铝合金燃油-液体热交换器制造技术

分析了燃油———液体热交换器的结构特点及翅片成形和芯体焊接难点,重点介绍了翅片成形和芯体盐浴钎焊工艺方法及获得的技术经济效果。     

抗氧化处理对3D C/C复合材料性能的影响

研究了采用化学气相反应法制备的SiC抗氧化涂层对3D整体编织C／C复合材料的密度、力学性能以及微观结构的影响。结果表明，3D C／C复合材料经抗氧化处理后，其密度、开孔率以及力学性能均有不同程度的提高。由SEM微观结构可以看出，其力学性能提高是由于气态Si渗入到材料基体内部，并与内部的C反应生成SiC，在一定程度上弥合了材料中的缺陷所致。     

带肋和双排出流孔通道的流动特性

研究了通道进口雷诺数和总出流比对带肋和双排出流孔通道流量系数和压力分布的影响。实验研究的通道入口雷诺数为3×104~1.5×105,通道总出流比为0.09~0.22。结果表明:通道总出流比较小时,流量系数沿流向减小。通道进口雷诺数增加,流量系数先增加,之后基本不变;通道总出流比较大时,流量系数基本不变;各工况下总压系数沿流向依次经历迅速减小、基本不变、继续减小的过程;沿流向各位置上的总压系数在通道进口雷诺数为6×104~9×104时最小;出流比增大,沿流向各位置上的总压系数随之增大。     

基于解析及特征造型的涡轮冷却叶片参数化设计

基于数学解析与特征造型技术相结合的方法,建立了基于构造过程的复杂涡轮冷却叶片的参数化设计技术。用五次多项式描述叶身型线,根据壁面厚度函数求解冷却通道外形,定义冷却通道隔板位置及厚度等参数,计算得到叶身及冷却通道各截面造型数据;以特征造型方法完成对涡轮冷却叶片转弯流道、缘板、榫头及叶片相关特征的参数化设计;利用CAD系统的二次开发接口,实现了多腔回流式涡轮冷却叶片的自动建模。     

倾斜30°锥形喷孔气膜冷却的流动和传热实验研究

对流向倾角为３０°、锥顶角分别为１５°和３０°的锥形气膜冷却喷口射流下游的流动和传热进行了详细的实验研究，并与相同实验条件下圆孔的射流情形进行了比较，发现锥形喷口下游的速度边界层的等值线具有三种基本分布形态。随着锥形出口面积的增大，射流的穿透能力明显减弱，核心区域速度明显降低，侧向扩展范围明显增加，纵向耦合涡迅速减弱并消失，从而显著地提高了气膜冷却效率，尤其是提高了喷孔两侧流向下游位置上的冷却效率。同时，大锥顶角的高吹风比下，射流具有十分良好的贴壁效应和非常可观的冷却效率。     

基于C/S结构的远程维护系统

提高计算机应用系统的可维护性，降低维护代价，一直是项目研发人员追求的目标。给出一种新的系统维护方法；系统采用客户机/服务器模式，通过Internet对远程机进行控制与操作，完成系统维护信息的搜集与发送，实现远程系统的故障诊断和软件的维护工作，对用VC 实现的核心技术做了说明。现已应用于自动化立体仓库系统远程维护工作中。     

基于FW-H方程的旋翼气动声学计算研究

由流体力学N S方程导出的非齐次波动方程———FfowcsWilliams Hawkings方程(简称FW H方程),可以精确地描述在静止流体中运动的物体与流体相互作用的发声问题。以FW H方程为理论模型,将旋翼桨叶运动发声问题等效为包含桨叶的任意运动控制面(声源面)的声辐射问题,并在旋翼绕流Euler方程数值模拟的基础上,在时域内计算了悬停旋翼和前飞旋翼的声场。应用于UH 1H和AH 1/OLS两种旋翼模型的气动声学计算表明:计算结果与噪声实验值符合良好;所研制的程序不仅能够较准确地计算单极子噪声和偶极子噪声,而且具有较强的跨音速四极子噪声预测能力。     

基于MSC/PATRAN的飞机结构强度静力试验数据实时跟踪与处理系统开发

 在Windows环境下,以MSC/PATRAN为平台，利用平台提供的二次开发语言PCL(Patran Command Language)，并结合C++语言，通过客户化、增设特定的命令和窗体等技术开发了飞机结构强度静力试验数据实时跟踪与处理系统TestDTAS（Test Data Tracking, Analyzing and Processing System）。在结构试验进行中，TestDTAS可以实时地监测结构试验件中应力和位移的变化情况，并与理论分析结果进行对比，而在试验结束后，TestDTAS可以进行试验数据回放和分析，从而将试验与理论分析有机的结合在一起，对结构静力试验和结构设计有很高的实用价值。     

C/C复合材料1 800℃抗氧化涂层探索研究

提出并制备了可以应用于1 800℃的抗氧化涂层体系,固渗法制备SiC内层,料浆涂刷法制备高温氧化物釉层和硼硅化物釉层.经扫描电镜分析涂层形貌及电子能谱分析其组成,发现C/C复合材料基材结构完整,没有发生次表面氧化.试验结果表明氧乙炔焰烧蚀20 s后,失重为0.06%;1 800℃自然对流氧化试验条件下,氧化物釉层30 min的平均失重速率为0.06g/(m2·s);硼硅化物釉层60min的平均失重速率为0.2g/(m2·s).说明涂层体系在1 800℃具有良好的抗氧化能力.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.