532 Wind Power Generation and Wind Turbine Design
In an investigation on the buffeting of long-span bridges, Minh et al. [ 17 ] used
the digital fi ltering ARMA method to numerically generate time-histories of wind
turbulence.
In simulating drag force time-histories on the tower, information on spatial cor-
relation, or coherence is necessary to be included. Coherence relates the similarity
of signals measured over a spatial distance within a random fi eld. Coherence is of
great importance, especially if gust eddies are smaller than the height of a struc-
ture. Some of the earliest investigations into the spatial correlation of wind forces
were carried out by Panofsky and Singer [ 18 ] and Davenport [ 19 ] and later aug-
mented by Vickery [ 20 ] and Brook [ 21 ]. Recent publications involving lateral
coherence in wind engineering include Højstrup [ 22 ], Sørensen et al. [ 23 ] and
Minh et al. [ 17 ].
2.4 Rotationally sampled spectra
In order to simulate the drag force time-histories on the rotating blades, a special
type of wind velocity spectrum is needed. Connell [ 24 ] reported that a rotating
blade is subjected to an atypical fl uctuating wind velocity spectrum, known as
a rotationally sampled spectrum. Due to the rotation of the blades, the spectral
energy distribution is altered, with variance shifting from the lower frequencies
to peaks located at integer multiples of the rotational frequency. Kristensen and
Frandsen [ 25 ], following on from work by Rosenbrock [ 26 ], developed a simple
model to predict the power spectrum associated with a rotating blade, and this was
signifi cantly different to a spectrum without the rotation considered. Though liter-
ature on this topic is limited, Madsen and Frandsen [ 27 ], Verholek [ 28 ], Hardesty
et al. [ 29 ] and Sørensen et al. [ 23 ] are some relevant references on this topic.
Rotationally sampled spectra are used to quantify the energy as a function of
frequency for rotor blades within a turbulent wind fl ow for representing the redis-
tribution of spectral energy due to rotation. The required redistribution of spectral
energy can be achieved by identifying the specifi c frequencies 1 Ω , 2Ω , 3 Ω , and
4 Ω ( Ω being the rotational frequency of the blades), and then deriving the Fourier
coeffi cients for those frequencies according to specifi c standard deviation values.
These values can be obtained based on some measurements or assumption
related to the rotational turbulence spectra. Madsen and Frandsen [ 27 ] observed
that the peaks of redistributed spectral energy in a rotationally sampled spec-
trum tend to become more pronounced as distance increases along the blade,
away from the hub.
The typical rotationally sampled turbulence spectra are shown in Fig. 2 [ 30 ]. It
has been assumed for the spectra that the variance values increase by an arbitrary
value of 10%, for each successive blade node radiating out from the hub. It is also
assumed that 30% of the total variance at each node is localized into peaks at 1 Ω ,
2 Ω , 3Ω , and 4Ω (15%, 7.5%, 4.5% and 3% of the total energy is allocated to the
different peaks). Nodal fl uctuating velocity time-histories with specifi c energy–
frequency relationships can be simulated from the spectra in Fig. 2 using a discrete
Fourier transform (DFT) technique.