Development and Evaluation of Airborne Multipath Error Bounds for L1-L5

J. Blanch, T. Walter, R. E. Phelts
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引用次数: 4

Abstract

Current aviation standards define a multipath error model that is valid after the smoothing filter is assumed to have converged (assuming a 100 s Hatch filter). The draft standards for dual frequency Satellite-based Augmentation Systems further specify an error model when the code has not been smoothed, and it is defined as a multiple of the converged value. In this paper, multipath and noise error bounds are derived as a function of smoothing time assuming a first order model for the code multipath and the receiver noise. These error bounds are evaluated using GPS and Galileo measurements collected in flight. The derived model appears to account well for the error reduction as a function of smoothing time. INTRODUCTION The standards for Satellite-based Augmentation Systems (SBAS) Dual Frequency Multi-constellation (DFMC) are currently being developed. With dual frequency, the residual ionospheric delay error (which is the largest contributor in single frequency) is no longer the dominant term. In particular, multipath and receiver noise is now a much more important term in the error budget. For this reason, and because of the introduction of new signals (L5 and E5a), these term is receiving more attention, and new data suggests that extrapolating L1 models to L5 and L1-L5 combination might not be sufficient [5]. This multipath and antenna group delay error model used in single frequency SBAS has been in place since 2000 [1]. This model is elevation dependent and only applies once the carrier smoothing filter has converged, which is assumed to occur after 360 s of smoothing. The current standards do not specify how the multipath error bound varies with smoothing time before convergence. The draft SBAS DFMC Minimum Operational Standards [2] (developed within EUROCAE) specifies an additional constraint: for unsmoothed code measurements, the standard deviation is ten times higher than the value at convergence. A strict application of this error model between t=0 and t = 360 s would result in very conservative error bounds, because in reality the actual errors decrease steadily as new measurements are added. In particular, it could result in significant performance losses in the presence of cycle slips. This is especially critical for environments with ionospheric scintillation (for example in low latitudes), where we expect a much higher cycle slip rate. And even if the receivers do use a less conservative multipath curve, service providers evaluating coverage would need to assume the minimum requirement, and therefore could be unable to claim availability where there might be. The goal of this paper is twofold: to derive a multipath error model that is valid before convergence, and to evaluate it using GNSS airborne measurements. In the first part, we develop three models: one corresponding to time invariant smoothing, one corresponding to time varying smoothing, and one where we start with a time varying smoothing that switches to time invariant after a set time interval. In the second part, we evaluate the multipath error model using GNSS data collected in flight. MULTIPATH ERROR MODEL AT CONVERGENCE In this paper, we will assume that the error model at convergence is given by the formulas specified in [2], which are based on the ones used in [1]: ( ) ( ) ( ) 4 4 2 2 1 5 & , , 2 2 2 1 5 L L air MP AGVD i noise i L L f f f f    + = + − (1) Where: ( ) 0.13[m] 0.53[m]exp( /10[deg]) MP    = + − (2) We will further assume that the temporal error model can be modeled as: ( ) ( ) ( )( ) ( )( ) 4 4 2 2 1 5 & , , 2 2 2 1 5 L L air MP MP AGVD i noise noise i L L f f k A k A k f f    + = + − (3) Where k is the time step, and AMP are Anoise are functions such that: ( ) ( ) ( ) ( ) 0 100, 360 1, 0 200, 360 1 MP
L1-L5机载多径误差界的发展与评估
当前的航空标准定义了一种多路径误差模型,该模型在平滑滤波器被假设为收敛后有效(假设是100秒的Hatch滤波器)。双频星载增强系统标准草案进一步明确了编码未平滑时的误差模型,并将其定义为收敛值的倍数。在假定码多径和接收机噪声为一阶模型的情况下,导出了多径和噪声误差边界作为平滑时间的函数。这些误差范围是使用GPS和伽利略在飞行中收集的测量值来评估的。导出的模型似乎很好地说明了作为平滑时间的函数的误差减小。星基增强系统(SBAS)双频多星座(DFMC)标准目前正在开发中。在双频条件下,残余电离层延迟误差(在单频条件下是最大的影响因子)不再占主导地位。特别是,多径和接收机噪声现在是误差预算中更重要的一个术语。由于这个原因,并且由于引入了新的信号(L5和E5a),这些术语受到了更多的关注,新的数据表明,将L1模型外推到L5和L1-L5组合可能是不够的。这种用于单频SBAS的多径和天线群延迟误差模型自2000年以来一直存在。该模型是仰角相关的,只有在载波平滑滤波器收敛后才适用,假设这发生在360秒的平滑之后。目前的标准没有规定收敛前多径误差界如何随平滑时间变化。SBAS DFMC最低操作标准草案[2](在EUROCAE内开发)规定了一个额外的约束:对于非平滑代码测量,标准偏差比收敛值高十倍。严格应用t=0和t= 360秒之间的误差模型会导致非常保守的误差界限,因为在现实中,随着新测量的增加,实际误差会稳步下降。特别是,在出现周期滑移的情况下,它可能导致显著的性能损失。这对于电离层闪烁的环境(例如在低纬度地区)尤其重要,我们预计在那里会有更高的周期滑移率。而且,即使接收器确实使用了不那么保守的多径曲线,服务提供商评估覆盖范围时也需要假设最低要求,因此可能无法在可能存在的地方宣称可用性。本文的目标有两个:推导出收敛前有效的多径误差模型,并使用GNSS机载测量对其进行评估。在第一部分中,我们开发了三个模型:一个对应于时不变平滑,一个对应于时变平滑,一个我们从时变平滑开始,在设定的时间间隔后切换到时不变。在第二部分中,我们使用飞行中收集的GNSS数据评估了多径误差模型。多路径误差模型在本文的融合,我们将假设收敛的误差模型是由[2]中指定的公式,给出基于[1中使用的 ]: ( ) ( ) ( ) 4 4 2 2 1 5 &,, 2 2 2 1 5 L L空气议员AGVD我噪音L L f f f f+ = +−(1):0.53 (0.13)[m] . [m] . exp(/ 10[度])议员= +−(2)我们将进一步假设时间误差模型可以建模为:( ) ( ) ( )( ) ( )( ) 4 4 2 2 1 5 &,, 2 2 2 1 5 L L空气议员议员AGVD我噪音噪音我k一个k k L L f f f f+ = +−(3)k是时间步,和安培是函数,这样声音吵醒 : ( ) ( ) ( ) ( ) 0 100 360 1 0 200 360 1像素
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