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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 A1.

Pitch-angle mean-square variations 〈(Δμ)2〉, as a function of the normalized time tΩ for the Ms ≃ 10 and MA ≃ 10 simulation. The initial pitch angle distribution is isotropic with rL/Lbox ≃ 8 × 10−3. The blue and red curves show results obtained using 103 and 104 particles, respectively. The gray dotted line marks the saturation value.

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