Theoretical and experimental study on the temperature distribution of H-shaped steel members under solar radiation

被引:61
|
作者
Liu, Hongbo [1 ]
Chen, Zhihua [1 ,2 ]
Zhou, Ting [1 ]
机构
[1] Tianjin Univ, Dept Civil Engn, Tianjin 300072, Peoples R China
[2] Tianjin Univ, Tianjin Key Lab Civil Engn Struct & New Mat, Tianjin 300072, Peoples R China
基金
中国国家自然科学基金;
关键词
Temperature; Solar radiation; H-shaped steel; Numerical analysis; Simplified calculation method;
D O I
10.1016/j.applthermaleng.2011.11.045
中图分类号
O414.1 [热力学];
学科分类号
摘要
Thermal effects on steel structures exposed to solar radiation are significant and complicated. Furthermore, the temperature variation within a year may result in damage in steel structures considering the solar radiation. In this paper, the temperature distribution of H-shaped steel members was investigated through a systematic experimental and theoretical study in the case of solar radiation. First, an H-shaped steel specimen was designed and its temperature distribution under solar radiation was obtained by a test. After that, a numerical method was proposed to obtain the temperature distribution under solar radiation. This method was based on transient thermal analysis and the analytical result was verified by the above experimental result. Furthermore, a parametric study was conducted to investigate the influence of various solar radiation parameters and orientation of H-shaped steel members on the temperature distribution under solar radiation. Finally, a simplified approach was developed to predict the temperature distribution under solar radiation. Both experimental and numerical results showed that the solar radiation had a significant effect on the temperature distribution of H-shaped steels. Considering the solar radiation, the temperature of the specimen is about 20.6 degrees C higher than the surrounding ambient air temperature. The temperature distribution under solar radiation was observed to be sensitive to the steel solar radiation absorption and orientation, but insensitive to the solar radiation reflectance. (C) 2011 Elsevier Ltd. All rights reserved.
引用
收藏
页码:329 / 335
页数:7
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