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高温吸热管内超临界CO2传热特性的数值模拟
引用本文:庄晓如,徐心海,杨智,赵延兴,余鹏. 高温吸热管内超临界CO2传热特性的数值模拟[J]. 物理学报, 2021, 0(3): 170-182
作者姓名:庄晓如  徐心海  杨智  赵延兴  余鹏
作者单位:南方科技大学力学与航空航天工程系;哈尔滨工业大学(深圳)机电工程与自动化学院;广东工业大学材料与能源学院;中国科学院理化技术研究所
基金项目:国家自然科学基金(批准号:51706048);中国科学院低温工程学重点实验室(理化技术研究所)(批准号:CRYO202002)资助的课题。
摘    要:
研究超临界CO2在高温吸热管内的传热特性是将其应用于聚光太阳能热发电技术中的基础.本文对此进行了数值模拟研究,分析了流体温度、流动方向、系统压力、质量流率和热流密度对对流传热系数和Nu数的影响.结果表明:高温区(800—1050 K)的对流传热系数和Nu数受流动方向和系统压力的影响均很小,但都随着质量流率的增大以及热流...

关 键 词:超临界CO2  传热  太阳能吸热管  数值模拟

Numerical investigation on heat transfer of supercritical CO in solar receiver tube in high temperature region
Zhuang Xiao-Ru,Xu Xin-Hai,Yang Zhi,Zhao Yan-Xing,Yu Peng. Numerical investigation on heat transfer of supercritical CO in solar receiver tube in high temperature region[J]. Acta Physica Sinica, 2021, 0(3): 170-182
Authors:Zhuang Xiao-Ru  Xu Xin-Hai  Yang Zhi  Zhao Yan-Xing  Yu Peng
Affiliation:(Department of Mechanics and Aerospace Engineering,Southern University of Science and Technology,Shenzhen 518055,China;School of Mechanical Engineering and Automation,Harbin Institute of Technology(Shenzhen),Shenzhen 518055,China;School of Materials and Energy,Guangdong University of Technology,Guangzhou 510006,China;CAS Key Laboratory of Cryogenics,Technical Institute of Physics and Chemistry,Chinese Academy of Sciences,Beijing 100190,China)
Abstract:
Supercritical CO2 can be used as a heat transfer fluid in a solar receiver,especially for a concentrating solar thermal power tower system.Such applications require better understanding of the heat transfer characteristics of supercritical CO2 in the solar receiver tube in a high temperature region.However,most of the existing experimental and numerical studies of the heat transfer characteristics of supercritical CO2 in tubes near the critical temperature region,and the corresponding heat transfer characteristics in the high temperature region are conducted.In this paper,a three-dimensional steady-state numerical simulation with the standard k-εturbulent model is established by using ANSYS FLUENT for the flow and heat transfer of supercritical CO2 in a heated circular tube with an inner diameter of 6 mm and a length of 500 mm in the high temperature region.The effects of the fluid temperature(823-1023 K),the flow direction(horizontal,downward and upward),the pressure(7.5-9 MPa),the mass flux(200-500 kg-m-2·s-1)and the heat flux(100-800 kW·m-2)on the convection heat transfer coefficient and Nusselt number are discussed.The results show that the convection heat transfer coefficient increases while Nusselt number decreases nearly linearly with fluid temperature increasing.Both fluid direction and pressure have negligible effects on the convection heat transfer coefficient and Nusselt number.Moreover,the convective heat transfer coefficient and Nusselt number are enhanced greatly with the increasing of mass flux and the decreasing of heat flux,which is more obvious at a higher heat flux.The influences of buoyancy and flow acceleration on the heat transfer characteristics are also investigated.The buoyancy effect can be ignored within the present parameter range.However,the flow acceleration induced by the high heat flux significantly deteriorates the heat transfer preformation.Moreover,eight heat transfer correlations of supercritical fluid in tubes are evaluated and compared with the present numerical data.The comparison indicates that the correlations based on the thermal property modification show better performance in the heat transfer prediction in the high temperature region than those based on the dimensionless number modification.And Nusselt number predicted by the best correlation has a mean absolute relative deviation of 8.1%compared with the present numerical results,with all predicted data points located in the deviation bandwidth of±20%.The present work can provide a theoretical guidance for the optimal design and safe operation of concentrating solar receivers where supercritical CO2 is used as a heat transfer fluid.
Keywords:supercritical CO2  heat transfer  solar receiver tube  numerical simulation
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