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    Upscale Evolution of MCSs: Doppler Radar Analysis and Analytical Investigation

    Source: Monthly Weather Review:;1997:;volume( 125 ):;issue: 006::page 1083
    Author:
    McAnelly, Ray L.
    ,
    Nachamkin, Jason E.
    ,
    Cotton, William R.
    ,
    Nicholls, Melville E.
    DOI: 10.1175/1520-0493(1997)125<1083:UEOMDR>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The development of two small mesoscale convective systems (MCSs) in northeastern Colorado is investigated via dual-Doppler radar analysis. The first system developed from several initially isolated cumulonimbi, which gradually coalesced into a minimal MCS with relatively little stratiform precipitation. The second system developed more rapidly along an axis of convection and generated a more extensive and persistent stratiform echo and MCS cloud shield. In both systems, the volumetric precipitation rate exhibited an early meso-?-scale convective cycle (a maximum and subsequent minimum), followed by reintensification into a modest mature stage. This sequence is similar to that noted previously in the developing stage of larger MCSs by McAnelly and Cotton. They speculated that the early meso-? convective cycle is a characteristic feature of development in many MCSs that is dynamically linked to a rather abrupt transition toward mature stage structure. This study presents kinematic evidence in support of this hypothesis for these cases, as derived from dual-Doppler radar analyses over several-hour periods. Mature stage MCS characteristics such as deepened low- to midlevel convergence and mesoscale descent developed fairly rapidly, about 1 h after the early meso-? convective maximum. The dynamic linkage between the meso-? convective cycle and evolution toward mature structure is examined with a simple analytical model of the linearized atmospheric response to prescribed heating. Heating functions that approximate the temporal and spatial characteristics of the meso-? convective cycle are prescribed. The solutions show that the cycle forces a response within and near the thermally forced region that is consistent with the observed kinematic evolution in the MCSs. The initial response to an intensifying convective ensemble is a self-suppressing mechanism that partially explains the weakening after a meso-? convective maximum. A lagged response then favors reintensification and areal growth of the weakened ensemble. A conceptual model of MCS development is proposed whereby the early meso-? convective cycle and the response to it are hypothesized to act as a generalized forcing?feedback mechanism that helps explain the upscale growth of a convective ensemble into an organized MCS.
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      Upscale Evolution of MCSs: Doppler Radar Analysis and Analytical Investigation

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4203841
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    contributor authorMcAnelly, Ray L.
    contributor authorNachamkin, Jason E.
    contributor authorCotton, William R.
    contributor authorNicholls, Melville E.
    date accessioned2017-06-09T16:11:18Z
    date available2017-06-09T16:11:18Z
    date copyright1997/06/01
    date issued1997
    identifier issn0027-0644
    identifier otherams-62899.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4203841
    description abstractThe development of two small mesoscale convective systems (MCSs) in northeastern Colorado is investigated via dual-Doppler radar analysis. The first system developed from several initially isolated cumulonimbi, which gradually coalesced into a minimal MCS with relatively little stratiform precipitation. The second system developed more rapidly along an axis of convection and generated a more extensive and persistent stratiform echo and MCS cloud shield. In both systems, the volumetric precipitation rate exhibited an early meso-?-scale convective cycle (a maximum and subsequent minimum), followed by reintensification into a modest mature stage. This sequence is similar to that noted previously in the developing stage of larger MCSs by McAnelly and Cotton. They speculated that the early meso-? convective cycle is a characteristic feature of development in many MCSs that is dynamically linked to a rather abrupt transition toward mature stage structure. This study presents kinematic evidence in support of this hypothesis for these cases, as derived from dual-Doppler radar analyses over several-hour periods. Mature stage MCS characteristics such as deepened low- to midlevel convergence and mesoscale descent developed fairly rapidly, about 1 h after the early meso-? convective maximum. The dynamic linkage between the meso-? convective cycle and evolution toward mature structure is examined with a simple analytical model of the linearized atmospheric response to prescribed heating. Heating functions that approximate the temporal and spatial characteristics of the meso-? convective cycle are prescribed. The solutions show that the cycle forces a response within and near the thermally forced region that is consistent with the observed kinematic evolution in the MCSs. The initial response to an intensifying convective ensemble is a self-suppressing mechanism that partially explains the weakening after a meso-? convective maximum. A lagged response then favors reintensification and areal growth of the weakened ensemble. A conceptual model of MCS development is proposed whereby the early meso-? convective cycle and the response to it are hypothesized to act as a generalized forcing?feedback mechanism that helps explain the upscale growth of a convective ensemble into an organized MCS.
    publisherAmerican Meteorological Society
    titleUpscale Evolution of MCSs: Doppler Radar Analysis and Analytical Investigation
    typeJournal Paper
    journal volume125
    journal issue6
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1997)125<1083:UEOMDR>2.0.CO;2
    journal fristpage1083
    journal lastpage1110
    treeMonthly Weather Review:;1997:;volume( 125 ):;issue: 006
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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