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Analytical and numerical study to assess the solar flux on a heliostat based central receiver

机译:基于定日镜的中央接收器评估太阳通量的分析和数值研究

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The objective of the study is to estimate the solar flux for a heliostat based central receiver system. Analytical and Monte Carlo ray tracing based numerical simulations have been performed to assess the solar flux on a fixed target. The simulations have been performed using a freeware Sol Trace released by NREL (National Renewable Energy Laboratory). A flat heliostat of (1×1 m2), which is located 10 m far from the base of a 15 m high tower, on which, (1.6×1.6 m2) target is considered for the study. Sketch up has been used for designing the model. NIT Warangal, India with a longitude 79.5 ° E and latitude 18 ° N is considered to predict the solar flux on the target on 1st April from 9 am to 5pm at the interval of one hour. Result obtained from analytical and numerical methods are compared in terms of solar flux on the target. It is observed that maximum variation between the two methods is within ±5%. The study could reveal that the field losses play an important role in the heliostat based central receiver system.
机译:该研究的目的是估计基于定日镜的中央接收器系统的太阳通量。已经进行了基于分析和蒙特卡洛射线追踪的数值模拟,以评估固定目标上的太阳通量。使用NREL(国家可再生能源实验室)发布的免费软件Sol Trace进行了仿真。平面定日镜(1×1 m2),距15 m高塔楼底部10 m,其目标为(1.6×1.6 m2)。草绘已用于设计模型。印度NIT瓦兰加尔(WIT)的经度为79.5°E,纬度为18°N,可以预测4月1日上午9点至下午5点之间目标间隔1小时的太阳通量。通过分析和数值方法获得的结果将根据目标的太阳通量进行比较。观察到两种方法之间的最大差异在±5%之内。研究表明,场损耗在基于定日镜的中央接收器系统中起着重要作用。

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