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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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