  Synthetic turbulence is a relevant tool to study complex astrophysical and
space plasma environments inaccessible by direct simulation. However,
conventional models lack intermittent coherent structures, which are essential
in realistic turbulence. We present a novel method, featuring coherent
structures, conditional structure function scaling and fieldline curvature
statistics comparable to magnetohydrodynamic turbulence. Enhanced transport of
charged particles is investigated as well. This method presents significant
progress towards physically faithful synthetic turbulence.
