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Relativistic electron beam-plasma instability and interaction with electromagnetic wave.

机译:相对论性电子束-等离子体的不稳定性以及与电磁波的相互作用。

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摘要

A plasma particle simulation was undertaken to study the growth rate of the relativistic beam-plasma electromagnetic instability. The linear dispersion relation for the relativistic beam-plasma electromagnetic instability is derived and solved numerically for the growth rate of the electromagnetic field. The linear growth rate is solved as a function of beam velocity and wavenumber. The results are compared with plasma particle simulations conducted using MAGIC, a particle in cell code developed by Mission Research Corporation under the auspices of the Air Force Office of Scientific Research. The resulting particle simulation growth rates, as a function of beam velocity and wavenumber, agree with linear theory. The saturation of the beam-plasma instability agrees with quasi-linear theory. Electromagnetic turbulence develops from the relativistic beam-plasma instability. The interaction of the electromagnetic turbulence with an incident electromagnetic wave, at {dollar}omega = omegasb{lcub}p{rcub}{dollar} where {dollar}omegasb{lcub}p{rcub}{dollar} is the plasma frequency, is studied by the use of Fourier spectrum. A scattered wave spectrum is observed at {dollar}omega = 2omegasb{lcub}p{rcub}.{dollar}
机译:进行了等离子体粒子模拟,以研究相对论性束-等离子体电磁不稳定性的增长率。推导了相对论性束-等离子体电磁不稳定性的线性色散关系,并用数值方法求解了电磁场的增长率。线性增长率是光束速度和波数的函数。将结果与使用MAGIC(由Mission Research Corporation在空军科学研究所主持下开发的单元代码中的粒子)进行的等离子体粒子模拟进行了比较。所得的粒子模拟增长率,作为束速度和波数的函数,与线性理论一致。束等离子体不稳定性的饱和度与准线性理论一致。电磁湍流是由相对论性束-等离子体不稳定性产生的。在{dollar} omega = omegasb {lcub} p {rcub} {dollar}处电磁湍流与入射电磁波的相互作用,其中{dollar} omegasb {lcub} p {rcub} {dollar}是等离子频率,通过使用傅立叶光谱进行研究。在{omega} omega = 2omegasb {lcub} p {rcub}处观察到散射波谱。{dollar}

著录项

  • 作者

    Masten, John Bingham.;

  • 作者单位

    Texas Tech University.;

  • 授予单位 Texas Tech University.;
  • 学科 Physics Fluid and Plasma.
  • 学位 Ph.D.
  • 年度 1995
  • 页码 76 p.
  • 总页数 76
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 等离子体物理学;
  • 关键词

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