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contributor authorFeliks, Yizhak
contributor authorTziperman, Eli
contributor authorFarrell, Brian
date accessioned2017-06-09T16:28:37Z
date available2017-06-09T16:28:37Z
date copyright2010/04/01
date issued2009
identifier issn0022-4928
identifier otherams-68563.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4210135
description abstractThe generalized stability of the secondary atmospheric circulation over strong SST fronts is studied using a hydrostatic, Boussinesq, two-dimensional f-plane model. It is shown that even in a parameter regime in which these circulations are stable to small perturbations, significant nonnormal growth of optimal initial perturbations occurs. The maximum growth factor in perturbation total energy is 250 and is dominated by the potential energy, which obtains a growth factor of 219 two to five hours after the beginning of the integration. This domination of potential energy growth is consistent with the observation that the available potential energy (APE) of the secondary circulation is larger by two orders of magnitude than the kinetic energy as well as with the transfer of kinetic to potential perturbation energy at the beginning of the growth of the perturbations. The norm kernel is found to significantly influence the structure of the optimal initial perturbation as well as the energy obtained by the mature perturbations, but the physical mechanism of growth and the structure of the mature perturbations are robust.
publisherAmerican Meteorological Society
titleNonnormal Frontal Dynamics
typeJournal Paper
journal volume67
journal issue4
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/2009JAS3214.1
journal fristpage1218
journal lastpage1231
treeJournal of the Atmospheric Sciences:;2009:;Volume( 067 ):;issue: 004
contenttypeFulltext


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