基于虚拟仪器的无线电设备检测仪

ATE是军用飞机测试技术的发展方向,利用虚拟仪器开发机载无线电台的检测系统是向ATE发展的重要一步。目前成熟的总线技术和虚拟仪器技术提供了技术实现途径,为此基于虚拟仪器技术设计了无线电设备的地面检测仪。     

基于EEG的驾驶舱告警信息设计研究

针对直升机驾驶舱人机交互中认知负荷问题,设计飞行模拟试验,探究视觉和听觉告警对飞行员认知负荷的影响。基于多元线性回归方法,通过主观评价结果、反应时间、准确率和脑电信号等指标,构建了直升机驾驶舱人机交互认知负荷评估模型。结果表明文字颜色、语音提示两种告警特征对飞行员信息加工均会产生影响,使用多元线形回归模型可对不同告警方式下受试对象的认知负荷水平进行评估,构建的评估模型能够较准确地评估直升机驾驶舱中飞行员的认知负荷,可为优化驾驶舱交互设计、降低飞行员认知负荷、减少人为差错提供依据。     

基于非连续算子广义变分不等式强解的存在性

在算子不连续的情况下,利用FKKM定理和Weierstrass定理及标量化方法得到了广义向量变分不等式的强解存在性定理.     

飞行管理系统下降路径构建及应用研究

在飞行管理系统下降设计中，通过下降路径的构建可为接近目的机场提供一个垂直轨迹，使飞机遵守终端区各种限制要求，从而精确控制下降路径，满足安全性要求。本文分析了下降路径的定义及其在典型机型中的构建方法，给出了下降路径的描述方法及实现途径，并对具体机型中的应用做了简要介绍。     

高速BPSK相干光通信系统对激光器线宽要求

文章概述了激光器相位噪声对零差相干检测光通信系统性能的影响，对特定的基于平衡探测的科斯塔斯（Costas）环路接收系统相位误差进行了详细的理论分析，最后获得了不同传输码速率下的零差相干检测光通信系统对激光器线宽的具体要求。     

CCSDS在我国航天领域的应用展望

CCSDS(空间数据系统咨询委员会)建议有利于增强测控系统互联互通互支持能力,满足未来航天任务对空间信息高速传输及灵活高效信息调度机制的要求,应当作为我国构建天地一体化信息网络的首选标准。提出了加强顶层设计、循序渐进地推进CCSDS建议在我国实现工程化应用的总体思路,并提出在应用过程中应当注重创新任务操作模式、关注信息安全、深化关键技术研究与验证。     

Variation in the ionospheric propagating factor M(3000)F2 at Ouagadougou,Burkina Faso

We use hourly monthly median values of propagation factor M(3000)F2 data observed at Ouagadougou Ionospheric Observatory (geographic12.4°N, 1.5°W; 5.9^o dip), Burkina Faso (West Africa) during the years Januar1987–December1988 (average F10.7 < 130 × 10⁻²² W/m²/Hz, representative of low solar flux conditions) and for January 1989–December1990 (average F10.7 ? 130 × 10⁻²² W/m²/Hz, representative of high solar epoch) for magnetically quiet conditions to describe local time, seasonal and solar cycle variations of equatorial ionospheric propagation factor M(3000)F2 in the African region. We show that that seasonal trend between solar maximum and solar minimum curves display simple patterns for all seasons and exhibits reasonable disparity with root mean square error (RMSE) of about 0.31, 0.29 and 0.26 for December solstice, June solstice and equinox, respectively. Variability Σ defined by the percentage ratio of the absolute standard deviation to the mean indicates significant dissimilarity for the two solar flux levels. Solar maximum day (10–14 LT) and night (22–02 LT) values show considerable variations than the solar minimum day and night values. We compare our observations with those of the IRI 2007 to validate the prediction capacity of the empirical model. We find that the IRI model tends to underestimate and overestimate the observed values of M(3000)F2, in particular, during June solstice season. There are large discrepancies, mainly during high solar flux equinox and December solstice between dawn and local midnight. On the other hand, IRI provides a slightly better predictions for M(3000)F2 between 0900 and 1500 LT during equinox low and high solar activity and equinox high sunspot number. Our data are of great importance in the area of short-wave telecommunication and ionospheric modeling.     

发动机不可控高推力适航部分豁免方法研究

介绍了发动机不可控高推力(UHT)问题的产生背景,论述了申请§25.901(c)条款有关不可控高推力的部分豁免的思路和方法.结合FAA关于不可控高推力的指导材料,给出了有关不可控高推力的持续适航工作建议,对于飞机申请§25.901条款有关不可控高推力的部分豁免具有一定的指导意义     

CLVD 法制备C/C复合材料工艺探索研究

研究了采用化学液气相沉积法制备C／C复合材料的工艺过程，分析了不同预制件、温度、浸泡时间等工艺参数对致密速度、效果的影响，并总结出了一套快速高效的致密方法。     

Beam-Park-Experiment-1/2000 with TIRA

A monostatic 24-h debris observation campaign (BPE-1/2000) has been prepared and conducted using FGAN's TIRA L-Band system. Based on experiences from previous Beam-park experiments a similar largely automated data processing is applied on an extended range window of 300–2000km. More than 1500 detections are encountered, 471 of them are verified as being real objects in Low-Earth-Orbit (LEO). PROOF's observation forecasting of catalogued objects is evaluated against the observed objects, and the difficulties obtaining radar cross-sections (RCSs) and object sizes from Beam-park experiments are discussed. Sidelobe detections are identified by using background information like two-line element (TLE) sets and/or catalogued RCSs.In comparison with previous experiments, the statistics show similarities confirming the concept of Beam-park experiments for space debris observations, despite the snapshot character of 24-h experiments. The comparison with MASTER/PROOF'99 and ORDEM2000 leads to a reasonable agreement between models and observations.