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...     

基于纠删码的遥测链路丢帧恢复技术

针对遥测系统在恶劣天气条件、航天器姿态调整、天线指向偏离、脉冲干扰等各种因素影响下出现的遥测信号闪断以至接收机丢帧问题,提出一种适用于闪断信道的纠删码技术,用于恢复丢失的数据帧.首先介绍LDPC（低密度奇偶校验）纠删码的编译码算法,然后构造一种以短码长的随机码为外码、IRA（不规则重复累积）LDPC码为内码的级联纠删码,最后给出纠删码的应用策略和实现纠删码所需的CCSDS（空间数据系统咨询委员会）协议扩展.通过仿真实验和分析,得到了LDPC纠删码和级联纠删码的纠删性能,得出级联纠删码与LDPC纠删码均可获得接近理想的纠删性能的结论,且级联纠删码的构造更为灵活,可适应不同的应用环境,对CCSDS协议进行适当扩展后即可支持纠删码在CCSDS遥测链路中的应用.     

光照处理中改进的Gamma矫正方法

在图像处理中，光照始终是影响图像质量的重要因素。为了有效弱化光照对图像质量的影响，利用非线性函数叠加的方法构造了一个合理的Gamma值变化曲线，使Gamma矫正方法充分适应了图像中光照变化的实际情况，并有效防止了Gamma矫正可能产生的图像失真。实验证明该方法在改善图像光照条件、提高图像质量方面具有良好的性能。     

渐开螺旋面啮合误差的广义圆柱坐标测量原理

论述了渐开螺旋面啮合误差测量的新方法——广义圆柱坐标法,给出了测量原理与实现方法、数学模型和数据处理算式;同时,指出了迄今一些文献中论述啮合误差测量时存在的错误。     

基于OEM的差分GPS基准站的设计

介绍了差分GPS(DGPS)的定位模型以及RTCM SC-104数据格式及其电文编码,提出了利用廉价的GPS-OEM(原始设备制造商)建立基准站的设计方案,方法是利用GPS-OEM和微处理器构成硬件系统,利用GPS-OEM输出的二进制差分修正数据,将其编码为RTCM SC-104电文来进行设计.实验结果表明这种DGPS基准站同样可以达到1~5?m的水平平面定位精度,因此具有性能价格比高,实用灵活的优点.     

实际检定工作中重复性引起不确定度的计算

论述采用合并样本标准差和B类不确定度评定方法计算重复性引起的不确定度，使可以在符合检定规将规定的较少测量次数中得到比较可靠的标准不确定度．     

关于灵敏系数命题的证明及应用

提出了“灵敏系数等于输入量导出的输出量的标准偏差和输入量自身标准偏差之比”的命题,并用数学逻辑给予了证明。     

An improved approach to model ionospheric delays for single-frequency Precise Point Positioning

PPP with low-cost, single-frequency receivers has been receiving increasing interest in recent years because of its large amount of possible users. One crucial issue in single-frequency PPP is the mitigation of ionospheric delays which cannot be removed by combining observations on different frequencies. For this purpose, several approaches have been developed, such as, the approach using ionospheric model corrections with proper weight, the GRAPHIC (Group and Phase Ionosphere Calibration) approach, and the method to model ionospheric delays over a station with a low polynomial or stochastic process. From our investigation on the stochastic characteristics of the ionospheric delay over a station, it cannot be precisely represented by either a deterministic model in the form of a low-order polynomial or a stochastic process for each satellite, because of its strong irregular spatial and temporal variations. Therefore, a novel approach is developed accordingly in which the deterministic representation is further refined by a stochastic process for each satellite with an empirical model for its power density. Furthermore, ionospheric delay corrections from a constructed model using GNSS data are also included as pseudo-observations for a better solution. A large data set collected from about 200 IGS stations over one month in 2010 is processed with the new approach and several commonly adopted approaches for validation. The results show its significant improvements in terms of positioning accuracy and convergence time with a negligible extra processing time, which is also demonstrated by data collected with a low-cost, handheld, single-frequency receiver.     

Improvement of the ADEOS-II/GLI sun-glint algorithm using concomitant microwave scatterometer-derived wind data

The tendency of over-estimation of sun-glint reflectance was found in GLI satellite ocean color data, after applying the traditional sun-glint model of Cox and Munk together with objective analysis wind data. ADEOS-II has provided a good opportunity to improve the glint model using data measured by GLI and SeaWinds, both onboard the satellite. With the help of simultaneous wind measurements achieved by SeaWinds, the Cox and Munk model is re-evaluated using GLI measurements to obtain a new relationship between the surface mean square slope and wind. The new model was found to be very close to the Cox and Munk under moderate wind speed but is much different under calm condition, where it shows similarity to the result reported by Ebuchi and Kizu. It also improves the ocean color data availability and the precision of sun-glint reflectance, based on the evaluation result of the generated Level 3 data products.     

基于简化误差修正的卫星姿态确定算法

针对典型的星敏感器/陀螺姿态卫星确定算法运算复杂这一问题,提出了一种基于简化误差修正的星敏感器/陀螺卫星姿态确定算法.通过对陀螺角速度进行简化修正,减少了滤波器的状态变量,降低滤波器的复杂性.仿真结果表明：该算法在保证姿态确定精度的条件下,能够减少运算量,提高算法的实时性.