FY-2C星数传与云图广播转发器分系统

介绍了风云二号(FY-2)气象卫星数传与云图广播转发器分系统的功能、组成,以及频率配置、传输信号特性和增益与功率等主要技术指标.给出了C星分系统转发器的技术改进.阐明了采用的收发多工器、射电天文保护滤波器、固体功率放大器(SSPA)和功能转换开关等关键技术.测试结果和在轨运行状况表明,C星数传与云图广播转发器的性能符合设计任务书要求,在轨运行正常稳定.     

高温超导谐振器技术及其应用研究综述

目前,用超导临界温度比较高、微波表面电阻Rs较小、超导性能稳定的高温超导薄膜制成的高温超导谐振器已在工程上得到广泛应用。高温超导谐振器较其他谐振器具有Q值高、噪声小、损耗低等优点。它不仅可作为高性能微波器件使用,还可用来开展超导薄膜或介质衬底材料的微波性能研究,在航天领域有望用于空间原子钟。文章对高温超导谐振器的原理、结构、各领域应用及国内外研究情况进行综述,并给出我国发展此项技术的建议。     

高温超导X波段带通滤波器研制

本文选用 10× 15× 0 .4 4 m m3双抛 L a Al O3衬底上外延生长的优质双面钇系高温超导 (HTSC)薄膜的Yba2 Cu3O7(YBCO) ,设计并制作了结构紧凑的高温超导发夹线微波窄带滤波器。该滤波器工作温度在 90 K以下 ,77K时指标为 :中心频率 9.4 8GHz,3d B相对带宽 1.1% ,带内最小插损 0 .36 d B,带外抑制大于 4 5 d B。另外 ,本文还介绍了高温超导滤波器的精确设计方法 ,并对高温超导滤波器的功率容载、制作等问题进行了讨论 ,同时还研制了具有实用意义的全密封高温超导滤波器外壳 ,仅需液氮制冷即可进入工作状态 ,输入、输出采用 SMA密封接头。     

高温超导滤波器国内外研究进展

近年来，国际上高温超导微波器件的应用取得了重大突破，国内的高温超导微波应用也取得了重要进展。文章介绍了高温超导滤波器的工作原理及其显著特点，回顾了国外高温超导滤波器的研究历史，详细叙述了国内近年在移动通信、卫星微波接收机和气象雷达三方面的应用情况。     

空间低频射电天文天线材质-观测性能分析

15MHz以下的射电天文信号由于受到电离层的阻挡只能通过空间卫星平台进行观测。采用空间展开的电小天线是目前普遍的做法。就电小天线的材质-接收性能方面进行分析，构建了基于材质磁导率、电导率对后端接收机噪声影响模型。通过计算结果比对和就天线材质空间展开难易程度的综合考虑，归纳总结了不同材质对空间低频射电天文观测噪声影响以及展开难度，为新天线的研制提供了数据依据。该项工作将为下一步L1点空间天气监测卫星中的太阳射电观测载荷提供技术支持。     

微波MEMS滤波器的研究进展

文章介绍了应用于射频微波系统的MEMS滤波器,结合最近几年国内外的MEMS滤波器研究成果,从MEMS滤波器的设计方法和滤波器性能等方面阐述了各种MEMS滤波器的技术发展状态。     

复杂电磁环境下雷达侦察系统的干扰抑制方法

研究了复杂电磁环境下雷达侦察系统的干扰抑制技术,分析了某雷达侦察系统采用的几种抗干扰方式,用试验数据论证干扰抑制方法的可行性,并指出其优势和劣势。最后展望了该领域的趋势和前景。     

高分三号卫星测控分系统设计与验证

高分三号(GF-3)卫星具有大角度快速机动及复杂电磁环境的特点,测控分系统常规设计难以满足卫星需求。文章提出射频设备的抗干扰设计及验证方法,介绍了GF-3测控分系统的设计、技术特点,并给出了地面试验及在轨运行验证结果,实现了测控分系统高灵敏度接收与大功率合成孔径雷达(SAR)之间复杂环境的电磁兼容性,同时首次采用高精度实时快速导航定位算法和自主健康管理方法,实现了导航子系统快速连续定位。     

伪码测距抗干扰容限分析

统一考虑射频干扰对伪码测距系统中码环稳定性能和测距精度性能的影响,推导并定义了系统稳定性能容限和测距精度性能容限,综合这两个容限给出了一定测距精度指标约束下的测距抗干扰容限。同时,设计了容限参考因子以定量分析两个性能容限对测距抗干扰容限的影响,并给出了一定应用场景中的容限和参考因子的快速计算方法。本文还针对窄带干扰环境,给出了更加简捷的分析方法,并通过数值分析进行了具体说明。测距抗干扰容限的分析与设计,科学全面且简捷高效,能够有效指导伪码测距系统的结构参数设计与系统性能评估。     

提高电子仪器电磁屏蔽性能的方法

要提高电子仪器可靠性，对电磁干扰和抗干扰技术需要进一步研究。有关电子仪器电磁屏蔽的机理和设计方法在本文中作了介绍。     

High Throughput Satellite System Capacity Analysis and Application Forecast

With the development of large numbers broadband Internet access,global satellite communications is moving towards High Throughput Satellites(HTS).Now,USA,Canada,Europe,Thailand,Japan,United Arab Emirates,Australia have already developed HTS systems.However,there is little research to analyze the factors influencing high throughput.Thus,from the design perspective,the throughput of HTS and influencing factors are calculated and compared at a system level.Finally,the application of HTS is analyzed and forecasted.     

四维超混沌射频隐身跳频通信设计方法

为提高飞行器通信系统的抗截获性能，提出了一种基于四维超混沌系统的射频隐身跳频通信设计方法。该方法构建了四维超混沌系统，扩展了系统解空间，有效增加了系统复杂度，并通过引入周期性扰动措施，解决了有限精度带来的短周期现象。在四维超混沌系统的基础上，利用超混沌系统生成的双通道超混沌序列，实现了跳频通信系统的频率序列和周期序列联合不确定设计方法。仿真结果表明：四维超混沌系统与传统混沌系统相比，其复杂度最优，在相同有限精度条件下，超混沌系统的周期性明显减弱。另外，基于四维超混沌设计的跳频系统，其截获概率优于常规跳频系统，具有较好的射频隐身性能。     

The gravitational lenses of alpha centauri a, b, c and of barnard''s star

The gravitational lenses of the three nearest stars, Alpha Centauri A, B and C (Proxima Centauri), are studied in this paper. For each star, the minimal focal distance is found, and turns out to equal 679.263, 563.485 and 112.138 AU, respectively, plus or minus the (large) uncertainties deriving from the uncertainties in the estimates of the star masses and radii. A comparison of these three minimal focal distances against the corresponding value for the Sun (550 AU, or, more correctly, 548.230 AU) is then made, but it is clearly pointed out that all these minimal focal distances are just the theoretical values given by Einstein's deflection formula for the corresponding “naked star”, i.e. the star as if it had no corona around! The study of the true focal distances that follow from taking the corona into account is much more difficult and uncertain, and has to be delayed to further research. For the naked stars, we study the deflection of radio waves for five different frequencies: the hydrogen line at 1.420 GHz, the water maser at 22 GHz, NASA's Interstellar Probe (ISP) telecommunication frequency at 32 GHz (K_a band), the Cosmic Microwave Background peak frequency at 160.378 GHz and finally the positronium frequency at 203.385 GHz. For each frequency the antenna patterns of the three naked stars gravitational lenses are given. Finally, all the above data are derived also for the fourth star in increasing distance from the Sun, Barnard's star.     

The SERENDIP SETI project: new instrumentation for SETI and results of recent observations

Over the past 30 years research into the existence of extraterrestrial life has focused on attempts to detect stable narrowband radio signals emitted in the microwave portion of the radio frequency (RF) spectrum. The SERENDIP SETI group is currently conducting search operations on the world’s largest radio telescope at the Arecibo Observatory in Puerto Rico.The third generation SERENDIP system, SERENDIP III, is a 4 million channel FFT-based spectrum analyzer with 0.6 Hz frequency resolution. In this paper, we will discuss the results of our recent 3.5 year sky survey. SERENDIP looked at 95% of the sky visible from Arecibo in the 424–436 MHz range, analyzed 10¹⁴ spectral bins, and logged information on over 2.5×10⁸ signals.The fourth generation SERENDIP system expands on the SERENDIP III design. SERENDIP IV computes 2×10¹¹ operations each second, providing spectral analysis on 160 million channels in 1.7 s. We will discuss the design and use of the SERENDIP IV system and future observing plans.     

Frequency management and SETI: threats to SETI observations in the 1–3 GHz band

The nature of a SETI search makes observations uniquely vulnerable to radio frequency interference because the frequency of a possible ETI signal is unknown. Sensitive radio telescopes, sophisticated software and enhanced signal detection equipment are employed to detect faint signals in the 1–3 GHz frequency range. Frequency management at SETI occurs within a policy environment of the ITU spectrum allocation process. Increased demand by commercial satellite services for access to spectrum adjacent to bandwidth allocated to radio astronomy creates severe international and domestic pressures on SETI observations. Strategies for addressing the RFI problem at the international level will be discussed that include a contingency ITU allocation plan for exclusive use of a particular frequency range by SETI in the event a signal is detected. The lunar farside is, by international agreement, a radio quiet zone for use by radio astronomers. Protected from most human-generated emissions, a SETI radio telescope array on the lunar farside would provide reliable data with minimum interference.     

中频软件无线电接收机的设计与实现

文章通过对软件无线电基本理论的研究,得出一种多相滤波数字正交变换的中频软件无线电结构,A/D的采样频率只有原采样频率的一半,这样就降低了对采样器件的要求。为了降低后续DSP处理速度需求压力,文中利用FPGA实现了多相滤波数字正交变换结构的延迟滤波,证明了这种结构的正确性和可行性。     

高温超导滤波器在航天技术中的应用

A way of the application of high temperature superconductive（HTS）filter in the space is presented,and advantages of the HTS filter used in the space technology field to improve the sensitivity of the receiver, reduce the noise factor of the receiver, decrease the antenna received area, increase the TT&C coverage of spacecrafts, and so on are analyzed. An on\|orbit verification device of the HTS filter is designed in this paper, this device has been successfully used in satellites of China.     

射频阵列仿真系统的目标位置精度分析

射频阵列仿真系统是一种比较理想的导弹武器系统抗干扰试验环境,目标位置精度是射频阵列仿真系统的关键指标。阐述了影响目标位置精度的主要原因,并结合测量数据对其进行分析,为工程应用提供了参考。