FINO1 Mast Correction A. Westerhellweg, T. Neumann; DEWI GmbH, Wilhelmshaven V. Riedel; DEWI North America Inc. A. Westerhellweg English Abstract Lateral speed-up effects, upwind flow retardation and downwind wake effects can be much more pronounced for offshore wind measurement masts than for onshore masts. Combined wind and wave loads require different mast designs, which may result in denser lattices, larger footprints and shorter booms as compared to onshore masts. In order to use such offshore wind measurement data for ener gy yield assessments, the disturbances caused by the mea surement mast need to be properly addressed. For this, DEWI has developed a mast correction method based on the vanishing vertical wind gradients during very unstable situations, thus enabling a “uniform ambient flow mast correction” (UAM). This mast correction scheme was devised by DEWI in 2007 for the FINO1 offshore wind mea surement platform [4]. In 2011, it has been re-assessed for a higher directional resolution (1° instead 10°) and has been extended to all cup and sonic anemometer measurement heights. The mast correction refers to the wind direction measured at FINO1 at 91.5 m LAT and the averaging interval of 10 minutes. During 2009 and 2010, a 1-year Lidar measurement campaign was performed on the FINO1 platform. The comparison with a mast correction based on 60 DEWI MAGAZIN NO. 40, FEBRUARY 2012 Lidar data showed high agreement and validated the performance of the UAM method [7]. The UAM method can be used for offshore masts if an undisturbed top anemometer is installed. The method, the correction results and the associated uncertainties for FINO1 are detailed below. Measurement Set-up The FINO1 mast [2] has a square cross-section. Cup anemometers are installed on booms on the south-east side of the mast (the main wind direction is south-west). Sonic anemometers and wind vanes are installed on the opposite north-west side of the mast. The mast is equipped with a top anemometer at the height of 103 m above LAT (lowest astronomical tide) located in a lightning protection cage. Temporarily, an additionally top anemometer was installed for correction purposes at a height level of 104.5 m LAT. An offshore wind measurement mast has to be designed to resist wind and wave loads which might not allow a measurement set-up according to IEC61400-12-1 standards [3]. In the case of FINO1, the lattice mast has a square footprint with a width that decreases linearly from 3.5 m (at 34 m LAT) to 1.4 m (at 91.5 m LAT). The boom lengths vary from 6.5 m to 3.0 m. The ratio of the boom Anemometer, height LAT Tab. 1: Measurement set-up details of the boom mounted anemometers at FINO1. Fig. 1: Offshore platform FINO1. Boom length Orientation Ratio (distance to mast centre)/ (mast width) [m] [m] [m] [°] [-] cup 91.5 1.375 3.0 135 2.7 cup 81.5 1.754 3.0 139 2.2 cup 71.5 2.124 4.0 143 2.4 cup 61.5 2.504 5.5 142 2.7 cup 51.5 2.875 5.5 140 2.4 cup 41.5 3.254 6.5 142 2.5 cup 34 3.532 6.5 143 2.3 sonic 81.5 1.754 3.0 311 2.2 sonic 61.5 2.504 5.5 308 2.7 sonic 41.5 3.254 6.5 308 2.5 Fig. 2: Left: Top anemometer at 103 m LAT in lightning cage and additional anemometer at 104.5 m LAT. Right: Ratio of the wind speeds of the additional and the top anemometer lengths to the mast width varies from 2.2 to 2.7 (Tab. 1) and is much smaller than recommended in the IEC. Furthermore, the length of the mounting tube of the topanemometer does not conform to the IEC standards. In the immediate mast wake, the wind speed reduction is very large and amounts to up to 40%. A mast correction of the data is necessary. Correction of Top Anemometer Data A short-term measurement campaign with an additional anemometer, installed at 1.5 m height above the original top anemometer, was initiated. The purpose of this additional measurement was to gather wind data that would allow a correction of the flow disturbances at the original top anemometer. These disturbances are caused by the lightning protection cage and possibly by systematic speedup effects at the mast top. While the original top anemometer is mounted at a height of 103 m above LAT, the additional top-mounted anemometer reaches a height of 104.5 m above LAT. The vertical carbon fibre boom is sufficiently stiff. The anemometer is calibrated according to MEASNET standard. A sector-wise correlation has been established between the original top anemometer and the additional top-mounted anemometer. Data sets with a Mast width wind speed > 4 m/s have been evaluated. After the determination of the correction factors with 1 degree resolution (moving average over 2 degrees in wind direction), these factors have been applied to the data of the original top anemometer in order to transfer the data towards the additional top mounted anemometer. The directional plot of the ratios of the measured wind speeds (Fig. 2) shows the flow distortion of the booms of the lightning protection cage at the wind directions 0°, 90°, 180° and 270°. In the wind direction sectors between the tubes of the lightning cage, systematic speed-up effects are present for the original top anemometer. The ratio of the two wind speed signals is not the same for all directions but is, on average, 0.98 for the north and 0.99 for the south wind directions. The difference between the north and south directions is caused by the position of the additional top anemometer on the north edge of the mast. To avoid this effect the additional anemometer has to be placed higher, which would have had other drawbacks. A first measurement campaign was performed during an 8-month period during 2005-11-15 - 2006-07-12. In 2008, the measurement has been re-installed with another anemometer but the identical measurement set-up. In the one-year period 2008-12-28 – 2009-12-29 the previous correction functions were confirmed. With the application DEWI MAGAZIN NO. 40, FEBRUARY 2012 61 120 Height LAT [m] 100 80 60 40 20 reduced data set (unstable stratification, wind direction sector [220°;230°]) wind profile between 91.5m and 41.5m 0 95% corrected wind profile 96% 97% 98% 99% 100% 101% 102% 103% Percentage deviation from wind speed measured at 104.5 m height LAT [-] Fig. 3: Wind profiles examined in direction sector [220°;230°] for unstable stratification. of the correction function, the reference height of these data changes from 103 m to a height level of 104.5 m LAT. Fig. 4: Wind profile for unstable stratification, the wind speed range above 4 m/s and the wind direction range [220°;230°], relative to the mean wind speed measured at 104.5m LAT. March 2004 until February 2006 (2 years) and February 2010 until January 2011 (12 months) have been evaluated. Uniform Ambient Flow Mast Correction Scheme The basic concept of the UAM method is to use a data set with no vertical wind gradient (uniform ambient wind flow), which allows to derive mast correction functions by sector-wise comparison of the boom and top mounted anemometers. In order to create a situation similar to putting the entire mast into a very large wind tunnel, weather situations are isolated during which the vertical wind speed gradient approaches zero. The remaining wind shear is corrected and the resulting wind speed ratios vtop/vboom constitute the mast correction functions. The correction method is explained below using the example of FINO1. The method consists of: a) Reduction of the measured wind data to periods where there is a strongly unstable stratification observed at the platform, determined by temperature measurements of the sea surface and of the air close above the sea. b) Correction of remaining wind shear. c) Calculation of the ratios vtop/vboom as the mast correction functions, separately for each height level. a) Reduction to periods with unstable stratification The wind data from the FINO1 platform have been reduced to periods where there was a strongly unstable stratification observed at the platform, i.e. whenever the air temperature at 30 m height is by more than 1 degree lower than the water temperature at -3 m depth. Although this is a very simple and pragmatic method of describing the stratification, it was shown to be sufficiently precise for the present purpose. The required temperature measurements are not available for the whole measurement period. Only the periods 62 DEWI MAGAZIN NO. 40, FEBRUARY 2012 b) Correction of remaining wind shear Even in unstable conditions, the wind shear is not zero (Fig. 3). The wind shear for unstable stratification is therefore approximated and considered in the mast correction functions. At FINO1, all boom-mounted cup anemometers are approximately oriented towards the same direction. The resulting data set of step (a) is reduced to the wind speed range above 4 m/s and the wind direction range [220,230] degree, which is perpendicular to the boom orientation of the cup anemometers. For this wind direction sector the smallest disturbance caused by the mast is expected theoretically. Fig. 3 shows the vertical wind profiles of the data sets examined in the evaluation period March 2004 – February 2006. For this reduced data set, a mean wind profile has been determined (see Fig. 4, red line). Presumably, there is a small lateral speed-up effect present at the mast for this wind direction range, which leads to too high wind speeds measured with the boom mounted anemometers. The observed wind shear, calculated using the boom mounted cup anemometer measurements within the wind direction sector [220°,230°] (Fig. 4, blue line) has been assumed to be representative up to the height of the top anemometer. It is therefore used to calculate the corrected mean wind speed for the lower height levels based on the undisturbed measurement in 104.5 m height. The resulting profile (see Fig. 4, yellow line), is called the corrected profile and is assumed to prevail at the FINO1 platform during unstable conditions. Fig. 5: The ratio vtop/vboom of the resulting data set serves as mast correction for each boom mounted anemometer c) The Ratio vtop/vboom represents the mast correction for each height. The unstable data set is evaluated for the mast correction. For the different heights, vboom is corrected according to the wind shear shown in Fig. 4 and the ratio vtop/vboom serves as mast correction for each boom mounted anemometer. The correction function is based on two different functional approximations; the data have been divided into two parts (mast wake and remaining data). As an example, Fig. 5 shows all data and the data used for the mast correction for 91.5 m LAT. In the four directions corresponding to the sections of the lightning protection cage, the variation was higher. These wind direction sectors have been cut out and excluded from the assessment of the mast correction. Finally, mast correction functions have been assessed for all boom mounted cup and sonic anemometers (Fig. 6). Validation with LIDAR Mast Correction A Leosphere Windcube Lidar device was installed on the FINO1 platform at about 10 m distance to the mast. One year worth of data have been evaluated for a mast correction (2009-08-01 – 2010-07-31). A mast correction function for the cup measurements at 71.5 m, 81.5 m and 91.5 m LAT has been assessed from the Lidar measurements and compared to the UAM results. For almost all wind directions, Lidar measurements are not influenced by mast effects and can be considered as undisturbed wind data. The Lidar data (ratio vlidar/vcup) have been used to assess a mast correction function. The whole correction function has been assessed based on two separate functional approximations; the data have been divided into two parts (mast wake and remaining data). In Fig. 7, the Lidar mast correction is compared to the UAM results for the cup anemometer data at 91.5 m and 71.5 m. The correction functions show excellent agreement, espe- cially for the lateral acceleration seen for the main wind direction sector SW, 210°-270°. Within the mast wake, around 315°, the UAM method leads to smaller corrections than the Lidar correction. Based on the Lidar measurements, it has been shown that the mast correction function does not significantly depend on wind speed, stability or turbulence intensity [7]. Estimation of the Mast Correction Uncertainty The uncertainty associated with the application of the UAM method varies with wind direction; this uncertainty is high for wind directions where anemometers are situated in or at the boundary of the mast wake. From the input data and the correction procedure, different uncertainty sources can be identified. The main uncertainty sources are uncertainties relating to: • wind direction (denoted in the following as u1) • the correction of the top anemometer (u2) • the identification of unstable atmospheric situations and the correction of the remaining wind shear (u3) • stability effects and wind speed dependencies which have not been considered in the calculation of the correction functions (u4) In the following the uncertainties of the mast correction are estimated. The uncertainties are described as standard uncertainty. Uncertainty in wind direction (u1) The mast correction functions for all measurement heights have been defined in terms of the wind direction measured at 91.5 m LAT. The wind direction at this height can differ from the wind directions at other height levels, mainly due to two reasons: Turbulent fluctuations of the wind direction, measured by its standard deviation, and systematic wind direction changes with height associated with the Ekman spiral, most pronounced during stable atmospheric DEWI MAGAZIN NO. 40, FEBRUARY 2012 63 1,8 UAM mast correction cup 41.5m LAT 1,7 ma ast correction [-] UAM mast correction cup 71.5m LAT 1,4 UAM mast correction cup 81.5m LAT 1,3 UAM mast correction cup 91.5m LAT 1,2 UAM mastt correction ti cup 34 34m LAT 1,1 1,3 1,2 1,1 0,9 0,9 Fig. 6: 30 60 90 120 150 180 210 wind direction [°] 240 270 300 330 360 0,8 60 1,8 FINO1 91.5m LAT 90 120 150 180 210 240 270 300 330 360 240 270 300 330 360 FINO1 71.5m LAT 1,7 1,6 1,6 UAM mast correction 1,5 ma ast correc ction [-] ma ast correction [-] 30 wind direction [°] 1,7 LIDAR mast correction 1,4 1,3 1,2 1,1 1,3 1,2 1,1 0,9 0,9 Fig. 7: 30 60 90 120 150 180 210 wind direction [°] 240 270 300 330 360 LIDAR mast correction 1,4 10 1,0 0 UAM mast correction 1,5 15 1,0 0,8 0 30 60 90 120 150 180 210 wind direction [°] Lidar mast correction and UAM mast correction for the heights of 91.5m and 71.5m LAT at FINO1. stratification. These uncertainties associated with the wind direction have been estimated to be in the range of udir=2°-6°. The uncertainty of the mast correction function with respect to the wind direction can be expressed as ο݉ܽݎݎܿݐݏ ߲݉ܽݎݎܿݐݏ ݑଵ ሺ݀݅ݎሻ ൌ ฬ ݑௗ ฬ ൎ ฬ ݑௗ ฬ ο݀݅ݎ ߲݀݅ݎ and are depicted in Fig. 8. Uncertainties concerning the top anemometer (u2) The met mast correction functions are based on simultaneous wind speed measurements with the boom and top mounted anemometers. The UAM method therefore relies on a high quality top anemometer installation. At FINO 1, the top anemometer wind data have been corrected for effects due to the lightning protection cage and systematic speed-up effects. The uncertainty of the mast correction 64 0 UAM mast correction for all boom mounted cup anemometers (left) and sonic anemometers (right) at FINO1. 1,8 0,8 UAM mast correction sonic 81.5m LAT 1,4 1,0 0 UAM mast correction sonic 61.5m LAT 1,5 1,0 0,8 UAM mast correction sonic 41.5m LAT 1,6 UAM mast correction cup 61.5m LAT 1,5 FINO1 sonic anemometer 1,7 UAM mast correction cup 51.5m LAT 1,6 ma ast correction [-] 1,8 FINO1 cup anemometer DEWI MAGAZIN NO. 40, FEBRUARY 2012 function due to this top anemometer correction has been estimated to be ± 0.0125. Uncertainties regarding wind shear (u3) The UAM method is based on vanishing vertical wind speed gradients during unstable atmospheric conditions. Small remaining wind shear is corrected. The uncertainty of this correction has been estimated from profile measurements with Lidar shown in [7]. The average wind speed increase under unstable conditions shown in [7] varies from 0.03% to 0.06% per m height difference with mean value 0.05% and standard deviation of 0.02%. The standard deviation of 0.02% per m height difference has been used to estimate the uncertainty of the mast correction function with respect to wind shear for each measurement height as shown in Tab. 2. 0,35 Uncertainty of mast correction in respect to wind direction Uncerttainty in re espect to w wind direction [-] 0,30 0,25 0 25 0,20 cup104.5 cup91.5 cup81.5 cup71.5 cup61.5 cup51.5 cup41.5 cup31.5 sonic81 5 sonic81.5 sonic61 5 sonic61.5 sonic41.5 0,15 0,10 0,05 0,00 0 30 60 90 120 150 180 210 wind direction [°] 240 270 300 330 360 Fig. 8: Uncertainty of mast correction in respect to wind direction. Height above LAT [m] Height difference to 104.5m Uncertainty of mast correction in respect to wind shear (0.02% per m height difference) 104.5 91.5 81.5 71.5 61.5 51.5 41.5 34 0 13 23 33 43 53 63 70.5 0.000 0.002 0.004 0.006 0.008 0.010 0.012 0.013 Tab. 2: Uncertainty of mast correction in respect to wind shear. 1,7 Mast correction 91.5m +/- uncertainty 1,6 Uncertainty of mast correction 91.5 m Mast correction c [-] Unccertainty of m mast correction n [-] 0,16 0,12 0,08 mast corr 15 1,5 mast corr + uncertainty mast corr - uncertainty 1,4 1,3 1,2 1,1 1 0,04 0,9 0,8 0,00 0 Fig. 9: 90 180 i d direction di ti [°] wind 270 360 90 180 wind direction [°] 270 360 Left: Uncertainty of the mast correction at FINO1, 91.5m LAT. Right: Mast correction at FINO1 91.5m LAT with domain of uncertainty. Uncertainties due to stability effects and wind speed dependencies (u4) The correction functions are assumed independent of wind speed, atmospheric stability and turbulence intensity. An additional uncertainty of 5% (in the mast wake) and 0.5% for all other directions has been associated with the use of this assumption, because it was shown in [7] that these parameters have only minor influence on the mast correction functions. Overall uncertainties of the mast correction The uncertainty of the mast correction is then combined from different uncertainty sources: ݑሺ݀݅ݎሻ ൌ ඥݑଵ ሺ݀݅ݎሻଶ ݑଶ ሺ݀݅ݎሻଶ ݑଷ ሺ݀݅ݎሻଶ ݑସ ሺ݀݅ݎሻଶ 0 The resulting uncertainties, depending on the wind direction, are shown in Fig. 9 as an example for the cup mea surement at 91.5 m LAT. Fig. 10 shows the uncertainty of the corrected wind speeds in respect to the mast correction as percentage for all cup and sonic measurements. The overall uncertainty is calculated as weighted mean over all wind direction bins with the long-term wind direction distribution at FINO1 from 2004-2009 and is given in Tab. 3, separately for each height level. Optionally the data can be filtered for a data set that omits the wind directions in the mast wake. If data are not filtered for a certain wind direction sector but the whole data set is used, the values of Tab. 3 apply for the uncertainty assessment. To calculate the overall uncertainty of the wind speed measurement after application of the mast correction, ad- DEWI MAGAZIN NO. 40, FEBRUARY 2012 65 30% 30% Uncertainty of corrected wind speeds in respect to the mast correction FINO1 cup p anemometers Uncertainty of corrected wind speeds in respect to the mast correction FINO1 - sonic anemometers 25% 20% cup31.5 cup41.5 cup51.5 cup51 5 cup61.5 cup61 5 cup71.5 cup81.5 cup91.5 cup104.5 Uncertain nty of mast correctio on [%] Uncertain nty of mast correctio on [%] 25% 15% 10% sonic41.5 sonic61.5 sonic81.5 20% 15% 10% 5% 5% 0% 0% 0 30 60 90 120 150 180 210 Wind Direction [°] 240 270 300 330 360 0 30 60 90 120 150 180 210 Wind Direction [°] 240 270 300 330 360 Fig. 10: Uncertainty of mast corrected wind speeds in respect to the mast correction for the FINO1 cup and sonic wind speed measurements as percentage. Anemometer Resulting overall uncertainty of mast correction cup104.5 cup91.5 cup81.5 cup71.5 cup61.5 cup51.5 cup41.5 cup31.5 sonic81.5 sonic61.5 sonic41.5 2% 2% 2% 3% 3% 3% 4% 4% 2% 2% 3% Tab. 3: Overall uncertainty of mast corrected wind speeds in respect to mast correction for the FINO1 cup and sonic wind speed measurements. ditional sources of uncertainty like calibration uncertainty and operational characteristics of the anemometers have to be taken into account (like described in IEC 61400-12-1 [9]). According to ISO-IEC GUM [10], the uncertainty of the mounting effects can be replaced by the uncertainty of the mast correction. References: [1] RAVE: Research at Alpha Ventus, www.rave-offshore.de. [2] FINO: Forschungsplattformen in Nord- und Ostsee, www.fino-offshore.de. [3] International Electrotechnical Commission (IEC): IEC61400-12-1 Wind turbines - Part 12-1: Power performance measurements of electricity producing wind turbines, 1st ed., 12/2005. [4] T. Neumann: FINO1 and the mast shadow effect, 52nd IEA Topical Expert meeting: Wind and Wave Measurements at Offshore Locations, Berlin, Germany, February 2007. 66 DEWI MAGAZIN NO. 40, FEBRUARY 2012 [5] A. Beeken, T. Neumann, A. Westerhellweg: Five years of operation of the first offshore wind research platform in the German Bight – FINO 1, DEWEK 2008, Bremen. [6] A. Westerhellweg, B. Canadillas, A. Beeken, T. Neumann: One Year of Lidar Measurements at FINO1-Platform: Comparison and Verification to Met-Mast Data. DEWEK 2010, Bremen. [7] A. Westerhellweg, V. Riedel, T. Neumann: Comparison of Lidar- and UAM-based offshore mast effect corrections, EWEA 2011, Brussels. [8] F. Kinder, A. Westerhellweg, T. Neumann: Meteorological measurements at FINO1 during the existence of the wind farm Alpha Ventus, EOW 2011, Amsterdam. [9] International Electrotechnical Commission (IEC): IEC61400-12-1 Wind turbines - Part 12-1: Power performance measurements of electricity producing wind turbines, 1st ed., 12/2005. [10]ISO-IEC Guide 98-3: Uncertainty of measurement-Part3: Guide to the expression of uncertainty in measurement (GUM: 1995), Switzerland, 2008.
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