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Ionospheric currents estimated simultaneously from CHAMP satelliteand IMAGE ground-based magnetic field measurements: a statisticalstudy at auroral latitudes

机译:从CHAMP卫星和IMAGE地面磁场测量同时估算的电离层电流:极光纬度的统计研究

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One important contribution to the magnetic field measured atsatellite altitude and at ground level comes from the externalcurrents. We used the total field data sampled by the OverhauserMagnetometer on CHAMP and the horizontal magnetic fieldmeasurements of the IMAGE ground-based magnetometer network tostudy the ionospheric Hall current system in the auroral regions.For the CHAMP data a current model consisting of a series of linesand placed at a height of 110km is fitted to the magnetic fieldsignature sampled on the passage across the polar region. Thederived current distributions depend, among others, on season andon the local time of the satellite track. At dawn/dusk the auroralelectrojets can be detected most clearly in the auroralregions. Their intensity and location are evidently correlatedwith the A E activity index. For a period of almost two years theresults obtained from space and the currents determined fromground-based observations are studied. For the full IMAGE stationarray a newly-developed method of spherical elementary currentsystems (SECS) is employed to compute the 2-D equivalent currentdistribution, which gives a detailed picture of an area coveringlatitudes 60° – 80° N and 10° – 30° E in theauroral region. Generally, the current estimates from satelliteand ground are in good agreement. The results of this surveyclearly show the average dependence of the auroral electrojet on season and localtime. This is particularly true during periods of increasedauroral activity. The correlation coefficient of the results isclose to one in the region of sizeable ionospheric currentdensities.Also the ratio of the current densities, as determined from aboveand below the ionosphere, is close to unity. It is the first timethat the method of Hall current estimate from a satellite has beenvalidated quantitatively by ground-based observations. Amongothers, this result is of interest for magnetic main fieldmodelling, since it demonstrates that ground-based observationscan be used to predict electrojet signatures in satellite magneticfield scalar data.Key words. Ionosphere (auroral Ionosphere; electric fieldsand currents; ionosphere-magnetosphere interactions)
机译:对卫星高度和地面测量的磁场的重要贡献来自外部电流。我们使用Overhauser磁力计在CHAMP上采样的总场数据和IMAGE地面磁力计网络的水平磁场测量来研究极光区域的电离层霍尔电流系统。在穿过极区的通道上采样的磁场信号拟合高度为110 km的信号。得出的电流分布尤其取决于季节和卫星轨道的当地时间。在黎明/黄昏时,可以在极光区域中最清晰地检测到极光电喷流。它们的强度和位置显然与 A E 活性指数相关。在近两年的时间里,从太空获得了结果,并研究了从地面观测获得的电流。对于完整的IMAGE测站阵列,采用了新开发的球形基本电流系统(SECS)方法来计算二维等效电流分布,从而给出了覆盖纬度60°– 80°N和10°– 30°E的区域的详细图片在戏剧领域。通常,从卫星和地面得出的当前估算值吻合良好。这项调查的结果清楚地表明了极光电喷对季节和当地时间的平均依赖性。在增加听觉活动的时期尤其如此。结果的相关系数在较大的电离层电流密度区域内接近于1.此外,从电离层的上方和下方确定的电流密度之比也接近于1。这是第一次通过地面观测对卫星的霍尔电流估计方法进行了定量验证。除其他外,该结果对于磁场主场建模很有意义,因为它表明可以使用基于地面的观测来预测卫星磁场标量数据中的电喷特征。 关键词。电离层(极光电离层;电场和电流;电离层-磁层相互作用

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