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contributor authorSchecter, David A.
date accessioned2017-06-09T16:18:53Z
date available2017-06-09T16:18:53Z
date copyright2008/08/01
date issued2008
identifier issn0022-4928
identifier otherams-65580.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4206820
description abstractThis paper discusses recent progress toward understanding the instability of a monotonic vortex at high Rossby number, due to the radiation of spiral inertia?gravity (IG) waves. The outward-propagating IG waves are excited by inner undulations of potential vorticity that consist of one or more vortex Rossby waves. An individual vortex Rossby wave and its IG wave emission have angular pseudomomenta of opposite sign, positive and negative, respectively. The Rossby wave therefore grows in response to producing radiation. Such growth is potentially suppressed by the resonant absorption of angular pseudomomentum in a critical layer, where the angular phase velocity of the Rossby wave matches the angular velocity of the mean flow. Suppression requires a sufficiently steep radial gradient of potential vorticity in the critical layer. Both linear and nonlinear steepness requirements are reviewed. The formal theory of radiation-driven instability, or ?spontaneous imbalance,? is generalized in isentropic coordinates to baroclinic vortices that possess active critical layers. Furthermore, the rate of angular momentum loss by IG wave radiation is reexamined in the hurricane parameter regime. Numerical results suggest that the negative radiation torque on a hurricane has a smaller impact than surface drag, despite recent estimates of its large magnitude.
publisherAmerican Meteorological Society
titleThe Spontaneous Imbalance of an Atmospheric Vortex at High Rossby Number
typeJournal Paper
journal volume65
journal issue8
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/2007JAS2490.1
journal fristpage2498
journal lastpage2521
treeJournal of the Atmospheric Sciences:;2008:;Volume( 065 ):;issue: 008
contenttypeFulltext


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