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Persistence of Precursor Waves in Two-dimensional Relativistic Shocks

  • Authors: Masanori Iwamoto, Takanobu Amano, Masahiro Hoshino, and Yosuke Matsumoto

2017 The Astrophysical Journal 840 52.

  • Provider: AAS Journals

Caption: Figure 10.

Downstream energy spectra of electrons: ﹩{\sigma }_{e}=3\times {10}^{-1}﹩ (left) and ﹩{\sigma }_{e}=3\times {10}^{-3}﹩ (right). The black dashed lines in the left and right panels indicate a 2D relativistic Maxwellian and a power-law distribution fitting result, respectively.

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