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Topology of currents in the high-latitude magnetosphere and magnetospheric response to variations in solar wind parameters

机译:高纬度磁层中电流的拓扑和磁层对太阳风参数变化的响应

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摘要

We consider a number of new approaches that arise when the topology of currents in the high-latitude magnetosphere is investigated. We note that the high correlation between magnetospheric processes and solar wind parameters is a well-known feature of the magnetospheric dynamics. The proposed explanations of the observed dependences run into difficulties related to the high level of observed turbulence in the magnetosheath and inside the magnetosphere. The topology of the high-latitude magnetosphere in the transition region from dipole magnetic field lines to those extending into the tail is also poorly known. We consider the topology of transverse magnetospheric currents using satellite measurements of the plasma pressure distribution. The currents of the nearest plasma sheet are shown to be closed inside the magnetosphere. The generation of field-aligned currents in Iijima and Potemra region currents 1 and large-scale magnetospheric convection are discussed. [PUBLICATION ABSTRACT]
机译:我们考虑研究高纬度磁层中电流拓扑时出现的许多新方法。我们注意到磁层过程与太阳风参数之间的高度相关性是磁层动力学的一个众所周知的特征。所提出的对观测到的依赖性的解释遇到了与磁石中和磁层内部的高水平湍流有关的困难。从偶极磁场线到延伸到尾部的磁场的过渡区域中的高纬度磁层的拓扑结构也鲜为人知。我们使用等离子压力分布的卫星测量来考虑横向磁层电流的拓扑。显示最近的等离子片的电流在磁层内部是封闭的。讨论了饭岛(Iijima)和波塔姆拉(Potemra)区域电流1中场对准电流的产生以及大规模磁层对流。 [出版物摘要]

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