Intermittency in fluid turbulence can be evidentiated through the analysis
of Probability Distribution Functions (PDF) for velocity fluctuations, whic
h display a strong non-Gaussian behaviour at small scales. In this paper, w
e investigate the occurrence of intermittency in plasma turbulence by study
ing the departure from the Gaussian distribution of PDF for both velocity a
nd magnetic fluctuations. We use data coming from two different experiments
, namely in situ satellite observations of the inner solar wind and turbule
nt fluctuations in a magnetically confined fusion plasma. Moreover, we inve
stigate also time intermittency observed in a simplified shell model which
mimics 3D MED equations, We found that the departure from a Gaussian distri
bution is the main characteristic of all cases. The scaling behaviour of PD
Fs are then investigated by using two different models built up in the past
years, in order to capture the essence of intermittency in turbulence. (C)
2001 Elsevier Science Ltd. All rights reserved.