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On the Mitigation of Solar Index Variability for High Precision Orbit Determination in Low Earth Orbit

机译:低地球轨道高精度轨道测定太阳能指标变异性的减轻

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Effective satellite mission operations are directly impacted by the ability to generate accurate and precise orbit predictions. High precision orbit determination processes rely on detailed force models to propagate an orbit solution and predict future orbit behavior. While gravity forces are typically well understood, the modeling of non-conservative forces is often more challenging, causing increased difficulty in achieving and maintaining high precision orbit predictions for satellites operating in low Earth orbit. In particular, the atmosphere models used to predict the drag force experienced by a satellite may rely on input parameters such as solar flux and geomagnetic indices, which are often difficult to predict. Multiple methods of selecting the solar flux and geomagnetic index parameters are examined in combination with a number of current and historically recommended atmospheric density models to assess the impact of uncertainty in the predicted index values. Geodetic satellites with high precision satellite laser ranging data are used as test cases for the Naval Research Laboratory's Orbit Covariance Estimation and ANal-ysis (OCEAN) tool to evaluate solution accuracy and predictive capabilities of each combination. In all test cases examined, using either the Naval Research Laboratory Mass Spectrometer and Incoherent Scatter Radar 2000 or Jacchia-Bowman 2008 atmospheric density model with solar flux and geomagnetic index values held constant, rather than using the predicted index values, provided the most accurate orbit predictions. Surprisingly, the exponential atmospheric density model, which does not take into account atmospheric parameters, yielded more accurate orbit predictions than any model using predicted solar flux and geomagnetic indices.
机译:有效的卫星任务操作是通过生成准确和精确的轨道预测的能力直接影响。高精度轨道确定过程中依靠详细的力模型传播的轨道解决方案,并预测未来的轨道行为。虽然重力通常是很好理解的,非保守势力的造型往往更具挑战性,导致在实现和维持在低地球轨道上运行的卫星高精度轨道的预测增加了难度。特别地,用于预测由卫星所经历的拖曳力的大气模型可以依赖于输入的参数,如太阳能通量和地磁指数,这往往是难以预料的。选择所述太阳能通量和地磁索引参数的多种方法被检查结合一些当前和历史推荐大气密度模型,以评估不确定性的所述预测指标值的影响。具有高精度卫星激光测距数据测地卫星被用作试验例为海军研究实验室的轨道协方差估计和肛门ysis(OCEAN)工具来评估解的精度和每个组合的预测能力。在所有测试情况下检查,即使用海军研究实验室质谱仪和非相干散射雷达2000或Jacchia-鲍曼2008大气密度模型与太阳能通量和地磁指数值保持恒定,而不是使用预测指标值,提供最精确的轨道预测。出人意料的是,指数大气密度模型,它不考虑大气参数,产生更精确的轨道预测比使用预测的太阳能通量和地磁指数的任何模型。

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