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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 5.

Time evolution of the precursor wave energy given in units of upstream bulk kinetic energy: ﹩{\sigma }_{e}=3\times {10}^{-1}﹩ (left) and ﹩{\sigma }_{e}=3\times {10}^{-3}﹩ (right). In both panels, the results with our fiducial resolution (﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/40﹩) are shown by the solid lines, whereas lower resolution results (﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/20﹩) are shown by the dashed lines.

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