一种基于小波技术的GPS/SINS组合导航技术及试验

GPS／SINS的组合被认为是比较理想的导航系统,是目前导航技术发展的主要方向。为了进一步提高GPS／SINS组合导航系统的精度,文章在介绍了小波去噪原理的基础上,提出了一种基于小波技术的GPS／SINS组合导航系统新方法,并通过实际的静态试验给予验证。试验结果表明,采用该方法以后,组合导航系统的各项导航参数精度得到了非常明显的提高。     

基于对偶原理的二子样划船补偿算法

划船补偿算法一般以典型划船运动为基础,利用最优化理论来进行推导.圆锥补偿算法不仅可利用最优化理论,还可利用Goodman-Robinson理论进行推导.利用对偶原理,将Goodman-Robinson理论下得到的二子样修正圆锥补偿算法推广至划船补偿算法设计中,得到一种改进的二子样划船补偿算法.在典型划船运动条件下,对得到的划船补偿算法进行了数字仿真,并与二子样优化划船补偿算法进行了对比研究.仿真结果表明,此改进二子样划船补偿算法能提高速度更新精度.     

基于投影寻踪的高光谱图像异常检测并行算法

投影寻踪方法能有效提取数据中的非高斯结构凸显异常信息,但在求解最优投影方向时存在计算量大、运行时间长的问题,为提高处理效率,提出一种机群环境下的并行算法.选用偏度和峰度组合作为投影指标,将所有像素光谱作为特定投影方向集依次搜索,求解最优投影方向.在并行计算各候选方向投影指标时,分割图像数据分布存储于各机群结点,数据子块朝候选方向并行投影后,将指标计算式变形分解,使各结点在指标计算过程中所需数据均为本地数据,解决数据局部性问题,并采用一种"轮流作主"的机制提高算法负载均衡程度.利用实用型模块化高光谱仪数据在机群系统上进行测试,达到了较好的加速效果,表明该并行算法具有良好的并行性能.     

结构光三维视觉检测中光条图像处理方法研究

在结构光视觉检测系统中,光条中心的提取精度直接影响到整个测量系统的测量精度.光条图像的处理是其中重要的一步,尤其是受到严重噪声干扰的图像.探讨了被多种噪声干扰的光条图像的处理和精确提取光条中心的方法.给出了一种消除环境干扰的滤波模板并实验验证了其滤波效果.使用这些光条图像处理方法使整个测量系统在200mm×200mm的测量范围内测量精度达到0.083mm.      

基于FGN输入流的G/D/1排队模拟

传统的排队理论不适于分析高速网络表现出的自相似流量.通过实验仿真,主要考察平均等待时间和在队列分别为无限和有限情形下的队列尾部特征等参数,并对以FGN为输入流的G/D/1排队模型作了定性分析.结果表明在输入流的强度和方差基本相等且系统利用律大于某一阈值的情况下,队列平均等待时间随Hurst参数增大而显著增长.同时指出在相同的条件下考察队列尾部特征,具有有限队列长度的G/D/1排队模拟结果要远优于无限队列长度下的理论分析结果.      

前后翼型装药结构SRM气固两相流动特性

基于可压缩流动强守恒型Navier-Stokes方程,运用颗粒轨道模型(PTM)和shear stress transfer(SST)k-ω湍流模型,采用计算单元内颗粒源法(PSIC)进行气固两相耦合计算,建立了某型前后翼型装药结构固体火箭发动机(SRM)工作初期的三维两相内流场数值计算模型.对比分析了纯气相和气固两相...     

Acceleration sensors based modal identification and active vibration control of flexible smart cantilever plate

Some flexible appendages of spacecrafts, such as solar panels, are cantilever plate structures. Thus, vibration problem is unavoidable when there is slewing maneuver or external disturbance excitation. Vibration of such cantilever plate structures includes coupled bending and torsional motion. Furthermore, the low amplitude vibration near the equilibrium point is very difficult to be quickly suppressed due to nonlinear factors of the hardware in the system, which is harmful to stability and attitude control accuracy. To solve these problems, acceleration sensor-based modal identification and active vibration control methods are presented for the first two bending and the first two torsional modes vibration of the cantilever plate. Optimal placements of three acceleration sensors and PZT patches actuators are performed to decouple the bending and torsional vibration of such cantilever plate for sensing and actuating, and identifications are achieved by experiments. A nonlinear control method is presented to suppress both high and low amplitude vibrations of flexible smart cantilever plate significantly. Experimental comparison researches are conducted by using acceleration proportional feedback and the presented nonlinear control algorithms. The experimental results demonstrate that the presented acceleration sensor-based methods can suppress the vibration of cantilever plate effectively.     

一种适用于颗粒非规则分布的阻止SPH数值断裂的方法

 〖HT5”H〗摘〓要〖HTSS〗: 光滑粒子流体动力学(SPH)方法已广泛应用于航空航天领域中大变形的碰撞计算。数值断裂是SPH计算中一种常见问题,可严重影响计算结果。把适用于颗粒规则分布的阻止SPH数值断裂的方法推广到颗粒非规则分布的情形,得到了一种适用于颗粒非规则分布的阻止数值断裂的加颗粒方法。然后将该方法应用于存在数值断裂的悬臂梁弯曲仿真计算,验证了其有效性。最后把该方法应用于弹丸撞击飞机蒙皮的非规则颗粒模型计算,并和规则颗粒模型得到的结果及试验结果进行比较。对比结果表明：对于非规则分布的颗粒模型,该加颗粒方法可有效地阻止数值断裂,提高计算精度,并可较为普遍使用。     

基于样条曲线的机动弹头再入轨迹优化研究

使用三次样条函数拟合再入飞行器纵向运动轨迹,以样条曲线上的控制节点为优化参数,将再入轨迹优化问题转化为静态参数优化问题.最后以纵向平面内的最优轨迹为例,以终点速度最大和飞行时间最短为优化目标,采用基于Pareto定级排序遗传算法求解了在末端状态受约束的最优再入轨迹问题,验证了该方法的有效性.     

Using high-energy proton fluence to improve risk prediction for consequences of solar particle events

The potential for exposure to large solar particle events (SPEs) with high energy levels is a major concern during interplanetary transfer and extra-vehicular activities (EVAs) on the lunar and Mars surface. Previously, we have used data from the last 5 solar cycles to estimate percentiles of dose to a typical blood-forming organ (BFO) for a hypothetical astronaut in a nominally shielded spacecraft during a 120-d lunar mission. As part of this process, we made use of complete energy spectra for 34 large historical SPEs to calculate what the BFO mGy-Eq dose would have been in the above lunar scenario for each SPE. From these calculated doses, we then developed a prediction model for BFO dose based solely on an assumed value of integrated fluence above 30 MeV (Φ₃₀) for an otherwise unspecified future SPE. In this study, we reasoned that since BFO dose is determined more by protons with higher energies than by those with lower energies, more accurate BFO dose prediction models could be developed using integrated fluence above 60 (Φ₆₀) and above 100 MeV (Φ₁₀₀) as predictors instead of Φ₃₀. However to calculate the unconditional probability of a BFO dose exceeding a pre-specified limit (“BFO dose risk”), one must also take into account the distribution of the predictor (Φ_30,Φ₆₀, or Φ₁₀₀), as estimated from historical SPEs. But Φ₆₀ and Φ₁₀₀ have more variability, and less available historical information on which to estimate their distributions over many SPE occurrences, than does Φ₃₀. Therefore, when estimating BFO dose risk there is a tradeoff between increased BFO dose prediction at a given energy threshold and decreased accuracy of models for describing the distribution of that threshold over future SPEs as the threshold increases. Even when taking the second of these two factors into account, we still arrived at the conclusion that overall prediction improves as the energy level threshold increases from 30 to 60 to 100 MeV. These results can be applied to the development of approaches to improve radiation protection of astronauts and the optimization of mission planning for future space missions.