The simulation of the Antarctic ozone hole by chemistry-climate models

While chemistry-climate models are able to reproduce many characteristics of the global total column ozone field and its long-term evolution, they have fared less well in simulating the commonly used diagnostic of the area of the Antarctic ozone hole i.e. the area within the 220 Dobson Unit (DU) con...

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Main Authors: Struthers, Hamish, Bodeker, Gregory E., Austin, John, Bekki, Slimane, Cionni, Irene, Dameris, Martin, Giorgetta, Marco, Grewe, Volker, Lefèvre, Franck, Lott, François, Manzini, Elisa, Peter, Thomas, Rozanov, Eugene, Schraner, Martin
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus 2009
Subjects:
Online Access:https://hdl.handle.net/20.500.11850/157204
https://doi.org/10.3929/ethz-b-000157204
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author Struthers, Hamish
Bodeker, Gregory E.
Austin, John
Bekki, Slimane
Cionni, Irene
Dameris, Martin
Giorgetta, Marco
Grewe, Volker
Lefèvre, Franck
Lott, François
Manzini, Elisa
Peter, Thomas
Rozanov, Eugene
Schraner, Martin
author_facet Struthers, Hamish
Bodeker, Gregory E.
Austin, John
Bekki, Slimane
Cionni, Irene
Dameris, Martin
Giorgetta, Marco
Grewe, Volker
Lefèvre, Franck
Lott, François
Manzini, Elisa
Peter, Thomas
Rozanov, Eugene
Schraner, Martin
author_sort Struthers, Hamish
collection ETH Zürich Research Collection
description While chemistry-climate models are able to reproduce many characteristics of the global total column ozone field and its long-term evolution, they have fared less well in simulating the commonly used diagnostic of the area of the Antarctic ozone hole i.e. the area within the 220 Dobson Unit (DU) contour. Two possible reasons for this are: (1) the underlying Global Climate Model (GCM) does not correctly simulate the size of the polar vortex, and (2) the stratospheric chemistry scheme incorporated into the GCM, and/or the model dynamics, results in systematic biases in the total column ozone fields such that the 220 DU contour is no longer appropriate for delineating the edge of the ozone hole. Both causes are examined here with a view to developing ozone hole area diagnostics that better suit measurement-model inter-comparisons. The interplay between the shape of the meridional mixing barrier at the edge of the vortex and the meridional gradients in total column ozone across the vortex edge is investigated in measurements and in 5 chemistry-climate models (CCMs). Analysis of the simulation of the polar vortex in the CCMs shows that the first of the two possible causes does play a role in some models. This in turn affects the ability of the models to simulate the large observed meridional gradients in total column ozone. The second of the two causes also strongly affects the ability of the CCMs to track the observed size of the ozone hole. It is shown that by applying a common algorithm to the CCMs for selecting a delineating threshold unique to each model, a more appropriate diagnostic of ozone hole area can be generated that shows better agreement with that derived from observations. ISSN:1680-7324 ISSN:1680-7375
format Article in Journal/Newspaper
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
id ftethz:oai:www.research-collection.ethz.ch:20.500.11850/157204
institution Open Polar
language English
op_collection_id ftethz
op_doi https://doi.org/20.500.11850/15720410.3929/ethz-b-00015720410.5194/acp-9-6363-2009
op_relation info:eu-repo/semantics/altIdentifier/doi/10.5194/acp-9-6363-2009
info:eu-repo/semantics/altIdentifier/wos/000269778500006
http://hdl.handle.net/20.500.11850/157204
op_rights info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/3.0/
Creative Commons Attribution 3.0 Unported
op_source Atmospheric Chemistry and Physics, 9 (17)
publishDate 2009
publisher Copernicus
record_format openpolar
spelling ftethz:oai:www.research-collection.ethz.ch:20.500.11850/157204 2025-03-30T14:54:23+00:00 The simulation of the Antarctic ozone hole by chemistry-climate models Struthers, Hamish Bodeker, Gregory E. Austin, John Bekki, Slimane Cionni, Irene Dameris, Martin Giorgetta, Marco Grewe, Volker Lefèvre, Franck Lott, François Manzini, Elisa Peter, Thomas Rozanov, Eugene Schraner, Martin 2009 application/application/pdf https://hdl.handle.net/20.500.11850/157204 https://doi.org/10.3929/ethz-b-000157204 en eng Copernicus info:eu-repo/semantics/altIdentifier/doi/10.5194/acp-9-6363-2009 info:eu-repo/semantics/altIdentifier/wos/000269778500006 http://hdl.handle.net/20.500.11850/157204 info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/3.0/ Creative Commons Attribution 3.0 Unported Atmospheric Chemistry and Physics, 9 (17) info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2009 ftethz https://doi.org/20.500.11850/15720410.3929/ethz-b-00015720410.5194/acp-9-6363-2009 2025-03-05T22:09:14Z While chemistry-climate models are able to reproduce many characteristics of the global total column ozone field and its long-term evolution, they have fared less well in simulating the commonly used diagnostic of the area of the Antarctic ozone hole i.e. the area within the 220 Dobson Unit (DU) contour. Two possible reasons for this are: (1) the underlying Global Climate Model (GCM) does not correctly simulate the size of the polar vortex, and (2) the stratospheric chemistry scheme incorporated into the GCM, and/or the model dynamics, results in systematic biases in the total column ozone fields such that the 220 DU contour is no longer appropriate for delineating the edge of the ozone hole. Both causes are examined here with a view to developing ozone hole area diagnostics that better suit measurement-model inter-comparisons. The interplay between the shape of the meridional mixing barrier at the edge of the vortex and the meridional gradients in total column ozone across the vortex edge is investigated in measurements and in 5 chemistry-climate models (CCMs). Analysis of the simulation of the polar vortex in the CCMs shows that the first of the two possible causes does play a role in some models. This in turn affects the ability of the models to simulate the large observed meridional gradients in total column ozone. The second of the two causes also strongly affects the ability of the CCMs to track the observed size of the ozone hole. It is shown that by applying a common algorithm to the CCMs for selecting a delineating threshold unique to each model, a more appropriate diagnostic of ozone hole area can be generated that shows better agreement with that derived from observations. ISSN:1680-7324 ISSN:1680-7375 Article in Journal/Newspaper Antarc* Antarctic ETH Zürich Research Collection Antarctic The Antarctic
spellingShingle Struthers, Hamish
Bodeker, Gregory E.
Austin, John
Bekki, Slimane
Cionni, Irene
Dameris, Martin
Giorgetta, Marco
Grewe, Volker
Lefèvre, Franck
Lott, François
Manzini, Elisa
Peter, Thomas
Rozanov, Eugene
Schraner, Martin
The simulation of the Antarctic ozone hole by chemistry-climate models
title The simulation of the Antarctic ozone hole by chemistry-climate models
title_full The simulation of the Antarctic ozone hole by chemistry-climate models
title_fullStr The simulation of the Antarctic ozone hole by chemistry-climate models
title_full_unstemmed The simulation of the Antarctic ozone hole by chemistry-climate models
title_short The simulation of the Antarctic ozone hole by chemistry-climate models
title_sort simulation of the antarctic ozone hole by chemistry-climate models
url https://hdl.handle.net/20.500.11850/157204
https://doi.org/10.3929/ethz-b-000157204