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C/N0 Estimator Based on the Adaptive Strong Tracking Kalman Filter for GNSS Vector Receivers

机译:基于自适应强跟踪卡尔曼滤波的GNSS矢量接收机C / N0估计。

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摘要

The carrier-to-noise ratio ( ) is an important indicator of the signal quality of global navigation satellite system receivers. In a vector receiver, estimating using a signal amplitude Kalman filter is a typical method. However, the classical Kalman filter (CKF) has a significant estimation delay if the signal power levels change suddenly. In a weak signal environment, it is difficult to estimate the measurement noise for CKF correctly. This article proposes the use of the adaptive strong tracking Kalman filter (ASTKF) to estimate . The estimator was evaluated via simulation experiments and a static field test. The results demonstrate that the ASTKF estimator can track abrupt variations in and the method can estimate the weak signal correctly. When jumps, the ASTKF estimation method shows a significant advantage over the adaptive Kalman filter (AKF) method in terms of the time delay. Compared with the popular algorithms, the narrow-to-wideband power ratio (NWPR) method, and the variance summing method (VSM), the ASTKF estimator can adopt a shorter averaging time, which reduces the hysteresis of the estimation results.
机译:载波噪声比()是全球导航卫星系统接收机信号质量的重要指标。在矢量接收机中,使用信号幅度卡尔曼滤波器进行估计是一种典型的方法。但是,如果信号功率电平突然变化,则经典的卡尔曼滤波器(CKF)会有很大的估计延迟。在弱信号环境中,很难正确估计CKF的测量噪声。本文提出使用自适应强跟踪卡尔曼滤波器(ASTKF)进行估计。通过仿真实验和静态测试对评估器进行评估。结果表明,ASTKF估计器可以跟踪突变,并且该方法可以正确估计微弱信号。跳跃时,ASTKF估计方法在时间延迟方面显示出优于自适应卡尔曼滤波器(AKF)方法的显着优势。与流行的算法,窄带宽功率比(NWPR)方法和方差求和方法(VSM)相比,ASTKF估计器可以采用更短的平均时间,从而减少了估计结果的滞后。

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