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Structural changes in the shallow and transition branch of the Brewer–Dobson circulation induced by El Niño

The global meridional overturning of mass in the stratosphere, generally known as the Brewer-Dobson circulation (BDC), plays a crucial role in Earth’s climate system by controlling the distributions of atmospheric constituents. The El Niño–Southern Oscillation (ENSO) is a major mode of climate variability that affects the BDC.

 Structural changes in the shallow and transition branch of the Brewer–Dobson circulation induced by El Niño

MLS measurements and simulations with a Lagrangian chemistry transport model driven by two meteorological reanalyses show substantial negative anomalies in lower stratospheric ozone during El Niño years (2006–2007, 2010–2011, 2015–2016) and positive anomalies during La Niña years (2008–2009, 2011–2012, 2013–2014). In particular, the El Niño event in 2015–2016 induced a record anomaly of –15% in the tropics according to MLS (bottom row) as a result of a strengthening of the tropical upwelling

Monthly mean ozone anomalies over the period 2005–2016 from the Aura Microwave Limb Sounder (MLS) and Lagrangian model simulations driven by two meteorological reanalyses are analyzed using a multiple regression model to elucidate the impact of ENSO on the BDC. The patterns of ENSO-induced variations in lower stratospheric ozone (negative in El Niño years, positive in La Niña years) seen in MLS data agree well with those from both model runs.

Regression analysis of various model diagnostics of the circulation strength reveals structural changes in the lower stratospheric branches of the BDC, with a weakening of the “transition” branch (~370–420 K) and a strengthening of the “shallow” branch (~420–500 K) during El Niño, and opposite changes during La Niña.

ENSO-related structural changes in the stratospheric mean meridional circulation affect the distributions of radiatively active gases in the upper troposphere / lower stratosphere, in turn affecting climate.

Technical description of figure:

Figure 2 of above reference. Latitude/time evolution of the ENSO impact on lower stratospheric O3 from (a) CLaMS simulations driven by ERA-I, (b) CLaMS simulations driven by JRA-55, and (c) MLS observations, in percent change from the monthly zonal mean climatology derived from the multiple regression fit and averaged between 380 and 425 K for the 2005–2016 period. Note the factor of two difference in the color scales in (a) and (b) versus (c), reflecting differences in the magnitude of the deseasonalized O3 mixing ratios between CLaMS and MLS that arise from model deficiencies. Panel (d) shows the multivariate ENSO index (MEI) in blue. The vertical black dashed line indicates the onset of a warm El Niño event in February 2015 that produced an extremely large negative O3 anomaly in the tropical lower stratosphere.

Scientific significance, societal relevance, and relationships to future missions:

The structural changes in stratospheric circulation associated with ENSO found in this study affect the distributions of radiatively active trace gases in the UTLS, which, in turn, impact the global radiation budget. Hence, the ENSO influence on the BDC provides a pathway for stratospheric influence on future climate. Since climate change is expected to increase the frequency of El Niño-like conditions in the future, the ENSO effect on the BDC will become increasingly important in determining UTLS trace gas distributions. Thus the results of this study underscore the critical need for continued monitoring of vertically resolved profiles of ozone (and other radiatively important trace gases) to detect and understand variability and trends. In addition to the continuing record from Aura MLS and other current sensors, vertically resolved limb measurements of O3 will be available from the planned Ozone Mapper and Profiler Suite Limb Profiler (OMPS-LP) scheduled to be launched on Joint Polar Satellite System (JPSS)-2 in 2022.

Data Sources:

Aura Microwave Limb Sounder version 4.2 measurements of O3, publicly available from http://disc.sci.gsfc.nasa.gov/Aura/data-holdings/MLS/index.shtml. MLS O3 is compared to simulated fields from the Chemical Lagrangian Model of the Stratosphere (CLaMS; McKenna et al., JGR 107, 2002; Konopka et al., JGR 109, 2004), available on request from the corresponding author, Mohamadou Diallo (m.diallo@fz-juelich.de). The model simulations were driven by temperatures, horizontal winds, and diabatic heating rates from both the European Centre for Medium-Range Weather Forecasts ERA-Interim (ERA-I) reanalysis (Dee et al., QJRMS 137, 2011; https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era-interim) and the Japan Meteorological Agency Japanese 55-year Reanalysis (JRA-55; Kobayashi et al., J. Meteorol. Soc. Jpn. 93, 2015).


References: Diallo, M., P. Konopka, M.L. Santee, R. Müller, M. Tao, K.A. Walker, B. Legras, M. Riese, M. Ern, and F. Ploeger, Structural changes in the shallow and transition branch of the Brewer–Dobson circulation induced by El Niño, Atmos. Chem. Phys., 19, 425--446, doi:10.5194/acp-19-425-2019, 2019.


6.2019


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