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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 10.

Top: profiles of the vertical ISM gas velocity 〈vz〉 (left), gas density 〈ρ〉 (middle), and ﹩\langle |{B}_{z}|/|{\boldsymbol{B}}|\rangle ﹩ (right), averaged in the x–y plane versus altitude z in kiloparsecs for three runs with different SN rate values, displayed in the caption. Bottom: profiles of the vertical ISM gas velocity 〈vz〉 (left), gas density ρ (middle), and ﹩\langle |{B}_{z}|/|{\boldsymbol{B}}|\rangle ﹩ (right), averaged in the x–y plane versus altitude z in kiloparsecs for two runs with different diffusion coefficient ﹩{D}_{\parallel }^{0}﹩ values, displayed in the caption. The captions in the left panels apply to all the plots in the row.

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