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    A Linear Stability Study of the Gradient Zone of a Solar Pond

    Source: Journal of Solar Energy Engineering:;2006:;volume( 128 ):;issue: 003::page 383
    Author:
    L. Kaffel Rebaï
    ,
    A. K. Mojtabi
    ,
    M. J. Safi
    ,
    A. A. Mohamad
    DOI: 10.1115/1.2210498
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: The linear stability of a plane layer with horizontal temperature and concentration stratification corresponding to gradient zone of a solar pond is investigated. The problem is described by Navier-Stokes equations with Boussinesq-Oberbeck approximation. Two source terms are introduced in the energy equations: the absorption of solar energy characterized by the extinction radiative coefficient μe and by the parameter f defined as the ratio of extracted heat flux to absorbed heat flux in the lower convective zone. The influence of the parameters μe and f on the onset of thermosolutal convection in the case of confined and infinite layers is analyzed. It is found that convection starts in an oscillatory state, independently of the RaS value. Different convection solutions were found for marginal stability and steady state.
    keyword(s): Stability , Temperature , Solar energy , Gradients , Steady state AND Convection ,
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      A Linear Stability Study of the Gradient Zone of a Solar Pond

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/134607
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    contributor authorL. Kaffel Rebaï
    contributor authorA. K. Mojtabi
    contributor authorM. J. Safi
    contributor authorA. A. Mohamad
    date accessioned2017-05-09T00:21:33Z
    date available2017-05-09T00:21:33Z
    date copyrightAugust, 2006
    date issued2006
    identifier issn0199-6231
    identifier otherJSEEDO-28397#383_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/134607
    description abstractThe linear stability of a plane layer with horizontal temperature and concentration stratification corresponding to gradient zone of a solar pond is investigated. The problem is described by Navier-Stokes equations with Boussinesq-Oberbeck approximation. Two source terms are introduced in the energy equations: the absorption of solar energy characterized by the extinction radiative coefficient μe and by the parameter f defined as the ratio of extracted heat flux to absorbed heat flux in the lower convective zone. The influence of the parameters μe and f on the onset of thermosolutal convection in the case of confined and infinite layers is analyzed. It is found that convection starts in an oscillatory state, independently of the RaS value. Different convection solutions were found for marginal stability and steady state.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleA Linear Stability Study of the Gradient Zone of a Solar Pond
    typeJournal Paper
    journal volume128
    journal issue3
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.2210498
    journal fristpage383
    journal lastpage393
    identifier eissn1528-8986
    keywordsStability
    keywordsTemperature
    keywordsSolar energy
    keywordsGradients
    keywordsSteady state AND Convection
    treeJournal of Solar Energy Engineering:;2006:;volume( 128 ):;issue: 003
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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