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    The Structure, Energetics and Propagation of Rotating Convective Storms. Part II: Helicity and Storm Stabilization

    Source: Journal of the Atmospheric Sciences:;1986:;Volume( 043 ):;issue: 002::page 126
    Author:
    Lilly, Douglas K.
    DOI: 10.1175/1520-0469(1986)043<0126:TSEAPO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Rotating ?supercell? thunderstorms are shown to be characterized by high helicity, the vector inner product of velocity and vorticity, which is obtained both from the mean flow in which they are embedded and from buoyancy enrichment. Some unique properties of supercell helical flow are described, including a tendency for trajectory rotation to be reversed from parcel vorticity. A simple helical (Beltrami) flow model resembles gross supercell structure and also provides a prediction of storm motion. Since theory, closure model calculations and numerical simulations indicate that helicity suppresses turbulent dissipation, it is suggested that supercells owe their noted stability and long life to this effect. Enhanced predictability of such storms is then expected and is apparently seen in some results of Wilhelmson and Klemp. It is concluded that rotating storm structure and propagation must involve a compromise between the energetic effects discussed by Lilly in Part I of this study and those considered here, but that the helicity effects seem to be dominant in long-lived storms.
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      The Structure, Energetics and Propagation of Rotating Convective Storms. Part II: Helicity and Storm Stabilization

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4155305
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    contributor authorLilly, Douglas K.
    date accessioned2017-06-09T14:26:10Z
    date available2017-06-09T14:26:10Z
    date copyright1986/01/01
    date issued1986
    identifier issn0022-4928
    identifier otherams-19213.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155305
    description abstractRotating ?supercell? thunderstorms are shown to be characterized by high helicity, the vector inner product of velocity and vorticity, which is obtained both from the mean flow in which they are embedded and from buoyancy enrichment. Some unique properties of supercell helical flow are described, including a tendency for trajectory rotation to be reversed from parcel vorticity. A simple helical (Beltrami) flow model resembles gross supercell structure and also provides a prediction of storm motion. Since theory, closure model calculations and numerical simulations indicate that helicity suppresses turbulent dissipation, it is suggested that supercells owe their noted stability and long life to this effect. Enhanced predictability of such storms is then expected and is apparently seen in some results of Wilhelmson and Klemp. It is concluded that rotating storm structure and propagation must involve a compromise between the energetic effects discussed by Lilly in Part I of this study and those considered here, but that the helicity effects seem to be dominant in long-lived storms.
    publisherAmerican Meteorological Society
    titleThe Structure, Energetics and Propagation of Rotating Convective Storms. Part II: Helicity and Storm Stabilization
    typeJournal Paper
    journal volume43
    journal issue2
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1986)043<0126:TSEAPO>2.0.CO;2
    journal fristpage126
    journal lastpage140
    treeJournal of the Atmospheric Sciences:;1986:;Volume( 043 ):;issue: 002
    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
    yabeshDSpacePersian