Rotating stratified turbulence in the Earth s atmosphere

Similar documents
2. Baroclinic Instability and Midlatitude Dynamics

ATMOSPHERIC AND OCEANIC FLUID DYNAMICS

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

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

Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

6 Two-layer shallow water theory.

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

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

Transformed Eulerian Mean

A Truncated Model for Finite Amplitude Baroclinic Waves in a Channel

Diagnosing the vertical structure of the eddy diffusivity in real and idealized atmospheres

Diagnosing the Vertical Structure of the Eddy Diffusivity in Real and Idealized Atmospheres

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

Nonlinear baroclinic dynamics of surface cyclones crossing a zonal jet

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

The impacts of stochastic noise on climate models

ROSSBY WAVE PROPAGATION

Equatorial Superrotation on Tidally Locked Exoplanets

Boundary layer controls on extratropical cyclone development

PHY2504 Course Project: Zonal Momentum Balance, Entropy Transport, and the Tropopause

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

A mechanistic model study of quasi-stationary wave reflection. D.A. Ortland T.J. Dunkerton NorthWest Research Associates Bellevue WA

Eliassen-Palm Theory

Lecture 10a: The Hadley Cell

Dynamics of Giant Planet Atmospheres. Tapio Schneider (with Junjun Liu) California Institute of Technology

Part-8c Circulation (Cont)

The general circulation: midlatitude storms

CHAPTER 4. THE HADLEY CIRCULATION 59 smaller than that in midlatitudes. This is illustrated in Fig. 4.2 which shows the departures from zonal symmetry

Imperial College London

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.

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

Dynamics of the Zonal-Mean, Time-Mean Tropical Circulation

Q.1 The most abundant gas in the atmosphere among inert gases is (A) Helium (B) Argon (C) Neon (D) Krypton

The general circulation of the atmosphere

GFD II: Balance Dynamics ATM S 542

Grand Challenges in Global Circulation Dynamics

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

SMS 303: Integrative Marine

The stratospheric response to extratropical torques and its relationship with the annular mode

8 Baroclinic Instability

Atmosphere, Ocean and Climate Dynamics Fall 2008

Dynamics of the Extratropical Response to Tropical Heating

Scales of Linear Baroclinic Instability and Macroturbulence in Dry Atmospheres

Equatorial superrotation in shallow atmospheres

Ocean dynamics: the wind-driven circulation

Schematic from Vallis: Rossby waves and the jet

Modeling the atmosphere of Jupiter

The General Circulation of the Atmosphere

The Planetary Circulation System

Chapter 3. Stability theory for zonal flows :formulation

ESCI 344 Tropical Meteorology Lesson 11 Tropical Cyclones: Formation, Maintenance, and Intensification

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

Macroturbulent cascades of energy and enstrophy in models and observations of planetary atmospheres

Vortices in the ocean. Lecture 4 : Baroclinic vortex processes

Dynamics Rotating Tank

warmest (coldest) temperatures at summer heat dispersed upward by vertical motion Prof. Jin-Yi Yu ESS200A heated by solar radiation at the base

t tendency advection convergence twisting baroclinicity

Geostrophic turbulence: How Jupiter got its stripes? D. Gurarie Math. Department CWRU Cleveland, Ohio

Ocean Dynamics. The Great Wave off Kanagawa Hokusai

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

Dynamics of Baroclinic Multiple Zonal Jets

Model equations for planetary and synoptic scale atmospheric motions associated with different background stratification

Spherical Shallow Water Turbulence: Cyclone-Anticyclone Asymmetry, Potential Vorticity Homogenisation and Jet Formation

Sensitivity of zonal-mean circulation to air-sea roughness in climate models

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

14.1 Simple model of global radiation balance

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

Persistent multiple jets and PV staircase

Frictional Damping of Baroclinic Waves

Reduction of the usable wind work on the general circulation by forced symmetric instability

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

Eddy-Mediated Regime Transitions in the Seasonal Cycle of a Hadley Circulation and Implications for Monsoon Dynamics

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

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

2/15/2012. Earth System Science II EES 717 Spring 2012

Chapter 13 Instability on non-parallel flow Introduction and formulation

Equilibration of Baroclinic Turbulence in Primitive Equations and Quasigeostrophic Models

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

Stratospheric Dynamics and Coupling with Troposphere and Mesosphere

A Uniform PV Framework for Balanced Dynamics

Modeling Large-Scale Atmospheric and Oceanic Flows 2

3. Midlatitude Storm Tracks and the North Atlantic Oscillation

A more detailed and quantitative consideration of organized convection: Part I Cold pool dynamics and the formation of squall lines

Recovery of atmospheric flow statistics in a general circulation model without nonlinear eddy-eddy interactions

Course , General Circulation of the Earth's Atmosphere Prof. Peter Stone Section 9: Numerical Models

Internal boundary layers in the ocean circulation

How does the stratosphere influence the troposphere in mechanistic GCMs?

Response of Baroclinic Life Cycles to Barotropic Shear

Climate Change and Variability in the Southern Hemisphere: An Atmospheric Dynamics Perspective

The Turbulent Oscillator: A Mechanism of Low-Frequency Variability

Climate Change on Jupiter. Philip Marcus University of California at Berkeley

Goals of this Chapter


STRATOSPHERIC DYNAMICS

Quasi-geostrophic system

Atmospheric dynamics and meteorology

Circulation and Vorticity

no eddies eddies Figure 3. Simulated surface winds. Surface winds no eddies u, v m/s φ0 =12 φ0 =0

QBO-Like Oscillation in a Three-Dimensional Minimal Model Framework of the Stratosphere Troposphere Coupled System

Transcription:

Rotating stratified turbulence in the Earth s atmosphere Peter Haynes, Centre for Atmospheric Science, DAMTP, University of Cambridge. Outline 1. Introduction 2. Momentum transport in the atmosphere 3. Self-organisation of turbulent flows 4. Mechanisms for variability 1

Background Physical parameters Coriolis parameter f 10 4 s 1. Buoyancy frequency N 10 2 s 1. Density scale height H 7 km. Depth of troposphere D 10 km. Radius a 6400 km. For large-scale circulation F r 1, Ro 1. Waves and Eddies Balanced: Rossby waves (sources include flow over topography, internal heating, dynamical instabilities). Non-balanced: Inertio-gravity waves (sources include flow over topography, convection). 2

Balanced motion is described by potential vorticity (PV) advection plus inversion operator Simplest paradigm: 2-D vorticity equation ζ t + u. ζ = ζ t + J(ψ, ζ) = 0 ζ determines ψ (and hence u) by solving the Poisson equation 2 ψ = ζ (requires boundary conditions on ψ or its gradient). ψ is determined by applying an inversion operator to ζ. ψ = 2 ζ. (Point vortex is example.) Vorticity (generalise to PV) is advected by flow and instantaneously determines all flow quantities. 3

Vertical momentum transport by gravity waves: the equatorial QBO Radiosonde data (Labitzke et al 2002) Numerical model (Horinuchi and Yoden 1998) 4

Organisation of momentum fluxes (Horinuchi and Yoden 1998) 5

Horizontal momentum transport by Rossby waves: equatorial superrotation Williams (2003) 6

Jets in β-plane turbulence. 2-D flow with random small-scale forcing. β = 0: upscale energy cascade, energy dissipated at largest available scale. β 0: formation of jets in x-direction, with finite separation (U/β) 1/2 (Rhines radius), where U is typical velocity. Danilov and Gurarie (2004) 7

Energy vs time, vorticity vs time, with and without friction (DG2004). 8

Dynamical self-organisation Jets are transport barriers, separated by mixing regions. PV has sharp jump across jet, approximately constant across mixing regions. Stirring and mixing is relatively inhibited by strong PV gradients, relatively enhanced by weak PV gradients. This suggests natural self-organisation into piecewise constant PV regions separated by sharp gradients. Role of long-range momentum transport by waves? Do we need analytical model before accepting this as fundamental process? 9

An idealised GFD Problem Continuously stratified quasi-geostrophic β-plane channel flow. Thermal relaxation (rate κ T ) towards a temperature profile consistent with a broad jet-like flow with vertical shear U e (y, z) (hence baroclinically unstable). Rigid upper and lower boundaries. Ekman friction κ M at lower boundary only. 10

QG PV equation (layer-wise 2D motion, with flow at given level determined by potential vorticity field over range of levels) Interior (PV advection) with ( t ψ y x + ψ x y )q = 0 q = 2 ψ x 2 + 2 ψ y 2 + z ( f 2 N 2 ψ z ) Horizontal boundaries (density/temperature advection) ( t ψ y x + ψ x y ) ψ z = 0 11

Results from 2-layer simulation Upper layer (central transport barrier) Lower layer (mixing across broad central region) 12

Transport and mixing structure in many-layer flow Transition level between upper and lower transport regimes 13

Doubly periodic simulations: multiple jets and multiple transport barriers Time development of flow Vertical structure of transport Vertical structure of velocity 14

Oceanic application? The Gulf Stream: barrier or blender? (Bower et al 1985). Horizontal tracer (O 2 ) gradient is large at upper levels, small at lower levels. Velocity structure continues below transition level in tracer gradient. 15

What determines position of tropopause? Radiative-equilibrium temperature profile is unstable near the ground, hence dynamical adjustment to temperature at low levels. Upper limit to this adjustment is the tropopause. Mechanism for dynamical adjustment? Moist-convective adjustment? OK in tropics, but in extratropics temperature profile is moist stable. Baroclinic eddies? (Held 1982) 16

Can a quasi-realistic extratropical tropopause arise solely through the action of baroclinic eddies? Numerical simulations in simplest possible model. Primitive equations on hemisphere. Only physics is thermal relaxation towards an equilibrium temperature profile that is smoothly varying in the vertical, and also in the horizontal, so that equilibrium state is baroclinically unstable. Integrate towards an equilibrium state determined by balance between baroclinic eddies and thermal relaxation 17

(a) PV in relaxation state (b), (c), (d) typical PV on different levels in statistical equilibrium flow (H, Greenslade and Scinocca, 2001) 18

Transport quantified by geometry of PV field mid-latitude transport barrier confined to upper regime 19

Longitudinal cross-sections Tropopause is mid-latitude transport barrier, plus mid- and high-latitude transition level. 20

Variability in jet/eddy dynamics: simple model (Lee 1997) 21

Variability in jet/eddy dynamics: 2000) atmosphere (Hartmann et al 22

Conclusion Many examples of counter-gradient eddy/wave momentum transport in atmosphere. Turbulence in presence of large-scale PV gradient naturally leads to multiple jets/transport barriers. Two-way feedback between eddies and jets is mechanism both for organisation and for variability. 23