Bolometric luminosities and brightness temperatures of BL Lac Objects and FR I radio galaxies

To understand the connection among the subclasses of BL Lac Objects, FR I radio galaxies and Flat spectrum radio quasars (FSRQs), here the correlations of the bolometric luminosities with redshifts and brightness temperatures of these objects are studied. The bolometric luminosities vary linearly with redshifts, but few objects are scattered at high redshift. The bolometric luminosity versus brightness temperature distribution shows a correlation between these two components, except a few scattered objects, mostly RBLs. The bolometric luminosities and brightness temperatures of FR I radio galaxies with low redshift (<0.1) and low spectral index (α_rx < 0.75) are comparable to those of XBLs and those characteristics of FR I radio galaxies, with relatively high redshift (>0.2) and high spectral index, can be comparable with RBLs with low redshift (z < 0.5) and low bolometric luminosity. Those scattered RBLs with high redshifts (z > 0.5) are believed to be in complex environment with companion galaxies, most of these RBLs are still unresolved. The bolometric luminosity and brightness temperature of these scattered RBLs are comparable to those of quasars. The FSRQs are at high redshifts and bolometric luminosities and the brightness temperatures are also high relative to BL Lac Objects. These results support the FRI/BL Lac unification scheme. It suggests that, the FR I radio galaxies may be the parent populations of the BL Lac Objects, but it needs more investigation to confirm the unification of FR I radio galaxies, XBLs and RBLs.     

轴对称推力矢量喷管冷态多柔体动力学仿真

采用实体板壳单元对矢量喷管关键部件进行了柔性化,基于机构的树状参数化处理技巧和MSC.ADAMS软件的宏命令批处理技术构建了矢量喷管的多柔体动力学仿真模型,模型中使用点线约束简化了部分接触约束,极大减小了计算规模.仿真了机构的冷态同步、摇头和摆头等工况,获得了机构各环节的受载和动态特性.研究工作对于矢量喷管的热态仿真及其虚拟设计和虚拟实验具有重要指导意义.      

Method of the HF wave absorption evaluation based on GIRO network data

High frequency (HF) communication is strongly dependent on the state of the ionosphere, which specifies the mode structure of the radio wave propagating in ionosphere. Another core factor defining the strength of the HF signal at the receiving site is the ionospheric absorption. Accurate modelling the effect of absorption is an essential part of many studies of the HF propagation in the ionosphere.This paper proposes a method for estimating the absorption. The method is based on analysis of vertical sounding ionograms. The main idea of the approach is to compare the main parameters retrieved from measured and simulated ionograms. The combination of Global Ionospheric Radio Observatory (GIRO, http://giro.uml.edu) data and ionograms modelling allows for developing the empiric absorption model available at near real-time. The ionogram simulation taking into account absorption utilizes the NIM-RT (North Ionospheric Model and Ray Tracing) software. As a result, the proposed technique provides more reliable and accurate evaluation of minimum frequency at which echoes are observed in vertical incidence ionosonde soundings. The values of these frequencies should be used in the following simulation to optimize parameters in the empirical formulae for defining absorption HF wave in ionosphere.The ultimate objective of this work is the designing the method, which allows the simulating of HF radio channel accounting for regular absorption due to UV radiation of the Sun. Eventually it could be considered as some kind of the HF propagation forecasting.     

一种基于探测器下行信号融合处理的无线电干涉测量方法

针对深空探测器常用下行信号体制,结合无线电干涉测量特点,提出了一种基于探测器DOR信标信号和数传信号融合处理的干涉测量方法。该方法首先通过相关处理得到DOR信号和数传信号的差分相位,利用DOR信号进行带宽综合得到时延估计,并构建时延模型;然后,利用时延模型得到DOR信号与数传信号在数传载波处的相位差,并以此对数传信号差分相位进行补偿;最后,利用DOR信号差分相位和补偿后的数传信号差分相位进行带宽综合,实现高精度干涉测量。深空探测网数据处理结果表明融合处理后时延估计随机误差明显降低;但受介质时延误差影响,融合处理对系统时延精度的改善幅度有所减小。该方法仅通过改进干涉测量数据处理方法即实现了时延估计随机误差的改善,不仅提高了信号使用效率,而且增强了航天测控系统的鲁棒性,在应急测控背景下具有特殊意义。     

非接触式超声泄漏检测系统设计及试验验证

非接触式超声泄漏检测方法在国外已应用于载人航天器在轨检漏。文章基于气体泄漏超声产生机理及声压与泄漏量的关系,搭建了一套超声泄漏检测系统,研究了泄漏判断及漏孔评估算法,并进行了综合试验测试。结果表明,该方法能有效地对泄漏是否发生进行判断,并可粗略评估泄漏量的大小和漏孔直径,为我国空间站密封舱在轨泄漏检测提供参考。     

基于直接升力与动态逆的舰尾流抑制方法

在复杂的作战和着舰环境下,舰尾气流扰动是着舰误差的最主要来源之一。如果在着舰下滑阶段利用直接升力控制（DLC）的快速性和解耦性能力,可以极大地减轻飞行员着舰操纵负担并且提高着舰最后阶段对舰尾流的抑制能力。从航迹调节和姿态稳定的解耦角度出发,提出在非线性动态逆（NDI）控制框架下实现基于直接升力的着舰控制律方法,并通过建立含有舰尾流扰动的E-2C全量飞机仿真模型进行验证。结果表明：在非线性动态逆控制中引入直接升力的舰载机着舰控制律,可以实现在着舰下滑阶段姿态稳定的同时,通过直接升力快速解耦调节航迹误差,并且在引入舰尾流干扰的情况下,具有快速修正下滑倾角误差、抑制舰尾流干扰的能力,最终达到显著提高着舰精度的效果。     

月球探测器天文测角/单程无线电时间差分测距/差分测速导航方法

月球探测器高精度导航技术是确保月球探测任务顺利实施的关键技术之一。当前,大多数月球探测器都是利用地面无线电进行导航和控制,但存在可测控弧段短、易受干扰等局限性,且对于月球背面探测,存在无法直接测控的不足。针对上述问题,提出了一种新的基于天文测角/单程无线电差分测距/差分测速的月球探测器组合导航方法。该方法使用了天文星光角距、探测器接收到的来自地面站或中继星的单程无线电时间差分测距和时间差分多普勒测速3种量测信息,可有效抑制星上时钟和频谱仪的时间和频率测量误差。收敛后的平均位置和速度估计误差分别为902.7 m和0.12 m/s,最大的位置和速度估计误差分别为1 548.2 m和0.24 m/s。仿真分析结果表明该方法具有较高自主导航精度。     

一种基于认知无线电的卫星网络信道接入策略

针对可用无线信道资源紧张与固定信道分配方式导致卫星网络信道利用率低下的问题,提出一种基于认知无线电的卫星网络信道接入策略。卫星用户以分时多址（TDMA）方式接入卫星信道,认知用户通过频谱感知发现卫星网络闲置信道资源,并以S-ALOHA方式接入信道。通过建立基于频谱感知与具有捕获效应的认知用户信道接入模型,分析认知用户最佳频谱感知时间,推导干扰信号在相干叠加与非相干叠加条件下的卫星网络吞吐率性能,并对影响网络吞吐率的因素进行仿真分析。结果表明,该信道接入策略能够在不明显降低高负载时卫星网络吞吐率的前提下有效提高低负载条件下的卫星网络吞吐率,且干扰信号相干叠加比非相干叠加对网络吞吐率性能的提升更为显著。     

光学线阵相机在轨几何定标平台设计与实现

文章采用一种基于探元指向角和相机安装角的星载线阵相机在轨几何定标模型,设计了适合于不同几何成像特点的在轨几何定标模式和流程,并对定标过程中的关键技术环节进行了分析说明。在此基础上设计并实现了星载线阵相机在轨几何定标软件,最后选择资源系列卫星数据,利用软件进行了实验验证。实验结果表明,设计和实现的多个模式定标软件能高效、高精度地完成多星、多相机的在轨几何定标任务,具有兼容多模式定标要求、可扩展至其他卫星型号的特点,能够作为统一的在轨几何定标软件平台。     

载人航天器的精细化软件研制技术管理方法

载人航天器软件研制具有技术新、难度大、新研配置项多等特点,必须研究一种新型的软件技术管理方法,以确保软件产品质量受控。文章介绍的精细化管理方法是在现有软件研制规范的基础上,通过软件研制工作的阶段化以及软件管理工作的划分,实现了软件的精细化管理。“天宫一号”目标飞行器软件研制工作的实践证明:该方法符合载人航天器型号研制的实际,可保证软件产品质量满足飞行任务要求。