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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 2.

Evolution along the representative trajectories associated with Figure 1. For Ms ≃ 1 (left) and Ms ≃ 10 (right), the panels show δB/〈B〉, the pitch-angle cosine μ, and the normalized first adiabatic invariant (1 − μ2)〈B〉/B as functions of tΩ. Red, blue, and green denote decoupled, intermediate, and strongly coupled runs. Approximate conservation of (1 − μ2)〈B〉/B indicates adiabatic mirror motion, whereas abrupt changes indicate nonadiabatic pitch-angle scattering.

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