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    Middle and High Latitude Southern Hemispheric Oscillations on the 35—60 Day Time Scale

    Source: Journal of the Atmospheric Sciences:;1988:;Volume( 046 ):;issue: 012::page 1826
    Author:
    Graves, Charles E.
    ,
    Stanford, John L.
    DOI: 10.1175/1520-0469(1989)046<1826:MAHLSH>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Geopotential height fluctuations are examined in the extratropical Southern Hemisphere on the 35?60 day time scale. These fluctuations, in 200 mb geopotential height one-point correlation maps and anomaly maps, are shown to behave like quasi-stationary wavetrains with eastward energy propagation. The wavetrains follow an elliptically shaped circuit identifiable from low Southern latitudes in the Indian Ocean to the coast of Antarctica near 70°W. Weak correlations are found between the midlatitude wavetrain and 35?60 day brightness temperatures over the Indian Ocean. Nevertheless, a puzzling lack of correlation exists between the midlatitude 35?60 day signals and the anticipated subtropical wavetrain entry?exit region south of the tropical correlations. Eliassen?Palm flux calculations reveal strong momentum fluxes in the upper troposphere while the divergence is mostly negative throughout the troposphere. These observational results constitute several tests for models, viz., the existence and amplification of the midlatitude fluctuations and their quasi-stationary nature.
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      Middle and High Latitude Southern Hemispheric Oscillations on the 35—60 Day Time Scale

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4156297
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    contributor authorGraves, Charles E.
    contributor authorStanford, John L.
    date accessioned2017-06-09T14:29:04Z
    date available2017-06-09T14:29:04Z
    date copyright1989/06/01
    date issued1988
    identifier issn0022-4928
    identifier otherams-20105.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4156297
    description abstractGeopotential height fluctuations are examined in the extratropical Southern Hemisphere on the 35?60 day time scale. These fluctuations, in 200 mb geopotential height one-point correlation maps and anomaly maps, are shown to behave like quasi-stationary wavetrains with eastward energy propagation. The wavetrains follow an elliptically shaped circuit identifiable from low Southern latitudes in the Indian Ocean to the coast of Antarctica near 70°W. Weak correlations are found between the midlatitude wavetrain and 35?60 day brightness temperatures over the Indian Ocean. Nevertheless, a puzzling lack of correlation exists between the midlatitude 35?60 day signals and the anticipated subtropical wavetrain entry?exit region south of the tropical correlations. Eliassen?Palm flux calculations reveal strong momentum fluxes in the upper troposphere while the divergence is mostly negative throughout the troposphere. These observational results constitute several tests for models, viz., the existence and amplification of the midlatitude fluctuations and their quasi-stationary nature.
    publisherAmerican Meteorological Society
    titleMiddle and High Latitude Southern Hemispheric Oscillations on the 35—60 Day Time Scale
    typeJournal Paper
    journal volume46
    journal issue12
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1989)046<1826:MAHLSH>2.0.CO;2
    journal fristpage1826
    journal lastpage1837
    treeJournal of the Atmospheric Sciences:;1988:;Volume( 046 ):;issue: 012
    contenttypeFulltext
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