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    A Shallow CISK, Deep Equilibrium Mechanism for the Interaction between Large-Scale Convection and Large-Scale Circulations in the Tropics

    Source: Journal of the Atmospheric Sciences:;2003:;Volume( 060 ):;issue: 002::page 377
    Author:
    Wu, Zhaohua
    DOI: 10.1175/1520-0469(2003)060<0377:ASCDEM>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: In this paper, the circulations driven by deep heating and shallow heating are investigated through analytically solving a set of linear equations and examining circulations simulated by a dry primitive equation model. Special emphasis is placed on the low-level mass (moisture) convergence associated with the forced circulation and the maintenance of the shallow and deep heat sources. It is found that the forced circulation driven by shallow heating is more likely to be trapped horizontally near the heating area but relatively extended in the vertical. As a consequence, diabatic heating cannot balance adiabatic cooling due to upward motion. At the levels slightly above the top of the heating, a negative vertical gradient of temperature perturbation appears. For the atmosphere driven by deep heating, however, the temperature perturbation cannot accumulate because the heating signals propagate away very fast, allowing an approximate equilibrium between the convective diabatic heating and adiabatic cooling due to upward motion. The converged moisture associated with circulation driven by shallow heating exceeds the amount needed to maintain the heat source. However, the circulation driven by deep heating does not feed back effectively to the moisture convergence, and thus cannot be self-sustaining. Based on these results, a new mechanism is proposed for the interaction between the large-scale convection and large-scale circulation. The new mechanism states that shallow heating drives a strong low-level moisture convergence so that the system of shallow heating and the forced large-scale circulation is unstable. When the unstable system reaches a certain amplitude, the stable cap layer immediately above the shallow heating erodes, and deep convection arises, which consumes most of the converged moisture at low levels without much feedback to the low-level convergence of moisture. The whole heating circulation system develops and dies; the estimated lifetime of such a system, based on the timescale of adjustment of tropical atmosphere to forcing, is on an intraseasonal timescale. Related observational and modeling evidence that support the new mechanism is discussed.
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      A Shallow CISK, Deep Equilibrium Mechanism for the Interaction between Large-Scale Convection and Large-Scale Circulations in the Tropics

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159796
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    contributor authorWu, Zhaohua
    date accessioned2017-06-09T14:38:07Z
    date available2017-06-09T14:38:07Z
    date copyright2003/01/01
    date issued2003
    identifier issn0022-4928
    identifier otherams-23255.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159796
    description abstractIn this paper, the circulations driven by deep heating and shallow heating are investigated through analytically solving a set of linear equations and examining circulations simulated by a dry primitive equation model. Special emphasis is placed on the low-level mass (moisture) convergence associated with the forced circulation and the maintenance of the shallow and deep heat sources. It is found that the forced circulation driven by shallow heating is more likely to be trapped horizontally near the heating area but relatively extended in the vertical. As a consequence, diabatic heating cannot balance adiabatic cooling due to upward motion. At the levels slightly above the top of the heating, a negative vertical gradient of temperature perturbation appears. For the atmosphere driven by deep heating, however, the temperature perturbation cannot accumulate because the heating signals propagate away very fast, allowing an approximate equilibrium between the convective diabatic heating and adiabatic cooling due to upward motion. The converged moisture associated with circulation driven by shallow heating exceeds the amount needed to maintain the heat source. However, the circulation driven by deep heating does not feed back effectively to the moisture convergence, and thus cannot be self-sustaining. Based on these results, a new mechanism is proposed for the interaction between the large-scale convection and large-scale circulation. The new mechanism states that shallow heating drives a strong low-level moisture convergence so that the system of shallow heating and the forced large-scale circulation is unstable. When the unstable system reaches a certain amplitude, the stable cap layer immediately above the shallow heating erodes, and deep convection arises, which consumes most of the converged moisture at low levels without much feedback to the low-level convergence of moisture. The whole heating circulation system develops and dies; the estimated lifetime of such a system, based on the timescale of adjustment of tropical atmosphere to forcing, is on an intraseasonal timescale. Related observational and modeling evidence that support the new mechanism is discussed.
    publisherAmerican Meteorological Society
    titleA Shallow CISK, Deep Equilibrium Mechanism for the Interaction between Large-Scale Convection and Large-Scale Circulations in the Tropics
    typeJournal Paper
    journal volume60
    journal issue2
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2003)060<0377:ASCDEM>2.0.CO;2
    journal fristpage377
    journal lastpage392
    treeJournal of the Atmospheric Sciences:;2003:;Volume( 060 ):;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