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\subsection{Intensity Statistics}  We show the colorplots for all intensity statistics in Figure ???. The PDF, Skewness, Kurtosis, PCA, and SCF produce similar colorplots and exhibit strong colorplots, exhibiting the strongest  sensitivities towardschanges in  stellar mass-loss rates. The Kurtosis   For these statistics, we find that the  largest distance metric values occur when comparing distances are obtained by pairing  a strong wind model (W1) with a purely turbulent model one  (t0). The second largest values occur when comparing a strong wing model to a weak one (W2). For the The  Kurtosis and Skewness plots, we find a clear distinction between these two distances. plots clearly show this orde.  Differences in magnetic field strengths appear to blur this distinction in our PDF, PCA, and SCF plots. Furthermore,   --Moment stats also slightly sensitive to T; PCA and SCF no!!!