Wind Speed At Height Log Power Law Calculator
Our meteorology & atmospheric science calculator computes wind speed at height log power law accurately. Get results you can export or share.
Reviewed for accuracy by Daniel Agrici, Founder & Lead Developer
Wind Speed At Height Log Power Law Calculator
Calculator
Adjust values & calculateEnter your values below. Every result is computed in your browser โ no data is sent to any server.
Formula: Log: V(z) = Vref*ln(z/z0)/ln(Zref/z0); Power: V(z) = Vref*(z/Zref)^alpha
Worked example โ Log: 13.58 m/s | Power: 13.49 m/s | Density: 1534 W/m2
Formula
Log: V(z) = Vref*ln(z/z0)/ln(Zref/z0); Power: V(z) = Vref*(z/Zref)^alpha
Where V(z) is speed at target height z, Vref is reference speed at Zref, z0 is roughness length, and alpha is the power law exponent.
Worked Examples
Example 1: Wind Turbine Hub Height Extrapolation
Problem:Weather station measures 10 m/s at 10 m. Extrapolate to 80 m hub height over agricultural terrain (z0=0.03 m, alpha=0.143).
Solution:Log: V(80) = 10*ln(80/0.03)/ln(10/0.03) = 10*7.888/5.809 = 13.58 m/s Power: V(80) = 10*(80/10)^0.143 = 10*1.349 = 13.49 m/s u* = 10*0.4/ln(10/0.03) = 0.689 m/s Power density = 0.5*1.225*13.58^3 = 1534 W/m2
Result:Log: 13.58 m/s | Power: 13.49 m/s | Density: 1534 W/m2
Example 2: Urban Wind Assessment
Problem:Estimate wind at 50 m over urban area (z0=1.0 m, alpha=0.30) given 5 m/s at 20 m.
Solution:Log: V(50) = 5*ln(50/1.0)/ln(20/1.0) = 5*3.912/2.996 = 6.53 m/s Power: V(50) = 5*(50/20)^0.30 = 5*1.316 = 6.58 m/s u* = 5*0.4/ln(20/1.0) = 0.668 m/s Power density = 0.5*1.225*6.53^3 = 171 W/m2
Result:Log: 6.53 m/s | Power: 6.58 m/s | Density: 171 W/m2
Frequently Asked Questions
What is the logarithmic wind profile?
The logarithmic wind profile describes how wind speed increases with height above ground in the atmospheric surface layer the lowest 50 to 200 meters. Derived from Monin-Obukhov similarity theory under neutral stability conditions it states that speed at height z equals friction velocity divided by the von Karman constant times the natural log of z over roughness length. This profile is most accurate in the constant-flux layer where wind direction is approximately constant and mechanical turbulence dominates. It is preferred for wind energy resource assessment air pollution dispersion modeling and meteorological analysis when roughness information is available.
What is the power law wind profile?
The power law is an empirical approximation relating wind speed at a target height to a reference using V(z) = Vref times (z/Zref) to the power alpha. It is simpler than the log profile requiring only reference speed two heights and an exponent without roughness length. The standard exponent of one-seventh or 0.143 was derived for flat terrain with moderate roughness. The two methods agree well for height extrapolation ratios up to about 3:1 but can diverge significantly for larger ratios or non-neutral stability. The power law is used when detailed surface characterization is unavailable while the log law is preferred for rigorous engineering.
What is aerodynamic roughness length?
Roughness length z0 characterizes the drag effect of the surface on the wind defined as the height where the log profile extrapolates to zero speed. It is not the physical obstacle height but roughly one-tenth of it. Smooth water has z0 around 0.0001 to 0.001 m while open grassland is about 0.01 to 0.05 m. Agricultural land ranges from 0.05 to 0.25 m and suburban areas are 0.3 to 1.0 m with dense urban exceeding 2 m. It is determined from multi-height wind measurements land use classification or topographic surveys using empirical relationships to obstacle geometry.
How does atmospheric stability affect wind profiles?
Atmospheric stability significantly modifies the vertical wind profile from its neutral logarithmic form by changing turbulent mixing intensity. In unstable conditions like sunny afternoons enhanced mixing brings momentum downward reducing shear and creating more uniform profiles. In stable conditions like clear nights suppressed mixing leads to stronger shear and potentially very light surface winds even with strong winds aloft. Monin-Obukhov theory accounts for stability through correction functions based on height to Obukhov length ratio. Ignoring stability can introduce 20 to 40 percent errors in wind speed extrapolation especially for large height differences.
Why is wind speed extrapolation important for wind energy?
Modern wind turbine hub heights have increased from about 30 m in the 1990s to 80 to 120 m or more but most weather stations measure wind at 10 m height. Extrapolating speed to hub height is essential for wind resource assessment and project feasibility analysis. Since wind power is proportional to the cube of speed even small errors in extrapolation produce large energy estimate errors. A 10 percent speed overestimate translates to roughly 33 percent power overestimate affecting project financial viability. Modern campaigns deploy met towers or lidar at hub height to reduce uncertainty in speed extrapolation.
What is friction velocity?
Friction velocity u-star is a scaling velocity defined as the square root of kinematic surface stress characterizing turbulent momentum transfer near the ground. It is derived not directly measured connecting surface drag force to wind profile structure. Typical values range from 0.1 m/s over calm water to 0.5 m/s or more over rough terrain with strong winds. In the log profile friction velocity determines overall speed magnitude while roughness length determines profile shape. It is used extensively in air pollution dispersion dust emission modeling sand transport prediction and boundary layer parameterization.
What is wind power density?
Wind power density is the kinetic energy rate through a unit area perpendicular to the wind calculated as 0.5 times air density times speed cubed in watts per square meter. It is the fundamental metric for comparing wind energy potential across locations because it incorporates the cubic speed relationship. NREL classifies resources into seven classes with Class 1 below 100 W/m2 at 10 m being poor and Class 7 above 800 W/m2 being outstanding. Because of the cubic relationship power density at 80 to 120 m hub heights can be 2 to 4 times greater than at 10 m measurement height. This justifies the economics of tall turbine towers despite higher construction costs.
How do coastal wind profiles differ from inland?
Coastal and offshore profiles differ substantially due to dramatically different surface roughness of water versus land. Ocean roughness lengths of 0.0001 to 0.001 m produce much weaker wind shear and more uniform profiles than rougher land surfaces. The power law exponent over open water is typically 0.10 to 0.12 compared to 0.14 to 0.20 over land terrain. At coastal locations profiles change abruptly at the shoreline as the internal boundary layer adjusts from sea to land roughness over several kilometers. Thermal land-sea contrasts create sea breezes producing complex non-logarithmic profiles near the coastline.
What is the von Karman constant?
The von Karman constant kappa is approximately 0.4 appearing in the logarithmic law of the wall describing turbulent flow near solid boundaries. Named after Theodore von Karman who proposed mixing length theory in the 1930s. In atmospheric profiles it relates friction velocity to the logarithmic velocity gradient: u-star equals kappa times velocity gradient times height. Extensive measurements and simulations establish its value at about 0.40 though values from 0.35 to 0.42 appear in different studies. Despite being called a constant there is ongoing debate about whether it varies slightly with Reynolds number or atmospheric stability.
How do you choose the power law exponent?
The power law exponent alpha varies with terrain roughness atmospheric stability and height range. For open flat terrain with short grass alpha is typically 0.10 to 0.14 which is why the one-seventh rule at 0.143 works well for standard conditions. Agricultural areas with scattered trees use 0.15 to 0.20 while suburban environments need 0.20 to 0.30. Dense urban areas may require 0.30 to 0.40 or higher for accurate extrapolation. During stable nighttime conditions alpha can reach 0.4 to 0.6 in the nocturnal boundary layer where low-level jets form. The most reliable approach is measuring at multiple heights and fitting to actual site data.
References
Background & Theory
History
Reviewed for accuracy by Daniel Agrici, Founder & Lead Developer ยท Editorial policy
Related Calculators
๐งฎOcean Current Speed Calculator
Calculate ocean current speed with inputs, formulas, and instant results.
๐งฎFlow Resistance Converter (nโf) Calculator
Calculate flow resistance converter (nโf) with inputs, formulas, and instant results.
๐งฎStream Power Index Calculator
Calculate stream power index with inputs, formulas, and instant results.
๐งฎTidal Heating Power Calculator
Calculate tidal heating power with inputs, formulas, and instant results.
๐งฎGeoid Height Calculator
Calculate geoid height with inputs, formulas, and instant results.
๐งฎDarcyโs Law Flow Rate Calculator (geologic)
Calculate darcyโs law flow rate (geologic) with inputs, formulas, and instant results.
๐งฎGlacial Flow Velocity (glenโs Law) Calculator
Calculate glacial flow velocity (glenโs law) with inputs, formulas, and instant results.
๐งฎCloud Base Height Calculator
Calculate cloud base height with inputs, formulas, and instant results.