三维瞬态导热温度场边界元计算及一阶数学奇异的处理

推导了三维瞬态导热温度场边界元解法的积分方程和离散代数方程，并编制了相应的计算机程序，采用坐标变换的解析消去法，处理边界元的一阶数学奇异点，从而提高了算法的数值精度。用本程序计算了正方体和圆柱环瞬态导热温度场，数值解与解析解的吻合程度令人满意。     

美陆军制导武器试验半实物仿真技术综述

主要综述美国陆军制导武器试验的仿真技术和设施，同时介绍仿真试验中使用的几种典型的目标景象投影技术，并说明了它们的应用范围和优缺点。最后介绍了当前制导武器试验仿真技术的发展趋势。     

热暴露对B/Al复合材料性能的影响

对经300℃、500℃高温热暴露的B／Al（LF6）复合材料的力学性能进行了研究，实验结果表明材料在300℃下热暴露时，性能下降速度较慢，100h后强度保留率约为76％，延伸率保留率为74％。而在500℃下热暴露时，5h以上强度就有明显降低。高温长时间热暴露后复合材料的断裂也从积累型转变为典型的非累积型断裂。通过透射电镜（TEM）及扫描电镜（SEM）对固态热压制造态和主温热暴露的界面状况进行了分析，认为界面反应是造成B／Al复合材料力学性能下降的主要原因。     

多孔陶瓷等效导热系数的近似计算

提出了一个近似计算多孔陶瓷等效导效系数的公式。该公式综合考虑了孔隙大小，孔隙度以及气相辐射与导热的影响，可用于在任意温度下具有任意孔隙度的多孔陶瓷的等效导热系数的计算，用文献数据检验表明，该公式在高温区有较高的计算精度。     

固体火箭发动机寿命预估的一种考虑

利用弹性－粘弹性对应原理，分析长期贮存固体推进剂药柱由环境温度变化引起的热应力，计算药柱损伤，并对发动机寿命进行预估。理论分析和算法具有普遍性，可供工程设计参考。     

测量机连续扫描控制系统设计

利用UCC1控制器作为核心,构建具有三维空间连续扫描功能的测量机控制系统的方法,并简要介绍了UCC1控制器的功能及控制系统硬件电路的设计。     

高能氧化剂二硝酰胺铵的热分解研究

为深入了解二硝酰胺铵(ADN)的热分解，为该氧化剂在推进剂中应用提供必要的技术保障和实验依据，采用热重分析法(TG)及差示扫描量热法(DSC)，实验研究了氮气流量、合成中间体烷基羰基N-硝酰胺铵(AUN)及硝酸铵(AN)对ADN热分解过程的影响，并利用model-free isoconversional方法模ADN热分解过程的活化能曲线。结果表明：氮气流量和硝酸铵(AN)对ADN的热分解过程有显著影响，而AUN可使ADN热分解曲线产生肩峰，但基本不影响ADN的热分解过程。     

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。     

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.