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Depth (m)<br />

50<br />

100<br />

150<br />

200<br />

a<br />

250<br />

2.5 3 3.5 4 4.5 5 5.5 6 6.5 7 7.5 8<br />

θ ( o C)<br />

8 x 10−3 Days since 31 August 1997<br />

Var θ , (K 2 )<br />

6<br />

4<br />

2<br />

b<br />

0<br />

0 50 100 150 200 250 300 350 400 450<br />

4<br />

x 10 −5<br />

c<br />

κ θ<br />

(m 2 /s)<br />

2<br />

0<br />

0 1 2 3 4 5 6 7 8 9 10<br />

L (m)<br />

Figure 3.11: (a) Potential temperature prole from 27 March 1998, ltered with a cut-o length of 3<br />

m (grey stars) and 50 m (black dots). Horizontal lines indicate the intrusion layer (90-170 m) used for<br />

the analysis; (b) time series of 〈θ ′2 〉 (stars) for all available temperature proles between 31 August 1997<br />

and 7 November 1998, and exponential t (dashed line); (c) vertical intrusion scale, L, vs. diusivity of<br />

heat, κ θ .<br />

variance associated with the intrusions,<br />

∂〈θ ′2 〉<br />

∂t<br />

〈 ( ) ∂θ<br />

′ 2 〉<br />

= −2κ θ<br />

∂z<br />

≈ −2κ θ<br />

〈θ ′2 〉<br />

L 2 , (3.9)<br />

where in the last step we have assumed that vertical gradients are characterised by the standard<br />

42

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