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    Nonnormal Frontal Dynamics

    Source: Journal of the Atmospheric Sciences:;2009:;Volume( 067 ):;issue: 004::page 1218
    Author:
    Feliks, Yizhak
    ,
    Tziperman, Eli
    ,
    Farrell, Brian
    DOI: 10.1175/2009JAS3214.1
    Publisher: American Meteorological Society
    Abstract: The 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.
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      Nonnormal Frontal Dynamics

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4210135
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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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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian