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    Inertial Instability and Rossby Wave Breaking in a Numerical Model

    Source: Journal of the Atmospheric Sciences:;1992:;Volume( 049 ):;issue: 012::page 991
    Author:
    O'Sullivan, Donal J.
    ,
    Hitchman, Matthew H.
    DOI: 10.1175/1520-0469(1992)049<0991:IIARWB>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A mechanistic model of the middle atmosphere is used to study the interaction between Rossby waves forced at the extratropical tropopause and inertial instability in the equatorial lower mesosphere. The impact of cross-equatorial shear strength and Rossby wave forcing amplitude is explored. Model results support the hypothesis, based on satellite temperature observations, that Rossby waves organize regions of equatorial inertial instability into coherent large-scale circulations. Horizontal convergence and divergence maxima are found stacked over the boundaries of regions of anomalous potential vorticity (PV). This supports observational diagnoses and theoretical expectations that parcel inertial accelerations arise in regions of anomalous PV, with divergence and convergence occurring at the boundaries. Although cross-equatorial shear determines the initial volume of inertially unstable air, Rossby waves arriving from the winter hemisphere deform PV contours such that zonally confined regions of anomalous PV extend well into the winter hemisphere and somewhat into the summer hemisphere. Significant parcel inertial accelerations are diagnosed to occur in anomalous PV tongues to 30° latitude in the winter hemisphere. Using a smaller cross-equatorial shear delays the penetration of anomalous PV into the winter hemisphere, while increasing the Rossby wave forcing amplitude causes a more rapid evolution of the low-latitude flow. These results suggest that inertial instability is intimately involved in Rossby wave breaking in the subtropical winter mesosphere. The horizontal scales of inertially unstable regions coevolve with those of PV anomalies, and so affect the breaking process from inception. The vertical scale of inertial circulations is much smaller than that of Rossby waves; hence, Rossby wave PV anomalies are eroded by vertical mixing as well as horizontal mixing. Gravity waves radiate away from the inertially unstable regions, which effectively convert energy from rotational to divergent modes. The interplay between inertial and gravitational instabilities and their role in causing irreversible mixing in the winter subtropics is explored. The effects of inertial instability on the seasonal evolution of PV is discussed from the point of view of ?PV thinking.?
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      Inertial Instability and Rossby Wave Breaking in a Numerical Model

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4156958
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    contributor authorO'Sullivan, Donal J.
    contributor authorHitchman, Matthew H.
    date accessioned2017-06-09T14:30:51Z
    date available2017-06-09T14:30:51Z
    date copyright1992/06/01
    date issued1992
    identifier issn0022-4928
    identifier otherams-20700.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156958
    description abstractA mechanistic model of the middle atmosphere is used to study the interaction between Rossby waves forced at the extratropical tropopause and inertial instability in the equatorial lower mesosphere. The impact of cross-equatorial shear strength and Rossby wave forcing amplitude is explored. Model results support the hypothesis, based on satellite temperature observations, that Rossby waves organize regions of equatorial inertial instability into coherent large-scale circulations. Horizontal convergence and divergence maxima are found stacked over the boundaries of regions of anomalous potential vorticity (PV). This supports observational diagnoses and theoretical expectations that parcel inertial accelerations arise in regions of anomalous PV, with divergence and convergence occurring at the boundaries. Although cross-equatorial shear determines the initial volume of inertially unstable air, Rossby waves arriving from the winter hemisphere deform PV contours such that zonally confined regions of anomalous PV extend well into the winter hemisphere and somewhat into the summer hemisphere. Significant parcel inertial accelerations are diagnosed to occur in anomalous PV tongues to 30° latitude in the winter hemisphere. Using a smaller cross-equatorial shear delays the penetration of anomalous PV into the winter hemisphere, while increasing the Rossby wave forcing amplitude causes a more rapid evolution of the low-latitude flow. These results suggest that inertial instability is intimately involved in Rossby wave breaking in the subtropical winter mesosphere. The horizontal scales of inertially unstable regions coevolve with those of PV anomalies, and so affect the breaking process from inception. The vertical scale of inertial circulations is much smaller than that of Rossby waves; hence, Rossby wave PV anomalies are eroded by vertical mixing as well as horizontal mixing. Gravity waves radiate away from the inertially unstable regions, which effectively convert energy from rotational to divergent modes. The interplay between inertial and gravitational instabilities and their role in causing irreversible mixing in the winter subtropics is explored. The effects of inertial instability on the seasonal evolution of PV is discussed from the point of view of ?PV thinking.?
    publisherAmerican Meteorological Society
    titleInertial Instability and Rossby Wave Breaking in a Numerical Model
    typeJournal Paper
    journal volume49
    journal issue12
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1992)049<0991:IIARWB>2.0.CO;2
    journal fristpage991
    journal lastpage1002
    treeJournal of the Atmospheric Sciences:;1992:;Volume( 049 ):;issue: 012
    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