低展弦比微型轴流涡轮弯叶片设计

针对微型轴流涡轮机面临的低展弦比、低雷诺数导致效率降低的问题,以某型200kW微型燃气轴流涡轮发电机高压涡轮为研究对象,采用数值模拟方法开展了低展弦比下微型弯曲轴流涡轮叶片设计技术研究。对展弦比为0.88的涡轮静叶,分析对比了正弯和J型弯静叶对微型涡轮流场的影响,结果显示:正弯静叶顶部出口气流角较大,造成下游动叶叶尖泄漏损失增大,整体效率下降;而J型弯方案抑制了下游动叶叶背中径的流动分离,整体性能较原型有所提升。然后,研究了J型静叶弯高和弯角对涡轮性能的影响规律,结果表明:采用大弯高小弯角设计的J型静叶提高了静叶根部通流能力,同时合理分配了静叶通道内的负荷以及出口气流方向,对涡轮级流场的改善效果更佳。J型静叶弯高为1、弯角为+5°时,级效率达到0.852,流量为1.205kg/s,较原型分别提高了0.77%和0.96%。     

基于J2ME-J2EE平台的移动电子商务系统的实现

为了解决移动电子商务开发中终端设备处理能力有限的问题,实现了基于J2ME-J2EE集成平台,将访问请求转发到服务端进行处理开发移动电子商务系统的方案。在该方案中,J2ME端的MIDP程序接收用户的访问请求,通过HTTP协议把请求转发到J2EE服务器端进行处理;J2EE端采用了流行的Web应用开发框架,分离了程序逻辑,简化了开发复杂度,提高了开发效率。     

超声速光学头罩流场的PIV研究

在马赫数Ma-3．8超声速风洞中,采用PIV（Particle Image Velocimetry,粒子图像测速）技术测量了超声速光学头罩流场的速度分布。PIV技术应用于超声速流场时,对系统的硬件配备、示踪粒子的跟随性以及PIV算法的精度有很高的要求。本文PIV系统选用高精度的同步控制器和高能量激光器;以纳米级粒径的粒子作为示踪粒子,通过斜激波响应实验分析了其在超声速流场中的跟随性;并采用多种高精度速度场算法对粒子图像进行处理。实验结果表明,示踪粒子在超声速流场中有很好的跟随性,采用的高精度速度场算法能够很好地反映超声速光学头罩流场的速度分布。     

定几何混压式轴对称超声速进气道设计及性能计算

给出了定几何混压式轴对称超声速进气道型面设计及性能计算方法,进行了算例计算。对亚临界状态下脱体激波的计算进行了研究,给出了进气道临界状态性能参数随飞行马赫数和高度的改变而变化的曲线。分析了进-发匹配过程,以及进气道的自调节能力。计算得到了基于进气道性能最优,即进气道工作在临界状态条件下,碳氢燃料冲压发动机的供油规律,为进气道大范围寻优设计打下了基础。      

含裂纹燃气涡轮叶片结构非概率可靠性分析

涡轮叶片是燃气轮机装置中失效最频繁的工作部件,其主要的失效模式之一为裂纹扩展而引起的疲劳断裂失效。以含裂纹燃气涡轮叶片为研究对象,根据其典型启动运行工况制定载荷谱,通过瞬态热弹塑性有限元分析确定叶片失效的危险部位,并据此建立含裂纹叶片的实体模型;根据瞬态热弹塑性分析结果和J积分强度判据,对含裂纹叶片进行非概率可靠性分析。通过工程实例,验证了结构非概率可靠性综合模型的可行性和可操作性,为非完善结构的可靠性分析评定提供了新的方法体系。     

Broad band X-ray properties of GRO J1948+32/KS 1947+300

We present here results obtained from three BeppoSAX observations of the transient X-ray pulsar GRO J1948+32 carried out during the declining phase of its 2000 November–2001 June outburst. Timing analysis of the data clearly shows a 18.7 s pulsation in the X-ray light curves in 0.1–100 keV energy band. The pulse profile of GRO 1948+32 is characterized by a broad peak with a sharp rise followed by a narrow dip. The dip in the pulse profile shows very strong energy dependence. Phase-averaged spectroscopy obtained with three of the BeppoSAX instruments shows that the 0.1–100 keV energy spectrum is described by a Comptonized component, a weak blackbody component (7% of the total emission) for soft X-rays, a narrow and weak iron emission line at 6.7 keV and low column density of material in the line of sight. The results obtained from the analysis are discussed in this paper.     

J2EE平台会话管理机制分析与改进

在分析J2EE平台会话管理机制的基础上,指出了J2EE会话管理机制在会话状态管理方面的不足,提出了解决方案,论述了实现该方案时要解决的五个关键问题。     

3J33C小孔镗削温度测量实验及有限元模拟

基于3J33C弹性合金小孔镗削温度测量实验及Advant Edge有限元温度仿真试验,验证了有限元模型及结果的可靠性,得到其不同镗削参数时基体最高温度的变化规律及温度范围。基于有限元仿真结果建立了3J33C小孔镗削的温度经验公式,结果表明,随着镗削转速、进给速度及径向切深的增大,镗削温度都呈现升高趋势,并且在这三个因素中镗削转速影响最大,进给速度影响次之,径向切深影响最小。     

‘Spectro-temporal’ characteristics and disk-jet connection of the outbursting black hole source XTE J1859+226

We re-investigated the ‘spectro-temporal’ behavior of the source XTE J1859+226 in X-rays during its outburst phase in 1999, by analysing the RXTE PCA/HEXTE data in 2–150 keV spectral band. Detailed analysis shows that the source evolves through different spectral states during its entire outburst as indicated by the variation in the spectral and temporal characteristics. Although the evolution pattern of the outburst followed the typical q-shaped profile, we observed an absence of ‘canonical’ soft state and a weak presence of ‘secondary’ emission during the decay phase of the outburst. The broad-band spectra, modeled with high energy cutoff, shows that the fold-energy increases monotonically in the hard and hard-intermediate states followed by a random variation in the soft-intermediate state. We attempted to estimate the mass of the source based on the evolution of Quasi-Periodic Oscillation (QPO) frequencies during rising phase modeled with the propagating oscillatory shock solution, and from the correlation of photon index and QPO frequency. It is also observed that during multiple ejections (observed as radio flares) the QPO frequencies are not present in the power spectra and there is an absence of lag in the soft to hard photons. The disk flux increases along with a decrease in the high energy flux, implying the soft nature of the spectrum. These results are the ‘possible’ indication that the inner part of the disk (i.e., Comptonized corona), which could be responsible for the generation of QPO and for the non-thermal Comptonized component of the spectrum, is disrupted and the matter gets evacuated in the form of jet. We attempted to explain the complex behavior of ‘spectro-temporal’ properties of the source during the entire outburst and the nature of the disk-jet connection before, during and after the ejection events in the context of two different types of accreting flow material, in presence of magnetic field.     

FJ44发动机关键性能参数趋势分析

以FJ44型发动机为研究对象,选择采集该型发动机的几个关键性能参数,对数据平滑处理后进行趋势分析,监控发动机状态,并为其故障诊断提供参考。