Numerical Simulation of a Parabolic Through Solar Collector with a Novel Geometric Design Equipped with an Elliptical Absorber Tube Under the Influence of Magnetic Field

IF 2.9 4区 综合性期刊 Q1 Multidisciplinary
Ali Golzar, Alireza Aghaei, Hamid Mohsenimonfared, Ali Hassani Joshaghani
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Abstract

The primary basis of the present study is the design of a new geometry of the parabolic through solar collector in order to achieve maximum thermal efficiency. Most of the absorber tubes used in solar system have a circular cross section. In this study, the cross section of the PTSC absorber tube is modeled as elliptical. Also, in this study, in order to make thermal properties more practical, DWCNT and GO nanoparticles were dispersed in Syltherm 800 base fluid. Syltherm 800 heat transfer oil is used as a condensing HT oil up to the highest temperature, because this BF has low viscosity and high thermal stability. Also, using this BF in TS prevents sedimentation and pollution. An innovative combined turbulator has been used to change the shape of flow lines to create turbulence in the path of the absorber tube. In addition, in the final stage of elliptical absorber tube, in the middle part where ICT is located, it is affected by the magnetic field, and different values of Hartmann number are checked on it. The obtained numerical results state that the most trend of changes in the average Nusselt number in EAT is due to the presence of ICT in the hybrid nanofluid flow path. However, in the next step, the most changes that can be seen in the \({\text{Nu}}_{{{\text{ave}}}}\) are due to the increase in the transverse ratio of ICT. Based on the results, it can be stated that the use of the MF in higher Ha has a significant effect on the hydrodynamic performance of the SS of the present study and increases the value of the PEC index to some extent compared to lower Ha. Also, based on the results, the Ha = 150 has the highest exergy efficiency \((\eta_{{{\text{ex}}}} )\) values in all the investigated Re ranges. After that, Ha = 100 and 50 are in successive positions. The highest exergy efficiency in the absence of a magnetic field occurs at a Reynolds number of 10,000, a volume fraction of 4%, and for ξ = 12 mm, which is around 55%. The lowest exergy efficiency with change of Hartmann number occurs at Reynolds number of 60,000, volume fraction of 4%, PR = 2, and in ξ = 12 mm.

Abstract Image

磁场影响下配备椭圆形吸收管的抛物面贯通式太阳能集热器的新型几何设计数值模拟
本研究的主要基础是设计一种新的抛物面直通式太阳能集热器的几何形状,以实现最高的热效率。太阳能系统中使用的大多数吸收管的横截面都是圆形的。在本研究中,PTSC 吸收管的横截面被模拟为椭圆形。此外,在本研究中,为了使热学特性更加实用,将 DWCNT 和 GO 纳米颗粒分散在 Syltherm 800 基础油中。Syltherm 800 导热油可用作最高温度的冷凝 HT 油,因为这种基础油具有低粘度和高热稳定性。此外,在 TS 中使用这种基础油可以防止沉淀和污染。创新的组合式湍流器用于改变流线的形状,从而在吸收管的路径上产生湍流。此外,在椭圆形吸收管的最后阶段,即信息和通信技术所在的中间部分,它受到磁场的影响,并对不同的哈特曼数值进行了检测。数值结果表明,EAT 中平均努塞尔特数的最大变化趋势是由于混合纳米流体流道中 ICT 的存在。然而,在下一步中,可以看到 \({\text{Nu}}_{{text{ave}}}}\) 的最大变化是由于 ICT 横向比的增加。基于这些结果,可以说在较高的 Ha 值下使用 MF 对本研究中 SS 的水动力性能有显著影响,与较低的 Ha 值相比,在一定程度上增加了 PEC 指数值。此外,根据研究结果,在所有研究的 Re 范围内,Ha = 150 的放能效率值最高。之后,Ha = 100 和 50 依次排序。在没有磁场的情况下,最高的放能效率出现在雷诺数为 10000、体积分数为 4%、ξ = 12 mm 时,约为 55%。随着哈特曼数的变化,在雷诺数为 60000、体积分数为 4%、PR = 2 和 ξ = 12 毫米时,放能效率最低。
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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来源期刊
Arabian Journal for Science and Engineering
Arabian Journal for Science and Engineering 综合性期刊-综合性期刊
CiteScore
5.20
自引率
3.40%
发文量
0
审稿时长
4.3 months
期刊介绍: King Fahd University of Petroleum & Minerals (KFUPM) partnered with Springer to publish the Arabian Journal for Science and Engineering (AJSE). AJSE, which has been published by KFUPM since 1975, is a recognized national, regional and international journal that provides a great opportunity for the dissemination of research advances from the Kingdom of Saudi Arabia, MENA and the world.
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