无人机总体与起飞性能匹配性设计优化

首先,提出了一种小推重比的低速螺旋桨无人机总体参数与起飞性能匹配性设计优化方法;其次,对该无人机起飞阶段的动力学和运动学特性进行了分析,明确了该无人机总体参数与起飞性能之间的最佳匹配关系,以实现无人机起飞性能的最优化;最后,通过分析得出结论:小推重比低速螺旋桨无人机总体设计参数的选取直接影响到起飞性能的优劣,“平衡”总体设计需求来发挥平台更佳的起飞性能是总体设计优化的重要内容.     

SiO2f/SiO2复合材料自身及其与铜、不锈钢的钎焊

采用AgCuTi活性钎料,在880℃/10min规范下成功实现了SiO2f/SiO2自身、SiO2f/SiO2与Cu和SiO2f/SiO2与1Cr18Ni9Ti三种接头的连接。实验结果表明,三种接头中靠近SiO2f/SiO2母材的界面处均形成了一层薄薄的扩散反应层组织,反应层中出现了Ti和O的富集,根据两者的原子比例推断生成了TiO2相;另外,三种接头中心区都形成了由灰色相和白色相共同组成的Ag-Cu共晶组织,其中灰色相为Cu基固溶体,白色相为Ag基固溶体。接头剪切强度结果显示,SiO2f/SiO2/Cu接头剪切强度为12.4MPa,SiO2f/SiO2/1Cr18Ni9Ti接头剪切强度为18.4MPa,接头中的残余应力是决定接头强度大小的重要因素之一。     

独立函数及其R/W谱在逻辑设计中的应用

本文提出基于独立函数的逻辑设计方法,即如何利用独立函数和它的Rademacher/Walsh谱系数进行组合逻辑设计。这是组合逻辑设计方法的另一新途径。它有利于数字系统的模块化。     

CVD技术制备Ta/W层状复合材料

运用化学气相沉积(Chemical Vapor Deposition,CVD)技术制备了W体积分数分别10%,13%和18%的Ta/W两层层状复合材料,采用金相显微镜(OM)、扫描电镜(SEM)和室温拉伸实验对复合材料的性能进行分析。结果表明:运用CVD技术可以制备W体积分数不同,且密度优于理论密度99.4%的层状复合材料;复合材料中Ta,W层的晶粒均为柱状晶粒,离界面越近,晶粒越细;沉积态复合材料的力学性能优于纯CVD Ta和CVD W;1600℃×2 h的热处理后,复合材料的界面扩散层宽度显著增大,力学性能高于沉积态的力学性能,最高抗拉强度可达660 MPa。     

Planetary waves according to simultaneous observations of <Emphasis Type="Italic">GPS</Emphasis> satellites and ground-based magnetic stations

On the basis of measurements made at Japanese magnetic stations and using GPS satellites for the 12 months of 2003, a comparison of simultaneous variations of three components of the magnetic field and total electron content (TEC) was carried out in the range of the planetary waves period. The correlation analysis has shown that almost synchronous variations exist within this range of periods at the ground-based magnetometer stations and in the TEC measurements both during strong magnetic disturbances and in quiet periods. The strong magnetic disturbances could be considered as a possible independent source of ionospheric variations within the planetary waves range, while the accompanying ionospheric storms could be a possible factor changing the conductivity of the lower ionosphere plasma. In quiet periods, the correlation of magnetic variations and disturbances in TEC is caused by the direct impact of atmospheric planetary waves on the lower ionosphere and can be related to variations of ionospheric currents due to the dynamo mechanism.     

New insights into SNR evolution revealed by the discovery of recombining plasmas

We report the discovery of recombining plasmas in three supernova remnants (SNRs) with the Suzaku X-ray astronomy satellite. During SNR’s evolution, the expanding supernova ejecta and the ambient matter are compressed and heated by the reverse and forward shocks to form an X-ray emitting hot plasma. Since ionization proceeds slowly compared to shock heating, most young or middle-aged SNRs have ionizing (underionized) plasmas. Owing to high sensitivity of Suzaku, however, we have detected radiative recombination continua (RRCs) from the SNRs IC 443, W49B, and G359.1–0.5. The presence of the strong RRC is the definitive evidence that the plasma is recombining (overionized). As a possible origin of the overionization, an interaction between the ejecta and dense circumstellar matter is proposed; the highly ionized gas was made at the initial phase of the SNR evolution in dense regions, and subsequent rapid adiabatic expansion caused sudden cooling of the electrons. The analysis on the full X-ray band spectrum of IC 443, which is newly presented in this paper, provides a consistent picture with this scenario. We also comment on the implications from the fact that all the SNRs having recombining plasmas are correlated with the mixed-morphology class.     

Effect of W addition on phase transformation and microstructure of powder metallurgic Ti-22Al-25Nb alloys during quenching and furnace cooling

Powder metallurgic Ti2 AlNb alloys with W addition are sintered at 900, 1000, 1070 °C,and 1150 °C(i.e., in the O + B2, a_2+ B2 + O, a_2+ B2, and single B2 phase regions, respectively)for 12 h, followed by water quenching and furnace cooling. Comparisons of phase and microstructure between quenched and furnace-cooled W-modified alloys are carried out to illustrate the phase transformation and microstructure evolution during the cooling process. Furthermore, a comparison is also made between W-modified and W-free alloys, to reveal the function of the W alloying.W addition accelerates the solutions of a_2 and O phases during the high-temperature holding, and a Widmannsta¨tten B2 + O structure, which contributes to the properties, is induced by furnace cooling from all the phase regions. The Widmannsta¨tten structure includes a B2 matrix, primary O, and secondary O precipitates. However, W alloying refines the Widmannsta¨tten structure only when the alloys are solution-treated and then cooled from the single B2 phase. Although the hardness of the W-modified alloys is lower than that of the W-free alloys sintered in the same phase region, an enhancement of hardness, 489 ± 18 HV, is obtained in the alloy solution-treated in the single B2 phase region for only 0.5 h.     

ZrCP/W复合材料在发动机试车条件下的热震烧蚀行为

采用热压烧结法制备了ZrCp／W复合材料环形试样，测试了该复合材料试样在发动机试车条件下的热震烧蚀性能。结果表明：ZrCp／W复合材料具有良好的抗热震和耐烧蚀性能．试验后试样整体结构完好，未出现炸裂和破碎的现象，线烧蚀率仅为-0．05mm／s。该复合材料的主要烧蚀机制是机械剥蚀，此外还有熔化烧蚀和热化学烧蚀。     

大尺寸弹丸喷丸成形2024-T351铝合金表面质量研究

针对2024-T351铝合金进行直径3mm大弹丸喷丸成形及直径0.58mm小弹丸喷丸强化试验,观测试样在不同喷丸参数下的表面形貌,并对表层显微硬度及残余应力分布进行测试,为整体壁板喷丸成形的工艺设计提供重要依据。     

W含量对单晶镍基合金组织与性能的影响

通过对两种成分单晶镍基合金进行蠕变曲线测定,长期时效处理及组织形貌观察,研究了元素W含量对单晶合金组织与性能的影响.结果表明:在Ni-A1-Cr-Ta-Co-x%W-5.5%Mo系单晶合金中,4wt%W合金在982℃,200MPa条件下,具有较长的蠕变寿命,随W含量增加到6wt%,合金的蠕变寿命明显降低.高W合金在有/无应力时效期间,析出针状μ相,使合金基体出现难溶元素的贫化区,是导致合金蠕变寿命降低的主要原因.其中μ相在(001)晶面沿<110>方向呈相互平行、或垂直的针状形貌析出,沿{111}晶面呈片状方式生长,且与γ′相相邻.