Correction technique for velocity and position error of inertial navigation system by celestial observations

F. Gul, F. Jiancheng
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引用次数: 17

Abstract

The residual sensor errors and misalignment of an inertial navigation system cause deviation from the true navigation solution. The navigation errors grow as function of time, sensor errors and vehicle dynamics. A celestial aided inertial navigation system (INS), carried on a space vehicle, has to rely on the independent INS output until the vehicle gets out of the dense atmospheric layer. The misalignment and gyro drift then can be corrected employing techniques for in-flight alignment by celestial observations. The accelerometer bias can be detected and compensated after the burn out point. Subsequent contribution to navigation error due to misalignment and sensor errors thus can be restricted. The accumulated velocity and position errors, however, cannot be directly determined from celestial observations and the knowledge of accelerometer bias. A technique for velocity and position error computation is presented. Simulations for strapdown inertial navigation system (SINS), mechanized in space stabilized reference frame, are carried out. Tremendous improvement in navigation accuracy is observed
利用天文观测修正惯性导航系统速度和位置误差的技术
惯性导航系统的残余传感器误差和不对准会导致与真实导航解的偏差。导航误差随时间、传感器误差和车辆动力学的变化而增大。空间飞行器携带的天体辅助惯性导航系统(INS),在飞行器脱离稠密的大气层之前,必须依赖独立的惯性导航系统输出。然后,可以利用天文观测的飞行对准技术来纠正陀螺偏差和漂移。在烧坏点之后,可以检测和补偿加速度计的偏差。因此,由于不对准和传感器误差导致的导航误差的后续贡献可以受到限制。然而,累积的速度和位置误差不能直接由天体观测和加速度计偏差的知识来确定。提出了一种计算速度和位置误差的方法。对空间稳定参考系下的捷联惯性导航系统进行了仿真研究。导航精度有了巨大的提高
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