Sc在L10-TiAl金属间化合物中占位的理论研究

基于密度泛函理论,运用第一原理赝势平面波方法,采用CASTEP量子力学能量软件包研究了Sc占据Ti位与Sc占据A l位的超胞晶格常数、原子形成热、超胞总态密度与电子密度差分图,两种情况对比下,在L10-TiA l合金中,Sc优先占据Ti位,这一结论为进一步研究三元系TiA l-Sc合金提供了理论研究的基础。     

有机高分子絮凝剂处理高浊度原水效果和机理研究

本文研究了有机高分子絮凝剂ＰＡＭ、ＣＴＡＢ及它们的复配ＰＡＭ＋ＣＴＡＢ处理高浊度原水的最佳实验条件、絮凝性能、效果和机理，为有机高分子絮凝剂的选择和管式絮凝器的研制提供了理论依据。     

CPL技术在FY—1C卫星中的应用

为使FY 1C卫星上的镉镍电池可向空间散热 ,以降低工作温度 ,采用了毛细泵回路 (CPL)技术。介绍CPL的工作原理、主要组成以及在卫星上控制星载设备温度应用的设计技术 ,给出了在地面进行的各项热性能试验情况。卫星在轨运行测试验证表明 ,卫星温度处于最佳状态 ,镉镍电池组的温度控制在 (4～ 9)℃的范围内 ,6台镉镍电池之间温差小于 3℃ ,满足镉镍电池的特殊温度要求     

Thermal Fatigue Behavior of Ni_3Al Based Superalloy IC6E

The thermal fatigue behavior of Ni3Al based superalloy IC6E during the cycles between 900 ℃/1 000 ℃ and the room tempera-ture was investigated. The experimental results indicate that the primary and secondary thermal fatigue cracks initiate inside or round the borides and then spread away along grain boundaries and/or in interdendritic areas. The fracture of borides and their separation from the matrix at interfaces are mainly responsible for the crack initiation and its spreading. At temperatures higher than 1 000 ℃, the grain boundary oxidation combined with cyclic stresses accelerates the crack growth.     

DS18B20在YWJC-1C型ECS原位检测仪中的应用

主要介绍在YWJC-1C型ECS原位检测仪中单线数字温度传感器DS18B20的测量原理、特性及其温度测量的硬件接口设计和软件设计。     

应变速率和温度对NiAl-30Cr-4Mo 共晶合金拉伸性能的影响

研究了温度和应变速率对NiAl-30Cr-4Mo共晶合金的拉伸性能的影响.研究结果表明在同一应变速率(1.67×10-4/s)下,随着温度的升高,材料的塑性增加;在韧脆转变温度(BDTT)923 K以上,随着应变速率的降低,合金的拉伸断口韧窝密集程度增大,合金塑性断裂的趋势越明显,且屈服强度随应变速率的降低而下降.     

用一种新型焊丝焊接TC18钛合金的接头性能与组织研究

对采用研制的焊丝和采用TC18同质焊材钨极氩弧焊焊接TC18钛合金的接头力学性能及微观组织进行了对比研究,结果表明:采用同质焊材焊接TC18钛合金只能保证接头的强度指标,而采用研制的新型焊丝焊接TC18钛合金,可以保证接头具有优良的综合力学性能.     

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.     

数字化机载环控地面检测系统的研究

通过采用两片PIC18F448及其外围器件实现了机载环控地面检测系统的数字化设计。通过I^2C总线实现两片单片机之间的数据传输与协调，并利用其CAN接口模块实现多套检测系统的网络化和远程控制操作。     

复合材料锥壳0°铺层的自动铺放成型方法研究

研究了一种基于自动铺带技术的复合材料锥壳0°铺层成型方法：根据锥壳构件尺寸将等宽预浸带数控分切成预定尺寸的直角梯形预浸带片，按特定方式铺放到锥壳表面并使每两片拼成一个等腰梯形单元，多个等腰梯单元形构成锥壳的0°铺层；并针对这种成型方法设计了一种实现锥壳0°铺层自动成型的装置。采用该方法及其设备可以实现锥壳0°铺层的自动化制造，提高成型效率、降低废料率、稳定工艺质量，降低装备制造成本。