Climate impact of stratospheric ozone recovery

International audience Past stratospheric ozone depletion has acted to cool the Earth's surface. As the result of the phase-out of anthropogenic halogenated compounds emissions, stratospheric ozone is projected to recover and its radiative forcing (RF-O 3 ~ -0.05 W/m 2 presently) might therefor...

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Published in:Geophysical Research Letters
Main Authors: Bekki, Slimane, Rap, Alexandru, Poulain, Virginie, Dhomse, Sandip, Marchand, Marion, Lefèvre, Franck, Forster, Piers M., Laval-Szopa, Sophie, Chipperfield, Martyn P.
Other Authors: 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), Institute for Climate and Atmospheric Science Leeds (ICAS), School of Earth and Environment Leeds (SEE), University of Leeds-University of Leeds, 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)), European Commission, U.K. Natural Environment Research Council, European Project: 226365,EC:FP7:ENV,FP7-ENV-2008-1,RECONCILE(2009)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2013
Subjects:
Online Access:https://hal.science/hal-00802252
https://hal.science/hal-00802252/document
https://hal.science/hal-00802252/file/Bekki_et_al-2013-Geophysical_Research_Letters.pdf
https://doi.org/10.1002/grl.50358
id ftinsu:oai:HAL:hal-00802252v1
record_format openpolar
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic Stratospheric ozone
Climate
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
[SDE.MCG]Environmental Sciences/Global Changes
spellingShingle Stratospheric ozone
Climate
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
[SDE.MCG]Environmental Sciences/Global Changes
Bekki, Slimane
Rap, Alexandru
Poulain, Virginie
Dhomse, Sandip
Marchand, Marion
Lefèvre, Franck
Forster, Piers M.
Laval-Szopa, Sophie
Chipperfield, Martyn P.
Climate impact of stratospheric ozone recovery
topic_facet Stratospheric ozone
Climate
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology
[SDE.MCG]Environmental Sciences/Global Changes
description International audience Past stratospheric ozone depletion has acted to cool the Earth's surface. As the result of the phase-out of anthropogenic halogenated compounds emissions, stratospheric ozone is projected to recover and its radiative forcing (RF-O 3 ~ -0.05 W/m 2 presently) might therefore be expected to decay in line with ozone recovery itself. Using results from chemistry-climate models, we find that, although model projections using a standard greenhouse gas scenario broadly agree on the future evolution of global ozone, they strongly disagree on RF-O 3 because of a large model spread in ozone changes in a narrow (several km thick) layer, in the northern lowermost stratosphere. Clearly, future changes in global stratospheric ozone cannot be considered an indicator of its overall RF. The multi-model mean RF-O 3 estimate for 2100 is +0.06 W/m 2 but with a range such that it could remain negative throughout this century or change sign and reach up to ~0.25 W/m 2 .
author2 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)
Institute for Climate and Atmospheric Science Leeds (ICAS)
School of Earth and Environment Leeds (SEE)
University of Leeds-University of Leeds
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))
European Commission
U.K. Natural Environment Research Council
European Project: 226365,EC:FP7:ENV,FP7-ENV-2008-1,RECONCILE(2009)
format Article in Journal/Newspaper
author Bekki, Slimane
Rap, Alexandru
Poulain, Virginie
Dhomse, Sandip
Marchand, Marion
Lefèvre, Franck
Forster, Piers M.
Laval-Szopa, Sophie
Chipperfield, Martyn P.
author_facet Bekki, Slimane
Rap, Alexandru
Poulain, Virginie
Dhomse, Sandip
Marchand, Marion
Lefèvre, Franck
Forster, Piers M.
Laval-Szopa, Sophie
Chipperfield, Martyn P.
author_sort Bekki, Slimane
title Climate impact of stratospheric ozone recovery
title_short Climate impact of stratospheric ozone recovery
title_full Climate impact of stratospheric ozone recovery
title_fullStr Climate impact of stratospheric ozone recovery
title_full_unstemmed Climate impact of stratospheric ozone recovery
title_sort climate impact of stratospheric ozone recovery
publisher HAL CCSD
publishDate 2013
url https://hal.science/hal-00802252
https://hal.science/hal-00802252/document
https://hal.science/hal-00802252/file/Bekki_et_al-2013-Geophysical_Research_Letters.pdf
https://doi.org/10.1002/grl.50358
genre Arctic
genre_facet Arctic
op_source ISSN: 0094-8276
EISSN: 1944-8007
Geophysical Research Letters
https://hal.science/hal-00802252
Geophysical Research Letters, 2013, 40 (11), pp.2796-2800. ⟨10.1002/grl.50358⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1002/grl.50358
info:eu-repo/grantAgreement/EC/FP7/226365/EU/Reconciliation of essential process parameters for an enhanced predictability of arctic stratospheric ozone loss and its climate interactions./RECONCILE
hal-00802252
https://hal.science/hal-00802252
https://hal.science/hal-00802252/document
https://hal.science/hal-00802252/file/Bekki_et_al-2013-Geophysical_Research_Letters.pdf
doi:10.1002/grl.50358
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1002/grl.50358
container_title Geophysical Research Letters
container_volume 40
container_issue 11
container_start_page 2796
op_container_end_page 2800
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spelling ftinsu:oai:HAL:hal-00802252v1 2024-04-28T08:04:45+00:00 Climate impact of stratospheric ozone recovery Bekki, Slimane Rap, Alexandru Poulain, Virginie Dhomse, Sandip Marchand, Marion Lefèvre, Franck Forster, Piers M. Laval-Szopa, Sophie Chipperfield, Martyn P. 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) Institute for Climate and Atmospheric Science Leeds (ICAS) School of Earth and Environment Leeds (SEE) University of Leeds-University of Leeds 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)) European Commission U.K. Natural Environment Research Council European Project: 226365,EC:FP7:ENV,FP7-ENV-2008-1,RECONCILE(2009) 2013 https://hal.science/hal-00802252 https://hal.science/hal-00802252/document https://hal.science/hal-00802252/file/Bekki_et_al-2013-Geophysical_Research_Letters.pdf https://doi.org/10.1002/grl.50358 en eng HAL CCSD American Geophysical Union info:eu-repo/semantics/altIdentifier/doi/10.1002/grl.50358 info:eu-repo/grantAgreement/EC/FP7/226365/EU/Reconciliation of essential process parameters for an enhanced predictability of arctic stratospheric ozone loss and its climate interactions./RECONCILE hal-00802252 https://hal.science/hal-00802252 https://hal.science/hal-00802252/document https://hal.science/hal-00802252/file/Bekki_et_al-2013-Geophysical_Research_Letters.pdf doi:10.1002/grl.50358 info:eu-repo/semantics/OpenAccess ISSN: 0094-8276 EISSN: 1944-8007 Geophysical Research Letters https://hal.science/hal-00802252 Geophysical Research Letters, 2013, 40 (11), pp.2796-2800. ⟨10.1002/grl.50358⟩ Stratospheric ozone Climate [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology [SDE.MCG]Environmental Sciences/Global Changes info:eu-repo/semantics/article Journal articles 2013 ftinsu https://doi.org/10.1002/grl.50358 2024-04-05T00:48:45Z International audience Past stratospheric ozone depletion has acted to cool the Earth's surface. As the result of the phase-out of anthropogenic halogenated compounds emissions, stratospheric ozone is projected to recover and its radiative forcing (RF-O 3 ~ -0.05 W/m 2 presently) might therefore be expected to decay in line with ozone recovery itself. Using results from chemistry-climate models, we find that, although model projections using a standard greenhouse gas scenario broadly agree on the future evolution of global ozone, they strongly disagree on RF-O 3 because of a large model spread in ozone changes in a narrow (several km thick) layer, in the northern lowermost stratosphere. Clearly, future changes in global stratospheric ozone cannot be considered an indicator of its overall RF. The multi-model mean RF-O 3 estimate for 2100 is +0.06 W/m 2 but with a range such that it could remain negative throughout this century or change sign and reach up to ~0.25 W/m 2 . Article in Journal/Newspaper Arctic Institut national des sciences de l'Univers: HAL-INSU Geophysical Research Letters 40 11 2796 2800