Computational fluid dynamical analysis of turbulent flow in a channel equipped with double-pass solar air collector

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dc.contributor.authorSaim, Rachid
dc.contributor.authorAbderrahim, Asma
dc.contributor.authorÖztop, Hakan Fehmi
dc.contributor.authorAbbdoui, Said
dc.contributor.authorAl-Salem, Khaled
dc.date.accessioned2026-08-12T17:04:24Z
dc.date.issued2015
dc.departmentFırat Üniversitesi
dc.description.abstractA numerical analysis is proposed to predict the thermal and flow field for turbulent flow in a double-pass solar collector. The conservation equations are solved by using finite volume method. The k-omega-SST turbulence model is used. The influence of the mass flow rate of air, which changes in range of 0.0139 kg/s and 0.062 kg/s, is chosen as the main parameter. The results show that the flow characteristics strongly depend on massflow rate of air and the geometry of the double pass solar air collector.
dc.identifier.endpage76
dc.identifier.issn1468-4349
dc.identifier.issn1741-5233
dc.identifier.issue6
dc.identifier.scopus2-s2.0-84946819946
dc.identifier.scopusqualityQ4
dc.identifier.startpage70
dc.identifier.urihttps://hdl.handle.net/11508/48712
dc.identifier.volume15
dc.identifier.wosWOS:000365453300005
dc.identifier.wosqualityQ4
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherInderscience Enterprises Ltd
dc.relation.ispartofProgress in Computational Fluid Dynamics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260511
dc.subjectdouble pass solar air collector
dc.subjectforced convection
dc.subjectturbulent flow
dc.subjectnumeric
dc.titleComputational fluid dynamical analysis of turbulent flow in a channel equipped with double-pass solar air collector
dc.typeArticle

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