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\subsection{Intensity Statistics}  We show the colorplots for all intensity statistics in Figure ??? ???. With the exception of the Cramer statistic (give background sentence here since this was not discussed in the results section), the intensity statistics produce similar colorplots and exhibit strong sensitivities towards changes in stellar mass-loss rates. We calculate the   PDF-Hellinger Distance; Kurt/Skew--Hellinger; PCA; Diff between 1st 50 eigenvalues (kind of like hellinger distance); SCF--Weigted Difference; Cramer--is a distance between two data sets