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Cross Linear Solar Concentration System for CSP

机译:CSP的交叉线性太阳能聚光系统

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The novel solar concentration system, Cross linear (CL) system, with which a high cosine factor above 0.85 can be achieved through the year even in winter season and at high latitudes, has been invented by Tokyo Institute of Technology. Theoretical expression of the cosine factor for CL system can be given by cosine factor = sin δ{ cos Φ (-cos μ) + sin Φ sin μ) + cos δ cos ω( sin Φ cos μ + cos Φ sin μ), where δ, Φ, μ, amd ω are solar declination, latitude, elevation angle of the reflection mirror, and hour angle, respectively. The value of tan μ corresponds to the ratio of the receiver height and mirror position distance from the receiver position for the receiver/mirror configuration of the CL concentration system. One simulation result for the CL system sample geometry (tan μ = 0.7, mirror length 1.5m, mirror number=13 in north side, and 2 in south side from the receiver) shows that we can get 7.7kWh/m~2/d for each mirror (as average) in December at 36.8°N latitude and 11.5 kWh/m~2/d in August, assuming DNI = 1.0kW/m~2 and collection efficiency = 1.0. Nearly the same result is obtained at high latitude of 40°N latitude. Thus, a higher cosine factor above 0.85 can be obtained in winter months even at the higher northern latitude. Also, the CL system can eliminate the end loss, and a comparison study shows that CL system can significantly increase the optical efficiency compared to Trough and LFR (Linear Fresnel Reflector system). Also, from the flux values above 100 kW/m~2 obtained by simulation for the CL system sample, it can be expected that a higher temperature around 600-700 °C can be reliably obtained and the air is heated up with a tubular receiver even in the winter season. With varying the parameters for CL system configuration, suitable solar concentration system with a high cosine factor could be designed depending on a wide temperature range of 300-700 °C. A joint collaboration between Japanese and Indian industries, institutes and universities has been launched to demonstrate and develop the CL system technology in Dec 2012.
机译:东京工业大学已经发明了新颖的太阳能聚集系统,即交​​叉线性(CL)系统,即使在冬季和高纬度地区,全年也可以达到0.85以上的高余弦因数。 CL系统的余弦因数的理论表达式可以由以下公式给出:余弦因数= sinδ{cosΦ(-cosμ)+ sinΦsinμ)+ cosδcosω(sinΦcosμ+ cosΦsinμ),其中δ,Φ,μ和amdω分别是太阳偏角,纬度,反射镜的仰角和小时角。 tanμ的值对应于CL浓度系统的接收器/反射镜配置的接收器高度与反射镜位置与接收器位置的距离之比。对CL系统样本几何形状的一个模拟结果(tanμ= 0.7,反射镜长度1.5m,在接收器的北侧为反射镜编号= 13,在南侧为2反射镜)表明,我们可以获得7.7kWh / m〜2 / d假设DNI = 1.0kW / m〜2且收集效率= 1.0,则12月在纬度36.8°N和8月11.5 kWh / m〜2 / d时(平均)的每个反射镜。在纬度为40°N的高纬度下,可获得几乎相同的结果。因此,即使在北部纬度较高的冬季,也可以在0.85以上获得较高的余弦因数。而且,CL系统可以消除端损耗,并且比较研究表明,与Trough和LFR(线性菲涅尔反射镜系统)相比,CL系统可以显着提高光学效率。另外,从通过CL系统样品的模拟获得的高于100 kW / m〜2的通量值,可以预期可以可靠地获得600-700°C左右的较高温度,并且通过管状接收器加热空气即使在冬季。通过改变CL系统配置的参数,可以根据300-700°C的宽温度范围设计合适的具有高余弦因数的太阳能聚光系统。日印两国工业界,研究所和大学之间的联合合作已于2012年12月启动,以展示和开发CL系统技术。

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