Total ozone variability and trends over the South Pole during the wintertime

The Antarctic polar vortex creates unique chemical and dynamical conditions when the stratospheric air over Antarctica is isolated from the rest of the stratosphere. As a result, stratospheric ozone within the vortex remains largely unchanged for a five-month period from April until late August when...

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Main Authors: Fioletov, Vitali, Zhao, Xiaoyi, Abboud, Ihab, Brohart, Michael, Ogyu, Akira, Sit, Reno, Lee, Sum Chi, Petropavlovskikh, Irina, Miyagawa, Koji, Johnson, Bryan J., Cullis, Patrick, Booth, John, McConville, Glen, McElroy, C. Thomas
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-773
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author Fioletov, Vitali
Zhao, Xiaoyi
Abboud, Ihab
Brohart, Michael
Ogyu, Akira
Sit, Reno
Lee, Sum Chi
Petropavlovskikh, Irina
Miyagawa, Koji
Johnson, Bryan J.
Cullis, Patrick
Booth, John
McConville, Glen
McElroy, C. Thomas
author_facet Fioletov, Vitali
Zhao, Xiaoyi
Abboud, Ihab
Brohart, Michael
Ogyu, Akira
Sit, Reno
Lee, Sum Chi
Petropavlovskikh, Irina
Miyagawa, Koji
Johnson, Bryan J.
Cullis, Patrick
Booth, John
McConville, Glen
McElroy, C. Thomas
author_sort Fioletov, Vitali
collection Niedersächsisches Online-Archiv NOA
description The Antarctic polar vortex creates unique chemical and dynamical conditions when the stratospheric air over Antarctica is isolated from the rest of the stratosphere. As a result, stratospheric ozone within the vortex remains largely unchanged for a five-month period from April until late August when the sunrise and extremely cold temperatures create favorable conditions for rapid ozone loss. Such prolonged stable conditions within the vortex make it possible to estimate the total ozone levels there from sparse wintertime ozone observations at the South Pole. The available records of focused Moon (FM) observations by Dobson and Brewer spectrophotometers at the Amundsen-Scott South Pole Station (for the periods 1964–2022 and 2008–2022, respectively) as well as integrated ozonesonde profiles (1986–2022) and MERRA-2 reanalysis data (1980–2022) were used to estimate the total ozone variability and long-term changes over the South Pole. Comparisons with MERRA-2 reanalysis data for the period 1980–2022 demonstrated that the uncertainties of Dobson and Brewer daily mean FM values are about 2.5 %–4 %. Wintertime (April–August) MERRA-2 data have a bias with Dobson data of -8.5 % in 1980–2004 and 1.5 % in 2005–2022. The mean difference between wintertime Dobson and Brewer data in 2008–2022 was about 1.6 %; however, this difference can be largely explained by various systematic errors in Brewer data. The wintertime ozone values over the South Pole during the last 20 years were about 12 % below the pre-1980s level, i.e., the decline there was nearly twice larger than that over southern midlatitudes. It is probably the largest long-term ozone decline aside from the springtime Antarctic ozone depletion. While wintertime ozone decline over the pole has hardly any impact on the environment, it can be used as an indicator to diagnose the state of the ozone layer, particularly because it requires data from only one station. Dobson and ozonesonde data after 2001 show a small positive, but not statistically significant, trend in ...
format Article in Journal/Newspaper
genre Amundsen-Scott
Antarc*
Antarctic
Antarctica
South pole
South pole
genre_facet Amundsen-Scott
Antarc*
Antarctic
Antarctica
South pole
South pole
geographic Amundsen Scott South Pole Station
Amundsen-Scott
Amundsen-Scott South Pole Station
Antarctic
Merra
South Pole
The Antarctic
geographic_facet Amundsen Scott South Pole Station
Amundsen-Scott
Amundsen-Scott South Pole Station
Antarctic
Merra
South Pole
The Antarctic
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00066549 2025-01-16T18:54:49+00:00 Total ozone variability and trends over the South Pole during the wintertime Fioletov, Vitali Zhao, Xiaoyi Abboud, Ihab Brohart, Michael Ogyu, Akira Sit, Reno Lee, Sum Chi Petropavlovskikh, Irina Miyagawa, Koji Johnson, Bryan J. Cullis, Patrick Booth, John McConville, Glen McElroy, C. Thomas 2023-05 electronic https://doi.org/10.5194/egusphere-2023-773 https://noa.gwlb.de/receive/cop_mods_00066549 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00065030/egusphere-2023-773.pdf https://egusphere.copernicus.org/preprints/2023/egusphere-2023-773/egusphere-2023-773.pdf eng eng Copernicus Publications https://doi.org/10.5194/egusphere-2023-773 https://noa.gwlb.de/receive/cop_mods_00066549 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00065030/egusphere-2023-773.pdf https://egusphere.copernicus.org/preprints/2023/egusphere-2023-773/egusphere-2023-773.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2023 ftnonlinearchiv https://doi.org/10.5194/egusphere-2023-773 2023-05-28T23:18:40Z The Antarctic polar vortex creates unique chemical and dynamical conditions when the stratospheric air over Antarctica is isolated from the rest of the stratosphere. As a result, stratospheric ozone within the vortex remains largely unchanged for a five-month period from April until late August when the sunrise and extremely cold temperatures create favorable conditions for rapid ozone loss. Such prolonged stable conditions within the vortex make it possible to estimate the total ozone levels there from sparse wintertime ozone observations at the South Pole. The available records of focused Moon (FM) observations by Dobson and Brewer spectrophotometers at the Amundsen-Scott South Pole Station (for the periods 1964–2022 and 2008–2022, respectively) as well as integrated ozonesonde profiles (1986–2022) and MERRA-2 reanalysis data (1980–2022) were used to estimate the total ozone variability and long-term changes over the South Pole. Comparisons with MERRA-2 reanalysis data for the period 1980–2022 demonstrated that the uncertainties of Dobson and Brewer daily mean FM values are about 2.5 %–4 %. Wintertime (April–August) MERRA-2 data have a bias with Dobson data of -8.5 % in 1980–2004 and 1.5 % in 2005–2022. The mean difference between wintertime Dobson and Brewer data in 2008–2022 was about 1.6 %; however, this difference can be largely explained by various systematic errors in Brewer data. The wintertime ozone values over the South Pole during the last 20 years were about 12 % below the pre-1980s level, i.e., the decline there was nearly twice larger than that over southern midlatitudes. It is probably the largest long-term ozone decline aside from the springtime Antarctic ozone depletion. While wintertime ozone decline over the pole has hardly any impact on the environment, it can be used as an indicator to diagnose the state of the ozone layer, particularly because it requires data from only one station. Dobson and ozonesonde data after 2001 show a small positive, but not statistically significant, trend in ... Article in Journal/Newspaper Amundsen-Scott Antarc* Antarctic Antarctica South pole South pole Niedersächsisches Online-Archiv NOA Amundsen Scott South Pole Station ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott South Pole Station ENVELOPE(139.273,139.273,-89.998,-89.998) Antarctic Merra ENVELOPE(12.615,12.615,65.816,65.816) South Pole The Antarctic
spellingShingle article
Verlagsveröffentlichung
Fioletov, Vitali
Zhao, Xiaoyi
Abboud, Ihab
Brohart, Michael
Ogyu, Akira
Sit, Reno
Lee, Sum Chi
Petropavlovskikh, Irina
Miyagawa, Koji
Johnson, Bryan J.
Cullis, Patrick
Booth, John
McConville, Glen
McElroy, C. Thomas
Total ozone variability and trends over the South Pole during the wintertime
title Total ozone variability and trends over the South Pole during the wintertime
title_full Total ozone variability and trends over the South Pole during the wintertime
title_fullStr Total ozone variability and trends over the South Pole during the wintertime
title_full_unstemmed Total ozone variability and trends over the South Pole during the wintertime
title_short Total ozone variability and trends over the South Pole during the wintertime
title_sort total ozone variability and trends over the south pole during the wintertime
topic article
Verlagsveröffentlichung
topic_facet article
Verlagsveröffentlichung
url https://doi.org/10.5194/egusphere-2023-773
https://noa.gwlb.de/receive/cop_mods_00066549
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00065030/egusphere-2023-773.pdf
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-773/egusphere-2023-773.pdf