C波段统一载波的微波集成下变频器

本文所介绍的是专为卫星工程地面站研制的C波段统一载波的微波集成下变频器。它具有三通道特性,每通道具有净增益20分贝,噪声系数小于8分贝,前中输出干扰电平小于12微伏。和与差信道问随机均方根相位差值小于0.3度;三通道间隔离度大于60分贝;一致性小于±0.5分贝。通过正确选择一本振频率,可以对27个信号进行跟踪和遥测。     

模型预测控制（MPC）在飞机自动着陆系统中的应用

进场着陆是飞行的复杂阶段,虽然仅占整个飞行的2%～3%,却大约有1/3的飞行事故发生在此阶段,而高速喷气式飞机的飞行事故有一半以上是发生在进场着陆阶段。本次仿真的对象是一种具有特殊外形的无人机,对侧向着陆精度要求很高。于是文中采取了预测控制器加经典PID控制器构成了分层控制系统。动态矩阵法的在线优化和反馈校正等特点有效地提高了系统的整体性能。结果表明,这种方法可以有效地提高着陆精度并严格控制接地时的滚转角。     

面向高安全数据分发服务的身份认证协议设计

为解决数据分发服务安全规范中身份认证与密钥协商协议存在共享密钥建立缺乏公平性、缺乏验证密钥一致性机制及会话过程缺乏完整性等安全问题,以协议为基础,设计一种新的高安全数据分发服务身份认证与密钥协商协议。新协议引入了ACK机制,并利用D－H密钥交换和非对称密码体制特点解决了原协议存在的安全问题,具备实用性和更高的安全性。     

双喷孔滑油喷嘴流动及流量特性的数值计算研究

为了研究双喷孔滑油喷嘴内部流动及流量特性,根据滑油喷嘴流动特点基于VOF (Volume of fluid)两相流方法建立了滑油喷嘴流动的数值计算模型。在验证数值计算方法可靠性的基础上,计算并分析了喷孔间距、孔径比和喷孔分布顺序对喷嘴流动及流量特性的影响。结果表明,双喷孔结构中各喷孔滑油流量均小于其单喷孔的滑油流量,孔径比相同时各喷孔流量与其单喷孔流量的差值均随喷孔距的增大而减小,孔径比为2.0、喷孔距为基准孔径的两倍时喷孔流量的最大偏差达到了4.4%;下游喷孔滑油流量随孔径比的增大而减小,孔径比越大、喷孔距越小时上游喷孔对下游喷孔的流动影响越大,下游喷孔流量与单喷孔流量相差越大,喷孔距为基准孔径的两倍、孔径比由1.0增大至2.0时下游喷孔的流量减小了2.8%;相同孔径喷孔在同一孔距下位于喷嘴主体上游时的滑油流量均大于其位于下游时的滑油流量,但滑油喷嘴总流量几乎相同。     

一种针刺C/C复合材料-40Cr配副的摩擦学性能

采用MMUD-10B型摩擦磨损试验机分别在干摩擦和水润滑两种不同环境下,固定转速为100 r/min,在不同载荷下(70、150和230 N)对摩擦配副C/C-40Cr进行摩擦学性能对比分析及表征。利用奥林巴斯GX51金相显微镜观察试样表面的磨痕、采用JJ324BC型的电子天平表征每次实验的磨损量、使用JSM-6510A型扫描电子显微镜(带有EDS能谱仪)观察磨屑的形貌及各元素的原子比。结果表明:在干摩擦中,试样的摩擦因数较大,在0.046～0.070波动,磨损量较少,且摩擦因数与磨损量随着载荷的增加而增加;在水润滑摩擦情况下,摩擦因数变化范围较小,在0.037～0.052,但磨损量较大。干摩擦和水润滑条件下的摩擦因数和磨损量与载荷的大小呈正相关趋势。此外磨屑中稳定存在碳纤维和片层状的40Cr,磨损机制为黏着磨损和磨粒磨损共同作用。     

导弹电子设备故障的组合预测方法研究

针对传统GM(1,1)的对纯指数型序列预测的局限性,引出了改进的离散灰色DGM(1,1)模型。应用DGM(1,1)模型与时间序列AR模型的组合模型对导弹电子设备进行故障预测,并通过实例对预测精度进行了检验。     

N2O单组元推力器预热过程有限元分析

以正交试验设计理论为指导,应用有限元分析软件针对采用N₂O推进剂的单组元微推力器的在真空环境下的预热过程开展了分析,计算结果表明加热功率及推力器外表面辐射率的大小对预热效果影响明显.所开展的微推力器壳体地面预热试验的试验结果与仿真计算结果吻合良好,验证了采用仿真方法来评估预热过程的可行性.为进一步的结构及试验设计提供了借鉴.      

The Search Coil Magnetometer for THEMIS

THEMIS instruments incorporate a tri-axial Search Coil Magnetometer (SCM) designed to measure the magnetic components of waves associated with substorm breakup and expansion. The three search coil antennas cover the same frequency bandwidth, from 0.1 Hz to 4 kHz, in the ULF/ELF frequency range. They extend, with appropriate Noise Equivalent Magnetic Induction (NEMI) and sufficient overlap, the measurements of the fluxgate magnetometers. The NEMI of the searchcoil antennas and associated pre-amplifiers is smaller than 0.76 pT $/\sqrt{\mathrm{Hz}}$ at 10 Hz. The analog signals produced by the searchcoils and associated preamplifiers are digitized and processed inside the Digital Field Box (DFB) and the Instrument Data Processing Unit (IDPU), together with data from the Electric Field Instrument (EFI). Searchcoil telemetry includes waveform transmission, FFT processed data, and data from a filter bank. The frequency range covered depends on the available telemetry. The searchcoils and their three axis structures have been precisely calibrated in a calibration facility, and the calibration of the transfer function is checked on board, usually once per orbit. The tri-axial searchcoils implemented on the five THEMIS spacecraft are working nominally.     

The GGS/POLAR magnetic fields investigation

The magnetometer on the POLAR Spacecraft is a high precision instrument designed to measure the magnetic fields at both high and low altitudes in the polar magnetosphere in 3 ranges of 700, 5700, and 47000 nT. This instrument will be used to investigate the behavior of fieldaligned current systems and the role they play in the acceleration of particles, and it will be used to study the dynamic fields in the polar cusp, magnetosphere, and magnetosheath. It will measure the coupling between the shocked magnetosheath plasma and the near polar cusp magnetosphere where much of the solar wind magnetosphere coupling is thought to take place. Moreover, it will provide measurements critical to the interpretation of data from other instruments. The instrument design has been influenced by the needs of the other investigations for immediately useable magnetic field data and high rate (100+vectors s^–1) data distributed on the spacecraft. Data to the ground includes measurements at 10 vectors per second over the entire orbit plus snapshots of 100 vectors per second data. The design provides a fully redundant instrument with enhanced measurement capabilities that can be used when available spacecraft power permits.     

火箭燃气喷流的数值和实验研究

通过数值计算和实验,研究了２１和９火箭发动机燃气喷流流场。数值计算采用激波高分辨率、二阶精度ＴＶＤ格式,得到包括射流边界、桶形激波、反射激波、Ｍａｃｈ盘和滑移线的清晰的流谱。实验测试应用Ｆ－Ｐ激光干涉仪和自动测压系统,得到流场Ｆ－Ｐ干涉照片和压强分布。计算结果与实验结果符合较好