基于CAD二次开发的飞行器隐身性能计算方法

在飞行器同雷达对抗时的不同威胁情况下,分析了在雷达仰视照射下飞行器的隐身性能。通过绘制雷达仰角图,得到了目标飞行器在某典型雷达照射下的暴露与隐身区域,从而量化了目标飞行器的隐身性能。通过CATIA二次开发技术实现了CAD模型的便捷修改,为优化外形隐身特性提供支持。最后通过一个具体算例验证种方法的效果,并说明方法具有实用意义。     

混合动网格方法研究

基于Delaunay图映射的动网格方法是一种快速、鲁棒的新型方法,其具有无需迭代、效率高、适用于任意拓扑结构的网格等特点。在分析影响Delaunay图映射方法变形能力主要因素的基础上,对Delaunay图映射方法进行了改进,通过在Delaunay图中增加辅助点,并结合弹簧原理动网格方法,消除了Delaunay图在大变形时出现交叉的问题。通过三维翼身组合体大变形算例验证了发展的混合动网格方法的可靠性和处理气弹问题时的计算效率。     

动态拖尾星图模拟算法研究

星图模拟技术是星图识别算法仿真和性能测试的基础.为了更好地模拟星敏感器在轨工作的情况,对星敏感器的软件开发以及自身性能进行有效的地面测试,提出一种动态拖尾星图模拟算法.该算法分为4个步骤:首先根据星敏感器指向在全天球范围内搜索导航星;接着利用小孔成像模型计算导航星在星敏感器成像面的投影位置;然后在考虑卫星运动引起的恒星拖尾的基础上,按照二维灰度分布规律置灰度值来模拟星像点像素;最后叠加杂散光背景及成像器件引起的噪声.提出的算法具有速度快、精度高及可实现性高等优点.     

一种空间非合作目标的稀疏点云配准算法

点云数据配准是三维重构的关键技术之一,为了提高空间非合作目标的稀疏扫描点云数据配准的速度和精度,提出一种改进的基于四点算法的全局配准算法进行初始配准,再使用迭代最近点算法精确配准.针对直接扫描所得到点云数据量大的问题,本文提出一种基于KD Tree点云均匀采样简化算法,并且对传统基于四点算法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.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,改进的四点算法配准耗时仅为几何哈希算法的42.49%.     

一种适合于旋翼前飞非定常流场计算的新型运动嵌套网格方法

针对旋翼流场计算中关键的运动嵌套网格技术,提出了一个新的网格单元关系快速判断方法。该方法通过计算特殊网格点在背景网格上的位置来建立桨叶网格在背景网格中所占据范围的关系,并用于嵌套网格洞单元的识别,又进一步将该方法推广用于Inverse Map的建立,在此基础上,建立了一套用于前飞流场计算的运动嵌套方法。通过多种前飞旋翼测试算例,分别评估了背景网格、桨叶网格尺寸改变对计算时间的影响,同时验证了该方法的可靠性,结果表明构建网格嵌套关系所用时间随桨叶网格和背景网格尺寸的变化幅度较小,且具有良好的鲁棒性,能够满足旋翼前飞状态计算的需要。最后,在基于前飞非定常N-S/Euler流场求解器中,采用该方法模拟了UH-60A和7A旋翼悬停/前飞状态的气动特性,通过计算时间的对比体现出该方法的高效性,并且流场计算结果与试验数据对比表明该方法可以有效地用于旋翼前飞非定常流场的计算。     

Image Smearing Modeling and Verification for Strapdown Star Sensor

To further extend study on celestial attitude determination with strapdown star sensor from static into dynamic field, one prerequisite is to generate precise dynamic simulating star maps. First a neat analytical solution of the smearing trajectory caused by spacecraft attitude maneuver is deduced successfully, whose parameters cover the geometric size of optics, three-axis angular velocities and CCD integral time. Then for the first time the mathematical law and method are discovered about how to synthesize the two formulae of smearing trajectory and the static Gaussian distribution function (GDF) model, the key of which is a line integral with regard to the static GDF attenuated by a factor 1/ L s (L s is the arc length of the smearing trajectory) along the smearing trajectory. The dynamic smearing model is then obtained, also in an analytical form. After that, three sets of typical simulating maps and data are simulated from this dynamic model manifesting the expected smearing effects, also compatible with the linear model as its special case of no boresight rotation. Finally, model validity tests on a rate turntable are carried out, which results in a mean correlation coefficient 0.920 0 between the camera images and the corresponding model simulated ones with the same parameters. The sufficient similarity verifies the validity of the dynamic smearing model. This model, after parameter calibration, can serve as a front-end loop of the ground semi-physical simulation system for celestial attitude determination with strapdown star sensor.     

Asymptotic Performance of Sparse Signal Detection Using Convex Programming Method

The detection of sparse signals against background noise is considered. Detecting signals of such kind is difficult since only a small portion of the signal carries information. Prior knowledge is usually assumed to ease detection. In this paper, we consider the general unknown and arbitrary sparse signal detection problem when no prior knowledge is available. Under a Neyman-Pearson hypothesis-testing framework, a new detection scheme is proposed by combining a generalized likelihood ratio test (GLRT)-like test statistic and convex programming methods which directly exploit sparsity in an underdetermined system of linear equations. We characterize large sample behavior of the proposed method by analyzing its asymptotic performance. Specifically, we give the condition for the Chernoff-consistent detection which shows that the proposed method is very sensitive to the 2 norm energy of the sparse signals. Both the false alarm rate and the miss rate tend to zero at vanishing signal-to-noise ratio (SNR), as long as the signal energy grows at least logarithmically with the problem dimension. Next we give a large deviation analysis to characterize the error exponent for the Neyman-Pearson detection. We derive the oracle error exponent assuming signal knowledge. Then we explicitly derive the error exponent of the proposed scheme and compare it with the oracle exponent. We complement our study with numerical experiments, showing that the proposed method performs in the vicinity of the likelihood ratio test (LRT) method in the finite sample scenario and the error probability degrades exponentially with the number of observations.     

B93铝合金热加工特性模拟研究

在Gleeble1500热模拟机上采用轴对称等温压缩实验,研究了B93铝合金在热加工中变形温度和应变速率对合金组织的影响,基于动态模型计算出B93铝合金加工图,分析合金热加工的流变失稳区并确定了合金热加工的最佳工艺参数。结果表明:变形速率和变形温度对B93铝合金的微观组织有影响;合金的峰值应力随变形温度的升高而降低,随变形速率的提高而增大;B93铝合金最佳的热加工制度为:变形温度420℃左右,应变速率0.001 s-1。     

一种基于三正交主轴平面的快速星图模拟方法

为在地面上进行星图模拟以测试星图识别算法和星敏感器性能, 提出了一种新的快速星图模拟方法. 该方法利用截面圆和固定区域的性质, 将单位天球按照三个正交主轴平面进行等分, 根据赤纬值求解恒星矢量与主轴平面夹角来确定选星条件, 进而根据坐标变换原理进行星图模拟. 为验证所提方法与现有方法相比的优势, 进行了大量的仿真实验. 实验结果表明, 与现有星图模拟方法相比, 本文方法在保证星图模拟精度的条件下, 选星速度提高了3倍以上.      

地磁图制备方法及其有效性评估

高精度地磁图制备是地磁匹配导航关键技术之一.在简单介绍4种网格插值方法原理的基础上(反距离加权插值法、克里金插值法、改进的谢别德插值法以及径向基函数法),应用实测地磁数据,选取测点分布较均匀区域,根据上述插值方法分别制备地磁图,并通过交叉验证统计准则对地磁图制备方法的有效性进行评估.结果表明,径向基函数插值法制备的地磁图"鸭蛋"形分布较少,地磁图等值线较圆滑,其标准偏差远小于其它方法的标准偏差,且其标准误差以及平均偏差也最小,具有较高的插值精度,能更好地反映该区域地磁场分布情况.