Figure 11 from Electron-scale shear instabilities: magnetic field generation and particle acceleration in astrophysical jets

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Electron-scale shear instabilities: magnetic field generation and particle acceleration in astrophysical jets

Authors: E P Alves, T Grismayer, R A Fonseca, L O Silva

E P Alves 2014 New Journal of Physics 16 035007.

Provider: IOP Publishing

Caption: Figure 11.

Evolution of the maximum growth rate as a function of the gradient length. Dashed curve: expression (81); plain curve: numerical algorithm; red dots: PIC simulations for ﹩{{v}_{0}}(x)/c=0.2\tanh (x/L)﹩.

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