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    Stability of Baroclinic Flows in a Zonal Magnetic Field: Part II

    Source: Journal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 002::page 119
    Author:
    Gilman, Peter A.
    DOI: 10.1175/1520-0469(1967)024<0119:SOBFIA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The equations of Part I are approximated to represent a two-layer model. All the theorems for the continuous case are shown to hold in the two-layer case as well. In addition, bounds are placed on the phase velocities of neutral waves. The stability of purely baroclinic flow (no horizontal shear) in a uniform zonal magnetic field is then studied. The minimum vertical shear needed for instability no longer depends upon the ?-effect or the static stability, but rather is determined by the zonal field strength. Short waves are destabilized by the magnetic field, long waves stabilized. Unstable waves convert available potential energy into kinetic energy of the disturbances, part of which in turn is converted into disturbance magnetic energy. Nonmagnetic changes in the initial state are similar to those of Phillips. Perturbation vertical magnetic fields and a single-celled meridional (poloidal) field are produced.
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      Stability of Baroclinic Flows in a Zonal Magnetic Field: Part II

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    contributor authorGilman, Peter A.
    date accessioned2017-06-09T14:14:04Z
    date available2017-06-09T14:14:04Z
    date copyright1967/03/01
    date issued1967
    identifier issn0022-4928
    identifier otherams-15294.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150950
    description abstractThe equations of Part I are approximated to represent a two-layer model. All the theorems for the continuous case are shown to hold in the two-layer case as well. In addition, bounds are placed on the phase velocities of neutral waves. The stability of purely baroclinic flow (no horizontal shear) in a uniform zonal magnetic field is then studied. The minimum vertical shear needed for instability no longer depends upon the ?-effect or the static stability, but rather is determined by the zonal field strength. Short waves are destabilized by the magnetic field, long waves stabilized. Unstable waves convert available potential energy into kinetic energy of the disturbances, part of which in turn is converted into disturbance magnetic energy. Nonmagnetic changes in the initial state are similar to those of Phillips. Perturbation vertical magnetic fields and a single-celled meridional (poloidal) field are produced.
    publisherAmerican Meteorological Society
    titleStability of Baroclinic Flows in a Zonal Magnetic Field: Part II
    typeJournal Paper
    journal volume24
    journal issue2
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1967)024<0119:SOBFIA>2.0.CO;2
    journal fristpage119
    journal lastpage129
    treeJournal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 002
    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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