Image Details
Caption: Figure 6.
Power spectra of the velocity (v, left) and vorticity (ω = ∇ × v, right) fields in the x−z plane (current sheet midplane) at different time steps of the simulation with S = 105, β = 2.0, Prm = 1, and Pinj = 0.5. The black dashed lines represents the 1D Kolmogorov turbulent power spectra of ﹩{ \mathcal P }(k)\propto {k}^{-8/3}﹩ (velocity) and ﹩{ \mathcal P }(k)\propto {k}^{-2/3}﹩ (vorticity).
© 2025. The Author(s). Published by the American Astronomical Society.