定日镜中央接收器上太阳通量的分析与数值研究

Manish Kumar, D. J. Krishna
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引用次数: 1

摘要

研究的目的是估计定日镜中央接收系统的太阳通量。利用解析法和蒙特卡罗射线追踪法对固定目标上的太阳通量进行了数值模拟。模拟是使用NREL(国家可再生能源实验室)发布的免费软件Sol Trace进行的。一个平面定日镜(1×1 m2),位于距离15米高的塔底10米远的地方,在塔底上考虑(1.6×1.6 m2)作为研究目标。模型的设计使用了Sketch up。考虑位于东经79.5°、北纬18°的印度NIT Warangal以1小时为间隔预测4月1日上午9时至下午5时在目标上的太阳通量。比较了用解析法和数值法计算的太阳通量对目标的影响。两种方法的最大差异在±5%以内。研究表明,磁场损耗在定日镜中央接收系统中起着重要的作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Analytical and numerical study to assess the solar flux on a heliostat based central receiver
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.
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