Published July 8, 2024 | Version v1
Journal article

Large-eddy simulations of turbulent wake flows behind helical- and straight-bladed vertical axis wind turbines rotating at low tip speed ratios

  • 1. Department of Mechanical Engineering, University of Houston, Houston, Texas 77204, USA
  • 2. National Renewable Energy Laboratory, Golden, Colorado 80401, USA
  • 3. Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland 20723, USA

Description

Turbulent wake flows behind helical- and straight-bladed vertical axis wind turbines (VAWTs) rotating at low tip speed ratios (TSRs) are studied numerically. The turbulent flows are simulated using the large-eddy simulation (LES) model, and the rotating turbine blades are modeled using the actuator line method. The helical VAWT has identical key parameters as the straight VAWT except for the 135 helical twist of the blades over the 0.3m vertical span. A set of LES runs are performed for two TSRs, 0.6 and 0.4, and the results are reported and analyzed. At these low TSRs, the wake behind the straight-bladed VAWT exhibits two-dimensional dominant flow motions (in the horizontal plane perpendicular to the straight blades) in the near-wake region that cause considerable spanwise expansion of the wake as it extends downstream. In contrast, the helical-bladed VAWT generates highly three-dimensional (3D) wake flow structures and upward/downward mean flow motions within the wake that cause the wake to expand mainly in the vertical direction. Turbulence statistical analyses also show that the 3D wake flow features induced by the helical blades accelerate the wake transition to turbulence and enhance the small-scale turbulent dissipation (as shown by the subgrid-scale turbulent dissipation in the LES), which leads to a more rapid decay of the wake turbulence intensity than that in the straight-bladed VAWT case at the same TSR. Compared with the straight-bladed VAWT, the helical-bladed VAWT also exhibits much smaller temporal variations for the torque and power coefficients during the rotation cycle, which can be beneficial for wind power generation.

Additional details

Identifiers

DOI
10.1103/PhysRevFluids.9.074603;
Crossref Funder ID
10.13039/100000001; 10.13039/100007144; 10.13039/100006233; 10.13039/100000015;

Publishing Information

Journal Title
Physical Review Fluids
Journal Volume
9
Journal Issue
7
Journal Page Range
35 pgs.
ISSN
2469-990X

Optional Information

Copyright
©2024 American Physical Society
Contract/Grant/Project number
1804214; DE-AC36-08GO28308
Notes
Present address: Department of Mechanical Engineering, Johns Hopkins University, Baltimore, Maryland 21218, USA.; Contact Email: Contact author: diyang@uh.edu; Record automatically processed
Funding organization
National Science Foundation; University of Houston; National Renewable Energy Laboratory; U.S. Department of Energy