Articles | Volume 17, issue 3
https://doi.org/10.5194/acp-17-1741-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/acp-17-1741-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Evolution of the eastward shift in the quasi-stationary minimum of the Antarctic total ozone column
Asen Grytsai
Taras Shevchenko National University of Kyiv, 01601 Kyiv, Ukraine
Andrew Klekociuk
Antarctica and the Global System Program, Australian Antarctic Division, Kingston, Tasmania 7050, Australia
Antarctic Climate and Ecosystems Cooperative Research Centre, Hobart, Tasmania 7000, Australia
Gennadi Milinevsky
CORRESPONDING AUTHOR
Taras Shevchenko National University of Kyiv, 01601 Kyiv, Ukraine
Main Astronomical Observatory, National Academy of Sciences of Ukraine, 03143 Kyiv, Ukraine
Oleksandr Evtushevsky
Taras Shevchenko National University of Kyiv, 01601 Kyiv, Ukraine
Kane Stone
School of Earth Sciences, University of Melbourne, Melbourne, Victoria 3010, Australia
ARC Centre of Excellence for Climate System Science, University of New South Wales, Sydney, New South Wales 2052, Australia
currently at: the Department of Earth, Atmospheric and Planetary Sciences,
Massachusetts Institute of Technology, Cambridge, Massachusetts 02139-4307, USA
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Cited
14 citations as recorded by crossref.
- Investigation of the Vertical Influence of the 11-Year Solar Cycle on Ozone Using SBUV and Antarctic Ground-Based Measurements and CMIP6 Forcing Data A. Grytsai et al. 10.3390/atmos11080873
- The Antarctic ozone hole during 2018 and 2019 A. Klekociuk et al. 10.1071/ES20010
- The evolution of zonally asymmetric austral ozone in a chemistry–climate model F. Dennison et al. 10.5194/acp-17-14075-2017
- The data processing and analysis methods for stratospheric ozone and planetary wave study Y. Shi et al. 10.33275/1727-7485.2.2022.698
- Long-term analysis of the Antarctic total ozone zonal asymmetry by MERRA-2 and CMIP6 data O. Ivaniha 10.33275/1727-7485.1.2020.378
- Decadal changes in the central tropical Pacific teleconnection to the Southern Hemisphere extratropics O. Evtushevsky et al. 10.1007/s00382-018-4354-5
- On the use of satellite observations to fill gaps in the Halley station total ozone record L. Zhang et al. 10.5194/acp-21-9829-2021
- Total Ozone over Vernadsky Antarctic Station: Ground-based and Satellite Measurements A. Grytsai et al. 10.33275/1727-7485.1(17).2018.33
- Antarctic planetary wave spectrum under different polar vortex conditions in 2019 and 2020 based on total ozone column data А. Grytsai et al. 10.33275/1727-7485.1.2022.687
- Assessment of the zonal asymmetry trend in Antarctic total ozonecolumn using TOMS measurements and CCMVal-2 models J. Siddaway et al. 10.33275/1727-7485.2.2020.652
- Current trends in the zonal distribution and asymmetry of ozone in Antarctica based on satellite measurements R. Yu et al. 10.33275/1727-7485.1.2024.725
- Persistent extreme ultraviolet irradiance in Antarctica despite the ozone recovery onset R. Cordero et al. 10.1038/s41598-022-05449-8
- Hemispheric asymmetry in stratospheric NO<sub>2</sub> trends M. Yela et al. 10.5194/acp-17-13373-2017
- The recent signs of total column ozone recovery over mid-latitudes: The effects of the Montreal Protocol mandate S. Ningombam et al. 10.1016/j.jastp.2018.05.011
14 citations as recorded by crossref.
- Investigation of the Vertical Influence of the 11-Year Solar Cycle on Ozone Using SBUV and Antarctic Ground-Based Measurements and CMIP6 Forcing Data A. Grytsai et al. 10.3390/atmos11080873
- The Antarctic ozone hole during 2018 and 2019 A. Klekociuk et al. 10.1071/ES20010
- The evolution of zonally asymmetric austral ozone in a chemistry–climate model F. Dennison et al. 10.5194/acp-17-14075-2017
- The data processing and analysis methods for stratospheric ozone and planetary wave study Y. Shi et al. 10.33275/1727-7485.2.2022.698
- Long-term analysis of the Antarctic total ozone zonal asymmetry by MERRA-2 and CMIP6 data O. Ivaniha 10.33275/1727-7485.1.2020.378
- Decadal changes in the central tropical Pacific teleconnection to the Southern Hemisphere extratropics O. Evtushevsky et al. 10.1007/s00382-018-4354-5
- On the use of satellite observations to fill gaps in the Halley station total ozone record L. Zhang et al. 10.5194/acp-21-9829-2021
- Total Ozone over Vernadsky Antarctic Station: Ground-based and Satellite Measurements A. Grytsai et al. 10.33275/1727-7485.1(17).2018.33
- Antarctic planetary wave spectrum under different polar vortex conditions in 2019 and 2020 based on total ozone column data А. Grytsai et al. 10.33275/1727-7485.1.2022.687
- Assessment of the zonal asymmetry trend in Antarctic total ozonecolumn using TOMS measurements and CCMVal-2 models J. Siddaway et al. 10.33275/1727-7485.2.2020.652
- Current trends in the zonal distribution and asymmetry of ozone in Antarctica based on satellite measurements R. Yu et al. 10.33275/1727-7485.1.2024.725
- Persistent extreme ultraviolet irradiance in Antarctica despite the ozone recovery onset R. Cordero et al. 10.1038/s41598-022-05449-8
- Hemispheric asymmetry in stratospheric NO<sub>2</sub> trends M. Yela et al. 10.5194/acp-17-13373-2017
- The recent signs of total column ozone recovery over mid-latitudes: The effects of the Montreal Protocol mandate S. Ningombam et al. 10.1016/j.jastp.2018.05.011
Discussed (final revised paper)
Latest update: 20 Nov 2024
Short summary
Twenty years ago we discovered that the ozone hole shape is asymmetric. This asymmetry is minimum over the Weddell Sea region and maximum over the Ross Sea area. Later we detected that the position of the ozone minimum is shifting east. We have continued to follow this event, and a couple years ago we revealed that the shift is slowing down and starting to move back. We connect all this movement with ozone hole increase; since 2000 the ozone layer has been stabilizing and recently recovering.
Twenty years ago we discovered that the ozone hole shape is asymmetric. This asymmetry is...
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Final-revised paper
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