频域盲源分离的非圆信号推广

作为盲源分离（BSS）问题的最有效解决方法之一,独立分量分析（ICA）算法可以分为时域和频域算法两类.将时域盲源分离的快速算法推广到频域,通过在频域中应用非圆信号的伪协方差矩阵,推导出一个新的固定点算法来解决线性瞬时混合的非圆信号盲源分离（BNSS）问题.仿真实验验证了该算法的有效性.     

酸性磺酞类染料共振Rayleigh散射光谱法测定奈替米星

用共振Rayleigh散射（RRS）光谱研究了酸性磺酞类染料溴甲酚绿和溴酚蓝分别与奈替米星的相互作用.溴甲酚绿和溴酚蓝在酸性介质中分别与奈替米星相互作用,导致RRS光谱显著增强,最大的RRS峰分别位于606nm和572nm处,散射强度与奈替米星的质量浓度在一定的范围内成正比.此方法具有很高的灵敏度,对于奈替米星的检测限（3σ）分别为30ng/mL和10ng/mL,据此发展了一种测定奈替米星的新方法.     

星间链路在空间态势感知中的应用研究

通过对星间链路和空间态势感知系统国内外发展现状的分析,指出星间链路在空间信息有效获取、安全传输和实时应用以及保障空间态势感知系统战场生存能力等方面起着重要的作用.针对星间链路在未来空间态势感知系统中的应用需求,提出包含空间通信模型和空间导航模型在内的空间感知体系基本架构,并对该架构下星间链路的设计要求或者特点进行分析,指出星间链路应该具有灵活可变的星间路由策略和联网结构,并能够支持高速可变和安全可靠的星间数据传输.分别从空间网络和卫星节点2个层面提出了系统实现的关键技术,并给出部分关键技术的研究重点和研究方法.上述研究结果可以为星间链路及相关领域的研究工作提供一定的借鉴和帮助.     

中国深空网首次△DOR联合测轨试验分析

通过分析中国深空网首次△DOR（Delta Differential One way Ranging,双差分单向测距）联合测轨试验的干涉测量事后数据,重点从观测量随机精度、闭合时延等方面讨论了国内深空网与国内VLBI（Very Long Baseline Interferometry,甚长基线干涉测量）观测网、国内深空网与国际深空网的联合干涉处理情况,并与ESOC（European Space Operation Center,欧洲空间操作中心）数据处理结果进行了比对.试验结果表明：我国深空网已具备独立或联合开展深空探测器导航测轨的系统支持能力;深空站系统具备高速率数据接收、采集、记录、传输能力,采集数据处理精度优于1 ns;深空网干涉测量信号处理中心具备多体制信号的干涉处理分析能力,其分析精度与ESOC处理精度差异在0.1 ns量级.     

Multi-h CPM遥测信号的定时频率联合估计技术

针对Multi-h CPM（Multi-h Continue Phase Modulation,多指数连续相位调制）遥测接收机的符号定时和载波频率同步问题,在分析MLSD（Maximum-likelihood Sequence Detection,最大似然序列检测）度量值是符号定时偏差和频率偏差的凸函数的基础上,提出一种基于迟/早门和升/降频门的符号定时和频率同步联合估计算法,通过似然值比较,对符号定时偏差和频率偏差进行迭代估计;并对该算法进行仿真,得到不同参数下的同步性能,给出同步参数选择建议.仿真结果表明：将该算法应用到Multi-h CPM遥测系统中,可实现低信噪比信号的快捕和高精度同步.     

单天基平台测向的空间非合作目标跟踪

针对仅含角度测量信息的单个天基平台可观测性较弱的问题,提出了一种含脉冲机动检测的空间非合作目标跟踪算法,并设计了非合作目标实时跟踪数据处理流程.该算法利用抗差估计技术和UKF（Unscented Kalman Filter,无迹卡尔曼滤波）算法构造目标跟踪滤波器,并综合残差多项式拟合和新息分布特征等方法实现目标机动检测,在天基平台观测信息类型有限和观测几何较差的情况下,可以同时排除孤立野值和成片测量野值的影响,实现非合作机动目标的连续稳定跟踪.数值实验验证了算法的可行性和有效性,也表明了跟踪精度和可靠性与测量精度密切相关.     

涡扇发动机故障诊断硬件在回路实时仿真平台

硬件在回路仿真是发动机故障诊断算法由理论转向实际工程应用的重要阶段,但目前航空发动机故障诊断算法的研究多数处于软件数字仿真阶段。构建民用涡扇发动机故障诊断算法硬件在回路实时仿真验证平台,开发考虑健康退化的民用涡扇发动机多维调度分段线性化模型,分析并模拟仿真民用涡扇发动机的四类典型常见故障。经过对相关诊断算法进行实验验证,表明该平台及使用的模型和方法都是行之有效的,具有一定的工程使用价值。     

RF communications subsystem for the Radiation Belt Storm Probes mission

The NASA Radiation Belt Storm Probes (RBSP) mission, currently in Phase B, is a two-spacecraft, Earth-orbiting mission, which will launch in 2012. The spacecraft's S-band radio frequency (RF) telecommunications subsystem has three primary functions: provide spacecraft command capability, provide spacecraft telemetry and science data return, and provide accurate Doppler data for navigation. The primary communications link to the ground is via the Johns Hopkins University Applied Physics Laboratory's (JHU/APL) 18 m dish, with secondary links to the NASA 13 m Ground Network and the Tracking and Data Relay Spacecraft System (TDRSS) in single-access mode. The on-board RF subsystem features the APL-built coherent transceiver and in-house builds of a solid-state power amplifier and conical bifilar helix broad-beam antennas. The coherent transceiver provides coherency digitally, and controls the downlink data rate and encoding within its field-programmable gate array (FPGA). The transceiver also provides a critical command decoder (CCD) function, which is used to protect against box-level upsets in the C&DH subsystem. Because RBSP is a spin-stabilized mission, the antennas must be symmetric about the spin axis. Two broad-beam antennas point along both ends of the spin axis, providing communication coverage from boresight to 70°. An RF splitter excites both antennas; therefore, the mission is designed such that no communications are required close to 90° from the spin axis due to the interferometer effect from the two antennas. To maximize the total downlink volume from the spacecraft, the CCSDS File Delivery Protocol (CFDP) has been baselined for the RBSP mission. During real-time ground contacts with the APL ground station, downlinked files are checked for errors. Handshaking between flight and ground CFDP software results in requests to retransmit only the file fragments lost due to dropouts. This allows minimization of RF link margins, thereby maximizing data rate and thus data volume.     

Initiation characteristics of oblique detonation waves from a finite wedge under argon dilution

In this paper, the flow field characteristics of Oblique Detonation Waves (ODWs) induced by a finite wedge under argon dilution are studied by solving the Euler equations with a detailed chemical model of hydrogen and air. First, the effects of the expansion waves, argon concentration, geometric parameters, and Mach number on the ODW are discussed. The results show that the changes of these parameters may make the oblique detonation not be initiated. Then, the ODW initiation criterion of the finite wedge is summarized, as the characteristic length of the induction zone L_C and the characteristic length of the oblique wedge L_W meet the condition L_C/L_W < 1, the initiation of the ODW occurs; otherwise, it does not occur. What’s more, the Constant Volume Combustion (CVC) theory is applied to study the characteristic length of induction zone. It is found that CVC theory is more suitable for the “smooth transition” type of ODW flow field, the theoretical and numerical characteristic length in induction regions are in good agreement. This work is of great significance for the design of oblique detonation engines for hypersonic vehicles.     

DME询问信号捕获的设计与实现

捕获询问信号是DME地面设备的一个重要功能组成部分。现役的地面设备中大多使用的捕获单元为分离器件电路设计，其电路复杂，控制难度大，改进与维护成本高。针对这些问题，本文设计采用ADC结合FPGA作为主要功能器件，并通过软件算法完成数字滤波、脉冲峰值提取和半幅点计算，实现询问信号的识别与捕获。不仅大幅减少元器件的使用，缩小设备体积，还可提高扩展性与可靠性。结合机柜验证测试，结果符合设计要求。