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@ARTICLE{Diallo:862051,
author = {Diallo, Mohamadou and Konopka, Paul and Santee, Michelle L.
and Müller, Rolf and Tao, Mengchu and Walker, Kaley A. and
Legras, Bernard and Riese, Martin and Ern, Manfred and
Ploeger, Felix},
title = {{S}tructural changes in the shallow and transition branch
of the {B}rewer–{D}obson circulation induced by {E}l
{N}iño},
journal = {Atmospheric chemistry and physics},
volume = {19},
number = {1},
issn = {1680-7324},
address = {Katlenburg-Lindau},
publisher = {EGU},
reportid = {FZJ-2019-02417},
pages = {425 - 446},
year = {2019},
abstract = {The stratospheric Brewer–Dobson circulation (BDC)
determines the transport and atmospheric lifetime of key
radiatively active trace gases and further impacts surface
climate through downward coupling. Here, we quantify the
variability in the lower stratospheric BDC induced by the El
Niño–Southern Oscillation (ENSO), using satellite trace
gas measurements and simulations with the Lagrangian
chemistry transport model, CLaMS, driven by ERA-Interim and
JRA-55 reanalyses. We show that despite discrepancies in the
deseasonalized ozone (O3) mixing ratios between CLaMS
simulations and satellite observations, the patterns of
changes in the lower stratospheric O3 anomalies induced by
ENSO agree remarkably well over the 2005–2016 period.
Particularly during the most recent El Niño in 2015–2016,
both satellite observations and CLaMS simulations show the
largest negative tropical O3 anomaly in the record.
Regression analysis of different metrics of the BDC
strength, including mean age of air, vertical velocity,
residual circulation, and age spectrum, shows clear evidence
of structural changes in the BDC in the lower stratosphere
induced by El Niño, consistent with observed O3 anomalies.
These structural changes during El Niño include a weakening
of the transition branch of the BDC between about 370 and
420 K (∼100–70 hPa) and equatorward of about 60∘
and a strengthening of the shallow branch at the same
latitudes and between about 420 and 500 K
(∼70–30 hPa). The slowdown of the transition branch is
due to an upward shift in the dissipation height of the
large-scale and gravity waves, while the strengthening of
the shallow branch results mainly from enhanced gravity wave
breaking in the tropics–subtropics combined with enhanced
planetary wave breaking at high latitudes. The strengthening
of the shallow branch induces negative tropical O3 anomalies
due to enhanced tropical upwelling, while the weakening of
the transition branch combined with enhanced downwelling due
to the strengthening shallow branch leads to positive O3
anomalies in the extratropical upper troposphere–lower
stratosphere (UTLS). Our results suggest that a shift in the
ENSO basic state toward more frequent El Niño-like
conditions in a warmer future climate will substantially
alter UTLS trace gas distributions due to these changes in
the vertical structure of the stratospheric circulation.},
cin = {IEK-7},
ddc = {550},
cid = {I:(DE-Juel1)IEK-7-20101013},
pnm = {244 - Composition and dynamics of the upper troposphere and
middle atmosphere (POF3-244)},
pid = {G:(DE-HGF)POF3-244},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000455810000001},
doi = {10.5194/acp-19-425-2019},
url = {https://juser.fz-juelich.de/record/862051},
}