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contributor authorCunning, John B.
contributor authorHolle, Ronald L.
contributor authorGannon, Patrick T.
contributor authorWatson, Andrew I.
date accessioned2017-06-09T13:58:52Z
date available2017-06-09T13:58:52Z
date copyright1982/07/01
date issued1982
identifier issn0021-8952
identifier otherams-10300.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4145403
description abstractThis paper investigates the interactions between the various scales of motion and, specifically, the inter-actions between convection and the surface boundary layer in the development of a mesoscale convective system within the Florida Area Cumulus Experiment (FACE) experimental area. Data used in the analysis are from a surface mesonetwork covering a 1500 km2 area which consisted of wind measuring stations, raingages, hygrothermographs, microbarographs and temperature, humidity and pressure transducers. Surface convergence was shown to exist up to 2 h before the development of precipitation over the convergence area within the mesonetwork. Convergence was not being balanced by divergence within the network, which implies mesoscale and/or synoptic-scale forcing. The subsidence warming and drying in the near environment of the mesoscale convective system appeared to play an important role in its evolution from the mature to the dissipating stage. Soundings taken in the near environment of the convective system showed a 0.8 km lowering in the depth of the moist layer in time. It is hypothesized that the entrainment of this drier air into the convective system, particularly the new convective elements, helps accelerate the mesoscale outflow away from the convective system, which causes the system to evolve into the dissipating stage. Surface pressure perturbations are shown to be very important in the feedback between developing convection and the boundary layer. Two types of pressure responses are shown, a mesoscale response which appears to affect the entire mesonetwork area and a convective-scale response which affects only a relatively small area beneath the developing cells. The surface pressure perturbations are shown to increase the surface convergence into the area, and as shown in previous papers, this increased surface convergence should then produce a larger and more intense convective system. The merger between the two convective systems which developed the mesoscale system on this day is described in terms of the radar, visual cloud and raingage characteristics. It is shown that new cloud development and differential motion between convective elements were the two main causes of merger.
publisherAmerican Meteorological Society
titleConvective Evolution and Merger in the FACE Experimental Area: Mesoscale Convection and Boundary Layer Interactions
typeJournal Paper
journal volume21
journal issue7
journal titleJournal of Applied Meteorology
identifier doi10.1175/1520-0450(1982)021<0953:CEAMIT>2.0.CO;2
journal fristpage953
journal lastpage977
treeJournal of Applied Meteorology:;1982:;volume( 021 ):;issue: 007
contenttypeFulltext


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