装有自由旋转尾翼的鸭式导弹的滚动发散

用解析的方法研究有自由旋转尾翼和鸭式控制面的导弹的滚动运动,确定了运动的平衡状态;探讨在所施加的铰链力矩不变时小扰动的情况;利用对平衡状态小偏差的线性运动方程,推导出稳定的显式条件,并用全运动方程数值解考察了大扰动情况和在俯仰、偏航上导弹自由度的影响,证明了大偏差的发散特性.研究结果表明,滚动运动在很大的参数范围内是发散的,产生发散的主要因素是气动力滚动阻尼的减少和离心力对控制面的作用.     

火箭发动机推力瞬变的测量

任何测力装置都能用一个质量弹簧系统来描述,最简单地说:即通过一个具有刚度 K 和质量 M 的简单弹簧来描述,其中它的阻尼为 c,位移为 x,于是有M(d~2x/dt~2) c(dx/dt) kx=T,这里 T 为外加力。而大多数系统只测量 kx 项,这对低频情况是足够的。为了精确地记录推力的变化,从而要提高装置的固有频率,使之相对于推力变化的频率来说足够高,有时这是不现实的。为克服这一困难有两种可采用的途径。第一种方法是把运动方程的所有项合并到远远超过装置的固有频率所给定外力上。第二种方法是一个质量块在沿轴向作用的轴承上被发动机自由加速,加速度计给出推力/时间曲线。通过使质量块停止所需要的力对所预定时间内的积分而得到总冲。     

碳/碳复合材料

引言近年来,欧洲动力公司(S.E.P.)对固体发动机喷管部件所用的碳材料,特别是碳/碳材料进行了研制。喷管材料具有耐烧蚀的特性,要经受3000℃以上的高温。由于喷管性能要求非常高,材料必须具有良好的耐烧蚀性能和较低的比重。考虑到在大多数喷管里,化学反应发生在还原介质中,我们认为所能使用的耐热材料中,碳是最可取的。在此文中,我们不评述构成喷管部件的碳结构材料,只简要地论述多晶石墨、热解石墨、碳增强酚醛复合材料和碳/碳材料,侧重介绍后两种,这是欧洲动力公司重点研制项目。     

论现有远地点发动机用于新航天飞行器的有关问题

为了使正进入鉴定阶段的远地点发动机(TE-M-616)用于广播试验卫星,本文介绍了该新航天飞行器对远地点发动机的各系统及分系统提出的要求。由于加拿大通讯技术卫星和广播试验卫星对远地点发动机在环境和性能要求上有所不同,为了解决此问题,必须使远地点发动机经受住最恶劣的环境。喷管设计以及远地点发动机与航天器的对接都利用现有设计结构。根据对远地点发动机分析的结果,已经表明,若保持安全系数不变,只需要对现在进行的试验计划做一些修改和补充。另一方面,对于航天器提出的技术条件必须进一步审核,以便使新航天飞行器设计有最大可能利用现有的远地点发动机。     

一种大变形多空间域连续体结构拓扑优化方法

针对大变形非线性结构拓扑优化问题,提出了基于混合细胞自动机(HCA, Hybrid Cellular Automata)多空间域连续体结构拓扑优化方法;采用密度法,建立了单元相对密度表示的材料弹-塑性模型;以单元相对密度和应变能作为细胞自动机(CA,Cellular Automata)的状态信息,利用CA局部控制规则,修改相对密度,迭代实现各设计空间域应变能均匀分布;设计了多空间域拓扑优化HCA算法,采取多个对象同时耦合优化迭代,各自收敛策略,解决了多空间域优化迭代算法收敛稳定性问题;最后,以汽车保险杆结构横梁和支撑等两个设计空间为例,施加大变形动态载荷作用,对提出的多空间结构优化算法进行了验证,优化后结构有效地降低了碰撞作用力峰值达54％,提高了结构安全性.     

DS/FH混合扩频快速捕获技术的研究

在DSFFH混合扩频通信系统中,快速捕获是一个非常关键的技术。通过采用快速扫描和等待式相结合的方法用来实现跳频信号的快速捕获,利用神经网络技术实现直扩信号的快速捕获,通过这2种方式,就可实现DSFFH混合扩频的快速捕获。     

The Physical Foundation of Forecasting Disturbances in the Geospace From Solar Disk Characteristics

The five main types of antisunward propagating energetic fluxes (particles and emission) may be thought of as well established to date, the effects of which lead to a particilar character of disturbance in the near-terrestrial environment (the Earth's magnetosphere, ionosphere and atmosphere). The strongest global restructuring of the magnetosphere and ionosphere is caused by fluxes of relatively dense n of 1-70 cm-3 at the Earth's orbit) Solar Wind (SW) quasi-neutral, low-energy (E ＜ 10 keV) plasma which cause magnetospheric and ionospheric storms lasting 24 hours or longer. For that reason, main attention is given to their study at the initial stage of research. The physical essence of the method of predicting disturbances in the near-terrestrial space environment, the amplitude of which can be expressed in, for example, the Kp index units, involves:(1) identifying all the most geo-effective SW streams of type, (2) determing their sources on the solar disk,and (3) quantifying the correlations between the characteristics of their solar sources with a maximum value of the Kp-index that is caused by the concerned type of SW stream. Semi-phenomenological relations have been obtained, which relate parameters of type SW stream sources to characteristics of geomagnetic storms:storm commencement, the time at which the storm intensity reaches its maximum values, the storm duration,as well as to the storm amplitude expressed in terms of geomagnetic indeces.      

Study of the Enhancement Events of Relativistic Electron at the Geosynchronous Orbit

The high flux of energetic electron on geostationary orbit can induce many kinds of malfunction of the satellite there, within which the bulk-charging is the most significant that several broadcast satellite failures were confirmed to be due to this effect. The electron flux on geostationary orbit varies in a large range even up to three orders accompanied the passage of interplanetary magnetic cloud and the following geomagnetic disturbances. Upon the investigation of electron flux enhancement events, two types of events were partitioned as recurrent events and random ones. Both of the two kinds of events relate to the interplanetary conditions such as solar wind parameters, IMF etc and their evolution characters as well. As for the recurrent events, we found that, (1) all of the events exhibits periodic recurrence about 27 days, (2) significant increase of electron flux relates to interplanetary index and characters of their distribution, (3) the electron flux also has relation to solar activity index. An artificial neural network was constructed to estimate the flux I day ahead. The random electron flux enhancement events are rare and present different distribution figures to the recurrent ones. The figure of the random events and the conditions of their occurrence is also discussed in this paper.      

电推进系统为何会扰乱MRO行业

<正>随着电推进系统研发工作取得持续的进展,航空维修领域非常有必要提前了解电推进的发展现状和未来走势,尤其是发动机维修售后市场参与者需要尽早参与电动飞机设计过程,以便获得对飞机维修性的最直接的实践反馈,并且及早建立与之相适应的维修能力、维修设施、维修模式和维修培训系统等。