deletions | additions       diff --git a/subsection_Fourier_Statistics_All_Fourier__.tex b/subsection_Fourier_Statistics_All_Fourier__.tex  index 7ec016c..909f546 100644  --- a/subsection_Fourier_Statistics_All_Fourier__.tex  +++ b/subsection_Fourier_Statistics_All_Fourier__.tex 
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Out of all of our statistics, the VCA demonstrates the weakest sensitivity towards magnetic field strength. The behavior of its color-plot suggests an invariance to turbulent structure, as distances only change with wind model and evolution time. This allows the VCA to clearly detect changes in stellar mass-loss rates of varying sizes. The color plot shows the statistic's outputs for strong wind models to be different from that of all other models. But, once we introduce weaker winds to our turbulent clouds, they begin to resemble each other. As time evolves, the outputs become more alike. The magnetic field's weak impact on this statistic allows us to clearly see this.  Despite the various degrees of sensitivities, many of the intensity statistics fail to produce distinct visual differences corresponding to feedback. As seen in section 3.2, the most common difference is horizontal offset, which is relatively minor (in taking observations?). The VCS does show