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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 1.

A 2D projection of the magnitude of an isotropic turbulent magnetic field as constructed according to Equation (16). A turbulence level of (δB/B0) = 1 is assumed, with B0 = 0.1 nT (the background field is not included in the present figure). Details regarding the spectral form employed for this field are provided in Section 2.5.

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