El Niño Southern Oscillation influence on the Asian summer monsoon anticyclone
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Published:2018-06-08
Issue:11
Volume:18
Page:8079-8096
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ISSN:1680-7324
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Container-title:Atmospheric Chemistry and Physics
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language:en
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Short-container-title:Atmos. Chem. Phys.
Author:
Yan Xiaolu, Konopka Paul, Ploeger Felix, Tao MengchuORCID, Müller RolfORCID, Santee Michelle L., Bian JianchunORCID, Riese MartinORCID
Abstract
Abstract. We analyse the influence of the El Niño Southern Oscillation (ENSO) on
the atmospheric circulation and the mean ozone distribution in the tropical
and subtropical UTLS region. In particular, we focus on the impact of ENSO on
the onset of the Asian summer monsoon (ASM) anticyclone. Using the
Multivariate ENSO Index (MEI), we define climatologies (composites) of
atmospheric circulation and composition in the months following El Niño
and La Niña (boreal) winters and investigate how ENSO-related flow
anomalies propagate into spring and summer. To quantify differences in the
divergent and non-divergent parts of the flow, the velocity potential (VP)
and the stream function (SF) are respectively calculated from the ERA-Interim
reanalysis in the vicinity of the tropical tropopause at potential
temperature level θ=380 K. While VP quantifies the well-known ENSO
anomalies of the Walker circulation, SF can be used to study the impact of
ENSO on the formation of the ASM anticyclone, which turns out to be slightly
weaker after El Niño winters than after La Niña winters. In addition,
stratospheric intrusions around the eastern flank of the anticyclone into the
tropical tropopause layer (TTL) are weaker in the months after strong El
Niño events due to more zonally symmetric subtropical jets than after La
Niña winters. By using satellite (MLS) and in situ (SHADOZ) observations
and model simulations (CLaMS) of ozone, we discuss ENSO-induced differences
around the tropical tropopause. Ozone composites show more zonally symmetric
features with less in-mixed ozone from the stratosphere into the TTL during
and after strong El Niño events and even during the formation of the ASM
anticyclone. These isentropic anomalies are overlaid with the well-known
anomalies of the faster (slower) Hadley and Brewer–Dobson circulations after
El Niño (La Niña) winter. The duration and intensity of El Niño-related anomalies may
be reinforced through late summer and autumn if the El Niño conditions
last until the following winter.
Publisher
Copernicus GmbH
Subject
Atmospheric Science
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