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    CISK-Barotropic-Baroclinic Instability and the Growth of Monsoon Depressions

    Source: Journal of the Atmospheric Sciences:;1978:;Volume( 035 ):;issue: 003::page 495
    Author:
    Shukla, J.
    DOI: 10.1175/1520-0469(1978)035<0495:CBBIAT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: A combined CISK-barotropic-baroclinic instability analysis of the observed monsoon flow has been performed using the quasi-equilibrium assumption for the parameterization of moist convection. Linear perturbation equations for a three-layer quasi-geostrophic model are numerically integrated to get the most unstable mode. A deep cloud model, in which the height of the base of the cloud does not change with time and entrainment occurs for the whole depth of the cloud but detrainment occurs only at the top, is used to parameterize the effects of moist convection. It is found that the maximum growth rate occurs for the smallest scales. The mechanism for scale selection is therefore not clear. The structure and energetics of the computed linear perturbations for a wavelength corresponding to that of the observed monsoon depressions is compared with the observations. The dominant energy transformation for the computed and the observed perturbations is found to be from eddy available potential energy to eddy kinetic energy. The primary source of heating is condensational heating. Reasonable agreements between the structure and the energetics of the computed perturbations and the observed monsoon depressions suggest that CISK may provide the primary driving mechanism for the growth of monsoon depressions.
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      CISK-Barotropic-Baroclinic Instability and the Growth of Monsoon Depressions

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4153341
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    contributor authorShukla, J.
    date accessioned2017-06-09T14:20:00Z
    date available2017-06-09T14:20:00Z
    date copyright1978/03/01
    date issued1978
    identifier issn0022-4928
    identifier otherams-17446.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153341
    description abstractA combined CISK-barotropic-baroclinic instability analysis of the observed monsoon flow has been performed using the quasi-equilibrium assumption for the parameterization of moist convection. Linear perturbation equations for a three-layer quasi-geostrophic model are numerically integrated to get the most unstable mode. A deep cloud model, in which the height of the base of the cloud does not change with time and entrainment occurs for the whole depth of the cloud but detrainment occurs only at the top, is used to parameterize the effects of moist convection. It is found that the maximum growth rate occurs for the smallest scales. The mechanism for scale selection is therefore not clear. The structure and energetics of the computed linear perturbations for a wavelength corresponding to that of the observed monsoon depressions is compared with the observations. The dominant energy transformation for the computed and the observed perturbations is found to be from eddy available potential energy to eddy kinetic energy. The primary source of heating is condensational heating. Reasonable agreements between the structure and the energetics of the computed perturbations and the observed monsoon depressions suggest that CISK may provide the primary driving mechanism for the growth of monsoon depressions.
    publisherAmerican Meteorological Society
    titleCISK-Barotropic-Baroclinic Instability and the Growth of Monsoon Depressions
    typeJournal Paper
    journal volume35
    journal issue3
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1978)035<0495:CBBIAT>2.0.CO;2
    journal fristpage495
    journal lastpage508
    treeJournal of the Atmospheric Sciences:;1978:;Volume( 035 ):;issue: 003
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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