In turbulent flows, the transfer of energy from large to small scales is st
rongly intermittent, in contradiction with Kolmogorov's (Dokl. Akad. Nauk.
SSSR 30 (1941) 299; hereafter K41) assumptions. The statistical proper-ties
associated with these energy transfer fluctuations at a given scale r have
been widely studied theoretically, experimentally and numerically over the
last 30 years or so. Such fluctuations are also encountered in various Pla
netary and Space Science domains. The present paper presents a review of la
boratory experiments which clearly display the fractal nature of the (spati
al or temporal) energy distribution at scale r, the departures from the K41
predictions being generally quantified through high-order moments of veloc
ity increments. (C) 2001 Published by Elsevier Science Ltd.