基于小波包变换及相关系数法的复合材料层合板冲击位置识别研究

复合材料较为广泛应用于航空、航天等工程领域,但对冲击载荷十分敏感。因此,对复合材料结构承受的冲击载荷进行在线监测以及冲击位置的实时识别具有重要意义。文章以复合材料层合板为研究对象,基于两个冲击位置的距离越靠近则接收到信号幅频特性相似度越高的特点,采用FBG光纤光栅传感器,通过小波包变换的方法来提取能量特征向量,同时结合相关系数法来实现复合材料层合板的冲击位置识别。在480 mm×480 mm的复合材料层合板上开展冲击实验,8次实验皆完成了冲击位置识别,其中7个点距离误差为0 mm,实现精准识别,另一个点误差在6%以内。     

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.     

基于局部洪泛优化的低轨星座分布式路由算法

针对传统分布式路由算法应用于大型低轨星座时拥塞控制能力有限的问题,提出了基于局部洪泛优化的分布式路由算法。该算法通过局部洪泛的机制收集星间链路的拥塞信息,以应对局部通信需求密集所导致的常见拥塞现象;通过局部路径优化,以较低运行开销实现了流量疏导和网络负载均衡。并且该算法可适用于多层低轨卫星网络结构,不会产生路由环路,对卫星随机故障具有宽适应性。仿真实验表明:该算法在通信需求分布不均的高网络负载情况下能降低2%~10%的丢包率,并对网络随机故障具有鲁棒的表现。     

小卫星星务系统的遥测技术研究

阐述了小卫星采用的“可控式遥测”和“统一遥测”两种实现技术,即通过遥控、程控和自主控制实施对遥测的状态设置,控制遥测处理流向,改变遥测内容,构成智能化遥测,以增强遥测能力和灵活性。首次提出“二维帧”概念,将卫星的两种遥测标准：PCM遥测和分包遥测统一,实现两者的兼容和平滑过渡,有可能形成新的统一遥测系统标准。在设备级上,统一遥测与PCM遥测一致。在功能层面上,它与分包遥测一致。文章还提出“软件遥测”概念,企望于提升遥测性能。     

发动机进排气系统对飞机气动特性影响的数值研究

为了分析发动机与飞机系统耦合过程中产生的气动力特性,准确获取实际使用条件下的飞机升阻特性,以带动力的某半模飞机模型为研究对象,开展了三维流场数值仿真计算,利用风洞试验数据对计算方法进行了验证,总结了溢流阻力及排气干扰阻力的变化规律,结果表明:发动机状态变化对飞机升阻特性影响明显,在选定的发动机工作参考状态下,溢流阻力在飞机系统升力与阻力方向的分量随捕获面积比的增大分别增大、减小,排气系统实际工作状态偏离选定的参考状态越远,干扰阻力在飞机系统升力和阻力方向分量的绝对值越大。     

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。     

Optimal planning for a multi-debris active removal mission with a partial debris capture strategy

In this paper, a new mission model, called a multi-debris active removal mission with partial debris capture strategy, is proposed. The model assumes that a platform only captures part of the scheduled debris at a time and then releases these debris pieces to a disposal orbit. This process is then repeated until all of the scheduled debris is removed. A genetic algorithm with a multiparameter concatenated coding method is designed to optimize the plan of a multi-debris active removal mission wit...