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    Propagation and the Vertical Structure of the Madden–Julian Oscillation

    Source: Monthly Weather Review:;2003:;volume( 131 ):;issue: 012::page 3018
    Author:
    Sperber, Kenneth R.
    DOI: 10.1175/1520-0493(2003)131<3018:PATVSO>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The Madden?Julian oscillation (MJO) dominates tropical variability on time scales of 30?70 days. During the boreal winter?spring it is manifested as an eastward propagating disturbance, with a strong convective signature over the Eastern Hemisphere. The space?time structure of the MJO is described using the National Centers for Environmental Prediction?National Center for Atmospheric Research reanalysis, Advanced Very High Resolution Radiometer outgoing longwave radiation, observed sea surface temperature, and the Climate Prediction Center Merged Analysis of Precipitation. Empirical orthogonal function analysis is used to identify the convective signature of the MJO, and regression is used to identify key relationships with the convection. Compared to analyzing successive years of data, the selection of years of strong MJO activity results in a more robust lead?lag structure and an increase in explained variance. The MJO exhibits a rich vertical structure, with low-level moisture convergence being well defined when the convective anomalies are strong, and there is evidence that free-tropospheric processes also play a role in the MJO life cycle. The westward vertical tilt is most apparent over the western Pacific. Over the Indian Ocean the system is more vertically stacked, principally because of the strong subsidence of the inactive phase of the MJO, which lies to the east of the convection. As the Kelvin wave decouples from the convection near the date line, a sea level low pressure surge, previously discussed by A. J. Matthews, transits the eastern Pacific and Atlantic Oceans. Here the link of the zonal wind stress and low-level divergence to the pressure surge is explored. The pressure gradient gives rise to westerlies that propagate rapidly to the east, and it may play role in the development of the MJO convection in the western Indian Ocean, which occurs in an easterly basic state, and conditions not consistent with the low-level moisture convergence paradigm.
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      Propagation and the Vertical Structure of the Madden–Julian Oscillation

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4205282
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    contributor authorSperber, Kenneth R.
    date accessioned2017-06-09T16:15:10Z
    date available2017-06-09T16:15:10Z
    date copyright2003/12/01
    date issued2003
    identifier issn0027-0644
    identifier otherams-64195.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4205282
    description abstractThe Madden?Julian oscillation (MJO) dominates tropical variability on time scales of 30?70 days. During the boreal winter?spring it is manifested as an eastward propagating disturbance, with a strong convective signature over the Eastern Hemisphere. The space?time structure of the MJO is described using the National Centers for Environmental Prediction?National Center for Atmospheric Research reanalysis, Advanced Very High Resolution Radiometer outgoing longwave radiation, observed sea surface temperature, and the Climate Prediction Center Merged Analysis of Precipitation. Empirical orthogonal function analysis is used to identify the convective signature of the MJO, and regression is used to identify key relationships with the convection. Compared to analyzing successive years of data, the selection of years of strong MJO activity results in a more robust lead?lag structure and an increase in explained variance. The MJO exhibits a rich vertical structure, with low-level moisture convergence being well defined when the convective anomalies are strong, and there is evidence that free-tropospheric processes also play a role in the MJO life cycle. The westward vertical tilt is most apparent over the western Pacific. Over the Indian Ocean the system is more vertically stacked, principally because of the strong subsidence of the inactive phase of the MJO, which lies to the east of the convection. As the Kelvin wave decouples from the convection near the date line, a sea level low pressure surge, previously discussed by A. J. Matthews, transits the eastern Pacific and Atlantic Oceans. Here the link of the zonal wind stress and low-level divergence to the pressure surge is explored. The pressure gradient gives rise to westerlies that propagate rapidly to the east, and it may play role in the development of the MJO convection in the western Indian Ocean, which occurs in an easterly basic state, and conditions not consistent with the low-level moisture convergence paradigm.
    publisherAmerican Meteorological Society
    titlePropagation and the Vertical Structure of the Madden–Julian Oscillation
    typeJournal Paper
    journal volume131
    journal issue12
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(2003)131<3018:PATVSO>2.0.CO;2
    journal fristpage3018
    journal lastpage3037
    treeMonthly Weather Review:;2003:;volume( 131 ):;issue: 012
    contenttypeFulltext
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