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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 13.

The ratios of the parallel (left panel) and perpendicular (right panel) MFPs computed for a field with ﹩{(\delta {B}_{z}/\delta B)}^{2}=25 \% ﹩ to those computed in the presence of only the transverse component of such a field, as a function of energy. Here, transverse turbulence levels (δBtr./B0) have been chosen so as to correspond to the previously considered total turbulence levels (δB/B0) of 0.48, 1.0, and 1.3. In these panels, dashed horizontal lines indicate MFP values which would correspond to no increase with respect to those computed in pure transverse turbulence.

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