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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 5.

Omnidirectional spectral forms measured from code output for turbulent magnetic fields with varying values of ﹩Z={(\delta {B}_{z}/\delta B)}^{2}﹩. The input minimum and maximum fluctuation wavenumbers ﹩{k}_{{\rm{\min }}}=2\pi /{\lambda }_{{\rm{\max }}}﹩ and ﹩{k}_{{\rm{\max }}}=2\pi /{\lambda }_{{\rm{\min }}}﹩ are indicated by dashed gray lines, and all proton energies under consideration, including the lowest value of 70 MeV, are found to correspond to resonant wavenumbers.

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