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    An Ensemble of Convective Systems on 11 February 1993 during TOGA COARE:Morphology, Rainfall Characteristics, and Anvil Cloud Interactions

    Source: Monthly Weather Review:;1999:;volume( 127 ):;issue: 006::page 1208
    Author:
    Halverson, Jeffrey B.
    ,
    Ferrier, Brad S.
    ,
    Rickenbach, Thomas M.
    ,
    Simpson, Joanne
    ,
    Tao, Wei-Kuo
    DOI: 10.1175/1520-0493(1999)127<1208:AEOCSO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: An active day during the Coupled Ocean?Atmosphere Response Experiment (COARE) Intensive Observation Period (IOP) is examined in which nine convective systems evolved and moved eastward across the region of shipboard radar coverage in the Intensive Flux Array (IFA) within westerly wind burst conditions. The detailed genesis, morphology, and interactions between these cloud systems are documented from a radar and satellite perspective. One of these systems was a large and complex elliptical cluster, among the largest observed during the Tropical Ocean Global Atmosphere COARE. Multiple, parallel deep convective lines spaced 20?30 km apart and embedded within this system were initially oriented from north-northwest to south-southeast, oblique to the storm motion. Furthermore, the lines underwent counterclockwise realignment as the system moved eastward. The influence of strong lower-tropospheric directional and speed shear on these convective system properties is examined in the context of a dynamic, large-scale near-equatorial trough/transequatorial flow regime. A daily analysis of flow conditions during the 119-day IOP revealed that this type of synoptic regime was present in the IFA at least 40% of the time. Radar-derived rainfall statistics are examined throughout the life cycles of each individual convective system. Spatial mapping of accumulated rainfall reveals long, linear swaths produced by the most intense cells embedded within convective lines. The evolution of rainfall properties includes an increase in the stratiform rainfall fraction and areal coverage in later generations of systems, with a peak in total rainfall production after local midnight. These trends can be explained by anvil cloud interactions originating within the sequence of closely spaced disturbances, including the effects of both enhanced midtropospheric moisture and also strong reversing (easterly) shear. The issue of boundary layer recovery between the frequent, intense convective systems on this day is also examined.
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      An Ensemble of Convective Systems on 11 February 1993 during TOGA COARE:Morphology, Rainfall Characteristics, and Anvil Cloud Interactions

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4204296
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    • Monthly Weather Review

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    contributor authorHalverson, Jeffrey B.
    contributor authorFerrier, Brad S.
    contributor authorRickenbach, Thomas M.
    contributor authorSimpson, Joanne
    contributor authorTao, Wei-Kuo
    date accessioned2017-06-09T16:12:25Z
    date available2017-06-09T16:12:25Z
    date copyright1999/06/01
    date issued1999
    identifier issn0027-0644
    identifier otherams-63307.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4204296
    description abstractAn active day during the Coupled Ocean?Atmosphere Response Experiment (COARE) Intensive Observation Period (IOP) is examined in which nine convective systems evolved and moved eastward across the region of shipboard radar coverage in the Intensive Flux Array (IFA) within westerly wind burst conditions. The detailed genesis, morphology, and interactions between these cloud systems are documented from a radar and satellite perspective. One of these systems was a large and complex elliptical cluster, among the largest observed during the Tropical Ocean Global Atmosphere COARE. Multiple, parallel deep convective lines spaced 20?30 km apart and embedded within this system were initially oriented from north-northwest to south-southeast, oblique to the storm motion. Furthermore, the lines underwent counterclockwise realignment as the system moved eastward. The influence of strong lower-tropospheric directional and speed shear on these convective system properties is examined in the context of a dynamic, large-scale near-equatorial trough/transequatorial flow regime. A daily analysis of flow conditions during the 119-day IOP revealed that this type of synoptic regime was present in the IFA at least 40% of the time. Radar-derived rainfall statistics are examined throughout the life cycles of each individual convective system. Spatial mapping of accumulated rainfall reveals long, linear swaths produced by the most intense cells embedded within convective lines. The evolution of rainfall properties includes an increase in the stratiform rainfall fraction and areal coverage in later generations of systems, with a peak in total rainfall production after local midnight. These trends can be explained by anvil cloud interactions originating within the sequence of closely spaced disturbances, including the effects of both enhanced midtropospheric moisture and also strong reversing (easterly) shear. The issue of boundary layer recovery between the frequent, intense convective systems on this day is also examined.
    publisherAmerican Meteorological Society
    titleAn Ensemble of Convective Systems on 11 February 1993 during TOGA COARE:Morphology, Rainfall Characteristics, and Anvil Cloud Interactions
    typeJournal Paper
    journal volume127
    journal issue6
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1999)127<1208:AEOCSO>2.0.CO;2
    journal fristpage1208
    journal lastpage1228
    treeMonthly Weather Review:;1999:;volume( 127 ):;issue: 006
    contenttypeFulltext
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