Natural convection in nanofluid-filled quadrantal cavities under magnetic field: Application of the SUPS formulation

dc.contributor.authorCengizci, Suleyman
dc.contributor.authorÖztop, Hakan Fehmi
dc.contributor.authorMulayim, Gulden
dc.date.accessioned2026-08-12T18:10:43Z
dc.date.issued2025
dc.departmentFırat Üniversitesi
dc.description.abstractA computational investigation of magnetohydrodynamic natural convection heat transfer phenomena, which find applications from energy conversation systems to lab-on-a-chip technologies, in nanofluid-filled quarter-circle-shaped (quadrantal) cavities with various temperature boundary conditions is presented. Toward that end, using the Boussinesq approximation for density, the Navier-Stokes equations of incompressible flows are coupled with the heat equation, and magnetic source terms are also incorporated into the governing equations. In computations, pure water serves as the base fluid; Cu (copper) or Al2O3 (alumina) serve as the nanoparticles, and it is assumed that the nanofluids are homogeneous. It is well known that when simulating incompressible flows within the classical framework of the Galerkin finite element method (GFEM), inappropriate choice of interpolation functions leads to nonphysical oscillations in the flow field, particularly for high Rayleigh numbers. In order to get around such numerical instabilities, the streamline-upwind/Petrov-Galerkin (SUPG) and pressure-stabilizing/Petrov-Galerkin (PSPG) stabilization terms are incorporated into the GFEM formulation. Numerical simulations are performed for various values of Rayleigh (Ra) and Hartman (Ha) numbers, ranging between 103 <= Ra <= 106 and 0 <= Ha <= 100. The proposed formulation and techniques work quite well even at high Rayleigh numbers, according to numerical simulations and comparisons with reported findings. Furthermore, it is demonstrated that the proposed formulation yields no significant numerical instabilities either locally or globally and that this is achieved only by using linear and equal-order interpolation functions, hence eliminating the requirement for adaptive mesh strategies and saving computing time considerably.
dc.description.sponsorshipThe authors express their gratitude to the anonymous reviewers for contributing their time and effort to improve the article's quality.
dc.identifier.doi10.1080/10407790.2024.2370515
dc.identifier.endpage3975
dc.identifier.issn1040-7790
dc.identifier.issn1521-0626
dc.identifier.issue11
dc.identifier.orcid0000-0002-4345-1253
dc.identifier.orcid0000-0001-8952-7658
dc.identifier.scopus2-s2.0-85197295742
dc.identifier.scopusqualityQ2
dc.identifier.startpage3953
dc.identifier.urihttps://doi.org/10.1080/10407790.2024.2370515
dc.identifier.urihttps://hdl.handle.net/11508/63404
dc.identifier.volume86
dc.identifier.wosWOS:001260207200001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherTaylor & Francis Inc
dc.relation.ispartofNumerical Heat Transfer Part B-Fundamentals
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260511
dc.subjectFinite elements
dc.subjectheat transfer
dc.subjectMHD natural convection
dc.subjectnanofluid
dc.subjectSUPS
dc.titleNatural convection in nanofluid-filled quadrantal cavities under magnetic field: Application of the SUPS formulation
dc.typeArticle

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