航空电子WDM网络的实时性能分析

对航空电子波分复用(WDM,Wavelength Division Multiplexing)网络实时性评估问题,采用网络演算理论,提出了一种周期消息在WDM复杂虚拓扑上多跳端对端最大延迟的计算方法.建立了波长路由器WDM网络模型,分析了消息流端对端延迟的组成部分.针对网络演算理论下的WDM网络通信模型,推导了消息经单节点和多节点波长路由器的最大延迟的计算公式.并结合实际航空电子系统对公式进行了修正,解决了突发度过大的问题.最终得到最大延迟的紧密上限.最后在OPNET仿真环境下验证了计算分析方法的有效性.     

小型化TDLAS发动机测温系统的研究及进展

在吸气式发动机研究中,需要监测其进气道气流流场分布、燃烧室温度分布和燃烧产物浓度来验证燃烧室内的燃烧理论模型并最终改进发动机设计;同时,这些参数的实时获取还可以用来控制发动机工作状态以实现燃烧效率优化。TDLAS(可调谐半导体激光吸收光谱)技术具有结构紧凑、响应快速、灵敏度高和非入侵式测量等优点,在高温、高速和剧烈振动等恶劣工作环境下可实现随机飞行的发动机测量,因此被国外多家研究机构采用。调研了高超声速燃烧发动机研究项目 HIFiRE及其在传感器小型化方面所采用的技术手段,介绍已有的小型化设计思路和取得的进展。已集成的小型化系统体积为30×15×10cm3,重量<5kg,功耗<10W。经验证,该系统可在发动机地面试验条件下稳定工作,给未来随发动机飞行的小型化测温系统设计提供了参考。     

基于GPS的广州地区电离层不规则体纬向漂移速度计算分析

利用广州站组建的两台短间距GPS电离层闪烁监测仪的观测数据, 分别对GPS卫星信号强度用功率谱和短间距台链互相关性两种方法计算了3次闪烁事件电离层不规则体的漂移速度. 分析结果表明, 同一不规则体会引起两台站闪烁事件的同时发生, 两种方法测量不规则体漂移速度通常在50～160m/s之间, 平均大小均在120m/s左右, 且纬向漂移速度在闪烁初期起伏较明显, 速度随闪烁时间有下降的趋势, 夜间纬向漂移方向由西向东, 广州地区漂移速度特性符合低纬其他地区不规则体漂移速度特征, 两种计算方法合理有效.      

电离层扰动的GPS探测

提出了一种利用短基线GPS接收阵探测研究电离层扰动的实验新技术,在此基础上发展了一种消除观测点运动速度的影响,从探测结果中确定扰动传播参量的数据分析算法．实验结果表明,短基线GPS接收阵用于探测研究TID一类电离层扰动时,精度高,可靠性好,并能有效地探测大范围电离层扰动的传播特性．     

空间短时飞行试验工具的应用与展望

空间短时飞行试验是指以探空火箭、气球、亚轨道重复发射工具等为主要实现手段,将待试验对象发射到一定高度,进行科学实验和技术验证的研究方法。对空间短时飞行试验工具的发展历史和应用现状进行综述,对探空火箭、气球、亚轨道重复发射工具在科学观测、新技术试验中发挥的作用进行总结和概括,以NASA飞行机会计划FOP为例,对其在有效载荷技术成熟度评估中的应用情况进行了重点阐述,结合我国空间科学探测和空间技术试验的迫切需求,对空间短时飞行试验工具在我国的应用前景进行了展望和预测。     

电离层短波射线追踪

本文以电离层等离子体参量的平均背景模式计算为基础, 给出一种电离层短波射线轨迹计算方法。供短波通信系统、工作于短波段的其它系统(如HF雷达的目标定位系统)及有关研究工作使用参考。      

纵向大迎角飞行品质对参数的灵敏度分析

采用等效系统,频域,时域等多种飞行品质评价方法和准则。根据数据计算结果分析了放宽带稳定的电传操纵飞机从小迎角到失速前大迎角纵短周期飞行品质对于气动及惯性参数变化的灵敏度。结果表明,飞行品质对操纵导数及惯矩的变化最灵敏,对升力线斜率变化呈一定的灵敏度,而对其它参数变化则不太灵敏,灵敏度具有体量值测随角而不同。     

Fast calibration of between-receiver GPS/Galileo/BDS differential phase bias with millimeter accuracy based on short baseline mode

The differential code and phase biases induced by the receiver hardware (including receiver, antenna, firmware, etc.) of the Global Navigation Satellite System (GNSS) have significant effects on precise timing and ionosphere sensing, thus deserve careful treatment. In this contribution, we propose an approach to fast fix the single-difference ambiguity to finally obtain the unbiased estimates of between-receiver differential phase bias (BR-DPB) and between-receiver differential code-phase bias (BR-DCPB) based on the short baseline mode. The key to this method is that the error sources can be significantly eliminated due to the length of the baseline is very short. At the same time, the empirical constraints and random characteristics of BR-DPB/BR-DCPB were considered, which is conducive to the resolution of single-difference ambiguity. Several sets of GNSS data (GPS L1/L2, Galileo E1/E5b, and BDS B1/B3), recorded by the short baselines in an interval of 30 s and covered a broad range of receiver/antenna types (JAVA, SEPT, LEIC, and TRIM), were used to verify the effectiveness of the proposed method. The numerical tests show that the proposed method is capable of fast fixing the single-difference ambiguity successfully within a few epochs and then providing the unbiased estimates of BR-DPB and BR-DCPB in an epoch-by-epoch manner. Experiments show that the estimated BR-DPB is in millimeter accuracy, which is of great significance for the millimeter-accuracy phase time transfer and ionospheric delay estimation. Furthermore, the calibrated BR-DPB/BR-DCPB can be treated as the known products for long-distance precise timing and ionosphere sensing based on the inter-station single-difference model.     

A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy

The past two decades have witnessed a renewed interest in low frequency radio astronomy, with a particular focus on frequencies above 30 MHz e.g., LOFAR (LOw Frequency ARray) in the Netherlands and its European extension ILT, the International LOFAR Telescope. However, at frequencies below 30 MHz, Earth-based observations are limited due to a combination of severe ionospheric distortions, almost full reflection of radio waves below 10 MHz, solar eruptions and the radio frequency interference (RFI) of human-made signals. Moreover, there are interesting scientific processes which naturally occur at these low frequencies. A space or Lunar-based ultra-low-frequency (also referred to as ultra-long-wavelength, ULW) radio array would suffer significantly less from these limitations and hence would open up the last, virtually unexplored frequency domain in the electromagnetic spectrum.A roadmap has been initiated by astronomers and researchers in the Netherlands to explore the opportunity of building a swarm of satellites to observe at the frequency band below 30 MHz. This roadmap dubbed Orbiting Low Frequency Antennas for Radio Astronomy (OLFAR), a space-based ultra-low frequency radio telescope that will explore the Universe’s so-called dark ages, map the interstellar medium, and study planetary and solar bursts in the solar system and search them in other planetary systems. Such a radio astronomy system will comprise of a swarm of hundreds to thousands of satellites, working together as a single aperture synthesis instrument deployed sufficiently far away from Earth to avoid terrestrial RFI. The OLFAR telescope is a novel and complex system, requiring yet to be proven engineering solutions. Therefore, a number of key technologies are still required to be developed and proven. The first step in this roadmap is the NCLE (Netherlands China Low Frequency Explorer) experiment, which was launched in May 2018 on the Chinese Chang’e 4 mission. The NCLE payload consists of a three monopole antenna system for low frequency observations, from which the first data stream is expected in the second half of 2019, which will provide important feedback for future science and technology opportunities.In this paper, the roadmap towards OLFAR, a brief overview of the science opportunities, and the technological and programmatic challenges of the mission are presented.     

短周期运动飞行品质的几种判据

飞机纵向短周期运动是影响其飞行品质的关键因素，根据国外近年来所进行的研究，综合，发纳出六种适用于小迎角飞行的短周期飞行品质标准，基于等效系统的控制期望参数（ＣＡＰ）等准则依然适用，并作了增补；对于不能用低阶系统等效的飞机提出了诸发带宽准则等相应判据，这六种准则各有其侧重点和适用范围，较全面地反映了飞机短周期运动特性，共同完成对飞行品质的评判和预估。