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临近空间飞行器INS/CNS深度组合导航方法

INS/CNS Deeply Integrated Navigation Method of Near Space Vehicles.

作者信息

Mu Rongjun, Sun Hongchi, Li Yuntian, Cui Naigang

机构信息

School of Aerospace Science and Technology, Harbin Institute of Technology, Harbin 150001, China.

出版信息

Sensors (Basel). 2020 Oct 17;20(20):5885. doi: 10.3390/s20205885.

DOI:10.3390/s20205885
PMID:33080901
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7589122/
Abstract

Celestial navigation is required to improve the long-term accuracy preservation capability of near space vehicles. However, it takes a long time for traditional celestial navigation methods to identify the star map, which limits the improvement of the dynamic response ability. Meanwhile, the aero-optical effects caused by the near space environment can lead to the colorization of measurement noise, which affects the accuracy of the integrated navigation filter. In this paper, an INS/CNS deeply integrated navigation method, which includes a deeply integrated model and a second-order state augmented H-infinity filter, is proposed to solve these problems. The INS/CNS deeply integrated navigation model optimizes the attitude based on the gray image error function, which can estimate the attitude without star identification. The second-order state augmented H-infinity filter uses the state augmentation algorithm to whiten the measurement noise caused by the aero-optical effect, which can effectively improve the estimation accuracy of the H-infinity filter in the near space environment. Simulation results show that the proposed INS/CNS deeply integrated navigation method can reduce the computational cost by 50%, while the attitude accuracy is kept within 10" (3 ). The attitude root mean square of the second-order state augmented H-infinity filter does not exceed 5", even when the parameter error increases to 50%, in the near space environment. Therefore, the INS/CNS deeply integrated navigation method can effectively improve the rapid response ability of the navigation system and the filtering accuracy in the near space environment, providing a reference for the future design of near space vehicle navigation systems.

摘要

天基导航对于提高近空间飞行器的长期精度保持能力是必不可少的。然而,传统的天基导航方法识别星图耗时较长,这限制了动态响应能力的提升。同时,近空间环境引起的气动光学效应会导致测量噪声的彩色化,影响组合导航滤波器的精度。本文提出了一种INS/CNS深度组合导航方法,包括深度组合模型和二阶状态增广H无穷滤波器,以解决这些问题。INS/CNS深度组合导航模型基于灰度图像误差函数优化姿态,无需星图识别即可估计姿态。二阶状态增广H无穷滤波器采用状态增广算法白化气动光学效应引起的测量噪声,可有效提高近空间环境下H无穷滤波器的估计精度。仿真结果表明,所提出的INS/CNS深度组合导航方法可将计算成本降低50%,同时姿态精度保持在10"(3)以内。在近空间环境中,即使参数误差增加到50%,二阶状态增广H无穷滤波器的姿态均方根也不超过5"。因此,INS/CNS深度组合导航方法可有效提高导航系统在近空间环境下的快速响应能力和滤波精度,为未来近空间飞行器导航系统的设计提供参考。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/977ff53172f0/sensors-20-05885-g015.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/f41f1d1e3fa1/sensors-20-05885-g013.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/bca55ed6f3fe/sensors-20-05885-g014.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/977ff53172f0/sensors-20-05885-g015.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/f41f1d1e3fa1/sensors-20-05885-g013.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/bca55ed6f3fe/sensors-20-05885-g014.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e4b4/7589122/977ff53172f0/sensors-20-05885-g015.jpg

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