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EUCLIPSE First Period Report

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perturbed future climate conditions are enforced by increasing the SST by 2K and by<br />

weakening the subsidence.<br />

Figure 6. Schematic of the stratocumulus to cumulus transitions as observed<br />

during the <strong>First</strong> Lagrangian of ASTEX. Five aircraft flights were performed<br />

between 12-14 June 1992.<br />

a. Set up of the ASTEX transition case<br />

For a model intercomparison case the time-dependent large-scale divergence rate, the<br />

sea surface temperature (SST), and the geostrophic wind components need to be<br />

prescribed. Because a Lagrangian trajectory is modelled the horizontal advection<br />

terms can be neglected.<br />

The SST is taken from Bretherton et al. (1999), who provide a best estimate of the<br />

time-varying SST along the ASTEX <strong>First</strong> Lagrangian trajectory on the basis of ECWMF<br />

SST fields that were obtained with a data assimilation procedure, direct<br />

measurements from the ship R/V Oceanus and radiometric observations from aircraft.<br />

In the subtropical parts over the oceans, the large-scale divergence of the horizontal<br />

winds is characterized by positive values in the lower part of the atmosphere, which is<br />

associated with a large-scale descending motion, which is often referred to as largescale<br />

subsidence. For the ASTEX area, there is a considerable uncertainty not only in<br />

the magnitude but also in the sign of the large-scale divergence. Bretherton et al.<br />

analysed ERA-40 data and found that the large-scale divergence in the column<br />

changed sign after approximately 15 hours (see Figure 7). By contrast, Ciesielski et<br />

al. (1999) calculated the large-scale divergence directly from radiosonde observations<br />

and found no change in the sign. Sigg and Svensson (2004) applied a spectral<br />

23

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