Image Details
Caption: Figure 3.
Similar to Figure 2, except that the CRs initially have cone distributions. Left panels: The spatial profiles of the magnetic field components at ﹩t\approx 7{\gamma }_{\,\rm{fast}\,}^{-1}﹩. The x-axes are normalized to λfast = 2π/kfast ≈ 50di. In the shaded zoomed-in part, the dominant wavelengths ∼λfast are prominent. Right panels: Time evolution of helicities Δϕ(k).
© 2026. The Author(s). Published by the American Astronomical Society.