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An algorithm for estimating field-aligned currents from single spacecraft magnetic field measurements: a diagnostic tool applied to Freja satellite data

机译:一种从单个航天器磁场测量值估计场对准电流的算法:一种应用于Freja卫星数据的诊断工具

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摘要

Introduces an algorithm which allows under certain assumptions to estimate the current density distribution along the track from single spacecraft magnetic field measurements. The assumptions are chosen that they meet at least partly the conditions encountered by the Freja satellite on its northernmost orbital segment, namely that all currents are field-aligned, ionospheric currents do not contribute significantly to the magnetic field measurements, and the velocity component perpendicular to the field direction is large (<5 km/s). Problems arise in the case of moving or temporally varying current systems. In those cases additional data like ground-based observations are needed to resolve the spatio-temporal ambiguity. With the help of simulated data the authors can show that for most of the encountered stationary current geometries the estimates fall into an uncertainty band of /spl plusmn/20%. Current density estimates are a local quantity with a spatial resolution of order 1 km. They are thus very suitable for use in studying the fine structure of auroral plasma processes.
机译:引入一种算法,该算法允许在某些假设下从单个航天器磁场测量值估计沿轨道的电流密度分布。选择的假设是,它们至少部分满足Freja卫星在其最北端的轨道段所遇到的条件,即所有电流都是场对准的,电离层电流对磁场测量的贡献不大,并且垂直于磁场方向很大(<5 km / s)。在移动或随时间变化的电流系统的情况下会出现问题。在这些情况下,需要其他数据(例如,地面观测)来解决时空模糊性。借助模拟数据,作者可以表明,对于大多数遇到的平稳电流几何形状,估计值落入了/ spl plusmn / 20%的不确定性范围内。当前的密度估算值是一个局部量,其空间分辨率约为1 km。因此,它们非常适合用于研究极光等离子体过程的精细结构。

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