局部凸空间中的压缩映射

本文将压缩映射原理推广到Ｈａｕｓｄｏｒｆｆ局部凸空间,证明了几个不动点定理。     

多台系统Weibull过程的Bayes统计推断方法

本文的目的是要给出多台系统Weibull过程的Bayes推断方法。获得了尺度参数、形状参数以及系统能达到的MTBF的Bayes点估计和区间估计。某些估计只涉及到一重数值积分。最后,用一个实例说明这些方法。     

三坐标测量机在我公司的应用

介绍了三坐标测量机的组成、测量原理主在我公司军品和民品生产中的应用，并将三坐测量机与其他测量仪器作了比较。     

The management of stray radiation issues in space optical systems

The performance of infrared and submillimeter systems can be severely degraded by stray light. Stray light includes off-axis radiation, system diffraction and scattering effects, and thermal self-emission. The purpose of this paper is to identify several keys to preventing system degradation due to stray radiation. The first key is to apply stray light design rules and analysis techniques early in the program before the design is finalized. A systems level analysis using stray light analysis software is often necessary in order to identify more subtle problems and to assess the magnitude of their effect on system performance. Another key is to address contamination control and the choice of surface coatings early in the program. The management of stray radiation issues is extremely cost-effective, if begun early in the program, and can reduce later schedule hardships.     

数字滤波器在定点DSP上的实现

介绍 FIR(Finite Impulse Response)和 IIR(Infinite Impulse Response)数字滤波器的网络结构及其在定点 DSP(Digital Signal Processing)上的实现方法 ,同时对定点 DSP软件设计中的关键问题——定标作了详细的阐述 ,并以二阶 IIR滤波器为例介绍定标的方法     

卫星全景图象的数字几何校正

文中提出了一种对卫星全景图象进行整幅几何粗处理的方法。该方法基于卫片和地面上一些固有的几何关系,既考虑卫星成像的物理过程,又不单纯依赖卫星参数,而是借助于精确测定的少量地标点和几何关系模型,对参数进行最优估计,最终达到对图象的校正。经仿真表明,文中所提出的方法是完全有效的。     

基于航天TDICCD相机像移分析的PSF估计及图像复原算法研究

根据时间延迟积分电荷耦合器件(TDICCD)特殊的工作原理,分析了其产生像移的原因 ,基于对TDICCD像移的分析估计出模糊图像的点扩散函数(PSF)。根据TDICCD像移产生的机 理,建立了图像退化的数学模型,并在功率谱均衡复原算法的基础之上提出了像移复原滤波的 数学表达式,对运动模糊图像进行了半盲恢复,通过Matlab仿真证明了图像复原算法的可行 性和有效性。
     

Analysis of the solar sail deformation based on the point cloud method

The deformation of the solar-sail membrane is an important factor for causing inaccuracies in the solar-sail missions. This paper describes the solar sail under deformation by using a new modelling technique based on point cloud and triangular mesh generation. Two types of deformation, stemming from wrinkling and billowing, are modelled. The changes in the solar radiation pressure force and the moment caused by deformation are calculated and compared to the ideal non-deformed case. The heliocentric spiral trajectory and the orbital angular momentum reversal trajectory are taken as examples to quantify the influence of the deformation from an orbit point of view. Additionally, point cloud simplification, based on the normal vector and bounding box, is utilized to simplify the original deformed-sail model. It involves a reasonable reduction and renewal of the points in the model considering the variation of surface curvature. The simplification and its modelling accuracy are numerically investigated as well as computational efficiency.     

The realization and convergence analysis of combined PPP based on raw observation

In order to speed up Precise Point Positioning (PPP)’s convergence, a combined PPP method with GPS and GLONASS which is based on using raw observations is proposed, and the positioning results and convergence time have been compared with that of single system. The ionospheric delays and receiver’s Differential Code Bias (DCB) corrections are estimated as unknown parameters in this method. The numerical results show that the combined PPP has not caused significant impacts on the final solutions, but it greatly improved Position Dilution of Precision (PDOP) and convergence speed and enhanced the reliability of the solution. Meanwhile, the convergence speed is greatly influenced by the receiver’s DCB, positioning results in horizontal which are better than 10 cm can be realized within 10 min. In addition, the ionosphere and DCB products can be provided with high precision.     

Studies on the imaging characteristics of Yohkoh Soft X-ray Telescope: Optical aberration and scattering

In order to better understand the characteristics of Yohkoh Soft X-ray Telescope (SXT) mirror, we have analyzed the in-flight overexposed image (the starburst image) obtained during the solar flare observation. It has been revealed from our study that the intensity distribution inside the shadows shown in the scattering difference image contains little of the scattered component of the PSF and matches almost correctly the extension of the PSF core profile. Also it is found that the scattering wing of the SXT PSF is connected smoothly to the PSF core within the distance of about 100–200 arcsec from the peak. With numerical simulations we have shown that an increase in energy affects not only the level of scattering wing, but also both the shape and the absolute level of the PSF core. The results have revealed, however, that the energy dependence for the SXT PSF cannot be easily estimated with the data obtained from one filter alone, which implies that the data analysis using multiple filters will enable us to determine the absolute amount of scattered component as well as the energy dependence of the SXT PSF. Details on the analysis of starburst image and the results from numerical simulations will be introduced and discussed thoroughly.