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International Journal of Fluid Mechanics Research

Publication de 6  numéros par an

ISSN Imprimer: 2152-5102

ISSN En ligne: 2152-5110

The Impact Factor measures the average number of citations received in a particular year by papers published in the journal during the two preceding years. 2017 Journal Citation Reports (Clarivate Analytics, 2018) IF: 1.1 To calculate the five year Impact Factor, citations are counted in 2017 to the previous five years and divided by the source items published in the previous five years. 2017 Journal Citation Reports (Clarivate Analytics, 2018) 5-Year IF: 1.3 The Eigenfactor score, developed by Jevin West and Carl Bergstrom at the University of Washington, is a rating of the total importance of a scientific journal. Journals are rated according to the number of incoming citations, with citations from highly ranked journals weighted to make a larger contribution to the eigenfactor than those from poorly ranked journals. Eigenfactor: 0.0002 The Journal Citation Indicator (JCI) is a single measurement of the field-normalized citation impact of journals in the Web of Science Core Collection across disciplines. The key words here are that the metric is normalized and cross-disciplinary. JCI: 0.33 SJR: 0.256 SNIP: 0.49 CiteScore™:: 2.4 H-Index: 23

Indexed in

Numerical Simulation of Forced Convection Heat Transfer from an Ellipsoid of Revolution, Using a Fourier Spectral Method

Volume 25, Numéro 1-3, 1998, pp. 31-40
DOI: 10.1615/InterJFluidMechRes.v25.i1-3.30
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RÉSUMÉ

Forced convection heat transfer from an ellipsoid of revolution is analyzed numerically. By assuming fluid properties to be constant, and introducing boundary-fitted conformal mapping coordinate system (in the plane), the energy equation can be decpomposed into Fourier components in one space coordinate using a form of Fourier series for temperature and a function relating to an axially symmetric stream function in the same space coordinate; the decomposed equation can be discretized in another spatial coordinate, using substantially doubly-exponential grid spacing, to get relatively accurate thermal field and a mean Nusselt number even at a relatively high Reynolds number flow past a body of revolution (from a thin prolate spheroid to an oblate spheroid.)

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