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    Free Convection in a Wavy Walled Cavity With a Magnetic Source Using Radial Basis Functions

    Source: Journal of Heat Transfer:;2019:;volume( 141 ):;issue: 004::page 42501
    Author:
    Pekmen Geridonmez, Bengisen
    DOI: 10.1115/1.4042782
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: In this study, free convection in a cavity with differentially heated wavy walls is numerically investigated in the presence of a magnetic source. Polyharmonic spline radial basis function (RBF) is utilized to discretize the governing dimensionless equations formulated by stream function-vorticity. The effects of dimensionless Hartmann number, Rayleigh number, the number of undulations, amplitude of wave, and the location of magnetic source are visualized in streamlines and isotherms as well as calculating average Nusselt number through the heated wall. Results show that primary vortex in streamlines is altered with the impact of magnetic source. The augmentation of undulations and amplitude causes convective heat transfer to decrease if Ra = 105. The impact of location of magnetic source is noted close to the top wall.
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      Free Convection in a Wavy Walled Cavity With a Magnetic Source Using Radial Basis Functions

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    contributor authorPekmen Geridonmez, Bengisen
    date accessioned2019-03-17T10:11:47Z
    date available2019-03-17T10:11:47Z
    date copyright2/25/2019 12:00:00 AM
    date issued2019
    identifier issn0022-1481
    identifier otherht_141_04_042501.pdf
    identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4255985
    description abstractIn this study, free convection in a cavity with differentially heated wavy walls is numerically investigated in the presence of a magnetic source. Polyharmonic spline radial basis function (RBF) is utilized to discretize the governing dimensionless equations formulated by stream function-vorticity. The effects of dimensionless Hartmann number, Rayleigh number, the number of undulations, amplitude of wave, and the location of magnetic source are visualized in streamlines and isotherms as well as calculating average Nusselt number through the heated wall. Results show that primary vortex in streamlines is altered with the impact of magnetic source. The augmentation of undulations and amplitude causes convective heat transfer to decrease if Ra = 105. The impact of location of magnetic source is noted close to the top wall.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleFree Convection in a Wavy Walled Cavity With a Magnetic Source Using Radial Basis Functions
    typeJournal Paper
    journal volume141
    journal issue4
    journal titleJournal of Heat Transfer
    identifier doi10.1115/1.4042782
    journal fristpage42501
    journal lastpage042501-9
    treeJournal of Heat Transfer:;2019:;volume( 141 ):;issue: 004
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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