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    Spring-to-Summer Transitions of Global Circulations during May–July 1979

    Source: Monthly Weather Review:;1987:;volume( 115 ):;issue: 009::page 2088
    Author:
    Nogues-Paegle, Julia
    ,
    Mo, Kingtse
    DOI: 10.1175/1520-0493(1987)115<2088:STSTOG>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: The seasonal transition from spring to summer in the Northern Hemisphere and from fall to winter in the Southern Hemisphere is studied for 1979 using gridded datasets produced by the Goddard Laboratory for Atmospheres. Winds at 200, 500 and 850 mb are decomposed into their rotational and divergent components. The streamfunction (?), velocity potential (?), and height fields (Z) are projected onto spherical harmonics to quantify the behavior of the lowest-order planetary modes. Comparison of the planetary scales with those at full resolution reveals that the low-order truncation represents over half of the total energy at 200 mb and that zonal deviations dominate the week-to-week time changes. The velocity potential spectrum is dominated by the wave component of largest meridional and zonal scale (?11). This mode exhibits a clear eastward propagation, circling the globe in about six weeks. This propagation is discussed in connection with observed changes of outgoing longwave radiation and related to the 30?60 day oscillation, which exhibited a strong signal during the 1979 summer season. It is found that ?11, ?21 and Z41 propagate with similar phase speeds, linking the planetary scale divergent patterns with those of the rotational flow and height field. The streamfunction is found to contain more of the 30?60 oscillation signal than the height fields for global scales. Analyses of outgoing longwave radiation and velocity potential at 5°N at full resolution are compared with the zonal wind at 34°S. It is found that the divergence pulse and low values of outgoing longwave radiation are observed up to one week before zonal-wind acceleration. These accelerations peak when the divergence pulse is at about 160°E, with high values of the subtropical jet at similar longitudes. Removal of the seasonally averaged circulation from the weekly averages reveals a dominant baroclinic structure, with the 250- to 850-mb wind shear exceeding the vertically averaged wind over extensive areas, which extend for particular weeks to the polar caps. A dominant barotropic structure emerges when the basic sate is included. The seasonal transition is found to occur abruptly during the middle of the 12-week periods considered here, with pronounced rearrangements of global patterns due to excitation of planetary scales.
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      Spring-to-Summer Transitions of Global Circulations during May–July 1979

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    contributor authorNogues-Paegle, Julia
    contributor authorMo, Kingtse
    date accessioned2017-06-09T16:06:27Z
    date available2017-06-09T16:06:27Z
    date copyright1987/09/01
    date issued1987
    identifier issn0027-0644
    identifier otherams-61090.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4201832
    description abstractThe seasonal transition from spring to summer in the Northern Hemisphere and from fall to winter in the Southern Hemisphere is studied for 1979 using gridded datasets produced by the Goddard Laboratory for Atmospheres. Winds at 200, 500 and 850 mb are decomposed into their rotational and divergent components. The streamfunction (?), velocity potential (?), and height fields (Z) are projected onto spherical harmonics to quantify the behavior of the lowest-order planetary modes. Comparison of the planetary scales with those at full resolution reveals that the low-order truncation represents over half of the total energy at 200 mb and that zonal deviations dominate the week-to-week time changes. The velocity potential spectrum is dominated by the wave component of largest meridional and zonal scale (?11). This mode exhibits a clear eastward propagation, circling the globe in about six weeks. This propagation is discussed in connection with observed changes of outgoing longwave radiation and related to the 30?60 day oscillation, which exhibited a strong signal during the 1979 summer season. It is found that ?11, ?21 and Z41 propagate with similar phase speeds, linking the planetary scale divergent patterns with those of the rotational flow and height field. The streamfunction is found to contain more of the 30?60 oscillation signal than the height fields for global scales. Analyses of outgoing longwave radiation and velocity potential at 5°N at full resolution are compared with the zonal wind at 34°S. It is found that the divergence pulse and low values of outgoing longwave radiation are observed up to one week before zonal-wind acceleration. These accelerations peak when the divergence pulse is at about 160°E, with high values of the subtropical jet at similar longitudes. Removal of the seasonally averaged circulation from the weekly averages reveals a dominant baroclinic structure, with the 250- to 850-mb wind shear exceeding the vertically averaged wind over extensive areas, which extend for particular weeks to the polar caps. A dominant barotropic structure emerges when the basic sate is included. The seasonal transition is found to occur abruptly during the middle of the 12-week periods considered here, with pronounced rearrangements of global patterns due to excitation of planetary scales.
    publisherAmerican Meteorological Society
    titleSpring-to-Summer Transitions of Global Circulations during May–July 1979
    typeJournal Paper
    journal volume115
    journal issue9
    journal titleMonthly Weather Review
    identifier doi10.1175/1520-0493(1987)115<2088:STSTOG>2.0.CO;2
    journal fristpage2088
    journal lastpage2102
    treeMonthly Weather Review:;1987:;volume( 115 ):;issue: 009
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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