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FW propagation and absorption in reactor plasmas in the ICR frequency range at the quasiperpendicular propagation

机译:FW在四边形传播的ICR频率范围内在反应堆等离子体中的传播和吸收

摘要

On the base of the numerical model, taking into account the strong transverse and longitudinal dispersion of plasma, the absorption and dispersion of the Fast Mode of fast magnetosonic wave (FW) near ICR harmonics ω=nωci at the quasiperpendicular propagation regime were investigated. It was shown that in the region of small longitudinal refractive index values NII there appears the additional absorption that provides the value of optical thickness τ being constant in the entire region of additional absorption. At first and second harmonics the additional absorption can be interesting for FW plasma heating in the reactor-size devices. For higher harmonics it can be important for HF diagnostic purposes and for investigation of astrophysical plasmas.
机译:在数值模型的基础上,考虑到等离子体的强横向和纵向色散,研究了在垂直七面体传播状态下ICR谐波ω=nωci附近的快磁声波(FW)快速模式的吸收和色散。已经表明,在小的纵向折射率值NII的区域中出现了附加的吸收,该附加的吸收提供了在附加的吸收的整个区域中恒定的光学厚度τ的值。在第一次和第二次谐波中,额外的吸收对于反应堆大小设备中的FW等离子体加热可能是令人感兴趣的。对于高次谐波,这对于HF诊断和天体等离子体的研究可能很重要。

著录项

  • 作者

    Pavlov S.S.;

  • 作者单位
  • 年度 2015
  • 总页数
  • 原文格式 PDF
  • 正文语种 en
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