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    Observational Evidence of Kelvin Waves in the Tropical Stratosphere

    Source: Journal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 005::page 900
    Author:
    Wallace, John M.
    ,
    Kousky, V. E.
    DOI: 10.1175/1520-0469(1968)025<0900:OEOKWI>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: This study of synoptic-scale wave motions in the equatorial stratosphere is based on the analysis of six months of radiosonde data from three tropical stations. Fluctuations in the zonal wind with an average period of 15 days, and amplitudes in the order of 8?12 m sec?1 are noted. Corresponding fluctuations are found in the temperature field with amplitudes of 3?5C and a phase lead of ¼ cycle with respect to the zonal wind. These wave motions which propagate phase downward do not appear to involve the meridional wind component. The observed fluctuations resemble Kelvin waves, which represent one of the solutions of the wave equation on an equatorial beta plane. One of the notable features of this type of wave is that it produces an upward flux of westerly momentum. The observations indicate that this flux is large enough to account for the westerly accelerations associated with the quasi-biennial oscillation.
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      Observational Evidence of Kelvin Waves in the Tropical Stratosphere

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4151183
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    contributor authorWallace, John M.
    contributor authorKousky, V. E.
    date accessioned2017-06-09T14:14:38Z
    date available2017-06-09T14:14:38Z
    date copyright1968/09/01
    date issued1968
    identifier issn0022-4928
    identifier otherams-15503.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151183
    description abstractThis study of synoptic-scale wave motions in the equatorial stratosphere is based on the analysis of six months of radiosonde data from three tropical stations. Fluctuations in the zonal wind with an average period of 15 days, and amplitudes in the order of 8?12 m sec?1 are noted. Corresponding fluctuations are found in the temperature field with amplitudes of 3?5C and a phase lead of ¼ cycle with respect to the zonal wind. These wave motions which propagate phase downward do not appear to involve the meridional wind component. The observed fluctuations resemble Kelvin waves, which represent one of the solutions of the wave equation on an equatorial beta plane. One of the notable features of this type of wave is that it produces an upward flux of westerly momentum. The observations indicate that this flux is large enough to account for the westerly accelerations associated with the quasi-biennial oscillation.
    publisherAmerican Meteorological Society
    titleObservational Evidence of Kelvin Waves in the Tropical Stratosphere
    typeJournal Paper
    journal volume25
    journal issue5
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1968)025<0900:OEOKWI>2.0.CO;2
    journal fristpage900
    journal lastpage907
    treeJournal of the Atmospheric Sciences:;1968:;Volume( 025 ):;issue: 005
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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