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97<br />

Stratospheric variability and its impact on surface climate<br />

Andreas Marc Fischer(1,2), Isla Simpson(3), Stefan Brönnimann(2), Eugene Rozanov(2,4), Martin<br />

Schraner(2)<br />

(1) Federal Office of Meteorology and Climatology, MeteoSwiss, Kraehbuehlstr. 58, 8044 Zurich, Switzerland<br />

(2) Institute for Atmospheric and Climate Science, ETH Zurich, 8092 Zurich, Switzerland. (andreas.fischer@env.ethz.ch)<br />

(3) Department of Physics, Imperial College, London, UK<br />

(2) PMOD/WRC, Dorfstrasse 33, 7260 Davos, Switzerland.<br />

1. Introduction<br />

The stratospheric layer plays a key role in communicating<br />

climate variability over vast regions of the Earth’s<br />

atmosphere. Some of its variability is attributable to natural<br />

drivers such as variations in El Niño Southern Oscillation<br />

(ENSO), solar irradiance, or volcanic eruptions and is<br />

manifest on different timescales from days to seasons and<br />

even longer timescales. Through downward wave<br />

propagation, variability in the stratosphere can impact on<br />

tropospheric climate variability modes and hence surface<br />

climate on different spatial scales. One of the most<br />

prominent stratospheric influence are sudden stratospheric<br />

warmings (SSWs) leaving an imprint on weather at the<br />

ground even a few weeks later (Baldwin and Dunkerton,<br />

2001).<br />

Figure 1 shows the observed surface air temperature (SAT)<br />

and sea level pressure (SLP) response with respect to five<br />

major tropical volcanic eruptions and to ENSO since 1880.<br />

The volcanic signal in the first boreal winter months after<br />

the eruption is characterized by a cooling over the oceans<br />

and a warming over the northern extra-tropical land masses.<br />

Several dynamical feedback mechanisms including the<br />

propagation of planetary waves have been proposed to<br />

explain the pathway of climate anomalies originating from<br />

the stratosphere (see e.g., Stenchikov et al., 2004).<br />

Over recent years much attention has been drawn to the<br />

climatic effect of El Niño on the northern extra-tropical<br />

stratosphere and its manifestation on surface. While the<br />

surface climate response over the North Pacific and North<br />

American region is well known, the signal over the North<br />

Atlantic European sector (negative North Atlantic<br />

Oscillation accompanied by cold (mild) temperatures over<br />

Northern (Southern) Europe) is subject to a large variability<br />

among individual El Niño events which complicates its<br />

interpretation. Ineson and Scaife (2009) provided evidence<br />

for a global teleconnection pathway from the Pacific region<br />

to Europe via the stratosphere. They showed that, in<br />

presence of SSWs, the stratosphere plays an active role in<br />

the manifestation of the European regional climate pattern.<br />

A better knowledge of the impact of stratospheric variability<br />

on regional surface climate is therefore highly relevant with<br />

respect to detection and attribution studies as well as<br />

improvements of seasonal prediction schemes.<br />

volcanic<br />

ENSO<br />

-1.8<br />

-0.6<br />

-0.6<br />

-0.2<br />

0.6<br />

0.2<br />

1.8<br />

0.6<br />

(°C)<br />

(°C/°C)<br />

Figure 1. Effect of tropical volcanic eruptions (top)<br />

and ENSO (bottom) on boreal winter (Jan-Mar) SAT<br />

and SLP since 1880. Temperature and SLP data<br />

were detrended. The top panel shows a composite of<br />

the first winters after five tropical eruptions<br />

(Krakatoa, Santa Maria, Mt. Agung, El Chichón,<br />

Pinatubo). The bottom panel shows regression<br />

coefficients using a NINO3.4 index (Sep-Feb<br />

average) after removing two winters after each<br />

major volcanic eruption<br />

2. Model Simulations<br />

To study stratosphere-troposphere exchange processes<br />

global chemistry-climate models (CCMs) have proven to<br />

be indispensable tools as they incorporate all relevant<br />

dynamical, radiative, and chemical processes in the<br />

atmosphere (Eyring et al., 2006).<br />

Here we present results of two different kinds of<br />

simulations with the CCM SOCOL (Schraner et al.,<br />

2008): (a) ensemble simulations (9 members) in transient<br />

mode across the 20 th century (Fischer et al., 2008a); (b)<br />

time-slice simulations (20 ensemble members) of an<br />

anomalously strong El Niño (1940-42) and a weak La<br />

Niña (1975-76) (Fischer et al., 2008b). SOCOL is a<br />

combination of the middle atmosphere version of<br />

ECHAM4 (MPI, Hamburg) and the chemistry-transport<br />

model MEZON (PMOD/WRC, Davos). The simulations

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