. Non-stationary mathematical model of the temperature distribution in solar panel layers

D.V. Zakharov, L.I. Knysh
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Abstract

This paper presents the results of mathematical modeling of non-stationary temperature fields in a typical solar panel under real environmental conditions. The mathematical model is based on a system of nonlinear ordinary differential equations with corresponding initial and boundary conditions. The model takes into account radiation losses from the surface of the panel, which are determined by the Stefan–Boltzmann law, and convective losses due to free and forced convection. The solar flux density was considered constant, but its value depended on the solar panel setting angle. The temperature dependence of the solar cell efficiency was calculated using a standard method. A computational algorithm was developed in C++ using standard mathematical libraries with a linearization of the system of ordinary differential equations. The results were visualized using the gnuplot graphing utility. The temperature distribution in each of the solar panel layers was obtained as a function of the ambient temperature. It was found that an increase in the ambient temperature leads to a significant decrease, up to 40%, in the solar panel efficiency. With increasing ambient temperature, the time of transition to steady operation increases. The solar panel temperature was related to the blackness degree of the protective glass. It was shown that in the Kirchhoff approximation it is necessary that the blackness degree of the selective coating of the protective glass be a maximum, which reduces the temperature of the system and increases its efficiency. The solar panel temperature was related to the wind speed. It was shown that the convective losses increase with the wind speed, which has a favorable effect on the solar panel temperature regime. The results of the study showed the effect of various external environmental factors on the temperature regime of a solar panel and a way to maximize its efficiency by optimizing its parameters. The results may be used in the development and production of improved solar panels with minimum temperature effects on their efficiency.
. 太阳能板层内温度分布的非平稳数学模型
本文给出了实际环境条件下典型太阳能电池板非稳态温度场的数学建模结果。数学模型建立在具有相应初始条件和边界条件的非线性常微分方程组的基础上。该模型考虑了面板表面的辐射损失(由Stefan-Boltzmann定律决定)以及自由对流和强制对流造成的对流损失。太阳通量密度被认为是恒定的,但它的值取决于太阳能电池板的安装角度。用标准方法计算了太阳能电池效率与温度的关系。利用标准数学库在c++中开发了一种计算算法,并对常微分方程组进行了线性化处理。使用gnuplot绘图实用程序将结果可视化。每个太阳能板层的温度分布作为环境温度的函数得到。研究发现,环境温度的升高会导致太阳能电池板效率的显著下降,最高可达40%。随着环境温度的升高,过渡到稳定运行的时间增加。太阳能板温度与保护玻璃的黑度有关。结果表明,在Kirchhoff近似下,保护玻璃选择性涂层的黑度必须达到最大值,这样可以降低系统温度,提高系统效率。太阳能板温度与风速有关。结果表明,对流损失随风速增大而增大,这对太阳能板的温度变化有有利的影响。研究结果显示了各种外部环境因素对太阳能电池板温度状态的影响,以及通过优化其参数来最大化其效率的方法。研究结果可用于开发和生产温度对效率影响最小的改进型太阳能电池板。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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