  Plasma turbulence involves complex, nonlinear interactions of electromagnetic
fields and charged particles across multiple scales. Studying these phenomena
in space plasmas, like the solar wind, is facilitated by the intrinsic scale
separations and the availability of in situ spacecraft observations. However,
the single-point or single-scale configurations of current spacecraft limit our
understanding of many properties of the turbulent solar wind. To overcome these
limitations, multipoint measurements spanning a range of characteristic scales
are essential. This paper prepares for the enhanced measurement capabilities of
upcoming multispacecraft missions by demonstrating that higher-order
statistics, specifically kurtosis, as a baseline for intermittency can be
accurately measured. Using synthetic turbulent fields with adjustable
intermittency levels, we achieve scale separations analogous to those in the
solar wind and apply these techniques to the planned trajectories of the
HelioSwarm mission. This approach promises significant advancements in our
understanding of plasma turbulence.
