Image Details
Caption: Figure 12.
Evolution of transverse magnetic field B⊥ for the runs PLI:5-400:p−3, PLI:5-400(p−4), and PLI:5-400:p−5. Inset: saturated magnetic field ﹩{\left({B}_{\perp }/{B}_{0}\right)}_{\,\rm{sat}\,}﹩ vs. anisotropy parameter ξ for these runs (green pentagon for p−5, pink square for p−4, blue nabla for p−3). The gray dashed line represents Equation (15).
© 2026. The Author(s). Published by the American Astronomical Society.