小型平板CPL实现高热流密度散热的研究

针对小型平板毛细抽吸两相流体回路(CPL)在高热流密度下的特点,分析了不同工质时系统的压力损失与毛细芯的毛细抽吸力,得出采用氨工质有着较好的传热性能和更高的毛细限,同时得出影响系统毛细限的主要因素是蒸汽联管管径和工质的蒸气密度,提出了工质传输系数作为选取工质的重要指标。建立了蒸发器多孔芯,金属壁面以及工质气、液空间区域的耦合数学模型,并运用SIMPLE算法进行求解,得出蒸发器内的温度分布及由于侧壁效应对多孔芯传热传质与传热极限的影响,同时提出小型平板CPL系统存在侧壁效应传热极限,它是影响系统最大传热量的一个重要极限,在设计小型平板CPL必须予以考虑。     

空间粉尘高速撞击对光学玻璃透过率影响的研究

航天器在轨服役期间会遭受到大量的微陨石及空间微小碎片撞击作用。这些微陨石和空间微小碎片可能吸附在航天器光学玻璃表面,也可能与光学玻璃表面碰撞产生陷坑等缺陷。文章采用爆炸式粉尘加速器加速微米级铝粉末撞击K8光学玻璃,在玻璃表面产生大量碰撞陷坑形成砂蚀磨损现象,利用CΦ-46型分光计测量光学玻璃的透过率。结果表明,光学玻璃磨损区域的透过率明显下降。透过率下降程度与陷坑数量成比例。通过对单个陷坑的计算,当陷坑深度大于或等于一个粒子直径时,光线衰减程度达到最大。     

飞航导弹电子对抗体系及其发展趋势

阐述了在电磁状况日益复杂的战场环境下,飞航导弹作为主战武器面临的几种主要的电子对抗威胁。对电子对抗体系的发展和特点进行了研究,并将国外的电子对抗体系分为雷达和光电两大类进行了介绍,总结了其发展趋势。对飞航导弹的研制及其电子对抗体系的建立提出了参考建议。     

高压静电场中油液射流特性的实验研究

依据静电学和液体荷电的基本原理,分析了高压静电场中荷电油液在射流区、过渡区和雾化区的特性,提出射流长度,雾化角和液滴粒径分布是描述液体荷电射流特性的主要指标。通过自行设计和组装实验装置,分别探讨了不同电压下油液的射流长度和雾化角随电压的变化关系以及液滴粒径在电场中的分布规律。研究表明：射流长度随着电压的增大,总趋势是减小的,但在不同区域,电压对射流长度的影响不同;雾化角随电压增大到一定程度后,逐渐减小,最后趋于稳定;液滴的粒径随着电压的升高不断减小,当电压在65kV左右时,粒径较小且分布最为均匀。     

蚌壳式反推装置打开时反推性能参数计算

根据自由流线理论建立了蚌壳式反推装置二维流动数学模型,得到蚌壳式反推装置打开时反向气流偏转角 与蚌壳式反推装置几何参数间的关联关系。将该模型和涡扇发动机性能计算模型耦合,得到了蚌壳式反推装置打开时反推参数的计算模型。以某型涡扇发动机为例,计算了着陆时反推气流角和反推装置几何参数,以及反推力随马赫数、发动机转速的变化关系,并与测量数据进行了对比分析。表明本文给出的蚌壳式反推装置打开时反推性能计算模型具有较好的计算精度。     

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.     

The dust content of clusters of galaxies

We have statistically investigated the infrared luminosity of clusters of galaxies in comparison with the known tracers of the cluster mass like the X-ray luminosity and the cluster richness (e.g. the number of member galaxies). Our results show that there is a clear positive correlation of the infrared luminosity with the cluster mass. Quantitatively speaking, the infrared luminosity is on average 20 times higher than the X-ray luminosity. Moreover, the infrared luminosity increases with the redshift. This probably shows that a major part of this infrared luminosity is due to star formation in the member galaxies. Another possible contribution would be the thermal emission from dust particles in the diffuse intracluster medium. However our method does not allow us to infer conclusions about this second hypothesis. Depending on their size and abundance, such particles would contribute to the infrared luminosity of galaxy cluster and have an impact on the cooling function of the baryons and thus on the formation of the large scale structures. This is an important cosmological question which still remains open.     

缓蚀剂在工业纯铁/盐酸体系中缓蚀能力的快速评价方法

研究了聚丙烯酸（ＰＡＡＣ）、苯扎溴铵（ＤＢＤＡＢ）在工业纯铁／盐酸体系中的缓蚀性能,推导了一种既能快速测出腐蚀缓蚀剂的缓蚀效率又能确定腐蚀缓蚀剂类型的新方法,定义了能够确定腐蚀缓蚀剂类型因子Ｐ。研究结果表明,Ｐ〉１．００的缓蚀剂为阳极型的缓蚀剂,Ｐ〈１．００的缓蚀剂为阴极型缓蚀剂。     

月球粉尘的研究现状

随着我国探月工程的开展,面临着月球粉尘危害性的问题,急需开展月球粉尘的研究。文章在调研的基础上,阐述了目前国外在月球粉尘方面的研究现状,主要是美国"阿波罗"计划中对月尘的特性、危害性、探测和防护方面的研究。     

卫星总装过程静电防护研究

静电防护是卫星总装过程中质量控制和安全保障的一个重要方面.为了提高航天器总装过程的静电控制水平,文章以某型号卫星为例,针对卫星总装实施特点,对卫星的总装过程进行了静电防护的相关试验和分析研究.首先使用FMEA分析表格,提出静电防护的关键项目,再利用静电检测手段,对这些关键项目进行静电测试.根据测试结果数据分析,查找出卫星总装过程中静电防护的薄弱环节,并针对性地提出相应的静电控制措施.这些研究成果为航天器总装静电控制的具体实施提供了技术支持,是对航天器总装过程静电防护深入研究的有益探索.