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contributor authorCOX, STEPHEN K.
date accessioned2017-06-09T15:59:07Z
date available2017-06-09T15:59:07Z
date copyright1969/09/01
date issued1969
identifier issn0027-0644
identifier otherams-58122.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4198535
description abstractBalloon-borne radiation sonde measurements during 1964 and 1965 are used to form composite, three-dimensional radiative cooling models for the following midlatitude synoptic features: stationary front; nascent cyclone; warm sector cyclone; occluded cyclone; and anticyclone. Composite water vapor distributions for the same synoptic features are used to model the pattern of atmospheric warming by solar radiation. Thickness tendency analyses of the 1000-500-mb layer for four synoptic features show that radiative cooling and warming may account for 10?30 percent of the observed maximum thickness tendency. The radiative thickness change components are of the same order of magnitude as the latent and the sensible heating terms. The nascent cyclone case shows a radiatively induced vorticity tendency of 6 ? 10?10 sec?2. This compares with a total expected vorticity tendency between 10?9 and 10?10 sec?2. The nascent cyclone, warm sector cyclone, and anticyclone cases show positive cyclonic development from radiative effects, while the occluded cyclone case shows negative cyclonic development.
publisherAmerican Meteorological Society
titleRADIATION MODELS OF MIDLATITUDE SYNOPTIC FEATURES
typeJournal Paper
journal volume97
journal issue9
journal titleMonthly Weather Review
identifier doi10.1175/1520-0493(1969)097<0637:RMOMSF>2.3.CO;2
journal fristpage637
journal lastpage651
treeMonthly Weather Review:;1969:;volume( 097 ):;issue: 009
contenttypeFulltext


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