基于MBD的检测数据和三维模型关联与可视化技术

针对目前机械零件的检测数据和三维数模相脱离的问题,提出了一种基于MBD的检测数据和三维模型的关联与可视化技术。给出了组合、交叉、聚合三种检测数据和三维模型的关联方式,在CATIA二次开发环境中对检测数据进行特征建模,并且最后将检测数据和三维模型的关联结果进行可视化显示并通过实例验证。     

CU-1型钇基重稀土对Be-Cu合金性能影响的研究

研究了CU-1型钇基重稀土对Be-Cu合金性能的影响。结果表明:Be-Cu合金经过微量CU-1型稀土的微合金化处理后,其显微硬度、耐磨性和耐腐蚀性均有不同程度的提高,热膨胀系数有所下降;随着稀土加入量的增加,Be-Cu合金的显微硬度逐渐提高,磨损量和平均腐蚀速率逐渐降低,热膨胀系数先减小后增大。     

大规模定制设计的产品簇匹配研究

采用基于规则与基于实例相结合的推理方法，给出典型的基于实例推理的专家系统解决问题的一般过程，本文重点研究大规模定制设计的产品簇匹配问题，实施二级匹配策略，先采用规则推理的方法对产品簇大类属性进行匹配，缩小匹配范围，后采用基于实例推理的方法对产品簇小类具体属性进行定量精确匹配，优化了设计手段，效果良好。     

空间机械臂的刚-柔耦合动力学研究

本文对作大范围运动的空间机械臂的刚-柔耦合动力学特性进行了研究，从连续介质力学理论出发，在变形位移中计及了耦合变形量，用Jourdain速度变分原理导出了作大范围运动的空间机械臂的动力学方程，分别用耦合模型和不计耦合变形量的零次近似模型计算了机械臂端点的变形位移，揭示了两种模型的动力学性质的差异。为了确定零次近似模型的适用范围，引入相关系数，仿真计算结果表明，零次近似模型仅适用于相关系灵敏的最大值小于0.1的情况。     

航空器RNP运行中飞行轨迹监测的研究与实现

从分析RNAV／RNP运行对航空器飞行时机载设备的性能特点出发，说明了RNAV／RNP运行初期对飞行品质的监测要求和意义，并就QAR数据作为监测数据源进行了精度分析．表明其可用性，进而给出了一种通过处理QAR数据．反演实际飞行的仿真轨迹，与设计轨迹之间实现了直观比对，并计算给出了比对差值的均值与方差，实现了监测飞行品质的目的。     

Properties of transit trajectory in the restricted three and four-body problem

In the restricted three-body problem if the Jacobi constant is just below the value corresponding to Lagrangian point only a little neck exists around the equilibrium point and capture trajectories are indicated as low-energy. Capture properties depend on the dynamics around these critical points and qualitative results can be obtained using linearized systems. In this paper, to study transit trajectory properties in the restricted three and four-body problem, the Earth–Moon–Sun–Satellite system is considered as example and studied using different models. In the circular restricted three-body problem (Earth–Moon–Satellite), transit, non transit and asymptotic trajectories, are easily identified by using the principal reference frame. Dynamics around Lagrangian point are then studied introducing the Moon eccentricity into the elliptical restricted three-body model. A preferential region for transit orbit is individuated and studied as a function of eigenvalue properties. To introduce the Sun effect, the bi-circular four-body model is considered and dynamics around Lagrangian points studied as a function of angular distance between Earth–Sun and Earth–Moon line. Finally, results obtained in the elliptical three-body model and bi-circular four-body model, are compared with numerical simulations using real Sun–Moon–Earth ephemeris.     

Study of the 28 October 2003 and 20 January 2005 solar flares by means of 2.223 MeV gamma-emission line

By the data on intensity-time profiles of the neutron capture line of 2.223 MeV we have studied some characteristics of two solar flares, 28 October 2003 and 20 January 2005 (INTEGRAL and CORONAS-F observations, respectively). The SINP code was applied making allowance for the main processes of neutron interactions and deceleration in the solar plasma, character of neutron source, losses of neutrons and density model of the solar atmosphere. Comparison of the computed time profiles of 2.223 MeV line with observed ones for the flare of 28 October 2003 confirms the results obtained earlier for three other flares. Namely, the effect of density enhancement (EDE) in the sub-flare region, as well as the variations (hardening) of accelerated particle spectrum in the course of the event have been confirmed. The usual modeling procedure by the SINP code, however, seems to be inapplicable to the event of 20 January 2005. Possible causes of density enhancements during some flares and peculiarities of the 20 January 2005 flare are discussed.     

Contingency and recovery options for the European Student Moon Orbiter

This paper presents an overview of the analysis performed on the lunar orbit and some of the possible contingencies for the European Student Moon Orbiter (ESMO). Originally scheduled for launch in 2014 –2015 as a piggyback payload, it was the only ESA planned mission to the Moon. By way of a weak stability boundary transfer, ESMO is inserted into an orbit around the Moon. Propellant use is at a premium, so the operational orbit is selected to be highly eccentric. In addition, an optimization is presented to achieve an orbit that is stable for 6 months without requiring orbit maintenance. A parameter study is undertaken to study the sensitivity of the lunar orbit insertion. A database of transfer solutions across 2014 and 2015 is used to study the relation between the robustness of weak capture and the planetary geometry at lunar arrival. A number of example recovery scenarios, where the orbit insertion maneuver partially or completely fails, are also considered.     

基于网络信息安全内容审计系统及相关技术研究

伴随着国家信息化不断推进和计算机网络飞速发展,网络信息安全内容审计(CASNI)成为了网络信息安全中不可或缺的重要组成部分.网络信息安全内容审计从网络关键点收集数据包,对其传送的内容进行审计分析,达到网络信息内容可控.本文描述了一种在高速网络环境下分布式、可扩展的高性能网络审计体系结构,分析了Linux(操作系统)捕获数据包的瓶颈,重点论述了使用NAPI (New Application Program Interface)技术和内存映射技术提高数据包捕获,解决审计系统中数据流高速处理的问题.     

现代战机导引系统及其关键技术

阐述了现代战机导引系统的功能、结构与工作方式.基于对导弹制导等相关问题的深入研究,以及对战机导引的特点分析,阐述了战机导引控制律设计中应当解决的关键技术与研究途径,包括远距导引、近距导引和机动导引不同阶段的特点、捕获域的定义与计算方法、战机导引律研究特点及其基本工作模态.本研究可为新一代战机导引系统的研制提供参考.