Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery

Depletion of stratospheric ozone in the Southern Hemisphere (SH) during the late twentieth century cooled local air temperature, which resulted in stronger stratospheric westerly winds near 60° S and altered SH surface climate. However, Antarctic ozone has been recovering since around 2001 thanks to...

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Published in:Nature Geoscience
Main Authors: Zambri, Brian, Solomon, Susan, Thompson, David W. J., Fu, Qiang
Format: Article in Journal/Newspaper
Language:unknown
Published: 2021
Subjects:
Online Access:https://ueaeprints.uea.ac.uk/id/eprint/85561/
https://doi.org/10.1038/S41561-021-00803-3
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spelling ftuniveastangl:oai:ueaeprints.uea.ac.uk:85561 2023-05-15T14:02:10+02:00 Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery Zambri, Brian Solomon, Susan Thompson, David W. J. Fu, Qiang 2021-09 https://ueaeprints.uea.ac.uk/id/eprint/85561/ https://doi.org/10.1038/S41561-021-00803-3 unknown Zambri, Brian, Solomon, Susan, Thompson, David W. J. and Fu, Qiang (2021) Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery. Nature Geoscience, 14 (9). 638–644. ISSN 1752-0894 doi:10.1038/S41561-021-00803-3 Article PeerReviewed 2021 ftuniveastangl https://doi.org/10.1038/S41561-021-00803-3 2023-01-30T21:57:14Z Depletion of stratospheric ozone in the Southern Hemisphere (SH) during the late twentieth century cooled local air temperature, which resulted in stronger stratospheric westerly winds near 60° S and altered SH surface climate. However, Antarctic ozone has been recovering since around 2001 thanks to the implementation of the Montreal Protocol, which banned production and consumption of ozone-depleting substances. Here we show that the post-2001 increase in ozone has resulted in significant changes to trends in SH temperature and circulation. The trends are generally of opposite sign to those that resulted from stratospheric ozone losses, including a warming of the SH polar lower stratosphere and a weakening of the SH stratospheric polar vortex. Observed post-2001 trends of temperature and circulation in the stratosphere are about 50–75% smaller in magnitude than the trends during the ozone depletion era. The response is broadly consistent with expectations based on modelled depletion-era trends and variability of both ozone and reactive chlorine. The differences in observed stratospheric trends between the recovery and depletion periods are statistically significant (P < 0.05), providing evidence for the emergence of dynamical impacts of the healing of the Antarctic ozone hole. Article in Journal/Newspaper Antarc* Antarctic University of East Anglia: UEA Digital Repository Antarctic The Antarctic Nature Geoscience 14 9 638 644
institution Open Polar
collection University of East Anglia: UEA Digital Repository
op_collection_id ftuniveastangl
language unknown
description Depletion of stratospheric ozone in the Southern Hemisphere (SH) during the late twentieth century cooled local air temperature, which resulted in stronger stratospheric westerly winds near 60° S and altered SH surface climate. However, Antarctic ozone has been recovering since around 2001 thanks to the implementation of the Montreal Protocol, which banned production and consumption of ozone-depleting substances. Here we show that the post-2001 increase in ozone has resulted in significant changes to trends in SH temperature and circulation. The trends are generally of opposite sign to those that resulted from stratospheric ozone losses, including a warming of the SH polar lower stratosphere and a weakening of the SH stratospheric polar vortex. Observed post-2001 trends of temperature and circulation in the stratosphere are about 50–75% smaller in magnitude than the trends during the ozone depletion era. The response is broadly consistent with expectations based on modelled depletion-era trends and variability of both ozone and reactive chlorine. The differences in observed stratospheric trends between the recovery and depletion periods are statistically significant (P < 0.05), providing evidence for the emergence of dynamical impacts of the healing of the Antarctic ozone hole.
format Article in Journal/Newspaper
author Zambri, Brian
Solomon, Susan
Thompson, David W. J.
Fu, Qiang
spellingShingle Zambri, Brian
Solomon, Susan
Thompson, David W. J.
Fu, Qiang
Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
author_facet Zambri, Brian
Solomon, Susan
Thompson, David W. J.
Fu, Qiang
author_sort Zambri, Brian
title Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
title_short Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
title_full Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
title_fullStr Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
title_full_unstemmed Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery
title_sort emergence of southern hemisphere stratospheric circulation changes in response to ozone recovery
publishDate 2021
url https://ueaeprints.uea.ac.uk/id/eprint/85561/
https://doi.org/10.1038/S41561-021-00803-3
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation Zambri, Brian, Solomon, Susan, Thompson, David W. J. and Fu, Qiang (2021) Emergence of Southern Hemisphere stratospheric circulation changes in response to ozone recovery. Nature Geoscience, 14 (9). 638–644. ISSN 1752-0894
doi:10.1038/S41561-021-00803-3
op_doi https://doi.org/10.1038/S41561-021-00803-3
container_title Nature Geoscience
container_volume 14
container_issue 9
container_start_page 638
op_container_end_page 644
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