f z = gbz ρ f = R bz T 9 Note that (x, y, ) is not a right-handed coordinate system. So while bz is a unit vector oint toward increasing z, and therefore uward, bz is a unit vector oint toward decreasing and therefore also uward.
7 182 CHAPTER 6. THE EQUATIONS OF FLUID MOTION
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 informationATM 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 informationThermal 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 information2.6 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 informationMET 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 informationNotes 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 information2 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 informationLecture 1. Equations of motion - Newton s second law in three dimensions. Pressure gradient + force force
Lecture 3 Lecture 1 Basic dynamics Equations of motion - Newton s second law in three dimensions Acceleration = Pressure Coriolis + gravity + friction gradient + force force This set of equations is the
More informationR 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 informationESCI 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 informationBaroclinic flows can also support Rossby wave propagation. This is most easily
17. Quasi-geostrohic Rossby waves Baroclinic flows can also suort Rossby wave roagation. This is most easily described using quasi-geostrohic theory. We begin by looking at the behavior of small erturbations
More informationThe 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 informationAtmosphere, 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 informationGeneral Circulation. Nili Harnik DEES, Lamont-Doherty Earth Observatory
General Circulation Nili Harnik DEES, Lamont-Doherty Earth Observatory nili@ldeo.columbia.edu Latitudinal Radiation Imbalance The annual mean, averaged around latitude circles, of the balance between the
More informationLecture 25: Ocean circulation: inferences from geostrophic and thermal wind balance
Lecture 25: Ocean circulation: inferences from geostrophic and thermal wind balance November 5, 2003 Today we are going to study vertical sections through the ocean and discuss what we can learn about
More informationThe 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 informationConservation 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 informationAE301 Aerodynamics I UNIT A: Fundamental Concepts
AE3 Aerodynamics I UNIT A: Fundamental Concets ROAD MAP... A-: Engineering Fundamentals Review A-: Standard Atmoshere A-3: Governing Equations of Aerodynamics A-4: Airseed Measurements A-5: Aerodynamic
More informationf 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 informationSynoptic 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 information1 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 informationPhase 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 information4. 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 informationdn 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 informationIntroduction to Atmospheric Circulation
Introduction to Atmospheric Circulation Start rotating table Cloud Fraction Dice Results from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/
More informationWinds and Currents in the Oceans
Winds and Currents in the Oceans Atmospheric Processes Density of air is controlled by temperature, pressure, and moisture content. 1. Warm air is less dense than cold air and moist air is less dense than
More informationIdeal 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 informationAtmosphere, Ocean and Climate Dynamics Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 12.003 Atmosphere, Ocean and Climate Dynamics Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Problem
More informationUseful 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 informationAtmosphere, 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 informationSIO 210 Problem Set 3 November 15, 2013 Due Nov. 22, 2013 Answerkey
SIO 210 Problem Set 3 November 15, 2013 Due Nov. 22, 2013 Answerkey 1. Dynamics: rotation (a) Draw the direction of an inertial current in (i) the northern hemisphere and (ii) the southern hemisphere and
More informationWhere: 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 information1. 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 informationa) Derive general expressions for the stream function Ψ and the velocity potential function φ for the combined flow. [12 Marks]
Question 1 A horizontal irrotational flow system results from the combination of a free vortex, rotating anticlockwise, of strength K=πv θ r, located with its centre at the origin, with a uniform flow
More information1. 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 informationStatics and dynamics: some elementary concepts
1 Statics and dynamics: some elementary concets Dynamics is the study of the movement through time of variables such as heartbeat, temerature, secies oulation, voltage, roduction, emloyment, rices and
More informationHEAT, WORK, AND THE FIRST LAW OF THERMODYNAMICS
HET, ORK, ND THE FIRST L OF THERMODYNMIS 8 EXERISES Section 8. The First Law of Thermodynamics 5. INTERPRET e identify the system as the water in the insulated container. The roblem involves calculating
More informationProject 2 Fronts
12.307 Project 2 Fronts Lodovica Illari and John Marshall March 2010 Abstract We inspect fronts crossing the country associated with day-to-day variations in the weather using real-time atmospheric observations.
More informationAtmospheric Fronts. The material in this section is based largely on. Lectures on Dynamical Meteorology by Roger Smith.
Atmospheric Fronts The material in this section is based largely on Lectures on Dynamical Meteorology by Roger Smith. Atmospheric Fronts 2 Atmospheric Fronts A front is the sloping interfacial region of
More informationGEF2200 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 informationF = ma. ATS 150 Global Climate Change Winds and Weather. Scott Denning CSU CMMAP 1. Please read Chapter 6 from Archer Textbook
Winds and Weather Please read Chapter 6 from Archer Textbook Circulation of the atmosphere and oceans are driven by energy imbalances Energy Imbalances What Makes the Wind Blow? Three real forces (gravity,
More informationThe Planetary Circulation System
12 The Planetary Circulation System Learning Goals After studying this chapter, students should be able to: 1. describe and account for the global patterns of pressure, wind patterns and ocean currents
More informationLiquid 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 information9.3 Laminar Flat-Plate Boundary Layer: Exact Solution w-19
9.3 Laminar Flat-Plate Boundary Layer: Exact Solution w-19 Laminar Flat-Plate Boundary Layer: Exact Solution The solution for the laminar boundary layer on a horizontal flat late was obtained by Prtl s
More informationdf 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 informationExamples of Pressure Gradient. Pressure Gradient Force. Chapter 7: Forces and Force Balances. Forces that Affect Atmospheric Motion 2/2/2015
Chapter 7: Forces and Force Balances Forces that Affect Atmospheric Motion Fundamental force - Apparent force - Pressure gradient force Gravitational force Frictional force Centrifugal force Forces that
More informationThe Circulation of the Atmosphere:
The Circulation of the Atmosphere: Laboratory Experiments (see next slide) Fluid held in an annular container is at rest and is subjected to a temperature gradient. The less dense fluid near the warm wall
More informationNonlinear baroclinic dynamics of surface cyclones crossing a zonal jet
Nonlinear baroclinic dynamics of surface cyclones crossing a zonal jet Jean-Baptiste GILET, Matthieu Plu and Gwendal Rivière CNRM/GAME (Météo-France, CNRS) 3rd THORPEX International Science Symposium Monterey,
More informationFUGACITY. 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 informationGeostrophy & Thermal wind
Lecture 10 Geostrophy & Thermal wind 10.1 f and β planes These are planes that are tangent to the earth (taken to be spherical) at a point of interest. The z ais is perpendicular to the plane (anti-parallel
More informationTransient and Eddy. Transient/Eddy Flux. Flux Components. Lecture 3: Weather/Disturbance. Transient: deviations from time mean Time Mean
Lecture 3: Weather/Disturbance Transients and Eddies Climate Roles Mid-Latitude Cyclones Tropical Hurricanes Mid-Ocean Eddies Transient and Eddy Transient: deviations from time mean Time Mean Eddy: deviations
More informationSynoptic Meteorology I. Some Thermodynamic Concepts
Synotic Meteoroloy I Some hermodynamic Concets 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
More informationChapter 6. Thermodynamics and the Equations of Motion
Chater 6 hermodynamics and the Equations of Motion 6.1 he first law of thermodynamics for a fluid and the equation of state. We noted in chater 4 that the full formulation of the equations of motion required
More informationThe Behaviour of the Atmosphere
3 The Behaviour of the Atmosphere Learning Goals After studying this chapter, students should be able to: apply the ideal gas law and the concept of hydrostatic balance to the atmosphere (pp. 49 54); apply
More informationMixing and Available Potential Energy in a Boussinesq Ocean*
APRIL 998 HUANG 669 Mixing and Available Potential Energy in a Boussinesq Ocean* RUI XIN HUANG Deartment of Physical Oceanograhy, Woods Hole Oceanograhic Institution, Woods Hole, Massachussetts (Manuscrit
More informationOcean Currents and Climate
Ocean Currents and Climate Ocean water contains streamlike movements of water called ocean currents. Currents are influenced by a number of factors, including weather, the Earth's rotation, and the position
More informationLecture 12: Angular Momentum and the Hadley Circulation
Lecture 12: Angular Momentum and the Hadley Circulation September 30, 2003 We learnt last time that there is a planetary radiative drive net warming in the tropics, cooling over the pole which induces
More informationChapter 5 Mass, Momentum, and Energy Equations
57:00 Mechanics of Fluids and Transort Processes Chater 5 Professor Fred Stern Fall 006 Chater 5 Mass, Momentum, and Energy Equations Flow Rate and Conservation of Mass. cross-sectional area oriented normal
More informationChapter 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 informationAtmospheric Pressure and Wind Frode Stordal, University of Oslo
Chapter 4 Lecture Understanding Weather and Climate Seventh Edition Atmospheric Pressure and Wind Frode Stordal, University of Oslo Redina L. Herman Western Illinois University The Concept of Pressure
More informationEvidence Linking Arctic Amplification with Changing Weather Patterns in Mid-Latitudes
Evidence Linking Arctic Amplification with Changing Weather Patterns in Mid-Latitudes Jennifer Francis Institute of Marine and Coastal Sciences Rutgers, the State University of New Jersey Steve Vavrus
More informationThe dynamics of high and low pressure systems
The dynamics of high and low pressure systems Newton s second law for a parcel of air in an inertial coordinate system (a coordinate system in which the coordinate axes do not change direction and are
More informationIII. 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 informationHydrostatic 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 informationSimplifications 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 informationThe 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 informationLecture 2. Lecture 1. Forces on a rotating planet. We will describe the atmosphere and ocean in terms of their:
Lecture 2 Lecture 1 Forces on a rotating planet We will describe the atmosphere and ocean in terms of their: velocity u = (u,v,w) pressure P density ρ temperature T salinity S up For convenience, we will
More informationGeneral Atmospheric Circulation
General Atmospheric Circulation Take away Concepts and Ideas Global circulation: The mean meridional (N-S) circulation Trade winds and westerlies The Jet Stream Earth s climate zones Monsoonal climate
More informationONE. 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 informationFundamental Meteo Concepts
Fundamental Meteo Concepts Atmos 5110 Synoptic Dynamic Meteorology I Instructor: Jim Steenburgh jim.steenburgh@utah.edu 801-581-8727 Suite 480/Office 488 INSCC Suggested reading: Lackmann (2011), sections
More informationChapter 10: Flow Flow in in Conduits Conduits Dr Ali Jawarneh
Chater 10: Flow in Conduits By Dr Ali Jawarneh Hashemite University 1 Outline In this chater we will: Analyse the shear stress distribution across a ie section. Discuss and analyse the case of laminar
More informationWinds and Global Circulation
Winds and Global Circulation Atmospheric Pressure Winds Global Wind and Pressure Patterns Oceans and Ocean Currents El Nino How is Energy Transported to its escape zones? Both atmospheric and ocean transport
More information2. Meridional atmospheric structure; heat and water transport. Recall that the most primitive equilibrium climate model can be written
2. Meridional atmospheric structure; heat and water transport The equator-to-pole temperature difference DT was stronger during the last glacial maximum, with polar temperatures down by at least twice
More informationAE301 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 informationLecture 14. Equations of Motion Currents With Friction Sverdrup, Stommel, and Munk Solutions Remember that Ekman's solution for wind-induced transport
Lecture 14. Equations of Motion Currents With Friction Sverdrup, Stommel, and Munk Solutions Remember that Ekman's solution for wind-induced transport is which can also be written as (14.1) i.e., #Q x,y
More informationLecture 8. Lecture 1. Wind-driven gyres. Ekman transport and Ekman pumping in a typical ocean basin. VEk
Lecture 8 Lecture 1 Wind-driven gyres Ekman transport and Ekman pumping in a typical ocean basin. VEk wek > 0 VEk wek < 0 VEk 1 8.1 Vorticity and circulation The vorticity of a parcel is a measure of its
More informationTransient/Eddy Flux. Transient and Eddy. Flux Components. Lecture 7: Disturbance (Outline) Why transients/eddies matter to zonal and time means?
Lecture 7: Disturbance (Outline) Transients and Eddies Climate Roles Mid-Latitude Cyclones Tropical Hurricanes Mid-Ocean Eddies (From Weather & Climate) Flux Components (1) (2) (3) Three components contribute
More informationSurface Circulation. Key Ideas
Surface Circulation The westerlies and the trade winds are two of the winds that drive the ocean s surface currents. 1 Key Ideas Ocean water circulates in currents. Surface currents are caused mainly by
More informationModelling 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 informationTHE 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 informationLecture 10 March 15, 2010, Monday. Atmospheric Pressure & Wind: Part 1
Lecture 10 March 15, 2010, Monday Atmospheric Pressure & Wind: Part 1 Speed, Velocity, Acceleration, Force, Pressure Atmospheric Pressure & Its Measurement Ideal Gas Law (Equation of State) Pressure Gradient
More information3. Midlatitude Storm Tracks and the North Atlantic Oscillation
3. Midlatitude Storm Tracks and the North Atlantic Oscillation Copyright 2006 Emily Shuckburgh, University of Cambridge. Not to be quoted or reproduced without permission. EFS 3/1 Review of key results
More informationAn-Najah National University Civil Engineering Departemnt. Fluid Mechanics. Chapter [2] Fluid Statics
An-Najah National University Civil Engineering Deartemnt Fluid Mechanics Chater [2] Fluid Statics 1 Fluid Statics Problems Fluid statics refers to the study of fluids at rest or moving in such a manner
More informationQuiz 2 Review Questions
Quiz 2 Review Questions Chapter 7 Lectures: Winds and Global Winds and Global Winds cont 1) What is the thermal circulation (thermal wind) and how does it form? When we have this type of circulation, how
More informationFE FORMULATIONS FOR PLASTICITY
G These slides are designed based on the book: Finite Elements in Plasticity Theory and Practice, D.R.J. Owen and E. Hinton, 1970, Pineridge Press Ltd., Swansea, UK. 1 Course Content: A INTRODUCTION AND
More information第四章 : 中纬度的经向环流系统 (III) 授课教师 : 张洋. - Ferrel cell, baroclinic eddies and the westerly jet
第四章 : 中纬度的经向环流系统 (III) - Ferrel cell, baroclinic eddies and the westerly jet 授课教师 : 张洋 2016. 10. 24 Outline Review! Observations! The Ferrel Cell!! Review: baroclinic instability and baroclinic eddy life
More informationSIO 210 Introduction to Physical Oceanography Mid-term examination November 3, 2014; 1 hour 20 minutes
NAME: SIO 210 Introduction to Physical Oceanography Mid-term examination November 3, 2014; 1 hour 20 minutes Closed book; one sheet of your own notes is allowed. A calculator is allowed. (100 total points.)
More informationVertical structure. To conclude, we will review the critical factors invloved in the development of extratropical storms.
Vertical structure Now we will examine the vertical structure of the intense baroclinic wave using three visualization tools: Upper level charts at selected pressure levels Vertical soundings for selected
More informationFirst 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 informationwarmest (coldest) temperatures at summer heat dispersed upward by vertical motion Prof. Jin-Yi Yu ESS200A heated by solar radiation at the base
Pole Eq Lecture 3: ATMOSPHERE (Outline) JS JP Hadley Cell Ferrel Cell Polar Cell (driven by eddies) L H L H Basic Structures and Dynamics General Circulation in the Troposphere General Circulation in the
More informationQuasi-Geostrophic Implications
Chapter 10 Quasi-Geostrophic Implications When you look at a weather chart with all its isolines and plotted data, you need a framework upon which to interpret what you see. Quasi-geostrophic theory provides
More information7 The General Circulation
7 The General Circulation 7.1 The axisymmetric state At the beginning of the class, we discussed the nonlinear, inviscid, axisymmetric theory of the meridional structure of the atmosphere. The important
More informationWind: Global Systems Chapter 10
Wind: Global Systems Chapter 10 General Circulation of the Atmosphere General circulation of the atmosphere describes average wind patterns and is useful for understanding climate Over the earth, incoming
More informationIn this chapter, we will examine
In this chapter, we will examine Surface and upper level pressure charts The forces that influence the winds The equations that govern atmospheric motion Simple balanced flows Geostrophic wind (quantitative)
More informationGFD 2 Spring 2010 P.B. Rhines Problem set 1-solns out: 5 April back: 12 April
GFD 2 Spring 2010 P.B. Rhines Problem set 1-solns out: 5 April back: 12 April 1 The Gulf Stream has a dramatic thermal-wind signature : the sloping isotherms and isohalines (hence isopycnals) not only
More informationThe Transfer of Heat
The Transfer of Heat Outcomes: S2-4-03 Explain effects of heat transfer within the atmosphere and hydrosphere on the development and movement of wind and ocean currents. Coriolis Effect In our ecology
More informationLecture 5: Atmospheric General Circulation and Climate
Lecture 5: Atmospheric General Circulation and Climate Geostrophic balance Zonal-mean circulation Transients and eddies Meridional energy transport Moist static energy Angular momentum balance Atmosphere
More informationLecture 11: Meridonal structure of the atmosphere
Lecture 11: Meridonal structure of the atmosphere September 28, 2003 1 Meridional structure of the atmosphere In previous lectures we have focussed on the vertical structure of the atmosphere. Today, we
More informationIntroduction to Physical Oceanography Homework 3 - Solutions. 1. Volume transport in the Gulf Stream and Antarctic Circumpolar current (ACC):
Laure Zanna 10/17/05 Introduction to Physical Oceanography Homework 3 - Solutions 1. Volume transport in the Gulf Stream and Antarctic Circumpolar current (ACC): (a) Looking on the web you can find a lot
More information