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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 11.

The MFPs as a function of compressibility, as shown in Figure 10, but for the AC field discussed in Section 2.4.

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