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    Structure and Evolution of North Australian Cloud Lines Observed during AMEX Phase I

    Source: Monthly Weather Review:;1989:;volume( 117 ):;issue: 006::page 1181
    Author:
    Drosdowsky, Wasyl
    ,
    Holland, Greg J.
    ,
    Smith, Roger K.
    DOI: 10.1175/1520-0493(1989)117<1181:SAEONA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: North Australian Clouds Lines are distinctive, squall-line phenomena that occur in easterly flow across northern Australia. Three basic types have been identified, ranging from a long, narrow line of convective clouds (Type 1) to a severe squall line (Type 3). In this paper we examine a group of Type 1 lines, which occurred during the first phase of the Australian Monsoon Experiment (AMEX). The lines occurred in an ambient easterly flow with a distinct maximum near 850 hPa. Most of the lines developed on the western side of deep convective cells along the sea-breeze front in a manner that had substantial similarities to the African squall-line development described by Bolton. The resolvable structure resembled a shallow version of the Moncrieff?Miller squall line.
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      Structure and Evolution of North Australian Cloud Lines Observed during AMEX Phase I

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4202211
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    contributor authorDrosdowsky, Wasyl
    contributor authorHolland, Greg J.
    contributor authorSmith, Roger K.
    date accessioned2017-06-09T16:07:21Z
    date available2017-06-09T16:07:21Z
    date copyright1989/06/01
    date issued1989
    identifier issn0027-0644
    identifier otherams-61431.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4202211
    description abstractNorth Australian Clouds Lines are distinctive, squall-line phenomena that occur in easterly flow across northern Australia. Three basic types have been identified, ranging from a long, narrow line of convective clouds (Type 1) to a severe squall line (Type 3). In this paper we examine a group of Type 1 lines, which occurred during the first phase of the Australian Monsoon Experiment (AMEX). The lines occurred in an ambient easterly flow with a distinct maximum near 850 hPa. Most of the lines developed on the western side of deep convective cells along the sea-breeze front in a manner that had substantial similarities to the African squall-line development described by Bolton. The resolvable structure resembled a shallow version of the Moncrieff?Miller squall line.
    publisherAmerican Meteorological Society
    titleStructure and Evolution of North Australian Cloud Lines Observed during AMEX Phase I
    typeJournal Paper
    journal volume117
    journal issue6
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1989)117<1181:SAEONA>2.0.CO;2
    journal fristpage1181
    journal lastpage1192
    treeMonthly Weather Review:;1989:;volume( 117 ):;issue: 006
    contenttypeFulltext
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