首页> 外文期刊>Journal of Wind Engineering and Industrial Aerodynamics: The Journal of the International Association for Wind Engineering >Computational fluid dynamics simulations and wind tunnel measurements of unsteady wind loads on a scaled model of a very large optical telescope: A comparative study
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Computational fluid dynamics simulations and wind tunnel measurements of unsteady wind loads on a scaled model of a very large optical telescope: A comparative study

机译:大型光学望远镜比例模型上的非稳态风荷载的计算流体动力学模拟和风洞测量:对比研究

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Thorough theoretical and experimental investigations were performed to analyze the main characteristics of unsteady flows past a 1:100-scale wind tunnel (WT) model of a very large optical telescope housed within a spherical enclosure. The investigations were focused on the prediction and measurements of unsteady pressures on the inner and outer surfaces of the enclosure and on the telescope primary mirror. The WT measurements were performed essentially to provide aerodynamic data on the telescope structure and also to build a database for correlation with numerical simulation of the flow using computational fluid dynamics (CFD). Unsteady viscous flow solutions were computed for different telescope orientations using the lattice Boltzmann method coupled with the RNG k-epsilon turbulence model. For WT testing, unsteady pressure measurements were performed in an open jet WT for different telescope orientations and wind speeds, using a number of pressure taps distributed around the inner and the outer surfaces of the enclosure and on the primary mirror surface. A smoke stream visualization technique was also used to study the flow behavior around and inside of the telescope enclosure. The flow solutions were computed using the WT flow conditions. Correlations were obtained between CFD and WT data in terms of the mean pressure coefficients on the enclosure and the primary mirror surfaces, and for their standard deviations. Power spectral density analyses were also carried out for a number of pressure signals collected on the primary mirror surface. Both CFD solutions and WT measurements demonstrated that the flow inside and outside the enclosure was unsteady and massively separated on the back of the enclosure. The mean values and standard deviations of the pressure coefficients on the enclosure and the primary mirror surfaces correlated well with the experimental data. Using the WT Mach number in the simulation, the shear layer over the enclosure opening and the resulting acoustic wave effects were well captured, and there was excellent agreement between the CFD results and the WT measurements. (c) 2007 Elsevier Ltd. All rights reserved.
机译:进行了彻底的理论和实验研究,以分析通过球形罩内的超大型光学望远镜的1:100比例风洞(WT)模型的非稳态流动的主要特征。研究集中在对外壳内外表面以及望远镜主镜上的非恒定压力的预测和测量上。进行WT测量主要是为了提供望远镜结构上的空气动力学数据,并建立一个数据库,以便使用计算流体力学(CFD)与流动的数值模拟进行关联。使用格子Boltzmann方法结合RNGk-ε湍流模型,针对不同望远镜方向计算了非定常粘性流解。对于WT测试,使用围绕外壳的内表面和外表面以及在主镜表面上分布的多个压力抽头,在开放式射流WT中针对不同的望远镜方向和风速进行了非恒定压力测量。烟流可视化技术还用于研究望远镜外壳周围和内部的流动行为。使用WT流动条件计算流动解。根据外壳和主镜表面上的平均压力系数及其标准偏差,获得了CFD和WT数据之间的相关性。还对收集在主镜表面上的许多压力信号进行了功率谱密度分析。 CFD解决方案和WT测量均表明,机箱内部和外部的流动不稳定,并在机箱背面大量分离。外壳和主镜表面上压力系数的平均值和标准偏差与实验数据很好地相关。在仿真中使用WT马赫数,可以很好地捕获外壳开口上方的剪切层和所产生的声波效应,并且CFD结果与WT测量值之间具有极好的一致性。 (c)2007 Elsevier Ltd.保留所有权利。

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