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    An Energy-Balance Analysis of Deep Convective Self-Aggregation above Uniform SST

    Source: Journal of the Atmospheric Sciences:;2005:;Volume( 062 ):;issue: 012::page 4273
    Author:
    Bretherton, Christopher S.
    ,
    Blossey, Peter N.
    ,
    Khairoutdinov, Marat
    DOI: 10.1175/JAS3614.1
    Publisher: American Meteorological Society
    Abstract: The spatial organization of deep moist convection in radiative?convective equilibrium over a constant sea surface temperature is studied. A 100-day simulation is performed with a three-dimensional cloud-resolving model over a (576 km)2 domain with no ambient rotation and no mean wind. The convection self-aggregates within 10 days into quasi-stationary mesoscale patches of dry, subsiding and moist, rainy air columns. The patches ultimately merge into a single intensely convecting moist patch surrounded by a broad region of very dry subsiding air. The self-aggregation is analyzed as an instability of a horizontally homogeneous convecting atmosphere driven by convection?water vapor?radiation feedbacks that systematically dry the drier air columns and moisten the moister air columns. Column-integrated heat, water, and moist static energy budgets over (72 km)2 horizontal blocks show that this instability is primarily initiated by the reduced radiative cooling of air columns in which there is extensive anvil cirrus, augmented by enhanced surface latent and sensible heat fluxes under convectively active regions due to storm-induced gustiness. Mesoscale circulations intensify the later stages of self-aggregation by fluxing moist static energy from the dry to the moist regions. A simple mathematical model of the initial phase of self-aggregation is proposed based on the simulations. In accordance with this model, the self-aggregation can be suppressed by horizontally homogenizing the radiative cooling or surface fluxes. Lower-tropospheric wind shear leads to slightly slower and less pronounced self-aggregation into bands aligned along the shear vector. Self-aggregation is sensitive to the ice microphysical parameterization, which affects the location and extent of cirrus clouds and their radiative forcing. Self-aggregation is also sensitive to ambient Coriolis parameter f, and can induce spontaneous tropical cyclogenesis for large f. Inclusion of an interactive mixed-layer ocean slows but does not prevent self-aggregation.
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      An Energy-Balance Analysis of Deep Convective Self-Aggregation above Uniform SST

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4218176
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    • Journal of the Atmospheric Sciences

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    contributor authorBretherton, Christopher S.
    contributor authorBlossey, Peter N.
    contributor authorKhairoutdinov, Marat
    date accessioned2017-06-09T16:52:40Z
    date available2017-06-09T16:52:40Z
    date copyright2005/12/01
    date issued2005
    identifier issn0022-4928
    identifier otherams-75801.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4218176
    description abstractThe spatial organization of deep moist convection in radiative?convective equilibrium over a constant sea surface temperature is studied. A 100-day simulation is performed with a three-dimensional cloud-resolving model over a (576 km)2 domain with no ambient rotation and no mean wind. The convection self-aggregates within 10 days into quasi-stationary mesoscale patches of dry, subsiding and moist, rainy air columns. The patches ultimately merge into a single intensely convecting moist patch surrounded by a broad region of very dry subsiding air. The self-aggregation is analyzed as an instability of a horizontally homogeneous convecting atmosphere driven by convection?water vapor?radiation feedbacks that systematically dry the drier air columns and moisten the moister air columns. Column-integrated heat, water, and moist static energy budgets over (72 km)2 horizontal blocks show that this instability is primarily initiated by the reduced radiative cooling of air columns in which there is extensive anvil cirrus, augmented by enhanced surface latent and sensible heat fluxes under convectively active regions due to storm-induced gustiness. Mesoscale circulations intensify the later stages of self-aggregation by fluxing moist static energy from the dry to the moist regions. A simple mathematical model of the initial phase of self-aggregation is proposed based on the simulations. In accordance with this model, the self-aggregation can be suppressed by horizontally homogenizing the radiative cooling or surface fluxes. Lower-tropospheric wind shear leads to slightly slower and less pronounced self-aggregation into bands aligned along the shear vector. Self-aggregation is sensitive to the ice microphysical parameterization, which affects the location and extent of cirrus clouds and their radiative forcing. Self-aggregation is also sensitive to ambient Coriolis parameter f, and can induce spontaneous tropical cyclogenesis for large f. Inclusion of an interactive mixed-layer ocean slows but does not prevent self-aggregation.
    publisherAmerican Meteorological Society
    titleAn Energy-Balance Analysis of Deep Convective Self-Aggregation above Uniform SST
    typeJournal Paper
    journal volume62
    journal issue12
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/JAS3614.1
    journal fristpage4273
    journal lastpage4292
    treeJournal of the Atmospheric Sciences:;2005:;Volume( 062 ):;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