In a toroidal plasma confined by a purely toroidal magnetic field the plasma transport is governed by electrostatic turbulence driven by the flute interchange instability on the low-field side of the torus cross section. In this paper we revisit experimental data obtained from the Blaamann torus at the University of Tromsø. On time-scales shorter than the poloidal rotation time, the time series of potential and electron density fluctuations measured on stationary Langmuir probes essentially reflect the spatial poloidal structure of the turbulent field (Taylor hypothesis). On these time scales the signals reveals an intermittent character exposed via analysis of probability density functions and computation of multifractal dimension spectra in different regimes of time scales. This intermittency is associated with the shape and distribution of pronounced spikes in the signal. On time scales much longer than the rotation period there are strong global fluctuations in the plasma potential which are shown to to be the result of low-dimensional chaotic dynamics.A useful classification of complex systems behavior should allow different behaviors to be distinguished through observation. For instance, in some cases observational spatiotemporal information is only available as fluctuations of one or more point observations, or at best as a scalar two-dimensional (2D) radiation field emitted from a system, while the internal 3D dynamics is not practically accessible to direct observation. Analysis of such fields reveals the existence of complex systems which at the same time exhibit statistical signatures that are traditionally attributed to either turbulence or selforganized critical avalanching dynamics (SOC). Examples are solar flare activity, polar aurora, fluctuations associated with anomalous transport in magnetic fusion plasma, and vortical fluid flows in ordered structures like dusty plasma quasi-crystals. For turbulent systems structure functions of the velocity field reveal an approximate scale-invariant structure, but the deviation from scaling ascribed to intermittency (or multifractality) has received a lot of attention in recent years. For a system in an SOC state local avalanche analysis reveals that the probability distributions of avalanche size and duration are approximately scale-free, but deviations from perfect scaling and their relation to the finite system size have been studied in different frameworks like finite-size scaling and multifractal scaling [1]. Appearance of intermittency has often been taken as a signature of turbulence. For instance, Consolini [2] interpreted multifractality in the time series of the auroral electrojet index as a signature that turbulence plays a major role in the magnetosphere-ionosphere interaction, and recently Govolchanskaya et al. [3] draw the same conclusion from observing spatial intermittency in auroral images. On the other hand, in the fusion literature, mono-fractal scaling with long-range time-dependence has