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contributor authorKumar, Vickal V.
contributor authorJakob, Christian
contributor authorProtat, Alain
contributor authorWilliams, Christopher R.
contributor authorMay, Peter T.
date accessioned2017-06-09T16:58:00Z
date available2017-06-09T16:58:00Z
date copyright2015/05/01
date issued2015
identifier issn0022-4928
identifier otherams-77180.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4219709
description abstractumulus parameterizations in weather and climate models frequently apply mass-flux schemes in their description of tropical convection. Mass flux constitutes the product of the fractional area covered by convection in a model grid box and the vertical velocity in cumulus clouds. However, vertical velocities are difficult to observe on GCM scales, making the evaluation of mass-flux schemes difficult. Here, the authors combine high-temporal-resolution observations of in-cloud vertical velocities derived from a pair of wind profilers over two wet seasons at Darwin with physical properties of precipitating clouds [cloud-top heights (CTH), convective?stratiform classification] derived from the Darwin C-band polarimetric radar to provide estimates of cumulus mass flux and its constituents. The length of this dataset allows for investigations of the contributions from different cumulus cloud types?namely, congestus, deep, and overshooting convection?to the overall mass flux and of the influence of large-scale conditions on mass flux. The authors found that mass flux was dominated by updrafts and, in particular, the updraft area fraction, with updraft vertical velocity playing a secondary role. The updraft vertical velocities peaked above 10 km where both the updraft area fractions and air densities were small, resulting in a marginal effect on mass-flux values. Downdraft area fractions are much smaller and velocities are much weaker than those in updrafts. The area fraction responded strongly to changes in midlevel large-scale vertical motion and convective inhibition (CIN). In contrast, changes in the lower-tropospheric relative humidity and convective available potential energy (CAPE) strongly modulate in-cloud vertical velocities but have moderate impacts on area fractions. Although average mass flux is found to increase with increasing CTH, it is the environmental conditions that seem to dictate the magnitude of mass flux produced by convection through a combination of effects on area fraction and velocity.
publisherAmerican Meteorological Society
titleMass-Flux Characteristics of Tropical Cumulus Clouds from Wind Profiler Observations at Darwin, Australia
typeJournal Paper
journal volume72
journal issue5
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/JAS-D-14-0259.1
journal fristpage1837
journal lastpage1855
treeJournal of the Atmospheric Sciences:;2015:;Volume( 072 ):;issue: 005
contenttypeFulltext


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