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Simulating Cosmic-Ray Diffusion Coefficients in the Presence of Synthetic Magnetic Turbulence with a Scalable Compressive Component: First Results for Heliosheath Parameters

  • Authors: J. S. Troskie, N. E. Engelbrecht

J. S. Troskie and N. E. Engelbrecht 2026 The Astrophysical Journal Supplement Series 286 .

  • Provider: AAS Journals

Caption: Figure 10.

The variation of MFPs with the compressibility ﹩{(\delta {B}_{z}/\delta B)}^{2}﹩. Left, center, and right columns correspond to λ, λ, and λ/λ, respectively, while rows correspond to different values for the turbulence level (δB/B0): 0.48, 1.0, and 1.3 from top to bottom. The particle energies considered in Figure 8 are here represented by different colors.

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