弹性飞机平衡的阵风外载荷计算与分析

连续紊流是适航规范中阵风载荷分析必须考虑的一种阵风模型,但其引起的阵风载荷在飞机结构设计中的应用一直存在困难.在平稳随机过程的假设下,基于von Karman连续紊流功率谱模型和线性系统连续紊流响应的功率谱方法,使用载荷累加法获得外载荷形式的阵风载荷.在此基础上,通过引入载荷响应的相关性推导并建立了一种生成多组连续紊流平衡外载荷分布的方法.垂向连续紊流情况下的算例结果表明:连续紊流外载荷分布是全机平衡的.平衡的外载荷分布可通过机动飞行载荷分析中的载荷包线方法识别载荷设计情况,从而应用于飞机结构的强度分析与设计.     

基于CWT-CNN的齿轮箱运行故障状态识别

针对传统故障诊断中提取的特征不具有自适应能力、很难匹配特定故障的问题,提出了一种基于连续小波变换（CWT）和二维卷积神经网络（CNN）的齿轮箱故障诊断方法。该方法对齿轮箱故障振动信号采用连续小波变换构造其时频图,以其为输入构建卷积神经网络模型,通过多层卷积池化形成深层分布式故障特征表达。利用反向传播算法调整网络各层的结构参数,使模型建立从信号特征到故障状态之间的准确映射。在不同工况和不同故障状态下的实验中,故障识别准确率达到了99.2%,验证了方法有效性。采用这种自适应学习信号中丰富的信息的方法,可以为故障诊断智能化提供基础。      

航天器资源约束的时间拓扑排序处理方法

针对航天器自主任务规划中的资源受限、约束复杂、活动并行等问题,提出了基于时间拓扑排序的航天器资源计算方法。考虑规划结果中资源产生及消耗,采用资源约束网络模型表示规划中动作的资源需求。通过分析资源变化与动作执行时间的关系,在资源处理过程中对资源约束网络的资源突变时刻进行拓扑排序,优化了流量推进路径的选择过程,时间复杂度为O(n 2 )。数值仿真结果表明,算法提高了规划过程中资源处理的效率。     

针对GPS接收机性能的压制干扰区域分析

针对采用扩频增益作为GPS接收机抗干扰容限的非普适性和不确定性,通过建立压制干扰造成GPS接收机不同性能指标下降与分析对象之间的对应关系,将干扰威力区域用受扰区、半失效区和失效区来进行划分。结合GPS接收机工作原理,从理论上推导和分析了在连续波（CW）和宽带高斯噪声干扰下不同相关积分时间的接收机捕获、跟踪和解调等环节的性能下降到临界值时所需干信比。考虑干扰源高度与接收机天线增益的关系,对各威力区的有效干扰距离随干扰源发射功率变化情况进行仿真计算。仿真结果表明,随着干扰功率的提高,干扰源高度对有效干扰距离的影响在逐渐减小。在相同干扰功率下,CW干扰性能要优于宽带高斯噪声干扰。尽管增加接收机相关积分时间会使半失效区和失效区的范围减小,但却会引起受扰区范围显著增大。     

多基线组合求解深空航天器载波相位模糊方法

针对深空航天器高精度定位需求,提出多基线组合求解载波相位模糊方法,获得比群时延更精确的相时延,极大地提高无线电干涉测量精度。首先建立多基线组合求解载波相位模糊的数学模型,推导该方法对长短基线组合的约束条件。然后利用美国甚长基线阵(VLBA)对本文方法进行仿真校验,结果表明航天器定位精度可以达到纳弧度量级。最后结合我国已有干涉测量网,分析在我国未来深空探测任务中采用多基线组合测量载波相时延的可行性,给出满足方法约束的站址选择建议,可为我国深空导航无线电干涉测量技术的发展和深空测控网的完善提供参考。     

一种用于深空导航定位的新型DOR信标

甚长基线干涉测量(VLBI)是深空探测器导航定位的重要手段之一,深空探测器的VLBI观测通常采用差分单程测距(DOR)信标和双差单程测距(Delta-DOR)测量体制,精确地测量深空探测器相对于河外射电源的角距.相位杂散是影响Delta-DOR测量精度的主要误差源之一,针对这项误差研究了一种基于伪随机噪声调制方式的新型...     

单模式LIPS-200离子推力器的寿命及可靠性定量评估

针对离子推力器产品工作寿命及可靠性定量评估的难题,结合单工作模式LIPS-200离子推力器产品成熟度提升需求,通过寿命主要影响因素耦合分析,应用试验数据、数值模型和数理统计方法,提出了单工作模式离子推力器寿命及可靠性定量评估的可行技术途径:通过分析模型、验证试验和数值模型之间的不断迭代实现各失效模式对应磨损模型的精细化...     

Overview of atmospheric ionizing radiation (AIR) research: SST-present.

The Supersonic Transport (SST) program, proposed in 1961, first raised concern for the exposure of pregnant occupants by solar energetic particles (SEP), and neutrons were suspected to have a main role in particle propagation deep into the atmosphere. An eight-year flight program confirmed the role of SEP as a significant hazard and of the neutrons as contributing over half of the galactic cosmic ray exposures, with the largest contribution from neutrons above 10 MeV. The FAA Advisory Committee on the Radiobiological Aspects of the SST provided operational requirements. The more recent lowering of ICRP-recommended exposure limits (1990) with the classification of aircrew as "radiation workers" renewed interest in GCR background exposures at commercial flight altitudes and stimulated epidemiological studies in Europe, Japan, Canada and the USA. The proposed development of a High Speed Civil Transport (HSCT) required validation of the role of high-energy neutrons, and this resulted in ER-2 flights at solar minimum (June 1997) and studies on effects of aircraft materials on interior exposures. Recent evaluation of health outcomes of DOE nuclear workers resulted in legislation for health compensation in year 2000 and recent European aircrew epidemiological studies of health outcomes bring renewed interest in aircraft radiation exposures. As improved radiation models become available, it is imperative that a corresponding epidemiological program of US aircrew be implemented.     

机会数字阵雷达概念与应用技术分析

机会数字阵雷达是以平台隐身性设计为核心,以数字阵列雷达为基础,兼具多功能、多模式的"一体化"新概念雷达系统.本文在对国外有关概念雏形描述理解基础之上,对其定义和涵义进行了深入透析,详细论述了"机会"一词的几层涵义.分析了机会数字阵雷达不同于传统相控阵雷达的技术特性和应用潜力,以及机会数字阵雷达所面临的技术难题,如3-D空间单元"机会性"分布优化选取和波束综合,信号传输与同步以及多自由度的系统资源优化管理等问题,并给出了初步的解决方案和仿真结果.     

Polarization pattern of low and mid-frequency magnetic pulsations in the polar cap: A comprehensive analysis at Terra Nova Bay (Antarctica)

The polarization pattern of ULF pulsations (f ≈ 1–100 mHz) at Terra Nova Bay (Antarctica, CGM λ ∼ 80°) has been determined for the entire 2003, soon after the solar maximum. A comparison with the results of previous investigations, conducted at the same station close to the solar minimum (1994–96), allows to focus common elements and major differences among different frequency bands which persist through the entire solar cycle. Basically, between f ∼ 1.5 and 5 mHz, the day can be divided into four sectors with alternate polarizations. The local time and latitudinal dependence of the observed pattern can be tentatively interpreted in terms of a latitude of resonant field lines reaching λ ∼ 80° in the noon sector; on the other hand, resonance effects of lower latitude field lines can be clearly identified also far from the noon meridian when the station moves into the deep polar cap. Moreover, in the morning sector the resonance region would extend to lower latitudes than in the evening sector. The proposed profile of the resonant region can interpret also the results obtained at other cusp/auroral stations and appears consistent with that one inferred in the northern hemisphere at smaller latitudes. The resonance region progressively shifts toward lower latitude with increasing frequency; correspondingly, the four-sector pattern progressively disappears at TNB. Above f ∼ 20 mHz, the experimental observations might suggest an additional contribution from Sunward propagating waves, possibly via the magnetotail lobes.