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    Longitudinal and Lateral Spectra of Turbulence in the Atmospheric Boundary Layer at the Kennedy Space Center

    Source: Journal of Applied Meteorology:;1970:;volume( 009 ):;issue: 001::page 51
    Author:
    Fichtl, George H.
    ,
    McVehil, George E.
    DOI: 10.1175/1520-0450(1970)009<0051:LALSOT>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: An engineering spectral model of turbulence is developed with horizontal wind observations obtained at the NASA 150-m meteorological tower at Cape Kennedy, Fla. Spectra, measured at six levels, are collapsed at each level with [nS(n)/u*02,f]-coordinates, where S(n) is the longitudinal or lateral spectral energy density at frequency n(Hz), u*0 the surface friction velocity, and f = nz/?, ? being the mean wind speed at height z. A vertical collapse of the dimensionless spectra is produced by assuming they are shape-invariant in the vertical. An analysis of the longitudinal spectrum in the inertial subrange, at the 18-m level, implies that the local mechanical and buoyant production rates of turbulent kinetic energy are balanced by the local dissipation and energy flux divergence, respectively.
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      Longitudinal and Lateral Spectra of Turbulence in the Atmospheric Boundary Layer at the Kennedy Space Center

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4222222
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    • Journal of Applied Meteorology

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    contributor authorFichtl, George H.
    contributor authorMcVehil, George E.
    date accessioned2017-06-09T17:06:15Z
    date available2017-06-09T17:06:15Z
    date copyright1970/02/01
    date issued1970
    identifier issn0021-8952
    identifier otherams-7944.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4222222
    description abstractAn engineering spectral model of turbulence is developed with horizontal wind observations obtained at the NASA 150-m meteorological tower at Cape Kennedy, Fla. Spectra, measured at six levels, are collapsed at each level with [nS(n)/u*02,f]-coordinates, where S(n) is the longitudinal or lateral spectral energy density at frequency n(Hz), u*0 the surface friction velocity, and f = nz/?, ? being the mean wind speed at height z. A vertical collapse of the dimensionless spectra is produced by assuming they are shape-invariant in the vertical. An analysis of the longitudinal spectrum in the inertial subrange, at the 18-m level, implies that the local mechanical and buoyant production rates of turbulent kinetic energy are balanced by the local dissipation and energy flux divergence, respectively.
    publisherAmerican Meteorological Society
    titleLongitudinal and Lateral Spectra of Turbulence in the Atmospheric Boundary Layer at the Kennedy Space Center
    typeJournal Paper
    journal volume9
    journal issue1
    journal titleJournal of Applied Meteorology
    identifier doi10.1175/1520-0450(1970)009<0051:LALSOT>2.0.CO;2
    journal fristpage51
    journal lastpage63
    treeJournal of Applied Meteorology:;1970:;volume( 009 ):;issue: 001
    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