Relativistic Shock Wave
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概要
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Perpendicular shock waves in rather strong magnetic fielcls (a..>ctc..) are studiedby a l - 2 /2 dimension (one dimension in real space and three dimension in velocityspace), fully relativistic, fully electromagnetic particle simulation with full ion andelectron dynamics. In that parameter regime relativistic effects become important infast magnetosonic shock waves, even if the thermal speeds of ions and electrons in theupstream region are much smaller than the speed of light; a sltock wave can trap someions and promptly accelerate them to relativistic energies. Furthermore, wuth themechanism different from that of ions, some electrons also gain relativistic energiesthrough interactions with strong electric fields in the shock region. By showingvarious simulation results, we discuss the acceleration procc:sses in detail.
- 社団法人日本物理学会の論文
- 1987-12-15
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関連論文
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- Simulation Studies on Stability of Hot Electron Plasma
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