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Comment on 'Mode Conversion of Waves in the Ion-Cyclotron Frequency Range in Magnetospheric Plasmas'

机译:关于“磁层等离子体中离子回旋加速器频率范围内波的模式转换”的评论

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摘要

Recently, Kazakov and Fueloep studied mode conversion (MC) at the ion-ion hybrid (IIH) resonance in planetary magnetospheric plasmas by simplifying the dispersion relation of the fast wave (FW) modes to describe a cutoff-resonance (CR) pair near the IIH resonance, which can be reduced to a Budden problem. They suggested that when the IIH resonance frequency (ω_S) approaches the crossover frequency (ω_(cr)), and the parallel wave number (k_‖) is close to the critical wave number k_‖~* ≡ (ω/c)[ε_S(ω=ω_(cr))]~(1/2), MC can be efficient for arbitrary heavy ion density ratios. In this Comment, we argue that (a) the FW dispersion relation cannot be simplified to the CR pair especially near ω_(cr) because in many parameter regimes there is a cutoff-resonance-cutoff (CRC) triplet that completely changes the wave absorption and (b) the maximum MC efficiency does not always occur near ω_S≈ω_(cr).
机译:最近,Kazakov和Fueloep通过简化快波(FW)模的色散关系来描述行星附近的截止共振(CR)对,研究了行星磁层等离子体中离子-离子杂化(IIH)共振下的模转换(MC)。 IIH共振,可以减少到Budden问题。他们提出,当IIH共振频率(ω_S)接近交叉频率(ω_(cr)),且平行波数(k_‖)接近临界波数k_′〜* /(ω/ c)[ε_S (ω=ω_(cr))]〜(1/2),MC对于任意的重离子密度比均可有效。在本评论中,我们认为(a)不能将FW色散关系简化为CR对,尤其是在ω_(cr)附近,因为在许多参数方案中,都有一个截止共振-截止(CRC)三重态完全改变了波吸收(b)最大MC效率并不总是出现在ω_S≈ω_(cr)附近。

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