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Effect of concentration areas in sensitive analysis of a hybrid solar Brayton cycle

dc.contributor.authorMoreno Gamboa, Faustino
dc.contributor.authorEspinel Blanco, E
dc.contributor.authorFlorez Solano, E
dc.date.accessioned2024-04-24T14:38:59Z
dc.date.available2024-04-24T14:38:59Z
dc.date.issued2021-06-11
dc.identifier.urihttps://repositorio.ufps.edu.co/handle/ufps/7030
dc.description.abstractA simple hybrid solar thermal Brayton cycle plant thermodynamic model is evaluated in northern Colombia, where the maximum solar radiation values in the country are found. The model considers the different irreversibilities of the cycle and is coupled to a model for estimating direct solar radiation as a complementary energy source for the plant. The stability in the operation of the cycle is determined by a combustion chamber that complements the energy supply. As a result of the analysis, this work presents the sensitivity analysis of different operating parameters of the plant as a function of the areas of the concentration ratio of the solar system when the contribution of this system is maximum. It is observed that fuel consumption is reduced by 34.7% when increasing the concentration ratio between 200 and 700.eng
dc.format.extent8 Páginasspa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.publisherJournal of Physics: Conference Seriesspa
dc.rightsEstá bajo una licencia Creative Commons Atribución 4.0 Internacional (CC BY 4.0).eng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/spa
dc.sourcehttps://iopscience.iop.org/article/10.1088/1742-6596/2073/1/012013spa
dc.titleEffect of concentration areas in sensitive analysis of a hybrid solar Brayton cycleeng
dc.typeArtículo de revistaspa
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dc.identifier.doi10.1088/1742-6596/2073/1/012013
dc.relation.citationeditionVol.2073 No. (2021)spa
dc.relation.citationendpage8spa
dc.relation.citationissue(2021)spa
dc.relation.citationstartpage1spa
dc.relation.citationvolume2073spa
dc.relation.citesF Moreno-Gamboa et al 2021 J. Phys.: Conf. Ser. 2073 012013
dc.relation.citesJournal of Physics: Conference Series 2073 (2021) 012013doi:10.1088/1742-6596/2073/1/012013
dc.rights.accessrightsinfo:eu-repo/semantics/openAccessspa
dc.rights.creativecommonsAtribución 4.0 Internacional (CC BY 4.0)spa
dc.type.coarhttp://purl.org/coar/resource_type/c_6501spa
dc.type.contentTextspa
dc.type.driverinfo:eu-repo/semantics/articlespa
dc.type.redcolhttp://purl.org/redcol/resource_type/ARTspa
oaire.accessrightshttp://purl.org/coar/access_right/c_abf2spa
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85spa
dc.type.versioninfo:eu-repo/semantics/publishedVersionspa


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Está bajo una licencia Creative Commons Atribución 4.0 Internacional (CC BY 4.0).
Except where otherwise noted, this item's license is described as Está bajo una licencia Creative Commons Atribución 4.0 Internacional (CC BY 4.0).