温湿度传感器检定系统设计

本文介绍了利用电子扫描开关,可一次检定多只温湿度传感器的检定系统的硬件和软件设计。     

航空工业发展中存在的问题与对策——以河南省为例

重视发展战略、重视国内市场、重视技术创新以及重视对外合作是航空工业发达国家发展航空工业的主要经验.我国航空工业目前存在着企业规模小、布局分散、"软实力"不足、产品多属民品、科研体制存在弊端等问题.加速我国航空工业的发展,需要制定长远的发展规划,以市场为导向,加大结构调整力度,进行一系列的体制机制创新以及重视现有航空产品的改进改型,广泛进行国际国内合作,等等.     

基于关联分析的机载电子设备SRU级故障诊断方法

针对机载设备二类检测设备将故障隔离到SRU的要求,对LRU的内部结构进行了分析,提出了点、底项、组底项的概念,用关联值表示点与点之间、点与SRU之间及组底项之间的关联关系;针对多SRU结构UUT,提出逐级排除法故障诊断方法.     

薄膜充气管充气展开特性试验

用展开导轨消除因重力产生的摩擦力,在不同充气速率与初始展开角条件下对薄膜材料充气管的充气展开特性进行了试验研究,获得了展开角,以及展开加速度和内气压的变化规律。试验及分析结果表明:充气管的充气膨胀与展开相互独立,充气膨胀过程近似为等压增容过程,折叠部位的气压变化特性与整体气压变化特性差异明显。     

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with primary goat embryonic fibroblast showed no difference from traditional feederlayer-based culture method used in mouse and human. The putative primary EG colonies were multilayer clumps ofcompact cel     

基于混合灵敏度下H∞控制在三滑块质量矩导弹上的应用

由于质量矩导弹是一个具有非线性和模型不确定性的多变量系统，为了进一步提高控制系统的鲁棒性，对三滑块质量矩导弹进行了鲁棒控制系统的研究。以所建立的质量矩导弹数学模型为基础，通过对模型合理的简化，得到一个耦合的非线性动力学系统，考虑到质量矩导弹的鲁棒性要求和三个滑块的协调控制问题，在混合灵敏度控制的基础上，采用H∞控制理论对导弹进行姿态控制系统的研究，仿真结果验证了这种方法的有效性。     

计算机帧时间对半实物仿真的影响

半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。     

Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

末制导雷达通用检测系统中开关量测量电路的设计

介绍了基于EMP7128S逻辑控制器件并已成功的应用于某型末制导雷达通用检测系统的开关量测量电路的设计和工作原理.     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.