Atmospheric Dynamics: lecture 11

Size: px
Start display at page:

Download "Atmospheric Dynamics: lecture 11"

Transcription

1 Atmospheric Dynamics: lecture 11 ( Chapter 9 Baroclinic waves and cyclogenesis What is a baroclinic wave? Quasi-geostrophic equations Omega equation Original articles:

2 Huib de Swart Baroclinic wave

3 Baroclinic wave

4 Baroclinic wave

5 Baroclinic wave

6 Baroclinic wave

7 Baroclinic wave

8 Baroclinic wave

9 Warm sector

10 Warm sector

11 Warm sector

12 Warm sector

13 warm seclusion occlusion

14

15

16 Upward motion

17 Atmospheric river

18 warm conveyor belt

19 warm conveyor belt

20 warm conveyor belt

21 Quasi-geostrophic theory Next we introduce the quasi-geostrophic approximation This leads to a system of two equations with two unknowns: vertical velocity and geopotential Omega (vert. vel.) equation gives insight into relation frontogenesis, vertical motion and cyclogenesis

22 Section 9.3 Section 1.30: Quasi-geostrophic approximation Primitive equations with pressure as vertical coordinate: dv = f k ˆ v Φ Φ p = RT p (Box 9.1, 12) (Box 9.1, 1) u x + v + ω p = 0 (Box 9.1, 14) t + u x + v S pω = J c p S p α c p p (Box 9.1, 8)

23 Section 9.3 Quasi-geostrophic approximation See also GFD dv = f k ˆ v Φ Φ p = RT p u x + v + ω p = 0 (Box 9.1, 12) (Box 9.1, 1) (Box 9.1, 14) t + u x + v S pω = J c p (Box 9.1, 8) Approximations: f f 0 + df dy y f 0 + βy v g = 1 f 0 ˆ k Φ dv d gv g d g t + v g = t + u g x + v g

24 Section 9.3 Quasigeostrophic equations dv d gv g = fk ˆ v Φ ( f 0 + βy) ˆ ( v a ) + f 0 ˆ k v g + k v g

25 Section 9.3 Quasigeostrophic equations dv d gv g = fk ˆ v Φ ( f 0 + βy) ˆ d g v g = βyk ˆ v g + v g >> v a ( v ) a f 0 ˆ ( v a ) + f 0 ˆ k v g + k v a βyk ˆ v g f 0 k ˆ v a k v g

26 Section 9.3 Quasigeostrophic equations dv d gv g = fk ˆ v Φ ( f 0 + βy) ˆ d g v g = βyk ˆ v g + v g >> v a ( v ) a f 0 ˆ ( v a ) + f 0 ˆ k v g + k v a βyk ˆ v g f 0 k ˆ v a k v g This is questionable!! (see fig lecture notes) Quasi-geostrophic approximation is difficult to justify completely from first principals, except under very restricted conditions. The justifications comes from practice: it works! (i.e. in hindsight)

27 Section 1.35 Jetstreak If β=0 then k ˆ d v v a = 1 f d v > 0 d v < 0 v a < 0 du = fv a v a > 0

28 Section 9.4 Quasigeostrophic vorticity d g v g equation = βy ˆ k v g f 0 ˆ k v a d g u g = f 0 v a + βyv g d g v g = f 0 u a βyu g

29 Section 9.4 Quasigeostrophic vorticity d g v g equation = βy ˆ k v g f 0 ˆ k v a d g u g = f 0 v a + βyv g d g v g u g = 1 Φ f 0 ;v g = 1 Φ f 0 x = f 0 u a βyu g x + v g = 0

30 Section 9.4 Quasigeostrophic vorticity d g v g equation = βy ˆ k v g f 0 ˆ k v a d g u g = f 0 v a + βyv g d g v g u g = 1 Φ f 0 ;v g = 1 Φ f 0 x = f 0 u a βyu g x + v g = 0 Quasi-geostrophic vorticity: ζ g = v g x = 1 f 0 2 Φ

31 Section 9.4 Quasigeostrophic vorticity d g v g equation = βy ˆ k v g f 0 ˆ k v a d g u g = f 0 v a + βyv g d g v g u g = 1 Φ f 0 ;v g = 1 Φ f 0 x = f 0 u a βyu g x + v g = 0 Quasi-geostrophic vorticity: ζ g = v g x = 1 f 0 2 Φ Quasi-geostrophic vorticity eqn: d g ζ g = 1 f 0 d g 2 Φ u = f a 0 x + v a βv g

32 Section 9.4 Geopotential and omega as unknowns Quasi-geostrophic vorticity eqn: d g ζ g = 1 f 0 d g 2 Φ u = f a 0 x + v a βv g

33 Section 9.4 Geopotential and omega as unknowns Quasi-geostrophic vorticity eqn: d g ζ g = 1 f 0 d g 2 Φ u = f a 0 x + v a βv g + continuity equation: u x + v + ω p = 0

34 Section 9.4 Geopotential and omega as unknowns Quasi-geostrophic vorticity eqn: d g ζ g = 1 f 0 d g 2 Φ u = f a 0 x + v a βv g + continuity equation: becomes: u x + v + ω p = 0 u a x + v a + ω p = 0 because x + v g = 0

35 Section 9.4 Geopotential and omega as unknowns Quasi-geostrophic vorticity eqn: d g ζ g = 1 f 0 d g 2 Φ u = f a 0 x + v a βv g + continuity equation: u x + v + ω p = 0 becomes: u a x + v a + ω p = 0 because x + v g = 0 Therefore: d g 2 Φ 2 ω = f 0 p β Φ x

36 Section 9.4 Quasi-geostrophic thermodynamic quation t + u x + v S pω = J c p Φ p = RT p From eq. 1.7c Derive an expression for S p

37 Section 9.4 Quasi-geostrophic thermodynamic quation t + u x + v S pω = J c p Φ p = RT p From eq. 1.7c Derive an expression for S p S p = α c p p

38 Section 9.4 Quasi-geostrophic thermodynamic quation t + u x + v S pω = J c p Φ p = RT p Quasi-geostrophic thermodynamic eq.: d g Φ p = σω RJ c p p σ R p S p

39 Section 9.4 Two equations and two unknowns Closed set of equations Quasi-geostrophic vorticity eq. d g 2 Φ 2 ω = f 0 p β Φ x Quasi-geostrophic thermodynamic eq. d g Φ p = σω RJ c p p This set of equations was used by the pioneers of numerical weather prediction

40 Section 9.4 Most important equations Quasi-geostrophic vorticity eq. d g 2 Φ 2 ω = f 0 p β Φ x Quasi-geostrophic thermodynamic eq. d g Φ p = σω RJ c p p Continuity equation u a x + v a + ω p = 0 Divergence of geostrophic wind = 0 x + v g = 0

41 Homework Problem 9.3 Geopotential field and Vertical motion (taken from Holton, 2004) Given the following expression for the geopotential field: Φ = Φ 0 p ( ) + l 1 sin l x ct ( ) + cf 0 y[ cos( πp / p 0 ) +1] [ ( )] where Φ 0 is a function of p alone, c is a constant speed, l a zonal wave number, and p 0 =1000hPa. (a) Use the quasi-geostrophic vorticity equation to obtain the horizontal divergence field consistent with this Φ-field. (Assume df/dy=0) (b) Assuming that ω(p 0 )=0, obtain an expression for ω(x, y, p, t) by integrating the continuity equation with respect to pressure. (c) Sketch the geopotential fields at 750 hpa and at 250 hpa. Indicate regions of positive and negative vertical velocity at 500 hpa.

42 Section 9.5 An equation for omega Meteorologists are most interested in omega because this variable gives a clear indication of where clouds and precipitation will form. In the following we derive a separate equation for omega, which is called the omega-equation

43 Section 9.5 Frontogenesis as a disturbance to thermal balance p = R pf 0 ; v g p = R pf 0 x Derive these two equations now

44 Section 9.5 Frontogenesis as a disturbance to thermal balance Using: d g u g = f 0 v a + βyv g Derive this now p = R pf 0 ; v g p = R pf 0 x and assuming β=0, and neglecting ageostrophic motion:

45 Section 9.5 Frontogenesis as a Using: disturbance to thermal balance d g u g d g p = f 0 v a + βyv g = p p = R pf 0 ; and assuming β=0, and neglecting ageostrophic motion: x v g p = R f 0 p x v g p = R pf 0 x + x

46 Section 9.5 Frontogenesis as a Using: disturbance to thermal balance d g u g d g p = f 0 v a + βyv g = p p = R pf 0 ; and assuming β=0, and neglecting ageostrophic motion: x v g p d g = R f 0 p x = v g v g p = R pf 0 x + x x * (J = 0) * (See also section 1.33, lecture notes)

47 Section 9.5 Frontogenesis as a Using: disturbance to thermal balance d g u g d g p = f 0 v a + βyv g = p p = R pf 0 ; and assuming β=0, and neglecting ageostrophic motion: x v g p d g = R f 0 p x = v g? * v g p = R pf 0 x + x x * (J = 0) (See also section 1.33, lecture notes)

48 Section 9.5 Frontogenesis as a Using: disturbance to thermal balance d g u g d g p = f 0 v a + βyv g = p and assuming β=0, and neglecting ageostrophic motion: x v g p d g = R f 0 p x Subtracting these two equations yields: d g f 0 p R x + v g = 0 p = 2 p = R pf 0 ; v g p = R pf 0 x = v g x + v g + x x * * (See also section 8.1, lecture notes) = 2Q g2 2 d g (J = 0)

49 Section 9.5 Frontogenesis as a disturbance to thermal balance d g f 0 p R p = 2 x + v g = 2Q g2 2 d g y-component of the geostrophic Q-vector Q-vector is vector frontogenesis function see section 1.33

50 Section 9.5 Frontogenesis as a disturbance to thermal balance d g f 0 p R p = 2 x + v g = 2Q g2 2 d g Disturbance to thermal wind balance y-component of the geostrophic Q-vector Q-vector is vector frontogenesis function see section 1.33

51 Section 9.5 Frontogenesis as a disturbance to thermal balance d g f 0 p R p = 2 x + v g = 2Q g2 2 d g Disturbance to thermal wind balance y-component of the geostrophic Q-vector Q-vector is vector frontogenesis function see sections 1.33 & 8.1 Now: let us include the ageostrophic flow

52 Section 9.5 Neglecting ageostrophic flow we have (previous slides): d g f 0 p R p = 2 x + v g = 2Q g2 2 d g

53 Section 9.5 Neglecting ageostrophic flow we have (previous slides): d g f 0 p R p = 2 x + v g = 2Q g2 2 d g Role of ageostrophic flow is to preserve thermal wind balance

54 Section 9.5 Neglecting ageostrophic flow we have (previous slides): d g f 0 p R p = 2 x + v g = 2Q g2 2 d g Role of ageostrophic flow Is to preserve thermal wind balance Repeating the derivation of the previous slides including ageostrophic flow yields d g f 0 p R p = 2Q g2 + f 0 R 2 p v a p pσ R ω

55 Section 9.5 Neglecting ageostrophic flow we have (previous slides): d g f 0 p R p = 2 x + v g = 2Q g2 2 d g Role of ageostrophic flow Is to preserve thermal wind balance Repeating the derivation of the previous slides including ageostrophic flow yields d g f 0 p R p = 2Q g2 + f 0 R 2 p v a p pσ R ω =0 If there conservation thermal wind balance

56 Section 9.5 From previous slide: 2Q g2 + f 2 0 p v a R p pσ R ω = 0 The x-component of thermal wind balance yields: 2Q g1 + f 2 0 p u a R p pσ R ω x = 0

57 Section 9.5 From previous slide: 2Q g2 + f 2 0 p v a R p pσ R ω = 0 The x-component of thermal wind balance yields: 2Q g1 + f 2 0 p u a R p pσ R ω x = 0 From this we can derive an equation for the vertical motion: + x

58 Section 9.5 From previous slide: 2Q g2 + f 2 0 p v a R p pσ R ω = 0 The x-component of thermal wind balance yields: 2Q g1 + f 2 0 p u a R p pσ R ω x = 0 From this we can derive an equation for the vertical motion: + x Omega-equation From the two equations above: σ 2 ω + f ω p 2 = 2R p Q g Where we have used u a x + v a + ω p = 0 and 2 2 x

59 Section 9.5 Omega equation:interpretation σ 2 ω + f ω p 2 = 2R p Q g Q g1 = x x + v g x ; Q g2 = x + v g.

60 Section 9.5 Omega equation:interpretation σ 2 ω + f ω p 2 = 2R p Q g Q g1 = x x + v g x ; Q g2 = x + v g. Since both T, u g and v g can all be expressed as a function of Φ, we can can calculate the vertical motion from the distribution of Φ only!!! ω w Q g i.e. upward (downward) motion if Q g -vector is convergent(divergent)

61 Next week: interpretation of the solution of the omega equation

Baroclinic wave. Atmospheric Dynamics: lecture 14 18/12/15. Topics. Chapter 9: Baroclinic waves and cyclogenesis. What is a baroclinic wave?

Baroclinic wave. Atmospheric Dynamics: lecture 14 18/12/15. Topics. Chapter 9: Baroclinic waves and cyclogenesis. What is a baroclinic wave? Atmospheric Dynamics: lecture 14 (http://www.staff.science.uu.nl/~delde102/) Topics Chapter 9: Baroclinic waves and cyclogenesis What is a baroclinic wave? Quasi-geostrophic equations Omega equation Original

More information

Dynamic Meteorology: lecture 12

Dynamic Meteorology: lecture 12 30/11/2018 (Friday) Dynamic Meteorology: lecture 12 Sections 9.5, 9.6 Omega equa)on Large scale ver)cal mo)on in a quasi-geostrophic atmosphere Two level model of the atmosphere 5/12/2017 (Wednesday!!!):

More information

Quasi-geostrophic system

Quasi-geostrophic system Quasi-eostrophic system (or, why we love elliptic equations for QGPV) Charney s QG the motion of lare-scale atmospheric disturbances is overned by Laws of conservation of potential temperature and potential

More information

2.5 Shallow water equations, quasigeostrophic filtering, and filtering of inertia-gravity waves

2.5 Shallow water equations, quasigeostrophic filtering, and filtering of inertia-gravity waves Chapter. The continuous equations φ=gh Φ=gH φ s =gh s Fig..5: Schematic of the shallow water model, a hydrostatic, incompressible fluid with a rigid bottom h s (x,y), a free surface h(x,y,t), and horizontal

More information

The dynamics of high and low pressure systems

The 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 information

Dust devils, water spouts, tornados

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

More information

DANISH METEOROLOGICAL INSTITUTE

DANISH METEOROLOGICAL INSTITUTE DANISH METEOROLOGICAL INSTITUTE SCIENTIFIC REPORT 3-11 Quasigeostrophic interpretation of extratropical cyclogenesis Niels Woetmann Nielsen COPENHAGEN 23 ISSN Nr. 9-3263 (printed) ISSN Nr. 1399-1949 (online)

More information

Atmospheric dynamics and meteorology

Atmospheric dynamics and meteorology Atmospheric dynamics and meteorology B. Legras, http://www.lmd.ens.fr/legras III Frontogenesis (pre requisite: quasi-geostrophic equation, baroclinic instability in the Eady and Phillips models ) Recommended

More information

Diagnosing Vertical Velocity: The Omega Equation. Robert Todd and Kaushik Srinivasan 15 May 2009

Diagnosing Vertical Velocity: The Omega Equation. Robert Todd and Kaushik Srinivasan 15 May 2009 Diagnosing Vertical Velocity: The Omega Equation Robert Todd and Kaushik Srinivasan 15 May 2009 Introduction The vertical velocity is much smaller then the horizontal velocity and therefore, difficult

More information

Class exercises Chapter 3. Elementary Applications of the Basic Equations

Class exercises Chapter 3. Elementary Applications of the Basic Equations Class exercises Chapter 3. Elementary Applications of the Basic Equations Section 3.1 Basic Equations in Isobaric Coordinates 3.1 For some (in fact many) applications we assume that the change of the Coriolis

More information

EAS372 Open Book Final Exam 11 April, 2013

EAS372 Open Book Final Exam 11 April, 2013 EAS372 Open Book Final Exam 11 April, 2013 Professor: J.D. Wilson Time available: 2 hours Value: 30% Please check the Terminology, Equations and Data section before beginning your responses. Answer all

More information

+ ω = 0, (1) (b) In geometric height coordinates in the rotating frame of the Earth, momentum balance for an inviscid fluid is given by

+ ω = 0, (1) (b) In geometric height coordinates in the rotating frame of the Earth, momentum balance for an inviscid fluid is given by Problem Sheet 1: Due Thurs 3rd Feb 1. Primitive equations in different coordinate systems (a) Using Lagrangian considerations and starting from an infinitesimal mass element in cartesian coordinates (x,y,z)

More information

Vorticity in natural coordinates

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

More information

Quasi-Geostrophic Implications

Quasi-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 information

SIO 210: Dynamics VI (Potential vorticity) L. Talley Fall, 2014 (Section 2: including some derivations) (this lecture was not given in 2015)

SIO 210: Dynamics VI (Potential vorticity) L. Talley Fall, 2014 (Section 2: including some derivations) (this lecture was not given in 2015) SIO 210: Dynamics VI (Potential vorticity) L. Talley Fall, 2014 (Section 2: including some derivations) (this lecture was not given in 2015) Variation of Coriolis with latitude: β Vorticity Potential vorticity

More information

8 Mechanisms for tropical rainfall responses to equatorial

8 Mechanisms for tropical rainfall responses to equatorial 8 Mechanisms for tropical rainfall responses to equatorial heating More reading: 1. Hamouda, M. and Kucharski, F. (2019) Ekman pumping Mechanism driving Precipitation anomalies in Response to Equatorial

More information

Lecture #2 Planetary Wave Models. Charles McLandress (Banff Summer School 7-13 May 2005)

Lecture #2 Planetary Wave Models. Charles McLandress (Banff Summer School 7-13 May 2005) Lecture #2 Planetary Wave Models Charles McLandress (Banff Summer School 7-13 May 2005) 1 Outline of Lecture 1. Observational motivation 2. Forced planetary waves in the stratosphere 3. Traveling planetary

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

Introduction to Conceptual Models

Introduction to Conceptual Models Zentralanstalt für Meteorologie und Geodynamik Introduction to Conceptual Models Veronika Zwatz-Meise IR Satellite Images with Satrep From Cloud systems in satellite images to Conceptual Models If we look

More information

6 Two-layer shallow water theory.

6 Two-layer shallow water theory. 6 Two-layer shallow water theory. Wewillnowgoontolookatashallowwatersystemthathastwolayersofdifferent density. This is the next level of complexity and a simple starting point for understanding the behaviour

More information

1/18/2011. From the hydrostatic equation, it is clear that a single. pressure and height in each vertical column of the atmosphere.

1/18/2011. From the hydrostatic equation, it is clear that a single. pressure and height in each vertical column of the atmosphere. Lecture 3: Applications of Basic Equations Pressure as Vertical Coordinate From the hydrostatic equation, it is clear that a single valued monotonic relationship exists between pressure and height in each

More information

Introduction to Isentropic Coordinates: a new view of mean meridional & eddy circulations. Cristiana Stan

Introduction to Isentropic Coordinates: a new view of mean meridional & eddy circulations. Cristiana Stan Introduction to Isentropic Coordinates: a new view of mean meridional & eddy circulations Cristiana Stan School and Conference on the General Circulation of the Atmosphere and Oceans: a Modern Perspective

More information

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

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

More information

Symmetry methods in dynamic meteorology

Symmetry methods in dynamic meteorology Symmetry methods in dynamic meteorology p. 1/12 Symmetry methods in dynamic meteorology Applications of Computer Algebra 2008 Alexander Bihlo alexander.bihlo@univie.ac.at Department of Meteorology and

More information

Occlusion cyclogenesis II

Occlusion cyclogenesis II Occlusion cyclogenesis II Upper level influences on cyclogenesis Vorticity Advection (CVA) and the 4-quadrant jet streak model (Uccellini) Potential Vorticity (PV) (Hoskins Theory) Rapid cyclogenesis 14

More information

EAS372 Open Book Final Exam 11 April, 2013

EAS372 Open Book Final Exam 11 April, 2013 EAS372 Open Book Final Exam 11 April, 2013 Professor: J.D. Wilson Time available: 2 hours Value: 30% Please check the Terminology, Equations and Data section before beginning your responses. Answer all

More information

Quasi-Geostrophic ω-equation. 1. The atmosphere is approximately hydrostatic. 2. The atmosphere is approximately geostrophic.

Quasi-Geostrophic ω-equation. 1. The atmosphere is approximately hydrostatic. 2. The atmosphere is approximately geostrophic. Quasi-Geostrophic ω-equation For large-scale flow in the atmosphere, we have learned about two very important characteristics:. The atmosphere is approximately hydrostatic.. The atmosphere is approximately

More information

BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity

BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere Need to introduce a new measure of the buoyancy Potential temperature θ In a compressible fluid, the relevant measure

More information

Part 4. Atmospheric Dynamics

Part 4. Atmospheric Dynamics Part 4. Atmospheric Dynamics We apply Newton s Second Law: ma =Σ F i to the atmosphere. In Cartesian coordinates dx u = dt dy v = dt dz w = dt 1 ai = F m i i du dv dw a = ; ay = ; az = x dt dt dt 78 Coordinate

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

Synoptic Meteorology II: Self-Development in the IPV Framework. 5-7 May 2015

Synoptic Meteorology II: Self-Development in the IPV Framework. 5-7 May 2015 Synoptic Meteorology II: Self-Development in the IPV Framework 5-7 May 2015 Readings: Section 5.3.6 of Midlatitude Synoptic Meteorology. Introduction In this and other recent lectures, we have developed

More information

Governing Equations and Scaling in the Tropics

Governing Equations and Scaling in the Tropics Governing Equations and Scaling in the Tropics M 1 ( ) e R ε er Tropical v Midlatitude Meteorology Why is the general circulation and synoptic weather systems in the tropics different to the those in the

More information

Chapter 7: Circulation and Vorticity

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

More information

Mesoscale Atmospheric Systems. Surface fronts and frontogenesis. 06 March 2018 Heini Wernli. 06 March 2018 H. Wernli 1

Mesoscale Atmospheric Systems. Surface fronts and frontogenesis. 06 March 2018 Heini Wernli. 06 March 2018 H. Wernli 1 Mesoscale Atmospheric Systems Surface fronts and frontogenesis 06 March 2018 Heini Wernli 06 March 2018 H. Wernli 1 Temperature (degc) Frontal passage in Mainz on 26 March 2010 06 March 2018 H. Wernli

More information

1/27/2010. With this method, all filed variables are separated into. from the basic state: Assumptions 1: : the basic state variables must

1/27/2010. With this method, all filed variables are separated into. from the basic state: Assumptions 1: : the basic state variables must Lecture 5: Waves in Atmosphere Perturbation Method With this method, all filed variables are separated into two parts: (a) a basic state part and (b) a deviation from the basic state: Perturbation Method

More information

Transformed Eulerian Mean

Transformed Eulerian Mean Chapter 15 Transformed Eulerian Mean In the last few lectures we introduced some fundamental ideas on 1) the properties of turbulent flows in rotating stratified environments, like the ocean and the atmosphere,

More information

Notes and Correspondence Higher-order corrections for Rossby waves in a zonal channel on the β-plane

Notes and Correspondence Higher-order corrections for Rossby waves in a zonal channel on the β-plane QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY Q. J. R. Meteorol. Soc. 33: 893 898 (7 Published online 4 October 7 in Wiley InterScience (www.interscience.wiley.com DOI:./qj.44 Notes and Correspondence

More information

Part-8c Circulation (Cont)

Part-8c Circulation (Cont) Part-8c Circulation (Cont) Global Circulation Means of Transfering Heat Easterlies /Westerlies Polar Front Planetary Waves Gravity Waves Mars Circulation Giant Planet Atmospheres Zones and Belts Global

More information

Dynamics Rotating Tank

Dynamics Rotating Tank Institute for Atmospheric and Climate Science - IACETH Atmospheric Physics Lab Work Dynamics Rotating Tank Large scale flows on different latitudes of the rotating Earth Abstract The large scale atmospheric

More information

Dynamic Meteorology (lecture 9, 2014)

Dynamic Meteorology (lecture 9, 2014) Dynamic Meteorology (lecture 9, 2014) Topics Assessment criteria High frequency waves (no rota5on) Boussinesq approxima/on Normal model analysis of the stability of hydrosta/c balance Buoyancy waves and

More information

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

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

More information

On the effect of forward shear and reversed shear baroclinic flows for polar low developments. Thor Erik Nordeng Norwegian Meteorological Institute

On the effect of forward shear and reversed shear baroclinic flows for polar low developments. Thor Erik Nordeng Norwegian Meteorological Institute On the effect of forward shear and reversed shear baroclinic flows for polar low developments Thor Erik Nordeng Norwegian Meteorological Institute Outline Baroclinic growth a) Normal mode solution b) Initial

More information

Internal boundary layers in the ocean circulation

Internal boundary layers in the ocean circulation Internal boundary layers in the ocean circulation Lecture 9 by Andrew Wells We have so far considered boundary layers adjacent to physical boundaries. However, it is also possible to find boundary layers

More information

An Optimal Control Problem Formulation for. the Atmospheric Large-Scale Wave Dynamics

An Optimal Control Problem Formulation for. the Atmospheric Large-Scale Wave Dynamics pplied Mathematical Sciences, Vol. 9, 5, no. 8, 875-884 HIKRI Ltd, www.m-hikari.com http://dx.doi.org/.988/ams.5.448 n Optimal Control Problem Formulation for the tmospheric Large-Scale Wave Dynamics Sergei

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

Isentropic Analysis. Much of this presentation is due to Jim Moore, SLU

Isentropic Analysis. Much of this presentation is due to Jim Moore, SLU Isentropic Analysis Much of this presentation is due to Jim Moore, SLU Utility of Isentropic Analysis Diagnose and visualize vertical motion - through advection of pressure and system-relative flow Depict

More information

Synoptic-Dynamic Meteorology in Midlatitudes

Synoptic-Dynamic Meteorology in Midlatitudes Synoptic-Dynamic Meteorology in Midlatitudes VOLUME II Observations and Theory of Weather Systems HOWARD B. BLUESTEIN New York Oxford OXFORD UNIVERSITY PRESS 1993 Contents 1. THE BEHAVIOR OF SYNOPTIC-SCALE,

More information

Synoptic Meteorology II: Potential Vorticity Inversion and Anomaly Structure April 2015

Synoptic Meteorology II: Potential Vorticity Inversion and Anomaly Structure April 2015 Synoptic Meteorology II: Potential Vorticity Inversion and Anomaly Structure 14-16 April 2015 Readings: Sections 4.2 and 4.4 of Midlatitude Synoptic Meteorology. Potential Vorticity Inversion Introduction

More information

The General Circulation of the Atmosphere: A Numerical Experiment

The General Circulation of the Atmosphere: A Numerical Experiment The General Circulation of the Atmosphere: A Numerical Experiment Norman A. Phillips (1956) Presentation by Lukas Strebel and Fabian Thüring Goal of the Model Numerically predict the mean state of the

More information

Multiscale Analyses of Inland Tropical Cyclone Midlatitude Jet Interactions: Camille (1969) and Danny (1997)

Multiscale Analyses of Inland Tropical Cyclone Midlatitude Jet Interactions: Camille (1969) and Danny (1997) Multiscale Analyses of Inland Tropical Cyclone Midlatitude Jet Interactions: Camille (1969) and Danny (1997) Matthew Potter, Lance Bosart, and Daniel Keyser Department of Atmospheric and Environmental

More information

Use of dynamical concepts in weather forecasting

Use of dynamical concepts in weather forecasting Use of dynamical concepts in weather forecasting Meteorol. Appl. 4, 345 352 (1997) E B Carroll, Meteorological Office, London Road, Bracknell, Berkshire RG12 2SZ, UK A divergence-based procedure for diagnosing

More information

Measurement of Rotation. Circulation. Example. Lecture 4: Circulation and Vorticity 1/31/2017

Measurement of Rotation. Circulation. Example. Lecture 4: Circulation and Vorticity 1/31/2017 Lecture 4: Circulation and Vorticity Measurement of Rotation Circulation Bjerknes Circulation Theorem Vorticity Potential Vorticity Conservation of Potential Vorticity Circulation and vorticity are the

More information

Occlusion Cyclogenesis

Occlusion Cyclogenesis Occlusion Cyclogenesis Part I: Occlusion cloud bands in comparison to CF and WFs Concepts for cyclogenesis Different types of cyclogenesis and examples Numerical parameters on isobaric and isentropic surfaces

More information

Chapter 12 Fronts & Air Masses

Chapter 12 Fronts & Air Masses Chapter overview: Anticyclones or highs Air Masses o Classification o Source regions o Air masses of North America Fronts o Stationary fronts o Cold fronts o Warm fronts o Fronts and the jet stream o Frontogenesis

More information

Eliassen-Palm Theory

Eliassen-Palm Theory Eliassen-Palm Theory David Painemal MPO611 April 2007 I. Introduction The separation of the flow into its zonal average and the deviations therefrom has been a dominant paradigm for analyses of the general

More information

= vorticity dilution + tilting horizontal vortices + microscopic solenoid

= vorticity dilution + tilting horizontal vortices + microscopic solenoid 4.4 Vorticity Eq 4.4.1 Cartesian Coordinates Because ζ = ˆk V, gives D(ζ + f) x minus [v momentum eq. in Cartesian Coordinates] y [u momentum eq. in Cartesian Coordinates] = vorticity dilution + tilting

More information

Dynamic Meteorology (lecture 13, 2016)

Dynamic Meteorology (lecture 13, 2016) Dynamic Meteorology (lecture 13, 2016) Topics Chapter 3, lecture notes: High frequency waves (no rota;on) Boussinesq approxima4on Normal mode analysis of the stability of hydrosta4c balance Buoyancy waves

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

Balanced Flow Geostrophic, Inertial, Gradient, and Cyclostrophic Flow

Balanced Flow Geostrophic, Inertial, Gradient, and Cyclostrophic Flow Balanced Flow Geostrophic, Inertial, Gradient, and Cyclostrophic Flow The types of atmospheric flows describe here have the following characteristics: 1) Steady state (meaning that the flows do not change

More information

t tendency advection convergence twisting baroclinicity

t tendency advection convergence twisting baroclinicity RELATIVE VORTICITY EQUATION Newton s law in a rotating frame in z-coordinate (frictionless): U + U U = 2Ω U Φ α p U + U U 2 + ( U) U = 2Ω U Φ α p Applying to both sides, and noting ω U and using identities

More information

Extratropical Cyclone Clouds: Impact on Cyclone Strength and Climate

Extratropical Cyclone Clouds: Impact on Cyclone Strength and Climate Extratropical Cyclone Clouds: Impact on Cyclone Strength and Climate James B. Polly William B. Rossow City College of the City University of New York NOAA NESDIS CORP Science Symposium 2014 September 09

More information

Reynolds Averaging. We separate the dynamical fields into slowly varying mean fields and rapidly varying turbulent components.

Reynolds Averaging. We separate the dynamical fields into slowly varying mean fields and rapidly varying turbulent components. Reynolds Averaging Reynolds Averaging We separate the dynamical fields into sloly varying mean fields and rapidly varying turbulent components. Reynolds Averaging We separate the dynamical fields into

More information

Dynamics of the Atmosphere. Large-scale flow with rotation and stratification

Dynamics of the Atmosphere. Large-scale flow with rotation and stratification 12.810 Dynamics of the Atmosphere Large-scale flow with rotation and stratification Visualization of meandering jet stream Upper level winds from June 10th to July 8th 1988 from MERRA Red shows faster

More information

Can a Simple Two-Layer Model Capture the Structure of Easterly Waves?

Can a Simple Two-Layer Model Capture the Structure of Easterly Waves? Can a Simple Two-Layer Model Capture the Structure of Easterly Waves? Cheryl L. Lacotta 1 Introduction Most tropical storms in the Atlantic, and even many in the eastern Pacific, are due to disturbances

More information

Nonlinear Balance on an Equatorial Beta Plane

Nonlinear Balance on an Equatorial Beta Plane Nonlinear Balance on an Equatorial Beta Plane David J. Raymond Physics Department and Geophysical Research Center New Mexico Tech Socorro, NM 87801 April 26, 2009 Summary Extension of the nonlinear balance

More information

Example of the "Vorticity Advection" Pitfall

Example of the Vorticity Advection Pitfall Example of the "Vorticity Advection" Pitfall NOGAPS 60 h Forecast for 500 mb Heights and Absolute Vorticity The 500 mb chart with absolute vorticity overlain is the first chart most operational meteorologists

More information

In two-dimensional barotropic flow, there is an exact relationship between mass

In two-dimensional barotropic flow, there is an exact relationship between mass 19. Baroclinic Instability In two-dimensional barotropic flow, there is an exact relationship between mass streamfunction ψ and the conserved quantity, vorticity (η) given by η = 2 ψ.the evolution of the

More information

Dynamic Meteorology (Atmospheric Dynamics)

Dynamic Meteorology (Atmospheric Dynamics) Lecture 1-2012 Dynamic Meteorology (Atmospheric Dynamics) Lecturer: Aarnout van Delden Office: BBG, room 615 a.j.vandelden@uu.nl http://www.staff.science.uu.nl/~delde102/index.php Students (background

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

A Uniform PV Framework for Balanced Dynamics

A Uniform PV Framework for Balanced Dynamics A Uniform PV Framework for Balanced Dynamics vertical structure of the troposphere surface quasigeostrophic models Dave Muraki Simon Fraser University Greg Hakim University of Washington Chris Snyder NCAR

More information

Dynamics of the Extratropical Response to Tropical Heating

Dynamics of the Extratropical Response to Tropical Heating Regional and Local Climate Modeling and Analysis Research Group R e L o C l i m Dynamics of the Extratropical Response to Tropical Heating (1) Wegener Center for Climate and Global Change (WegCenter) and

More information

Chapter 10: Mid-latitude Cyclones Mid-Latitude Cyclones

Chapter 10: Mid-latitude Cyclones Mid-Latitude Cyclones Chapter 10: Mid-latitude Cyclones Mid-Latitude Cyclones Mid-latitude cyclones form along a boundary separating polar air from warmer air to the south. Life Cycle of Cyclone Cyclone Structures Steering

More information

Chapter 10: Mid-latitude Cyclones

Chapter 10: Mid-latitude Cyclones Chapter 10: Mid-latitude Cyclones Life Cycle of Cyclone Cyclone Structures Steering of Cyclone Mid-Latitude Cyclones Mid-latitude cyclones form along a boundary separating polar air from warmer air to

More information

Circulation and Vorticity

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

More information

Steady Flow: rad conv. where. E c T gz L q 2. p v 2 V. Integrate from surface to top of atmosphere: rad TOA rad conv surface

Steady Flow: rad conv. where. E c T gz L q 2. p v 2 V. Integrate from surface to top of atmosphere: rad TOA rad conv surface The Three-Dimensional Circulation 1 Steady Flow: F k ˆ F k ˆ VE 0, rad conv where 1 E c T gz L q 2 p v 2 V Integrate from surface to top of atmosphere: VE F FF F 0 rad TOA rad conv surface 2 What causes

More information

The dynamics of a simple troposphere-stratosphere model

The dynamics of a simple troposphere-stratosphere model The dynamics of a simple troposphere-stratosphere model by Jessica Duin under supervision of Prof. Dr. A. Doelman, UvA Dr. W.T.M. Verkley, KNMI August 31, 25 Universiteit van Amsterdam Korteweg-de vries

More information

Atmospheric Dynamics Fall 2008

Atmospheric Dynamics Fall 2008 Atmospheric Dynamics Fall 2008 AT601, the first semester of Atmospheric Dynamics, is based on the course notes available over the web and on the highly recommended texts listed below. The course notes

More information

Nonlinear baroclinic dynamics of surface cyclones crossing a zonal jet

Nonlinear 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 information

ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves

ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves Reference: An Introduction to Dynamic Meteorology (4 rd edition), J.R. Holton Atmosphere-Ocean Dynamics, A.E. Gill Fundamentals of Atmospheric

More information

Geostrophic and Quasi-Geostrophic Balances

Geostrophic and Quasi-Geostrophic Balances Geostrophic and Quasi-Geostrophic Balances Qiyu Xiao June 19, 2018 1 Introduction Understanding how the atmosphere and ocean behave is important to our everyday lives. Techniques such as weather forecasting

More information

Using simplified vorticity equation,* by assumption 1 above: *Metr 430 handout on Circulation and Vorticity. Equations (4) and (5) on that handout

Using simplified vorticity equation,* by assumption 1 above: *Metr 430 handout on Circulation and Vorticity. Equations (4) and (5) on that handout Rossby Wave Equation A. Assumptions 1. Non-divergence 2. Initially, zonal flow, or nearly zonal flow in which u>>v>>w. 3. Initial westerly wind is geostrophic and does not vary along the x-axis and equations

More information

McGraw Hill Yearbook of Science & Technology Extratropical cyclone occlusion. McGraw Hill 2008 Yearbook of Science & Technology.

McGraw Hill Yearbook of Science & Technology Extratropical cyclone occlusion. McGraw Hill 2008 Yearbook of Science & Technology. McGraw Hill Yearbook of Science & Technology 0 Extratropical cyclone occlusion Journal: McGraw Hill 0 Yearbook of Science & Technology Manuscript ID: draft Manuscript Type: Date Submitted by the Author:

More information

u g z = g T y (1) f T Margules Equation for Frontal Slope

u g z = g T y (1) f T Margules Equation for Frontal Slope Margules Equation for Frontal Slope u g z = g f T T y (1) Equation (1) is the thermal wind relation for the west wind geostrophic component of the flow. For the purposes of this derivation, we assume that

More information

ATM OCN 452. The Frontal Cyclone. Fall 2013

ATM OCN 452. The Frontal Cyclone. Fall 2013 ATM OCN 452 The Frontal Cyclone Fall 2013 Instructor: Dr. Jonathan E. Martin 1425A Meteorology and Space Science jemarti1@wisc.edu 262-9845 Office Hours: Wed. 12:30 2:25 (or by appointment) T. A.: Andrew

More information

Conference on Teleconnections in the Atmosphere and Oceans November 2008

Conference on Teleconnections in the Atmosphere and Oceans November 2008 1968-38 Conference on Teleconnections in the Atmosphere and Oceans 17-20 November 2008 Mid-latitude - MJO teleconnection over East Asia in the Northern winter KIM Baekmin Yonsei University Dept. of Atmospheric

More information

Chapter 9. Barotropic Instability. 9.1 Linearized governing equations

Chapter 9. Barotropic Instability. 9.1 Linearized governing equations Chapter 9 Barotropic Instability The ossby wave is the building block of low ossby number geophysical fluid dynamics. In this chapter we learn how ossby waves can interact with each other to produce a

More information

Barotropic geophysical flows and two-dimensional fluid flows: Conserved Quantities

Barotropic geophysical flows and two-dimensional fluid flows: Conserved Quantities Barotropic geophysical flows and two-dimensional fluid flows: Conserved Quantities Di Qi, and Andrew J. Majda Courant Institute of Mathematical Sciences Fall 2016 Advanced Topics in Applied Math Di Qi,

More information

( ) (9.1.1) Chapter 9. Geostrophy, Quasi-Geostrophy and the Potential Vorticity Equation. 9.1 Geostrophy and scaling.

( ) (9.1.1) Chapter 9. Geostrophy, Quasi-Geostrophy and the Potential Vorticity Equation. 9.1 Geostrophy and scaling. Chapter 9 Geostrophy, Quasi-Geostrophy and the Potential Vorticity Equation 9.1 Geostrophy and scaling. We examined in the last chapter some consequences of the dynamical balances for low frequency, nearly

More information

Background Error Covariance Modelling

Background Error Covariance Modelling Background Error Covariance Modelling Mike Fisher Slide 1 Outline Diagnosing the Statistics of Background Error using Ensembles of Analyses Modelling the Statistics in Spectral Space - Relaxing constraints

More information

1/25/2010. Circulation and vorticity are the two primary

1/25/2010. Circulation and vorticity are the two primary Lecture 4: Circulation and Vorticity Measurement of Rotation Circulation Bjerknes Circulation Theorem Vorticity Potential Vorticity Conservation of Potential Vorticity Circulation and vorticity are the

More information

Errata: Midlatitude Synoptic Meteorology (July, 2014)

Errata: Midlatitude Synoptic Meteorology (July, 2014) Errata: Midlatitude Synoptic Meteorology (July, 2014) My apologies for the various inevitable errors contained in this first-edition text. We are working diligently to correct them. I gratefully acknowledge

More information

Synoptic Meteorology

Synoptic Meteorology M.Sc. in Meteorology Synoptic Meteorology [MAPH P312] Prof Peter Lynch Second Semester, 2004 2005 Seminar Room Dept. of Maths. Physics, UCD, Belfield. Part 9 Extratropical Weather Systems These lectures

More information

The Eady problem of baroclinic instability described in section 19a was shown to

The Eady problem of baroclinic instability described in section 19a was shown to 0. The Charney-Stern Theorem The Eady problem of baroclinic instability described in section 19a was shown to be remarkably similar to the Rayleigh instability of barotropic flow described in Chapter 18.

More information

Final Examination, MEA 443 Fall 2008, Lackmann

Final Examination, MEA 443 Fall 2008, Lackmann Place an X here to count it double! Name: Final Examination, MEA 443 Fall 2008, Lackmann If you wish to have the final exam count double and replace your midterm score, place an X in the box above. As

More information

Lower-Tropospheric Height Tendencies Associated with the Shearwise and Transverse Components of Quasigeostrophic Vertical Motion

Lower-Tropospheric Height Tendencies Associated with the Shearwise and Transverse Components of Quasigeostrophic Vertical Motion JULY 2007 N O T E S A N D C O R R E S P O N D E N C E 2803 Lower-Tropospheric Height Tendencies Associated with the Shearwise and Transverse Components of Quasigeostrophic Vertical Motion JONATHAN E. MARTIN

More information

Effective Depth of Ekman Layer.

Effective Depth of Ekman Layer. 5.5: Ekman Pumping Effective Depth of Ekman Layer. 2 Effective Depth of Ekman Layer. Defining γ = f/2k, we derived the solution u = u g (1 e γz cos γz) v = u g e γz sin γz corresponding to the Ekman spiral.

More information

Lecture 25: Ocean circulation: inferences from geostrophic and thermal wind balance

Lecture 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 information

2 Transport of heat, momentum and potential vorticity

2 Transport of heat, momentum and potential vorticity Transport of heat, momentum and potential vorticity. Conventional mean momentum equation We ll write the inviscid equation of onal motion (we ll here be using log-pressure coordinates with = H ln p=p,

More information

http://www.ssec.wisc.edu/data/composites.html Red curve: Incoming solar radiation Blue curve: Outgoing infrared radiation. Three-cell model of general circulation Mid-latitudes: 30 to 60 latitude MID-LATITUDES

More information

Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States

Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States See CalTech 2005 paper on course web site Free troposphere assumed to have moist adiabatic lapse rate (s* does

More information