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- W2886032492 abstract "The effect of perpendicular (to the direction of shock propagation) magnetic fields on electron shock-surfing acceleration (ESSA) is investigated. Two-dimensional particle-in-cell simulations show that the strength of background magnetic fields can significantly affect the shock formation process and the electrostatic field structure near the leading edge of the shock. It is found that ESSA is most efficient when the ratio of electron cyclotron frequency to plasma frequency is about 0.1. In this case, there are two types of electrostatic field structures near the shock edge, namely, small-scale filamentary and large-scale dipole electric fields, induced by the Buneman instability and fluid compression, respectively. In such a mixed field structure, the affected electrons can undergo multiple accelerations and gain much higher energies than that under weaker or stronger background magnetic fields." @default.
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- W2886032492 date "2018-08-01" @default.
- W2886032492 modified "2023-10-15" @default.
- W2886032492 title "Electron shock-surfing acceleration in the presence of magnetic field" @default.
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- W2886032492 doi "https://doi.org/10.1063/1.5030184" @default.
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