Abstract

Abstract. In wind energy, the effect of turbulence upon turbines is typically simulated using wind “input” time series based on turbulence spectra. The velocity components' spectra are characterized by the amplitude of turbulent fluctuations, as well as the length scale corresponding to the dominant eddies. Following the IEC standard, turbine load calculations commonly involve use of the Mann spectral-tensor model to generate time series of the turbulent three-dimensional velocity field. In practice, this spectral-tensor model is employed by adjusting its three parameters: the dominant turbulence length scale LMM (peak length scale of an undistorted isotropic velocity spectrum), the rate of dissipation of turbulent kinetic energy ε, and the turbulent eddy-lifetime (anisotropy) parameter Γ. Deviation from “ideal” neutral sheared turbulence – i.e., for non-zero heat flux and/or heights above the surface layer – is, in effect, captured by setting these parameters according to observations. Previously, site-specific {LMM,ε,Γ} values were obtainable through fits to measured three-dimensional velocity component spectra recorded with sample rates resolving the inertial range of turbulence (≳1 Hz); however, this is not feasible in most industrial wind energy projects, which lack multi-dimensional sonic anemometers and employ loggers that record measurements averaged over intervals of minutes. Here a form is derived for the shear dependence implied by the eddy-lifetime prescription within the Mann spectral-tensor model, which leads to derivation of useful forms of the turbulence length scale. Subsequently it is shown how LMM can be calculated from commonly measured site-specific atmospheric parameters, namely mean wind shear (dU∕dz) and standard deviation of streamwise fluctuations (σu). The derived LMM can be obtained from standard (10 min average) cup anemometer measurements, in contrast with an earlier form based on friction velocity. The new form is tested across several different conditions and sites, and it is found to be more robust and accurate than estimates relying on friction velocity observations. Assumptions behind the derivations are also tested, giving new insight into rapid-distortion theory and eddy-lifetime modeling – and application – within the atmospheric boundary layer. The work herein further shows that distributions of turbulence length scale, obtained using the new form with typical measurements, compare well with distributions P(LMM) obtained by fitting to spectra from research-grade sonic anemometer measurements for the various flow regimes and sites analyzed. The new form is thus motivated by and amenable to site-specific probabilistic loads characterization.

Highlights

  • Of the atmospheric parameters which are generally input into wind turbine load calculation codes, several stand out due to their prominence in load contributions: the “mean” wind speed U, the standard deviation of streamwise turbulent velocity σu, the shear dU/dz or shear exponent α, and the characteristic turbulence length scale L corresponding to the most energetic turbulent motions (e.g., Wyngaard, 2010). Dimitrov et al (2015) explored the importance of shear (α); Dimitrov et al (2017) found that both fatigue and extreme turbine loads can be sensitive to L in addition to the dominant influences of mean wind speed U and streamwise turbulence “strength” σu1

  • Relation of the turbulence length scale to measurable statistics is possible through the eddy-lifetime form of Mann (1994), where the latter is defined in terms of the isotropic von Kármán spectrum that is distorted using rapid-distortion theory (RDT)

  • Using Eq (9) in Eq (7) we get a relation for the isotropic turbulence length scale implied by the lifetime model (3), LMM

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Summary

Introduction

Of the atmospheric parameters which are generally input into (or required by) wind turbine load calculation codes, several stand out due to their prominence in load contributions: the “mean” wind speed U , the standard deviation of streamwise turbulent velocity σu, the shear dU/dz or shear exponent α, and the characteristic turbulence length scale L corresponding to the most energetic turbulent motions (e.g., Wyngaard, 2010). Dimitrov et al (2015) explored the importance of shear (α); Dimitrov et al (2017) found that both fatigue and extreme turbine loads can be sensitive to L in addition to the dominant influences of mean wind speed U and streamwise turbulence “strength” σu. Within the “Mann model”, which uses rapid-distortion theory (RDT) to account for shear-induced distortion of isotropic turbulence (e.g., Savill, 1987; Pope, 2000), there is a prescription for the scale-dependent time over which turbulent eddies of a given size are distorted This timescale is key to proper representation of atmospheric turbulence and reproduction of component spectra via RDT. Constraints implied by fitting the Mann model to measured spectra in nonneutral conditions, given eddy lifetime and mixing-length relations, are tested. This includes dependence of predicted velocity variance on model anisotropy parameter ( ), as well as implications in the surface layer and connection to previous findings in boundary-layer meteorology. The length scale obtained from conventional 10 min wind measurements via the new expression is compared to the length scale found from fits of Mann-model output to measured component spectra; this is done using data from multiple sites, representing several types of site conditions

Theory
Eddy lifetime
Characteristic length scale
Relation to observations
Ideal neutral surface-layer implications
Observations and results
Testing of assumptions and predicted constraints
Discussion
Findings
Conclusions
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