一种基于DRFM和数字信道化技术的 宽带雷达目标干扰模拟器设计

提出了一种DRFM和数字信道化技术的宽带雷达目标干扰模拟器设计方案,详细讨论了宽带雷达信号的数字信道化接收算法和基于DRFM的扩展目标/干扰生成方法。仿真分析结果表明,该方案可以实现1 GHz带宽的雷达导引头目标干扰信号模拟,并可推广用于宽带雷达导引头干扰机和宽带雷达导引头数据采集系统设计。     

26 m射电望远镜副面调整机构误差分析

新疆乌鲁木齐南山26 m射电望远镜（NSRT）采用 Stewart 并联机构实现副反射面（简称副面）五自由度运动调整。为确保并联机构的运动精度能满足射电望远镜高精度的指向要求,对影响副面调整机构运动精度的各项误差进行了分析。几何误差模拟结果显示,为使并联机构达到要求的精度,应保证杆长误差小于0.08 mm,铰链误差小于0.04 mm。通过对实测结果与仿真结果分析比较,得出回零误差是造成并联机构误差的主要原因。由于并联机构的回零检测装置主要由增量式编码器与限位开关组成,其中限位开关反馈信号的异常,会引起并联机构的回零误差,分析得到该因素是造成NSRT副面并联机构工作偏差的主要原因,这对并联机构的误差补偿具有指导意义。     

C-R样条用于低散射目标爬行波求解

C-R(Catmull-Rom)样条具有直观、稳定、灵活、不需反求控制顶点等优点,特别适用于具有复杂外形的飞行器进行几何描述. 利用 (G¹,k=1) Catmull-Rom样条及其张量积曲面对低散射目标进行几何建模,并求解低散射目标爬行波RCS贡献,通过计算结果与实验结果比较,获得令人满意的结果.     

出口宽高比及旋流角对双涵道S弯喷管温度分布的影响

采用数值方法研究了出口宽高比及旋流角对基于真实排气混合器构型的双涵道S弯喷管内/外流场温度分布的影响.结果显示:在圆转方弯曲构型的作用下,波瓣混合器及尾锥诱导产生的流向涡在第二弯通道及等直段内部卷吸着热流冲击S弯喷管壁面形成"热斑".在完全遮挡高温部件准则的约束下,随着出口宽高比的增加,S弯喷管壁面的"热斑"温度先增大...     

小波变换与SVD结合的射频信号消噪方法

射频信号因具备空间远距离传输特性被广泛应用于航天测控等领域,但空间磁场、信道、设备元器件等会引入大量噪声干扰,对射频信号的传播及后续分析处理造成影响。而目前关于射频信号消噪的研究很少,针对此问题,对比研究了传统滤波器消噪、小波阈值法及SVD(Singular Value Decomposition,奇异值分解)法在射频信号消噪方面的应用,仿真分析了各算法对有用射频信号的提取效果,从而发现3种方法均能起到噪声抑制的作用,但是,滤波器法明显会降低信号能量,小波变换法易使重构信号失真,而SVD法则运算时间较长。为此,提出将小波阈值法与SVD相结合,用于射频信号消噪。再通过比对各方法消噪的性能指标,验证了将2种方法结合,可有效提高运算效率及噪声抑制能力。     

宽带综合射频前端三种实施方案

首先描述了军机上射频传感器的现状，介绍了综合射频收发机三种实施方案及其优缺点和应用，其次针对各种不同实施方案存在的缺点给出了改进措施，最后给出了未来综合射频前端的发展趋势及努力方向。 [关键词] 综合射频前端技术；发射机；接收机；中频架构；零中频；数字收发机     

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.     

等效地球半径法应用中的问题

为阐明等效地球半径法应用的范围和应用中应该注意的问题,从等效地球半径法的定义推导了等效地球半径模型与实际地球模型之间量的映射关系.给出并证明了等效过程中等效地球半径模型与实际地球模型下的射线高度、仰角、长度相等,而地心角在转换过程中约为3/4的映射关系.讨论了需要利用地心角映射关系进行计算时的两种情况,同时给出计算结果和误差分析.     

Assessment of the suitability of public mobile data networks for aircraft telemetry and control purposes

This paper provides a review of the state of the art of relevant work on the use of public mobile data networks for aircraft telemetry and control proposes. Moreover, it describes the characterisation for airborne uses of the public mobile data communication systems known broadly as 3G. The motivation for this study was to explore how this mature public communication systems could be used for aviation purposes. An experimental system was fitted to a light aircraft to record communication latency, line speed, RF level, packet loss and cell tower identifier. Communications was established using internet protocols and connection was made to a local server. The aircraft was flown in both remote and populous areas at altitudes up to 8500 ft in a region located in South East Queensland, Australia. Results show that the average airborne RF levels are better than those on the ground by 21% and in the order of −77 dbm. Latencies were in the order of 500 ms (1/2 the latency of Iridium), an average download speed of 0.48 Mb/s, average uplink speed of 0.85 Mb/s, a packet of information loss of 6.5%. The maximum communication range was also observed to be 70 km from a single cell station. The paper also describes possible limitations and utility of using such communications architecture for both manned and unmanned aircraft systems.     

用AM300型函数信号发生器建立相位测量标准装置

提出了一种建立相位测量标准装置的方法。该标准装置以AM300型函数信号发生器为主标准器,相位计、示波器、失真度测量仪、数字电压表为配套设备。对AM300型函数信号发生器的量值指标进行了测试和实验,包括：相位增量误差测试、相位绝对零度误差测试、60°幅相误差测试、测量的重复性实验和长期稳定性实验。结果表明：该标准装置测试结果准确,性能稳定可靠,具有造价低、实用性强的特点。