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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 9.

The same B/C and 10Be/9Be plots as in the previous Figure 8, for the A2 and A3 models, only differing from the fiducial case by the SN rate. The left panels have an SN rate of 60 kpc−2 Myr−1, while the right panels have one of 20 kpc−2 Myr−1.

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