基于无奇异变换的卫星广播星历拟合算法

针对导航卫星轨道偏心率近似为0,致使卫星轨道的近地点角距定义模糊,在数据拟合过程中会导致法矩阵（H^TH）奇异的问题,本文提出基于无奇异变换的广播星历参数拟合算法,引入无奇异轨道根数代替经典开普勒根数,推导了空间目标位置矢量对基于无奇异轨道根数的广播星历参数偏导数矩阵,利用变换后的观测方程迭代拟合得到改进广播星历参数,再将结果归一化到基于开普勒根数的广播星历参数。最后利用仿真算例验证了所推公式和算法的合理性。     

一种地球紫外中心快速提取方法

针对地球紫外中心指向高精度提取问题,提出一种基于梯度统计的快速、低存储需求的紫外地平圆盘中心提取算法。首先,考虑到星载计算机与高内存消耗的滤波算法、实时导航需求的冲突,采用结合Sobel边缘算子与局部二值模式（LBP）算子的改进边缘快速提取方法,有效剔除背景噪声并准确提取地球紫外临边特征。然后对非完整临边边缘采用最小二乘拟合得到中心的精确位置。实验结果表明,该方法抗噪声,可实现亚像素级地球中心提取,并显著降低存储需求和计算时间开销。对于1046×746的图像,该算法需要的存储空间仅为1100kByte,运算时间在20ms内,满足自主导航的需求。     

A two-step robust adaptive filtering algorithm for GNSS kinematic precise point positioning

In kinematic navigation and positioning, abnormal observations and kinematic model disturbances are one of the key factors affecting the stability and reliability of positioning performance. Generally, robust adaptive filtering algorithm is used to reduce the influence of them on positioning results. However, it is difficult to accurately identify and separate the influence of abnormal observations and kinematic model disturbances on positioning results, especially in the application of kinematic Precise Point Positioning (PPP). This has always been a key factor limiting the performance of conventional robust adaptive filtering algorithms. To address this problem, this paper proposes a two-step robust adaptive filtering algorithm, which includes two filtering steps: without considering the kinematic model information, the first step of filtering only detects the abnormal observations. Based on the filtering results of the first step, the second step makes further detection on the kinematic model disturbances and conducts adaptive processing. Theoretical analysis and experiment results indicate that the two-step robust adaptive filtering algorithm can further enhance the robustness of the filtering against the influence of abnormal observations and kinematic model disturbances on the positioning results. Ultimately, improvement of the stability and reliability of kinematic PPP is significant.     

高分辨率多径时延测量算法

提出一种基于最小二乘准则的高分辨率多径信号时延测量方法。对参考信号作三阶样条插值获得每条多径信号最小二乘意义的最优估计,用每条多径信号的测量值重构接收信号,通过反复迭代使重构信号是接收信号最小二乘意义的最优估计,实现多径信号的时延测量。仿真结果表明：新算法在低信噪比、窄带信号条件下仍能获得较高的时延测量精度,性能优于MUSIC类时差测量算法。     

一种提高热电阻测温准确性方法研究

分析了工业铂、铜热电阻电阻-温度特性,以工业铂电阻温度传感器为例,给出了一种提高热电阻测温准确度的方法。通过对工业铂电阻进行多点测试,利用最小二乘法对测得数据进行拟合,得出新的电阻-温度转换公式和分度表。通过试验数据的比较表明,使用该方法可以提高传感器的测温准确性。     

A point-wise least squares spectral analysis (LSSA) of the Caspian Sea level fluctuations,using TOPEX/Poseidon and Jason-1 observations

The Caspian Sea has displayed considerable fluctuations in its water level during the past century. Knowledge of such fluctuation is vital for understanding the local hydrological cycles, climate of the region, and construction activities within the sea and along its shorelines. This study established a point-wise satellite altimetry approach to monitor the fluctuations of the Caspian Sea using a complete dataset of TOPEX/Poseidon for the period 1993 to the middle of 2002, and its follow-on Jason-1 for the period 2002 to August 2009. Therefore, 280 virtual time-series were constructed to monitor the fluctuations. The least squares spectral analysis (LSSA) method is, then employed to find the most significant frequencies of the time-series, while the statistical method of principle component analysis (PCA) is applied to extract the dominant variability of level variations. The study also used the observations of TOPEX/Poseidon and Jason-1 over the Volga River along with 5 years of Volga’s water discharge to study its influence on the Caspian Sea level changes. The LSSA results indicate that the lunar semidiurnal (M2) and the Sun semidiurnal (S2) frequencies are the main tidal frequencies of the Caspian Sea with the mean amplitude of 4.2 and 2.8 cm, respectively. A statistically significant long-term frequency (12.5-years period) is also found from altimetry and tide gauge observations. A phase lag, related to the inter-annual frequencies of the Volga River was detected from the point-wise time-series showing level propagation from the northwest to the southeast of the sea. The cross-correlation between the power spectrum of Volga and that of the northern-most, middle, and southern-most points within the Caspian Sea were respectively 0.63, 0.51 and 0.4 of zero-lag correlation, corroborating the influence of the Volga River. The result of PCA also shows that different parts of the Caspian Sea exhibit different amplitudes of level variations, indicating that the point-wise approach, when employing all available satellite measurements could be a suitable method for a preliminary monitoring of this inland water resource as it gives accurate local fluctuations.     

DSSS卫星通信中窄带干扰的盲检测与消除研究

建立了干扰条件下的接收信号模型,提出了干扰抑制方案。利用信号谱包络的相似性 ,给出了基于滑动窗最小二乘的干扰盲检测方法,进而根据对消的思想消除窄带干扰。仿真 结果表明该方法能有效抑制DSSS卫星通信中常见的窄带干扰。     

利用条件平差实现导航星座自主守时方法

针对导航星座自主导航系统的重要组成部分———自主守时系统,提出了一种简便易行的新算法:根据星间测距数据,采用条件平差进行自主守时计算;并且介绍了此方法基本原理和实现思路。自主守时仿真计算表明,此方法守时同步误差不累积,距离测量误差0.1m时,时间同步误差均方根小于0.4m。     

递推的TLS参数估计方法及其在飞轮FDD中的应用

飞轮是很多卫星姿态控制系统中的重要执行部件，其星上自主故障诊断是一个很有意义的研究课题。本文根据飞轮系统的特点，在最小二乘（ＬＳ）参数估计方法的基础上提出了全最小二乘（ＴＬＳ）参数估计的递推形式，证明了它对飞轮参数估计的收敛性，并用于飞轮缓变故障的检测和诊断，取得了较好结果。     

多传感器目标识别的优化融合

对于工作在复杂环境下的多传感器目标识别系统,确保其稳健性和准确性的关键是有效处理被融合信息的不确定性。根据影响信息不确定性的因素,文章把传感器本地识别信息的可信度分为了统计可信度和环境可信度;采用最小二乘法和神经网络实现统计可信度的估计,自适应神经模糊推理实现环境可信度估计;并利用这两种可信度实现以一致理论为基础的多传感器目标识别的优化融合。经实验仿真证明,该融合方案是有效的。