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contributor authorStaley, D. O.
contributor authorGall, R. L.
date accessioned2017-06-09T14:20:49Z
date available2017-06-09T14:20:49Z
date copyright1979/06/01
date issued1979
identifier issn0022-4928
identifier otherams-17707.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4153631
description abstractThe barotropic instability of a tornado described by Hoecker is investigated. It is found that wavenumbers of the order of 1 to 5 are significantly unstable, with growth rates of the order of 0.1 to 0.5 s?1, yielding e-folding times small compared to tornado lifetimes. The instability is related to departures from the wind distribution of a combined Rankine vortex. Small departures can yield significant growth rates. Also investigated is the barotropic instability of an idealized vortex with a core of constant angular velocity and constant vorticity surrounded by a belt with twice the core vorticity, extending out to the wind maximum, beyond which the vorticity vanishes. Growth rates of the order of 0.1 s?1 are found at wavenumbers between 3.6 and 4.0, with negligible growth rates outside this region. It is suggested that the instability may lead ultimately to the ?suction vortices? described by Fujita in connection with tornadoes and dust devils.
publisherAmerican Meteorological Society
titleBarotropic Instability in a Tornado Vortex
typeJournal Paper
journal volume36
journal issue6
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1979)036<0973:BIIATV>2.0.CO;2
journal fristpage973
journal lastpage981
treeJournal of the Atmospheric Sciences:;1979:;Volume( 036 ):;issue: 006
contenttypeFulltext


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