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.