New investigations on solar thermochemical storage and other high temperature process are starting at the University of Antofagasta. A small cavity-type solar rotary reactor will be constructed to develop gas-solid reactions. For this reactor concept, is expected that the most part of the solid reactants will remain in the central sector of the drum. Thus, high temperatures at this area will benefit the process performance. Since the radiation profile feeding the solar reactor could have a significant effect on the temperature distribution, in this work it is presented a numerical model to analyze how the use of different concentrators affects the cavity walls temperature. First, a reference case was simulated with flat profile radiation. Then, a solar simulator composed of an elliptical mirror and a high power lamp and a multi-faceted concentrator were considered for the analysis. Their radiation profiles were obtained by ray tracing simulations and integrated in a CFD model that predicts the cavity temperature. It was found a relation between the flux profile and the temperature distribution. This way, higher temperatures were achieved at the back side of the cavity, where the most part of the radiation impinged. The most homogeneous temperature distribution was achieved for the multi-faceted concentrator case, in which lower differences between the back and the lateral wall were found.
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31 May 2016
SOLARPACES 2015: International Conference on Concentrating Solar Power and Chemical Energy Systems
13–16 October 2015
Cape Town, South Africa
Research Article|
May 31 2016
Numerical approach to the flux distribution effect on a solar rotary kiln performance
Alessandro Gallo;
Alessandro Gallo
a)
1
University of Antofagasta. Centro de Desarrollo Energético Antofagasta
, Chile. Avda. Angamos, 601, 1270300, Antofagasta, Chile
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Elisa Alonso;
Elisa Alonso
b)
1
University of Antofagasta. Centro de Desarrollo Energético Antofagasta
, Chile. Avda. Angamos, 601, 1270300, Antofagasta, Chile
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Ricardo Pérez-Enciso;
Ricardo Pérez-Enciso
c)
2
University of Sonora. Blvd. Encinas y Rosales s/n. Hermosillo
, 83000 Sonora, México
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Edward Fuentealba;
Edward Fuentealba
d)
1
University of Antofagasta. Centro de Desarrollo Energético Antofagasta
, Chile. Avda. Angamos, 601, 1270300, Antofagasta, Chile
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Carlos Pérez-Rábago
Carlos Pérez-Rábago
e)
3Instituto de Energías Renovables.
Universidad Nacional Autónoma de México
. Avda. Xochicalco s/n, A.P. 34.Temixco, 62580 Morelos, México
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AIP Conf. Proc. 1734, 030016 (2016)
Citation
Alessandro Gallo, Elisa Alonso, Ricardo Pérez-Enciso, Edward Fuentealba, Carlos Pérez-Rábago; Numerical approach to the flux distribution effect on a solar rotary kiln performance. AIP Conf. Proc. 31 May 2016; 1734 (1): 030016. https://doi.org/10.1063/1.4949068
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