基于IEEE-1394b的惯导数据传输系统设计

针对惯导系统中应用较为成熟的RS232、RS422、RS485、CAN 等数据传输 方法传输带宽低、可靠性低、距离近并且引入电磁干扰等问题,将基于IEEE-1394b 的光 通信引入惯导系统。利用惯导系统中FPGA 资源配合物理层芯片和光电转化模块,搭建 基于IEEE-1394b 的数据传输系统。详细介绍了各个模块的工作流程,为满足数据传输特 殊需求对链路层请求方式和数据包进行惯导专用化改进。借助QuartusⅡ 集成开发环境 提供的SignalTapⅡ逻辑分析仪进行验证。结果表明,数据传输系统可以使用立即请求发 送广播形式的异步数据包,也可以进行点对点异步数据传输,实现了预期目标。该方法 不仅屏蔽了惯性导航系统的外界电磁干扰,还实现了惯导系统的大带宽、高可靠传输, 具有很高的工程应用价值。     

基于线粒体COI基因序列的挂墩稻弄蝶分类地位研究

对稻弄蝶属Parnara 4种20个样本的线粒体COI基因序列(1 380 bp)的特征、遗传距离进行了分析,并以2种谷弄蝶Pelopidas为外群,采用最大简约法(MP)和贝叶斯法(BI)构建系统树.结果表明:种间最小序列差异为3.3%,种内个体间最大序列差异为0.9%;系统树显示挂墩稻弄蝶Parnara batta与直纹稻弄蝶Parnara guttata是2个明显不同的分支;其种间的平均遗传距离为3.5%.综合地理分布与形态差异,挂墩稻弄蝶应该是一个独立的种.     

Turbo码在802.11b协议物理层中的应用研究

给出用 Turbo码代替现行 80 2 .11b协议中物理层的信道纠错码——卷积码的方法 ,通过性能仿真和译码复杂程度比较 ,验证在该协议的物理层上采用 Turbo码来提高无线局域网的性能是可行的。     

航空电子系统的光纤网络结构与技术

针对先进航空电子系统对数据网络的高速和混合通信的需求,基于分布式控制、实时存取和故障容忍的设计思想,进行了分布式光纤网络的结构设计和协议选择.重点分析了光纤链路、介质访问控制协议、拓扑、容错技术和网络管理软件.分析结果表明,基于1394b总线的分布式容错光纤网络能提供确定和可靠的通信,同时该吉比特光纤链路满足误码率要求且功率余量达13dB.因此它是具有高带宽、低延迟和易扩展优势的高综合网络结构.      

Upgrade of the GOCE Level 1b gradiometer processor

This paper describes the upgrade of the GOCE Level 1b gradiometer processing as part of ESA’s Payload Data Segment (PDS). Four processing steps have been identified which can be improved: 1. The optimal determination of the angular rates of the satellite, based on a combination of star sensor and gradiometer data. This is the so-called angular rate reconstruction. 2. The optimal determination of the spacecraft’s attitude, again based on a combination of star sensor and gradiometer data. 3. The combination of data of all simultaneously available star sensors. And, 4. the calibration of the measured accelerations is improved by taking the time dependence of selected calibration parameters into account.     

HCFC-141b 型聚氨酯泡沫塑料耐环境性能

对比分析经历模拟特定环境的环境交变试验、盐雾试验、加速老化试验和太阳辐射试验前后泡沫塑料的压缩强度、闭孔率、线胀系数和热导率等性能。结果表明,HCFC-141b型聚氨酯泡沫塑料经历环境老化后,压缩强度和热导率增加,线胀系数减小,闭孔率略有增加,热导率增加。太阳辐照试验对泡沫性能影响最大,试样SD-4压缩强度提高32%,闭孔率先增加后减少,线胀系数降低19%,热导率升高30%。     

Plant mineral nutrition,gas exchange and photosynthesis in space: A review

Successful growth and development of higher plants in space rely on adequate availability and uptake of water and nutrients, and efficient energy distribution through photosynthesis and gas exchange. In the present review, literature has been reviewed to assemble the relevant knowledge within space plant research for future planetary missions. Focus has been on fractional gravity, space radiation, magnetic fields and ultimately a combined effect of these factors on gas exchange, photosynthesis and transport of water and solutes.     

Gamma rays from accreting matter onto collapsed objects

In the spherical accretion onto massive objects, the matter may be heated up to temperatures as high as 10¹² °K. In such a hot plasma, the thermal bremsstrahlung (e-e and e-p) and π° decay from inelastic collisions of protons are the main γ-ray sources. We determined the γ -ray production spectra from the π° decay and from bremsstrahlung for different temperatures. The expected γ-ray spectra were evaluated too in order to fit experimental data. We have fitted COS B data from 3C 273 using a two temperatures plasma model. The best fit is for

Full-size image (1K)

(M₈ is the black hole mass in 10⁸ M) which gives . The hard X-ray measurements do not contradict the bremsstrahlung spectrum.     

γ-ray spectroscopy in Mars orbit during solar proton events

Understanding the evolution of Mars requires determining the composition of the surface and atmosphere of the planet. The European Space Agency’s ExoMars rover mission, which is expected to launch in 2016, is part of the Aurora programme. The instruments on the rover will search for evidence of life on Mars and will map a sub-section of the Martian surface, extracting compositional information. Currently our understanding of the bulk composition (and mineralogy) of Mars relies on orbital data from instruments on-board satellites such as 2001 Mars Odyssey, Mars Reconnaissance Orbiter and Mars Express, in addition to in-situ instrumentation on rovers such as Spirit and Opportunity. γ-ray spectroscopy can be used to determine the composition of Mars, but it has yet to be successfully carried out in-situ on Mars. This study describes some of the results obtained from the γ-ray spectrometer on 2001 Mars Odyssey during solar proton events and discusses whether the increased emissions are useful in γ-ray spectroscopy. The study shows that although increased γ-ray emissions were expected from the Martian surface during a solar proton event, they were not detected from orbit probably due to insufficient signal-to-background. However, this does not preclude the possibility of measuring changes in γ-ray flux corresponding to changes in solar activity on the surface of the planet.