基于轨道动力学模型的分布式SAR卫星编队CDGPS相对定位
doi: 10.11728/cjss2009.05.515 cstr: 32142.14.cjss2009.05.515
CDGPS Relative Position Determination of Distributed SAR Satellite Formation Based on Dynamic Orbit Model
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摘要: 针对分布式SAR卫星编队星间基线的高精度确定问题, 提出了基于轨道动力学模型的分布式SAR卫星编队CDGPS相对定位方法. 根据CDGPS原理及基于轨道动力学模型的星间相对定位原理,在CDGPS测量的基础上, 引入轨道动力学模型提供的先验约束信息, 对长弧段的观测数据进行解算, 克服了运动学逐点解算方法在观测几何较差或观测数据不足情况下无法应用的缺点. 此方法能够有效抑制测量中的随机误差, 提高相对定位精度, 提供了一种可实现mm量级星间基线确定的技术途径. 通过仿真计算验证了动力学方法的有效性. 计算结果表明, 动力学方法可以显著提高相对定位精度. 相对于运动学方法, 前者L1固定解的精度提高了68%, 而消电离层固定解的精度提高了95%.Abstract: To determine the baseline of distributed SAR satellite formation at high accuracy, a CDGPS relative position method of distributed SAR satellite formation based on dynamic orbit model is presented. At first, CDGPS principle is introduced. And then, intersatellite relative position method based on dynamic orbit model is introduced. Based on CDGPS measurement, this method introduces prior restricted information provided by dynamic orbit model, and overcomes the disadvantage that kinematic single point position determination can not be used when observation geometry is bad or observations are not enough. This method can restrain the random errors in measurement, improve relative position accuracy and provide a technology approach to realize intersatellite baseline determination at mm level. At last, simulation computation verifies the efficiency of the dynamic method. Computational results show that the dynamic method can improve the relative position accuracy remarkably. Compared with kinematic method, the fixed solution accuracy of L1 is improved by 68%, and the fixed solution accuracy of ionosphere free combination is improved by 95%.
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Key words:
- Distributed SAR /
- Baseline /
- CDGPS /
- Dynamic orbit model
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