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contributor authorTrapp, Robert J.;Marion, Geoffrey R.;Nesbitt, Stephen W.
date accessioned2018-01-03T11:02:34Z
date available2018-01-03T11:02:34Z
date copyright9/27/2017 12:00:00 AM
date issued2017
identifier otherjas-d-16-0331.1.pdf
identifier urihttp://138.201.223.254:8080/yetl1/handle/yetl/4246465
description abstractAbstractStrong to violent tornadoes cause a disproportionate amount of damage, in part because the width and length of a tornado damage track are correlated to tornado intensity (as now estimated through enhanced Fujita scale ratings). The tendency expressed in the observational record is that the most intense tornadoes are often the widest. Herein the authors explore the simple hypothesis that wide intense tornadoes should form more readily out of wide rotating updrafts. This hypothesis is based on an application of Kelvin?s circulation theorem, which is used to argue that the large circulation associated with a wide intense tornado is more plausibly associated with a wide mesocyclone. Because a mesocyclone is, strictly speaking, a rotating updraft, the mesocyclone width should increase with increasing updraft width. A simple mathematical model that is quantified using observations of mesocyclones supports this hypothesis, as do idealized numerical simulations of supercellular thunderstorms.
publisherAmerican Meteorological Society
titleThe Regulation of Tornado Intensity by Updraft Width
typeJournal Paper
journal volume74
journal issue12
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/JAS-D-16-0331.1
journal fristpage4199
journal lastpage4211
treeJournal of the Atmospheric Sciences:;2017:;Volume( 074 ):;issue: 012
contenttypeFulltext


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