Omnidirectional spectra, compensated by k^5/3, of magnetic (red) and kinetic (green) energies, with total (solid), parallel (dashed), and perpendicular (dotted) components. In the left panel, we show spectra for the R02 run at t = 40, while the case R11 at t = 10 is shown in the right panel (both times are after the peak of turbulence, see the corresponding blue curves in Fig. 2. Horizontal black lines indicate a k^−5/3 slope, while the kinetic spectra for R11 are better fit by a k^−4/3 slope.