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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 2.

Magnitude projections of a turbulent field with an isotropic component as depicted in Figure 1, but with a compressibility Z of 75%. The spatial variation of the field strength is shown both in planes perpendicular (left panel) and parallel (right panel) with respect to the background field direction. Spectral forms are discussed in Section 2.5.

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