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\subsection{Intensity statistics}  We show the colorplots for all intensity statistics in Figure ???. With the exception of the Cramer statistic, we find that these statistics exhibit strong sensitivities to changes in stellar mass-loss rates. rate.  As seen in their colorplots, the largest distances appear when any strong wind model (W1) is compared to either a weak wind model (W2) or a purely turbulent model (TXt0).The Kurtosis, Skewness, and SCF are clear examples of this, as they display a sensitivity trend among pairings. These statistics yield the largest distances between pairs of W1 and TXt0, followed by pairs of W1 and W2. And, they capture similar, weaker sensitivities between pairs of W2 and TXt0. %mention the role of evolutionary time here? More time=greater difference causes via feedback