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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 12.

Comparison of 1D PIC simulations for ﹩\sigma =3\times {10}^{-1}﹩ at two different resolutions: ﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/10﹩ (left) and ﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/40﹩ (right). Top to bottom: electron number density Ne, z component of the magnetic field Bz, x component of the electric field Ex, and phase-space plots in xux and xuy at ﹩{\omega }_{\mathrm{pe}}t=500﹩, respectively.

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