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    An Estimate of the Chemical and Radiative Perturbation of Stratospheric Ozone Following the Eruption of Mt. Pinatubo

    Source: Journal of the Atmospheric Sciences:;1993:;Volume( 050 ):;issue: 019::page 3260
    Author:
    Pitari, G.
    ,
    Rizi, V.
    DOI: 10.1175/1520-0469(1993)050<3260:AEOTCA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: In this work a numerical assessment is attempted of trace species interactions with aerosols injected in the stratosphere by the eruption of Mt. Pinatubo. A photochemical two-dimensional model is used for this purpose, with heterogeneous chemical conversion of odd nitrogen into nitric acid taken as the basic perturbation on nitrogen, chlorine, and ozone. In addition, it is shown that the radiative perturbation induced by the aerosols is an important depletion mechanism for ozone at least at tropical latitudes where the optical thickness of volcanic particles has remained sufficiently high for several months after the eruption. The radiative interaction with stratospheric trace species not only takes place through changes in photodissociation frequency but is also a consequence of solar and planetary radiation absorption by the aerosol particles. The resulting heating rates produce a nonnegligible equatorial upwelling whose effects on dynamics and transport have been studied using a three-dimensional model. They are presented here, along with photochemical calculations, in order to assess the different contributions to the ozone depletion after the eruption. The magnitude of the radiative perturbation is found to be comparable to that of heterogeneous chemistry except at the northern midlatitudes during winter and spring where the chemical perturbation dominates. In addition, the radiative perturbation is found to be largely determined by photolysis in the tropics, while the effects on circulation are most significant at high latitudes. The total radiative effect on the ozone column is that of an ?5% depletion in the tropics along with a wintertime increase poleward of 50° latitude (about 4%?6% in the Northern Hemisphere). Both magnitude and features of the ozone depletion resulting from this numerical calculation are successfully compared to recent observations taken at tropical latitudes during 1991.
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      An Estimate of the Chemical and Radiative Perturbation of Stratospheric Ozone Following the Eruption of Mt. Pinatubo

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4157338
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    contributor authorPitari, G.
    contributor authorRizi, V.
    date accessioned2017-06-09T14:31:50Z
    date available2017-06-09T14:31:50Z
    date copyright1993/10/01
    date issued1993
    identifier issn0022-4928
    identifier otherams-21042.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4157338
    description abstractIn this work a numerical assessment is attempted of trace species interactions with aerosols injected in the stratosphere by the eruption of Mt. Pinatubo. A photochemical two-dimensional model is used for this purpose, with heterogeneous chemical conversion of odd nitrogen into nitric acid taken as the basic perturbation on nitrogen, chlorine, and ozone. In addition, it is shown that the radiative perturbation induced by the aerosols is an important depletion mechanism for ozone at least at tropical latitudes where the optical thickness of volcanic particles has remained sufficiently high for several months after the eruption. The radiative interaction with stratospheric trace species not only takes place through changes in photodissociation frequency but is also a consequence of solar and planetary radiation absorption by the aerosol particles. The resulting heating rates produce a nonnegligible equatorial upwelling whose effects on dynamics and transport have been studied using a three-dimensional model. They are presented here, along with photochemical calculations, in order to assess the different contributions to the ozone depletion after the eruption. The magnitude of the radiative perturbation is found to be comparable to that of heterogeneous chemistry except at the northern midlatitudes during winter and spring where the chemical perturbation dominates. In addition, the radiative perturbation is found to be largely determined by photolysis in the tropics, while the effects on circulation are most significant at high latitudes. The total radiative effect on the ozone column is that of an ?5% depletion in the tropics along with a wintertime increase poleward of 50° latitude (about 4%?6% in the Northern Hemisphere). Both magnitude and features of the ozone depletion resulting from this numerical calculation are successfully compared to recent observations taken at tropical latitudes during 1991.
    publisherAmerican Meteorological Society
    titleAn Estimate of the Chemical and Radiative Perturbation of Stratospheric Ozone Following the Eruption of Mt. Pinatubo
    typeJournal Paper
    journal volume50
    journal issue19
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(1993)050<3260:AEOTCA>2.0.CO;2
    journal fristpage3260
    journal lastpage3276
    treeJournal of the Atmospheric Sciences:;1993:;Volume( 050 ):;issue: 019
    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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