Michael Graham - Wind Energy Handbook

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Wind Energy Handbook: краткое содержание, описание и аннотация

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Discover this fully updated and authoritative reference to wind energy technology written by leading academic and industry professionals  The newly revised Third Edition of the 
 delivers a fully updated treatment of key developments in wind technology since the publication of the book’s Second Edition in 2011. The criticality of wakes within wind farms is addressed by the addition of an entirely new chapter on wake effects, including ‘engineering’ wake models and wake control. Offshore, attention is focused for the first time on the design of floating support structures, and the new ‘PISA’ method for monopile geotechnical design is introduced. 
The coverage of blade design has been completely rewritten, with an expanded description of laminate fatigue properties and new sections on manufacturing methods, blade testing, leading-edge erosion and bend-twist coupling. These are complemented by new sections on blade add-ons and noise in the aerodynamics chapters, which now also include a description of the Leishman-Beddoes dynamic stall model and an extended introduction to Computational Fluid Dynamics analysis. 
The importance of the environmental impact of wind farms both on- and offshore is recognised by extended coverage, which encompasses the requirements of the Grid Codes to ensure wind energy plays its full role in the power system. The conceptual design chapter has been extended to include a number of novel concepts, including low induction rotors, multiple rotor structures, superconducting generators and magnetic gearboxes.
References and further reading resources are included throughout the book and have been updated to cover the latest literature. Importantly, the core subjects constituting the essential background to wind turbine and wind farm design are covered, as in previous editions. These include: 
The nature of the wind resource, including geographical variation, synoptic and diurnal variations and turbulence characteristics The aerodynamics of horizontal axis wind turbines, including the actuator disc concept, rotor disc theory, the vortex cylinder model of the actuator disc and the Blade-Element/Momentum theory Design loads for horizontal axis wind turbines, including the prescriptions of international standards Alternative machine architectures The design of key components Wind turbine controller design for fixed and variable speed machines The integration of wind farms into the electrical power system Wind farm design, siting constraints and the assessment of environmental impact Perfect for engineers and scientists learning about wind turbine technology, the 
 will also earn a place in the libraries of graduate students taking courses on wind turbines and wind energy, as well as industry professionals whose work requires a deep understanding of wind energy technology.

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2.7 Gust wind speeds

It is often useful to know the maximum gust speed that can be expected to occur in any given time interval. This is usually represented by a gust factor G , which is the ratio of the gust wind speed to the hourly mean wind speed. G is obviously a function of the turbulence intensity, and it also clearly depends on the duration of the gust – thus the gust factor for a one‐second gust will be larger than for a three‐second gust, because every three‐second gust has within it a higher one‐second gust.

Figure 28 Gust factors calculated from Eq 246 While it is possible to - фото 97

Figure 2.8 Gust factors calculated from Eq. (2.46)

While it is possible to derive expressions for gust factors starting from the turbulence spectrum (Greenway 1979; ESDU 1983), an empirical expression due to Weiringa (1973) is often used because it is much simpler and agrees well with theoretical results. Accordingly, the t ‐second gust factor is given by

(2.46) where I uis the longitudinal turbulence intensity Figure 28shows the gust - фото 98

where I uis the longitudinal turbulence intensity. Figure 2.8shows the gust factors for several different turbulence intensities and gust durations calculated according to this expression.

2.8 Extreme wind speeds

In addition to the foregoing descriptions of the average statistical properties of the wind, it is clearly of interest to be able to estimate the long‐term extreme wind speeds that might occur at a particular site.

A probability distribution of hourly mean wind speeds such as the Weibull distribution will yield estimates of the probability of exceedance of any particular level of hourly mean wind speed. However, when used to estimate the probability of extreme winds, an accurate knowledge of the high wind speed tail of the distribution is required, and this will not be very reliable because almost all of the data that was used to fit the parameters of the distribution will have been recorded at lower wind speeds. Extrapolating the distribution to higher wind speeds cannot be relied upon to give an accurate result.

Fisher and Tippett (1928) and Gumbel (1958) have developed a theory of extreme values that is useful in this context. If a measured variable (such as hourly mean wind speed картинка 99) conforms to a particular cumulative probability distribution F ( картинка 100), that is, F ( картинка 101) → 1 as картинка 102increases, then the peak values of hourly mean wind speed in a given period (a year, for example) will have a cumulative probability distribution of F N, where N is the number of independent peaks in the period. In the UK, for example, according to Cook (1982), there are about 100 independent wind speed peaks per year, corresponding to the passage of individual weather systems. Thus, if as for a Weibull distribution the wind speed peaks in 1 year will have a - фото 103as for a Weibull distribution, the wind speed peaks in 1 year will have a cumulative probability distribution given approximately by However as indicated previously this is unlikely to give accurate estimates - фото 104. However, as indicated previously, this is unlikely to give accurate estimates for extreme hourly means, because the high‐wind tail of the distribution cannot be considered to be reliably known. However, Fisher and Tippett (1928) demonstrated that for any cumulative probability distribution function that converges towards unity at least exponentially (as is usually the case for wind speed distributions, including the Weibull distribution), the cumulative probability distribution function for extreme values will always tend towards an asymptotic limit 247 as the observation period - фото 105will always tend towards an asymptotic limit

(2.47) as the observation period increases U is the most likely extreme value or - фото 106

as the observation period increases. U ′is the most likely extreme value, or the mode of the distribution, while 1/ a represents the width or spread of the distribution and is termed the dispersion .

This makes it possible to estimate the distribution of extreme values based on a fairly limited set of measured peak values, for example, a set of measurements of the highest hourly mean wind speeds картинка 107recorded during each of N storms. The N measured extremes are ranked in ascending order, and an estimate of the cumulative probability distribution function is obtained as

(2.48) Wind Energy Handbook - изображение 108

where m( картинка 109) is the rank, or position in the sequence (starting with the lowest), of the observation Then a plot of against is used to estimate the mode U and disper - фото 110. Then a plot of against is used to estimate the mode U and dispersion 1 a by fitting a - фото 111against картинка 112is used to estimate the mode U ′and dispersion 1/ a by fitting a straight line to the data points. This is the method due to Gumbel.

An illustration of the Gumbel method is provided in Figure 2.9, using some sample extreme wind data for a particular 29‐year period. The upper plot shows the sample of extreme values. The middle plot shows the estimated cumulative distribution obtained by ordering these values, with the dashed line showing the fitted distribution obtained using the Gumbel method. The lower plot shows how that fit is obtained, giving a mode U ′= 27.8 m/s with a dispersion of 2.52 m/s from the inverse slope.

Lieblein (1974) has developed a numerical technique that gives a less biased estimate of U ′and 1/ a than a simple least squares fit to a Gumbel plot.

Having made an estimate of the cumulative probability distribution of extremes F ( картинка 113), the M ‐year extreme hourly mean wind speed can be estimated as the value of картинка 114corresponding to the probability of exceedance F = 1 − 1/ M .

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