PAPER 333 FLUID DYNAMICS OF CLIMATE

Similar documents
Note that Rossby waves are tranverse waves, that is the particles move perpendicular to the direction of propagation. f up, down (clockwise)

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

Ocean dynamics: the wind-driven circulation

Atmosphere, Ocean and Climate Dynamics Fall 2008

OCN/ATM/ESS 587. The wind-driven ocean circulation. Friction and stress. The Ekman layer, top and bottom. Ekman pumping, Ekman suction

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

6 Two-layer shallow water theory.

Lecture 8. Lecture 1. Wind-driven gyres. Ekman transport and Ekman pumping in a typical ocean basin. VEk

Internal boundary layers in the ocean circulation

) 2 ψ +β ψ. x = 0. (71) ν = uk βk/k 2, (74) c x u = β/k 2. (75)

Lecture 17 ATOC 5051 INTRODUCTION TO PHYSICAL OCEANOGRAPHY. Learning objectives: understand the concepts & physics of

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

Chapter 5. Shallow Water Equations. 5.1 Derivation of shallow water equations

PAPER 345 ENVIRONMENTAL FLUID DYNAMICS

Boundary Layers: Homogeneous Ocean Circulation

PAPER 84 QUANTUM FLUIDS

Vorticity and Potential Vorticity

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

2. Baroclinic Instability and Midlatitude Dynamics

Lecture 14. Equations of Motion Currents With Friction Sverdrup, Stommel, and Munk Solutions Remember that Ekman's solution for wind-induced transport

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

PAPER 331 HYDRODYNAMIC STABILITY

PAPER 57 DYNAMICS OF ASTROPHYSICAL DISCS

General Comment on Lab Reports: v. good + corresponds to a lab report that: has structure (Intro., Method, Results, Discussion, an Abstract would be

Wind Gyres. curl[τ s τ b ]. (1) We choose the simple, linear bottom stress law derived by linear Ekman theory with constant κ v, viz.

Gravity Waves. Lecture 5: Waves in Atmosphere. Waves in the Atmosphere and Oceans. Internal Gravity (Buoyancy) Waves 2/9/2017

10 Shallow Water Models

t tendency advection convergence twisting baroclinicity

Candidates must show on each answer book the type of calculator used. Log Tables, Statistical Tables and Graph Paper are available on request.

The General Circulation of the Atmosphere: A Numerical Experiment

Islands in locally-forced basin circulations

Transformed Eulerian Mean

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

SAMPLE CHAPTERS UNESCO EOLSS WAVES IN THE OCEANS. Wolfgang Fennel Institut für Ostseeforschung Warnemünde (IOW) an der Universität Rostock,Germany

+ φ zz. (1a) v t = -gη Y

Contents. Parti Fundamentals. 1. Introduction. 2. The Coriolis Force. Preface Preface of the First Edition

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

ROSSBY WAVE PROPAGATION

SIO 210 Problem Set 3 November 15, 2013 Due Nov. 22, 2013 Answerkey

Stability of meridionally-flowing grounded abyssal currents in the ocean

Jet Formation in the Equatorial Oceans Through Barotropic and Inertial Instabilities. Mark Fruman

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

Eliassen-Palm Theory

Wind-Driven Circulation: Stommel s gyre & Sverdrup s balance

The equation we worked with for waves and geostrophic adjustment of a 1-layer fluid is η tt

PAPER 68 ACCRETION DISCS

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

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

MATHEMATICAL TRIPOS Part III PAPER 53 COSMOLOGY

Ocean currents: some misconceptions and some dynamics

Quasi-geostrophic ocean models

The Shallow Water Equations

The General Circulation of the Oceans

Chapter 3. Shallow Water Equations and the Ocean. 3.1 Derivation of shallow water equations

GFD I: Midterm Exam Solutions

Stationary Rossby Waves and Shocks on the Sverdrup Coordinate

Chapter 13 Instability on non-parallel flow Introduction and formulation

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

Physical Oceanography, MSCI 3001 Oceanographic Processes, MSCI Dr. Katrin Meissner Ocean Dynamics.

Module Contact: Dr Xiaoming Zhai, ENV Copyright of the University of East Anglia Version 2

Modeling the atmosphere of Jupiter

Internal boundary layers in the ocean circulation

EART164: PLANETARY ATMOSPHERES

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator.

Circulation and Vorticity

Introduction to Synoptic Scale Dynamics

Mathematical Concepts & Notation

Diagnosis of a Quasi-Geostrophic 2-Layer Model Aaron Adams, David Zermeño, Eunsil Jung, Hosmay Lopez, Ronald Gordon, Ting-Chi Wu

A few examples Shallow water equation derivation and solutions. Goal: Develop the mathematical foundation of tropical waves

Chapter 9. Barotropic Instability. 9.1 Linearized governing equations

Boundary Layers. Lecture 2 by Basile Gallet. 2i(1+i) The solution to this equation with the boundary conditions A(0) = U and B(0) = 0 is

Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C5: PHYSICS OF ATMOSPHERES AND OCEANS TRINITY TERM 2016

Exam Questions & Problems

The Influence of the Agulhas leakage on the overturning circulation from momentum balances

LFV in a mid-latitude coupled model:

Chapter 9. Geostrophy, Quasi-Geostrophy and the Potential Vorticity Equation

Balanced Flow Geostrophic, Inertial, Gradient, and Cyclostrophic Flow

of Friction in Fluids Dept. of Earth & Clim. Sci., SFSU

ESCI 343 Atmospheric Dynamics II Lesson 11 - Rossby Waves

Eddy PV Fluxes in a One Dimensional Model of Quasi-Geostrophic Turbulence

Sound Generation from Vortex Sheet Instability

Eliassen-Palm Cross Sections Edmon et al. (1980)

5. Two-layer Flows in Rotating Channels.

Nonlinear Balance on an Equatorial Beta Plane

5 Shallow water Q-G theory.

Modeling Large-Scale Atmospheric and Oceanic Flows 2

GFD 2012 Lecture 1: Dynamics of Coherent Structures and their Impact on Transport and Predictability

Rotating stratified turbulence in the Earth s atmosphere

PAPER 58 STRUCTURE AND EVOLUTION OF STARS

Wind-driven Western Boundary Ocean Currents in Terran and Superterran Exoplanets

Baroclinic Rossby waves in the ocean: normal modes, phase speeds and instability

7. Basics of Turbulent Flow Figure 1.

Review of fluid dynamics

( ) = 1005 J kg 1 K 1 ;

The general circulation: midlatitude storms

Effective Depth of Ekman Layer.

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

Dynamic Meteorology - Introduction

Chapter 3. Stability theory for zonal flows :formulation

Dynamics of wind-forced coherent anticyclones in the open ocean

Transcription:

MATHEMATICAL TRIPOS Part III Wednesday, 1 June, 2016 1:30 pm to 4:30 pm Draft 21 June, 2016 PAPER 333 FLUID DYNAMICS OF CLIMATE Attempt no more than THREE questions. There are FOUR questions in total. The questions carry equal weight. STATIONERY REQUIREMENTS Cover sheet Treasury Tag Script paper SPECIAL REQUIREMENTS None You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator.

1 2 The wind blows on the surface of the ocean and exerts horizontal stresses (X,Y) in the x and y directions, respectively. By consideration of the net force on a thin horizontal slab, show that the linearised horizontal momentum equations on an f-plane are u t fv = 1 ρ p x + 1 ρ X z, v t +fu = 1 ρ p y + 1 ρ Y z, where the usual notation is applied and subscript indicates partial differentiation. The wind produces an Ekman layer near the surface where stresses are important and a lower region where they are not. Divide the flow into a pressure-drivenpart (u P,v P ) outside the surface Ekman layer and a stress-driven part (u E,v E ) inside the Ekman layer, and write down the momentum equations for both parts. By integrating across the Ekman layer show, for steady flow, that the vertical Ekman velocity w E at the base of the Ekman layer is where (X s,y s ) are the surface stresses. w E = 1 ρf (Y s x X s y), In the case where the surface stress is transmitted by laminar viscosity ν, by considering u E +iv E, find the velocity profile in the Ekman layer and show that and fν fν X s = ρ 2 (up v P ), Y s = ρ 2 (up +v P ), w E = 1 ν ρf 2f (p xx +p yy ). Now consider the ocean as a shallow layer of depth H and free surface elevation η. The forced, linearised shallow water equations below the Ekman layer are where w E = η E t. u t fv = gη x, v t +fu = gη y, η t +H(u x +v y ) = η E t, This pumping causes the ocean to spin down on a time scale τ. Assuming fτ 1 show that (η xx +η yy f2 c 2 η) t = 1 fν H 2 (η xx +η yy ), where c = gh. Find the spin down timescale τ for a sinusoidal disturbance of wavenumber κ and show that it is independent of κ for disturbances with scales small

3 compared with the Rossby radius of deformation. In the case when the scales are large compared to the deformation scale show that disturbances decay with a diffusivity K E fν K E = g 2 /f2. [TURN OVER

2 4 The linearised shallow water equations for a single layer of fluid of constant depth H on a f-plane reduce to a single equation for the free surface elevation η η tt +f 2 η c 2 (η xx +η yy ) = Hf q, where q = h u ηf/h, h is the horizontal gradient operator c 2 = gh and f = f. Give a physical interpretation of q Consider a layer of fluid initially at rest and for which at t = 0, η(x,0) = η 0 sgn(x). Show that this initial state adjusts to a final state given by η = η 0 { 1 e x/r D, x > 0, 1+e x/r D, x < 0, where R D = c/f. Show also that the volume flux of the adjusted flow in the y direction is 2c 2 η 0 /f. Now consider the case where the depth is discontinuous along the x axis H = { H, y < 0, H +, y > 0, where H < H +, so that the flux leaving the step y > 0 is greater than that arriving from the shallow side y < 0. This difference is accommodated by a double Kelvin wave in which flow is directed along the step and surface elevation approaches η 0 as y ± given by η = η 0 sgn(x) A(x,t)e y /R± D, where R ± D = gh ± f 1, and where A(x,t) is to be determined. Using geostrophy and the fact that Hv is continuous at y = 0, show that where c = gh + gh. A t + ca x = cη 0 δ(x), (1) Find the solution of (1) subject to A(x,0) = 0, and show that the step acts as a complete barrier to the flow.

5 3 The shallow water potential vorticity (PV) is q = f +ζ H, (1) where f is the Coriolis parameter, ζ is the vertical component of the relative vorticity, and H is the fluid depth. i) Describe the response of a parcel of fluid in the two following scenarios, providing a brief physical interpretation in each case: a) A vertical column of fluid moves into deeper water at the same latitude b) A vertical column of fluid moves towards the equator without changing its relative vorticity. ii) Starting from the shallow water PV conservation equation, or otherwise, derive an expression for the quasi-geostrophic PV. Explicitly state all assumptions required. iii) A depth-independent(barotropic) jet, U(y), flows from the west to the east. Starting from the QG equations and invoking the beta-plane approximation, derive the dispersion relation for linear plane waves. iv) A uniform wind, U, blows from the west to the east over an isolated mountain and generates waves whose phase is stationary with respect to the ground. Using your result from the previous part, find an expression for the wavelength and group velocity of these waves. Sketch the region containing all waves generated between times 0 < t < τ. What happens if the wind instead blows from the east to the west? [TURN OVER

4 6 Potential vorticity conservation for forced shallow water flow in the ocean can be written ( ) D f +ζ = F Dt H H r ζ, (1) H where D/Dt is the material derivative, ζ is the vertical component of the relative vorticity, f is the Coriolis parameter, H is the fluid depth, F represents forcing by a wind stress curl, and r is a decay rate associated with bottom stress. i) Show that the depth-integrated velocity can be written in terms of a streamfunction, ψ, and obtain an expression relating the streamfunction to the vorticity, ζ. ii) Consider steady circulation with small Rossby number, but do not assume that changes in the fluid depth, H are small relative to the total depth. Show that the streamfunction satisfies the following equation ũ ψ = r H ψ H 2 ψ F r H 2, (2) and obtain an expression for the pseudovelocity, ũ. Find the general solution for ψ for the unforced problem with r = F = 0. iii) A uniform depth fluid is forced by a sinusoidal wind stress curl, F = sin(2πy/l y ) in the domain 0 y L y. If the bottom stress is relatively weak compared with the wind stress, find the corresponding solution for Sverdrup flow. Define dimensional scales and state when Eq. 2 approximately satisfies Sverdrup balance. iv) Consider forcing by a point source, F = δ(x x 0 ). For a uniform depth fluid under the β-plane approximation, sketch contours of ψ satisfying Eq. 2 far from boundaries but without assuming that r is small. Note, you do not need to obtain an explicit expression for ψ. v) Consider a rectangular basin in the region 0 x L x, 0 y L y, where the fluid depth, H(x), is a parabolic function of x and H(x = 0) = H(x = L x ) = 0. Invoking the β-plane approximation, find an expression for the pseudovelocity, ũ, defined above. Sketch contours of ψ associated with the steady state circulation associated with a sinusoidal wind stress curl F = sin(2πy/l y ). Comment on the possible connection with your sketch and western boundary currents. You do not need to obtain an explicit expression for ψ. END OF PAPER