飞月轨道引力捕获设计方法研究

利用太阳引力摄动与月球绕飞设计的地月转移轨道（飞月轨道），与霍曼转移相比，虽然飞行时间较长（约三、四个月），但可显著节省速度增量（可达１５０米／秒），对无人月球探测器尤为适合。应用平面圆型限制性四体问题动力学模型，选择从月球出发的初始条件。借助“地心距－时间曲线”，从平面圆型限制性四体问题转换为一般的限制性四体问题。通过典型模拟计算，分析负向积分（从月球轨道出发）初始轨道参数及太阳方位对月球探测器     

Relative position and attitude estimation of spacecrafts based on dual quaternion for rendezvous and docking

The capacity to acquire the relative position and attitude information between the chaser and the target satellites in real time is one of the necessary prerequisites for the successful implementation of autonomous rendezvous and docking. This paper addresses a vision based relative position and attitude estimation algorithm for the final phase of spacecraft rendezvous and docking. By assuming that the images of feature points on the target satellite lie within the convex regions, the estimation of the relative position and attitude is converted into solving a convex optimization problem in which the dual quaternion method is employed to represent the rotational and translational transformation between the chaser body frame and the target body frame. Due to the point-to-region correspondence instead of the point-to-point correspondence is used, the proposed estimation algorithm shows good performance in robustness which is verified through computer simulations.     

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.     

基于可靠性分析的立方星网络维护架构优化

立方星编队或星座构成分布式空间传感器网络，可提高立方星执行复杂空间任务的能力。然而立方星易发生故障，其故障时间不确定性也导致了传感器网络性能的不稳定，这凸显了对立方星网络进行在轨维护的重要性。考虑立方星传感器网络的功能维持问题，描述了一种网络维护架构，通过定期发射、在轨备份立方星以及时更换故障立方星，从而提高网络对单星随机失效事件的快速响应与恢复能力。建立了该架构的运行成本模型，包括固定成本、储存成本和短缺成本。收集整理了真实的立方星寿命数据，并使用最大化拟合优度参数估计方法得到最优立方星寿命的随机模型。采用基于蒙特卡罗仿真的遗传算法优化备用立方星的补给时刻和补给数量，在备份成本与系统性能下降所带来的损失之间进行权衡，使得系统的综合收益最优。     

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.     

一种提高后掠侧压式进气道流量系数的有效措施

在一种双楔顶压、侧板中置的常规后掠侧压式进气道基础上通过减小顶板第二压缩角,引入圆弧压缩面设计了一种具有较高流量系数的进气道.利用Fluent商业计算软件对比研究了该进气道与常规进气道在Ma=6和Ma=4下的流动特征及性能.研究发现,新的改进措施能在几乎不降低进气道总压恢复系数的前提下大幅度提高流量系数:在Ma=6来流条件下,改进后的进气道流量系数为0.87,比常规进气道提高14.5%;在Ma=4来流条件下,流量系数为0.69,提高了19%.     

求解双曲型守恒律的高精度,无波动样条逼近有限体积方法

本文从三次样条逼近出发，提出了求解流体力学双曲型守恒律的一种高精度、无波动的数值方法。针对样条函数的特性，本文提出了一种新的通量限制技术，使该方法在光滑区可以达到四阶精度，在流动参数的空间分布出现拐点或极值点时分别退化为二阶或一阶精度的格式。数值实验表明，该方法对流场中的激波和接触间断有很高的分辨率，优于二阶精度的ＴＶＤ格式。     

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.