Neck-spinning quality analysis and optimization of process parameters for plunger components: Simulation and experimental study

The plunger component is a key part of the plunger pump in the aircraft hydraulic system. Neck-spinning process is commonly used to fabricate plunger components, of which the quality of the spinning process significantly affects the performance of plunger pumps. One of the bottlenecks faced by the industry in the spinning process is to choose a suitable neck-spinning process so as to ensure the quality of plunger components. It is necessary to propose a reliable method to optimize the process parameters which affect the neck-spinning quality of plunger components. In this study, a calculable finite element analysis (FEA) model is established to simulate the three-roller neck-spinning process of the plunger component, which includes six typical slipper structures, two roller structures, and two spinning parameters. The FEA model is then validated by comparing the simulated spinning forces with the corresponding experimental results. The influence of the process conditions on the neck-spinning quality is investigated. And the orthogonal simulation results are analyzed by a combination of range method and fuzzy mathematical analysis method to recommend a reasonable slipper structure, roller structure and neck-spinning parameters. This study provides a promising method to improve the manufacturing quality of the typical plunger components.     

机载雷达测控站性能分析CSCD

陆基、海基测控设备在跟踪低空特别是超低空飞行目标时受视距影响大,作用距离有限,而机载测控站作为空中测量平台,不受视距影响,有很大发展空间。介绍了机载测控站的组成、功能和工作原理,分析了机载测控站相关参数关系和工作能力,提出了提高跟踪能力的方法措施;给出了系统跟踪距离计算公式,通过几种典型目标速度分析了系统的跟踪能力,并与陆基、海基测控设备的跟踪能力进行了比对。结果表明,机载测控站在跟踪低空目标时作用距离较远,在低弹道大射程目标飞行试验中具有较大的应用空间。     

对测量雷达的一些新需求与精细测量技术

新一代测量雷达在发展各种先进武器平台与航空航天及空间技术方面有广泛的应用前景。本文讨论对测量雷达的一些新的需求及相关技术,对雷达精细测量的需求与有关技术是本文讨论重点。     

一种双通道测速应答机及其精度分析

介绍了一种双通道测速应答机的工作原理,并对其非相参通道的测速精度进行了定性分析。     

微波统一测控系统的电子防护能力分析与对策建议

通过对微波统一测控系统的电子防护能力和安全威胁分析,给出了进一步提高电子防护能力的对策建议。     

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。     

弹道导弹故障弹道计算方法研究

从靶场安全控制对故障弹道的需求出发,给出了弹道简化计算方法,阐述了通过改变发动机动力曲线、飞行程序角参数方式模拟导弹故障模式,并讨论了故障弹道的计算方法,仿真计算的结果满足靶场安全控制演练要求。     

混合星座导航系统的加权几何精度因子分析

不同类型卫星构成的混合星座导航系统或兼容系统中,考虑到广播星历精度不等导致的测距误差不等,用加权几何精度因子(WGDOP)代替几何精度因子(GDOP)作为最佳星座选择、定位精度评估和完好性监测的依据。对静止轨道卫星(GEO)/中高轨道卫星(MEO)构成的混合星座中不同卫星组合的WGDOP和GDOP进行了比较,实验结果表明WGDOP能更准确地反映星座性能和评估定位精度。在对定位精度或完好性监测的可靠性要求较高等场景,要用加权几何精度因子进行分析。     

The Radio Observatory on the Lunar Surface for Solar studies

The Radio Observatory on the Lunar Surface for Solar studies (ROLSS) is a concept for a near-side low radio frequency imaging interferometric array designed to study particle acceleration at the Sun and in the inner heliosphere. The prime science mission is to image the radio emission generated by Type II and III solar radio burst processes with the aim of determining the sites at and mechanisms by which the radiating particles are accelerated. Specific questions to be addressed include the following: (1) Isolating the sites of electron acceleration responsible for Type II and III solar radio bursts during coronal mass ejections (CMEs); and (2) Determining if and the mechanism(s) by which multiple, successive CMEs produce unusually efficient particle acceleration and intense radio emission. Secondary science goals include constraining the density of the lunar ionosphere by searching for a low radio frequency cutoff to solar radio emission and constraining the low energy electron population in astrophysical sources. Key design requirements on ROLSS include the operational frequency and angular resolution. The electron densities in the solar corona and inner heliosphere are such that the relevant emission occurs at frequencies below 10 MHz. Second, resolving the potential sites of particle acceleration requires an instrument with an angular resolution of at least 2°, equivalent to a linear array size of approximately 1000 m. Operations would consist of data acquisition during the lunar day, with regular data downlinks. No operations would occur during lunar night.     

Future Instrumentation for the Study of the Warm-Hot Intergalactic Medium

We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.