落体粒子接收器石英半壳管孔径罩的光线追踪性能建模

J. Yellowhair, C. Ho
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引用次数: 4

摘要

1 MWt落粒接收器原型在桑迪亚国家实验室的国家太阳能热测试设施(NSTTF)进行了设计、建造和评估。目前的原型有一个面向北部场地的1平方米的孔径。当前的孔径配置容易受到通过接收器孔径的热量和颗粒损失的影响。除了将接收器效率提高到90%的目标水平外,正在考虑为下一次设计迭代提供几种选择,以减少热量和颗粒损失的风险。一种选择是用一种高度耐用的透射材料(如石英玻璃)覆盖接收器孔径。石英玻璃在波长小于2.5微米时透光率高,而在波长大于2.5微米时透光率低,这有助于将热量困在接收器内。为了评估接收器的光学性能,建立了几种不同孔径盖配置的光线跟踪模型。下落粒子接收器被建模为一个在北侧墙上有一个1 m2孔径的盒子。箱体尺寸为宽1.57米×高1.77米×深1.67米。墙壁由模拟为兰伯曲面的RSLE材料组成,原始状态的反射率为0.9,污染墙壁的反射率为0.5。石英半壳管长1.46 m,内径105 mm,外径110 mm。所述半壳管垂直布置,顶部向前倾斜30度。考虑了四种配置:半壳的凹面朝向接收器孔径,(1)无间距,(2)管间间距大;半壳的凹面朝向孔径,(3)管间无间距,(4)管间间距大。在第一种建模方法中,粒子幕被建模为具有透光率、反射率和吸收率值的漫射表面,这些值是基于先前对不同粒子流速率的实验估计的。入射辐射来自全NSTTF定日镜场,在接收器光圈中心有一个瞄准点。从内部接收器表面发射的直接入射光线以及反射和散射光线作为净入射辐照度记录在内壁上和粒子幕表面上。将不同孔径盖结构的内壁和粒子幕上的净入射辐照度与基线配置进行了比较。在所有情况下,仅从光学性能来看,净入射辐照度从基线降低。然而,预计石英半壳将减少通过孔径的对流和热辐射损失。这些射线追踪结果将用作计算流体动力学(CFD)分析的边界条件,以确定净接收器效率和石英半壳的最佳配置,从而最大限度地减少热损失并最大化热效率。
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Optical Ray-Tracing Performance Modeling of Quartz Half-Shell Tubes Aperture Cover for Falling Particle Receiver
A 1 MWt falling particle receiver prototype was designed, built and is being evaluated at Sandia National Laboratories, National Solar Thermal Test Facility (NSTTF). The current prototype has a 1 m2 aperture facing the north field. The current aperture configuration is susceptible to heat and particle losses through the receiver aperture. Several options are being considered for the next design iteration to reduce the risk of heat and particle losses, in addition to improving the receiver efficiency to target levels of ∼90%. One option is to cover the receiver aperture with a highly durable and transmissive material such as quartz glass. Quartz glass has high transmittance for wavelengths less than 2.5 microns and low transmittance for wavelengths greater than 2.5 microns to help trap the heat inside the receiver. To evaluate the receiver optical performance, ray-tracing models were set up for several different aperture cover configurations. The falling particle receiver is modeled as a box with a 1 m2 aperture on the north side wall. The box dimensions are 1.57 m wide × 1.77 m tall × 1.67 m deep. The walls are composed of RSLE material modeled as Lambertian surfaces with reflectance of either 0.9 for the pristine condition or 0.5 for soiled walls. The quartz half-shell tubes are 1.46 m long with 105 mm and 110 mm inner and outer diameters, respectively. The half-shell tubes are arranged vertically and slant forward at the top by 30 degrees. Four configurations were considered: concave side of the half-shells facing away from the receiver aperture with (1) no spacing and (2) high spacing between the tubes, and concave side of the half-shells facing the aperture with (3) no spacing and (4) high spacing between the tubes. The particle curtain, in the first modeling approach, is modeled as a diffuse surface with transmittance, reflectance, and absorptance values, which are based on estimates from previous experiments for varying particle flow rates. The incident radiation is from the full NSTTF heliostat field with a single aimpoint at the center of the receiver aperture. The direct incident rays and reflected and scattered rays off the internal receiver surfaces are recorded on the internal walls and particle curtain surfaces as net incident irradiance. The net incident irradiances on the internal walls and particle curtain for the different aperture cover configuration are compared to the baseline configuration. In all cases, just from optical performance alone, the net incident irradiance is reduced from the baseline. However, it is expected that the quartz half-shells will reduce the convective and thermal radiation losses through the aperture. These ray-tracing results will be used as boundary conditions in computational fluid dynamics (CFD) analyses to determine the net receiver efficiency and optimal configuration for the quartz half-shells that minimize heat losses and maximize thermal efficiency.
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