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contributor authorBirner, Thomas
contributor authorWilliams, Paul D.
date accessioned2017-06-09T16:22:59Z
date available2017-06-09T16:22:59Z
date copyright2008/10/01
date issued2008
identifier issn0022-4928
identifier otherams-66862.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4208245
description abstractSudden stratospheric warmings (SSWs) are usually considered to be initiated by planetary wave activity. Here it is asked whether small-scale variability (e.g., related to gravity waves) can lead to SSWs given a certain amount of planetary wave activity that is by itself not sufficient to cause a SSW. A highly vertically truncated version of the Holton?Mass model of stratospheric wave?mean flow interaction, recently proposed by Ruzmaikin et al., is extended to include stochastic forcing. In the deterministic setting, this low-order model exhibits multiple stable equilibria corresponding to the undisturbed vortex and SSW state, respectively. Momentum forcing due to quasi-random gravity wave activity is introduced as an additive noise term in the zonal momentum equation. Two distinct approaches are pursued to study the stochastic system. First, the system, initialized at the undisturbed state, is numerically integrated many times to derive statistics of first passage times of the system undergoing a transition to the SSW state. Second, the Fokker?Planck equation corresponding to the stochastic system is solved numerically to derive the stationary probability density function of the system. Both approaches show that even small to moderate strengths of the stochastic gravity wave forcing can be sufficient to cause a SSW for cases for which the deterministic system would not have predicted a SSW.
publisherAmerican Meteorological Society
titleSudden Stratospheric Warmings as Noise-Induced Transitions
typeJournal Paper
journal volume65
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/2008JAS2770.1
journal fristpage3337
journal lastpage3343
treeJournal of the Atmospheric Sciences:;2008:;Volume( 065 ):;issue: 010
contenttypeFulltext


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