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    The Mixing of Mass and Momentum by Kelvin-Helmboltz Billows

    Source: Journal of the Atmospheric Sciences:;1995:;Volume( 052 ):;issue: 014::page 2509
    Author:
    Scinocca, J. F.
    DOI: 10.1175/1520-0469(1995)052<2509:TMOMAM>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The mixing of mass and momentum induced by the full life cycle of stratified shear instability is considered. In particular, the nonlinear numerical simulation of a stratified shear layer that is unstable to Kelvin?Helmholtz (K?H) waves is undertaken in three spatial dimensions. The numerical experiments are designed to model the secondary convective instability of the K?H billow previously indicated by linear stability analyses and identified in tilted-tank experiments. The initial parallel flows considered in the present study allow for the presence of constant stratification external to the shear layer. For weakly unstable stratified shear layers good agreement is found between the numerical simulations and similar physical (tilted tank) experiments. For strongly unstable stratified shear layers there is less agreement since the final state of the numerical simulations is a long-lived, two-dimensional vortex associated with the primary K?H instability. Quantitative estimates of the efficiency of mixing are made by calculating the flux Richardson number of the modeled mixing events. It is found that the flux Richardson number can strongly depend on the relative strength of the stratification external to the shear layer.
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      The Mixing of Mass and Momentum by Kelvin-Helmboltz Billows

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    contributor authorScinocca, J. F.
    date accessioned2017-06-09T14:33:13Z
    date available2017-06-09T14:33:13Z
    date copyright1995/07/01
    date issued1995
    identifier issn0022-4928
    identifier otherams-21523.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4157872
    description abstractThe mixing of mass and momentum induced by the full life cycle of stratified shear instability is considered. In particular, the nonlinear numerical simulation of a stratified shear layer that is unstable to Kelvin?Helmholtz (K?H) waves is undertaken in three spatial dimensions. The numerical experiments are designed to model the secondary convective instability of the K?H billow previously indicated by linear stability analyses and identified in tilted-tank experiments. The initial parallel flows considered in the present study allow for the presence of constant stratification external to the shear layer. For weakly unstable stratified shear layers good agreement is found between the numerical simulations and similar physical (tilted tank) experiments. For strongly unstable stratified shear layers there is less agreement since the final state of the numerical simulations is a long-lived, two-dimensional vortex associated with the primary K?H instability. Quantitative estimates of the efficiency of mixing are made by calculating the flux Richardson number of the modeled mixing events. It is found that the flux Richardson number can strongly depend on the relative strength of the stratification external to the shear layer.
    publisherAmerican Meteorological Society
    titleThe Mixing of Mass and Momentum by Kelvin-Helmboltz Billows
    typeJournal Paper
    journal volume52
    journal issue14
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1995)052<2509:TMOMAM>2.0.CO;2
    journal fristpage2509
    journal lastpage2530
    treeJournal of the Atmospheric Sciences:;1995:;Volume( 052 ):;issue: 014
    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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