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    A Comparison of Turbulence Generated by 3DS Sparse Grids with Different Blockage Ratios and Different Co-frame Arrangements

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    Type
    Conference Paper
    Authors
    Usama, M. Syed
    Malik, Nadeem A.
    Date
    2021-08-30
    Online Publication Date
    2021-08-30
    Print Publication Date
    2021
    Permanent link to this record
    http://hdl.handle.net/10754/672160
    
    Metadata
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    Abstract
    A new type of grid turbulence generator, the 3D sparse grid (3DS), is a co-planar arrangement of co-frames each containing a different length scale of grid elements [Malik, N. A. US Patent No. US 9,599,269 B2 (2017)] and possessing a much bigger parameter space than the flat 2D fractal square grid (2DF). Using DNS we compare the characteristics of the turbulence (mean flow, turbulence intensity, energy spectrum) generated by different types of 3DS grids. The peak intensities generated by 3DS can exceed the peaks generated by the 2DF by 80%; we observe that a 3DS with blockage ratio 24% produces turbulence similar to the 2DF with blockage ratio 32% implying lower energy input for the same turbulence.
    Citation
    Usama, M. S., & Malik, N. A. (2021). A Comparison of Turbulence Generated by 3DS Sparse Grids with Different Blockage Ratios and Different Co-frame Arrangements. Recent Developments in Mathematical, Statistical and Computational Sciences, 325–334. doi:10.1007/978-3-030-63591-6_30
    Sponsors
    The authors acknowledge the support from King Abdullah University of Science and Technology (KAUST) for making available the High Performance Computing facility Shaheen 2 for this project.
    Publisher
    Springer International Publishing
    Conference/Event name
    International Conference on Applied Mathematics, Modeling and Computational Science, AMMCS 2019
    ISBN
    9783030635909
    DOI
    10.1007/978-3-030-63591-6_30
    arXiv
    2006.04713
    Additional Links
    https://link.springer.com/10.1007/978-3-030-63591-6_30
    ae974a485f413a2113503eed53cd6c53
    10.1007/978-3-030-63591-6_30
    Scopus Count
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