Figure 13 from Persistence of Precursor Waves in Two-dimensional Relativistic Shocks

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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 13.

Wavenumber power spectra for precursor waves normalized by the upstream ambient magnetic field at ﹩{\omega }_{\mathrm{pe}}t=500﹩ for ﹩{\sigma }_{e}=3\times {10}^{-1}﹩: ﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/10﹩ (left) and ﹩{\rm{\Delta }}x/(c/{\omega }_{\mathrm{pe}})=1/40﹩ (right).

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