deletions | additions       diff --git a/subsection_Fourier_statistics_All_Fourier__.tex b/subsection_Fourier_statistics_All_Fourier__.tex  index d922267..532feb3 100644  --- a/subsection_Fourier_statistics_All_Fourier__.tex  +++ b/subsection_Fourier_statistics_All_Fourier__.tex 
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Out of all of the statistics, the VCA demonstrates the weakest sensitivity towards magnetic field strength. The behavior of its color-plot suggests an insensitivity 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. The color plot shows the distances for strong wind models to be different from those of all other models. But as time evolves, the weak wind distances more closely resemble the strong wind distances. This trend is clear because of the magnetic field's weak impact on the statistic.  Despite the various degrees of sensitivities, many of the Fourier statistics fail to produce distinct visual differences corresponding to feedback. As discussed in section 3.2, the most common difference is horizontal offset/power spectra/characteristic energy scale, which is relatively minor (in taking observations?). minor.  The VCS does produce distinct responses, but its color plot suggests sensitivities to parameters other than stellar mass-loss rates.