Analysis of TDOA/FDOA State Estimation Accuracy of Cislunar Objects for Space Situational Awareness

Kullen W. Waggoner, D. Curtis, Bryan D. Little
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Abstract

This paper demonstrates an innovative approach for cislunar Space Situational Awareness (SSA) by demonstrating state estimation using time difference of arrival (TDOA)/frequency difference of arrival (FDOA) from radio frequency (RF) signals transmitted by a cislunar traversing satellite. Traditional SSA methods such as electro-optical (EO) and radar have challenges that include illumination, light saturation, and signal power loss over long distances. These can be avoided with an architecture that relies on passive RF TDOA and FDOA. For this paper, RF signals are modeled as having been collected at two or more receivers and stochastic estimation techniques are applied to determine the transmitter's state estimate and covariance. To simulate the performance of the TDOA/FDOA system, this paper uses additive Gaussian white noise on the RF TDOA/FDOA measurements. The circularly restricted three body problem dynamics (CR3BP) are utilized to model the movement of the space object as it traverses cislunar space. To assess performance of this method, this paper models three two-node space-based receiver architectures and three three-node architectures and compares them to show potential advantages and disadvantages of each. All modeled receivers are in earth centered Keplerian orbits. Each receiver has knowledge of all receivers' locations and compares its collected signals with the other receivers to create the TDOA/FDOA measurements. Iterative batch least-squares estimation techniques were used for each scenario to estimate the transmitter's position and velocity as it moves in a periodic CR3BP orbit about one of the earth-moon Lagrange points. Finally, this paper analyzes how the stability of the transmitter's orbit impacts the accuracy of TDOA/FDOA state estimation.
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面向空间态势感知的地月目标TDOA/FDOA状态估计精度分析
本文展示了一种创新的顺月空间态势感知(SSA)方法,通过演示使用顺月穿越卫星传输的射频(RF)信号的到达时间差(TDOA)/到达频率差(FDOA)进行状态估计。传统的SSA方法,如电光(EO)和雷达,面临着包括照明、光饱和度和长距离信号功率损失在内的挑战。这些可以通过依赖于无源射频TDOA和FDOA的架构来避免。在本文中,射频信号被建模为在两个或多个接收器上收集,并应用随机估计技术来确定发射机的状态估计和协方差。为了模拟TDOA/FDOA系统的性能,本文在射频TDOA/FDOA测量中使用加性高斯白噪声。利用圆约束三体问题动力学(CR3BP)对空间物体在顺月空间中的运动进行建模。为了评估该方法的性能,本文对三种双节点天基接收机架构和三种三节点架构进行了建模,并对它们进行了比较,以显示每种架构的潜在优点和缺点。所有模型接收器都位于以地球为中心的开普勒轨道上。每个接收器都知道所有接收器的位置,并将其收集的信号与其他接收器进行比较,以创建TDOA/FDOA测量值。每个场景都使用迭代批最小二乘估计技术来估计发射机在地球-月球拉格朗日点附近的周期性CR3BP轨道上运行时的位置和速度。最后,分析了发射机轨道稳定性对TDOA/FDOA状态估计精度的影响。
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