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We present the results of a velocity correlation study of the high latitudecloud MBM16 using a fully sampled $^{12}$CO map, supplemented by new $^{13}$COdata. We find a correlation length of 0.4 pc. This is similar in size to theformaldehyde clumps described in our previous study. We associate thiscorrelated motion with coherent structures within the turbulent flow. Suchstructures are generated by free shear flows. Their presence in this non-starforming cloud indicates that kinetic energy is being supplied to the internalturbulence by an external shear flow. Such large scale driving over long timesis a possible solution to the dissipation problem for molecular cloudturbulence.Comment: Uses AAS aasms4.sty macros. Accepted for publication in Ap

A Dynamical Study of the Non–Star‐forming Translucent Molecular Cloud MBM 16: Evidence for Shear‐driven Turbulence in the Interstellar Medium