  An extended data set of extreme ultraviolet images of the solar corona
provided by the SOHO spacecraft are analyzed using statistical methods common
to studies of self-organized criticality (SOC) and intermittent turbulence
(IT). The data exhibits simultaneous hallmarks of both regimes, namely power
law avalanche statistics as well as multiscaling of structure functions for
spatial activity. This implies that both SOC and IT may be manifestations of a
single complex dynamical process entangling avalanches of magnetic energy
dissipation with turbulent particle flows.
