4.7 Article

Effects of reanalysis forcing fields on ozone trends and age of air from a chemical transport model

Journal

ATMOSPHERIC CHEMISTRY AND PHYSICS
Volume 22, Issue 16, Pages 10635-10656

Publisher

COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/acp-22-10635-2022

Keywords

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Funding

  1. National Natural Science Foundation of China [41675039, 91837311]
  2. Natural Science Foundation for universities in Jiangsu province [20KJD170001, 21KJB510007]
  3. Scientific Research Project of Nanjing Xiaozhuang University [2019NXY42]
  4. Natural Environment Research Council [NE/R001782/1]
  5. National Centre for Earth Observation [NE/R016518/1]
  6. NCAS [NE/R015244/1]

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This study used a 3D offline chemical transport model to analyze seasonal behavior and long-term trends in stratospheric ozone and mean age of air. The results show that models forced by different meteorological reanalysis data sets can reproduce variations in stratospheric ozone, but may not accurately simulate observed changes, especially in the lower stratosphere.
We use TOMCAT, a 3-dimensional (3D) offline chemical transport model (CTM) forced by two different meteorological reanalysis data sets (ERA-Interim and ERAS) from the European Centre for MediumRange weather Forecasts (ECMWF) to analyse seasonal behaviour and long-term trends in stratospheric ozone and mean age of air. The model-simulated ozone variations are evaluated against two observation-based data sets. For total column ozone (TCO) comparisons, we use the Copernicus Climate Change Service (C3S) data (1979-2019), while for ozone profiles we use the Stratospheric Water and OzOne Satellite Homogenized (SWOOSH) data set (1984-2019). We find that the CTM simulations forced by ERA-Interim (A_ERAI) and ERA5 (B_ERA5) can both successfully reproduce the spatial and temporal variations in stratospheric ozone. Also, modelled TCO anomalies from B_ERA5 show better agreement with C3S than A_ERAI, especially in Northern Hemisphere (NH) mid latitudes, except that it gives somewhat larger positive biases (> 15 DU, Dobson units) during winter-spring seasons. Ozone profile comparisons against SWOOSH data show larger differences between the two simulations. In the lower stratosphere, ozone differences can be directly attributed to the representation of dynamical processes, whereas in the upper stratosphere they can be directly linked to the differences in temperatures between ERAI and ERA5 data sets. Although TCO anomalies from B_ERA5 show relatively better agreement with C3S compared to A_ERAI, a comparison with SWOOSH data does not confirm that B_ERA5 performs better at simulating the variations in the stratospheric ozone profiles. We employ a multivariate regression model to quantify the TCO and ozone profile trends before and after peak stratospheric halogen loading in 1997. Our results show that, compared to C3S, TCO recovery trends (since 1998) in simulation B_ERAS are significantly overestimated in the Southern Hemisphere (SH) mid latitudes, while for A_ERAI in the NH mid latitudes, simulated ozone trends remain negative. Similarly, in the lower stratosphere, B_ERAS shows positive ozone recovery trends for both NH and SH mid latitudes. In contrast, both SWOOSH and A_ERAI show opposite (negative) trends in the NH mid latitudes. Furthermore, we analyse age of air (AoA) trends to diagnose transport differences between the two reanalysis data sets. Simulation B_ERAS shows a positive AoA trend after 1998 and somewhat older age in the NH lower stratosphere compared to A_ERAI, indicating that a slower Brewer-Dobson circulation does not translate into reduced wintertime ozone buildup in the NH extratropical lower stratosphere. Overall, our results show that models forced by the most recent ERAS reanalyses may not yet be capable of reproducing observed changes in stratospheric ozone, particularly in the lower stratosphere.

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