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    Influence of Aperture Height and Width on Interzonal Natural Convection in a Full-Scale Air-Filled Enclosure

    Source: Journal of Solar Energy Engineering:;1989:;volume( 111 ):;issue: 004::page 278
    Author:
    Charles R. Boardman
    ,
    Ren Anderson
    ,
    Allan Kirkpatrick
    DOI: 10.1115/1.3268322
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: The topic of this paper is the influence of aperture height and width on interzonal high Rayleigh number, natural convection heat transfer. Experiments were conducted in an 8 ft. air-filled cube divided into two zones by a vertical partition which was centered between a constant flux hot wall and an isothermal cold wall. The partition was configured to form doorway-like apertures. The aperture height relative to test cell height range from 1/8 to 1 and the aperture width relative to test cell width ranged from 0.009 to 1. The zone-to-zone temperature difference and the overall Nusselt number were determined experimentally, and correlated with the overall Rayleigh number, aperture, and enclosure geometry, using a series resistance model for the enclosure. A turbulent boundary layer resistance was used to represent the hot and cold boundary layer flow, while an orifice resistance was used to represent the aperture flow. For flux Rayleigh numbers between 5*1011 and 5*1012 , the enclosure Nusselt numbers ranged between 15 and 165, with a strong dependence on aperture height.
    keyword(s): Natural convection , Rayleigh number , Electrical resistance , Interior walls , Flow (Dynamics) , Temperature , Heat transfer , Boundary layers , Boundary layer turbulence AND Geometry ,
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      Influence of Aperture Height and Width on Interzonal Natural Convection in a Full-Scale Air-Filled Enclosure

    URI
    https://yetl.yabesh.ir/yetl1/handle/yetl/105925
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    • Journal of Solar Energy Engineering

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    contributor authorCharles R. Boardman
    contributor authorRen Anderson
    contributor authorAllan Kirkpatrick
    date accessioned2017-05-08T23:30:56Z
    date available2017-05-08T23:30:56Z
    date copyrightNovember, 1989
    date issued1989
    identifier issn0199-6231
    identifier otherJSEEDO-28217#278_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/105925
    description abstractThe topic of this paper is the influence of aperture height and width on interzonal high Rayleigh number, natural convection heat transfer. Experiments were conducted in an 8 ft. air-filled cube divided into two zones by a vertical partition which was centered between a constant flux hot wall and an isothermal cold wall. The partition was configured to form doorway-like apertures. The aperture height relative to test cell height range from 1/8 to 1 and the aperture width relative to test cell width ranged from 0.009 to 1. The zone-to-zone temperature difference and the overall Nusselt number were determined experimentally, and correlated with the overall Rayleigh number, aperture, and enclosure geometry, using a series resistance model for the enclosure. A turbulent boundary layer resistance was used to represent the hot and cold boundary layer flow, while an orifice resistance was used to represent the aperture flow. For flux Rayleigh numbers between 5*1011 and 5*1012 , the enclosure Nusselt numbers ranged between 15 and 165, with a strong dependence on aperture height.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleInfluence of Aperture Height and Width on Interzonal Natural Convection in a Full-Scale Air-Filled Enclosure
    typeJournal Paper
    journal volume111
    journal issue4
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.3268322
    journal fristpage278
    journal lastpage285
    identifier eissn1528-8986
    keywordsNatural convection
    keywordsRayleigh number
    keywordsElectrical resistance
    keywordsInterior walls
    keywordsFlow (Dynamics)
    keywordsTemperature
    keywordsHeat transfer
    keywordsBoundary layers
    keywordsBoundary layer turbulence AND Geometry
    treeJournal of Solar Energy Engineering:;1989:;volume( 111 ):;issue: 004
    contenttypeFulltext
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