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Low frequency wave sources in the outer magnetosphere, magnetosheath, and near Earth solar wind

机译:外部磁层,磁石表面以及地球太阳风附近的低频波源

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The interaction of the solar wind with the Earth magnetosphere generates abroad variety of plasma waves through different mechanisms. The four Clusterspacecraft allow one to determine the regions where these waves are generatedand their propagation directions. One of the tools which takes fulladvantage of the multi-point capabilities of the Cluster mission is the wavetelescope technique which provides the wave vector using a plane waverepresentation. In order to determine the distance to the wave sources, thesource locator – a generalization of the wave telescope to spherical waves– has been recently developed. We are applying the source locator tomagnetic field data from a typical traversal of Cluster from the cusp regionand the outer magnetosphere into the magnetosheath and the near Earth solarwind. We find a high concentration of low frequency wave sources in theelectron foreshock and in the cusp region. To a lower extent, low frequencywave sources are also found in other magnetospheric regions.
机译:太阳风与地球磁层的相互作用通过不同的机制在国外产生了各种等离子波。四个“星际飞船”可以确定这些波的产生区域及其传播方向。充分利用“聚类”任务多点能力的工具之一是Wavetelescope技术,它使用平面波表示来提供波矢。为了确定到波源的距离,最近开发了源定位器(将波望远镜概括为球面波)。我们正在将源定位器应用于从簇的典型遍历开始的磁场数据,该簇从尖端区域和外磁层进入磁层和近地太阳风。我们在电子前震和尖端区域发现了高浓度的低频波源。在较低的程度上,在其他磁层区域也发现了低频波源。

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