一种基于主星的导航星座构造方法

提出了一种基于主星的导航星座构造方法,利用不等式约束下多变量函数最优化问题的求解方法实现了导航主星的选取和导航星座的构造。实验表明,采用该方法构造的导航星座数据库,既不会造成导航星的丢失,又显著地减少了需要存储的识别基元的数量,从而有效地降低了导航星座数据库的存储容量。     

惯性敏感器与星敏感器之间在轨自主标定比较研究

惯性敏感器与星敏感器组合定姿是航天器高精度姿态确定的常用手段。通常将惯性敏感器的常值漂移作为扩展状态进行标定,而将星敏感器的常值偏差作为扩展状态进行估计也是可能的。本文对这两种方法的定姿精度进行了分析比较,给出了选用的准则。     

浇注温度对K4169高温合金晶粒组织影响的计算机模拟

利用Fortran语言编程,采用有限差分法分别解用热焓法处理结晶潜热的圆柱坐标系一维不稳定热传导方程,模拟了K4169高温合金圆柱锭某一横截面凝固过程中温度的变化,它正确地反映了在不同铸造工艺条件下合金铸件横截面上温度的变化规律。通过固相分数,将合金铸件凝固温度场模拟及其连续形核模型、枝晶尖端生长的动力学模型相耦合,计算了不同浇注温度下K4169高温合金圆柱锭凝固过程中晶粒组织的特征值,包括晶粒密度和平均晶粒尺寸,并参考二维CellularAutomaton方法,实现了在计算机屏幕上晶粒形成的动态显示,模拟结果和实验结果吻合较好。     

A robust star identification algorithm with star shortlisting

A star tracker provides the most accurate attitude solution in terms of arc seconds compared to the other existing attitude sensors. When no prior attitude information is available, it operates in “Lost-In-Space (LIS)” mode. Star pattern recognition, also known as star identification algorithm, forms the most crucial part of a star tracker in the LIS mode. Recognition reliability and speed are the two most important parameters of a star pattern recognition technique. In this paper, a novel star identification algorithm with star ID shortlisting is proposed. Firstly, the star IDs are shortlisted based on worst-case patch mismatch, and later stars are identified in the image by an initial match confirmed with a running sequential angular match technique. The proposed idea is tested on 16,200 simulated star images having magnitude uncertainty, noise stars, positional deviation, and varying size of the field of view. The proposed idea is also benchmarked with the state-of-the-art star pattern recognition techniques. Finally, the real-time performance of the proposed technique is tested on the 3104 real star images captured by a star tracker SST-20S currently mounted on a satellite. The proposed technique can achieve an identification accuracy of 98% and takes only 8.2?ms for identification on real images. Simulation and real-time results depict that the proposed technique is highly robust and achieves a high speed of identification suitable for actual space applications.     

热输入对AZ31镁合金FSP试样力学性能的影响

分别利用普通钢制垫板和自制的带有冷水通道的铜制垫板,对AZ31镁合金进行了搅拌摩擦加工。利用光学显微镜(OM)、SEM、显微硬度仪和拉伸设备,研究了被加工件厚度、搅拌头焊接速率和冷却条件对试样搅拌区力学性能的影响。研究表明:试样搅拌区从上层至中层和底层,再结晶晶粒尺寸依次减小。通过减小被加工件厚度、增大搅拌头焊接速率和加快冷却速率等方法,抑制了试样搅拌区晶粒长大。在搅拌头转速和焊接速率分别为800r/min和90mm/min的条件下,得到的搅拌区底部平均晶粒尺寸约为450nm,该区域显微硬度为96HV,与普通钢制垫板制备的试样相比,硬度提高了24HV,其屈服强度、抗拉强度和伸长率分别提高为原材料的1.27倍、1.6倍和2.2倍。     

Systematic centroid error compensation for the simple Gaussian PSF in an electronic star map simulator

Simulated star maps serve as convenient inputs for the test of a star sensor, whose standardability mostly depends on the centroid precision of the simulated star image, so it is necessary to accomplish systematic error compensation for the simple Gaussian PSF（or SPSF, in which PSF denotes point spread function）. Firstly, the error mechanism of the SPSF is described, the reason of centroid deviations of the simulated star images based on SPSF lies in the unreasonable sampling positions（the centers of the covered pixels） of the Gaussian probability density function. Then in reference to the IPSF simulated star image spots regarded as ideal ones, and by means of normalization and numerical fitting, the pixel center offset function expressions are got, so the systematic centroid error compensation can be executed simply by substituting the pixel central position with the offset position in the SPSF. Finally, the centroid precision tests are conducted for the three big error cases of Gaussian radius r = 0.5, 0.6, 0.671 pixel, and the centroid accuracy with the compensated SPSF（when r = 0.5） is improved to 2.83 times that of the primitive SPSF, reaching a 0.008 pixel error, an equivalent level of the IPSF. Besides its simplicity, the compensated SPSF further increases both the shape similarity and the centroid precision of simulated star images, which helps to improve the image quality and the standardability of the outputs of an electronic star map simulator（ESS）.     

考虑卫星轨道运动和像移影响的星敏感器星图模拟方法

星图模拟技术是星图识别算法和星敏感器性能测试的基础.提出一种新的高精度星图模拟方法.该方法分为三个步骤:首先,利用两行轨道数据(TLE,Two-Line Orbital Element)与简化常规/深空扰动的近似解模型(SGP4/SDP4)计算出卫星在轨运行参数,进而获得卫星姿态矩阵;然后,根据星敏感器的方位和俯仰角度,确定星敏感器视场中的导航星及星敏感器安装矩阵,利用小孔成像模型,获得导航星在星敏感器成像面的投影位置;最后,为更准确模拟实际星像点的灰度扩散,在考虑卫星运动引起的恒星像移的基础上,按照二维高斯分布规律置灰度值来模拟星像点像素.在此基础上,还详细分析了不同曝光时间下,恒星像移对恒星位置测量的影响.     

等通道转角挤压工艺制备超细化合金的研究与进展

等通道转角挤压技术（简称ECAP）是制备超细晶粒金属块材的最新研究领域之一。本文阐述了ECAP的研究目的与意义。说明了ECAP的原理，探讨了ECAP的国内外研究现状及进展，指出了ECAP急待解决的五大问题，具有较好的实用价值。     

LY12铝合金型材粗晶对性能的影响

介绍了LY12铝合金型材低倍粗晶及细晶状态下的性能对比试验情况 ,并得出了试验结论 ,为今后对呈现低倍组织粗晶的LY12或其他类似的铝合金型材审理使用提供了技术依据     

药柱通用坐标计算法计算结果跳动的原因分析及解决途径

对药柱通用坐标计算法计算结果跳动的原因进行了分析,提出了解决途径和方法,并对提高计算准确度的问题也进行了讨论。经实例计算证明解决途径和方法是有效的,与解析法计算结果比较误差不大于0.85％。