Geostationary orbit determination using SATRE

A new strategy of precise orbit determination (POD) for GEO (Geostationary Earth Orbit) satellite using SATRE (SAtellite Time and Ranging Equipment) is presented. Two observation modes are proposed and different channels of the same instruments are used to construct different observation modes, one mode receiving time signals from their own station and the other mode receiving time signals from each other for two stations called pairs of combined observations. Using data from such a tracking network in China, the results for both modes are compared. The precise orbit determination for the Sino-1 satellite using the data from 6 June 2005 to 13 June 2005 has been carried out in this work. The RMS (Root-Mean-Square) of observing residuals for 3-day solutions with the former mode is better than 9.1 cm. The RMS of observing residuals for 3-day solutions with the latter mode is better than 4.8 cm, much better than the former mode. Orbital overlapping (3-day orbit solution with 1-day orbit overlap) tests show that the RMS of the orbit difference for the former mode is 0.16 m in the radial direction, 0.53 m in the along-track direction, 0.97 m in the cross-track direction and 1.12 m in the 3-dimension position and the RMS of the orbit difference for the latter mode is 0.36 m in the radial direction, 0.89 m in the along-track direction, 1.18 m in the cross-track direction and 1.52 m in the 3-dimension position, almost the same as the former mode. All the experiments indicate that a meter-level accuracy of orbit determination for geostationary satellite is achievable.     

太阳紫外辐射对星上光学膜层的影响

光学遥感是当前卫星遥感的重要手段, 而卫星温控和能源系统也广泛采 用光学膜层, 它们在空间环境条件下的性能对卫星应用任务的完成, 乃至卫星寿命、安全将起着非常重要的作用. 本文给出了太阳紫外辐射对星上光学膜层影响的主要机制, 分析了这一影响的主要规律和原子氧剥蚀、高能粒子和静电场的作用, 综述了太阳紫外辐射对星上光学系统表面膜层影响的测量结果, 最后提出了星上光学膜层污染防护中应重点关注的几个方面.      

高准确度惯性测量装置全温测试系统的校准

阐述了高准确度捷联惯性测量装置全温测试系统的校准测试方法。通过对软硬件进行校准测试,验证了该系统可以完成不同种类的惯性测量装置误差建模和综合测试。     

93k集成电路测试系统校准原理及实现方法研究

介绍了93k集成电路测试系统校准原理与实现方法,讨论了校准过程中的量值传递关系;以HPP-MU为例,给出了量值传递的实现过程,并分析了93k校准原理与方法在确保量值准确、一致性上的优点。     

基于GNSS的高轨卫星定位技术研究

利用全球卫星导航系统(GNSS)进行导航定位具有全球、全天候、实时和高精度的优点,应用于高地球轨道(HEO)卫星的定位,能够提供精确的轨道和姿态确定,并且可以克服目前主要利用地面测控系统对HEO卫星进行定位的设备复杂、投资高等缺点,使得自主导航成为可能.本文对利用GNSS的高轨卫星定位相关技术进行了研究,分析了单一GNSS系统和多个GNSS组合系统的卫星可见性、动态性和几何精度因子(GDOP).通过仿真分析表明,利用组合GNSS系统并通过提高GNSS接收机灵敏度的方法,可以解决GNSS进行HEO卫星定位的相关问题,并能保证HEO卫星定位精度的要求.      

航天光学相机地面测控设备通用化研究

文章提出了航天光学相机控制系统测试设备通用化研究的思路，制定了通用化方案，对各功能模块进行了通用化设计。     

Estimation of optical maturity parameter for lunar soil characterization using Moon Mineralogy Mapper (M3)

Prolonged exposure of the microscopic outer layer of the lunar surface to the space environment leads to the maturation of the surface. Maturation can be quantified and it may be expressed in terms of optical maturity (OMAT). Optical maturity estimations are very much helpful in the identification and mapping of the major minerals present on the lunar regolith. Estimation of the maturation and mineral mapping using remote sensing techniques are achieved, by coupling spectral reflectance of the lunar surface with an optimized origin. The present work estimates the optical maturity and Ferrous oxide content of the Goldschmidt and Schrodinger craters, through the recalibration of the classical method of Lucey et al. (2000a) with an origin of (0.08, 1.18) and Moon Mineralogy Mapper (M3) data. The overall recalibration results assure that the craters are highly matured.     

带摆镜的制冷型中波红外像方扫描光学系统设计

基本形式的像方扫描光学系统依然需要复杂的二维回转机构带动成像镜组做二维扫描,所以二维回转机构需要承担较大载荷。分析了基本形式的像方扫描光学系统形式,并在基本形式基础上加入摆镜,只通过二维摆镜的旋转达到扫描像面的目的,大大减小二维回转机构载荷,提高扫描速度,简化了系统结构,减小了系统体积。加入摆镜后的光学系统除具有基本形式像方扫描光学系统的性质外,还有了新的限制条件,对带摆镜的像方扫描光学系统进行了分析,提出了设计条件及设计方法,并设计出具有较大视场的像方扫描光学系统。     

多随机变量的桁架结构系统的可靠性分析及优化设计

针对桁架结构系统，采用随机有限元法（SFEM）计算结构系统的响应量，考虑内力重新分配，建立失效模式的安全余量方程，用验算点法计算失效模式安全余量的可靠性指标，用改进的分枝限界法，寻找主要失效模式，通过对主要失效模式方程线性化研究，计算失效模式安全余量之间的相关系数，寻找主要失效模式，通过对主要失效模式方程线性化研究，计算失效模式安全余量之间的相关系数，最后用PNET法计算出结构系统的失效概率，同时给出多随机变量的结构系统可靠度的敏度表达式，采用最佳矢量法，求解了大型桁架结构系统基于可靠性指标约束下的最小重量的优化设计问题，最后，给出了实际算例，计算结果表明；采用随机有限元法能更好地考虑结构系统的多个随机变量对系统可靠性产生的影响；所采用的可靠性分析方法和优化方法是有效的。     

Microstructure and Optical Characterization of Magnetron Sputtered NbN Thin Films

Some fundamental studies on the preparation, structure and optical properties of NbN films were carried out. NbN thin films were deposited by DC reactive magnetron sputtering at different N2 partial pressures and different substrate temperatures ranging from –50 ℃ to 600 ℃. X-ray diffraction analysis (XRD) and scanning electron microscopy (SEM) were employed to characterize their phase com- ponents, microstructures, grain sizes and surface morphology. Optical properties inclusive of refractive indexes, extinction coefficients and transmittance of the NbN films under different sputtering conditions were measured. With the increase in the N2 partial pressure, δ-NbN phase structure gets forming and the grain size and lattice constant of the cubic NbN increasing. The deposited NbN film has relatively high values of refractive index and extinction coefficient in the wavelength ranging from 240 nm to 830 nm. Substrate tem- perature exerts notable influences on the microstructure and optical transmittance of the NbN films. The grain sizes of the δ-NbN film remarkably increase with the rise of the substrate temperature, while the transmittance of the films with the same thickness decreases. Ultra-fine granular film with particle size of several nanometers forms when the substrate is cooled to –50 ℃, and a remarkable aug- mentation of transmittance could be noticed under so low a temperature.