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Fig. 6.


Top: total particle spectrum as a function of the dimensionless total particle momentum, u = γβ for all the magnetizations explored in this study and at the same time ωpet = 3920. Bottom: effect of the striped wind filling factor on the final particle spectrum, Ls/Ly for σ0 = 10 at the same time as in the top panel. The black dotted line shows a power law dN/du ∝ up of index 2.2. The black dashed line is a 2D relativistic Maxwellian distribution for comparison.

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