  We have previously generated elongated Taylor double-helix flux rope plasmas
in the SSX MHD wind tunnel. These plasmas are remarkable in their rapid
relaxation (about one Alfv\'en time) and their description by simple analytical
Taylor force-free theory despite their high plasma beta and high internal flow
speeds. We report on the turbulent features observed in these plasmas including
frequency spectra, autocorrelation function, and probability distribution
functions of increments. We discuss here the possibility that the turbulence
facilitating access to the final state supports coherent structures and
intermittency revealed by non-Gaussian signatures in the statistics.
Comparisons to a Hall-MHD simulation of the SSX MHD wind tunnel show similarity
in several statistical measures.
