宽直线连接的处理方法

宽直线广泛应用于工程制图、PCB板图绘制等方面,宽直线的效果直接影响着最终输出图形的质量。宽直线的生成涉及许多问题[1],线接头是宽直线生成过程中必须要处理的问题之一,通过使用本文所介绍的两种方法,能有效解决宽直线圆连接和斜切连接的问题,并能获得所希望的效果。     

微放电效应预测研究

分析了几种类型结构方同轴线的特性,利用FDTD数值方法对方同轴线的微放电效应阈值电平进行预测计算,并给出了阈值曲线.结合实验数据说明了预测方法是有效的,该阈值曲线可以作为微放电效应部件设计参考曲线.     

一种新型压气机叶片造型方法的平面叶栅试验验证

为验证一种新型超/跨声压气机叶片造型方法——B样条控制中线角叶型、贝塞尔曲线控制叶型厚度方法 (BMAA方法)的有效性,分别与原有的可控扩散叶型定制造型和任意中线造型进行平面叶栅对比试验。结果表明,BMAA方法得到的跨声叶型,具有比定制叶型更优的气动性能;BMAA方法得到的超声叶型,具有与任意中线叶型相似的气动性能;与传统叶片造型方法相比,BMAA方法具有更高的效率,可提高叶片的气动负荷。     

自适应多点悬挂重力补偿系统研究

大型桁架式可展开航天结构在地面试验时,存在大挠度变形、精度低、泛用性差等结构特点,为提高地面试验有效性,提出了一种自适应多点悬挂重力补偿控制方法。首先,设计系统辨识算法和控制器算法,解决了多点耦合问题。其次,建立Simulink与Adams联合仿真平台,通过仿真分析选择算法参数,验证了算法的可行性。最后,以大型桁架式航天天线为对象,搭建重力补偿系统实验平台并进行实验验证。实验结果表明:控制系统在稳态环境和动态环境下均能快速收敛。稳态环境下,平均稳态误差为0.5503%;动态环境下,平均稳态误差0.526%。完成了航天结构天线的重力补偿,为多点重力补偿系统方案的实施提供建议和改进措施。     

The gamma-ray observatory mission objectives and its significance for gamma-ray astronomy

The Gamma Ray Observatory (GRO) is an approved NASA mission, programmed for launch in 1988. Its complement of four detectors has established goals: 1) to study the nature of compact γ-ray sources such as neutron stars and black holes, or objects whose nature is yet to be understood; 2) to search for evidence of nucleosynthesis especially in the regions of supernovae; 3) to study structural features and dynamical properties of our galaxy; 4) to explore other galaxies, especially the extraordinary types such as radio, Seyferts, and quasars; and 5) to study cosmological effects by examining the diffuse radiation in detail. This paper discusses the design, objectives, and expected scientific results of each of the GRO instruments in view of the GRO mission goals.     

Nucleosynthesis from non-thermal particles

The long-standing problem of nucleosynthesis from non-thermal charged particles is reviewed with emphasis on some novel points. Recent theoretical results predict very efficient acceleration of nuclei (up to GeV range) by violent systems with energy release in the form of multiple shock waves —OB associations and coronae of AGNs and black holes candidates in galactic accretion disks. A detection of gamma-line emission from the Orion complex by theCOMPTEL telescope on board ofGRO could confirm theoretical predictions. Production of lithium by non-thermal particles in Orion-like objects is discussed. The mechanism can be responsible for the observed variations of abundance of isotopes.     

Wind tunnel test of gust load alleviation for a large-scale full aircraft model

Wind tunnel test is an important way to test the performance of Gust Load Alleviation(GLA). At present, some component-level wind tunnel tests have been carried out in big aviation countries, but there is a lack of full aircraft model GLA tests. In this study, a set of large-scale GLA test system in low-speed wind tunnel is developed, which includes a gust generator, a fivedegree-of-freedom suspension system, a full elastic aircraft model with control system, and gust load measuring devices. Two...     

Microstructure evolution and mechanical anisotropy of M50 steel ball bearing rings during multi-stage hot forging

This study aimed to explore the evolution of flow lines and microstructures of M50-steel bearing ring and the anisotropy of its tensile mechanical properties after Multi-Stage Hot Forging (MSHF) and subsequent spheroidizing annealing (MSHFA). To this end, the present study mainly employed stereo microscopy, Optical Metallurgical Microscopy (OMM), Scanning Electron Microscopy (SEM), and Electron Backscatter Diffraction (EBSD) to characterize and analyze the workpiece at each processing stage of MSHF while performing microhardness measurement and uniaxial tensile experiment to test and analyze the mechanical properties of the workpiece. Macro-structure observation showed that the simulation results of flow lines at each stage were consistent with the experimental results. Microscopic observation showed that, after MSHF, deformation gradually became less significant along the outward radial direction of the bearing ring. After MSHFA, the microstructures of the bearing ring became uniform, whereas primary carbides did not dissolve. The mechanical properties were better in the axial direction (AD) than in the radial (RD) and circumferential directions (CD) after MSHF due to the smaller grain width. After MSHFA, the mechanical properties in the ADs and CDs were better than those in the RDs, which was due to the large cross-sectional area of carbides along the flow-line direction.     

对江西省输电线路覆冰预警的探讨

通过2008年冰灾对江西省输电线路造成的严重打击以及对江西省电网布局、输电线路设计标准、覆冰厚度大导致倒塔(杆)原因的掌握,在现有的观测和预报水平下,参照<气象灾害预警信号及防御指南>对江西省输电线路覆冰预警进行了探讨.     

一种新型宽频带单脉冲天馈系统

提出了一种新近研制成功的结构紧凑的S~C波段新型的宽频带单脉冲天馈系统.其关键部件包括天线单元、宽频带魔T及宽频带功分器.通过对渐变槽线天线单元的分析和计算、天线阵列的分布及阵因子的计算、微带-槽线双重接头及其构成的魔T的研究,而获得了高增益的宽频带单脉冲天馈系统.天馈系统的实测结果与理论设计相吻合.