船载星敏感器测星数据蒙气差实时修正方法

针对船载星敏感器安装在航天测量船上而引起的测星数据如何进行蒙气差实时修正问题,在分析船载经纬仪目前使用的蒙气差修正方法和中国天文年历提供的蒙气差修正方法的修正精度的基础上,提出船载星敏感器测星数据的蒙气差实时修正方法,给出蒙气差常数R0和温度变差乘数A的改正量α的计算公式,解决了工程应用上的高精度和实时性问题;同时,在分析大气温度、大气压力对船载星敏感器测星数据蒙气差影响的基础上,提出工程应用中的气象数据采集与使用的具体方案。     

喷管模型试验器六分量天平校准技术

为了提高喷管内流试验台六分量测力天平的静态和动态校准的精度和准度,采用了理论计算与标模试验相结合的方法,开展了天平校准技术研究.对静校的原始数据进行1次项与3次项对比分析,得出了天平在安装、调试阶段的经验模型,重复性标模试验表明完善的数据处理方法可以极大地提高天平动校精度和准度,试验结果与四分量天平比较,证明了天平性能的可靠性以及以喷管落压比为基准修正测力系统附加力、附加力矩的正确性.该六分量天平校准方法可对其他多分量测力系统的校准提供参考.      

大气电波折射引起无线定位误差的试验研究

由于空中大气介质的不均匀性使得电波传播速度减慢射线产生弯曲,从而产生折射误差。因此要提高无线电定位的精度,就必须进行电波折射修正。本文提出了电波折射误差快速算法及修正。     

数字逻辑设计的冗余与检错纠错

在分析数字逻辑电路的特点及其给实现容错目标带来的困难基础上,阐述了冗余类型与可靠性设计（检错纠错）间的关系,给出了一种改进的单元加固型容错触发器结构设计。     

数字控制APFC电路的设计与仿真研究

研究了数字控制APFC的原理和方法。利用先进的数字信号处理芯片DSP的高运算能力以及丰富的外设,加入PI控制算法,运用电压、电流双闭环控制,使输入电流跟踪输入电压,两者相位保持一致,输入功率因数接近于1,并在Matlab/Simulink环境下进行仿真研究,取得了理想的效果。     

弧焊机器人旋转电弧传感实时焊缝纠偏系统的开发

本论文研究了以高速旋转传感电弧为传感器智能弧焊机器人实时焊缝纠偏系统,着重讨论了焊纠偏系统的硬件组成和软件结果。     

速度梯度对圆柱探针测量的影响及修正

圆柱探针在测量有横向速度梯度的流场时,会得出偏离真实值的结果.通过数值与实验研究,发现此影响主要为对来流方向的测量偏差,与真实值的差异为向低速区的一个偏差角;另外一个影响是使测得的速度值偏大一点.通过详细的数值模拟得出了偏差角及速度大小与来流速度梯度之间的关系,并在实验中得到了验证.最后将此修正方法用于叶栅实验测量数据,得到了较好的修正效果.      

A new method for improving the performance of an ionospheric model developed by multi-instrument measurements based on artificial neural network

There are remarkable ionospheric discrepancies between space-borne (COSMIC) measurements and ground-based (ionosonde) observations, the discrepancies could decrease the accuracies of the ionospheric model developed by multi-source data seriously. To reduce the discrepancies between two observational systems, the peak frequency (foF2) and peak height (hmF2) derived from the COSMIC and ionosonde data are used to develop the ionospheric models by an artificial neural network (ANN) method, respectively. The averaged root-mean-square errors (RMSEs) of COSPF (COSMIC peak frequency model), COSPH (COSMIC peak height model), IONOPF (Ionosonde peak frequency model) and IONOPH (Ionosonde peak height model) are 0.58 MHz, 19.59 km, 0.92 MHz and 23.40 km, respectively. The results indicate that the discrepancies between these models are dependent on universal time, geographic latitude and seasons. The peak frequencies measured by COSMIC are generally larger than ionosonde’s observations in the nighttime or middle-latitudes with the amplitude of lower than 25%, while the averaged peak height derived from COSMIC is smaller than ionosonde’s data in the polar regions. The differences between ANN-based maps and references show that the discrepancies between two ionospheric detecting techniques are proportional to the intensity of solar radiation. Besides, a new method based on the ANN technique is proposed to reduce the discrepancies for improving ionospheric models developed by multiple measurements, the results indicate that the RMSEs of ANN models optimized by the method are 14–25% lower than the models without the application of the method. Furthermore, the ionospheric model built by the multiple measurements with the application of the method is more powerful in capturing the ionospheric dynamic physics features, such as equatorial ionization, Weddell Sea, mid-latitude summer nighttime and winter anomalies. In conclusion, the new method is significant in improving the accuracy and physical characteristics of an ionospheric model based on multi-source observations.     

Contribution analysis of QZSS to single-frequency PPP of GPS/BDS/GLONASS/Galileo

The Quasi-Zenith Satellite System (QZSS) established by the Japan Aerospace Exploration Agency mainly serves the Asia-Pacific region and its surrounding areas. Currently, four in-orbit satellites provide services. Most users of GNSS in the mass market use single-frequency (SF) receivers owing to the low cost. Therefore, it is meaningful to analyze and evaluate the contribution of the QZSS to SF precise point positioning (PPP) of GPS/BDS/GLONASS/Galileo systems with the emergence of GNSS and QZSS. This study compares the performances of three SF PPP models, namely the GRoup and PHase Ionospheric Correction (GRAPHIC) model, GRAPHIC with code observation model, and an ionosphere-constrained model, and evaluated the contribution of the QZSS to the SF PPP of GPS/BDS/GLONASS/Galileo systems. Moreover, the influence of code bias on the SF PPP of the BDS system is also analyzed. A two-week dataset (DOY 013–026, 2019) from 10 stations of the MGEX network is selected for validation, and the results show that: (1) For cut-off elevation angles of 15, 20, and 25°, the convergence times for the static SF PPP of GLONASS + QZSS are reduced by 4.3, 30.8, and 12.7%, respectively, and the positioning accuracy is similar compared with that of the GLONASS system. Compared with the BDS single system, the convergence times for the static SF PPP of BDS + QZSS under 15 and 25° are reduced by 37.6 and 39.2%, the horizontal positioning accuracies are improved by 18.6 and 14.1%, and the vertical components are improved by 13.9 and 21.4%, respectively. At cut-off elevation angles of 15, 20, and 25°, the positioning accuracy and precision of GPS/BDS/GLONASS/Galileo + QZSS is similar to that of GPS/BDS/GLONASS/Galileo. And the convergence times are reduced by 7.4 and 4.3% at cut-off elevation angles of 20 and 25°, respectively. In imitating dynamic PPP, the QZSS significantly improves the positioning accuracy of BDS and GLONASS. However, QZSS has little effect on the GPS-only, Galileo-only and GPS/BDS/GLONASS/Galileo. (2) The code bias of BDS IGSO and MEO cannot be ignored in SF PPP. In static SF PPP, taking the frequency band of B1I whose multipath combination is the largest among the frequency bands as an example, the vertical component has a systematic bias of approximately 0.4–1.0 m. After correcting the code bias, the positioning error in the vertical component is lower than 0.2 m, and the positioning accuracy in the horizontal component are improved accordingly. (3) The SF PPP model with ionosphere constraints has a better convergence speed, while the positioning accuracy of the three models is nearly equal. Therefore the GRAPHIC model can be used to get good positioning accuracy in the absence of external ionosphere products, but its convergence speed is slower.     

运载火箭全捷联惯性/星光复合制导研究

全捷联惯性/星光复合制导是运载火箭空间快速响应发射的重要途径.针对捷联惯性制导系统中初始定位定向误差、初始调平对准误差及惯性器件漂移等3类主要误差因素,建立了运载火箭的数字平台基准偏差模型和导航误差模型,并提出了一种双星修正策略方案.数值仿真分析了各误差因素对捷联惯性导航精度的影响,并进一步验证了该复合制导方案的可行性...