A study on turbulence transportation and modification of Spalart–Allmaras model for shock-wave/turbulent boundary layer interaction flow

It is of great significance to improve the accuracy of turbulence models in shock-wave/ boundary layer interaction flow. The relationship between the pressure gradient, as well as the shear layer, and the development of turbulent kinetic energy in impinging shock-wave/turbulent boundary layer interaction flow at Mach 2.25 is analyzed based on the data of direct numerical simulation(DNS). It is found that the turbulent kinetic energy is amplified by strong shear in the separation zone and the adverse pressure gradient near the separation point. The pressure gradient was non-dimensionalised with local density, velocity, and viscosity. Spalart–Allmaras(S–A) model is modified by introducing the non-dimensional pressure gradient into the production term of the eddy viscosity transportation equation. Simulation results show that the production and dissipation of eddy viscosity are strongly enhanced by the modification of S–A model. Compared with DNS and experimental data, the wall pressure and the wall skin friction coefficient as well as the velocity profile of the modified S–A model are obviously improved. Thus it can be concluded that the modification of S–A model with the pressure gradient can improve the predictive accuracy for simulating the shock-wave/turbulent boundary layer interaction.     

机载大功率超导发电机发展现状与展望

新一代飞机对电力的需求越来越大,尤其是定向能武器的使用,将需要兆瓦(MW)级的电源系统。由于超导发电机发电功率大、结构简单、重量轻,是机载大功率用电设备的理想电源。本文综述了机载超导发电机的类型、研究进展和关键技术,分析指出了其未来的发展前景。     

METHIS: Mercury thermal infrared spectrometer

The BepiColombo mission to Mercury is devoted to the thorough exploration of Mercury and its environment, with the aim to understand the processes of planetary formation and evolution in the hottest part of the protoplanetary nebula. This mission represents an unique opportunity for the European community to extend the understanding of the Solar Nebula evolution from its outer edge – ideally represented by comets – to its inner and warmer edge. Obviously this exploration asks for a detailed knowledge of the main constituents of the matter present in the different Solar System areas. Spectroscopy is a powerful tool to acquire this knowledge. We have participated with a large consortium of European researchers to the development of the Rosetta imaging spectrometer. We propose here to use our experience to develop a newly designed spectrometer to investigate the mineralogical composition of the Mercurial surface. Given the particular thermodynamical situation of the Mercurial surface, we have developed a concept that combines a medium IR low spectral resolution imager with a moderate spectral resolution NIR point spectrometer. The main goal of METHIS is to provide the mineralogical characterisation of the surface with sufficient spectral resolution in a scientifically diagnostic spectral range.     

高压涡轮导叶非轴对称端壁优化设计

为使高压涡轮导叶非轴对称端壁造型在减少二次流损失、提高气动性能方面更好的发挥作用,以某一级高压涡轮为研究对象,采用端壁参数化造型、三维Navier-Stokes（N-S）方程流场求解和基于人工神经网络的遗传算法相结合的优化方法对涡轮导叶进行非轴对称端壁的优化设计。优化目标为在控制涡轮导叶进口质量流量、出口马赫数及出口气流角的情况下,导叶出口总压损失系数和出口二次流动能最小化。对比分析优化前后端壁对涡轮导叶出口参数和涡轮级性能的影响。结果表明：优化后得到的非轴对称端壁有效地改善了涡轮导叶通道内的流场,抑制了通道内二次流涡系的发展,降低了导叶出口处的流动损失,涡轮导叶出口总压损失系数降低了14．85％,高压涡轮级等熵效率提高了0．456％。     

纹理能量模板若干性质的研究

从实验出发,对纹理能量模板存在的内在规律及其纹理区域变化所具有的特点进行了探讨,从中总结出了一些有用的性质,获得了满意的试验结果。     

Future X-ray astronomy missions of Japan

Japanese future space programs for high energy astrophysics are presented. The Astro-E2 mission which is the recovery mission of the lost Astro-E has been approved and now scheduled to be put in orbit in early 2005. The design of the whole spacecraft remains the same as that of Astro-E, except for some improvements in the scientific instruments. In spite of the five years of delay, Astro-E2 is still powerful and timely X-ray mission, because of the high energy resolution spectroscopy (FWHM 6 eV in 0.3–10 keV) and high-sensitivity wide-band spectroscopy (0.3–600 keV). The NeXT (New X-ray Telescope) mission, which we propose to have around 2010, succeeds and extends the science which Astro-E2 will open. It will carry five or six sets of X-ray telescopes which utilize super-mirror technology to enable hard X-ray imaging up to 60–80 keV. In mid-2010s, we would participate in the European XEUS mission, which explores the early (z>5) “hot” universe.     

用光纤半圆阵列测量准二维工件表面粗糙度参数的仿真研究

提出了一种反散射计算的简单、快速方法,用于用光纤半圆阵列的光散射技术测量准二维工件表面的粗糙度参数。这些参数包括高度特性参数 R_a、间距特性参数λ_a 和混合参数△_a。我们的研究证明了上述测量方法的正确性。因而,这种测量方法可用于测量工件表面粗糙度参数仪器的设计。     

新型含能材料──CL－20

综述了ＣＬ－２０结构特征、合成方法及热分解性能，并对其作为固体推进剂氧化剂的能量特性进行了计算分析。结果显示ＣＬ－２０具有能量密度高、感度适中等特点，同时具有较好热稳定性和不同于ＨＭＸ的热分解特性，是一种有潜力的高能量密度材料。     

SEP数值法在寿命预测中的应用

 为了预测精密构件如涡轮盘材料的蠕变-疲劳寿命,经实践证明应变能区分法（SEP）优于应变范围区分法（SRP）,特别是对高强度低延性材料,SEP的优越性更明显。