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    Convective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental Results

    Source: Journal of Solar Energy Engineering:;1983:;volume( 105 ):;issue: 001::page 29
    Author:
    A. M. Clausing
    DOI: 10.1115/1.3266342
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: Cavity solar receivers are generally believed to have higher thermal efficiencies than external receivers due to reduced losses. A simple analytical model was presented by the author which indicated that the ability to heat the air inside the cavity often controls the convective loss from cavity receivers. Thus, if the receiver contains a large amount of inactive hot wall area, it can experience a large convective loss. Excellent experimental data from a variety of cavity configurations and orientations have recently become available. These data provided a means of testing and refining the analytical model. In this manuscript, a brief description of the refined model is presented. Emphasis is placed on using available experimental evidence to substantiate the hypothesized mechanisms and assumptions. Detailed comparisons are given between analytical predictions and experimental results. Excellent agreement is obtained, and the important mechanisms are more clearly delineated.
    keyword(s): Solar energy , Cavities , Mechanisms , Testing AND Heat ,
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      Convective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental Results

    URI
    https://yetl.yabesh.ir/yetl1/handle/yetl/97642
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    contributor authorA. M. Clausing
    date accessioned2017-05-08T23:16:29Z
    date available2017-05-08T23:16:29Z
    date copyrightFebruary, 1983
    date issued1983
    identifier issn0199-6231
    identifier otherJSEEDO-28156#29_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/97642
    description abstractCavity solar receivers are generally believed to have higher thermal efficiencies than external receivers due to reduced losses. A simple analytical model was presented by the author which indicated that the ability to heat the air inside the cavity often controls the convective loss from cavity receivers. Thus, if the receiver contains a large amount of inactive hot wall area, it can experience a large convective loss. Excellent experimental data from a variety of cavity configurations and orientations have recently become available. These data provided a means of testing and refining the analytical model. In this manuscript, a brief description of the refined model is presented. Emphasis is placed on using available experimental evidence to substantiate the hypothesized mechanisms and assumptions. Detailed comparisons are given between analytical predictions and experimental results. Excellent agreement is obtained, and the important mechanisms are more clearly delineated.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleConvective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental Results
    typeJournal Paper
    journal volume105
    journal issue1
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.3266342
    journal fristpage29
    journal lastpage33
    identifier eissn1528-8986
    keywordsSolar energy
    keywordsCavities
    keywordsMechanisms
    keywordsTesting AND Heat
    treeJournal of Solar Energy Engineering:;1983:;volume( 105 ):;issue: 001
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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