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    Rotating Compressible Flow Over the Edge of a Finite Disk

    Source: Journal of Applied Mechanics:;1981:;volume( 048 ):;issue: 002::page 249
    Author:
    M. Toren
    ,
    A. Solan
    DOI: 10.1115/1.3157605
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: Numerical and asymptotic solutions of the similarity equations governing the laminar compressible rotating flow near the edge of a finite disk are presented for a wide range of the Prandtl and Eckert numbers and the disk-to-external flow ratios of azimuthal velocity and temperature. By appropriate transformations, the compressible flow is reduced to a formulation similar to that of the incompressible flow. Wall heating and dissipation effects are shown to be equivalent to an increment of the velocity of the disk in the sense opposite to that of the outer flow. In the limit of small velocity or temperature difference between the disk and the outer flow, the solutions show how an Ekman layer is started at the edge.
    keyword(s): Disks , Compressible flow , Flow (Dynamics) , Temperature , Energy dissipation , Ekman dynamics , Equations AND Heating ,
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      Rotating Compressible Flow Over the Edge of a Finite Disk

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/94151
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    contributor authorM. Toren
    contributor authorA. Solan
    date accessioned2017-05-08T23:10:22Z
    date available2017-05-08T23:10:22Z
    date copyrightJune, 1981
    date issued1981
    identifier issn0021-8936
    identifier otherJAMCAV-26177#249_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/94151
    description abstractNumerical and asymptotic solutions of the similarity equations governing the laminar compressible rotating flow near the edge of a finite disk are presented for a wide range of the Prandtl and Eckert numbers and the disk-to-external flow ratios of azimuthal velocity and temperature. By appropriate transformations, the compressible flow is reduced to a formulation similar to that of the incompressible flow. Wall heating and dissipation effects are shown to be equivalent to an increment of the velocity of the disk in the sense opposite to that of the outer flow. In the limit of small velocity or temperature difference between the disk and the outer flow, the solutions show how an Ekman layer is started at the edge.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleRotating Compressible Flow Over the Edge of a Finite Disk
    typeJournal Paper
    journal volume48
    journal issue2
    journal titleJournal of Applied Mechanics
    identifier doi10.1115/1.3157605
    journal fristpage249
    journal lastpage254
    identifier eissn1528-9036
    keywordsDisks
    keywordsCompressible flow
    keywordsFlow (Dynamics)
    keywordsTemperature
    keywordsEnergy dissipation
    keywordsEkman dynamics
    keywordsEquations AND Heating
    treeJournal of Applied Mechanics:;1981:;volume( 048 ):;issue: 002
    contenttypeFulltext
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