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International Journal of Fluid Mechanics Research

Publicou 6 edições por ano

ISSN Imprimir: 2152-5102

ISSN On-line: 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

Thermal Radiation of an Optically Thick Gray Gas in the Presence of Indirect Natural Convection

Volume 34, Edição 6, 2007, pp. 515-520
DOI: 10.1615/InterJFluidMechRes.v34.i6.30
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RESUMO

The effects of thermal radiation of a viscous incompressible fluid occupying a semi-infinite region of space bounded by an infinite horizontal moving hot plate in the presence of indirect natural convection by way of an induced pressure gradient, is considered. The fluid is a gray, absorbing-emitting radiation but a non-scattering medium. An exact solution is obtained for the flow by applying Laplace transform technique. The numerical results of velocity distributions are depicted graphically for different values of radiation parameter K1 and Grashof number Gr, taking the Prandtl number Pr = 0.71 and t = 0.2 are kept fixed. It is observed that the velocity slightly decreases with increasing the value of radiation parameter while the velocity is slightly decreases with increase in Gr whereas there exists a reverse flow on increasing Gr due to the presence of induced pressure gradient.

CITADO POR
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  2. Ahmed Sahin, Kalita Karabi, Magnetohydrodynamic transient flow through a porous medium bounded by a hot vertical plate in the presence of radiation: a theoretical analysis, Journal of Engineering Physics and Thermophysics, 86, 1, 2013. Crossref

  3. Ahmed Sahin, Batin Abdul, J. Chamkha Ali, Finite difference approach in porous media transport modeling for magnetohydrodynamic unsteady flow over a vertical plate , International Journal of Numerical Methods for Heat & Fluid Flow, 24, 5, 2014. Crossref

  4. Naroua Harouna, Modeling of unsteady MHD free convection flow with radiative heat transfer in a rotating fluid, Natural Science, 02, 12, 2010. Crossref

  5. Jana Rabindra Nath, Ghosh Swapan Kumar, Radiative Heat Transfer of an Optically Thick Gray Gas in The Presence of Indirect Natural Convection, World Journal of Mechanics, 01, 02, 2011. Crossref

  6. Bibi Sk. Nuslin, Padma G., Chemical reaction and soret, Dufour effect on radiation-convection flow with porous medium, INTERNATIONAL CONFERENCE ON MULTIFUNCTIONAL MATERIALS (ICMM-2019), 2269, 2020. Crossref

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