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Experimental investigation of peak wind loads on tandem operating heliostats within an atmospheric boundary layer

机译:大气边界层内串联峰值风荷载峰值的实验研究

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During the operation of a concentrating solar thermal (CST) power tower plant, heliostat mirrors inclined at different angles act as bluff bodies that are exposed to large drag loads from the wind. This experimental study investigates the aerodynamic loads on a heliostat in a tandem configuration, to determine the significance of the shielding effect from an upstream heliostat. To understand the effect of turbulence on the peak wind loads, scale model heliostats with square facets were positioned within a part-depth atmospheric boundary layer (ABL) with a Power Law velocity profile. Peak drag coefficients on the instrumented downstream heliostat in the tandem configuration were normalized with respect to those on a single (isolated) heliostat. A range of tandem configurations were tested to determine the effects of elevation angle, azimuth angle, and gap spacing between the tandem heliostats. Findings show that peak drag loads are reduced by up to 60% on the downstream heliostat relative to an isolated heliostat at an elevation angle of 90 (A) over cap degrees and a gap spacing of two chord lengths, but at higher gap spacing the shielding effect is either marginal or non-existent. Peak hinge moment coefficients on a downstream heliostat in tandem are up to seven times the load on an isolated heliostat, with the maximum occurring at 90 (A) over cap degrees elevation and 180 (A) over cap degrees azimuth. Base-overturning moment coefficients are less affected, as the changes in the centre of pressure location are relatively small compared to the length of the support pylon. Strouhal number analysis of the fluctuating surface pressures indicated that the dominant frequency of the pressure spectra on the downstream heliostat is over three times the value on an isolated heliostat at 45 (A) over cap degrees elevation and azimuth angles. Hence, both static and dynamic effects must be considered separately in the wind load design for heliostats at typical operating angles.
机译:在浓缩太阳能热(CST)动力塔架的操作期间,以不同角度倾斜的光晕镜用作从风中暴露于大的阻力负荷的虚张体。该实验研究研究了在串联配置中的Heliostat上的空气动力学载荷,以确定屏蔽效果的显着性来自上游的Heliostat。为了了解湍流对峰值风荷载的影响,具有方面的比例模型定位在具有电力法速度分布的部分深度大气边界层(ABL)内。串联配置中仪表下游光晕峰值的峰值拖曳系数是关于单个(孤立)Heliostat上的那些标准化的。测试了一系列串联配置,以确定垂直角,方位角和串联光晕岩之间的间隙间距的影响。调查结果表明,在下游光升降阀上,峰值阻力负载相对于盖帽度为90(a)的仰角的隔离角度,并且两个弦长的间隙间隔,但在屏蔽的较高间隙间距下,升高的半弦和两个弦长的间隙间距下降效果是边缘或不存在的。串联下游光晕峰值的峰值铰链矩系数最多七倍隔离的光晕峰值,最大在90(a)上,在帽子升高和180(a)上方的帽子方位角上。基础推翻时刻系数受影响较小,因为与支撑塔的长度相比,压力位置中心的变化相对较小。波动表面压力的Strouhal数分析表明,下游光谱上的压力光谱的显性频率是在45(a)上的隔离光晕峰值上的三倍于帽升高和方位角。因此,静态和动态效果必须在典型的操作角度下分别在风载设计中分别考虑。

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