一种深空天文测角导航中的星历误差抑制方法

以火星探测器为例，提出一种以星光角距/时间差分星光角距作为量测量的星历误差抑制方法，分析了火卫一星历误差对导航精度的影响，建立了火卫一时间差分星光角距的量测模型。通过将火星星光角距和火卫一星光角距相结合，发挥了两种量测的优势，实现了对火卫一星历误差的抑制。仿真结果表明，基于星光角距/时间差分星光角距天文导航方法的位置误差是传统基于星光角距天文导航方法的64%，是基于时间差分星光角距导航方法的58%。此外，还分析了导航恒星个数、火星敏感器精度、火卫一敏感器精度、星历误差大小和滤波周期对导航性能的影响。     

同时纠检错时某些线性分组码的不可检错误概率

研究同时纠错和检错时，线性分组码的不可检错误概率，证明了二元完备码及其扩展码是最佳纠检错码，而某些ＢＣＨ码不是最佳纠检错码。     

对称联系组合定标法检测CMM空间误差

分析了现有三坐标测量机误差检测方法，提出了对称联系组合定标法。详细论述了该方法的测量原理及其简练新颖的数学模型，并通过实验比对，验证了该方法的正确性和实用性。     

SOCIT4 collisional-breakup test data analysis: With shape and materials characterization

In this paper we revisit the 1995 Kaman database of the SOCIT4 fragment characteristics with added analysis of a subset of the cataloged fragments from the test. This database was compiled from the last of a series of four hypervelocity impact tests conducted under a U.S. Department of Defense program in 1991–1992. This test targeted a flight-ready, U.S. Transit navigation satellite, yielding collision fragments in the size regime of sub-millimeter through tens of centimeters. Results in this database were used in the 1998 NASA Standard Breakup Model to represent characteristic length (size) and area-to-mass distributions of fragments smaller than 10 cm.     

光子TOA与自转频率误差对Crab脉冲星脉冲TOA估计的影响

为量化分析Crab脉冲星X射线波段光子到达时间（TOA）测量误差和自转频率误差对脉冲TOA估计的影响，仿真生成了13 200组带有不同光子TOA测量误差的光子TOA数据。采用含有不同大小自转频率误差的Crab脉冲星星历，通过历元折叠建立积分脉冲轮廓，与标准脉冲轮廓作互相关运算获得各组仿真观测的脉冲TOA测量误差，进一步计算出各误差参数组的仿真观测脉冲TOA测量误差均方根（RMS）。仿真结果表明，为使Crab脉冲星脉冲TOA短期测量精度达到30 ~300 μs量级的要求，有效面积为6 000 cm2和30 cm2的探测器脉冲星自转频率误差均应小于3×10-6 Hz，30 cm2的探测器光子TOA的偶然误差同时应控制在500 μs以内。     

封闭圆柱形粉尘爆炸罐内扬尘诱导湍流特性的确定

采用热线风速仪和系综平均法测定和研究了封闭圆柱形粉尘爆炸罐内扬尘湍流的瞬态特性，并与球形爆炸容器内已测定的扬尘湍流瞬态特性进行了比较，对系综平均法用于扬尘湍流的测量误差与测量次数的关系进行了探讨。     

速率捷联惯导系统陀螺仪误差分段补偿技术研究

分析标度因数误差补偿的必要性和可行性,提出了对陀螺按照角速度 大小分段进行标定比例系数的方法,以补偿由于角速度变化而引起的陀螺标度 因数误差。通过计算机仿真验证了误差补偿方法的正确性,为实际应用提供了 理论依据。     

风洞流场实时全息研究中的误差分析

基于作者的实验及相关理论，着重分析了实时全息用于风洞流场显示研究可能出现的误差及检定、消除方法。实践表明，配以适当的光源和显示、记录系统，实时全息使全息干涉显示直接再现，现场可视、可调控，免除了实验的盲目性和大量的后续处理，便于灵活选用干涉项，在高速流场尤其是其它光学诊断方法举步维艰的强发光高温等离子体的瞬态及迅变过程的实时连续监测显示诊断研究中亦有一定的优势。现场实验过程中系统只要没有大的过阻尼型的范性移动，用于风洞实验是有效而可靠的。     

提高数字化设计钣金件精度的方法

针对数字化设计钣金件加工误差比较隐蔽的问题,分析了在建模过程中产生的误差以及可能采取的消除措施,分析了在数控测量中误差积累的问题。另外,分析了测量点云与零件表面最佳拟合后的结果,给出了关于误差评定新的判断准则。通过上述措施,可以减少零件加工误差,提高零件的合格率。     

Reducing variability in short term orbital lifetime prediction

Within the last year three major re-entries occurred. The satellites UARS, ROSAT and Phobos-Grunt entered Earth’s atmosphere with fragments reaching the surface. Due to a number of uncertainties in propagating an object’s trajectory the exact place and time of a satellite’s re-entry is hard to determine. Major influences when predicting the re-entry time are the changing precision of the available orbital data, the satellite’s ballistic coefficient, the activity of the sun which influences the Earth’s atmosphere and the underlying quality of the atmospheric model. In this paper a method is presented which can reduce the variability in short-term orbital lifetime prediction induced by fluctuating orbital data accuracies. A re-entry campaign is used as a reference for this purpose. For a window of a few weeks before the re-entry the position data of a synthetic object is disturbed considering different degrees of orbital data errors. As a result different predictions will exist for the generated position data of a given day. Using a regression algorithm on the available data an average position is obtained, which is then used for the orbital lifetime prediction. The effect of this measure is a more consistent prediction of the orbital lifetime. The paper concludes with the comparison of the generated re-entry windows in various test cases for the original and the averaged data.