基于熵与TOPSIS法的空中目标威胁判断

针对舰艇对空防御空中目标威胁判断指标属性权重与属性值均为区间数的情况,通过以各方案与理想方案偏差最小、与负理想方案偏差最大,以及权系数熵的最大化为优化目标,用拉格朗口乘子法给出模型的最优解,得到指标的权重值;基于区间数的4种不同的距离度量方式,建立基于TOPSIS法的威胁判断模型;通过实例对比在不同距离度量下的排序效果...     

AUSM+-up格式在无网格算法中的推广

将AUSM -up格式推广运用到了无网格算法中.在点云离散的基础上,运用曲面拟合和AUSM -up格式求得数值通量;采用四步龙格-库塔方法进行时间推进,并引入当地时间步长和残值光顺等加速收敛措施.为了验证本文方法的计算精度和鲁棒性,对NACA0012翼型跨声速流动、某三段翼型低速绕流、平行错位NACA0012双翼超声速、高超声速流动进行了数值模拟.     

基于POD曲线的预警机雷达检飞概率模型

针对预警机雷达检飞试验中距离取样间隔及检飞航线边界条件的确定问题,以保证发现概率(POD)曲线的覆盖率与精确性为目标,提出基于POD曲线的预警机雷达检飞概率模型.首先,根据POD曲线的覆盖率和精确性要求确定检飞试验拟合曲线所需的采样点数.然后,根据POD曲线的经验分布函数建立检飞试验中最小探测距离和最大探测距离的计算方法,并由此确定检飞航线上距离取样间隔的长度.最后,根据发现概率的统计特性得到距离取样间隔内采样点数以及航次数等试验参数,为雷达检飞试验设计与预警性能评定提供定量依据.      

Alternative transfer to the Earth–Moon Lagrangian points L4 and L5 using lunar gravity assist

Lagrangian points L4 and L5 lie at 60° ahead of and behind the Moon in its orbit with respect to the Earth. Each one of them is a third point of an equilateral triangle with the base of the line defined by those two bodies. These Lagrangian points are stable for the Earth–Moon mass ratio. As so, these Lagrangian points represent remarkable positions to host astronomical observatories or space stations. However, this same distance characteristic may be a challenge for periodic servicing mission. This paper studies elliptic trajectories from an Earth circular parking orbit to reach the Moon’s sphere of influence and apply a swing-by maneuver in order to re-direct the path of a spacecraft to a vicinity of the Lagrangian points L4 and L5. Once the geocentric transfer orbit and the initial impulsive thrust have been determined, the goal is to establish the angle at which the geocentric trajectory crosses the lunar sphere of influence in such a way that when the spacecraft leaves the Moon’s gravitational field, its trajectory and velocity with respect to the Earth change in order to the spacecraft arrives at L4 and L5. In this work, the planar Circular Restricted Three Body Problem approximation is used and in order to avoid solving a two boundary problem, the patched-conic approximation is considered.     

样本重复使用失效响应曲线分析结构可靠度方法

用基于样本重复使用失效响应曲线逼近法,为充分利用迭代过程中的样本点,提出了样本重复使用的思想,并由此发展出一种结构可靠度的计算方法.利用可靠度指标作为收敛条件,从迭代收敛后的所有样本点中选取靠近失效界线处的样本点构造失效曲线响应函数,最后通过蒙特卡洛抽样的方法计算可靠度.多个算例表明:该响应函数避免了对传统意义上的功能函数响应面的模拟,降低了模型维数,又由于适当地 引入了带交叉项、具有曲线旋转功能的响应函数,因此能够很好地逼近失效曲线,有效地提高可靠度计算精度.      

卫星多径信道下SOFDM插值估计算法的对比分析

在卫星多径衰落信道环境中传输正交频分复用信号时,工程上可以考虑采用以插值运算为核心的信道估计方法对接收信号进行信道估计。文章首先给出并研究了线性插值、三次样条插值和拉格朗日函数插值这三种插值估计算法的基本原理,然后对各种算法的计算复杂度、插值估计的均方误差以及系统的误比特率这三项性能指标进行了对比分析,最后通过综合评估总结出了＂在慢多径衰落信道环境下宜采用线性插值估计算法＂和＂在快多径衰落信道环境下宜采用三次样条插值估计算法或拉格朗日函数插值估计算法＂的结论。     

基于统计学方法的卫星在轨热变形快速分析

为使用在轨实测温度数据辅助完成成像载荷视轴指向的在轨标定,首次将应用于地统计学中的普通克里格法用于卫星在轨温度场的无偏估计,提出了一种基于统计学方法的在轨热变形快速分析方法。应用热试验过程中星上少量温度实测数据进行卫星温度场的无偏估计,并将温度计算结果赋值到有限元模型,进而完成了热变形分析。应用此种方法,相比通过热物理方法进行温度场分析,可将热变形分析的工期缩短数日,且载荷变形的分析结果与试验实测结果的误差在1′左右,可较准确地得到载荷视轴在热变形作用下的指向变化。文章可为卫星在轨热变形的快速分析提供参考。     

空间非合作目标的多视角点云配准算法研究

为了提高相邻视角间稀疏扫描点云数据配准的速度和精度,实现多视角点云精确配准,提出一种基于KD Tree点云均匀采样简化算法,并且对传统四点算法（4 PointsCongruentSetsAlgorithm,4PCS）中的阈值参数进行了统一,确定了各误差阈值参数和点云密度之间的关系,通过基于姿态校正的方法有效解决了对称视角点云引起的误配准问题。仿真结果表明,该方法能够快速、有效地实现卫星稀疏点云的配准。     

Autonomous navigation to quasi-periodic orbits near translunar libration points

Libration-point missions have been very useful and successful. Due to the unstable nat-ures of most of these orbits, the long-time stationkeeping demands frequent maneuvers and precise orbit determinat...     

Dynamic orbit propagation in a gravitational field of an inhomogeneous attractive body using the Lagrange coefficients

The analytical methods have nearly been replaced by the numerical methods due to their higher accuracy and accessibility of computation facilities. The semi-analytical Lagrange method of orbit propagation using f and g series is a competitive alternative to the numerical integration technique if the Lagrange coefficients are derived in a full gravitational field. In this paper, a generalization of the Lagrange method of orbit propagation is introduced. In other words, we introduce a complete form of the Lagrange coefficients in all force fields developed in the spherical harmonics for example full gravitational field of the Earth. The method is numerically compared with the numerical integration technique. In order to show the numerical performance of the method, it has been implemented for orbit propagation of a GPS-like MEO and CHAMP-like LEO satellites. Discrepancy at centimeter level for CHAMP-like and sub-millimeter accuracy for GPS-like satellites shows relatively high performance of the developed algorithm. Compared to integration method, the proposed Lagrange method is nearly faster by a factor two for small Nmax and four for large Nmax.