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    Optimization of Flow Passage Geometry for Air-Heating, Plate-Type Solar Collectors

    Source: Journal of Solar Energy Engineering:;1981:;volume( 103 ):;issue: 004::page 323
    Author:
    K. G. T. Hollands
    ,
    E. C. Shewen
    DOI: 10.1115/1.3266260
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: The effect of the choice of shape and dimensions of the air flow passages in plate-type, air-heating solar collectors is assessed. Particularly examined is their effect on the overall heat transfer coefficient Upf between the air stream and the plate, which has an important effect on collector efficiency. It is emphasized in this study that in comparing various designs of flow passage, they should be compared for the same pressure drop Δp suffered by the air in passing through the collector, and for the same mass flow rate m per unit of collector area. On the basis of this type of comparison, two main conclusions are drawn. First, when the length of the air flow passage L is made less than about 1 m, Upf increases dramatically with decreasing values of L. Second, outside the transition regime, the value of Upf for a V-corrugated absorber plate is from 47 to 300 percent higher than that for a flat absorber plate, depending on whether the flow is laminar or turbulent, and on whether the V-corrugated plate is thermally bonded to the back plate. The first conclusion has led to a proposal for a novel air-heating solar collector design, called the “short-path” design.
    keyword(s): Flow (Dynamics) , Optimization , Solar collectors , Geometry , Heating , Air flow , Design , Turbulence , Dimensions , Pressure drop , Shapes AND Heat transfer coefficients ,
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      Optimization of Flow Passage Geometry for Air-Heating, Plate-Type Solar Collectors

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    http://yetl.yabesh.ir/yetl1/handle/yetl/95080
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    contributor authorK. G. T. Hollands
    contributor authorE. C. Shewen
    date accessioned2017-05-08T23:12:00Z
    date available2017-05-08T23:12:00Z
    date copyrightNovember, 1981
    date issued1981
    identifier issn0199-6231
    identifier otherJSEEDO-28145#323_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/95080
    description abstractThe effect of the choice of shape and dimensions of the air flow passages in plate-type, air-heating solar collectors is assessed. Particularly examined is their effect on the overall heat transfer coefficient Upf between the air stream and the plate, which has an important effect on collector efficiency. It is emphasized in this study that in comparing various designs of flow passage, they should be compared for the same pressure drop Δp suffered by the air in passing through the collector, and for the same mass flow rate m per unit of collector area. On the basis of this type of comparison, two main conclusions are drawn. First, when the length of the air flow passage L is made less than about 1 m, Upf increases dramatically with decreasing values of L. Second, outside the transition regime, the value of Upf for a V-corrugated absorber plate is from 47 to 300 percent higher than that for a flat absorber plate, depending on whether the flow is laminar or turbulent, and on whether the V-corrugated plate is thermally bonded to the back plate. The first conclusion has led to a proposal for a novel air-heating solar collector design, called the “short-path” design.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleOptimization of Flow Passage Geometry for Air-Heating, Plate-Type Solar Collectors
    typeJournal Paper
    journal volume103
    journal issue4
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.3266260
    journal fristpage323
    journal lastpage330
    identifier eissn1528-8986
    keywordsFlow (Dynamics)
    keywordsOptimization
    keywordsSolar collectors
    keywordsGeometry
    keywordsHeating
    keywordsAir flow
    keywordsDesign
    keywordsTurbulence
    keywordsDimensions
    keywordsPressure drop
    keywordsShapes AND Heat transfer coefficients
    treeJournal of Solar Energy Engineering:;1981:;volume( 103 ):;issue: 004
    contenttypeFulltext
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