动态测角仪测量误差检测方法研究

检测高速测角仪的测量误差,其检测（方法）装置必须有高的动态响应和高的检测准确度。介绍了动态测角仪测量准确度检测系统的检测原理、测量系统的总体设计及实验结果。     

微机对一种位移系统的点位控制

本文介绍了一个 Z—80单板微型计算机控制的位移系统。该系统以步进电机作为驱动器件,以光栅位移检测装置作为位移检测反馈器件,采用点位控制原理,形成一个闭环似移控制系统。该系统工作可靠,位移控制精度达到±2.5μm,并可扩展为多路并行的点位控制系统。     

VCR-2宽带接收机的设计与仿真

介绍了一种用于检测计算机视频信号电磁泄漏发射的宽带接收机,并给出其设计和仿真过程。     

数字近景摄影大尺寸三坐标测量系统V-STARS的测试与应用

介绍了数字近景摄影大尺寸柔性三坐标测量系统V—STARS的配置、测量原理和测量过程,对其三维坐标及平面度的测量重复性进行了实际测试,与激光跟踪仪进行了平面度的比对测试,并将V—STARS系统成功应用于某17m网状天线的型面测量与调整工程实践中。     

？abry—Perot测风干涉仪数据处理

针对自主研制的星载法布里一珀罗干涉仪（Fabry—Perot Interferometer,FPI）样机,介绍了Fabry—Perot（F—P）的测风原理和风速反演算法,阐述了F—P测风干涉数据的自动化处理方法,包括干涉条纹图像滤波、分割、细化和特征数据的提取．滤波包括中值滤波和背景补偿,分割采用区域平均灰度值阈值法,借助数学形态学计算填充和消除二值化条纹的断裂点和毛刺．最后,按照骨架提取思想细化成干涉条纹线条,提取其特征数据．应用VC＋＋编程语言开发软件平台,对上述F—P测风仪数据自动化处理方法进行了验证,结果表明其可行性高、适应性强．     

一种可扩展的末制导雷达通用检测系统

介绍了采用ＩＥＥＥ－４８８总线标准实现的末制导雷达通用检测系统,概述了其硬件的组成和系统特点。并针对末制导雷达的测试规程和要求,阐述了软件系统的模块化设计思想,介绍了采用虚拟面板和虚拟仪器技术的ＡＴＥ软件设计方法。     

泄漏检测技术在航天器中的应用

介绍了国内航天器应用的泄漏检测技术及国外先进的航天器泄漏检测技术和泄漏检测标准；分析了航天器泄漏检测技术的发展趋势。     

J2级经纬仪竖盘指标自动补偿误差不确定度

介绍了按照ＪＪＧ４１４—９４《光学经纬仪》检定、校准Ｊ２级经纬仪竖盘指标自动补偿误差时，依据“’９３国际指南”要求，对其测量不确定度进行的分析、计算。     

光电跟踪仪激光测距器性能检测方法研究

介绍了光电跟踪仪激光测距器的特点,提出了其重要性能指标一测距能力和精度的检测方法。采用半实物仿真技术测试反映测距能力的消光比参量;采用精密延时法,实现了测距精度的测量。检测装置的耦合透镜部件放置于平行光管靶面,容易与测试光电跟踪设备其它模块的装置进行集成。     

航天器发射过程故障容错控制

根据航天器发射过程的故障特点,提出了利用容错技术对其故障进行控制的设计方法。着重对故障信息的获取,故障检测与诊断方法的选择,故障容错控制方案及其实现等进行了介绍。     

薄板激光弯曲温度场的数值模拟与校验

采用MSC.Marc非线性有限元软件,对薄板激光弯曲过程中的温度场进行了数值模拟 ,得到了引起薄板激光弯曲变形的温度场的变化规律.通过温度传感器测量与激光扫描线相 对应的薄板下表面温度变化的规律来验证数值模拟的结果.模拟值与实测值基本吻合,表明 数值模拟结果可作为激光加工工艺参数选择的依据.     

成形极限预测韧性断裂准则及屈服准则的影响

将韧性断裂准则用于预测板材成形极限,通过数值模拟HS钢、IF钢和6111-T4铝合金3种板材在单向拉伸、平面应变和双向等拉等不同应变路径下的变形过程,获得试件中心区域主应变最大单元的应变历史,结合成形极限实验数据计算韧性断裂准则的材料常数;通过对接近平面应变变形路径下的模拟结果与实验获得的网格应变相比较分析了Hill48,Hill90和Barlat89 3种各向异性屈服准则对模拟获得的应变路径的影响.结果表明,Barlat89屈服准则可以较好地描述单元的应变路径;在此基础上比较了几种韧性断裂准则用于预测板材断裂成形极限的计算结果, Cockcroft-Latham准则和总塑性功准则的计算结果比较理想,材料常数的确定也较为简单.      

A European probe to comet Halley

A European probe to comet Halley is proposed. The probe's model payload consists of 8 scientific instruments, viz. neutral, ion and dust impact mass spectrometers, magnetometer, medium energy ion and electron analyzer, camera, dust impact detectors and plasma wave experiment. Fly-by of the comet Halley nucleus will take place on November 28th, 1985, at about 500 km miss distance. The main spacecraft serves as relay link to transmit the observed data to Earth. As probe, a modified ISEE 2 design is proposed. Because of the cometary dust hazard expected in the coma a heavy dust shield (27 kg) is required, consisting of a thin front sheet and a 3 layer rear sheet. The probe is spin-stabilized (12 rpm), has no active attitude and orbit control capability and uses battery power only to provide about 1000 Wh for a measuring phase. A despun antenna transmits up to 20 kbit/s, in X-band. The total probe mass is estimated at 250 kg. The 3 model development programme should start in mid 1981 with Phase B.     

W波段多注交错双栅行波放大器的高频特性

提出了一种采用平面线性排列的3个圆形电子注代替平面带状电子注的W波段交错双栅行波放大器微型化慢波高频结构,并重点对其行波传输特性和输入输出耦合特性进行了仿真设计和参数优化.结果表明,这种平面微型化高频结构的行波传输色散特性良好且有很大的工作带宽,所产生的强轴向电场分布非常有利于电子注与高频场的能量交换和相互作用.在保证平面微型结构中圆形注通道直径和带状注通道高度相同的情况下,得到的耦合阻抗是带状注交错双栅慢波高频系统2~3倍,为行波放大器高效率的注波互作用和高功率输出提供了新的研究思路.为了与该交错双栅高频系统相匹配,提出了一种更为简单易行的输入与输出耦合结构,仅采用三周期渐变过渡段就可以实现反射系数S₁₁在较宽频带内低于-20dB的良好结果,更有利于行波放大器未来的工程实现与应用.      

Multi-case Study of Current Sheet Flapping Motions Induced by Non-adiabatic Ions

In this paper, the y-component of magnetic field line curvature in the plasma sheet was analyzed, and two kinds of shear structures of the flapping current sheet were found, i.e. symmetric and antisymmetric. The alternating bending orientations of the guiding field are exactly corresponding to alternating north-south asymmetries of the bouncing ion population in the sheet center. Those alternating asymmetric plasma sources consequently induce the current sheet flapping motion as a driver. In addition, a substantial particle population with downward motion was observed in the center of a bifurcated current sheet. This population is identified as the quasi-adiabatic particles, and provides a net current opposite to the conventional cross-tail current.      

高温不锈钢的磨削温度测量与烧伤现象分析

针对高温不锈钢1Cr11Ni2W2MoV磨削过程中磨削区内部瞬时温度、磨削表面平均温度的测量方法以及工件表面平均温度与烧伤程度之间的关系进行了研究,分析了工件表面烧伤程度对材料金相组织的影响.通过研究得到了陶瓷结合剂CBN砂轮磨削1Cr11Ni2W2MoV时磨削区内部瞬时温度,证明工件表面的烧伤最直接因素是磨削表面的平均温度,在不同的磨削参数下,表面平均温度超过540℃就形成黄色的微烧伤,随着温度的升高,烧伤程度不断加重.同时,表面烧伤会使马氏体晶格变成细小的退火微晶变质层,烧伤越严重,微晶变质层的厚度越大.     

用不均匀钢带法测量对流换热系数的测量技术研究

对用不均匀钢带进行换热测量做了研究。制作了贴有14块扇形不均匀加热钢带作为测量面的换热盘。推导了计算不均匀加热钢带热流密度的三种不同的关系式,并对他们做了比较验证。计算了造成主要测温误差的热阻,方法是采用热电偶和热像仪相结合来比较他们的测温结果。对换热盘进行测试验证的结果表明其可以进行旋转盘的换热测量。通过换热实验,采用不均匀钢带加热、热电偶测温和遥测仪采集数据的方法,由测量出的盘面温度分布计算换热系数。     

ISEE-1 and 2 observations of field-aligned currents in the distant midnight magnetosphere

Magnetic field measurements obtained in the nightside magnetosphere by the co-orbiting ISEE-1 and 2 spacecraft have been examined for signatures of field-aligned currents (FAC). Such currents are found on the boundary of the plasma sheet both when the plasma sheet is expanding and when it is thinning. Plasma sheet boundary layer current structure and substorm associated dynamics can be determined using the two spacecraft, although for slow traversals of the FAC sheet the spatial/temporal ambiguity is still an issue. We often find evidence for the existence of waves on the plasma sheet boundary, leading to multiple crossings of the FAC sheet. At times the boundary layer FAC sheet orientation is nearly parallel to the X-Z GSM plane, suggesting ‘protrusions’ of plasma sheet into the lobes. The boundary layer current polarity is, as expected, into the ionosphere in the midnight to dawn local time sector, and outward near dusk. Current sheet thicknesses and velocities are essentially independent of plasma sheet expansion or thinning, having typical values of 1500 km and 20–40 km/s respectively. Characteristic boundary layer current densities are about 10 nanoamps per square meter.     

North-south asymmetries of the solar magnetic field in conjunction with the location of the heliospheric current sheet on both sides of the solar equator

Reported heliospheric current-sheet displacements from the equatorial plane have been found to be in agreement with north-south asymmetries of the solar magnetic field. Mean heliospheric sector width estimations in the period 1947–1977 have shown that the heliospheric current sheet demonstrates an asymmetric placement with respect to the solar equator. This asymmetry is very prominent in the epochs of the solar cycle minima while it almost disappears in the epochs of maxima. At the same time, the sums of the maxima values of the sunspot magnetic field intensity showed in the epochs of minimum a characteristic asymmetry which implies an essential conjunction among the heliospheric current sheet, the solar cycle and the solar magnetic field. The main conclusion which could be derived of these observations is that the heliospheric current sheet has its origin on the solar surface while its location with respect to the solar equator appears to be affected by the variability of the lower layers of the solar interior.