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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 8.

The dependence of the parallel and perpendicular MFPs (left and middle columns, respectively) as well as the ratio λ/λ (right column) on proton kinetic energy. Turbulence levels of (δB/B0) = 0.48, 1.0, and 1.3 correspond to the top, middle, and bottom rows. For all panels shown, three different values are considered for the compressibility ﹩{(\delta {B}_{z}/\delta B)}^{2}﹩: 0.25, 0.75, and 0.95.

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