空间激光通信系统中的信道纠错编码技术

由于空间激光通信系统的信道状态和链路捕获跟踪的不确定性,多种形式的信道纠错编码技术正被广泛发展研究。结合空间激光通信链路中误码性能的主要影响因素,分别选择合适的编码方案进行分析。通过仿真实验可知,对于在大气结构参数为1.5×10~(-14) m~(-2/3)、风速为20 m/s的空地激光链路的环境下,在系统数据速率为2 Gbit/s、要求误码率为10~(-6)时,LDPC码结合交织码相对未编码系统有3 dB的等效编码增益,LT码相对未编码系统有3.8 dB的等效编码增益。提供了一种能快速生成、扩展和校验的编码和交织实现方法,以抵抗大气湍流的快速变化对系统性能产生的影响。     

WSO-UV project

During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan.     

Do RadioAstron detections correlate with flaring states? An initial study of seven southern AGN

We examine the state of seven southern radio sources at the time of their RadioAstron AGN Survey observations. Both ATCA flux density monitoring data and Fermi light-curves are considered in determining the relative activity of the source. A simple hypothesis, that sufficiently compact source structure exists for detections on RadioAstron baselines when the source is in a flaring state, is qualitatively tested. We find four instances of RadioAstron detections during flaring radio states and four instances of RadioAstron non-detections during fading or quiescent radio states, in support of the hypothesis. However, we also find three instances of RadioAstron detections during quiescent or fading radio states, and two non-detections during a flaring state, indicating that the situation is (not unexpectedly) more complex. Radio and gamma-ray monitoring such as that described here, together with the full RadioAstron AGN Survey results, will allow a more thorough investigation of the dependencies of detections on baselines of >10 Earth diameters.     

基于CCSDS标准的航天器上行遥控链路 协议体系与可靠性技术

针对航天测控领域中上行遥控业务的协议体系选择与可靠性设计问题,在对我国现行国军标技术指标要求与现有航天测控系统天地基遥控技术特点进行归纳梳理的基础上,基于空间段信息传输无线链路特点与CCSDS(Consultative Committee for Space Data Systems,空间数据系统咨询委员会)标准规范,研究给出了适用于我国航天测控任务的空间段遥控协议体系与可靠性措施,利用梳理统计方法对上行遥控体制进行了数学建模分析,并与CCSDS给出的应用算例进行了对比分析.分析结果表明,所涉及的上行遥控体制与CCSDS标准规范的工作效能基本相当,能够满足我国航天任务上行遥控任务使用需求.     

航天测量船外测数据误差分析的小波方法

使用动态数据建模与误差分离技术以及小波分频方法,对船载外测数据进行处理分析,成功地分离出随机误差和船测数据特有的船体误差,并对船体误差给出了分析和合理的解释。结论表明,小波分频对认识和研究船测数据的误差是一种非常有效的方法。     

基于健康蜕化的航空发动机传感器故障诊断(英文)

改进在线故障诊断算法使其能适应发动机健康蜕化是目前故障诊断所面临的困难,如果诊断算法没有自适应能力,在发动机健康蜕化后将失去其诊断功能。为了解决此问题,提出在线故障诊断算法,采用跟踪滤波器估计发动机的健康状况,机载模型根据跟踪滤波器的估计结果进行更新。更新后的机载模型能够与真实的发动机相匹配。这使得当发动机健康蜕化后在线故障诊断仍能保持其有效性。最后采用一组卡尔曼滤波器来对航空发动机传感器故障进行诊断与隔离。通过设计好的一组卡尔曼滤波器,能够诊断并隔离出故障。本文使用非线性发动机模型来验证此方法,仿真结果表明本文提出的在线诊断方法在发动机健康蜕化后仍能保持其有效性。     

连续爆轰发动机的二维数值模拟研究

介绍了连续爆轰发动机(Continuous detonation engine,简称CDE)的物理模型及爆轰波传播的物理机理,并对CDE流场的波结构进行了分析.使用两步化学反应模型对简化的CDE模型做了二维数值模拟研究.计算了圆柱面展开二维平面的多个爆轰循环过程.模拟结果较好地匹配了相关CDE实验所获得的流场结构.数值计算结果使我们可以更加透彻地理解CDE各方面的参数,对于CDE的进一步研究具有一定的指导意义.      

预爆管式脉冲爆震原型机试验研究

为了实现多循环吸气式脉冲爆震发动机（PDE）在较短距离内缓燃向爆震的转捩,降低主爆管通过障碍物触发爆震的内部阻力损失,设计了预爆管和主爆管以同种混气（汽油/空气）为工作介质的两相PDE原型机,试验研究了爆震燃烧过程。研究表明：当预爆管出口扩张角度为45°时,可以实现爆震波在主爆管内向衍射面上、下游传播;设计的预爆管式PDE原型机可以实现最高频率为66.7 Hz的稳定间歇工作。