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    Resolving Convection in a Global Hypohydrostatic Model

    Source: Journal of the Atmospheric Sciences:;2007:;Volume( 064 ):;issue: 006::page 2061
    Author:
    Garner, S. T.
    ,
    Frierson, D. M. W.
    ,
    Held, I. M.
    ,
    Pauluis, O.
    ,
    Vallis, G. K.
    DOI: 10.1175/JAS3929.1
    Publisher: American Meteorological Society
    Abstract: Convection cannot be explicitly resolved in general circulation models given their typical grid size of 50 km or larger. However, by multiplying the vertical acceleration in the equation of motion by a constant larger than unity, the horizontal scale of convection can be increased at will, without necessarily affecting the larger-scale flow. The resulting hypohydrostatic system has been recognized for some time as a way to improve numerical stability on grids that cannot well resolve nonhydrostatic gravity waves. More recent studies have explored its potential for better representing convection in relatively coarse models. The recent studies have tested the rescaling idea in the context of regional models. Here the authors present global aquaplanet simulations with a low-resolution, nonhydrostatic model free of convective parameterization, and describe the effect on the global climate of very large rescaling of the vertical acceleration. As the convection expands to resolved scales, a deepening of the troposphere, a weakening of the Hadley cell, and a moistening of the lower troposphere is found, compared to solutions in which the moist convection is essentially hydrostatic. The growth rate of convective instability is reduced and the convective life cycle is lengthened relative to synoptic phenomena. This problematic side effect is noted in earlier studies and examined further here.
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      Resolving Convection in a Global Hypohydrostatic Model

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4218524
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    contributor authorGarner, S. T.
    contributor authorFrierson, D. M. W.
    contributor authorHeld, I. M.
    contributor authorPauluis, O.
    contributor authorVallis, G. K.
    date accessioned2017-06-09T16:53:42Z
    date available2017-06-09T16:53:42Z
    date copyright2007/06/01
    date issued2007
    identifier issn0022-4928
    identifier otherams-76112.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4218524
    description abstractConvection cannot be explicitly resolved in general circulation models given their typical grid size of 50 km or larger. However, by multiplying the vertical acceleration in the equation of motion by a constant larger than unity, the horizontal scale of convection can be increased at will, without necessarily affecting the larger-scale flow. The resulting hypohydrostatic system has been recognized for some time as a way to improve numerical stability on grids that cannot well resolve nonhydrostatic gravity waves. More recent studies have explored its potential for better representing convection in relatively coarse models. The recent studies have tested the rescaling idea in the context of regional models. Here the authors present global aquaplanet simulations with a low-resolution, nonhydrostatic model free of convective parameterization, and describe the effect on the global climate of very large rescaling of the vertical acceleration. As the convection expands to resolved scales, a deepening of the troposphere, a weakening of the Hadley cell, and a moistening of the lower troposphere is found, compared to solutions in which the moist convection is essentially hydrostatic. The growth rate of convective instability is reduced and the convective life cycle is lengthened relative to synoptic phenomena. This problematic side effect is noted in earlier studies and examined further here.
    publisherAmerican Meteorological Society
    titleResolving Convection in a Global Hypohydrostatic Model
    typeJournal Paper
    journal volume64
    journal issue6
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/JAS3929.1
    journal fristpage2061
    journal lastpage2075
    treeJournal of the Atmospheric Sciences:;2007:;Volume( 064 ):;issue: 006
    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