Energy Injection into Two-dimensional Turbulence: a Scaling Regime - - PowerPoint PPT Presentation
Energy Injection into Two-dimensional Turbulence: a Scaling Regime - - PowerPoint PPT Presentation
Energy Injection into Two-dimensional Turbulence: a Scaling Regime Controlled by Drag Yue-Kin Tsang Scripps Institution of Oceanography University of California, San Diego William R. Young Forced-dissipative 2D Systems Conducting fluid layer
Forced-dissipative 2D Systems
Conducting fluid layer
Paret and Tabeling (1998) http://www.fluid.tue.nl
f(x, t) ∼ I(t) × B(x) bottom wall friction
Forced-dissipative 2D Systems
Conducting fluid layer
Paret and Tabeling (1998) http://www.fluid.tue.nl
f(x, t) ∼ I(t) × B(x) bottom wall friction Soap film
Burgess et al. (1999)
driving belt induced motion drag from surrounding gas
Forced-dissipative 2D Systems
Conducting fluid layer
Paret and Tabeling (1998) http://www.fluid.tue.nl
f(x, t) ∼ I(t) × B(x) bottom wall friction Soap film
Burgess et al. (1999)
driving belt induced motion drag from surrounding gas The Ocean
wind✲
- J. M. Toole (1996)
wind forcing, lunisolar tide sea floor drag, instabilities
Forced-dissipative 2D Systems
Conducting fluid layer
Paret and Tabeling (1998)
Soap film The Ocean
wind✲
- J. M. Toole (1996)
Forcing (energy input) Nonlinear interaction (energy redistributed) Dissipation (energy removed)
How much power is needed to drive these systems?? =
ε
Energy Injection Rate
Pulling a block on a rough surface by a constant force Newton’s second law, F − µv = mdv dt Steady state velocity, v = F µ Energy injection rate (Power input), ε = Fv = F
- F
µ
- ∼ µ−1
Dependence of ε on µ
Forced harmonic oscillator ¨ x + ω 2
0 x = −µ ˙
x + A cos ωt instantaneous : εint(t) = ˙ x(t) A cos ωt averaged : ε = 1 T T εint(t′) dt′
Dependence of ε on µ
Forced harmonic oscillator ¨ x + ω 2
0 x = −µ ˙
x + A cos ωt instantaneous : εint(t) = ˙ x(t) A cos ωt averaged : ε = 1 T T εint(t′) dt′
ε
µ µ∗(ω) ∼µ ∼µ−1
Two-dimensional turbulence
ζt + u · ∇ζ = f(x, t) − µζ + ν∇2ζ u = (u, v) ζ ≡ vx − uy = ∇2ψ Energy injection rate ε = −ψ f Power Integral (conservation of energy) ε = µ u2 + v2
- εµ
+ ν ζ2
- εν
small-scale forcing: f = τ−2
f cos(kfx), k−1 f
≪ box size drag is the main dissipative mechanism: εµ ≫ εν
Numerical Model
ζt + u · ∇ζ = cos x − µζ − ν∇8ζ L = 32(2π) N = 10242 µ = 0.007 ν = 10−5 ε = ζ cos x εint(t) = ζ cos x
x,y
Instantaneous energy injection rate
1000 2000 3000 4000
t/τf
0.0 0.1 0.2 0.3
instantaneous energy injection rate, energy dissipation due to drag hyperviscous energy dissipation
5 10 15 20 Probability density function of 0.1 0.2 0.3
mean = 0.154 standard deviation = 0.019
εint(t)
εint(t)
εint(t) = 1 L2
- ζ(x, y, t) cos x dxdy
ε = 1 t1 − t0 t1
t0
εint(t′) dt′
Energy Injection Rate vs. Drag
0.0 0.2 0.4 0.6 0.8 0.0 0.2 0.4 0.6 0.8 1.0
ε µ
ζL = cos x
µ+ν
ε ≈
1 2µ
✚ ✚ ❂ ❏ ❏ ❪ ❆ ❆ ❑ ✛
Scaling Law for ε(µ)
0.001 0.010 0.100 µ 0.1 0.5 ε
L=32(2π), ν=10
−5
, N=1024
2
L=128(2π), ν=2.5x10
- 3
, N=2048
2
4 8 16 32 64
L/2π
0.12 0.14 0.16
0.45
1 3
µ=0.004
/ Results are insensitive to ν and (large enough) L
Theory: The Model
ζ(x, y, t) = A(t) cos(k fx) + B(t) sin(k fx)
- forced mode, ˆ
ζ(x,t)
+ ˜ ζ(x, y, t) ε = (k f/τ f)2 ˆ ζ cos(k fx)
- Random Sweeping Model
ˆ ζt + U ˆ ζx + V ˆ ζy = τ−2
f cos(k fx) − µ ˆ
ζ − η ˆ ζ (1) ε ≈ µU2 + V2 ≈ 2µU2 (2)
Theory: The Model
ζ(x, y, t) = A(t) cos(k fx) + B(t) sin(k fx)
- forced mode, ˆ
ζ(x,t)
+ ˜ ζ(x, y, t) ε = (k f/τ f)2 ˆ ζ cos(k fx)
- Random Sweeping Model
ˆ ζt + U ˆ ζx + V ˆ ζy = τ−2
f cos(k fx) − µ ˆ
ζ − η ˆ ζ (1) ε ≈ µU2 + V2 ≈ 2µU2 (2) advection by large-scale eddies (U, V) isotropic: U2 = V2 = U2
rms
vary on scales ≫ k−1
f
large-eddy turnover time ∼ µ−1 ≫ Urmsk f
Theory: The Model
ζ(x, y, t) = A(t) cos(k fx) + B(t) sin(k fx)
- forced mode, ˆ
ζ(x,t)
+ ˜ ζ(x, y, t) ε = (k f/τ f)2 ˆ ζ cos(k fx)
- Random Sweeping Model
ˆ ζt + U ˆ ζx + V ˆ ζy = τ−2
f cos(k fx) − µ ˆ
ζ − η ˆ ζ (1) ε ≈ µU2 + V2 ≈ 2µU2 (2) advection by large-scale eddies (U, V) isotropic: U2 = V2 = U2
rms
vary on scales ≫ k−1
f
large-eddy turnover time ∼ µ−1 ≫ Urmsk f nonlinear energy transfer out of the forced mode η ≫ µ ≫ ν
Theory: The Solution
ˆ ζt + U ˆ ζx + V ˆ ζy = τ−2
f cos(k fx) − µ ˆ
ζ − η ˆ ζ Neglect µ (η ≫ µ) and seek steady-state solution, U ˆ ζx = τ−2
f cos(k fx) − η ˆ
ζ Since U(x, y) varies on the large scales, ˆ ζ ≈ cos(k fx − φ) τ2
f
- η2 + (Uk f)2
, tan φ = Uk f η
Theory: The Solution
ˆ ζt + U ˆ ζx + V ˆ ζy = τ−2
f cos(k fx) − µ ˆ
ζ − η ˆ ζ Neglect µ (η ≫ µ) and seek steady-state solution, U ˆ ζx = τ−2
f cos(k fx) − η ˆ
ζ Since U(x, y) varies on the large scales, ˆ ζ ≈ cos(k fx − φ) τ2
f
- η2 + (Uk f)2
, tan φ = Uk f η ˆ ζ Forcing
small U φ → 0 large U φ → π/2
Theory: The Scaling Law
typical η Ukf ∼ η Urmskf = transfer rate sweeping rate ≡ α η ∼ shear at kf ∼ ε
1 3
( shear ∼ k [kE(k)]
1 2 )
Urmskf ∼ ε
1 2 µ− 1 2
(ε ≈ 2µU2
rms)
α ∼ µ
4 9
(anticipate ε ∼ µ
1 3 )
Theory: The Scaling Law
typical η Ukf ∼ η Urmskf = transfer rate sweeping rate ≡ α η ∼ shear at kf ∼ ε
1 3
( shear ∼ k [kE(k)]
1 2 )
Urmskf ∼ ε
1 2 µ− 1 2
(ε ≈ 2µU2
rms)
α ∼ µ
4 9
(anticipate ε ∼ µ
1 3 )
From definition of ε, ε ∼ ˆ ζ cos(kfx)
- ∼
- η
η2 + (Ukf )2
- Let U′ = U/Urms and η′ = η/η ,
ε ∼ 1 Urms
- αη′
(αη′)2 + U′2 P(U′, η′) dU′dη′
Theory: The Scaling Law
small φ
typical η Ukf ∼ η Urmskf = transfer rate sweeping rate ≡ α η ∼ shear at kf ∼ ε
1 3
( shear ∼ k [kE(k)]
1 2 )
Urmskf ∼ ε
1 2 µ− 1 2
(ε ≈ 2µU2
rms)
α ∼ µ
4 9
(anticipate ε ∼ µ
1 3 )
From definition of ε, ε ∼ ˆ ζ cos(kfx)
- ∼
- η
η2 + (Ukf )2
- Let U′ = U/Urms and η′ = η/η ,
ε ∼ 1 Urms
- αη′
(αη′)2 + U′2
- δ(U′) as α→0
P(U′, η′) dU′dη′
Theory: The Scaling Law
small φ
typical η Ukf ∼ η Urmskf = transfer rate sweeping rate ≡ α η ∼ shear at kf ∼ ε
1 3
( shear ∼ k [kE(k)]
1 2 )
Urmskf ∼ ε
1 2 µ− 1 2
(ε ≈ 2µU2
rms)
α ∼ µ
4 9
(anticipate ε ∼ µ
1 3 )
From definition of ε, ε ∼ ˆ ζ cos(kfx)
- ∼
- η
η2 + (Ukf )2
- Let U′ = U/Urms and η′ = η/η ,
ε ∼ 1 Urms
- αη′
(αη′)2 + U′2
- δ(U′) as α→0
P(U′, η′) dU′dη′ So, ε ∼ U−1
rms and ε ≈ 2µU2 rms imply:
ε ∼ µ
1 3
Summary
study energy injection rate ε in two-dimensional turbulence with drag µ and a prescribed small-scale body force discover a new scaling regime: ε ∼ µ
1 3
as µ → 0 random sweeping model suggests energy input is mainly due to regions with small velocity
0.001 0.010 0.100 µ 0.1 0.5 ε
L=32(2π), ν=10
−5
, N=1024
2
L=128(2π), ν=2.5x10
- 3
, N=2048
2
4 8 16 32 64
L/2π
0.12 0.14 0.16
0.45
1 3
µ=0.004