Turbulent kinetic energy spectra as in Figure 14, but at t _pb = 250 ms. Shown are 2D and 3D results for both s15 and s27. At this time, large-scale radial outflow has set in as the models transition to explosion. Notably, the 3D cases show relatively more energy at large scales than for the earlier time shown in Figure 14. The overall normalization of the spectra is lower than for the earlier epoch, reflecting that a large amount of the earlier, non-radial kinetic energy has gone into powering radial outflow.