27.02.2013 Views

Wind Energy

Wind Energy

Wind Energy

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

24<br />

Scaling Turbulent Atmospheric Stratification:<br />

A Turbulence/Wave <strong>Wind</strong> Model<br />

S. Lovejoy and D. Schertzer<br />

Summary. Twenty years ago, it was proposed that atmospheric dynamics are<br />

scaling and anisotropic over a wide range of scales characterized by an elliptical<br />

dimension Ds = 23/9, shortly thereafter we proposed the continuous cascade<br />

“fractionally integrated flux” (FIF) model and somewhat later, causal space–time<br />

extensions with Dst =29/9. Although the FIF model is more physically satisfying<br />

and has been strikingly empirically confirmed by recent lidar measurements (finding<br />

Ds =2.55±0.02, Dst =3.21±0.05) in classical form, its structures are too localized,<br />

it displays no wave-like phenomenology.<br />

We show how to extend the FIF model to account for more realistic wavelike<br />

structures. This is achieved by using both localized and unlocalized space–time<br />

scale functions. We display numerical simulations which demonstrate the requisite<br />

(anisotropic, multifractal) statistical properties as well as wave-like phenomenologies.<br />

24.1 Introduction<br />

According to a growing body of analysis and theory (e.g., [1–5] and references<br />

therein) the 1D horizontal sections of the atmosphere follow Kolmogorov laws:<br />

∆ν = ε 1/3 ∆x 1/3 and (assuming no overall advection/wind): ∆ν = ε 1/2 ∆t 1/2 ,<br />

where ε is the energy flux. However, 1D vertical sections follow the Bolgiano–<br />

Obukov law: ∆ν = φ 1/5 ∆z 3/5 , φ the buoyancy variance flux. The generalization<br />

to arbitrary space–time displacements ∆R = (∆r, ∆t), ∆r =<br />

(∆x, ∆y, ∆z), and multifractal statistics is the 23/9D spatial model, 29/9D<br />

space–time model. The anisotropic extension of the Kolmogorov law for the<br />

velocity (v) and of the Corrsin–Obukov law for passive scalar density (ρ)<br />

satisfy<br />

∆v (∆R) =ε 1/3<br />

[∆R] [[∆R]]1/3 ; ∆ρ (∆R) =χ 1/2<br />

[∆R] ε−1/6<br />

[∆R] [[∆R]]1/3 , (24.1)<br />

where ε and χ are the (multifractal) energy and passive scalar variance fluxes;<br />

the subscripts indicate the scale at which they are averaged. The key idea<br />

of this model is that the physical scale function [[∆R]] replaces the usual

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!