热障涂层在线/离线磷光温度测量技术研究进展

精确测量涡轮叶片表面热障涂层温度对航空发动机和地面燃气轮机设计和研制具有极其重要的意义。近年来,基于热像磷光材料磷光特性的热障传感涂层在线测温技术与热历史磷光涂层离线测温技术得到了迅猛发展。前者通过在线测量高温下磷光信号来获取实时温度信息,后者通过离线测量经高温服役后的磷光材料不可逆磷光信号变化来获取服役温度信息。这两项技术都适用于高温、高腐蚀环境下热障涂层非干涉、非接触式和高精度温度测量,具有广阔的应用前景。从热障涂层在线/离线测温原理与方法、磷光材料与制备及应用3个方面详细介绍了热障涂层在线/离线测温技术的研究现状与技术特点,并对这两种技术的发展进行了展望。     

Investigation of the Influence of Magnetic Anomalies on Ion Distributions at Mars

Using data from the Mars Express Ion Mass Analyzer (IMA) we investigate the distribution of ion beams of planetary origin and search for an influence from Mars crustal magnetic anomalies. We have concentrated on ion beams observed inside the induced magnetosphere boundary (magnetic pile-up boundary). Some north-south asymmetry is seen in the data, but no longitudinal structure resembling that of the crustal anomalies. Comparing the occurrence rate of ion beams with magnetic field strength at 400 km altitude below the spacecraft (using statistical Mars Global Surveyor results) shows a decrease of the occurrence rate for modest (< 40 nT) magnetic fields. Higher magnetic field regions (above 40 nT at 400 km) are sampled so seldom that the statistics are poor but the data is consistent with some ion outflow events being closely associated with the stronger anomalies. This ion flow does not significantly affect the overall distribution of ion beams around Mars.     

液晶聚合物分子复合材料研究进展

回顾了液晶聚合物和分子复合材料的发展历史,介绍了溶致型和热致型液晶聚合物分子复合材料及其常用制备方法,简述了原位复合材料的增强机理、界面相容性、影响液晶聚合物成纤的因素以及分子复合材料深入发展的相关问题.     

RPC-ICA: The Ion Composition Analyzer of the Rosetta Plasma Consortium

The Ion Composition Analyzer (ICA) is part of the Rosetta Plasma Consortium (RPC). ICA is designed to measure the three-dimensional distribution function of positive ions in order to study the interaction between the solar wind and cometary particles. The instrument has a mass resolution high enough to resolve the major species such as protons, helium, oxygen, molecular ions, and heavy ions characteristic of dusty plasma regions. ICA consists of an electrostatic acceptance angle filter, an electrostatic energy filter, and a magnetic momentum filter. Particles are detected using large diameter (100 mm) microchannel plates and a two-dimensional anode system. ICA has its own processor for data reduction/compression and formatting. The energy range of the instrument is from 25 eV to 40 keV and an angular field-of-view of 360° × 90° is achieved through electrostatic deflection of incoming particles.     

深空探测先进电源技术综述

先进电源技术是保障深空探测任务顺利进行的前提和基础。在梳理我国后续深空探测任务(月球极区探测、小天体探测、火星探测、木星探测等)对电源系统需求的基础上,对涉及空间应用的电源技术(化学能、太阳能、同位素及空间核反应堆电源)进行概述;针对深空探测对电源系统的需求特点,分别阐述了锂离子蓄电池、太阳能电源、钚-238放射性同位素电源和空间堆核反应电源的特点、发展简史、在深空探测中应用限制及发展建议,重点分析了钚-238同位素电源和空间核反应堆电源技术的关键技术、应用情况及应用前景,为深空探测先进电源技术的长足发展提供参考。     

分子污染对卫星太阳电池翼输出功率的衰减研究

分子污染是引起卫星太阳电池翼输出功率衰减的因素之一。用直接模拟蒙特卡罗（Direct Simulation Monte Carlo）方法分析了空间分子污染物的传输过程，采用十组不同的输入参数计算了在轨运行期间分子污染物在某型号卫星太阳电池翼表面的沉积膜厚度，分析了太阳电池翼输出功率的衰减情况。     

对叔丁基苯甲酸稀土杂化发光材料的研究

本文合成了几种稀土金属离子（Eu^3＋，Tb^3＋，Dy^3＋）与对叔丁基苯甲酸的二元有机配合物，且将其不同浓度的光活性组分引入TEOS（正硅酸乙酯）基质中利用溶胶-凝胶法水解缩聚得到粉末状固体材料。同时采用了紫外吸收，荧光激发与发射光谱，扫描电镜等手段对样品进行了表征，表明该材料具较高的发光性能，得到了理想的稀土离子特征荧光且发射强度随配合物浓度增加而递增，没有出现明显的浓度淬灭现象。     

“嫦娥一号”卫星观测近月太阳风离子特征

"嫦娥一号"卫星的太阳风离子探测器(SWIDs)的科学目标是研究太阳风与月球的相互作用以及相应的近月空间等离子体环境。文章利用"嫦娥一号"卫星SWIDs探测器在2007年12月30日的观测数据对近月太阳风等离子体环境,包括向阳侧太阳风离子、"拾起"离子以及在月球尾迹边界处的太阳风离子的特征进行分析,得到以下主要观测结果:1)在慢速太阳风中观测到双峰结构,分别为太阳风中的氢离子和二价氦离子;2)在行星际磁场具有明显昏向(+By)分量期间,在月球向阳侧持续观测到有月表散射或反射后被拾起的太阳风离子;3)与入射的太阳风离子不同,这些拾起的太阳风离子具有明显的角度分布特征;4)在行星际磁场昏向(晨向)期间,太阳风中的氢离子在月球尾迹北半球的边界处呈现减速(加速)特征并进入尾迹;而并未发现氦离子进入尾迹的特征。"嫦娥一号"卫星的这些观测数据对于认识近月空间等离子体环境有着重要的意义。     

Catalytic activity of interstellar grains: Formation of molecular hydrogen on amorphous silicates

Silicates constitute an important class of interstellar grain material and are the site of catalytic activities, most notably the formation of molecular hydrogen. Here we report an analysis of experiments conducted in the laboratory to measure the efficiency of formation of molecular hydrogen on amorphous silicates, a realistic analogue of interstellar dust grains. From the measurements, we also obtain the energetics of key processes in the reaction and information on the mechanism of reaction. Comparison with earlier measurements of molecular hydrogen formation on a sample of polycrystalline olivine shows that amorphous materials are more efficient catalysts.     

Numerical investigation of the nonreacting and reacting flow fields in a transverse gaseous injection channel with different species

The mixing and combustion process has an important impact on the engineering realization of the scramjet engine. The nonreacting and reacting flow fields in a transverse injection channel have been investigated numerically, and the predicted results have been compared with the available experimental data in the open literature, the wall pressure distributions, the separation length, as well as the penetration height. Further, the influences of the molecular weight of the fuel and the jet-to-crossflow pressure ratio on the wall pressure distribution have been studied. The obtained results show that the predicted results show reasonable agreement with the experimental data, and the variable trends of the penetration height and the separation distance are almost the same as those obtained in the experiment. The vapor pressure model is suitable to fit the relationship between the penetration height, the separation distance and the jet-to-crossflow pressure ratio. The combustion process mainly occurs upstream of the injection port, and it makes a great difference to the wall pressure distribution upstream of the injection port, especially when the jet-to-crossflow pressure ratio is large enough, namely 17.72 and 25.15 in the range considered in the current study. For hydrogen, the combustion downstream of the injection port occurs more intensively, and this may be induced by its smaller molecular weight.