TC6钛合金超塑性变形

对TC6钛合金在800~900℃温度区间内,分别进行应变速率为0.0001~0.1 s-1的恒应变速率法拉伸实验和最大m值法超塑性拉伸实验,获得拉伸过程应力-应变曲线,并采用金相显微镜对拉伸后断口附近显微组织进行分析。结果表明：TC6合金表现出良好的超塑性性能,随着应变速率或温度的升高,伸长率先增大后减小,恒应变速率拉伸时,在温度850℃、应变速率0.001 s-1条件下伸长率可达到993%;在同一变形温度下最大m值法拉伸能获得比恒应变速率法更好的超塑性,850℃时伸长率达到1353%;TC6合金在超塑性变形过程中发生了明显的动态再结晶,并随着应变速率和温度的升高动态再结晶行为增强。     

热变形对TC4氩弧拼焊板拉伸与疲劳性能的影响

在700℃下,对TC4氩弧拼焊板进行了3个变形量(主应变0.5％、1.6％、2.7％)的等双向拉伸成形,研究了热变形对TC4氩弧拼焊板单向拉伸性能和疲劳寿命的影响.结果表明:等双拉变形前后,TC4氩弧拼焊板拉伸试样均断裂在焊接热影响区,热影响区的强度低于母材和焊缝.随着等双拉热变形量增加,TC4拼焊板试样疲劳寿命有所增加,这是因为一定变形量的热成形释放了焊接残余应力.     

不同冶炼工艺对1Cr18Ni10Ti钢夹杂物的影响

通过试验研究了1Cr18Ni10Ti不锈钢的4种冶炼工艺:真空感应+电渣重熔、真空感应(陶瓷过滤器)、真空感应(陶瓷过滤器)+电渣重熔、真空感应+真空自耗,得到钢锭中夹杂物的种类、大小以及数量的变化.对比试验结果可知,采用真空感应(陶瓷过滤器)冶炼工艺与真空感应+真空自耗之后的钢锭的夹杂物水平相当,D类夹杂物数量最少,大颗粒夹杂物占比也最小.     

FOD缺口型损伤对TC4疲劳极限强度的影响

针对TC4钛合金风扇/压气机叶片前缘常遭受的外物损伤(FOD)缺口型损伤,进行了不同冲击角度下高速弹道冲击试验研究、损伤特征与应力集中分析,开展了冲击后不处理和冲击后去残余应力退火试样的高循环疲劳试验和疲劳极限强度预测。结果表明:随着冲击角度的增大入射侧损伤尺寸和应力集中系数基本保持不变,出射侧缺口损伤深度和损伤长度减小。损伤深度范围为0.6~1.5mm,应力集中系数范围为2.6~3.4。缺口型损伤试样的疲劳极限强度下降为光滑试样的27%~53%,与应力集中系数并不是呈反比关系。退火试样的高循环疲劳(HCF)性能或略微下降或基本不变,表明残余应力影响较小,残余应力对疲劳极限强度的影响程度不足光滑试样的10%。缺口型损伤试样的HCF性能与损伤底部半径的相关性不明显,随着最大损伤深度和损伤长度的增加而下降,表明制定维修手册时应着重考虑缺口型损伤的最大深度和损伤长度。Peterson经验公式对HCF性能的预测精度不理想,误差最大为45%,需要发展高精度的FOD缺口型损伤构件HCF性能预测方法。      

Balloon altitude studies of southern hemisphere hard X-ray sources by the Imperial College-University of Tasmania-INPE collaboration

Hard X-ray balloon altitude measurements with a 1600 cm² phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

A Revisit of the Phobos Events

The magnetic field disturbances detected by the Phobos-2 spacecraft in 1989 have been suggested to be caused by a ring of dust and/or gas emitted from the Martian moon, Phobos. The physical nature of these ``Phobos events' is examined using results from related investigations over the last twenty years. It is concluded that there is no clear evidence at present to support the association of magnetic field disturbances in the solar wind with Phobos. The situation will be further clarified taking advantage of the multi-spacecraft observations of the Yinghuo-1(YH-1), Mars Express and MAVEN missions beginning in 2012. It is expected that many novel features of solar wind interaction with Phobos (and possibly also Deimos) itself will also be revealed.      

New results and questions of lunar exploration from SELENE,Chang’E-1, Chandrayaan-1 and LRO/LCROSS

The moon has longstanding questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure and possible life. The recent lunar missions, e.g., SELenological and ENgineering Explorer “KAGUYA” (SELENE), Chang’E-1, Chandrayaan-1, and Lunar Reconnaissance Orbiter/Lunar CRater Observation and Sensing Satellite (LRO/LCROSS), have provided new opportunities to explore and understand these issues. In this paper, we reviewed and presented the results and findings in the fields of lunar gravity, magnetic field, atmosphere, surface geomorphology and compositional variations, volcano, craters, internal structure, water and life science from new lunar exploration missions. In addition, the new objectives and scientific questions on lunar explorations in near future are presented and discussed.     

中俄联合火星电离层星-星掩星探测

中俄联合火星星-星掩星探测是人类首次在火星空间环境进行此类的联合试验。用于探测火星电离层的星-星掩星技术较以前星地间的探测技术相比,有可接收高信噪比信号,反演精度高,可探测火星上太阳天顶角大于43°,或者小于138°的区域电离层等优点。本文介绍了中俄联合火星星-星掩星探测方案、基本原理,给出了主要技术指标、地面模拟测试结果。     

LALR(1)分析器快速生成

根据LR(0)自动机的构造理论及Deremer和Pennello的LALR(1)向前看符号集计算公式,提出求解公式中的lookback关系和includes关系的高效算法. 研究过程表明,LR(0)项目集闭包计算和项目集的查找是LR(0)分析器构造过程中的主要性能瓶颈.对这两个计算过程给出了高效的数据结构和算法设计,实现了LALR(1)分析器的快速生成.系统实现及实验数据表明,LALR(1)分析器的生成速度超过了自由软件基金会的LALR(1)分析器生成器Bison.