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contributor authorReasor, Paul D.
contributor authorMontgomery, Michael T.
contributor authorMarks, Frank D.
contributor authorGamache, John F.
date accessioned2017-06-09T16:13:04Z
date available2017-06-09T16:13:04Z
date copyright2000/06/01
date issued2000
identifier issn0027-0644
identifier otherams-63518.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4204530
description abstractThe asymmetric dynamics of the hurricane inner-core region is examined through a novel analysis of high temporal resolution, three-dimensional wind fields derived from airborne dual-Doppler radar. Seven consecutive composites of Hurricane Olivia?s (1994) wind field with 30-min time resolution depict a weakening storm undergoing substantial structural changes. The symmetric and asymmetric mechanisms involved in this transformation are considered separately. To zeroth order the weakening of the primary circulation is consistent with the axisymmetric vortex spindown theory of Eliassen and Lystad for a neutrally stratified atmosphere. Vertical shear, however, increased dramatically during the observation period, leading to a strong projection of the convection onto an azimuthal wavenumber 1 pattern oriented along the maximum vertical shear vector. Recent theoretical ideas elucidating the dynamics of vortices in vertical shear are used to help explain this asymmetry. The role of asymmetric vorticity dynamics in explaining some of the physics of hurricane intensity change motivates a special focus on Olivia?s vorticity structure. It is found that an azimuthal wavenumber 2 feature dominates the asymmetry in relative vorticity below 3-km height. The characteristics of this asymmetry deduced from reflectivity and wind composites during a portion of the observation period show some consistency with a wavenumber 2 discrete vortex Rossby edge wave. Barotropic instability is suggested as a source for the wavenumber 2 asymmetry through a series of barotropic numerical simulations. Trailing bands of vorticity with radial wavelengths of 5?10 km are observed in the inner core approximately 20 km from the storm center, and may be symmetrizing vortex Rossby waves. Elevated reflectivity bands with radial scales comparable to those of the vorticity bands, also near 20?25-km radius, may be associated with these vorticity features.
publisherAmerican Meteorological Society
titleLow-Wavenumber Structure and Evolution of the Hurricane Inner Core Observed by Airborne Dual-Doppler Radar
typeJournal Paper
journal volume128
journal issue6
journal titleMonthly Weather Review
identifier doi10.1175/1520-0493(2000)128<1653:LWSAEO>2.0.CO;2
journal fristpage1653
journal lastpage1680
treeMonthly Weather Review:;2000:;volume( 128 ):;issue: 006
contenttypeFulltext


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