UV光固化胶粘剂的研制

研制出了一种适用于高档家具玻璃、玻璃工艺器、水晶玻璃，光学玻璃等胶接用的丙烯酸系UV光固化胶粘剂，该胶粘接强度高、耐水性能好，玻璃接头在沸水中煮数十小时不剥离。     

磁探仪应召搜潜建模与仿真

依据经典的磁探仪应召搜潜方法,以某型反潜巡逻机为背景,建立了反潜巡逻机利用磁探仪执行平行航线、扩展矩形和螺旋形搜潜模型.对3种方法的搜潜概率进行分析,仿真了相同潜艇运动模型条件下,潜艇初始位置散布、初始距离、潜艇经济航速和海洋环境磁噪声对搜潜概率的影响.实验结果表明:相同条件下,螺旋形搜潜效能最高;潜艇只进行航速机动时...     

CTS-26型超声探伤仪典型故障的分析与排除

在简要介绍CTS-26型超声探伤仪工作原理及组成的基础上。对其几种典型故障作了具体的分析和处理。     

光离子化技术在肼类气体监测中的应用

肼类化合物是一种广泛应用于航天领域的液体火箭燃料。如在运输或操作中不慎泄露 ,可造成严重的环境污染 ,甚至会危害人员的生命健康。文章介绍了光离子化检测器在肼类气体监测中的应用 ,阐述了监测仪的设计思想。该仪器采用了光离子检测器 ,使其具有结构紧凑 ,体积小 ,质量小等特点。监测仪可对周围环境中肼类气体浓度的变化进行实时监测 ,并能自动予以声、光报警。实际使用表明 ,使用了光离子检测器的监测仪便于携带 ,监测准确度高 ,性能稳定 ,操作简单 ,既适用于野外现场监测 ,也适用于室内环境监控。     

环境气象条件对光学探测器性能的影响研究

环境气象条件对光学探测器的性能影响很大。针对南、北方的典型气象条件计算了两个波段下的大气透过率和天空辐射亮度,给出了大气环境条件对探测器探测能力的影响分析。     

低轨星载粒子探测器布局优化研究

基于卫星工具包(STK)、MATLAB软件和国际地磁参考场(IGRF)模型,对粒子探测器在低轨卫星任务中的投掷角测量范围进行了仿真,并给出了其探测器的星上布局优化方法。研究结果表明:粒子探测器的星上布局选择与任务的探测目标相关。如果探测目标是束缚在磁场中作弹跳运动的粒子,应将探测器在朝向卫星轨道坐标系±Y轴的基础上向卫星的前进方向偏转;如果探测目标是处于损失锥中的沉降粒子,应将探测器在朝向卫星轨道坐标系-Y轴的基础上向天顶方向偏转;为实现全投掷角探测范围的探测,要使用多个探测器通过构型布局优化进行联合探测。文章提出的投掷角测量范围分析与优化方法,可推广到多种轨道高度的粒子探测卫星总体设计中,为提升卫星的总体分析设计水平提供支持。     

电容近感探测目标多样性研究

基于探测器探测目标的多样性,从静电场出发,对极间电位移和电场强度特性进行了研究,进而分析了极问电容变化的本质并进行仿真。仿真结果表明目标切割电力线长度和目标相对电容率是影响极间电容变化的两个重要目标参数,目标切割电力线越长,极间电容变化越大;目标相对电容率对极间电容变化的影响很小,与Marconi公司实测的电容探测器炸高散布小的结论一致。     

Laboratory calibration measurements of a piezoelectric lead zirconate titanate cosmic dust detector at low velocities

A cosmic dust monitor for use onboard a spacecraft is currently being developed using a piezoelectric lead zirconate titanate element (PZT). Its characteristics of the PZT sensor is studied by ground-based laboratory impact experiments using hypervelocity particles supplied by a Van de Graaff accelerator. The output signals obtained from the sensor just after the impact appeared to have a waveform that was explicitly related to the particle’s impact velocity. For velocities less than ∼6 km/s, the signal showed an oscillation pattern and the amplitude was proportional to the momentum of the impacting particle. For higher velocities, the signal gradually changed to a single waveform. The rise time of this single waveform was proportional to the particle’s velocity for velocities above ∼6 km/s. The present paper reports on results for the low velocity case and especially discusses the effect of an outer coating of the sensor with a paint, which is used to reduce heating by solar radiation.     

R3D-B2 – Measurement of ionizing and solar radiation in open space in the BIOPAN 5 facility outside the FOTON M2 satellite

Solar and space radiation have been monitored using the R3D-B2 radiation risks radiometer-dosimeter on board a recent space flight on the Russian satellite Foton M2 within the ESA Biopan 5 facility mounted on the outside of the satellite exposed to space conditions. The solar radiation has been assayed in four wavelength bands (UV-C, 170–280 nm, UV-B, 280–315 nm), UV-A (315–400 nm) and PAR (photosynthetic active radiation, 400–700 nm). The data show an increasing tumbling rotation of the satellite during the mission. The photodiodes do not show a cosine response to the incident light which has been corrected. After calibration of the signals using the extraterrestrial spectrum, doses have been calculated for each orbit, for each day and for the total mission as basic data for the biological material which has been exposed in parallel in the Biopan facility. Cosmic ionizing radiation has been monitored and separated in 256 deposited energy spectra, which were further used for determination of the absorbed dose rate and flux. Basic data tables were prepared to be used by other Biopan 5 experiments. The paper summarizes the results for the Earth radiation environment at the altitude (262–304 km) of the Foton M2 spacecraft. Comparisons with the predictions of NASA Earth radiation environment experimental models AE-8 and AP-8, and the PSB97 model are also presented, which calculate the fluxes of ionizing radiation from a simulation. AP-8 is a model for trapped radiation.     

Instrument study of the Lunar Dust eXplorer (LDX) for a lunar lander mission

One of the highest-priority issues for a future human or robotic lunar exploration is the lunar dust. This problem should be studied in depth in order to develop an environment model for a future lunar exploration. A future ESA lunar lander mission requires the measurement of dust transport phenomena above the lunar surface. Here, we describe an instrument design concept to measure slow and fast moving charged lunar dust which is based on the principle of charge induction. LDX has a low mass and measures the speed and trajectory of individual dust particles with sizes below one micrometer. Furthermore, LDX has an impact ionization target to monitor the interplanetary dust background. The sensor consists of three planes of segmented grid electrodes and each electrode is connected to an individual charge sensitive amplifier. Numerical signals were computed using the Coulomb software package. The LDX sensitive area is approximately 400 cm². Our simulations reveal trajectory uncertainties of better than 2° with an absolute position accuracy of better than 2 mm.