玻璃材料非球面的加工方法

着重阐述了现有玻璃材料非球面加工方法,介绍各种方法的加工原理,并给出了各自的优缺点。     

微重力环境下推进剂贮箱中三维气液平衡界面的数值模拟

以部分管理表面张力贮箱的管理舱为研究对象,利用三维气液平衡界面计算程序Surface Evolver,在无重力和微重力且几何边界条件比较复杂的环境下对管理舱内的气液平衡界面进行数值模拟;计算结果与已经应用卫星的理论计算完全吻合。     

离心压气机通流/造型/CFD参数化优化设计集成反问题方法

在自主开发的离心压气机通流/造型反问题设计程序的基础上, 发展了一套离心压气机的通流/造型/CFD于优化设计程序系统下集成的反问题方法, 建立了离心压气机的参数化优化设计平台.采用“试验设计+响应曲面模型+近似优化”的快速优化算法, 对一个10 daN推力级微型涡喷发动机的离心压气机进行了多准则气动优化.结果表明, 这种过程集成的快速优化方法是很有效的.      

Plasma Niobium Surface Alloying of Pure Titanium and its Oxidation at 900℃

A niobium-modified layer on pure titanium surface was obtained by means of double glow plasma surface alloying technique. The modified layer was uniform, continuous, compact and well adhered to the substrate. The niobium composition in the modified layer decreased gradually from the surface to the substrate. The oxidation behavior of the niobium-modified layer was investigated and com- pared with the untreated surface at 900 ℃ for 100 h. Characterization of the layers was performed using X-ray diffraction and scanning electron microscope, respectively. The test results show that the oxidation behavior of pure titanium was improved by niobium alloying process. Niobium has a positive influence on the oxidation resistance.     

水上飞机浮筒外形设计的微机系统

本文介绍了一个水上飞机浮简外形设计的微机系统FCDS。浮筒外形是一张须满足流体静、动力等性能要求的复杂的三维曲面。FCDS以性能优良的库模型作为外形曲面生成的基础,使曲面的进一步设计有了一定的流体性能上的保证。系统用非均匀有理B样条来作曲线曲面的拟合和交互设计。不仅继承了普通多项式非均匀B样条重节点、重顶点等设计技巧,而且增加了形状调节的能力,同时可将二次曲线曲面统一在三次有理式中。系统提供了用穗坂卫法直接光顺空间曲线和曲面的功能,可对浮筒外形进行光顺处理,提供直接用于制造的数据。文中还对FCDS这类专业曲面CAD系统的设计构思、结构组成作了探讨。系统设计的通用性构思,使FCDS稍作修改即可用于其他飞机部件的外形设计。     

ΔDsat,a QB50 CubeSat mission to study rarefied-gas drag modelling

A CubeSat mission to study the impact of flow incidence angle, surface material and surface roughness on gas–surface interactions on spacecraft in low Earth orbits has been designed. To accomplish this scientific goal the CubeSat deploys a variable geometry aerofoil capable of exposing different surfaces to the flow at different incident angles. By using the on-board GPS measurements and an orbit determination technique the drag experienced by the CubeSat can be estimated. The CubeSat has been designed to be part of the QB50 mission, and hence it carries a sensor that can take in-situ measurements of the atmosphere. This is then used to estimate the atmospheric density and hence to extract information on the drag coefficient. To minimise any bias present in the measurement chain a differential approach is used. Therefore no absolute drag coefficients are estimated, instead, ratios of drag coefficients are computed. This allows direct comparisons of the drag coefficients of different materials, different surface roughness or different incident angles. Simulations indicate that this CubeSat mission will be able to obtain drag coefficient ratios with an uncertainty level of less than 5%.     

水泥混凝土路面损坏的原因及防治措施

水泥混凝土路面具有强度高、使用寿命长、稳定性好、不易变形等特点,在建设中广泛采用。但在行车荷载和环境因素的作用下会出现不同类型的损坏,本文据此有针对性地采取了防治措施,以避免水泥混凝土路面损坏。     

MESSENGER and the Chemistry of Mercury’s Surface

The instrument suite on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft is well suited to address several of Mercury’s outstanding geochemical problems. A combination of data from the Gamma-Ray and Neutron Spectrometer (GRNS) and X-Ray Spectrometer (XRS) instruments will yield the surface abundances of both volatile (K) and refractory (Al, Ca, and Th) elements, which will test the three competing hypotheses for the origin of Mercury’s high bulk metal fraction: aerodynamic drag in the early solar nebula, preferential vaporization of silicates, or giant impact. These same elements, with the addition of Mg, Si, and Fe, will put significant constraints on geochemical processes that have formed the crust and produced any later volcanism. The Neutron Spectrometer sensor on the GRNS instrument will yield estimates of the amount of H in surface materials and may ascertain if the permanently shadowed polar craters have a significant excess of H due to water ice. A comparison of the FeO content of olivine and pyroxene determined by the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) instrument with the total Fe determined through both GRNS and XRS will permit an estimate of the amount of Fe present in other forms, including metal and sulfides.     

月球表面及月壤内温度分布特征的数值模拟

文章建立了月表辐射与月壤内二维非稳态导热的耦合传热模型,采用控制容积法数值模拟月壤内的温度分布,主要研究了月表、月壤内温度的分布和变化规律及探测器对局部月表温度的影响。计算结果表明一昼夜期间月壤内存在明显的温差:浅层月壤处的昼夜温差较大且受纬度的影响明显;随着深度的增加,月壤昼夜温差降低并趋于稳定,且受纬度的影响较小。探测器的存在遮挡了月表接受的太阳辐射,导致其阴影区域内月表温度发生突变,新的平衡温度接近探测器底面温度,且受探测器驻留时间的影响较小;当探测器移开,月表温度又迅速恢复到原有的变化规律。