一种大负荷低压涡轮叶型的气动性能

基于Lantry-Menter转捩模型,分别对Zweifel升力系数为1.2的一种大负荷低压涡轮叶型在定常来流不同湍流度、雷诺数条件下,上游非定常、周期性尾迹作用下的流动进行了数值模拟.计算结果表明,定常来流低雷诺数条件下,湍流度对该大负荷叶型的气动性能影响较大;上游非定常、周期性尾迹对叶型吸力面分离泡的抑制作用可进一步减小低雷诺数条件下的叶型损失.计算结果揭示了该大负荷叶型在低压涡轮内部真实流动环境中的表面流动及损失特征,对国内现行低压涡轮设计有着较好的启示.      

Usage of pre-flight data in short rendezvous mission of Soyuz-TMA spacecrafts

The paper describes the reduction of the vehicle autonomous flight duration before docking to the ISS. The Russian Soyuz-TMA spacecraft dock to the ISS two days after launch. Due to the limited volume inside Soyuz-TMA the reduction of time until docking to the ISS is very important, since the long stay of the cosmonauts in the limited volume adds to the strain of the space flight. In the previous papers of the authors it was shown that the existing capabilities of Soyuz-TMA, the ISS and the ground control loop make it possible to transfer to the five-orbit rendezvous profile. However, the analysis of the cosmonauts' schedule on the launch day shows that its duration is at the allowable limit and that is why it is necessary to find a way to further reduce the flight duration of Soyuz-TMA before docking to less than five orbits. In a traditional rendezvous profile, the calculation of rendezvous burns begins only after determination of the actual vehicle insertion orbit. The paper describes an approach in which the first two rendezvous burns are performed as soon as the spacecraft reaches the reference orbit and the values of the burns are calculated prior to the launch based on the pre-flight data for the nominal insertion. This approach decreases the duration of the rendezvous by one orbit. The demonstration flight of a Progress vehicle using the proposed profile was implemented on August 1, 2012 and completely confirmed the correctness of the imbedded principles. The paper considers the possible improvements of the proposed approach and recovery from the contingencies.     

对信息检索系统应用技术的数学表示模型的分析

页面表示、用户兴趣模型、页面链接排序是信息检索系统中的关键技术,分析相应的数学模型,并例举在一个智能搜索引擎中的应用,通过动态的更新用户兴趣模型和由此而引起的WEB页面更新,有效地适应用户兴趣的变化。     

脉冲星导航试验卫星科学观测数据分析

脉冲星导航试验卫星是我国发射的一颗专用试验卫星.经过4个多月的在轨观测,该卫星已成功获取了大量观测数据.介绍利用该卫星搭载的掠入射聚焦型X射线探测器在近4个月中对PSR B0531+21获得的观测数据第一批处理结果.本文详细阐述掠入射聚焦型X射线探测器的观测模式,给出脉冲星观测数据的处理方法以及脉冲星参数的拟合过程,利用基于第一手观测数据的脉冲星精化参数验证掠入射聚焦型探测器在轨工作性能,得以回答使用国产X射线探测器是否能够“看得见”脉冲星问题.     

导弹助推器分离过程数值模拟研究

应用了结构网格中的Chimera重叠网格技术和Favre平均三维N-S方程以获得流场解.采用k-ε湍流模型模拟气体的湍流粘性影响,计算中分别考虑空气和两种火箭发动机喷流等三种不同流动介质,采用时间相关边界模拟发动机拖尾段的非定常流动,最终求解带约束的六自由度弹道方程模拟了导弹助推器的分离脱落过程.并对发动机喷流对助推器分离的影响开展研究.所做工作可对于精确确定火箭助推器分离轨迹及姿态提供方法参考.      

宽带相控阵雷达各模块幅相失真对成像的影响

宽带LFM信号作为一种广泛应用于宽带相控阵雷达系统中的信号,在实际应用中一般可采用Stretch处理的方法,实现高距离分辨成像,并大大减少数据采集难度.但它需要很大的瞬时带宽,传统上认为当瞬时带宽较大时,系统的幅相频率特性难以满足要求.通过对实测数据的分析,发现当有源相控阵模块较多时,由于模块之间幅相失真的综合作用,虽然单个模块存在较大的幅相误差,但最终雷达成像性能仍满足设计要求.     

大涵道比风扇设计技术发展趋势

风扇部件是民用涡扇发动机关键部件之一,自20世纪60年代以来在气动设计等方面发生了显著变化,其发展支撑了民机的更新换代。对民机风扇叶片的发展历史进行了回顾,对典型设计特征和参数进行了总结。着重介绍了民机风扇叶片的叶片数、叶尖切线速度、气动叶型设计、降噪设计、材料工艺等发展变化,对其内在原因进行了分析,并评述了其发展趋势。     

基于参数化建模的凸轮动态优化方法

为解决传统凸轮型线优化设计过程中的动力学模型简单、几何精度低以及设计流程自动化程度低的问题,利用MSC.ADAMS平台的参数化建模技术,对设计流程重新进行组织和安排,提出"面向参数化样机的凸轮动态优化方法"的解决方案.本文建立了配气机构的参数化样机,对凸轮型线进行了动态优化设计.优化在考虑零件柔性的同时,提高了几何精度以及设计流程的自动化程度.     

高空低雷诺数二维叶栅叶型优化设计研究

在高空、低速、低雷诺数下,进行具有较强抗分离能力的新叶型研究,探索叶型设计的新概念和新方法,并发展相应的低雷诺数压气机叶片二维设计技术是十分关键的。本文进行了低雷诺数条件下二维压气机叶栅流场计算与对比,在探索高空、低速、低雷诺数对压气机叶型性能影响的基础上,以发展适应低雷诺数流动的、具有较强抗分离能力的新叶型为最终目标,进行叶型设计新理论和新方法的探索,为最终突破低雷诺数下叶型设计的关键技术提供了可行的途径,并为三维叶片优化造型打下了基础。     

Photospheric flows in the active regions (asymmetric and localized Doppler velocities)

We observed 10 active regions through their disk passage during June 25–August 25, 1988, with the Tower Vector Magnetograph (TVM) of Marshall Space Flight Center. The TVM was used in scanning mode to measure the photospheric Doppler velocities with the Line-Center-Magnetogram (LCM) technique in the spectral line of FeI 5250.2 Å. In this paper we present the result of a subset of observations obtained while the active regions were situated away from the solar limb. A wide range of magnetic complexity and associated chromospheric activity characterized these active regions. It was found that the value of zero-crossing wavelength of the integrated Stokes-V profile of two opposite magnetic polarities were different, corresponding to Doppler velocities ranging from ∼100 m s⁻¹ to ∼1475 m s⁻¹. The measurements of relative velocities between different locations, connected by magnetic flux tubes as inferred from YOHKOH soft X-ray and TRACE 171 Å Fe IX images, showed widely different values of dominant localized flows. The region of parasite polarity, which showed recurrent chromospheric activity, was blue shifted with respect to the main “magnetic element” of the same polarity. Some of them were also the sites of sheared magnetic field configuration. The magnitude of the relative velocity between the leading and following polarity is more for the active regions of higher “field asymmetry”.