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Numerical study of the turbulent flow around the stern of ship models

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dc.contributor.author Tzabiras, GD en
dc.date.accessioned 2014-03-01T01:08:13Z
dc.date.available 2014-03-01T01:08:13Z
dc.date.issued 1991 en
dc.identifier.issn 0271-2091 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/10345
dc.relation.uri http://www.scopus.com/inward/record.url?eid=2-s2.0-0026254470&partnerID=40&md5=e3f7d7dd0cc54064d6a5d21675b4e4b3 en
dc.subject REYNOLDS EQUATIONS en
dc.subject FINITE VOLUME METHODS en
dc.subject STERN FLOWS en
dc.subject TURBULENCE MODELING en
dc.subject.classification Computer Science, Interdisciplinary Applications en
dc.subject.classification Mathematics, Interdisciplinary Applications en
dc.subject.classification Mechanics en
dc.subject.classification Physics, Fluids & Plasmas en
dc.subject.other Fluid Dynamics--Mathematical Models en
dc.subject.other Mathematical Techniques--Approximation Theory en
dc.subject.other Mathematical Techniques--Numerical Methods en
dc.subject.other Ship Models en
dc.subject.other Finite Volume Approximations en
dc.subject.other Reynolds Equations en
dc.subject.other Stern Flows en
dc.subject.other Flow Of Fluids en
dc.subject.other Models en
dc.subject.other Turbulent Flow en
dc.subject.other Vessels en
dc.title Numerical study of the turbulent flow around the stern of ship models en
heal.type journalArticle en
heal.language English en
heal.publicationDate 1991 en
heal.abstract The present work is concerned with the numerical calculation of the turbulent flow field around the stern of ship models. The finite volume approximation is employed to solve the Reynolds equations in the physical domain using a body-fitted, locally orthogonal curvilinear co-ordinate system. The Reynolds stresses are modelled according to the standard k-epsilon turbulence model. Various numerical schemes (i.e. hybrid, skew upwind and central differencing) are examined and grid dependence tests have been performed to compare calculated with experimental results. Moreover, a direct solution of the momentum equations within the near-wall region is tried to avoid the disadvantages of the wall function approach. Comparisons between calculations and measurements are made for two ship models, i.e. the SSPA and HSVA model. en
heal.publisher JOHN WILEY & SONS LTD en
heal.journalName International Journal for Numerical Methods in Fluids en
dc.identifier.isi ISI:A1991GQ68100007 en
dc.identifier.volume 13 en
dc.identifier.issue 9 en
dc.identifier.spage 1179 en
dc.identifier.epage 1204 en


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