钼-铌合金原料品质对单晶制备的影响

主要讨论了钼-铌合金原料品质,包括烧结条的制备、原料的化学成分、原料棒的尺寸规格等对单晶制备的影响。结果表明:高温真空烧结钼-铌合金烧结条由于C、O等杂质含量过高,在20 kW电子束悬浮区域熔炼炉上区域熔炼时未能直接生长制备出单晶,但其经过两次电子束熔炼获得的Ф(12~17)mm原料棒C元素质量分数降为6.3×10-3%、O元素质量分数降低了近2个数量级,仅为1.4×10-3%,能稳定地生长制备出Ф31 mm×735 mm的大尺寸钼-铌合金单晶,而直径超过Ф18 mm或小于Ф11 mm原料棒在区域熔炼时未能获得钼-铌合金单晶。     

SCR技术制备A2017半固态材料及其触变性能的研究

单辊搅拌技术 (SCRShearing/CoolingRollProcess)技术制备的A2 0 17半固态材料比常规铸造坯组织优良 ;SCR技术制备的A2 0 17半固态材料在 5 30～ 5 70℃范围内 ,可以进行触变成形 ;半固态成形平均屈服强度比热加工时的屈服强度低 10MPa ;A2 0 17半固态材料触变过程分为四个阶段 ,稳定触变阶段A2 0 17半固态材料的触变性能稳定 ,半固态加工时容许的最大加工变形范围为 6 4 %～ 72 %。     

LC9高强度铝合金过时效工艺试验

通过对ＬＣ９高强度铝合金过时效工艺试验，并与ＬＣ９ＣＳ状态作性能对比，证实该材料具有良好的耐应力腐蚀及抗裂纹扩展性能，从而确认ＬＣ９ＣＧＳ３铝合金在飞机上推广使用的可行性。     

应用ART1神经网络仿真车间分组

阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。     

高强度铸造铝合金ZL205微弧氧化陶瓷膜的耐腐蚀性能研究

采用中性盐雾腐蚀试验法研究厚度对高强度铸造铝合金ZL205微弧氧化陶瓷膜的耐腐蚀性能的影响.结果表明,微弧氧化处理能显著提高ZL205的耐腐蚀性能,随着厚度的增加,陶瓷膜的耐腐蚀性能提高,但在厚度达到一定值后,陶瓷膜的耐腐蚀性能提高不明显.SEM和XRD结果表明,随着厚度的增加,微弧氧化膜的表面形貌和相结构都发生变化,从而导致微弧氧化膜的耐腐蚀性能发生变化.     

铝合金管材热态内高压成形研究

通过热拉伸实验研究5A02铝合金管材在不同温度下的力学性能.根据热拉伸实验结果进行管材热态液压胀形数值模拟,并进行初步的实验研究.数值模拟结果和实验结果表明,5A02铝合金管材的成形性能随着温度的升高而得到明显改善,理想成形温度为200～230℃.对数值模拟结果与实验结果之间的差别进行分析和讨论.     

Expectations for Infrared Spectroscopy of 9P/Tempel 1 from Deep Impact

The science payload on the Deep Impact mission includes a 1.05–4.8 μm infrared spectrometer with a spectral resolution ranging from R∼200–900. The Deep Impact IR spectrometer was designed to optimize, within engineering and cost constraints, observations of the dust, gas, and nucleus of 9P/Tempel 1. The wavelength range includes absorption and emission features from ices, silicates, organics, and many gases that are known to be, or anticipated to be, present on comets. The expected data will provide measurements at previously unseen spatial resolution before, during, and after our cratering experiment at the comet 9P/Tempel 1. This article explores the unique aspects of the Deep Impact IR spectrometer experiment, presents a range of expectations for spectral data of 9P/Tempel 1, and summarizes the specific science objectives at each phase of the mission.     

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.     

钛的相变织构及其影响因素研究

通过晶体学取向分布函数（ＣＯＤＦ）法研究了冷轧形变量、再结晶退火和相变循环次数等因素对钛相变织构形成的影响。结果表明冷轧形变量对相变织构的形成影响最大。再结晶退火后钛的相交织构漫散。多次循环相变并不改变相变织构的类型。     

钛合金表面镍包石墨喷涂层的耐磨性能

为了提高钛合金的表面耐磨性,利用氧乙炔热喷涂枪,在TC4合金表面上制备出镍包石墨涂层。采用MXP-2000型销盘式摩擦磨损实验机,进行钛合金及其镍包石墨涂层的干摩擦磨损实验,并利用扫描电镜对磨损表面进行观察和分析。实验结果发现,镍包石墨涂层的摩擦系数只有钛合金的一半左右,前者磨损量为后者的1/6,说明镍包石墨涂层可以大大提高钛合金的表面耐磨性能。TC4合金的磨损机制以黏着磨损为主,喷涂层的磨损机制以磨粒磨损为主,喷涂层中的石墨润滑相是其耐磨性高的主要原因。