星地时间比对大气误差修正及其影响因素分析

Analysis of atmospheric error correction in satellite-ground time comparison and its influencing factors

  • 摘要: 由于空间环境较为复杂,大气对无线电微波信号的影响是星地高精度时间比对的主要误差源之一. 针对星地高精度时间比对的需求,研究了双向测量体制下的电离层误差修正方法及对流层色散延迟修正方法,对影响大气误差修正的主要因素展开了讨论,并对不同场景下大气误差修正情况及星地时间比对结果进行了仿真分析. 仿真结果表明:当卫星姿态误差控制在100 as以内、相位中心标定误差控制在5 mm以内、精密定轨误差控制在30 cm以内时,通过相应的误差修正算法修正后,电离层误差残差的RMS值小于0.006 ps,对流层误差残差的RMS值小于0.06 ps,星地时间比对精度优于皮秒量级.

     

    Abstract: Due to the complex space environment, the influence of the atmosphere on the radio and microwave signals is one of the main error sources for the high-precision satellite-to-earth two-way time matching. In order to meet the requirements of the satellite-ground time comparison, the ionospheric error correction method and dispersive troposphere delays correction method in the triple-frequency system are studied, the main factors affecting the atmospheric error correction are discussed, and the atmospheric error correction and the satellite-ground time comparison results under different scenarios are simulated and analyzed. The simulation results show that when the satellite attitude error is controlled within 100 as, the phase center calibration error is controlled within 5 mm, and the orbit position error is controlled within 30 cm.The root mean square (RMS) of ionospheric and tropospheric error residual are less than 0.006 ps and 0.06 ps respectively after correction, and the accuracy of star-ground time comparison is better than ps level.

     

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