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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

The atmospheric response to solar cycle variability simulated by MAECHAM5 with <strong>an</strong>d<br />

without oce<strong>an</strong> coupling<br />

Misios Stergios , Schmidt Hauke<br />

Max Pl<strong>an</strong>ck <strong>Institut</strong>e for Meteorology<br />

The 11-year solar cycle variation has a well demonstrated impact on the Northern Hemisphere<br />

winter stratosphere. During early winter of maximum solar activity years the stratospheric<br />

vortex tends to be stronger <strong>an</strong>d col<strong>der</strong> in contrast to minimum activity. While there is a<br />

relative consensus on the stratospheric response, the pathways through which the solar signal<br />

is propagated into the troposphere are still un<strong>der</strong> debate. The surface response in particular<br />

regions, as in the Equatorial Pacific, further perplexes our un<strong>der</strong>st<strong>an</strong>ding. In this work, we<br />

explore the inseparable troposphere-stratosphere response of the 11-yr solar cycle with the aid<br />

of fully coupled atmosphere-oce<strong>an</strong> general circulation model (GCM).<br />

Simulations with the MAECHAM5 GCM with a realistic time varying solar forcing (as<br />

observed from 1955 to 2006) <strong>an</strong>d prescribed ozone <strong>an</strong>omalies are carried out. No other<br />

external forcing is consi<strong>der</strong>ed. The quasi-biennial oscillation (QBO) is spont<strong>an</strong>eously<br />

generated in the model. We conduct 9 ensemble runs over 52 years each with MAECHAM5<br />

coupled to the MPI oce<strong>an</strong> model (MPIOM) <strong>an</strong>d compare the results to <strong>an</strong>other 9 member<br />

ensemble with prescribed sea surface temperature (SST).<br />

In this study, the domain of interest is the equatorial <strong>an</strong>d subtropical stratosphere <strong>an</strong>d<br />

troposphere with a special focus on the Pacific region. Our <strong>an</strong>alysis reveals that the<br />

tropospheric response in the coupled runs differs subst<strong>an</strong>tially from the uncoupled. The<br />

prescribed SSTs damp the temperature solar signal <strong>an</strong>d statistically signific<strong>an</strong>t results are<br />

obtained only in the experiments with time varying SSTs. Both coupled <strong>an</strong>d uncoupled<br />

simulations show a pronounced secondary maximum in the lower equatorial stratosphere<br />

which is somewhat stronger in the coupled ensemble. In the equatorial Pacific a tongue of<br />

weak negative temperature <strong>an</strong>omalies c<strong>an</strong> also be found. In our presentation, we further<br />

elaborate on the mech<strong>an</strong>isms that may explain the simulated solar response.

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