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    Inertial Instability of Nonparallel Flow on an Equatorial β Plane

    Source: Journal of the Atmospheric Sciences:;1993:;Volume( 050 ):;issue: 016::page 2744
    Author:
    Dunkerton, Timothy J.
    DOI: 10.1175/1520-0469(1993)050<2744:IIONFO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A simple theoretical model was developed to investigate the inertial instability of zonally nonuniform, non-parallel flow near the equator. The basic state was independent of height and time but included cross-equatorial shear with longitudinal variation, as observed in the tropical mesosphere and elsewhere. Numerical solutions were obtained for the most unstable modes. It is shown that, in addition to previously known ?global? (symmetric and nonsymmetric) modes of inertial instability, there exist ?local? modes within regions of anomalous potential vorticity. Local modes may be exactly stationary or display zonal phase propagation, but are distinguished from global modes by their zero group velocity and concentration of amplitude within, or downstream from, the region of most unstable flow. Local stationary instability has the largest growth rate and occurs in strong inhomogeneous shear when the in situ mean flow is near zero, that is, quasi-stationary with respect to the (stationary) basic-state pattern. This situation is expected in an equatorial Rossby wave critical layer. The local mode has properties similar to those of ?absolute? instability of nonparallel flow as discussed elsewhere in fluid dynamics.
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      Inertial Instability of Nonparallel Flow on an Equatorial β Plane

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4157298
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    contributor authorDunkerton, Timothy J.
    date accessioned2017-06-09T14:31:43Z
    date available2017-06-09T14:31:43Z
    date copyright1993/08/01
    date issued1993
    identifier issn0022-4928
    identifier otherams-21006.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4157298
    description abstractA simple theoretical model was developed to investigate the inertial instability of zonally nonuniform, non-parallel flow near the equator. The basic state was independent of height and time but included cross-equatorial shear with longitudinal variation, as observed in the tropical mesosphere and elsewhere. Numerical solutions were obtained for the most unstable modes. It is shown that, in addition to previously known ?global? (symmetric and nonsymmetric) modes of inertial instability, there exist ?local? modes within regions of anomalous potential vorticity. Local modes may be exactly stationary or display zonal phase propagation, but are distinguished from global modes by their zero group velocity and concentration of amplitude within, or downstream from, the region of most unstable flow. Local stationary instability has the largest growth rate and occurs in strong inhomogeneous shear when the in situ mean flow is near zero, that is, quasi-stationary with respect to the (stationary) basic-state pattern. This situation is expected in an equatorial Rossby wave critical layer. The local mode has properties similar to those of ?absolute? instability of nonparallel flow as discussed elsewhere in fluid dynamics.
    publisherAmerican Meteorological Society
    titleInertial Instability of Nonparallel Flow on an Equatorial β Plane
    typeJournal Paper
    journal volume50
    journal issue16
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1993)050<2744:IIONFO>2.0.CO;2
    journal fristpage2744
    journal lastpage2758
    treeJournal of the Atmospheric Sciences:;1993:;Volume( 050 ):;issue: 016
    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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