Computational manipulation of a radiative MHD flow with Hall current and chemical reaction in the presence of rotating fluid
A numerical analysis of transient radiative MHD(MagnetoHydroDynamic) natural convective flow of a viscous, incompressible, electrically conducting and rotating fluid along a semi-infinite isothermal vertical plate is carried out taking into consideration Hall current, rotation and first order chemic...
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Veröffentlicht in: | Journal of physics. Conference series 2018-04, Vol.1000 (1), p.12144 |
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description | A numerical analysis of transient radiative MHD(MagnetoHydroDynamic) natural convective flow of a viscous, incompressible, electrically conducting and rotating fluid along a semi-infinite isothermal vertical plate is carried out taking into consideration Hall current, rotation and first order chemical reaction.The coupled non-linear partial differential equations are expressed in difference form using implicit finite difference scheme. The difference equations are then reduced to a system of linear algebraic equations with a tri-diagonal structure which is solved by Thomas Algorithm. The primary and secondary velocity profiles, temperature profile, concentration profile, skin friction, Nusselt number and Sherwood Number are depicted graphically for a range of values of rotation parameter, Hall parameter,magnetic parameter, chemical reaction parameter, radiation parameter, Prandtl number and Schmidt number.It is recognized that rate of heat transfer and rate of mass transfer decrease with increase in time but they increase with increasing values of radiation parameter and Schmidt number respectively. |
doi_str_mv | 10.1088/1742-6596/1000/1/012144 |
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The difference equations are then reduced to a system of linear algebraic equations with a tri-diagonal structure which is solved by Thomas Algorithm. The primary and secondary velocity profiles, temperature profile, concentration profile, skin friction, Nusselt number and Sherwood Number are depicted graphically for a range of values of rotation parameter, Hall parameter,magnetic parameter, chemical reaction parameter, radiation parameter, Prandtl number and Schmidt number.It is recognized that rate of heat transfer and rate of mass transfer decrease with increase in time but they increase with increasing values of radiation parameter and Schmidt number respectively.</description><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/1000/1/012144</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Algorithms ; Chemical reactions ; Convective flow ; Difference equations ; Finite difference method ; first-order chemical reaction ; Fluid flow ; Hall effect ; Incompressible flow ; Linear algebra ; Magnetic properties ; Magnetohydrodynamics ; Mass transfer ; MHD ; Nonlinear differential equations ; Numerical analysis ; Parameters ; Partial differential equations ; Physics ; Prandtl number ; Radiation ; Rotating fluids ; rotation ; Schmidt number ; Skin friction ; Temperature profiles ; Velocity distribution</subject><ispartof>Journal of physics. Conference series, 2018-04, Vol.1000 (1), p.12144</ispartof><rights>Published under licence by IOP Publishing Ltd</rights><rights>2018. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c378t-8df47fb9e7b2c1f1e0b6705b445cd3a42ef7177fb89d306c799d66b96784cfdc3</citedby><cites>FETCH-LOGICAL-c378t-8df47fb9e7b2c1f1e0b6705b445cd3a42ef7177fb89d306c799d66b96784cfdc3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1742-6596/1000/1/012144/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,780,784,27924,27925,38868,38890,53840,53867</link.rule.ids></links><search><creatorcontrib>Suba, Subbu Alias</creatorcontrib><creatorcontrib>Muthucumaraswamy, R</creatorcontrib><title>Computational manipulation of a radiative MHD flow with Hall current and chemical reaction in the presence of rotating fluid</title><title>Journal of physics. Conference series</title><addtitle>J. Phys.: Conf. Ser</addtitle><description>A numerical analysis of transient radiative MHD(MagnetoHydroDynamic) natural convective flow of a viscous, incompressible, electrically conducting and rotating fluid along a semi-infinite isothermal vertical plate is carried out taking into consideration Hall current, rotation and first order chemical reaction.The coupled non-linear partial differential equations are expressed in difference form using implicit finite difference scheme. The difference equations are then reduced to a system of linear algebraic equations with a tri-diagonal structure which is solved by Thomas Algorithm. The primary and secondary velocity profiles, temperature profile, concentration profile, skin friction, Nusselt number and Sherwood Number are depicted graphically for a range of values of rotation parameter, Hall parameter,magnetic parameter, chemical reaction parameter, radiation parameter, Prandtl number and Schmidt number.It is recognized that rate of heat transfer and rate of mass transfer decrease with increase in time but they increase with increasing values of radiation parameter and Schmidt number respectively.</description><subject>Algorithms</subject><subject>Chemical reactions</subject><subject>Convective flow</subject><subject>Difference equations</subject><subject>Finite difference method</subject><subject>first-order chemical reaction</subject><subject>Fluid flow</subject><subject>Hall effect</subject><subject>Incompressible flow</subject><subject>Linear algebra</subject><subject>Magnetic properties</subject><subject>Magnetohydrodynamics</subject><subject>Mass transfer</subject><subject>MHD</subject><subject>Nonlinear differential equations</subject><subject>Numerical analysis</subject><subject>Parameters</subject><subject>Partial differential equations</subject><subject>Physics</subject><subject>Prandtl number</subject><subject>Radiation</subject><subject>Rotating fluids</subject><subject>rotation</subject><subject>Schmidt number</subject><subject>Skin friction</subject><subject>Temperature profiles</subject><subject>Velocity distribution</subject><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqFkMtOxCAYRonRxHH0GSRxXQstBbo042VMxrjRNaFcHCZtqbTVmPjw0qkZl7KBP3zfIRwALjG6xojzFDOSJbQoaYoRQilOEc4wIUdgcbg5Ppw5PwVnfb9DKI-LLcD3yjfdOMjB-VbWsJGt68Z6P0JvoYRBahfHDwOf1rfQ1v4TfrphC9eyrqEaQzDtAGWrodqaxqnICEaqfd-1cNga2AXTm1aZiRf89FT7FkGj0-fgxMq6Nxe_-xK83t-9rNbJ5vnhcXWzSVTO-JBwbQmzVWlYlSlssUEVZaioCCmUziXJjGWYxQQvdY6oYmWpKa1KyjhRVqt8Ca5mbhf8-2j6Qez8GOJ_e5EVLMM0IyWNKTanVPB9H4wVXXCNDF8CIzGpFpNEMQkVk2qBxaw6NvO56Xz3h_6v9QOfZoIr</recordid><startdate>20180401</startdate><enddate>20180401</enddate><creator>Suba, Subbu Alias</creator><creator>Muthucumaraswamy, R</creator><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope></search><sort><creationdate>20180401</creationdate><title>Computational manipulation of a radiative MHD flow with Hall current and chemical reaction in the presence of rotating fluid</title><author>Suba, Subbu Alias ; 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The primary and secondary velocity profiles, temperature profile, concentration profile, skin friction, Nusselt number and Sherwood Number are depicted graphically for a range of values of rotation parameter, Hall parameter,magnetic parameter, chemical reaction parameter, radiation parameter, Prandtl number and Schmidt number.It is recognized that rate of heat transfer and rate of mass transfer decrease with increase in time but they increase with increasing values of radiation parameter and Schmidt number respectively.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/1000/1/012144</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Algorithms Chemical reactions Convective flow Difference equations Finite difference method first-order chemical reaction Fluid flow Hall effect Incompressible flow Linear algebra Magnetic properties Magnetohydrodynamics Mass transfer MHD Nonlinear differential equations Numerical analysis Parameters Partial differential equations Physics Prandtl number Radiation Rotating fluids rotation Schmidt number Skin friction Temperature profiles Velocity distribution |
title | Computational manipulation of a radiative MHD flow with Hall current and chemical reaction in the presence of rotating fluid |
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