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

机译:低地球轨道上高精度轨道确定中太阳指数变异性的缓解

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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:有效的卫星任务运行直接受到产生准确和精确的轨道预测的能力的影响。高精度的轨道确定过程依靠详细的力模型来传播轨道解并预测未来的轨道行为。虽然通常很容易理解重力,但非保守力的建模通常更具挑战性,导致在低地球轨道上运行的卫星获得和维持高精度轨道预测的难度增加。特别是,用于预测卫星所受阻力的大气模型可能依赖于通常难以预测的输入参数,例如太阳通量和地磁指数。结合多种当前和历史上推荐的大气密度模型,研究了选择太阳通量和地磁指数参数的多种方法,以评估不确定性对预测指数值的影响。具有高精度卫星激光测距数据的大地测量卫星被用作海军研究实验室的轨道协方差估计和ANal-ysis(OCEAN)工具的测试用例,以评估每种组合的解决方案准确性和预测能力。在所有测试用例中,使用海军研究实验室质谱仪和不相干散射雷达2000或Jacchia-Bowman 2008大气密度模型,使太阳通量和地磁指数值保持恒定,而不是使用预测的指数值,从而提供了最准确的轨道预测。令人惊讶的是,没有考虑大气参数的指数大气密度模型比使用预测的太阳通量和地磁指数的任何模型产生的轨道预测更准确。

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