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Simulations of Ion Acceleration at Non-relativistic Shocks. II. Magnetic Field Amplification

  • Authors: D. Caprioli and A. Spitkovsky

Caprioli & Spitkovsky 2014 The Astrophysical Journal 794 46.

  • Provider: AAS Journals

Caption: Figure 9.

Comparison of runs with different transverse size for M = 20 parallel shock (Run A is five times larger than Run B; see Table 1). Left panel: magnetic field profiles, as in the legend; langBrang and max B correspond to the average over y and the maximum of Btot(x, y), as a function of x. max B in Run B is not shown since it almost coincides with langBrang. The averaged profiles are quite similar in the two runs, even if the spread from the mean value may locally be quite large in Run A. Right panel: time evolution of non-thermal spectra for Run A (dashed lines) and B (solid lines). Spectra agree very well until , after which the diffusion length at Emax becomes comparable with the box size in Run A.

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