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Implementation of Cosmic Ray Energy Spectrum (CRESP) Algorithm in PIERNIK MHD Code. II. Propagation of Primary and Secondary Nuclei in a Magnetohydrodynamic Environment

  • Authors: Antoine Baldacchino-Jordan, Michał Hanasz, Mateusz Ogrodnik, Dominik Wóltański, Artur Gawryszczak, Andrew W. Strong, Philipp Girichidis

Antoine Baldacchino-Jordan et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 11.

The same B/C and 10Be/9Be plots as the previous Figures 8 and 9 for the B1 and C1 models, only differing from the fiducial case by the diffusion coefficient and diffusion power index. The left panels have ﹩{D}_{\parallel }^{0}=6\times 1{0}^{28}\ {\mathrm{cm}}^{2}\,{{\rm{s}}}^{-1}﹩ and δ = 0.3, and the right panels have ﹩{D}_{\parallel }^{0}=3\times 1{0}^{28}\ {\mathrm{cm}}^{2}\,{{\rm{s}}}^{-1}﹩ and δ = 0.5.

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