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    Mean-State Convective Circulations over Large-Scale Tropical SST Gradients

    Source: Journal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 009::page 1578
    Author:
    Yano, Jun-Ichi
    ,
    Grabowski, Wojciech W.
    ,
    Moncrieff, Mitchell W.
    DOI: 10.1175/1520-0469(2002)059<1578:MSCCOL>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The dynamical balance of the mean tropical atmospheric circulation maintained over large-scale SST gradients is analyzed. To first order, the strength of the circulation is determined by the subsidence rate in the dry descent region that balances the radiative cooling. The divergent component of the horizontal wind is then proportional to the domain size. The convective intensity is determined by the balance between convective heating and the sum of the radiative cooling and adiabatic cooling by large-scale vertical ascent. A key result is that the amplitude of the SST gradients does not directly determine the strength of the large-scale circulation. A second-order analysis shows that the tropospheric temperature responds to SST only through the residual convective heating, which is the deviation of convective heating from the first-order estimate. This decreases the temperature gradient that drives the observed Walker circulation to only a small fraction of the SST gradient across the Pacific. This argument is analogous to Lindzen and Nigam's ?back pressure.? The suppression of the SST gradients by the residual convective heating further increases with decreasing horizontal extent of the large-scale circulation, as well as with increasing SST contrast. Therefore, the horizontal air temperature gradient required to drive the large-scale circulation is consistent with the first-order estimate. Analyses of cloud-resolving numerical simulations suggest that when the domain size is small, the suppression of SST gradients by residual convective heating is strong enough to generate a secondary convergence in the middle troposphere. This generates a mean circulation consisting of two shallow cells (third baroclinic mode). This shallower circulation maintains a horizontal flow strength comparable to that in a large domain. Two variables remain undetermined: the ratio between the ascending and the descending areas, and a closed expression for the residual heating rate.
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      Mean-State Convective Circulations over Large-Scale Tropical SST Gradients

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    https://yetl.yabesh.ir/yetl1/handle/yetl/4159629
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    • Journal of the Atmospheric Sciences

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    contributor authorYano, Jun-Ichi
    contributor authorGrabowski, Wojciech W.
    contributor authorMoncrieff, Mitchell W.
    date accessioned2017-06-09T14:37:39Z
    date available2017-06-09T14:37:39Z
    date copyright2002/05/01
    date issued2002
    identifier issn0022-4928
    identifier otherams-23104.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159629
    description abstractThe dynamical balance of the mean tropical atmospheric circulation maintained over large-scale SST gradients is analyzed. To first order, the strength of the circulation is determined by the subsidence rate in the dry descent region that balances the radiative cooling. The divergent component of the horizontal wind is then proportional to the domain size. The convective intensity is determined by the balance between convective heating and the sum of the radiative cooling and adiabatic cooling by large-scale vertical ascent. A key result is that the amplitude of the SST gradients does not directly determine the strength of the large-scale circulation. A second-order analysis shows that the tropospheric temperature responds to SST only through the residual convective heating, which is the deviation of convective heating from the first-order estimate. This decreases the temperature gradient that drives the observed Walker circulation to only a small fraction of the SST gradient across the Pacific. This argument is analogous to Lindzen and Nigam's ?back pressure.? The suppression of the SST gradients by the residual convective heating further increases with decreasing horizontal extent of the large-scale circulation, as well as with increasing SST contrast. Therefore, the horizontal air temperature gradient required to drive the large-scale circulation is consistent with the first-order estimate. Analyses of cloud-resolving numerical simulations suggest that when the domain size is small, the suppression of SST gradients by residual convective heating is strong enough to generate a secondary convergence in the middle troposphere. This generates a mean circulation consisting of two shallow cells (third baroclinic mode). This shallower circulation maintains a horizontal flow strength comparable to that in a large domain. Two variables remain undetermined: the ratio between the ascending and the descending areas, and a closed expression for the residual heating rate.
    publisherAmerican Meteorological Society
    titleMean-State Convective Circulations over Large-Scale Tropical SST Gradients
    typeJournal Paper
    journal volume59
    journal issue9
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2002)059<1578:MSCCOL>2.0.CO;2
    journal fristpage1578
    journal lastpage1592
    treeJournal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 009
    contenttypeFulltext
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    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian
     
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian