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    Reconstruction and Simulation of Stratospheric Ozone Distributions during the 2002 Austral Winter

    Source: Journal of the Atmospheric Sciences:;2005:;Volume( 062 ):;issue: 003::page 748
    Author:
    Randall, C. E.
    ,
    Manney, G. L.
    ,
    Allen, D. R.
    ,
    Bevilacqua, R. M.
    ,
    Hornstein, J.
    ,
    Trepte, C.
    ,
    Lahoz, W.
    ,
    Ajtic, J.
    ,
    Bodeker, G.
    DOI: 10.1175/JAS-3336.1
    Publisher: American Meteorological Society
    Abstract: Satellite-based solar occultation measurements during the 2002 austral winter have been used to reconstruct global, three-dimensional ozone distributions. The reconstruction method uses correlations between potential vorticity and ozone to derive ?proxy? distributions from the geographically limited occultation observations. Ozone profiles from the Halogen Occultation Experiment (HALOE), the Polar Ozone and Aerosol Measurement III (POAM III), and the Stratospheric Aerosol and Gas Experiment II and III (SAGE II and III) are incorporated into the analysis. Because this is one of the first uses of SAGE III data in a scientific analysis, preliminary validation results are shown. The reconstruction method is described, with particular emphasis on uncertainties caused by noisy and/or multivalued correlations. The evolution of the solar occultation data and proxy ozone fields throughout the winter is described, and differences with respect to previous winters are characterized. The results support the idea that dynamical forcing early in the 2002 winter influenced the morphology of the stratosphere in a significant and unusual manner, possibly setting the stage for the unprecedented major stratospheric warming in late September. The proxy is compared with ozone from mechanistic, primitive equation model simulations of passive ozone tracer fields during the time of the warming. In regions where chemistry is negligible compared to transport, the model and proxy ozone fields agree well. The agreement between, and changes in, the large-scale ozone fields in the model and proxy indicate that transport processes, particularly enhanced poleward transport and mixing, are the primary cause of ozone changes through most of the stratosphere during this unprecedented event. The analysis culminates with the calculation of globally distributed column ozone during the major warming, showing quantitatively how transport of low-latitude air to the polar region in the middle stratosphere led to the diminished ozone hole in 2002.
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      Reconstruction and Simulation of Stratospheric Ozone Distributions during the 2002 Austral Winter

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4217872
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    contributor authorRandall, C. E.
    contributor authorManney, G. L.
    contributor authorAllen, D. R.
    contributor authorBevilacqua, R. M.
    contributor authorHornstein, J.
    contributor authorTrepte, C.
    contributor authorLahoz, W.
    contributor authorAjtic, J.
    contributor authorBodeker, G.
    date accessioned2017-06-09T16:51:55Z
    date available2017-06-09T16:51:55Z
    date copyright2005/03/01
    date issued2005
    identifier issn0022-4928
    identifier otherams-75526.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4217872
    description abstractSatellite-based solar occultation measurements during the 2002 austral winter have been used to reconstruct global, three-dimensional ozone distributions. The reconstruction method uses correlations between potential vorticity and ozone to derive ?proxy? distributions from the geographically limited occultation observations. Ozone profiles from the Halogen Occultation Experiment (HALOE), the Polar Ozone and Aerosol Measurement III (POAM III), and the Stratospheric Aerosol and Gas Experiment II and III (SAGE II and III) are incorporated into the analysis. Because this is one of the first uses of SAGE III data in a scientific analysis, preliminary validation results are shown. The reconstruction method is described, with particular emphasis on uncertainties caused by noisy and/or multivalued correlations. The evolution of the solar occultation data and proxy ozone fields throughout the winter is described, and differences with respect to previous winters are characterized. The results support the idea that dynamical forcing early in the 2002 winter influenced the morphology of the stratosphere in a significant and unusual manner, possibly setting the stage for the unprecedented major stratospheric warming in late September. The proxy is compared with ozone from mechanistic, primitive equation model simulations of passive ozone tracer fields during the time of the warming. In regions where chemistry is negligible compared to transport, the model and proxy ozone fields agree well. The agreement between, and changes in, the large-scale ozone fields in the model and proxy indicate that transport processes, particularly enhanced poleward transport and mixing, are the primary cause of ozone changes through most of the stratosphere during this unprecedented event. The analysis culminates with the calculation of globally distributed column ozone during the major warming, showing quantitatively how transport of low-latitude air to the polar region in the middle stratosphere led to the diminished ozone hole in 2002.
    publisherAmerican Meteorological Society
    titleReconstruction and Simulation of Stratospheric Ozone Distributions during the 2002 Austral Winter
    typeJournal Paper
    journal volume62
    journal issue3
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/JAS-3336.1
    journal fristpage748
    journal lastpage764
    treeJournal of the Atmospheric Sciences:;2005:;Volume( 062 ):;issue: 003
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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