Corresponds to points at 2 o'clock on the previous image.		Corresponds to data at about 4 o'clock (only 1 or 2 points, very close to the star's outline)
	For this phase, the timesteps 31, 27, 55, 20, 22, 23, 60, 21, 35, 41, 47, 32, 46, and 36 contribute to the redshifted wing on the line profile.	This isn't the most helpful image, but it's a start. I picked one of the zones that contributes to the redshifted part of the line profile randomly and plotted in it's original xz-coordinates (like the 2D contours) where the highest EM points are that contribute to the redshifted emission. Occulation has not been taken into account, but the magnetic equator should be visible to the obsever. There's one point where it looks like infall is the only explanation, but it's still very difficult to say.	Well, if this isn't convincing evidence for infall as the source of the redshifted emission then I don't know what is.	Guess who's completely sold now? That's right, me.