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dc.contributor.authorGurbuz, Merve
dc.contributor.authorTezer-Sezgin, M.
dc.date.accessioned2020-12-26T10:47:00Z
dc.date.available2020-12-26T10:47:00Z
dc.date.issued2019
dc.identifier.issn1683-3511en_US
dc.identifier.urihttp://hdl.handle.net/11727/5214
dc.description.abstractIn this study, the radial basis function (RBF) approximation is applied for solving the unsteady fluid flow and magnetohydrodynamic (MHD) convection flow problems with the use of explicit Euler time discretization and relaxation parameters to accelerate the convergence. The stability analysis is also carried out in terms of the spectral radius of related RBF discretized coefficient matrices. The optimal choices of the time increment, relaxation parameters and physical problem parameters are found for achieving stable solutions. It is observed that the maximum eigenvalues of the coefficient matrices decrease with an increase in the time increment when the relaxation parameters are decreasing. Although the time derivative is discretized using explicit Euler method, one does not need to use small time increment for obtaining stable results. The flow, isotherms and pressure behaviors are simulated at steady-state for several values of problem parameters using time increment and relaxation parameters which lead to stable solutions.en_US
dc.language.isoengen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectRadial Basis Functionen_US
dc.subjectStability Analysisen_US
dc.subjectNavier-Stokes Equationsen_US
dc.subjectMHD Convection Flowen_US
dc.titleNUMERICAL STABILITY OF RBF APPROXIMATION FOR UNSTEADY MHD FLOW EQUATIONSen_US
dc.typearticleen_US
dc.relation.journalAPPLIED AND COMPUTATIONAL MATHEMATICSen_US
dc.identifier.volume18en_US
dc.identifier.issue2en_US
dc.identifier.startpage123en_US
dc.identifier.endpage134en_US
dc.identifier.wos000472595900002en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergien_US


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