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Robust Inertial-Astronomic Attitude Determination Algorithm with Adaptive Star Geometrical Error Model for HCVs

机译:HCV的自适应星几何误差模型的鲁棒惯性-天文姿态确定算法

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摘要

Inertial/astronomic integration is an effective way to improve the accuracy of attitude determination of hypersonic cruise vehicles (HCVs). Compared with common low-dynamic aircraft, the environmental affection during hypersonic flight leads to the non-Gaussian noise character of astronomic observation. Meanwhile, rapid star geometry changing during HCVs' rapid movement causes redistribution of errors in astronomic measurements and significant variation of its main Gaussian characteristic. A kind of robust inertial/astronomic attitude determination algorithm with adaptive star geometrical error model is proposed. The adaptive star geometrical error distribution model is established for obtaining the main Gaussian model of astronomic measurement misalignment errors in flight. After that, inertial/astronomic integration model-based on misalignment errors is proposed, which avoids Euler angle transformation. On these bases, the improved robust filter algorithm is designed, which utilizes real-time astronomic error distribution as the weighting standard of Huber-based optimal estimation. Simulation results indicate that by taking the changing of main Gaussian distribution into consideration, the accuracy of inertial/astronomic integration is improved approximately 30% more than traditional algorithms adopting constant main Gaussian model in non-Gaussian HCV navigation environments.
机译:惯性/天文结合是提高高超音速巡航舰(HCV)姿态确定精度的有效方法。与普通的低动力飞机相比,高超声速飞行过程中的环境影响导致天文观测的非高斯噪声特征。同时,HCV快速移动期间恒星几何形状的快速变化会导致天文测量误差的重新分布,并导致其主要高斯特性发生明显变化。提出了一种具有自适应恒星几何误差模型的鲁棒惯性/天文姿态确定算法。建立自适应星几何误差分布模型,以获取飞行中天文测量失准误差的主要高斯模型。在此基础上,提出了基于失准误差的惯性/天文积分模型,避免了欧拉角变换。在此基础上,设计了改进的鲁棒滤波算法,该算法利用实时天文误差分布作为基于Huber的最优估计的加权标准。仿真结果表明,通过考虑主高斯分布的变化,惯性/天文积分的精度比在非高斯HCV导航环境中采用恒定主高斯模型的传统算法提高了约30%。

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