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Multi-spacecraft observations of small-scale fluctuations in density and fields in plasmaspheric plumes

机译:等离子球羽密度和场小范围波动的多航天器观测

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摘要

In this event study, small-scale fluctuations in plasmaspheric plumes with time scales of~10 s to minutes in the spacecraft frame are examined. In one event, plasmaspheric plumes are observed byCluster, while IMAGE measured density enhancement at a similar location.Fluctuations in density exist in plumes as detected by Cluster andare accompanied byfluctuations in magnetic fields and electric fields. Magnetic fluctuationsare transverse and along the direction of the plumes. The E/B ratio issmaller than the Alfvén velocity.Another similar event is briefly presented. We then consider physical properties ofthe fluctuations.Alfvén mode modulated by the feedbackinstability is one possibility, although non-local generation is likely.It is hard to show that the fluctuations represent a fast mode.Interchange motion is possible due to the consistencybetween measurements and expectations. The energy source could be apressure or density gradient in plasmaspheric plumes. When more events are accumulatedso that statistical analysis becomes feasible, this type of study will be useful to understand the time evolution of plumes.
机译:在本事件研究中,研究了在航天器框架内等离子球羽的小规模波动,时间尺度约为10 s至数分钟。在一个事件中,Cluster观测到了等离子球状羽流,而IMAGE在相似的位置测量了密度的增强.Cluster检测到羽状流中存在密度波动,并伴随着磁场和电场的波动。磁波动是横向的,沿着烟羽的方向。 E / B 的比率小于Alfvén速度。简要介绍了另一个类似的事件。然后我们考虑了波动的物理性质。虽然可能发生非局部生成,但由反馈不稳定调制的Alfvén模式是一种可能。很难证明波动代表了一种快速模式。由于测量值和期望值之间的一致性,交换运动是可能的。能源可以是等离子球状羽流中的压力或密度梯度。当积累了更多的事件以便进行统计分析时,这种类型的研究将有助于理解羽流的时间演变。

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