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In Figure 2.5 are shown the probability density functions of
vorticity fluctuations
at various ,
rescaled by their rms value
.
As the separation decreases, the probability of
observing very weak or very intense vorticity excursions increases
at the expense of fluctuations of average intensity.
This phenomenon goes under the name of intermittency.
The non-similarity of the probability density functions
reflects in the non-linear behavior for the scaling exponents
predicted by Eq. (2.33).
Figure:
Probability density functions of normalized vorticity
increments
.
Here, (),
(), (
).
For large separations the statistics is close to Gaussian,
becoming increasingly intermittent for smaller .
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Stefano Musacchio
2004-01-09