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Reanalysis of plasma measurements at geosynchronous orbit

机译:重新分析地球同步轨道上的等离子体测量

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Retrospective analyses of spacecraft anomalies, especially surface charging, require information about the local plasma environment. Such information is usually not available at geosynchronous orbit because most vehicles lack appropriate sensors. We have constructed a nearly continuous hourly database covering four plasma moments at geosynchronous orbit: density and temperature for hot (energies > 100 eV) protons and electrons. The four moments are provided for 24 hourly fiducial local time bins and cover the years 1990–2005. We apply an ensemble of simple models to “fill in” the local time gaps between plasma measurements at geosynchronous orbit made by Los Alamos sensors. Validation on artificial data gaps shows that the reconstruction has rank order correlations ranging from 0.65 to 0.97, depending on bulk moment and local time. As a demonstration, we include a comparison of our reanalysis electron temperature to on-orbit surface charging measurements at a vehicle that lacks a plasma sensor. In addition to anomaly analyses, the reanalysis database we have produced can be used to provide geosynchronous boundary conditions for numerical simulations of the inner magnetosphere and temporal variations at a single location for statistical studies.
机译:航天器异常,尤其是表面电荷的回顾性分析,需要有关本地等离子体环境的信息。由于大多数车辆缺少适当的传感器,因此在地球同步轨道上通常无法获得此类信息。我们已经建立了一个几乎连续的每小时数据库,涵盖了地球同步轨道上的四个等离子体矩:热(能量> 100 eV)质子和电子的密度和温度。这四个时刻提供了24小时的基准当地时区,并涵盖了1990-2005年。我们应用简单模型的集合来“填充” Los Alamos传感器在地球同步轨道上进行等离子测量之间的局部时间间隙。对人工数据缺口的验证表明,重建具有的阶序相关性在0.65至0.97范围内,具体取决于体力矩和当地时间。作为演示,我们将比较分析电子温度与缺少等离子传感器的车辆的在轨表面电荷测量进行了比较。除了异常分析外,我们产生的重新分析数据库还可用于为内部磁层的数值模拟和单个位置的时间变化提供地理同步边界条件,以进行统计研究。

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