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Mooring Time Periods 〈u〉(cm/s) 〈v〉(cm/s) |V | max(cm/s)<br />

Pre-inow<br />

NE 30.8.1997 - 27.11.1997 −1.9 2.4 22.6<br />

SW 30.8.1997 - 26.12.1997 0.5 −3.0 19.1<br />

Inow<br />

NE 28.11.1997 - 6.5.1998 −3.1 4.2 29.0<br />

SW 27.12.1997 - 25.5.1998 0.9 −4.0 32.2<br />

Post-inow<br />

NE 7.5. - 21.7.1998 −0.5 0.3 12.1<br />

SW 26.5. - 21.7.1998 −1.7 −2.5 20.6<br />

Table 3.1: Averaged zonal 〈u〉 and meridional 〈v〉 velocities at moorings NE and SW before, during and<br />

after the inow, as well as maximum hourly speeds (|V | max ).<br />

at 170 m depth on a basin scale which is forced and/or maintained by rotationally deected<br />

near-bottom gravity currents entering the EGB above its eastern topographic ank. Associated<br />

uctuations in their forcing generate pulses of warm water intrusions propagating roughly along<br />

the deep isobaths from the mooring NE towards that of the position SW. Thus, these observations<br />

conrm the scenario of the deep water circulation in the EGB proposed by Lehmann<br />

and Hinrichsen (2000) and Zhurbas et al. (2003) developed on the base of numerical<br />

experiments from dierent hydrodynamic models.<br />

3.1.2 MESODYN data<br />

The two hydrographic snapshots, part of the MESODYN project, compare stagnant deep<br />

water conditions (M-7) with those measured after the inow event (M-8) at the times indicated<br />

in Fig. 3.1 a. The overall θ-S diagrams of the two hydrographic surveys (Fig. 3.2)<br />

describe the changes in water composition and variability induced by the inow for layers<br />

deeper than 60 m. Obtained relations are compared with the 'climatological state' monitored<br />

at the BMP271 station (1968-1998). Before the inow, potential temperatures are below the<br />

30 year averages, and their θ-S cluster is located inside the standard deviations of the climatological<br />

data (Fig. 3.2 a). Associated thermohaline changes can be described by comparing<br />

these pre-inow characteristics with those of the M-8 campaign. The isopycnal variability of<br />

θ-S properties, embedded in the potential density layer of the halocline (σ θ = 6.8-8.5 kg/m 3 )<br />

was very small during the pre-inow period. This is conrmed by the spatially computed<br />

standard deviations on selected density surfaces. Further towards the sea bed, (8.5 ≤ σ θ ≤<br />

26

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