基于UDDI的应用服务注册中心的设计与实现

Web服务是当前基于Web的分布式计算与应用的关键技术基础.通用描述发现集成协议(UDDI)是Web服务的核心技术标准,提供了Web服务的信息注册查找规范,解决了Web服务的描述、发布以及查找问题.UDDI规范仅提供了标准接口及数据结构,缺乏对UDDI注册中心的安全性、可管理性等明确的定义和实现机制.基于Web服务及UDDI技术分析,设计实现了基于UDDI的应用服务注册中心(ASC).ASC由ASC客户端、ASC服务器、ASC管理控制台组成,支持Web服务的发布、查找、管理等操作.根据实际应用需求,设计并实现了发布者声明关联匹配算法,扩展了UDDI标准的应用编程接口,提供了安全、管理等功能,形成了一个具有较强安全性和易管理性的应用服务注册系统.     

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.     

Zr-Al-(Ni-Cu)合金的非晶形成能力及热学性能

采用喷射铜模铸造法研究了Ni和Cu含量对Zr-Al-(Ni-Cu)四元合金的非晶形成能力的影响.利用X射线衍射仪分析了铸态合金的相结构,利用差示扫描量热仪研究了非晶合金的热学性能.结果表明:Zr-Al-(Ni-Cu)四元合金的非晶形成能力远大于Zr-Al-Ni和Zr-Al-Cu三元合金的非晶形成能力.Zr65Al7.5Ni10Cu17.5合金显示最高的非晶形成能力,其非晶形成临界直径可以达到7 mm.相似元素Ni和Cu在一定比例下共存,使液态合金的熵值增加,自由能降低,从而有效提高了合金的非晶形成能力.     

空间黏附爬行机器人足端预压力优化与控制

基于仿生干黏附材料的空间足式爬行机器人可附着于航天器外表面并代替宇航员完成舱外巡检、维护等工作,是无人自主化在轨服务与维护的有效途径。为保证足式爬行机器人与航天器的稳定附着,本文针对空间爬行机器人足端在与航天器接触时预压力对黏附稳定性影响的问题,提出一种足端预压力优化与控制方法。首先结合仿生黏附材料特性,建立黏附材料在预压阶段和黏附阶段的稳定性约束;其次在稳定性约束下基于二次规划方法优化足端力,保证预压力足够的同时减小对其他足的脱附力;最后通过基于环境刚度辨识的导纳控制实现优化后的力分配。结果表明：基于环境刚度辨识的导纳控制可实现预压力的柔顺控制,优化后的预压力可减小对其他黏附足的法向脱附力的影响,保证黏附爬行稳定性。     

航空管路补偿器耐久性计算方法对比分析

本文研究了管路补偿器补偿位移疲劳寿命和耐久振动寿命的有限元分析计算方法。通过对某型管路补偿器有限元仿真计算结果和传统工程计算法计算的结果进行对比分析,研究管路补偿器补偿位移疲劳寿命的有限元计算方法,探索耐久振动寿命的有限元计算流程,并将结果同试验数据对比,以验证其设计方法的计算精度。结果表明,补偿位移的疲劳寿命有限元法的计算精度优于工程设计法;耐久振动寿命有限元法能够给出确定的振动应力分布情况,并预测出耐久振动寿命时间,工程设计法仅能计算出管路补偿器的自振频率,不能明确振动应力和寿命。     

含硅芳炔树脂改性氰酸酯树脂的性能

将双酚E型氰酸酯(BEDCy)与含硅芳炔树脂(PSA)用溶液共混的方法制备了共混树脂(BEDCy/PSA);通过DSC和原位红外研究了共混树脂的固化反应,使用TGA和DMA表征了树脂的耐热性能;还考察了共混树脂的介电性能和力学性能.结果表明,PSA树脂能够降低BEDCy树脂的固化温度;随着PSA树脂的添加,氮气和空气氛...     

复合材料层合板低速冲击损伤的预测模型

在低速冲击载荷作用下,建立了一种适用于铺层总数较多的复合材料层合板的损伤预测模型。采用三维Puck失效准则预测层内纤维与基体的破坏,并获得基体失效时的断裂面角度。根据低速冲击下复合材料层合板的层间分层损伤机理,同时考虑面内横向正应力、厚度方向正应力、层间剪应力和相邻铺层的损伤状态等因素对界面分层的影响,发展了一种新的冲击分层失效准则。为快速有效地预测铺层总数较多的复合材料层合板的冲击损伤,通过对单元积分点处的应变进行线性插值,提出了在单个实体单元内预测多个铺层损伤的数值计算方法。模型成功预测了受冲击层合板具体的失效模式,预测的分层形状和尺寸与试验值吻合较好,并显著减少了有限元模型的规模,表明本文所发展的数值方法对预测复合材料层合板低速冲击损伤的有效性。     

Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm

The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere.