Issue |
EPJ Web Conf.
Volume 143, 2017
EFM16 – Experimental Fluid Mechanics 2016
|
|
---|---|---|
Article Number | 02096 | |
Number of page(s) | 8 | |
Section | Contributions | |
DOI | https://doi.org/10.1051/epjconf/201714302096 | |
Published online | 12 May 2017 |
https://doi.org/10.1051/epjconf/201714302096
Research on high-temperature heat receiver in concentrated solar radiation system
AGH University of Science and Technology, Faculty of Energy and Fuels, Department of Sustainable Energy Development, A. Mickiewicza Av. 30, 30-059 Kraków, Poland
* Corresponding author: esterap@agh.edu.pl
Published online: 12 May 2017
The article presents the results of experimental and computer simulations studies of the high temperature heat receiver working in the concentrated solar radiation system. In order to study the radiation absorption process and heat exchange, the two types of computer simulations were carried out. The first one was used to find the best location for absorber in the concentrating installation. Ray Tracing Monte Carlo (RTMC) method in Trace Pro software was used to perform the optical simulations. The results of these simulations were presented in the form of the solar radiation distribution map and chart. The data obtained in RTMC simulations were used as a second type boundary conditions for Computational Fluid Dynamics (CFD) simulations. These studies were used to optimize the internal geometry of the receiver and also to select the most effective flow parameters of the working medium. In order to validate the computer simulations, high temperature heat receiver was tested in experimental conditions. The article presents the results of experimental measurements in the form of temperature, radiation intensity and power graphs. The tests were performed for varied flow rate and receiver location. The experimental and computer simulation studies presented in this article allowed to optimize the configuration of concentrating and heat receiving system.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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