Preprints
https://doi.org/10.5194/egusphere-2026-560
https://doi.org/10.5194/egusphere-2026-560
10 Feb 2026
 | 10 Feb 2026

Analysis of Antarctic ozone trends from 1979 to 2023

Haotian He, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Shujie Chang, Yajuan Li, Mark Weber, and Saffron Heddell

Abstract. Antarctic ozone has shown a sustained recovery since 2000, but levels were distinctly low during 20202023, potentially affecting estimates of ozone recovery and long-term trends. To assess the impact of recent low ozone on long-term variability, we analyze total column ozone (TCO) data from World Ozone and Ultraviolet Radiation Centre, multi-sensor reanalysis, and Total Ozone Mapping Spectrometer/Ozone Monitoring Instrument. Ozone fields from TOMCAT, a 3-D chemical transport model, are also used to gain better insight ozone changes. Multiple linear regression (MLR) is applied to estimate ozone trends over Antarctica from 1979 to 2023, incorporating proxies representing key chemical and dynamical processes such as the El Niño-Southern Oscillation and the Brewer-Dobson circulation (BDC).

Our analysis suggests that before 2000, all datasets show significant declines in annual TCO of about 2 and 6 Dobson Units per year (DU/yr) for September and October, respectively. For the 20012023 period, the magnitude of the October trend shifted to 1.5 DU/yr. The MLR effectively captures long-term ozone changes as well as unusual dynamical events such as the sudden stratospheric warmings in 2002 and 2019. As dynamical proxies show the largest influence, we use TOMCAT simulations to illustrate the impact of the BDC on the Antarctic ozone. Two sensitivity simulations further demonstrate that the strengthening (weakening) of the circulation leads to high (low) ozone values in spring. These findings suggest that after ozone-depleting substances were strictly controlled, dynamical processes have played an increasingly important role in controlling the ozone recovery patterns in Antarctica.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Journal article(s) based on this preprint

10 Jul 2026
Analysis of Antarctic ozone trends from 1979 to 2023
Haotian He, Shujie Chang, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Saffron G. Heddell, Yajuan Li, and Mark Weber
Atmos. Chem. Phys., 26, 9741–9756, https://doi.org/10.5194/acp-26-9741-2026,https://doi.org/10.5194/acp-26-9741-2026, 2026
Short summary
Haotian He, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Shujie Chang, Yajuan Li, Mark Weber, and Saffron Heddell

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2026-560', Anonymous Referee #1, 11 Mar 2026
    • AC1: 'Reply on RC1', Haotian He, 04 May 2026
  • RC2: 'Comment on egusphere-2026-560', Anonymous Referee #2, 16 Mar 2026
    • AC2: 'Reply on RC2', Haotian He, 04 May 2026
  • CC1: 'Comment on egusphere-2026-560', Hannah Kessenich, 17 Mar 2026
    • AC3: 'Reply on CC1', Haotian He, 04 May 2026

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2026-560', Anonymous Referee #1, 11 Mar 2026
    • AC1: 'Reply on RC1', Haotian He, 04 May 2026
  • RC2: 'Comment on egusphere-2026-560', Anonymous Referee #2, 16 Mar 2026
    • AC2: 'Reply on RC2', Haotian He, 04 May 2026
  • CC1: 'Comment on egusphere-2026-560', Hannah Kessenich, 17 Mar 2026
    • AC3: 'Reply on CC1', Haotian He, 04 May 2026

Peer review completion

AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Haotian He on behalf of the Authors (04 May 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (05 May 2026) by Jens-Uwe Grooß
ED: Publish subject to minor revisions (review by editor) (07 May 2026) by Jens-Uwe Grooß
AR by Haotian He on behalf of the Authors (16 May 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (18 May 2026) by Jens-Uwe Grooß
AR by Haotian He on behalf of the Authors (24 May 2026)  Manuscript 

Journal article(s) based on this preprint

10 Jul 2026
Analysis of Antarctic ozone trends from 1979 to 2023
Haotian He, Shujie Chang, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Saffron G. Heddell, Yajuan Li, and Mark Weber
Atmos. Chem. Phys., 26, 9741–9756, https://doi.org/10.5194/acp-26-9741-2026,https://doi.org/10.5194/acp-26-9741-2026, 2026
Short summary
Haotian He, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Shujie Chang, Yajuan Li, Mark Weber, and Saffron Heddell
Haotian He, Martyn P. Chipperfield, Sandip S. Dhomse, Wuhu Feng, Shujie Chang, Yajuan Li, Mark Weber, and Saffron Heddell

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Short summary
Overall, in the long-term, Antarctic ozone evolution reflects the interplay of multiple processes, with dynamical drivers holding a particularly strong influence on recovery patterns. The Brewer-Dobson circulation perturbations play a significant role in the long-term ozone trend, requiring more research and continued attention to the ozone hole and dynamic processes to improve our understanding of long-term ozone variability and predict future changes in the Antarctic ozone hole.
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