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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 7.

Perpendicular MFPs computed in the case of ﹩{(\delta {B}_{z}/\delta B)}^{2}=100 \% ﹩, as a function of energy. Left, center, and right panels correspond to turbulence levels of 0.48, 1.0, and 1.3, respectively. Also shown, as pink dots, are perpendicular MFPs computed from the theoretical expression of V. Florinski et al. (2024), as given in Equation (1).

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