The proposed methodology begins with identifying a region of interest for wind potential assessment. Subsequently, three days from each month are randomly selected, constituting 10% of the month’s duration. This selection is grounded in the statistical premise that this subset adequately represents the entire month.
A high-resolution NWP model is employed to simulate atmospheric conditions for these three chosen days of the month to estimate the wind potential. The simulation results are averaged, comprehensively representing the average wind potential for the specific location during that month. This process is very cost-effective and eliminates the need for extensive and time-consuming simulations.
The effectiveness of this methodology is demonstrated using recent wind measurement data obtained over 10 months from the Greek island of Crete. Our aim is twofold: (i) to introduce the “10% sampling condition” and demonstrate through simulations how it works; and (ii) to present data for topography in Southern Europe, where such a study has not been published before. A comparison between the model-generated and actual wind measurement data is provided. Remarkable agreement between the two data sets is observed, indicating that the proposed methodology accurately captures and represents the wind potential of the selected location.
2.1. Wind Measurements in Crete
The Greek island of Crete, due to its location in the eastern Mediterranean Sea and its convoluted topography, has been the subject of many studies over the past decades regarding its wind potential [
26,
27,
28,
29,
30]. The first vital effort to investigate the wind potential of Crete was presented in [
31].
In particular, the northeastern region of Crete is highly important in wind energy studies since it constitutes one of the highest wind potential areas in the Eastern Mediterranean Sea. This is demonstrated in
Figure 1a, where indicative results for wind velocities are presented from the Global Wind Atlas online framework [
32], where the northeastern region of Crete displays wind velocities over 10 m/s at 100 m above ground level (agl), averaged between the years of 2008 and 2017. Where the Global Wind Atlas (GWA) framework was utilized, all data, information and maps were obtained from the Global Wind Atlas version 3.3, a free, web-based application developed, owned and operated by the Technical University of Denmark (DTU). The Global Wind Atlas version 3.3 is released in partnership with the World Bank Group, utilizing data provided by Vortex, using funding provided by the Energy Sector Management Assistance Program (ESMAP). For additional information see [
33]. The following section will give further details about GWA comparisons with numerical predictions. In that region, at the site of Toplou (35°13′36″ N, 26°13′33″ E) at an altitude of approximately 213 m above sea level (
Figure 1b), a 30 m mast surface wind station was installed [
34] as recently as 2019. It provided continuous measurements between March and December 2019 (
Figure 2). The site was carefully chosen to be representative of the Toplou topography and landscape, characterised by smooth hills on an extended ridge with sharp slopes to the north towards the coastline.
All measurements were made at 20 m, 28.5 m, and 30 m agl, in full compliance with the standards set by the World Meteorological Organization (WMO) for wind energy assessment studies [
36]. The measurements consist of 10 min time averages, each taken from 30 sequential 20 s mean samples. The recorded wind data consists of the mean wind velocity and direction and their standard deviations and minimum and maximum speeds obtained from the thirty 20 s means during ten minutes. Consequently, the maximum velocities quoted here are lower than extreme wind velocities and gusts, often lasting a few seconds. The wind velocity is accurate to two decimal digits when expressed in m/s. At the same time, the wind direction was measured in degrees, clockwise, from 0° (north) to 360° and is accurate to one decimal digit. It is important to note that the minimum wind velocity that can be measured is 0.3 m/s. It must also be noted that the weather station provided full 10 min meteorological data, apart from wind velocities and directions, i.e., temperature, pressure, humidity, and rainfall min, max, average and standard deviation.
2.2. Toplou Wind Statistics
An analysis of the Toplou anemometric data is presented below. Eight 45-degree azimuthal direction sectors were used, the first centred along the geographic north with the rest continuing clockwise, namely north (N), northeast (NE), east (E), southeast (SE), south (S), southwest (SW), west (W), and northwest (NW). Measurements from the reference height of 20 m agl were chosen. The 20 m agl height represents a practical trade-off for representing free-flowing wind conditions by (a) minimising the impact of ground effects and (b) capturing the crucial characteristics of the lower atmosphere. Wherever necessary, some basic theoretical background is provided for better understanding.
Table 1 gives the distribution of measurements, or measurement occurrence, per wind direction sector and month of the year. All values in this table are expressed in percentages. In this way, we know what percentage of the wind blows from which direction during each month. As becomes evident from
Table 1, the two dominant directions are the western and northwestern directions for each examined month.
Figure 3 presents the corresponding wind rose of all observations. We have split the velocities into five fixed bands, namely: (a) from 0 to 4.99 m/s, (b) 5 to 9.99 m/s, (c) 10 to 14.99 m/s, (d) 15 to 19.99 m/s, and (e) velocities greater than 20 m/s. It is important to note that the highest measured velocity during the studied period was 23 m/s. Wind roses are graphical representations of the distribution of wind directions at a specific location over a certain period. They are commonly used in meteorology, climatology, and environmental science to visualise prevailing wind patterns. Wind roses provide valuable insights into the frequency and intensity of winds coming from different directions. For more information on wind roses, please refer to [
37]. The wind rose confirms that the most common direction of wind speed was the northwestern one and, successively, the western one, making up approximately 75% of the wind direction occurrence. Moreover, wind velocities over 10 m/s appeared for more than 40% of the examined 10-month period. A strong northwestern component of velocities over 15 m/s may be observed. It also becomes apparent that, as we moved towards higher velocity bands, the direction seemed more biased towards the northwestern and western components.
Table 2 presents the mean wind velocity per direction sector and month of the year, as well as a weighted average for the mean velocities of each month, based on the frequency of occurrence of
Table 1. A trend became obvious from the presented results (despite missing data from January and February): the wind was lower during the spring and autumn and picked up during the summer and winter. This was expected, since it is established that the atmospheric instability during the winter influences the wind strength [
38]. Moreover, the steadily strong Etesian winds are crucial in maintaining high wind velocities in the Eastern Mediterranean Sea during the summer [
39]. The monthly mean wind velocities ranged from 5.4 to 12.27 m/s, and July, August, and September had mean velocities higher than 10 m/s. The overall mean wind velocity for the Toplou site was 8.6 m/s, which, according to the National Renewable Energy Laboratory (NREL) classification, corresponds to a region of wind power class 7 (outstanding wind resource potential) [
40]. The NREL wind classification system is a method used to categorise wind resources based on their speed and consistency. This system is commonly used in wind energy assessment and site selection for wind farms. It categorises areas into seven classes (1 being the lowest and 7 being the highest) based on the average wind speed and its variation over time.
The cumulative density function (CDF) is widely used in studies of wind potential and is particularly useful in wind energy calculations [
41]. In the present study, the CDF was used to represent the wind velocity variation by calculating the probability of the velocity being equal to or larger than a certain value. For a velocity
V, the CDF is given by the following equation [
42]:
The parameters
c and
k are the two Weibull parameters. Parameter
c is a scale parameter with dimensions of velocity (m/s), whereas parameter
k is dimensionless and relates to the distribution’s shape. Various methods to estimate the Weibull parameters fit the measured frequency of wind velocity occurrence [
41,
43]. In this analysis, the parameters were estimated based on the measured distribution and were found to be
and
m/s.
Figure 4 shows the CDF for the wind velocity data at 20 m agl. The CDF drops slowly with increasing velocity, which was expected due to the high probability of high wind velocities. For instance, velocities higher than 10 m/s occurred approximately 45% of the time.
The wind power density, i.e., wind energy per unit area and time, constitutes an index for assessing wind potential. It is often used in conjunction with the mean annual velocity to define a region’s Wind Energy Class (i.e., on a scale from 1–7, its ability for generating wind energy based on its wind resource potential) [
44]. In this analysis, the mean power density
over a time interval with N measurements was computed from the expression [
45]
where
is the air density, which decreases with altitude,
is the
i-th measured velocity,
is the wind velocity turbulence intensity, and
N is the number of measurements. Using the above expression and taking
to decrease exponentially (which is valid for an isothermal atmosphere [
45]), i.e.,
where
kg/m
3 at sea level,
h is the site altitude in km and
H the lower atmosphere scale height (that is equal approximately to 8 km), we obtain
Table 3 for wind power density. It is important to note that, in this calculation, we have also included the turbulent fluctuation contribution in wind velocity which is represented by the term
;
is the measured standard deviation of the wind velocity [
46]. The contribution of this term, however, was of the order of 2% to 3%, i.e., rather small.
Table 3 presents the mean power density in W/m
2 per direction sector and month of the year for all available data. It is important to note that, in the direction sectors where no wind velocity was observed, the power density is taken as zero. The annual mean was 758 W/m
2 for Toplou at 20 m agl and, according to the International Electrotechnical Commission’s (IEC) classification, corresponds to a region of Wind Energy Class 6 (on a scale from 1–7, excellent wind resource potential) [
44]. This confirms the region around Toplou as a highly promising region regarding wind energy exploitation.
2.3. NWP Model Predictions
This section presents results for the wind field in the region of interest, obtained from high-resolution simulations using the Weather Research and Forecasting (WRF) numerical model. The main objective of this analysis is to examine the validity of the statistical “10% sampling condition”. After randomly choosing [
47] three days of each month for the period March 2019–December 2019 (which represents 10% of the month), we compared wind statistics, that is, the velocity and direction of the wind, with the overall station data (100% of the month). It is important to note that the results for velocities from the WRF were obtained at 10 m agl and had to be extrapolated to 20m agl to match the station data. For this reason, the appropriate equations will be given and discussed.
The WRF model [
48] represents a cutting-edge regional- to global-scale NWP model, extensively utilised for operational forecasting and academic research worldwide. It is configurable in serial, parallel (MPI), and mixed-mode (OpenMP and MPI) forms, tailored for optimal performance on massively parallel computers [
49]. The WRF was chosen as the appropriate model since it has been extensively validated over the years and constitutes one of the most robust and reliable NWP models [
50,
51,
52,
53,
54]. In recent years, attempts to utilise the WRF, coupled with or without CFD models, for the study of wind potential can be found in the literature [
55,
56,
57,
58,
59,
60,
61]. However, none of these works have attempted to go below 500 m spatial resolution and, to the best of our knowledge, no research has attempted to utilise and test the validity of the “10% sampling condition” for the study of wind potential. Both points are considered for the first time in this paper.
In this study, WRF Version 4.1.3 [
48] was utilised. All simulations were conducted carefully, employing state-of-the-art numerical algorithms with strict convergence criteria to solve prognostic and diagnostic equations on a high-resolution grid to ensure error minimisation during the solution process [
62]. These simulations were performed on the TYPHOON High-Performance Computing (HPC) Cluster of the Department of Mathematics and Applied Mathematics of the University of Crete. The system comprises a Fujitsu blade cluster featuring 12 Intel Xeon E5-2430 @ 2.2 GHz CPUs (Intel Corporation, Intel Corporation, Ireland, Ireland). Each blade accommodates a pair of CPUs with 16 GB RAM and a 146 GB SAS hard drive (Seagate, Penang, Malaysia). Optimal results were achieved through a distributed-memory parallelism (dmpar) build, leveraging MPI. Because of the cluster’s modest size, a hybrid build with shared-memory parallelism (smpar, i.e., dmpar+smpar) was employed in all reported runs. Hyper-threading was deactivated, as it contributed only marginally or negligibly to computing performance improvement.
NCEP-FNL 6-hourly data of 0.25° × 0.25° spatial resolution were used to determine the initial and boundary conditions of the model [
63]. These are data from terrestrial meteorological stations, marine observations, satellite data, etc., supplemented by GFS climatic framework data for regions where no observations were readily available. Also, for the most accurate description and analysis of the phenomena in the region of Crete, nested domains were considered, where information exchange occurred between them, to minimise the dependence of the smallest domain (where the results were derived from) on the boundary conditions that were very much apart, both in space and time. Nesting is a standard technique employed to refine the spatial resolution of simulations in specific regions of interest within a larger domain. This technique allows for more detailed modelling of phenomena in areas requiring higher resolution while still utilising coarser resolutions in surrounding regions to conserve computational resources [
64]. The largest domain (domain 1), which included most of Western Europe, had a horizontal grid size of 10.8 km. Domain 2, representing the Balkans, had a horizontal grid size of 3.6 km. Domain 3, which represented Crete, had a horizontal grid size of 1.2 km. Finally, the smallest domain (domain 4), representing Central and Eastern Crete, had a horizontal grid size of 400 m. This is believed to be the smallest size recorded in the literature for this application. To be able to resolve the complex topography of the region, a Digital Elevation Model (DEM) of 60 m spatial resolution [
65] was employed for the two finer grids (domains 3 and 4). The four domains, from coarsest to finest, are presented in
Figure 5.
All modelling domains had 50 layers in the vertical dimension, with the model top being set at 50 hPa. The model was run with a variable time step, which was not allowed to exceed 180 s for the coarsest domain. Appropriate physical parametrisations, based on previous experience [
65], were invoked to represent the correct physics with regards to radiation, convection, microphysical, and planetary boundary layer processes. For more details on the numerical schemes, please see [
48]. Convection schemes were turned off for the two smallest domains since the microphysics resolved convection [
66]. For each simulation, there was an allowance for 12 h of model spin-up time [
67]. The CPU time was a 36 h simulation (one full day plus 12 h of spin-up) on the TYPHOON HPC cluster for the four nested domains in the order of 10 min, indicating the proposed methodology’s computational efficiency.
Wind velocity and direction every 10 min were taken as output from the WRF model. However, the velocity at which the model output was 10 m agl. Since this was the closest to the first observation level, all analyses and comparisons were performed by extrapolating velocity from 10 m to 20 m agl, where wind direction was assumed to be unaltered, as has been found in the literature (see, e.g., [
68]). The velocity was extrapolated to 20 m by using the logarithmic law [
69]
The velocity
is at height
z, given that the velocity
at height
h is known. This law is used in wind energy studies under conditions of neutral atmospheric stability and is valid for wind velocities ranging from 1 m/s up to 30 m/s, a range which does not include extreme phenomena, such as hurricanes, tornadoes, etc. (see, e.g., [
70]). The parameter
in the equation is called roughness length and may be calculated from the raw velocity data using the following equation [
71]:
where
is the turbulence intensity and can be calculated through velocity measurements and their standard deviations (see
Section 2.1). The roughness length is a parameter entering the wind flow equation in the atmospheric boundary layer, where friction forces affect the wind field and its variation with height. The roughness length represents the height above the surface at which the wind speed is zero [
70].
Table 4 presents the roughness length, as was calculated through the use of the entire data set for every month and for each direction sector; the last column presents weighted averages (depending on the frequency of occurrence from
Table 1). A lower roughness length implies less exchange between the surface and the atmosphere and stronger wind near the ground. In the direction sectors where no wind velocities were recorded, the roughness length was taken as 0, indicating that these directions do not contribute to overall wind power production. The respective values for each direction sector were utilised to extrapolate the velocities from 10 m to 20 m.
Table 5 and
Table 6 provide the frequency of occurrence per direction sector and month and the mean wind velocity per month and direction, as calculated from the WRF model. Eight wind direction sectors were selected to compare with the observations. The velocity was extrapolated to 20 m agl, as explained earlier; however, the directions from the WRF were taken from 10 m, as it was assumed that no significant change in wind direction would result between 10 and 20 m above ground in an open area, such as the one in which the meteorological mast was situated [
68]. As evident from
Table 5, the two dominant directions are, again, the western and northwestern ones. However, the results of the WRF model indicate that the western component seemed to be the most dominant of the two. This is confirmed by the corresponding wind (
Figure 6, where the velocities were again split into five fixed bands), with the W and SW components making up approximately 75% of the wind direction occurrence. Once more, wind velocities over 10 m/s are present for more than 40% of the examined 10-month period. It also becomes apparent that, as we move towards higher velocity bands, the direction seems more biased towards the western and northwestern components.
Table 5 indicates a stronger bias towards these components than the measurements.
Table 6 repeats the trend of the measurements, whereby the wind is lower during the spring and autumn and picks up during the summer and winter. The monthly mean wind velocities range from 6.22 to 13.45 m/s, with four months (March, June, August, and September) predicted to have mean velocities higher than 10 m/s. The overall mean wind velocity for the Toplou site was predicted to be 9.83 m/s.
Table 7 presents the predicted wind power density results for the different direction sectors for all months, following the equations given in the previous section. A weighted average, based on the frequency of occurrence given in
Table 5, is also given for every month. It is important to note that the power density is zero in the direction sectors where no wind velocity was detected. The mean wind power density was predicted to be 910 W/m
2, a high value which asserts that the Toplou region is of high anemological interest.
2.4. Error Analysis
The performance of the WRF model is assessed below. The Relative Error (RE) for the annual mean velocities and power densities was calculated as an initial error indicator. The RE was computed using the formula . It was found that mean velocities’ RE was 14%, whereas the mean power densities’ RE was 20%. These values are sufficiently small and indicate a high level of agreement between model predictions and the observed values. It is important to note that the error in the power density was expected to be higher than the error in the velocity since velocity comes into the power density equation raised to the power of 3.
To assess the performance of the WRF in more detail, the various statistical metrics for wind velocity and direction for the actual random days that the model was run were calculated. All actual 10-min interval outputs from the model and observations were utilised for this comparison. Bias and Relative Bias (RB) (for velocities) and Direction Accuracy (DACC) index for wind direction [
72] were calculated. Bias measures the model’s overall overestimation or underestimation of wind velocities. RB measures the overestimation or underestimation relative to the bulk of the observations. The DACC index represents the percentage of times when the circular distance (i.e., the angular difference in wind direction) between modelled and observed wind directions was lower than a threshold, chosen as 30° for this study. The DACC index varies between 0 (very bad correlation) and 100 (excellent correlation). Let
and
denote the
i-th of
N modelled and observed values, respectively, of a quantity. Then, the equations for Bias and RB are
where
.
To compute the DACC index, the circular distance
for any two angles
and
that the wind might be coming from needs to be defined:
. Then, the DACC index is given by
where
is 1 if
or 0 otherwise.
Table 8 presents the Bias, RB and DACC calculated by comparing the three days from each month with the corresponding three days of the station data.
Bias and RB were mostly positive, indicating an overestimation of the wind velocities by the model. Bias was very small for 8 out of 10 months, and RB had a maximum value of 47.98, with all other values being less than 21. This indicated that the absolute RB (a measure of the error) was less than 21%. Moreover, the DACC index was, for 8 out of 10 months, greater than 70, with the highest value being 99.32, which indicates the numerical model’s remarkable ability to represent the wind direction correctly.
The results show that the high-resolution simulations with the WRF numerical model and the “10% sampling condition” accurately depict all main wind characteristics (velocity, direction, and trend) for the examined period. Therefore, the "10% sampling condition" seems valid, at least for the Toplou region.
2.5. Comparisons with the Global Wind Atlas Framework
The GWA framework is an essential online resource. It grants users access to comprehensive wind resource data worldwide, assisting them in evaluating the viability of wind energy generation across diverse regions. The GWA provides detailed maps and data on wind speed and direction at varying altitudes using high-resolution global wind climate data and Geographic Information Systems (GIS) technology. This wealth of information proves invaluable for developers, policymakers, and researchers engaged in the strategic planning and execution of wind energy initiatives. For a full review of the GWA framework, please see [
32].
For the case of Toplou, wind data are available through the GWA between 2008 and 2017. The framework can provide information averaged in space (9 km
2 square box around the location of the mast) and time (10 years) at heights of 10 m, 50 m, 100 m, 150 m, and 200 m agl.
Figure 7 presents the averaged data over 10 years at the height of 10 m agl, with the mean values for wind velocity and power density reported as 7.66 m/s and 548 W/m
2, respectively. The wind rose diagram confirms our research findings: the main wind directions are northwestern and western, with other directions having minimal contribution. Since WRF data for wind velocities were calculated at 10 m agl, we may directly compare the WRF and the GWA. All available WRF velocity data were averaged, and the mean wind velocity was 8.81 m/s. Equation (
2) was utilised to derive the wind power density, and a mean wind power of 648 W/m2 was calculated. The results are summarised in
Table 9, where the REs’ between the mean quantities are also given. As may be seen, both velocity and power density have been overestimated by the WRF by 15% and 18%, respectively. However, these results are considered extremely promising, based on the fact that they have been produced with the “10% sampling condition” and confirm the ability of the proposed methodology to be utilised in calculations of the wind potential of a region. We have identified a problem with the WGA framework: it relies on past data, which is not updated regularly. The proposed methodology does not rely on past data. Still, it may utilise more recent ones (NCEP-FNL data that the WRF model requires to calculate initial and boundary conditions, produced and freely available at the end of each day). Hence, one additional advantage of our method is that it can utilise up-to-date data and perform studies which depict the current situation at a location of interest. Being able to perform such studies is paramount, especially today, as anthropogenic climate change poses significant challenges to the environment; variability in wind patterns may become more pronounced in the short term due to increased weather instability caused by climate change [
73,
74].