Uncertainties and assessments of chemistry-climate models of the stratosphere

In recent years a number of chemistry-climate models have been developed with an emphasis on the stratosphere. Such models cover a wide range of time scales of integration and vary considerably in complexity. The results of specific diagnostics are here analysed to examine the differences amongst in...

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Main Authors: Austin, J., Shindell, Drew, Beagley, Stephen R., Brühl, Christoph, Dameris, Martin, Manzini, Elisa, Nagashima, Tatsuya, Newman, Paul, Pawson, Steven, Pitari, Giovanni, Rozanov, Eugene, Schnadt, Christina, Shepherd, Theodore G.
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus 2003
Subjects:
Online Access:https://hdl.handle.net/20.500.11850/57487
https://doi.org/10.3929/ethz-b-000057487
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author Austin, J.
Shindell, Drew
Beagley, Stephen R.
Brühl, Christoph
Dameris, Martin
Manzini, Elisa
Nagashima, Tatsuya
Newman, Paul
Pawson, Steven
Pitari, Giovanni
Rozanov, Eugene
Schnadt, Christina
Shepherd, Theodore G.
author_facet Austin, J.
Shindell, Drew
Beagley, Stephen R.
Brühl, Christoph
Dameris, Martin
Manzini, Elisa
Nagashima, Tatsuya
Newman, Paul
Pawson, Steven
Pitari, Giovanni
Rozanov, Eugene
Schnadt, Christina
Shepherd, Theodore G.
author_sort Austin, J.
collection ETH Zürich Research Collection
description In recent years a number of chemistry-climate models have been developed with an emphasis on the stratosphere. Such models cover a wide range of time scales of integration and vary considerably in complexity. The results of specific diagnostics are here analysed to examine the differences amongst individual models and observations, to assess the consistency of model predictions, with a particular focus on polar ozone. For example, many models indicate a significant cold bias in high latitudes, the "cold pole problem", particularly in the southern hemisphere during winter and spring. This is related to wave propagation from the troposphere which can be improved by improving model horizontal resolution and with the use of non-orographic gravity wave drag. As a result of the widely differing modelled polar temperatures, different amounts of polar stratospheric clouds are simulated which in turn result in varying ozone values in the models. The results are also compared to determine the possible future behaviour of ozone, with an emphasis on the polar regions and mid-latitudes. All models predict eventual ozone recovery, but give a range of results concerning its timing and extent. Differences in the simulation of gravity waves and planetary waves as well as model resolution are likely major sources of uncertainty for this issue. In the Antarctic, the ozone hole has probably reached almost its deepest although the vertical and horizontal extent of depletion may increase slightly further over the next few years. According to the model results, Antarctic ozone recovery could begin any year within the range 2001 to 2008. The limited number of models which have been integrated sufficiently far indicate that full recovery of ozone to 1980 levels may not occur in the Antarctic until about the year 2050. For the Arctic, most models indicate that small ozone losses may continue for a few more years and that recovery could begin any year within the range 2004 to 2019. The start of ozone recovery in the Arctic is therefore ...
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Arctic
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geographic Antarctic
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op_doi https://doi.org/20.500.11850/5748710.3929/ethz-b-00005748710.5194/acp-3-1-2003
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spelling ftethz:oai:www.research-collection.ethz.ch:20.500.11850/57487 2025-03-30T14:53:32+00:00 Uncertainties and assessments of chemistry-climate models of the stratosphere Austin, J. Shindell, Drew Beagley, Stephen R. Brühl, Christoph Dameris, Martin Manzini, Elisa Nagashima, Tatsuya Newman, Paul Pawson, Steven Pitari, Giovanni Rozanov, Eugene Schnadt, Christina Shepherd, Theodore G. 2003 application/application/pdf https://hdl.handle.net/20.500.11850/57487 https://doi.org/10.3929/ethz-b-000057487 en eng Copernicus info:eu-repo/semantics/altIdentifier/doi/10.5194/acp-3-1-2003 info:eu-repo/semantics/altIdentifier/wos/000180329600001 http://hdl.handle.net/20.500.11850/57487 info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/2.5/ Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic Atmospheric Chemistry and Physics, 3 info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2003 ftethz https://doi.org/20.500.11850/5748710.3929/ethz-b-00005748710.5194/acp-3-1-2003 2025-03-05T22:09:17Z In recent years a number of chemistry-climate models have been developed with an emphasis on the stratosphere. Such models cover a wide range of time scales of integration and vary considerably in complexity. The results of specific diagnostics are here analysed to examine the differences amongst individual models and observations, to assess the consistency of model predictions, with a particular focus on polar ozone. For example, many models indicate a significant cold bias in high latitudes, the "cold pole problem", particularly in the southern hemisphere during winter and spring. This is related to wave propagation from the troposphere which can be improved by improving model horizontal resolution and with the use of non-orographic gravity wave drag. As a result of the widely differing modelled polar temperatures, different amounts of polar stratospheric clouds are simulated which in turn result in varying ozone values in the models. The results are also compared to determine the possible future behaviour of ozone, with an emphasis on the polar regions and mid-latitudes. All models predict eventual ozone recovery, but give a range of results concerning its timing and extent. Differences in the simulation of gravity waves and planetary waves as well as model resolution are likely major sources of uncertainty for this issue. In the Antarctic, the ozone hole has probably reached almost its deepest although the vertical and horizontal extent of depletion may increase slightly further over the next few years. According to the model results, Antarctic ozone recovery could begin any year within the range 2001 to 2008. The limited number of models which have been integrated sufficiently far indicate that full recovery of ozone to 1980 levels may not occur in the Antarctic until about the year 2050. For the Arctic, most models indicate that small ozone losses may continue for a few more years and that recovery could begin any year within the range 2004 to 2019. The start of ozone recovery in the Arctic is therefore ... Article in Journal/Newspaper Antarc* Antarctic Arctic ETH Zürich Research Collection Antarctic Arctic The Antarctic
spellingShingle Austin, J.
Shindell, Drew
Beagley, Stephen R.
Brühl, Christoph
Dameris, Martin
Manzini, Elisa
Nagashima, Tatsuya
Newman, Paul
Pawson, Steven
Pitari, Giovanni
Rozanov, Eugene
Schnadt, Christina
Shepherd, Theodore G.
Uncertainties and assessments of chemistry-climate models of the stratosphere
title Uncertainties and assessments of chemistry-climate models of the stratosphere
title_full Uncertainties and assessments of chemistry-climate models of the stratosphere
title_fullStr Uncertainties and assessments of chemistry-climate models of the stratosphere
title_full_unstemmed Uncertainties and assessments of chemistry-climate models of the stratosphere
title_short Uncertainties and assessments of chemistry-climate models of the stratosphere
title_sort uncertainties and assessments of chemistry-climate models of the stratosphere
url https://hdl.handle.net/20.500.11850/57487
https://doi.org/10.3929/ethz-b-000057487