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Modeling tethered satellite systems for detection and orbit determination

机译:对系留卫星系统进行建模以进行检测和确定轨道

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Detection that a satellite in a two-satellite tethered system is tethered using observations of that satellite alone over a relatively short time is more difficult when the system has a relatively short tether and/or significant libration. The estimation of the sate of the system using the same information is also more difficult under these conditions. In this paper, two different formulations of the equations of motion of a two-body tethered satellite system with a massless tether are used to see which resutls in the best performance of detection and sate estimation algorithms. The two formulations involve the use of differnet state variables. In the first, the position and velocity of the observed satellite are used. In the second formulation, we use the position and velocity of the observed satellite and its position and velocity relative to the center of mass of the system as variables. The second formulation provides equations that may be solved approximately for small libration angles to obtain an analytical solution that describes the motion better than a similar solution based on the first formulation. However, both formulations appear to provide essentially the same detection/state estimation results.
机译:当系统具有相对较短的系链和/或明显解放时,仅在相对较短的时间内仅通过对该卫星的观察来检测该卫星是否已被拴系,将更加困难。在这些条件下,使用相同信息来估计系统状态也更加困难。在本文中,使用具有无质量束缚的两体束缚卫星系统的运动方程的两种不同公式,来查看哪种方法能获得最佳性能的检测和状态估计算法。这两种表述涉及使用differnet状态变量。首先,使用被观测卫星的位置和速度。在第二种表述中,我们使用被观测卫星的位置和速度及其相对于系统质心的位置和速度作为变量。第二个公式提供的方程可以针对较小的自由角近似求解,从而获得比基于第一个公式的相似解决方案更好地描述运动的解析解。但是,两种配方似乎都提供了基本相同的检测/状态估计结果。

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