Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.     

K4169高温合金组织细化研究

研究了 K4 1 6 9高温合金在不同浇注温度及向熔体中加入细化剂时的晶粒组织。结果表明 ,降低浇注温度可以明显细化凝固后基体的晶粒和提高铸件断面等轴晶的比例。在通常的浇注温度 1 4 0 0℃和 1 4 2 0℃下 ,并对合金熔体进行均匀化处理时 ,加入所研制的复合细化剂可使圆柱锭的晶粒分别细化至 ASTM1 .7级和 ASTMM1 0 .5级 ;断面等轴晶的比例分别达 96 %和 90 %以上。本文提出了晶粒细化的机理并分析了晶粒细化后断面等轴晶比例增大的现象     

TH230无线数传电台工作原理及应用

ＴＨ２３０是集成无线和数传专业技术，用于数据传输、无线遥控的多功能电台。介绍ＴＨ２３０专业无线电台的工作原理及其在供配电系统中的应用。     

亚毫米波大气传输计算及分析

主要研究了在近亚毫米波段的大气传输特性，通过分析红外区和毫米波区的大气２模型，给出了亚毫米波段的大气传输模型参及加权项的表达形式。在吸收模型的理论的基础上，推导了以宏观气象条件为参变量的解析表达式，并由实验数据加权后的模型进行了验证分析，加权模型与实验数据基本吻合。在散射模型中，提出了以粒子的统计分布均值代替一般的密度分布，从而提高了计算精度。分别推导了Ｍｉｅ和Ｒａｙｌｅｉｇｈ散射系数求解的数学表     

多载波CDMA技术在航天测控通信系统中的应用

针对传统航天测控通信系统在测距精度、数据传输速率和抗干扰等方面的不足，将多载波码分多路存取(MC—CDMA)应用于航天测控通信系统。该方法不仅可以使测距精度达到数米，数据传输速率达到几十兆字节每秒，而且还具有抗干扰能力强、易于实现多目标测控和系统实现简单等优点。     

空间太阳望远镜高速数据传输系统设计

空间太阳望远镜(SST)是中国未来重要的太阳观测卫星，中国科学院国家天文台和航天部五院目前正在开展该卫星的研制工作。本文介绍高数据传输速率(60Mbps)的科学数据传输系统(DTS)，该系统将SST每天采集的超大容量科学数据传送到卫星地面站，其协议与国内卫星地面站现有协议兼容。文中分析SST对DTS的系统需求；计算DTS系统星地传输链路的系统余量；侧重描述DTS的信道编码卡(CEC)的详细设计，包括设计原理、方法和实验室基带测试系统，CEC格式化海量存储器中的科学数据，插入伪随机编码(PN)及帧同步信号，生成的数据流适应四相相移键控(QPSK)射频调制及地面数据恢复系统的需求。本文最后讨论DLS检错和纠错编、解码(EDEC)的实现方法，以及如何分别利用软件、硬件或可编程器件实现系统功能优化分配。我们已研制出CEC地面样机及其测试设备，并成功验证了CEC的全新设计方法，如使用较低的工作频率完成高数据速率的传送等。     

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.     

基于高级在轨系统的测控数传一体化方案

针对测控与数据传输信道一体化的需求,采用AOS(Advanced Orbiting System,高级在轨系统)空间链路层的等时业务,设计了一种测控数传信道一体化方案,可在上下行信道采用非相干信息帧同时传输测量信息及高速载荷数据.该方案设计了2种工作模式,模式一在上下行信道同时使用AOS传输帧,双向数据传输速率最高3 Mbit/s,测距精度优于2 m;模式二上行信道使用遥控扩频帧,可进行多站测距,抗多址干扰能力不低于15 dB,抗单频干扰能力不低于23 dB,下行信道使用AOS传输帧,最高数据传输速率3 Mbit/s,测距精度优于1 m.     

Wave propagation analysis for a second strain gradient rod theory

In this work, an enriched model describing the longitudinal wave propagation is established based on Mindlin’s Second Strain Gradient (SSG) theory, which can describe the heterogeneity caused by the micro-structure interactions in the frame of continuum mechanics. The governing equation and associated boundary conditions are derived based on Hamilton's principle, then the dispersion relation of non-classical longitudinal wave together with the extra-waves appearing exclusively in SSG theory model are investigated. The investigations are based on the modal density, energy flow, and forced response of the rod. Wave transmission and reflection through planar interfaces based on the proposed model have been calculated. Finally, the results of the enriched model are well interpreted by comparing with the classical theory results, and some useful conclusions are derived on the SSG theory based model in the wave propagation characterization.     

Time variations of the total electron content in the Southeast Asian equatorial ionization anomaly for the period 2006–2011

This study presents the time variations of the total electron content in the South East Asian equatorial ionization anomaly. The time variation of the TEC is analyzed through the period 2006–2011 by using a latitudinal chain of GPS stations extending in the northern and southern hemisphere. The data shows that the shape of the diurnal variation of the TEC depends on the latitude: a plateau is observed at the stations near the equator and a Gaussian at the station distant from the equator. We observe a semiannual pattern in all the stations with maxima at equinox. In both hemispheres, the amplitude of the crest is larger in spring than autumn from 2006 to 2008 and smaller in spring than in autumn from 2009 to 2011. We also observe an asymmetry between the amplitude and the position of the two crests of ionization. There is a very high level of correlation between the amplitude of the TEC at the two crests and the sunspot number: ∼0.88. During the deep solar minimum 2008–2009, the amplitude of crests of ionization becomes small during several months in summer and winter. The results show that both crests move significantly equatorward in winter than other seasons and there is a tendency for both crests to appear earlier in winter and later in summer.