A Procedure for Directly Calculating CEP in DF Fixing

The cumulative probability for a circular error probability (CEP) radius can be developed as a power series which converges efficiently for cases of practical interest and is suitable for numerical solution with simple iteration methods. The procedure can be applied with equal facility to circles of arbitrary probability level.     

导弹作战使用命中精度CEP评定方法研究

针对导弹命中精度评定方法的不足,提出了导弹射击的CEP评定方法,构造了使用固定母体统计量,通过对不同射程下误差的计算与合成,得到了不同射程下的作战使用CEP评定模型.该项研究对减少导弹武器研制定型中的试验子样、提高作战使用能力具有指导意义.     

Error Measures for Normal Random Variables

Four commonly used measures of error are the root mean square error (RMSE), the geometric mean error (GME), the mean radial error (MRE), and the circular or spherical error probable (CEP, SEP). Exact or approximate closed form expressions are given. for each for zero mean, normal random variables in two and three dimensions. Numerical comparison of the measures suggests the relationship GME ? SEP(CEP) < MRE ? RMSE.     

Gravity modeling in aerospace applications

The science of inertial navigation has evolved to the point that the traditional gravity model is a principal error source in advanced, precise systems. Specifically, the unmodeled vertical deflections of the earth's gravitational field are a major contributor to CEP (circular error probable) divergence in precise terrestrial inertial navigation systems (INS). Over the years, several studies have been undertaken to the development of advanced techniques for accurate, real-time compensation of gravity disturbance vectors. More complex on-board gravity models which compute vertical deflection components will reduce the CEP divergence rate, but imperfect modeling due to on-board processing limitations will still cause residual vertical deflection errors. In order to eliminate or reduce gravity-induced errors in the INS requires measurement of gravity disturbance values and in-flight compensation to the inertial navigator. It is assumed in this paper that gravity disturbance values have been measured prior to the airborne mission and various techniques for compensation are to be considered. As part of a screening process in this study, several gravity compensation techniques (both deterministic and stochastic models) were investigated. The screening process involved identification of gravity models and algorithms, and developments of selection criteria for subsequent screening of the candidates.     

高稳定高可靠多平台兼容RTK 精密定位系统设计与实现

针对RTK精密定位系统存在的稳定性差、可靠性低、系统兼容能力低等问题，提出了高稳定高可靠多平台兼容RTK精密定位系统设计方法。该系统基于冗余式方法设计GNSS定位单元，以提高系统兼容性；基于工作距离设计冗余式修正信息交互方式，并设计了基于ARM+DSP架构的AM5728实时解算RTK修正信息，通过复合型高速通信链路共享信息。以精密标定点为参考测试其定位精度并采用CEP评估其定位精准性，评估结果表明，CEP=0.0071m，说明定位精度高且可靠性好，解决了稳定性差、可靠性低、系统兼容能力低的问题，有效弥补了RTK精密定位系统领域受限的不足。     

高稳定高可靠多平台兼容RTK精密定位系统设计与实现

针对RTK精密定位系统存在的稳定性差、可靠性低、系统兼容能力低等问题,提出了高稳定高可靠多平台兼容RTK精密定位系统设计方法。该系统基于冗余式方法设计GNSS定位单元,以提高系统兼容性;基于工作距离设计冗余式修正信息交互方式,并设计了基于ARM+DSP架构的AM5728实时解算RTK修正信息,通过复合型高速通信链路共享信息。以精密标定点为参考测试其定位精度并采用CEP评估其定位精准性,评估结果表明,CEP=0.0071m,说明定位精度高且可靠性好,解决了稳定性差、可靠性低、系统兼容能力低的问题,有效弥补了RTK精密定位系统领域受限的不足。     

确定时间序列协方差函数的方法

提出一种确定时间序列协方差函数的方法,它首先根据(多元)时间序列构造其互协方差函数随机序列、互相关函数随机序列或自协方差函数随机序列、自相关函数随机序列,然后采用谱分析和多点平均方法对互协方差函数随机序列、互相关函数随机序列或自协方差函数随机序列、自相关函数随机序列的趋势项进行分离,分别求得其周期项和非周期项的函数表达式,再综合给出整个趋势项函数。从而得到原时间序列的互协方差函数、互相关函数或自协方差函数、自相关函数的函数形式,并通过最小二乘方法确定其中的待定参数。该方法可用于时间序列协方差函数的建模、分析和预测,并且计算简单易行、精度高,便于实际应用。      

提高瞄准棱镜安装精度稳定性

平台瞄准棱镜组件是平台方位光学瞄准的基准, 用于全箭初始对准, 其安 装精度的稳定性会直接影响火箭的落点精度。分析了影响瞄准棱镜安装精度稳定性的几 种原因,找到其关键因素,并针对影响精度稳定性的关键因素提出了改进设计的方法, 并进一步通过试验验证,证实了设计改进的正确性。     

On Truncation Error Bounds for Sampling Representations of Band-Limited Signals

All sampling representations of band-limited signals involve infinite sums. The truncation error associated with a given representation is defined as the difference between the signal and an approximating sum utilizing a finite number of terms. In this paper truncation error is expressed as a contour integral for Lagrange interpolation, general Hermite interpolation, the Shannon series (cardinal series), the Fogel derivative series, and multidimensional sampling expansions. Truncation error bounds are obtained under various constraints on the signal magnitude, spectral smoothness, and energy content.     

亚音速升力面理论的一种新解法

本文提供了亚音速升力面理论的一种新解法,可求解亚音速流中有限翼展机翼的载荷分布。计算中采用传统的弦向级数和展向分条。证明了Mangler二重奇异积分可交换积分次序,从而使积分可解析地求出。对弦向积分的被积函数作多项式分段逼近,可使核函数的表达式成为封闭形式的有限和,导致性态很好的系数矩阵。计算结果与实验及其它方法的结果作了比较,并给出了计算效率。     

尖端具有非线性吸附接触的界面裂纹的动态特性研究

 研究一类尖端具有非线性吸附接触型裂纹模型的弹性波散射问题。利用积分变换和积分方程方法推导了确定这类问题基本变量的奇异积分方程组,采用围道积分技术和切比雪夫多项式展开技术得到了待定系数的非线性代数方程组。最后给出了裂纹尖端接触区的大小和接触应力的数值结果,揭示了这种接触型裂纹模型的动力学特征及物理上的合理性。     

三元流闭式叶轮组合电加工技术研究Ⅲ——数控电火花精加工关键技术

 数控电火花（NC-EDM）精加工,是三元流闭式叶轮组合电加工的最终加工工序,是决定三元流闭式叶轮整体制造精度的关键工序。本文专题介绍了其主要关键技术,包括工具电极、运动轨迹以及工装夹具设计。基于关键技术的解决,进行了某型三元流闭式叶轮组合电加工工艺试验,试制加工了合格零件。研究结果表明,数控电解(NC-ECM)预加工可充分发挥电解加工高效率的特点,而数控电火花精加工又可保证对复杂整体构件加工需要万无一失的高可靠性和高精度的要求。两者结合,可以实现高效、精密、可靠、整体制造三元流闭式叶轮的目标。     

含孔边裂纹有限大板的解析变分解法

 本文利用复变函数方法导出了含孔边单侧裂纹有限大板应力与位移的全场表达式,满足所有基本方程、裂纹表面边界条件与复连通域位移单值条件。应用变分原理满足其余的边界条件并由此求解应力强度因子与应力集中系数。在变分方程中,只存在线积分,没有面积分。故本方法收敛迅速、节省机时。     

时间推进积分方程法求解非定常跨声速流动

本文提出了一种求解非定常跨声速流动的新方法——时间推进积分方程法,此法克服了时间线化积分方程法的限制,能较好地模拟激波的运动。本文首先用一维波(?)问题——模型问题阐明此法的基本思想,然后将它应用于二维非定常跨声速流动中。本文还首次引入拟速度位的概念,使时间推进积分方程式得到简化,尾涡条件和Kutta条件更易处理。数值计算表明时间推进积分方程法是合理可靠的。     

空面导弹命中精度最优测试评定方法

空面导弹命中精度试验结果评定方法对空面导弹的研制和使用具有显著的影响.在给定圆概率偏差的条件下,根据导弹飞行试验的数据、研制方风险、使用方风险、评定分辨率等参数,确定评定方案,给出在不考虑系统偏差时的落点检验域的划定方法以及导弹是否满足战术技术要求等评定指标.仿真实例以某一具体型号为例,验证了该方法的有效性.该方法可用于空面导弹的精度评估中.     

无扩口管路连接件疲劳寿命预估的损伤力学-有限元法

 以损伤热力学为基础,构建分式形式的损伤演化方程。针对管路连接件等轴对称形式的构件,引入等效应力和等效应变。根据损伤力学守恒积分原理,得到恒幅重复载荷下应力与寿命关系的级数表达式,根据标准件疲劳试验结果拟合得到损伤演化方程中的材质参数。利用APDL语言编程对ANSYS软件进行了开发,使得借助ANSYS软件的损伤力学-有限元数值解法成为可能。利用该方法预估了TC6钛合金标准件疲劳裂纹萌生寿命,其结果与试验数据吻合。进一步,预估了管路连接件裂纹萌生寿命,预测了裂纹扩展路径并预估了疲劳裂纹扩展寿命。本文为采用损伤力学方法来预估构件的疲劳寿命提供了一种可行的方法。     

三维粘弹性大变形动力响应分析

将大变形增量问题的Ｔｏｔａｌ Ｌａｇｒａｎｇｉａｎ法应用于粘弹性结构的动力响应分析，利用Ｐｒｏｎｇ级数导的Ｋｉｒｃｈｈｏｆｆ应力和Ｇｒｅｅｎ应变表示的粘弹性积分型增量本构方程及其递推公式，从而给出一种计算三维粘弹性大变形动力响应的有限元增量迭加方法，经算例验证，所述方法及其相应程序具有机器内存少、计算量小和效率高的优点。     

反舰导弹命中精度评估方法

研究了基于Bayes方法的反舰导弹命中精度评估方法,提出了导弹命中点系统误差评估方法、Bayes检验方案和CEP评估方法。     

亚音速升力面气动敏感性导数计算

具有任意曲线前缘的亚音速升力面的气动敏感性导数由核函数法给出。用自适应积分法计算弦向积分,用Multhopp法结合抽去奇点,计算Mangler积分主值。将积分核展成Chebyshef多项式的渐近展开式以保证结果的收敛性。最后将广义力系数及其敏感性导数表示成简单形式,对椭圆、矩形和后掠机翼作了计算,所得结果在升力面理论精度范围内与直接由核函数法得到的结果一致;而且所得到的偏导数可在飞机设计中分析综合用于多学科优化。     

The Cusp as a Source of Magnetospheric Energetic Particles, Currents, and Electric Fields: A New Paradigm

Energetic particle instrumentation on the Polar satellite has discovered that significant fluxes of energetic particles are continuously present in the region of the dayside magnetosphere where they cannot be stably trapped. This region is associated with either open magnetic field lines or a magnetic topology associated with pseudo-trapping. Two distinct features [Time-Energy Dispersion (TED) signatures and Cusp Energetic Particle (CEP) events] are observed in these energetic particle fluxes that strongly suggest a local acceleration of mostly shocked solar wind particles. As the solar wind particles ram themselves into the cusp geometry, they form diamagnetic cavities with strong turbulence that are capable of accelerating particles to energies of 100s and 1000s of kiloelectronvolts. This process forms a layer of energetic particles on the magnetopause as well as permits such particles to enter via drift the equatorial nightside magnetosphere to distances as close as six Earth radii under the influence of gradient and curvature effects in the local magnetic field. The fluxes of these particles have all of the properties associated with the ring current and can supply the magnitude of the cross tail current required. ISEE-1 energetic particle data and their pitch angle distributions [PAD] are examined at the magnetic equatorial plane on the night side to investigate and possibly validate the insights gains from the Polar data and energetic particle trajectory tracing in a realistic magnetic field. The existence and properties of butterfly-type PADs strongly supports the concept of a dayside high latitude source of energetic particle fluxes. Because the CEP process is impulsive and time variable the charge separation produced by the drifting electrons (eastward) and ions (westward) on the magnetospheric nightside may be responsible for the cross tail electric field that has been ascribed to the reconnection/convection process.