Symptoms of total ozone recovery inside the Antarctic vortex during Austral spring

Andrea Pazmino 1 Sophie Godin-Beeckmann 1 Alain Hauchecorne 1 Chantal Claud 2 Sergey Khaykin 3 Florence Goutail 1 Wolfram Elian 4 Jacobo Salvador 4, 5, 6 Eduardo Quel 4
1 SHTI - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
2 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)
3 TROPO - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
4 CEILAP - Centro de Investigaciones en Laseres y Aplicaciones
5 UTN-FRBA - Facultad Regional Buenos Aires
6 UNPA - Universidad Nacional de la Patagonia Austral
Abstract : The long-term evolution of total ozone column inside the Antarctic polar vortex is investigated over the 1980–2016 period. Trend analyses are performed using a multilinear regression (MLR) model based on various proxies (heat flux, Quasi-Biennial Oscillation, solar flux, Antarctic Oscillation and aerosols). Annual total ozone column corresponding to the mean monthly values inside the vortex in September and during the period of maximum ozone depletion from September 15th to October 15th are used. Total ozone columns from combined SBUV, TOMS and OMI satellite datasets and the Multi-Sensor Reanalysis (MSR-2) dataset are considered in the study. Ozone trends are computed by a piecewise trend model (PWT) before and after the turnaround in 2001. In order to evaluate total ozone within the vortex, two classification methods are used, based on the potential vorticity gradient as a function of equivalent latitude. The first standard one considers this gradient at a single isentropic level (475 K or 550 K), while the second one uses a range of isentropic levels between 400 K and 600 K. The regression model includes a new proxy that represents the stability of the vortex during the studied month period. The determination coefficient (R2) between observations and modeled values increases by ~ 0.05 when this proxy is included in the MLR model. The higher R2 (0.93–0.95) and the minimum residuals are observed for the second classification method for both datasets and months periods. Trends in September are statistically significant at 2 sigma level over 2001–2016 period with values ranging between 1.85 and 2.67 DU yr−1 depending on the methods and data sets. This result confirms the recent studies of Antarctic ozone healing during that month. Trends after 2001 are 2 to 3 times lower than before the turnaround year as expected from the response to the slowly ozone-depleting substances decrease in Polar regions. Estimated trends in the 15 Sept–15 Oct period are smaller than in September. They vary from 1.15 to 1.78 DU yr−1 and are hardly significant at 2σ level. Ozone recovery is also confirmed by a steady decrease of the relative area of total ozone values lower than 150 DU within the vortex in the 15 Sept–15 Oct period since 2010. Comparison of the evolution of the ozone hole area in September and October shows a decrease in September, confirming the later formation of the ozone hole during that month.
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Article dans une revue
Atmospheric Chemistry and Physics Discussions, European Geosciences Union, 2017, pp.(Under Review)
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https://hal-insu.archives-ouvertes.fr/insu-01662115
Contributeur : Catherine Cardon <>
Soumis le : mardi 12 décembre 2017 - 17:04:40
Dernière modification le : jeudi 31 mai 2018 - 20:18:01

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Andrea Pazmino, Sophie Godin-Beeckmann, Alain Hauchecorne, Chantal Claud, Sergey Khaykin, et al.. Symptoms of total ozone recovery inside the Antarctic vortex during Austral spring. Atmospheric Chemistry and Physics Discussions, European Geosciences Union, 2017, pp.(Under Review). 〈insu-01662115〉

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