基于TCP/IP的双机自动连接与通信

介绍了双机通信所必需的硬件连接和IP地址设置,分析了TCP服务器的注册和TCP客户端的自动连接,并以平显训练模拟系统为例,分析了双机通信和画面参数的传输。     

1997年1月6—11日日地连接事件：对磁暴—环电流—对流电场的讨论

给出了1997年1月6—11日日地连接事件的太阳风和行星际扰动及由此产生的地磁扰动特征．利用这些资料对磁暴-环电流-对流电场的分析表明,磁暴主相（或环电流）的开始主要是IMF南向分量形成的对流电场直接驱动的结果;对流电场在磁暴主相的形成中有极为重要的作用;但在主相发展的不同阶段作用不同     

拉伸载荷下管路连接副的密封性分析

研究了航空发动机钛合金管路连接副在拉伸载荷下的密封性能.首先,建立了连接副的等效刚性模型, 分析其在拉伸载荷下的受力,研究了密封面的接触力随拉伸载荷的变化规律,从机理上分析了拉伸载荷下管路连接副的密封性.第二,建立了管路连接副在拉伸载荷下的多体弹性接触模型,并对其进行有限元分析.采用初始渗透接触法,实现连接副的预紧状态,在此基础上施加拉伸载荷,然后再进行有限元求解.同时,研究了连接副密封面的接触力、接触面积和接触应力随拉力的变化规律,从而定量地分析连接副的密封性.      

考虑连接非线性的大型桁架天线分散协调控制

针对含非线性连接的大型桁架式天线,考虑铰链非线性所产生的影响,基于连接子结构模态综合建模方法,建立其低阶非线性动力学模型。在此基础上,将动力学模型转换为分散参数化模型,并考虑状态变量不完全可测因素,设计适用于一致性理论的最优观测器。然后基于图论的思想提出桁架式天线的一致性形面保持控制方法,不仅实现了桁架式天线的高精度形面保持控制,同时对作动执行机构的失效具有容错性。仿真结果表明了所提控制方法的有效性。     

A mask R-CNN based method for inspecting cable brackets in aircraft

In the aviation industry, cable bracket is one of the most common parts. The traditional assembly state inspection method of cable bracket is to manually compare by viewing 3D models. The purpose of this paper is to address the problem of inefficiency of traditional inspection method. In order to solve the problem that machine learning algorithm requires large dataset and manually labeling of dataset is a laborious and time-consuming task, a simulation platform is developed to automatically generate synthetic realistic brackets images with pixel-level annotations based on 3D digital mock-up. In order to obtain accurate shapes of brackets from 2D image, a brackets recognizer based on Mask R-CNN is trained. In addition, a semi-automatic cable bracket inspection method is proposed. With this method, the inspector can easily obtain the inspection result only by taking a picture with a portable device, such as augmented reality (AR) glasses. The inspection task will be automatically executed via bracket recognition and matching. The experimental result shows that the proposed method for automatically labeling dataset is valid and the proposed cable bracket inspection method can effectively inspect cable bracket in the aircraft. Finally, a prototype system based on client-server framework has been developed for validation purpose.     

环柱式天线展开过程耦合动力学分析

针对环柱式天线展开过程中斜拉绳索释放运动与桁架展开运动之间耦合动力学分析困难的问题,采用非线性欧拉梁单元对斜拉绳索建模,基于几何精确梁理论对环形桁架建模,提出了环柱式天线多体系统模型,实现了结构展开过程中绳索释放与桁架展开耦合动力学的精准仿真,揭示了绳索柔性等因素对桁架伸展起阻碍作用的机理。仿真结果表明,在环柱式天线展开过程中,减小绳索模量,降低绳索直径,采用单绳索分布设计,有利于提高桁架的展开稳定性。另外,绳索柔性对桁架展开中间阶段影响最为显著。该分析结果为环柱式天线在轨展开动力学预示和优化设计提供了指导作用。     

医学院校大学英语与医学英语教学衔接浅析

基础英语教学与专业英语教学是为同一教学目标构建的两个层面,是不可截然分离,相辅相成的。而两者在衔接过程中,存在着师资、教材等种种问题。针对这些问题,提出了相应的对策及建议。     

Multi-scale strength analysis of bolted connections used in integral thermal protection system

Efficient and accurate strength analysis of bolted connections is essential in analyzing the integral thermal protection system(ITPS) of hypersonic vehicles, since the system bears severe loads and structural failures usually occur at the connections. Investigations of composite mechanical properties used in ITPS are still in progress as the architecture of the composites is complex. A new method is proposed in this paper for strength analysis of bolted connections by investigating the elastic behavior and failure strength of three-dimensional C/C orthogonal composites used in ITPS. In this method a multi-scale finite element method incorporating the global–local method is established to ensure high efficiency in macro-scale and precision in meso-scale in analysis.Simulation results reveal that predictions of material properties show reasonable accuracy compared with test results. And the multi-scale method can analyze the strength of connections efficiently and accurately.     

‘Spectro-temporal’ characteristics and disk-jet connection of the outbursting black hole source XTE J1859+226

We re-investigated the ‘spectro-temporal’ behavior of the source XTE J1859+226 in X-rays during its outburst phase in 1999, by analysing the RXTE PCA/HEXTE data in 2–150 keV spectral band. Detailed analysis shows that the source evolves through different spectral states during its entire outburst as indicated by the variation in the spectral and temporal characteristics. Although the evolution pattern of the outburst followed the typical q-shaped profile, we observed an absence of ‘canonical’ soft state and a weak presence of ‘secondary’ emission during the decay phase of the outburst. The broad-band spectra, modeled with high energy cutoff, shows that the fold-energy increases monotonically in the hard and hard-intermediate states followed by a random variation in the soft-intermediate state. We attempted to estimate the mass of the source based on the evolution of Quasi-Periodic Oscillation (QPO) frequencies during rising phase modeled with the propagating oscillatory shock solution, and from the correlation of photon index and QPO frequency. It is also observed that during multiple ejections (observed as radio flares) the QPO frequencies are not present in the power spectra and there is an absence of lag in the soft to hard photons. The disk flux increases along with a decrease in the high energy flux, implying the soft nature of the spectrum. These results are the ‘possible’ indication that the inner part of the disk (i.e., Comptonized corona), which could be responsible for the generation of QPO and for the non-thermal Comptonized component of the spectrum, is disrupted and the matter gets evacuated in the form of jet. We attempted to explain the complex behavior of ‘spectro-temporal’ properties of the source during the entire outburst and the nature of the disk-jet connection before, during and after the ejection events in the context of two different types of accreting flow material, in presence of magnetic field.