Temporal evolution of the radial distribution of the different pressure components as a function of distance from the star. The pressure components are thermal, dynamic, magnetic, and total. Plots show the radial distribution along extracted lines in the equatorial plane at four longitudes: 0 (first column), 90 (second column), 180 (third column), and 270 (fourth column) degrees. These are sample snapshots for t = 0 (top panels) and t = 108 hr (bottom panels). An animation of this figure is available. The animation starts at t = 0 and ends at t = 108:30 hr in 30 minute steps. The real-time duration of the animation is 36 s, and it covers the full 108.5 hr of the simulation. 

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.