跨声速翼型绕流的Euler／边界层方程干扰数值解

本文利用Euler方程和可压缩湍流边界层积分方程研究绕跨声速翼型的有粘与无粘强干扰流动。应用有限差分法在贴体的网格上求解时间相关的Euler方程,以剪功积分方法求解翼面贴附和分离湍流边界层流动,并引入一个松弛方程描述剪应力对上游湍流历程的延迟响应。有粘/无粘干扰采用表面源模型。计算结果表明,对翼面存在强干扰流动情况,获得了与实验值基本吻合的结果。     

基于铱星/INS组合定位技术在船舶中的应用研究

GNSS拒止环境下惯性/GNSS组合导航系统的性能会严重恶化,通过利用并提取机会信号中的有用观测量,可以实现机会信号和惯性系统的联合动态定位。提出了利用铱星/INS组合定位技术实现船舶的动态定位。首先深入研究了铱星的信号体制,建立了利用铱星瞬时多普勒频移进行定位的算法模型;然后,提出了利用基于扩展卡尔曼滤波(EKF)技术的铱星机会信号与INS组合定位算法;最后,通过船舶航行实测数据对所提算法进行了试验验证。结果表明,提出的利用铱星机会信号和INS组合定位方法可以有效改善无GNSS信号条件下的INS定位精度,在GNSS信号拒止环境下解决了船舶定位问题,具有重要的研究意义和实用价值。     

二维C/C复合材料高温力学、热物理性能研究

研究了二维C/C(2D -C/C)复合材料在高温下层剪强度、弯曲强度和模量、热导率和线膨胀系数的变化规律。结果表明 ,所制得的 2D -C/C复合材料的层剪强度随温度的升高变化不大、弯曲强度随测试温度的升高而增加 ;2 0 0 0℃的层剪强度、弯曲强度分别达到 1 4 .8MPa和 2 2 7.4MPa ,较室温分别提高了9.6 %和 6 0 %。弯曲模量在 1 0 0 0℃时增加到 39.4GPa ,在 2 0 0 0℃则下降 ,低于室温数值。 2D -C/C复合材料的热导率、线膨胀系数在z向和x -y向都具有明显的各向异性。未石墨化 2D -C/C复合材料 2 0 0℃的z向热导率是 4 .4 1W / (m·K) ,且随温度的升高而增加 ;而石墨化 2D -C/C复合材料 2 0 0℃的z向、x -y向热导率分别是 1 8.0 2W / (m·K)和 73.2 9W / (m·K) ,随温度的升高而下降。 2D -C/C复合材料在z向的线膨胀系数较大 ,80 0℃以内在 8× 1 0 - 6 /K～ 1 0× 1 0 - 6 /K之间 ;而在x -y向线膨胀系数在 80 0℃以内都很小 ,基本上接近于零     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

The History and Dynamics of Comet 9P/Tempel 1

Since its discovery in 1867, periodic comet 9P/Tempel 1 has been observed at 10 returns to perihelion, including all its returns since 1967. The observations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary nucleus. The successful nongravitational acceleration model did not assume any change in the comet’s ability to outgas from one apparition to the next and the outgassing was assumed to reach a maximum at perihelion. The success of this model over the 1967–2003 interval suggests that the comet’s spin axis is currently stable. Rough calculations suggest that the collision of the impactor released by the Deep Impact spacecraft will not provide a noticeable perturbation on the comet’s orbit nor will any new vent that is opened as a result of the impact provide a noticeable change in the comet’s nongravitational acceleration history. The observing geometries prior to, and during, the impact will allow extensive Earth based observations to complement the in situ observations from the impactor and flyby spacecraft.     

不同制备工艺对MoSi2涂层抗氧化性能的影响

为解决MoSi2和SiC线膨胀系数差异,在带有SiC外涂层的C/C复合材料表面采用等离子喷涂、电弧沉积和固渗等工艺制备MoSi2涂层。涂层表面形貌分析发现,等离子喷涂MoSi2涂层多孔不致密,电弧沉积MoSi2涂层易开裂剥落;而固渗MoSi2涂层致密均匀,且界面结合力好。氧化试验也表明,固渗MoSi2涂层性能较好。     

基于IGES的CAD/CAM后置处理器的实现

IGES是实现不同CAD/CAM系统之间的数据转换的文件标准,介绍了IGES的主要特点以及基于IGES的CAD/CAM平台后置处理器设计的基本过程。将一种CAD/CAM平台的模型数据通过IGES转换标准导入另一种CAD/CAM平台中,实现了模型数据的共享。     

DD6单晶合金的高温蠕变/疲劳损伤研究

利用高频感应加热的方法对DD6单晶合金的高温蠕变／疲劳损伤性能损伤统一本构方程对其各向异性特点和损伤发展规律进行了有限元数值计算。研究发现，DD6单晶合金的高温蠕变／疲劳性能存在明显的方向性，同时在高温条件下蠕变损伤对试件破坏起重要作用，蠕变与疲劳的交互作用会大大缩短材料的循环寿命。     

G/K织物混杂增强复合材料层合板冲击损伤特性研究

采用空气炮实验装置、渗透剂增强的X射线照相法和高强光背射法对中心受到横向冲击的G／K织物混杂增强复合材料层合板的冲击损伤情况进行研究，讨论了G、K织物交替铺层时层合板的应力特征与损伤状况，分析了面、背板与芯板材质变化时层合板的应力与冲击损伤的关系、铺层角变化时层合板的损伤特征。结论强调指出，为提高复合材料层合板的抗弹能力，应采用混杂铺层、铺层角的错配方式，并避免将Kevlar作为背板使用。