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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 4.

Dimensionless diffusion coefficients as functions of Alfvénic Mach number in solenoidally driven single-fluid turbulence. The left and right panels show Ms ≃ 1 and Ms ≃ 10, respectively. Solid and dashed curves denote D/(cLbox) and D/(cLbox) for rL/Lbox ≃ 8 × 10−3 and 8 × 10−2. Increasing MA reduces D and drives D/D toward unity.

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