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    船用天文导航设备星体跟踪测量误差建模与校正方法研究

    Modeling and Correction Methods for Stellar Tracking Measurement Errors in Marine Celestial Navigation Equipment

    • 摘要: 针对船用小视场天文导航设备中星体跟踪测量误差补偿问题,开展误差建模与校正方法研究。建立了星体跟踪直角坐标系体系,系统分析了星体跟踪测量误差源及误差传播过程,并基于小角度误差约束构建了经典星体跟踪测量误差模型。经典模型在轴系存在非线性安装误差或光学成像存在畸变的情况下,其适用性受到限制。为此,进一步研究了基于神经网络的星体跟踪测量误差建模与校正方法。利用实测星体跟踪测量数据进行试验验证,结果显示:经典方法对星体跟踪测量的方位差补偿精度为0.034′(RMS),高度差补偿精度为0.041′(RMS),神经网络方法的方位差补偿精度为0.018′(RMS),高度差补偿精度为0.035′(RMS)。试验结果证明了两种方法的有效性,并且神经网络方法在补偿精度上优于经典方法,可展现出更好的校正性能。

       

      Abstract: To address the compensation and correction of stellar tracking measurement errors in marine celestial navigation equipment with a small field of view, this study investigates error modeling and correction methods. A rectangular coordinate system for stellar tracking is established, and the sources of measurement errors along with their propagation processes are analyzed. A classical stellar tracking error model is constructed under small-angle error constraints. However, the classical model's reliance on small-angle approximations imposes stringent requirements on machining, alignment precision of the tracking axis, and optical system imaging accuracy, making it unsuitable for cases involving nonlinear installation errors or optical distortion. To overcome this limitation, a neural network-based approach for stellar tracking error modeling and correction is further explored, including input-output design, network architecture, model training, and error compensation implementation. Experimental validation using real-world stellar tracking data demonstrates that the classical method achieves a compensation accuracy of 0.034′ (RMS) for azimuth error and 0.041′ (RMS) for elevation error in stellar tracking measurements, while the neural network method achieved accuracies of 0.018′(RMS) for azimuth error and 0.035′(RMS) for elevation error. The results confirm the effectiveness of both approaches, with the neural network method outperforming the classical one in compensation precision.

       

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