Cosmic ray transport and acceleration in an evolving shock landscape

Open Access

Fig. 13.

Energy spectra over time at the moving shocks (top) and downstream (bottom) at 5 kpc at for E₀ = 100 E_SN, B₀ = 10 μG (left) and E₀ = 10 E_SN, and B₀ = 100 μG (right).

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