Publishers version - DTU Orbit
Publishers version - DTU Orbit
Publishers version - DTU Orbit
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
Satellites in sun-synchronous polar orbit observe a given local area at a certain local time in<br />
ascending (northbound) track and 12-hour shifted in descending (southbound) track. There<br />
are differences in the local acquisition time of the various satellites carrying radar instruments.<br />
If a local site has pronounced daily wind speed variations, the two fixed observational times<br />
may not be fully representative of the diurnal cycle. Far offshore diurnal variation is typically<br />
less pronounced than in some coastal areas, e.g. sites with pronounced land-sea breezes.<br />
Using observations from several satellites with different fixed observational times would be a<br />
possibility, but this has not yet been achieved.<br />
Another challenge of using SAR for wind resource assessment is the relatively few observations<br />
available. For some sites less than 200 scenes may be available. In European coastal<br />
waters Envisat provides a somewhat higher number of observation. In the later years of operation<br />
many wide swath mode scenes were recorded. This makes it a unique archive for wind<br />
resource assessment. The available scenes can be seen at http://earth.esa.int/EOLi.<br />
Barthelmie & Pryor (2003) and Pryor et al. (2004) investigated based on statistical analysis<br />
and using offshore meteorological observations from the Baltic Sea and North Sea, the<br />
number of randomly sampled wind observations necessary to carry out wind resource analysis<br />
within certain statistical bounds. The conclusion was that around 70 samples are sufficient<br />
to estimate mean wind speed and the Weibull scale parameter but around 2,000 samples are<br />
needed to estimate energy density and the Weibull shape parameter at the 10% confidence<br />
level (significance 95%). The result makes it clear that the accuracy of SAR-based wind resource<br />
statistics is adequate for pre-feasibility studies. In other words, the SAR-based wind<br />
resource map may be used as guide to site an offshore meteorological mast in a wind farm<br />
project. Alternatively, if high-quality offshore observations exist, the local wind gradients at<br />
10 m above sea level may be evaluated from SAR wind resource maps. Also, combining or<br />
blending SAR wind resource statistics and mesoscale wind resource modelling is an option<br />
(Badger et al., 2010b).<br />
When planning clusters of wind farms that cover 100 km 2 or more, it is advisable to have<br />
two meteorological masts if the wind resource should be assessed as accurately as possible. It<br />
is most likely that significant wind gradients exist within such areas, in particular in coastal<br />
zones (Barthelmie et al., 2007). At Horns Rev the first wind farm is located 14 to 21 km<br />
offshore from the closest coastal point and the second wind farm is located 26 to 31 km<br />
offshore. Using SAR, winds at 1 − 2 km grid scale allow quantification of the local wind<br />
gradients. A third wind farm at Horns Rev in the North Sea is in planning.<br />
15.10 S-WAsP<br />
In-house software was developed for SAR wind resource wind mapping at <strong>DTU</strong> Wind Energy.<br />
The Satellite-WAsP (S-WAsP) software reads SAR wind fields from ANSWRS and SARTool<br />
(SOPRANO). In earlier <strong>version</strong>s of S-WAsP other formats were used as input (Nielsen et al.,<br />
2004; Hasager et al., 2008). The first step is to ensure geographical collocation of the series<br />
of wind fields (through a database) and select the desired data. The second step is to run<br />
the wind resource application routines to calculate the wind resource statistics: mean wind<br />
speed, Weibull scale, Weibull shape, and energy density and the statistical uncertainty for<br />
each parameter. The final results are output maps of the parameters (Hasager et al., 2012).<br />
The number of satellite observations in a single directional bin may be small. Therefore to<br />
make it possible to fit a distribution, all data is used to derive the shape parameter. The shape<br />
parameter is assumed valid for every bin. The Weibull scale parameter is then estimated by<br />
the average wind speed in each sector. The frequency ofoccurrence in each sectoris uncertain<br />
when observations are sparse and there is a risk of observing sectors without any observation<br />
and no estimate of the mean wind. An alternative to simple bin counting is to sort all<br />
observations after directions, estimate the probability density between the observations by<br />
the angle separating between them, and finally resample the densities in the standard sectors<br />
(Nielsen et al., 2004).<br />
The available wind powerdensity, E W/m 2 that is proportional to the wind speed cubed,<br />
<strong>DTU</strong> Wind Energy-E-Report-0029(EN) 287