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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 3.

Snapshots of the ISM density evolution (left) and vertical velocity evolution (right) in the stratified box over 500 Myr in the y–z plane at x = 0 for the model case A1 with SN rate = 80 kpc−2 Myr−1, ﹩{D}_{\parallel }^{0}=3\times 1{0}^{28}\,{\mathrm{cm}}^{2}\,{{\rm{s}}}^{-1}﹩. The ISM presents CR-driven buoyancy structures, generating outflows in the vertical direction. The vertical velocity snapshots indicate the presence of outflows, meaning that advection for CRs is present.

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