Examines dynamic power output influenced by atmospheric turbulence in wind turbines, suggesting potential improvements in power forecasting.
This study examines how coherent turbulent structures in the atmospheric boundary layer influence the dynamic power output of a horizontal-axis wind turbine. The spanwise velocity distribution upstream of the rotor and the concurrent power output were simultaneously measured in a wind tunnel using an array of five hot-wire probes coupled and a high-frequency data acquisition system. Results reveal a 1.37 s lag in power response relative to velocity fluctuations, attributed to rotor inertia and electromagnetic damping. The correlation between single-point velocity and instantaneous power is below 0.35, highlighting the critical role of turbulence spatial non-uniformity. Reconstructing the flow field using Taylor's frozen turbulence hypothesis shows that the spatial distribution of large-scale turbulent structures across the rotor plane, combined with the turbine's dynamic response, governs the instantaneous power and its fluctuations. A multi-point convolution model based on real-time spatial mapping was developed to account for inflow dynamics and spatial variability. Validation shows the five-probe model achieves a relative error of 0.32% and R2 = 0.803, significantly outperforming the conventional (11.89% error) and single-point models (0.7% error, R2 = 0.785). This work provides a physical basis for predicting instantaneous wind power fluctuations and understanding turbine dynamic response under turbulent inflow.
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Ma et al. (2026) studied this question.
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