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Low-frequency wave characteristics in the upstream and downstream regime of the terrestrial bow shock

机译:低频波上游的特征和下游政权的陆地弓冲击

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摘要

Collisionless shocks in space are accompanied by the low-frequency waves of the magnetic field both upstream and downstream of the shock. However, characteristics of these waves in the plasma rest frame are poorly understood, since spatial scale such as wavelength is hardly determined using single or at best two spacecraft observations. Taking advantage of multipoint measurements of the Cluster spacecraft, we present a statistical study to reveal the rest frame properties of the waves in the terrestrial bow shock environment such as frequencies, wave numbers, phase velocities, propagation directions, polarization and transport ratios for the quasi-parallel and the quasi-perpendicular shock regimes and in the upstream region, the outer, the middle, and the inner magnetosheath. We find that the quasi-parallel shock upstream waves (or the foreshock waves) exhibit properties of the fast mode wave excited by the ion beam instability. Upstream of the quasi-perpendicular shock the waves also exhibit similar properties to the foreshock waves, but the wave mode identification needs further investigations. In the magnetosheath the waves exhibit properties which are persistent from the outer to the inner magnetosheath. They can be interpreted as the mirror mode coupled to the plasma inhomogeneity or as the slow mode. We also find an organization in the wave propagation pattern that the upstream waves propagate toward upstream, while the magnetosheath waves propagate toward the flank region and toward the magnetopause. It is concluded that wave properties are different between the upstream and the downstream regions, but they are similar between the quasi-parallel and the quasi-perpendicular shock regimes, suggesting that the upstream waves are not transmitted to the downstream region across the shock and that the downstream waves do not depend on the shock angle (between the upstream magnetic field and the shock normal direction).
机译:在太空中都伴随着无碰撞的冲击的低频波磁场上游和下游的冲击。然而,这些波的特征等离子体静止坐标是知之甚少,因为空间尺度,如波长很难确定使用单或最多两艘宇宙飞船观察。集群航天器的测量,我们目前的统计研究,揭示了休息帧属性海浪的陆地弓形激波环境如频率、波数字、相速度传播方向,极化和运输率quasi-parallel和quasi-perpendicular冲击政权和上游地区外,中间,和内心的磁鞘。我们发现quasi-parallel冲击上游波(或前震)展览属性快速模式波兴奋的离子束不稳定。海浪冲击也表现出类似的属性前震的波浪,但波模式识别需要进一步调查。磁鞘海浪展览属性从外到内持久磁鞘。镜像模式耦合等离子体不均匀性或缓慢的模式。在上游的波传播模式电波传播向上游,而磁鞘向侧面波传播地区和磁层。得出的结论是,波性质是不同的上游和下游之间的区域,但他们quasi-parallel之间是相似的quasi-perpendicular冲击政权,表明上游波传递给下游地区的震惊和下游波不依赖之间的冲击角(上游磁场和冲击正常的方向)。

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  • 来源
    《Journal of Geophysical Research, A. Space Physics: JGR》 |2006年第1期|A01203-1-A01203-14-0|共14页
  • 作者单位

    Centre d'Etude Spatiale des Rayonnements, Centre National de la Recherche Scientifique, Toulouse, France;

    Institut fur Geophysik und extraterrestrische Physik, Technische Universit?t Braunschweig, Braunschweig, Germany Max-Planck-Institut fur Sonnensystemforschung, Katlenburg-Lindau, Germany;

    Institut fur Geophysik und extraterrestrische Physik, Technische Universitat Braunschweig, Braunschweig, GermanyMax-Planck-Institut fur extraterrestrische Physik, Garching, GermanyInstitut fur Geophysik und extraterrestrische Physik, Technische Universit?t Braunschweig, Braunschweig, GermanyInstitut fur Theoretische Physik, Technische Universit?t Braunschweig, Braunschweig, Germany;

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  • 原文格式 PDF
  • 正文语种 英语
  • 中图分类
  • 关键词

    Upstream; waves; magnetic fieldmagnetosheathDownstream3' Region;

    机译:上游,波;磁fieldmagnetosheathDownstream3的地区;

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