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contributor authorShimizu, Shingo
contributor authorUyeda, Hiroshi
contributor authorMoteki, Qoosaku
contributor authorMaesaka, Takeshi
contributor authorTakaya, Yoshimasa
contributor authorAkaeda, Kenji
contributor authorKato, Teruyuki
contributor authorYoshizaki, Masanori
date accessioned2017-06-09T16:21:10Z
date available2017-06-09T16:21:10Z
date copyright2008/07/01
date issued2008
identifier issn0027-0644
identifier otherams-66307.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4207629
description abstractThe structure and formation mechanism of a supercell-like storm in a moist environment below a melting layer were investigated using dual-Doppler radar analysis and a cloud-resolving storm simulator (CReSS). The supercell-like storm developed over the Kanto Plain, Japan, on 24 May 2000. The environment of the supercell-like storm possessed large convective available potential energy (1000 J kg?1), strong vertical wind shear (4.2 ? 10?3 s?1 between the surface and 5 km above sea level), and a moist layer (the relative humidity was 60%?90% below a melting layer at 3 km in height). The dual-Doppler radar analysis with a variational method revealed that the supercell-like storm had similar structures to those of a typical supercell in a dry environment below a melting layer, such as that in the Great Plains in the United States. The structures included a hook echo, an overhanging echo structure, and a strong updraft with strong vertical vorticity. However, some of the characteristics of the supercell-like storm differed from those of a typical supercell. For example, a weak downdraft, a weak outflow, a weak inflow, and a short time maintenance of a single cyclonically rotating updraft (about 30 min) were noted. Dual-Doppler radar analysis revealed that the convergence between the weak outflow and the weak inflow kept its location just under the updraft for about 30 min; in other words, the strength of the outflow balanced the strength of the inflow. The observed features were simulated well using CReSS, and the thermodynamical features of the formation mechanism were revealed. The weak downdraft with a small evaporative cooling rate was simulated in a moist layer below the melting layer at 3 km in height. The small evaporation cooling was a major cause of the weak downdraft and the weak outflow. Because the outflow was weak and did not cut off the initial updraft, the weak inflow was able to keep supplying warm air to the initial updraft for about 30 min. Therefore, the present supercell-like storm could form as a result of the balance of the strengths of the weak inflow and the weak outflow in a moist environment.
publisherAmerican Meteorological Society
titleStructure and Formation Mechanism on the 24 May 2000 Supercell-Like Storm Developing in a Moist Environment over the Kanto Plain, Japan
typeJournal Paper
journal volume136
journal issue7
journal titleMonthly Weather Review
identifier doi10.1175/2007MWR2155.1
journal fristpage2389
journal lastpage2407
treeMonthly Weather Review:;2008:;volume( 136 ):;issue: 007
contenttypeFulltext


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