k 2 E ( k , t ) dk E ( t ) = E ( k , t ) dk , Z ( t ) = start at - - PowerPoint PPT Presentation

k 2 e k t dk e t e k t dk z t start at k 0 go to k 1 k 0
SMART_READER_LITE
LIVE PREVIEW

k 2 E ( k , t ) dk E ( t ) = E ( k , t ) dk , Z ( t ) = start at - - PowerPoint PPT Presentation

Coherent Structures in Geophysical Turbulence Jeffrey B. Weiss University of Colorado, Boulder motivated by atmospheres and oceans study high resolution computations see organization into coherent structures model as dynamical


slide-1
SLIDE 1

Coherent Structures in Geophysical Turbulence

  • motivated by atmospheres and oceans
  • study high resolution computations
  • see organization into coherent structures
  • model as dynamical systems of interacting structures

Jeffrey B. Weiss University of Colorado, Boulder Collaborators: Bracco, di Frischia, von Hardenberg, McWilliams, Provenzale, Siegel, Yavneh

slide-2
SLIDE 2

What is Geophysical Turbulence?

  • large scale motion of atmospheres and oceans
  • extremely turbulent

large Reynolds number: Re =UL/ ν ~ O(108)

  • past many bifurcations

complex temporal behavior

  • large range of scales

room for complex spatial behavior

  • high dimensional

low-dimensional models inadequate but not 1023 - statistical mechanics inappropriate

  • needs fast computers with lots of memory
slide-3
SLIDE 3

Classes of Turbulence

  • 3D homogeneous isotropic turbulence
  • turbulent convection
  • geophysical turbulence
  • stable
  • rotating

weak vertical motions

  • anisotropic

thin fluid

  • similarities to 2D
slide-4
SLIDE 4

Environmental Influences

  • fast rotation

small Rossby number: Ro = U/ Lf <<1

  • strong stable stratification

small Froude number: F = U/ NH <<1

  • rotation and stratification => anisotropy
  • small vertical velocity

w << u, v

  • inverse turbulent cascade

=> coherent structures

slide-5
SLIDE 5

Inverse Cascade

  • inviscid invariants
  • energy spectrum
  • start at k0, go to k1=k0/2, k2=2k0:

E(k0) = E(k1)+E(k2) k0

2 E(k0) = k1 2 E(k1) + k2 2 E(k2)

=> E(k1) = 4 E(k2): inverse energy cascade => Z(k1) = Z(k2)/4: direct enstrophy cascade

E = 1 2 u2dV Z

= 1 2 q2dV

E(t) = E(k,t)dk, Z(t) =

k 2E(k,t)dk

slide-6
SLIDE 6

Dissipation

  • time dependence
  • since dZ/dt ≤ 0, Z(t) ≤ Z(0), and as ν ->0, dE/dt ->0
  • energy is conserved
  • enstrophy gradients grow so enstrophy dissipation

remains finite

  • enstrophy decays
  • connection to cascade:
  • dissipation acts at small scales

dE dt ~ −νZ dZ dt ~ −ν ∇Z

2

slide-7
SLIDE 7

Hurricane Dennis: August 1999

slide-8
SLIDE 8

Gulf Stream and Vortices

slide-9
SLIDE 9

Jupiter

from Cassini spacecraft, Nov 2000

slide-10
SLIDE 10
  • what we really want to predict
  • spatially localized
  • partly unknown how to derive them from PDE
  • provide reduced description
  • degrees of freedom:
  • N ~ O(10-100) structures
  • location
  • internal degrees of freedom
  • plus random component?
  • conjecture:

population of structures define attractor

Coherent Structures

slide-11
SLIDE 11

Structures vs. Wavenumbers

  • traditional theories of turbulence:
  • wavenumber space
  • random phase approx. common
  • structures:
  • local in physical space
  • random phase approximation fails
slide-12
SLIDE 12

Basic Approach

  • seek generic properties of planetary fluids
  • study simple planetary fluids
  • extrapolate to atmospheres and oceans
  • simple systems provide roadmap
slide-13
SLIDE 13

2D and QG Equations

  • same vorticity equation:

vorticity streamfunction

  • different vorticity - streamfunction relation

2D QG

qt +ψxqy −ψyqx = D + F q = ∇2D

2 ψ

q = ∇2D

2 ψ + ∂z

1 S(z)∂zψ

S=1

 →   ∇3D

2 ψ

q( r x ,t) ψ( r x ,t)

slide-14
SLIDE 14

2D Turbulence

vorticity colored blue (-) to red (+)

slide-15
SLIDE 15

2-Fluid View of 2D Turbulence

  • 1. coherent vortices
  • 2. classical turbulent background

structures arrest cascade, cause cascade theories to fail full field background

Bracco, et al, 2000a Siegel and W, 1997

slide-16
SLIDE 16

Vortex Dynamical Systems

  • structured component:
  • system of interacting vortices
  • statistics of vortex population
  • reduced degrees of freedom
  • conservative motion:
  • valid when structures well separated
  • Hamiltonian dynamics
  • hierarchy of models

– point vortices – elliptical vortices – etc.

slide-17
SLIDE 17

Dissipation

  • dissipation:
  • high Re => dissipation small, but not zero
  • character of dissipation:

– occurs when vortices close => rare – rapidly, and strongly transforms vortices – intermittency

  • punctuated dynamical system
  • Hamiltonian evolution
  • dissipative transformation at isolated points in time

jumps to new Hamiltonian

  • Re -> dissipation becomes more intermittent

slide-18
SLIDE 18

Simple Vortex Behavior in 2D Turbulence

same-sign merger four-vortex scattering

  • pposite-sign dipole

tripole merger

slide-19
SLIDE 19

Point Vortex Dynamics

  • N vortices
  • position zi=(xi,yi), circulation Γi
  • close pair decouples
  • isolated pair integrable

H = Γ

i i, j

Γj ln| zi − z j |

Γi dzi dt = J∇ ziH H = Hpair + Hothers +ε(t)Hinteraction

slide-20
SLIDE 20

More pv dynamics

  • low D integrable subsystem within high D

chaotic system

  • close pairs have long lifetimes
  • Cantori?
  • close pairs have high speeds
  • same-sign pairs rotate
  • opposite-sign pairs translate
slide-21
SLIDE 21

Point Vortex Velocity PDF

  • N=100, long integration, O(100 tturnover)
  • episodes of fast velocity due to close pairs

(Weiss, et al, 1998)

slide-22
SLIDE 22

More vel pdf

  • close pairs => flights
  • pdfs with long tails
  • non/slow ergodicity

Gaussian time avg ensemble avg

slide-23
SLIDE 23

2D Turbulence Velocity PDF

  • long tails due to vortices

(Bracco, et al, 2000b)

induced by background

induced by vortices

vort tot backgnd Gaussian

slide-24
SLIDE 24

3D QG Turbulence

potential vorticity colored blue (-) to red (+)

slide-25
SLIDE 25

Structure Based Scaling Theory

  • mean vortex theory
  • avg size, amplitude, …
  • global quantities due to vortex component
  • assumes
  • algebraic evolution t α
  • self-similar temporal evolution
  • a few exponents, predicts others

(Bracco, et al, 2000a)

slide-26
SLIDE 26

Scaling theory graphs

  • works well for 2D simulations
  • some controversy in experiments
  • OK in 3D QG simulations

(Bracco, et al, 2000a) (McWilliams, et al, 1999)

2D 3D QG

slide-27
SLIDE 27

Ocean Basin Turbulence

  • ocean more QG than atmosphere
  • basins boundaries
  • inhomogeneous
  • variation of Coriolis force with latitude
  • β-plane
  • horizontal anisotropy
  • allows jets
  • stationary turbulence
slide-28
SLIDE 28

Ocean Circulation

slide-29
SLIDE 29

QG Ocean Basin Model

(Siegel, et al, 2001)

  • QG PV eqn on β-plane
  • rectangular basin
  • 3200 x 3200 x 5 km
  • solid, no slip sides and bottom
  • vary horizontal resolution
  • six vertical levels
  • forcing
  • steady, zonal surface wind
  • bottom Ekman drag
  • massively parallel state-of-the-art code
slide-30
SLIDE 30

QG Ocean Basin Turbulence

increasing Reynolds number

slide-31
SLIDE 31

QG Ocean Basin Turbulence

Low Re: N = 256 Δx = 12.5 km

slide-32
SLIDE 32

QG Ocean Basin Turbulence

High Re: N = 2048 Δx = 1.6 km

slide-33
SLIDE 33

Jet as transport barrier

  • effective barrier at low Re
  • not a barrier at high Re
slide-34
SLIDE 34

′ v ′ q

q

′ v ′ q

q

′ v ′ q = −κ ∂q ∂y

N=256 N=2048

Eddy Diffusion:

κ > 0 κ < 0 κ > 0

slide-35
SLIDE 35

Ocean Basin Velocity PDF

  • long tails in models and obs
  • same cause?

QG Model and GCM Ocean Floats (Bracco, et al, 2000c)

Entire Basin

slide-36
SLIDE 36

Conclusions

  • coherent structures ubiquitous
  • seen empirically (obs and models)
  • no theory for existence
  • represent reduced degrees of freedom
  • dynamical system of interacting structures
  • punctuated dynamics
  • intermediate D = low D + high D?
  • coherent vortices responsible for non-Gaussian pdf?
  • eddies in ocean model cause
  • cross-jet transport
  • negative eddy diffusivity
slide-37
SLIDE 37

Blank