评价复合固体推进剂中填料/粘合剂相互作用的新方法

为了便于评价复合固体推进剂中填料／粘事剂的相互作用，从填料充填弹性体应力应变公式出发，提出了一种简单而直观地评价填料／粘合剂相互作用的新方法。其在几种不同填料体系的应用表明，该方法不仅可以评价填料／粘合剂的相互作用，还可表征键合剂的作用效果，这一方法具有较大的使用价值。     

Effect of Counterface Material on Friction and Wear Behavior of Ni-Cr-W-Al-Ti-MoS_2 Composites

Ni-Cr-W-Al-Ti-MoS2 self-lubricating composites were prepared through the powder metallurgy (P/M) method. Their friction properties were investigated by a pin-on-disk tribometer in the range from the room temperature to 600 ℃. Alumina, silicon nitride and nickel-iron-sulfide alloys were selected as the counterface materials. Results indicate that the lowest friction coefficients under 0.22 can be obtained at 600 ℃ when rubbed against alumina. When rubbed against nickel-iron-sulfide alloys, are presented the lowest wear rates in the magnitude of 10-6 mm3/N·m, one order of magnitude lower than those when rubbed against ceramics. In the case of three rubbing pairs, the wear rates of the composite containing MoS2 present themselves inversely proportional to friction coefficients. With alumina ceramics used as a counterface, transfer films and glaze layers will form on the contact surface playing a main role in lubrication at high temperatures. However, when silicon nitride and nickel-iron-sulfide alloy are used, the lubricating transfer films appear not to be promi-nent.     

一种基于P2P MMOG的分布式消息分发算法

提出了一种适合于P2P MMOG的分布式消息分发算法。游戏世界通过N-Tree划分为若干个子区域,并从每个子区域中选举出一个协调者节点。对于区域内玩家交互过程中产生的事件,由该玩家通过多播机制发送给其兴趣域中的其他玩家和区域协调者,协调者仅负责保存区域内的对象的状态信息并周期性的进行更新。实验表明该算法能够满足游戏状态的一致性需求,并且能够在较大的程度上降低协调者负载和通信开销,节省了大量的计算资源和宝贵的带宽。     

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.     

一种基于P2P技术的免疫网络入侵检测模型研究

提出一种基于对等网(P2P)技术的免疫网络入侵检测方法,建构了一个P2P免疫网络,定义自体/非自体,实现了免疫学习、疫苗接种等过程.仿真实验表明,该方法能有效提高免疫学习效率,降低免疫计算的FP.     

石墨填料对浸渗热解-熔融浸渗方法制备的C/SiC复合材料结构和性能的影响

采用石墨树脂浆料浸渍三维针刺碳毡增强体,热解后得到C/C多孔体,并采用反应熔体浸渗法制备C/SiC复合材料.研究了石墨填料对C/C多孔体的结构以及C/SiC复合材料力学性能的影响.结果 表明,石墨树脂浆料浸渍时树脂填充束间小孔形成结构致密的亚结构单元,而石墨可以有效填充胎网层等大孔隙,一次浸渍热解后碳产率有效提高.所得...     

聚苯乙烯粉末选择性激光烧结成型机理的研究

分析了聚苯乙烯粉末材料选择性激光烧结成型机理,并通过填充改性方法提高其成型性能.结果表明,添加无机填料可提高聚苯乙烯粉末材料烧结性能,而且,多种填料同时添加,效果更明显.     

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.     

基于CAN总线改进的机车数据采集系统

介绍了基于CAN总线改过的机车数据采集系统.采用内嵌CAN控制器的微处理器(P87C591)来改进传统模拟仪表,使它们成为具有相互通讯能力的智能仪表(节点),通过CAN总线和上位机通讯,对各仪表测量数据采集、存储、分析和管理来监测机车运行状况,保证机车的正常运行.具有记录面广、存储容量大、数据处理灵活等优点,有广泛的应用前景.     

The Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First Results

The Grain Impact Analyser and Dust Accumulator (GIADA) onboard the ROSETTA mission to comet 67P/Churyumov–Gerasimenko is devoted to study the cometary dust environment. Thanks to the rendezvous configuration of the mission, GIADA will be plunged in the dust environment of the coma and will be able to explore dust flux evolution and grain dynamic properties with position and time. This will represent a unique opportunity to perform measurements on key parameters that no ground-based observation or fly-by mission is able to obtain and that no tail or coma model elaborated so far has been able to properly simulate. The coma and nucleus properties shall be, then, clarified with consequent improvement of models describing inner and outer coma evolution, but also of models about nucleus emission during different phases of its evolution. GIADA shall be capable to measure mass/size of single particles larger than about 15 μm together with momentum in the range 6.5 × 10⁻¹⁰ ÷ 4.0 × 10⁻⁴ kg m s⁻¹ for velocities up to about 300 m s⁻¹. For micron/submicron particles the cumulative mass shall be detected with sensitivity 10⁻¹⁰ g. These performances are suitable to provide a statistically relevant set of data about dust physical and dynamic properties in the dust environment expected for the target comet 67P/Churyumov–Gerasimenko. Pre-flight measurements and post-launch checkouts demonstrate that GIADA is behaving as expected according to the design specifications. The International GIADA Consortium (I, E, UK, F, D, USA).