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    Instability of the Distorted Polar Night Vortex: A Theory of Stratospheric Warmings

    Source: Journal of the Atmospheric Sciences:;1981:;Volume( 038 ):;issue: 011::page 2514
    Author:
    Plumb, R. Alan
    DOI: 10.1175/1520-0469(1981)038<2514:IOTDPN>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The properties and stability of forced planetary waves in a continuous baroclinc shear are investigated gated using a weakly nonlinear analysis. A steady solution exists which under certain conditions may be unstable via interaction with a free traveling wave of the same wavenumber. This wave then grows at the expense of the zonal mean available potential energy. The parameter range in which instability occurs is extended by finite-amplitude perturbations. Theoretical predictions are compared with results from a highly truncated model of the winter atmosphere. Agreement is good, even after assumptions of the theory have broken down. The theory does become inapplicable, however, following a mean wind reversal (stratosphere warming); in an cases studied, such warming were found to occur subsequent to the instability. The theory appears to explain many features of observed and model warmings. Results of the study suggest that warmings arise from the intrinsic instability of the winter atmosphere. They can occur in the presence of steady forcing?no precursor tropospheric pulse of planetary wave energy is necessary. In these experiments, interaction with critical lines (of zero wind speed) plays no part in the generation of warmings.
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      Instability of the Distorted Polar Night Vortex: A Theory of Stratospheric Warmings

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4154225
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    contributor authorPlumb, R. Alan
    date accessioned2017-06-09T14:22:40Z
    date available2017-06-09T14:22:40Z
    date copyright1981/11/01
    date issued1981
    identifier issn0022-4928
    identifier otherams-18241.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4154225
    description abstractThe properties and stability of forced planetary waves in a continuous baroclinc shear are investigated gated using a weakly nonlinear analysis. A steady solution exists which under certain conditions may be unstable via interaction with a free traveling wave of the same wavenumber. This wave then grows at the expense of the zonal mean available potential energy. The parameter range in which instability occurs is extended by finite-amplitude perturbations. Theoretical predictions are compared with results from a highly truncated model of the winter atmosphere. Agreement is good, even after assumptions of the theory have broken down. The theory does become inapplicable, however, following a mean wind reversal (stratosphere warming); in an cases studied, such warming were found to occur subsequent to the instability. The theory appears to explain many features of observed and model warmings. Results of the study suggest that warmings arise from the intrinsic instability of the winter atmosphere. They can occur in the presence of steady forcing?no precursor tropospheric pulse of planetary wave energy is necessary. In these experiments, interaction with critical lines (of zero wind speed) plays no part in the generation of warmings.
    publisherAmerican Meteorological Society
    titleInstability of the Distorted Polar Night Vortex: A Theory of Stratospheric Warmings
    typeJournal Paper
    journal volume38
    journal issue11
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1981)038<2514:IOTDPN>2.0.CO;2
    journal fristpage2514
    journal lastpage2531
    treeJournal of the Atmospheric Sciences:;1981:;Volume( 038 ):;issue: 011
    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
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