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Slow Cosmic-Ray Diffusion in Supersonic and Super-Alfvénic Turbulence

  • Authors: Yue Hu

Yue Hu 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

Representative CR trajectories with rL/Lbox = 8 × 10−3 (rL = 10 cells) overlaid on the normalized magnetic fluctuation δB/〈B〉 in a slice through each particle’s initial position. Blue arrows indicate the in-plane magnetic-field direction. The left and right columns show decoupled and strongly coupled two-fluid turbulence, respectively; the upper and lower rows show Ms ≃ 1 and Ms ≃ 10, with MA ≃ 1 in all panels. Trajectory color denotes tΩ, and green and red markers indicate the initial and final positions.

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