The Spontaneous Imbalance of an Atmospheric Vortex at High Rossby NumberSource: Journal of the Atmospheric Sciences:;2008:;Volume( 065 ):;issue: 008::page 2498Author:Schecter, David A.
DOI: 10.1175/2007JAS2490.1Publisher: American Meteorological Society
Abstract: This 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.
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| contributor author | Schecter, David A. | |
| date accessioned | 2017-06-09T16:18:53Z | |
| date available | 2017-06-09T16:18:53Z | |
| date copyright | 2008/08/01 | |
| date issued | 2008 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-65580.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4206820 | |
| description abstract | This 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. | |
| publisher | American Meteorological Society | |
| title | The Spontaneous Imbalance of an Atmospheric Vortex at High Rossby Number | |
| type | Journal Paper | |
| journal volume | 65 | |
| journal issue | 8 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/2007JAS2490.1 | |
| journal fristpage | 2498 | |
| journal lastpage | 2521 | |
| tree | Journal of the Atmospheric Sciences:;2008:;Volume( 065 ):;issue: 008 | |
| contenttype | Fulltext |