4.7 Article

Self-nested large-eddy simulations in PALM model system v21.10 for offshore wind prediction under different atmospheric stability conditions

Journal

GEOSCIENTIFIC MODEL DEVELOPMENT
Volume 16, Issue 12, Pages 3553-3564

Publisher

COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/gmd-16-3553-2023

Keywords

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Large-eddy simulation (LES) is used to resolve large-scale turbulence and parametrize small-scale turbulence. In wind turbine wakes, resolving micro-scale turbulence requires small grid spacing and a large domain. Nesting interface effectively decreases computational time, but introduces another source of uncertainty. This study verifies the nesting effects on shear-driven flow in LES using the PALM model system.
Large-eddy simulation (LES) resolves large-scale turbulence directly and parametrizes small-scale turbulence. Resolving micro-scale turbulence, e.g., in wind turbine wakes, requires both a sufficiently small grid spacing and a domain large enough to develop turbulent flow. Refining a grid locally via a nesting interface effectively decreases the required computational time compared to the global grid refinement. However, interpolating the flow between nested grid boundaries introduces another source of uncertainty. Previous studies reviewed nesting effects for a buoyancy-driven flow and observed a secondary circulation in the two-way nested area. Using a nesting interface with a shear-driven flow in LES, therefore, requires additional verification. We use PALM model system 21.10 to simulate a boundary layer in a cascading self-nested domain under neutral, convective, and stable conditions and verify the results based on the wind speed measurements taken at the FINO1 platform in the North Sea. We show that the feedback between parent and child domains in a two-way nested simulation of a non-neutral boundary layer alters the circulation in the nested area, despite spectral characteristics following the reference measurements. Unlike the pure buoyancy-driven flow, a nonneutral shear-driven flow slows down in a two-way nested area and accelerates after exiting the child domain. We also briefly review the nesting effect on the velocity profiles and turbulence anisotropy.

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