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    Teleconnection Pathways of ENSO and the IOD and the Mechanisms for Impacts on Australian Rainfall

    Source: Journal of Climate:;2011:;volume( 024 ):;issue: 015::page 3910
    Author:
    Cai, Wenju
    ,
    van Rensch, Peter
    ,
    Cowan, Tim
    ,
    Hendon, Harry H.
    DOI: 10.1175/2011JCLI4129.1
    Publisher: American Meteorological Society
    Abstract: mpacts of El Niño?Southern Oscillation (ENSO) and the Indian Ocean dipole (IOD) on Australian rainfall are diagnosed from the perspective of tropical and extratropical teleconnections triggered by tropical sea surface temperature (SST) variations. The tropical teleconnection is understood as the equatorially trapped, deep baroclinic response to the diabatic (convective) heating anomalies induced by the tropical SST anomalies. These diabatic heating anomalies also excite equivalent barotropic Rossby wave trains that propagate into the extratropics. The main direct tropical teleconnection during ENSO is the Southern Oscillation (SO), whose impact on Australian rainfall is argued to be mainly confined to near-tropical portions of eastern Australia. Rainfall is suppressed during El Niño because near-tropical eastern Australia directly experiences subsidence and higher surface pressure associated with the western pole of the SO. Impacts on extratropical Australian rainfall during El Niño are argued to stem primarily from the Rossby wave trains forced by convective variations in the Indian Ocean, for which the IOD is a primary source of variability. These equivalent-barotropic Rossby wave trains emanating from the Indian Ocean induce changes to the midlatitude westerlies across southern Australia, thereby affecting rainfall through changes in mean-state baroclinicity, west?east steering, and possibly orographic effects. Although the IOD does not mature until austral spring, its impact on Australian rainfall during winter is also ascribed to this mechanism. Because ENSO is largely unrelated to the IOD during austral winter, there is limited impact of ENSO on rainfall across southern latitudes of Australia in winter. A strong impact of ENSO on southern Australia rainfall in spring is ascribed to the strong covariation of ENSO and the IOD in this season. Implications of this pathway from the tropical Indian Ocean for impacts of both the IOD and ENSO on southern Australian climate are discussed with regard to the ability to make seasonal climate predictions and with regard to the role of trends in tropical SST for driving trends in Australian climate.
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      Teleconnection Pathways of ENSO and the IOD and the Mechanisms for Impacts on Australian Rainfall

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4213874
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    contributor authorCai, Wenju
    contributor authorvan Rensch, Peter
    contributor authorCowan, Tim
    contributor authorHendon, Harry H.
    date accessioned2017-06-09T16:40:17Z
    date available2017-06-09T16:40:17Z
    date copyright2011/08/01
    date issued2011
    identifier issn0894-8755
    identifier otherams-71928.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4213874
    description abstractmpacts of El Niño?Southern Oscillation (ENSO) and the Indian Ocean dipole (IOD) on Australian rainfall are diagnosed from the perspective of tropical and extratropical teleconnections triggered by tropical sea surface temperature (SST) variations. The tropical teleconnection is understood as the equatorially trapped, deep baroclinic response to the diabatic (convective) heating anomalies induced by the tropical SST anomalies. These diabatic heating anomalies also excite equivalent barotropic Rossby wave trains that propagate into the extratropics. The main direct tropical teleconnection during ENSO is the Southern Oscillation (SO), whose impact on Australian rainfall is argued to be mainly confined to near-tropical portions of eastern Australia. Rainfall is suppressed during El Niño because near-tropical eastern Australia directly experiences subsidence and higher surface pressure associated with the western pole of the SO. Impacts on extratropical Australian rainfall during El Niño are argued to stem primarily from the Rossby wave trains forced by convective variations in the Indian Ocean, for which the IOD is a primary source of variability. These equivalent-barotropic Rossby wave trains emanating from the Indian Ocean induce changes to the midlatitude westerlies across southern Australia, thereby affecting rainfall through changes in mean-state baroclinicity, west?east steering, and possibly orographic effects. Although the IOD does not mature until austral spring, its impact on Australian rainfall during winter is also ascribed to this mechanism. Because ENSO is largely unrelated to the IOD during austral winter, there is limited impact of ENSO on rainfall across southern latitudes of Australia in winter. A strong impact of ENSO on southern Australia rainfall in spring is ascribed to the strong covariation of ENSO and the IOD in this season. Implications of this pathway from the tropical Indian Ocean for impacts of both the IOD and ENSO on southern Australian climate are discussed with regard to the ability to make seasonal climate predictions and with regard to the role of trends in tropical SST for driving trends in Australian climate.
    publisherAmerican Meteorological Society
    titleTeleconnection Pathways of ENSO and the IOD and the Mechanisms for Impacts on Australian Rainfall
    typeJournal Paper
    journal volume24
    journal issue15
    journal titleJournal of Climate
    identifier doi10.1175/2011JCLI4129.1
    journal fristpage3910
    journal lastpage3923
    treeJournal of Climate:;2011:;volume( 024 ):;issue: 015
    contenttypeFulltext
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