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2D Turbulence

Paul Cueva and Sean Seyler

Cornell University

pdc23@cornell.edu, sls374@cornell.edu

December 14, 2011

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 1 / 28

Overview

1 Why 2D turbulence?

2 2D turbulence: the inverse cascade of energy to long length-scales

3 A brief review of fluid dynamics

4 Band-limited forcing and power laws

5 Energy transfer in 2D versus 3D turbulence

6 Applying RG methods to 2D turbulence?

7 Stochastic forcing of 2D N-S

8 A nice way to conclude our discussion

9 Acknowledgments

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 2 / 28

Approximate 2D systems: atmospheric dynamics

Turbulence on the sphere

Assume surface effects dominate

Weather prediction

Figure: Earth’s atmosphere

Source: The New Republic (website)

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 3 / 28

2D turbulence: the inverse cascade of energy to longlength-scales

Bubbles

Immiscible liquids

Figure: Turbulence on a soap film

Source: Fotolog website

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 4 / 28

Tractable problem: conformal solution by Polyakov

Shown to exist for every case

Doesn’t mean it’s easy to understand...

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 5 / 28

Tractable problem: allegorical/numerical solution byOnsager, Kraichnan

Problem related to solvable ones: lattice/vortex gas

Can get scaling and statistics

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 6 / 28

Tractable problem: statistical solution by Miller and Cross

Equilibrium solution maximizes entropy

Quite different from standard stat physics (more on this soon)

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 7 / 28

2D turbulence: the inverse cascade of energy to longlength-scales

〈 vor nf early.mov 〉 〈 psi nf early.mov 〉

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 8 / 28

2D turbulence: the inverse cascade of energy to longlength-scales

〈 psi nf late.mov 〉

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 9 / 28

A brief review of fluid dynamics

2D Navier-Stokes:

∂u

∂t+ u · ∇u = −∇p

ρ+ ν∇2u

Incompressibility:∇ · u = 0

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 10 / 28

A brief review of fluid dynamics

2D Navier-Stokes and incompressibility

∂u

∂t+ u · ∇u = −∇p + ν∇2u ∇ · u = 0

In 2D, the vorticity is a scalar (in the z-direction):

ω = (∇× u) · z

For 2D only, we can define the stream function ψ, where:

u = −z×∇ψ

ω = −∇2ψ

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 11 / 28

A brief review of fluid dynamics

Fourier transformed 2D vorticity equation

∂ωk

∂t+∑k′

Mk,k′ωk′ωk−k′ = νk2ωk k · u(k, t) = 0

Mk,k′ takes care of the nonlinear term:

Mk,k′ =z · (k× k′)

2

(1

k ′− 1

k

)

Nonlinear advection term responsible for energy transfer to differentlength-scales

Energy transfer T (k , q, p) occurs between a triad of wave numbers:

k → k k ′ → q k − k ′ → p

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 12 / 28

Constants of motion for 2D turbulence

Infinite number of constants of motion of the form:∮u · dl =

∫ω · dS = const

The only other invariants are quadratic in ω:

Conservation of energy

∂E

∂t=

∂

∂t〈|uk |2〉 = 〈ω

2k

k2〉 = 0

Conservation of enstrophy

∂

∂tΩ =

∂

∂t〈k2 |uk |2〉 =

∂

∂t〈ω2

k〉 = 0

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 13 / 28

Power laws in the band-limited forcing (BLF) energyspectrum

Figure: Long-time energy spectrum of 2D N-Swith BLF

Figure: Energy pileup at small wavenumbersdue to finite grid size

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 14 / 28

The inverse cascade as seen from the BLF energy spectrum

Inverse cascade?

The energy ”cascades” or ”is pumped” from shorter to longer length scales

〈 bl spec 256.mov 〉

This phenomenon is due solely to the nonlinear term in N-S

If dissipative (viscous) forces dominate (the nonlinear term):

There will be no cascade

The power law will be flat for k < kforcing

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 15 / 28

Features of 2D turbulence

Locality of energy transfer

Small eddies swept along by large eddies

Similar-sized eddies coalesce

(Board algebra to introduce 2D energy transfer)

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 16 / 28

Comparison with features of 3D turbulence

3D vortex stretching

Kolmogorov energy cascade

Equilibrium (direct cascade)

Energy goes to high wavenumbers

Viscosity damps out high wavenumbers

For numerical solutions, grid cell size can act as viscous cutoff

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 17 / 28

Power law prediction through dimensional analysis

(More board work to reproduce energy and enstrophy cascade powerlaws)

2D gives ”inverse energy cascade” and ”direct enstrophy cascade”

→ energy cascades to small wavenumbers

→ enstrophy cascades to large wavenumbers

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 18 / 28

Power law prediction through dimensional analysis

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 19 / 28

Onsager/Kraichnan’s point vortex gas

Considers point vortices interacting with near neighbors

End up with vortex segregation with disorder/”temperature” comingfrom forcing

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 20 / 28

Point vortex simulation using particle-in-cell method

Source: Joyce and Montgomery

Red and green regionscorrespond to oppositely-signedpoint vortices

Left snapshot at t = 0 withchecker board initial condition

Right shows like-signed pointvortices clustering at t = 50

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 21 / 28

Stochastic forcing of 2D N-S

FT 2D stream function equation with stochastic forcing

ψk +∑k′

Mk,k′ψk′ψk−k′ + νk2ψk = Wk(t)

The stochastic (white noise) term Wk has:

an amplitude selected at random from a time-scaled Gaussiandistribution at each time step

a randomly-selected phase at each time step

→ Scaled random walk in time applied at each k (Brownianmotion)

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 22 / 28

Stochastic forcing of 2D N-S

FT 2D stream function equation with stochastic forcing

ψk +∑k′

Mk,k′ψk′ψk−k′ + νk2ψk = Wk(t)

To get the stochastic term Wk:

Using theory of hydrodynamic fluctuations, consider fluctuations inpressure tensor δP

δP turns out to be anti-symmetric

Taking curl of N-S (to get vorticity equation) gives white noisefluctuation term: ∇2W

ω = −∇2ψ → only have W in equation of motion for stream function

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 23 / 28

White-noise Forcing of 2D N-S

〈 vor wn.mov 〉 〈 psi wn.mov 〉

Ising-model-like scale invariance

Like-signed vortices cluster → correlation with neighbors

Striking similarities to MD simulations of Onsager’s discrete vortexmodel

Thermal fluctuations give rise to discrete vortices on dissipation scale?

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 24 / 28

Energy spectrum for white noise forced fluid

Figure: Energy spectrum shows evidence of k−5/3 power law

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 25 / 28

Miller and Cross and a thermodynamic explanation of theinverse cascade

Final state of 2D turbulent system should maximize entropy

Clustering of local regions of vorticity maximizes number ofmicrostates

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 26 / 28

Acknowledgments

Charles Seyler - Mentor, architect and designer of code used forsimulation

Jane Wang - Informal guide in the world of turbulence

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 27 / 28

References

C. Seyler (1975)

Guiding-Center Plasmas and Inviscid Navier-Stokes Fluids in Two Dimensions

Ph.D. thesis, University of Iowa

G. Joyce and D. Montgomery (1973)

Negative Temperature States for the Two-Dimensional Guiding-Centre Plasma

J. Plasma Physics 10, 1, pp. 107-121

J. Miller, P. Weichmann, and M. Cross (1992)

Statistical Mechanics, Euler’s Equation, and Jupiter’s Red Spot

Phys. Rev. A 45, 2328-2359

M. Bajic (2010)

Onsager Theory of Hydrodynamic Turbulence

Seminar, University of Ljubljana

M. Rivera (2000)

The Inverse Energy Cascade of Two-Dimensional Turbulence

Ph.D. Thesis, University of Pittsburgh

R. Kraichnan (1967)

Inertial Ranges in Two-Dimensional Turbulence

Phys. Fluids 10, 1417

R. Kraichnan and D. Montgomery (1980)

Two-dimensional Turbulence

Rep. Prog. Phys. 43, 43547

Paul Cueva and Sean Seyler (Cornell) 2D Turbulence December 14, 2011 28 / 28