火星探测器使命轨道捕获策略研究

分析了火星探测器使命轨道捕获策略研究需求,给出了三种可用的典型捕获策略,建立了速度纵向平面内的飞行动力学方程,对三种典型策略进行了飞行动力学仿真,给出了各策略完成捕获所需速度增量、任务耗时及过。通过对仿真结果的分析比较,得出研究结论为：直接制动捕获任务耗时及过载较小,但速度增量需求较大;多次穿越后捕获任务耗时较长,但速度增量需求和过载较小;一次穿越后捕获速度增量需求较小且任务耗时较短,但过载较大。     

Area-oriented coordinated trajectory planning of dual-arm space robot for capturing a tumbling target

The growing amount of space debris poses a threat to operational spacecraft and the long-term sustainability of activities in outer space. According to the orbital mechanics, an uncontrolled space object will be tumbling, bringing great challenge to capture and remove it. In this paper, a dual-arm coordinated ‘‘Area-Oriented Capture"(AOC) method is proposed to capture a non-cooperative tumbling target. Firstly, the motion equation of the tumbling target is established, based on which, the dynamic properties are analyzed. Then, the ‘‘Area-Oriented Capture"concept is presented to deal with the problem of large pose(position and attitude) deviation and tumbling motion. An area rather than fixed points/devices is taken as the object to be tracked and captured. As long as the manipulators' end-effectors move to a specified range of the objective areas(not fixed points on the target, but areas), the target satellite will be hugged by the two arms.At last, the proposed method and the traditional method(i.e. fixed-point oriented capture method)are compared and analyzed through simulation. The results show that the proposed method has larger pose tolerance and takes shorter time for capturing a tumbling target.     

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.     

偶发组播数据丢包问题研究

针对传输关键控制数据的某型冗余备份网络架构在大背景流量下偶发组播数据丢包的问题,分析了丢包机理,提出配置静态组播组的方法,同时进行了实验验证。结果表明,该方法能有效解决工程实践中出现的问题。因此,在网络结构设计时,要充分考虑传输链路中会对组播传输产生洪泛的设备,采取有效措施消除影响,确保组播数据传输的正确性与完整性。     

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.     

小波包分析在内燃机车静液压齿轮箱故障诊断中的应用

本文简述了小波变换的基本原理及利用小波包对振动信号进行分解的方法。小波分析良好的时频局部化性质，适于检测正常信号中夹带的瞬态反常现象并展示其成分，这在旋转机械状态监侧及早期故障诊断中具有重要意义。本文给出利用小波包分析在内燃机车静液压齿轮箱故障诊断中提取微弱轴承冲击故障特征的实例。     

三维球坐标系下重力波波包非线性传播过程听数值研究

采用全隐欧拉（FICE）格式，对三维球坐标系下重力波波包在中层大气的非线性传播过程进行了数值模拟，模拟结果完整地反映了重力波波包在中层大气的非线性传播过程，并与线性重力波理论进行了定量比较。