Simulation and experimental study of an air tube-cavity solar receiver
Simulation and experimental study of an air tube-cavity solar receiver
复制标题
空气管腔太阳能接收器的仿真与实验研究
DOI:
10.1016/j.enconman.2015.07.013
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发表时间:
2015-10
影响因子:
10.4
通讯作者:
Kefa Cen
中科院分区:
文献类型:
--
作者:
Kunzan Qiu;Liang Yan;Mingjiang Ni;Cheng Wang;Gang Xiao;Zhongyang Luo;Kefa Cen
High temperature air is a potential candidate as a heat transfer fluid to transport energy from concentrated solar power to gas turbines. A 15-turn helically coiled tube cavity receiver with an optical splitter at the bottom is designed and fabricated. Its performance is investigated with a five 7-kW Xe-arc lamps array system as heat source. Eight K-type thermocouples are placed from top to bottom with an equal interval. The outlet temperature experimentally ranges from 593 °C to 546 °C when the air flow rate increases from 1 m3/h to 5 m3/h for up-flows, while it ranges from 662 °C to 570 °C for down-flows, when the average flux on aperture is around 120 kW/m2. The Monte-Carlo ray-tracing method and the Lambert testing method with a charge-coupled device (CCD) camera are used to simulate and evaluate the concentrating radiation energy distribution on the cavity’s internal walls, and then the actual flux distribution of each turn of the helically coiled tube is obtained. A comprehensive simulation model is proposed and validated by the experimental results, where the outlet temperature deviations are within 8.0% and 2.5% for down and up-flows, respectively. The model provides a detailed analysis of heat flows at different conditions, and indicates optimization ways to improve the efficiency and reduce heat losses. The simulation results show that the outlet temperature can increase up to around 800 °C at 5 m3/h under an average flux of 300 kW/m2, and the thermal efficiency can be improved from around 56% to around 64% by decreasing the inner radius from 6 mm to 4 mm at the expense of increasing pressure drop of around 56 kPa.
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DOI:
10.1016/j.egypro.2014.03.031
发表时间:
2014
期刊:
Energy Procedia
影响因子:
--
作者:
F. Bai;Yunfan Zhang;Xue-Heng Zhang;Fushun Wang;Yupei Wang;Z. Wang
通讯作者:
F. Bai;Yunfan Zhang;Xue-Heng Zhang;Fushun Wang;Yupei Wang;Z. Wang
影响因子:
11.2
作者:
G. Xiao;Kaikai Guo;Zhong-yang Luo;M. Ni;Yanmei Zhang;Cheng Wang
通讯作者:
G. Xiao;Kaikai Guo;Zhong-yang Luo;M. Ni;Yanmei Zhang;Cheng Wang
DOI:
--
发表时间:
2008-03
期刊:
--
影响因子:
--
作者:
L. Amsbeck;R. Buck;P. Heller;Jens Jedamski;R. Uhlig
通讯作者:
L. Amsbeck;R. Buck;P. Heller;Jens Jedamski;R. Uhlig
DOI:
10.1016/j.egypro.2015.03.042
发表时间:
2015-05
期刊:
Energy Procedia
影响因子:
--
作者:
A. D. Río;Román Korzynietz;José Antonio Brioso;M. Gallas;I. Ordóñez;M. Quero;Clemente Diaz
通讯作者:
A. D. Río;Román Korzynietz;José Antonio Brioso;M. Gallas;I. Ordóñez;M. Quero;Clemente Diaz
影响因子:
10.4
作者:
Mario Biencinto;L. González;E. Zarza;L. Díez;Javier Muñoz-Antón
通讯作者:
Mario Biencinto;L. González;E. Zarza;L. Díez;Javier Muñoz-Antón