The updated trends and solar response in stratospheric ozone based on satellite data and model simulations
ID:2314 View Protection:PRIVATE Updated Time:2023-04-27 13:14:39 Hits:1767 Invited speech

Start Time:2023-05-07 08:15(Asia/Shanghai)

Duration:15min

Session:13B 13B、大气物理与气象气候 » 13B-113B-1 大气物理和大气探测

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Abstract
We use the TOMCAT 3-D off-line chemical transport model (CTM) to investigate the seasonal ozone trends and solar response in stratospheric ozone. The model simulations forced with European Centre for Medium-Range Weather Forecasts (ECMWF) reanalyses (ERA-Interim and ERA5) data, A_ERAI and B_ERA5, are compared to observation-based data sets, the Stratospheric Water and OzOne Satellite Homogenized (SWOOSH, Davis et al., 2016) database (1984-2020) and machine learning based satellite-corrected data (ML-TOMCAT, Dhomse et al., 2021) for the 1979-2020 time period. We find large differences between the modeled and observed ozone profiles and simulation B_ERA5 does not perform better in simulating the observed stratospheric ozone when compared to A_ERAI (Li et al., 2022).
We employ a multi-variate regression model (MLR) to estimate the trends and solar cycle signals (SCS) in both the modelled and observed ozone profiles. Both the ordinary least squares (OLS) and regularised regression methods (Ridge/Lasso) are used for comparison. The MLR includes independent linear trends before and after peak stratospheric halogen loading in 1997, Quasi-Biennial Oscillation (QBO) terms at 30 hPa and 10 hPa, El-Nino Southern Oscillation (ENSO), Arctic Oscillation (AO), Antarctic Oscillation (AAO) index as well as the vertical component of the E-P flux or the age-of-air (AoA) tracer to account for the effects of dynamical variability. We find that both ozone trends and SCS vary with the fit methods, datasets and analysis periods. ML-TOMCAT data agree better with SWOOSH data in ozone trends and SCS than the two model simulations do. AoA associated transport changes the lower stratospheric ozone trends as well as the solar cycle estimates, which suggests the stratospheric dynamics might have influenced the stratospheric ozone, particularly in the lower stratosphere, resulting in the significantly different SCS.
References:
Davis, S.M., Rosenlof, K.H., Hassler, B., Hurst, D.F., Read, W.G., Vömel, H., Selkirk, H., Fujiwara, M. and Damadeo, R., 2016. The Stratospheric Water and Ozone Satellite Homogenized (SWOOSH) database: a long-term database for climate studies. Earth system science data, 8(2), pp.461-490.
Dhomse, S.S., Arosio, C., Feng, W., Rozanov, A., Weber, M. and Chipperfield, M.P., 2021. ML-TOMCAT: machine-learning-based satellite-corrected global stratospheric ozone profile data set from a chemical transport model. Earth System Science Data, 13(12), pp.5711-5729.
Li, Y., Dhomse, S. S., Chipperfield, M. P., Feng, W., Chrysanthou, A., Xia, Y., and Guo, D., 2022. Effects of reanalysis forcing fields on ozone trends and age of air from a chemical transport model, Atmos. Chem. Phys., 22, 10635–10656.
 
Keywords
ozone,trends,stratosphere,solar response
Speaker
李亚娟
南京晓庄学院

Submission Author
LiYajuan Nanjing Xiaozhuang University
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Important Date
  • Conference Date

    May 05

    2023

    to

    May 08

    2023

  • Mar 31 2023

    Draft paper submission deadline

  • May 25 2023

    Registration deadline

Sponsored By
青年地学论坛理事会
中国科学院青年创新促进会地学分会
Organized By
武汉大学
中国科学院精密测量科学与技术创新研究院
中国地质大学(武汉)
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