Sebastiano Stipa, Arjun Ajay, D. Allaerts, J. Brinkerhoff
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In the current study, we introduce the open-source, finite-volume, large-eddy simulation (LES) code TOSCA (Toolbox fOr Stratified Convective Atmospheres) and demonstrate its capabilities by simulating the flow around a finite-size wind farm immersed in a shallow, conventionally neutral boundary layer (CNBL), ultimately assessing gravity-wave-induced blockage effects. Turbulent inflow conditions are generated using a new hybrid off-line–concurrent-precursor method. Velocity is forced with a novel pressure controller that allows us to prescribe a desired average hub-height wind speed while avoiding inertial oscillations above the atmospheric boundary layer (ABL) caused by the Coriolis force, a known problem in wind farm LES studies. Moreover, to eliminate the dependency of the potential-temperature profile evolution on the code architecture observed in previous studies, we introduce a method that allows us to maintain the mean potential-temperature profile constant throughout the precursor simulation. Furthermore, we highlight that different codes do not predict the same velocity inside the boundary layer under geostrophic forcing owing to their intrinsically different numerical dissipation. The proposed methodology allows us to reduce such spread by ensuring that inflow conditions produced from different codes feature the same hub wind and thermal stratification, regardless of the adopted precursor run time. Finally, validation of actuator line and disk models, CNBL evolution, and velocity profiles inside a periodic wind farm is also presented to assess TOSCA’s ability to model large-scale wind farm flows accurately and with high parallel efficiency.\n","PeriodicalId":509667,"journal":{"name":"Wind Energy Science","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-02-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"TOSCA – an open-source, finite-volume, large-eddy simulation (LES) environment for wind farm flows\",\"authors\":\"Sebastiano Stipa, Arjun Ajay, D. Allaerts, J. Brinkerhoff\",\"doi\":\"10.5194/wes-9-297-2024\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract. The growing number and growing size of wind energy projects coupled with the rapid growth in high-performance computing technology are driving researchers toward conducting large-scale simulations of the flow field surrounding entire wind farms. This requires highly parallel-efficient tools, given the large number of degrees of freedom involved in such simulations, and yields valuable insights into farm-scale physical phenomena, such as gravity wave interaction with the wind farm and farm–farm wake interactions. In the current study, we introduce the open-source, finite-volume, large-eddy simulation (LES) code TOSCA (Toolbox fOr Stratified Convective Atmospheres) and demonstrate its capabilities by simulating the flow around a finite-size wind farm immersed in a shallow, conventionally neutral boundary layer (CNBL), ultimately assessing gravity-wave-induced blockage effects. Turbulent inflow conditions are generated using a new hybrid off-line–concurrent-precursor method. Velocity is forced with a novel pressure controller that allows us to prescribe a desired average hub-height wind speed while avoiding inertial oscillations above the atmospheric boundary layer (ABL) caused by the Coriolis force, a known problem in wind farm LES studies. Moreover, to eliminate the dependency of the potential-temperature profile evolution on the code architecture observed in previous studies, we introduce a method that allows us to maintain the mean potential-temperature profile constant throughout the precursor simulation. Furthermore, we highlight that different codes do not predict the same velocity inside the boundary layer under geostrophic forcing owing to their intrinsically different numerical dissipation. The proposed methodology allows us to reduce such spread by ensuring that inflow conditions produced from different codes feature the same hub wind and thermal stratification, regardless of the adopted precursor run time. 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引用次数: 0
摘要
摘要风能项目的数量和规模不断增加,加上高性能计算技术的快速发展,促使研究人员对整个风电场周围的流场进行大规模模拟。由于此类模拟涉及大量自由度,因此需要高度并行高效的工具,并能对风电场规模的物理现象(如重力波与风电场的相互作用以及风电场与风电场之间的尾流相互作用)提出有价值的见解。在当前的研究中,我们介绍了开源、有限体积、大涡模拟(LES)代码 TOSCA(Toolbox fOr Stratified Convective Atmospheres,分层对流大气工具箱),并通过模拟浸没在浅层常规中性边界层(CNBL)中的有限尺寸风电场周围的流动来展示其功能,最终评估重力波引起的阻塞效应。湍流流入条件是通过一种新的混合离线-共流-前导方法产生的。速度是通过新型压力控制器强制产生的,该控制器允许我们设定所需的轮毂高度平均风速,同时避免科里奥利力引起的大气边界层(ABL)上方的惯性振荡,这是风电场 LES 研究中的一个已知问题。此外,为了消除以往研究中观察到的势温剖面演变对代码结构的依赖性,我们引入了一种方法,使我们能够在整个前兆模拟过程中保持平均势温剖面不变。此外,我们还强调,不同的代码由于其内在的数值耗散不同,在地营强迫下预测的边界层内速度也不相同。所提出的方法使我们能够减少这种差异,确保不同代码产生的流入条件具有相同的枢纽风和热分层,而不管所采用的前兆运行时间。最后,我们还介绍了对推杆线和盘模型、CNBL 演变以及周期性风电场内部速度剖面的验证,以评估 TOSCA 以高并行效率准确模拟大规模风电场流动的能力。
TOSCA – an open-source, finite-volume, large-eddy simulation (LES) environment for wind farm flows
Abstract. The growing number and growing size of wind energy projects coupled with the rapid growth in high-performance computing technology are driving researchers toward conducting large-scale simulations of the flow field surrounding entire wind farms. This requires highly parallel-efficient tools, given the large number of degrees of freedom involved in such simulations, and yields valuable insights into farm-scale physical phenomena, such as gravity wave interaction with the wind farm and farm–farm wake interactions. In the current study, we introduce the open-source, finite-volume, large-eddy simulation (LES) code TOSCA (Toolbox fOr Stratified Convective Atmospheres) and demonstrate its capabilities by simulating the flow around a finite-size wind farm immersed in a shallow, conventionally neutral boundary layer (CNBL), ultimately assessing gravity-wave-induced blockage effects. Turbulent inflow conditions are generated using a new hybrid off-line–concurrent-precursor method. Velocity is forced with a novel pressure controller that allows us to prescribe a desired average hub-height wind speed while avoiding inertial oscillations above the atmospheric boundary layer (ABL) caused by the Coriolis force, a known problem in wind farm LES studies. Moreover, to eliminate the dependency of the potential-temperature profile evolution on the code architecture observed in previous studies, we introduce a method that allows us to maintain the mean potential-temperature profile constant throughout the precursor simulation. Furthermore, we highlight that different codes do not predict the same velocity inside the boundary layer under geostrophic forcing owing to their intrinsically different numerical dissipation. The proposed methodology allows us to reduce such spread by ensuring that inflow conditions produced from different codes feature the same hub wind and thermal stratification, regardless of the adopted precursor run time. Finally, validation of actuator line and disk models, CNBL evolution, and velocity profiles inside a periodic wind farm is also presented to assess TOSCA’s ability to model large-scale wind farm flows accurately and with high parallel efficiency.