Image Details

Choose export citation format:

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 3.

Dimensionless CR transport coefficients in two-fluid turbulence at MA ≃ 1. The upper and lower rows show Ms ≃ 1 and Ms ≃ 10, respectively. Panels (a), (e), (b), and (f) give D/(cLbox) and D/(cLbox) as functions of rL/Lbox. Panels (c), (d), (g), and (h) give Dμμ/Ω as a function of μ0 for rL/Lbox ≃ 8 × 10−3 and 8 × 10−2 (rL = 10 and 100 cells). Red, blue, and green denote decoupled, intermediate, and strongly coupled runs; shaded regions indicate statistical uncertainties. The blue dotted lines in panels (a), (b), (e), and (f) denote the decoupling scale of the intermediate decoupled run.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse