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74 François G. Schmitt<br />

13.2 Scaling and Intermittency of Velocity Fluctuations<br />

The scaling and intermittent properties of wind velocity have been studied in<br />

the turbulence community for several decades (see reviews in [1,3,4]). We recall<br />

here some basic properties of this framework. The Richardson–Kolmogorov<br />

energy cascade develops on the inertial range, between the large injection<br />

scale (of the order of several tens or hundreds of meters) towards dissipative<br />

scales (of the order of millimeters). In the inertial range, wind velocity<br />

fluctuations are scaling: they possess a power-law spectrum<br />

E(k) � k −β<br />

(13.1)<br />

with β =5/3 for K41 turbulence [5]; intermittency however leads to a β value<br />

slightly larger than 5/3. Here we may define intermittency as the property<br />

of having large fluctuations at all scales, having a correlated structure:<br />

large fluctuations are much more frequent than what would be obtained<br />

for Gaussian processes [1, 3, 4]. Intermittency is then classically characterized<br />

considering the probability density function (pdf) or the moments of<br />

the velocity fluctuations ∆Vℓ = |V (x + ℓ) − V (x)|. For large mean velocities,<br />

Taylor’s hypothesis may be invoked to relate time variations ∆Vτ =<br />

|V (t+τ)−V (t)| to spatial fluctuations; one may then study time intermittency<br />

of wind velocity considering the scaling property of moments of order q>0<br />

of the fluctuations ∆Vτ<br />

〈(∆Vτ ) q 〉�τ ζ(q) , (13.2)<br />

where ζ(q) is the scale invariant moment function, which seems rather universal<br />

for fully developed turbulent flows in the laboratory or the atmosphere,<br />

for moments small than 7. This function is nonlinear and concave; ζ(3) = 1<br />

is a fixed point; ζ(2) = β − 1 relates the second order moment to the<br />

power spectrum scaling exponent; the knowledge of the full (q, ζ(q)) curve for<br />

integer and noninteger moments provides a full characterization of velocity<br />

fluctuations at all scales and all intensities.<br />

13.3 Gusts for Fixed Time Increments<br />

and Their Recurrent Times<br />

<strong>Wind</strong> gusts may be generally defined choosing a time increment τ and a<br />

threshold velocity δ: a gust corresponds to a situation when |V (t1)−V (t2)| >δ<br />

with |t1 − t2| < τ [6]. In practice, for such event to occur, the condition<br />

|V (t1) − V (t2)| > δ should also be realized for some times verifying<br />

|t1 − t2| = τ. We then choose here to fix a small time increment τ and to consider<br />

large fluctuations at this scale. In the following we choose τ = 3 since<br />

3 − s extreme gust correspond to a standard of the American Society of Civil

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