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GPS code tracking in high altitude orbiting receivers

机译:高空轨道接收器中的GPS代码跟踪

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There is interest in the application of the GPS for navigation of satellites with altitudes greater than that of the GPS constellation itself. Candidate missions include geostationary (GEO) and High Earth Orbit (HEO) satellites, particularly those with large eccentricities. The challenges for HEO missions are the reduced power of the GPS signal at apogee and the large differences in line of sight dynamics between apogee and perigee. In this paper, design studies of the Delay Lock Loop (DLL) were performed to determine the closed loop bandwidth and the predetection integration time as a function of orbit position, allowing the tracking loops to adapt to expected signal strength and dynamic conditions. Approximations for the tracking threshold, based on discriminator error variance and steady state dynamic error were used to assess the number of satellites for which tracking was possible at specific receiver orbital positions. Tracking required that the error remain within the linear regime of the discriminator. Loops designed with these thresholds were then simulated using a Monte Carlo approach. These simulations used a nonlinear model for the early minus late discriminator function, a loop filter producing a second order closed loop transfer function, and simulated thermal noise. Line of sight dynamics were approximated as constant acceleration during tracking. Measurements of the time it takes the loop to diverge were computed for the simulated "path" of each satellite in view. Satellite visibility statistics were generated by averaging results over independent simulations computed for a range of GPS constellation epochs. Results of the Monte Carlo simulations are presented for the apogees of the Magnetospheric Multi-Scale (MMS) mission. Demodulation of the 50 bps data message (which requires a carrier lock) is not considered in these simulations. Several techniques for obtaining current ephemerides, without requiring this demodulation, are outlined. Analytical models based upon the integration of stochastic differential equations are presented, and the application of these models to the tracking and acquisition problem is examined.
机译:对于将GPS用于高度大于GPS星座本身的高度的卫星导航,存在着兴趣。候选任务包括对地静止(GEO)和高地球轨道(HEO)卫星,尤其是那些偏心率较大的卫星。 HEO任务面临的挑战是近地点的GPS信号功率降低,以及近地点和近地点之间的视线动力学差异很大。在本文中,对延迟锁定环(DLL)进行了设计研究,以确定闭环带宽和预检测积分时间与轨道位置的关系,从而使跟踪环能够适应预期的信号强度和动态条件。基于鉴别器误差方差和稳态动态误差的跟踪阈值的近似值用于评估在特定接收机轨道位置可能进行跟踪的卫星数量。跟踪要求误差保持在鉴别器的线性范围内。然后使用蒙特卡洛方法对以这些阈值设计的循环进行仿真。这些仿真使用了非线性非线性模型来实现早期负差分函​​数,产生二阶闭环传递函数的环路滤波器以及模拟的热噪声。视线动力学近似为跟踪过程中的恒定加速度。针对每个卫星的模拟“路径”,计算了环路发散所需时间的测量值。卫星可见性统计数据是通过对针对一系列GPS星座历元计算出的独立仿真结果进行平均得出的。给出了磁层多尺度(MMS)任务最高点的蒙特卡罗模拟结果。在这些模拟中不考虑解调50 bps数据消息(需要载波锁定)。概述了在不需要这种解调的情况下获得当前星历表的几种技术。提出了基于随机微分方程积分的分析模型,并研究了这些模型在跟踪和捕获问题中的应用。

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