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首页> 外文期刊>IEEE Transactions on Plasma Science >Electrostatic waves in the Earth's magnetotail and in comets, and electromagnetic instabilities in the magnetosphere and the solar wind
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Electrostatic waves in the Earth's magnetotail and in comets, and electromagnetic instabilities in the magnetosphere and the solar wind

机译:地球磁尾和彗星中的静电波,以及磁层和太阳风中的电磁不稳定

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摘要

The role of electrostatic ion-beam instabilities in the generation of the broadband electrostatic noise in the Earth's magnetotail and in electrostatic bursts in comets is discussed. The theory of electromagnetic ion-cyclotron instabilities in multicomponent plasmas is reviewed by using the semicold approximation. The method is applied to ring current proton precipitation and to the generation of electromagnetic ion-cyclotron waves at the geostationary altitude. The semicold approximation is also applied to the propagation of electromagnetic ion-cyclotron waves in the solar wind. Due to the large proton thermal anisotropy in the core of the proton distribution function in the fast solar wind, strong electromagnetic ion-cyclotron waves can be generated. The waves can resonate with the alpha particles which, because of the resonant interaction, can be accelerated to velocities well in excess of the proton bulk velocity, provided that initially the alpha-proton drift velocity is larger than zero.
机译:讨论了静电离子束不稳定性在地球磁尾中产生宽带静电噪声以及彗星中的静电爆发中的作用。使用半冷近似方法复述了多组分等离子体中电磁离子回旋加速器不稳定性的理论。该方法适用于环流质子沉淀以及对地静止高度的电磁离子回旋波的产生。半冷近似还应用于电磁离子回旋波在太阳风中的传播。由于快速太阳风中质子分布函数的核心具有较大的质子热各向异性,因此可以产生强电磁离子回旋波。这些波可以与α粒子发生共振,由于共振相互作用,它们可以被加速到远远超过质子体积速度的速度,但前提是最初的α-质子漂移速度大于零。

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