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...
Main Authors: | , , , , , , , , , , , , , |
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Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Copernicus
2009
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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 |