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    ON THE MERIDIONAL DISTRIBUTION OF SOURCE AND SINK TERMS OF THE KINETIC ENERGY BALANCE

    Source: Monthly Weather Review:;1970:;volume( 098 ):;issue: 012::page 911
    Author:
    KUNG, ERNEST C.
    DOI: 10.1175/1520-0493(1970)098<0911:OTMDOS>2.3.CO;2
    Publisher: American Meteorological Society
    Abstract: The latitude-height distributions of the kinetic energy generation and dissipation over North America are presented in a series of cross sections from 25° to 70° N, and from the surface to the 50-mb level. The generation was computed using the twice-daily observed wind and geopotential data for a 1-yr period. The dissipation was obtained for a 3-mo summer period as the residual term of the kinetic energy equation. Throughout all latitudes, the generation and dissipation have a maximum in the planetary boundary layer. They gradually reach a minimum in the mid-troposphere, then increase to another maximum at the jet stream level except in middle latitudes. In the upper troposphere, there seems to be a characteristic meridional distribution both for generation and dissipation. The generation is significantly large north and south of the middle latitude where the kinetic energy is adiabatically destroyed. Those latitudes of large generation in the upper troposphere are also characterized by high frictional dissipation values. Reference is also made to the results in available numerical experiments for comparison and discussion.
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      ON THE MERIDIONAL DISTRIBUTION OF SOURCE AND SINK TERMS OF THE KINETIC ENERGY BALANCE

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    https://yetl.yabesh.ir/yetl1/handle/yetl/4198699
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    contributor authorKUNG, ERNEST C.
    date accessioned2017-06-09T15:59:30Z
    date available2017-06-09T15:59:30Z
    date copyright1970/12/01
    date issued1970
    identifier issn0027-0644
    identifier otherams-58271.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4198699
    description abstractThe latitude-height distributions of the kinetic energy generation and dissipation over North America are presented in a series of cross sections from 25° to 70° N, and from the surface to the 50-mb level. The generation was computed using the twice-daily observed wind and geopotential data for a 1-yr period. The dissipation was obtained for a 3-mo summer period as the residual term of the kinetic energy equation. Throughout all latitudes, the generation and dissipation have a maximum in the planetary boundary layer. They gradually reach a minimum in the mid-troposphere, then increase to another maximum at the jet stream level except in middle latitudes. In the upper troposphere, there seems to be a characteristic meridional distribution both for generation and dissipation. The generation is significantly large north and south of the middle latitude where the kinetic energy is adiabatically destroyed. Those latitudes of large generation in the upper troposphere are also characterized by high frictional dissipation values. Reference is also made to the results in available numerical experiments for comparison and discussion.
    publisherAmerican Meteorological Society
    titleON THE MERIDIONAL DISTRIBUTION OF SOURCE AND SINK TERMS OF THE KINETIC ENERGY BALANCE
    typeJournal Paper
    journal volume98
    journal issue12
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1970)098<0911:OTMDOS>2.3.CO;2
    journal fristpage911
    journal lastpage916
    treeMonthly Weather Review:;1970:;volume( 098 ):;issue: 012
    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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