BTi-62421S 高温钛合金超塑性能及应用

对BTi-62421S高温钛合金进行了高温超塑性拉伸实验,通过研究超塑条件下的力学性能、金相组织及拉伸断口形貌,确定了该合金高温拉伸条件下的断裂机制及超塑成形最佳变形工艺参数,在此基础上进行了BTi-62421S钛合金框架零件的超塑性成形实验。结果表明:BTi-62421S钛合金在920℃,应变速率10-3/s时具有最佳超塑性能,伸长率达到448.5%;该合金拉伸断裂机制以韧性断裂为主,但在不同变形参数下伴随着不同程度的脆性断裂;在超塑条件下可以成形出满足使用要求的航天用钛合金框架零件。     

航空CAE品牌调查报告

计算机辅助工程(CAE)是用计算机对工程结构与产品的性能及其生产加工过程,进行分析、模拟、预测、评价、优化,是工业装备和产品创新设计的核心技术,也是国防和军工装备研制的战略技术.经过几十年的发展,CAE技术在航空、航天、机械、汽车、船舶等领域获得成功应用,已成为制造业信息化深化应用的关键技术.     

浅谈超声衍射时差法(TOFD)检测技术

介绍了TOFD的基本原理、系统参数的设置、缺陷定性定量分析以及TOFD的优点和局限性,为TOFD检测技术的应用、推广提供参考.     

硅烷偶联剂改性Al2 O3p/TDE-85 的力学性能

利用硅烷偶联剂对Al2O3颗粒进行表面改性,制备了Al2O3颗粒增强的TDE-85树脂基复合材料,研究了表面改性对其力学性能的影响,采用差热分析仪测定复合材料的固化反应温度,并计算了固化反应活化能。利用扫描电子显微镜分析了拉伸断口形貌。研究发现,当Al2O3用量为2wt%时,固化反应速度较快,硅烷偶联剂用量为4wt%时,冲击强度为13.2 kJ/m2;拉伸强度为65.2 MPa;弹性模量为2.66 GPa;最大伸长率为3.35%,此时对Al2O3颗粒的表面改性综合效果最好。     

金属粉末熔化快速成型技术的研究进展

SLM技术代表了快速制造领域的发展方向,运用该技术能直接成型复杂结构、高尺寸精度、高表面质量的致密金属零件,减少制造金属零件的工艺过程,为产品的设计、生产提供更加快捷的途径,进而加快产品的市场响应速度,更新产品的设计理念和生产周期.SLM技术在未来将会得到更好、更快的发展.     

PVC糊树脂对交联PVC泡沫塑料的影响

通过水煮发泡制备交联聚氯乙烯泡沫塑料,讨论了聚氯乙烯(PVC)糊树脂对泡沫制备过程中经制糊、模压和发泡工艺得到的产物的影响,研究了PVC糊树脂对制备的交联PVC泡沫压缩性能的影响.结果表明:制备交联聚氯乙烯泡沫塑料适宜的糊黏度是4～9 Pa·s;PVC糊树脂的K值较大或水萃取液pH值呈碱性可有效防止模压过程中PVC的降解;PVC糊树脂的水萃取液pH值呈碱性可催化发泡反应,有利于得到低密度泡沫且缩短发泡时间;随着其K值增加,制备的泡沫压缩强度增大,但是K值过大时,制备的泡沫泡孔较大,压缩强度反而降低,适宜的K值为70～80.     

The Magnetic Field of Mercury

The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and observationally to distinguish the internal field from that due to the solar wind interaction. Conversely, the small field also means that Mercury offers an important opportunity to advance our understanding both of planetary magnetic field generation and magnetosphere-solar wind interactions. The observations from the Mariner 10 magnetometer in 1974 and 1975, and the MESSENGER Magnetometer and plasma instruments during the probe’s first two flybys of Mercury on 14 January and 6 October 2008, provide the basis for our current knowledge of the internal field. The external field arising from the interaction of the magnetosphere with the solar wind is more prominent near Mercury than for any other magnetized planet in the Solar System, and particular attention is therefore paid to indications in the observations of deficiencies in our understanding of the external field. The second MESSENGER flyby occurred over the opposite hemisphere from the other flybys, and these newest data constrain the tilt of the planetary moment from the planet’s spin axis to be less than 5°. Considered as a dipole field, the moment is in the range 240 to 270 nT-R _M ³ , where R _M is Mercury’s radius. Multipole solutions for the planetary field yield a smaller dipole term, 180 to 220 nT-R _M ³ , and higher-order terms that together yield an equatorial surface field from 250 to 290 nT. From the spatial distribution of the fit residuals, the equatorial data are seen to reflect a weaker northward field and a strongly radial field, neither of which can be explained by a centered-dipole matched to the field measured near the pole by Mariner 10. This disparity is a major factor controlling the higher-order terms in the multipole solutions. The residuals are not largest close to the planet, and when considered in magnetospheric coordinates the residuals indicate the presence of a cross-tail current extending to within 0.5R _M altitude on the nightside. A near-tail current with a density of 0.1 μA/m² could account for the low field intensities recorded near the equator. In addition, the MESSENGER flybys include the first plasma observations from Mercury and demonstrate that solar wind plasma is present at low altitudes, below 500 km. Although we can be confident in the dipole-only moment estimates, the data in hand remain subject to ambiguities for distinguishing internal from external contributions. The anticipated observations from orbit at Mercury, first from MESSENGER beginning in March 2011 and later from the dual-spacecraft BepiColombo mission, will be essential to elucidate the higher-order structure in the magnetic field of Mercury that will reveal the telltale signatures of the physics responsible for its generation.     

纳米隔热材料导热机理与特性研究

以SiO2气凝胶为研究对象,对其气相和固相导热机理进行了研究,进而为SiO2气凝胶材料传热设计提供理论指导.建立了SiO2气凝胶固相结构单元导热模型,在考虑对声子平均自由程的各种限制条件基础上,运用动力学理论分析了影响SiO2气凝胶固相结构单元热导率的影响因素.根据SiO2气凝胶微观结构特点,建立了几种纳米孔隙模型,计算了各种条件下SiO2气凝胶的当量热导率,研究了SiO2气凝胶各物性参数对其当量热导率的影响,并对比了几种纳米孔隙模型下SiO2气凝胶的当量热导率,并与实验值做了比较.     

Elemental Abundances in Coronal Structures

A great deal of evidence for elemental abundance variations among different structures in the solar corona has accumulated over the years. Many of the observations show changes in the relative abundances of high- and low-First Ionization Potential elements, but relatively few show the absolute elemental abundances. Recent observations from the SOHO satellite give absolute abundances in coronal streamers. Along the streamer edges, and at low heights in the streamer, they show roughly photospheric abundances for the low-FIP elements, and a factor of 3 depletion of high-FIP elements. In the streamer core at 1.5 R·, both high- and low-FIP elements are depleted by an additional factor of 3, which appears to result from gravitational settling. This revised version was published online in June 2006 with corrections to the Cover Date.     

基于云纹干涉与钻孔法的等离子热障涂层残余应力实验研究

应用云纹干涉法与钻孔法结合的光测力学实验方法,研究了等离子热障涂层基体材料镍基高温合金DZ125的残余应力。通过实验和计算获得了等离子喷涂工艺下基体DZ125的残余变形场、残余应变场和残余应力,并描述了其主要特征。结果表明,采用云纹干涉法与钻孔法结合测定热障涂层残余应力具有全场测量和高灵敏度等优点,这对于采用光学手段研究热障涂层残余应力有着积极的意义。