Image Details
Caption: Figure 10.
The omnidirectional spectrum of B⊥ as a function of ∣k∣ for each simulation taken at tpeak. Each spectrum is multiplied by k5/3 such that a Kolmogorov-type spectrum would result in a horizontal line. All spectra are approximately flat across the low-k inertial range before breaking around k di = 1 due to the low-pass filter in dHybridR.
© 2026. The Author(s). Published by the American Astronomical Society.