Image Details
Caption: Figure 2.
(a)–(d) Magnetic energy spectra eM(k) at a given Pm for models listed in the legends. The k3/2 Kazantsev scaling is indicated in the lower left (dotted dark blue line). (e)–(h) Corresponding kinetic energy spectra eK(k). The k−5/3 Kolmogorov scaling is indicated in the upper center (dotted dark blue line).
© 2026. The Author(s). Published by the American Astronomical Society.