SiC含量对Ti3SiC2/SiC复合材料性能的影响

采用反应热压烧结法制备了Ti3SiC2/SiC复合材料,针对SiC含量对该复合材料致密化程度、力学性能以及应力.应变行为的影响进行了研究.结果表明:(1)随着SiC含最的增加,试样难于致密,试样需要在更高的温度才能达到较高的致密度;(2)随SiC含量的增加,Ti3SiC2/SiC复合材料弯曲强度和断裂韧性提高,但SiC含量达到50%时,由于复合材料含有较多的孔洞,使强度和断裂韧性降低;(3)Ti3SiC2/SiC复合材料在常温下表现为非脆性断裂.     

美国BMDS网络化作战核心系统C2BMC的发展

随着网络化作战的发展,实现弹道导弹防御系统(BMDS)之间及其与信息源之间的互连、互通和互操作将成为一种必然的趋势,为此,美国导弹防御局提出了指挥控制、作战管理和通信(C2BMC)系统.主要从整个BMDS网络化作战建设的角度,分析了C2BMC的构成与功能、研制进展、具体应用和发展趋势.     

A synchrotron-based facility for the in-situ location,chemical and mineralogical characterization of ∼10 μm particles captured in aerogel

NASA’s Stardust mission collected dust from the coma of Comet Wild-2 on January 2nd, 2004, by direct capture into aerogel cells that flew through the dust coma at ∼6 km/s. Stardust collected several hundred comet particles >10 μm in size. These comet samples were delivered to Earth on January 15th, 2006. We developed a facility at the National Synchrotron Light Source at Brookhaven National Laboratory (Upton, NY, USA) for the in-situ characterization of ∼10 μm particles collected in aerogel. These analytical instruments allow us to perform extensive chemical, mineralogical, and size-frequency characterization of particles captured in aerogel. These analyses are conducted without any invasive extraction, minimizing the possibility of contamination or particle loss during preparation. This facility was used to determine the chemical composition, the oxidation state, the mineralogy and to provide an indication of the grain size of the Wild-2 particles before they were removed from the aerogel. This information provides a catalog of particle types, allowing a more reasoned allocation of the particles to subsequent investigators based on a relatively detailed knowledge of the chemical composition and mineralogy of each particle. These measurements allowed a comparison of the chemical and mineralogical properties of the Wild-2 particles with other types of extraterrestrial materials, including interplanetary dust particles and meteorites. The success of in-situ analysis for Wild 2 particles demonstrates that synchrotron-based facilities will be important for the analysis of particles collected in aerogel on future earth-orbiting satellites and spacecraft.     

三维实体模型向二维工程图纸的转化

本文在基于ＡｕｔｏＣＡＯＲ１２支撑软件的基础上，利用其ＡＤＳ和ＡＭＥ函数，讨论了三维实体模型向二维工程图纸的转化的问题，分析了三维实体的三向投影及三个视图的对齐关系。     

Bottom side profiles for two close stations at the southern crest of the EIA: Differences and comparison with IRI-2012 and NeQuick2 for low and high solar activity

Bottom side electron density profiles for two stations at the southern crest of the Equatorial Ionization Anomaly (EIA), São José dos Campos (23.1°S, 314.5°E, dip latitude 19.8°S; Brazil) and Tucumán (26.9°S, 294.6°E, dip latitude 14.0°S; Argentina), located at similar latitude and separated by only 20° in longitude, have been compared during equinoctial, winter and summer months under low (year 2008, minimum of the solar cycle 23/24) and high solar activity (years 2013–2014, maximum of the solar cycle 24) conditions. An analysis of parameters describing the bottom side part of the electron density profile, namely the peak electron density NmF2, the height hmF2 at which it is reached, the thickness parameter B₀ and the shape parameter B₁, is carried out. Further, a comparison of bottom side profiles and F-layer parameters with the corresponding outputs of IRI-2012 and NeQuick2 models is also reported. The variations of NmF2 at both stations reveal the absence of semi-annual anomaly for low solar activity (LSA), evidencing the anomalous activity of the last solar minimum, while those related to hmF2 show an uplift of the ionosphere for high solar activity (HSA). As expected, the EIA is particularly visible at both stations during equinox for HSA, when its strength is at maximum in the South American sector. Despite the similar latitude of the two stations upon the southern crest of the EIA, the anomaly effect is more pronounced at Tucumán than at São José dos Campos. The differences encountered between these very close stations suggest that in this sector relevant longitudinal-dependent variations could occur, with the longitudinal gradient of the Equatorial Electrojet that plays a key role to explain such differences together with the 5.8° separation in dip latitude between the two ionosondes. Furthermore at Tucumán, the daily peak value of NmF2 around 21:00 LT during equinox for HSA is in temporal coincidence with an impulsive enhancement of hmF2, showing a kind of “elastic rebound” under the action of the EIA. IRI-2012 and NeQuick2 bottom side profiles show significant deviations from ionosonde observations. In particular, both models provide a clear underestimation of the EIA strength at both stations, with more pronounced differences for Tucumán. Large discrepancies are obtained for the parameter hmF2 for HSA during daytime at São José dos Campos, where clear underestimations made by both models are observed. The shape parameter B₀ is quite well described by the IRI-2012 model, with very good agreement in particular during equinox for both stations for both LSA and HSA. On the contrary, the two models show poor agreements with ionosonde data concerning the shape parameter B₁.     

Assessment of depth to magnetic sources using high resolution aeromagnetic data of some parts of the Lower Benue Trough and adjoining areas,Southeast Nigeria

High resolution airborne magnetic data acquired between 2005 and 2010 were used to determine depth to shallow and deep magnetic sources in some parts of Southeastern Nigeria. Various depth estimation methods such as standard Euler deconvolution (SED), source parameter imaging (SPI), spectral depth analysis (SDA) and two dimensional (2-D) forward modeling were applied. Results obtained from SED, SPI and models of profiles 1 and 2 indicate that the Abakaliki Anticlinorium (AA) and Ikom-Mamfe Rift (IMR) regions are dominated by short wavelength magnetic anomalies caused by extensive tectonic events. The SED map showed depth to shallow and deep magnetic sources ranging from ~ 16.6 to ~ 338.3 m and ~ 394.3 to ~ 5748.1 m respectively. Likewise, depth estimates from the SPI map varies from ~ 147.1 to ~ 554.2 m (shallow magnetic sources) and ~ 644.2 to ~ 6141.6 m (deep magnetic sources). The result obtained from SDA revealed depths to deep magnetic basement in the range of ~ 769 to ~ 6666 m with an average of ~ 3449 m. Also, it showed that depth to shallow magnetic sources vary between ~ 119 and ~ 434 m with mean of ~ 269 m. The 2-D forward modelling showed maximum depth values of ~ 4700, ~4600 and ~ 6500 m in the models of profiles 1, 2 and 3 within the Anambra Basin (AB), Afikpo Syncline (AS) and Calabar Flank (CF) respectively. Generally, from all the various methods applied the results indicate that AB, AS and CF are dominated by long wavelength anomalies. The 2-D models indicated that the basement framework is undulant. Also, depth estimates involving the various methods used in this study correlate strongly with each other in the AB, AS and CF geological regions.     

密闭空间内氢气和二氧化碳甲醇化系统的非均相模型及反应特性

在载人密闭空间内通过电解水方式为乘员供氧会产生副产物氢气（H₂）。此外,乘员还呼出二氧化碳（CO₂）。将H₂和CO₂催化合成甲醇（CH₃OH）是消除载人密闭空间内富余H₂和CO₂的最优方式之一。对其开展反应过程建模及反应特性研究有助于进行反应过程的控制,更好地维持载人密闭空间内的大气平衡。本文采用微元法建立了H₂和CO₂催化合成甲醇的物料计算模型和温度一维非均相模型,研究了不同反应压力、冷却介质温度以及入口反应气体中CO₂与CO比值等反应条件下的反应特性变化规律。结果显示,反应压力的增加、冷却介质的温升以及入口气体中CO₂与CO比值的减小均能促进各反应速率增加,进而使得H₂和CO₂消除量增加、甲醇合成率上升以及催化剂和反应气体最高温度上升。在保证反应速率增加且催化剂最高温度不超过合理反应温度区间的最大值573.15 K时需维持反应压力不大于8 MPa,冷却介质温度不高于538.15 K以及CO₂与CO比值不小于1。     

TiC／Ti3AlC2复合材料的原位合成

以Ti粉、铝粉和活性碳粉为反应原料,利用高能球磨及热压工艺合成了TiC/Ti3AlC2复合材料.研究了在Ti-Al-C体系中,温度对TiC/Ti3AlC2复合材料的影响,并重点分析了反应过程热力学机理及材料微结构的影响.结果表明:通过高能球磨及热压烧结,在1 300℃时得到了物相比较均匀、致密的TiC/Ti3AlC2复合材料.通过高能球磨使得晶粒不断得到细化,使Ti3AlC2的烧结温度降低,同时分析TiC/Ti3AlC2复合材料微观结构的增韧机理,发现TiC是以颗粒增韧方式镶嵌在Ti3AlC2基体中.     

二硫化钼对二次电子倍增效应的抑制作用研究

基于镀银铝合金材料的微波部件在高真空及大功率工作时容易产生二次电子倍增效应,引起噪声电平抬高,输出功率下降,导致微波部件失效。有效抑制二次电子倍增效应,对于空间微波部件的正常运行极为重要。二硫化钼不仅具有与石墨烯类似的结构,而且其带隙可调,具有出色的电学、光学等性能。通过水热法制备了二硫化钼,并将其涂覆在镀银铝合金材料的表面,研究了复合材料的二次电子发射特性。结果表明,合成的二硫化钼具有花瓣状的纳米结构,并可以显著降低镀银铝合金表面的二次电子发射系数至0.63,原因是三维形态的纳米花瓣状二硫化钼可在微波部件表面构建无数个“微陷阱”,使得二次电子被捕获的几率增加,从而降低其逸出材料表面的概率。表面涂覆二硫化钼的镀银铝合金材料可望用于提高大功率微波部件的阈值功率。     

机动弹道对抗导弹防御系统的效能分析

为了研究机动弹道对抗导弹防御系统的突防效能,梳理了弹道导弹防御系统的组成与作战流程,通过剖析系统的信息流向与处理过程,提炼出机动弹道突防导弹防御系统的机理,即采用机动弹道可使导弹预警信息处理能力下降,从而破坏、瘫痪导弹防御系统,实现导弹的有效突防.通过仿真滑翔机动弹道和椭圆弹道,并对计算的跟踪弧段、弹道估计和预报误差进行比较,结果表明：采用机动弹道,观测弧段压缩44％,弹道估计误差增大数倍,有效预报时间大大缩短.因此,采用机动弹道是导弹突防的一种有效手段.