Long-term ozone changes and associated climate impacts in CMIP5 simulations

International audience Ozone changes and associated climate impacts in the Coupled Model Intercomparison Project Phase 5 (CMIP5) simulations are analyzed over the historical (1960-2005) and future (2006-2100) period under four Representative Concentration Pathways (RCP). In contrast to CMIP3, where...

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Published in:Journal of Geophysical Research: Atmospheres
Main Authors: Eyring, V., Arblaster, J. M., Cionni, I., Sedláček, J., Perlwitz, J., Young, P., Bekki, Slimane, Bergmann, D., Cameron-Smith, P., Collins, W., Faluvegi, G., Gottschaldt, K.-D., Horowitz, L. W., Kinnison, D. E., Lamarque, J.-F., Marsh, D. R., Saint-Martin, D., Shindell, D. T., Sudo, K., Szopa, S., Watanabe, S.
Other Authors: DLR Institut für Physik der Atmosphäre = DLR Institute of Atmospheric Physics (IPA), Deutsches Zentrum für Luft- und Raumfahrt Oberpfaffenhofen-Wessling (DLR), Centre for Australian Weather and Climate Research (CAWCR), National Center for Atmospheric Research Boulder (NCAR), Agenzia Nazionale per le nuove Tecnologie, l’energia e lo sviluppo economico sostenibile = Italian National Agency for New Technologies, Energy and Sustainable Economic Development (ENEA), Institute for Atmospheric and Climate Science Zürich (IAC), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich), NOAA Earth System Research Laboratory (ESRL), National Oceanic and Atmospheric Administration (NOAA), Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado Boulder -National Oceanic and Atmospheric Administration (NOAA), STRATO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Lawrence Livermore National Laboratory (LLNL), Met Office Hadley Centre (MOHC), United Kingdom Met Office Exeter, Department of Meteorology Reading, University of Reading (UOR), NASA Goddard Institute for Space Studies (GISS), NASA Goddard Space Flight Center (GSFC), NOAA Geophysical Fluid Dynamics Laboratory (GFDL), Centre national de recherches météorologiques (CNRM), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), Graduate School of Environmental Studies Nagoya, Nagoya University, Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Modélisation du climat (CLIM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Japan Agency for Marine-Earth Science and Technology (JAMSTEC)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2013
Subjects:
Online Access:https://hal.science/hal-03048322
https://hal.science/hal-03048322/document
https://hal.science/hal-03048322/file/jgrd.50316.pdf
https://doi.org/10.1002/JGRD.50316
id ftutoulouse3hal:oai:HAL:hal-03048322v1
record_format openpolar
institution Open Polar
collection Université Toulouse III - Paul Sabatier: HAL-UPS
op_collection_id ftutoulouse3hal
language English
topic [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces
environment
spellingShingle [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces
environment
Eyring, V.
Arblaster, J. M.
Cionni, I.
Sedláček, J.
Perlwitz, J.
Young, P.
Bekki, Slimane
Bergmann, D.
Cameron-Smith, P.
Collins, W.
Faluvegi, G.
Gottschaldt, K.-D.
Horowitz, L. W.
Kinnison, D. E.
Lamarque, J.-F.
Marsh, D. R.
Saint-Martin, D.
Shindell, D. T.
Sudo, K.
Szopa, S.
Watanabe, S.
Long-term ozone changes and associated climate impacts in CMIP5 simulations
topic_facet [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces
environment
description International audience Ozone changes and associated climate impacts in the Coupled Model Intercomparison Project Phase 5 (CMIP5) simulations are analyzed over the historical (1960-2005) and future (2006-2100) period under four Representative Concentration Pathways (RCP). In contrast to CMIP3, where half of the models prescribed constant stratospheric ozone, CMIP5 models all consider past ozone depletion and future ozone recovery. Multimodel mean climatologies and long-term changes in total and tropospheric column ozone calculated from CMIP5 models with either interactive or prescribed ozone are in reasonable agreement with observations. However, some large deviations from observations exist for individual models with interactive chemistry, and these models are excluded in the projections. Stratospheric ozone projections forced with a single halogen, but four greenhouse gas (GHG) scenarios show largest differences in the northern midlatitudes and in the Arctic in spring ( 20 and 40 Dobson units (DU) by 2100, respectively). By 2050, these differences are much smaller and negligible over Antarctica in austral spring. Differences in future tropospheric column ozone are mainly caused by differences in methane concentrations and stratospheric input, leading to 10 DU increases compared to 2000 in RCP 8.5. Large variations in stratospheric ozone particularly in CMIP5 models with interactive chemistry drive correspondingly large variations in lower stratospheric temperature trends. The results also illustrate that future Southern Hemisphere summertime circulation changes are controlled by both the ozone recovery rate and the rate of GHG increases, emphasizing the importance of simulating and taking into account ozone forcings when examining future climate projections.
author2 DLR Institut für Physik der Atmosphäre = DLR Institute of Atmospheric Physics (IPA)
Deutsches Zentrum für Luft- und Raumfahrt Oberpfaffenhofen-Wessling (DLR)
Centre for Australian Weather and Climate Research (CAWCR)
National Center for Atmospheric Research Boulder (NCAR)
Agenzia Nazionale per le nuove Tecnologie, l’energia e lo sviluppo economico sostenibile = Italian National Agency for New Technologies, Energy and Sustainable Economic Development (ENEA)
Institute for Atmospheric and Climate Science Zürich (IAC)
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich)
NOAA Earth System Research Laboratory (ESRL)
National Oceanic and Atmospheric Administration (NOAA)
Cooperative Institute for Research in Environmental Sciences (CIRES)
University of Colorado Boulder -National Oceanic and Atmospheric Administration (NOAA)
STRATO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Lawrence Livermore National Laboratory (LLNL)
Met Office Hadley Centre (MOHC)
United Kingdom Met Office Exeter
Department of Meteorology Reading
University of Reading (UOR)
NASA Goddard Institute for Space Studies (GISS)
NASA Goddard Space Flight Center (GSFC)
NOAA Geophysical Fluid Dynamics Laboratory (GFDL)
Centre national de recherches météorologiques (CNRM)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
Graduate School of Environmental Studies Nagoya
Nagoya University
Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Modélisation du climat (CLIM)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Japan Agency for Marine-Earth Science and Technology (JAMSTEC)
format Article in Journal/Newspaper
author Eyring, V.
Arblaster, J. M.
Cionni, I.
Sedláček, J.
Perlwitz, J.
Young, P.
Bekki, Slimane
Bergmann, D.
Cameron-Smith, P.
Collins, W.
Faluvegi, G.
Gottschaldt, K.-D.
Horowitz, L. W.
Kinnison, D. E.
Lamarque, J.-F.
Marsh, D. R.
Saint-Martin, D.
Shindell, D. T.
Sudo, K.
Szopa, S.
Watanabe, S.
author_facet Eyring, V.
Arblaster, J. M.
Cionni, I.
Sedláček, J.
Perlwitz, J.
Young, P.
Bekki, Slimane
Bergmann, D.
Cameron-Smith, P.
Collins, W.
Faluvegi, G.
Gottschaldt, K.-D.
Horowitz, L. W.
Kinnison, D. E.
Lamarque, J.-F.
Marsh, D. R.
Saint-Martin, D.
Shindell, D. T.
Sudo, K.
Szopa, S.
Watanabe, S.
author_sort Eyring, V.
title Long-term ozone changes and associated climate impacts in CMIP5 simulations
title_short Long-term ozone changes and associated climate impacts in CMIP5 simulations
title_full Long-term ozone changes and associated climate impacts in CMIP5 simulations
title_fullStr Long-term ozone changes and associated climate impacts in CMIP5 simulations
title_full_unstemmed Long-term ozone changes and associated climate impacts in CMIP5 simulations
title_sort long-term ozone changes and associated climate impacts in cmip5 simulations
publisher HAL CCSD
publishDate 2013
url https://hal.science/hal-03048322
https://hal.science/hal-03048322/document
https://hal.science/hal-03048322/file/jgrd.50316.pdf
https://doi.org/10.1002/JGRD.50316
genre Antarc*
Antarctica
Arctic
genre_facet Antarc*
Antarctica
Arctic
op_source ISSN: 2169-897X
EISSN: 2169-8996
Journal of Geophysical Research: Atmospheres
https://hal.science/hal-03048322
Journal of Geophysical Research: Atmospheres, 2013, 118 (10), pp.5029-5060. ⟨10.1002/JGRD.50316⟩
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hal-03048322
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https://hal.science/hal-03048322/document
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op_doi https://doi.org/10.1002/JGRD.50316
container_title Journal of Geophysical Research: Atmospheres
container_volume 118
container_issue 10
container_start_page 5029
op_container_end_page 5060
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spelling ftutoulouse3hal:oai:HAL:hal-03048322v1 2024-04-28T08:00:16+00:00 Long-term ozone changes and associated climate impacts in CMIP5 simulations Eyring, V. Arblaster, J. M. Cionni, I. Sedláček, J. Perlwitz, J. Young, P. Bekki, Slimane Bergmann, D. Cameron-Smith, P. Collins, W. Faluvegi, G. Gottschaldt, K.-D. Horowitz, L. W. Kinnison, D. E. Lamarque, J.-F. Marsh, D. R. Saint-Martin, D. Shindell, D. T. Sudo, K. Szopa, S. Watanabe, S. DLR Institut für Physik der Atmosphäre = DLR Institute of Atmospheric Physics (IPA) Deutsches Zentrum für Luft- und Raumfahrt Oberpfaffenhofen-Wessling (DLR) Centre for Australian Weather and Climate Research (CAWCR) National Center for Atmospheric Research Boulder (NCAR) Agenzia Nazionale per le nuove Tecnologie, l’energia e lo sviluppo economico sostenibile = Italian National Agency for New Technologies, Energy and Sustainable Economic Development (ENEA) Institute for Atmospheric and Climate Science Zürich (IAC) Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology Zürich (ETH Zürich) NOAA Earth System Research Laboratory (ESRL) National Oceanic and Atmospheric Administration (NOAA) Cooperative Institute for Research in Environmental Sciences (CIRES) University of Colorado Boulder -National Oceanic and Atmospheric Administration (NOAA) STRATO - LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Lawrence Livermore National Laboratory (LLNL) Met Office Hadley Centre (MOHC) United Kingdom Met Office Exeter Department of Meteorology Reading University of Reading (UOR) NASA Goddard Institute for Space Studies (GISS) NASA Goddard Space Flight Center (GSFC) NOAA Geophysical Fluid Dynamics Laboratory (GFDL) Centre national de recherches météorologiques (CNRM) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Graduate School of Environmental Studies Nagoya Nagoya University Laboratoire des Sciences du Climat et de l'Environnement Gif-sur-Yvette (LSCE) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Modélisation du climat (CLIM) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Japan Agency for Marine-Earth Science and Technology (JAMSTEC) 2013-05-27 https://hal.science/hal-03048322 https://hal.science/hal-03048322/document https://hal.science/hal-03048322/file/jgrd.50316.pdf https://doi.org/10.1002/JGRD.50316 en eng HAL CCSD American Geophysical Union info:eu-repo/semantics/altIdentifier/doi/10.1002/JGRD.50316 hal-03048322 https://hal.science/hal-03048322 https://hal.science/hal-03048322/document https://hal.science/hal-03048322/file/jgrd.50316.pdf doi:10.1002/JGRD.50316 info:eu-repo/semantics/OpenAccess ISSN: 2169-897X EISSN: 2169-8996 Journal of Geophysical Research: Atmospheres https://hal.science/hal-03048322 Journal of Geophysical Research: Atmospheres, 2013, 118 (10), pp.5029-5060. ⟨10.1002/JGRD.50316⟩ [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment info:eu-repo/semantics/article Journal articles 2013 ftutoulouse3hal https://doi.org/10.1002/JGRD.50316 2024-04-04T17:34:01Z International audience Ozone changes and associated climate impacts in the Coupled Model Intercomparison Project Phase 5 (CMIP5) simulations are analyzed over the historical (1960-2005) and future (2006-2100) period under four Representative Concentration Pathways (RCP). In contrast to CMIP3, where half of the models prescribed constant stratospheric ozone, CMIP5 models all consider past ozone depletion and future ozone recovery. Multimodel mean climatologies and long-term changes in total and tropospheric column ozone calculated from CMIP5 models with either interactive or prescribed ozone are in reasonable agreement with observations. However, some large deviations from observations exist for individual models with interactive chemistry, and these models are excluded in the projections. Stratospheric ozone projections forced with a single halogen, but four greenhouse gas (GHG) scenarios show largest differences in the northern midlatitudes and in the Arctic in spring ( 20 and 40 Dobson units (DU) by 2100, respectively). By 2050, these differences are much smaller and negligible over Antarctica in austral spring. Differences in future tropospheric column ozone are mainly caused by differences in methane concentrations and stratospheric input, leading to 10 DU increases compared to 2000 in RCP 8.5. Large variations in stratospheric ozone particularly in CMIP5 models with interactive chemistry drive correspondingly large variations in lower stratospheric temperature trends. The results also illustrate that future Southern Hemisphere summertime circulation changes are controlled by both the ozone recovery rate and the rate of GHG increases, emphasizing the importance of simulating and taking into account ozone forcings when examining future climate projections. Article in Journal/Newspaper Antarc* Antarctica Arctic Université Toulouse III - Paul Sabatier: HAL-UPS Journal of Geophysical Research: Atmospheres 118 10 5029 5060