Hi content in cluster and supercluster galaxies

In this lecture I review part of the published and unpublished observational evidence showing that cluster spiral galaxies are hydrogen deficient. Always using observational data, it is argued that the deficiency is due to the interaction between the galaxies and the intergalactic medium. Furthermore it is shown that the stellar population of deficient galaxies has also been affected and a brief discussion is given of the mechanisms at work.     

北京航天指控中心卫星任务数字仿真软件的设计

首先给出了北京航天指控中心仿真软件的设计模型,阐述了仿真软件仿真的内容,并详细介绍了仿真软件的总体结构和关键进程的设计方法,最后显示了仿真的结果,在实际应用中该软件得到了验证。     

Investigating the Coronal Mass Ejections associated with DH type-II radio bursts and solar flares during the ascending phase of the solar cycle 24

We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (～62%), while the partial HCMEs comprised ～35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts.     

机载综合无线电平台的中频数据传输总线优选分析

在综合无线电平台中，根据硬件平台通用化要求，需要选择一种总线同时满足CNI 不同波形的中频 数据传输对延时、带宽和误码率的要求。本文针对不加协议的GTX 和加上高速串行通信协议的Aurora、SRIO 进行测试，得到这三种高速串行总线在延时、带宽和误码率的对比分析，从而选择一种总线作为多波形综合的 中频数据传输总线。     

K8V变稳飞机飞行试验验证系统

介绍了Ｋ８Ｖ变稳飞机飞行试验验证系统的组成及功能,分别阐述了该系统的飞控软件综合验证子系统、机上地面试验数据采集与处理子系统和飞行试验数据处理分析子系统等三部分的组成、工作原理、以及在飞行试验各个阶段的不同特点和作用。通过Ｋ８Ｖ变稳飞机飞行试验的应用,表明该系统能够满足变稳飞机的软件维护、系统验收试飞及后续的应用研究,具有实时,快速,准确,自动化等优点,可为Ｋ８Ｖ变稳飞机应用研究提供重要的支持手段     

宇宙噪声的电离层闪烁与电离层不规则结构的结构参数

利用宇宙噪声是均匀的。各向同性的背景电磁辐射的假设,对电子密度涨落空间分布波数谱为负幂律函数的电离层不规则结构,用射线光学方法导出了闪烁功率谱的表示式。与射电星和轨道人造卫星信标的电离层闪烁相比,减少了因相对运动弓队的变量。用数值计算方法研究了电离层不规则结构的结构参量L_y、l_y、p、η对功率谱的影响。与实测资料比较,发现电离层吸收事件期间且Riometer记录的闪烁资料中,60%以上相应的不规则结构有L_y>103,η>η₀(0.2<η₀<0.5).      

基于卷积盲分离的强干扰下通信信号分离算法

针对目前通信辐射源个体识别算法在实际试验中由于各类干扰信号和多径衰落导致识别率较低的问题,提出一种用于识别算法前端的信号分离算法,可有效地减少其他电磁信号对于识别算法输入信号的影响,从而提高在复杂电磁环境中通信辐射源个体识别的正确识别率。该算法将灾变策略和搜索状态的自适应引入量子粒子群算法,通过对混合信号的联合对角化从截获的观测信号中提取出目标通信辐射源的有用信号。为了更加系统、直观地衡量算法的分离效果,提出分离熵来量化算法的整体性能。仿真结果表明,该分离算法可以把目标通信辐射源的有用信号从复杂电磁环境中提取出来,从而提高通信辐射源个体识别在复杂电磁环境中的正确识别率,具有较好的可行性和有效性。     

TlcsVTE原型中功能覆盖率算法的实现

TlcsVTE原型是针对某型号上位测控软件研制的测试环境,旨在对该型号的上位测控软件进行确认测试。本文重点阐述TlcsVTE中功能覆盖率算法的实现思路。该算法是基于被测软件运行环境的体系结构以及被测软件的功能分解进行设计的。该原型中采用了本文所述的算法辅助测试人员对被测软件进行功能测试以及覆盖率的实时统计。应用该原型测试被测软件,功能覆盖率可达100%。     

脉冲多卜勒引信实时校准技术初步研究

脉冲多卜勒引信实时校准技术主要对引信回波模拟源的无线电引信技术指标进行准确评定,以达到校准的目的。目前对该类专用测试设备的校准仍停留在分项校准的状态,无法全面地对整个专用测试设备进行评定,本文利用"宽带数字接收+软件无线电"技术和解调算法,实现对引信回波模拟源的系统级校准的目的。     

陆基超远程无线电导航发展研究

定位导航和授时(PNT)系统是保障现代社会正常运转必不可少的基础设施,为了提供可靠的PNT信息服务,需要研发不依赖于卫星导航的PNT系统。介绍了国内外陆基超远程导航系统的发展情况,提出了发展基于甚低频无线电信号的陆基超远程无线电系统架构、关键技术及发展建议,陆基超远程导航系统可以在卫星导航不可用时提供备份,对于构建冗余可靠的国家PNT体系、保障PNT信息的安全及可靠性具有重要意义。