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    Nonseparable Baroclinic Instability. Part II: Primitive-Equations Dynamics

    Source: Journal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 010::page 1223
    Author:
    Moore, G. W. Kent
    ,
    Peltier, W. R.
    DOI: 10.1175/1520-0469(1990)047<1223:NBIPIP>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The problem of the origin of midlatitude cyclonic disturbances having characteristic spatial scales of 1000 km or less has remained outstanding for most of this century. Although the theory of baroclinic instability of Charney and Eady has often been assumed to account for their appearance, Charney himself recognized that this was not so. In an attempt to develop a unique explanation for the observed scale of these systems we have been reinvestigating the classical problem of the baroclinic instability of synoptic-scale frontal zones. This work has shown that when the stability of such regions is analyzed using the hydrostatic primitive equations, a new mode of baroclinic instability is revealed, which has precisely the required scale. The new mode is completely filtered out in both the quasi-geostrophic and semigeostrophic systems. In the present paper we return to the primitive equations system to further analyze this problem and to refine the numerical formulation so as to enable an accurate investigation of the sensitivity of the growth rate and spatial scale of the new mode to the detailed properties of the background frontal flow. This demonstrates that focusing of the region of low Richardson number near the surface is most conducive to the growth of the cyclone wave.
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      Nonseparable Baroclinic Instability. Part II: Primitive-Equations Dynamics

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4156539
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    contributor authorMoore, G. W. Kent
    contributor authorPeltier, W. R.
    date accessioned2017-06-09T14:29:43Z
    date available2017-06-09T14:29:43Z
    date copyright1990/05/01
    date issued1989
    identifier issn0022-4928
    identifier otherams-20323.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156539
    description abstractThe problem of the origin of midlatitude cyclonic disturbances having characteristic spatial scales of 1000 km or less has remained outstanding for most of this century. Although the theory of baroclinic instability of Charney and Eady has often been assumed to account for their appearance, Charney himself recognized that this was not so. In an attempt to develop a unique explanation for the observed scale of these systems we have been reinvestigating the classical problem of the baroclinic instability of synoptic-scale frontal zones. This work has shown that when the stability of such regions is analyzed using the hydrostatic primitive equations, a new mode of baroclinic instability is revealed, which has precisely the required scale. The new mode is completely filtered out in both the quasi-geostrophic and semigeostrophic systems. In the present paper we return to the primitive equations system to further analyze this problem and to refine the numerical formulation so as to enable an accurate investigation of the sensitivity of the growth rate and spatial scale of the new mode to the detailed properties of the background frontal flow. This demonstrates that focusing of the region of low Richardson number near the surface is most conducive to the growth of the cyclone wave.
    publisherAmerican Meteorological Society
    titleNonseparable Baroclinic Instability. Part II: Primitive-Equations Dynamics
    typeJournal Paper
    journal volume47
    journal issue10
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1990)047<1223:NBIPIP>2.0.CO;2
    journal fristpage1223
    journal lastpage1242
    treeJournal of the Atmospheric Sciences:;1989:;Volume( 047 ):;issue: 010
    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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