Self-contained calibration determination by jointly solving the attitude estimation and calibration problem in the steering vector domain

S. Zorn, M. Niestroj, M. Meurer, Friederike Wendler, M. Cuntz
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引用次数: 4

Abstract

Antenna calibration is a mandatory requirement to determine the attitude of a multi-antenna receiver. Moreover, knowing the antenna attitude can vastly improve detection and mitigation of spoofers and / or Radio Frequency Interferences (RFIs). In todays receivers the time-varying phase offset introduced by the active elements like amplifiers, downconverters as well as various filters and unequal cable lengths are usually calibrated using a pilot signal, which is injected in the antenna signal. This method, however, does not only complicate the manufacturing process, but also increases the complexity of the receiver architecture and power consumptions. New approaches developed recently use GNSS live signals for calibration. These methods are established based on the fact that for each incoming GNSS signal the direction of arrival (DOA) is exactly known by means of the ephemeris data, which is transmitted from each satellite. In order to estimate the calibration phases, the DOAs of the received satellite signals are compared with their corresponding expected DOAs, which are determined based on the ephemeris data. The problem, however, lies in the fact, that the expected DOAs are given in the East-North-Up (ENU) coordinate frame, whereas the measured DOAs are given in the local coordinate frame and are additionally affected by the unknown phase offsets to be calibrated. The proposed algorithm therefore solves the attitude estimation and calibration problem jointly. This paper proposes a novel algorithm and validates it using measurement data.
通过联合解决航向矢量域的姿态估计和定标问题,实现自包含定标
天线校准是确定多天线接收机姿态的强制性要求。此外,了解天线的姿态可以极大地提高对欺骗器和/或射频干扰(rfi)的检测和缓解。在当今的接收机中,由放大器、下变频器等有源元件以及各种滤波器和不等电缆长度引入的时变相位偏移通常使用注入天线信号的导频信号进行校准。然而,这种方法不仅使制造过程复杂化,而且增加了接收器结构的复杂性和功耗。最近开发的新方法使用GNSS实时信号进行校准。这些方法的建立是基于这样一个事实,即对于每个传入的GNSS信号,到达的方向(DOA)是通过星历数据精确地知道的,星历数据是从每个卫星传输的。为了估计定标相位,将接收到的卫星信号的doa与星历数据确定的相应期望doa进行比较。然而,问题在于,期望的doa是在East-North-Up (ENU)坐标系中给出的,而测量的doa是在局部坐标系中给出的,并且还受到待校准的未知相位偏移的影响。该算法同时解决了姿态估计和标定问题。本文提出了一种新的算法,并用实测数据对其进行了验证。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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