Numerical analyses of the concentrated solar receiver pipes with superheated steam

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dc.authoridKurt, Erol/0000-0002-3615-6926
dc.authoridDemirci, Mustafa/0000-0002-7050-8323
dc.contributor.authorKurt, Erol
dc.contributor.authorDemirci, Mustafa
dc.contributor.authorSahin, Haci M.
dc.date.accessioned2024-09-29T16:05:02Z
dc.date.available2024-09-29T16:05:02Z
dc.date.issued2022
dc.departmentKarabük Üniversitesien_US
dc.description.abstractIn this paper, numerical analyses on a concentrated solar receiver pipes have been performed. The fluid is considered to be superheated steam phase. The pressure drops and temperature distribution in the absorber tubes of the parabolic trough solar collector (PTSC) have been explored in detail. In the numerical studies, the experimental data received from the solar test facility located at the Plataforma Solar de Almeria, Spain has been used for the real world application in order to shed a light on the superheated phase of the plant. The RNG k-epsilon turbulence model is considered for the Computational Fluid Dynamics analyses. In the explorations, especially the fluid behavior at different mass flows has been taken into account. The process has been evaluated for different temperate T and pressure P cases such as Case 1: p = 3.21 MPa, T = 240.4 degrees C and Case 2: p = 10 MPa, T = 500 degrees C. According to the results, the numerical results have been in good agreement within the error rate of 0.79% for the experimental temperature measurements. Therefore, the proposed numerical technique can be generalized for different steam parameters of PTSC in order to estimate the steam characterization for the experimental facility.en_US
dc.description.sponsorshipEuropean Commission [228296]en_US
dc.description.sponsorshipThe authors would like to thank the European Commission for the financial support within the frame of Solar Facilities for the European Research Area (SFERA) project under the code of 228296 in CIEMAT-PSA Spain.en_US
dc.identifier.doi10.1177/09576509221074524
dc.identifier.endpage910en_US
dc.identifier.issn0957-6509
dc.identifier.issn2041-2967
dc.identifier.issue5en_US
dc.identifier.scopus2-s2.0-85125718027en_US
dc.identifier.scopusqualityQ2en_US
dc.identifier.startpage893en_US
dc.identifier.urihttps://doi.org/10.1177/09576509221074524
dc.identifier.urihttps://hdl.handle.net/20.500.14619/6473
dc.identifier.volume236en_US
dc.identifier.wosWOS:000764201500001en_US
dc.identifier.wosqualityQ3en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherSage Publications Ltden_US
dc.relation.ispartofProceedings of the Institution of Mechanical Engineers Part A-Journal of Power and Energyen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectComputational fluid dynamics modelingen_US
dc.subjectparabolic trough solar collectoren_US
dc.subjectfriction factoren_US
dc.subjecttemperature distributionen_US
dc.subjectpressure dropen_US
dc.titleNumerical analyses of the concentrated solar receiver pipes with superheated steamen_US
dc.typeArticleen_US

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