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Algorithms for Eliminating User Position Biases Caused by Satellite Constellation Changes or Differential Signal Gain or Loss in Kalman Filter and Weighted Least Squares Solutions

机译:用于消除由卫星星座变化或差分信号增益或卡尔曼滤波器和加权最小二乘解的差分信号增益或损耗引起的用户位置偏差的算法

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Loss or gain of positioning satellites and loss or gain of a differential correction signal are events that lead to undesirable GPS user position biases. These biases appear in the form of instantaneous jumps in a Weighted Least Squares WLS solution and drifts in a Kalman Filter KF solution. As a result, in both solutions, GPS positioning becomes problematic in various types of applications. For instance, on an agricultural field, when the user is trying to maintain long, parallel and straight swaths that are tightly close to one another, these position biases occur causing the vehicle to divert from its straight line path. Although, a bias might lead to a more accurate position in the absolute sense, in this work, what is sought-after is relative accuracy to a selected initial epoch comprising its satellite constellation and differential signal status which are considered the reference of truth. All gains or losses of constellation satellites or the differential signal that occur after the initial epoch are considered problematic and the biases they create must be eliminated. To deal with this task, in the case of WLS, a position bias filter PBF was implemented in the position domain. The PBF simply tracks and calculates the WLS position biases caused by every event and accumulates them in a position bias vector that is subtracted from the WLS solution’s position vector. Unfortunately a PBF cannot be used with a KF solution because the KF diffuses the instantaneous position jumps, encountered in WLS, into drifts over the course of several epochs, making it difficult to assess the biases in the position domain during these epochs. However, since pseudorange measurements are part of the input to a KF, another bias filter, called PseudoRange Bias Filter PRBF, that does the position bias elimination in the pseudorange domain, is introduced. The PRBF-KF combination demonstrates the ability to reap the benefits of both: position bias filtering and Kalman filtering in the same solution. This paper presents the two algorithms for position bias filtering: the PBF for the WLS solution and the PRBF for the KF solution, under all possible scenarios of satellite constellation and differential signal changes.
机译:定位卫星和差分校正信号的损耗或增益的损失或增益是导致不希望的GPS用户位置偏差的事件。这些偏差在加权最小二乘WLS解决方案中瞬时跳跃的形式出现,并在卡尔曼滤波器KF解决方案中漂移。结果,在两个解决方案中,GPS定位在各种类型的应用中成为问题。例如,在农业领域,当用户试图保持彼此紧密靠近的长,平行和直的条子时,发生这些位置偏差导致车辆从其直线路径转移。虽然,偏差可能导致绝对意义上的更准确的位置,在这项工作中,所寻求的是所选择的初始时代的所选初始时代的初始初始初始的位置,该初始时代包括其卫星星座和差分信号状态,这些初始时期被认为是真理的参考。星座卫星的所有收益或损失或初始时代发生的差分信号被认为是有问题的,并且必须消除它们创造的偏差。要处理此任务,请在WLS的情况下,在位置域中实现位置偏置滤波器PBF。 PBF简单地追踪并计算由每个事件引起的WLS位置偏差,并在从WLS解决方案的位置向量中减去的位置偏置向量中累积它们。不幸的是,PBF不能与KF解决方案一起使用,因为KF扩散了在WLS中遇到的瞬时位置跳跃,以在几个时期的过程中漂移,使得难以在这些时期期间评估位置域中的偏差。然而,由于伪距测量值是输入的一部分为KF,另一个偏置滤波器,称为伪距偏置滤波器PRBF,但这在伪距域的位置偏压消除被引入。 PRBF-KF组合演示了获得两者的益处的能力:在同一解决方案中的位置偏置滤波和卡尔曼滤波。本文介绍了适用于位置偏置滤波的两种算法:在所有可能的卫星星座和差分信号变化的所有可能场景下,WLS解决方案的PBF和KF解决方案的PBF。

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