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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Inverse cascade feature in current disruption
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Inverse cascade feature in current disruption

机译:在当前中断逆级联功能

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[1] We investigate the origin of waves leading to current disruption and dipolarizationobserved by a THEMIS satellite at XGSM —8 RE in the magnetotail near a substormexpansion onset on 29 January 2008. Continuous wavelet transform of the magneticactivity associated with current disruption shows a clear inverse cascade feature of wavesstarting at frequencies slightly below the ion cyclotron frequency to waves at lowfrequencies that correspond to the time scale of dipolarization. There was no other low-frequency wave associated with the time scale of dipolarization. On the basis of thisinverse cascade feature, we provide a preliminary theoretical analysis to propose thatthe initial excited waves causing eventual dipolarization in this event may originate fromthe drift-driven electromagnetic ion cyclotron instability, which is an electromagneticversion of the Weibel instability, or an ordinary mode instability similarly driven by thecross-field ion drift.
机译:[1]我们研究波导致的起源当前的混乱和dipolarizationobserved忒弥斯卫星XGSM 8再保险磁尾附近substormexpansion 29日2008年1月。magneticactivity与电流有关中断了一个清晰的逆级联功能在频率略低于wavesstarting离子回旋频率波lowfrequencies对应的时间尺度dipolarization。低频波与时间尺度有关dipolarization。级联功能,我们提供一个初步的理论分析提出,最初的最终dipolarization兴奋波引起这事件可能产生从drift-driven电磁离子回旋不稳定,是一个electromagneticversion韦贝尔不稳定,或一个普通模式不稳定同样由thecross-field离子漂移。

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