• Login
    View Item 
    •   DSpace Home
    • ASME
    • Journal of Solar Energy Engineering
    • View Item
    •   DSpace Home
    • ASME
    • Journal of Solar Energy Engineering
    • View Item
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    A Novel Approach for Computational Fluid Dynamics Analysis of Mean Wind Loads on Heliostats

    Thumbnail
    View/Open
    sol_144_6_061008.pdf (2.066Mb)
    Date
    2022
    Author
    Durán
    R.L.;Hinojosa
    J.F.;Sosa-Flores
    P.
    Metadata
    Show full item record
    Abstract
    A computational fluid dynamics study about the aerodynamic loads over a heliostat due to an atmospheric boundary layer flow using a modified k–ɛ turbulence model is presented. A new formulation is used, in which the model quantities vary with the velocity field. Modified wall functions for roughness were used at the bottom of the computational domain to achieve horizontal homogeneity of the airflow. Good horizontal homogeneity for the streamwise and spanwise velocity and turbulence intensity profiles were found. The incident profiles were compared with the inlet ones. The average percentage differences were 0.22% for velocity and 0.43% for turbulent intensity. Good agreement was found between the numerical data and theoretical values of the streamwise and spanwise shear stress at the bottom of the domain. The aerodynamic coefficients of the heliostat at different elevation angles were obtained, and a good agreement was found between the numerical data concerning the wind tunnel experimental values. An average percentage difference of 3.1% was found for drag, 6.5% for lift, and 6.0% for overturning. A significant improvement was obtained by using this new formulation with respect to a non-modified k–ɛ turbulence model. The average differences of the aerodynamic coefficients were 6.6% for drag, 12.4% for lift, and 10.1% for overturning. The velocity, turbulent kinetic energy, and pressure fields at different elevation angles were analyzed. It was found that at an elevation of 60 deg, the stagnation point of the flow occurs at the superior edge of the heliostat, causing the maximum lift force over the structure.
    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4287437
    Collections
    • Journal of Solar Energy Engineering

    DSpace software copyright © 2002-2015  DuraSpace
    Contact Us | Send Feedback
    Theme by 
    @mire NV
     

     

    Browse

    All of DSpaceCommunities & CollectionsBy Issue DateAuthorsTitlesSubjectsThis CollectionBy Issue DateAuthorsTitlesSubjects

    My Account

    LoginRegister

    Statistics

    View Usage Statistics

    DSpace software copyright © 2002-2015  DuraSpace
    Contact Us | Send Feedback
    Theme by 
    @mire NV