Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids
This work presents a novel design of microchannel central receiver for pressurised gases and supercritical fluids in solar tower plants. It consists of a radial arrangement of vertical absorber panels that converge on the central axis of the tower. The absorber panels comprise compact structures, wh...
| Autores: | , , , , , |
|---|---|
| Formato: | artículo |
| Fecha de publicación: | 2023 |
| País: | España |
| Recursos: | Universidad Nacional de Educación a Distancia |
| Repositorio: | e-spacio. Repositorio Institucional de la UNED |
| Idioma: | inglés |
| OAI Identifier: | oai:e-spacio.uned.es:20.500.14468/12405 |
| Acesso em linha: | https://hdl.handle.net/20.500.14468/12405 |
| Access Level: | acceso abierto |
| Palavra-chave: | Solar central receiver Radial configuration Light-trapping geometry Increasing compactness Supercritical fluid Pressurised gases |
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Proposal of a new design of central solar receiver for pressurised gases and supercritical fluidsGuedez Mata, RafaelLinares Hurtado, José IgnacioGonzález Aguilar, JoséRomero, ManuelMontes Pita, María JoséD Souza, David JonathanSolar central receiverRadial configurationLight-trapping geometryIncreasing compactnessSupercritical fluidPressurised gasesThis work presents a novel design of microchannel central receiver for pressurised gases and supercritical fluids in solar tower plants. It consists of a radial arrangement of vertical absorber panels that converge on the central axis of the tower. The absorber panels comprise compact structures, whose compactness is increased in one flow pass compared to the previous one, as the fluid is heated. This concept reduces radiation heat losses due to its light-trapping geometry and increases heat transfer to the thermal fluid without over penalising its pressure drop. For the receiver assessment, it has been developed a thermal resistance model characterising the fluid heating along the panel height and the temperature gradient between parallel channel rows of the compact structure across the panel thickness. Once the thermal and optical boundary conditions are defined, an optimisation analysis of the main geometrical parameters of the receiver has been accomplished. The receiver performance is evaluated by means of a global exergy efficiency referred to the solar subsystem, which computes the receiver heat losses, the fluid pressure drop and the optical efficiency of the heliostat field in which the receiver is integrated. For each parametric optimisation, the configuration that maximises this efficiency is identified.Elseviere-Spacio UNED20242024-05-2020232023-07-1020232023-07-10journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14468/12405reponame:e-spacio. Repositorio Institucional de la UNEDinstname:Universidad Nacional de Educación a DistanciaInglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/deed.esoai:e-spacio.uned.es:20.500.14468/124052026-06-06T12:38:31Z |
| dc.title.none.fl_str_mv |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| title |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| spellingShingle |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids Guedez Mata, Rafael Solar central receiver Radial configuration Light-trapping geometry Increasing compactness Supercritical fluid Pressurised gases |
| title_short |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| title_full |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| title_fullStr |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| title_full_unstemmed |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| title_sort |
Proposal of a new design of central solar receiver for pressurised gases and supercritical fluids |
| dc.creator.none.fl_str_mv |
Guedez Mata, Rafael Linares Hurtado, José Ignacio González Aguilar, José Romero, Manuel Montes Pita, María José D Souza, David Jonathan |
| author |
Guedez Mata, Rafael |
| author_facet |
Guedez Mata, Rafael Linares Hurtado, José Ignacio González Aguilar, José Romero, Manuel Montes Pita, María José D Souza, David Jonathan |
| author_role |
author |
| author2 |
Linares Hurtado, José Ignacio González Aguilar, José Romero, Manuel Montes Pita, María José D Souza, David Jonathan |
| author2_role |
author author author author author |
| dc.contributor.none.fl_str_mv |
e-Spacio UNED |
| dc.subject.none.fl_str_mv |
Solar central receiver Radial configuration Light-trapping geometry Increasing compactness Supercritical fluid Pressurised gases |
| topic |
Solar central receiver Radial configuration Light-trapping geometry Increasing compactness Supercritical fluid Pressurised gases |
| description |
This work presents a novel design of microchannel central receiver for pressurised gases and supercritical fluids in solar tower plants. It consists of a radial arrangement of vertical absorber panels that converge on the central axis of the tower. The absorber panels comprise compact structures, whose compactness is increased in one flow pass compared to the previous one, as the fluid is heated. This concept reduces radiation heat losses due to its light-trapping geometry and increases heat transfer to the thermal fluid without over penalising its pressure drop. For the receiver assessment, it has been developed a thermal resistance model characterising the fluid heating along the panel height and the temperature gradient between parallel channel rows of the compact structure across the panel thickness. Once the thermal and optical boundary conditions are defined, an optimisation analysis of the main geometrical parameters of the receiver has been accomplished. The receiver performance is evaluated by means of a global exergy efficiency referred to the solar subsystem, which computes the receiver heat losses, the fluid pressure drop and the optical efficiency of the heliostat field in which the receiver is integrated. For each parametric optimisation, the configuration that maximises this efficiency is identified. |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023 2023-07-10 2023 2023-07-10 2024 2024-05-20 |
| dc.type.none.fl_str_mv |
journal article http://purl.org/coar/resource_type/c_6501 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/20.500.14468/12405 |
| url |
https://hdl.handle.net/20.500.14468/12405 |
| dc.language.none.fl_str_mv |
Inglés eng |
| language_invalid_str_mv |
Inglés |
| language |
eng |
| dc.rights.none.fl_str_mv |
open access http://purl.org/coar/access_right/c_abf2 info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/4.0/deed.es |
| rights_invalid_str_mv |
open access http://purl.org/coar/access_right/c_abf2 https://creativecommons.org/licenses/by-nc-nd/4.0/deed.es |
| eu_rights_str_mv |
openAccess |
| dc.format.none.fl_str_mv |
application/pdf |
| dc.publisher.none.fl_str_mv |
Elsevier |
| publisher.none.fl_str_mv |
Elsevier |
| dc.source.none.fl_str_mv |
reponame:e-spacio. Repositorio Institucional de la UNED instname:Universidad Nacional de Educación a Distancia |
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Universidad Nacional de Educación a Distancia |
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e-spacio. Repositorio Institucional de la UNED |
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e-spacio. Repositorio Institucional de la UNED |
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1869405718731292672 |
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15.811543 |