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    Observational Evidence of a Saturated Gravity Wave Spectrum in the Troposphere and Lower Stratosphere

    Source: Journal of the Atmospheric Sciences:;1988:;Volume( 045 ):;issue: 012::page 1741
    Author:
    Fritts, David C.
    ,
    Tsuda, Toshitaka
    ,
    Kato, Susumu
    ,
    Sato, Toru
    ,
    Fukao, Shoichiro
    DOI: 10.1175/1520-0469(1988)045<1741:OEOASG>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Radial velocity and temperature data obtained at the MU Radar Observatory during October and November 1986 are used to examine the character of the motion spectrum in the troposphere and lower stratosphere. It is found that the spectrum is dominated by low-frequency gravity waves with an upward sense of propagation in the lower stratosphere and both upward and downward propagation in the troposphere. Vertical wavenumber spectra of velocity and temperature are used to examine the consistency of the motion spectrum with the saturated spectrum of gravity waves proposed by Smith et al. Results indicate excellent agreement of the observed and predicted velocity and temperature spectra in both amplitude and slope. Vertical wavenumber spectra in area-preserving form reveal a dominant vertical wavelength of ?2.5 km, systematic variations in energy density and the dominant vertical scale with time, and consistency between the temporal variations of velocity and temperature variance. Taken together, our results provide strong support both for the view that velocity and temperature fluctuations are due primarily to internal gravity waves and for the saturated spectrum theory and its imposed constraints on wave amplitudes and spectral shape.
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      Observational Evidence of a Saturated Gravity Wave Spectrum in the Troposphere and Lower Stratosphere

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4155992
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    contributor authorFritts, David C.
    contributor authorTsuda, Toshitaka
    contributor authorKato, Susumu
    contributor authorSato, Toru
    contributor authorFukao, Shoichiro
    date accessioned2017-06-09T14:28:16Z
    date available2017-06-09T14:28:16Z
    date copyright1988/06/01
    date issued1988
    identifier issn0022-4928
    identifier otherams-19832.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4155992
    description abstractRadial velocity and temperature data obtained at the MU Radar Observatory during October and November 1986 are used to examine the character of the motion spectrum in the troposphere and lower stratosphere. It is found that the spectrum is dominated by low-frequency gravity waves with an upward sense of propagation in the lower stratosphere and both upward and downward propagation in the troposphere. Vertical wavenumber spectra of velocity and temperature are used to examine the consistency of the motion spectrum with the saturated spectrum of gravity waves proposed by Smith et al. Results indicate excellent agreement of the observed and predicted velocity and temperature spectra in both amplitude and slope. Vertical wavenumber spectra in area-preserving form reveal a dominant vertical wavelength of ?2.5 km, systematic variations in energy density and the dominant vertical scale with time, and consistency between the temporal variations of velocity and temperature variance. Taken together, our results provide strong support both for the view that velocity and temperature fluctuations are due primarily to internal gravity waves and for the saturated spectrum theory and its imposed constraints on wave amplitudes and spectral shape.
    publisherAmerican Meteorological Society
    titleObservational Evidence of a Saturated Gravity Wave Spectrum in the Troposphere and Lower Stratosphere
    typeJournal Paper
    journal volume45
    journal issue12
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1988)045<1741:OEOASG>2.0.CO;2
    journal fristpage1741
    journal lastpage1759
    treeJournal of the Atmospheric Sciences:;1988:;Volume( 045 ):;issue: 012
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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