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Heavy ion effects on substorm loading and unloading in the Earth's magnetotail

机译:重离子对亚暴加载和影响卸载在地球磁尾

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We have performed a statistical study investigating how substorm triggering and unloading is affected by the heavy ion content of the magnetotail plasma sheet. During the substorm growth phase, magnetic flux is accumulated in the tail lobes until the magnetotail reaches an unstable state. A near-Earth neutral line then forms, and this excess flux is reconnected. The increased lobe magnetic flux during the substorm growth phase increases the magnetopause flaring angle. As a result, a greater fraction of the solar-wind dynamic pressure is observed in the tail lobes and plasma sheet. Therefore, the increase and decrease of the lobe magnetic flux can be monitored by observing the increase and decrease in the magnetotail pressure. Using Cluster data from 2001 to 2004, we have determined how the maximum pressure (or flaring angle) and the rate of change of pressure (or flaring angle) during substorms depend on the O~+ content of the plasma sheet. In addition, we have estimated the maximum magnetic flux, and rate of change of the magnetic flux. Our results show that both the maximum tail pressure and the rate of change in the pressure are positively correlated with the amount of O~+ in the plasma sheet. When the measurements are normalized to account for the external solar-wind pressure and the different Cluster locations in the tail, the maximum accumulated flux and the unloading rate still correlate positively with the O~+ density and O~+/H~+ ratio. This suggests that the additional O ~+ makes it more difficult to trigger the substorm onset, but once it is triggered, the unloading is faster. This could either indicate that the presence of O~+ increases the reconnection rate, or that it initiates reconnection over a broader width of the tail. Key Points The heavy ion effects on substorm triggering and unloading rate were tested.The maximum accumulated flux and the unloading rate increase with the O~+.More O~+ prevent substorm triggering but speed the unloading.
机译:我们已经进行了统计研究调查亚暴触发和卸载是重离子内容的影响磁尾等离子体单。积累的增长阶段,磁通尾叶,直到磁尾达到不稳定的状态。连接形式,这多余的流量。增加叶磁通量在亚暴增长阶段增加磁层燃除角。太阳风中观察到的动态压力尾叶和等离子板。叶磁通量增加和减少可以通过观察增加和监控减少磁尾的压力。集群的数据从2001年到2004年,我们拥有的如何确定最大压力(或燃烧角)和的变化率(或压力扩口角度)在亚暴取决于O ~ +等离子体的内容表。估计的最大磁通和速度磁通的变化。最大的尾巴压力和速度压力的变化是积极的与O ~ +在等离子体的数量表。占外部和太阳风的压力不同集群的位置在尾巴,最大累积通量和卸货率仍然与O ~ +浓度正相关和O ~ + / H ~ +比值。额外的O ~ +使它更加困难触发亚暴发病,但一旦触发,卸货速度更快。要么表明O ~ +的存在增加了重联率,或者它启动重新连接在一个更广泛的宽度尾。亚暴触发和卸载速率测试。卸货速率增加O ~ +。防止亚暴触发但速度卸载。

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